Half-hours with the Telescope: Being a Popular Guide to the Use of the Telescope as a Means of Amusement and Instruction.Proctor, Richard A. (Richard Anthony)
Science
Half-hours with the Telescope: Being a Popular Guide to the Use of the Telescope as a Means of Amusement and Instruction.
Proctor, Richard A. (Richard Anthony)
Astronomy; Telescopes
The telescope should be well balanced for vision with the small
astronomical eye-pieces. But as there is often occasion to use
appliances which disturb the balance, it is well to have the means of at
once restoring equilibrium. A cord ring running round the tube (pretty
tightly, so as to rest still when the tube is inclined), and bearing a
small weight, will be all that is required for this purpose; it must be
slipped along the tube until the tube is found to be perfectly balanced.
Nothing is more annoying than, after getting a star well in the field,
to see the tube shift its position through defective balance, and thus
to have to search again for the star. Even with such an arrangement as
is shown in fig. 8, though the tube cannot readily shift its position,
it is better to have it well balanced.
The quality of the stand has a very important influence on the
performance of a telescope. In fact, a moderately good telescope,
mounted on a steady stand, working easily and conveniently, will not
only enable the observer to pass his time much more pleasantly, but will
absolutely exhibit more difficult objects than a finer instrument on a
rickety, ill-arranged stand. A good observing-chair is also a matter of
some importance, the least constraint or awkwardness of position
detracting considerably from the power of distinct vision. Such, at
least, is my own experience.
But the mere examination of the glasses, tube, mounting, &c., is only
the first step in the series of tests which should be applied to a
telescope, since the excellence of the instrument depends, not on its
size, the beauty of its mounting, or any extraneous circumstances, but
on its performance.
The observer should first determine whether the chromatic aberration is
corrected. To ascertain this the telescope should be directed to the
moon, or (better) to Jupiter, and accurately focussed for distinct
vision. If, then, on moving the eye-piece towards the object-glass, a
ring of purple appears round the margin of the object, and on moving the
eye-glass in the contrary direction a ring of green, the chromatic
aberration is corrected, since these are the colours of the secondary
spectrum.
Public-domain text, read in full here on John Shaqi.
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