The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomyDick, Thomas
Science
The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomy
Dick, Thomas
Astronomical instruments; Astronomy; Telescopes
There are some objects connected with astronomy which cannot be
perceived without having recourse to instruments and to powers of
great magnitude. But it is a vulgar error to imagine that very large
and very expensive telescopes are absolutely necessary for viewing
the greater part of the more interesting scenery of the heavens. Most
of the phenomena of the planets, comets and double stars and other
objects, are visible with instruments of moderate dimensions, so that
every one who has a relish for celestial investigations, may, at a
comparatively small expense, procure a telescope, for occasional
observations, which will show the principal objects and phenomena
described in books on astronomy. Many persons have been misled by some
occasional remarks which Sir W. Herschel made, in reference to certain
very high powers which he sometimes put, by way of experiment, on some
of his telescopes, as if these were the powers requisite for viewing
the objects to which he refers. For example, it is stated that he once
put a power of 6450 times on his 7 feet Newtonian telescope of 6-3/10
inches aperture; but this was only for the purpose of an experiment,
and could be of no use whatever when applied to the moon, the planets
and most objects in the heavens. Herschel, through the whole course of
his writings, mentions his only having used it _twice_, namely on the
stars α Lyræ, and γ Leonis, which stars can be seen more distinctly and
sharply defined with a power of 420. To produce a power of 6450 on such
a telescope, would require a lens of only 1/77th of an inch in focal
distance, and it is questioned by some whether Herschel had lenses of
so small a size in his possession, or whether it is possible to form
them with accuracy.
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