The nature of the physical worldEddington, Arthur Stanley, Sir
Philosophy
The nature of the physical world
Eddington, Arthur Stanley, Sir
Physics -- Philosophy; Science -- Philosophy
Perhaps you will object that astronomers do not in practice lay
measuring rods end to end through interplanetary space in order to
find out where the planets are. Actually the position is deduced from
the light rays. But the light as it proceeds has to find out what
course to take in order to go “straight”, in much the same way as the
metre rod has to find out how far to extend. The metric or curvature
is a sign-post for the light as it is a gauge for the rod. The light
[Pg 151]
track is in fact controlled by the curvature in such a way that it is
incapable of exposing the sham law of curvature. And so wherever the
sun, moon and earth may have got to, the light will not give them away.
If the law of curvature predicts an eclipse the light will take such a
track that there is an eclipse. The law of gravitation is not a stern
ruler controlling the heavenly bodies; it is a kind-hearted accomplice
who covers up their delinquencies.
I do not recommend you to try to verify from Fig. 6 that the number
of rods in (full line) and (dotted line) is the
same. There are two dimensions of space-time omitted in the picture
besides the extra dimensions in which space-time must be supposed to
be bent; moreover it is the spherical, not the cylindrical, curvature
which is the gauge for the length. It might be an instructive, though
very laborious, task to make this direct verification, but we know
beforehand that the measured distance of the earth from the sun must
be the same for either track. The law of gravitation, expressed
mathematically by , means nothing
more nor less than that the unit of length everywhere is a constant
fraction of the directed radius of the world at that point. And as
the astronomer who predicts the future position of the earth does not
assume anything more about what the earth will choose to do than is
expressed in the law so we shall
find the same position of the earth, if we assume nothing more than
that the practical unit of length involved in measurements of the
position is a constant fraction of the directed radius. We do not
need to decide whether the track is to be represented by or
, and it would convey no information as to any observable
phenomena if we knew the representation.
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Public-domain text, read in full here on John Shaqi.
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