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
If Mars stood still while the earth went round the sun, then a second
opposition, as at A, would occur at the end of one year from the first;
but, while the earth is performing this circuit, Mars is also moving the
same way, more than half as fast; so that, when the earth returns to A,
the planet has already performed more than half the same circuit, and
will have completed its whole revolution before the earth comes up with
it. Indeed Mars, after having been seen once in opposition, does not
come into opposition again until after two years and fifty days. And
since the planet is then comparatively near to us, as at M, while the
earth is at A, and appears very large and bright, rising unexpectedly
about the time the sun sets, he surprises the world as though it were
some new celestial body. But on account of the slow progress of Saturn
and Uranus, we find, after having performed one circuit around the sun,
that they are but little advanced beyond where we left them at the last
opposition. The time between one opposition of Saturn and another is
only a year and thirteen days.
It appears, therefore, that the superior planets steadily pursue their
course around the sun, but that their apparent retrograde motion, when
in opposition, is occasioned by our passing by them with a swifter
motion, of which we are unconscious, like the apparent backward motion
of a vessel, when we overtake it and pass by it rapidly in a steam-boat.
Such are the real and the apparent motions of the planets. Let us now
turn our attention to the _laws of the planetary orbits_.
There are three great principles, according to which the motions of the
earth and all the planets around the sun are regulated, called KEPLER'S
LAWS, having been first discovered by the astronomer whose name they
bear. They may appear to you, at first, dry and obscure; yet they will
be easily understood from the explanations which follow; and so
important have they proved in astronomical inquiries, that they have
acquired for their renowned discoverer the appellation of the
'_Legislator of the Skies_.' We will consider each of these laws
separately; and, for the sake of rendering the explanation clear and
intelligible, I shall perhaps repeat some things that have been briefly
mentioned before.
[Illustration Fig. 63.]
Public-domain text, read in full here on John Shaqi.
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