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
But these and other difficulties were at length overcome by
the judgment and perseverance of this ingenious artist.
It appears, however, that Dollond was not the only person who had
the merit of making this discovery--a private gentleman, Mr. Chest,
of Chest-hall, a considerable number of years before, having made a
similar discovery, and applied it to the same purpose. This fact was
ascertained in the course of a process raised against Dollond at the
instance of Watkins, optician at Charing-cross, when applying for a
patent. But as the other gentleman had kept his invention a secret,
and Dollond had brought it forth for the benefit of the public, the
decision was given in his favour. There was no evidence that Dollond
borrowed the idea from his competitor, and both were, to a certain
extent, entitled to the merits of the invention.
One of the greatest obstructions to the construction of large
achromatic telescopes is, the difficulty of procuring large discs of
flint glass of an uniform refractive density--of good colour, and free
from veins. It is said that, fortunately for Mr. Dollond, this kind
of glass was procurable when he began to make achromatic telescopes,
though the attempts of ingenious chemists have since been exerted to
make it without much success. It is also said, that the glass employed
by Dollond in the fabrication of his best telescopes, was of the same
melting, or made at the same time, and that, excepting this particular
treasure, casually obtained, good dense glass for achromatic purposes,
was always as difficult to be procured as it is now. The dispersion of
the flint glass, too, is so variable, that, in forming an achromatic
lens, trials on each specimen require to be made before the absolute
proportional dispersion of the substances can be ascertained. It is
owing, in a great measure, to these circumstances, that a large and
good achromatic telescope cannot be procured unless at a very high
price. Mr. Tulley of Islington--who has been long distinguished as a
maker of excellent achromatic instruments--showed me, about six years
ago, a rude piece of flint glass about five inches diameter, intended
for the concave lens of an achromatic object glass, for which he paid
eight guineas. This was before the piece of glass was either figured
or polished, and, consequently, he had still to perform the delicate
operation of figuring, polishing, and adjusting this concave to the
convex lenses with which it was to be combined; and during the process
some veins or irregularities might be detected in the flint glass which
did not then appear. Some years before, he procured a disc of glass
from the continent about seven or eight inches diameter, for which he
paid about thirty guineas, with which an excellent telescope, twelve
feet focal length, was constructed for the Astronomical Society of
London. It is obvious therefore, that large achromatic telescopes must
be charged at a pretty high price.
Public-domain text, read in full here on John Shaqi.
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