The Einstein Theory of Relativity: A Concise StatementLorentz, H. A. (Hendrik Antoon)
Science
The Einstein Theory of Relativity: A Concise Statement
Lorentz, H. A. (Hendrik Antoon)
Einstein, Albert, 1879-1955; Relativity (Physics)
This result is of importance, because thereby the theory is excluded,
or at least made extremely improbable, that the phenomenon of
refraction is to be ascribed to, a ring of vapor surrounding the
sun for a great distance. Indeed, such a refraction should cause a
deviation in the observed direction, and, in order to produce the
displacement of one of the stars under observation itself a slight
proximity of the vapor ring should be sufficient, but we have every
reason to expect that if it were merely a question of a mass of
gas around the sun the diminishing effect accompanying a removal
from the sun should manifest itself much faster than is really the
case. We cannot speak with perfect certainty here, as all the factors
that might be of influence upon the distribution of density in a sun
atmosphere are not well enough known, but we can surely demonstrate
that in case one of the gasses with which we are acquainted were held
in equilibrium solely by the influence of attraction of the sun the
phenomenon should become much less as soon as we got somewhat further
from the edge of the sun. If the displacement of the first star, which
amounts to 1.02-seconds were to be ascribed to such a mass of gas, then
the displacement of the second must already be entirely inappreciable.
So far as the absolute extent of the displacements is concerned, it
was found somewhat too great, as has been shown by the figures given
above; it also appears from the final result to be 1.98 for the edge
of the sun--i.e., 13 per cent, greater than the theoretical value
of 1.75. It indeed seems that the discrepancies may be ascribed to
faults in observations, which supposition is supported by the fact
that the observations at Prince's Island, which, it is true, did not
turn out quite as well as those mentioned above, gave the result,
of 1.64, somewhat lower than Einstein's figure.
(The observations made with a second instrument at Sobral gave a
result of 0.93, but the observers are of the opinion that because of
the shifting of the mirror which reflected the rays no value is to
be attached to it.)
DIFFICULTY EXAGGERATED
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