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
Mercury and Venus are called _inferior_ planets, because they have their
orbits nearer to the sun than that of the earth; while all the others,
being more distant from the sun than the earth, are called _superior_
planets. The planets present great diversities among themselves, in
respect to distance from the sun, magnitude, time of revolution, and
density. They differ, also, in regard to satellites, of which, as we
have seen, three have respectively four, six, and seven, while more than
half have none at all. It will aid the memory, and render our view of
the planetary system more clear and comprehensive, if we classify, as
far as possible, the various particulars comprehended under the
foregoing heads. As you have had an opportunity, in preceding Letters,
of learning something respecting the means which astronomers have of
ascertaining the distances and magnitudes of these bodies, you will not
doubt that they are really as great as they are represented; but when
you attempt to conceive of spaces so vast, you will find the mind wholly
inadequate to the task. It is indeed but a comparatively small space
that we can fully comprehend at one grasp. Still, by continual and
repeated efforts, we may, from time to time, somewhat enlarge the
boundaries of our mental vision. Let us begin with some known and
familiar space, as the distance between two places we are accustomed to
traverse. Suppose this to be one hundred miles. Taking this as our
measure, let us apply it to some greater distance, as that across the
Atlantic Ocean,--say three thousand miles. From this step we may advance
to some faint conception of the diameter of the earth; and taking that
as a new measure, we may apply it to such greater spaces as the distance
of the planets from the sun. I hope you will make trial of this method
on the following comparative statements respecting the planets.
_Distances from the Sun, in miles._
1. Mercury, 37,000,000
2. Venus, 68,000,000
3. Earth, 95,000,000
4. Mars, 142,000,000
5. Vesta, 225,000,000
6. Juno, }
7. Ceres, } 261,000,000
8. Pallas, }
9. Jupiter, 485,000,000
10. Saturn, 890,000,000
11. Uranus, or Herschel, 1800,000,000
The _dimensions_ of the planetary system are seen from this table to be
vast, comprehending a circular space thirty-six hundred millions of
miles in diameter. A rail-way car, travelling constantly at the rate of
twenty miles an hour, would require more than twenty thousand years to
cross the orbit of Uranus.
_Magnitudes._
Diam. in miles.
1. Mercury, 3140
2. Venus, 7700
3. Earth, 7912
4. Mars, 4200
5. Ceres, 160
6. Jupiter, 89,000
7. Saturn, 79,000
8. Uranus, 35,000
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