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
This practice seems to be expeditious enough, because the angles V and
X, taken in second minutes, if you please, being very small, it will
be sufficient to find two or three of their first figures. But it is
likewise sufficiently accurate to answer to the theory of the planet's
motions. For even in the orbit of Mars, where the greatest equation of
the centre amounts to ten degrees, the error will scarcely exceed one
second. But when the angle of the mean motion equated BHP is found, the
angle of the true motion BSP, and the distance SP, are readily had by
the known methods.
And so far concerning the motion of bodies in curve lines. But it may
also come to pass that a moving body shall ascend or descend in a right
line; and I shall now go on to explain what belongs to such kind of
motions.
SECTION VII.
Concerning the rectilinear ascent and descent of bodies.
PROPOSITION XXXII. PROBLEM XXIV.
Supposing that the centripetal force is reciprocally proportional
to the square of the distance of the places from the centre; it is
required to define the spaces which a body, falling directly, describes
in given times.
CASE 1. If the body does not fall perpendicularly, it will (by Cor.
1[Pg 160] Prop. XIII) describe some conic section whose focus is placed in
the centre of force. Suppose that conic section to be ARPB and its
focus S. And, first, if the figure be an ellipsis, upon the greater
axis thereof AB describe the semi-circle ADB, and let the right line
DPC pass through the falling body, making right angles with the axis;
and drawing DS, PS, the area ASD will be proportional to the area
ASP, and therefore also to the time. The axis AB still remaining the
same, let the breadth of the ellipsis be perpetually diminished, and
the area ASD will always remain proportional to the time. Suppose
that breadth to be diminished in infinitum; and the orbit APB
in that case coinciding with the axis AB, and the focus S with the
extreme point of the axis B, the body will descend in the right line
AC, and the area ABD will become proportional to the time. Wherefore
the space AC will be given which the body describes in a given time
by its perpendicular fall from the place A, if the area ABD is taken
proportional to the time, and from the point D the right line DC is let
fall perpendicularly on the right line AB. Q.E.I.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account