The story of the sun, moon, and starsGiberne, Agnes
Science
The story of the sun, moon, and stars
Giberne, Agnes
Astronomy -- Juvenile literature
William Herschel proposed the name of _Georgium Sidus_ “the Star of
George,” just as Galileo had given the name of “Medicean stars” to
the satellites of Jupiter discovered by him, and as Horace had said
_Julium Sidus_. Others proposed the name of _Neptune_, in order to
maintain the mythological character, and to give to the new body the
trident of the English maritime power; others, _Uranus_, the most
ancient deity of all, and the father of Saturn, to whom reparation
was due for so many centuries of neglect. Lalande proposed the name
of _Herschel_, to immortalize the name of its discoverer. These last
two denominations prevailed. For a long time the planet bore the
name of Herschel; but custom has since declared for the mythological
appellation, and Jupiter, Saturn, and Uranus succeed each other in
order of descent--son, father, and grandfather.
The discovery of Uranus extended the radius of the Solar System from
885,000,000 to 1,765,000,000 of miles.
The apparent brightness of this planet is that of a star of the
sixth magnitude; observers whose sight is very piercing may succeed
in recognizing it with the naked eye when they know where to look for
it. Uranus moves slowly from west to east, and takes no less than
eighty-four years to make the complete circuit of the sky. In its
annual motion round the sun the earth passes between the sun and Uranus
every 369 days--that is to say, once in a year and four days. It is at
these times that this planet crosses the meridian at midnight. We can
observe it in the evening sky for about six months of every year.
Everybody supposed that now, at least, the outermost member of all was
discovered. But a very strange and remarkable thing happened.
Astronomers know with great exactness the paths of the planets in
the heavens. They can tell, years beforehand, precisely what spot in
space will be filled at any particular time by any particular planet.
I am speaking now of their movements round the sun and in the Solar
System--not of the movements of the whole family with the sun, about
which little is yet known.
Each planet has its own particular pathway; its own particular distance
from the sun, varying at each part of its pathway; its own particular
speed in traveling round the sun, changing constantly from faster to
slower or slower to faster, according to its distance from the sun, and
according to the pull backwards or forwards of our neighboring planets
in front or in rear. For as the orbits of all the planets are ovals,
with the sun not in the middle, but somewhat to one side of the middle,
it follows that all the planets, in the course of their years, are
sometimes nearer to and sometimes farther from the sun.
Public-domain text, read in full here on John Shaqi.
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