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
For letting all things stand as in the foregoing Proposition, the force
SV, with which the body Q revolving in any plane PQR is attracted
towards the centre S, is as the distance SQ; and therefore because SV
and SQ, TV and CQ are proportional, the force TV with which the body
is attracted towards the given point C in the plane of the orbit is as
the distance CQ. Therefore the forces with which bodies found in the
plane PQR are attracted towards the point C, are in proportion to the
distances equal to the forces with which the same bodies are attracted
every way towards the centre S; and therefore the bodies will move
in the same times, and in the same figures, in any plane PQR about
the point C, as they[Pg 184] would do in free spaces about the centre S; and
therefore (by Cor. 2, Prop. X, and Cor. 2, Prop. XXXVIII.) they will in
equal times either describe ellipses in that plane about the centre C,
or move to and fro in right lines passing through the centre C in that
plane; completing the same periods of time in all cases. Q.E.D.
SCHOLIUM.
The ascent and descent of bodies in curve superficies has a near
relation to these motions we have been speaking of. Imagine curve
lines to be described on any plane, and to revolve about any given
axes passing through the centre of force, and by that revolution to
describe curve superficies; and that the bodies move in such sort
that their centres may be always found in those superficies. If those
bodies reciprocate to and fro with an oblique ascent and descent,
their motions will be performed in planes passing through the axis,
and therefore in the curve lines, by whose revolution those curve
superficies were generated. In those cases, therefore, it will be
sufficient to consider the motion in those curve lines.
PROPOSITION XLVIII. THEOREM XVI.
If a wheel stands upon the outside of a globe at right angles
thereto, and revolving about its own axis goes forward in a great
circle, the length of the curvilinear path which any point, given in
the perimeter of the wheel, hath described since the time that it
touched the globe (which curvilinear path we may call the cycloid or
epicycloid), will be to double the versed sine of half the arc which
since that time has touched the globe in passing over it, as the sum of
the diameters of the globe and the wheel to the semi-diameter of the
globe.
PROPOSITION XLIX. THEOREM XVII.
If a wheel stand upon the inside of a concave globe at right angles
thereto, and revolving about its own axis go forward in one of the
great circles of the globe, the length of the curvilinear path which
any point, given in the perimeter of the wheel, hath described since it
touched the globe, will be to the double of the versed sine of half the
arc which in all that time has touched the globe in passing over it,
as the difference of the diameters of the globe and the wheel to the
semi-diameter of the globe.
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