Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
[37] Mr. Gore has recently made some remarkable deductions, with regard
to the amount of light which we get from the stars. He considers that
most of this light comes from stars below the sixth magnitude; and
consequently, if all the stars visible to the naked eye were to be
blotted out, the glow of the night sky would remain practically the same
as it is at present. Going to the other end of the scale, he thinks also
that the combined light which we get from all the stars below the
seventeenth magnitude is so very small, that it may be neglected in such
an estimation. He finds, indeed, that if there are stars so low as the
twentieth magnitude, one hundred millions of them would only be equal in
brightness to a single first-magnitude star like Vega. On the other
hand, it is possible that the light of the sky at night is not entirely
due to starlight, but that some of it may be caused by phosphorescent
glow.
CHAPTER XXVI
THE STELLAR UNIVERSE--_continued_
It is very interesting to consider the proper motions of stars with
reference to such an isolated stellar system as has been pictured in the
previous chapter. These proper motions are so minute as a rule, that we
are quite unable to determine whether the stars which show them are
moving along in straight lines, or in orbits of immense extent. It
would, in fact, take thousands of years of careful observation to
determine whether the paths in question showed any degree of curving. In
the case of the more distant stars, the accurate observations which have
been conducted during the last hundred years have not so far revealed
any proper motions with regard to them; but one cannot escape the
conclusion that these stars move as the others do.
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