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 A to be the principal vertex, S the focus, and O the centre
of the ellipsis APB; and let P be the place of the body to be
found. Produce OA to G so as OG may be to OA as OA to OS. Erect the
perpendicular GH; and about the centre O, with the interval OG,
describe the circle GEF; and on the ruler GH, as a base, suppose the
wheel GEF to move forwards, revolving about its axis, and in the mean
time by its point A describing the cycloid ALI. Which done, take GK to
the perimeter GEFG of the wheel, in the ratio of the time in which the
body proceeding from A described the arc AP, to the time of a whole
revolution in the ellipsis. Erect the perpendicular KL meeting the
cycloid in L; then LP drawn parallel to KG will meet the ellipsis in P,
the required place of the body.
For about the centre O with the interval OA describe the semi-circle
AQB, and let LP, produced, if need be, meet the arc AQ, in Q, and
join[Pg 157] SQ, OQ. Let OQ meet the arc EFG in F, and upon OQ let fall
the perpendicular SR. The area APS is as the area AQS, that is, as
the difference between the sector OQA and the triangle OQS, or as
the difference of the rectangles
, and
,
that is, because is given, as the
difference between the arc AQ and the right line SR; and therefore
(because of the equality of the given ratios SR to the sine of the arc
AQ, OS to OA, OA to OG, AQ to GF; and by division, AQ - SR to GF - sine
of the arc AQ) as GK, the difference between the arc GF and the sine of
the arc AQ. Q.E.D.
SCHOLIUM.
Public-domain text, read in full here on John Shaqi.
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