Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schools — John Shaqi
Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schoolsServiss, Garrett Putman
Science
Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schools
Serviss, Garrett Putman
Astronomy -- Juvenile literature
As it is very important to have a clear conception of this subject, we
may illustrate it in this way: Take a ball to represent the earth, and
around it draw a circle to represent the equator. Then, through the
centre of the ball, and at right angles to its equator, put a long pin
to represent the axis. Set it afloat in a tub of water, weighting it so
that it will be half submerged, and placing it in such a position that
the pin will be not upright but inclined at a considerable angle from
the vertical. Now, imagine that the sun is situated in the centre of the
tub, and cause the ball to circle slowly round it, while maintaining the
pin always in the same position. Then the surface of the water will
represent the plane of the ecliptic, or plane of the earth's orbit, and
you will see that, in consequence of the inclination of the pin, the
plane of the equator does not coincide with that of the ecliptic (or the
surface of the water), but is tipped with regard to it in such a manner
that one half of the equator is below and the other half above it.
Instead of actually trying this experiment, it will be a useful exercise
of the imagination to represent it to the mind's eye just as if it were
tried.
We have said that the inclination of the equator to the ecliptic amounts
to 23½°, and this angle should be memorised. Now, since both the
ecliptic and the equator are great circles of the celestial sphere, _i.
e._, circles whose planes cut through the centre of the sphere, they
must intersect one another at two opposite points. In the experiment
just described, these two points lie on opposite sides of the ball,
where the equator cuts the level of the water. These points of
intersection of the equator and the ecliptic on the celestial sphere are
called the equinoxes, or equinoctial points, because when the sun
appears at either of those points it is perpendicular over the equator,
and when it is in that position day and night are of equal length all
over the earth. (Equinox is from two Latin words meaning “equal night.”)
[Illustration:
=Saturn=
From a drawing by Trouvelot.
]
[Illustration:
=Saturn=
Photographed at the Lick Observatory.
]
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