A Popular History of Astronomy During the Nineteenth Century: Fourth EditionClerke, Agnes M. (Agnes Mary)
History
A Popular History of Astronomy During the Nineteenth Century: Fourth Edition
Clerke, Agnes M. (Agnes Mary)
Astronomy -- History -- 19th century
Now all incandescent solid or liquid substances, and even gases ignited
under great pressure, give what is called a "continuous spectrum;" that
is to say, the light derived from them is of every conceivable hue.
Sorted out with the prism, its tints merge imperceptibly one into the
other, uninterrupted by any dark spaces. No colours, in short, are
missing. But gases and vapours rendered luminous by heat emit rays of
only a few tints, which accordingly form an interrupted spectrum,
usually designated as one of lines or bands. And since these rays are
perfectly definite and characteristic--not being the same for any two
substances--it is easy to tell what kind of matter is concerned in
producing them. We may suppose that the inconceivably minute particles
which by their rapid thrilling agitate the ethereal medium so as to
produce light, are free to give out their peculiar tone of vibration
only when floating apart from each other in gaseous form; but when
crowded together into a condensed mass, the clear ring of the
distinctive note is drowned, so to speak, in a universal molecular
clang. Thus prismatic analysis has no power to identify individual kinds
of matter, except when they present themselves as glowing vapours.
A spectrum is said to be "reversed" when lines previously seen bright on
a dark background appear dark on a bright background. In this form it is
equally characteristic of chemical composition with the "direct"
spectrum, being due to _absorption_, as the latter is to _emission_. And
absorption and emission are, by Kirchhoff's law, strictly correlative.
This is easily understood by the analogy of sound. For just as a
tuning-fork responds to sound-waves of its own pitch, but remains
indifferent to those of any other, so those particles of matter whose
nature it is, when set swinging by heat, to vibrate a certain number of
times in a second, thus giving rise to light of a particular shade of
colour, appropriate those same vibrations, and those only, when
transmitted past them,--or, phrasing it otherwise, are opaque to them,
and transparent to all others.
It should further be explained that the _shape_ of the bright or dark
spaces in the spectrum has nothing whatever to do with the nature of the
phenomena. The "lines" and "bands" so frequently spoken of are seen as
such for no other reason than because the light forming them is admitted
through a narrow, straight opening. Change that opening into a fine
crescent or a sinuous curve, and the "lines" will at once appear as
crescents or curves.
Public-domain text, read in full here on John Shaqi.
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