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
To determine the motions of two bodies which attract each other with
forces reciprocally proportional to the squares of the distance between
them, and are let fall from given places.
The bodies, by the last Theorem, will be moved in the same manner
as if they were attracted by a third placed in the common centre of
their gravity; and by the hypothesis that centre will be quiescent at
the beginning of their motion, and therefore (by Cor. 4, of the Laws
of Motion) will be always quiescent. The motions of the bodies are
therefore to be determined (by Prob. XXV) in the same manner as if they
were impelled by forces tending to that centre; and then we shall have
the motions of the bodies attracting each other mutually. Q.E.I.
PROPOSITION LXIII. PROBLEM XXXIX.
To determine the motions of two bodies attracting each other with
forces reciprocally proportional to the squares of their distance,
and going off from given places in given directions with given
velocities.
The motions of the bodies at the beginning being given, there is given[Pg 199]
also the uniform motion of the common centre of gravity, and the motion
of the space which moves along with this centre uniformly in a right
line, and also the very first, or beginning motions of the bodies in
respect of this space. Then (by Cor. 5, of the Laws, and the last
Theorem) the subsequent motions will be performed in the same manner in
that space, as if that space together with the common centre of gravity
were at rest, and as if the bodies did not attract each other, but were
attracted by a third body placed in that centre. The motion therefore
in this movable space of each body going off from a given place, in a
given direction, with a given velocity, and acted upon by a centripetal
force tending to that centre, is to be determined by Prob. IX and XXVI,
and at the same time will be obtained the motion of the other round the
same centre. With this motion compound the uniform progressive motion
of the entire system of the space and the bodies revolving in it, and
there will be obtained the absolute motion of the bodies in immovable
space. Q.E.I.
PROPOSITION LXIV. PROBLEM XL.
Supposing forces with which bodies mutually attract each other to
increase in a simple ratio of their distances from the centres; it is
required to find the motions of several bodies among themselves.
Suppose the first two bodies T and L to have their common centre of
gravity in D. These, by Cor. 1, Theor. XXI, will describe ellipses
having their centres in D, the magnitudes of which ellipses are known
by Prob. V.
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