Appletons' Popular Science Monthly, January 1900: Vol. 56, November, 1899 to April, 1900Various
Science
Appletons' Popular Science Monthly, January 1900: Vol. 56, November, 1899 to April, 1900
Various
Science -- Periodicals; Technology -- Periodicals
The satisfaction of viewing with one’s own eyes some of the things the
astronomers write and talk about is very great, and the illumination
that comes from such viewing is equally great. Just as in foreign
travel the actual seeing of a famous city, a great gallery filled with
masterpieces, or a battlefield where decisive issues have been fought
out illuminates, for the traveler’s mind, the events of history, the
criticisms of artists, and the occurrences of contemporary life in
foreign lands, so an acquaintance with the sights of the heavens gives
a grasp on astronomical problems that can not be acquired in any other
way. The person who has been in Rome, though he may be no archæologist,
gets a far more vivid conception of a new discovery in the Forum than
does the reader who has never seen the city of the Seven Hills; and
the amateur who has looked at Jupiter with a telescope, though he may
be no astronomer, finds that the announcement of some change among the
wonderful belts of that cloudy planet has for him a meaning and an
interest in which the ordinary reader can not share.
[Illustration: JUPITER SEEN WITH A FIVE-INCH TELESCOPE. Shadow of a
satellite visible.]
Jupiter is perhaps the easiest of all the planets for the amateur
observer. A three-inch telescope gives beautiful views of the great
planet, although a four-inch or a five-inch is of course better. But
there is no necessity for going beyond six inches’ aperture in any
case. For myself, I think I should care for nothing better than my
five-inch of fifty-two inches’ focal distance. With such a glass more
details are visible in the dark belts and along the bright equatorial
girdle than can be correctly represented in a sketch before the
rotation of the planet has altered their aspect, while the shadows
of the satellites thrown upon the broad disk, and the satellites
themselves when in transit, can be seen sometimes with exquisite
clearness. The contrasting colors of various parts of the disk are also
easily studied with a glass of four or five inches’ aperture.
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