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
Suppose CA, CB to be semi-axes of the ellipsis; GP, DK, conjugate
diameters; PF, QT perpendiculars to those diameters; Qv
an ordinate to the diameter GP; and if the parallelogram
QvPR be completed, then (by the properties of the conic
sections) the rectangle PvG will be to as
to ; and (because of the similar
triangles QvT, PCF), to
as to ; and, by composition,
the ratio of PvG to is compounded of the
ratio of to , and of the ratio
of to , that is, vG to
as to
. Put QR
for Pv, and (by Lem. XII)
for ; also (the points P and
Q coinciding) 2PC for vG; and multiplying[Pg 115] the extremes
and means together, we shall have
equal to .
Therefore (by Cor. 5, Prop. VI), the centripetal force is reciprocally
as ;
that is (because is given),
reciprocally as ; that is, directly as the
distance PC. Q.E.I.
The same otherwise.
In the right line PG on the other side of the point T, take the point
u so that Tu may be equal to Tv; then take
uV, such as shall be to vG as to
. And because is to PvG as
to (by the conic sections), we
shall have . Add the
rectangle uPv to both sides, and the square of the chord
of the arc PQ will be equal to the rectangle VPv; and therefore
a circle which touches the conic section in P, and passes through the
point Q, will pass also through the point V. Now let the points P and
Q meet, and the ratio of uV to vG, which is the same
with the ratio of to , will become
the ratio of PV to PG, or PV to 2PC; and therefore PV will be equal
to . And therefore the force
by which the body P revolves in the ellipsis will be reciprocally as
(by Cor.
3, Prop. VI); that is (because
is given) directly as PC. Q.E.I.
COR. 1. And therefore the force is as the distance of the body from the
centre of the ellipsis; and, vice versa, if the force is as the
distance, the body will move in an ellipsis whose centre coincides with
the centre of force, or perhaps in a circle into which the ellipsis may
degenerate.
COR. 2. And the periodic times of the revolutions made in all ellipses
whatsoever about the same centre will be equal. For those times in
similar ellipses will be equal (by Corol. 3 and 8, Prop. IV); but in
ellipses that have their greater axis common, they are one to another
as the whole areas of the ellipses directly, and the parts of the areas
described in the same time inversely; that is, as the lesser axes
directly, and the velocities of the bodies in their principal vertices
inversely; that is, as those lesser axes directly, and the ordinates to
the same point of the common axes inversely; and therefore (because of
the equality of the direct and inverse ratios) in the ratio of equality.
SCHOLIUM.
Public-domain text, read in full here on John Shaqi.
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