The story of the sun, moon, and starsGiberne, Agnes
Science
The story of the sun, moon, and stars
Giberne, Agnes
Astronomy -- Juvenile literature
We have been thinking a good deal about single stars and double stars,
as seen from earth. Now we have to turn our attention to groups,
clusters, _masses_ of stars, in the far regions of space.
Have you ever noticed on a winter night, when the sky was clear and
dotted with twinkling stars, a band of faintly-glimmering light
stretching across the heavens from one horizon to the other? The band
is irregular in shape, sometimes broader, sometimes narrower; here more
bright, there more dim. If you were in the Southern Hemisphere you
would see the same soft belt of light passing all across the southern
heavens. This band or belt is called the Milky Way.
But what is the Milky Way? It is made up of stars. So much we know.
As the astronomer turns his telescope to the zone of faintly-gleaming
light, he finds stars appearing behind stars in countless multitudes;
and the stronger his telescope, the more the white light changes into
distant stars.
Our sun we believe to be one of the stars of the Milky Way; merely
one star among millions of stars; merely one golden grain among the
millions of sparkling gold-dust grains scattered lavishly through
creation. Scattered, not recklessly, not by chance, but placed,
arranged, and guided each by its Maker’s upholding hand.
The Milky Way, or the Galaxy, as it has been called, has great interest
for astronomers. Many have been the attempts made to discover its
actual size, its real shape, how many stars it contains, how far
it extends; but to all such questions the only safe answers to be
returned are fenced around with “perhaps” and “may be.” There are many
very remarkable clusters of stars to be seen in the heavens--some
few visible as faint spots of light to the naked eye, though the
greater number are only to be seen through a telescope. Either with
the naked eye, or in telescopes of varying power, they show first as
mere glimmers of light, which, viewed with a more powerful telescope,
separate into clusters of distant stars.
[Illustration: A CLUSTER OF STARS IN CENTAURUS.]
The most common shape of these clusters is globular--to the eye
appearing simply round. Stars gather densely near the center, and
gradually open out to a thin scattering about the edge. Thousands of
suns are often thus collected into one cluster.
The clusters are to be seen in all parts of the sky; but the greater
number seem to be gathered into the space covered by the Milky Way and
by the famous south Magellanic Clouds.
Some of them are beautifully colored; as, for instance, a cluster in
Toucan, not visible from England, the center of which is rose-colored,
bordered with white. No doubt it contains a large number of bright red
suns, surrounded by a scattering of white suns.
Public-domain text, read in full here on John Shaqi.
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