The Heavens Above: A Popular Handbook of AstronomyRolfe, W. J. (William James)
Science
The Heavens Above: A Popular Handbook of Astronomy
Rolfe, W. J. (William James)
Astronomy
The equality of days and nights when the sun is on the celestial
equator is also evident from the following considerations: one-half
of the earth is in sunshine all of the time; when the sun is on the
celestial equator, it is directly over the equator of the earth, and
the illumination extends from pole to pole, as is evident from Figs.
70 and 71, in the former of which the sun is represented as on the
eastern horizon at a place along the central line of the figure, and
in the latter as on the meridian along the same line. In each
diagram it is seen that the illumination extends from pole to pole:
hence, as the earth rotates on its axis, every place on the surface
will be in the sunshine and out of it just half of the time.
61. _Day and Night when the Sun is at the Summer Solstice._--When the
sun is at the summer solstice, it will be 23-1/2° north of the celestial
equator. The diurnal circle described by the sun will then be 23-1/2°
north of the celestial equator; and more than half of this diurnal
circle will be above the horizon at all places north of the equator, and
less than half of it at places south of the equator: hence _the days
will be longer than the nights at places north of the equator, and
shorter than the nights at places south of the equator_. At places
within 23-1/2° of the north pole, the entire diurnal circle described by
the sun will be above the horizon, so that the sun will not set. At
places within 23-1/2° of the south pole of the earth, the entire diurnal
circle will be below the horizon, so that the sun will not rise.
[Illustration: Fig. 72.]
[Illustration: Fig. 73.]
The illumination of the earth at this time is shown in Figs. 72 and
73. In Fig. 72 the sun is represented as on the western horizon
along the middle line of the figure, and in Fig. 73 as on the
meridian. It is seen at once that the illumination extends 23-1/2°
beyond the north pole, and falls 23-1/2° short of the south pole. As
the earth rotates on its axis, places near the north pole will be in
the sunshine all the time, while places near the south pole will be
out of the sunshine all the time. All places north of the equator
will be in the sunshine longer than they are out of it, while all
places south of the equator will be out of the sunshine longer than
they are in it.
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