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 the differences of the motions tending towards the same parts, and
the sums of those that tend towards contrary parts, are, at first (by
supposition), in both cases the same; and it is from those sums and
differences that the collisions and impulses do arise with which the
bodies mutually impinge one upon another. Wherefore (by Law II), the
effects of those collisions will be equal in both cases; and therefore
the mutual motions of the bodies among themselves in the one case will
remain equal to the mutual motions of the bodies among themselves in
the other. A clear proof of which we have from the experiment of a
ship; where all motions happen after the same manner, whether the ship
is at rest, or is carried uniformly forwards in a right line.
COROLLARY VI.
If bodies, any how moved among themselves, are urged in the
direction of parallel lines by equal accelerative forces, they will all
continue to move among themselves, after the same manner as if they had
been urged by no such forces.
For these forces acting equally (with respect to the quantities of the
bodies to be moved), and in the direction of parallel lines, will (by
Law II) move all the bodies equally (as to velocity), and therefore
will never produce any change in the positions or motions of the bodies
among themselves.
SCHOLIUM.
Hitherto I have laid down such principles as have been received by
mathematicians, and are confirmed by abundance of experiments. By
the first two Laws and the first two Corollaries, Galileo discovered
that the descent of bodies observed the duplicate ratio of the time,
and that the motion of projectiles was in the curve of a parabola;
experience agreeing with both, unless so far as these motions are a
little retarded by the resistance of the air. When a body is falling,
the uniform force of its gravity acting equally, impresses, in equal
particles of time, equal forces upon that body, and therefore generates
equal velocities; and in the whole time impresses a whole force, and
generates a whole velocity proportional to the time. And the spaces
described in proportional times are as the velocities and the times
conjunctly; that is, in a duplicate ratio of the times. And when a body
is thrown upwards, its uniform gravity impresses forces and takes off
velocities proportional to the times; and the times of ascending to
the greatest heights are as the velocities to be taken off, and those
heights are as the velocities and the times conjunctly, or in the
duplicate ratio of the velocities. And if a body be projected in any
direction, the motion arising from its projection is compounded with
the[Pg 90] motion arising from its gravity.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account