Chapter 12

CHAP. V.Of Gravity.

Of Gravity.

The last Thing subservient to our Globe, that I shall take notice of, isGravity[a], or that Tendency which Bodies have to the Centre of the Earth.

In myAstro-Theology,Book 6. Ch. 2.I have shewn of what absolute Necessity, and what anoble Contrivance this of Gravity is, for keeping the several Globes of the Universe from shattering to Pieces, as they evidently must do in a little Time by their swift Rotation round their own Axes[b]. The Terraqueous Globe particularly, which circumvolves at the rate of above 1000 Miles an Hour[c],would by the centrifugal force of that Motion, be soon dissipated and spirtled into the circumambient Space, was it not kept together by this noble Contrivance of the Creator, this natural inherent Power, namely, the Power of Attraction or Gravity.

And as by this Power our Globe is defended against Dissipation, so all its Parts are kept in their proper Place and Order. All material Things do naturally gravitate thereto, and unite themselves therewith, and so preserve its Bulk intire[d]. And the fleeting Waters, the most unruly of all its Parts, do by this means keep their constant æquipoise in the Globe[e], and remain inthat Place which, the Psalmist saith,God had founded for them; a bound he had set, which they might not pass; that they turn not again to cover the Earth, Psal. civ. 8, 9. So, that even in a natural Way, by virtue of this excellent Contrivance of the Creator, the Observation of the Psalmist is perpetually fulfilled,Psal.lxxxix. 9.Thou rulest the raging of the Sea; when the Waves thereof arise, thou stillest them.

To these, and an hundred other Uses of Gravity that I might have named, I shall only just mention another Thing owing to it, and that isLevity[f], that, whereby what we call light Bodies swim, a Thing no less useful to the World than its opposite,Gravity, is in many Respects, to divers Tribes of Animals, but particularly serviceable to the raising up of Vapours[g], and to their Conveyance about the World.

And now from this transient View of no other than the Out-works, than the bare Appendages of the Terraqueous Globe, we have so manifest a Sample of the Wisdom, Power, and Goodness of the infinite Creator, that it is easy to imagine the whole Fabrick is of a Piece, the Work of at least a skilful Artist. A Man that should meet with a Palace[h], beset with pleasant Gardens, adorned with stately Avenues, furnished with well-contrived Aqueducts, Cascades, and all other Appendages conducing to Convenience or Pleasure, would easily imagine, that proportionable Architecture and Magnificence were within: But we should conclude the Man was out of his Wits that should assert and plead that all was the Work of Chance, or other than of some wise and skilful Hand. And so when we survey the bare Out-works of this our Globe, when we see so vast a Body, accouter’d with so noble a Furniture of Air, Light and Gravity; with every Thing, in short, that is necessary to the Preservation and Security of the Globe it self, or that conduceth to the Life, Health, and Happiness, to the Propagation and Increase of all the prodigious Variety of Creatures the Globe is stocked with; when we see nothing wanting, nothing redundant or frivolous, nothing botching or ill-made, but that every thing, even in the very Appendages alone, exactly answereth all its Ends and Occasions: What else can be concluded, but that all was made with manifest Design, and that all the whole Structure is the Work of some intelligent Being; some Artist, of Power and Skill equivalent to such a Work?

FOOTNOTES:[a]That there is such a Thing asGravity, is manifest from its Effects here upon Earth; and that the Heavenly Bodies attract or gravitate to one another, when placed at due Distances, is made highly probable by SirIsaac Newton. This attractive or gravitating Power, I take to be congenial to Matter, and imprinted on all the Matter of the Universe by the Creator’sFiatat the Creation. What theCauseof it is, theNewtonian Philosophydoth not pretend to determine for want of Phænomena, upon which Foundation it is that that Philosophy is grounded, and not upon chimerical and uncertain Hypotheses: But whatever the Cause is, thatCause penetrates even to the Centers of the Sun and Planets, without any Diminution of its Virtue; and it acteth not according to the Superficies of Bodies (as Mechanical Causes do) but in proportion to the Quantity of their solid Matter;and lastly, it acteth all round it at immense Distances, decreasing in duplicate proportion to those Distances, as SirIsaac Newtonsaith,Princip.pag. ult. What useful Deductions, and what a rational Philosophy have been drawn from hence, may be seen in the same Book.This Attraction, or Gravity, as its Force is in a certain proportion, so makes the Descent of Bodies to be at a certain rate. And was it not for the Resistence of the Medium, all Bodies would descend to the Earth at the same rate; the lightest Down, as swiftly as the heaviest Mineral: As is manifest in theAir-Pump, in which the lightest Feather, Dust,&c.and a piece of Lead, drop down seemingly in the same Time, from the top to the bottom of a tall exhausted Receiver.The rate of the Descent of heavy Bodies, according toGalileo, Mr.Huygens, and Dr.Halley(after them) is 16 Feet one Inch in one Second of Time; and in more Seconds, as the Squares of those Times. But in some accurate Experiments made in St.Paul’sDome, June 9. 1710, at the Height of 220 Feet, the Descent was scarcely 14 Feet in the first Second. The Experiments were made in the Presence of some very considerable Members of the Royal Society, by Mr.Hawksbee, their Operator, with glass, hollow Balls, some empty, some filled with Quick-silver, the Barometer at 297, the Thermometer 60 Degrees above Freezing. The Weight of the Balls, their Diameters, and Time of the Descent is in this Table.Balls filled with ☿.Empty Balls.Weight.Diameter.Time.Weight.Diameter.Time.Grains.Tenth inch.½ Secᵈˢ.Grains.Inch.Tenth.½ Secᵈˢ.90888510511799388 less.64252168668859951167477½8 more.5155 nearly16½8087½84835 nearly177847½8 more.6415216The Reason why the heavy, full Balls fell in half the Time of the hollow ones, was the Resistence of the Air: Which Resistence is very ingeniously and accurately assigned by Dr.Wallis, inPhilos. Trans.Nᵒ. 186. And the cause of the Resistence of all Fluids, (as SirIsaac Newton,Opt.Q. 20.) is partly from theFrictionof the Parts of the Fluid, partly from theInertiathereof. The Resistence a spherical Body meets with from Friction, is as the right Angle under the Diameter, and the Velocity of the moving Body: And the Resistence from theVis Inertia, is as the Square of that Product.For a farther Account of the Properties and Proportions,&c.of Gravity in the Fall or Projection of Bodies, I shall refer to the larger Accounts ofGalilæus,Torricellius,Huygens, SirIsaac Newton, &c. or to the shorter Accounts of Dr.Halleyin Philos. Trans. abridged by Mr.Lowthorp, Vol. I. p. 561. or Dr.Clarkein his Notes onRohault,Phys.2. c. 28. §. 13, 16. And for the Resistence of Fluids, I refer to Dr.Wallisbefore-cited, and theAct. Erudit. Lips.May 1693. where there is a way to find the Force of Mediums upon Bodies of different Figures.[b]That the heavenly Bodies move round their own Axes, is, beyond all doubt, manifest to our Eye, in some of them, from the Spots visible on them. The Spots on the Sun (easily visible with an ordinary Glass) do manifest him to revolve round his own Axis in about 25¼ Days. The Spots on ♃ and ♂ prove those two Planets to revolve also from East to West, as Dr.Hookdiscover’d in 1664, and 1665. And ♀ also (although near the strong Rays of the Sun) hath, from some Spots, been discovered by Mr.Cassini, in 1666, and 1667, to have a manifest Rotation.V.Lowth. Abridg.Vol. 1. p. 382, and 423, 425. And such Uniformity hath theCreatorobserv’d in the Works of Nature, that what is observable in one, is generally to be found in all others of the same kind. So that since ’tis manifest the Sun, and three of his Planets whirl round, it is very reasonable to conclude all the rest do so too, yea, every Globe of the Universe.[c]The Earth’s Circumference being 25031½ Miles, (according toBook II. Chap. 2. Note (a).) if we divide that into 24 Hours, we shall find the Motion of the Earth to be nearly 1043 Miles in an Hour. Which, by the by, is a far more reasonable and less rapid Rate, than that of the Sun would be, if we suppose the Earth to stand still, and the Sun to move round the Earth. For according to the Proportions inNote (e), of the preceding Chapter, the Circumference of theMagnus Orbisis 540686225EnglishMiles, which divided by 24 Hours, gives 22528364 Miles in an Hour. But what is this to the Rapidity of the fixt Stars, if we suppose them; not the Earth, to move? Which is a good Argument for the Earth’s Motion.[d]Nihil majus, quàm quòd ita stabilis est Mundus, atque ita cohæret ad permanendum, ut nihil nè excogitari quidem possit aptius. Omnes enim partes ejus undique medium locum capessentes, nituntur æqualiter: maximè autem corpora inter se juncta permanent, cum quodam quasi vinculo circumdata colligantur: quod facit ea natura, quæ per omnem mundum omnia Mente, & Ratione conficiens, funditur, & ad medium rapit, & convertit extrema, Cic. de Nat. Deor. l. 2. c. 45.[e]Eâdem ratione Mare, cùm supra terram sit, medium tamen terræ locum expetens, conglobatur undique æqualiter, neque redundat unquam, neque effunditur.Id. paulo post.[f]That there is no such Thing aspositive Levity, but that Levity is only a less Gravity, is abundantly manifested by the acuteSeig. Alph. Borelli de Mot. à Grav. pend.cap. 4. See also the Annotations of the learned and ingenious Dr. Clark onRohaulti Phys.p. 1. c. 16. Note 3. Also the Exper. of theAcad. del Cimento, p. 118, &c. Dr.Wallis’sDisc. of Gravity and Gravitation before the Royal Society, Nov. 12. 1674. p. 28,&c.[g]I have before inNote (a), Chap. 3.shewn whatVapoursare, and how they are rais’d. That which I shall here note, is their Quantity: Concerning which the before-commended Dr.Halleyhath given us some curious Experiments in ourPhil. Transact.which may be met with together in Mr.Lowthorp’sAbridg.Vol. II.p. 108.and126.Mr.Sedileaualso atParisobserved it for near three Years. By all their Observations it appears, that in the Winter Months the Evaporations are least, and greatest in Summer, and most of all in windy Weather. And byMonsieur Sedileau’s Observations it appears, that what is raised in Vapours, exceeds that which falleth in Rain. In the seven last Months of the Year 1688, the Evaporations amounted to 22 Inches 5 Lines; but the Rain only to Inches 6⅓ Lines: In 1689, the Evaporations were 32 Inches 10½ Lines; but the Rain 18 Inches 1 Line: In 1690, the Evaporations 30 Inches 11 Lines; the Rain 21 Inches ⅓ of a Line.Vid.Mem. de Math. Phys. Ann. 1692.p. 25.If it be demanded, What becomes of the Overplus of Exhalations that descend not in Rain? I answer, They are partly tumbled down and spent by the Winds, and partly descend in Dews, which amount to a greater quantity than is commonly imagined. Dr.Halleyfound the descent of Vapours in Dews so prodigious at St.Helena, that he makes no doubt to attribute the Origine of Fountains thereto. And I my self have seen in a still, cool Evening, large thick Clouds hanging, without any Motion in the Air, which in two or three Hours Time have been melted down by Degrees, by the cold of the Evening, so that not any the least Remains of them have been left.[h]SeeBook II. Chap. 3. Note (c).

[a]That there is such a Thing asGravity, is manifest from its Effects here upon Earth; and that the Heavenly Bodies attract or gravitate to one another, when placed at due Distances, is made highly probable by SirIsaac Newton. This attractive or gravitating Power, I take to be congenial to Matter, and imprinted on all the Matter of the Universe by the Creator’sFiatat the Creation. What theCauseof it is, theNewtonian Philosophydoth not pretend to determine for want of Phænomena, upon which Foundation it is that that Philosophy is grounded, and not upon chimerical and uncertain Hypotheses: But whatever the Cause is, thatCause penetrates even to the Centers of the Sun and Planets, without any Diminution of its Virtue; and it acteth not according to the Superficies of Bodies (as Mechanical Causes do) but in proportion to the Quantity of their solid Matter;and lastly, it acteth all round it at immense Distances, decreasing in duplicate proportion to those Distances, as SirIsaac Newtonsaith,Princip.pag. ult. What useful Deductions, and what a rational Philosophy have been drawn from hence, may be seen in the same Book.This Attraction, or Gravity, as its Force is in a certain proportion, so makes the Descent of Bodies to be at a certain rate. And was it not for the Resistence of the Medium, all Bodies would descend to the Earth at the same rate; the lightest Down, as swiftly as the heaviest Mineral: As is manifest in theAir-Pump, in which the lightest Feather, Dust,&c.and a piece of Lead, drop down seemingly in the same Time, from the top to the bottom of a tall exhausted Receiver.The rate of the Descent of heavy Bodies, according toGalileo, Mr.Huygens, and Dr.Halley(after them) is 16 Feet one Inch in one Second of Time; and in more Seconds, as the Squares of those Times. But in some accurate Experiments made in St.Paul’sDome, June 9. 1710, at the Height of 220 Feet, the Descent was scarcely 14 Feet in the first Second. The Experiments were made in the Presence of some very considerable Members of the Royal Society, by Mr.Hawksbee, their Operator, with glass, hollow Balls, some empty, some filled with Quick-silver, the Barometer at 297, the Thermometer 60 Degrees above Freezing. The Weight of the Balls, their Diameters, and Time of the Descent is in this Table.Balls filled with ☿.Empty Balls.Weight.Diameter.Time.Weight.Diameter.Time.Grains.Tenth inch.½ Secᵈˢ.Grains.Inch.Tenth.½ Secᵈˢ.90888510511799388 less.64252168668859951167477½8 more.5155 nearly16½8087½84835 nearly177847½8 more.6415216The Reason why the heavy, full Balls fell in half the Time of the hollow ones, was the Resistence of the Air: Which Resistence is very ingeniously and accurately assigned by Dr.Wallis, inPhilos. Trans.Nᵒ. 186. And the cause of the Resistence of all Fluids, (as SirIsaac Newton,Opt.Q. 20.) is partly from theFrictionof the Parts of the Fluid, partly from theInertiathereof. The Resistence a spherical Body meets with from Friction, is as the right Angle under the Diameter, and the Velocity of the moving Body: And the Resistence from theVis Inertia, is as the Square of that Product.For a farther Account of the Properties and Proportions,&c.of Gravity in the Fall or Projection of Bodies, I shall refer to the larger Accounts ofGalilæus,Torricellius,Huygens, SirIsaac Newton, &c. or to the shorter Accounts of Dr.Halleyin Philos. Trans. abridged by Mr.Lowthorp, Vol. I. p. 561. or Dr.Clarkein his Notes onRohault,Phys.2. c. 28. §. 13, 16. And for the Resistence of Fluids, I refer to Dr.Wallisbefore-cited, and theAct. Erudit. Lips.May 1693. where there is a way to find the Force of Mediums upon Bodies of different Figures.

This Attraction, or Gravity, as its Force is in a certain proportion, so makes the Descent of Bodies to be at a certain rate. And was it not for the Resistence of the Medium, all Bodies would descend to the Earth at the same rate; the lightest Down, as swiftly as the heaviest Mineral: As is manifest in theAir-Pump, in which the lightest Feather, Dust,&c.and a piece of Lead, drop down seemingly in the same Time, from the top to the bottom of a tall exhausted Receiver.

The rate of the Descent of heavy Bodies, according toGalileo, Mr.Huygens, and Dr.Halley(after them) is 16 Feet one Inch in one Second of Time; and in more Seconds, as the Squares of those Times. But in some accurate Experiments made in St.Paul’sDome, June 9. 1710, at the Height of 220 Feet, the Descent was scarcely 14 Feet in the first Second. The Experiments were made in the Presence of some very considerable Members of the Royal Society, by Mr.Hawksbee, their Operator, with glass, hollow Balls, some empty, some filled with Quick-silver, the Barometer at 297, the Thermometer 60 Degrees above Freezing. The Weight of the Balls, their Diameters, and Time of the Descent is in this Table.

The Reason why the heavy, full Balls fell in half the Time of the hollow ones, was the Resistence of the Air: Which Resistence is very ingeniously and accurately assigned by Dr.Wallis, inPhilos. Trans.Nᵒ. 186. And the cause of the Resistence of all Fluids, (as SirIsaac Newton,Opt.Q. 20.) is partly from theFrictionof the Parts of the Fluid, partly from theInertiathereof. The Resistence a spherical Body meets with from Friction, is as the right Angle under the Diameter, and the Velocity of the moving Body: And the Resistence from theVis Inertia, is as the Square of that Product.

For a farther Account of the Properties and Proportions,&c.of Gravity in the Fall or Projection of Bodies, I shall refer to the larger Accounts ofGalilæus,Torricellius,Huygens, SirIsaac Newton, &c. or to the shorter Accounts of Dr.Halleyin Philos. Trans. abridged by Mr.Lowthorp, Vol. I. p. 561. or Dr.Clarkein his Notes onRohault,Phys.2. c. 28. §. 13, 16. And for the Resistence of Fluids, I refer to Dr.Wallisbefore-cited, and theAct. Erudit. Lips.May 1693. where there is a way to find the Force of Mediums upon Bodies of different Figures.

[b]That the heavenly Bodies move round their own Axes, is, beyond all doubt, manifest to our Eye, in some of them, from the Spots visible on them. The Spots on the Sun (easily visible with an ordinary Glass) do manifest him to revolve round his own Axis in about 25¼ Days. The Spots on ♃ and ♂ prove those two Planets to revolve also from East to West, as Dr.Hookdiscover’d in 1664, and 1665. And ♀ also (although near the strong Rays of the Sun) hath, from some Spots, been discovered by Mr.Cassini, in 1666, and 1667, to have a manifest Rotation.V.Lowth. Abridg.Vol. 1. p. 382, and 423, 425. And such Uniformity hath theCreatorobserv’d in the Works of Nature, that what is observable in one, is generally to be found in all others of the same kind. So that since ’tis manifest the Sun, and three of his Planets whirl round, it is very reasonable to conclude all the rest do so too, yea, every Globe of the Universe.

[c]The Earth’s Circumference being 25031½ Miles, (according toBook II. Chap. 2. Note (a).) if we divide that into 24 Hours, we shall find the Motion of the Earth to be nearly 1043 Miles in an Hour. Which, by the by, is a far more reasonable and less rapid Rate, than that of the Sun would be, if we suppose the Earth to stand still, and the Sun to move round the Earth. For according to the Proportions inNote (e), of the preceding Chapter, the Circumference of theMagnus Orbisis 540686225EnglishMiles, which divided by 24 Hours, gives 22528364 Miles in an Hour. But what is this to the Rapidity of the fixt Stars, if we suppose them; not the Earth, to move? Which is a good Argument for the Earth’s Motion.

[d]Nihil majus, quàm quòd ita stabilis est Mundus, atque ita cohæret ad permanendum, ut nihil nè excogitari quidem possit aptius. Omnes enim partes ejus undique medium locum capessentes, nituntur æqualiter: maximè autem corpora inter se juncta permanent, cum quodam quasi vinculo circumdata colligantur: quod facit ea natura, quæ per omnem mundum omnia Mente, & Ratione conficiens, funditur, & ad medium rapit, & convertit extrema, Cic. de Nat. Deor. l. 2. c. 45.

[e]Eâdem ratione Mare, cùm supra terram sit, medium tamen terræ locum expetens, conglobatur undique æqualiter, neque redundat unquam, neque effunditur.Id. paulo post.

[f]That there is no such Thing aspositive Levity, but that Levity is only a less Gravity, is abundantly manifested by the acuteSeig. Alph. Borelli de Mot. à Grav. pend.cap. 4. See also the Annotations of the learned and ingenious Dr. Clark onRohaulti Phys.p. 1. c. 16. Note 3. Also the Exper. of theAcad. del Cimento, p. 118, &c. Dr.Wallis’sDisc. of Gravity and Gravitation before the Royal Society, Nov. 12. 1674. p. 28,&c.

[g]I have before inNote (a), Chap. 3.shewn whatVapoursare, and how they are rais’d. That which I shall here note, is their Quantity: Concerning which the before-commended Dr.Halleyhath given us some curious Experiments in ourPhil. Transact.which may be met with together in Mr.Lowthorp’sAbridg.Vol. II.p. 108.and126.Mr.Sedileaualso atParisobserved it for near three Years. By all their Observations it appears, that in the Winter Months the Evaporations are least, and greatest in Summer, and most of all in windy Weather. And byMonsieur Sedileau’s Observations it appears, that what is raised in Vapours, exceeds that which falleth in Rain. In the seven last Months of the Year 1688, the Evaporations amounted to 22 Inches 5 Lines; but the Rain only to Inches 6⅓ Lines: In 1689, the Evaporations were 32 Inches 10½ Lines; but the Rain 18 Inches 1 Line: In 1690, the Evaporations 30 Inches 11 Lines; the Rain 21 Inches ⅓ of a Line.Vid.Mem. de Math. Phys. Ann. 1692.p. 25.If it be demanded, What becomes of the Overplus of Exhalations that descend not in Rain? I answer, They are partly tumbled down and spent by the Winds, and partly descend in Dews, which amount to a greater quantity than is commonly imagined. Dr.Halleyfound the descent of Vapours in Dews so prodigious at St.Helena, that he makes no doubt to attribute the Origine of Fountains thereto. And I my self have seen in a still, cool Evening, large thick Clouds hanging, without any Motion in the Air, which in two or three Hours Time have been melted down by Degrees, by the cold of the Evening, so that not any the least Remains of them have been left.

If it be demanded, What becomes of the Overplus of Exhalations that descend not in Rain? I answer, They are partly tumbled down and spent by the Winds, and partly descend in Dews, which amount to a greater quantity than is commonly imagined. Dr.Halleyfound the descent of Vapours in Dews so prodigious at St.Helena, that he makes no doubt to attribute the Origine of Fountains thereto. And I my self have seen in a still, cool Evening, large thick Clouds hanging, without any Motion in the Air, which in two or three Hours Time have been melted down by Degrees, by the cold of the Evening, so that not any the least Remains of them have been left.

[h]SeeBook II. Chap. 3. Note (c).

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