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. Hence the greatest and least altitudes of the bodies, that is, the
apsides of the trajectories, may be found very readily. For the apsides
are those points in which a right line IC drawn through the centre falls
perpendicularly upon the trajectory VIK; which comes to pass when the
right lines IK and NK become equal; that is, when the area ABFD is
equal to ZZ.
[Pg 171]
COR. 2. So also the angle KIN, in which the trajectory at any place
cuts the line IC, may be readily found by the given altitude IC of the
body: to wit, by making the sine of that angle to radius as KN to IK;
that is, as Z to the square root of the area ABFD.
COR. 3. If to the centre C, and the principal vertex V, there be
described a conic section VRS; and from any point thereof, as R, there
be drawn the tangent RT meeting the axis CV indefinitely produced in
the point T; and then joining CR there be drawn the right line CP,
equal to the abscissa CT, making an angle VCP proportional to the
sector VCR; and if a centripetal force, reciprocally proportional to
the cubes of the distances of the places from the centre, tends to
the centre C; and from the place V there sets out a body with a just
velocity in the direction of a line perpendicular to the right line
CV; that body will proceed in a trajectory VPQ, which the point P will
always touch; and therefore if the conic section VRS be an hyperbola,
the body will descend to the centre; but if it be an ellipsis, it will
ascend perpetually, and go farther and farther off in infinitum.
And, on the contrary, if a body endued with any velocity goes off from
the place V, and according as it begins either to descend obliquely to
the centre, or ascends obliquely from it, the figure VRS be either an
hyperbola or an ellipsis, the trajectory may be found by increasing
or diminishing the angle VCP in a given ratio. And the centripetal
force becoming centrifugal, the body will ascend obliquely in the
trajectory VPQ, which is found by taking the angle VCP proportional to
the elliptic sector VRC, and the length CP equal to the length CT, as
before. All these things follow from the foregoing Proposition, by the
quadrature of a certain curve, the invention of which, as being easy
enough, for brevity's sake I omit.
PROPOSITION XLII. PROBLEM XXIX.
The law of centripetal force being given, it is required to find the
motion of a body setting out from a given place, with a given velocity,
in the direction of a given right line.
Public-domain text, read in full here on John Shaqi.
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