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
COR. 1. In non-resisting spaces or mediums, if the areas are not
proportional to the times, the forces are not directed to the point in
which the radii meet; but deviate therefrom in consequentia, or
towards the parts to which the motion is directed, if the description
of the areas is accelerated; but in antecedentia, if retarded.
COR. 2. And even in resisting mediums, if the description of the areas
is accelerated, the directions of the forces deviate from the point in
which the radii meet, towards the parts to which the motion tends.
SCHOLIUM.
A body may be urged by a centripetal force compounded of several
forces; in which case the meaning of the Proposition is, that the force
which results out of all tends to the point S. But if any force acts
perpetually in the direction of lines perpendicular to the described
surface, this force will make the body to deviate from the plane of
its motion: but will neither augment nor diminish the quantity of the
described surface, and is therefore to be neglected in the composition
of forces.
PROPOSITION III. THEOREM III.
Every body, that by a radius drawn to the centre of another body,
howsoever moved, describes areas about that centre proportional to the
times, is urged by a force compounded out of the centripetal force
tending to that other body, and of all the accelerative force by which
that other body is impelled.
Let L represent the one, and T the other body; and (by Cor. 6 of the
Laws) if both bodies are urged in the direction of parallel lines, by
a new force equal and contrary to that by which the second body T is
urged, the first body L will go on to describe about the other body
T the same areas as before: but the force by which that other body T
was urged will be now destroyed by an equal and contrary force; and
therefore (by Law I.) that other body T, now left to itself, will
either rest, or move uniformly forward in a right line: and the first
body L impelled by the difference of the forces, that is, by the
force remaining, will go on to describe about the other body T areas
proportional to the times. And therefore (by Theor. II.) the difference
of the forces is directed to the other body T as its centre. Q.E.D.
[Pg 107]
COR. 1. Hence if the one body L, by a radius drawn to the other body T,
describes areas proportional to the times; and from the whole force,
by which the first body L is urged (whether that force is simple, or,
according to Cor. 2 of the Laws, compounded out of several forces), we
subduct (by the same Cor.) that whole accelerative force by which the
other body is urged; the whole remaining force by which the first body
is urged will tend to the other body T, as its centre.
COR. 2. And, if these areas are proportional to the times nearly, the
remaining force will tend to the other body T nearly.
COR. 3. And vice versa, if the remaining force tends nearly to
the other body T, those areas will be nearly proportional to the times.
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