A History of Science — Volume 5Williams, Henry Smith
History
A History of Science — Volume 5
Williams, Henry Smith
Science -- History
The theory of the decomposition of the elements is closely bound up with
the meteoritic theory. In a word, it may be said of each that Professor
Lockyer is firmly convinced that all the evidence that has accumulated
in recent years is so strongly in favor as to bring these theories
almost to a demonstration. The essence of the meteoritic theory, it
will be recalled, is that all stars have their origin in nebulae which
consist essentially of clouds of relatively small meteorites. It will be
recalled further that Professor Lockyer long ago pointed out that
stars pass through a regular series of changes as to temperature, with
corresponding changes of structure, becoming for a time hotter and
hotter until a maximum is reached, and then passing through gradual
stages of cooling until their light dies out altogether. Very recently
Professor Lockyer has been enabled, through utilization of the multiform
records accumulated during years of study, to define the various typical
stages of the sidereal evolution; and not merely to define them but
to illustrate them practically by citing stars which belong to each
of these stages, and to give them yet clearer definition by naming the
various elements which the spectroscope reveals as present in each.
His studies have shown that the elements do not always give the same
spectrum under all conditions; a result quite at variance with the
earlier ideas on the subject. Even in the terrestrial laboratory it
is possible to subject various metals, including iron, to temperatures
attained with the electric spark at which the spectrum becomes different
from that, for example, which was attained with the lower temperature
of the electric arc. Through these studies so-called series-spectra
have been attained for various elements, and a comparison of these
series-spectra with the spectra of various stars has led to the
conclusion that many of the unknown lines previously traced in the
spectra of such stars are due to the decomposition products of familiar
elements; all of which, of course, is directly in line of proof of the
dissociation hypothesis.
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