Wonders of physical scienceFournier d'Albe, E. E. (Edmund Edward)
General
Wonders of physical science
Fournier d'Albe, E. E. (Edmund Edward)
Physics -- Juvenile literature
But although the great men of Europe used the telescope on many
occasions both in peace and in war, Galileo put it to a greater use.
He conceived the idea of turning it to the heavens and examining the
celestial bodies. In doing so he obtained a most surprising series of
revelations. He first of all turned it on the moon, and saw at once
that the markings on the surface of the moon were really mountains and
level plains. He could watch the shadows of the mountains grow and
diminish with the varying direction of the sun’s rays, and he could
even prove that some of the mountains were higher than others. He then
turned his telescope on the great planet Jupiter, and noticed to his
great surprise that Jupiter had near it four smaller companions which
circled round it in a few days. In fact, he found that Jupiter has four
moons where the earth has only one. This discovery was entirely opposed
to the ancient idea, then universally held, that there were only seven
planets or moving stars, namely: the Sun, the Moon, Mercury, Venus,
Mars, Jupiter, and Saturn.
On pointing the telescope to another great planet, Saturn, Galileo
found that another surprise awaited him. It looked as if the planet had
two handles, like a jug. This strange appearance was really owing to
the fact that Saturn is surrounded by a fiat ring, which being slightly
tilted gave the appearance of the two handles. This, of course, was
not known at that time to Galileo, but he certainly was the first to
observe that Saturn had a very unusual appearance.
[Illustration: Fig. 27.--The Planet Saturn and its Rings.]
Galileo next turned his telescope on the sun at a time when it was near
the horizon, and not strong enough to blind him. He observed that the
sun was not evenly bright all over its surface, but that there were
spots on it. These spots came and went, and could be seen to appear
at one edge of the sun, to move round, and to disappear at the other
edge about a fortnight later. This gave Galileo the idea that the sun
revolves on its axis.
After that, Galileo turned his attention to the planet Venus, and
found, contrary to all accepted opinions, that this glorious planet
showed phases like the moon, and was sometimes seen in the shape of a
crescent. Such appearances were not presented by Jupiter or Saturn, and
it struck Galileo that the probable explanation of this must be that
Venus revolves round the sun at a lesser distance than the earth, and
the other planets at a greater distance.
[Illustration: Fig. 28.--Photograph of the Sun on two successive days,
showing Sun-Spots and the Rotation of the Sun.]
Public-domain text, read in full here on John Shaqi.
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