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
The observation is very unlike those of which we have hitherto
spoken. The object is not to ascertain the actual position in the
sky of the two stars, but their relative position to each other.
A spider's thread of the finest strands is moved from one star to
the other by turning an exquisitely fine screw; this enables us
to measure their distance apart. Another spider thread at right
angles to the first is laid through the centres of both stars, and
a divided circle enables us to read the angle which this line makes
to the true east and west direction. Such observations repeated
year after year on many stars have enabled the orbits of not a few
to be laid down with remarkable precision; and we find that their
movements are completely consistent with the law of gravitation.
Further, just as Neptune was pre-recognized and discovered
from noting the irregularities in the motion of Uranus, so the
discordances in the place of Sirius led to the belief that it was
attracted by a then unseen companion, whose position with respect to
the brighter star was predicted and afterwards seen.
[Illustration: THE SOUTH-EAST DOME WITH THE SHUTTER OPEN.]
Gravitation thus appears, indeed, to be the Bond of the Universe,
yet it leaves us with several weighty problems. The observation of
the positions of stars shows that though we call them fixed they
really have motions of their own. Of these motions, a great part
consists of a drift away from one portion of the heavens towards a
point diametrically opposite to it, a drift such as must be due, not
to a true motion of the individual stars, but to a motion through
space of our sun and its attendant system. The elder Herschel was
the first to discover this mysterious solar motion. Sir George Airy
and Mr. Edwin Dunkin, for forty-six years a member of the Greenwich
staff, and from 1881-1884 the Chief Assistant, contributed important
determinations of its direction.
What is the cause of this motion, what is the law of this motion,
is at present beyond our power to find out. Many years ago a
German astronomer made the random suggestion that possibly we were
revolving in an orbit round the Pleiades as a centre. The suggestion
was entirely baseless, but unfortunately has found its way into many
popular works, and still sometimes is brought forward as if it were
one of the established truths of astronomy. We can at present only
say that this solar motion is a mystery.
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