A Text-Book of AstronomyComstock, George C. (George Cary)
Science
A Text-Book of Astronomy
Comstock, George C. (George Cary)
Astronomy
87. ABSORPTION SPECTRA.--There is another kind of spectrum, of greater
importance than either of those above considered, which is well
illustrated by the spectrum of sunlight (Fig. 50). This is a nearly
continuous spectrum crossed by numerous _dark_ lines due to absorption
of radiant energy in a comparatively cool gas through which it passes on
its way to the spectroscope. Fraunhofer, who made the first careful
study of spectra, designated some of the more conspicuous of these lines
by letters of the alphabet which are shown in the plate, and which are
still in common use as names for the lines, not only in the spectrum of
sunlight but wherever they occur in other spectra. Thus the double line
marked _D_, wave length 5893, falls at precisely the same place in the
spectrum as does the double (sodium) line which we have already seen in
the yellow part of the arc-light spectrum, which line is also called _D_
and bears a very intimate relation to the dark _D_ line of the solar
spectrum.
The student who has access to colored crayons should color one edge of
Fig. 50 in accordance with the lettering there given and, so far as
possible, he should make the transition from one color to the next a
gradual one, as it is in the rainbow.
Fig. 50 is far from being a complete representation of the spectrum of
sunlight. Not only does this spectrum extend both to the right and to
the left into regions invisible to the human eye, but within the limits
of the figure, instead of the seventy-five lines there shown, there are
literally thousands upon thousands of lines, of which only the most
conspicuous can be shown in such a cut as this.
The dark lines which appear in the spectrum of sunlight can, under
proper conditions, be made to appear in the spectrum of an arc light,
and Fig. 51 shows a magnified representation of a small part of such a
spectrum adjacent to the _D_ (sodium) lines. Down the middle of each of
these lines runs a black streak whose position (wave length) is
precisely that of the _D_ lines in the spectrum of sunlight, and whose
presence is explained as follows:
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