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
The theory has, however, to be considered under still another aspect. It
frequently happens that the contortions or displacements due to motion
are seen to affect a single line belonging to a particular substance,
while the other lines of _that same substance_ remain imperturbable.
Now, how is this most singular fact, which seems at first sight to imply
that a body may be at rest and in motion at one and the same instant, to
be accounted for? It is accounted for, on the present hypothesis, easily
enough, by supposing that the rays thus discrepant in their testimony,
do _not_ belong to one kind of matter, but to several, combined at
ordinary temperatures to form a body in appearance "elementary." Of
these different vapours, one or more may of course be rushing rapidly
towards or from the observer, while the others remain still; and since
the line of sight across the average prominence-region penetrates, at
the sun's edge, a depth of about 300,000 miles,[661] all the
incandescent materials separately occurring along which line are
projected into a single "flame" or "cloud," it will be perceived that
there is ample room for diversities of behaviour.
The alternative mode of escape from the perplexity consists in assuming
that the vapour in motion is rendered luminous under conditions which
reduce its spectrum to a few rays, the unaffected lines being derived
from a totally distinct mass of the same substance shining with its
ordinary emissions.[662] Thus, calcium can be rendered virtually
monochromatic by attenuation, and analogous cases are not rare.
Sir Norman Lockyer only asks us to believe that effects which follow
certain causes on the earth are carried a stage further in the sun,
where the same causes must be vastly intensified. We find that the
bodies we call "compound" split asunder at fixed degrees of heat
_within_ the range of our resources. Why should we hesitate to admit
that the bodies we call "simple" do likewise at degrees of heat
_without_ the range of our resources? The term "element" simply
expresses terrestrial incapability of reduction. That, in celestial
laboratories, the means and their effect here absent should be present,
would be an inference challenging, in itself, no expression of
incredulity.
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