Recreations in Astronomy: With Directions for Practical Experiments and Telescopic WorkWarren, Henry White
Religion
Recreations in Astronomy: With Directions for Practical Experiments and Telescopic Work
Warren, Henry White
Astronomy
The subject becomes clearer by a study of the chromolithic plate.
No. 1 represents the solar spectrum, with a few of its lines on an
accurately graduated scale. [Page 51] No.3 shows the bright line of
glowing sodium, and, corresponding to a dark line in the solar
spectrum, shows the presence of salt in that body. No. 2 shows that
potassium has some violet rays, but not all; and there being no dark
line to correspond in the solar spectrum, we infer its absence from
the sun. No.6 shows the numerous lines and bands of barium--several
red, orange, yellow, and four are very bright green ones. The lines
given by any volatilized substances are always in the same place on
the scale.
A patient study of these signs of substances reveals, richer results
than a study of the cuniform characters engraved on Assyrian slabs;
for one is the handwriting of men, the other the handwriting of
God.
One of the most difficult and delicate problems solved by the
spectroscope is the approach or departure of a light-giving body
in the line of sight. Stand before a locomotive a mile away, you
cannot tell whether it approaches or recedes, yet it will dash by
in a minute. How can the movements of the stars be comprehended
when they are at such an immeasurable distance?
It can best be illustrated by music. The note C of the G clef is
made by two hundred and fifty-seven vibrations of air per second.
Twice as many vibrations per second would give us the note C an octave
above. Sound travels at the rate of three hundred and sixty-four
yards per second. If the source of these two hundred and fifty-seven
vibrations could approach us at three hundred and sixty-four yards
per second, it is obvious that twice as many waves would be put
into a given space, and we should hear the upper C when only waves
enough were made for the lower C. The same [Page 52] result would
appear if we carried our ear toward the sound fast enough to take up
twice as many valves as though we stood still. This is apparent to
every observer in a railway train. The whistle of an approaching
locomotive gives one tone; it passes, and we instantly detect
another. Let two trains, running at a speed of thirty-six yards a
second, approach each other. Let the whistle of one sound the note
E, three hundred and twenty-three vibrations per second. It will be
heard on the other as the note G, three hundred and eighty-eight
vibrations per second; for the speed of each train crowds the
vibrations into one-tenth less room, adding 32+ vibrations per
second, making three hundred and eighty-eight in all. The trains
pass. The vibrations are put into one-tenth more space by the
whistle making them, and the other train allows only nine-tenths of
what there are to overtake the ear. Each subtracts 32+ vibrations
from three hundred and twenty-three, leaving only two hundred and
fifty-eight, which is the note C. Yet the note E was constantly
uttered.
Public-domain text, read in full here on John Shaqi.
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