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
For if the force with which the body is attracted from T towards C be
expressed by the right line TZ taken proportional to it, that force
will be resolved into two forces TY, YZ, of which YZ drawing the body
in the direction of the length of the thread PT, does not at all change
its motion; whereas the other force TY directly accelerates or retards
its motion in the curve STRQ. Wherefore since that force is as the
space to be described TR, the accelerations or retardations of the body
in describing two proportional parts (a greater and a less) of two
oscillations, will be always as those parts, and therefore will cause
those parts to be described together. But bodies which continually
describe together parts proportional to the wholes, will describe the
wholes together also. Q.E.D.
COR. 1. Hence if the body T, hanging by a rectilinear thread AT from
the centre A, describe the circular arc STRQ, and in the mean time
be acted on by any force tending downwards with parallel directions,
which is to the uniform force of gravity as the arc TR to its sine TN,
the times of the several oscillations will be equal. For because TZ,
AR are parallel, the triangles ATN, ZTY are similar; and therefore TZ
will be to AT as TY to TN; that is, if the uniform force of gravity
be expressed by the given length AT, the force TZ, by which the
oscillations become isochronous, will be to the force of gravity AT, as
the arc TR equal to TY is to TN the sine of that arc.
COR. 2. And therefore in clocks, if forces were impressed by some
machine upon the pendulum which preserves the motion, and so compounded
with the force of gravity that the whole force tending downwards should
be always as a line produced by applying the rectangle under the arc
TR and the radius AR to the sine TN, all the oscillations will become
isochronous.
PROPOSITION LIV. PROBLEM XXXVI.
Granting the quadratures of curvilinear figures, it is required
to find the times in which bodies by means of any centripetal force
will descend or ascend in any curve lines described in a plane passing
through the centre of force.
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