Einstein's Theories of Relativity and Gravitation: A selection of material from the essays submitted in the competition for the Eugene Higgins prize of $5,000Bird, J. Malcolm (James Malcolm)
Philosophy
Einstein's Theories of Relativity and Gravitation: A selection of material from the essays submitted in the competition for the Eugene Higgins prize of $5,000
Bird, J. Malcolm (James Malcolm)
Relativity (Physics)
When we speak of a body as being "in motion," we mean that this
body is changing its position "in space." Now it is clear that the
position of an object can only be determined with reference to other
objects: in order to describe the place of a material thing we must,
for example, state its distances from other things. If there were no
such bodies of reference, the words "position in space" would have
no definite meaning for us.]24 [The number of such external bodies of
reference which it is necessary to cite in order to define completely
the position of a given body in space depends upon the character
of the space dealt with. We have seen that when we visualize the
space of our experience as a surface of any character, two citations
are sufficient; and that when we conceive of it as surrounding us
in three dimensions we require three. It will be realized that the
mathematician is merely meeting this requirement when he sets up his
system of coordinate axes to serve as a reference frame.]*
[What is true of "place" must be true also of "motion," since the
latter is nothing but change of place. In fact, it would be impossible
to ascribe a state of motion or of rest to a body poised all alone
in empty space. Whether a body is to be regarded as resting or as
moving, and if the latter at what speed, depends entirely upon the
objects to which we refer its positions in space.]24 [As Einstein
sits at his desk he appears to us to be at rest; but we know that
he is moving with the rotation of the earth on its axis, with the
earth in its orbit about the sun, and with the solar system in its
path through space--a complex motion of which the parts or the whole
can be detected only by reference to appropriately chosen ones of the
heavenly bodies. No mechanical test has ever been devised which will
detect this motion,]182 [if we reserve for discussion in its proper
place the Foucault pendulum experiment which will reveal the axial
rotation of our globe.]* [No savage, if he were to "stand still,"
could be convinced that he was moving with a very high velocity
or in fact that he was moving at all.]30 [You drop a coin straight
down a ship's side: from the land its path appears parabolic; to a
polar onlooker it whirls circle-wise; to dwellers on Mars it darts
spirally about the sun; to a stellar observer it gyrates through
the sky]263 [in a path of many complications. To you it drops in a
straight line from the deck to the sea.]* [Yet its various tracks
in ship-space, sea-space, earth-space, sun-space, star-space, are
all equally real,]263 [and the one which will be singled out for
attention depends entirely upon the observer, and the objects to
which he refers the motion.]* [The earth moves in the solar system,
which is itself approaching a distant star-cluster. But we cannot say
whether we are moving toward the cluster, or the cluster toward us,]18
[or both, or whether we are conducting a successful stern chase of it,
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