The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
I do not, indeed, believe that this opinion as to the ultimate
resolvability of all nebulæ could have been shared by those who had much
practical experience in the actual observation of these objects with the
great telescopes, for the particular classes of nebulæ which in
telescopes of superior powers resolved themselves into groups of stars
had a characteristic appearance. After a little experience the observer
soon learned to recognise those nebulæ which promised to be resolvable.
The object might not indeed be resolvable with the powers at his
disposal, but yet from its appearance he often felt that the nebula
would be probably resolved if ever the time should come that greater
powers were applied to the task.
It is easy to illustrate the question at issue by the help of the
photograph of the Cluster in Hercules in Fig. 9. Each of the stars is
there distinct, except where they are much crowded in the centre. If,
however, the photograph be examined through one of those large lenses
which are often used for the purpose, and if the lens be held very much
out of focus, the stars will not be distinguishable separately, and the
whole object will be merely a haze of light. This illustration may help
to explain how the different optical conditions under which an object is
looked at may exhibit, at one time as a diffused nebula, an object which
in better circumstances is seen to be a star-cluster.
The astronomer who was fortunate enough to have the use of a really
great telescope would not fail to notice that, in addition to the
so-called nebulæ already referred to, which were presumably resolvable,
there were certain other objects, generally characterised by a bluish
hue, which in no circumstances whatever presented the appearance of
being composed of separate stars. We now know for certain that these
bluish objects are not clusters of stars, but that they are in the
strictest sense entitled to the name of nebulæ, and that they are
gaseous masses or mists of fire-cloud. The full demonstration of this
important point was not effected until 1864.
Public-domain text, read in full here on John Shaqi.
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