Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent AstronomersOlmsted, Denison
Science
Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent Astronomers
Olmsted, Denison
Astronomy
URANUS.--Uranus is the remotest planet belonging to our system, and is
rarely visible, except to the telescope. Although his diameter is more
than four times that of the earth, being thirty-five thousand one
hundred and twelve miles, yet his distance from the sun is likewise
nineteen times as great as the earth's distance, or about eighteen
hundred millions of miles. His revolution around the sun occupies nearly
eighty-four years, so that his position in the heavens, for several
years in succession, is nearly stationary. His path lies very nearly in
the ecliptic, being inclined to it less than one degree. The sun
himself, when seen from Uranus dwindles almost to a star, subtending, as
it does, an angle of only one minute and forty seconds; so that the
surface of the sun would appear there four hundred times less than it
does to us. This planet was discovered by Sir William Herschel on the
thirteenth of March, 1781. His attention was attracted to it by the
largeness of its disk in the telescope; and finding that it shifted its
place among the stars, he at first took it for a comet, but soon
perceived that its orbit was not eccentric, like the orbits of comets,
but nearly circular, like those of the planets. It was then recognised
as a new member of the planetary system, a conclusion which has been
justified by all succeeding observations. It was named by the discoverer
the _George Star_, (Georgium Sidus,) after his munificent patron, George
the Third; in the United States, and in some other countries, it was
called _Herschel_; but the name _Uranus_, from a Greek word, (= Ouranos=,
_Ouranos_,) signifying the oldest of the gods, has finally prevailed. So
distant is Uranus from the sun, that light itself, which moves nearly
twelve millions of miles every minute, would require more than two hours
and a half to pass to it from the sun.
And now, having contemplated all the planets separately, just cast your
eyes on the diagram facing page 236, Fig. 53, and you will see a
comparative view of the various magnitudes of the sun, as seen from each
of the planets.
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