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
In a sphere described about the centre S with the interval
SA, if there be taken SI, SA, SP
continually proportional; I say, that the attraction of a corpuscle
within the sphere in any place I is to its attraction without
the sphere in the place P in a ratio compounded of the
subduplicate ratio of IS, PS, the distances from the
centre, and the subduplicate ratio of the centripetal forces tending to
the centre in those places P and I.
As if the centripetal forces of the particles of the sphere be
reciprocally as the distances of the corpuscle attracted by them; the
force with which the corpuscle situate in I is attracted by the entire
sphere will be to the force with which it is attracted in P in a ratio
compounded of the subduplicate ratio of the distance SI to the distance
SP, and the subduplicate ratio of the centripetal force in the place I
arising from any particle in the centre to the centripetal force in the
place P arising from the same particle in the centre; that is, in the
subduplicate ratio of the distances SI, SP to each other reciprocally.
These two subduplicate ratios compose the ratio of equality, and
therefore the attractions in I and P produced by the whole sphere are
equal. By the like calculation, if the forces of the particles of
the sphere are reciprocally in a duplicate ratio of the distances,
it will be found that the attraction in I is to the attraction in P
as the distance SP to the semi-diameter SA of the sphere. If those
forces are reciprocally in a triplicate ratio of the distances, the
attractions in I and P will be to each other as SP2 to SA2; if in a
quadruplicate ratio, as SP3 to SA3. Therefore since the attraction
in P was found in this last case to be reciprocally as PS3 × PI, the
attraction in I will be reciprocally as SA3 × PI, that is, because
SA3 is given reciprocally as PI. And the progression is the same in
infinitum. The demonstration of this Theorem is as follows:
The things remaining as above constructed, and a corpuscle being in
any[Pg 232] place P, the ordinate DN was found to be as
.
Therefore if be drawn, that ordinate for any other place
of the corpuscle, as I, will become (mutatis mutandis) as
.
Suppose the centripetal forces flowing from any point of
the sphere, as E, to be to each other at the distances
and as to
(where the number n denotes the index of the powers of PE
and IE), and those ordinates will become as
and
whose ratio to each other is as
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