A Century's Progress in AstronomyMacpherson, Hector
History
A Century's Progress in Astronomy
Macpherson, Hector
Astronomy -- History
The eighth satellite, Japetus, was shown by Herschel to rotate on its
axis in a period equal to that of its revolution, and his observations
were confirmed by modern observers. “I cannot,” Herschel said, “help
reflecting with some pleasure on the discovery of an analogy which shows
that a certain uniform plan is carried on among the secondaries of our
Solar System; and we may conjecture that probably most of the satellites
are governed by the same law.” In April 1805 Herschel observed the globe
of Saturn to present not a spherical but a “square-shouldered” aspect.
It was for long believed that this was an optical illusion; but Proctor
and others have shown that it is quite possible for storms in Saturn’s
atmosphere to cause the planet’s apparent distortion in shape.
Herschel paid much attention to the planet Uranus, which he discovered
on March 13, 1781. The discovery of Uranus, which was mentioned in a
previous chapter, was in a sense the most striking of Herschel’s
achievements. Uranus was the first planet discovered within the memory
of man: besides, the discovery enlarged the diameter of the Solar System
from 886 to 1772 millions of miles. Throughout his lifetime Herschel
referred to the planet as the “Georgium Sidus,” out of gratitude to
George III. for appointing him King’s Astronomer; but the astronomers of
France and Germany, who, as Sir Robert Ball remarks, “saw no reason why
the King of England should be associated with Jupiter and Saturn,”
opposed this term. Lalande called the planet “Herschel,” but Herschel’s
countrymen, the Germans, named it Uranus, in keeping with the custom of
designating the planets from the Greek mythology. The name of Uranus
ultimately prevailed.
In January 1787 Herschel discovered two satellites to Uranus, with the
aid of his 20-foot telescope. These satellites he believed to revolve
round Uranus in 8 days and 13 days respectively, and accordingly he made
a drawing of what their positions should be on February 10. On that day
he found them in their predicted places. In 1797 he announced that the
satellites revolved round Uranus in orbits at right angles to the
ecliptic, and in a retrograde direction. In subsequent years Herschel
believed that he had discovered other four satellites to Uranus, but he
was unable to confirm his belief. As Mr Gore says, some of the
satellites “must, therefore, have been either optical ‘ghosts’ or else
small fixed stars which happened to be near the planet’s path at the
time of observation. Herschel also suspected that he could see traces of
rings round Uranus like those round Saturn, but his observation was
never confirmed, either by himself or other observers.”
Public-domain text, read in full here on John Shaqi.
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