A Popular History of Astronomy During the Nineteenth Century: Fourth EditionClerke, Agnes M. (Agnes Mary)
History
A Popular History of Astronomy During the Nineteenth Century: Fourth Edition
Clerke, Agnes M. (Agnes Mary)
Astronomy -- History -- 19th century
The extravagantly long telescopes of the seventeenth century were
designed to _avoid_ this evil (as well as another source of indistinct
vision in the spherical shape of lenses); but no attempt to _remedy_ it
was made until an Essex gentleman succeeded, in 1733, in so combining
lenses of flint and crown glass as to produce refraction without
colour.[313] Mr. Chester More Hall was, however, equally indifferent to
fame and profit, and took no pains to make his invention public. The
_effective_ discovery of the achromatic telescope was, accordingly,
reserved for John Dollond, whose method of correcting at the same time
chromatic and spherical aberration was laid before the Royal Society in
1758. Modern astronomy may be said to have been thereby rendered
possible. Refractors have always been found better suited than
reflectors to the ordinary work of observatories. They are, so to speak,
of a more robust, as well as of a more plastic nature. They suffer less
from vicissitudes of temperature and climate. They retain their
efficiency with fewer precautions and under more trying circumstances.
Above all, they co-operate more readily with mechanical appliances, and
lend themselves with far greater facility to purposes of exact
measurement.
A practical difficulty, however, impeded the realisation of the
brilliant prospects held out by Dollond's invention. It was found
impossible to procure flint-glass, such as was needed for optical
use--that is, of perfectly homogeneous quality--except in fragments of
insignificant size. Discs of more than two or three inches in diameter
were of extreme rarity; and the crushing excise duty imposed upon the
article by the financial unwisdom of the Government, both limited its
production, and, by rendering experiments too costly for repetition,
barred its improvement.
Up to this time, Great Britain had left foreign competitors far behind
in the instrumental department of astronomy. The quadrants and circles
of Bird, Cary and Ramsden were unapproached abroad. The reflecting
telescope came into existence and reached maturity on British soil. The
refracting telescope was cured of its inherent vices by British
ingenuity. But with the opening of the nineteenth century, the almost
unbroken monopoly of skill and contrivance which our countrymen had
succeeded in establishing was invaded, and British workmen had to be
content to exchange a position of supremacy for one of at least partial
temporary inferiority.
Public-domain text, read in full here on John Shaqi.
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