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Einstein, Albert, 1879-1955

"Relativity : the Special and General Theory"

Thus great accuracy
was necessary in making the adjustments required for the taking of the
photographs, and in their subsequent measurement.
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 :
Table 01: file table01.gif
(c) Displacement of Spectral Lines Towards the Red
In Section 23 it has been shown that in a system K1 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 = wr
where w represents the angular velocity of rotation of the disc K1
with respect to K. If v[0], represents the number of ticks of the
clock per unit time (" rate " of the clock) relative to K when the
clock is at rest, then the " rate " of the clock (v) when it is moving
relative to K with a velocity V, but at rest with respect to the disc,
will, in accordance with Section 12, be given by
eq.


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