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
IV. Absolute motion is the translation of a body from one absolute
place into another; and relative motion, the translation from one
relative place into another. Thus in a ship under sail, the relative
place of a body is that part of the ship which the body possesses;
or that part of its cavity which the body fills, and which therefore
moves together with the ship: and relative rest is the continuance of
the body in the same part of the ship, or of its cavity. But real,
absolute rest, is the continuance of the body in the same part of that
immovable space, in which the ship itself, its cavity, and all that
it contains, is moved. Wherefore, if the earth is really at rest, the
body, which relatively rests in the ship, will really and absolutely
move with the same velocity which the ship has on the earth. But if the
earth also moves, the true and absolute motion of the body will arise,
partly from the true motion of the earth, in immovable space; partly
from the relative motion of the ship on the earth; and if the body
moves also relatively in the ship; its true motion will arise, partly
from the true motion of the earth, in immovable space, and partly from
the relative motions as well of the ship on the earth, as of the body
in the ship; and from these relative motions will arise the relative
motion of the body on the earth. As if that part of the earth, where
the ship is, was truly moved toward the east, with a velocity of 10010
parts; while the ship itself, with a fresh gale, and full sails, is
carried towards the west, with a velocity expressed by 10 of those
parts; but a sailor walks in the ship towards the east, with 1 part of
the said velocity; then the sailor will be moved truly in immovable
space towards the east, with a velocity of 10001 parts, and relatively
on the earth towards the west, with a velocity of 9 of those parts.
Absolute time, in astronomy, is distinguished from relative, by the
equation or correction of the vulgar time. For the natural days are
truly unequal, though they are commonly considered as equal, and used
for a measure of time; astronomers correct this inequality for their
more accurate deducing of the celestial motions. It may be, that there
is no such thing as an equable motion, whereby time may be accurately
measured. All motions[Pg 79] may be accelerated and retarded, but the true,
or equable, progress of absolute time is liable to no change. The
duration or perseverance of the existence of things remains the same,
whether the motions are swift or slow, or none at all: and therefore
it ought to be distinguished from what are only sensible measures
thereof; and out of which we collect it, by means of the astronomical
equation. The necessity of which equation, for determining the times of
a phænomenon, is evinced as well from the experiments of the pendulum
clock, as by eclipses of the satellites of Jupiter.
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