The Book of Stars: Being a Simple Explanation of the Stars and Their Uses to Boy LifeCollins, A. Frederick (Archie Frederick)
Science
The Book of Stars: Being a Simple Explanation of the Stars and Their Uses to Boy Life
Collins, A. Frederick (Archie Frederick)
Astronomy -- Juvenile literature; Stars -- Juvenile literature
A comet is really made up of three parts, which are, (1) a bright head
or core, called a _nucleus_, and this is covered with (2) a layer of
hazy light, called a _coma_, to which there is attached (3) a luminous
_tail_, all of which is shown in Fig. 128. The nucleus of a comet is
formed of a bunch of stones and pieces of iron, all widely separated
and which are held together by attraction as they speed through space.
As a comet nears the Sun it begins to get hot and to throw off burning
gases, which make up its coma, and these bright gases streaming along
form its tail.
There are several ways in which a comet can be told from the planets.
In the first place, new comets, that is, comets which have never been
discovered before, appear suddenly and in any part of the sky, though
they may be very dim at first, and after a while they fade away,
sometimes never to return again.
[Illustration: FIG. 129.—AN ELLIPSE, PARABOLA AND HYPERBOLA.]
Second, they shine chiefly with their own light like the stars; third,
they do not travel in small circles around the Sun like the planets;
but the paths they take are either long ovals, called _ellipses_,
or great curves whose ends never meet, called _parabolas_ and
_hyperbolas_, as shown in Fig. 129; fourth, they do not travel through
space in a line with the planets and Sun, but shoot in and out of our
solar system from and to every direction; and fifth and last, they
travel at enormously high speeds.
Now, a comet, however great it may grow to be, never bursts into view,
big, bright and beautiful, but when one is found it is usually seen as
a little, dim patch of light, and it would quite likely be mistaken for
a _nebula_, if it did not move along so swiftly.
[Illustration: FIG. 130.—HEAD AND TAIL OF COMET DO NOT OBEY THE SAME
LAWS.]
A comet can be told by its movement and its movement can be plotted in
the same way I have described for plotting the position of a planet
in Chapter IV; and so, if you see a dim, little ball of light in the
sky and find that it changes its position when compared with the fixed
stars near it you may guess that you have discovered a comet.
The next thing you should make sure of is, that you have not found one
of our old familiar friends, the planets. If it is really a great comet
coming toward the Sun, it will grow larger and brighter every night,
and you will soon be able to see its tail, which is the real earmark of
a really truly comet.
When a comet is nearest us its head may shine far brighter than any of
the planets, and its great tail may be millions of miles in length, and
spread out in a glowing arc and light up the whole sky.
When this time comes a comet is by far a greater sight to the naked eye
than it is when seen through the largest telescope. You should observe
the comet often and carefully, for another one may not appear for a
long time.
[Illustration: FIG. 131.—HALLEY’S COMET, FROM PHOTO.]
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