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. 4. If the body L, by a radius drawn to the other body T, describes
areas, which, compared with the times, are very unequal; and that other
body T be either at rest, or moves uniformly forward in a right line:
the action of the centripetal force tending to that other body T is
either none at all, or it is mixed and compounded with very powerful
actions of other forces: and the whole force compounded of them all, if
they are many, is directed to another (immovable or moveable) centre.
The same thing obtains, when the other body is moved by any motion
whatsoever; provided that centripetal force is taken, which remains
after subducting that whole force acting upon that other body T.
SCHOLIUM.
Because the equable description of areas indicates that a centre is
respected by that force with which the body is most affected, and by
which it is drawn back from its rectilinear motion, and retained in its
orbit; why may we not be allowed, in the following discourse, to use
the equable description of areas as an indication of a centre, about
which all circular motion is performed in free spaces?
PROPOSITION IV. THEOREM IV.
The centripetal forces of bodies, which by equable motions describe
different circles, tend to the centres of the same circles; and are
one to the other as the squares of the arcs described in equal times
applied to the radii of the circles.
These forces tend to the centres of the circles (by Prop. II., and Cor.
2, Prop. I.), and are one to another as the versed sines of the least
arcs described in equal times (by Cor. 4, Prop. I.); that is, as the
squares of the same arcs applied to the diameters of the circles (by
Lem. VII.); and therefore since those arcs are as arcs described in any
equal times, and the diameters are as the radii, the forces will be as
the squares of any arcs described in the same time applied to the radii
of the circles. Q.E.D.
COR. 1. Therefore, since those arcs are as the velocities of the
bodies[Pg 108] the centripetal forces are in a ratio compounded of the
duplicate ratio of the velocities directly, and of the simple ratio of
the radii inversely.
COR. 2. And since the periodic times are in a ratio compounded of the
ratio of the radii directly, and the ratio of the velocities inversely,
the centripetal forces, are in a ratio compounded of the ratio of the
radii directly, and the duplicate ratio of the periodic times inversely.
COR. 3. Whence if the periodic times are equal, and the velocities
therefore as the radii, the centripetal forces will be also as the
radii; and the contrary.
COR. 4. If the periodic times and the velocities are both in the
subduplicate ratio of the radii, the centripetal forces will be equal
among themselves; and the contrary.
COR. 5. If the periodic times are as the radii, and therefore the
velocities equal, the centripetal forces will be reciprocally as the
radii; and the contrary.
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