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
Bode's Law did good service in the quest for a trans-Uranian planet by
affording ground for a probable assumption as to its distance. A
starting-point for approximation was provided by it; but it was soon
found to be considerably at fault. Even Uranus is about 36 millions of
miles nearer to the sun than the order of progression requires; and
Neptune's vast distance of 2,800 million should be increased by no less
than 800 million miles, and its period of 165 lengthened out to 225
years,[223] in order to bring it into conformity with the curious and
unexplained rule which planetary discoveries have alternately tended to
confirm and to invalidate.
Within seventeen days of its identification with the Berlin achromatic,
Neptune was found to be attended by a satellite. This discovery was the
first notable performance of the celebrated two-foot reflector[224]
erected by Mr. Lassell at his suggestively named residence of Starfield,
near Liverpool. William Lassell was a brewer by profession, but by
inclination an astronomer. Born at Bolton in Lancashire, June 18, 1799,
he closed a life of eminent usefulness to science, October 5, 1818, thus
spanning with his well-spent years four-fifths of the momentous period
which we have undertaken to traverse. At the age of twenty-one, being
without the means to purchase, he undertook to construct telescopes, and
naturally turned his attention to the reflecting sort, as favouring
amateur efforts by the comparative simplicity of its structure. His
native ingenuity was remarkable, and was developed by the hourly
exigencies of his successive enterprises. Their uniform success
encouraged him to enlarge his aims, and in 1844 he visited Birr Castle
for the purpose of inspecting the machine used in polishing the giant
speculum of Parsonstown. In the construction of his new instrument,
however, he eventually discarded the model there obtained, and worked on
a method of his own, assisted by the supreme mechanical skill of James
Nasmyth. The result was a Newtonian of exquisite definition, with an
aperture of two, and a focal length of twenty feet, provided by a novel
artifice with the equatoreal mounting, previously regarded as available
only for refractors.
Public-domain text, read in full here on John Shaqi.
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