The Popular Science Monthly, September, 1900: Vol. 57, May, 1900 to October, 1900Various
Science
The Popular Science Monthly, September, 1900: Vol. 57, May, 1900 to October, 1900
Various
Science -- Periodicals; Technology -- Periodicals
The ‘Atlas of Representative Stellar Spectra, together with a
Discussion of the Evolutional Order of the Stars,’ by Sir Wm. Huggins,
K. C. B., and Lady Huggins (Wesley & Son), is not only a sumptuous
and beautifully illustrated volume, but is also of great scientific
value. Sir Wm. Huggins belongs to that group of men in England who,
unconnected with any university, devote themselves to research for the
pure love of truth. His distinguished services to science received
recognition on the occasion of the Queen’s diamond jubilee, when with
only two other scientific men he received the order of knighthood. His
accomplished wife, who is his constant coadjutor, was the only woman
mentioned in the list of Jubilee honors. Sir Wm. Huggins may be said
to be the founder of the so-called ‘New Astronomy,’ for scarcely more
than a quarter of a century ago his spectroscope, turned upon a newly
discovered star, first revealed the cause of the sudden lighting up of
these beacons in the heavens, and turned upon the nebula showed them
to be of glowing gas. Since that time the telescope of the Tulse Hill
Observatory, armed with spectroscope and camera, has been constantly
and laboriously analyzing the light of star, comet and nebula, to solve
the mystery of their constitution. “We never go anywhere,” said Lady
Huggins; “astronomy, at best, is a heart-breaking object of devotion
beneath English skies, and we are always at home to catch every gleam
between the clouds.”
This book gives, in charming narrative, which would be read with
interest by one previously ignorant of the subject, the history of the
pioneer work “when nearly every observation revealed a new fact, and
almost every night’s work was red-lettered by some discovery.”
There follow full details of later work, especially of the first
detection, by the shifting of the lines of their spectra, of the motion
of stars towards us or from us in the line of sight. We learn also how
terrestrial chemistry has been enriched by this study of the stars, and
how the nature of long known elements like hydrogen and the existence
of undiscovered elements like helium have been first made out from
stellar spectra.
Public-domain text, read in full here on John Shaqi.
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