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. 2. Hence also follow what Sir Christopher Wren and M.
Huygens have discovered concerning the vulgar cycloid. For
if the diameter of the globe be infinitely increased, its spherical
superficies will be changed into a plane, and the centripetal force
will act uniformly in the direction of lines perpendicular to that
plane, and this cycloid of our's will become the same with the common
cycloid. But in that case the length of the arc of the cycloid between
that plane and the describing point will become equal to four times the
versed sine of half the arc of the wheel between the same plane and the
describing point, as was discovered by Sir Christopher Wren. And
a pendulum between two such cycloids will oscillate in a similar and
equal cycloid in equal times, as M. Huygens demonstrated. The
descent of heavy bodies also in the time of one oscillation will be the
same as M. Huygens exhibited.
The propositions here demonstrated are adapted to the true constitution
of the Earth, in so far as wheels moving in any of its great circles
will describe, by the motions of nails fixed in their perimeters,
cycloids without the globe; and pendulums, in mines and deep caverns
of the Earth, must oscillate in cycloids within the globe, that those
oscillations may be performed in equal times. For gravity (as will be
shewn in the third book) decreases in its progress from the superficies
of the Earth; upwards in a duplicate ratio of the distances from the
centre of the Earth; downwards in a simple ratio of the same.
PROPOSITION LIII. PROBLEM XXXV.
Granting the quadratures of curvilinear figures, it is required
to find the forces with which bodies moving in given curve lines may
always perform their oscillations in equal times.
Let the body T oscillate in any curve line STRQ, whose axis is AR
passing through the centre of force C. Draw TX touching that curve in
any place of the body T, and in that tangent TX take TY equal to the
arc TR. The length of that arc is known from the common methods used[Pg 191]
for the quadratures of figures. From the point Y draw the right line YZ
perpendicular to the tangent. Draw CT meeting that perpendicular in Z,
and the centripetal force will be proportional to the right line TZ.
Q.E.I.
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