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
Any kind of centripetal force being supposed, and the centre of
force, and any plane whatsoever in which the body revolves, being
given, and the quadratures of curvilinear figures being allowed; it
is required to determine the motion of a body going off from a given
place, with a given velocity, in the direction of a given right line in
that plane.
[Pg 183]
Let S be the centre of force, SC the least distance of that centre from
the given plane, P a body issuing from the place P in the direction of
the right line PZ, Q the same body revolving in its trajectory, and PQR
the trajectory itself which is required to be found, described in that
given plane. Join CQ, QS, and if in QS we take SV proportional to the
centripetal force with which the body is attracted towards the centre
S, and draw VT parallel to CQ, and meeting SC in T; then will the force
SV be resolved into two (by Cor. 2, of the Laws of Motion), the force
ST, and the force TV; of which ST attracting the body in the direction
of a line perpendicular to that plane, does not at all change its
motion in that plane. But the action of the other force TV, coinciding
with the position of the plane itself, attracts the body directly
towards the given point C in that plane; and therefore causes the body
to move in this plane in the same manner as if the force ST were taken
away, and the body were to revolve in free space about the centre C
by means of the force TV alone. But there being given the centripetal
force TV with which the body Q revolves in free space about the given
centre C, there is given (by Prop. XLII) the trajectory PQR which the
body describes; the place Q, in which the body will be found at any
given time; and, lastly, the velocity of the body in that place Q. And
so è contra. Q.E.I.
PROPOSITION XLVII. THEOREM XV.
Supposing the centripetal force to be proportional to the distance
of the body from the centre; all bodies revolving in any planes
whatsoever will describe ellipses, and complete their revolutions in
equal times; and those which move in right lines, running backwards and
forwards alternately, will complete their several periods of going and
returning in the same times.
Public-domain text, read in full here on John Shaqi.
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