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. 1. From the three last Propositions it follows, that if any body P
goes from the place P with any velocity in the direction of any right
line PR, and at the same time is urged by the action of a centripetal
force that is reciprocally proportional to the square of the distance
of the places from the centre, the body will move in one of the conic
sections, having its focus in the centre of force; and the contrary.
For the focus, the point of contact, and the position of the tangent,
being given, a conic section may be described, which at that point
shall have a given curvature. But the curvature is given from the
centripetal force and velocity of the body being given; and two orbits,
mutually touching one the other, cannot be described by the same
centripetal force and the same velocity.
COR. 2. If the velocity with which the body goes from its place P is
such, that in any infinitely small moment of time the lineola PR may be
thereby described; and the centripetal force such as in the same time
to move the same body through the space QR; the body will move in one
of the conic sections, whose principal latus rectum is the quantity
in its ultimate state, when the
lineolæ PR, QR are diminished in infinitum. In these Corollaries
I consider the circle as an ellipsis; and I except the case where the
body descends to the centre in a right line.
PROPOSITION XIV. THEOREM VI.
If several bodies revolve about one common centre, and the
centripetal force is reciprocally in the duplicate ratio of the
distance of places from the centre; I say, that the principal latera
recta of their orbits are in the duplicate ratio of the areas, which
the bodies by radii drawn to the centre describe in the same time.
[Pg 121]
For (by Cor. 2, Prop. XIII) the latus rectum L is equal to the
quantity in its
ultimate state when the points P and Q coincide. But the lineola QR
in a given time is as the generating centripetal force; that is (by
supposition), reciprocally as SP2. And therefore
is as QT2 × SP2; that is, the
latus rectum L is in the duplicate ratio of the area QT × SP. Q.E.D.
COR. Hence the whole area of the ellipsis, and the rectangle under the
axes, which is proportional to it, is in the ratio compounded of the
subduplicate ratio of the latus rectum, and the ratio of the periodic
time. For the whole area is as the area QT × SP, described in a given
time, multiplied by the periodic time.
PROPOSITION XV. THEOREM VII.
The same things being supposed, I say, that the periodic times in
ellipses are in the sesquiplicate ratio of their greater axes.
Public-domain text, read in full here on John Shaqi.
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