Astronomy with an Opera-glass: A Popular Introduction to the Study of the Starry Heavens with the Simplest of Optical InstrumentsServiss, Garrett Putman
Science
Astronomy with an Opera-glass: A Popular Introduction to the Study of the Starry Heavens with the Simplest of Optical Instruments
Serviss, Garrett Putman
Astronomy
Mars, being both more distant and smaller than Venus, does not present
so splendid a scene, and yet when it is at or near opposition it is a
superb object even for an opera-glass, its deep reddish-yellow color
presenting a fine contrast to that of most of the stars. It can often be
seen in conjunction with, or near to, the moon and stars, and the beauty
of these phenomena is in some cases greatly enhanced by the use of a
glass. To find Mars (and the same remark applies to the other planets),
take its right ascension and declination for the required date from the
Nautical Almanac, and then mark its place upon a planisphere or any good
star-map. This planet is at the present time (1888) slowly drawing
nearer to the earth at each opposition, and in 1892 it will be closer to
us than at any time since 1877, when its two minute satellites were
discovered. It will consequently grow brighter every year until then.
How splendidly it shines when at its nearest approach to the earth may
be inferred from the fact that in 1719 it was so brilliant as actually
to cause a panic. This was doubtless owing to its peculiar redness. I
well remember the almost startling appearance which the planet presented
in the autumn of 1877. Mars is especially interesting because of the
apparently growing belief that it may be an inhabited world, and because
of certain curious markings on its surface that can only be seen under
favorable conditions. The recent completion of the great Lick telescope
and other large glasses, and the approach of the planet to a favorable
opposition, give reason to hope that within the next few years a great
deal of light will be cast upon some of the enigmatical features of
Mars's surface.
[Illustration: JUPITER AND HIS MOONS. (SEEN WITH A FIELD-GLASS; SEVEN
DIAMETERS.)]
Jupiter, although much more distant than Mars, is ordinarily a far more
conspicuous phenomenon in the sky on account of his vast bulk. His
interest to observers with an opera-glass depends mainly upon his four
moons, which, as they circle about him, present a miniature of the solar
system. With a strong opera-glass one or two of Jupiter's little family
of moons may occasionally be caught sight of as excessively minute dots
of light half-hidden in the glare of the planet. If you succeed under
favorable circumstances in seeing one of these moons with your glass,
you will be all the more astonished to learn that there are several
apparently well-authenticated instances of one of the moons of Jupiter
having been seen with the naked eye.
With a field-glass, however, you will have no difficulty in seeing all
of the moons when they are properly situated. If you miss one or more of
them, you may know that it is either between you and the planet, or
behind the planet, or buried in the planet's shadow, or else so close to
the planet as to be concealed by its radiance.
Public-domain text, read in full here on John Shaqi.
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