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
The preceding Proposition may be likewise demonstrated after this
manner. In any circle suppose a polygon to be inscribed of any number
of sides. And if a body, moved with a given velocity along the sides
of the polygon, is reflected from the circle at the several angular
points, the force, with which at every reflection it strikes the
circle, will be as its velocity: and therefore the sum of the forces,
in a given time, will be as that velocity and the number of reflections
conjunctly; that is (if the species of the polygon be given), as the
length described in that given time, and increased or diminished in the
ratio of the same length to the radius of the circle; that is, as the
square of that length applied to the radius; and therefore the polygon,
by having its sides diminished in infinitum, coincides with the
circle, as the square of the arc described in a given time applied to
the radius. This is the centrifugal force, with which the body impels
the circle; and to which the contrary force, wherewith the circle
continually repels the body towards the centre, is equal.
PROPOSITION V. PROBLEM I.
There being given, in any places, the velocity with which a body
describes a given figure, by means of forces directed to some common
centre: to find that centre.
Let the three right lines PT, TQV, VR touch the figure described in as
many points, P, Q, R, and meet in T and V. On the tangents erect the
perpendiculars PA, QB, RC, reciprocally proportional to the velocities
of the body in the points P, Q, R, from which the perpendiculars were
raised; that is, so that PA may be to QB as the velocity in Q to the
velocity in P, and QB to RC as the velocity in R to the velocity in Q.
Through the ends A, B, C, of the perpendiculars draw AD, DBE, EC, at
right angles, meeting in D and E: and the right lines TD, VE produced,
will meet in S, the centre required.
For the perpendiculars let fall from the centre S on the tangents PT,
QT, are reciprocally as the velocities of the bodies in the points P
and Q[Pg 110] (by Cor. 1, Prop. I.), and therefore, by construction, as the
perpendiculars AP, BQ directly; that is, as the perpendiculars let fall
from the point D on the tangents. Whence it is easy to infer that the
points S, D, T, are in one right line. And by the like argument the
points S, E, V are also in one right line; and therefore the centre S
is in the point where the right lines TD, VE meet. Q.E.D.
PROPOSITION VI. THEOREM V.
In a space void of resistance, if a body revolves in any orbit about
an immovable centre, and in the least time describes any arc just
then nascent; and the versed sine of that arc is supposed to be drawn
bisecting the chord, and produced passing through the centre of force:
the centripetal force in the middle of the arc will be as the versed
sine directly and the square of the time inversely.
Public-domain text, read in full here on John Shaqi.
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