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
It is indeed a matter of great difficulty to discover, and effectually
to distinguish, the true motions of particular bodies from the
apparent; because the parts of that immovable space, in which those
motions are performed, do by no means come under the observation of our
senses. Yet the thing is not altogether desperate; for we have some
arguments to guide us, partly from the apparent motions, which are the
differences of the true motions; partly from the forces, which are the
causes and effects of the true motions. For instance, if two globes,
kept at a given distance one from the other by means of a cord that
connects them, were revolved about their common centre of gravity, we
might, from the tension of the cord, discover the endeavour of the
globes to recede from the axis of their motion, and from thence we
might compute the quantity of their circular motions. And then if any
equal forces should be impressed at once on the alternate faces of the
globes to augment or diminish their circular motions, from the increase
or decrease of the tension of the cord, we might infer the increment
or decrement of their motions; and thence would be found on what faces
those forces ought to be impressed, that the motions of the globes
might be most augmented; that is, we might discover their hindermost
faces, or those which, in the circular motion, do follow. But the faces
which follow being known, and consequently the opposite ones that
precede, we should likewise know the determination of their motions.
And thus we might find both the quantity and the determination of this
circular motion, even in an immense vacuum, where there was nothing
external or sensible with which the globes could be compared. But now,
if in that space some remote bodies were placed that kept always a
given position one to another, as the fixed stars do in our regions, we
could not indeed determine from the relative translation of the globes
among those bodies, whether the motion did belong to the globes or to
the bodies. But if we observed the cord, and found that its tension was
that very tension which the motions of the globes required, we might
conclude the motion to be in the globes, and the bodies to be at rest;
and then, lastly, from the translation of the globes among the bodies,
we should find the determination of their motions. But how we are to
collect the true motions from their causes, effects, and apparent
differences; and, vice versa, how from the motions, either true
or apparent, we may come to the knowledge of their causes and effects,
shall be explained more at large in the following tract. For to this
end it was that I composed it.
[Pg 83]
AXIOMS, OR LAWS OF MOTION.
LAW I.
Every body perseveres in its state of rest, or of uniform motion in
a right line, unless it is compelled to change that state by forces
impressed thereon.
Public-domain text, read in full here on John Shaqi.
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