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. 1. Hence if the centripetal force be as any power of the altitude,
that power may be found from the motion of the apsides; and so
contrariwise. That is, if the whole angular motion, with which the body
returns to the same apsis, be to the angular motion of one revolution,
or 360 deg., as any number as m to another as n, and
the altitude called A; the force will be as the power
of the altitude A; the index of which power is .
This appears by the second example. Hence it is plain that the
force in its recess from the centre cannot decrease in a greater than
a triplicate ratio of the altitude. A body revolving with such a
force, and parting from the apsis, if it once begins to descend, can
never arrive at the lower apsis or least altitude, but will descend
to the centre, describing the curve line treated of in Cor. 3, Prop.
XLI. But if it should, at its parting from the lower apsis, begin to
ascend never so little, it will ascend in infinitum, and never
come to the upper apsis; but will describe the curve line spoken of
in the same Cor., and Cor. 6, Prop. XLIV. So that where the force in
its recess from the centre decreases in a greater than a triplicate
ratio of the altitude, the body at its parting from the apsis,
will either descend to the centre, or ascend in infinitum,
according as it descends or ascends at the beginning of its motion.
But if the force in its recess from[Pg 181] the centre either decreases in
a less than a triplicate ratio of the altitude, or increases in any
ratio of the altitude whatsoever, the body will never descend to
the centre, but will at some time arrive at the lower apsis; and,
on the contrary, if the body alternately ascending and descending
from one apsis to another never comes to the centre, then either the
force increases in the recess from the centre, or it decreases in
a less than a triplicate ratio of the altitude; and the sooner the
body returns from one apsis to another, the farther is the ratio of
the forces from the triplicate ratio. As if the body should return
to and from the upper apsis by an alternate descent and ascent in 8
revolutions, or in 4, or 2, or ; that is, if m
should be to n as 8, or 4, or 2, or to 1,
and therefore , be , or
, or , or ;
then the force will be as ,
or , or ,
or ; that is, it
will be reciprocally as ,
or , or ,
or . If the body
after each revolution returns to the same apsis, and the apsis
remains unmoved, then m will be to n as 1 to 1, and
therefore will be equal to
, or ; and therefore
the decrease of the forces will be in a duplicate ratio of the
altitude; as was demonstrated above. If the body in three fourth
parts, or two thirds, or one third, or one fourth part of an entire
revolution, return to the same apsis; m will be to n
as or or or
to 1, and therefore
is equal to , or
or , or
; and therefore the force is either reciprocally
as or , or
directly as or . Lastly if the body
in its progress from the upper apsis to the same upper apsis again,
Public-domain text, read in full here on John Shaqi.
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