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 the spherical bodies A, B be suspended by the parallel and equal
strings AC, BD, from the centres C, D. About these centres, with those
intervals, describe the semicircles EAF, GBH, bisected by the radii CA,
DB. Bring the body A to any point R of the arc EAF, and (withdrawing
the body B) let it go from thence, and after one oscillation suppose
it to return to the point V: then RV will be the retardation arising
from the resistance of the air. Of this RV let ST be a fourth part,
situated in the middle, to wit, so as RS and TV may be equal, and
RS may be to ST as 3 to 2 then will ST represent very nearly the
retardation during the descent from S to A. Restore the body B to its
place: and, supposing the body A to be let fall from the point S, the
velocity thereof in the place of reflexion A, without sensible error,
will be the same as if it had descended in vacuo from the point
T. Upon which account this velocity may be represented by the chord
of the arc TA. For it is a proposition well known to geometers, that
the velocity of a pendulous body in the lowest point is as the chord
of the arc which it has described in its descent. After[Pg 91] reflexion,
suppose the body A comes to the place s, and the body B to the
place k. Withdraw the body B, and find the place v, from
which if the body A, being let go, should after one oscillation return
to the place r, st may be a fourth part of rv, so
placed in the middle thereof as to leave rs equal to tv,
and let the chord of the arc tA represent the velocity which the
body A had in the place A immediately after reflexion. For t
will be the true and correct place to which the body A should have
ascended, if the resistance of the air had been taken off. In the same
way we are to correct the place k to which the body B ascends,
by finding the place l to which it should have ascended in
vacuo. And thus everything may be subjected to experiment, in the
same manner as if we were really placed in vacuo. These things
being done, we are to take the product (if I may so say) of the body
A, by the chord of the arc TA (which represents its velocity), that we
may have its motion in the place A immediately before reflexion; and
then by the chord of the arc tA, that we may have its motion
in the place A immediately after reflexion. And so we are to take the
product of the body B by the chord of the arc Bl, that we may
have the motion of the same immediately after reflexion. And in like
manner, when two bodies are let go together from different places, we
are to find the motion of each, as well before as after reflexion; and
then we may compare the motions between themselves, and collect the
effects of the reflexion. Thus trying the thing with pendulums of ten
feet, in unequal as well as equal bodies, and making the bodies to
concur after a descent through large spaces, as of 8, 12, or 16 feet,
I found always, without an error of 3 inches, that when the bodies
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