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저자: Albert Einstein

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The second class of facts to which we have alluded has reference
to the question whether or not the motion of the earth in space
can be made perceptible in terrestrial experiments. We have
already remarked in Section V that all attempts of this nature
led to a negative result. Before the theory of relativity was put
forward, it was difficult to become reconciled to this negative
result, for reasons now to be discussed. The inherited prejudices
about time and space did not allow any doubt to arise as to the
prime importance of the Galileian transformation for changing
over from one body of reference to another. Now assuming that the
Maxwell-Lorentz equations hold for a reference-body K, we then
find that they do not hold for a reference-body K′ moving
uniformly with respect to K, if we assume that the relations of
the Galileian transformation exist between the co-ordinates of K
and K′.

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