Six Lectures on Light: Delivered In The United States In 1872-1873Tyndall, John
Science
Six Lectures on Light: Delivered In The United States In 1872-1873
Tyndall, John
Light
Firstly then you notice, when a fragment of sodium is placed in a
platinum spoon and introduced into a Bunsen's flame, an intensely
yellow light is produced. It corresponds in refrangibility with the
yellow band of the spectrum. Like our tuning-fork, it emits waves of a
special period. When the white light from the electric lamp is sent
through that flame, you will have ocular proof that the yellow flame
intercepts the yellow of the spectrum; in other words, that it absorbs
waves of the same period as its own, thus producing, to all intents
and purposes, a dark Fraunhofer's band in the place of the yellow.
In front of the slit (at L, fig. 56) through which the beam issues is
placed a Bunsen's burner (_b_) protected by a chimney (C). This beam,
after passing through a lens, traverses the prism (P) (in the real
experiment there was a pair of prisms), is there decomposed, and forms
a vivid continuous spectrum (S S) upon the screen. Introducing a
platinum spoon with its pellet of sodium into the Bunsen's flame, the
pellet first fuses, colours the flame intensely yellow, and at length
bursts into violent combustion. At the same moment the spectrum is
furrowed by an intensely dark band (D), two inches wide and two feet
long. Introducing and withdrawing the sodium flame in rapid
succession, the sudden appearance and disappearance of the band of
darkness is shown in a most striking manner. In contrast with the
adjacent brightness this band appears absolutely black, so vigorous is
the absorption. The blackness, however, is but relative, for upon the
dark space falls a portion of the light of the sodium flame.
[Illustration: Fig. 56.]
I have already referred to the experiment of Foucault; but other
workers also had been engaged on the borders of this subject before it
was taken up by Bunsen and Kirchhoff. With some modification I have on
a former occasion used the following words regarding the precursors of
the discovery of spectrum analysis, and solar chemistry:--'Mr. Talbot
had observed the bright lines in the spectra of coloured flames, and
both he and Sir John Herschel pointed out the possibility of making
prismatic analysis a chemical test of exceeding delicacy, though not
of entire certainty. More than a quarter of a century ago Dr. Miller
gave drawings and descriptions of the spectra of various coloured
flames. Wheatstone, with his accustomed acuteness, analyzed the light
of the electric spark, and proved that the metals between which the
spark passed determined the bright bands in its spectrum. In an
investigation described by Kirchhoff as "classical," Swan had shown
that 1/2,500,000 of a grain of sodium in a Bunsen's flame could be
detected by its spectrum. He also proved the constancy of the bright
lines in the spectra of hydrocarbon flames. Masson published a prize
essay on the bands of the induction spark; while Van der Willigen, and
more recently Plücker, have also given us beautiful drawings of
spectra obtained from the same source.
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