A Text-Book of AstronomyComstock, George C. (George Cary)
Science
A Text-Book of Astronomy
Comstock, George C. (George Cary)
Astronomy
The radiant energy which is analyzed by the spectroscope has its source
in the atoms and molecules which make up the luminous body from which
the energy is radiated, and these atoms and molecules are able to
impress upon the ether their own peculiarities in the shape of waves of
different length and amplitude. We have seen that by varying the
conditions of the experiment different kinds of waves may be produced in
a bucket of water; and as a study of these waves might furnish an index
to the conditions which produced them, so the study of the waves
peculiar to the light which comes from any source may be made to give
information about the molecules which make up that source. Thus the
molecules of iron produce a system of waves peculiar to themselves and
which can be duplicated by nothing else, and every other substance gives
off its own peculiar type of energy, presenting a limited and definite
number of wave lengths dependent upon the nature and condition of its
molecules. If these molecules are free to behave in their own
characteristic fashion without disturbance or crowding, they emit light
of these wave lengths only, and we find in the spectrum a series of
bright lines, pictures of the slit produced by light of these particular
wave lengths, while between these bright lines lie dark spaces showing
the absence from the radiant energy of light of intermediate wave
lengths. Such a spectrum is shown in the central portion of Fig. 47,
which, as we have already seen, is produced by the space between the
carbons of the arc lamp. On the other hand, if the molecules are closely
packed together under pressure they so interfere with each other as to
give off a jumble of energy of all wave lengths, and this is translated
by the spectroscope into a continuous ribbon of light with no dark
spaces intervening, as in the upper and lower parts of Figs. 47 and 48,
produced by the incandescent solid carbons of the lamp. These two types
are known as the continuous and discontinuous spectrum, and we may lay
down the following principle regarding them:
A discontinuous spectrum, or bright-line spectrum as it is familiarly
called, indicates that the molecules of the source of light are not
crowded together, and therefore the light must come from an incandescent
gas. A continuous spectrum shows only that the molecules are crowded
together, or are so numerous that the body to which they belong is not
transparent and gives no further information. The body may be solid,
liquid, or gaseous, but in the latter case the gas must be under
considerable pressure or of great extent.
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