On Molecular and Microscopic Science, Volume 1 (of 2)Somerville, Mary
History
On Molecular and Microscopic Science, Volume 1 (of 2)
Somerville, Mary
Matter -- Constitution; Microscopy; Natural history
When seventy dark lines on the spectrum of the star Aldebaran, and
eighty on that of α Orionis (Betelgeux) were compared with the bright
lines on the spectra of the vapours of a variety of the terrestrial
simple elements, it was found that Aldebaran contained nine terrestrial
substances and α Orionis five: that is, there were only nine out of
seventy of the dark lines of Aldebaran coincident with bright lines, and
five out of eighty of those of α Orionis. Yet the seventy and eighty
dark lines that were compared represented some of the strongest only of
the numerous lines which were seen on the spectra of these stars. Some
of those remaining were probably due to the vapours of other terrestrial
elements which were not compared with these stars, but Mr. Huggins
concludes that many of those dark lines are due to new unknown elements
existing in these stars, and that we cannot assume that the sixty-five
simple terrestrial elements constitute the entire primary material of
the universe. A community of matter, however, exists throughout the
visible creation; for the stars contain many of the elements common to
the sun and earth. ‘It is remarkable that the elements most widely
diffused through the host of stars are some of those most closely
connected with the living organism of our globe, including hydrogen,
sodium, magnesium and iron. May it not be that, at least, the brighter
stars are like our sun, the upholding and energizing centres of systems
of worlds adapted to the abode of living beings?’
With regard to the nebulæ Mr. Huggins’s observations show that nine are
gaseous, the spectra of six exhibiting three bright lines, one shows an
additional faint line also, while the spectra of the dumb-bell nebula
and the annular nebula in Lyra show the brightness of three green lines
only. The spectra of eight other nebulæ were continuous, showing that
their light has not undergone any modification on its way to us.
Mr. Huggins has been able to discriminate between the light of the
nucleus of a comet and that of its tail. The nucleus is self-luminous,
and its substance is in the form of ignited gas. The coma shines by
reflected light as clouds do, and observations of the spectra give
reason to believe that comets chiefly consist of nitrogen and another
elementary body different from nitrogen combined with it.
Public-domain text, read in full here on John Shaqi.
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