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
For the accelerative attractions of all the bodies B, C, D, towards
A, are by the supposition equal to each other at equal distances; and
in like manner the accelerative attractions of all the bodies towards
B are also equal to each other at equal distances. But the absolute
attractive force of the body A is to the absolute attractive force of
the body B as the accelerative attraction of all the bodies towards A
to the accelerative attraction of all the bodies towards B at equal
distances; and so is also the accelerative attraction of the body B
towards A to the accelerative attraction[Pg 217] of the body A towards B.
But the accelerative attraction of the body B towards A is to the
accelerative attraction of the body A towards B as the mass of the body
A to the mass of the body B; because the motive forces which (by the
2d, 7th, and 8th Definition) are as the accelerative forces and the
bodies attracted conjunctly are here equal to one another by the third
Law. Therefore the absolute attractive force of the body A is to the
absolute attractive force of the body B as the mass of the body A to
the mass of the body B. Q.E.D.
COR. 1. Therefore if each of the bodies of the system A, B, C, D, &c.
does singly attract all the rest with accelerative forces that are
reciprocally as the squares of the distances from the attracting body,
the absolute forces of all those bodies will be to each other as the
bodies themselves.
COR. 2. By a like reasoning, if each of the bodies of the system A, B,
C, D, &c., do singly attract all the rest with accelerative forces,
which are either reciprocally or directly in the ratio of any power
whatever of the distances from the attracting body; or which are
defined by the distances from each of the attracting bodies according
to any common law; it is plain that the absolute forces of those bodies
are as the bodies themselves.
COR. 3. In a system of bodies whose forces decrease in the duplicate
ratio of the distances, if the lesser revolve about one very great one
in ellipses, having their common focus in the centre of that great
body, and of a figure exceedingly accurate; and moreover by radii drawn
to that great body describe areas proportional to the times exactly;
the absolute forces of those bodies to each other will be either
accurately or very nearly in the ratio of the bodies. And so on the
contrary. This appears from Cor. of Prop. XLVIII, compared with the
first Corollary of this Prop.
SCHOLIUM.
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