The Royal Observatory, Greenwich: A Glance at Its History and WorkMaunder, E. Walter (Edward Walter)
History
The Royal Observatory, Greenwich: A Glance at Its History and Work
Maunder, E. Walter (Edward Walter)
Astronomy -- History; Royal Observatory, Greenwich
It was for this reason that Pond set up a pair of mural circles,
one on the east side of its supporting pier and the other on
the west.[3] His plan was not only to have each star observed
simultaneously in the two instruments, a plan by which, at the cost
of some additional labour, he would have got rid, to a large extent,
of the individual errors of the two separate instruments, inasmuch
as, on the whole, it might have been expected that the errors of
the two instruments would have been very nearly equal in amount,
but of opposite character. The differences, too, between the two
instruments would have afforded the means for tracing these small
errors to their respective causes, and so ascertaining the laws to
which they were subject.
[3] The second circle was intended for the Cape Observatory, but
Pond obtained leave to retain it. In 1851 it was transferred to the
Observatory of Queen's College, Belfast.
Pond went further still. He added to the mural circle a simple
instrument, the extreme value of which every astronomer recognizes
to-day--the mercury trough. Not only was the star to be observed by
both circles when the two telescopes were pointing directly to it,
it was also to be observed by reflection; the telescopes were to
be pointed down towards a basin of mercury, in which the image of
the star would be seen reflected. The mercury being a liquid, its
surface is perfectly horizontal; and, since the law of reflection
is that the angle of incidence is equal to the angle of reflection,
it follows that the telescope, when pointed down toward the mercury
trough, points just at as great an angle below the horizon as, when
it is set directly on the star, it points above it. If the circle,
therefore, be carefully read at both settings, half the difference
between the two readings will give the angular elevation of the
star above the horizon. A combination, therefore, of all four
observations, that is to say, one reflection and one direct with
each of the telescopes, would give an exceedingly exact value for
the star's altitude. The conception of this method gives a striking
idea of Pond's thoroughness and skill as a practical observer, and
it is a distinct blot upon Airy's justly high reputation in the same
line that he discontinued the system upon his accession to office.
Public-domain text, read in full here on John Shaqi.
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