ns 'OGDEN li . A COMPLEAT SYSTEM O F General Geography : EXPLAINING The Nature and Properties of the EARTH; riz. It's Figure, Magnitude, Motions, Situation, Contents, and Divifion into Land and Water, Mountains, Woods, Defarts, Lakes, Rivers, f)V. With particular Accounts of the different Appearances of the Heavens in different Countries ; the Seafons of the Year over all the Globe ; the Tides of the Sea ; Bays, Capes, Ifhnds, Rocks, Sand-Banks, and Shelves. The State of the Atmofphere ; the Nature of Exhala- tions; Winds, Storms, Tornados, bV. The Origin of Springs, Mineral- Waters, Burning Moun- tains, Mines, t3c. The Ufes and Making of Maps, Globes, and Sea-Charts. The Foundations of Dialling; the Art cf Measuring Heigbts and Diflancer, the Art of Ship-Building, Navigation, and the Ways of Finding //^LONGITUDE AT SEA. Originally written in LATIN By BERNHARD VARENIUS, M. D. Since Improved and Illuftrated By Sir ISAAC NEWTON and Dr J u R i N ; And nowTranflated into Englijh-, with additional Notts, Cop- per-Plates, an Alphabetical Index, and other Improvements. Particularly ufeful to Students in the Univerjities ; Travellers, Sailors, and all thofe who defire to be acquainted with Mixed Mathematics, Geography, Agronomy, and Navigation* By MrDUGDJLE. The whole Revifed and Corrected by P E T E R SHAW, M. D. 3Et)e g>econD (fcDttion, toitfj large 2tDDttion0. In i vVO VOLUMES. LONDON: Printed for STEPHEN AUSTEN, at the AngelzK& Bible, in St Paul's Cburcb-Yard. 1734. V.I I HAVE perufed this SYSTEM of GENERAL GEOGRAPHY; and I do recommend it as the moil Ufeful Book upon this Subject JAMES HODGSON, Majler of the Royal Mathematical ChriJl-Hofpital, School; And Fellow of the Dec. 14. 1732, Royal Society. THE TRANSLATOR'S PREFACE- HE Original of this Work was Re-printed at Cam- bridge in the Year 1672, for the Ufe of the Students in that Univerfity ; and an Advertilement was given of it, the Beginning of the Year following, in the Pbilofophical Tranfaftions (a). THE Dutch Edition being then out of Print, was carefully corrected, in many (a) Phil. Tranfaft. No. 91. Pag. 5172. BERN- HARD i VARENII, M. D. Geographia Gene- ral is ; in qua Affeftiones ge- nerates Telluris explicantur, fumma cura quam plurimls in- Loci s emendata, &* 33 Scbematilus nvui$ i are in- A 2 ci/ts, una cum Tabulis alt' quoty qu 4* 5- Definitions of a right Line, Circle 9 Dia~ ^ and Arc. 6. ft x The CONTENTS. 6. To ereft a Perpendicular upon a given Line. j. To divide a Circle and it's Periphery into four Quadrants. 8. To divide the Periphery of a Circle into^6o De- grees. 9. To find the Contents of a Reftangled-Triangle. 10. Having the Semi-diameter given, to find the Pe- riphery of a Circle. 11. Having the Periphery given to find the Diameter. 12. The Diameter of a Sphere being given , to find it's curve Surface , and Solidity , or folid Content. 13. Definitions of a Triangle ', Sine, Tangent, and ma- thematical Canon. 14. Two necejfary Theorems. 15. Four necejfary Problems. 1 6. An Explanation of different Meafures. CHAP. III. Of the Figure of the Earth. Page 27. 1 . Various Opinions concerning the Figure of the Earth. 2. The Earth's Figure ', the primary Property where- on the reft depend. 3. The Arguments that prove it fpherical. 4. taken from the Heavens. 5. taktnfrom the Earth. 6. Objections anfwered. CHAP. IV. Of the Menfuration and Magnitude of the Earth. Page 41. 1. The Menfuration of the Earth requires a Know- ledge of three Particulars ; viz. Ltnes y Surface, and Solidity. 2. The different Authors who have attempted ths Menfuration of the Earth. The C O N T E N T S. * 3 . The Method of the Arabians. 4. Eratofthenes. 5. Pofidonius. 6. Snellius. 7. Thefirjl Terr eftrial Method. 8. Thefecond. 9. 7&J. i o. The Circumference of the Earth ; it's Diameter^ Surf ace ) and Solid 'Content , z' linear ? fquare, and cubic Miles. 11. The Errors and Defefts of the federal -preceding Methods of meafuring the Earth. 12. The Meafure of the Parallels of the Earth. CHAP. V. Of the Motion of the Earth. Page 64. 1. The Motion cf the Earth the Caufe of the Celejlial Appearances^ upon the Copernican Hypothecs. 2. A double Motion^ le fides the third, which is ra- ther an Inclination of the Earth's Axis. 3. The Arguments for proving tbefe Motions. 4. Objections anfwered. 5. The Velocity of this Motion in different Parts of the Earth. CHAP. VI. Of the Earth's Place in the Syftem of the World. Page 78 1. Common Opinion places the Earth in the Centre of the World. 2. The Situation of the Earth > and the Order cf the Planets. 3. The Situation of the Earth upon the Copernican Hypothecs. 4. The Diftance the Earth from the Planets. 5: The Dijlance of the Earth from the Jixed Stars. 2 CHAP. xil The C O N T E N T S. CHAP. VII. Of the Subftance, internal Strufture, and Comp o- fition of the Earth. Page 87 1. To explain of what Subjlances the Earth is com- pofed. 2. The Earth divided into a confident and fluid Part? and the Atmofpbere ; or into Earth, Water, and Air. 3. How the Earth and Water bold together, and conftitute one Globe. 4. The Surface of the Earth continued, but not the Surface of the Waters. 5. How the Parts of the Earth are, from the Sur- face to the Center, is uncertain. 6. 'That Earth has it's Conjtftency and Coherence from Salt. 7. Different kinds of Earth variously mixed in the Globe. 8. The Situation and Difpofition oflbe Parts of the Earth different at different Times. CHAP. VIII. Of the Divifion of the Parts of the Earth into integrant Parts of the Sea. Page 103 i. Part of the Earth covered with Water, and Part not. z. The dry Paris feparated from each other by the Waters between. 3 . Four great Continents enumerated. 4. Ten great IJlands enumerated. 5. Ten moderate IJlands enumerated. 6. Ten fmall Ifiands enumerated. 7. The fmalleft IJlands enumerated. 8. The PeninfulaS) IftbmuJJes^ and Capes, or Head- Lands. . Fourteen The C O N T E N T S. xiii 9. Fourteen Peninfula's enumerated. 10. The more remarkable Jjlmvjfes enumerated. CHAP. IX. Of Mountains in general, and the Ways of taking their Altitude. Page 1 1 9 1. The Parts of the Earth are of different Al- titudes. 2. To fnd the Height of a Mountain by Al- timetry. 3. The Height of a Mountain Icing given , to fnd it's Dijlancefrom a certain Place. 4. The Diftance being given from whence the Top of a Mountain is frft feen to fnd it's Height. 5. The Height of a Mountain being known, to fnd the utmoft Diftance whereto it may be feen. 6. The Sun's Height above the Horizon being given at any Time, and the Length of the Shadow of the Mountain at that Time, to fnd the Height of the Mountain. 7. The Height of Mountains bears no fenfible Pro- portion to the Semidiameter of the Earth, or does not hinder the Sphericity of the Globe. 8. To explain the Origin of Mountains. 9. Why Rains and watery Meteors are frequent on the Tops of Mountains, wbilft it is fair below. 10. Whet her the Surface of a Mountain be more ca^ facious than the Plain it ftands on. CHAP, X. Of the Differences of Mountains. Page 135 1 . Some Mountains are large, others fmall. 2. The more famous Mountains enumerated. . Tbt xiv The CONTENTS. 3. 'The Tops of Mountains in mo ft I/lands and Head" Lands reach to the middle Region of the Air. 4. To enumerate the Mountains remarkable for their Height. 5. To enumerate the Burning Mountains. 6. To explain the Differences of Mountains. 7. Some Mountains are open, others clofe. 8. To enumerate the more famous Promontories. 9. Caves, deep Pits, &c. oppofed to Mountains. CHAP. XI. Of Mines, Woods, and Defarts. Page 158 1 . The Difference of Mines, and the more famous of them enumerated. 2. The Difference of Woods, and the more famous enumerated. 3 . The Differences of Defarts and the more famous enumerated. CHAP. XII. Of the Divifion of the Ocean by the Interpofition of the Land. Page 165 1. The Ocean furrounds the Earth in a continued Extent. 2. The Parts if the Ocean are of three kinds, viz. Seas, Bays, and Streights 3. The Ocean divided into four grand Parts, or Oceans, 4. The Parts of the Ocean named. 5. The eminent Bays enumerated, with their Diffe- rences. 6. The Enumeration and Differences of Streights. "j.TheSea-Coajls traced over the four Barters, and the Communication of the Parti of the Ocean, CHAP. The C O N T E N T S. X v CHAP. XIII. Of certain Properties of the Ocean. Page 181 1 . The Surface of the Ocean fpherical. 2. The Sea not higher than the Land. 3. Why the Sea feems to rife higher when viewed at a Diflance from the Shore. 4. To explain the Origin of Bays and Streigbts. 5. Whether the Ocean be every where of the fame Height. 6. The Depth of the Ocean may be found in many Places but not in all. 7. The Ocean has no -proper Springs. 8. The Saltnefs of the Ocean from the Particles of Salt diffolved in it. 9. Whether Sea Water be fweeter at the Bottom. 10. The Sea grows falter towards the Equator, and the Seafons of it's being unequally fait. 11. Why the Rain is fweet on the Sea. 12. Different Sea Waters are heavier than each other, and than common Water. 13. Sea-Water does not freeze fo foon as River- Water. 14. Why the Ocean becomes no larger by receiving fo many Rivers. 1 5 . Different Parts of the Ocean have different Colours. 16. Certain Peculiarities in certain Parts of the Ocean. 17. Why the Sea appears luminous ; or Jhines^ by Night, efpecially when the Waves are violent. 1 8. The Ocean throws up terrejlrial and confident , Bodies to the Shore. CHAP. XIV. Of the Motions of the Ocean, particular it's Flux and ReBux. Page 230 i. Water has only one natural Motion. 2. When xvi The CONTENTS. 2. When a Part of the Ocean moves, the whole is moved. 3. To obferve the Point of the Compafs wherein the Sea moves. 4. The Motion of the Sea is either direft, vortical, concujjbry^ or tremulous. 5. Some Motions of the Sea are general, fome particular, and the reft contingent. 6. The Wind caufes the contingent Motions of the Sea. 7. The general Motions of the Ocean double, viz. continued, and ebbing and flowing. 8. Winds often alter the general Motions of the Ocean. 9. The Caufe of the general Motion uncertain. 10. What the Motion of the Flux and Reflux is. 1 1 . The Caufe of that Motion. 12. Why at new ana full Moon the general Mo- tion of the Sea is more violent ; and alfo the Swell larger. 13. Why on the Days of the Equinoxes the general Motion and Swell of the Sea is greater. 14. A great Flux and Reflux on fome Shores, and on others fcarce fenfible. 15. The Flux of the Sea violent, the Reflux natural. 1 6. The Flux large ft in thofe Places where the Moon is vertical. 17. The Quantity of the Flux not conflant. 1 8. The Time of the beginning and ending of the Flux different in different Places. 19. In moft Places the Sea flows to the Shore fix Hours, and ebbs as many ; but in fome Places it flows longer than it ebbs, and vice versa. 20. Whether the Flood begins when the Moon touches the Horizon. 21. The Hour being given, wherein the Flood is at ifs greatefl Height in any Place, on the Day ef new Moon ; to find the Hour of it's greateft Height for the following Days. 2 22. The The CONTENTS. xvii 22. The Winds prolong and Jhorten the Duration of the Flux and Reflux. 23. A great Diverftty in the particular Motion of . tbe Sea. 24. Tbe frft particular perpetual Motion. 15. Thefecond 26. Tbe third 27. The fourth 28. Tbe fifth 29. Tbe fixtb 30. The feventh 3 1 . The particular periodical Motions enumerated. 32. Two kinds of Vortices in the Sea. 33. Tbe Caufe of the Tremor in the Sea, with Examples. 34. Wbj the Pacific Ocean is fo calm in fair Weather, but eaftly moved with gentle Winds. CHAP. XV. Of Lakes, Moors and Bogs. Page 280 1. Lakes, Moors, and Bogs defined. 2. Four kinds of Lakes. 3. To explain the Origin of thofe Lakes that neither receive nor fend out Rivers*; and to enumerate them. 4. To explain the Origin of thofe that fend out Rivers, but receive none. 5. To explain the Origin of thofe that receive Rivers, but fend none out. 6. To explain tbe Origin of thofe that both re- ceive and fend out Rivers. 7. Moft Lakes contain afrejh but fame a fait Water. 8. Whether the Cafpian Sea be a Lake or a Bay. 9. Whether the Euxine be a Lake or a Bay. jo. The Lakes enumerated that have IJlands in tbe middle. VOL. I. a ii. To xviii The C O N T.E N T S. 11. 2*0 make a Lake in a Place aj/igned ; if ikt thing be pojfible. 12. 'To dry or drain up a Lake. 13. Bogs of two kinds. 14. Bogs contain a fulphureous Earth. 15. %4 dry a Bog. CHAP. XVI. Of Rivers in general. Page 295 1 . The Definition of Rivers, Rivulets, and Springs, &c. 2. Torrents and Rivers fometimes produced by violent Rains, and melted Snow. 3. Moft Rivulets rife from Springs, and Rivers from a Conflux of Rivulets. 4. Rivers enlarged by Rains and melted Snow at different Times of the Tear. 5 . The Caufcs of Springs, or the Origin of Spring- Water. 6. Some Rivers dip under Ground, and rife again. 7. Rivers difembogue into the Sea, or Lakes. 8. Few Rivers become jlagnant. 9. Whether the Cbanels, and Windings of Rivers were made by Nature or human Induftry. 10. Cbanels, the nearer to the Spring- Head the higher ; and the nearer to the River's mouth the deeper. 11. Of Cataratls. 1 2. Why Rivers are broader in one Part than another. 13. The Cbanels of Rivers fink more or lefs in one Part than another. 14. Why fome Rivers are rapid, others gentle ; and why the fame River is more rapid in one Place than another. 15. Some few Rivers run a dirett Courfe ; but mojl a winding one, to their Exits. 1 6. The Lakes tbro* which certain Rivers have their Courfe. 17. Moft Rivers the nearer their Mouths, the tbe\ become, 18. ne The C O N T E N T S. xix 18, The Water of Rivers contains many Particles of different Metals, Minerals, Sands, oleaginous and other Subftances ; as alfo certain fubtils Spirits of Vitriol^ Salt, Sulphur, &c. ig. 'The Rivers that have Gold-Sand enumerated. 20. The Waters of mofi Rivers differ in Colour 9 Gravity, and other Qualities. 21. Certain Rivers are fo inlarged, at Jlated Times, as to overflow their Banks. 22. To enumerate thefe Rivers, and their Caufes. 23. To explain the Origin and Rife of Springs. 24.- To find whether a Spring, or Well, may be made in a Place ajjigned. 25. To make a Well in a given Spot ; if the Thing be poffible. 26. To make an apparent Spring in a Place ajjigned ; if the Thing be poffible. 27 .To bring a River from a Spring, or from another River, to a given Place, if the Thing be pojjible. 28. The Art of Levelling, or taking the Fall of Wa- ter, &c. 29. The great Rivers of a long Courfe enumerated. 30. Certain Rivers have Whirlpools and Swallows* 31. River- Water lighter than Sea- Water. CHAP. XVII. Of Mineral -Waters, Hot- Springs, &V. Page 359 1 . No Water found pure and elementary. 2. Mineral Waters defined. 3 . Three general Kinds of Mineral Waters. 4. To explain the Origin of Mineral Waters. 5. That the particular Species of Mineral Waters are infinite. 6. To enumerate the more remarkable and extra- ordinary Differences of Waters. 7. Of the Acidulse, or tart Waters. 8. Of Hot Springs. a 2 9. Of xx The C O N T E N T S. 9. Of oily and uncJuous Waters. 10. Of bitter Waters. 11. Of extreamly cold Springs. 12. Offuch Waters as tranfmute or alter Subftanfts. 13. Of poifonous and Mortal Waters. 14. Of coloured Waters. 15. Of Salt-Waters. 1 6. Of bubbling^ or boiling, Springs, andfuch as break forth with a violent Spirit. 17. Springs that run only at flat ed Times. CHAP. XVIII. Of the Change, and Origin of dry Parts and watery, on the Earth. Page 395 1. To examine the extant Surface of the Earth, and that covered with Water. 2. The Surface of the Land and Water not perpe- tually the fame. 3. To compute how much Sand, and how much Water the Earth contains. 4. Waters forfake the Shores, and leave them dry on many Accounts ; andfirft, as in Mears and Bogs. 5. Rivers forfake their Banks and Cbanels, and af- ford new Land. 6. Lakes are dried up, and changed to Land. 7. S freights are dried up. 8 Bays are dried up. 9. Parts of the Ocean are dried up. 10. To explain the Origin of Sand- Banks. 11. Whether Sand- Banks may become a part of the neighbouring Continent. 12. I/lands are formed feveral Ways. 13. The more extraordinary Ways wherein IJlands art formed. 1 4. Of Floating IJlands. 15. Rivers change their Chanels many Ways, or run over new Trafts of Land, 16. Lakes The C O N T E N T S. xxi 1 6. Lakes, Meers, and Bogs poffefs Spaces of Land they did not occupy before. 17. 'The Ocean poffeffes new Trafls of Land, where it did not appear before. 1 8. Whether the entire Surface of the Earth may be folely poffeffcd by Water alone, or Land alone. 19. Why there are few I/lands in the middle of the Ocean ; but many Shoals of them near Continents, or larger I/lands. 20. Why Lands prove fertile or barren ; and why on the Sea-Shore the kind of Earth alters that covers the Fields. CHAP. XIX. Of the Air and Atmofphere. Page 419 j . Exhalations continually rife from the Parts of the Earth. 2. 'The State of the Atmofphere. 3. Exhalations are thicker or thinner at different Times, and in different Places. 4. Various Kinds of Exhalations. 5. The Particles of the Air rcfleft the Surfs Rays, like a Speculum. 6. The upper Parts of the Atmofphere are more rarijied than the lower. 7. Exhalations are driven upwards by a violent Mo- tion ', tho y their natural 'Tendency is downwards. 2. The Atmofphere when warmed poffeffes a larger Space, and when cold a lefs. 9. To make a Thermometer, or Weather-Glafs. 10. How, or to what Degree, the Air may be rarijied. 1 1 . Why the Air is generally thick and Cloudy in the Frigid Zone. 12. Why the Air is thin and clear in violently frojly Weather. 13. Why the Air appears thicker at the Horizon. 14. Whether the Air, or Atmofpbtre, be of the fame Height in all Places, 15. flfc xxii The C O N T E N T S. 15. < Tbe Condenfation and Rarifaftion of the Air does not alter it's Height. 16. The Height of the Air the fame at all Times, and in all Places. 17. The Ah- more condenfed in the Winter, and at Night, than in the Summer, and by Day. 1 8. The different Denjity of the Air in different Places. 19. The middle Region of the Air nearer the Earth in Places contiguous to the Pole. 20. In Places adjacent to the Pole the hot Region of the Air, or the beginning of the upper Region, is more remote. 21. We Rays of the Sun, Moon, and Stars are re- framed in the Air. 22. On Account of this Refraftion the Sun and Moon appear to rife fooner than they ought. 23. The thicker the Air , the greater the Refratlion. 24. The thicker the Air, the fooner the Sun and Moon appear to rife. 25. The lower the Air that caufes the Refratlion, the fooner the Stars appear to rife. 26. The Rejraftion of a Star may be the fame in the fame Situation, tho* the Height of the Air be different. 27. If the Air be thicker, or lower, in one Place than in another, the Sun or Moon will appear fooner in the former than in the latter. 28. If the Air be thicker and higher in one Place than another, the Stars will accordingly be feen to rife fooner, or later. 29. Two Refractions being taken at two Altitudes, to find from thence both the Height and Thicknefs of the Air, with Refpeft to the ALlber, or the Law of Refraction. go. To find the leaft poffible Height of the Atmofpbere. 3 1 . To find the Law of Refraction. 32. To find the Refraction at any Inclination. 33. To find the Refraction at the given Height of a Star. 34. The Light of the Stars, particularly the Sun and Moon t are rcflefted by the Particles of Air. 35- The CONTENTS, xxiii 35. This Reflection is the principal Caufe of the Twilight. 36. When the Twilight begins. 37. 'The Height of the Air not to be found from the Quantity of the Twilight. 38. The Height of the Air^ upon a Suppofition that a double Reflection is the Caufe of the Twilight. 39. The Height of the Air being given ^ to compute it's Quantity. 40. The Air has certain Peculiarities, in certain Places. CHAP. XX. Of the Motion of the Air, Winds in general, and the Points of the Compafs. Page 477 j . Winds defined. 2. Moft Winds blow from one Point to the oppofite. 3 . Points of the Compafs defined. 4. The Number of Points and Winds. 5. Two and thirty Points and Winds. 6. A more accurate Enumeration of the Points and Winds. 7. The Winds according to the Antients enumerated. 8. Another Enumeration of the Winds. 9. Oppofite Winds. 10. Various Caufes of Winds. 11. Why Winds may blow perpendicularly to the Ho- rizon of a Place. 12. Why the Winds blow not in continued^ but inter- rupted Blafts. 13. Why Winds veryfetdom blow perpendicularly upon a Place from above, but generally oblique. 14. Why the South and Weft Winds are warm. 15. Why the Weft Winds blow feldomer than the Eaft. 1 6. Why the North and Eaft Winds are ftronger, and the South and Weft Winds weaker. 17. Why a fmall, thick, and blacki/h Cloud for et eh Wind from that Quarter. 1 8 . Wby Winds are frequent in the Spring and Autumn. 19. At xxiv The CONTENTS. 19. At what Height, or in what Region of the dir, the Winds How. 20. To what Diftance one and the fame Wind may reach. CHAP. XXI. Of particular Winds, and Storms or Tempefts. Page 491 1. Some Winds are conflant, others not. 2 . Some Winds are general, others particular. 3. The Caufe of the general Winds. 4. Some Winds periodical and jlated ; others uncer- tain and contingent. 5. The periodical Winds enumerated. 6. The Caufe of the Eteftan Winds. 7. Why the Etefian are not found in many Places. 8. Some Winds peculiar ', others common. 9. Certain winds periodical at certain Hours. jo. Northern Winds moft frequent in Places near the North Pole. 1 1 . Four Species of Winds. 12. Certain impetuous and fudden Winds. 13. Their Kinds exemplified. 14. Tornados, or Travados. 15. Cataracts, or Exbydrias. i 6. Ecnephias, or leffer Exhydrias. 17. Typbon, or Orancban. 1 8. Whether certain Winds burft out of the Earth, or rife from the Water. 19. Whether a certain Wind may rife from the Flood of the Sea and Rivers. 20. the Caufe s of the Brothers at Sea ; or Caftor, Pollux, and Helena in Tempejls. 2 1 . Why Calms are fo frequent in Part of the Ethiopic Ocean, under the Equator ; efpecially on the Gui- nea Coaft. az. Storms and Tempejls anniverfary in certain Places^, THE THE ABSOLUTE PART O F Univerfal Geography. SECT. I. P R E L I M IN A R I E S. CHAP, j?^ Of //^DEFINITION, DIVISION, METHOD, &c, ofGEOGR/tPHT. T hath been an antient Cuflom for thole that fully treat of any Art, or Science, to premife fomewhac of it's Origin^ Nature^ Conjlilul'ion^ &c. And this Procedure is not improper, provided it be clear t>f all fophiftical Equivocation *, be- caufe from fuch Preliminaries the Reader may con- ceive an Idea of the Work, or at leaft the Sub- ftance thereof, and fo proceed more advifedly there- in. We fhall therefore here offer a few Particu- lars as to the Nature, Ufe* and Defign of Geography. VOL. I. B 2& 2 Ibe Abjolute Part SECT. I, The Definition of Geography. GEOGRAPHT'is that part of mix'd Mathe- matics, which explains the State of the Earth, and of it's Parts, depending on Quantity, viz. it's Figure, Place, Magnitude, and Motion, with the Celeflial Appearances, &c. B Y fome it is taken in too limited a Senfe, for a bare Defcription of the feveral Countries ; and by others too extenfively, who along with fuch a De- fcription would have their Political Conftitution. But the Authors who proceed thus are excufable, becaofe they do it only to excite and delight the .-Reader, who might otherwife be the lefs attentive to a bare Enumeration and Defcription of the Coun- tries, without fome Knowledge of the Manners, and Cuftoms of the Inhabitants. The Divifton of Geography. WE divide Geography into General and Special, or Univerfal and Particular. Golnitzius fays, Geo- graphy is to be explained externally and internally ; but thefe Terms are improper, and ill chofen, Uni- verfal and Particular being much more pertinent. We call that Univerfal Geography which confiders the whole Earth in general, and explains it's Pro- perties without regard to particular Countries : But Special or Particular Geography defcribes the Confti- tution and Situation of each fingle Country by itfelf ; which is twofold, viz. Cborograpbical, which de- fcribes Countries of a confiderable Extent ; or Topo- graphical, which gives a View of fome place or fmall Tract of the Earth. I N this Book, we mail exhibit Univerfal Geogra- phy, which may be divided into three Parts, Abfo- lute, Relative, and Comparative. In the dbfolute Part CHAP.- I. of Univerfal Geography* 3 Part we fhall handle what refpects the Body of the Earth itfelf, it's Parts and peculiar Properties -, as it's .Figure, Magnitude, and Motion , it's Lands, Seas, and Rivers, &c. In the Relative Part we lhall account for the Appearances and Accidents that happen to it from Celt lial Caufes : and, laftly, the Comparative Part lhall contain an Explication of thofe Properties, which arife from comparing dif- ferent Parts of the Earth together (a). The Subjeff of Geography. THE Object,- or Subject, of Geography is the Earth , efpecially it's Superficies and exterior Parts. 'The Properties of Geography* THE Things which feem to be moft worthy of Obfervation in every Country are of three kinds, viz. Celeftial, Terrejlrial, and Human. The Celejlial Pro- perties are fuch as affect us by reafon of the apparent Motion of the Sun, arid Stars. Thefe are eight in Number : i . The Elevation of the Pole, or the Dif- tance of a Place from the Equator. 2. The Obliquity of the Diurnal Motion of the Stars above the Horizon of that Place. 3. The time of the longejl and Jhortejl (a) The Honour of reducing Miftakes, and hath left us a Me- Geography to Art and Syftem thod of difcovering his own. was refer ved to Ptolemy j who There is one thing yet very by adding Mathematical Advan- lame in our Geography, the fix- tages to the Hiftorical Method, ing the true Longitude of in which it had been treated of Places ; and tho' feveral new before, has defcribed the World Ways have been lately tried, to in a much more Intelligible redrefs this Inconvenience, both Manner: he has delineated it from exaft Pendulums, and from Under more certain Rules, and Obfervations upon the Immer- by fixing the Bounds of Places, fions and Emerfions of Jupiter '/ from Longitude and Latitude, Satellites, yet they have not al- hath both difcovercd others together preved effectual. B 2 Day. 4 f&e AbfdutePart SECT. I. Day f 4. The Climate and Zone. 5. Heat, Cold, andtheSeafonsoftbe Tear-, with Rain, Snow, Wind, and other Meteors : and tho j thefe may feem Ter- reftrial Properties, yet becaufe they chiefly depend upon the Motion of the Sun, and the four Seafons of the Year, we have reckoned them among the Celeftial Matters. 6. The Rifmg, Appearance, and Continuance, of the Stars above the Horizon. 7. The Stars that pafs thro' the Zenith of a Place. 8. The Celerity of the Motion with which, according to the Co- pernican Hypotbe/is, every Place conjlantly revolves, And according to Aftrologers a ninth Property may be added ; for they afiign fome Country or other to every one of the twelve Signs of the Zodiac, and the Planets which are Lords of thefe Signs , but fuch imaginary Qualities feem fuperftitious and vain to me ; nor do I perceive any reafonable Foundati- on for them (a). Thus far the Celeftial Properties. W E call thofe Terreftrial Properties that are ob- ferved in the Face of every Country ; which are ten in Number, i . The Limits and Bounds of each Country. 2. It's Figure. 3. It's Magnitude. 4, It's Mountains. 5. It's Waters, viz. Springs, Rivers, and Bays. 6. It' s Woods and Defarts. 7. The Fruit- fulnefs and Barrennefs of the Country, with it's various kinds of Fruits. 8. The Minerals and FoJJils. 9. The living Creatures there. 10. The Longitude of the Place: which might be comprehended under the firft of thefe Properties. {a} Tho' this Art be of great to this Day, veaerated in moft Antiquity, it is rejefted and Eaftern Countries, efpecially a- exploded by moft knowing Peo- mong the Indians ; where no- pie of this Age ; and only Im- thing is done of any Confe- poftors, or fome weak Pre- quence, before the Aftrologcr tenders to Learning, now pra- determines a fortunate Hour ftife it, in thefe Parts of the to undertake it. Set Robaulfs World. It is however, even Pbtftt Part z. Chap. 27. THE CHAP. I. of Univerfal Geography. $ THE third kind of Obfervations, to be made in every Country, we call Human, becaufe they chiefly refpect the Inhabitants of the Place ; and thefe are alfo ten in Number, i. Weir Stature, Shape, Colour, and the length of their Lives ; their Origin, Meat, and Drink. 2. "Their Arts, and the Profits which arife from them -, with the Merchandife and Wares they barter with one another. 3. 'Their Virtues and Vices, Learning, Capacities, and Schools. 4. 'Their Ceremonies at Births, Marriages, and Fu- nerals. 5. 'The Language which the Inhabitants ufe. 6. 'Their Political Government. 7. Their Religion and Church Government. 8. 'Their Cities and famous Places. 9. Their remarkable Hi/lories. 10. 'Their famous Men, Artificers, and the Inventions of the Natives. T H E S E are the three kinds of Occurrences to be explained jn Special Geography , and tho' the laft Sort feem not fo properly to belong to this Science, yet we are obliged to admit them for Cuftom fake, and the Information of the Reader. IN Univerfal Geography (which is the Subject of this Book) the abfolute Divifion of the Earth, and the Conftitution of it's Parts, will firft be exa- mined , then the Celeftial Phenomena, in general, that are to be applied to their refpective Countries, in Special Geography ; and laftly there will follow in the Comparative Part fuch Confiderations as occur from comparing the Phenomena of one Place with another. The Principles of Geography, THE Principles from which Arguments are drawn for proving Proportions in Geography are of three forts, i. Geometrical, Arithmetical, and Trigonometrical Propofitions. 2. Aftronomical Precepts and Theorems (tho' it may feem ftrange B 3 we 6 ?be Abfolute Part SECT. I. we mould have Recourfe to the Celeftial Bodies, which are diftant from us fo many Millions of Miles, for Underftanding the Nature of the Earth we inhabit). 3. Experience; becaufe the greateft JPart of Geography, and chiefly the Special, is founded only upon the Experience and Obferva- tions of thofe who have defcribed the feveral Coun- ts, *Thc Order of Geography, THE Order we have thought moft conve? nient to follow in General Geography, is already mentioned in the Divifion and Explication of it's Properties ; yet there remains a Doubt as to the Order to be obferved in explaining thefe Properties : viz. whether we mould apply them to their relative Countries in which they are found, or refer the Countries themfelves to the Properties accounted for, in general. Ariftotle, in his firft Book of A- nimals, moves the fame Doubt ; and argues at large, whether the Properties mould be adjufled to the general Account of Animals, or the Ani- mals ranked under the Account of their Proper- ties. The like Difficulty occurs in other Parts of Philofophy. However we mall here firft explain fome general Properties ; and after apply them to $hcir reipetive Countries. the Proof of Geography. I N proving Geographical Propofitions we are to obferve ; that feveral Properties, and chiefly the Celeftial, are confirmed by proper Demonftrar tions : But in Special Geography (excepting the Ce- leftials) almoft every Thing is explained without pemonftration , being either grounded on Expe- rience and Obfervation, or on the Teftimony of our CHAP. I. of Unherfal Geography. 7 our Senfes : nor can they be proved by any other Means. For Science is taken either for that Know- ledge which is founded on Things highly proba- ble j or for a certain Knowledge of Things which is gained by the force of Argument, or the Tefti- mony of Senfe ; or for that Knowledge which a- rifes from Demonftration in a ftrid Senfe, fuch as is found in Geometry, Arithmetic, and other Ma- thematical Sciences; excepting Chronology and Geography *, to both which the Name of Science, taken in the fecond Senfe, doth moft properly belong. THERE are alfo feveral Propofitions proved, or rather expofed to view, by the artificial Ter- reftrial Globe, or by Geographical Maps -, moft of which might be confirmed by a ftric~t Demonftrati- on ; tho' omitted on Account of the Incapacity of fome Readers. Other Propofitions cannot be Ib well proved, yet are received as apparent Truths. Thus tho' we fuppofe all Places on the Globe, and in Maps, to be laid down in the fame Order as they really are on Earth ; neverthelefs in thefe Mat- ters we rather follow the Defcriptions that are given by Geographical Authors. Globes and Maps, in- deed, made from fuch Obfervations, ferve well enough for Illuftration, and the more eafy Compre- henfion of the Thing. The Origin of Geography. THE Origin of Geography is not of late Date, nor was it brought into the World as it were at one Birth ; neither was it invented by one Man : but it's Foundations were laid many Ages ago. It is true, indeed, the old Geographers were employed only in defcribing particular Countries, either in whole, or in part. The Romans, when they had overcome and fubdued any Province, ufed to ex- B 4 pofe 8 *lhe Abfolute Part SECT. I. pofe the Cborograpby thereof to the Spectators in their Triumphs, delineated upon a Table, and flourifhed round with Pictures. There were alfo at Rome, in the Portico of Lucullus, feveral Geographi- cal Tables expofed to public View. The Senate of Rome, about one hundred Years before the Birth of Chrift, lent Geographers and Surveyors into the fe- veral parts of the Earth, that they might meafure the whole ; tho' they fcarce vifited a twentieth Part of it. Neco, alfo, King of Egypt, many Ages be- fore Chrift, commanded that the Extremities of Africa mould be diligently fearched into -, which was performed by the Phoenicians in the fpace of three Years. Darius commanded that the Mouths of the River Indus, and the whole sEthiopic Sea, to the eaftward, mould be diligently examined into. Alex- ander the Great, as Pliny tells us, jn his Af f atic Ex- pedition, carried along with him two Geographers, Diogenes and Beto, to meafure and delineate to him his Journies ; from whofe Journals and Obfervations the Geographers of fucceeding Ages borrowed many Things. And tho' the Study of all other Arts was almoft aboliihed by the Wars, Geography and For- tification were improved thereby. NEVERTHELESS the Geography of the Antients was very imperfect, and commonly full of falfe Relations ; becaufe they knew little or nothing of thcfe Places of the Earth which are of moft Con^ fequence to be known -, or at leaft they had no cer- tain Experience about them. For, i . all America \yas entirely unknown to them. 2. So were the re- moteft Northern Countries. 3. The South Conti- nent and the Country of Magellan. 4. They knew not that the World coijld be failed round, or that the Earth was furrounded by the Ocean, in an un- interrupted Continuity : Some indeed of the Anti- cuts I confefs were of this Opinion, but I deny they had any Certainty of it. 5. They knew not that CHAP. i. tf Unfaerfal Geography. 9 that the Torrid Zone was inhabited, by an alinoft in- finite number of People. 6. They were ignorant of the true Meafure of the Earth, tho* they writ a great deal on that Subject. 7. They did not think that Africa could be failed round, (b) becaufe the South Parts thereof were unknown to them. 8. Both the Greeks and Romans wanted true Defcripti- ons of the Countries remote from them, and have kit us a great many forged and fabulous Stories, concerning the People that live in the Borders of Afia^ and thofe that inhabit the Northern Parts of the Earth (c). 9. They were ignorant of the ge- neral Motion of the Sea, and the Difference of Cur- rents in particular Places. 10. The Grecians, even Ariftotle himfelf, did not know the Reafon of the Ebbing and Flowing of the Sea. 1 1 . Few of them underftood the Variation of the Winds ; and the (b} It is likely the antient Et alibi, cauda villofa famines Egyptians had fome Knowledge nafci pernicitatis fximiand Origin. 2. Their Arts, Profits, Commodities, and Trade. 3^ Their Virtues and Vices; their Capacities and Learning. 4. Their Ceremonies at Births, Marriages, and Funerals. 5. Their Speech and Language. 6. Their Political Government. 7. Their Religion and Church Government. 8. Their Cities. 9. Their memorable Hiftories. 10. Their famous Men and Women, Artificers and Inventions. H CHAP. II. Some Propofitiotu in Geometry and Trigonometry, of ufe in Geography. PL A TO very juftly called Geometry and Arith- metic the two Wings whereby the Minds of Men might mount up to Heaven ; that is, in fearch- ing after the Motions and Properties of the Celeftial Bodies. Thefe Sciences are no lefs uferul in Geogra- phy ; if we defire to underftand it's fublime and in- tixcare Parts, without any Hinderance. It is true, a lefs fhare of Mathematics will ferve for Geography* than 4ftronomy : but becaufe feveral are taken with the -i$ Tfa Abfolute Part SECT. I the Study of Geography who do not underftand thefe Sciences, we fliall here let down a few Propo- fitions from them, fuch as we think moft necefiary j that the Reader may proceed the more readily with- out Interruption in his Study. Tho% by the way, we "do not at all encourage that bad Cuftom fome young Gentlemen have got, in applying themfelves unadvifedly to other Parts of Philofophy, before they have a competent Knowledge in Arithmetic and Geometry. The Fault is very often in their Matters and Tutors, who are for the moft Part ig- norant of thefe Things themfelves, and therefore cannot admonifh Youth to Ihun fo pernicious a Cuftom. In Arithmetic we fuppofe the Reader to know the four common Rules of Numeration, viz. Addition, SubftracJion^ Multiplication , and Divifion, with the Golden Rule, or Rule of fbree ; and there- fore mail not treat of them here. If any one under- ftand them not, he may learn them much better from fome able Teacher, than from Books. 1 . BUT as to Geometry, it treats of three forts of Magnitudes, by which every Thing is meafu- red j viz. Lines, Superficies, and Solids : neither can there be found in Nature a Body of any other Dimenfion. 2. A LINE is either ftraight or curved ; and a Curve again is either uniform as circular, or ciiflf- milar and variable, as the ^Ellipfe, the Conchoid, and Spiral Line. 3. A CIRCLE is a Space or plain Super- ficies bounded with a curve Line, wherein there is a Point from which all right Lines drawn to the Curve are equal. The curve Line which bounds that Space is called the Circumference, or Periphery of the Circle i and the middle Point is called the Center (a). (} Euclid Lib. i. Vef. 15,1 6, , THE CHAP. 2. ofUnmer/al Geography. \j 4. T H E Diameter of a Circle is a right Line drawn thro' the Center, and terminated at both ends by the Periphery : one half of which is called the Semidiameter, or Radius (a). 5. AN Arch is part of the Periphery of a Circle. A Quadrant is a fourth Part ot the whole Periphery. What an Arch wants of a Quadrant is called the Complement of that Arch : and it's Diffe- rence from a Semicircle it called it's Supplement (b). PROBLEM. 6. HAVING aright Line given and a Point either in, or out of it, to draw thro* that Point a Line perpendicular to the former. LET the Line given (Fig. 2.) be AB, and the Point C : open the Compafles fo, that fetting one Foot in C, you may with the other cut the Line given in df; then one Foot being placed at d, with the other defcribe an Arch, as g h ; allb make/ the Center, and with the fame. Radius de- fcribe another Arch, which will cut the former in g and h , fo draw the Line g b ; which will be the Perpendicular required. 7. TO divide a Circle and ifs Periphery into four equal Parts. Draw a Diameter, and from the Center raife to it a Perpendicular, which prolonged will be alfo a Diameter ; whereby both the Circle and it's Periphery will be divided into four equal Pans (c). 8 . TO divide the Periphery of a Circle into Degrees. A Degree is the 36oth Part of the Circumference. Mathematicians always divide the Periphery into (a) Euclid Lib. \..Def. 17. (c) ttid. Prop. 4. Lib. iv. (*) lb. Prop, M, , 2 . Lib. i. V O L. I. C fo 1 8 fbe Abjohitc Part SECT. I. fo many equal Parts tf) ; and each of thefc Par ts into 60 fmaller Divifions, called firft Minutes; alfo each Minute into 60 Seconds, &c. commonly writ thus, 3 degr. 2. min. 5 fee. that is, 3 Degrees, 2 Minutes, 5 Seconds. Hence the Quadrant con- taineth 90 Degr. the Semicircle 180, and the fixth Part of a Circle 60 Degrees. THEREFORE to folve this Problem, di- vide the Periphery into Quadrants, then take off the Semidiameter, and with it's Length cut an Arch from the Periphery (*), which will be equal to 60 Degr. fo there remains in the fame Qua- drant 30 Degr. which being bifected you will have 1 5 Degr. this again mechanically trifected will give 5 Degr. which divided into five equal Parts make fo many Degrees, Q. E. F. But this is done more artificially by mathematical Inftruments (/). 9. TO find the Area of a Quadrangle, or a Space contained in a Figure of four Sides, and four Right Angles. Multiply one fide by the other, and the Product is the Area. It is to be obfcrved that Lines are meafured by Lines, and Superficies by Meafures that are Superficies, or Squares ; alfo the Contents of folid Bodies, which have their Dimen- fions, are computed in folid Meafure, or fo many Cubes. Thus we meafure the Sides of a Houfe by a lineal Foot, the Floors and Wainfcot by a (d) This Division of a Circle from the fame Point lay on thd into 360 Parts, or Degrees, is Chord of two Degr. fo of three becaufe that number can be di- Degr. &c. 'till you come to 90 vided into more Aliquot Parts, Degr. then begin again as before than any other convenient 'till the whole Periphery is di- Number, viz. into 2,3,4,5, vided. By this means you will 6, 8 and 9 Parts. avoid the Errors which may a- (e) Euclid. Prop. 15. Lib.\v. rife from the intermediate Di- (f) By a Line of Chords vifions, and tho' thefe Errors truly divided; thus, from any fmgly confidered are very, fmall. Point in the Periphery lay on yet in fo many Degr. they will ihe Chord of one Degr. then produce one very fenfiblc. 2 iquare CHAP. 2. ef Univerfal Geography * 19 fquare Foot, and the Space it enclofeth, confider- ed as a Solid, by a cubical Foot. 10. HAVING the Diameter or Semidiameter of a Circle, to find the Periphery in the fame Meafure : and converfly, having the Periphery given to find the Diameter as near as pojjlble (g). The Solution of this Problem depends upon die determined Pro- portion of the Diameter to the Periphery, which is nearly as 7 to 22 ; as is demonftrated by Archi- medes 9 or more accurately, as 10000000000 is to 21415926535 (). For Example, let the Dia- meter be 1 2 Foot ; by the Golden Rule, as 7 is to 22 : fo is 12 to the Periphery of the Circle ; or if you ufe the other Proportion it will be much the fame. BUT if the Periphery be given, and the Dia- meter be required, fay ; as 22 is to 7, or as. 31415926535 to 10000000000, fo is the Peri- phery given to the Diameter required. 11. THE Diameter and Periphery of a Circle ', or either of them, being given in Miles or Feet, to find (g) See Tacquefs felel The- who carried his Calculation to orems of dr chime des, Prop. 5. 3 5 places of Decimal Fractions. (b) Tho' it be well known Or if he would flill be more that the Periphery of a Circle nice and curious, he may have is incommensurable to the Dia- recourfe to Mr Abr. Sharp's meter, yet either of thefe Pro- Calculation, to double the Num- portions will ferve well enough bcr of Fait Caulerfs Fractions, for common Ufe. But no Pro- By which Exaftnefs the Cir- portion in fmall Numbers is fo cumferance of the Terraqueous exact as that of Andrew Me- Globe, may be computed to a tius, viz- 113 to 355, which Degree leis than the Breadth is found not to differ from the of a Grain of Sand : yea, more Truth above T ^ r J__-. But than this, the number of the if the Reader defirech the niceft Grains of Sand, that would be Computation of the Proportion contained in a Space as big as of the Diameter of a Circle to the Sphere of the Fixt Stars, the Circumference (ahho 1 that might be truly computed by of Mtftiui comes very near,J, let this means. Vid. Math. Tables him have recourfe to the labo- printed for Mr Mount, p-ge ricus Calculus gf Van Ceulen, 53, &c. C 2 be 20 The Absolute Part SECT.!. the Area of that Circle in fquare Miles, or fquare Feet. Multiply one half of the Periphery into the Semi- diameter, and the Product will be the Area requi- red (i) : but if you have only one of them given, you may find the other by the laft Problem : Or it may be done without it (k). 12. THE Diameter, or Semidiameter^ of a Globe being given; to find it's Superficies in Square, or it's Solidity in Cubic Meafure. A Globe is a round folid Body, having a certain Point in the Center of it, from whence all right Lines drawn to the Surface are equal : and a Line drawn thro' this Point is the Diameter, about which if the Globe be revolved it is called it's Axis (/;. Moreover if a Globe be cut any how by a right Line, the Section is a Circle ; if thro* the Center the Circle will have the fame Diameter as the Globe itfelf ; and fuch are called the greater Circles of the Sphere or Globe, and the reft letter Circles. To folve the Problem (m) : By the tenth Article, find the Periphery -, then multiply the Di- ameter into this Periphery, and the Product will be the Superficies of the Globe in fquare Meafure, which multiplied into the % of the Diameter, will produce the Solidity of the Globe in cubic Meafure. (/) As is demonflrated by i i j j Archimedes, Prop. \ . De Di~ j- \- men/tone Circuit. 357 9 (k) By faying, as the Square I I i j of i f which is i) is to 7854 -j- ._L (the Area of a Circle whofe 1 1 13 15 '17 Diameter is \) fo is the Square of any other Diameter to it's __ ___ -j 1, & c . Area; By Prop. z. Lib. ii. of IQ ' 2l' Euclid. The famons M. Leib- nitz has demonftrated, that if M Eucltd - Ll *-"- ^ e f- 4 the Diameter of a Circle be i, '5; l6 ' 7- , (m) See this demonftrated in the true Area will be Taequet'i Select Theorem s of Ar- thimedef, Scholium z, of Prop. 24. and that of Prop. 28. C H A P. 2. of Univerfal Geography. 2 1 13. A R 1 G HT angled Triangle hath two fides perpendicular to each other (or make an Angle of 90 Degr.) which two (ides are called the Catbeti, or Perpendiculars, and the third fide the Hypo- tenufe. THE Meafure of an Angle is the Length of an Arch defcribed from the angular Point as a Center : that is, as many Degrees as the Arch be- tween the Legs of the Angle doth contain -, fo many Degrees the Angle is faid to be of. Thus a right Angle is 90 Degr. becaufe the Arch fo de- fcribed is a Quadrant. THE right Sine of an Arch is a right Line drawn from the one end of the Arch perpendicular to the Diameter, which paffeth thro' the other end (). THE Tangent of an Arch is a right Line which touches the Arch at one end, and is bounded at the other with a Line drawn thro* the Center, and the other end of the Arch ; which Line is called the Secant of that Arch. MOREOVER, the Sine, Tangent, and Secant 9 of an Angle, are the fame of the Arch which meafureth the Angle. (n) Mr Whiflon in his Notes A B D, the Square of A B // e- upon Tacquefs Euclid, has neat- qualto the Square of A D and ly explained the Origin of Sines, B D. Therefore let the Semi- Tangents, and Secants. CorolL diameter A 8 be fquared, and to the 47 ch Prop. Lib.'i. which from that Square fubjlr a fl the we (hall here tranfcrihe. Let Square of B D : The Remainder A C the Semidiameter of aCircle will be the Square of A D or ( Fl S- 3-) be f 100.000 Parts, of the Co-fine B F equal to it: and toe Jng/eBA Dof$o Deg. out of which extraft the f quart becaufe the Chord or Sub ten ft of Root, and you will have the 60 Degr. is equal to AC the Line B F or A D. Then by this Semidiameter (by Prop. \ 5. Lib. Analogy at A B : BD : : A E : iv. Euclid] B D the Sine 0/30 C E or A D : B D : : A C : C E, Degrees Jkall be equal to ont jo you have the Tangent C E. half the Semidiame'.er, or And if the Square of A C be ad- AC; and therefore Jhall con- ded tv the Square ofCE, the tain 50.000 Parts. But now Root of the Sum being extracted in the right-angled Triangle will be the Saant A . $> E. I. C 3 IT 22 The Abfblutt Part SECT.I. I T is alfo necefiary to be known that Tables have been calculated by the great Labour and In- duftry of fome Mathematicians, in which the Dia- meter being taken for 100000, &c. the Sines, Tangents, and Secants, are found out in propor- tional Numbers; as of 2 Degr. 10 Degr. 20 Degr. 32 Min. &V. Thefe Tables are called mathema- tical Canons, and are of extraordinary ufe in all mathematical and phyfical Sciences-, wherefore I am willing to give fome Hints of thefe things to the young Geographer. But becaufe fpherical Triangles have fome Difficulty in their manage- ment, and regard none but thofe who defire to be deeper (killed in this Science, we mail pafs them by ; and only treat of right-angled Triangles, the meafuring of which is as eafy as neceflary. two THEOREMS. 14. THE three Angles of every Triangle^ taken together, are equal to two right Angles, or 180 Degr. and therefore the two acute Angles of a right angledi Triangle make exactly 90 Degr. (0). Alfo if a right Line touch a Circle, and there be drawn from the Point of Contatt another right Line to the Center, that Line makes a right Angle with the Tangent (/>). 15. THE mod neceflary Problems are thefe. I. THE Hypotenufe and one fide of a right angled Triangle being given, to find either of the acute Angles. Say by the Golden Rule , As the given Hypote- nufe is to the given fide: io is the Radius 100000 (which_ Number is aflumed equal to the Semidia- meter in the Tables J to the Sine of the oppofite Angle ^ which Sine being found in the Tables (o) Euclid. ?r 3 p. 3 z. Lib. \. (p) ibid. Prop. 18. Ub. iii. will CHAP. 2. ofUniverfal Geography. 23 will mew the Quantity of the Arch or Angle op- polite to the Side given ; and the other Angle is the complement of that now found, to 90 Degr. II. NE fide and the acute Angle next it being given, to find the Hypctenufe. Say as before i As the Sine of the Complement of the given Angle is to the Radius 1000000 : fo is the Side given to the Hypotenufe fought. III. HAVING two Sties given, to find either of the acute Angles. Say, As either of the Sides is to the other, fo is the Radius 100000 to the Tangent of the Angle adjacent to the Side firft aflumed. IV. HAVING the Hypotenufe and one acute Angle given, to find either of the Sides : Say ; As the Radius 100000 is to the Sine of the Angle op- pofite to the Side required : So is the given Hy- potenufe to that Side. Of Divers Meafures. BECAUSE theufe of Meafures is frequent in Geography, and fince divers Nations ufe dif- ferent Meafures, 'tis proper to premife fomewhat concerning them ; partly that the Reader may the better underftand the Writings of the antient Geo- graphers and Hiftorians , and partly that he may compare together thofe in ufe at this Day. THE Length of a Foot is almoft univerfally made ufe of, tho* a Foot in one Place differs from that in another. Mathematicians frequent- ly meafure by the Rhinland Foot of Snellius, which he proves to be equal to the old Roman Foot. And becaufe Snellius was very diligent and accu- rate in meafuring the Earth, that Rbinland Foot C 4 ot 24 fk Abfdute Part SECT.!. of his is defervedly taken as a Standard for all other Mcafures ($). See half it's Length, Fig. i. A P R C H or Pole ought to conlift of ten fuch Feet. But the Surveyers in Holland make 1 2 Feet a Rhinland Perch, and in Germany they com- pute 1 6 ; which is very incommodious in Calcula- tion. Sneliim makes the Holland Mile equal to 1500 RbitilandPerchts (each Perch being 12 Foot) or 1800 Rhinland Feet. THESE two Meafures, a Perch and a Mile arile from the repetition of a Foot , but a Palm an Inch) and a Barley-Corn (which are fometimes ufed in Holland] proceed from it's Divifion. An Inch is the twelfth Part of a Foot. A Palm is 4 Inches. A Barley-Corn is the fourth Part of an Inch. However it would be much better to divide the Foot into 10 Inches, and the Inch into jo Subdivifions or Seconds. &c. THESE are the Meafures now made ufe of by the Dutch in Geography. It remains that fome others be alfo taken Notice of ; viz. thofe of the Antients, whether Greeks, Romans, Perfiam, ;gyp- tiam ; and thofe alfo of later Times as of the Turks, Polanden, Germans, Mofcovites, Italians, Spaniards, French, and Englijb. (q) Becaufe the Knowledge Bernard's Treatife of Weights cfan Eng Hjh, Frereb, and Rbin- and Meafures, where he moft landijh Foot will be of ufe in learnedly confutes the great Er- what follows, we will here give ror ofStieHius in this Matter. their Proportions ; to which we If an Englijb Foot be divided fliall add the Meafure of the old into 1000 Parts, and a French fcoman Foot, taken from Dr Foot into 1440. Then 1309 THE C IT A P . 2 . of Univerfal Geography. 2 5 THE Grecian Stadium, or Furlong, is fuppofed to be 600 of their Feet, which make 625 Roman , or Rbinland, Feet , their Foot being a little larger than the Roman. A GERMAN Mile (15 of which Geogra- phers allow to a Degree) contains 22800 Rbuaand Feet, and is accounted 4000 Paces, or 32 Fur- longs. It is in Proportion to the Rbinland Mile, as 19 to 15. THE Italian or Roman Mile is i ooo Paces, which is equal to 4000 Rbinland Feet. Note, The Romans ufed to call their Mile Lapis, becaufe a Stone was creeled at the end of every Mile ; efpe- cially in Places adjacent to the City. ^GEOMETRICAL Prfttis exactly 5 Feet; and a Fathom 6 Feet ; which is thought by fome to have been the Pace of the Grecians. A C U BIT is fuppofed to be a Foot and a half. THE Parafange, or Perfian Mile, is thought to be 30 Furlongs, or 3000 Perfian Paces. THE Scbanus, or ^Egyptian, Mile, according to Herodotus, contains 60 Furlongs, tho* only 40 according to Pliny. Perhaps their Length diffe- red in divers Places, or the Furlongs of the Au- thors might be unequal : Or very likely their Books are corrupted. THE French League is in Proportion to the Rbinlandijh Mile, as 19 to 25 i and the Spanijh League is to the fame Mile, as 19 to 27! : But becaufe in feveral Parts of France and Spain their League is found to differ, we cannot be well allu- red of the Length of thefe Meafures. THE Engli/h Mile is in Proportion to the Rhinlandijh, as 19 to 55, or as 19 to 60, (r). But there (r) The leaft Part < Englijh and well dried ; whereof 3 in Meafure i a Barley-Corn, taken Length make and Inch, ts'e. as out of the middle of the Ear in the following Table. A TaM* 26 The Abfolute Part SECT.!. there are three forts of Englijh Miles, whereof 27 i of the longelt, 50 of the middle Kind, and 60 of the fhorteit, make a Degree or 19 Dutch Miles. THE Dw> and Swedijh Mile is to the Rbin- landifb Mile as 19 to 10 ; tho' in fome Places they life the German Mile. THE Pore/}, or Rujfian, Mile is as 19 to 80. THE Turkijh League or Mile is faid to be e- qual to the Italian Mile ; of which 60 make a Degree. THE Arabian League was formerly accounted the twenty fifth Part of a Degree, or 19 Holland Miles: but they now ufe another of which 56 make a Degree. AHUNDRED Indian Miles are thought to equal a Degree. Tho' the Indians cpmmonly de- fcribe Diftances by a Day, or an Hour's Journey. THE Inhabitants of Cambaya and Guzaraf, ufe a Meafure which they call Coffa 9 of which 30 make a Degree. THE Cbinefe obferve three Meafures in their Journies, which they call Li, Pu, and Uchan. Li is the Diftance at which a Man's loud Voice may be lieard on a Plain, in a calm Air ; which is accounted 300 Geometrical Paces. Their Pu contains 10 Li's ; fo A 'Table of Englifb Meafure. Bar. C. feh, Fftt ?W. ~ Pace 3 36 12 I OX 3 6 3 i He 60 6 Zlt 72 2 i-i 594 198 i6i 5^ 4-ro i i o! 40/ar/. 8hoj 320) fc A//7/I 23760 7920 660 220 132 i 80090 63360 ^28011760 1050 CHAP. 2. of Vnherfal Geography. 27 fo that 20 Pu's make a Degree. And 10 PH'S make an Ucban, or 30000 Paces ; which they account a day's Journey. Note, A Square Rh'mland Mile confifts of Square Feet and a Cubic Mile of Cubic Feet. Alfo a Mile multiplied into itfelf makes a Square Mile ; and that again by a Mile makes a Cubic Mile. The fame is to be underftood of a Square and Cubic Foot. SECT. II. Containing fome general and absolute Properties of the Earth, in jive Chapters. CHAP. III. Of the Figure of the Earth. TH E firft and nobleft Property of the Earth fas exceeding the reft in being more ufeful and neceffary) is it's Figure ; without the Knowledge of which there can be nothing well underftood or demonftrated in this Science ; and all the following Propofitions almoft entirely depend on, or imme- diately flow from, this; which for that Reafon ought to be firft treated of. THERE have been, and are to this Day, fe- veral Opinions about the Figure of the Earth ; for the Vulgar that underftand not Geography, imagine it to be extended into a vaft Plain bounded with a Circular Line ; except where Mountains and Val- lies interpofe. Of this ftrange Opinion was Laftan- tius and others of the Fathers, who ftrenuoufly ar- gued that the Earth was extended infinitely down- wards, 28 Tbe Abfolute Part SECT. II. wards, and eftablifhed upon feveral Foundations (a}. This they were inclined to think from fome Places of Scripture which they either ill underftood or wrong interpreted. Heraclitus, that antient Philo- fopher, is faid to have been of their Opinion : tho' others fay, he fuppofed the Earth to be in the Shape of a Skiff or Canoo, very much hollowed. But what is more ftrange Francis Patricius (a modern Philofopher of no fmall Repute in the laft Age; ftrenuoufly endeavoured to prove, that the Earth was horizontally ftretched out and plain under Foot. Anazimander is faid by Peucerus to have fuppofed the Earth like a Cylinder ; tho* that is not fo pro- bable, becaufe he tried to meafure it, and alfo in- vented a fort of a Dial at Laced.y.v\. that the true Figure of the 'Chap. 9. De Civil. Dei. They Earth, which Men have inha- thought their Opinion was fa- bited for fo many thoufand voured by the Pfalmijt. Pfal. Years, is but now begun to be xxiv. 2. and cxxxvi. 6. known a few Years ago. For (*) Among the many excel- that which all Men thought to lent and wonderful Inventions be globular and truly fpherical, ,. 1 modern Pil kpher5, is now found to imitate rather this here is not certainly in the an oval Figure, or that of an laft Place, nor hath the lealt Eiiipfis revolved about it's letter Axis C H A P . 3 . of Umverfal Geography. Axis: So that thofe Diameters are longeft which come nearelt the Equator, and leffen as they become more remote, but the lealt Diameter of all is the Axis which joineth the two Poles. The Thing will perhaps be bet- ter underitood if it be reprefea- ted by a Figure. Ltttepqp (Fig. \.) be a cir- cular Section of the Earth made by the Meridian, fuch as it was thought to be formerly and p p the Axis or Dumeter joining the Poles, and a q the Diameter of the Equator : then the oval Line & P QJ>, delcribed upon the Diameter JE Q^and P P, will reprefent the Seftion or true Meridian Line, which for Diilindlion fake is made here to differ more from a Circle than it really ought to do ; but in truth, the Proportion is as 692 to 689. So that the Line C Q^ meafuring the Altitude of the Earth at the Equator, exceeds CP the Altitude at the Pole 85200 Parii Feet, or about 17 Miles. This Affair is well worthy to be traced to it's Original, and to be backed by a Demonttration, fo far asour Purpofe will permit. See the Hiflory of the Royal A- lademy of Sciences by du Hamel. Pag. I I o, i 56, 206, Alfo Hijl. de FAcad. Ruy. 1700, 1701. The Fremh made an Experi- ment about forty Years ago, IhewingthataPendulum (which is a well known Inltrument for meafuring of Timej vibrates fo much the flower, by how much the nearer it is brought to the Equator : that is, the Gravity, of Celerity of Defcent of the Pendulum, and of all other Bo- 29 dies, is lefs in Countries ap- proaching the Equator than in Places near either Pole. The two famous Philofophers New- ten and Huygens being excited by the Novelty of the Thing, and fcarching more narrowly in- to the Caufe of it, found thereby that the Earth muft have fome other Figure than what was known ; and alfo demonflrated that this Diminution of Weight doth naturally arife from the Rotation of the Earth round it's Axis ; which Rotation, accord- ing to the Laws of circular Mo- tion, repels all heavy Bodies from the Axis of Motion : fo that this Motion being fwifter under the Equator than in Parts more remote, the Weight of Bodies mull alfo be much lefs there than nearer the Poles. Therefore the Parts of the O- cean under the Equator being made lighter, and according to the Nature of all Fluids, preffed and forced on either fide by the Waters nearer the Poles, they muft be raifed up to a greater Height, that fothey may better fupport and balance the greater Weight of the contiguous Wa- ters. Which mutual Libration is demonitrated upon Suppofi- tion of that Inequality of the Diameters which we mentioned above. The Figure of the Sea being refembled by the Lands adjacent, which are every where raifed above the Sea, the afore- faid Form muft be attributed to the whole terraqueous Globe. They that would be more fully informed in this Matter may confult Newton's PrincipiaLib. iii. Prop. 19. or Huvgen' 1 * Trea- tife of the Caufe of Gravity. The 3 The Abfolute Part S E c T. IL THE Arguments indeed which Authors offer to confirm the Truth of this, are handled fo obfcure- Iy and confafedly, that they are almoft inefficient to convince the fhenuous and obftinate Defenders of the contrary Opinion. We fhall therefore as much as is poflible, clear up and examine thefe Argu- ments ; that the Reader may have a diftind Know- ledge of them, and know the better how to ufe them. WE mall not here take notice of fuch Reafons as are of lefs Weight, and at beft only probable, or perhaps fophiftical. Such as, i. A fpherical Fi- gure is the moft capacious , and therefore the Earth ought to have fuch a Figure. i. All the Parts of the Earth tend to the fame Center ; therefore all thefe The fame Inequality of Dia- meter is alfo found in the Pla- net Jupiter, by the Obfervations of thofe Excellent Aftronomers CaJJini and Flam/lead, and that much more than in our Earth ; becaufe the diurnal Rotation of that Planet is more than twice as fwift as the Rotation of the Earth : which plainly proves, that the Difference arifes from no other Caufe than the circu- lar Motion. Juritfs Appendix, Dr Derbam fin his Pbyfico- Tbeof. B ii. C i . Note a) doth not feem to entertain any doubts concerning the terraqueous Globe, and the other Planets, being of a prolate fpheroidal Fi- gure ; but he faith, That altho' he hath often viewed Jupiter ; and other Planets, with very good Glafles, which he hath of 72 feet, and the Royal Society's Glafe of above i zo feet, yet he never could perceive them to be otherwife than perfectly globu- lar. And he thinks it next to impoffible, to take an exaft mea- f ure of the Polar and ^Equatoreal Diameters, by reafon of the Smallnefs of their apparent Dia- meters in a Micrometer, and theirMotion all the time of mea- furing them. And as to the Variation of the Vibrations of Pendulums, under the Line, and in the Northern and Southern Latitudes, he hath no doubt, but different Diftances from the Earth's Center, may caufe different Vibrations ; but yet he (hews, from good Expe- riments he made with Pendu- lums in the Air-Pump, that thofe Alterations might, in fome meafure, be from the Rarity and Denfity of the Air, in the different Zones. And I may add to Dr Derbams Experiments, the Lengthening of Iron Rod* by Heat, and their Shortening by Cold; which I have found to be very confiderable, by ve- ry exadt Experiments. Parts C H A P . 3 . of Univerfal Geography. 3 1 Parts ought to make up a globular Figure. 3 .When at the firft Creation the Waters were confufedly mixed with the Earth, it was then without doubt moift and foft , but the Figure of all moift and li- quid Bodies is fpherical : and fo ought the Earth to remain after the feparation of the moift Parts from the dry. I SAY, neglecling thefe and fuch like Argu- ments, let us look out for better , which are of three kinds. Of the firfl there is only one deduced a priori, as they call it : thofe of the other two kinds are de- monftrated a pofleriori ; or from Celeftial or Ter- reftrial Obfervations and Appearances. THE firft Argument is taken from the Nature of Water, and borrowed either from Ariftotle or Archi- medes. Arijiotle in his fecond Book de Ccelo^ chap. 5th, propofes it as his own, after this manner, (tho j it is likely he borrowed it from fome Philofopher before him). If we take it for granted (fays he) that Wa- ter of it's own Nature tends always down to the moft concave or loweft Place ; it will neceflarily follow, that the Superficies of the Water is round or fpherical ; but that Place is moft concave that is neareft the Center of the Earth, therefore let there be drawn from the Center a. two right Lines * and a-y i and from to y the Line y ; to which from * let fall the Perpendicular *s. (c) It is plain the Line <*^ (Fig. 5.) is lefs than */3or *y, and there- fore the Place , and T are equal, that is, 'till *fK- 3 9 10 2822 28149 28061 ' Miles Per cb ; 1 8 1223"" i 8 i i 49 i 8 1067 Miles M.n. 14 51 1448 14 46 Mites Mm. ~ 9 ~*T~ 59 16 ?9 6 ii 12 '3 '4 15 27976 27877 27769 27653 27526 1 8 976 18 877 8 769 .8 65? 1 8 529 H 43 14 40 M 37 H 33 14 20 58 55 58 42 58 29 5814 57 58 16 7 18 ; 19 20 27396 27255 27105 26947 26781 18 396 .8 255 18 105 7 H47 17 1281 14 25 1421 14 16 - 14 ii 14 6 57 42 57 24 57 4 56 44 56 24 21 22 23 24 25 26607 26425 26234 26036 __2$g3o , 17 1107 17 925 '7 734 17 536 17 130 14 o 3 54 13 48 13 42 13 36 56 o 55 3 6 55 12 54 48 54 24 26 3 29 JO 3 32 33 34 3? 25616 2 5394 25164 24927 ^2468 1 24429 24169 23902 23628 23346 17 1 16 16 1394 i 6 i i 64 16 927 16 681 '6 4*5"" 16 169 15 1402 15 1128 - 15 846 3 29 I 3 22 5 5 - !J 7. 'T 59 12 5I 12 43 9 I2-35L 12 26 12 17 54 53 28 53 o 52 28 _lj^ 96 51 24 50 52 50 20 49 44 49 8 30 g 39 40 4i 42 43 44 4j 23057 22761 22458 22149 21832 21509 21180 20843 20501 201 s Z 5 557 15 261 14 1458 14 1149 14 832 14 509 14 1 80 3 1343 13 1001 13 6^2 12 8 11 59- ii 49 '' 39 ii 29 ii Tg"" ' 9 10 58 10 47 10 36 48 32 47 S.6 47 1 6 46 39 46 o - 4-5 16 44 36 43 S 2 43 8 : 4.2 24 40 47 48 19798 19437 19070 13 298 13 o 12 1070 10 25 10 14 10 2 41 40 ; 41 o 4o 8 C H A P. 4. of Univerfal Geography. Lati- tude- Perches in T Dfgr. Holland Miles German Miles Italian Miles De%. Mi let Perch- VLilet Mm Miles Min 49 18698 18319 12 698 12 ^IQ 9 5 9 38 39 20 38 32 5 1 5 2 53 54 55 17936 17546 17152 .1.675 2 16347 II 1436 II "1046 I I 652 11 252 10 1347 9 20 9 H 9 * 8 49 8 36 37 44 37 36 8 35 26 34 2 4 56 ; 57_ '5937 .15522 14679 14250 i.o 937 id 522 10 id3 ; 9 H79 9 750 K? 7 57 7 44 7 30 33 3 2 32 40 31 48 31 o 30 o 61 62 63 64 65 13817 13380 12939 12494 12045 9 3'7 8 1380 8 939 8 494 8 45 7 16 6 48 634 6 20 29 4 28 8 27-12 26 16 25 20 66 68 69 70 11592 11136 10676 10213 9748 7 1092 7 6 39 7 *7" 6 1213 6 748 6 6 5 5 2 5 38 S3 24 24 23 28 22 32 21 32 20 32 7' 73 74 7s 9279 8807 8 333 7846 7376 6 279 5 '37 5 933 5 346 4 i 376 4 53 4 38 4 23 4 * 3 53. 19 32 l8 32 17 3* 16 32 76 77 78 79 80 6*95 6411 5925 5438 4949 4 895 r//4< 4" 3 1425 3 938 3 449. 3 3^ 3 23 3 8 2 52 2.36 14 32 13 32 12 32 II 23 io 24 81 82 83 84 85 3*966 3473 2 979 2484 2 1458 2 966 * 473 i 1479 i 984 2 20 2 5 I 50 34 r 18 9 20 8 20 7 to 6 12 /O CO 00 00 OC 1 O NO 00>J O> 1988 1492 995 497 i 488 o 1492 o 991 o 498 1 3 o 47 o 31 o 10 o b 4 12 3 12 2 4 4 o o The Abfolute Part SECT. II. CHAP. V. Of the Motion of the Earth. TH E Pythagorean Motion or Circumvolution of the Earth (not a Nutation or Quaking) is according to the Copernicans the Caufe of moft of the Changes in the Celeftial Appearances, which would otherwife be conftantly the fame in every Place (a). Tho' indeed there is not any Property of (a) This Syftem was not in- vented by Pythagoras, as fome imagine, for Diogenes LaPrtius exprefsly faith, that Pythago- ras'* Opinion was, That the World was round, containing the Earth in the middle of it ; and that Philolaus, the Pythago- rean, was the firft that faid the Earth moved in a Circle : But fome fay Hercetas the Syracu- fian* Derham's Aftro-Theology* Pythagoras, who Jived in So- ciety with the Egyptian Priefls feven Years, and was initiated into their Religion, carried home from thence, befides fe- veral Geometrical Inventions, the true Syftem of the Uni- verfe, and was the firft that taught in Greece, that the Earth and Planets turned round the Sun, which was immovea- ble in the Center; and that the Diurnal Motion of the Sun and fixed Surs, was not real but ap- parent, arifing from the Mo- tion of the Earth round it's Axis. The next Perfon who made a confiderable Figure this way, was Ptolemy with his Cycles, Epicycles, and Eccentrics, he quite burthened Nature, and his Hypothefis mews too much of Art ; thefe are all now explo- ded, and his folid Spheres broke to pieces; he left behind him a Work entitled Almageft, or the great Conftrudion, which v?as founded on tke Obfervations of Hipparchus. Copernicus had the Honour to reftore' the ancient Pytha- gorean Syftem, notwithftandihg the Prepofleffion the Ptolemaic had gained in the World. To thefe fucceeded the No- ble Dane, fycbo Brahe, whofe Hypothefis in a great Meafure is compounded of the other two, and feems dcfigned to account CHAP. 5. of Unfoerfal Geography* 6$ of the Earth fo much difputed againft and cavil- led at as this ; fo as even not long ago to have undergone the Cenfure of the Romijh Church. However, becaufe it feems very probable to many that there is fuch a Motion, we mall endeavour to explain it. I T is known to all, even the Vulgar, that the Sun, Moon, and Stars, appear to move from Eaft to Weft, and to return to almoft the fame Places again in the Heavens, in the Space of twenty four .Hours. So that either they muft really move, or we our felves be moved ; and attribute our Motion to them. For it is a felf-evident Prin- ciple, that if two Things change their [Diftance from one another, one of them, at leaft, muft have moved. T H A T the Earth is fixed, or at Reft, and the Stars with the Heavens in Motion, was a common Opinion ; and is fo ftill among thofe that are ac- counted Ptolemaic Aftronomers : But the Pythago- reans of old maintained, that the Stars conftantly kept their Places ; and that the Earth was revol- ved about it*s Center. Of which Seel: was the celebrated Ariftarcbus of Samos ; who, for defend- ing this Opinion, was by his Enemy and Adver^ fary accufed, before the Bench of the Areopagites^ of having violated the Laws of Religion ; but was fortunately abfolved by them *. Afterwards, but very for the difficulties of both of the Celeftial Bodies obferve in them, and fo is liable to feveral their Motion, and laid the Objections in them both. He Ground -work of the Modern was very skillful in obferving, Philofophy. Thus I have given a and in the Furniture of his Ob- fhort Sketch of the Rife and fcrvatory exceeded even Prin- Perfe&ion of this Science, ces and Kings. * The Great Galilao, the John Kepler, the laft I mall Modern Affertor of the fame mention, by the help of Tycbo's DoStrine, met with the fare of Labours, found ouc the "Laws the ancient &wz/rfPlulofopher; VOL. J. F He 66 fbe Abfolute Part SECT. II. very few affented to this Opinion ; fo that it lay hid, or, as it were, buried in Oblivion for many Ages ; infomuch that we find not the leaft men- tion of it in the Schools, till the famous Aftrono- mer Copernicus , about 200 Years ago, brought it again into Estimation, and backed it with feveral Arguments, fo that many excellent Aftronomers af- ter him embraced it ; among whom flourifhed not long fmce the great Kepler , Profeffor of Mathema- tics to the Emperor ; and Galllceo an Italian, Ma- thematician to the great Duke of Tufcany ; as alfo Lanfberg a Dutchman. AND whereas we obferve two apparent Mo- tions in the Heavenly Bodies (one by which all the Stars both fixed and wandering feem to be car- ried about the Earth, and to rife to the Meridian, and fet under the Horizon nearly in the fame or equal Times: The other, which is called their Annual Motion ; by which the Planets with dif- ferent Motions, and the fixed Stars with equal Ve- locity, are carried the contrary Way from Weft to Eaft) the Ptokmaics affirm both thefe Motions to be in the Stars themfelves, or in their Orbs ; But the Copernicans attribute this firft apparent Mo- tion to that real one of the Earth, not in being transferred from one Place to another, but to it's Rotation about it's Axis from Weft to Eaft, while it continues ftill in it's own Place (which caufeth the apparent Motion of all the Stars the contraiy way). And they alfo free the Sun and the fixed Stars from the afore&id annual Motion, by attri- He was brought before the proper Center. The poor Man Inquifition, snd obliged folemn- was forced to fay, that he did, ly to abjure his Aflronomical with a fincere Heart, and Faith Tenets, that the Sun flood im- unfeigned, abjure, curfe, and movable in the Midft of the deteft, the afore&id Errors and Univerfe, and that the Earth Herefies. moved round it, as about ift bating C H A P. 5. of Unfoerfal Geography. 67 buting the apparent Motion of thefe to the real an- nual Motion of the Earth round the Sun ; and to the Inclination of it's Axis: Notwithftanding they aflign this faid annual Motion to the reft of the Planets ; only they deny the Sun to be a Planet, and advance him to the Center of the Syftem, where Ptolemy had placed the Earth ; and make the reft of the Plantts, Saturn, Jupiter, Mars, the Earth, Venus, and Mercury, revolve round him. THE Reafons for the Copernican H-jpothefis are thefe. 1. T H E Motion df the Earth round it's Axis, continuing in the fame Place, will beft account for the Appearance of fuch a vaft Number of Stars which feem to perform their Revolutions round the Earth in 24 Hours ; and therefore this Mo- tion is moil agreeable to Reafon : As it happens with us when we lit in a Ship^ failing towards o- thers at Reft in the Harbour ; tho 5 they feem to approach and come nearer us, yet we do not affign that to any Motion in them. And as Nature ne- ver performs that by many means which may be done by a few 5 it is very likely the fame Rule is obferved here. 2. THE Motion of the Stars Would thus be incredibly fwift and beyond all Imagination ; be- caufe their Biftance, in Reipect of us, is almoft infi- nite, and the Orbit they have to run round fo prodigioufly great, that they muft move at leaft i ooooo Miles in a Minute: On the other hand, if this Motion be affigned to the Earth, we need not introduce a progrejfive Celerity ; for tho' fhe re- mains ftill in the fame part of Space, me folves the Phaenomena by revolving about her Axis. 3. THIS Argument is the ftronger if we com- pare the vaft Bulk of the Celeftial Bodies with the Bulk of the Earth. For as the Sun is at leaft 200 F 2 times 68 The Abfolute Part SECT. II. times bigger than the Earth, and feme of the fixed Stars 1000 times; it is much more probable, that the Earth revolves round it's Axis with an eary natural Motion, than that fuch vaft Bodies mould move from one Place to another with incredible Swiftnefs. 4. THE moft celebrated Aftronomers are, with Vycbo 9 forced, by the Phenomena, to deny that there are folid Orbs, fuch as the Ancients made ufe of the better to explain their imaginary Motion of the Stars ; hence their Arguments for this diurnal Rotation about the Earth, are lefs co- gent. The Reafon why they are forced to deny this, is, becaufe that one Planet is often feen with- in the Orb of another ; which muft caufe a mutual Penetration. 5. NO Reafbn can be given why the Stars Jhould move round the Earth : But, on the other hand, it is moft agreeable to Reafon, that the- Earth, and the reft of the Planets, Jhould move about the Sun. 6. NEITHER the Pole nor the Am about which the Stars are fuppofed to revolve, is real : On the contrary, there is a known Pole and Axis in die Earth. 7. FOR this Reafon alfo Navigation is much eafier from Weft to Eaft than the contrary Way. For they can fail from Europe to India in about four Months ; but can fcarce return in fix Months : becaufe in their going they move to the fame Point with the Earth ; but in their returning they fleer contrary to the Earth's Motion. 8. BECAUSE the Cekftial Phenomena, fuch as the rifmg and fetting of the Stars, the Inequali- ty of Days, &c. cannot be accounted for, by any other Motion than that of the Earth. And the Commodioufnefs and Neceflity of this Hypothefis, is more particularly perceived in the wonderful Ap- pearances C H A P. 5. of Unfoerfal Geography. 69 pearances of the Planets ; for explaining of which the Ptolemaics are forced to fuppofe feveral unnecef- fary interfering Circles, Epicycles, and Eccentrics, without any Reafon : Whereas the Copernicans can naturally account for them all, (without any pre- vious Suppofitions,) by the annual Motion of the Earth, or it's Revolution round the Sun, viz. i. Why the Planets feem fometimes retrograde; and why Saturn is oftener and continues longer fo than Jupiter ; and Jupiter oftener and longer fo than Mars, &c. and alfo why they are carried fometimes with a fwifter Motion, and at other times appear ftationary. 2. Why Mercury and Venus can never be feen a whole Night together. 3. Why Venus is never carried 'further from the Sun than 48 degr. and Mercury never more than 28 ; and fo can never be feen in Oppofition to the Sun. 4. Why Venus may be feen in the Evening after the Sun is fet ; and the next day in the Morn- ing before the Sun rifes, &V . I FORBEAR to mention any more Phse- nomena, (thefe being the principal from whence a folid Argument may be drawn for the Motion of the Earth^ fince they are all eafily and naturally accounted for upon this Hypothecs ; fo that it would be ftrange if the Earth mould not move, when fuch evident Appearances require fuch a Mo- tion. And tho* thefe Arguments are not demon- ftrative, yet they render this Hypothefis prefera- ble to the other, which fuppoieth the Motion of the Heavens. And we mult admit of the one or the other. BUT the Arguments which fome alledge to the contrary are eafily anfwered ; fuch as, j . The Earth is not fit for Motion, becaufe of it's Gravi- ty. 2. The Parts of the Earth naturally tend in a right Line to the Center ; and therefore a circu- lar Motion is againft Nature. 3. If the Earth F 3 wer Abfolutt Part SECT. II. were moved, a Stone dropped from the Top of a Tower would not fall juft at the Foot of it. 4. A Ball fhot from a Cannon Eaftward at a Mark, could not come home to it, if the Mark with the whole Earth did at the fame Time move towards the Eaft : or at Jeaft would hit the Mark fooner when mot towards the Weft, Alfo a Bird flying towards the Eaft would be retarded : but forward- ed in flying the contrary Way. 5. Towers and Buildings could not ftand upright, but would fall : and Men, by the quick Rotation, would become giddy. 6. Becaufe (fay theyj the Stars are obfer- ved to change their Places, but not the Earth f 7. Becaufe the Earth is in the Center of the World ; tut die Center of any Thing is not moved. 8. Be- caufe the holy Scriptures confirm the Stability of the Earth, T O all which the Copermcam anfwer thus. To the firft^ that the whole Earth, taken together, is not abfolutely heavy. For Gravity confifts in the Tendency of the homogeneous Parts to the whole j and tho' this kind of Gravity be found in the Sun and Moon, they are neverthelefs not accountetf weighty. T O the fecond they anfwer, that the circular Motion of the whole does in no wife hinder the relative Motion of the Parts, which are moved in in a direft Line towards the Center ; as appears by the Parts of the Sun and Moon. T O the tbird they anfwer three ways, i . That heavy Bodies are not carried directly towards the Center of the Earth, but in the fhorteft Lines po fible to it's Superficies ; which are thofe parallel to the Tower , as Iron does not tend to the Center of the Loadftone, but to the Loadftone it felf. 2. The whole Atmofphere adheres to the Earth, and is moved along with it : therefore when Bo- dies a.re thus let fall, they partake ojf this circular Motion, C H A P. 5. of Unherfal Geography. 7 1 Motion, and are carried downwards as it were in a Veflel. B- Gaffendus, by repeated Experiments, found, that if a Body be projected from another Body in Motion, it will partake of the Motion of that other Body ; as a Stone dropped from the Top of a Maft, while the Ship is in a very fwift Motion, is not left by the Ship but falls at the Foot of the Maft. Alfo a Ball (hot perpendicu- larly from the Foot of the Maft falls in the very fame Place. Therefore the Objection is of no Force. T O the fourth they anfwer as to the third. THE fifth Objection hath no Place, becaufe the Motion of the Earth is even and uniform, with- out darning or ftriking againft any other Body 5 and the Buildings being heavy Bodies, and homo- geneous to the Earth, are moved as if they were in a Ship ; which tho* it fails either fwiftly or (low- ly, yet if the Motion be even and fteady without Waves and on fmooth Water, Bodies fet upright will not be overturned, nor a Glafs of Wine be fpilt. T O the ftxth we anfwer, that we are not fen- fible of any Change of Place in the Stars, only of their Situation in Refpect of our felves ; which may appear and really be, whether we with the Earth, or the Stars themfelves are moved ; or even tho' both we and the Stars fhould be in Mo- tion (b). I N (b] Molt of thefe Objeftions the Top T, in the fame Time are anfwered by the Laws of that the Ship moves from M Mechanics, thus: Let W, E be to D. From the Conjunction the Line of Motion of a Ship of thefe two Forces (M T the from Wto E, reprefenting the Projection, and MD the Ship's Motion of the Earth from Weft Motion) it is manifeft, by the to Eaft. Let MT (in Fig. 9) known Laws of Motion, that be a Maft, from the Foot of the Body will not be carried which, M, fuppofe a Body to perpendicularly to the place be thrown perpendicularly to T, but in the Diagonal Lin F 4 MB, 72 fbe Abfolute Part SECT. II. IN diefeventh Objedion both the Aflertions are falfe j or at leaft doubtful. TO M B, fo as to accompany the Malt in it's Motion from M T to BD. Then fuppofe the Body to fall from the topoftheMaft B to the foot D, in the fame Time the Ship moves from D to G ; and it is plain, that, by the mutual aftingofBD, the centripetal Force, and BF=DG, the Ship's Motion, the Body will fall in the diagonal Line B G, and alfo accompany the Maft in it's Motion from D to G; fo that tho' it was really carried in the Lines MB, BG, yet it will feem to have moved, only upwards and downwards, paral- lel to the Line FG. Alfo (in Kg. 10.) let M T be the fame Maft, and fuppofe a Projeftile to be caft eaft- ward from the Stern S, to the top of the Maft T, in the Time the Ship moves alfo eaftward from M to D ; then will it's Motion upwards defcribe the Diagonal S B; where let it be obftrucled fo as to feem to fall perpendicularly to D, in the Time the Ship moves from D to G ; then, as before, it will defcribe the Diagonal B G, tho' it feemedto move upwards only in the Line TS, and down wards inFG So (in Fig. II.) if a Body be projected weft ward from the Head of the Ship H to the top of the MaftT, in the Time it moves eaftward, H G equal to the Diftance M H, then will it's Motion upwards defcribe the perpendicular Line H B. And if in the fame rime it feems to defcend from B to H that the Maft moves H G=s G =M H, it's Motion down- wards will defcribe the Diago- nal B G. So that, in this Cafe, it afcends by a perpendicular Line, and falls by an inclining Line; tho' itfeemed to afcend by the inclined Line b F, and to fall by the perpendicular Line F G. Hence it is plain that Bodies may appear to have a Motion, direftly contrary to their real and abfolute Motion : fo that it is pleafant to conceive, how falfly we may judge of the Mo- tion of Bodies by their unequal Diftance from us; not confider- ing that we may be infenfibly moved from them. Hence alfo is deduced that ingenious Experiment of Gali- lua x. 12, 13. the Sun is or- dered to ft and flill upon mount Gibeon, and the Moon in the valley of Ajalon. But it would be very abfurd to take this in a flrift literal Senfe, and imagine thofe two great Luminaries were confined to thofe two Pla- ces, otherwife than in Appea- lance to the victorious jrae- lites. And if fo confiderable a Part . of the Tranfaftion be fpoken according to it's Ap- pearance, why may not the whole ? Why might not this Station as well be an Arreft of the Earth's Motion, as that of the Heavens ? If the whole Miracle was not (as fome not improbably think) effe&ed by Means of fome preternatural Refractions, or extraordinary Meteors, &c. And fo for the Recefs of the Sun, or it's Sha- dow in Hezekiab's Cife(z Kings xx. 10. and Ifai. xxxviii. 8.) which in appearance feemed to be the Sun, is, by divers learned Men, thought to have been the Effeft of fuch like extraordi- nary Refraftions or Meteors, as mentioned in the laft Cafe: Or if it was a real Regrefs, why not of the Earth rather than the Sun and whole Heavens? See Derham's Ajiro-Tbeol. Be- fides, Hiftoriographers feldora confine themfelves to a Geo- metrical or Aftronomical nicety in their Defcriptions of Things. As, in i Kings vii. 23. it is written, that Solomon made a malttn fea t ten (ubits from oni C H AP. 5, cfUnherfal Geography. 7$ More Places might be quoted, but thefe are fuffi- cient 5 for the holy Scriptures were not given us to philofophize by, but to increafe our Piety. 2. Some Places of Scripture are alfo produced, which do not fpeak of the Mobility of the Earth, but of it's Stability and Permanency ; as that in Job aforefaid (g), THUS we have declared in brief what that Motion is, which the Copernicam afifign to the Earth ; the more full and accurate Explication of which belongs to dftronomy. And this Motion being fuppofed, all the Phenomena we obferve in a jGlobe revolved about it's Axis, mull be applied to the Earth, viz. That the Axis upon which it is turned, is one of the Diameters : That the Poles are two immoveable Points in the Extremities of the Axis : That the great Circle, or Perimeter, in which the Rotation is made, is the Equator with jt's Parallels, &c. L E T us now confider the Velocity of the Earth's Motion ; which, in that about it's Axis, is not over all the Earth equal, but different according to the Pittance from the Equator ; being there trim to the other, round all hended to be 25031,4 Miles, flbout, and a line of thirty tu- which, divided into 24 Hours, bits did compafs it round about, makes the Revolution to be But as 7 : 22 :: 10 : 31^- Cu- at the Rate of about 1043 bits is very near the true Length Miles in an Hour ; a Rotation of the Line that ought to en- that would as eafily throw off compafs a round Veffel of ten the Parts of the Earth, efpe- Cubits Diameter. dally the Waters, as the whirl- (g) Such as Pfal. xciii. I. ing round of a Wheel, or a cxix. 90. civ. 5. Ectlef. i. 4. Globe, would the loofe Duft and \ Cbron. xvi. 30. which and Water thereon ; but by Texts are all underftood by Reafon the Gravitating Power learned Commentators to mean exceeds the Centrifugal, as the unalterable Condition, Se- 2174 exceeds 7,54,064, that curity, Peace, and Tranquility, is, above 288 times ; there- of the Earth. fore all Parts lie quiet and ie- The Ambit of the Earth, cure in their refpeaive Place*. \>y the moft accurate, jsappre- fterbanfs ^ftro-'Tbcol p. 149. fwifteft 76 The Abfolute Part SECT. II. fwifteft as paffing thro* a greater Space, and fo by Degrees flower towards the Poles, as paffing thro* a lefs Space in the fame Time. Therefore fmce every Part of the Earth is moved thro' the Space of it's Periphery (or 360 Degr.) in 24 Hours ; the Space of one Hour's Motion is found by dividing 360 by 24, which gives in the Quo- tient 15 Degr. and fo much doth any Place on the Earth move (whether in the Equator or without it) in an Hour. Alfo 15 Degr. in the Equator make 125 German Miles, therefore it revolves 15 fuch Miles Cor one Degr J in 4 nan. and in one mm. 3^ Miles. BUT Places without the Equator, lying to- wards either Pole, are in the fame Time revolved the fame Number of Degrees : but thefe Degrees are much lefs than thofe in the Equator ; fo that the Celerity of Motion, or Progrefiion, is as the Sines of the Arches by which thefe Places are diftant from the Pole. Example. The Diftance from the Equator (or Elevation of the Pole) of Amsterdam is 52 degr. 23 mm. therefore the Di- ftance from the Pole (or Complement of Latitude,) is 37 degr. 37 mm. whofe Sine is 61037. Suppofe another Place, under the Equinoctial, diftant from the Pole 90 Degr. whofe Sine alfo is 100000, but the Place under the Equinoctial moves 15 Miles in 4 mm. and 225 an Hour. Therefore by the Golden Rule, as 100000 : 61037 : : 15 : 9 Miles, or fo is 225 to 137 Miles. So that Amsterdam is carried every Hour 137 Miles, and in 4 min. 9 Miles, by this Motion. THIS is more eafily found by the foregoing Table , for by dividing 360 by 24 we find each Place to more 15 Degr. of it's own Circle in an Hour, and therefore i Degr. in 4 min. &V. con- fulting the Table with the Latitude of the Place, we find how many Miles it moves in 4 min. For Ex ample $ CHAP. 5. tfUniverfal Geography. 77 Example ; The Latitude of Stockholm is about 60 Degr. oppofite to which in the Table is 71 Miles. Therefore Stockholm revolves fo many Miles in 4 win. and fuch is the firft Motion in divers Places. THE Second Motion of the Earth, is it's Change of Place ; whereby every Part of it moves the fame Space with the fame Velocity. This Motion is determined by the Diftance of the Earth from the Sun, or the Semidiameter of the Orbit in which it performs it's annual Revolution, moving in a Day about a Degr. and in an Hour 2! mm. A S to the third Motion of the Earth, becaufe it is more difficult to conceive, we mall leave it to Aftronomers, who have found it necefiary to be fuppofed. Origanus moves a Doubt about the fecond Motion ; and fuppofes the Earth to be on- ly moved by the firft, but the Sun and fixed Stars by the fecond: Tho' the above-cited Appearan- ces, in the Motions of the Planets, fuificiently confirm this Annual Motion (&). (b) This imaginary third and the Rfgrefs of the Nodes ; Motion of the Earth they were from which Thing never the left ebliged to fuppofe, to account no Variation of Declination,prt~ for the difputed Inequality of ferfy fo called, can arife. Wbi- the Declination of the Ecliptic, ftoitt Aftron. Left. pag. 57. which is now by moft Aftro- That there is fuch a Nutation nomers thought to be always whereby the Axis of the Earth the fame ; feeing there is no- doth twice incline towards the thing which Jhould diflurb the Ecliptic, and twice return to- ferpetual ParalleUfm of the it's former Pofition, fee in artb, on which this Equality Newton's Prin. Phil, Nat. Soti depends, except it Jhould be the iii. Prop, 21. igfenfible Nutatien of tbt Axis t CHAF, 73 the Atylute Part SECT. IL CHAP, VI, Of the Situation, or Place, of the Earth, in Re* fpetf of the Planets andjixed Stars. TH E Situation of the Earth, in the Syftem of the World, in refped to the reft of the Pla- nets, hath fome Relation to the Account we gave of the Earth's Motion, in the preceeding Chap- ter. For it is the general Opinion of the Ptolemaic Aftronomers and Philofophers, that the Earth, being the Center of the World, is placed in the middle of the Stars and Planets (a] : But the Co* pernicans, with the antient Pythagoreans, place the Sun in the Center of all the Stars, and make the Earth a Planet performing an annual Revolution about him, between Mars and Venus ; as is beft underftood by a Diagram of the Syftem. Never- thelefs they both agree in this, that the Earth may be accounted the apparent Center of the diurnal Motion, by which the Stars feem to be carried a- bout in twenty four Hours. For both Aftronomy and Geography require this Suppofition ; ib that whether we adhere to the Ptolemaic or Copernican Hypothecs, we do not detract from the Certainty of general Aftronomy or Geography. Becaufe the Difference of thefe Opinions conflfts only in this -, that the Ptolemaici will have this Motion to (a] Since the World, orUni- by the World here is only our vcrfe, is infinite, the central Solar Syftem, in which Senfe PJace of it cannot be determi- he inuft be taken in what fol- fced: What our Author means low*. be C H A P. 6. of Unherfal Geography. 79 be in the Stars themfelves, but the Pythagoreans in the Earth ; the Stars in the mean time retting : neither of which need be determined in Geography or common Aflronomy. A C C O R D I N G to the Ptolemaics the Situa- tion of the Earth, in refpect of the Planets and fixed Stars, is this ; The Earth in the Center , then the Moon, Mercury, Venus, The Sun, Mars, Ju- piter, Saturn, and the Fixed Stars. ACCORDING to the Copernicans ; The Sun is placed in the Center of the Syftem, as the Heart and Focus of the World ; and next him is the Orbit of Mercury, then that of Venus, the Earth, with the Moon, Mars, Jupiter, Saturn, and the Fixed Stars. I F it be required how far diftant we are from each of the Planets, we muft know that the Di- fiance is not always the fame, but continually chang- ing ; and therefore Aftronomers reckon three De- grees of Diftance, viz. the leaft, greateft, and mean or middle Diftance -, which laft of the Earth, from the reft of the Planets, is as follows, accor* ding to moft Aftronomers (). 1 The Earth is diftant from ' The Moon Co ' Mercury no ^of it's Semi. > diameters. T I'he Sun 1150 Man about 5000 Jupiter about 1 1 ooo b Saturn about- 1 8000 _ NEVERTHELESS the Diftance of the Earth from Mars, Jupiter, Saturn, and the fixed (V) Se$ Note (m) at the cad of this Chapter. 2 Stars 8o ' the Abfolute Part SECT. II. Stars, is not fo perfectly determined, for want of -Certainty in their Parallaxes. Alfo in the Coperni- can Syftem the Diftance varieth, not only from the Motion of the Planets ; but alfo from the Mo- tion of the Earth itfelf. THE Reafon for either Opinion, (viz. of the Ptolemaic and Copernican] about the Situation of the Earth, are much the fame with thofe we dif- cufled in the preceeding Chapter about the Earth's Motion. For this Difpute is of great Affinity with the former. Becaufe, if the Sun hath an an- nual Motion, then the Earth and not the Sun pof- fefifes the middle Place : But if the Earth fo move, the Sun and not the Earth will certainly be in the Center. THE following Arguments favour the Coper- mcan Hypothecs. 1 . T H E Sun is not only the glorious Fountain of Light, which like a clear mining Torch, illu- minates the Earthy Moon, Venus , and, without doubt, the reft of the Planets -, but is alfo the Focus of Heat, and the Source of vital Spirits ; whereby the whole Univerfe is fubfifted and nourifhed: and therefore very probably poffefleth the Center about which they all revolve. 2. I T is more likely that the Earth, with the reft of the Planets, fhould revolve about the Sun, when they receive Light and Heat from him j than that the Sun mould move about the Earth, when he receives nothing from it. 3. THERE are many Caufes why the Sun fliould poffefs the middle Place, and the reft of the Planets revolve round him, (efpecially if we embrace the Hypothefis of Kepler concerning the Motion of the Planets) the chief of which is, that the Sun, being a vaft Body, is moved about it*s Ms, and by a ftrpng [ftftory] Force exciteth tha 2 Earth CHAP. 6. of Univer/a/ Geography. 8 1 Earth and the reft of the Planets to a circular Mo- tion (c). 4. THIS Rotation of the Sun about it's Axis is proved from the Obfervations of the Spots upon it's Surface by Galileo (d), Scbeiner, &c. and we may reafonably prefume, it is owing to this com- mon Caule that the reft of the Planets revolve j> bout theirs ; but we cannot perceive a likelihood of any Motion in this Luminary (e). 5- IF (c] The fagacious Kepler was the Founder of the New- tonian Pbilofopby : it was he that firft found out the true Syftem of the World, and the Laws which theceleftial Bodies obferve in their Motions ; it was he that determined the true Path of the Earth, and the reft of the PJanets about the Sun, and difcovered the har- monic Proportions and Concin- nities of their Diftances and Motions : and tho' he did not demonftrate (and fhew a Reafon for the neceffity of) fuch Laws and Proportions ; yet he gave a Hint, and laid a Foundation for that Prince of Geometers Sir IS A AC NEWTON, to demonftrate an abfolute Necef- fity of thefe Laws ; and that without a total Subverfion of the Laws of Nature, no other Rule could take Place in the Revolutions of the heavenly Bo- dies. (d] He was the firft that allied a Telefcope to the Hea- vens, and Ay iff means difco- vered a great may new fur- frijing Phenomena; as the Means or Satellites of Jupiter, and their Motions ; the various VOL. I. Phafes of Saturn ; the Increafe and Decreafe of the Light of Venus; the mountainous and uncertain Surface of the Moon ; the Spots of the Sun ; and the Revolution of the Sun about it's own Axis : all which were firft difcovered and objerved by this great Pbilofopher. Keill's Aftron. Left. Pref. Pag. 1 1 . (e) From the later Obfer- vations of Aftronomers it is manifeft to our Sight, that al- fo every Heavenly Body we have any good Views of, is turned round fome principal Point, and alfo it's own Axis, viz. hath the like Annual Revolutions, and Diurnal Mo- tions as thofe are which we afcribe to the Earth ; yea even the more mafly Globes of Sa- turn and Jupiter, which feem not in their own Nature more fitted for fuch Rotations. Wherefore we may certainly conclude, that it is as poffible, and as probable, that this our lefler Globe, mould perform it's Revolutions according to the fame Law which is obferved in the reft of the Planets, whereby the beautiful Order and Hirmony of Motions is G every 82 Tfc Abfolute Part S E c T. II. 5. IF we fuppofe the Earth placed betwixt Mirj and Venus, and alfo place the Sun in the Cen- ter of the Syftem ; the Motion of each of the Pla- nets will be exactly in Proportion to their feveral Diftances from that Center : But this will not hold in the Ptolemaic Hypothefis, as is manifeft by comparing the Motion of the Sun, Venus, Mercury, &c. (/). 6. T H E Celeflial Phenomena, mentioned in the former Chapter, to prove the annual Motion of the Earth, do likewife as effectually prove that this is the right Place in which it ought to be moved, viz. The Retrograde Motion, and feeming Immo- bility of the Planets -, the admirable apparent Mo- tion [and Pbafa] of Venus and Mercury, &c (g). For fmce the annual Motion of the Earth is prefup- poied in this Place, or in fome other very near it ; :re pr of Nai the Frame of Nature. (f) Sir Ifaac Neat tit's De- monftration, That the Squares of the Planets Revolutions are as the Cubes of their Di- jlances, every where takes Place, if the Sun be fuppofed the Center of the Planets about him ; but does not hold at all in Relation to the Earth; for if the Moon revolve round the Eirth in (27^ Days) a Perio- dical Month, as it certainly does, the Sun, as being at a greater Diibnce, will take no lels than 54700 Years, according 1 to the aforefaid Law, to make his Re- volution about the Earth. But fince this Law, is found to be obferved not only in the pri- mary Planets about the Sun, but alfo in the Secondaries a- bout Jupiter, Saturn, and the Earth, it is an inconteftable Ar- gument that the Sun is as much the Center of the Earth and Planets about him, as the Earth is of the Moon. (g) Thefe Obfervations, which utterly overthrow the Ptolemaic Hypothefis, are ow- ing to later Aftronomers. For they, by their Glafles, have found out that the fpherical Fi- gure of Venus and Mercury, feen from the Earth, will be altered, and have the fame va- riety of Phafes as the Moon hath, viz. will appear opake, horned, bifetled, gibbous, and full, at proper Diltances from the Sun, as explained upon the Copernican Hypothefis ; which certainly eftablifhes and confirms that Order and Situa- tion, namely that Venus and Mercury revolve about the Sun in Orbits that are included within the Earth's Orbit. this C H A p. 6. of Umverfal Geography. 8 j this Argument, in my Opinion, is the beft to de- fend it by i fmce this fituation of the Earth cannot be proved immediately from it's diurnal Motion '. Becaufe it might poffefs the Center of the Univerfe, and have a diurnal Motion, tho* it wanted the an-- nual ; as Origanus fuppofed. 7. B Y this Hypctbefis likewife, the Variation of the Diftances of the Planets from the Earth is ac- counted for. THE Ptolemaics, on the other hand, oppofe the Pythagorean Opinion, and endeavour to prove that the True Place of the Earth is in the Center of the World, by the following Arguments, i, That heavy Bodies are all naturally carried towards the Center ^ but that the Earth is more ponderous than the reft, therefore it ought to refide in the Center (/&). 2. Heavy Bodies would recede from the Earth towards the Center of the World, if the Earth itfelf was not in the Center. 3. The Center is the bafeft Place, and the Earth the igno- blefl Part of the Creation ; therefore it ought to be placed in the Center. 4. If the Earth was placed out of the Center of the World, and was not the Center of the Stars and Planets Motion, then would the Stars and Conftellations at fome Seaibns of the Year appear greater than at others (z). 5. The Medium of the Heavens could not always be percep- tible, nor would Taurus rife when Scorpio fets. 6. Neither would there be Equinoxes. 7. Nor would the Moon fet, nor be eclipfed when the Sun was rifing. 8. -Neither could an equal Number of () This Aflertion is falfe : far greater in the middle of See the Note at the end of this their RegrefTes than in the Chapter. middle of their Progress, be- (;') Tho' this does not hold caofe the Earth, in their Re- in the fixed Stars, becaufe of grefles, comes nearer thefe their immenfe Diftance ; yet Planets an entire Diameier of all the luperior Planets feem the Orbit Magnus. G 2 Miles 84 *fbe Abfolute Tart SECT. II. Miles on the Earth anfwer to each Degree in the Heavens. THE Copernicans eafily refute thefe Arguments of the Ariflotelians. For the firft and fecond is re- jected, becaufe the Motion of heavy Bodies is not towards the Center of the Univerfe, but towards the Earth, a homogeneous Body ; as is proved from the Parts of the Sun and Moon, and of the Loadftone. In the third both the AfTumptions are falfc , For the Center is an Honourable Place , and the Earth is no ways dilhonourable. The reft of the Arguments are eafily difproved by a Defcrip- tion of the Syftem , it being firft prefuppofed that tho* the Earth's Diftance from the Sun be very great, yet if compared with the Diftance of the fixed Stars, it is fo fmall, that it hath no Pro- portion to it ; which feems to fome a great Poftu- latum in the Copernican 4/lronomy (k}. (k) To find this Variation Skill, determine any fenfible of the Diftance of the fixed Parallax at all (only they dif- Stars (arifing from the annual covered a feeming new Motion Motion of the Earth, and cal- of the fixed Stars, which (ai- led their annual Parallax) hath lowing the progreffive Motr- been often attempted by the on of Light) does in fome Mea- Copernican Aflronomers i be- fure demonftrate the annual caufe that the annual Motion Motion of the Earth^. There of the Earth would thereby be appearing therefore, after all, not only made probable, but no fenfible Parallax in the fix- certainly demonstrated. This, ed Stars, the Anti-Copertiicans I fay, was attempted without have ftill room, on that Ac- Succefs, 'till Dr Hook and count, to objeft againft the Mo- Mr Flamfteed, by new inven- tion of the Earth. And the ted accurate Inftruments, feem- Copernicans are ftifl obliged to ed to have found out this an- hold, that the Orbis Magnus Bual Parallax to be at ieaft as is but as a Point in Compari- much again as the double of fon of the Diftance of the near- the Sun T s diurnal Parallax, viz. eft fixed Stars; which is cer- 47 Seconds. But Mr Mofy- tainly (as our Author obferveth) r.eaux and Mr Bradley, by a great Blot in the Copernican their late accurate Obfervati- Aftronomy, left to be wiped ens, coulti not, with all their out by future Ages. i IT C H A P. 6. of Univerfal Geography. 8 5 IT belongs to this Place to explain this Theorem ; that the Diftances of the fixed Stars, and fuperior Planets, Mars, Jupiter, and Saturn, are fo great from the Earth that it's Semidiameter hath no fenfible Proportion thereto ; tho' it is not fo in the Diftance of the Moon, Mercury, and fonus : And if there is any Proportion between the Earth's Semidiameter, and the Sun's Diftance, it is fo very fmall that we are ftill not able fenfibly to difcover it (/). THIS Theorem is thus demonftrated. i . The fixed Stars, and fuperior Planets appear to rife the very fame Moment in our fenfible Horizon, that they are found by Calculation to do, if we were at the Center of the Earth ; therefore our Diftances from the Center Cor the Earth's Semidia- meter) hath no Proportion to the Diftance of the fixed Stars. 2. If we take the Meridian (or other) Altitude of a fuperior Planet, or any of the fixed Stars, with an Inftrument, we find it the fame as if we had obferved it at the Center of the Earth : Therefore the Semidiameter of the Earth is nothing in refpecl of their Diftance. 3 . If there were any fuch Proportion, the Diftance of two fixed Stars would appear lefs near the Horizon than at the Me- ridian, where they are nearer the Earth by almoft it's Semidiameter. THIS alfo is true in the Sun, whofe apparent Diameter is not perceived greater in the Meridian than in the Horizon. &) rallax The quantity of the Pa- Diftances of the Planets from of Mars is determined, the Sun, we have, in effedl, ac- by M. Caflini'i and Flamjieed^ quired the Parallax of the Sun Obfervations, to have been fcarce itfelf, and of the reft of the Pla- 30 Sec. when in Oppofition to nets, and alfo their Diameters the Sun, and alfo in his Peri- and Diftances from the Sun helion ; from whence having and the Earth j of which fee the the true Proportions of the Note at the end of this Chapter. G3 BUT $6 *fbe AbjoluU Part S E c T. II. BUT -the apparent Diameter of the Moon is found to be Ibmewhat enlarged in the Meridian -, becaufe Ihe is there nearer us, than when fhe is in the Horizon, almoft a whole Semjdiameter of the Earth (). CHAP. (n) Here follow the Di- ded Means for determining the fiances, Periods, Diameters, fame, as Mr Wbifton has cal- Gravities, and Quantities of culated them from the lateft Matter, in thofe of the Cele- Obfervations, by Sir IJaac New- Jtial Bodies which have affor- tan's Rules. Mercury Venus The Earth Mars Jupiter Saturn Mercury Venus The Earth Mars Jupiter Saturn Mercury Venus The Earth Mars Jupiter Saturn The Sun The Moon n:;3 iris 1-^ , The Moon The Earth The Sun Jupiter Saturn i, Diftances, 32.000000 59.000.000 diftant from the Sun, Englijh ) 81.000.000 Miles, each 5280 Feet 2* Periods, revolves about the Sun in the Space of -'-.f A H. M. 87. 23. i 6. 224. 17. 49 . 365. 6. 9. 686. 23. 27. 4332- 12. 20. 10759. 7- 36- 3. Bwmeiers. rT.Li?, ;rj r-i ' :~ ,- : r { L E ] contains 'in Diameter, EngUJb 4240 7906 7935 4444 81155 67870 763460 contains in Denfuy, Parts, 5. Gravitia. f C H A P. 7. of Univerfal Geography. 8 7 CHAP. VII. Of the Sub/lance and Conjiitution of the Earth. IN the preceding Chapters we have confidered Four general Properties of the Earth, without Regard to it's Subftance or Conftitution : it will therefore be here proper to confider what kind of Body the Earth is, that we may not be ignorant how it's Parts cleave or are cemented together : which tho' it feem more to belong to Pbyftcs ; ne- verthelefs becaufe it renders the Knowledge of the Earth more perfect, we mail here briefly difcufs it ; leaving the accurate Theory thereof to Natu- ral Pbilofophers. The Moon The Earth The Sun Jupiter Saturn 5. Gravities. .-:, evSi'oc! ..^U> { ? contains in Gravity, or quan- tity of Matter, Parts, ^229600 ' 208 72 97.328 6. The Weight of Bo- dies on the Surface' of the 7. The Time of the' Rotation about it's , Axis of the - - - . to,>;l : ' ' Sun is 24 Parts kEarth is. i Jupiter is i .99 /Saturn is .... j.y .Moon is---------- 0515 Sun is 25 Days Earth is - i Day Moon is- 29 Days Jupiter is 10 Hours Mars is 24.;|Hours Venus is '- - - - 23 Hours o: G 4 P R 0- 88 The Abfolutt Part SECT. II, PROPOSITION L 70 fljew of what fimpk or fimilar Bodies the Earth may confift, or be compounded. T H E R E are feveral Opinions of Philofophers concerning this matter. The Peripatetics reckon four Elements in the Earth and the whole Sublu- nary World, fufficiently known to every on, viz, Fire, Air, Water, and Earth. Many of the An- cients, as Democritus, Leucippus, &c. were of Opi- nion, that the whole World confuted of very fmall folid Particles, which only differed in Mag- nitude and Shape. Which Opinion is followed by feveral of the Moderns ; and fome time fmce, des Cartes endeavoured to account for all the Phenomena of Nature upon this Hypothefis. THE Chymifts imagine that there are three Principles of Nature, viz. Salt, Sulphur, and Mer- cury, to which fome reafonably add Caput Mortu- um. But there feems to me upon a thorough Confideration of the Matter (to drop all ambiguous terms and quibbles), to be frvefjmple Bodies which are the firft Elements or Principles of all things, viz. Water, Oil or Sulphur, Salt, Earth, and a fixed Spirit ; which fome call an Acid, and is per^ haps like the Mercury of the Chymifts (a}. For it (a) The illuftrious Sir Jfe, 'aat Newton thus explains the true Principles of Nature. " It feems probable to me (fays be] that God in the Beginning form- ed Matter in folid, mafiy, hard, impenetrable, move- able Particles, of fuch Sizes and Figures, and with fuch other Properties, and in fuch Proportion to Space, as moft conduced to the End for which he formed them ; and that thefe primitive Particles being folid, are incompara- bly harder than any porous Bodies compounded of them ; even fo very hard as never $o wear or break in Pieces : no ordinary Power being able " to C H A P. 7- f Univerfal Geography. 89 it is plain that all Bodies, and Parts of the Earth, may be refolved into thefe five elementary Sub* ftances. Neverthelefs I do not fuppofe them to differ fo much in their particular Efiences, as in the Variety of their feveral Shapes and Magni- tudes. O F thefe Bodies, mixed after different manners, is the whole Earth compofed j from which pro- ceeds fuch a furprifing Variety in the Nature of Bodies , tho* they are apparently fimilar (). But fince the more accurate Explication of thefe things belongs to Phyfics, we mail fay no more to them here j but handle them at large in another Place. PROPOSITION II. ^fhe Earth is divided into dry and moift Parts, or in- to Land and Water ; to which feme add the At- mofpbere. THIS is the common Divifion of Geography. But then Water is taken, in a large Senfe, for all forts of Liquids and Fluids ; and Land for the whole dry and confiftent Parts of the Globe : whilft the Beginning. And there- fore, that Nature may be lafting, the Changes of cor- poreal things are to be placed only in the various Separa- tions, and new Aflbciations and Motions of thefe perma- nent Particles ; compound Bo- dies being apt to break, not in the midft of folid Particles, but where thofe Particles are laid together, and only touch in a few Points.* Newton's Optics, Pag. 375. (b) See the Notes below on Prof. 6 and 7 of this Chap. both ' to divide what God himfelf ' rnade one in the firft Crea- ' tion. While the Particles ' continue entire, they may * compofe Bodies of one and * the fame Nature and Texture * in all Ages : But mould they ' wear away, or break in Pie- ' ces, the Nature of Things ' depending on them would be ' phanged. Water and Earth ' compofed of old worn Parti- ' cles, and Fragments of Parti- ' cles, would not be of the fame * Nature and Texture now, * with Water and Earth com- ? pofed of entire Particles ia go ' fbe Abfolute Part .S E c T. II. both comprehend various Bodies of Different Na- tures. To the Earth belong, i . Sand, Gravel, Clay, and Mineral Earth ; alfo Chalk, Minium, Oker, Terra Sigillata, Earth of Samos, Bole-Arme- xiac, and feveral other Kinds of Earth. 2. Stones of various forts. 3. Metals; as Gold, Silver, Cop- per, .jTin, Lead, Mercury or Quick-filver, &c. 4. Sulphur, Salt, Nitre, All-urn, Bitumen, Vi- triol, Antimony, 6JV. 5. Herbs, Animals, &c. TO the Water belong, i . The Ocean and Seas, 2. Rivers and frefh Waters. 3 . Lakes and Marmes. 4. MineralWaters, as Hot Baths^ Spaw Waters^ &c. THE Atmofphere is a fubtile Body which fur- rounds the whole Globe of the Earth, and in- cludes the Air, Clouds, and Rain, &c. So that the Earth is beft divided into thefe three Parts. PROPOSITION III. 70 explain bow the Earth and Water cleave one to another ; and conftitute the Terraqueous Globe. THE Earth, that is the dry Part of the Globe, is not terminated by an even and fmooth Surface ; but is here and there hollowed into Cavities, and in other Places elevated into Protuberances. In the Cavities found all over the Earth is contained the Ocean or Sea ; fo that this Part of the fuperficies of the Earth is covered with Water, and the other Part is raifed and appeareth above the Waters. Thefe Cavities are not deprefled into an equal hol- lo wnefs, but are in fome Places rugged and rocky ; and in others funk down into Gulphs and Whirl- Pools. Alfo thofe Places of the Earth which are raifed above the Waters, have in the middle of them, as it were, certain Navels or Eminences ; and fome Parts are either raifed or deprefled more than others. Hence the Water /unrounding the whole C H A p. 7. of Univerfa! Geography. ty i whole Globe is hindred from covering the higher Parts which appear above the Surface of the Ocean ; and are called I/lands : whereof fome are great and others are fmall. * BESIDES that continued Cavity or Chanel in the Sarface of the Earth, there are alfo within it's Bowels innumerable Openings, Recefies, Fiffures, Chafms, Mazes, Swallows, Water Pafiages, and vaft Receptacles ; fome of which arc filled with fait Water, viz. fuch as are joined by iubterra- neous PafTages to the Main Ocean ; others with frefh Water, Rivers and Brooks , in fome alfo are fulphureous Vapours, and fmoaking Subftan- ces. So that Seneca feems to be in the right when he fays, That he trufts too much to his Sight, who does not believe that there is a large Quantity of Sea in the hidden Receffes of the Earth. Nor do I perceive why there mould not be much Sea Water receiv- ed by thefe fubterraneous Swallows ; and formed into Bays by Banks or Bounds. And from the fol- lowing Observations we cannot doubt, that there are a great many Cavities in the Bowels of the Earth. For feveral fubterraneous Rivers are found in Places where the Earth is dug to a considerable Depth ; as is common in Mines. 2 . The Depth of the Sea is in fome Places unfathomable. 3. There are in feveral Places, Caverns difcovered nea^ the Sur- face of the Earth. Thus in the Weft part of the Ifland of Hifpaniola^ there is a Mountain of a vaft Height all hollowed within, into feveral Dens and Openings, in which Rivers rum precipitantly with fuch a violent Torrent and Noife of Waters, that they may be heard at five Miles diftance. 4. Se- veral Whirl-Pools are found in the Sea, and called in the Dutch Language Maelflroom. 5. Earth- quakes alfo mew that there are fuch fubterraneous Caverns. 6. Several Rivers hide themfelves under the Earth, as the Niger., Tigris , &c. 7. Brackifh Fountains $2 ' The Abfolute Part SECT. II. Fountains are obferved in feveral Places, moft of which certainly flow from the Sea. 8 . In many Places the Ground trembles when People walk up- on it, as at the Abby of S. Omer in Flanders -, and in the Province of Brabant upon Peel Marijh. COROLLARY Hence it is evident, that the Opinion of thofe old Philofophers, who maintained that die Earth at firft floated upon the Waters, is falfe ; for by this Means there would be no Chanels in the Sea, but it would be every where of an immenfe Depth. Some indeed of the Antients (efpecially Democrilus} are faid to have been of the following Opinion, viz. that the Waters were formerly mixed with the Earth ; and that the whole Mafs being perfectly fpherical, was foft and of an indifferent Confiftence betwixt wet and dry : But afterwards when the Particles of Water were gathered into one Body, according to the natural Property obferved in Water, the earthly Particles, being feparated from the watery, came together and were curdled into Earth and wrought into Chanels by the Water in feveral Places. The fame Hypothefis is embra- ced by many modern Chriftian Philofophers, who think thefe Words of Mofes (or rather of GOD delivered to us by Mofes} Let the Waters be gather- ed together into one Place, and let the dry Land appear, ought to be thus underftood. But the Fathers of the Primitive Church thought otherwife about this ; for they judged that the Waters were feparated from the earthy Particles [before the Creation] and covered the Face of the whole Earth j and fo oc- cupied their natural Place ; and then miraculoufly receded, and uncovered the Earth by the Power of thefe words of Jehovah ; and that to this day they are hindred and reftrained, by the efpecial Providence C H AP. 7. oflfniverfal Geography. 93 Providence of God, from flowing back and cover- ing the Face of the whole Earth as before ; fo that the prefent Constitution of the Earth and Sea is by them accounted a perfect Miracle. But that there is no great Occafion to think it fo much a Miracle we mail prove in Chap. xiii. where we mail mew, that the Inundation of the Waters, or Ocean, up- on the adjacent Land, is hindred by the Altitude and Confidence of the Earth, which if removed by fome certain Caufes, whereof there are many, the Ocean will foon overflow the dry Land and cover it : whence there is manifeftly, no need of a Mi- racle in the matter. Neither does the beforemen- tioned Opinion of the Antients want it's Defects ; for if the Earth and Water had been once mixed into one Mafs , why did not the earthly Particles rather fubfide, and the Waters, being of lefs Gra- vity, cover the whole Earth ? This they arc for- ced to afcribe to a fortuitous Motion and Conjun- ction of the watery and earthly Particles. Thefe things are faid, by the way, to gratifie fome that earneftly enquire into fuch matters , tho* they do not fo properly belong to Geography ; which hath no Regard to the Opinions of the Ancients, nor need fly to Miracles in explaining the Properties of the Earth (r). PROPOSITION IV. The Superficies of the Earth Is continued, but not that of the Waters. THE Superficies of that Part of the Earth which is raifed above the Waters, is continued to the Superficies of the Chanel of the Sea, and that again to other elevated Parts of the Earth* Alfo ((} Sec Dr Woodward 'sE/ay towards a Nat, Hijt. of the Earth, Sec, the 94 ?be Abfilute Tart SECT. IL the Ocean, Bays and Rivers have one continued Superficies; but all Waters have not: for there are fome Lakes whofe Superficies are not joined with that of the Ocean, as the Lake Parime, and the Cafyian Sea, &V. PROPOSITION V, fbe Conftitution of the Eartb^ far within the Sur- face (which is our Habitation) towards the Center, is uncertain. SOME think that Water taketh up the loweft Place about the Center ; but it is more likely that dry Earth fhould occupy that Place (d}. Gilbert was (d) The learned and faga- cious Dr Halle-), to account for the Changes of the Needle's Variation, hath fhewed a Pof- iibility that the exterior Parts of the terraqueous Globe are formed inwardly like the con- cave Surface of a petrified Shell; and the internal as a Nucleus, or inner Globe, included with- in ours, with a fluid Medium between, which moves along with it, as having the fame common Cehter, without fenfi- bly approaching one Side or ano- ther, like the Globe of Saturn environed with his Ring. ' And tho' (fays be) thefe included Globes can be of very little Service to the Inhabitants of this outward World, nor can the Sun be of Service to them : yet fince we . fee all Parts of the Creation abound with animate Beings, why ihooid we think it ftrange that the prodigious Mafs of Matter, whereof this Globe doth confift, fhould be capable of fome other Improvements, than barely to ferve to fup- port it's Surface ? Why may we not rather fuppofe, that the exceeding fmall quantity of Matter in refpedl of the fluid Either, is fo difpofed by the Almighty Wifdom, as to yield as great a Surface for the Ule of living Crea- tures, as can confift with the Conveniency and Security of the whole. ' And tho' without Light there can be no living, yet there are many Ways of pro- ducing Light which we are wholly ignorant of: The Me- dium itfelf may be always lu> minous after the Manner of our Igna Fa tut: The con- cave Arches may in feveral Place* Ihine with fuch a Sub- ' fiance C H A P. 7. of Univerfal Geography. 9 was of Opinion that the Body of the Earth with- in is nothing but a very hard Loadftone ; and that thefe exteriour Parts towards the Surface, which are penetrated into by digging, and on which Herbs grow and we live, are but as it were the Bark and Cruft of the Earth, and the Seat of perpetual Generation and Corruption. The Opi- nion of des Cartes is not much different from this ; for he believed there were three Strata in the Bo- dy of the Earth of divers Confidences. The firft and innermoft porTeffing the Center, the fecond of a denfe and opaque Nature, confifting of the minuteft Particles ; the third (being replete with Men and Animals) he fuppofes to be compoun- ded of Particles not flicking fo clofe together. NEVERTHELESS, for want of Obfer- vation, we cannot affirm any Thing for Certainty in this Matter ; and tho' it be true that in feveral fubterrarieous Places, there is a glowing Heat, and that Smoke and fulphureous Fumes are ex- haled from feveral hot Baths : and alfo tho* Thurn-* heufsr affirms, that he found by Experience that the nearer they digged to the Center of the Earth, there was the lefs Water in Mines , yet we are ftill in a Doubt, and cannot pofitively depend upon his particular Obfervation. fiance as invefls the Surface ' been ; and a Notion not fo of the Sun; nor can we, with- ' much as ftarted in the World out a Boldnefs unbecoming a ' before.' Philofopher, adventure to af- Thus far Dr Halley. Hovr fert the Impoflibility of pe- he accounts for the Variation of culiar Luminaries below, of the Needle from this Hypothe- which we have no fort of fis; See the Notes upon Cbap. Idea. 38. Prop. 4. of the Comparative Thus have I fliewn a Pof- P-rt, or Plilof, Tranfatt. N fibility of a much more ample 148. Pag. 208. and N 195.., Creation than has hitherto Pag. 564. PRO- 96 ' Vhe Abfolute Part SECT. II. PROPOSITION VL fbe Confidence or Coherence of the Particles of the Earth is from Salt. THE artificial Separation of the Particles of Bodies demonftrate, that in the Competition of the whole there is a certain kind of Salt which is more abundant in harder Bodies, as in Metals, Stones, &V. (a few oily Subftances only excepted) (*). And that all folid Bodies are concreted by Salt, is manifeft from the artificial Petrefaftion of thofe that are foft, to any Degree of Hardnefs by it. (e] Tho' moft forts of Bo- dies are replete with faline and vitriolic Particles, fuch as may in fome Means contribute to their Coagulation and Confo- lidation; yet the primary and naturally indivifible Corpufcles, of which the Particles of all Bodies are compofed, are not connected by fait or hooked Atoms, as fome imagine ; nor glewed together by Reft, which is an occult Quality or nothing, nor ftick together by confpiring Motions, but rather cohere and are united by mutual Attraction. So that the fmalkfl Particles of Matter may cohere by the jftrongeft\Attratlions, and compofe digger Particles of weaker Vir- tue ; and many of tbefe may co- bere t and compofe bigger P'ar ti- tles tohofe Virtue is Jlill wea- ker. See Newton's Optics, Pag. 37- Hence Particles of Bodies which touch one anotherin large Superficies's, by a ftrong mutual Attraction of their Parts, corfl- pofe a Body very bard', and if thefe Particles are not fo ftrong- ly attracted or entangled with each other, the Body will be brittle ; if they touch one ano- ther in lefs Superficies, the Body is not fo hard, but yet may be more folid ; if they only approach each other, without flipping one under another, the Body is Elaftic, and fprings to it's former Figure; if they flip under each other the Body is foft, and eafily yields to the Stroke of the Hammer ; if they fcarce touch one another the Body is crumbling, or fuch whofe Parts may be eafily feparated ; if they are fmall, round, flip- pery, and eafily agitated by Heat, the Body is fluid ; if thefe Particles are of an unequal Superficies, and hooked or en- tangled one with another, then is the ^Bo^y flexile or pliant, &c. See Dr Clarke's Notes up- on Robaulfs Pbyjicf. So CHAP. 7. of Univerja I Geography. 97 So that if Salt be feparated from Bodies, their Particles will no longer be cemented ; but they will become Powder, which cannot be brought to a Coherence without the Admixtion of ialine Particles. PROPOSITION VII. Various kinds of Bodies are feveral Ways mixed to- gether in the Globe of the Earth. I N Mines there are found Particles of Gold, Silver, Lead, &c> not gathered into a Mafs and feparate from others , but fometimes mixed a r mong themfelves, and fometimes with ufelefs Earth, in fuch very imall Particles that the beft Judges in Metals cannot at firft Sight difcover what fort of Mineral is contained in fome Me- talline Earths (/). Alfo in the Fields, Sand is fometimes (f) The indefatigable Dr Woodward, in his Ejfay towards a Natural Hi/tory of the Earth, reafonably fuppofes all thele Commixtures of the Particles of Bodies in the Strata of the Earth, to proceed from thofe ftrange Alterations that were every where made in the Ter- reftrial Globe at the Deluge, when the whole Globe was difiblved, and the Particles of Stone, Marble, and all other folid Foflils diflevered, taken up into the Water, and there fuftained together with Sea Shells, and other animal and vegetable Bodies: that at length all thefe fubfided from the Wa- ter, according to the Nature of their Gravity; the heavieft Bo- dies firft, then thofe that were VOL. I. lighter ; but all that had the fame Degree of Gravity fettled down at the fame Time ; fo that thofe Shells, or other Bo- dies, that were of the fame fpe- cific Gravity with Clay, Chalk, Sand, &c. funk down together with them, and fo were in- cloled in the Strata of Chalk, Clay, Sand, or Stone, which their Particles formed; (hat at the general Subfidence, Metals and Minerals, as well thofe which were amafled into Lumps as thofe which continued afun- der, and in fingle Corpufcles, funk down to the Bottom along with Sand, Coal, Marble, &(. .and fo were lodged widi the Strata which the Sand, &(. conllituted. That all the metal- lic and mineral Matter which H is ^8 ' fbe Abfolute Part S E c T. II. fometimes mixed with Clay or Lime, and fome- times with Salt, &V. Not long fmce at Amfterdam^ -when the Earth was digged up to the Depth of two hundred thirty two Feet to make a Well, thefe kinds of Earth were gradually difcovered. Firft feven Foot of Garden Mould, then nine Foot of black combuftible Earth, which is called Peat, (not like that they properly call Dutch Turf) then nine Foot of foft Clay, then eight Foot of Sand and four of common Earth, then ten Foot of Clay, and again four of common Earth, next that ten Foot of fuch Sand as the Foundations of the Houfes in Arnfterdam are laid in, then two Foot of Clay, next four Foot of white Gravel, then five Foot of dry Earth, and one Foot of Mud, again fourteen Foot of Sand, then three Foot of fandy Clay or Mire, afterwards five Foot of Sand mixed with Clay, and next four Foot of Sand mixed with little Sea-Shells, then there was a Stratum of Clay one hundred and two Foot deep, and laftly thirty one Foot of Gravel, where the Shaft was fmifhed. (>' f ati'ii is now found in the Fiflures, ted Strata, Tome elevated and or perpendicular Intervals of the others deprefled, by which Strata, was originally lodged in Means all the Inequalities of fingle Particles among the Sand, the Globe, Fiffures, Grotto's, &V. having been detached and Mountains, Vallies, Iflands, drawn thence by little and little the Chanel of the Sea, and all by the Water, which continual- others, were formed, and chat ly pervades the Strata ; and the whole Terraqueous Globe that Trees, which are found in (with all it's Materials) was, at great Plenty in Moffes, Fens, the Time of the Deluge, put or Bogs,were depofited thereby nearly into the Condition that the Deluge ; fo that the prefent we at this Day behold it. See .Earth was formed out of this Woodward's EJay, or Pbilo- rjromifcuous mixed Mafs of fopbital franfaftions N 217. Sand, Earth, Shells, and Me- p. ijr. tills, and of broken and difloca- PRO- CHAP. 7< vfUmverfal Geography < yg PROPOSITION VIII. *he Cavities of the Earth ^ and the external .and in- ternal Difpofetion, or Situation of it's PartSj are not perpetually the fame, but different at different THE Sea not only makes many Devailations and Changes in the Parts of the Earth, by fome of it's Pallages being Hopped, and others more opened ; but alfb that fpirituous and fulphureous. Sabftance which here and there lies hid in the in- terior Parts, when it begins to heat and evapo- rate, impetuoufly makes the exterior Parts of the Earth, raifing them up, as is ufual in Earthquakes. And it is probable the like Eruditions may of- ten happen in the more interior Parts of die Earth j which for the moft part we have no Notion of. W E mall treat of the mutual Changes of Land and Water in Chapter 1 8 . hereafter, The Terraqueous Globe is divided inter Earth whofe J" covered with Water, or raifed a- Surface is \ bove the Waters ; and into Water '. THE Superficies of that Part of the Earth which appeareth above the Waters, is, by the In- terflux of the Sea thus divided. I. INTO large Continents, or great Iflands,- which we fuppofe to be four. ~ North by the Hyperbc- rean Frozen and Tarlaric H 2 Ocean. i. The 100 The Abfolute Part SECT. II. Eaft by the i.TheO/Jc Europe * > and is Pacific and World which P Afia and ( > bounded < IndianOcean. containeth - t Africa ; > on the South by the Southern Oce- an. Weft by the Atlantic^ or We fern Oce- ' an. 2. The New C North World which ^ and contained! - - C South bound- 4 ed on the North by Davift Streights. Eaft by the Atlan- tic Ocean* South by the Streights. of Magel- lan. Weft by the Pacific L Ocean. 3. THE Arftic Continent , or Greenland is fur- rounded on every Side with Seas and Streights. 4. THE Antarctic Continent^ or Terra Au- Jlralis Incognita. II. INTO Peninfula's, or Cberfonefu/es, which are Parts of thefe Continents. Of which fome C Africa. are of a round Fi- [North and South America] gure, whofe Lon- J Peloponnefus, or the Morea in gitude and Lati-| Greece -, Taurica Cberfonefitf or tude are almoft e- Crim-fartary. qual, as [ Cambaya or Guzarat. Others CHAP. 7. Others ob- long of which there are ma-' ny, as Others which are almoft like Peninfula's, which are of Um'ver/a/ Geography. i o i Cberfonefa a" or, or Malacca in India. Cimbrica, or Jutland ', contiguous to Holftein. Corea contiguous to tfartary. * California, Tucatan, the Cherfonefus of Romania. Ionia [as Smyrna'] Cnidus and Myndus. Italy, Greece, and proper Achaia. Spain, Afia minor ; and Arabia. Norway, with Sweden , and Lap- land. Patagon near the Streights of Magellan and New Guinea. Indoflan, Cochinchina, New Bri- tain^ Monopatapa, &c. III. INTO Iflands of which there are three Claflfes, viz. (Britain *Japa Britain n[Ele- | * Japan oeri\ very <^ Iceland large ones I James Ifland] I Sumatra L 2. [Eleven]\f il y , of a middle l?** , 1 Hifpamola Luconia] Madagascar * Nova Zembla Newfoundland] California. Size Cuba s, j. Landia c j. Sardinia , . , Mindanao. Gihlo, Amboina, Timor, among the Indians Iflands 3 . LJ L.* t j . Corfica, Majorca^ Cyprus ^ Negropont^ lefler ones in the Mediterranean Zealand in Denmark, and Jamaica in the Gulf of Mexico. /> #Wj f ^ fx/ Chapter. H 3 Very *fbg Abfolutf Part SECT. II, Very many fmall ones, of which we rec- ' The Canary Iflands The Azores Cape F^Ifland^ The Antilln The Maldivia Ifland The Comoro Iflands The rrioft remarkable Solitary ones, are Rhodes, Malta, Lemnos, $1 Helena, St Thomas, Madera, &c. The noted Clufters of Iflands which lie near one another in great Numbers afe The Molucca and Ban- dana Iflands. The Philippine Iflands The Ladrone Iflands Thofe in the JEgean Sea The Britannic Iflands The Iflands of Solomon. IV. IJlbmuSs or narrow Necks of Land. That of Suez, between Africa and Afia. That of Corinth, joining the Morea to Ackaia. That of Panama, in America, longer than any of the reft. That between Jutland and Holflein, TJrat joining Malacca to India. SECT. C H A P. 8. if Utiiverfal Geography. 1 03 SECT. III. In which the Conftitution of the Earfb, or the dry Part of the terraqueous Globe., is explai- ned, in four Chapters. CHAP. VIII. Of the natural Divifion of the Earth into Parts by the circumfluent Ocean. WH A T we mall exhibit in this Chapter, con- cerning the Divifion of the Earth, and that in Chap. xv. about the Diftribution of the Sea, will be of great ufe to young Students, for underftand- ing, and remembring the Bounds and Situation of the feveral Countries on the Earth's Superficies : wherefore thefe two Chapters ought to be read throughout with great Attention, and compared with Maps, or the artificial terreflrial Globe. We faid before, in the preceding Chapter, that the Terraqueous Globe, as to it's condiment Parts, may be bed divided into a Body of a firm Con- fiftence as Earth, and a fluid matter as Water ; to which may be added the Atmofphere as a circun> ambient Fluid or Covering. I N the firft Place, we fhall treat of the Earth, or that Part of the Globe which hath Confi- itence, H 4 104 *Tbe Abjolute Part SECT. III. PROPOSITION I. Part of the Earth is covered with Water , and Part, of it is raifed above the Superficies of the Water, and fur rounded thereby. THE Truth of this Proportion is manifeft from Experience. Neverthelefs there are fome Places which are now and then covered with Water, and at other Times dry and confpicuous, as the Iflands near Norway, Scotland, and other Countries, to which may be added Sand-beds or Shelves, and Sea- fhores -, but becaufe thefe are fo fmall in compa- rifon of the reft, we fhall take no notice of them at prefent. Nor mail we trouble our felves here with difputing whether the greater Part of the Superficies of the Globe be taken up by Land or Water, but leave it to be difcufled in Chap, xviii. and confider here only the apparent Parts of the Earth which we call JJJands, PROPOSITION II. The Parts of the Earth, which are raifed above the Waters, are not always joined together by one continued Superficies, but often feparated one from another, and formed into I/lands by the Interflux of the Sea. THESE may be djftributed into five Clafles, viz. Plats of Land or I/lands, that are great, and Continents that are greateft , fome fmall, and others that are fmalleft; and laftly fome of a middle Size. W E mail treat of the Origin, and Caufe of thefe Iflands in the proper Place, Chap, xviii, CHAP, 8. of Umverfal Geography. 105 T H O* all the feparate and apparent Parts of the Earth ought to be called I/lands, becaufe an Ifland is nothing but a Part of the dry Land every where environed with Water ; yet, in the common Way of fpeaking, this Word is feldom ufed to ex- prefs thefe iarge Traces of Land whofe Boundaries by the main Ocean, (by reafon of their vaft Ex- tent,; are not fo perceptible. Such as thofe are frequently called the Terra firma, or great Conti- nents^ which peculiar name they ought to be di- ftinguimed by on account of their Magnitude, in refpect of the reft of the Iflands, which are very fmall in comparifon of them. Therefore we mall, in what follows, call them the Terra firma or great Continents. But the word Continent is frequently ufed to exprefs feveral Parts of the Terra firma as well as the whole. And fometimes it is taken ftrictly for a Part of the Earth, on no fide conti- guous to the Sea : Or in a large Senfe for a Country bounded by the Sea on one fide, and on the other joined to a large Tract of the Terra firma. It is alfo often taken in general for a Part of the Earth joined to another, whether by a large or a narrow Tract of Land. In thefe Senfes the Word Continent differs from that in which it is frequently ufed to exprefs large I (lands. PROPOSITION III. Thefe large TraRs of Land, Continents or Terra fir- ma, (which you will pleafe to call them) are accoun- ted four in Number. j. T H E old World. 2. The new World, or America. 3. The Northern Continent, or Terra Arftica. 4. The Southern Continent, or Terra Auftralis. 2 I. THE io6 fbe Abfolute Part SECT. III. 1. 'J'HE Old World (being the moft famous of the four, which we inhabit, and which was only known to the Ancients) is divided, by the Sea into two Parts, which are only joined one to a- nother by a fmall neck of Land, whereof one is Africa , while Europe and Afia jointly make the other. It is thus environed by the Ocean. O N the North by the Icy or North Sea, the White Sea, and the Tartaric Ocean. O N the Eaft by the Great South Sea and Pa- cific Ocean. O N the South by the Indian Sea, the Southern and j&thiopic Ocean. ON the Weft by the Atlantic Sea, THE aforefaid Divifion of this Continent is made by the Mediterranean, f and Arabian Gulph or Red Sea. The Diftance of thefe two Bays, or the Breadth of the intervening Tract of Land being about 40 German Miles , fo that Africa would have been an entire Terra firma, and numbred a- mong the Continents, but for this fmall Iftbmus. THE Old World is not far diftant from America in the Eaft about the \_fuppofed~] Streights of Anian [or Uries,~\ if there be fuch , but the leaft [known'] Diftance of Europe from America is between Nor- way and Newfoundland. THE Diftance between the Old World, and the Arctic Continent is fhorteft about the [Icy Sea] -, alfo the Old World is not far diftant from the South Continent about New Guinea. 2. THE New World, or America, is thus encom- paired by the Ocean. O N the North we are in Doubt whether there be Sea or Land beyond the Streights of Davis. O N the Eaft it is bounded by the Atlantic Ocean. O N the South by the Magellanic Streights. i ON CHAP. 8. of Univerfal Geography. 107 O N the Weft by the Pacific Ocean. THE New World is alfo nearly divided into two Iflands at Panama and Nombre de Dios, where the Atlantic and Pacific Ocean are hindred from meeting by a very fmall Ridge of Land. AMERICA is not far diftant from the Old "World about the Streights of Anian [or the Sea of Japan] , and not far again from the Arctic Continent at Davids Streights, and feparated from the South Continent only by the Streights [of la Maire\ and the Magellanic Sea. THE Arctic and AntarcJic Continents are every where environed with Sea, the former [as is fuppof- ed] with the North Sea at the Streights of Davis, [Uries or] Anian, [and the Icy Sea] -, the later with die South Sea, Pacific and Indian Ocean, and the Streights [of la Malri\. 3. THE ArcJic Continent is not far diftant from the Old World [at the Icy Sea], nor from America at Davis's Streights ; but it is feparated from the South Continent by a vaft Interval. 4. THE Antarctic Continent is not far removed from the old World at the Peninfula of New Guinea, and feparated from America by the Streights of Ma- gellan [and la Maire]. B U T we have.not been able to find for certain whether the Old World, America, and the Northern Continent, be each of them encompafled with Sea, and feparated one from another ; tho' it be very probable that they are, by reafon of the feveral Bays and Entrances of Streights that run in from the Ocean to the Landward. Only the Southern Continent hath been actually failed round, and therefore is certainly known to be environed on all fides with Sea, and therefore feparated from the reft. But this has not yet been done by the other . The Abfolute Part SECT. III. other Parts , for men have not failed about the Old World much further then Streigbts of ffai- gats, tho' the whole Weftern, Southern, and Ori- ental Shores have been vifited, and there is but a fmall Part of the North [Eaft] Coaft that remains to be difcovered (a). America alfo hath been failed round (a) All the Attempts made by the Europeans to difcover a Nortb-EaJl-Pa/age to the Ori- ental Countries have been hi- therto unfuccefsful. The Rea- fon was formerly thought in a great meafure owing to the Difcoverers not fleering their Courfe near enough the North Pole ; being either mifled by an Opinion, that that Part of the Sea which lies betwixt Nova Zembla and the Continent of Tartarj had been paflable; or that they might have coafted it along the North ofNova'Lembla and Tartary, till they had enter- ed the Streights ofjeffb, which could never be effected by Rea- fon that moft of thefe northern Coafts are frozen up many Leagues from the Shore, efpe- cially in the Winter, tho' in the open Sea it is not fo, even under the Pole itfelfj unlefs, for Example, upon the Approach of the Summer when the Froft breaketh, and the Ice, whichwas congealed near 40 or 50 Leagues from the Shore, goes off from the Land and floats up and down in the Sea ; whereby fe- veral have been forced to quit their Defign and (land back for their own Country. See Pbilof. Tranf. NO. nS.Pag. 417. Big with this laft notion our Coun- try-man Capt. John Wwd, the lateft Adventurer who attempt- ed the North- Eaft Paflage, in the year 1676, fteered direftly NE from the North Cape of Norway, in order to fall in between Green/and and Nova Zembla ; but he could find no Sea or Inlet between thofe Countries ; on the contrary, he obferved the Ice to adhere im- movably to the Coaft of Nova Zembla, and that all the Englijb and Dutch Pilots had been mif- taken in their Conjeftures of an open Sea thereabouts, for he could pafs no further this Way than to the 76 Degr. of Lati- tude, on account of the Ice, which muft have then taken up fome Centuries to thaw. He concludes therefore thatGrray- land and Nwa Zembla muft be the fame Continent, by Reafon there was no Current found there, but only a fmall Tide which rifes about eight Foot, and ebbs back again. And ifit fhould be admitted, to the con- trary, that the Continent of dfia and America are feparated by the Ocean, yet we may now reft fatisfied that the Difficulties to be met with in a North-Eaft PafTage are not to be furmount- ed, and poffibly will never be attempted again. Salmon's Pre- fent State of alt Nations. Vol. 6. Pag. 380. [I forbear CHAP. 8. ofUniverfal Geography. 109 round except a Part of the Northern Shores, on account of the Uncertainty of the Streights and other Difficulties. This therefore is the Situation of the four Continents. PROPOSITION IV. :# V '-ft "-::*". -:.'*>V. ^fc V- To enumerate the great Iflands difperfed over the Sur- face of the Terraqueous Globe : viz. 1. BRITAIN^ comprehending England and. Scotland, is fuppofed to be the greateft of thofe com- monly called Iflands (thofe in the preceding Pro- pofition excepted). It lies betwixt Europe and A- tnerica, near France and Flanders. It is furrounded by the Atlantic Ocean^ and it's Form is oblong. 2. J A P A JV, in Maps and Globes is reprefented of a lefs Magnitude than it ought to be -, for they that have been there affirm it to be larger, or at lead no lefs, than Britain (b). It lies eaftward of Afia not far from China. It is furrounded by the Pacific Ocean , and is of a curve Figure. 3. LUCONIA, which is alfo called, from it's Metropolis, Manilba, is the Principal of the Pbilip- [ I forbear to enlarge upon an of JeJ/o, the Inhabitants of Account given us lately, as ad- both Countries doubt; becaufe vices from Muftovy, of an Ex- vaft and inacceflable Mountains pedition entered upon, under interpofe which hinder the the Commandofone Capt. Ber- Communication. Neither doth ring, to find out this Nor thEajl- it as yet clearly appear, whe- PaJJage, whofe Voyage is now ther this Land of JeJjTo is a. faid to be Printing at Mofcow, Part ofTartary, or whether it in which he affirms, that there is by an Arm of the Sea divid- is a free and open Sea to about ed from it. The Cbinefe affirm the North-Eaft Point of Tartary, that Tartary runs 300 China and believes it to be likewife Leagues beyond their famous open to the Sea of China, or, as Wall ; fo that if we follow them fome Geographers call it, the the Country ofjejfi, and alfo Japan, may feem not to be Iflands (b) Whether Japan be an Iflands but annexed to Tartary. Ifland, or annexed to the Land Pbilof. Tranf. N 1 1 8 . 1 10 The Abfolute Part SECT. HI. fines, which are thefurtheft, of the Oriental Iflands, on the Borders of Afia. Some will have it to be larger than Britain -, but they who have been there fay it is fomething lefs. It is encompafTed by the [great South Sea,] and is of a curved oblong Figure, with many Inlets and Windings. 4. MADAGASCAR, or the Ifland of St Laurence, lies on the eaftern Shore of Africa, not far from the Streights of [Edbelmandel or\ the Red Sea. It is environed by the Indian Ocean (all the Sea between Africa and India being now called by that Name). It's Form is oblong, 5. SUMATRA, thought by fome Geogra- phers to be the Taprobana of the Ancients, lies near the Borders of Afia among the [Sunda Iftands] not far from the Peninfula of Malacca (c}. It ftretches to a great Length, and is furrounded by the Indian Ocean. 6. BO RNEO is fituated in the Indian Sea not far from Sumatra : ii's Form is almoft round. There is a great Difference among Authors about it's Ex- tent j fome make it's Circumference to be about 2100 Miles, and will have it to be the greateft among the Indian Iflands: others but about 300. 7. 1C EL AND, Part of which is fituated in the Temperate, and Part in the Frigid Zone, be- twixt Greenland, and Norway, is encompafled by die Northern Ocean, and it's Form is 'oblong. 8. NEWFOUNDLAND is an Ifland adjacent to Canada, in North America. It is fomething larger than it is mewed in our common Maps. It is en- vironed by the Northern Ocean, and receiveth the Sea in at a great many Creeks. (f) Not Sumatra but Ceylon called by the Indians Tenerafin, is thought, by all modern Geo- i. e. A Land of Delights, as graphers, to be the Taprobane it was reprefented by the of the Ancients. And it is itill Ancients. C H A p . 8 . of Univerfal Geography. i i * 9. [JAME&sor Cumberland's IJland~] lies in the Northern Qcean near the Arffic Continent^ between Davis's arid Hudfon's Streights. I have not found it in any Map before that of Vifcherm, printed in 1 594. It is a large I/land of an oval Figure. 10. NOVA Zembla is fituated between the Arftic Continent and the Land of the Samoieds and [Oftiacs]. It is bounded on the North by the Icy and [Mufco- vian\ Sea, and feparated from Europe at the Land of the Samoieds by the Streights ofWajgats (d). It's Form is oval. 11. CyfL7FO/?A^/^maybeaddedtothefe if it be an Ifland, and not a Part of America (ej. The Dutch found in a Spanijb Ship a large Geogra- phical Map) in which California was repreiented as an I/land not contiguous to America, but furrounded with the Sea. (d] Mr Witfen tells us, in Pbilof. Tranf, N 101. Pag. 3. ' That he had received out of " Mufcovy, a new Map of Neva Zembla and Waygats, as it had been difcovered by the exprefs Order of the Czar ; by which it appears, that Nuva Zetnbla is not an LQand, as hitherto believed, and that the Mare Glaciate is not a il> 5J?H? \M.-. irw' s I CHAP. 8. of Univerfal Geography. PROPOSITION IX. Befides thefe I/lands there are other Parts of the Earth y whofe Surfaces are different in Shape or Figure 3 fetch as Peninfulas'; and Ifthmufles. A Peninfula, called by the Greeks Cherfonefus, is a Part of the Earth joined to another by a narrow Neck of Land, and on every Side elfe encompaf- fed with the Sea. That narrow Tract or (Irak Paf- fage, whereby one Country hath communication with another by Land, is called an Ifthmus. We muft alfo here obferve thofe Parts of the Earth that are flretched out into the Sea, but are joined by a larger Tra6t to the main Land, for fuch extended Parts form a Species of Peninfula's, and may in fome fenfe be fo called. S U C H are Italy, Spain, part of England, Greece and proper Achaia, Afia minor, Norway with Swe- den and Lapland, Indoftan, New Guinea in the South Continent, [New Holland'] New Britain, and [New Scotland] in America, Cambodia, Patagon, the ex- tream Parts of Africa, &c. PROPOSITION X. To enumerate the Peninfula's. THESE Peninfula's are oblong, viz. 1. CHERSONESAd' or, or Malacca, contigu- ous to India. 2. C I MB RICA, or Jutland, contiguous to Holjlein. 3. C AL IFO R NIA, on the Weftern Shore of 'North America, is thought, by fome, to be a Penin- fula ; J)ut commonly reprefented in our Maps as an Jjland. I 3 4. TUCATAN 1 1 8 fbe Abfolute Part SECT. III. 4. TUCATAN, in the Bay of Mexico, contigu- ous to New Spain. 5. THE Cherfonefus of Romania, near the Hel- lefpont. 6. CORE A ', was formerly thought to be an Ifland, and not a Peninfula. In fome Maps I have feen it joined to Tartar*}, and in others furrounded with the Sea. Neverthelefs, the lateft Obfervations make it a Peninfula -, but even now it is not fettled among Geographers. 7. TO thefe may be added the three fmall ones of Ionia in leffer Afia [or Smyrna], Melajfo, and Hali- carnajjiis. THESE Six Peninfula's are roundifh, viz. i. AFRICA, a great Part of the old World, furrounded by the Mediterranean, Atlantic, Mthio- pc, Indian, and Red Sea. It is joined to Afia by a narrow Neck of Land near ASgypt. 2.3. NORTH and South America viz. Mexico and Peru. They are joined together by the Streights of Panama. 4. PELOPONNESUS, now called the Mbrea, a Part of Greece. 5. 7 'AURIC A Cherfonefus, now called [Crim Tartary] in the Black Sea, near the Streigbts ofCaffa* 6. CAMBATA, or Guzarat, in India. PROPOSITION*!. There are as many Ifthmus's as Peninfula's. Tbofe of mojl note are, 1. THAT of Suez, which joins Africa to Afia. 2. THAT of Corinth, which joins the [More* to Achaia.~\ 3. THAT of Panama, which joins North Ame- rica to South America. 4. THAT joining Malacca to India. And, 5. THAT joining [Crini to Precop Tartary."] CHAP, C H A P. 9. of Um'ver/at Geography. 1 1 ^ CHAP. IX. Of Mountains in general MANY Things occur worthy of particular Notice, in explaining the Nature of Moun- tains, and therefore they are copioufly handled by Geographical Writers, efpecially the Computation of their Altitudes , becaufe they feem to many to make againft the Earth's Rotundity. PROPOSITION I. A Mountain is an elevated Part of the dry Land^ over- topping the adjacent Country j and a Hill or Cliff is a fmall kind of Mountain. A Promontory, if a Mountain jlr etching it felf into the Sea, and Rocks are Stones raifed above the Sea or Land> in the Form of Mountains, "We mufl know that all the Parts of the Earth which appear plain, are not exactly of the fame Altitude, but commonly elevated towards the In- land Parts, and depreflfed towards the Sea Shores, as is manifeft from the Origin and Courfe of Ri- vers , for that Part towards which they flow, is al- ways more deprefled than that where they Spring ; and Fountains feldom are increafed into Rivers, unlefs they take their Origin from Mediterranean or inland Countries : which mews, that thofe Coun- tries are more elevated than the Maritime Parts. So Bohemia is known to be higher than Holflein^ be- I 4 caufe 120 fbe Abfolute Part SECT. III. caufe the River Elbe rifes in the former, and falls into the later. Alfo from the Danube, the Wefer^ the Rhine ^ and the Mofelle^ we perceive the greater .Altitude of thofe inland Countries, from whence they flow. For this feafon, Switzerland and the Country of the Grifon^ are accounted the higheft Lands in Europe ; becaufe the Rhine^ the Danube^ and the Rhone, derive their fource from them. Moreover, the inland Countries are elevated above the maritime Parts, according to the different De- clivity and Rapidity of the Rivers. HERE follow fome Problems, by which we may form a Judgment upon the controverfial Wri- tings handed down to us, about the different Alti- tudes of Mountains. PROPOSITION II. I'o take the Height of a Mountain by AUimetry, THIS is performed the fame Way as we take the Height of a Tower, provided the very Top of the Mountain be perceptible by any Mark. LET AB (Fig. 12.) be the Altitude of a Mountain, A the Foot of it, B the Mark feen at the Top. Take the Line FC at a convenient Diftance, fo that neither of the Angles A F C or A C F may be very acute, but nearly equal. Let the Angles BFC and BCF be obferved ; and the Sum of their Degrees being taken from 180 the Remainder will give the Angle CBF (a]. Then let C F the Diftance of the two Stations be accurately meafured ; which done, fay, as the Sine of the Angle F B C, to the Sine of the Angle CFB: (orofFCB: if you would find FB) fo (a] By Article 14. of Chap, ii. above. CH AP. 9. ofUmverfat Geography. 121 is F C to B C the Diftance of the Top of the Mountain from C. Then [with a Telefcope fxed to a Quadrant or otberwife\ take the Angle B C A, and you will have alfo the Angle ABC, becaufe the Triangle CAB is rectangular *. T H E R E F O R E in the Triangle ABC, As the Radius 10000000, is to the Sine of the Angle BC A : fo is the Diftance BC, to the perpendicular Altitude of the Mountain AB. FOR Example. Let us fuppofe that Xenagora^ the Son of Eumelus, ufed fome fuch Method as this to find the Height of the Mountain Olympus, which he is laid to have meafured exadly. Where- fore if he found the Angle BFC 84 degr. 18 min. and the Angle B C F 85 degr. 34 min. then was CBF i o degr. 8 min. And fuppofe, by meafuring, or fome other Method, he found FC 1200 Grecian Feet, or 2 Furlongs. Therefore as the Sine of the Angle CBF 10 degr. 8 min. 17594 is to the Sine of the Angle BCF 85 degr. ^^.min. 99701: fo is CF 1200 Feet to BF68oo Feet, the Diftance from the Top. Likewife the Angle BFA being found, by fome Inftrument then in Ufe to be 63 degr. 30 min. by faying, in the Triangle FAB, As Rad. i ooooo to the Sine of the Angle BFA 89500 : foisFB 6800 to AB 6096 Feet, the Altitude of Mount Olympus. But 600 Feet make a Grecian Furlong ; therefore dividing 6096 by 600, the Quotient, 10 Furlongs 96 Feet, is the Height of Mount Olympus in Grecian Meafure, as Xenagoras found it. Note, Each of thefe Furlongs is about rs of a German Mile. ARISTOTLE and feveral others affirm, that this Mountain, Olympus, is fo high, that there is no Rain, nor the leaft Motion of Air upon the Top of it ; which he, and the Ancients underftood By Article 14 ofCbaji. ji. from 122 *fbe Abfolute Part SECT. III. from their finding the Draughts of Letters made in Afhes, which had been regularly fcattered, to remain entire and frefh as they were at firft, with- out being either confufed or defaced in many Years , therefore they fuppofed it to be raifed a- bove the fecond Region of the Air. THERE is alfo another Method of taking the Altitude of Mountains, by two Stations in the fame Plane, with the perpendicular Height of the Mountain , but this is fubjedt to Error becaufe of the fmall Difference of the Angles (). ALSO () There is a very pleafant and expeditious Method of tak- ing the Height of Mountains by the Barometer, thus: It is to be obferved how many Inches or Parts of Inches the Quick- filver is deprefled at the Top of the Mountain, we have a mind to meafure, below the Altitude it hath acquired, at the fame Time, at the Bottom, or Su- perficies of the Sea; from whence the true Height of the Mountain is found by an efta- blifhed Proportion. This Pro- portion may be known by the Table we have added below to Chap. xix. Prop. 7- Alfo, by this Table, the Height of the Quickfilver at the Surface of the Sea may be feund, by obferving it's Height at any Place, whofe Altitude above the Sea is known. But this is to be obferved, that the Altitudes found this way will be more accurate, the near- er the Height of the Quickfd- ver is to 28 French Inches or Jurat* Appendix. This way of taking the Height of Mouxtainit is very expeditious and pleafant, as Dr Jurin faith, and with due care may be very ufeful to fe- veral purpofes; particularly in meafuring the Height of Iflands above the Sea, by two Obfer- vers, with well adjufted Baro- meters ; and at the fame Inftant of time, obferving the Baro- metrical Heights, by the Sea- fide, and on the higheft Part of the IJland. So alfo it may ferve to give an Eftimate of the Height of a Fountain, or Ri- ver, that we would have con- veyed to fome Miles Diftance. But in all thoi'e Experiments, it is neceflary that the Barometer (as I faid) mould be well ad- jufted, and (if two Obfervers) that the Obfervations mould be made at the fame time, to pre- vent errors that may arife from errors in the Barometer, or from the Alteration of the Weight of the Atmofpbere\ which fometimes changes in the very time of Obfervation, if we are not fpeedy therein. For the Diff every of a Moun- tain's, or any other, Height, Dr Halley (from Barometrical Obfeiva, CHAP. 9. of Univerfal Geography. 123 ALSO having the Height of a Tower given, and it's Diftance from the Mountain, we may more accurately find the Height, of the Mountain itfelf 5 thus, fuppofe F to be a Tower 300 Foot high, and from it's Top, or fome convenient Place, let BFP be obferved to be 83 degr. 30 min. then will BP be found to be 5796 Feet, to which the Height of the Tower is to be added : P A. PROPOSITION III. *The perfpicuous Altitude of a Mountain being given, tf find what Diftance we are from it ; by a Quadrant [Theodolite] or any other Surveying Inftrument, for taking Heights or Angles. LET the Height of the Mountain A B be known beforehand, by the Obfervations of others, to be 10 Grecian Furlongs 96 Feet, or 6096 Feet. And let the Place of Obfervation be at F ; (Fig. 13.) the Diftance FA is fuppofed to be required. Let the Angle BFA by a Quadrant or [Theodolite] be found 63 degr. 30 min. Then in the right- angled Triangle B A F, where three Things are given, it will be as the Radius 100000 is to the Tangent of the Angle ABF 26 degr. 30 min. 49858 : fo is AB 6096 to AF 3040 Feet, or 5 Furlongs Obfervations on Snowdm-Hill) with excellent Inftruments at concludes, that the Quickfilver divers Altitudes in St Paul's defcends a Tenth of an Inch, Dome, and when the Barometer every 30 Yards of A fcent. And was at a different Height, he Dr Derham (by good Obferva- found, at near go Feet, the tions on the Monu me nt in Lon- Quickfilver funk n>, and at don) reckons 82 Feet for every fomewhatlefs than double, and tenth of an Inch. Vid. Low- treble that Height, ,% and ,^, fborfs Abridg. Vol. 2. p. 13, according to Dr Halle fs Table, fcjV. But by very nice Obfer- ibid. p. 16, and Mr Cajfinfs yatipn? he aftef waf ds made referred to in this Note (b.) 40 Feet I 24 *fbe Abfolute Part SECT. III. 40 Feet, the Diftance required between the Place of Obfervation and the Mountain. THERE are fome Inftruments by which you may perform this, without making ufe of the Canon of Sines, &c. as is apparent from their De- fcription, but the Refult is this way lefs accurate, for Want of Exactnefs in the Lines of Propor- tion. Note. In both thefe Problems we have taken the Diftance FA for a right Line, becaufe of the fmall Difference between it and a Curve ; but mall confider it as Part of the Periphery of the Earth in the following Methods. PROPOSITION IV. Having the Dijlance between a Mountain and the Place where it's Top may be firft feen, given : to find Geographically the Height of the Mountain. L E T us take, for Example, the prodigious high Mountain in the Ifland ofTeneriff, one of the Canaries, commonly called the Pike of Tenerif. Let AFC. -(Fig. 14.) whole Center is R, be the Periphery of the Earth, or the Meridian of the Mountain, and let AB be the Mountain itfelf. Draw from B the right Line BF a Tangent to the Periphery, and F will be the firft or laft Point from which the Top of the Mountain can be feen. (Then Draw R F.) Mariners affirm, that they firft difcover the Top of this Mountain when they are 4 Degr. of the Meridian diftant from it (and they need not be at a lofs for finding the Diftance from any Mountain in Degrees when they are failing under the fame Meridian it is in). Therefore, fup- pofmg their Relation to be true, and the firft vifual Ray B F to come in a direct Line from the Top B, let us endeavour to find out the Alti- 2 tude CHAP. 9. ofUniverfal Geography. tude of the Mountain. In the Triangle BRF there are three Things known, i. RF the Semidiame- ter of the Earth. 2. The Right-angle BFR. And 3 . Becaufe the Arch F A is 4 Degr. the Angle B R F is alfo 4 Degr. Therefore fay, As the Ra- dius (100000000) is to the Secant of the Angle B RF 4 Degr. (10024419) fo is RF (3440 Italian Miles or 860 German Mifes) to RB (3448 Italian Miles or 860 German Milesj ; fubftract RA C344O or 86oj and there will remain BA (8 Italian Miles, or 2 German Miles, for the Height of the Moun- tain- \wbicb is extraordinary, and even above the Computations of the Antienti}. Therefore we muft know that there; are two Things affumed as Truths which are actually falfe. i . It is fuppofed that the Ray of Light which firft ftrikes the Eye, comes from B in a right Line, when it is known on the contrary to be curved, or refracted, by Reafon of the Denfity of the Atmofphere. For a Right Line cannot be drawn from the Top B to F (FA being 4 Degr.) without palling thro* a Part of the Earth, and therefore the Top B cannot be feen in a right Line from the Place F, but by the bowed Ray BTF, being the firft of the refracted Rays that can touch F. From whence we may reafonably infer, that this Refraction caufes the Mountain to be difcovered fooner by i Degr. (or 1 5 German Miles) than if there had been no Re- fraction at all ; fo that fuppofmg A F but 3 Degr; the Height of the Mountain will be found but 46 Furlongs, or 5 Italian Miles. 2. It is to be con- fidered, that Sailors allow themfelves a Liberty of fpeaking largely, efpecially about their Diftances ; if therefore, in Confideration of this, we deduct half a Degr. more, and fuppofe the Top firft feen jat 22. Degr. or 38 German Miles equal 'to F A ; then will the Altitude of the Mountain A B be ttfcwn'D found I 2 6 f&e Abfolute Part SECT. IIL found by the former Calculation to be a Mile, or thereabouts. I F a Mountain be firft feen at 2 Degr. diftance, (fetting afide the Refraction) it will be found 2 Italian Miles high ; but if at i Degr, or 15 German Miles, it will be half an Italian Mile/ or 5 Furlongs high* To this Purpofe is calculated the following Table t If the Altitude of \ L Ger. I A I a Mountain be 8 Mil. 7 BUT thefe are all to be underftood without Refraction, whereby the apparent Height and Diftance is generally increased, as may be feen by the Figure j where the refracted Ray T F being produced to N, gives the apparent Altitude N A. PROPOSITION V. Having the Altitude of a Mountain given, to find Geographically it's Diftance from the Place y whence it may be firft feen. >u';x>U: . --;^^:;; ;'.,! *Hl THIS is but the converfe of the laft Propofi- tion, and may be had from the foregoing Table : but Calculation will give a more accurate Solution. LET therefore A B be the Height of a Moun- tain given, and fuppofe it to be firft feen at F, to find the Diftance A F. (Fig. 14.) In the right an- gled Triangle B F R, the Angle F is a right An- gle, and the two Sides F R, R B are given, the former being the Semidiameter of the Earth, and the later the fame added to A B, which fuppofe half a German Mile 5 fo that R F or R A being 860 CHAP. 9. cfUniverfal Geography. 12 j 860 Miles, BR will be 86oz. Therefore fay, as R B 86o is to F R 860 : fo is the Radius 10000000 to the Sine of the Angle R B F 9994186. 88 degr. 2 min. 40 fee. Wherefore B R F or the Arch A F will be i. degr. 57 min. 20. fee. which being turned into German Miles make 291, the Diftance from whence a Mountain whofe Altitude is half a Mile, may be firft feen without any Refraction, upon which Account we may add 8 Miles, fo that it may be actually feen 37* Miles off. But the Refraction varies according to the different Altitude of the Sun, or the different Denfity of the Air, when the Sun, is below the Horizon ; as we mall mew more at large, when we come to treat of the Atmofphere ; and in the third Part of this Book, where we mall Difcourfe of the vifible Horizon. PROPOSITION VI. *jt ^Tbe Length of the Shadow of a Mountain, and the Altitude of the Sun at the fame Time^ being given, to fnd the Altitude of the Mountain. W E propofe this Problem more for the Anti- quity and Elegancy of it, than for any Accuracy we believe to be in the Method. Plutarch and Pliny have writ, that Mount Atbos, on the Mace- donian Shore, is fo high as that it overfhadoweth the Ifle ofLemnoSy [now c ailed Stalimene~] as far as the Market-place of the City of Myrrhina [or Lemnos], when the Sun is in the Summer Solftice ; where the ancient Inhabitants for the Curiofity of the Appear- ance erected a Brazen Calf, at the termination of the Shadow, as is teftified by the old Greek Mo- noftich, which may bt thus Engli/hed. 2 Mount 128 The Abfokte Part SECT. III. Mount Atho's Shadow covers half The Bulk of Lemno'j molten Calf, (c) . FLINT writes, that the Diftance between Atbos and the Ifle of Le mnos y was accounted 87000 Paces, or 87 Italian Miles, but neither he nor any other Author have determined the Altitude of the Sun, at the Time of this Shadow ; tho' it is pro- bable, it was projected upon the Town of Myrrhina when Mount Athos, a little before Sun-fet, began to intercept their View of the Sun-Beams , the Sun being then in the fame vertical Circle, which pafleth over Atbos and Myrrhina (becaufe Athos is fituated weftward of Myrrbina}. We may fup- pofe the Sun to have been almoft in the very Ho- rizon of Myrrhina F O, and fo the Ray O F, paf- fing the Top of the Mountain, to llave projected the Shadow AF. (Fig. 15). Here OF is a Tan- gent to the Periphery, and from having the Angle FB R given, and alfo FR, ("or FA in the Trian- gle, BAF taken as a right Line; B A will be found to be 8 Furlongs, or i Italian Mile for the Height of the Mountain. But becaufe in this Pofi- tion of the Sun, the Shadow would be infinitely continued, and therefore it's Extent could not be obferved ; and as the Interpofition of the Houfes in the Town, would alfo intercept the neighbour- ing Rays, to thofe that bounded the Shadow ; there- fore, we" muft allow the Sun to have been elevated at leaft 2 Degr. above the Horizon of Myrrbma j * 'A'.AyNx 1C /Ji^Tsrij . J tO'"A$f f KAX^ei :. *Mv S ft faw the Shadow of the Pike of htiuvist< fiobf. Tenerif upon the Sea reaching . Mr Salmon looks upon this to over the Ifland Camera, and the be a very ridiculous Aflertion, Shadow of the upper Part, viz. aiid tells us that there never was of the Sugar/oaf to be imprinted a Shadowdifcernableat lO'Miles like another Pike in the Sky it Diftance from the Hill that made felf. See Salmon's Prefent State it. But in Oppofition to this, of all Nat. Vol. 5. Pag. 396. and Mr Idem fays, that he aftually Pbilof. Tranf.N 345- Pag. 3 1 7. For C H A P. 9. of Um'ver/a! Geography. 129 For Example, to S ; fo that S F O may be 2 Degr. and S F a Ray of the Sun pafimg the Vertex of the Mountain T, and terminating the Shadow in F. THERE FORE in the oblique angled Tri- angle RFT, the Angle TFR 92 Degr. and F R T i degr. 6 min. (i. e. the Diftance F A 87 Ita- lian Miles, turned into Degr.) hence F T R 86 degr. 54 min. and alib the Semidiameter FR, 860 Ger- man Miles, being all given; the Side T R may be found by this Proportion. As the Sine of the An- gle F T R 86 degr. 54 min. is to the Sine of the An- gle T F R 92 degr. fo is FR 860, to JIT 861 Ger- man Miles. So that AT, the Altitude of Mount Athos, is i German Mile, -or 3 2 Furlongs, which is too much i for the Grecians account it not above ii Furlongs I F we aiTume the Altitude of the Sun to be but one Degr. the Altitude of the Mountain will be found but 20 Furlongs. BUT Pliny, I fuppofe, has given us too large a Diftance betwixt Atbos and Myrrbina, which may perhaps be a Reafon, that too great a Height arifes from this Calculation : and in moft of our modern Maps of Greece, the Diftance F A feems to be but about 55 Italian Miles ; wherefore the Angle FRT will be but about 55 min. So that fuppofing the Sun's Altitude to be i degr. 30 min. the Angle TFR will be 91 degr. 30 min. and FT R 87 degr. 35 min. Therefore in the Triangle FRT, as the Sine of the Angle FRT 87 degr. 35 min. is to the Sine of the Angle TFR 91 degr. 30 min. fo is FR 860 to RT. OR in the Triangle TFA right angled at A, TFA will be i degr. 30 min. and FA, fuppofed a right Line, 55 Miles, from whence the Height TA will be found by this Proportion. As the Ra- dius is to the Tangent of the Angle TFA, i degr. 30 min. fo is FA $5 Miles to AT, tte Altitude of the Mountain. VOL. I. K TO 1 30 The Abfolute Part S E c T. III. T O this Place belongs the Solution of this Pro^ blem, vifs. Having the difference of Time be- tween the Sun's rifing (or fettingj on the Top of a Mountain, and it's firft Appearance to (or Occul- tation from) an Obferver at the Bottom, to find, if required, the Height of the Mountain -, and con- verfly, having the Height of the Mountain, to find this difference of Time. Artftotle and Pliny, have, by this Method of Calculation, fuppofed fome Mountains to be of incredible Altitudes, as ap- pears from their Writings. However, fince the Solution of thefe Problems depends upon anodier, which we have referred to the fecond Part of this Work, we mail refer them to Chapter xxx. PROPOSITION VII. tfbe bigbeft Mountains have no fettfible Proportion to tbe Semidiameter of the' Earth ; or fo little, that their Altitude no more ajfefts it's Rotundity, than a fpeck or particle of Duft upon the Surface of tbe artificial Globe does it's Rotundity. ,~. J : r. 'J ; f. J t ' 'J. WE have mewed, that the Mountain in the Ifland of Teneriff, called tbe Pike, is at moft no higher than a German Mile, or a German Mile and a half; and we are affured, that there are but few Mountains in the World higher than that : There- fore fince the Earth's Semidiameter is 860 fuch Miles, the Altitude of this high Mountain is to the Earth's Semidiameter as i to 860. But few Moun- tains are of this Height, moft of them not exceed- ing a quarter of a .Mjle ; wherefore they -nq more obftract the Earth's fpherical Figure, than, the fmall inequality obferved in Globes turned artifi- cially, does their Rotundity 5 and Nature hath not i yet OT .1 .JCV C H A p. 9. of Univerfal Geography. 131 yet been able to produce a Body of an exad Geo- metrical Roundnefs (d). PROPOSITION VIII. 50 explain the Origin of Mountains. THIS is a great Queftion with fome Philofo- phers, but others think it fuperfluous, and not fit to be enquired into ; becaufe they fuppofe Moun-* tains to have had a Being ever fmce the Creation. Neverthelefs Hiftory acquaints us, that not a few Mountains have been undermined by interiof Ruins, and funk down into fubterraneous Chafms and Receptacles, or wafted by fome other Means ; fo that fmce we can perceive a natural Decay and Corruption of them, we may judge they do not proceed from a fupernatural Origin. Moreover, that feveral Mountains were raifed fuccc-flively, and at feveral Times, is apparent from the Quantities of Sea-lhells that are found in fome of them, as in thofe of Gelderland, &c. Such Mountains as thefe feem to be generated by a rapid Wind, carrying Sand and Gravel by Degrees into the form of the Moun- tain, which is afterwards foaked and made folid by the Rain. This is to be underftood in little Moun- tains, as to the very large ones it is probable, they (d)' Tho' the Body of the when flie is viewed thro' a good Moon be three times as little as Telefcope, we can fee the out- the Earth, and the Protuberan- ward Edge of her Disk notched ces or Mountains upon her Sur- and made rugged, by the Tops of face, three Times as high as the the Mountains rifing far above higheftupon the Earth's Surface; the other Parts of the Surface ; yet when me is at the full, and which need not feem ftrange, obferved with the naked Eye, when the beft polifhed Globe we cannot perceive that thefe that ever was made, being vaft Mountains in the leaft ob- viewed thro 1 a good Microf- ftruft, or deface her apparent cope, is found not to be free Rotundity. On th contrary, from fuch Rugofities. K 2 arc 132 *fbe Abfdute Part SECT. III. are of the fame Age and Origin with the Earth it- felf. They that argue more Theologically, fup- pofe the Globe of the Earth to have been at firft created perfectly round, and with a foft Surface, without any eminent Parts or Mountains, without any Fiffures or Grottos-, and afterwards, when GOD commanded the Waters to be gathered 'together in one Place, then there were Chanels made to receive the Waters, and the Earth that was remov- ed out of thefe Chanels, was converted into Moun- tains. But we leave it to them to prove, whether the Mountains be fo many, and fo large, as to fill all the Chanels of the Sea (*). PROPOSITION IX. To explain the Caufes, why Rain, Mifts, and Snows, are frequent upon the 'Tops of the Mountains ; when in the neighbouring Fallies, the Air is ferene and calm without any fuch Meteors. W E are informed by thofe, that have travelled over the Mountains of Afia, Peru, and other Coun- tries, (*) ' Dr Woodward, in his ' Efiay towards a Natural Hi- * ftory of the Earth, propofes ' to prove, that the Strata at * firft, whether of Stone, of Chalk, of Coal, of Earth, or * whatever other Matter they ' confiftcd of, (lying each up- * on other) were all originally ' parallel : that they were plain, ' even, and regular; and the ' Surface of the Earth like- ' wife even and fpherical : that * they were continuous, and ' not interrupted or broken : * and that the whole Mafs of * the Water lay then above I them all, and conftituted a fluid Sphere environing the whole Globe. That after fome Time the Strata were broken on all fides of the Globe : that they were dif- located and their Situation varied, being elevated in forne Places, and deprefied in others. That the Inequa- lities and Irregularities of the Terreftrial Globe, were cauf- ed by this Means : date their Original from this Difrup- tion, and are entirely owing unto it. That the more eminent Parts of the Earth, Mountains C H A P. 9. of Univerfal Geography. 1 3 3 tries, that while they were on their Tops, they were frequently attacked with Showers of Rain, Snow, and thick Fogs ; but defcending thence in- to the neighbouring Vallies, they obferved no fuch Meteors, but enjoyed a ferene arid pleafant Air. We alfo obferve the fame in the Mountains of our own Country. SOME fay, theCaufe of this Phenomenon is owing to an occult Power that Mountains have of attracting Air, Clouds, and other Meteors ; but fmce they cannot explain this Power, they fay nothing to the Purpofe (/). The following Ex- plication feems to me the moft rational, viz. That Vapours and Exhalations being condenfed into fmall Drops, in the middle Region of the Air, (into which the Tops of feveral Mountains rife) begin to defcend and fall upon the Tops of the fubjacent Mountains which are nearer them than the Vallies, and coming there firft to Ground, they leave their Places in the Air, which are prefently taken up by the fmall Drops that are next them ; thefe be- ing prefled and forced downwards by others, ei- ther to avoid a Vacuum, or becaufe it is the Na- Mountains and Rocks, are Agitation, and, in fome mea- only the Elevations of the fure, condenfed by Winds, or Strata; thefe wherever they other external Caufes, they ga- were folid, rearing jpgainft ther themfeves inro Clouds and and fupporting each other in Mifts, and by their own fpeci- the Pofture wherein they fie Gravity, fall downwards, till were put, by the burfting they meet with fuch Air as is or breaking up of the heavy and able to fupport them, Sphere of the Earth.' with which they mix and fwim Woodward's Eflay. Pag. 90, about, and are every way difper- 91, 92. fed in it, whereby the Sky is (f) The Air in Vallies is made ferene and clear : but if much heavier than the Vapours, they meet not with fuch Air, and therefore fitted to fupport or light upon the Top of a them better than that light Air Mountain before they come at which is upon the Tops of high fuch Air, then they are formed Mountains. Therefore when the into Drops, and fall down to yapours are put into a violent the Ground, K 3 tre 134 ft* Abfolute Part SECT. III. ture of Water to flow to the loweft Place, or to that Place where the Flux was firft begun. PROPOSITION X. tfbere happen to Mountains, Ruins, Ruptures, Tranf- pofitions, &c. I T is but feldom fuch Accidents happen, yet fome Inftances are found in Hiftory, -^ecially of Ruptures, whereof we fhall give lome Examples in the following Chapter. PROPOSITION XI. Whether the Superficies of a Mountain be more ca- facious than the Plane whereon it ft ands? T HAT it is larger is proved from Geometry : But whether it can fupport a greater Number of living Creatures, or produce a larger Quantity of Corn is another Queftion ; to which I anfwer in the Affirmative. For tho j every thing placed upon the Surface of the Mountain, is fuppofed to {land perpendicular to the fubjacent Plane, yet there is a greater Quantity of Earth, and a larger Superficies. CHAP. CHAP. 10. of Urn 'verfal Geography, 135 CHAP. X. Of the Difference of Mountains and their Ex- tent, and particularly of Burning Mountains. PROPOSITION I. Some Mountains are of fmall Extent ', and others run out to a great Diftance. H E latter Sort, called Ridges, or Chains of Mountains, are found almoft in every Country throughout the World ; and fuch might be account- ed one continued Mountain, if it were not for fmall Breaches or PafTages that fometimes intervene. They are indifferently extended feveral Ways ; fome from North to South, others from Eaft to Weft, and fome to other Points collateral to the four Cardinal ones. THE moft celebrated Ridges of Mountains are, i . THE Alps, which feparate Italy from the neighbouring Provinces, extending themfelves over vaft Tracts of Land, and ftretching out their Arms, or Branches, into distant Countries, viz. thro' France to Spain, where they are called the Pyreneans ; and thro* Rhcstia [i. e. the Country of the Grifons'] where they are called the Rhetian Mountains ; alfo thro* Hungary, where they are named the Hungarian Mountains ; and above Dal- tnalia, where they receive the Name of the Dal- matian Mountains i from whence they are ftretch- K 4 cd 136 ke Abfolute Part S E c T. III. cdthro* Macedonia into [Romama~] t and even to the Coaft of the Bla,ck-Sea. But becaufe there is in Dalmatia a confiderable Space between the dips and the Dalmatian Mountains, the former is reck- oned by fome to end here. Neverthelefs they fend out one continued Ridge, which pafleth, with a winding Courfe, in the Form of a Half-Moon, thro* the whole Length of Italy, and divides it into two Parts even to the Streights of [Meffina] ; tho* it does not run every where directly for- ward in one Tract, but here and there fends out collateral Branches that run fideways from it. Se- veral of thefe Mountains are diltinguiflied by par- ticular Names, by Reafon of their Altitude, or for fome other Caufe, as Monte Majfo, Gaurus, Monte di Capua , the burning Mount Vefu- vius, &c. 2. THE Ridge of Mountains in Peru [called the Andes] is the longeft in the World. They run in a continued Tract about 800 German Miles, (whereof 1 5 make a Degree) thro' all South Ame- rica^ from the Equator to the Streights of Ma- gellan, and feparate the Kingdom of Peru, from other Provinces. And fo high are the Tops of thefe Mountains, that they are reported to tire the Birds in their Flight over them -, there being but one only Paffage over them as yet difcovered, and that very difficult. Many of them are covered with perpetual Snow, as well in Summer as in Winter. The Tops of others are hid in the Clouds, and fome are raifed above the middle Region of the Air. Several of the Spaniards, with their Horfes, have fuddenly expired upon the Tops of thefe Mountains, in their PafTage from Nicaragua to Peru, and growing ftiff with the Cold, they, in a Moment, became immoveable d.s Statues. The Caufe of which feems to be no other than the Want of fuch Air as was fit for CHAP. 10. of Unfoerfal Geography. 137 for Refpiration. There are alfo found among this Ridge of Mountains feveralthat SLTQ fulf bureaus and fmoaking. 3. THERE are many other Ridges of Mountains between Peru and Brafil, which arc ftretched out thro* unknown Countries as far as the Streights of Magellan, where their Tops are cover- ed with continual Snow, tho' they lie in the La- titude of 52 Degrees. 4. TO thefe may be added the Ridges of Mountains in Canada , and New England, whofe Tops are alfo perpetually covered with Snow, tho* they are not fo famous as the reft. 5. MOUNT Taurus, in Afia, was antiently thought to make a Part of the largeft and nobleft Ridge of Mountains in the World. It begins to mew itfelf in the Leffer Afia near [the Gulpb of Slatalla], and runs from Weft to Eaft, under fe- veral Names, thro* divers large Kingdoms, and Countries, even to India , whereby all Afia is di- vided into two Parts, of which that on the North Side is called Afia intra Taurum, and that on the South, Afia extra Taurum. This Ridge is as it were fenced on either Side with feveral others that accompany it, among which the moft celebrated are the Greater and Leffer Antitaurus, which fepa- rate the Greater Armenia from the Leffer ; alfo where Taurus itfelf pafies between Armenia and Mefopotamia, it fends forth many Branches towards the North and South. 6. THE Mountain Imaus is extended North and South, and alfo Eaft and Weft, in the Form of a Crofs. The North Portion of it, is now called Alkai : It is ftretched out fouthward as far as the Borders of India, to the very Head of the River Ganges, and is computed in Length about 400 Ger- rntn Miles. It divides [Afiatic Tartary] into two Pans 138 The Abfolute Part S E CT. III. Parts, formerly called Scytbia infra fcf extra I- maiitn. 7. THE Mountains of Caucafus are about 50 Miles in Breadth, and extend themfelves length- way from the Confines of the Cafpian-Sea towards the Euxine-Sea. They are a fure Sea-Mark to thofe that fail in the Cafpian-Sea^ to fleer their Courfe by. An Arm of them reaches to Mount Ararat in Armenia, upon which it is faid, in Sacred Scrip- ture, the Ark of Noah refted ; and the 'Turks and Perfians will have it to be prefervcd there to this very Day. Ararat is alfo not far .from Mount Taurus, where all thefe Mountains are contiguous. We mail treat of the Height of Mount Caucafus in Chapter xxx. 8. T H E long Range of Hills in China, which comprehends the Damajian Mountains of the An- tients towards the Weft, and the Oltorocoran to- wards the North. This Range is compofed of a vaft Number of Mountains, not altogether conti- nued, but here and there affording a Paffage be- tween them. The Mountains of Cambodia feem al- fo to be a Part of this Range. 9. THE Mountains of AraUa are drawn out in three Ranks, whereof the holy Mount Sinai is a Part. 10. MOUNT Atlas, in Africa, is made famous by the innumerable Fictions of the Greek Poets. It's Rile is near the weftern Shore of Africa, from whence it ftretches itfelf to the eaftward as far as the Confines of Egypt. Moft of the Rivers in this Continent take their Rife from it -, and tho* it lie in the Torrid Zone it is cold and covered with Snow in feveral Places, 11. THE Mountains of the Moon, near Monotno- tapa in Africa, fendeth out feveral Branches, which furround almofl. all Monomolapa, and are diftin- guifhed by divers Names, as Zetb, \Gibel , Capb,"\ &e. CHAP. 10. ofUniverfal Geography. 139 &c. There are almoft innumerable other Branches in Africa, feparated one from another only by nar- row PafTages, infomuch that they all leem to be Parts of the fame Range of Mountains. 12. TYLE.Ripbean Mountains, in Europe, run from the White-Sea^ or Mufcovian-Bay^ to the Mouth of the River Oby ; from whence they are called fometimes -by that Name. The Mufcovites call them Weliki Kamenypoys, i. e. the great ftony Girdle ; becaufe they fuppofe them to encompafs the whole Earth. Near thefe there is another Ridge of Mountains, which the Ruffians call Joe- goria ; they reach from the South Borders of Tar- tary to the Northern Ocean. Several Rivers take their Rife from them, viz. Witfagda, Neem, Wiffera^ and Pelfiora. Thefe are none of them well re- prefented in Maps, and very often totally omit- ted. Alfo between Rujfia and Siberia there are, befides thefe, a triple Range of Mountains run- ning from North to South. The firft of thefe the Rujfiam call Cofvinfcoy Camen, which is two Days in palling over. The next to this (fome Vallies intervening) is called Cbirginfeoy Camen, which is alfo two Days Journey over. The third, being higher than the reft, is named Podvinfcoy Carney and in feveral Places is all the Year round co- vered with Snow and Fogs, fo that a PafTage is, with great Difficulty, obtained in four Days. The Town of Vergatena^ in Siberia, is near this Range. 13. [THE Dofrine Hills ,~\ which feparate Swe~ den from Norway, arife near the South Pro- montory of Norway, and proceed in feveral Ranges to the fartheft Part of Lapland, being al- fo diftinguifhed by feveral Names, as Fillefiel y Do* frefel, &c. 14. THE Hercynian Mountains in Germany now Fiechtelberg Mountains] furround Bohemia ; and 140 *fhe Abfolute Part SECT. III. and various Ways extend themfelves into divers Countries where they have different Names. In die Dukedom of Brunfuuic they retain fomething of their antient Name, being called Der Hark*, Mount Brufterus is a Part of this Ridge. PROPOSITION II. Inmofl IJlands, and Parts of tbe Continent that run out into the Sea, the Ridges of Mountains are fo fituated as to take their Courfe thro* the middle of them, and divide them into two Parts. I N Scotland the Grampian Mountain (or Granf- lain as the Inhabitants call it) runs from Weft to Eaft tho' the middle of this Peninfula ; and di- vides it into two Parts, which very much differ both in the Nature of the Soil, and the Inhabi- tants. So in the Iflands of Sumatra, Borneo, Lu- conia, Celebes, Cuba, Hifpaniola, &c. Chains of Mountains are found which arife gradually to a great Height, from the Sea-Shore to the Inland Parts. THUS die Mountain Gate, in India, begins at the Extremity of Mount Caucafus, and reaches to Cape Comorin ; whereby the Peninfula of India is divided, from North to South, into two Parts, whereof that Part which lies on this Side Gate, towards the Weft, is called Malabar ; and the other beyond the Mountain towards the Eaft is called Cormandel. Part of the fame Ridge of Mountains is alfo ftretched out into that Part of India which is now called Bengal, and from thence thro* Pegu 9 Siam, to the extream Parts of Malacca. THERE is the like Ridge of Mountains in the Peninfula ofCambaya, and in the Hand, or Peninfula, of California -, alfo in the procurrent Pans of Africa, there is a Ridge which reaches frorn CHAP. 10. of Uniwrfal Geography. 141 from the Morafs of Zaire to the Cape of Good-Hope. In Italy there are the Apennine Mountains j and the like in Corea^ &c. A S to the Origin of thefe Ridges, whether they are of the fame Date with the Earth, or were af- terwards generated from natural Caufes, is uncer- tain (a). PRO- (a) The learned Dr Wood- * ward, in his EfTay abovemen- ' tioned Page 280, proves, ' that there were Rivers as well ' as Sea in the Antediluvian * Earth, from the great quan- ' tides of River- Shells that were * then brought forth, and left in- clofed among others in the Strata of Stone, &V. And ' if there were Rivers, there ' muft needs alfo have been ' Mountains ; for they will not f flow unlefs upon a Declivity, ' and their Sources be raifed a- ' bove the Earth's ordinary Sur- ' face, fo that they may run ' upon a Defcent. Mofes alfo, ' treating upon the Deluge, ' faith in Gen. vii. 19. &c. * And the waters prevailed ex- f ceedingly upon the earth ; and ' all the high hi Hi that were * under the whole heaven were 4 (nvered. Fifteen cubits up- * ward, did the waters prevail t * and the mountains were tover- * ed. And all flejh died: * ell in whofe noftrils was the * breath of life. Here he ' plainly makes thefe Antedilu- ' vian Mountains the Standards ' and Meafures of the Rife of ' the Water ; which they could ' never have been, had they not * been Handing when it did fo f rife and overpower the Earth. ' His Intention, in the whole, ' is to acquaint us, that aH * Land Creatures whatever, Both Men, Quadrupeds, ' Birds, and Infefts, periihed, ' and were deftroyed by the ' Water ; Noah, only exceptcd, ' and they that were with ' him in the ark. And at the ' fame Time to let us fee the Truth and Probability of the * Thing: to convince us there was no Way for any one to efcape, and particularly that none could fave themfelves ' by climbing up to the Tops of ' the Mountains thatthenwere, * he affures us that they, even ' the higheft of them, were all ' covered and buried under ' Water. Now to fay that ' there was then no Mountains * and that this is meant of ' Mountains that were not for- ' med 'till afterwards, makes k ' not intelligible, and indeed ' hardly common Senfe/ Thus far Dr Woodward. But at the univerfal Deluge, the Mountains in general were de- faced, levelled, and diflblved, as it were, and promifcuoufly mix- ed with the Waters, which ran - facked and tore up their very Foundations, fo as to make one common confufed Mafs. There- fore thefe Mountains of our pre- fers I4Z fbe Abfolute Part SECT. III. PROPOSITION III. 30 enumerate the Mountains famous for their Height. i. THE Pike offencriff, which the Inhabitants call Pico de Terraira, is accounted the higheft Mountain in the World ; and it's Top is plainly perceived at Sea 60 Miles before we come up to it, as was faid in the preceding Chapter. There is no afceriding it but in the Months of July and jlugujl, for at other Times it is covered with Snow, tho* there is never any feen in the reft of the Ifland, or in the neighbouring Canaries. It's Top doth plainly appear to be above die Clouds, which are often feen to furround the middle Part v but becaufe it is ufually covered with Snow, it is certainly, not elevated above the middle Region of the Air. It requires three Days to afcend this, Mountain, whofe Vertex is not Iharp-pointed but plain ; from whence, on a clear Day, one may fee diftin&ly the reft of the Canaries^ tho* fome of them are fifty Miles remote from it. In the two Months abovemention'd great Quantities of ful- phureous Stones are dug out of the Side of this Mountain, and carried into Spain. Scaliger writes, that this Mountain continually vomited out burn- fent Earth, are not the fame juft as the fubfiding Waters with the Antediluvian Moun- happened to dafh out, or pile tains, but were formed at the up, their Particles, by wafhing Deluge, out of the confuied and hollowing their Sides, or Heaps of feveral forts of Mat- carrying the loofe and unfet- ter, which (when the Caufe of. tied Earth, towards the Drains the general Devaftation ceafed) and Sluices which were natu- began to curdle as it were, and rally formed to carry the Wa- fettle in innumerable Forms and ter downward to the Ocean. Shapes; fome extending them- How the Antediluvian Moun- felves into long Ridges, others tains were formed fee Chapter into round and rugged Shapes ; vii. Note (f) above. ing C H A p. I o. of Unherfal Geography. 1 4 3 ing Coals formerly (). I am ignorant from what Author he had it, and never found any fuch Thing in thole I have read. 2. I N one of the Azores , or weftern Iflands, near the Ifland Fayal, there is found a Mountain called the Pike of St George, from whence the Ifland itfelf is called Pico. It is faid to be as high as the Pike of Teneriff^ or fomething higher. 3. T H E Ridge of the Cordileras, or Andes, in South- America, which feparates Peru from other Countries, is one of the vafteft and higheft Moun- tains in the World. It is extended from the Streights of Magellan to Panama. 4. y TN A, a Mountain in Sicily ; when it caft- eth forth Fire the Sparks are feen from the Ifland of Malta, from whence it is fuppofed to be at leaft a [German] Mile high ; but that this is a Decep- tion of Sight we have Ihewed in the preceding Chapter. 5. HECLA a Mountain in Iceland.- 6. PICO de Adam in the Ifland of Ceylon. 7 . M O U N T Brufterus and Abnoba in Germany. 8. MOUNT Figenojamma in Japan is thought to reach above the Clouds. 9. MOUNT Caucafus was thought to be of an incredible Height by die Antients. : . -iHT ,M (b] It; is very likely this fine Brimftone, or Sulphur, Mountain might burn former- flicking to them. Alfo at the ly, for there is a Crater, or Bottom there are Stones which Tunnel, on the Top, that pro- fhine, and look like Drofs that duceth a fort of fulphureous comes out of a Smith's Forge; Earth, which, being rolled up which, without Doubt, was long-ways, and put to a Can- occafioned by the extream Heat die, will burn like Brimftone; of the Place they came from, and feveral Places upon the This is teftified by Mr Edens Ledges of the Pike are even who made a Journey thither in now burning or fmoaking ; and the Year 1715, which fee in in fome Places, if you turn up Pbilof. Tranf. No. 345. Page she Stoocs, you will find very 317. I0 . PELION 144 ?t> e dbfolute Part SECT. III. 10. PELION [now Petras] a Mountain in Macedonia. Pliny fays, that the Mathematician Dicearcbus Siculut meafured this Mountain by the Command, and at the Expence, of fome Princes, and found it to be 1250 Paces, that is io Fur- longs, or | of a German Mile : and Geminus tells us, that the fame Dicearcbus found the Mountain Cylltne to be of the fame Altitude. 11. MOUNT At bos was thought by Mela to be fo high as to rife above the highefl Clouds, and therefore never to be rained upon. This O- pinion had it's Rife from the Ames which were left upon the Altars, erected at the Top of it, being not warned away, but found upon a Heap as they had been left. It runs out with a long Ridge into the Sea. Xerxes, when he made his Expedi- tion to Greece, cut thro* this Mountain in that Place where it is joined to the Continent, and let the Sea in at the Breach, whereby it was made navigable. 12. MOUNT Olympus in leffer Afia, of which we have treated in the preceding Chapter. 13. CASIUS [now Lifon] a Mountain in A- fia y which is faid by Pliny to the four Miles high. 14. MOUNT Hamut [now Balkan] is faid by Martianus Capella to be fix Miles high. 15. THE Rock of Sifimetbra, Strabo tells us, was found to be fifteen Furlongs high ; and the Rock Sodiane twice the Height. 1 6. MOUNT Atlas in Africa, which we fpoke of before. The Poets feigned it fo high, that it fupported the Heavens upon it's Shoulders ; but Experience hath taught us that it's Height is not fo very confiderable. PRO- CHAP. 10. of Univerfal Geography. 145 PROPOSITION IV. 20 enumerate the remaining Differences cf Mo I N the former Proportions we have explained three Differences, viz. 1. SOME are extended in a long Tradt, o- thers are bounded with narrow Limits. 2. S OM.E run thro' the middle of Countries, others are extended here and there in them. 3. SO ME are of a remarkable Altitude, o- thers of a middle, and fome very low. To theie we may add, 4. S O M E are Cindy, others rocky, fome chalky, and others of Clay, &c. $. SOME produce Fountains and Heads of Rivers, others are without them. 6. S O M E are adorned with Woods, others are bare and deftitute of Trees. 7. S O M E are burning and fmoking, others without Fire or Smoke. -8. SOME Mountains yield Metals, as Gold, Silver, Iron, &c. others produce no fort of Metal. 9. S O M E are continually covered with Snow, others have none in Summer. PROPOSITION V, To enumerate the burning Mountain^ andfucb as caft out Fire. SUCH Mountains are called Vulcano^ a Name firft ufed by the Portuguese Sailors, and now they are commonly fo called. I . T H E moft famous of thefe is Mount Mtna y (now Gibel} in Sicily t whofe Erupticns of Flame VOL. I. L and 146 The Abfolute Part SECT. III. and Smoke are difcovered at a great Diftance, by thofe that fail on the Mediterranean^ even as far as the Harbour of Malta, which is 40 German Miles from the Shore of Sicily. Tho* Fire and Smoke are continually vomited up by it, yet at fome particular Times, it rages with greater Vio- lence. In the Year 1536 it fhook all Sicily, from the firft to the twelfth of May : after that, there was heard a moft horrible bellowing and crack- ing, as if great Guns had been fired : then were a great many Houfes overthrown throughout the whole Ifland. When this Storm had continued a- bout eleven Days, the Ground opened in feveral Places, and dreadful Gapings appeared here and there, from which ifiiied forth Fire and Flame with great Violence, which in four Days confumed and burnt up all that were within five Leagues of /Etna. A little after, the Funnel, which is on the Top of the Mountain, difgorged a great Quantity of hot Embers and Ames, for three whole Days together, which were not only difperfed through- out the whole liland, but alfo carried beyond Sea to Italy -, and feveral Ships that were failing to Ve- nice, at 200 Leagues diftance fufFered Damage (<:). Farellus hath given us an Hiftorical Account of the Eruptions of this Mountain, and fays, that the Bottom of it is i oo Leagues in Circuit. 2. HRCLA, a Mountain in Iceland, rages fome- times with as great Violence as Mtna, and cafts out great Stones. The imprifoned Fire often, by want- ing Vent, caufes horrible Sounds, like Lamenta- tions and Howlings, which make fome credulous People think it the Place of Hell, where the Souls of the wicked are tormented. (c) Mr QMenbcrge hath alfo na, which fee in Pbilof. Tranf. given us an Hiftorical Account, N. 48. Pag. 967. ef the Eruptions of Mount J5V- . -VESUVIUS CHAP. 10. of Univerfal Geography. 147 3. VESUVIUS (now Monte de Soma) in Cam- fama^ not far from the Town of Naples, tho* it be planted with mod fruitful Vines, and at other Times yieldeth the beft Mufcadd Wine ; yet it is Very often annoyed with violent Eruptions ( d ). Dion (d) That the Reader may have a better Idea of thefe turn- ing Mountains, and their dread- ful Eruptions, 1 Jkall tranfcribe (from Philof. Tranf. N. 354. Pag. 708.) an Extra ft of a Let- ter of Mr Edward Berkeley from Naples, giving an Account of the Eruptions of Fire and Smoke, from Mount Vefuvius. Communicated to the Royal So- ciety by Dr John Arbuthnot, M. D. and R. S. S. as follows: ' April if. 1 71 7. With much Difficulty I reached the Top of Vefuvius, in which I faw a vaft Aperture fullof Smoke, which hindred the feeing it's Depth and Figure. I heard within that horrid Gulph certain odd Sounds, which feemed to pro- ceed from the Belly of the Mountain ; a fort of Murmur- ing, Sighing, Throbbing , Churning, dafhing (as it were) of Waves, and between whiles a Noife like that of Thunder or Cannon, which was con- ftantly attended with clatter- ing, like that of Tiles falling from the Tops of Houfes on the Streets. Sometimes as the Wind changed, the Smoke grew thinner, difcovering a very ruddy Flame, and the Jaws of the Pan, or Crater, itreaked with red, and feveral fhades of Yellow. After an Hour's Hay, the Smoke being moved by the Wind, gave us fhort and partial Pro- fpefts of the great Hollow in the flat Bottom, of which I could difcern two Furnaces, al- moft contiguous; that on the left, feeming about 3 Yards in Diameter, glowed with red Flame, and threw up red hot Stones, with a hideous Noife, which as they fell back caufed the forementioned clattering. May 8. In the Morning I af- cended to the Top of Velui.*- us a fecond Time, and found a different Face of Things. The Smoke afcending up- right, gave a full Profpeft of the Crater, which as I cou'd judge, is about a Mile in Circumference, and a hun- dred Yards deep. A conical Mount had been formed fince my laft Vifit in the middje of rhe Bottom. This Mount I could fee was made of the Stones thrown up and fallen back again into the Crater. In this new Hill remained the two Mouths or Furnaces already mentioned : that on our left Hand was in the Ver- tex of the Hill, which it had formed round it, and rnged more violently than before, throwing up every three or four Minutes, with a dread- ful bellowing, a v.ift Num- ber of red hot Stones, fo,m- L 2 times 148 fbe Abfolute Part SECT. III. Dion Coffins relates, that in the Reign of Vefpafian^ there was fuch a dreadful Eruption of impetuous Flames, that great quantities of Afhes and fulphu- reous Smoke were carried not only to Rome by the Wind, but alfo, beyond the Mediterranean ^ into Africa^ ( times, in Appearance, above 1 1000, and at Jeaft 300, Foot 1 higher than my Head as I 1 flood upon the Brink. But ' there being little or no Wind, ' they fell back perpendicular- 1 ly into the Crater, increafing ; the conical Heap. The other 1 Mouth was lower in the Side of the fame new formed Hill, ; I could difcern it to be filled with red hot liquid Matter, 1 like that in the Furnace of a Glafs-houfe, which raged ; and wrought, as the Waves of the Sea, caufing a fhort a- brupt Noife, like what may be imagined to proceed from a Sea of Quickfilver, dafhing among uneven Rocks. This fluff would ibmetimes fpew over, and run down the con- vex Side of the conical Hill, and appearing at firft red hot, it changed Colour, and hard- ned as it cooled, {hewing the firil Rudiments of an Erup- tion, or, if I may fo fay, an Eruption in Miniature. Had the Wind driven in our Face, we had been in no fimll Danger of Rifling by the ful- phureous Smoke, or being knocked, on the Head, by lumps of molten Minerals, which we law hjd fometimes fallen on the Brink of the Crater, upon thofe fhot from the Gulph at the Bottom. But as the Wind was favour- able, I had an Opportunity to furvey this odd Scene for above an Hour and a half to- gether; during which it was very obfervable, that all the Vollies of Smoke, Flame, and burning Stones came only out of the Hole to our left, while the liquid fluff in the other Mouth wrought and over- flowed, as hath been already defcribed. June 5. After a horrid Noife, the Mountain was feen at Naples to fpew a little out of the Crater. The fame continued the 6 th . The 7 tJ >. nothing was obferved till within two Hours of Night, when it began a hi- deous bellowing, which con- tinued all that Night, and the next Day till Noon, cauf- ing the Window?, and, as fome affirm, the very Houfes in Naples to fhake. From that time it fpevved vaft Quantities of molten Stuff to the South, which ftreamed down the Side of the Moun- tain, like a Pot boiling over. This Evening I returned from a Voyage thro' dpulia, and was furprized, paffing by the North Side of the Mountain, to fee a great Quantity of ruddy Smoke lie along a huge Traft of Sky over the River of molten Stuff, which was itfelf C H A p. io. of Unherfal Geography. 149 Africa^ and even into Egypt. Moreover, Birds were fuffocated in the Air, and fell down dead upon the Ground, and Fifhes perifhed in the neighbouring Waters, which were made hot and infeded by it. There happened another Eruption in itfelf out of Sight. The 9 th , Vefuvius raged lefs violently ; that Night we faw from Na- ples, a Column of Fire moot between whiles out of it's Summit. The io th , when we thought all would have been over, the Mountain grew very outragious again, roaring and groaning moft dreadfully. You cannot form a jufler Idea of this Noife, in the violent Fits of it, than by imagining a mix'd Sound made up of the raging of a Tempeft, the murmur of a troubled Sea, and the roaring of Thunder and Artillery, confufed all together. It was very terrible, as we heard it in the further End of Naples, at the Diltance of above i 2 Miles. This moved my Cu- riofity to approach the Moun- tain. Three or four of us got into a Boat, and were fet afhore at Torre del Greco, a Town fituate at the Foot of Vefuvius to the South Weft, whence we rode four or five Miles before we came to the burning River, which was a- bout Midnight. The roaring of the Vulcano grew exceed- ing loud and horrible as we approached. I obferved a mixture of Colours in the Cloud over the Crater, green, yellow, red, and blue; there was Ukewife a ruddy difmal Light in the Air over that Tradl of Land, where the burning River flowed ; Ames continually fhowered on us all the Way from the Sea- Coaft. All which Circum- ftances, fet off and augmen- ted by tlie horror and filence of the Night, made a Scene the moft .uncommon and a- ftonifhing I ever faw ; which grew ftill more extraordinary as we came nearer the Stream. Imagine a vaft Torrent of li- quid Fire rolling from the Top down the Side of the Mountain, and \vith irrefilti- ble Fury bearing down and confuming Vines,. Olives, Fig-trees, Houies, in a word, every Thing that flood in it's Way. The largeft Stream feemed half a Mile broad at leaft, and five Miles long. I walked fo far before my Com- panions up the Mountain, a- long the Side of the River of Fire, that I was obliged to retire in hafle, the fulphure- ous Steam having furprizcd me, and almoft taken away my Breach. During our Re- turn, which was about three o'Clock in the Morning, we conftantly heard the murmur and groaning of the Moun- tain, which between whiles would burlt out into louder Peals, throwing up huge fpouts of Fire, and burning L 3 ' Stones, 1 50 7 he Abfolute Part SECT. HI, in Martial's Time, which he elegantly defcribes in one of his Epigrams, and laments the fad Change of the Mountain, which he faw firil in it's Ver- dure, and immediately after black with Ames and Embers. When the Burning ceafed, the Rain and Pew watered the Surface of the Mountain, and made thefe fulphureous Allies and Embers fruitful, fo that they produced a large Increafe of excellent Wine , but when the Mountain began to burn again, and to difgorge Fire and Smoke afrem (which fometimes happened within a few Years) then were the neighbouring Fields burnt up, and the High-ways made dangerous to Travellers. 4. A Mountain in Java, not far from the Town of Panacura, in the Year 1586, was mattered to Pieces by a violent Eruption of glowing Sulphur, (tho s it had never burnt before) whereby (as it was reported) i oooo People perifhed in the underland Fields : it threw up large Stones, and caft them as far as Pancras, and continued for three Days to throw out fo much black Smoke, mixed with Stones, which falling down ag:.in, re'embled the Srars in our Rockets. Sometimes I observed two, at others three, diilinfl Columns of Flame, and fometimes one vaft one, th.u feemetl to fill the whole Crater. Thefe burning Co- lumns, and the fiery Stones, feemed to be fhot 1000 Foot perpendicular above the Sum- mit of the Vuhano. The \ i^ at Night, I ohferved it from a Terrafs at Naples, to throw up incefiantly a vatt Body of Fire and gre.it Stones, to a furpr.'fing Height. Thei2 tf ? in the Morning, it darkened the Sun with Afh.es and Smoke, caufing a fort of E- clipfe. Horrid Bellowings, this and the foregoing Day, were heard at Naples, whi- ther Part of the Afhes alfo reached. Qn the 13 th , the Wind changing, we law aPil- hr of black Smoke fhoot up- right to a prodigious Height. The 1 5 th in the Morning, the Court and Walls of our Houfe in N.ipks were covered with Afhes. In the Evening, Flame appeared on the Moun- tain thro' the Cloud. The 1 7^, the Smoke appeared much di- minifhec!, fat and greafy. The i8' h , the whole Appearance ended, the Mountain remain- ing perfectly quiet without a- ny vifible Smoke or Flame.' Flame C H A P. I O. of Umverfal Geography. 1 5 1 f Flame and hot Embers, that it darkened the Face of the Sun, and made the Day appear as dark as the Night. 5. MOUNT Gonnapij in one of the Band* Iflands, when it had burnt for 1 7 Years together, in April 1586, broke out with a terrible bellowing Noife, anddifgorged fuch large Quantities of great Stones, and thick fulphureous burning Matter all over the Sea and Land, that it threatned Deftru- ftion to all that were near it. Hot Ames and Em- bers were vomited out with fuch a Force, and in fuch great Quantities, that they covered the great Guns of the Dutch, which were planted upon the Walls of their Citadel, and rendered them unfer- viceable. Red hot Stones above a Span long, were caft into the Sea, and fuch a Number of little ones, that fmall Ships had fcarcely a free Pafiage out of the Harbour. The Water near the Shore was heaved up, and feemed to boil for feveral Hours, as if it had been fet over a Fire ; and feveral dead Fifties were found floating upon die Surface. 6. MOUNT Balaluanum in Sumatra^ vomi- teth Flame and Smoke as ^Etna doth. 7. T H E Ground in feveral Places in the Mo- lucca Iflands belches out Fire with a raging Noife -, but none are fo terrible as the Spiracle in the Ifland Ternata. The Mountain, which is fteep and difficult to afcend, is covered towards the Bottom with thick Woods, but the Top which is .elevated to the Clouds, is made bare and rugged by the Fire, The Funnel is a vaft Hollow, which goes fhelving down, and by Degrees becomes lefs and lefs, like the infide of an Amphitheatre , from whence, in Spring and Harveft Time, or about the Equinoxes, when fome particular Winds blow, ffpecially from the North, there are caft forth, with a rumbling Noife, Flames mixed with black L 4 Smoke, I ^2 be Abfolute Part SECT. III. Smoke, and hot Embers , whereby all the Places far and near are ftrewed with Ames. The Inhabi- tants vifit it at fome certain Times of the Year, to gather Sulphur, tho' in fome Places the Hill can- not be afcended, but t>y Ropes faftned to Iron Hooks. 8. There is an Ifland about 60 Leagues from the Moluccas^ (being one of thole that belong to the Moors] which is often all together fhaken with Earthquakes and Eructations of Fire and Ames in abundance } fo that whole Rocks and Mountains are often made red hot by the Heat of the fubter- raneous Fire, and burning Stones are blown up in- to the Air, as large as the Trunks of Trees. When there is a brifker Wind than ordinary, fuch Clouds of Ames are blown all over the Country, that People labouring in the Fields are forced to haften Home, half covered with them ; and Boars, and other living Creatures, are found buried in them, after the Storm is over. Fifhes near the S'ja Shore are poifoned with the Ames, and Ib are the Inhabitants if they tafte any of the Water wherewith they are mixed. This difafterous black and poifonous Fire breaketh out, from the Top of a Mountain, with a difmal rumbling Noife like Thunder-claps, or the report of great Guns, and bringeth up with it abundance of Ames, and burnt Pumice Stvnts. 9. THERE is a Mountain injapan^ which continually vomiteth forth Flames ; where it is re- ported the Devil mews himfelf, farrounded with a bright Cloud, to fome particular Perfons after they have, for Performance of their Vows, kept themfelves lean for a long Time. 10. THERE are feveral other Vulcanos in the Japan Iflands -, about feventy Miles from Fi- randv there is one, and in a fmall Ifland between Tanaxima and the Seven Sijien (Iflands fo named) there CHAP, i o. of Umverfal Geography. 153 there is another, which now and then is obferved to burn, and at other Times to fmoke. 11. NEAR the Cape Spirit u Sanfto in landa^a^ one of the Philippines, there are found fome fmall Vulcanos , and one in Marinda, which is a Part of the faid Iflands. 12. IN Nicaragua a Province of America, thirty Leagues from the Town of Leon, there is a Moun- tain, of a vafl Height, which difgorgeth fuch quantities of Flame, that they may be perceived at ten Miles diilance. 13. IN the Peruvian Range of Mountains (called the Cordilleras] there are in feveral Places burning Rocks and Mountains, fome vomiting Fire and Flame, and others fmoaking ; eipecial- ly thofe in Carrapa a Province of Popaiana, which are perceived in clear Weather to emit a deal of Smoke. 14. NEAR Arequipa, a Town in Peru, about ninety Leagues from Lima, there is a Moun- tain which continually vomits fulphureous Fire, which, the Inhabitants are afraid, will fome Time or other burft and overthrow the Town adjacent to it. 15. IN Peru, near the Vale called Mulahallo 9 about fifty Leagues from Quito, there is a Vulcano, or fulphureous Mountain, which, fome Time fince, burft and threw out great Stones, with a dreadful Noife, which frighted People even at a great Di- itance. 1 6. I N one of the Iflands called Papons, which La Maire difcovered (tho 5 perhaps it be not an Ifland, but is joined to the eaftern Shore of New Guinea} there is a Mountain which, at that Time, burnt and fmoked. 17. THERE are feveral Mountains fas the ites tell us) in the Country of the Ton-Gvi- fins, 1 54 Th* Absolute Part SECT. III. fas, upon the Eaft of the River Jenifer fome Weeks Journey from the River Oby, wliich pro- duce Vulcanos and fmoking Mountains. 1 8 . THERE are alfo fome of this fort near the River Pefida beyond the Country of the Ton- Gui/ins. 19. THERE is a Mountain in Fez, called Beni-Gua-zeval, which hath a Cave in the Side of it, that vomiteth out Fire, 20. IN Croatia, not far from the Sea- Shore near the Town of Apolknia, there is a rocky Mountain, from whole Top there often breaks out Fire and Smoke , and, in the adjacent Places, feveral of the Springs are hot. THERE are alfo fome Mountains which have left off burning ; fuch as that in the I (land Queimoda upon the Shore of Brafil, not far from the Mouth of the Silver River, or Rio de la Plata, which burnt formerly, but now ceafes. Likewife the Mountains in Congo or Angola ; alfo thofe in the Azores (efpecially in Tercera and St Michael) which ufed formerly to burn in feveral Places, but at prefent only emit, now and then, Smoke and Vapours -, whence they are annoyed with more frequent Earthquakes. The Iflands of St Helena and Afcenfton produce Earth which feems to be compofed of Drofs, Afhes, and burnt Cinders ; Co that in Time paft it is probable the Mountains in thefe Iflands burned , and further, becaufe in thefe, as well as in the Azores, there are found iulphureous Earths and Slags, like die Recrements of Smithy Coal, which are every Way fit to take Fire, and make Smoke ; it will be no wonder if ew Vulcanos mould, fome Time hence, be kind- led and break forth in thefe Iflands ; for the Caufe of thefe burning Mountains is a fulphureous and bitumi- C H A P. I o. of Univerfal Geography. bituminous Matter, which is contained and kind- led in them (*). (e) Earthquakes and Vulca- nos are both produced from the fame Caufe ; which may be thus explained. Thofe Countries which yield great ftore of Sul- phur and Nitre, or where Sul- phur is fublimed from the Py- rites, are by far the moft inju- red and incommoded by Earth- quakes; for where there are fuch Mines they muft fend up Exha- lations, which meeting with fub- terraneous Caverns, they muft ftick to the Arches of them, as Soot does to the Sides of our Chimnies, where they mix themfelves with the Nitre or Saltpeter, which comes out of thefe Arches, in like manner as we fee it come out of the In- fide of the Arch of a Bridge, and fo makes a kind of Cruft, which will very eafily take Fire. There are feveral ways by which this Cruft may take Fire, viz. I . By the inflammable Breath of the Pyrites, which is a kind of Sulphur that naturally takes Fire of itfelf. 2. By a Fermentation of Vapours to a degree of Heat, equal to that of Fire and Flame. 3. To the falling of fome great Stone, which is undermined by Water, and ftriking againft ano- ther, produces fome Sparks which fet Fire to the combufti- ble Matter that is near; which, being a kind of natural Gun- Powder, at the Appulfe of the Fire, goes oft" (if I may fo fay) with a fudden Blaft or violent Explofion, rumbling in the Bowels of the Earth, and lift- ing up the Ground above it, fo as fometimes to make mife- rable Havcck and Deftrudion, 'till it gets Vent or a Difchargc. Burning Mountains and Vulca- nos are only fo many Spiracles ferving for the Difcharge of this fubterranean Fire, when it is thus preternaturally affembled. And where there happens to be fuch a Structure and Confor- mation of the interior Parts of the Earth, that the Fire may pafs freely and without Impedi- ment from the Caverns therein, it aflembles unto thefe Spiracles, and then readily and eafily get* out, from Time to Time, with- out fhaking or difturbing the Earth. But where fuch Com- munication is wanting, or the Paffages not fufficiently large and open, fo that it cannot come at the faid Spiracles without firft forcing and removing all Ob- ftacles, it heaves up and mocks the Earth, till it hath made it's Way to the Mouth of the Vul- cano; where it ruftieth forth, fometimes in mighty Flames, with great Velocity, and a ter- rible bellowing Noife. See Woodwards E/ay Page 157, 158. Robaufrs Pbyjtfs Pa rt 3 . Chap. 9. S>#. 23, 24. Pbilof. Vranj. NO 157. Pag. 512. 156 T&e Abfolnte Tart SECT. III. j * - >-*-. i, ,- ' |i n toi-Mf? PROPOSITION .VI. Some Ranges of Mountains afford no Apertures, as ctfars afford many , and fame are difcontinued but in one or two Places. THESE Streights, or PafiTages, were for- merly called fbffmopylee, of which the moft fa- mous are, i . The ttermopyltg of Mount Oeta [or Banina] in VbtJ/alia, [now called Bocca de Lupo] which gave Name to the reft. 2. The Cafpian Streights, thro' which there is a Pafiage between the Cafpian Mountains. 3. The Pafiage thro' the Ridge of the Cordilleras in Peru. 4. The Paffage thro' the Mountains on the Weft-fide of the Ara- lian Gulph, by which Merchandize is carried from Aty/mia into Arabia. 5. The two PafTages thro* Mount Caucafus, &V. PROPOSITION VII. When a Mountain rum out into the Sea, or feems \to Mariners'] to overtop the reft of the Country , it is called a Promontory, Cape, or Head-land. 3he mojl famous are, 1. THE Cape of Good Hope at the extream Point of Africa, which muft be doubled by thofe that fail into India. 2 . CAPE Viftory at the further end of the Streights of Magellan. 3. CAPE Verd^ the moft weftern Point of Africa^ where the Coaft begins to wind towards the Eaft, 4. CAPE Vincent in Spain. 5. T H E Promontory of Atlas was, fome Ages ago, called a Head-land by Mariners, be- caufe they fuppofed it unpaffable, or that if any failed CHAP. io f ofUmverfal Geography. failed beyond it they could not return fafe ; where- fore it was the utmoft Bound of their Navigation on the African Coaft. Other Promontories may be feen in Maps. PROPOSITION VIII. To Mountains are oppofed Chafms, deep Pits, and Caves, -which are found in feme Places of the Earth. THERE is a flinking fulphureous Cave in Ireland, which was formerly very famous, now called St Patrick's Purgatory ; and in Italy there is that called Grotto, del Cane (/). Leo Africanm mentions one which emits Fire on a Mountain in Fez, called Beni-gua-zeval. I N Bardefay, an Ifland adjacent to the Princi- pality of Wales in Britain, there is a Rock near the Sea in which there is a Cave, unto which if you apply your Ear, you will hear the Strokes of a Hammer, the blowing of Bellows, and the riling of Iron, as if it were in a Smith's Shop. NOT far from the Town of BeJJe in Aquitain* there is a Cave, called by the Natives Du Souley* in which there is heard a Noife like Thunder in the Summer Seafon. I N fevend Places there are found among Mountains, Vallies of fuch a prodigious Depth, that they ftrike the Beholders with Horror, and caufe a Giddinefs in the Head. (f) See Stur mius Pbilof. pours which would otherwi r e, Exercit. II. de Terra Mot. being imprifoned, occafion fre-' Cbnp. 3. where fome of themoft quent Succuffions, and dreadful eminent Specus's are enumera- Convulfions of the Earth. Set ted, and lome of their Ufes, the Note above. And for more viz- that they ferve for Spiracles to this purpofe, fee the Pbilo- and Funnels to the Countries fopbical Tranfaftions, and French where they are to vent and Memoirs: fa/Jim. difcharge the Damps and Va- CHAP. 158 The Abfolute Part SECT. III. CHAP. XI. Of Mines, Woods, andDefarts. MINES, Woods, zndDefarts, make feveral Tracts of the Earth remarkable, of which, tho* but little can be faid, yet it will not be unne- ceflary for the more perfect Knowledge of the Parts of the Earth's Superficies, to confider thefe Places, and to trace out their Situations , which we lhall briefly do in this Chapter. PROPOSITION I. Mines are Places in the Earth, out of which Metals^ Minerals, and other Kinds of Earth are dug. S O many different Kinds of Foflils as there are, fo many various Names have their Mines, viz. Gold- Mines, Silver-Mines, Copper -Mines, Iron- Mines, Coed-Mines, Salt-Mines, and fuch as produce Gems, &fr. THE moft celebrated Gold and Silver-Mines, are. i . T H O S E of Peru, and Caftetta del O0,which are the richeft in the World, yielding Gold and Sil- ver in abundance, and not being deftitute of other Metals ; infomuch that the Natives of Peru, and the Spaniards uied to boaft, that this Kingdom was founded upon Gold and Silver, Girava, a Spanijb 1 Writer CHAP. 11. of Umverjat Geography. Writer affirms, that there were formerly Mines about the Town of Quijo, which produced more Gold than Earth. And when the Spaniards made their firft Expedition into this Golden Country, they found feveral Houfes, efpecially in the Regal City Cufco, which were all covered over within and with- out with Plates of mafTy Gold. And the Officers of the Peruvian Forces, not only wore Silver Ar- mour, but all their Arms were made of pure Gold. The moft rich and advantageous Mine of Silver is in the Mountains of Potofi, where 20000 Work- men are daily employed to dig it, and carry it up at leaft 400 Steps. Thefe Mines produce that vaft Quantity of Gold and Silver, which the King of Spain receives out of America every Year, to the Mortification of other Kings and Potentates , and which, he therefore keeps fortified with ilrong Forts and Garrifons. 2. T H E R E are excellent rich Mines of Silver in the Japan I (lands, whence they are called by the Spaniards, the Silver Iflands. There are alfo fome Mines of Gold found there , but thefe are not fo rich as formerly. 3. THERE were more plentiful Gold-Mines formerly in Arabia, than at prefent. 4. I N the Mountains of Perfia, and in China, there are fome Silver-Mines. 5. I N Guinea there are feveral Mountains, that produce Gold, but they are remote from the Shore, and the Gold-Duft that is brought from thence, is not dug out of the Ground , but gathered up and down by the Natives. Their in- land Kings are how- ever faid to poffefs each his Mine, the Product of which he fells to the Neighbouring Merchants, and they again to others, till it reaches the Sea-Shore, where it is exclianged with the Europeans, .6. IN 160 The Abfolute Part SECT. Ill; 6. I N Monomotapa, there are found rich Mines of Gold and Silver, and alfo in Angola, both which are thought to be Parts of one continued Vein. 7. G E R MA NT excels the reft of the King- doms of Europe for plenty of Mines, of which fome produce fmall Quantities of Gold, others abundance of Silver, and a great many of them Copper, Iron, Lead, Vitriol, Antimony, &c. about which confult the Descriptions of Germany. 8. SWEDEN 'is enriched with the beft Cop- per-Mine of any hitherto difcovered ; it is in a vaft high Mountain, which they call Kopperberg, out of which as much Copper is dug as makes up a third Part of the King's Revenue. Here are alfo Iron-' Mines, and fome Silver- Mines, but they fcarcely defray the Expence of digging them. 9. THERE are Mines of precious Stones found in the Ifland of Ceylon, and alfo in Congo ( where there is a Silver-Mine, and fo much Marble, that the Earth under Ground is thought to be all Mar- ble ) and in Peru, about Portovejo in Smaragdina ) and in Guiana, near the Coail of which there is a fmall Ifland, called St Maria, which yields abun- dance of Gold , even i oo Pound Weight every Year, if we may believe the Dutch. In the King- dom of Golunda , there is a Mine which yieldeth precious Stones , particularly Diamonds in abui> dance, but it is not now dug. i o. I N Chili, there are Mines yielding Gold, Sil- ver, and Gems, but the warlike Inhabitants, fet- ting more by Iron Weapons than Gold or Silver, have partly killed, and partly driven away the Spa- niards , and demolifhed the Mines that were but newly begun. ii. THE Ifland Madagascar abounds in Iron and Tin, with a moderate Quantity of Silver, a little Gold, but no Lead. Wherefore the Natives value Lead Spoons above Silver ones. 12. IN C H A p. 1 1 . of Umverjat Geography. 1 6 1 12. IN the Ifland of Sumatra, it is reported, that there are rich Mines of Gold, Silver, Brafs, and Iron ; and that the King in one Year (viz. 1 62p ) received into his Treafure 1000 Pound Weight of Gold. 13. I N the Philippine Iflands, and in Java, Hi- fpaniola, Cuba, and others ; there are found Mines of Gold, Silver, Copper, and Iron : and in the Mountains of Siam there is got Gold, Silver, and Tin. 14. THERE are Mines of Salt in Poland at Pocb- nia, four Miles from Cracow ; ( where huge Lumps of tranfparent white Salt are cut out of the Ground) in Tranfifaania, in the County of 'Tyrol in Spain, in Leffer Afea, and in Places near the Cafpian Sea, not far from the River JVolga , over-againft the Ifland Kiftowat, where the Ruffians dig their Salt and boil it to a more pure Subflance, and after tranfport it to all Parts of Ruffia, Jn Cuba, there is a whole Mountain of Salt. All the Mountains in the Ifland of Ormus, at the Mouth of the Perfian Gulph, are of Salt, which may be gathered in any Part of them, in fuch great Quantities, that the very Walls of their Houfes are built of cryftalline Salt. In a Valley in Peru, about eighteen Miles from Lima to the North- ward , are found deep and large Pits of Salt, where every one may take away what Quantity he pleafes, beeaufe it continually increafeth, and feenv eth impoflible to be exhaufted. In Africa there is no other Salt ufed, but fuch as is dug out of Pits, or Quarries, like Marble, of a white, greenifh, or Afh, Colour. All India fetch their Salt from the great Salt-Mines of Bagnagar in Cormandel, &c. We fhall treat of Salt-Springs in another Chapter. VOL. f, M PRO- 162 fbe Abfolute Part SECT. III. PROPOSITION II. A Wood is a multitude of Trees extended over a large IraEt of Land, which fpring up without planting, and grow without being cultivated. S EVE R A L Woods produce only one fort of Trees, from which they receive their Names ; fo that as there is a great Variety in Trees, there is alfo the fame in Woods, viz. Palm Woods, Oak Woods, Ofier Woods, Beech Woods, &c. Groves and Forefts, are alfo thus diftinguifhed. Divers Coun- tries, especially thofe more remote, produce diffe- rent Sorts of Woods. In Africa, about Cape Verd, there are whole Woods of Lemon and Orange- Trees, which the Sailors may pluck for a very fmall Matter. In France, there are whole Woods of Chefnut-Trees : In Ceylon there are Woods of Trees, whofe Bark yieldeth Cinnamon : In the Mo- lucca Iflands, there grow Clove-Trees : In the Ban- da Iflands, there groweth plenty of Nutmegs : In Brazil there groweth a hard fort of Wood, which we call Brazil Wood : In Africa, efpecially in Nu- midia, there grow Grapes, of which are made Rai- fins of the Sun : In the Ifland Madagafcar, and in other Places of India, there are Trees which bear Tamarinds : In Mount Lebanon there are Cedars, and whole Woods of them in Japan ; of which they make Marts of Ships. In Spain, France, and Italy , there are whole Woods of Olive and Myrtle Trees. In Germany there are Woods that produce Fir, Oak, Alder, Beech, Pine, Juniper, Maple, Po- plar, Am, and Elm. THE moft noted Woods are, the Hercynian Foreft, which formerly overfpread almoft all Germany, and at this Day taketh up large Tracts of Land in feveral Countries, and under feveral Names. The C H A p. 1 1. of Univerfal Geography. 163 The ancient Caledonian Wood in Scotland, with feve- ral others in other Countries ; efpecialJy in Nor- way, where there grow more large Trees than in any other Country, and from whence all Europe procures Mafts for their Shipping. Lithuania is alfo overfpread with Woods, and Forefts ; ; from whence large Taxes are raifed for the King of Po- land. PROPOSITION .III. Defarts are vaft Drafts of Land uninhabited by Men. THESE are of two forts, fuch whofe Soil is barren and unfruitful, properly called Defarts; and fuch whofe Ground is fertile enough, but are never- thelefs faid to be defart, becaufe they are unculti- vated by Men. In Mufcovy, and in Places near the Cafpian Sea, along the Banks of the Wolga , there are large Tracts of fertile and fat Meadow Ground, which lie defart and uncultivated -, in the former Place, by reafon of it's Plenty, and the Lazinefs of the Inhabitants : And in the later, by the Wars of Tamerlane, when thefe Countries were laid wafte, and depopulated. But fuch as thefe are impro- perly called Defarts. THERE are four kinds of Defarts (properly fo called) viz. fandy Defarts, marjhy Defarts, ftony Defarts, and heathy Defarts ; which laft produce Woods and Forefts in feveral Places, and are more ufeful and eafy to be cultivated. i . THE Defarts of Africa are almoft all fandy, and there is not any part of the Earth fo much over-run with Defarts. Thofe in Libya furround all Egypt; and are accounted the largeil upon Earth. M 7. 2. THE 164 The Abfilute Part SECT. III. 2. THE Defarts of Arabia, are fomeofthem fandy, and others ftony : the greateft is vulgarly called the Sand-Sea. 3. THE Defarts about the Mountain Imaiis. The fandy Defart of [Kama] in Mongul, where the rich Kingdom of Catbaia formerly was (tho ? falfly) fuppofed to be. 4. THE Defarts of Cambodia. 5. THE rocky Defarts of Nova Zembla. 6. T H E Defarts of Norway, Lapland, Sweden, and Finland. 7. T H E Defarts of Germany, are all Heath -, hence thofe in Lunenburg, are called Lunenburg- tJeath, &c. SECT. CHAP. 12. ofUniverfal Geography. 165 SECT. IV. Containing HTDRO GRAPHT-, which is explained infix Chapters. CHAP. XII. Of the Divifion of the Ocean by the Interpofition of Lands. HA V I N G treated of the Divifion of the Earth > and it's Parts, in the foregoing Chapters ; Order requires that we alfo confider the Situation and Divifion of the WAFERS , which make the other Part of the Terraqueous Globe , and explain fuch of their Properties as belong to Geo- graphy. I N the fecond Propofition of Chapter vii. we divided the Waters into four Species, viz. i . The Ocean and Seas. 2. Rivers and frefh Water. 3. Lakes and Marines. 4. Mineral Waters. In this Chapter we fhall Difcourfe of the Divifion of the Ocean. PROPOSITION I. The Ocean, in a continued Extent, encompajjeth the whole Earth, and all it's Parts, nor is it's Superficies any where interrupted, cr altogether broken by the inter pofed Earth ; only a larger Traft of Sea, or a wider Communication is in fame Places wanting. THE Truth of this Propofition cannot be proved but by Experience, which is chiefly gained M 3 by 1 66 Tke Mfolute Part SECT. IV. by failing round the Earth, which hath been often attempted and happily accomplimed ; firft by the Spaniards under Capt. Magellan, who firft diicove- red the Streights, called by his Name ; then by the Englijh, viz. by Sir Francis Drake, Sir Thomas Ca- vendijh, and others , after by the Dutch, &c. THE Antients never doubted that the O- cean was .thus continued , for they fuppofed the old World to be raifed above the Waters , and every where furrounded thereby (and fome of them thought it floated). But when America was dif- covered (which is extended in a long Tract from North to South, and feems to hinder tjie Conti- nuation of the Ocean ) and alfo the Arctic and Antarctic Continent, then they began to think o- therwife ; for they imagined, that America was join- ed to fome Part of the South Continent ( which was not unlikely ) in like Marnier as moil of our modern Geographers, fuppofe that North America is joined to Greenland. If both thefe Conjectures had been true, then indeed the Ocean had not en- compafled the whole Earth. But Magellan removed all Doubts and Scruples about it, by difcovering, in the Year 1520, the Streights between America and the South Continent, which join the Atlantic to the Pacific Ocean. What therefore the Antients hap- pened to ftumble upon, by a wrong way of ar- guing, we have found out to be a real Truth by Experience. The fame may be faid about Africa ; for the Antients, without any Hefitation, fuppofed it to be bounded to the Southward by the Ocean, and not to be extended fo far beyond the Equa- tor, as it really is , but when the Portuguese had fail- ed along the weftern Coaft of Africa, and found it to be extended a great way beyond the Equator, it was queftioned whether Africa could be failed round ( fo far as to afford a PafTage to India ), that is, whether Africa was extended Southward or encom- C H A P. 1 2 . of Univerfal Geography. 1 67 encompafled by the Ocean. But this Doubt was alfo removed by Vafco di Gramma -, who, in the Year 1497, firft failed round the moft fouthern Promontory of Afric, called, 'The Cape of Good- Hope -, which Name it had received from John II, King of Portugal, in the Year 1494, when Bar- tbel Diaz ( who firft returned from it, tho* he did not double the Cape for want of Provifion, and by Reafon of tempeftuous Weather ) had given him a large Account of the itormy troubled Sea about this Promontory. PROPOSITION II. The Ocean, taken altogether ', is formed by the Land into fever al Portions, of which there are three Spe- cies , viz. i. Oceans, or great Seas. 2. Bays or ' Gulphs. 3. 'Streights. 1 . THE Word Ocean is taken in a double Senfe, fometimes for that general Collection of Wa- ters which furround the whole Earth : and very of- ten for a Part of that Collection, which is joined on both fides to other Parts by broad Tracts. Thus we fay , The Atlantic Ocean , The German Ocean, The Ethiopic Ocean, and Indian Ocean. We mall here ufe the Word Ocean fometimes in the later Senfe according to Cuftom, inftead of Sea ; which alfo is a Part of the whole Ocean, becaufe the Word Sea is often ufed in a fomewhat dif- ferent Senfe, as will be fhewed by and by. 2. A BAY, orGulph, is a Part of the Ocean which flows between two Shores, and is every where environed with Land, except where it communi- cates with other Bays, or the main Ocean. It is very often called a Sea. A STR EIGHT is a narrow Paflage, ei- ther joining a Gulph to the Neighbouring Ocean, M 4 or 168 fbe Abfolute Part S E c T. IV. or one Part of the Sea or Ocean to another. Thefe Differences are found in the Ocean, as will appear from what tollows. PROPOSITION lit. *fbe mam Ocean is divided into four large and parti- cular Parts, 'which are alfo each of them called Oce- ans, and anfwer to the four Continents, or great Ijlands of the Earth. Thefe are, 1 . T H E Atlantic Ocean, which is placed be- tween the weftern Shore of the old World, and the eaftern Shore of the new World. It is alfo called the weftern Ocean, becaufe it lieth to the weftward of Europe. It is beft divided into two Parts, by the Equator , whereof the one is contiguous to the Hyperborean Ocean, the other to the Icy or South Sea. 2. T H E Pacific Ocean, or great South Sea, which is placed between the weftern Shore of Ame- rica and Afea, and is extended to China, and the Philippine Iflands. 3. THE Hyperborean, or northern Ocean, a- bout the Arftic Continent. 4. THE fouthern Ocean , about the South Continent, of which the Indian Ocean is a Part, OTHER Geographers divide the main Ocean into four Parts, after this Manner : They make the Atlantic one Part, but do not extend it beyond the Equator, where they begin the Ethiopic : They alfo reckon with us the Pacific, and add thereto the Indian , but we , in our Divifion, have more regard to the four great Continents. Some make but three Parts, viz. the Atlantic, Pacific, and In- dian ; but then they extend the Atlantic further. Let every one ufe what Divifion he likes beft, it is no ' . W C H A P. 1 2 . of Umverfal Geography. 169 no great matter which , for thefe are not made by Nature, but contrived by the Fancy. PROPOSITION IV. Some Parts of the Ocean borrow a Name from the Countries which they bound. THUS we fay the German Ocean, the Briti/b Sea, the Indian Ocean, the Gulph of Venice* &c. PROPOSITION V. Some Bays are oblong, others broad ; fome primary, and others fecondary ; the former flow out of the Ocean , the latter out of fome other Bay : and fucb may be called Arms or Branches. The oblong are, i . THE Mediterranean Sea, which breaks out from the Ocean, between Spain and Barbary ; and runs a long fpace between Europe and Africa, even as far as Syria, Afia-minor and Thracia. The entrance is called by way of Eminence the Streights. Hence to fail up the Streights, is to vifit by Sea, Italy Greece , Syria, Sicily, Venice, and the reft of the Countries that lie upon the Coaft of this Bay. THERE are feveral fecondary Bays, or Arms, which proceed from it, viz. the Adriatic, Sea, or Gulph of Venice, the Archipelago, &c. I T may be reafonably enquired, whether the Euxine Sea be a Part of this Bay. Of which fee Chap. xv. THE Mediterranean hath divers Names from the feverai Coafts it reaches ; on the North it hath Spain, France, Italy, Sicily, Sclavonia, Greece, Can- dia, Romania, Afia-minor ; on the South it hath Morocco, Fez, Tunis, Tripoli, Egypt. From whence k is called the Gulph of Lyons, the Tufcan Sea, the Ionian 170 The Abfolute Part S E CT. IV. Ionian Sea, the Levant, &c. It is extended from Weft to Eaft, and receives into it many Rivers. 2. THE Baltic (or Eaft Sea, improperly fo cal- led) breaketh out from the Ocean between Zeeland and Gotland, part of the Continent of Sweden, and alfo between Zeeland and Jutland, from whence it flows a long way to the South-Eaft, and afterwards winding to the northward, it reaches a prodigious length between the Provinces of Mecklenburg, Pome- rania, Courland, and Livonia, on the Eaft ; and on the Weft, Sweden and Lapland. It fends out two Arms, viz. the BotbnicRay, and the Gulphof Fin- land -, to which may be added the Livonian Sea, or Gulph of Riga. It receiveth feveral great Rivers. 3. T H E Arabian Gulph, or Red Sea, floweth out of the Indian Ocean between Aden, a Town in Ara- lia, and Cape Mujledon in Africa, having Africa on the W T eft, and Arabia on the Eaft. It runs to the Eaftward as far as the Ifthmus of Africa, to the Town of Suez, where there is a Harbour for the Turkijb Fleet, and receiveth only a few fmall Rivers, but not one out of Africa. It is extended from the South-Eaft to the North- Weft. 4. THE Perfian Gulph [or Gulph of Balfora] floweth out of the Indian Ocean, near the Ifland of Ormus, from the South-Eaft to the North -Weft, between Perfia on the Eaft, and Arabia on the Weft, as far as the ancient Cbald&a, where it receiveth the Euphrates and Tigris, joined a little before in one Chanel ; but few Rivers of note befides. 5. THE Gulph of California, or Red-Sea, runs from South to North, between the Weft of Mexico in America and California, and ends at Tatonteac, an unknown Part of America. Modern Difcoverers will have California to be an Ifland ; and this not to be a Gulph or Bay, but a Streight or Sea (a). (a) See Note (e) Chap. viii. CHAP. 12. ofUnherfal Geography. 171 6. T H E Gulph of Nankin [or Gang] runs north- wards, between Corea and China, towards Tartary, where fome place Tenduc, in the Kingdom of Ca- tbaia : others will have Corea to be an Ifland. It receiveth but a few Rivers. T O thefe may be added feveral leffer Bays, fuch as the Gulph Cambaya, &c. Only the two firft of thefe, viz. The Mediterranean and the Baltic, afford fecondary Bays. PROPOSITION VI. The broad and open Bays arefeven in Number , viz. 1 . T H E Gulph or Sea of Mexico, which flows out of the Atlantic Ocean from Eaft to Weft , be- tween North and South America, where it is flop- ped by the long Ifthmus that joins thefe two Conti- nents, and feparates the Atlantic from the Pacific Ocean. It receiveth a great many Rivers and for Multitude of Iflands may compare with the Archi- pelago. 2. THE Gulph of Bengal, or Ganges, ftrikes out from the Indian Ocean, towards the North, be- tween India and the Peninfula of Malacca , it i$ bounded by Orixa, Bengal, Pegu, &c. Kingdom? of India, and receives, befides the Ganges, a great many famous Rivers. 3. THE Bay of Siam, between Cambodia and Malacca, is extended northward to the Kingdom of Siam. 4. T H E White-Sea , or Ruffian Gulph, flows from the Northern Ocean towards the South, be- tween Lapland, and the remote Shores of RuJJia. It flretcheth out an Arm towards Lapland, and endeth at Archangel in Mufcovy ; which is a Mart much frequented by the Englijh and Dutch. It receives feveral great Rivers. 5. THE 172 fbe Abfolute Part SECT. IV. 5. THE Lantcbidal Sea, is a Bay between [New Holland] and New Guinea ; two Peninjula's of the South Continent. It is extended Southward, and terminated at Carpentaria. 6. THERE is another Gulph a little to the weftwardofthe laft, between [Nuyt's Land] and Van Diemen's Land (two Sea Captains, by whom thefe Parts were difcoveredj. 7. HUDSON'S Bay is bounded by New Britain, New France, New Denmark, &c. and runneth out of the Northern Ocean. To which may be added, Baffin's Bay, the Bay of Bifeay, &c, PROPOSITION VIL Streights either join the Ocean to the Ocean , or tbf Ocean to a Bay, or one Bay to another. O F Straights we reckon fifteen, viz. i. T H E Streights of Magellan, tho* they may yield to others for Antiquity, are neverthelefs, ac- counted very famous for their exceeding long Reach, thro* which there is a free PafTage from the Atlan- tic to the Pacific Ocean. The Streight is in Length, from Eaft to Weft one Hundred and ten Leagues ; but the Breadth is various , in fome Places two Leagues, one League , and in fome Places but a quarter of a League. Magellan firft difcovered it, and failed thro* it in the Year 1520., Tno J it is re- ported, that Vafcus Nunnius of Balboa, l^d before (viz. in the Year 1513) taken notice of it when he failed that Way, to make Difcoveries to the Southward. It lierh in 52 degr. 30 mm. South La- titude, between Patagon, a Part of South America on the North, and the Iflands of Terra del Fuego on the South. 2. A little further, to the fouthward, are the Streights of La Maire> which are much ihorter than thofe CHAP. 12. of Uniwrfal Geography. thofe of Magellan. They have a Part of the South Continent on the Eaft, and the Iflands of Terra del Fuego on the Weft. A Paffage is more expediti- ouQy made thro* thefe into the great South-Sea, than the other, They lie in 54 degr. 30 min. South Latitude. 3 . T H E Streights of Manila, between Luconla and Mindanao, and others of the Philippine Iflands, are faid to be one hundred Leagues in Length, and are a very dangerous Paflage to Ships, by reafon of dreadful Quick-fands in feveral Places. They are extended from Eaft to Weft, and join, in part, the Pacific to the Indian Ocean, which are alfo not far from thence, joined by broader Streights in ma- ny Places. 4. T H E R E are feveral other Streights among the Indian Ifles, and between them and the Conti- nent ; as between Ceylon and India ; between Suma- tra and Malacca , between Sumatra and Java, &c, 5. T H E Streights of Way gats, thro' which there is fuppofed to be a Paflage from the Ruffian or North Sea, into the Tartarian Ocean ; but it is fo Ihut up with Ice, that it never could be failed thro* by the Europeans (). It lies between Samoie- da and Nova Zemtta. 6. T H E Icy Sea, between Nova Zembla and Spitsbergen, or New Greenland. 7. DAVIS's Streights, between North America and Greenland, have not been yet failed thro ; there- fore we are in a doubt, whether it be a Streight or a narrow Sea. 8. FQRBISHER's Streights, which afford a Paflage from the Atlantic Ocean into Hudforfs Bay. 9. THE Streights of Anian, between North America and Tartary in Afta, through which there }s faid to be a Paflage between the Tartarian Ocean, (b) 174 fh Abfolute Part SECT. IV. and the Pacific Sen \ but this is as yet unfettled. They who have failed in that Part of the Pacific Ocean pretend to be certain, that there are Streights, or Sea, both between America and Tar- tar -y, and alfo between America and Greenland r , by reafon that for feven hundred Leagues from Japan towards North America, the Currents fet ftrongly from the North North- Weft, tho* the Wind be va- riable, and blow from other Points of the Compafs : but when they are come within one hundred Leagues of New Spain, thefe Currents ceafe, and others flow to the Northward, as if it were to fome broad Sea on the North of New Spain. Alfo in thefe feven hundred Leagues failing, Whales are daily feen, and other forts of Fifh, that are known to delight in Streights and narrow Seas, which it is proba- ble, come from the Streights of Anian, to that Part of the Pacific Ocean ; becaufe they are not found elfewhere (c}. However, feveral of our modern Geographers take no notice of thefe Streights, but place a vaft unknown Ocean, between Tartary or Core a and America. 10. THE Streights of Gibraltar, thro' which the Atlantic Ocean gufheth into the Mediterranean Sea. They lie between Spain and Africa, and are about two Leagues over at the ftraiteft Place, but much longer. The Ancients believed that there (c) It is certain the Sea of Whale pafled from Spitsberg Corea and Japan, is annexed thro* the neareft Arm of the to the Tartaric Ocean, and alfo Sea, rather than thro' the more to the Sea of Green/and; be- remote. But be it how it will, caufe that fome Hollanders af we may hence fafely conclude, firm, (who were fhipwreck'd that the Sea which lies beyond upon Corea, a Peninfula of Japan and Spitsberg, is pafla- Cbina) that they faw there a ble ; and thro* more perhaps Whale, upon whofe Back ftuck than one Arm or Chanel, by a Harpon Iron of Gafcony, which they communicate, . Set which not being queftioned Note (a) Chap. viii. and Pbilof. by any, it is mod probable Tranfaft. abridged by Lowtborp. to be conjeftured, that this Vol. iii. Page 612. were CHAP. 12. of Univerfal Geography. were no fuch in the firft Ages of the World, but that they were made by the breaking in of the Sea upon the Land. n. THE Streights of Denmark [or the SoundJ lie between Zeeland and Scbonen, thro* which the Atlantic, in part, flows into the Baltic, where they are ftraitelt. They are about half a German Mile over. Near to this there are two other fmall Streights, the one between Zeeland and Funen, and the other called the Belt, between Funen and Jut- land. 12. T H E Streights of BaMmandel, at the Mouth of the Arabian Gulph, near the Sea-Port Aden, thro' which there is a Paflage out of the Indian Ocean into the Red-Sea. 13. THE Streights [ofOrmus] at the Mouth, of the Perfian Gulph, are not properly ib called, becaufe they are but little narrower than the Gulph itfelf. 14. THE Hellefpont, a Streight famous among the Grecians, thro' which there is a Paflage from the Archipelago to the Propontis , near to this there is another narrow Sea, called the Tbracian Bofpbo- rui, which joins Propontis to the Euxine Sea. 15. T H E Faro, or Streights, of Me/ma, be- tween Italy and Sicily. MANY have been of Opinion, that there were Streights fomewhere northward of Virginia, which is in 40 degr. North Latitude, whereby the Atlantic is joined to the Pacific Ocean, and thro* which they might find a free and open Paflage to China, and the Philippine Iflands : but this, in the Year 1 609, was in vain attempted thro* Hudson's Streights. THUS have we explained and pointed out the Parts of the Ocean, diflinguifhed by the Situation of the Land, in like manner as in Chapter viii. we de- fcribed the different Plans of Countries, occafioned by the breaking in of the Ocean. That the Geo- grapher 176 fbe Abfolutt Part SECT. IV. grapher may keep all thefe in his Memory, it will not be unferviceable to him to trace out the Peri- meter of the Sea Coaft, and to take a tranfient View of the Shores and Bounds of each Country, and alfo how they are fituated, and joined one to PROPOSITION VIIL b trace out the Sea Coafts, that environ the four Quarters of the Earth ', viz. The old and new World, and the North and South Continent.'} i. THE old World, (comprehending Europe, Aft a, and Africa,} is extended northward to the Streights of Waygats, adjoining to Samoieda ; up- on the Weft of which is the Kingdom of Mufco^ vy, where the White Sea is received into a large Bay from the North ; on the further Side of which is Lapland, and next to that, on the Weft, Norway, whofe Shore runs North and South i then winding to the Eaft, we came to the Shore of Gotland and Schonen, where there is a Gulph that receiveth the Baltic Sea, which is bounded by Sweden, Finland, Livonia, Pruffia, Courland, Pomerania^ Mecklenburg, Holftein, and Jutland ; then turning fouthward on the further Side of Jutland and Holjlein, we find the Shores of Weftphalia, Holland, Flanders, France, and Spain ; where there is another Inlet that re- ceives into a vaft Bay the Mediterranean Sea, which is hemmed in by Spain, France, My, Sclavonia, Greece, Romania, Afia minor, Egypt, Barbary, an4 Morocco, over-againft the Spanijh Shore ; then we turn along the Weftern Shore of Africa, to Cape Ver d -, and from thence the Shore bends eaftward along Guinea, and fouthward by Congo and Angola^ to the Cape of Good Hope ; where it is again refle- dted northward, and gives Bounds to Sofala % Zam- CHAP. 12* of Umverfa! Geography. 1 77 guebar, and [Anian] -, here the Arabian Gulph, or Red-Sea, is extended to Egypt, which is joined to the Arabian Shore, and to the Shores of the Perfu.n Gulph : upon the Eaft of thefe, are the Shores of Perjia, Cambaya, Indoftan, Malacca in India, Bengal, Cambodia, China, Tartary at Corea, to the Streights of Uries -, where follow the unknown Coaft of Nor- thern Tartary, and the Samoieds, which is [very like- ly] joined to the Streights of Waygats, where we began. 2. AMERICA is thus encompafied by the Ocean. On the North at the Streights of Davis, there is Hudfon's Bay, from whence follow in order to the fouthward the Shores of New- Britain, New- England, New-France, Virginia, Florida, Mexico, and New-Spain, on the Ifthmus ; then New-Caftle, Guinea, Brafil, and Pat agon, at the Streights of Magellan, where the Shore from running fouthward begins to turn towards the Weft; thence from South to North are extended the Shores of Chili, Peru, New-Spain and New- Mexico, which is bound- ed by the Gulph of California. -, [where follow the un- known Shores of Mozembec, &c. (bounded perhaps by the Streights of Anian} which may be contiguous (for any thing that we know) to thofe of DaviSs Streights.] 3 . THE Arttic Continent is extended to Da~ VH'S Streights, and from thence begin the Shores of Greenland, which run a little to the South, and then return northward to Spit/berg, where they are called the Shores of New-Greenland: thefe are llretched out over againft Nova Zembla, and the North of Tartary ; from whence the reft of the Shore to Davifs Streights is unknown. 4- THE South Continent ft retches to the Streights of La Maire, whence the Shore is per- haps continued to New-Holland, where the Lant- cbidd Sea is received into a Gulph, on the other VOL. I. N Side 178 The Abfolute Part SECT. IV. Side whereof is Ntw Guinea, which [very proba- bly] is contiguous to the Shores at the Streights of La Maire. L E T us now trace out the Perimeter of the Ocean. Between Davis' s Streights, and Nova Zembla there is the northern Ocean, and Icy Sea, or Sea of Greenland , which is continued till be- tween Europe and America, where it is called the German Ocean, the Briti/h Ocean, the French and Spanijb Ocean, and, in the whole, the Atlantic Ocean ; (and maketh three Bays, viz. the Mediter- ranean, the Baltic, and the Mexican Gulph) which, when it comes between the Coafts of Africa and Brafil, is called the Ethiopian Sea on the one Hand, and on the other the Sea of Magellan : fur- ther to the Eaft, between Africa and the South Con- tinent, is the fouthern Ocean, and between Afia and the fame Continent the [eaftern or] Indian Ocean ; alfo between Afia and South America is the Pacific Ocean [or great South Sea] which is extended northward to the Streights of Waygats and Anian, and fouthward to the Streights of Magellan [and La Maire~\ by which it is joined to the Atlantic. It goes under feveral Names along the Coaft of America, as the Sea of Chili 9 Peru, Mexico, California, &c. The Terraqueous Globe is divided into Land and Water. Again Water is divided into the main Ocean, Lakes, Morafles, and Ri- vers. The main Ocean is formed by the Earth into three forts of Portions. i. be Ocean, wbofe prime Parts are four. i. The CHAP. 12, of Unfoerf al Geography. 179 i. The Atlantic [or weftern Ocean] with the Etbiopic Sea, be- tween Europe and A- C The Britannic O;ean, frica on the one Hand, < The German Oc^an, and America on the o- C The Spanijh Ocean, fee* ther. It obtains vari- ous Names from the Places it watereth, viz. 2. THE Pacific Ocean, or great South Sea, between the furthefl Parts of Ajia and the In- dian Iflands, 6n the one hand i and the weftern Shore of America on the other. 3. THE northern Ocean, about die Arftic Continent, fometimes called the Icy Sea, Tarta- rian Ocean, &c. 4. THE fouthern Ocean, about the Antarctic Continent, a Part of which is the Indian Ocean. 2. 'Bay} or Gulpbs. t [TlKTyrrbene . The Mediterranean J%\ Sea. Sea between Europe(z}T\\z Ionian and Africa as far asQc < \ Sea. Afia minor - - -J-"/The Lev 'ant ', " The Gulph of Venice',, P Bays III 2. The Baltic Sea with it's fecondary Bays," viz. the Both/lie Bay, the Gulph of Finland, the Livonian Sea, &c. 3. The Arabian Gulph, or Red-Sea, between Africa and Arabia. 4. The Perfian Gulph, or Gulph of Balfora, between Arabia and Perfia. 5. The Sea of California, between California and New-Mexico. 6. The Gulph of Nankin, between Corea and China. N 2'- Thefe o 2& ^ t>n g-E j 80 Vbe Abfolute Part SECT. IV. 1. The Gulph of Mexico, between North p and South America. 2. The Gulph of Bengal, between Indujlan and Malacca. 3. The Bay [of Siam] between Malacca and Cambodia. 4. The White Sea, between Lapland and Mufcovy. 5. The Lantcbidol Sea, between New-Hol- land and New-Guinea. 6. The Gulph between Nuyt's Land, and Van Diemen's Land. 7. Hudfon's Bay , between New-France and New-Denmark. * v 3. S freights. 1 . T H E Streights of Magellan, which join the Atlantic to the Pacific Ocean. Thefe are longer than any of the reft. 2. THE Streights of La Mairs near thoie of Magellan, and of the ime ufe. 3. THE fuppofed Streights of Anian, which join the Pacific to the 'Tartarian Ocean. 4. DA VIS's Streights which join [Baffin's Bay] to the Atlantic, near which arc Forbi/herfs Streights. 5". THE Streights of Waygats, which join the Icy Sea, perhaps, to the Tartarian Ocean, if the Ice do not interpofe. 6. T H E Streights of Gibr alter, which join the Atlantic to the Mediterranean Sea. 7. T H E Streights of Denmark, or the Sound, join the Atlantic to the Baltic. 8. THE Streights of Babelmandel, at the mouth of the Arabian Gulph. 9. THE Streights of Ormus, at the mouth of the Ptrfian Gulph. 10. THE C H A P. 1 3- f Univerfal Geography. 1 8 1 10. THE Hellefpont and Bofphorus, which join the Archipelago to the Euxine or Black Sea. WHETHER the Cafpain Sea be a Lake or a broad Bay, which is joined to the main Ocean by fome fubterraneous Streights, is not fettled a- mong Geographers, CHAP. XIII. Of the Ocean, and certain Properties of ifs Parts. PROPOSITION I. The Surface of the Ocean, and of all other Liquids, is round and fpherical : Or the Surface of the watery Part joined to the Surface of the dry Part, do both together make up the Superficies of the terra- queous Globe. TH E Truth of this Theorem is proved from the Arguments ufed in Chapter iii. to prove the fpherical Figure of the Earth, for they hold as well here as there -, but becaufe thofe Proofs are chiefly built upon the Phenomena that are rea- fonably fuppofed to proceed from fuch a Figure, that is, rather from the Effects than the Caufe ; we mail propofe, in this Place, a Demonftration which is wholly founded upon natural Caufes, and by which Archimedes proved the Superficies of all liquid Bodies to be fpherical : in order to which he N 3 took 1 82 9 Abjbhie "Part SEC t. IV. took for granted the three following Poftulata : i. That the Earth hath a Center, and is therefore fphe- rical. .2. That it is the Nature of all Liquids, whofe Parts are continueid jmd lie at equal Di- ilances from the Center, that the Parts lefs pref- fed are expelled from their Places by thofe that are more preffed, as is manifeft from Experience. 3. That every Part of the Liquid is prefled by that Part which is above it ? perpendicularly 'towards the Center of the Earth, if the whole 'be defcending, or is prefled by any other Body. Befides thefe Poftulata, Archimedes ufes a Geome- trical Propofition which is not found demonftrated any where in the Elements , and therefore he demon- ftrates it himfelf, which is this: If a Superficies be " cut by feveral Planes, kll palling thro' one 'Point, and each Section be the Periphery of a Circle, whofe Center is that one Point, then will the Su- perficies be fpherical, and that Point the Center of the Sphere ', as is eafily demonftrated, LET the Superficies of any Body be cut by the Plane I F K E P (Fig.. .16.) thro' D, and let the Perimeter of the Section I F K E P be circujar, ha- ving D for it's Center ; alfo let every other Section, made thro' P, have circular Perimeters, and D for their Center. It is to be mewn, that the Superficies of this Body is fpherical, and that D is it's Center , i. e. that all the Points in. the Su- perficies are equidiftant from D. For we may imagine feveral right Lines to be drawn from D to other Points of the Superficies, and' we mult prove them to be all equal, We may fuppofe a Plane to pafs thro* any of them drawn from D to the Superficies, and alfo thro' DF (for two right Lines cutting one .another, or meeting, are in the fame Plane by Euclid Lib. ii. Prop. 2.) and the Periphery of the Section will be circular by the Hypothefis ; tlierefore, the fuppofed Line 2 drawn CHAP. 13. of Unherfal Geography. 183 drawn will be equal to D F, and fo will all other Lines drawn from D to the Superficies be in like manner equal to D F (#). Hence we prove the Superficies to be fpherical, having D for it's Cen- ter (by. This being premifed, the Superficies of all Liquids are thus demonftrated to be fpherical. Let us fuppofe a Liquid at Reft, in the form of EFGH, (Fig. 17.) and let the Earth's Center be D, and imagine this Liquid to be cut by a Plane palling thro' D, fo as the Section may be repre- lented in the Superficies by EFGH. We are firft to prove that this Line EFGH is circular, or an Arch of the Periphery of a Circle, whofe Center is D. If it were pofiible not to be cir- cular, then would two Lines, drawn from D to it, be unequal. Let the unequal Lines D E, D G be drawn, viz. let D G be greater than D E, alib let the one be the leaft, and the other the greateft that can be drawn from D. Then draw another right Line D F to E F G H, bifedling the Angle G D E, fo as to be longer than D E, but morter than D G. With this D F as a Radius up- on the Center D, defcribe in the fame Plane the Arch I F K H, which will cut the Line D E pro- duced in the Point I, and the . Line D G on this Side G, in the Point K. LIKEWISE with the Radius D L, fomething lefs than D E, upon the Center D, defcribe the Arch LMN within the Liquid in the fame Plane I F K H. Then are the Parts of the Liquid within the Arch LMN continued, and at equal diftances from the Center D : but the Parts between M N are more prefled than thofe between L M, having above them a greater Quantity, and therefore a greater Weight of Water. f/j) By the Definition of a I (b] By the Definition of a Circle Chap. ii. Article 3. j Globe Chap, it Article i z- N 4 AND j 84 Tbe Absolute Part S E c T. IV. AND the Parts of the Liquid within L M, being lefs prefTed, are driven out of their Places by thofe witiiin M N which take them up, and put the Liquid in Motion. But it was before fuppofed to lie in this Form at Reft, and flill : So that the Liquid, by this, will be both at Reft and in Motion,, which is inconfiftent. Wherefore the right Lines, drawn from D to E FGH, are not unequal, but equal ; and fo the Line E F G H is an Arch of a Circle, whofe Center is D. The fame may be demonftrated in all Planes cutting the Superficies of the Liquid, and pafling thro* D, wfz. that the Section is an Arch of a Circle whofe Center is D. Therefore fince, in the Su- perficies of Liquids, all Planes pafling any how thro' D, are found to produce circular Sections, it will follow, from the foregoing Proposition, that the Superficies of all Liquids is fpherical j having the Point D, that is, the Center of the Earth, for their Center ; as will more manifeftly appear from the Proof of the following Propofition. PROPOSITION II, The Sea is not higher than the Land, and therefore the Earth and Water are almoft every where of the fame Attitude, high Mountains excepfed. 'jflr.-; "j , T'-" r^ -"-*) .*,-, ; * THE Truth of this is demonftrated by the preceeding Propofition. For if the Superficies of the Ocean be fpherical, and have the fame Center with the Superficies of the Earth, and alfo if the Sea, near the Shore, be no higher than the Land, neither will the middle of the Ocean be elevated above the Earth, becaufe both their Surfaces make up the Superficies of one and the fame Sphere. But foine perhaps will not believe the former Pro- pofition, by Reafon of the affumed Hypothefis j 2 therefore CHAP. 13. of Univerfal Geography. therefore we fhall mew the Truth of this Theorem, without that, from it's known Effects. 1. WE know, by Experience, that Water, if it is not hindred, will flow from a higher to a lower Place. If therefore there were about the Shore any Place lower than the middle of the Ocean, the Water would continually fettle from thence towards the Shore, and be always flowing, and in Motion ; but the contrary is obferved when the Weather is calm. 2. IF the Ocean, far remote from the Shore, was much higher than the Sea Coaft, it might be feen at a greater Diftance than if it were fphe- rical, even over all the intervening Parts that were of a lefs Altitude. But Experience fheweth to the contrary, that when we come from die Inland Parts nearer the Shore, we difcover by little and little the more remote Parts of the Sea, and the nearer we approach the Shore, the further we can fee upon the Ocean. Therefore the remote Parts of the Ocean are not elevated above the Sea Coaft, but are of the fame Altitude with them and the Earth. 3. SAILORS cannot difcover any Difference between their Altitude, at the Sea Coaft, and in the middle of the main Ocean, tho f they ufe the moft accurate Inftruments ; which certainly they might, if the remote Parts were elevated above the reft, as a Tower, or a Mountain, For as we can find the Altitude of a Mountain, or Tower, above the Places of Obfervation by Inftruments, fo might they (if there were any) find the fupe- rior Altitude of the middle of the Ocean above the Parts next it, by fuch accurate Inftruments as are now in Ufe. 4. THERE are found, in feveral Places, great Numbers of Iflands, which are, fome of them, extended far into the main Ocean, and others The Abfolute Part .SECT. IV. pthers almoft contiguous to the Continent. There- fore no Part of the main Ocean is higher than the Land ; becaufe it is not higher than the Shores -of thefe Iflands. 5. THE Waves upon the Ocean never keep long upon a Heap, but are naturally diffufed 'till they make a fmooth Surface : wherefore it is un- realbnable to fuppofe, that the Water mould be heaped up towards the middle of the Ocean. 6. I F the Waters in the main Ocean are higher than the reft, why do they not flow into the Chanels of the Rivers, whofe Waters are more deprefied? for we find, by Experience, that Wa- ter naturally flows from the Place where it is, to a- ny other that is lower, which is the Caufe of fo many Inundations* F R O M the whole I think it fufficiently appears, that the Sea is not higher than the Shores; and but very few Shores are elevated to the Height of the Inland Parts, for thefe .are often obferved to rife gradually above the other, 'till they be- come high Mountains : from whence we conclude that no Part of the Ocean is higher than the Su- perficies of the Earth, That the Inland Parts are more elevated than the Sea Shores, appears alfo from the Rife and Currents of Rivers, which, for the moft part, breakout, and are directed, from thefe Mediterranean Places, towards the Ocean. Thefe Places therefore are higher than the mari- time Parts, becaufe they pour down their Waters upon them. Not but that there are fome Countries which are iituated a little lower than the Surface of the Ocean, but then they are defended either by the Altitude of the Shores, or by Banks, or long Ridges, of interpofed Ground. Some Coun- tries alfo are not fenced with Banks, becaufe they fear a calm and fettled Sea mould overflow them, but left, when it is ruffled with Winds and made impetuous, B CHAP. 13. ofUniverfal Geography. 187 impetuous, it fhould violently break in upon them. ' ' I T is therefore in vain to tell us, that the Sea is higher than the Land, and that by a miraculous Pro- vidence it is kept from overflowing the whole Earth, and caufing another Univerfal Deluge ; for we have fliewed, that both Land and Water are included within our fpherical Superficies, and that moft Parts of the Earth, at leaft the Shores are higher than the middle of the Ocean, which for that Rea- fon cannot overflow Countries, or caufe a Deluge, unlefs the Shore or Banks are wafted, and their Height diminimed, or a greater Quantity of Wa- ter force them open, or overpower them, and then indeed there may happen an Inundation. Neither is it impoffible, or contrary to Nature, that the whole Earth by fuch Means might be overflowed, as will be made evidently appear at the End of 'this Chapter. -'- - - i . ."' . H ilf ''v '-"f t\ %' ^ff* snj mo ; PROPOSITION III. the Ocean, feenfrom the Shore, appears to rife and fwell to a greater Altitude, by bow much the more remote it is. THIS is a Deception of Sight, or to fpeak more accurately, in the Eftimation, which hath brought many into an Error, and by which divers have fuppofed the Sea to be in fome Places feve- ral Furlongs higher than the Land. But it is a wonder they have never taken notice of a common Experiment, which is to be met with every Day, whereby this Fallacy is eafily detected. If we look upon a long Pavement, r Area, or upon a row of Pillars, r i88 mould be removed, then the Red-Sea would be joined to the Mediterranean ', and they both be- come Streights, and afford a Paflage to the Indian Ocean. PROPOSITION V. Whether the Ocean le every where of the fame Altitude. IT appears from the firft Proportion, that the Face of the Ocean in it's natural Situation, and when no Obftacle hinders, is every where of the fame Altitude, having, as was there proved a fpherical Surface, and being concentrical with the Earth : but it may be here doubted, whether for fome Reafons, it may not in one Place be higher than in another ; which is very worthy of Obfervation, and of great Moment to be well underftood, by not an Ifland from the Begin- every Day on both Sides, was nirtg, but was formerly joined wore away and wafted. The to France by an Iftbmus t be- great Dr Wallis was of this O- tween Dgver and Calais, and pinion, and fo was DrMi/Jgrav e. that this Iftb'mus, in procefs of See both their Arguments in, Time, being continually beat Pbilof. Tranf. abridged by Motte. upon by two impetuous Tides Par 14. Page 35,40. thofc tgz he Abfolute Part SECT. IV* thofe that propofe the cutting thro* of Ifthmus's, and joining one Part of the Ocean to another. SEVERAL will have both the Sea and Land to be higher towards the Northern Parts, than about the Equator, and this was Arijiotle's Thought (in Lib. 2. Chap. ii. de Cxlo) (c) t The Reafon they bring for it is, that the Ocean feems to flow from the Northern Parts as from a Fountain ; but this does not prove it's fuperior Altitude there: for whether the Northern Countries, or rather the Nor- thern Chanels, be higher or lower than the Cha- nels near the Equator (as is yet doubtful, or at leaft not fufficiently proved from that Motion which is not generally found in all the Northern Parts) it does not follow, if they were fo admitted, that the Ocean is there higher ; becaufe that to lower that fuperior Height, and to make the other equal with it, the Ocean is conftantly flowing towards the Equator. Ariftotle in the forecited Place adds ano- ther fabulous Reafon, taken from the Poets, which is not worth an Anfwer, viz. that the Sun when it fets, hides itfelf beyond the great Bulk of the Nor- thern Regions. THIS Opinion of the fuperior Altitude of the North Pole, feems to arife from hence ; that when we turn our Faces that way, we imagine the Pole to be raifed above the Horizon of the Place we are in, and therefore judge the Countries thereabouts to be elevated above us. SOME think the Indian Ocean to be higher than the Atlantic^ which they endeavour to prove from the Flux of the Sea in at the Streights of Gi- It -alter , and of the Arabian Gulph: but then, this doubt is to be confidered, whether the Altitude of Bays, efpecially in their extream Parts, be the fame (} The Earth and Ocean are highcft about the Equator. See the Note (b] on Chap. Hi. with CHAP. 13. of Univerfal Geography. 193 with that of the Ocean, or lefs ; and chiefly thofe Bays which are joined by very narrow Streights to the Ocean. THAT the Atlantic and Indian Ocean are higher than the extream Parts of the Mediterranean, near Egypt and Afia minor, none need doubt ; for unlefs the Streights ofGibralter (where the Atlantic floweth into the Mediterranean} were fomething lower than the Ocean, there would not be fuch a ftrong Current there as it is. Perhaps at the- Streight's mouth there may be but little difference ; but then further, to continue the Flux all over that large Tract between Europe and Africa, the depref- fion of the Bay muft by Degrees be greater, other- wife the Water 'could not flow when it is fo often obftrucled by Rocks, Iflands, Peninfula's, and o- ther Obftacles, which repel the Current of the Wa*. ter, and diminifh the Force of the Influx. We need not doubt of this, if it be true what is record- ed of Sefoftris, Darius, and other Kings of Egypt, by fome Authors of good Credit, how they at- tempted to cut a Chanel between the Red-Sea and the Nile, that out of the Indian Ocean and thro* the Red-Sea, they might fail that Way from the Mouth of the Nile into the Mediterranean ; which would be of great Advantage to Egypt and other. Countries upon the Coaft of the Mediterranean. But they were forced to defift from this Enterprife, when the Red-Sea was difcovered by the Artificers to be much higher than the Inner Egypt. If there- fore the Red-Sea be higher than the Land of Egypt, ' it will be alfo higher than the Water of the Nile and the Mediterranean itielf, into which the Nile flows ; and confequently the Red- Sea, and alfo the Indian Ocean, are both higher than the Mediterra- nean, efpecially the furtheft Parts of it about E- gypt, Romania, and the Archipelago. VOL.1. O MORE- 194 The Abfolute Part SECT. IV. MOREOVER, otlier Kings of Egypt of old, and of late the Egyptian Sultans, and Turkijk Em- perors, had frequent Confultations about cutting through that IJtbmiu that joins Africa to Afia, and feparates the Mediterranean from the Red-Sea ; but the Reafon, as we are told, why they did not fet about it was, that the Indian and Red-Sea were found to be much higher than the Shores of the Mediter- ranean: and therefore it was feared, that the Red- Sea mould overflow them, efpecially Egypt, which is reckoned by every one to be a very low Coun- try. THAT tht Red-Sea is higher than the Medi- terranean appeareth from thefe Obfervations ; but this, not without Caufe, may be doubted by fome, bccaufe they are both Bays, the one of the Atlan- tic and the other of the Indian Ocean. Therefore to give a plaufible Reafon, why the one mould be higher than the other, it will not be amifs to con- fider; that tho' they are both deprefTed more than the Seas from which they flow , yet the Difference is lefs fenfiblc in the extream Part of the Red-Sea^ which is nearer the Indian Ocean, than the extream Parts of the Mediterranean are to the Atlantic. For J cannot think that the Indian Ocean is higher than the Atlantic^ as fome imagine. IF therefore the Ifthmus was cut through, no doubt but a great Quantity of Water would flow from the Red-Sea into the Mediterranean ; but I can- not think fo much as to bring Egypt, and other Places about the Levant, into danger of being over- flowed : becaule if the Indian Ocean poured in more Water, the Atlantic^ would very liktly emit lefs, that fo they might each retain the fame Altitude in Proportion. BESIDES this, I fuppofe the Sultans of Egypt and the Turks, were induced by other Political i Caufes CHAP. i 3. of Univerfal Geography. 195 Caufes and Reafons to omit cutting through this lithmus. THE firft fcruple was no doubt the greatnefs of the Work, for it would be no fmall Labour and Expence to cut thro' an Ifthmus, whofe Breadth at the narroweft Part is at leaft forty German Miles, and the Earth rocky ; befides there muft have been Dams and Wears made in feveral Places, which could not have been done without fkillful Work- men, which thofe Nations have always wanted. THE lecond Reafon was, becaufe they fup- pofed the Chriftian Nations in -Italy, Venice, France ', Spain, &c. would receive greater Benefit than they themfelves from this Canal, by failing thro* it to Perfea and India, and bringing thence thofe pre- cious Commodities, which the Turks and Egyptians at prefent carry at their own Prices by Land, and for which they receive large Duties, which bring confiderable Revenues into the Grand Seignior*s Coffers. See Mafeus's Hiftory of India, Book iii. where he tells us, how much the Sultans of Egypt were formerly offended at the Portuguefe failing and trading into India. A third Caufe why they neglected this was per- haps, becaufe they knew the Chriftians excelled them in Navigation , and were therefore afraid left they mould invade thofe Streights, and the adjacent Countries, or even Medina itielf, the Sepulchre of Mahomtt. For a confiderable Fleet would in a fhort time tranfport a great Army of Men, and all neceffary Provisions from Europe to Arabia, by this Canal. BUT Alpbonfus Albuquerce, Governor of the Portuguefe Indies, was of another Opinion, when he had intended to have turned the Nile from Egypt, by cutting a Chanel thro' Abyffima (which borders upon Egypt, only a few Defarts interpo- fing) to the Red-Sea, that by this means he might O 2 render 196 'The Abfolute Part SECT. IV. render Egypt barren and unfruitful to the Turks ; but he died before he could undertake it. THUS far, concerning the Altitude of the Mediterranean compared with that of the Red-Sea^ Atlantic, and Indian Ocean. We were obliged to explain it ; becaufe from thence fome take Occafion to argue the unequal Altitude of fome Parts of the Ocean. BUT thefe things may be confirmed by ano- ther Example, if we may compare great Things with fmall. The German Ocean, which is a Part of the Atlantic , running between Friejland and Hol- land, forms a Bay ; which tho' it be but fmall, in comparifon of thefe famous ones juft now men- tioned, yet it is called a Sea, and watereth Am- fterdam the Capital of Holland. Not far from thence is the Lake of Harlem, which is alfo called the Sea of Harlem : this is as high as the foremen- tioned Bay, and fends cut a Branch to Leyden ; where it is divided into feveral lefler Canals. And becaufe neither the Lake nor the Bay overflows the bordering Country (when they are fettled and at quiet, and they have Bulwarks provided againft a Storm) it appears that they are not higher than the Lands of Holland. But that the German Ocean is higher than thefe Countries, hath been experien- ced by the Inhabitants of Leyden, when they under- took to cut a Canal from their City to the German Shore, near the Town of Catwic, which is about two Holland Miles in Length -, ib that the Sea be- ing let in, they might fail into the German Ocean, and from thence to other Countries. But when they had finifhed a great Part of it, they were for- ced to leave off, having at length found, by Ob- fervation, that the.. German Ocean was higher than the Ground between it and Le\den\ from whence the Place where they left off is called by the Dutch, ffet malle Gat. i. e, unprofpercus. Therefore the i German CHAP. 13. ofUniverfal Geography. 197 German Ocean is fomething higher than [the Zuy- der Zee or] the Bay of Holland. BUT all Bays are not depreffed below the Ocean, for thofe that run out into the Land at broad and open Paffages, fuch as thofe of Mexico^ Bengal, &c. are, without doubt, of the fame Al- titude with the Ocean itfelf : tho* I know the Spa- niards doubted this (whether the Pacific Ocean was higher than the Bay of Mexico) when they conful- ted about cutting thro* the Ifthmus of Panama^ that they might with more Expedition fail to Peru, China, and the Indian Iflands. But befides this Sufpenfe, we underftand that they had a Political Reafon for not doing it ; they were afraid left the Engiijh, Dutch, and other Nations mould make ufe of it, and lie in wait at the Entrances, or in- vade Peru. For the Englijh and Dutch would not care to make fuch long and dangerous Voyages thro' the Streights of Magellan or La Maire, when, with a well furnimed Fleet, they could force their way thro' thofe Streights, and perhaps take Peru, or at leaft crufh the force of the Spaniards there. THAT we may put an end to this, it is beft to determine, that the divers parts of the Ocean and broad Bays are all of the fame Altitude, (as was proved in the firft Propofition) but long Bays, and chiefly thofe produced from narrow Streights, are fomewhat depreffed, efpecially at their extream Parts : but I could wilh there were more diligent and accurate Obfervations made by thofe who have the Opportunities of making them, to remove, ifpoilible, the following Doubts, viz. i. Whether the Indian, Atlantic, and Pacific Ocean are of the fame Altitude, or the Atlantic be lower than the other two. 2. Whether the northern Ocean, near the Pole, and within the Frigid Zone, be higher than the Atlantic. 3. Whether the Red-S^a be higher than the Mediterranean. 4. Whether the O 3 Pacific 1 98 *fbe Abfolute Part S E c T. I V. Pacific Sea be higher than the Mexican Bay. 5. Whether the Baltic be as high as the Atlantic. And thefe Differences ought to be obferved in hudfotfs Bay, the Streights oi' Magellan, and others. We fhall treat of the Euxine Sea in Chapter xv. THE continual Flux and Reflux of" the Sea, and Currents, make the Face of the Ocean mutable, and it's Parts of a different Altitude, at different Times i but thefe arife from external Caufes, and we here only confider the natural Con- ftitution of the Water : betides, they do not feem to alter the Altitude fo much in the middle of the Ocean, as near the Shores. COROLLART. THEREFORE we cannot affent to Papy- rius Fabianus and Cleomedes, who determined the greateft Height of the Ocean to be fifteen Furlongs, or half a German Mile ; unlefs they mean the Depth, which is not at all well expreffed by the Word Alti- tude, as it appears in the Tranflation of Arijlotle, Book i. Meteor. Chap. xi. at the end, where &6ta. 7* T'OVTX is explained of the Altitude of the Sea. PROPOSITION VI. Fbe Depth of the Sea, or Ocean, in moft Parts may be tried yoith a founding Lead ; and there are but few Places where the Bottom cannot be reached. THE Depth of the Ocean varies according to the greater or lefier Depreflion of the Chanels j being found $o of a German Mile, 3*0, ro, 5, *, &c. deep , and in a few Places a whole German Mile or more, where the Line was commonly not long enough to try how much, tho* even there it is likely the Bottom is not at a vaft Diftance, unlefs CHAP. 13. of Univerfal Geography. 199 unlefs perhaps in fome Places theie may be deeper Pits than ordinary, or fubterranecus PafTages. THE Depth of Bays is not ib great as that of the Ocean, and their Chanels are lefs hollowed by being nearer the Land : for the fame Reafort the Ocean is not fo deep near the Shore, as in re- mote Places i which happens by reafon of the con- cave Shape of the Chanel. SAILORS find the Sea's Depth with a found- ing Lead, in the Shape of a Pyramid, of about twelve Pound Weight, fattened to a Line about two hundred Perches long, tho* fome require a Lead of a greater Weight : yet they may be fome- times deceived in this Obfervation if the Line fhould be carried away by a Current or Whirl- pool, fo as not to deicend perpendicularly, but obliquely. BUT when the Depth is fo great that no Line is fuffkient to found it, fome have thought of a Method to try it thus (d}. In the firft Place they obferve, how long a known Weight of Lead will be in defcending a known Depth ; then they fatten 04 a Cork (//) The learned Dr Hook has Wire C, with a bended End F, given us a Method (much like and into the (aid Staple, prefs in, the following) to found the with your Fingers, the fpring- Depth of the Sea without a ing Wire on the bended End : Line, which, becaufe it pro- and on it hang the Weight D, mifeth Succefs, we (hall here by it's Hook E, and fo let the defcribe from the Pbilof. Tranf. Globe and all fink gently into N 9. Page 147. the Water, in the Pollure repre- Take a Globe of Fir, or fented in the Figure, to the Maple, or other light Wood, Bottom, where the Weight, D, as A ; (Fig. \g.) let it be well touching firft, is thereby ilop- fecured by Varnifti, Pitch, or o- ped ; but the Bail, being by ther wife, from imbibing Water; the Impetus it acquired in def- than take a Piece of Lead, or cending carried downwards a Stone, D, confiderably heavier little after the Weight is Hop- than will fink the Globe: let ped, fuffers the fpringing Wire there be a long wire Staple B to fly back, and thereby lets in the Ball A, and a fpringing itfelf at Liberty to re-afcend. And 200 the Abfolute Part SECT. IV. a Cork or a blown Bladder to the Lead, fo as it may be difengaged from it, as foon as the Lead mall touch the Bottom : this being done, they let down the Lead, and obierve the time between it's touching the Bottom, and the Cork's rifing to the Surface of the Sea , from whence by comparing this with the aforefaid Oblervations, and ftated Pro- And by obferving the Time of the Ball's ftay under Water, (which may be done by a Watch, or a good Minute Glafs, or beft of all by a Pendu- lum vibrating Seconds, (which muft be three Foot three Inches and one fifth of an Inch long) you may by the help of fome A wooden Ball A weighed - Another wooden Ball B A Lead A Another Lead B The Ball B and the Lead B were let down at fixteen Fa- thoms ; and the Ball returned in forty eight fingle Strokes of a Pendulum, held in the Hand, vibrating fifty eight fin- gle Strokes in a Minute. A fecond time repeated with the fame Succefs ; wherefore the Motion was four Foot every Second. Again the Ball A, and the Lead B, whofe Nail was bend- ed into a (harper Angle ; the Ball returned in thirty nine Strokes. A fecond time repeat- ed with the fame Succefs, at the fame Depth. Ball A, Lead A, at eight Fa- thoms and one Foot, returned at twenty; repeated at eight Fathoms, returned at nineteen. Tried the third time at ten Tables, come to know any Depth of the Sea. Which Ta- bles may be calculated from the following Experiments made by the Lord Vifc. Brounker, Sir Robert Murray, and Mr Hook* in the Chanel at Sbeernefsi mentioned in Pbilof. Tranf. N 24. Page 43 9. Oz. Gr. - 5 2 r6 oo 30 20 30 oo 30^ oo Fathoms four Foot, returned at twenty eight. A fourth Tryal at the fame Depth, juft the fame. A fifth, at ten Fathoms five Foot, returned at twenty feven. A fixth Tryal, juft the fame. A feventh at twelve Fathoms five Foot, returned in thirty- feven. An eighth Tryal juft the fame. But if it be alledged, that it muft be known, when a light Body afcends from the Bottom of the Water to the Top, in what Proportion of Time it rifes ; it may be confidered, that in thefe Experiments the Times of the Defcent and Afcent arc both taken and computed to- gether ; fo that for this Pur- pofe, there needs not the Nice- ty which is alledged. portions, C H A P. 1 3 . of Univerfal Geography. 201 portions, they find the Depth of the Ocean. But there is fuch a Nicety required in making thefe Try- als, and the time of Obfervation is Ib ihort, that it is very rare to find the true Depth by this Me- thod. However it appeareth, that the Depth of the Ocean is every where finite, and not extended to the Antipodes', becaufe if two Portions of Earth were divided by any Part of the Ocean, which might be continued thro* the Center to the oppo- fite Side of the Globe, unlefs they were fupported with Arches, they would immediately fall together at the Center, becaufe the Earth is heavier than the Water. Befides, the whole Bulk of Earth and Wa- ter is finite and fpherical ; and therefore the Depth of the Ocean cannot be infinite. MOREOVER, from the Obfervations of the Depth in divers Places, it is manifeft, that the Cha- nels in Depth are nearly equal to the Mountains and inland Parts in Elevation, that is, as much as the one is raifed, fo much the other is deprefled, and as the Altitude of the inland Parts is gradually increafed from the Shore, fo is the Sea deeper and deeper towards the Middle of the Ocean, where the Depth is for the moft part greateft. THE Depth of the Sea, is in the fame Place often altered by thefe or the like Caufes. I . By the Flux and Reflux. 2. by the Increafe and Decreafe of the Moon. 3. By the Winds. 4. By the moul- dering and fubfiding of the Shores -, whence the Chanel is made higher in procefs of time by Sand and Mud. PROPOSITION VII. Vhe Ocean doth not flow from Springs, but is contained within the Cavities of the Earth ; tho* it is not al- way* numerically the fame ^ but continually increafeng and dimimfe'wg. WE 202 fbe Abfolute Part S E c T. I V. W E know by Experience that the Water o* Rivers is produced by Springs, and becaufe it hath been io for many Ages pait, it necefiarily follows, that the Water which is continually flowing to the Sea, returns again to the Fountains, either by fub- terraneous Duels, or fome other way. The Phi- lofophers of old were alfo of Opinion, that the Sea i filled forth at feveral Springs ; neither could the Magnitude nor the Perpetuity of it's Bulk convince them of their Error, for they faid, that it was con- veyed by fubterraneous Fiflures to thefe Fountains, which therefore kept continually flowing. Ariftotle (Book ii. Meteor. Chap, ii.) endeavours to prove the contrary, and to refute the Arguments of the Ancients, but fays very little to the Purpofe ; we think thefe following will be more effectual to dif- prove them. If the Ocean have Springs they muft either be in the raifed Parts of the Earth, or in that Part which is covered with die Ocean, that is r in the very Chanel of the Sea, That there are no fuch upon the dry Land is apparent, becaufe there were never yet found any ; and to fay that they are in the unknown Countries towards the North or South Pole is to take a Thing for granted with- out any manner of Reafon for it, becaufe moft of thefe Countries are covered with Ice continually, and as many as are difcovered of them afford no Springs at all. Neither can they pretend to fay that they are in the Chanel of the Sea ; for if they were, they would be no further diftant from the Center than the Ocean itfelf; and therefore the Water in them would not flow, but be at Reft, becaufe it is againft Nature that it mould afcend from a lower to a higher Place ; and the Springs of all Rivers are higher than the Waters they emit. Some indeed may object that this Motion is vio- lent, becaufe that the Bottom of the Ocean, being perforated into Ducts, Meanders, Fiflures, or Ca- nals, CHAP. 13. cfUnherfal Geography. 203 nals, (which you'll pleafe to call themj is not ter- minated in the Earth's Bowels, but extended to a- nother Part of the Bottom of the Ocean by more Intercourfes than one ; fome of which convey the Water one way, and fome another, fo that it iilii- cth out of each, as if they were fo many Springs. And fmce (fay they) it is not contrary to Reafon to fuppofe many of thefe Paflages or Intercourfes, nothing hinders but that there may be alfo as many Springs in the very Chanel of the Ocean. But thefe are all vain Fancies, and no way agreeing with the Nature of Water , for tho' the Water be continued thro* thefe Orifices, it will not flow thro* one or the other, but be at Reft, unlefs it be ur- ged by fome external Caufe -, and tho' it be prefled by the incumbent Water on this fide the Inter- courfe, it will not difcharge itfelf at the other ; becaufe it is as much prefled by the incumbent Water there, which keeps it in dSquilibrio, and at Reft, as may be proved by Experiment thus : r^ Let ABC D (Fig. 20.) be a Veflel full of Wa- ter, and A B it's fpherical Superficies. Let R P E F be a hollow Beam of Wood, lying obliquely un- der Water, fo that the whole at g under A may be higher than the Hole at b under B. Then the Water will flow in at both ends of the Beam 'till the hollow Part be full ; but there will be no Flux at either Orifice , not at g becaufe it is higher nor at h, becaufe, tho' it be lower than g, yet the greater Weight of the Water about B will ftop the Flux *. (&Lfame particular > and others accidental. (a] The Method that Sailors rent, and ride as firmly as if commonly ufe, in the Gulph of it were fattened by the llrangeft Mexico, to keep the Boat im- Cable nnd Anchor to the Bot- moveable where rhe Sea is deep, torn ; this Method will perhaps and perhaps not to be founded fucceed in fcveral other Places isthis. They fink downa Plum- where there are under-Currents, met of Lead about forty or fifty fuch as have been obferved in Pound Weight, to a certain the Downs, at the StreigbJs- number of Fathoms deep, as Mouth, and in the Baltic. See they are taught by Experience, Dr Stulb's Obfervations in a and tho' the Lead is nothing Voyage to the Caribbee Ifonds. near the Bottom, yet will the PbiloJ. Tranf. No 27. Boat turn Head againfl the Cur- I call CHAP. 1 4. ofUniverfal Geography. 233 I call that a general Motion of the Sea, which is obferved in all it's Parts, and at all Times. I call thofe proper or particular Motions, where- by only fome Parts of the Ocean are moved, which are twofold, either perpetual or anniverfary ; the former continue without Ceffation or Intermif- fion *, the latter are inconftant, and only obferved at fome certain Months or Days. THE accidental Motions of the Sea are fuch as now and then happen, without any regular Order j and fuch as thefe are infinite, PROPOSITION VI. The Winds caufe the accidental Motions of the Sea, by blowing the Waters toward fome oppojite Point j nor is the Sea ever free from fuch Motions. THE Wind, being nothing but a violent Mo- tion of the Air, and a Preffure of it towards the Earth, endeavours to impel the Water of the Sea out of it's Place *, and becaufe the Sea is a Fluid, and cannot refift the Force and Preffure of the Air, it is hereby moved out of it's Place, towards the oppofite Point, and drives the adjacent Water before it, and that again the Water before it, and fo on. AND fince there is always fome Wind in the Air towards one Point of the Compafs or ano- ther, and very often towards different Points, in divers Countries, at the fame Time ; it follows, that fome of thefe Motions continually affect the Sea, but more fenfibly where the Wind blows hardeft ; becaufe it being a Fluid is foon put in Agitation t>y fo violent an Agent, PRO. 234 ?*' Abfolute Part S E c T. IV. PROPOSITION VII. The general Motion of the Sea is twofold -, the one is conflant, and from Eafi to Weft : the other is com- fofed of two contrary Motions, and called the Flux and Reflux of the Sea, by which, at certain Hours, it flows toward* the Shores, and at others back again. T H A T the Ocean is continually moving from Eaft to Weft, is chiefly proved from the Motion of the Sea which lies between the Tropics in the Torrid Zone ; where it is ftrongeft, and lels impe- ded by other Motions. THIS Motion of the Sea is manifeftly per- ceived by thofe that fail from India to Madagafcar, and Africa ; alfo in the Pacific Ocean between New- Spain and China, and the Moluccas , likewife in the Ethiopic Ocean, between Africa and Brafil. THUS the Currents fet ftrongly, and run with a rapid Motion, from Eaft to Weft, thro* the Streights of Magellan -, which induced the firft Difcoverer (whether Magellan, or fome other be- fore him) to conjecture, that there were Streights thro' which they might fail out of the Atlantic into the Pacific Ocean. Ships are carried by the Currents, from Eaft to Weft, thro* the Streights of Manilha, and alfo thro* the little Chanels be- tween the Maldivies. The Sea runs impetuoufly into the Gulph of Mexico, between Cuba and Yu- catan, and flows out again, thro* a rapid Chanel, between Cuba and Florida. There is fo rapid a Flux into the Gulph of Paria, that the Streights are called the Dragon's Jaw. This Motion is alfo remarkable at the Land of Cana'da. The Sea ieems to run out of the Tartarian Ocean thro* the Streights of Waygats> as appears by the fetting of CHAP. 14. ofUniverfal Geography. 235 of the Current, and the great Flakes of Ice which are commonly found in thefe Streights. Upon the northern Coaft of America, the Pacific Ocean flows towards the Streights of Anian ; there is alfo a Current from Japan towards China ; and another from Eaft to Weft, thro* the Streights of Ma- coffer. In fhort, the whole Atlantic Ocean makes towards the Shores of America, and the Pacific from them, as is moft remarkable about Cape Correntes 9 between Panama and Lima. PROPOSITION VIII. The Winds frequently change the general Motion of the Sea, efpecially thofe called Periodical Winds^ or Monfoons^ which we Jhall treat of in Chapter xxi. BECAUSE thefe Winds blow moft frequent- ly from the North or South, or from other col- lateral Points, they muft needs obftruct the ge- neral Motion of the Sea, which is from Eaft to Weft, and caufe it to turn afide, from the Weft, towards the North- Weft, or South- Weft. And even the conftant, or Trade-Winds, which fel- dom blow directly from the Eaft, but from fome other collateral Points, change this general Motion of the Sea in many Places. Alfo the North Winds make a moft fenfible Difference in this general Motion in the northern Ocean, where thefe Currents are not ftrong, except in a few Places. PROPOSITION IX. The Caufe of this general Motion of the Sea from Eaft to Weft is uncertain. THE The Abfolute Part THE Ariftoteliam (tho* neither they, nor their Matter, nor any European Philofopher, had the feaft Notion of thefe Things, before the Portu- guefe failed thro* the Ocean in the horrid Zone) iuppofe, that it is caufed by the Prime Motion of the Heavens, which is common not only to all the Stars, but even, in part, to the Air and O- cean ; and by which they, and all things, are car- ried from Eaft to Weft. Some Coper means (as Kepler, &V.) altho' they acknowledge the Moon, to be the prime caufe of this Motion, yet they make the Motion of the Earth not a little contri- bute to it, by reafon that the Water, being not joined to the Earth, but contiguous only, cannot keep up with it's quick Motion towards the Eaft ; hut is retarded and left towards the Weft ; and fo the Sea is not moved from one Part of the Earth to another, but the Earth leaves the Parts of the Sea one after another. OTHERS, who are fatisfied with neither of thefe Caufes, have recourfe to the Moon ; which they will have to be the Governefs of all Fluids, and therefore to draw the Ocean round with her from Eaft to Weft. If you alk, how fhe performs this ? They Anfwer, it is, by an occult Quality, a cer- tain Influence, a Sympathy, her Vicinity to the Earth, and fuch like. It is very probable indeed the Moon, fome way or other, caufes this Motion, becaufe it is obferved to be much more violent at the New and Full Moon, than about the Qua- dratures, when it is, for the moft Part, but fmall. THE ingenious da Cartes mechanically explains how the Moon may caufe this Motion, both in the Water, and the Air. He fuppofes, according to his general Hypothecs, that there are an infinite number of Atoms, which re- solve about the Earth, and fill up the Space be- tween CHAP. 14. of Univerfal Geography. 237 tween it and the Orbit of the Moon, fo as not to leave any Vacuum; this Space he calls the Earth's Vortex (b). Let FEHG (Fig. 22.) be the Earth* 2143 the Water, 6587 the Air, BADC the Vortex of the Earth, and B the Moon. Now, fays he, if there was no Moon in the Vortex BADC, it's Particles would without any Impe- diment revolve about the Center T ; but fince the Moon is there, die Space, thro* which the cele- ftial Matter flows, is narrowed between B and T j therefore this Matter flows fwifter between B and T, and by that means prefies both the Super- ficies of the Air at 6, and of the Water at 2, more than if the Moon had not been in the Dia- meter of the Vortex B D : and becaufe both the Air and the Water are Fluids, and eafily give (b) The Flux and Reflux of the Sea, which des Cartes has endeavoured to explain, by an imaginary Plenum and Vor- tices, may be more eafily and fully explained upon other Principles (as mall be fhewn hereafter); for thefe are mere Fi&ions, and no way agreeable to Nature and Motion, as ap- pears from the following Ar- guments. i . If fome Vacuities were not fuppofed to be interfperfed among the Particles of Bodies, it would be very hard to con- ceive how Motion could be any way performed. For if we fuppofe every Place to be abfolutely full, a fmall Body cannot move ever fo little, with- out moving all the Bodies in the Univerfe, and whither, or to what Place they mould move, when all Places are already full is not ealy to conceive. 2. Since Comets are carried with a continual Motion thro* the heavenly Spaces, from every Part, and all Ways, and to all Parts; it is evident from thence, that the heavenly Spaces muft be void of any fenfible Refiftance, and con- fequently of any fenfible Matter. Newton's Optics, Page 310. 3. The Hypothefis of Vor- tices, and a Plenum, direftly contradifts the Attronomical Phenomena, and tends more to confound the celeftial Motions than to explain them, See Newton's Princip. Book 2. Schol. to Prop. 53, and the general Scholium at the end ; and C/arke's Notes upon Re- baitlfs Phyfics. Part i. Chap. 8. Art. 2. and on Part 2. Chap. 25, Art. 22. way 238 The Abfolute Part S E CT. IV. way to Prefiure, they ought to become lower under B, at 2, and higher under A, at r. And while the Earth is turned from E, by F, towards G, or from Weft to Eaft, the fwelling of the Water 412, and of the Air 856, which is now higheft at E, moves by little and little to the weft- ward, and in fix Hours time is higheft at the Part of the Earth H, and after twelve Hours at G. Hence it follows, that both the Water and the Air are perpetually moving from Eaft to Weft. Thus far des Cartes. The ftrefs of his Demon- ftration lies here; that the Earth EFGH, and Water 1234, are revolved round the Center T, together with the celeftial Matter in theVortex, be- tween BADC and 6587 ; but the Moon, being in B, makes the Space B6 narrower, whereby the ce- leftial Matter is fqueezed thro*, and in it's PafTage prefles the Air and Water below B, at 6 and 2, towards 5 and i , and while E pafles beneath B, it is prefied towards H and F, and fo round. Nor doth this celeftial Matter, ftrained between B and 6, rebound upward being fupprefled, be- caufe all things are full of Matter. And tho* it prefs the Air and Water from 62 F not only towards the Weft E 15, but alfo towards the Eaft 73 G, yet becaufe the Parts between F and G, to the eaftward, are, by degrees, removed from the Streight B6, and the Pans towards E, to the weftward, do more and more approach it, there- fore this Force is chiefly received by thefe. BUT the following Particulars feem wanting in this ingenious Explanation. i . IT mould then follow, that the Sea would fettle when the Moon approached it, and rife in thofe Places that are diftant a Quadrant, or fix Hours, from it, viz. it would fall at 2, where the Moon is vertical, and rife at 6. But this is contrary to Experiences for at 2, under the CHAP. 14. of Uniwrfal Geography. 239 the Moon, it rifes, and at i it falls. How this Abfurdhy may be avoided, we lhall Ihew in the following Proportion. 2. IT is not plainly mewed (des Cartes himfelf totally omitting it) why, when the celeftial Matter in the Streight B6 prefles the Air at 6, and the Water at 2, it is not equally moved towards 637, feeing that the Earth, and Air, and Water, are all carried that way, as well as the celeftirfl Matter, which mould therefore enforce the Air and Wa- ter rather towards the Eaft than the Weft. 3 . T H E Moon approaching any Sea, there ftiould a ftronger Wind blow from Eaft to Weft than at other Times , but this feldom happens. 4. I T is more likely that the Sun mould caufe this Motion of the Air, and thefe conftant Winds, becaufe in many Places they are obferved to blow frefher a little before, or about, Sun-rifmg, when it is diftant a Quadrant from the Vertex of the Place (c\ Thefe things are worthy to be confi- dered in the aforefaid Explication, not to fay any thing for or againft the Hypothefis itfelf. I very much doubt whether this Motion of the Sea has any relation to the general, or Trade- Winds ; becaufe thefe Winds, in the 'Torrid Zone* are conftant , and therefore mould caufe the Mo- tion of the Water to be conftant alfo ( d). Indeed when the Wind blows harder the Motion is per- ceived to be greater; but this is no Argument that they have a Dependance, or proceed one from another. What hinders is, that there appears to be (i] See the Notes upon ftant one, without doubt, Jsef- Chap. xxi. Prop. 2 below, fefted by the Trade- Winds, where the Caufe of thefe Trade- which conftantly blow from Eaft Winds is explained. to Weft, tho* notwithftanding (d) As periodical Currents the Moon may interfere, and are produced by the fhifting alter or divert it's ordinary Winds or Monfoons : fo this con- Courfe. a Corrc* 240 ^be Abfolute Part SECT. IV. a Correfpondence between the Motion of the Sea, and that of the Moon, for when this approaches the other, it caufes it to fwell at 2, and the Cur- rents are obferved to fet ftronger to the weftward at the New and Full Moon, than at the Quadra- tures. This laft is excellently explained by des, Cartels Method ; for fince the Moon is nearer the Earth at the New or Full than when ihe is in the Quadratures, the Pafiage for the celeftial Matter, B6, is then made narrower, and therefore the PrefTure is greater (*). I F any fliould alledge, that perhaps the greater Light of the Moon, at Full, caufes the greater Intumefcence ; I anfwer, that at the Change all her Light is taken away ; which fhews that Light is not the Caufe of this Motion, but rather that Prefiure of des Cartes, which we fhall further ex- plain below. PROPOSITION X. $be fecond general Motion of the Sea, is it 9 3 Flux and Re flux i by which, in about twelve Hours and a half's Time, the Water is found to flow towards the generality of Shores, and to ebb back again, viz. to flow when the Moon approaches the Me- ridian Circle above or below ; and to ebb when it departs from thence towards the Horizon. (e) ' Neither the Moon's ' greateft Diftance, nor her leaft, Falls in the Quadratures ' but both there and in the * Conjun&ion or Oppofition; ' contrary to the Opinion of des Cartes ; who aflerts, that the Orbit is elliptical indeed, ' but fo that the leffer Axis of WE it is always in the Conjun- ctions and Oppofitions, or pafleth thro' the Center of the Sun, and the greater in the Quadratures. Which Aflertion is very wide of the Truth. Wbifion's Aftrono- mical Leftures, Page 107. C H A P. 1 4. of Univerfal Geography. 241 W E are firft to enquire whether the Sea flows towards one certain Point by this Motion, viz. from Eaft to Welt, or from Weft to Eail. FOR the Shores of Bays, and the Chanels of Rivers, where this Flux and Reflux is chiefly obferved, more dian in the main Ocean, are di- vers ways extended ; fome from Weft to Eaft 4 as the Mediterranean Sea, and others from South to North, as the Arabian Gulph, &V. And in all thefe the Water flows thro* the Streights towards the furtheft Point of their extent , and therefore in different Bays, this Flux of the Ocean tends towards divers Points of the Compafs. We muft therefore firft be refolved, whether this Flux, or Motion, tends indifferently to any Point, or only, obferves two, viz. the Weft in flowing, and the Eaft in ebbing ; or even only the Weft in both ebb- ing and flowing ? In my Opinion the laft is trueft, viz. that the whole Ocean is moved from Eaft to Weft, both in it's Flux and Reflux, and that the difference is, diat in it's Flux it is moved with greater violence and in a greater Quantity : but^ in it's Reflux (or more properly it's Deflux) tho* it be not moved a contrary Way, yet it feems to be fo, becaufe there flows a lefs Quantity of Water. HENCE we may determine, that the Flux and Reflux of the Sea is no way diftinct from that general Motion, which we explained in the former Propofition, whereby the Ocean is perpe- tually moved from Eaft to Weft , for it is only a certain Mode or Property of that Motion. And therefore if this Motion be obferved, and rightly confidcred in the main Ocean, where it is not ob- ftrucled, we mail find it not to be fo much a Flax and Reflux of the Sea, as a Flux and De- flux, or (that we may diftinguifh, by proper Terms, the Quality of the Motion or Flux from the Mo- VOL. I. R tion 242 *fbe Abfilute Part SECT. IV, tion or Flux itfelf), it is moil aptly called the Swelling and Swaging of the Sea. FOR the Sea perpetually flows from Eaft to Weft, and only feems to flow back again, when h*s more violent Force is flackened and wafted, which a little before was quickened and augmented. But this is called the Reflux, becaufe the Sea feems, on Shores and in Bays, to approach and retire by fits, which is not owing to the quality of the Mo- tion itfelf, but to the Situation of the Shores and Bays, which requires that the Water fhould fall back to the contrary Point; but the fettling of the Sea in general doth not proceed from the Situa- tion of the Shores, but from the quality of the Mo- tion of the W T ater. BUT the Motion of the Sea can by no means be eftimated by it's approach to the Shores, for whatever this Motion be, or to what Point ibever it is made, it will always fluctuate towards the Shores , which happens by reafon of the fluid Na- ture of the Water. T H A T the Sea moves towards the fame Point, that is, from Eaft to Weft both in the Flux and Reflux (or Swelling and Swaging) and never moves the contrary way appears from the fol- lowing Obfervations, i. In the main Ocean be- tween the Tropics, there is no other Motion per- ceived than this from Eaft to Weft. 2. In Streights that join the Parts of the Ocean and run directly Eaft and Weft, as the Streigltfs of Magel- lan, Mamlha, Java, and others among the Indian Iflands.-, in thefe, I fay, the Sea rifes and fettles in 1 2 Hours Time, but in fettling it doth not flow back out of the Streights to the eaftward ; but is carried by other Paflages, ftill to the weftward - 9 which is a plain Sign that this Ebbing and Flow- ing are not two contrary Motions, but a Modifi- cation, of the general Motion from Eaft to Weft. *!Ci2 I SO CHAP.- 14. of Univerfal Geography. 343 So that Scaliger and all the reft are deceived, who reprefent this as a double Motion to and again. IT is to be underflood, that when we fay this Motion is from Eaft to Weft, we do not mean punctually the two cardinal Points, but include all their Collaterals, even to the North and South Poles, towards which however the Motion is weaker. PROPOSITION XI. 70 explain the Caufe of the Swelling and Swaging of the Sea, vulgarly called it's Flux and Reflux (/). THERE (f) Sir Ifaac Newton moft fuccefsfuliy explains as well the Flux and Reflux of the Sea, as raoft other Appearances of Na- ture, from his univerfal Princi- ple of Gravity or Attraction. Gravitation is a certain Force im- printed on all Bodies by the Au- thor of Nature, by which they mutually endeavour to accede; but how this Force is exerted we know not. Thus the Globe of the Sun and Planets gravitate mutually towards each other in proportion to their feveral Mag- nitudes, and Diftances from one another. As to this Earth of ours, it hath but little Commu- nication with the other Planets, whofe Bodies are too fmall to ajFeft us much, at iuch a vaft Diftance ; only the Sun and Moon are refpedled by it, the one becaufe it is placed fo near us, and the other by reafon pf the Bulk of it's Body; which tho' it be at a vaft Diftance, yet afts with a ftrong attractive Force. F^r a Bo4y is more forcibly attracted by how much the Diftance of the Attrahent }s nearer, or it's Bulk greater. i. Thus; Let L (Fig. 23.) be the Moon, fuppofed to be above any Part of the Earth* covered with the Ocean as b ; it is evident that this Place, being nearer the Moon than any 6- ther Part of the Earth, is more ftrongly drawn thereby, and fwelleth up towards it: But the Water in the Place a be- ing diametrically oppofitc to the Place b, and further off from the Moon than the rell-of the Earth, hath a lefs Tendency towards it than the other Parts} and therefore, being left as it were by the Earth, is lifted up, orfwelled, the contrary Way m a. Henc the Water flowing from d to e towards A and B, makes two Protuberances in the Ocean, the one in B direftly under the Moon, the other in A juft oppofite to it ; and thefe always fhift and accompany the Moon in it's feeming Motion, R 2 aboO, 244 e Abfolute Part SECT. IV, THERE is no Phenomenon in Nature that hath fo much exereifed and puzzkd the Wits of Philofo-r of the Month and the time of the Year. 3. For, becaufe the attractive Force of the Sun reaches the Earth as well as that of the Moon; when both thefe Forces confpire, or are united, they raife the Waters higheft, and make what we call Spring Tides ; but when the Sun depreffes what the Moon heaves up, then hap- pen the loweft or Neap Tides. Thus we oblerve higher Tides when the Sun and Moon in Con- junction or Oppofition, are right over any Place B, or diametrical- ly oppofite over A and B, than when they are in the Quadra- tures, viz. when the Sun is in the Point H or I, and the Moon in the intermediate Point A or B. But the Force of the Sun is fmall compared with that of the Moon; becaufe the Semidia- meter of the Earth C B, by which the Water in B is nearer the Sun than the Center C, is fcarce fenfible, if compared with the immenfe Diftance of the Sun. 4. Since the Eminences of Water are carried round the Earth by the diurnal Motion, the Motion, Agitation, and Height, of the Tides, are the greater, the larger the Circle is in which the Watersrevolve. So the Mssn being in the Equino- ftial, and leading about the two oppofite Eminences of Water in the Equator, makes greaterTides (cteteris paribus] than when Ihc is in the Tiopics. Hence about the Earth, and occafion thereby two Floods and Ebbs in the fame Place, every five and twenty Hoars. 2. Of thefe two Tides that happen in the Time of one di- urnal Revolution in any Place, that is the greateft, wherein the Place cometh neareit the Eminence of the Water A or B. Thus, in fuch a Figure as the Jaft, let, P/> (Fig 24.) be the Poles, JE Q_ the Equator, FG a Parallel to it, which a- ny place defcribes by it's diur- nal Motion ; it appears that the two High- waters happen in the Place, when it is fituated in G or F, having the Moon in the Meridian ; but the higheft Tide is found in the Point G, which comes neareft the Eminence of the Waters in B. It further appears from the Figure, that the Moon, in the Time of the higheft Tide, is above the Hori- zon of the Place, if (he is on the fame fide of the Equator with the Place itfelf: but if (he decline the contrary Way, flie is under the Horizon in the Point A, at the Time ofthe highea Tide. For Example, in Europe the diurnal Tides are the higheft of the two when the Moon is found in the elevated Semicircle ofthe Meridian, or in the Northern Signs of the Ecliptic; but the loweft when fhe is in the South- ern Signs. .Moreover, the Height ofthe Tides is varied generally all over the Earth, according to the day CHAP. 14. of Umverfal Geography. 245 Philofophers and learned Men as this. Some have thought the Earth and Sea to be a living Creature, whicn, by it's Refpiration, caufeth this ebbing and flowing. Others imagined that it proceeds, and is provoked, from a great Whirl-pool near Norway, which, for fix Hours, abforbs the Water, and afterwards difgorges it in the fame fpace of Time. Scaliger, and others, fuppofed that it is caufed by the oppofite Shores, efpecially of America, where- by the general Motion of the Sea is obftru&ed and reverberated. But moft Philofophers, who have obferved the Harmony that thefe Tides have with the Moon, have given their Opinion, that they are entirely owing to the Influence of that Lumina- ry. But the Queflion is, what is this Influence ? To which they only anfwer, that it is an occult Hence alfo both the Lumi- naries, placed in the Equinoctial at the Time of their Conjun- ftionorOppofition, which hap- pens near the Equinoxes in March, or September, produce the higheft Tides in the whole Year. Which Experience alfo con- firms, becaufe the Sun is a little nearer the Earth in the Winter than in the Summer; therefore the higheft Spring Tides happen a little before the Vernal Equinox, and a lit- tle after the Autumnal, viz. in February and OHober, rather than precifely upon the Equino- flial Days. 5. The librating Motion of the Waters, which are apt to retain the Motion imprefied up- on them, and continue to move tho' the Actions of the Lumina- ries ceafe, make the greateft menjlrual Spring Tidei (explain'd in Artie. 3.) not precifely on the New and Full Moons, but gene- rally they are the third Tides af- ter them. 6. Things would happen con- ftantly and regularly thus, if the whole Earth were covered with very deep Sea ; but by reafon of great and fmall I {lands which ftop the Tide, and the Streights between them, alfo the Shelves and Shallows along which the Tides are to be propagated, the Variety of this Phenomenon is almoft infinite, and fcarcely to be explained by this Theory ; but when juft Obfervations are diligently made, all thefe parti- cular Caufes may be found out and known. See Newton's Prm. Math. Phil. Book 3. Prop. 24. Greg. Phyf. and Geometr. Aftron. Book 4. Prop. 64, 6$. al- fo HalleyV Di/ertation in Phil. Tranf. No 226. J tariff t Appendix. R 3 Quality. 246 The Abjblute Part SECT. IV, Quality, or Sympathy, whereby the Moon at- tracts all moift Bodies. But thefe are only Words, and figniry no more than that the Moon does it by ibme means or other, but they do not know how : Which is the Thing we want. D E S Cartes explains it by his general Hypo- thefis thus : In the forementioned Figure of Pro- pofition 9. let A B C D be the Vortex, with the Earth in it's Center, and which, with the Earth and Moon in it, is carried in a larger Vortex a- bout the Sun. Let M be the Center of the firft Vortex, EFGH the Earth, 1234 the Superficies of the Sea, which for plainnefs we will fuppoie to cover the whole Earth , and 5678 the Superficies of the Air furrounding the Sea. If therefore there were no Moon in the Vortex, the Point T, the Center of the Earth, would coincide with the Point M, the Center of the Vortex -, but fmce the Moon is about B, the Center of the Earth muft be betv/een M and D ; becaufe, fmce the celeftial Matter of this Vortex moves fomething Iwiiter than the Earth or Moon, which is carried only with it, unlefs the Point T were a little further diftarit from B than from D, the Pretence of the Moon would hinder it from moving fo freely between B and T, as between T and D ; and feeing the Place of the Earth in the Vortex is not determined, but by the equal Force of the circumambient celeftial Matter, it is plain that it ought therefore to ap- proach fomewhat towards D. And for the fame Reafon, when the Moon mail be in C, the Center of the Earth ought to be between M and A, fo that always the Earth may recede a little from the Moon. Moreover, finCe we fuppofed the Moon to be about B, not only die Space between B ancj T, but alfo that between T and D, thro' both which the celeftial Matter flows, is made fome- thing narrower 5 hence it follows, that the cele^ " CHAP. 14. of Univerfal Geography. 247 itial Matter floweth fafter there, and therefore prefleth more, both the Superficies of the Air at 6 and 8, and of the Water at 2 and 4, than if" .the Moon had not been in tjje Diameter of the Vortex B D, Now feeing the -Air and Water are both Fluids, and eafily give way to the Pref- fure, they muft be more depreffed about F and H, than they would be if the Moon were not in this Diameter B D ; and alfo more elevated towards G and E, where both their Superficies bulge or are prominent. And further, becaufe the Part of the Earth at F, under B, where the Sea is now loweft, in fix Hours Time will be at G, under C, where it is now highefl, and after other fix Hours in H, under D, and fo on : or rather, becaufe the Moon is moving a little in the mean Time from B towards C, fo as to perform the whole Revolution A B C D in a Month, by which t he part of the Earth that is now in F under the Moon's Body, will be in fix Hours, twelve Mi- nutes Time, or .thereabouts, a little further thaa G, in that Diameter of the Vortex, which is 90 Degr. diftant from the Place into which die Moon in the mean Time hath moved ; therefore the Wa- ter will in that Time increafe and be higheft at F, and in other fix Hours, twelve Minutes, wheji the Moon is got beyond D, will fettle and be loweft there, tsV. Hence it is plain, that the Wa^ ter of the Sea mull conftantly ebb and flow in the fame Place, every twelve Hours, twenty four Minutes Time. THIS is des Cartels Demonftration, which is very ingenioufly contrived to account both for the Tides that happen when the Moon is in the Me- ridian of the Place, and thofe alfo that occur when Ihe is in the oppofite Point of the Meridian Circle ^sader the Horizon. R 4 BUT 248 *Tbe Absolute Part SECT. IV. BUT according to what we obferved in the ninth Propofition, there are feveral Imperfections in this DemOiiftration. As firft, it is a wonder that des Cartes did not confider, that, according to his Demonftration, the Water ought to ebb at 2 and 4, when the Moon approaches the Me- ridian B : and, on the contrary, to flow, when the Earth or Moon ('viz. either of tnem) is removed fix Hours from each other , but this is contrary to Ex- perience, for when the Moon approaches the Meri- dian of any Place, theWaters flow in that Place, and ebb, back again, at it's departure. But both des Cartels Words and Figure fhow the contrary ; fo that to take away the Abfurdity (and in des Cartels Method) let us fuppofe the Vortex of the Earth A BCD, and the Waters 1234, to be interfper- fed equally about the Center T without any Pro- tuberance, and to revolve with the Earth and the celeftial Matter between A BCD and 5678. Let us fuppofe again the Moon to happen into this Vor- tex at B, and therefore the Space T B to become narrower, and the Water at 2 to be preffed towards E by the celeftial Matter fqueezing thro' it. THEN while the Water is expelled from 2 to E, I afk where the greateft fwelling will be, whether in the Place E, which is diftant a Qua- drant from F (where the Moon is vertical), or in the Place next to F towards E ? If you anfwer, the fwelling is greateft about the former Place E, I deny it, becaufe it is contrary to Experience -, but Experience mews the latter to be true, and even Reafon convinces us, that when the Moon is over the Place F, the Water will be forced from 2 towards i, which happens becaufe the greateft fwelling is about 2, not about i, for here it will be leaft , hence the Places to the weftward have their Tides later, as we know by Experience. And Reafon and the Laws of Hydroftatics require this. For CHAP. 14. of Unherfal Geography. 249 For if Water be poured in at 2, that it may flow towards E, there will be the greateft quantity of Water at 2, and a little lefs in the next Place, but leaft of all at E ; and the fame Thing will happen if it be expelled or driven towards E. But by the Circumrotation of the Earth, E comes into the Place of F, where at length there will be the greateft Protuberance at E, and the Water will be repelled towards H. THEREFORE^ Cartels Figure and De- monftration is to be changed, that the fwelling may arife fomewhere about 2, viz. where the Moon is vertical. What more might be faid here we refer to our Treatife upon dfs Cartel's Pbyjics. PROPOSITION XII. The general Motion of the Sea from Eajl to Weft is Jlronger, and the Tides are higher at New and Full Moon, than at the Quadratures. THE Truth of this Propofition appears from, Experience. For People that ufe the Sea teftify, that at New and Full Moon, the Face of the Ocean is conftantly rough and troubled, but calm and quiet at the Quadratures. This is eafily ac- counted for by the aforefaid Hypothefis ; for when the Moon is at the New or Full, me is nearer the Earth than at any other Time of her Age, and is furtheft diftant in her Qua- dratures, as is fhewn by Aftronomers (g). But when the Moon is nearer the Earth, that is, when the Space BT is lefs, the celeftial Matter being hindered, or obftructed, prefles with greater force the Water from 2 towards i. But happens o- therwife in the Quadratures. fc) This is falfe. Sit tie Nate ( e) bn. YET 250 The Abfolute Part SECT. IV. YET in fome Places there are higher Tides at the Full Moon than at the New, which I can- not account for, unlefs they be the Effecls of it's greater Light at that time. Nor can it be o- therwife explained, why at the Full Moon Vege- tables and Animals are impregnated wkh a greater quantity of Sea Moifture, than at the New, tho* even then the Tides are every whit as high. It |s very wonderful what one ffejf?, a Dutchman^ relates in his Defer iption of India. He fays, that in the Kingdom ofGuzarat (where he lived many Years) their Oyfters, and Crabs, and other Shell- Fifh, are not fo fat and juicy at the Full Moon as at the New, contrary to their Nature in all other Places. Nor is it lefs admirable, that on the Coaft of the fame Kingdom, near the Mouths of the River Indus^ the Sea fwells, and is troubled, at the New Moon, when not far from hence, viz. in the Sea of Calicut the greateft Rile of the Wa- ters is at the Full. But it is requifite that we fhould have repeated Enquiries and Obfervations about thefe Matters, before we pretend to folve their Phenomena. PROPOSITION XIIL tte Flux and Reflux of the Sea varies with the Seafons of the Tear, and the Tides are obferued to le bigbeft about the Equinoxes ; i. e. at the Spring and Fall * but kweft at the Soljlices. .'.. .( '-. i 4\'. : - -^ -i ,\ t <"'j Liil^fSniH D E S Carles pretends to account for this Phe- nomenon by his Hypothefis, but I cannot ap- prehend his Meaning by his Words, nor how it can- be deduced- from it (6). It is probable, that the Sun and the general Winds may contribute much (b) See the true Reafan eftkis in Artie. 3. of Note (f) above. C H A P. 1 4. of Univerfal Geography. 3 5 1 to raife thcfe Tides, when, in the Equinoxes, the Sun is vertical to the Ocean in the middle of the Torrid Zone^ and therefore may caule both the Wind and Water to rage, and the former to a- gitate the latter. The contrary of which may, happen about the Solftices. Or we may fay, that thefe extraordinary Tides then happen by the fame Reafon, and proceed from the fame Caufe that frequent Rains and Inundations proceed from in thefe Seafons. PROPOSITION XIV. Infome Parts of the Ocean, Bays, and Shores., the Tides ebb and flow very high ; and in others but low: and in fame few Places ihsre are no fenfible Tides at all. THOSE Places have the greateft Tides; i. which are in the Torrid Zone between the Tropics, where the Moon, being almoft conftantly vertical, preffes the Water with greater force -, 2. thofe which lie direftly Eaft and Weft with their Col- laterals ; 3 . thole Bays that are long and narrow ; 4. thole Places where there are but few Iflands or Forelands. THE Tides are therefore greater or lefs in a Place, according as it is fituated or extended. THE greateft known Tides are obferved in the Bay of Guzarat, at one of the Mouths of the River Indus^ and has ftruck many with Admira- tion. The W T ater there recedes from the Shore very quick, and leaves it uncovered for a great Space ; fo that this Bay is, not without Reafon, thought to be the fame into which Alexander the Great failed, when he attempted to tranfport his Army by Sea into India y but was hindered, as it is reported, by the Sea which retired quick from 252 The Abfohite Part SECT. IV. from the Shore, and left all his Ships a-ground, .fo that he could not proceed further, but thought that the Gods had there fixed Bounds to his Expedition. This Story is reported for a Truth by the Inhabitants of Cambaya. The Caufe of this is the fhallownefs of the Chanel, which makes the Water in it's Ebbing leave fo much more Ground uncovered, tho' perhaps fome other Caufe may confpire with this. A T the Town of Daman, not far from Surat in India, the Tide rifes and falls two Fathoms and a half, and the Sea recedes from the Shore half a German Mile. IN the Bay of Cambaya the Tide flows five (or as fome fay feven) Fathoms high, which vio- lent Flux caufes many Ships to be loft by unex- perienced Seamen , for at the Ebb, when the Wa- ter falls back, they are frequently fplit upon the Rocks. UPON the Shores and Bays at the Magellanic Streights, there is no conftant Time obferved be- tween the Tides, which ebb and flow irregularly, fometimes in three Hours, and fometimes in twelve Hours -, which variety is caufed by the violent breaking of the Sea into thefe Streights, and the frequent Agitation of it by the Winds. PRODIGIOUS high Tides are obferved a- bout Malacca-, and in the Streights of Sunda. I N the Aralian Gulph, or Red-Sea, the Tide of Ebb is fo great, that as fome of the Antients have writ, (quoted by ScaRger) Mofei, and the Jfraelitts? migh , at low Water, have pafled thro* it without a Miracle. But this is falfe, for it ne- ver ebbs fo much as to leave the Chanel dry. I N Button's Bay, near Hudfon's Streights, when Mr 'Thomas Button, an Engli/hman, wintered there in the Latitude of 57 Degr. North Latitude, he obferved the Tide of Flood to rife fifteen Foot and above : CHAP. 14, ofUniverfal Geography. 253 above : and in the Latitude of 60 Degr. the Summer after, he found it to come up to the fame Height ; tho* in neither Hudfon's nor JameSs Bay it rifes- much above two Foot. T H E R E are prodigious high Tides upon the Coaft of China, and about the Iflands of Japan. A T Panama, a Town on the Coaft of America, the Pacific Sea flows very high, and immediately ebbs again , at the Full Moon the Agitation is fo great that it drives the Water into the Houfes of the Town. All along this Shore the Tides of the great South Sea are ftrangely high -, fo that in ' their Reflux they retreat two Miles of Ground, and in fome Places the Water falls of out Sight. I N the Bay of Bengal, on the Shore of Siam 9 the Tide rifes fifteen Foot. BUT in the Mediterranean Sea, which flows from Weft to Eaft thro* the Streights of Gibralter, there is no fenfible Tide at all ; becaufe it's En- trance is fituated oppofite to that Point, to which the Ocean Sea in general flows. It may perhaps increafe a little, but in the main it is not fenfible, only in the Gulph of Venice there is a fmall Agi- tation perceived, by reafon of the great length and narrownefs of the Bay, which, in the broader Parts of the Mediterranean, is no where percep- tible. Therefore the Flux and Reflux of the Sea was unknown to the Grecians, and alfo to the Romans in the Time of Scipio Africanus ; and there- fore when they found it in other Places, accounted it a Miracle ; as appears from the forementioned Expedition of Alexander the Great, and the Wars of Scipio with Carthage j but in Cicero's Time this was well enough known to the Romans. A fmali Tide is obferved at Marfeilles in France^ and an inconfiderable Rifing is perceived along the Coaft of Barban. IN Attfolute Part SECT. IV; I N the Baltic Sea, and all over the northern Ocean beyond England and Norway the Tides are ngt in the leaft perceptible j nor in the northern Parts of the Pacific Ocean (i). The Reafon is not well known, unlefs we fix it upon the great Di- ftance thefe Seas are from the way of the Moon, and their being extended from Weft to Eaft, and North-eaft, with the many Iflands and Forelands, all which confpire to obftruct the Flux of the Tides in thefe Places. But this cannot be faid of Hudjotfs Bay ; which is properly extended from Eaft to Weil, to receive the Flux of the Tides ; and therefore it is no Wonder if they are much more remarkable here than in the Baltic, or in the northern Ocean. PROPOSITION XV. fbe Flux of the Sea is forced by a Jlrong Impulfe > but the Reflux is the natural Motion of the Water. THE Flux is caufed by the Preffure of the Moon, or the celeftial Matter, between it and the Sea, and continues no longer than the Caufe forces it : but in the Ebb, the Sea only flows from a higher to a lower Place, which is the natural Motion of the Water. (*) The Tides are very fimll on the Coaft ofNovaZemb/a the in feveral Parts of the Northern Water was obferved by Capt. Ocean, yet they may be felt in Wood to rife eight Foot. See fome particular Places. Thus Note [a] on Chap. 8. above. LEMMA CHAP. 14. ofUnherfal Geography. 255 LEMMA. The Place of the Afyon in the Zodiac being known, from an Ephemeris, or by Calculation* or Aftrono- micai Observation, and alfo it's Latitude, and the Hour of the Day ; to fad, on the Terreftrial Globe^ what Place the Moon will be vertical to at the given Hour, and to Jhew all the Place* that the Moon will pafs over, one after another, that Day. THIS Problem is of great Ufe for obferving the Flux and Reflux of the Sea. You will find the Method of folving it in Chapter xxx. Propo- fition 14. where it is more commodioufly explain- ed. However the more knowing Reader may anticipate it here, or learn it aforehand from the Rules there delivered. PROPOSITION XVI. Ihe Ttdes are higheft in thofe Places over which the Moon is vertical, unlefe fame of the Obftacles above- mentioned in Proportion 1 4 hinder ; but the fur- ther any Place is from that, the lefs (cseteris pari- bus) is the Flux and Reflux. BECAUSE thofe Places are more prefled, and the fwelling of the Sea is greater, over which the Moon fqueezeth the celeftial Matter, where- by greater Tides are produced : but where the in- cumbent Matter is lefs fqueezed, and other Caufes confpire, the Alteration will be lefs. PRO* 256 The Abplute Part S E c T . I V. PROPOSITION XVII. The Altitude of the Tides are divers in the fame Place at different Times^ and they are high and low^ ac- cording as the Moon is further from or nearer to the Zenith of the Place. SINCE the Moon every Day changes her Place in the Ecliptic, me will be vertical now to one Place, and then to another, and confequently varies her Diftance from the Zenith of any particu- lar Place. Which being granted, it follows, as a Corollary of the laft Propofition, that the Tides in any one Place are conftantly altering, whether their Variation be fenfible, or infenfible. PROPOSITION XVIII. The greateft fwelling of the Ocean, or High-Water, ought to be in that Place when the Moon is in the Meridian Circle (above or below} ; but in divers Places it h High-Water when the Moon is otherwife fofited. SINCE the Moon, in the Meridian, is nearer any Place than when fhe is in the Horizon, (be- caufe the Hypotenufe of any right-angled Tri- angle is longer than the Perpendicular) it follows (by Propofition 16, of this Chapter) that then it ought to be High-Water in that Place (where fhe is full SouthJ. And when fhe is full North, or in the lower Part of the Meridian Circle, it ought to be alfo High- Water in the fame Place, becaufe, tho* fhe be not there, yet the oppofite Part of the Vortex of the Earth is ftraitned, and hath the fame Effect, as if the Body of the Moon itfelf were prefent. BUT CHAP. 14. of Unherfal Geography. 257 BUT there are many Places and Shores where it is not High- Water precifely at the Time of the Moon's fouthing or northing in the Meridian Circle, (as the Philolbphers of the former Age thought) but perhaps a little before, or after, me makes her appulfe to the Meridian, viz. when me approacheth a Vortex fomething diftant from it, Eaft or Weft. Neither doth a full Tide always happen when the Moon is in the fame Azimuth ; but it is very often High- Water, efpecialry at the New and Full Moon, a little before the conftant Time, or before the Moon approaches that Azimuth. At London it is High-Tide when the Moon is three Hours from the Meridian, or South- Weft, and North-Eaft (). On the Shore of China , in the Harbour of Maccao, a Portttguefe Sailor thus fta- ted the Time of High- Water. The Elevation of the Pole, or the Latitude of the Place, is 22 degr. 20 min. In the Year 1584 on the nineteenth Day of September it was Full Moon, and the fame Day, it was High- Water half an Hour, or three quar- ters, pad Eight in the Morning -, fo that the Moon was then three Hours and a quarter diftant from the Meridian-, hence the Azimuth, or Point me was then in, may be found by a Problem in Chapter xxx. I N the Year 1585, February the third, which was alfo the third from the New Moon, it was obferved to be High-Tide a little after twelve ; and therefore at the New Moon, which was February the firft, it was full Sea about forty Minutes af- ter Ten. HENCE the Azimuth the Moon was then in may be found. (k) See the Nott (m) VOL. I. S IN 258 We Abfohte Tart SECT. IV, I N the Year 1585, February the fixteenth, it was obferved to be High- Water, at Full Moon, almoft at Noon, viz. at half an Hour paft Eleven. IN the Year 1585, June the fecond, which was the fourth Day after the New Moon, it was High-Tide exactly at twelve, therefore at the Conjunction it was High-Tide at nine in the Fore- noon. THE fame Sailor adds, that the Time of High and Low- Water doth not agree with the Time that is computed from the Motion of the Moon, except for five Days before and after the New Moon. But there is fome Ambiguity in thefe Words, and others following, which we have there- fore omitted. But the Caufe of this Variation is, that the Sea rifes nine Hours in the Port of Mac- coo, and ebbs only three, as is obferved in the next Proportion. HERE follow fome Obfervations made by a Dutch Sailor of the Time of High-Water, on the Days of the New and Full Moon, at different Places. AT twelve o 5 Clock (on the New and Full Moon Days) it is High- Water along the Shore of Flanders, at Enckhuyfen in Holland, at Hoorn, at Emden in Eaft Friejland, at the Mouth of the River Elbe, at the Mouth of the Eyder, at the Iflands of Jutland, at Dover in England, &c. AT forty five Minutes paft twelve, at Flujb- ing in Zealand. AT half an Hour paft one, at the weftern Shore of the Ifle of Height, at Calais, at the Mouth the River Thames in England, along the Shores of Zealand, at the Mouth of the River Schelde, in the Meitfe, at [Gorcum\. AT three o'Clock, at Amflerdam, Rotterdam, Dort, and Newcaftle in England, before the Fle- ffii/b Sand-Banks, at Armenlier in Flanders, at the i Mputh CHAP. 14. of Univerfal Geography. 259 Mouth of the River Garonne, along the South Shore of England, on the Coaft of France, Gafeoigne, Bif- ca-j, Gallicia, Portugal, and Spain -, on the weilern Shore of Ireland, all the way to Shetland. A T a quarter before four in the Afternoon, at Rohan in France, in the Maefe, at Rochelle in France, in the River Garonne, in the Bays upon the Shore of Spain, Portugal, Gallicia, in the Bays on the Southern Shore of Bretagne in France, on the Shore of Gafeoigne, on the weftern Shore of Ireland. AT half an Hour paft four, from the I'exel to the fouthern Shore of Ireland. A T a quarter paft five, in all the Ports on the South of Ireland, at Plymouth in England, and at other fouthern Places between that and Wales. A T fix o'Clock in the Morning and Evening, at Hamburgh in the Elbe, at Bremen, on the Eaft fide of the I'exel, at Antwerp, in the Englijb Cha- nel as far as the Stilly Iflands. AT a quarter before feven in the Evening, at Falmouth, and in Brtftol Chanel, at St Nicolas and PodeJJamke, as far as Weymouth and Hartpool. AT half an Hour paft feven at the Road in the Texel, at Kilduyna, in the middle of the Cha- nel, befide Plymouth, and as far as the Foreland of Lizard-Point. A T a quarter paft eight in the Evening, about the Ifle of Wight, at the Weft fide of the File Ifland. A T nine o'Clock, at die Mouth of the River Eems in Friejland, on the Eaft fide of the Flie Ifland, along the Shores of Friejland, and on the eaftern Shore of the Ifle of Wight. A T half an Hour paft ten, at the Mouth of the River 'Thames, on the Shore of Normandy and S* AT 260 fbe Abfolute Part SECT. IV. A T a quarter paft eleven, in the River Thames, and other Places in England. I T is very difficult to explain the Caufe of thefe 'wonderful, and extraordinary Differences of the Tides in all Places, tho* it properly belongs to Naturalifts, and Geographers, to do it. It is like- ly that the various windings of the Shores, and their different Situation to the Sea-ward, the Re- fiftance of the Iflands, the Concurrence of feve- ral Tides, the Diftance of Places from the Moon's Way, the various Winds, chiefly thofe that are general and conftant, the Declivity and Shoalnefs of the Shores, and other things, very much con- tribute to this furprifing Diverfity. For Ex- ample, at the Port of London the Tide rifes 'till the Moon comes to the South- Weft, when me hath South Latitude, and only then begins to ebb, not when me approaches the Meridian : for which we give this Reafon, viz. that while the Moon is moving from the Meridian of London towards Brafil (or from Brafil towards London} the Water ought not to fettle, but ftill to rife, becaufe the Shore of America repels the Water towards Eng- land^ which is drawn thitherward by the Moon, fince there is no Paflage for it to proceed any fur- ther. But it may be afked why, when the Moon hath North Latitude, it mould happen to be High- Water before me approaches the Meridian of London, viz. when me is in the South- Eaft Point ? To which I anfwer, that when the Moon hath North Latitude me is much nearer England than when Ihe hath South, and therefore raifes up the Water fooner -, and the Reafon why the Flux is not continued fo long as 'till the Moon approaches the Meridian is, becaufe me impels the Ocean more towards the American Coaft, and Hudfon's, -Bay, where the greateft Floods are then obferved. AND CHAP. 14. .ofUmverfal Geography. 26 r AND for this Rcafon it is. High- Water along the Coafts of China, before .the Appulfe of the IVj oon to the Meridian, becaufe the continual Eaft Winds drive the Sea towards the Weft. BUT all thefe Allegations are not fufficient to fatisfie me in thefe Matters, and therefore I would have the curious Naturalifts examine them with greater Scrutiny. For to find the true Caufe, it is requifite, that we be furnifhed with accurate Obfervations how the Tides ebb and flow in dif- ferent Places, and what Azimuth the Moon is in when it is High-Water in thofe Places ; and how her Bearing varies according to her Place at the Change and Full ; efpecially in thole Places where the Moon is vertical, and thofe that bear from them diredly Eaft, Weft, North, and South (/). It is alfo to be diligently obferved, what height the Tides flow at thefe times j when the Moon is in the North Part of her Orbit, and moves not over fo much Sea, but over that vaft Tradl of Land which lies between China, and the weftern Shore of Africa. For fince me prefTes not the Water directly when fhe moves over thefe Mediterranean (/) The following Directions 3. Obfcrve the Increafe and are of excellent ufe for oblerv- Decreafeof the Velocity of the itg the Tides, given by Sir Ro- Currents. bert Murray, in Pfrilof. Tranf. 4. Meafure the Height ofeve- N* 1 7. ry utmoft High Water and Low i. Obferve the Situation of Water, from one Spring Tide the Place of Obfervation, viz to another, what Currents, Seas, Iflands, 5. Meafure the exaft Height Bays, Shores, Shelves, &c. are of SpringTides and Spring Ebbs, neat it. 6. Obferve the Pofuion and z. Obferve in what proportion Strength of the Wind, the State the Increafes of the Tides from of the Weather; the Height of the Neap to the Spring Tides, the Barometer, &c. and their Decrenfes, and the Ri- 7. Calculate rhe Moon's Age fings and Fallings of the Ebbs, and Phce in ail Refpecls. happen to be in regard of one See Lowthorp's ^^ria^iaeHt 0/Philof. Tranfaft. p. 260. S 3 262 ld it will be South about three of the Clock, and it will be Jiigh Tide three Hours after- THAT wards, that is at fix of the Clock. But now by this Rule, if you count this Tiine of the Moon's coming to the South in the Cir- cumference, the perpendicular Line which comes from three to nine, cuts the Diameter at 45 Min. which fhews that fo much is to be abated from the Time of High Tide in the New and Full CHAP. 14. of Univerjal Geography. 267 THAT is, at the end of the firft Day of the Moon's Age it is High- Water later by forty eight Minutes, &f. BUT Full Moon ; fo that it is High Tide 45 Min. before fix ; that is, at five Hours i 5 Min. and not at fix, according to the common Rule. The like you may do for any other Port, or Place, knowing the Time of High Water at the New and Full Moon in that Place : And you may do it the more readily, if you fet down the Time of High Water at the New and Full Moon under the Diameter, as I have done for London where it is high Tide at three of the Clock : So when the Moon is fouth at three of the Clock or nine, the Perpen- dicular cuts the Diameter at two Hours 1 5 Min. which, added to the aforefaid three or nine, gives the Time of high Water as a- bove. Thus you may eafily make a Table which by the Southing of the Moon mail readily tell you the Time of High Tide in any Place. The following is for London. Moon Tide Moon Tide Moon ! Tide Moon Tide South. Lnd South. Land. South Load. Scutb. Land. H, M\H. M. H. M H. M H M. \H. M. H M H. M. xn o \ o II 5 *5 VI O 7 30 x c 1 '5 10 i 9 IO 5 21 10 7 40 1C i 29 20 3 18 20 5 27 2C 7 52 2C ' 43 3 i 27 3 5 3: 30 8 4 3 C ii 57 40 3 36 40 5 4 4 8 15 40 2 10 ?o 3 40 50 5 4^ 5 i 25 5 C 2 24 I 3 54 [V C 5 5 2 vn o|g 36 X C .2 37 10 4 2 1C 5 59 1C 8 48 1C 12 50 20 1-