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
Resuming in a sentence what has been already explained, we find that the
prismatic analysis of the heavenly bodies was founded upon three classes
of facts: First, the unmistakable character of the light given by each
different kind of glowing vapour; secondly, the identity of the light
absorbed with the light emitted by each; thirdly, the coincidence
observed between rays missing from the solar spectrum and rays absorbed
by various terrestrial substances. Thus, a realm of knowledge,
pronounced by Morinus[400] in the seventeenth century, and no less
dogmatically by Auguste Comte[401] in the nineteenth, hopelessly out of
reach of the human intellect, was thrown freely open, and the chemistry
of the sun and stars took at once a leading place among the experimental
sciences.
The immediate increase of knowledge was not the chief result of
Kirchhoff's labours; still more important was the change in the scope
and methods of astronomy, which, set on foot in 1852 by the detection of
a common period affecting at once the spots on the sun and the magnetism
of the earth, was extended and accelerated by the discovery of spectrum
analysis. The nature of that change is concisely indicated by the
heading of the present chapter; we would now ask our readers to
endeavour to realise somewhat distinctly what is implied by the
"foundation of astronomical physics."
Just three centuries ago, Kepler drew a forecast of what he called a
"physical astronomy"--a science treating of the efficient causes of
planetary motion, and holding the "key to the inner astronomy."[402]
What Kepler dreamed of and groped after, Newton realized. He showed the
beautiful and symmetrical revolutions of the solar system to be governed
by a uniformly acting cause, and that cause no other than the familiar
force of gravity, which gives stability to all our terrestrial
surroundings. The world under our feet was thus for the first time
brought into physical connection with the worlds peopling space, and a
very tangible relationship was demonstrated as existing between what
used to be called the "corruptible" matter of the earth and the
"incorruptible" matter of the heavens.
Public-domain text, read in full here on John Shaqi.
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