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
This was the celebrated discovery of the Aberration of Light,
a triumph of exact observation and of clear insight. As to the
exactness of Bradley's observations, it is sufficient to say that
his determination of the value of the 'Constant of Aberration' gave
it as 20·39´´; the value adopted to-day is 20·47´´.
On the death of Halley, in 1742, Bradley was appointed to succeed
him. He found the Observatory in as utterly disheartening a
condition as his predecessors had done. As already mentioned, Halley
had not the same qualifications as an observer that Flamsteed
had. He was, further, an old man when appointed to the post, he
had no assistant provided for him, and the last five years of his
life his health and strength had entirely given way. Under these
circumstances, it was no wonder that Bradley found the instruments
of the Observatory in a deplorable state. Nevertheless, he set to
work most energetically, and in the year of his appointment he
made 1500 observations in the last five months of the year. He was
particularly earnest in examining the condition and the errors of
his instruments; and as their defects became known to him, he was
more and more anxious for a better equipment. He moved the Royal
Society, therefore, to apply on his behalf for the instruments he
required; and a petition from that body, in 1748, obtained what
in those days must be considered the generous grant of £1000,
the proceeds of the sale of old Admiralty stores. The principal
instruments purchased therewith were a mural quadrant and a transit
instrument, both eight feet in focal length, still preserved on the
walls of the transit-room. It is interesting also to note that,
following in the steps of Halley, and forecasting, as it were, the
magnetic observatory which Airy would found, he devoted £20 of the
grant to purchasing magnetic instruments.
Meantime he had continued his observations on aberration, and had
discovered that the aberration theory was not sufficient entirely
to account for the apparent changes in places of stars which he had
discovered. A second cause was at work, a movement of the earth's
axis, a 'wobble' in its inclination, technically known as Nutation,
which is due to the action of the moon, and goes through its course
in a period of nineteen years.
Public-domain text, read in full here on John Shaqi.
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