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
For if the ellipses described were equal to each other, their periodic
times by the last Theorem would be in a subduplicate ratio of the body
S to the sum of the bodies S + P. Let the periodic time in the latter
ellipsis be diminished in that ratio, and the periodic times will
become equal; but, by Prop. XV, the principal axis of the ellipsis
will be diminished in a ratio sesquiplicate to the former ratio; that
is, in a ratio to which the ratio of S to S + P is triplicate; and
therefore that axis will be to the principal axis of the other ellipsis
as the first of two mean proportionals between S + P and S to S + P.
And inversely the principal axis of the ellipsis described about the
movable body will be to the principal axis of that described round the
immovable as S + P to the first of two mean proportionals between S + P
and S. Q.E.D.
PROPOSITION LXI. THEOREM XXIV.
If two bodies attracting each other with any kind of forces, and not
otherwise agitated or obstructed, are moved in any manner whatsoever,
those motions will be the same as if they did not at all attract each
other mutually, but were both attracted with the same forces by a third
body placed in their common centre of gravity; and the law of the[Pg 198]
attracting forces will be the same in respect of the distance of the
bodies from the common centre, as in respect of the distance between
the two bodies.
For those forces with which the bodies attract each other mutually, by
tending to the bodies, tend also to the common centre of gravity lying
directly between them; and therefore are the same as if they proceeded
from an intermediate body. Q.E.D.
And because there is given the ratio of the distance of either body
from that common centre to the distance between the two bodies, there
is given, of course, the ratio of any power of one distance to the
same power of the other distance; and also the ratio of any quantity
derived in any manner from one of the distances compounded any how with
given quantities, to another quantity derived in like manner from the
other distance, and as many given quantities having that given ratio
of the distances to the first. Therefore if the force with which one
body is attracted by another be directly or inversely as the distance
of the bodies from each other, or as any power of that distance; or,
lastly, as any quantity derived after any manner from that distance
compounded with given quantities; then will the same force with which
the same body is attracted to the common centre of gravity be in like
manner directly or inversely as the distance of the attracted body
from the common centre, or as any power of that distance; or, lastly,
as a quantity derived in like sort from that distance compounded with
analogous given quantities. That is, the law of attracting force will
be the same with respect to both distances. Q.E.D.
PROPOSITION LXII. PROBLEM XXXVIII.
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