Beacon Lights of History, Volume 3 part 2: Renaissance and ReformationLord, John
History
Beacon Lights of History, Volume 3 part 2: Renaissance and Reformation
Lord, John
History
Having now reached the limit of discovery with his present
instrument, he makes another of still greater power, and points it
to the planet Jupiter. On the 7th of January, 1610, he observes
three little stars near the body of the planet, all in a straight
line and parallel to the ecliptic, two on the east and one on the
west of Jupiter. On the next observation he finds that they have
changed places, and are all on the west of Jupiter; and the next
time he observes them they have changed again. He also discovers
that there are four of these little stars revolving round the
planet. What is the explanation of this singular phenomenon? They
cannot be fixed stars, or planets; they must then be moons.
Jupiter is attended with satellites like the earth, but has four
instead of one! The importance of this last discovery was of
supreme value, for it confirmed the heliocentric theory. Old
Kepler is filled with agitations of joy; all the friends of Galileo
extol his genius; his fame spreads far and near; he is regarded as
the ablest scientific man in Europe.
His enemies are now dismayed and perplexed. The principal
professor of philosophy at Padua would not even look through the
wonderful instrument. Sissi of Florence ridicules the discovery.
"As," said he, "there are only seven apertures of the head,--two
eyes, two ears, two nostrils, and one mouth,--and as there are only
seven days in the week and seven metals, how can there be seven
planets?"
But science, discarded by the schools, fortunately finds a refuge
among princes. Cosimo de' Medici prefers the testimony of his
senses to the voice of authority. He observes the new satellites
with Galileo at Pisa, makes him a present of one thousand florins,
and gives him a mere nominal office,--that of lecturing
occasionally to princes, on a salary of one thousand florins for
life. He is now the chosen companion of the great, and the
admiration of Italy. He has rendered an immense service to
astronomy. "His discovery of the satellites of Jupiter," says
Herschel, "gave the holding turn to the opinion of mankind
respecting the Copernican system, and pointed out a connection
between speculative astronomy and practical utility."
But this did not complete the catalogue of his discoveries. In
1610 he perceived that Saturn appeared to be triple, and excited
the curiosity of astronomers by the publication of his first
"Enigma," Altissimam planetam tergeminam observavi. He could not
then perceive the rings; the planet seemed through his telescope to
have the form of three concentric O's. Soon after, in examining
Venus, he saw her in the form of a crescent: Cynthiae figuras
aemulatur mater amorum, "Venus rivals the phases of the moon."
At last he discovers the spots upon the sun's disk, and that they
all revolve with the sun, and therefore that the sun has a
revolution in about twenty-eight days, and may be moving on in a
larger circle, with all its attendant planets, around some distant
centre.
Public-domain text, read in full here on John Shaqi.
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