The story of the sun, moon, and starsGiberne, Agnes
Science
The story of the sun, moon, and stars
Giberne, Agnes
Astronomy -- Juvenile literature
Some of the chief and more distinct lines were named by Fraunhofer
after certain letters of the alphabet, and by those letter-names they
are still known. He began with A in the red and went on to H in the
violet. Fraunhofer made a great many experiments connected with these
mysterious lines, anxious to discover, if possible, their meaning. For
although he now saw the lines, which had scarcely so much as been seen
before, he could not understand them--he could not read what they said.
They spoke to him, indeed, about the sun; but they spoke in a foreign
language, the key to which he did not possess. He tried making use of
prisms of different materials, thinking that perhaps the lines might be
due to something in the nature of the prism employed. But let the prism
be what it might, he found the lines still there. Then he examined
the light which shines from bright clouds, instead of capturing a ray
direct from the sun. And he found the lines still there. For cloudlight
is merely reflected sunlight.
Then he examined the light of the moon, to see if perchance the
spectrum might be clear of breaks. And he found the lines still
there. For moonlight is only reflected sunlight. Next he set himself
to examine the light which travels to us from some of the planets,
imagining that a different result might follow. And he found the lines
still there. For planet-light again is no more than reflected sunlight.
[Illustration: SPECTRA, SHOWING THE DARK LINES.]
Lastly, he turned his attention to some of the brighter stars,
examining, one by one, the ray which came from each. And, behold! he
found the lines _not_ there. For starlight is not reflected sunlight.
That is to say, the identical lines which distinguish sunlight were
not there. Each star had a spectrum as the sun has a spectrum, and
each star-spectrum was crossed by faint dark lines, more or less in
number. But the spectra of the stars differed from the spectrum of the
sun. Each particular star had its own particular spectrum of light,
different from that of the sun, and different from that of every other
star. For now, Fraunhofer was examining, not sunlight, but starlight;
not the light of our sun, either direct from himself or reflected from
some other body, such as planet or moon or cloud, but the light of
other suns very far distant, each one varying to some extent from the
rest in its make. The fact of the stars showing numerous sets of black
lines, all unlike those of our sun, showed conclusively that those
lines could not possibly be due to anything in our earthly atmosphere.
Sunlight and starlight travel equally through the air, and are equally
affected by it. If our atmosphere were the cause of the black lines in
sunlight, it would cause the _same_ lines in starlight. But the sun and
each individual star has its own individual lines, quite irrespective
of changeful states of the air.
Public-domain text, read in full here on John Shaqi.
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