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
To the Arabians is due the credit of having kept alive the study of the
stars during the dark ages of European history. They erected some fine
observatories, notably in Spain and in the neighbourhood of Bagdad.
Following them, some of the Oriental peoples embraced the science in
earnest; Ulugh Beigh, grandson of the famous Tamerlane, founding, for
instance, a great observatory at Samarcand in Central Asia. The Mongol
emperors of India also established large astronomical instruments in the
chief cities of their empire. When the revival of learning took place in
the West, the Europeans came to the front once more in science, and
rapidly forged ahead of those who had so assiduously kept alight the
lamp of knowledge through the long centuries.
The dethronement of the older theories by the Copernican system, in
which the earth was relegated to its true place, was fortunately soon
followed by an invention of immense import, the invention of the
Telescope. It is to this instrument, indeed, that we are indebted for
our knowledge of the actual scale of the celestial distances. It
penetrated the depths of space; it brought the distant orbs so near,
that men could note the detail on the planets, or measure the small
changes in their positions in the sky which resulted from the movement
of our own globe.
It was in the year 1609 that the telescope was first constructed. A
year or so previous to this a spectacle-maker of Middleburgh in Holland,
one Hans Lippershey, had, it appears, hit upon the fact that distant
objects, when viewed through certain glass lenses suitably arranged,
looked nearer.[8] News of this discovery reached the ears of Galileo
Galilei, of Florence, the foremost philosopher of the day, and he at
once applied his great scientific attainments to the construction of an
instrument based upon this principle. The result was what was called an
"optick tube," which magnified distant objects some few times. It was
not much larger than what we nowadays contemptuously refer to as a
"spy-glass," yet its employment upon the leading celestial objects
instantly sent astronomical science onward with a bound. In rapid
succession Galileo announced world-moving discoveries; large spots upon
the face of the sun; crater-like mountains upon the moon; four
subordinate bodies, or satellites, circling around the planet Jupiter;
and a strange appearance in connection with Saturn, which later
telescopic observers found to be a broad flat ring encircling that
planet. And more important still, the magnified image of Venus showed
itself in the telescope at certain periods in crescent and other forms;
a result which Copernicus is said to have announced should of necessity
follow if his system were the true one.
Public-domain text, read in full here on John Shaqi.
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