Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
In the summer of 1872, Young spent several weeks at Sherman, Wyoming, at
an elevation exceeding 8,300 feet. He carried with him the 9.4-inch
telescope of Dartmouth College, where he was then professor, and this
was the first expedition on which a large glass was used by a very
skillful observer at great elevation. He found the number of good days
and nights small, but the sky was exceedingly favorable when clear. Many
7th magnitude stars could be detected with the naked eye. Young's
observations at Sherman were mainly spectroscopic, however, and they
demonstrated the immense advantage of a high-level station, far above
the dust and haze of the lower atmosphere. He pronounced the 9.4-inch
glass at 8,000 feet the full equivalent of a 12-inch at sea level.
Mont Blanc of 15,000 feet elevation was another summit where the veteran
Janssen of Paris maintained a station for many years; but the
continental conditions of atmospheric moisture and circulation were not
favorable on the whole. Janssen was mainly interested in the sun, and
the daylight seeing is rarely benefited, owing to the strong upward
currents of warm air set in motion by the sun itself.
Mountains in the beautiful climate of California were among the earliest
investigated, and when in 1874 the trustees of Mr. James Lick's estate
were charged with equipping an observatory with the most powerful
telescope in existence, they wisely located on the summit of Mount
Hamilton. It is 4,300 feet above sea level, and Burnham and other
astronomers made critical tests of the steadiness of vision there by
observing double stars, which afford perhaps the best means of comparing
the optical quality of the atmosphere of one region with another. The
writer was fortunate in having charge of the observations of the transit
of Venus in 1882 on the mountain, when the Observatory was in process of
construction, and the quality of the photographs obtained on that
occasion demonstrated anew the excellence of the site. Particularly at
night, for about nine months of the year, the seeing is exceptionally
good, especially when fog banks rolling in from the Pacific, cover the
valleys below like a blanket, preventing harmful radiation from the soil
below.
Public-domain text, read in full here on John Shaqi.
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