Pleasures of the telescope: An Illustrated Guide for Amateur Astronomers and a Popular Description of the Chief Wonders of the Heavens for General ReadersServiss, Garrett Putman
Science
Pleasures of the telescope: An Illustrated Guide for Amateur Astronomers and a Popular Description of the Chief Wonders of the Heavens for General Readers
Turning to Delphinus, we find a very beautiful double in gamma,
magnitudes four and five, distance 11", p. 273 deg., colors golden and
emerald. The leader alpha, which is not as bright as its neighbor beta,
and which is believed to be irregularly variable, is of magnitude four,
and has a companion of nine and a half magnitude at the distance 35", p.
278 deg.. At a similar distance, 35", p. 335 deg., beta has an
eleventh-magnitude companion, and the main star is also double, but
excessively close, and much beyond our reach. It is believed to be a
swiftly moving binary, whose stars are never separated widely enough to
be distinguished with common telescopes.
CHAPTER VI
FROM LYRA TO ERIDANUS
"This Orpheus struck when with his wondrous song
He charmed the woods and drew the rocks along."--MANILIUS.
[Illustration: MAP NO. 17.]
We resume our celestial explorations with the little constellation Lyra,
whose chief star, Vega (alpha), has a very good claim to be regarded as
the most beautiful in the sky. The position of this remarkable star is
indicated in map No. 17. Every eye not insensitive to delicate shades of
color perceives at once that Vega is not white, but blue-white. When the
telescope is turned upon the star the color brightens splendidly.
Indeed, some glasses decidedly exaggerate the blueness of Vega, but the
effect is so beautiful that one can easily forgive the optical
imperfection which produces it. With our four-inch we look for the
well-known companion of Vega, a tenth-magnitude star, also of a blue
color deeper than the hue of its great neighbor. The distance is 50", p.
158 deg.. Under the most favorable circumstances it might be glimpsed with
the three-inch, but, upon the whole, I should regard it as too severe a
test for so small an aperture.
Vega is one of those stars which evidently are not only enormously
larger than the sun (one estimate makes the ratio in this case nine
hundred to one), but whose physical condition, as far as the
spectroscope reveals it, is very different from that of our ruling orb.
Like Sirius, Vega displays the lines of hydrogen most conspicuously, and
it is probably a much hotter as well as a much more voluminous body
than the sun.
Public-domain text, read in full here on John Shaqi.
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