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. 2. Whence if the velocity of a body in the principal vertex
D is given, the orbit may be readily found; to wit, by taking its
latus rectum to twice the distance DS, in the duplicate ratio of this
given velocity to the velocity of a body revolving in a circle at the
distance DS (by Cor. 3, Prop. XVI.), and then taking DH to DS as the
latus rectum to the difference between the latus rectum and 4DS.
COR. 3. Hence also if a body move in any conic section, and is forced
out of its orbit by any impulse, you may discover the orbit in which it
will afterwards pursue its course. For by compounding the proper motion
of[Pg 125] the body with that motion, which the impulse alone would generate,
you will have the motion with which the body will go off from a given
place of impulse in the direction of a right line given in position.
COR. 4. And if that body is continually disturbed by the action of
some foreign force, we may nearly know its course, by collecting the
changes which that force introduces in some points, and estimating the
continual changes it will undergo in the intermediate places, from the
analogy that appears in the progress of the series.
SCHOLIUM.
If a body P, by means of a centripetal force tending to any given point
R, move in the perimeter of any given conic section whose centre is C;
and the law of the centripetal force is required: draw CG parallel to
the radius RP, and meeting the tangent PG of the orbit in G; and the
force required (by Cor. 1, and Schol. Prop. X., and Cor. 3, Prop. VII.)
will be as .
SECTION IV.
Of the finding of elliptic, parabolic, and hyperbolic orbits, from
the focus given.
LEMMA XV.
If from the two foci S, H, of any ellipsis or
hyperbola, we draw to any third point V the right lines
SV, HV, whereof one HV is equal to the principal
axis of the figure, that is, to the axis in which the foci are
situated, the other, SV, is bisected in T by the
perpendicular TR let fall upon it; that perpendicular TR
will somewhere touch the conic section: and, vice versa, if it does
touch it, HV will be equal to the principal axis of the
figure.
[Pg 126]
For, let the perpendicular TR cut the right line HV, produced, if need
be, in R; and join SR. Because TS, TV are equal, therefore the right
lines SR, VR, as well as the angles TRS, TRV, will be also equal.
Whence the point R will be in the conic section, and the perpendicular
TR will touch the same; and the contrary. Q.E.D.
PROPOSITION XVIII. PROBLEM X.
From a focus and the principal axes given, to describe elliptic and
hyperbolic trajectories, which shall pass through given points, and
touch right lines given by position.
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