The story of the universe. Volume 1 (of 4) : $b The starry skies
History
The story of the universe. Volume 1 (of 4) : $b The starry skies
Astronomy; Earth (Planet); Natural history
Let us go back to Fig. 2. If we draw a straight line through the two
stars marked α and β which form the right side of the square, and
produce it beyond α to a distance equal to five times that from β
to α, or to a distance equaling that from α to the end of the tail,
η, we find a star a little less brilliant than at the extremity of
a figure similar to the Great Bear, but smaller and pointing in
the opposite direction. This is the _Little Bear_, or the _Little
Chariot_, also formed of seven stars. The star to which our line
leads us—that which is at the tip of the tail of the Little Bear, or
at the end of the pole of the Little Chariot—is the _polar star_.
[Illustration: Fig. 3]
The polar star enjoys a certain fame, like all persons who are
distinguished from the common, because, among all the bodies which
scintillate in the starry night, it alone remains motionless in the
heavens. At any moment of the year, by day or by night, when you
observe the sky, you will always find it. All the other stars, on the
contrary, turn in twenty-four hours round it, taken as the centre of
this immense vortex. The pole star remains motionless at the pole of
the world, from whence it serves as a fixed point to navigators on
the trackless ocean, as well as to travelers in the unexplored desert.
[Illustration: Fig. 4]
In looking at the pole star, motionless in the midst of the northern
region of the sky, we have the south behind us, the east to the
right, the west to the left. All the stars turn round the pole star
in a direction contrary to that of the hands of a watch; they should,
then, be recognized according to their mutual relations rather than
by reference to the cardinal points.
On the other side of the pole star, with reference to the Great
Bear, is found another constellation which we can also recognize
at once. If from the middle star, δ, we draw a line to the pole,
and produce this line by the same distance (see Fig. 3), we arrive
at _Cassiopeia_, formed of five principal stars arranged somewhat
like the strokes of the letter M. The little star χ, which completes
the square, gives the constellation the form of a _chair_. This
group assumes all possible positions in turning round the pole; it
is found sometimes above, sometimes below, sometimes to the right,
and sometimes to the left; but it is always easily recognized, for,
like the preceding group, it never sets, and is always opposite to
the Great Bear. The pole star is the axle round which both these
constellations turn.
[Illustration: Fig. 5 Fig. 6]
Public-domain text, read in full here on John Shaqi.
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