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. 6. If the periodic times are in the sesquiplicate ratio of the
radii, and therefore the velocities reciprocally in the subduplicate
ratio of the radii, the centripetal forces will be in the duplicate
ratio of the radii inversely; and the contrary.
COR. 7. And universally, if the periodic time is as any power Rn of
the radius R, and therefore the velocity reciprocally as the power
of the radius, the centripetal force will be
reciprocally as the power of the radius; and
the contrary.
COR. 8. The same things all hold concerning the times, the velocities,
and forces by which bodies describe the similar parts of any similar
figures that have their centres in a similar position with those
figures; as appears by applying the demonstration of the preceding
cases to those. And the application is easy, by only substituting the
equable description of areas in the place of equable motion, and using
the distances of the bodies from the centres instead of the radii.
COR. 9. From the same demonstration it likewise follows, that the arc
which a body, uniformly revolving in a circle by means of a given
centripetal force, describes in any time, is a mean proportional
between the diameter of the circle, and the space which the same body
falling by the same given force would descend through in the same given
time.
SCHOLIUM.
The case of the 6th Corollary obtains in the celestial bodies (as Sir
Christopher Wren, Dr. Hooke, and Dr. Halley have severally observed);
and therefore in what follows, I intend to treat more at large of those
things which relate to centripetal force decreasing in a duplicate
ratio of the distances from the centres.
Moreover, by means of the preceding Proposition and its Corollaries,
we[Pg 109] may discover the proportion of a centripetal force to any other
known force, such as that of gravity. For if a body by means of its
gravity revolves in a circle concentric to the earth, this gravity
is the centripetal force of that body. But from the descent of
heavy bodies, the time of one entire revolution, as well as the arc
described in any given time, is given (by Cor. 9 of this Prop.).
And by such propositions, Mr. Huygens, in his excellent book De
Horologio Oscillatorio, has compared the force of gravity with the
centrifugal forces of revolving bodies.
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