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
Saturn was a sore puzzle to the early telescopic observers. They did not
for a long time grasp the fact that it was surrounded by a ring--so slow
is the human mind to seek for explanations out of the ordinary course of
things. The protrusions of the ring on either side of the planet, at
first looked to Galileo like two minor globes placed on opposite sides
of it, and slightly overlapping the disc. He therefore informed Kepler
that "Saturn consists of three stars in contact with one another." Yet
he was genuinely puzzled by the fact that the two attendant bodies (as
he thought them) always retained the same position with regard to the
planet's disc, and did not appear to revolve around it, nor to be in any
wise shifted as a consequence of the movements of our earth.
About a year and a half elapsed before he again examined Saturn; and, if
he was previously puzzled, he was now thoroughly amazed. It happened
just then to be one of those periods when the ring is edgewise towards
the earth, and of course he only saw a round disc like that of Jupiter.
What, indeed, had become of the attendant orbs? Was some demon mocking
him? Had Saturn devoured his own children? He was, however, fated to be
still more puzzled, for soon the minor orbs reappeared, and, becoming
larger and larger as time went on, they ended by losing their globular
appearance and became like two pairs of arms clasping the planet from
each side! (see Plate XVI., p. 242).
Galileo went to his grave with the riddle still unsolved, and it
remained for the famous Dutch astronomer, Huyghens, to clear up the
matter. It was, however, some little time before he hit upon the real
explanation. Having noticed that there were dark spaces between the
strange appendages and the body of the planet, he imagined Saturn to be
a globe fitted with handles at each side; "ansæ" these came to be
called, from the Latin _ansa_, which means a handle. At length, in the
year 1656, he solved the problem, and this he did by means of that
123-foot tubeless telescope, of which mention has already been made. The
ring happened then to be at its edgewise period, and a careful study of
the behaviour of the ansæ when disappearing and reappearing soon
revealed to Huyghens the true explanation.
[Illustration: PLATE XVI. EARLY REPRESENTATIONS OF SATURN
From an illustration in the _Systema Saturnium_ of Christian Huyghens.
(Page 242)]
THE PLANETS URANUS AND NEPTUNE
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