Scientific American Supplement, No. 288, July 9, 1881Various
Science
Scientific American Supplement, No. 288, July 9, 1881
Various
Science -- Periodicals
Another result followed the use of the micrometer: the detection of the
proper motion of the stars. For several thousand years the stars have
been called "fixed," but the fine rulings of the filar micrometer tell a
different story. There are catalogues of several hundred moving stars,
whose motion is from one-half second to eight seconds annually. The
binary star, Sixty-one Cygni, the nearest north of the equator, moves
eight seconds every year, a displacement equal in three hundred and
sixty years to the apparent diameter of the moon. The fixed stars have
no general motion toward any point, but move in all directions.
Thus the micrometer revealed to man the magnitude and general structure,
together with the motions and revolutions of the sidereal heavens. Above
all, it demonstrated that gravity extends throughout the universe. Still
the longings of men were not appeased; they brought to view invisible
suns sunk in space, and told their weight, yet the thirst for knowledge
was not quenched. Men wished to know what all the suns are made of,
whether of substances like those composing the earth, or of kinds of
matter entirely different. Then was devised the spectroscope, and with
it men audaciously questioned nature in her most secluded recesses. The
basis of spectroscopy is the prism, which separates sunlight into seven
colors and projects a band of light called a spectrum. This was known
for three hundred years, and not much thought of it until Fraunhofer
viewed it with a telescope, and was surprised to find it filled with
hundreds of black lines invisible to the unaided eye. Could it be
possible that there are portions of the solar surface that fail to send
out light? Such is the fact, and then began a twenty years' search to
learn the cause. The lines in the solar spectrum were unexplained until
finally metals were vaporized in the intense heat of the electric arc
and the light passed through a spectroscope, when behold the spectra of
metals were filled with bright lines in the same places as were the
dark lines in the spectrum of the sun. Another step: if when metals are
volatilized in the arc, rays of light from the sun are passed through
the vapor and allowed to enter the spectroscope, a great change is
wrought; a reversal takes place, and the original black bands reappear.
A new law of nature was discovered, thus: "Vapors of all elements absorb
the same rays of light which they emit when incandescent." Every element
makes a different spectrum with lines in different places and of
different widths. These have been memorized by chemists, so that when an
expert having a spectroscope sees anything burn he can tell what it is
as well as read a printed page. Men have learned the alphabet of the
universe, and can read in all things radiating light, the constituent
elements. The black lines in the solar spectrum are there because in the
atmosphere of the sun exist vapors of metals, and the light from the
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