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Since
the ancients (as we are told by Pappas), made great account of the science
of mechanics in the investigation of natural things; and the moderns,
lying aside substantial forms and occult qualities, have endeavoured to
subject the phænomena of nature to the laws of mathematics, I have in
this treatise cultivated mathematics so far as it regards philosophy. The
ancients considered mechanics in a twofold respect; as rational, which
proceeds accurately by demonstration; and practical. To practical
mechanics all the manual arts belong, from which mechanics took its name.
But as artificers do not work with perfect accuracy, it comes to pass that
mechanics is so distinguished from geometry, that what is perfectly
accurate is called geometrical; what is less so, is called mechanical. But
the errors are not in the art, but in the artificers. He that works with
less accuracy is an imperfect mechanic; and if any could work with perfect
accuracy, he would be the most perfect mechanic of all; for the
description of right lines and circles, upon which geometry is founded,
belongs to mechanics. Geometry does not teach us to draw these lines, but
requires them to be drawn; for it requires that the learner should first
be taught to describe these accurately, before he enters upon geometry;
then it shows how by these operations problems may be solved. To describe
right lines and circles are problems, but not geometrical problems. The
solution of these problems is required from mechanics; and by geometry the
use of them, when so solved, is shown; and it is the glory of geometry
that from those few principles, brought from without, it is able to
produce so many things. Therefore geometry is founded in mechanical
practice, and is nothing but that part of universal mechanics which
accurately proposes and demonstrates the art of measuring. But since the
manual arts are chiefly conversant in the moving of bodies, it comes to
pass that geometry is commonly referred to their magnitudes, and mechanics
to their motion. In this sense rational mechanics will be the science of
motions resulting from any forces whatsoever, and of the forces required
to produce any motions, accurately proposed and demonstrated. This part of
mechanics was cultivated by the ancients in the five powers which relate
to manual arts, who considered gravity (it not being a manual power, no
otherwise than as it moved weights by those powers. Our design not
respecting arts, but philosophy, and our subject not manual but natural
powers, we consider chiefly those things which relate to gravity, levity,
elastic force, the resistance of fluids, and the like forces, whether
attractive or impulsive; and therefore we offer this work as the
mathematical principles of philosophy; for all the difficulty of
philosophy seems to consist in this – from the phænomena of motions to
investigate the forces of nature, and then from these forces to
demonstrate the other phænomena; and to this end the general propositions
in the first and second book are directed. In the third book we give an
example of this in the explication of the System of the World; for by the
propositions mathematically demonstrated in the former books, we in the
third derive from the celestial phænomena the forces of gravity with
which bodies tend to the sun and the several planets. Then from these
forces, by other propositions which are also mathematical, we deduce the
motions of the planets, the comets, the moon, and the sea. I wish we could
derive the rest of the phænomena of nature by the same kind of reasoning
from mechanical principles; for I am induced by many reasons to suspect
that they may all depend upon certain forces by which the particles of
bodies, by some causes hitherto unknown, are either mutually impelled
towards each other, and cohere in regular figures, or are repelled and
recede from each other; which forces being unknown, philosophers have
hitherto attempted the search of nature in vain; but I hope the principles
here laid down will afford some light either to this or some truer method
of philosophy.
In the publication of this work the most acute and universally learned
Mr. Edmund Halley not only assisted me with his pains in correcting the
press and taking care of the schemes, but it was to his solicitations that
its becoming public is owing; for when he had obtained of me my
demonstrations of the figure of the celestia1 orbits, he continually
pressed me to communicate the same to the Roya1 Society, who afterwards,
by their kind encouragement and entreaties, engaged me to think of
publishing them. But after I had begun to consider the inequalities of the
lunar motions, and had entered upon some other things relating to the laws
and measures of gravity, and other forces; and the figures that would be
described by bodies attracted according to given laws; and the motion of
several bodies moving among themselves; the motion of bodies in resisting
mediums; the forces, densities, and motions, of mediums; the orbits of the
comets, and such like; deferred that publication till I had made a search
into those matters, and could put forth the whole together. What relates
to the lunar motions (being imperfect), I have put all together in the
corollaries of Prop. 66, to avoid being obliged to propose and distinctly
demonstrate the several things there contained in a method more prolix
than the subject deserved, and interrupt the series of the several
propositions. Some things, found out after the rest, I chose to insert in
places less suitable, rather than change the number of the propositions
and the citations. I heartily beg that what I have here done may be read
with candour; and that the defects in a subject so difficult be not so
much reprehended as kindly supplied, and investigated by new endeavours of
my readers.
[Source: Isaac Newton, Principia
(1687), Translated by Andrew Motte (1729). Newton's Principia
is currently in the process of being digitized. Click here
to see what's been completed.]
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