A Text-Book of AstronomyComstock, George C. (George Cary)
Science
A Text-Book of Astronomy
Comstock, George C. (George Cary)
Astronomy
209. STELLAR COLORS.--We have already seen that one star differs from
another in respect of color as well as brightness, and the diligent
student of the sky will not fail to observe for himself how the luster
of Sirius and Rigel is more nearly a pure white than is that of any
other stars in the heavens, while at the other end of the scale
α Orionis and Aldebaran are strongly ruddy, and Antares presents an
even deeper tone of red. Between these extremes the light of every star
shows a mixture of the rainbow hues, in which a very pale yellow is the
predominant color, shading off, as we have seen, to white at one end of
the scale and red at the other. There are no green stars, or blue stars,
or violet stars, save in one exceptional class of cases--viz., where the
two components of a double star are of very different brightness, it is
quite the usual thing for them to have different colors, and then,
almost without exception, the color of the fainter star lies nearer to
the violet end of the spectrum than does the color of the bright one,
and sometimes shows a distinctly blue or green hue. A fine type of such
double star is β Cygni, in which the components are respectively
yellow and blue, and the yellow star furnishes eight times as much light
as the blue one.
The exception which double stars thus make to the general rule of
stellar colors, yellow and red, but no color of shorter wave length, has
never been satisfactorily explained, but the rule itself presents no
difficulties. Each star is an incandescent body, giving off radiant
energy of every wave length within the limits of the visible spectrum,
and, indeed, far beyond these limits. If this radiant energy could come
unhindered to our eyes every star would appear white, but they are all
surrounded by atmospheres--analogous to the chromosphere and reversing
layer of the sun--which absorb a portion of their radiant energy and,
like the earth's atmosphere, take a heavier toll from the violet than
from the red end of the spectrum. The greater the absorption in the
star's atmosphere, therefore, the feebler and the ruddier will be its
light, and corresponding to this the red stars are as a class fainter
than the white ones.
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