The Story of the Solar SystemChambers, George F. (George Frederick)
Science
The Story of the Solar System
Chambers, George F. (George Frederick)
Solar system
If the movements of an inferior planet are followed sufficiently long by
the aid of a star map, it will be seen that sometimes it appears to be
proceeding in a forward direction through the signs of the zodiac; then
for a while it will seem to stand still; then at another time it will
apparently go backwards, or possess a retrograde motion. All these
peculiarities have their originating cause in the motion of the Earth
itself, for the absolute movement of the planet never varies, being
always in the same direction, that is, forwards in the order of the
signs.
Turning now to the superior planets, we have to face an altogether
different succession of circumstances. A superior planet is not, as it
were, chained to the Sun so as to be unable to escape beyond the limits
of morning or evening twilight; it may have any angular distance from
the Sun up to 180°, reaching which point it approaches the Sun on the
opposite side, step by step, until it again comes into conjunction with
the Sun. As applied to a superior planet, the term “conjunction” means
the absolute moment when the Earth and the Sun and the planet are in the
same straight line, the Sun being in the middle. In such a case, to us
on the Earth the planet is lost in the Sun’s rays, whilst to a spectator
on the planet the Earth would appear similarly lost in the Sun’s rays,
as the Earth would be at that stage of her orbit which we, speaking of
_our_ inferior planets, call superior conjunction.
For a clear comprehension of all the various matters which we have just
been speaking of, a careful study of diagrams of a geometrical
character, or better still, of models, would be necessary.
Something must now be said about the phases of the planets. Mercury and
Venus, in regard to their orbital motions, stand very much on the same
footing with respect to the inhabitants of the Earth as the Moon does,
and accordingly both those planets in their periodical circuits round
the Sun exhibit the same succession of phases as the Moon does. In the
case, however, of the superior planets things are otherwise. Two only of
them, Mars and Jupiter, are sufficiently near the Earth to exhibit any
phase at all. When they are in quadrature (_i. e._, 90° from the Sun on
either side) there is a slight loss of light to be noticed along one
limb. In other words, the disc of each ceases for a short time, and to a
slight extent, to be truly circular; it becomes what is known as
“gibbous.” This occasional feature of Mars may be fairly conspicuous,
or, at least, noticeable; but in the case of Jupiter it will be less
obvious unless a telescope of some size is employed.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account