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. The force with which the body T is accelerated or retarded in any
place T of the cycloid, is to the whole weight of the same body in the
highest place S or Q as the arc of the cycloid TR is to the arc SR or
QR.
PROPOSITION LII. PROBLEM XXXIV.
To define the velocities of the pendulums in the several places, and
the times in which both the entire oscillations, and the several parts
of them are performed.
About any centre G, with the interval GH equal to the arc of the
cycloid RS, describe a semi-circle HKM bisected by the semi-diameter
GK. And if a centripetal force proportional to the distance of the
places from the centre tend to the centre G, and it be in the perimeter
HIK equal to the centripetal force in the perimeter of the globe QOS
tending towards its centre, and at the same time that the pendulum T is
let fall from the highest place S, a body, as L, is let fall from H to
G; then because the[Pg 189] forces which act upon the bodies are equal at the
beginning, and always proportional to the spaces to be described TR,
LG, and therefore if TR and LG are equal, are also equal in the places
T and L, it is plain that those bodies describe at the beginning equal
spaces ST, HL, and therefore are still acted upon equally, and continue
to describe equal spaces.
Therefore by Prop. XXXVIII, the time in which the body describes the
arc ST is to the time of one oscillation, as the arc HI the time in
which the body H arrives at L, to the semi-periphery HKM, the time in
which the body H will come to M. And the velocity of the pendulous
body in the place T is to its velocity in the lowest place R, that
is, the velocity of the body H in the place L to its velocity in the
place G, or the momentary increment of the line HL to the momentary
increment of the line HG (the arcs HI, HK increasing with an equable
flux) as the ordinate LI to the radius GK, or as
to SR. Hence, since in unequal oscillations there
are described in equal time arcs proportional to the entire arcs of
the oscillations, there are obtained from the times given, both the
velocities and the arcs described in all the oscillations universally.
Which was first required.
[Pg 190]
Public-domain text, read in full here on John Shaqi.
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