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 phenomena mentioned above are about all that a small telescope
will reveal. Occasionally a dark streak, which large instruments show
is connected with the mysterious system of “canals,” can be detected,
but the “canals” themselves are far beyond the reach of any telescope
except a few of the giants handled by experienced observers. The
conviction which seems to have forced its way into the minds even of
some conservative astronomers, that on Mars the conditions, to use
the expression of Professor Young, “are more nearly earthlike than on
any other of the heavenly bodies which we can see with our present
telescopes,” is sufficient to make the planet a center of undying
interest notwithstanding the difficulties with which the amateur is
confronted in his endeavors to see the details of its markings.
[Illustration: THE ILLUMINATION OF VENUS’S ATMOSPHERE AT THE BEGINNING
OF HER TRANSIT ACROSS THE SUN.]
In Venus “the fatal gift of beauty” may be said, as far as our
observations are concerned, to be matched by the equally fatal gift of
brilliance. Whether it be due to atmospheric reflection alone or to the
prevalence of clouds, Venus is so bright that considerable doubt exists
as to the actual visibility of any permanent markings on her surface.
The detailed representations of the disk of Venus by Mr. Percival
Lowell, showing in some respects a resemblance to the stripings of
Mars, can not yet be accepted as decisive. More experienced astronomers
than Mr. Lowell have been unable to see at all things which he draws
with a fearless and unhesitating pencil. That there are some shadowy
features of the planet’s surface to be seen in favorable circumstances
is probable, but the time for drawing a “map of Venus” has not yet come.
The previous work of Schiaparelli lends a certain degree of probability
to Mr. Lowell’s observations on the rotation of Venus. This rotation,
according to the original announcement of Schiaparelli, is probably
performed in the same period as the revolution around the sun. In other
words, Venus, if Schiaparelli and Lowell are right, always presents the
same side to the sun, possessing, in consequence, a day hemisphere and
a night hemisphere which never interchange places. This condition is
so antagonistic to all our ideas of what constitutes habitability for
a planet that one hesitates to accept it as proved, and almost hopes
that it may turn out to have no real existence. Venus, as the twin of
the earth in size, is a planet which the imagination, warmed by its
sunny aspect, would fain people with intelligent beings a little fairer
than ourselves; but how can such ideas be reconciled with the picture
of a world one half of which is subjected to the merciless rays of a
never-setting sun, while the other half is buried in the fearful gloom
and icy chill of unending night?
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