A Century's Progress in AstronomyMacpherson, Hector
History
A Century's Progress in Astronomy
Macpherson, Hector
Astronomy -- History
The study of our own planet can hardly be said to belong to the realm of
astronomy. Nevertheless, it is through astronomical observation that the
motion of the North Pole has been discovered. For many years it has been
a problem whether there is a variation of latitude resulting from the
motion of the pole. Euler had declared, from theoretical investigation,
that, were there such a motion, the period must be 10 months. The
question was revived in 1885 by the observations of _Seth Carlo
Chandler_ (born 1846) at Cambridge, Mass., with his newly-invented
instrument, the “almucantar,” which indicated an appreciable variation
of latitude. This was confirmed by _Friedrich Küstner_ (born 1856), now
director of the Observatory at Bonn. The idea now occurred to Chandler
to search through the older records to discover if there was any trace
of the variation of latitude, with the result that he brought out a
period of 14 months instead of 10. This aroused much interest, and many
prominent astronomers denied Chandler’s results, which were announced in
1891. As a well-known astronomer has expressed it, “Euler’s work had
shown what period the motion must have, and any appearance of another
period must be due to some error in the observations. Chandler replied
to the effect that he did not care for Euler’s mathematics: the
observations plainly showed 14 months, and if Euler said 10, _he_ must
have made the mistake. I do not exaggerate the situation in the least;
it was a deadlock: Chandler and observation against the whole weight of
observation and theory.” It was now shown by Newcomb that Euler had
assumed the Earth to be an absolutely rigid body, while modern
investigations show that it is not so. Chandler’s discovery is now
accepted, and proves that the North Pole is not fixed in position, but
has a small periodic motion, though never twelve yards from its mean
position. That the small resulting variation in the position of the
stars has been noticed at all is a striking illustration of the accuracy
of astronomical observation.
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