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. 7. If a body, in a medium whose density is reciprocally as
the distances of places from the centre, revolves in any curve AEB
about that centre, and cuts the first radius AS in the same angle
in B as it did before in A, and that with a velocity that shall be
to its first velocity in A reciprocally in a subduplicate ratio of
the distances from the centre (that is, as AS to a mean proportional
between AS and BS) that body will continue to describe innumerable
similar revolutions BFC, CGD, &c., and by its intersections will
distinguish the radius AS into parts AS, BS, CS, DS, &c., that are
continually proportional. But the times of the revolutions will be as
the perimeters of the orbits AEB, BFC, CGD, &c., directly, and the
velocities at the beginnings A, B, C of those orbits inversely; that
is as , ,
. And the whole time in which
the body will arrive at the centre, will be to the time of the
first revolution as the sum of all the continued proportionals
, ,
, going on ad infinitum, to the
first term ; that is, as the first term
to the difference of the two first
, or as
to AB very nearly. Whence the whole time
may be easily found.
COR. 8. From hence also may be deduced, near enough, the motions of
bodies in mediums whose density is either uniform, or observes any
other assigned law. From the centre S, with intervals SA, SB, SC, &c.,
continually proportional, describe as many circles; and suppose the
time of the revolutions between the perimeters of any two of those
circles, in the medium whereof we treated, to be to the time of the
revolutions between the same in the medium proposed as the mean density
of the proposed medium between those circles to the mean density of the
medium whereof we treated, between the same circles, nearly: and that
the secant of the angle in which the spiral above determined, in the
medium whereof we treated, cuts the radius AS, is in the same ratio
to the secant of the angle in which the new spiral, in the proposed
medium, cuts the same radius: and also that the number of all the
revolutions between the same two circles is nearly as the tangents of
those angles. If this be done every where between every two circles,
the motion will be continued through all the circles. And by this means
one may without difficulty conceive at what rate and in what time
bodies ought to revolve in any regular medium.
[Pg 291]
COR. 9. And although these motions becoming eccentrical should be
performed in spirals approaching to an oval figure, yet, conceiving
the several revolutions of those spirals to be at the same distances
from each other, and to approach to the centre by the same degrees as
the spiral above described, we may also understand how the motions of
bodies may be performed in spirals of that kind.
PROPOSITION XVI. THEOREM XIII.
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