Newton's Principia : $b The mathematical principles of natural philosophyNewton, Isaac
General
Newton's Principia : $b The mathematical principles of natural philosophy
Newton, Isaac
Celestial mechanics -- Early works to 1800; Mechanics -- Early works to 1800
PROPOSITION LXXIII. THEOREM XXXIII.
If to the several points of a given sphere there tend equal
centripetal forces decreasing in a duplicate ratio of the distances
from the points; I say, that a corpuscle placed within the sphere is
attracted by a force proportional to its distance from the centre.
In the sphere ABCD, described about the centre S, let there be placed
the corpuscle P; and about the same centre S, with the interval SP,
conceive described an interior sphere PEQF. It is plain (by Prop. LXX)
that the concentric sphærical superficies, of which the difference
AEBF of the spheres is composed, have no effect at all upon the body
P, their attractions[Pg 221] being destroyed by contrary attractions. There
remains, therefore, only the attraction of the interior sphere PEQF.
And (by Prop. LXXII) this is as the distance PS. Q.E.D.
SCHOLIUM.
By the superficies of which I here imagine the solids composed, I do
not mean superficies purely mathematical, but orbs so extremely thin,
that their thickness is as nothing; that is, the evanescent orbs of
which the sphere will at last consist, when the number of the orbs is
increased, and their thickness diminished without end. In like manner,
by the points of which lines, surfaces, and solids are said to be
composed, are to be understood equal particles, whose magnitude is
perfectly inconsiderable.
PROPOSITION LXXIV. THEOREM XXXIV.
The same things supposed, I say, that a corpuscle situate without
the sphere is attracted with a force reciprocally proportional to the
square of its distance from the centre.
For suppose the sphere to be divided into innumerable concentric
sphærical superficies, and the attractions of the corpuscle arising
from the several superficies will be reciprocally proportional to the
square of the distance of the corpuscle from the centre of the sphere
(by Prop. LXXI). And, by composition, the sum of those attractions,
that is, the attraction of the corpuscle towards the entire sphere,
will be in the same ratio. Q.E.D.
COR. 1. Hence the attractions of homogeneous spheres at equal distances
from the centres will be as the spheres themselves. For (by Prop.
LXXII) if the distances be proportional to the diameters of the
spheres, the forces will be as the diameters. Let the greater distance
be diminished in that ratio; and the distances now being equal, the
attraction will be increased in the duplicate of that ratio; and
therefore will be to the other attraction in the triplicate of that
ratio; that is, in the ratio of the spheres.
COR. 2. At any distances whatever the attractions are as the spheres
applied to the squares of the distances.
COR. 3. If a corpuscle placed without an homogeneous sphere is
attracted by a force reciprocally proportional to the square of its
distance from the centre, and the sphere consists of attractive
particles, the force of every particle will decrease in a duplicate
ratio of the distance from each particle.
PROPOSITION LXXV. THEOREM XXXV.
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