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
The great telescope mounted in 1888, a 36-inch refractor by Alvan Clark,
has fulfilled every expectation of its projectors, and justified the
selection of the site in every particular. The elevation, although
moderate, is still high enough to secure very marked advantage in
clearness and steadiness of the air, and at the same time not so high
that the health and activities of the observers are appreciably affected
by the thinner air of the summit. This telescope is known the world over
for the monumental contributions to science made by the able astronomers
who have worked with it: among them Barnard who discovered the fifth
satellite of Jupiter in 1892; Burnham, Hussey, and Aitken, who have
discovered and measured thousands of close double stars; Keeler, who
spent many faithful years on the summit; and Campbell, the present
director, whose spectroscopic researches on stellar movements have added
greatly to our knowledge of the structure of the universe. Among the
many lines of research now in progress at the Lick Observatory and in
the D. O. Mills Observatory at Santiago, Chile, are the discoveries of
stars whose velocities in space are not constant, but variable with the
spectral type of the star. Mr. Lick's bequest for the Observatory was
about $700,000. So ably has this scientific trust been administered that
he might well have endowed it with his entire estate, exceeding
$4,000,000.
Another California mountain that was early investigated is Mount
Whitney. Its summit elevation is nearly 15,000 feet, and in 1881 Langley
made its ascent for the purpose of measuring the solar constant. He
found conditions much more favorable than on Mount Etna,
Sicily--elevation about 10,000 feet--which he had visited the year
before. But the height of Mount Whitney was such as to occasion him much
inconvenience from mountain sickness, an ailment which is most
distressing and due partly to lack of oxygen and partly to mere
diminution of mechanical pressure. Mount Whitney was also visited many
years after by Campbell for investigating the spectrum of Mars in
comparison with that of the moon. Langley found on Mount Whitney an
excellent station lower down, at about 12,000 feet elevation; and by
equipping the two stations with like apparatus for measuring the solar
heat, he obtained very important data on the selective absorption of the
atmosphere.
Public-domain text, read in full here on John Shaqi.
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