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
Perhaps you have never reflected upon all the reasons, why the several
changes of position, with respect to the horizon, which the sun
undergoes in the course of the year, occasion such a difference in the
amount of heat received from him. Two causes contribute to increase the
heat of Summer and the cold of Winter. The higher the sun ascends above
the horizon, the more directly his rays fall upon the earth; and their
heating power is rapidly augmented, as they approach a perpendicular
direction. When the sun is nearly over head, his rays strike us with far
greater force than when they meet us obliquely; and the earth absorbs a
far greater number of those rays of heat which strike it
perpendicularly, than of those which meet it in a slanting direction.
When the sun is near the horizon, his rays merely glance along the
ground, and many of them, before they reach it, are absorbed and
dispersed in passing through the atmosphere. Those who have felt only
the oblique solar rays, as they fall upon objects in the high latitudes,
have a very inadequate idea of the power of a vertical, noonday sun, as
felt in the region of the equator.
The increased length of the day in Summer is another cause of the heat
of this season of the year. This cause more sensibly affects places far
removed from the equator, because at such places the days are longer and
the nights shorter than in the torrid zone. By the operation of this
cause, the solar heat accumulates there so much, during the longest days
of Summer, that the temperature rises to a higher degree than is often
known in the torrid climates.
Public-domain text, read in full here on John Shaqi.
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