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
Let S be the focus, and A the principal vertex of the parabola; and
suppose 4AS × M equal to the parabolic area to be cut off APS, which
either was described by the radius SP, since the body's departure from
the vertex, or is to be described thereby before its arrival there. Now
the quantity of that area to be cut off is known from the time which
is proportional to it. Bisect AS in G, and erect the perpendicular
GH equal to 3M, and a circle described about the centre H, with the
interval HS, will cut the parabola in the place P required. For letting
fall PO perpendicular on the axis, and drawing ,
there will be
(= ) = .
[Pg 154]
Whence . For write
;
then dividing all the terms by 3PO, and multiplying them by 2AS, we shall have
= to the area
= to the area APS. But GH was 3M, and therefore
is 4AS × M. Wherefore
the area cut off APS is equal to the area that was to be cut off 4AS ×
M. Q.E.D.
COR. 1. Hence GH is to AS as the time in which the body described the
arc AP to the time in which the body described the arc between the
vertex A and the perpendicular erected from the focus S upon the axis.
COR. 2. And supposing a circle ASP perpetually to pass through the
moving body P, the velocity of the point H is to the velocity which the
body had in the vertex A as 3 to 8; and therefore in the same ratio is
the line GH to the right line which the body, in the time of its moving
from A to P, would describe with that velocity which it had in the
vertex A.
COR. 3. Hence, also, on the other hand, the time may be found in which
the body has described any assigned arc AP. Join AP, and on its middle
point erect a perpendicular meeting the right line GH in H.
LEMMA XXVIII.
There is no oval figure whose area, cut off by right lines at
pleasure, can be universally found by means of equations of any number
of finite terms and dimensions.
Public-domain text, read in full here on John Shaqi.
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