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
COR. 7. It also follows, from what was before laid down, that the axis
of the ellipsis described by the body P, or the line of the apsides,
does as to its angular motion go forwards and backwards by turns, but
more forwards than backwards, and by the excess of its direct motion is
in the whole carried forwards. For the force with which the body P is
urged to the body T at the quadratures, where the force MN vanishes,
is compounded of the force LM and the centripetal force with which
the body T attracts the body P. The first force LM, if the distance
PT be increased, is increased in nearly the same proportion with that
distance, and the other force decreases in the duplicate ratio of the
distance; and therefore the sum of these two forces decreases in a less
than the duplicate ratio of the distance PT; and therefore, by Cor. 1,
Prop. XLV, will make the line of the apsides, or, which is the same
thing, the upper apsis, to go backward. But at the conjunction and
opposition the force with which the body P is urged towards the body
T is the difference of the force KL, and of the force with which the
body T attracts the body P; and that difference, because the force KL
is very nearly increased in the ratio of the distance PT, decreases in
more than the duplicate ratio of the distance PT; and therefore, by
Cor. 1, Prop. XLV, causes the line of the apsides to go forwards. In
the places between the syzygies and the quadratures, the motion[Pg 207] of the
line of the apsides depends upon both of these causes conjunctly, so
that it either goes forwards or backwards in proportion to the excess
of one of these causes above the other. Therefore since the force
KL in the syzygies is almost twice as great as the force LM in the
quadratures, the excess will be on the side of the force KL, and by
consequence the line of the apsides will be carried forwards.
The truth of this and the foregoing Corollary will be more easily
understood by conceiving the system of the two bodies T and P to be
surrounded on every side by several bodies S, S, S, &c., disposed about
the orbit ESE. For by the actions of these bodies the action of the
body T will be diminished on every side, and decrease in more than a
duplicate ratio of the distance.
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