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
Let now any pendulous bodies oscillate in different cycloids described
within different globes, whose absolute forces are also different; and
if the absolute force of any globe QOS be called V, the accelerative
force with which the pendulum is acted on in the circumference of
this globe, when it begins to move directly towards its centre, will
be as the distance of the pendulous body from that centre and the
absolute force of the globe conjunctly, that is, as CO × V. Therefore
the lineola HY, which is as this accelerated force CO × V, will be
described in a given time; and if there be erected the perpendicular
YZ meeting the circumference in Z, the nascent arc HZ will denote
that given time. But that nascent arc HZ is in the subduplicate
ratio of the rectangle GHY, and therefore as
.
Whence the time of an entire oscillation in the cycloid QRS (it being
as the semi-periphery HKM, which denotes that entire oscillation,
directly; and as the arc HZ which in like manner denotes a given time
inversely) will be as GH directly and
inversely; that is, because GH and SR are equal, as
,
or (by Cor. Prop. L.) as
.
Therefore the oscillations in all globes and cycloids, performed
with what absolute forces soever, are in a ratio compounded of the
subduplicate ratio of the length of the string directly, and the
subduplicate ratio of the distance between the point of suspension and
the centre of the globe inversely, and the subduplicate ratio of the
absolute force of the globe inversely also. Q.E.I.
COR. 1. Hence also the times of oscillating, falling, and revolving
bodies may be compared among themselves. For if the diameter of
the wheel with which the cycloid is described within the globe is
supposed equal to the semi-diameter of the globe, the cycloid will
become a right line passing through the centre of the globe, and the
oscillation will be changed into a descent and subsequent ascent in
that right line. Whence there is given both the time of the descent
from any place to the centre, and the time equal to it in which
the body revolving uniformly about the centre of the globe at any
distance describes an arc of a quadrant. For this time (by Case 2)
is to the time of half the oscillation in any cycloid QRS as 1 to
.
Public-domain text, read in full here on John Shaqi.
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