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. 2. If the orbit VPK be an ellipsis, having its focus C, and its
highest apsis V, and we suppose the ellipsis upk similar and
equal to it, so that pC may be always equal to PC, and the angle
VCp be to the angle VCP in the given ratio of G to F; and for
the altitude PC or pC we put A, and 2R for the latus rectum
of the ellipsis, the force with which a body may be made to revolve
in a movable ellipsis will be as , and
vice versa. Let the force with which a body may
revolve in an immovable ellipsis be expressed by the quantity
, and the force in V will be
. But the force with which a body
may revolve in a circle at the distance CV, with the same velocity as
a body revolving in an ellipsis has in V, is to the force with which
a body revolving in an ellipsis is acted upon in the apsis V, as half
the latus rectum of the ellipsis to the semi-diameter CV of the circle,
and therefore is as ; and the
force which is to this, as GG - FF to FF, is as
:
and this force (by Cor. 1 of this
Prop.) is the difference of the forces in V, with which the body P
revolves in the immovable ellipsis VPK, and the body p in
the movable ellipsis upk. Therefore since by this Prop. that
difference at any other altitude A is to itself at the altitude CV
as to , the
same difference in every altitude A will be as
.
Therefore to the force ,
by which the body may revolve
[Pg 176]
in an immovable ellipsis VPK add the excess
,
and the sum will be the whole force
by which a body may revolve in the same
time in the movable ellipsis upk.
COR. 3. In the same manner it will be found, that, if the immovable
orbit VPK be an ellipsis having its centre in the centre of the forces
C, and there be supposed a movable ellipsis upk, similar,
equal, and concentrical to it; and 2R be the principal latus rectum of
that ellipsis, and 2T the latus transversum, or greater axis; and the
angle VCp be continually to the angle VCP as G to F; the forces
with which bodies may revolve in the immovable and movable ellipsis,
in equal times, will be as
and
respectively.
COR. 4. And universally, if the greatest altitude CV of the body
be called T, and the radius of the curvature which the orbit
VPK has in V, that is, the radius of a circle equally curve,
be called R, and the centripetal force with which a body may
revolve in any immovable trajectory VPK at the place V be called
, and in other places P be
indefinitely styled X; and the altitude CP be called A, and G be taken
to F in the given ratio of the angle VCp to the angle VCP;
the centripetal force with which the same body will perform the same
motions in the same time, in the same trajectory upk revolving
with a circular motion, will be as the sum of the forces
.
COR. 5. Therefore the motion of a body in an immovable orbit being
given, its angular motion round the centre of the forces may be
increased or diminished in a given ratio; and thence new immovable
orbits may be found in which bodies may revolve with new centripetal
forces.
Public-domain text, read in full here on John Shaqi.
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