Round the year with the stars: The chief beauties of the starry heavens as seen with the naked eyeServiss, Garrett Putman
Science
Round the year with the stars: The chief beauties of the starry heavens as seen with the naked eye
Serviss, Garrett Putman
Astronomy -- Popular works
Of the effect of the Precession of the Equinoxes, to which Emerson
refers, we have already spoken. But it is a long time in the future
that Vega will begin, or rather resume, its reign as the Star of
the North. And, curiously enough, when that time comes the northern
hemisphere will have its Summer Solstice when the sun is just opposite
to the place which it now occupies at that season, and when Antares
will be no more a summer star, but will flash its ruddy light upon the
snows of a winter longer and colder than the winters that we know,
while Orion will blaze above the summer landscapes. This immense
revolution, some have thought, may be the measure of the “Great Year”
of Plato, and if the chronology adopted for dating the early remains of
civilization recently uncovered in Crete is correct, we have evidence
that mankind has persisted through one of these vast periods, and that
nations flourished round the Mediterranean when Vega was formerly the
Pole-star.
The beauty of Vega, which has been admired and commented on from the
earliest times, is much enhanced when it is viewed with a telescope.
Then the blueness of its light becomes evident, and one is the more
astonished at the unquestionable fact that it outshines the sun a
hundred times. A _sapphire_ sun, a hundred times more brilliant than
ours! The proper motion of the solar system, which carries us through
space about twelve miles per second, is bearing us almost directly
toward Vega, so that as future ages unroll the star should become
brighter and brighter with decrease of distance, until eventually it
may outshine every other orb in the firmament, and put Sirius himself
to shame by its overpowering splendor.
The little star Epsilon (ε), the northernmost one of the pair near
Vega, is a celebrated quadruple, easily seen as such with a telescope
of moderate power.
A little less than half way from Beta (β) to Gamma (γ) the telescope
discovers the wonderful “Ring Nebula,” a delicate circle of nebulous
light with a star in the centre. This star is more conspicuous in
photographs than in telescopic views. This object has been regarded as
a visual proof of the correctness of Laplace’s theory of the origin of
the solar system from nebulous rings surrounding a central sun, but
the Lick photographs show that the ring in this case is of a strangely
complex constitution. Beta is both a binary and a variable star.
Public-domain text, read in full here on John Shaqi.
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