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المؤلف: Albert Einstein

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The results of the measurements confirmed the theory in a
thoroughly satisfactory manner. The rectangular components of the
observed and of the calculated deviations of the stars (in
seconds of arc) are set forth in the following table of results:
image054
(c) Displacement of Spectral Lines Towards the Red
In Section XXIII it has been shown that in a system K which is
in rotation with regard to a Galileian system K, clocks of
identical construction, and which are considered at rest with
respect to the rotating reference-body, go at rates which are
dependent on the positions of the clocks. We shall now examine
this dependence quantitatively. A clock, which is situated at a
distance r from the centre of the disc, has a velocity relative
to K which is given by
v = ωr,

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