Absolute and Relative Space, Time, and Motion
by Isaac Newton
from
Scholium to the definitions in Philosophiae Naturalis Principia
Mathematica, Bk. 1 (1689). Hitherto I have laid down the definitions of such words as are less known
and explained the sense in which I would have them to be understood in the
following discourse. I do not define time, space, place, and motion, as being
well known to all. Only I must observe that the common people conceive those
quantities under no other notions but from the relation they bear to sensible
objects. And thence arise certain prejudices, for the removing of which it
will be convenient to distinguish them into absolute and relative, true and
apparent, mathematical and common. 1. Absolute, true, and mathematical time, of itself and from its own
nature, flows equably without relation to anything external, and by another
name is called "duration"; relative, apparent, and common time is
some sensible and external (whether accurate or unequable) measure of
duration by the means of motion, which is commonly used instead of true time,
such as an hour, a day, a month, a year.
3. Place is a part of space which a body takes up and is, according to
the space, either absolute or relative. I say, a part of space; not the
situation nor the external surface of the body. For the places of equal
solids are always equal; but their surfaces, by reason of their dissimilar
figures, are often unequal. Positions properly have no quantity; nor are they
so much the places themselves as the properties of places. The motion of the
whole is the same with the sum of the motions of the parts; that is, the
translation of the whole, out of its place, is the same thing with the sum of
the translations of the parts out of their places; and therefore the place of
the whole is the same as the sum of the places of the parts, and for that
reason it is internal and in the whole body. 4. 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 the 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 10,010
parts, while the ship itself, with a fresh gale and full sails, is carried
toward the west with a velocity expressed by 10 of those parts, but a sailor
walks in the ship toward the east with 1 part of the said velocity; then the
sailor will be moved truly in immovable space toward the east, with a
velocity of 10,001 parts, and relatively on the earth toward 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 apparent 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 that they may measure the
celestial motions by a more accurate time. It may be that there is no such
thing as an equable motion whereby time may be accurately measured. All
motions may be accelerated and retarded, but the flowing of absolute time is
not liable to any 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 this duration ought to be distinguished from what are only
sensible measures thereof and from which we deduce it, by means of the
astronomical equation. The necessity of this equation, for determining the
times of a phenomenon, is evinced as well from the experiments of the
pendulum clock as by eclipses of the satellites of Jupiter. As the order of the parts of time is immutable, so also is the order
of the parts of space. Suppose those parts to be moved out of their places,
and they will be moved (if the expression may be allowed) out of themselves.
For times and spaces are, as it were, the places as well of themselves as of
all other things. All things are placed in time as to order of succession and
in space as to order of situation. It is from their essence or nature that
they are places, and that the primary places of things should be movable is
absurd. These are therefore the absolute places, and translations out of
those places are the only absolute motions. But because the parts of space cannot be seen or distinguished from
one another by our senses, therefore in their stead we use sensible measures
of them. For from the positions and distances of things from any body
considered as immovable we define all places; and then, with respect to such
places, we estimate all motions, considering bodies as transferred from some
of those places into others. And so, instead of absolute places and motions,
we use relative ones, and that without any inconvenience in common affairs;
but in philosophical disquisitions, we ought to abstract from our senses and
consider things themselves, distinct from what are only sensible measures of
them. For it may be that there is no body really at rest to which the places
and motions of others may be referred.
It is a property of motion that the parts which retain given positions
to their wholes do partake of the motions of those wholes. For all the parts
of revolving bodies endeavor to recede from the axis of motion, and the
impetus of bodies moving forward arises from the joint impetus of all the
parts. Therefore, if surrounding bodies are moved, those that are relatively
at rest within them will partake of their motion. Upon which account the true
and absolute motion of a body cannot be determined by the translation of it
from those which only seem to rest; for the external bodies ought not only to
appear at rest, but to be really at rest. For otherwise all included bodies,
besides their translation from near the surrounding ones, partake likewise of
their true motions; and though that translation were not made, they would not
be really at rest, but only seem to be so. For the surrounding bodies stand
in the like relation to the surrounded as the exterior part of a whole does
to the interior, or as the shell does to the kernel; but if the shell moves,
the kernel will also move, as being part of the whole, without any removal
from near the shell. A property near akin to the preceding is this, that if a place is moved,
whatever is placed therein moves along with it; and therefore a body which is
moved from a place in motion partakes also of the motion of its place. Upon
which account all motions, from places in motion, are no other than parts of
entire and absolute motions; and every entire motion is composed of the
motion of the body out of its first place and the motion of this place out of
its place; and so on, until we come to some immovable place, as in the
before-mentioned example of the sailor. Wherefore entire and absolute motions
cannot be otherwise determined than by immovable places; and for that reason
I did before refer those absolute motions to immovable places, but relative
ones to movable places. Now no other places are immovable but those that, from
infinity to infinity, do all retain the same given position one to another,
and upon this account must ever remain unmoved and do thereby constitute
immovable space. The causes by which true and relative motions are distinguished, one
from the other, are the forces impressed upon bodies to generate motion. True
motion is neither generated nor altered but by some force impressed upon the
body moved, but relative motion may be generated or altered without any force
impressed upon the body. For it is sufficient only to impress some force on
other bodies with which the former is compared that, by their giving way,
that relation may be changed in which the relative rest or motion of this
other body did consist. Again, true motion suffers always some change from
any force impressed upon the moving body, but relative motion does not
necessarily undergo any change by such forces. For if the same forces are
likewise impressed on those other bodies with which the comparison is made,
that the relative position may be preserved, then that condition will be
preserved in which the relative motion consists. And therefore any relative
motion may be changed when the true motion remains unaltered, and the
relative may be preserved when the true suffers some change. Thus, true
motion by no means consists in such relations. The effects which distinguish absolute from relative motion are the
forces of receding from the axis of circular motion. For there are no such
forces in a circular motion purely relative, but in a true and absolute
circular motion they are greater or less, according to the quantity of the
motion. If a vessel, hung by a long cord, is so often turned about that the
cord is strongly twisted, then filled with water and held at rest together
with the water, thereupon by the sudden action of another force it is whirled
about the contrary way, and while the cord is untwisting itself the vessel
continues for some time in this motion, the surface of the water will at
first be plain, as before the vessel began to move; but after that the
vessel, by gradually communicating its motion to the water, will make it
begin sensibly to revolve and recede by little and little from the middle,
and ascend to the sides of the vessel, forming itself into a concave figure
(as I have experienced); and the swifter the motion becomes, the higher will
the water rise, till at last, performing its revolutions in the same times
with the vessel, it becomes relatively at rest in it. This ascent of the
water shows its endeavor to recede from the axis of its motion; and the true
and absolute circular motion of the water, which is here directly contrary to
the relative, becomes known and may be measured by this endeavor. At first,
when the relative motion of the water in the vessel was greatest, it produced
no endeavor to recede from the axis; the water showed no tendency to the
circumference, nor any ascent toward the sides of the vessel, but remained of
a plain surface, and therefore its true circular motion bad not yet begun.
But afterward, when the relative motion of the water had decreased, the
ascent thereof toward the sides of the vessel proved its endeavor to recede
from the axis; and this endeavor showed the real circular motion of the water
continually increasing, till it bad acquired its greatest quantity, when the
water rested relatively in the vessel. And therefore this endeavor does not
depend upon any translation of the water in respect of the ambient bodies;
nor can true circular motion be defined by such translation. There is only one
real circular motion of any one revolving body, corresponding to only one
power of endeavoring to recede from its axis of motion, as its proper and
adequate effect; but relative motions, in one and the same body, are
innumerable, according to the various relations it bears to external bodies,
and, like other relations, are altogether destitute of any real effect, any
otherwise than they may perhaps partake of that one only true motion. And
therefore in their system who suppose that our heavens, revolving below the
sphere of the fixed stars, carry the planets along with them, the several
parts of those heavens and the planets, which are indeed relatively at rest
in their heavens, do yet really move. For they change their position one to
another (which never happens to bodies truly at rest) and, being carried
together with their heavens, partake of their motions and, as parts of
revolving wholes, endeavor to recede from the axis of their motions. Wherefore relative quantities are not the quantities themselves whose
names they bear, but those sensible measures of them (either accurate or
inaccurate) which are commonly used instead of the measured quantities
themselves. And if the meaning of words is to be determined by their use,
then by the names "time," "space," "place," and
"motion" their [sensible] measures are properly to be understood;
and the expression will be unusual, and purely mathematical, if the measured
quantities themselves are meant. On this account, those violate the accuracy
of language, which ought to be kept precise, who interpret these words for
the measured quantities. Nor do those less defile the purity of mathematical
and philosophical truths who confound real quantities with their relations
and sensible measures. 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
center of gravity, we might, from the tension of the cord, discover the
endeavor 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 hindmost 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.
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