Astronomy with an Opera-glass: A Popular Introduction to the Study of the Starry Heavens with the Simplest of Optical InstrumentsServiss, Garrett Putman
Science
Astronomy with an Opera-glass: A Popular Introduction to the Study of the Starry Heavens with the Simplest of Optical Instruments
Serviss, Garrett Putman
Astronomy
Point a good glass upon the star marked Nu ([nu]), and you will see,
somewhat less than a degree and a half to the west of it, what appears
to be a faint star of between the seventh and eighth magnitudes. You
will have to look sharp to see it. It is with your mind's eye that you
must gaze, in order to perceive the wonder here hidden in the depths of
space. That faint speck is a nebula, unrivaled for interest by many of
the larger and more conspicuous objects of that kind. Lord Rosse's great
telescope has shown that in form it resembles the planet Saturn; in
other words, that it consists apparently of a ball surrounded by a ring.
But the spectroscope proves that it is a gaseous mass, and the
micrometer--supposing its distance to be equal to that of the stars, and
we have no reason to think it less--that it must be large enough to fill
the whole space included within the orbit of Neptune! Here, then, as has
been said, we seem to behold a genesis in the heavens. If Laplace's
nebular hypothesis, or any of the modifications of that hypothesis,
represents the process of formation of a solar system, then we may
fairly conclude that such a process is now actually in operation in this
nebula in Aquarius, where a vast ring of nebulous matter appears to have
separated off from the spherical mass within it. This may not be the
true explanation of what we see there, but, whatever the explanation is,
there can be no question of the high significance of this nebula, whose
shape proclaims unmistakably the operation of great metamorphic forces
there. Of course, with his insignificant optical means, our observer can
see nothing of the strange form of this object, the detection of which
requires the aid of the most powerful telescopes, but it is much to know
where that unfinished creation lies, and to see it, even though
diminished by distance to a mere speck of light.
Turn your glass upon the star shown in the map just above Mu ([mu]) and
Epsilon ([epsilon]). You will find an attractive arrangement of small
stars in its neighborhood. The star marked 104 is double to the naked
eye, and the row of stars below it is well worth looking at. The star
Delta ([delta]) indicates the place where, in 1756, Tobias Mayer
narrowly escaped making a discovery that would have anticipated that
which a quarter of a century later made the name of Sir William Herschel
world-renowned. The planet Uranus passed near Delta in 1756, and Tobias
Mayer saw it, but it moved so slowly that he took it for a fixed star,
never suspecting that his eyes had rested upon a member of the solar
system whose existence was, up to that time, unknown to the inhabitants
of Adam's planet.
Public-domain text, read in full here on John Shaqi.
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