Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
Or in lieu of this, let us attempt to get in mind a picture of the solar
system by means of Sir William Herschel's apt illustration: "Choose any
well-leveled field. On it place a globe two feet in diameter. This will
represent the sun; Mercury will be represented by a grain of mustard
seed on the circumference of a circle 164 feet in diameter for its
orbit; Venus, a pea on a circle of 284 feet in diameter; the Earth also
a pea, on a circle of 430 feet; Mars a rather larger pin's head on a
circle of 654 feet; the asteroids, grains of sand in orbits of 1,000 to
1,200 feet; Jupiter, a moderate sized orange in a circle of nearly half
a mile across; Saturn, a small orange on a circle of four-fifths of a
mile; Uranus, a full-sized cherry or small plum upon the circumference
of a circle more than a mile and a half; and finally Neptune, a
good-sized plum on a circle about two miles and a half in diameter....
To imitate the motions of the planets in the above mentioned orbits,
Mercury must describe its own diameter in 41 seconds; Venus in 4
minutes, 14 seconds; the Earth in 7 minutes; Mars in 4 minutes 48
seconds; Jupiter in 2 minutes 56 seconds; Saturn in 3 minutes 13
seconds; Uranus in 2 minutes 16 seconds; and Neptune in 3 minutes 30
seconds."
Now, let us look earthward from our imaginary station near the north
pole of the ecliptic. All these planetary bodies would be seen to be
traveling eastward round the sun, that is, in a counter-clockwise
direction, or contrary to the motions of the hands of a timepiece. Their
orbits or paths of motion are very nearly circular, and the sun is
practically at the center of all of them except Mercury and Mars; of
Venus and Neptune, almost at the absolute center. The planes of all
their orbits are very nearly the same as that of the ecliptic, or plane
in which the earth moves. These and many other resemblances and
characteristics suggest a uniformity of origin which comports with the
idea of a family, and so the whole is spoken of as the solar system, or
the sun and his family of planets.
Public-domain text, read in full here on John Shaqi.
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