BOOK III. PROPOSITION VI. THEOREM VI.

_That all bodies gravitate towards every planet; and that the weights

of bodies towards any the same planet, at equal distances from the

centre of the planet, are proportional to the quantities of matter

which they severally contain._

It has been, now of a long time, observed by others, that all sorts of

heavy bodies (allowance being made for the inequality of retardation

which they suffer from a small power of resistance in the air) descend

to the earth _from equal heights_ in equal times; and that

equality of times we may distinguish to a great accuracy, by the help

of pendulums. I tried the things in gold, silver, lead, glass, sand,

common salt, wood, water, and wheat. I provided two wooden boxes,

round and equal; I filled the one with wood, and suspended an equal

weight of gold (as exactly as I could) in the centre of oscillation

of the other. The boxes hanging by equal threads of 11 feet made a

couple of pendulums perfectly equal in weight and figure, and equally

receiving the resistance of the air. And, placing the one by the

other, I observed them to play together forwards and backwards, for

a long time, with equal vibrations ... and the like happened in the

other bodies. By these experiments, in bodies of the same weight, I

could manifestly have discovered a difference of matter less than

the thousandth part of the whole, had any such been. But, without

all doubt, the nature of gravity towards the planets is the same

as towards the earth.... Moreover, since the satellites of Jupiter

perform their revolutions in times which observe the sesquiplicate

proportion of their distances from Jupiter’s centre--that is, equal

at equal distances. And, therefore, these satellites, if supposed

to fall _towards Jupiter_ from equal heights, would describe

equal spaces in equal times, in like manner as heavy bodies do on

our earth.... If, at equal distances from the sun, any satellite, in

proportion to the quantity of its matter, did gravitate towards the

sun with a force greater than Jupiter in proportion to his, according

to any given proportion, suppose of _d_ to _e_; then the

distance between the centres of the sun and of the satellite’s orbit

would be always greater than the distance between the centres of the

sun and of Jupiter nearly in the sub-duplicate of that proportion; as

by some computations I have found. And if the satellite did gravitate

towards the sun with a force, lesser in the proportion of _e_ to

_d_, the distance of the centre of the satellite’s orbit from

the sun would be less than the distance of the centre of Jupiter from

the sun in the sub-duplicate of the same proportion. Therefore if, at

equal distances from the sun, the accelerative gravity of any satellite

towards the sun were greater or less than the accelerative gravity of

Jupiter towards the sun but one 1-1000 part of the whole gravity, the

distance of the centre of the satellite’s orbit from the sun would be

greater or less than the distance of Jupiter from the sun by one 1-2000

part of the whole distance--that is, by a fifth part of the distance

of the utmost satellite from the centre of Jupiter; an eccentricity of

the orbit which would be very sensible. But the orbits of the satellite

are concentric to Jupiter, and therefore the accelerative gravities of

Jupiter, and of all its satellites towards the sun, are equal among

themselves....

But further; the weights of all the parts of every planet towards

any other planet are one to another as the matter in the several

parts; for if some parts did gravitate more, others less, than for

the quantity of their matter, then the whole planet, according to the

sort of parts with which it most abounds, would gravitate more or less

than in proportion to the quantity of matter in the whole. Nor is it

of any moment whether these parts are external or internal; for if,

for example, we should imagine the terrestrial bodies with us to be

raised up to the orb of the moon, to be there compared with its body;

if the weights of such bodies were to the weights of the external parts

of the moon as the quantities of matter in the one and in the other

respectively; but to the weights of the internal parts in a greater or

less proportion, then likewise the weights of those bodies would be to

the weight of the whole moon in a greater or less proportion; against

what we have showed above.

Cor. 1. Hence the weights of bodies do not depend upon their forms and

textures; for if the weights could be altered with the forms, they

would be greater or less, according to the variety of forms in equal

matter; altogether against experience.

Cor. 2. Universally, all bodies about the earth gravitate towards the

earth; and the weights of all, at equal distances from the earth’s

centre, are as the quantities of matter which they severally contain.

This is the quality of all bodies within the reach of our experiments;

and therefore (by rule 3) to be affirmed of all bodies whatsoever....

Cor. 5. The power of gravity is of a different nature from the power of

magnetism; for the magnetic attraction is not as the matter attracted.

Some bodies are attracted more by the magnet; others less; most bodies

not at all. The power of magnetism in one and the same body may be

increased and diminished; and is sometimes far stronger, for the

quantity of matter, than the power of gravity; and in receding from

the magnet decreases not in the duplicate but almost in the triplicate

proportion of the distance, as nearly as I could judge from some rude

observations.

Classics of modern science · 第 2 / 8 章