Popular lectures on scientific subjects : $b Second series, with an autobiography of the authorHelmholtz, Hermann von
Science
Popular lectures on scientific subjects : $b Second series, with an autobiography of the author
Helmholtz, Hermann von
Science; Universities and colleges -- Germany
All life and all motion on our earth is, with few exceptions, kept up
by a single force, that of the sun’s rays, which bring to us light
and heat. They warm the air of the hot zones, this becomes lighter
and ascends, while the colder air flows towards the poles. Thus is
formed the great circulation of the passage-winds. Local differences
of temperature over land and sea, plains and mountains, disturb the
uniformity of this great motion, and produce for us the capricious
change of winds. Warm aqueous vapours ascend with the warm air, become
condensed into clouds, and fall in the cooler zones, and upon the
snowy tops of the mountains, as rain and as snow. The water collects
in brooks, in rivers, moistens the plains, and makes life possible;
crumbles the stones, carries their fragments along, and thus works at
the geological transformation of the earth’s surface. It is only under
the influence of the sun’s rays that the variegated covering of plants
of the earth grows; and while they grow, they accumulate in their
structure organic matter, which partly serves the whole animal kingdom
as food, and serves man more particularly as fuel. Coals and lignites,
the sources of power of our steam engines, are remains of primitive
plants--the ancient production of the sun’s rays.
Need we wonder if, to our forefathers of the Aryan race in India and
Persia, the sun appeared as the fittest symbol of the Deity? They were
right in regarding it as the giver of all life--as the ultimate source
of almost all that has happened on earth.
But whence does the sun acquire this force? It radiates forth a more
intense light than can be attained with any terrestrial means. It
yields as much heat as if 1,500 pounds of coal were burned every hour
upon each square foot of its surface. Of the heat which thus issues
from it, the small fraction which enters our atmosphere furnishes
a great mechanical force. Every steam-engine teaches us that heat
can produce such force. The sun, in fact, drives on earth a kind
of steam-engine whose performances are far greater than those of
artificially constructed machines. The circulation of water in the
atmosphere raises, as has been said, the water evaporated from the
warm tropical seas to the mountain heights; it is, as it were, a
water-raising engine of the most magnificent kind, with whose power no
artificial machine can be even distantly compared. I have previously
explained the mechanical equivalent of heat. Calculated by that
standard, the work which the sun produces by its radiation is equal to
the constant exertion of 7,000 horse-power for each square foot of the
sun’s surface.
Public-domain text, read in full here on John Shaqi.
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