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
The sun is the chief member of our system. It controls the motions of
the planets by its immense gravitative power. Besides this it is the
most important body in the entire universe, so far as we are concerned;
for it pours out continually that flood of light and heat, without which
life, as we know it, would quickly become extinct upon our globe.
Light and heat, though not precisely the same thing, may be regarded,
however, as next-door neighbours. The light rays are those which
directly affect the eye and are comprised in the visible spectrum. We
_feel_ the heat rays, the chief of which are beyond the red portion of
the spectrum. They may be investigated with the _bolometer_, an
instrument invented by the late Professor Langley. Chemical rays--for
instance, those radiations which affect the photographic plate--are for
the most part also outside the visible spectrum. They are, however, at
the other end of it, namely, beyond the violet.
Such a scale of radiations may be compared to the keyboard of an
imaginary piano, the sound from only one of whose octaves is audible to
us.
The brightest light we know on the earth is dull compared with the light
of the sun. It would, indeed, look quite dark if held up against it.
It is extremely difficult to arrive at a precise notion of the
temperature of the body of the sun. However, it is far in excess of any
temperature which we can obtain here, even in the most powerful electric
furnace.
A rough idea of the solar heat may be gathered from the calculation that
if the sun's surface were coated all over with a layer of ice 4000 feet
thick, it would melt through this completely in one hour.
The sun cannot be a hot body merely cooling; for the rate at which it is
at present giving off heat could not in such circumstances be kept up,
according to Professor Moulton, for more than 3000 years. Further, it is
not a mere burning mass, like a coal fire, for instance; as in that case
about a thousand years would show a certain drop in temperature. No
perceptible diminution of solar heat having taken place within historic
experience, so far as can be ascertained, we are driven to seek some
more abstruse explanation.
Public-domain text, read in full here on John Shaqi.
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