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
Another research of exceptional promise will be undertaken, which is of
great importance in a general study of stellar evolution; and that is
the determination of the spectral-energy curves of stars of various
classes, for the purpose of measuring their surface temperatures. A very
few of the nebulæ are found to be variable, and their peculiarities need
investigation, also special problems of variable stars and temporary
stars, and the spectra of the components of close double stars which are
beyond the power of all other instruments to photograph.
Such a program of research conveys an excellent idea of many of the
great problems that are under investigation by astronomers to-day, and
gives some notion of the instrumental means requisite in executing
comprehensive plans of this character. It will not escape notice that
the climax of instrumental development attained at Mount Wilson has only
been made possible by an unbroken chain of progress, link by link, each
antecedent link being necessary to the successful forging of its
following one. In very large part, and certainly indispensable to these
instrumental advances, has the art of working in glass and metals been
the mainstay of research. As we review the history of astronomical
progress, from Galileo's time to our own, the consummate genius of the
artisan and his deft handiwork compel our admiration almost equally with
the keen intelligence of the astronomer who uses these powerful engines
of his own devising to wrest the secrets of nature from the heavens.
CHAPTER XXIV
OUR SOLAR SYSTEM
Now let us go upward in imagination, far, far beyond the tops of the
highest mountains, beyond the moon and sun, and outward in space until
we reach a point in the northern heavens millions and millions of miles
away, directly above and equally distant from all points in the
ecliptic, or path in which our earth travels yearly round the sun. Then
we should have that sort of comprehensive view of the solar system which
is necessary if we are to visualize as a whole the working of the vast
machine, and the motions, sizes, and distances of all the bodies that
comprise it. Of such stupendous mechanism our earth is part.
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