Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
If the axis of the earth stood "straight up," so to speak, while the
earth revolved in its orbit, the sun would plainly keep always on a
level with the equator. This is equivalent to stating that, in such
circumstances, a person at the equator would see it rise each morning
exactly in the east, pass through the _zenith_, that is, the point
directly overhead of him, at midday, and set in the evening due in the
west. As this would go on unchangingly at the equator every day
throughout the year, it should be clear that, at any particular place
upon the earth, the sun would in these conditions always be seen to move
in an unvarying manner across the sky at a certain altitude depending
upon the latitude of the place. Thus the more north one went upon the
earth's surface, the more southerly in the sky would the sun's path lie;
while at the north pole itself, the sun would always run round and round
the horizon. Similarly, the more south one went from the equator the
more northerly would the path of the sun lie, while at the south pole it
would be seen to skirt the horizon in the same manner as at the north
pole. The result of such an arrangement would be, that each place upon
the earth would always have one unvarying climate; in which case there
would not exist any of those beneficial changes of season to which we
owe so much.
The changes of season, which we fortunately experience, are due,
however, to the fact that the sun does not appear to move across the sky
each day at one unvarying altitude, but is continually altering the
position of its path; so that at one period of the year it passes across
the sky low down, and remains above the horizon for a short time only,
while at another it moves high up across the heavens, and is above the
horizon for a much longer time. Actually, the sun seems little by little
to creep up the sky during one half of the year, namely, from mid-winter
to mid-summer, and then, just as gradually, to slip down it again during
the other half, namely, from mid-summer to mid-winter. It will therefore
be clear that every region of the earth is much more thoroughly warmed
during one portion of the year than during another, _i.e._ when the
sun's path is high in the heavens than when it is low down.
Once more we find appearances exactly the contrary from the truth. The
earth is in this case the real cause of the deception, just as it was in
the other cases. The sun does not actually creep slowly up the sky, and
then slowly dip down it again, but, owing to the earth's axis being set
aslant, different regions of the earth's surface are presented to the
sun at different times. Thus, in one portion of its orbit, the northerly
regions of the earth are presented to the sun, and in the other portion
the southerly. It follows of course from this, that when it is summer in
the northern hemisphere it is winter in the southern, and _vice versâ_
(see Fig. 13, p. 176).
[Illustration: FIG. 13.--Summer and Winter.]
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.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account