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
CASE 1. If the figure DES is a circle, or a rectangular hyperbola,
bisect its transverse diameter AS in O, and SO will be half the latus
rectum. And because TC is to TD as Cc to Dd, and TD to
TS as CD to SY; ex æquo TC will be to TS as CD × Cc to
SY × Dd. But (by Cor. 1, Prop. XXXIII) TC is to TS as AC to AO;
to wit, if in the coalescence of the points D, d, the ultimate
ratios of the lines are taken. Wherefore AC is to AO or SK as CD ×
Cc to SY × Dd. Farther, the velocity of the descending
body in C is to the velocity of a body describing a circle about the
centre S, at the interval SC, in the subduplicate ratio of AC to AO
or SK (by Prop. XXXIII); and this velocity is to the velocity of a
body describing the circle OKk in the subduplicate ratio of SK
to SC (by Cor. 6, Prop IV); and, ex æquo, the first velocity
to the last, that is, the little line Cc to the arc Kk,
in the subduplicate ratio of AC to SC, that is, in the ratio of AC
to CD. Wherefore CD × Cc is equal to AC × Kk, and
consequently AC to SK as AC × Kk to SY × Dd, and thence
SK × Kk equal to SY × Dd, and equal
to , that is, the area
KSk equal to the area SDd. Therefore in every moment
of time two equal particles, KSk and SDd, of areas are
generated, which, if their magnitude is diminished, and their number
increased in infinitum, obtain the ratio of equality, and
consequently (by Cor. Lem. IV), the whole areas together generated are
always equal. Q.E.D.
[Pg 164]
CASE 2. But if the figure DES is a parabola, we shall find, as above,
CD × Cc to SY × Dd as TC to TS, that is, as 2 to 1; and
that therefore , is equal to
. But the velocity of
the falling body in C is equal to the velocity with which a circle may
be uniformly described at the interval (by
Prop. XXXIV). And this velocity to the velocity with which a circle may
be described with the radius SK, that is, the little line Cc
to the arc Kk, is (by Cor. 6, Prop. IV) in the subduplicate
ratio of SK to ; that is, in the ratio of
SK to . Wherefore
is equal to , and
therefore equal to ;
that is, the area KSk is equal to the area SDd, as above.
Q.E.D.
PROPOSITION XXXVI. PROBLEM XXV.
To determine the times of the descent of a body falling from a given
place A.
Upon the diameter AS, the distance of the body from the centre at the
beginning, describe the semi-circle ADS, as likewise the semi-circle
OKH equal thereto, about the centre S. From any place C of the body
erect the ordinate CD. Join SD, and make the sector OSK equal to the
area ASD. It is evident (by Prop. XXXV) that the body in falling will
describe the space AC in the same time in which another body, uniformly
revolving about the centre S, may describe the arc OK. Q.E.F.
PROPOSITION XXXVII. PROBLEM XXVI.
To define the times of the ascent or descent of a body projected
upwards or downwards from a given place.
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