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DISCOVERING
THE
FINGERPRINTS OF THE ATOMS
That’s what teachers call the spectrum of the
light atoms emit. Go out after dark and explore the spectra of
distant night lights by holding a diffraction grating in front of
your eye. You’ll see mostly bands of color, but also some narrow
lines. These are direct evidence that atoms have sharp energy
levels as described by quantum mechanics.
Unfortunately, what used to be a simple night
time adventure just got harder, due to improvements in lamp
efficiency. Phosphors have been added to (low pressure Hg)
fluorescent lamps so that what you mostly see is bands of red,
green, blue, and violet colors.
Even the twisty “green” light bulbs are
fluorescent lamps. Low pressure sodium lamps are seldom used for
street lighting, leaving the distinctive yellow sodium lamps largely
to medical institutions. So today a big challenge is to find old
fashioned fluorescent lamps.
If you find an old fluorescent lamp, look
carefully at the yellow doublet whose wavelengths are 577 and
579nm. See whether your diffraction grating can resolve the double
lines in the yellow (577 & 579nm wavelength).
Modern street lighting is mostly pinkish-yellow
high pressure sodium. It’s true that you still see the distinctive
black (self absorption) line in the yellow region, but it’s far
broader than the low pressure doublet visible in low pressure sodium
lamps.
New light emitting diode (LED) flashlights are
easy to find, as are red (neon) lasers at checkout scanners in
libraries and super markets. Are their line-widths comparable?
New cars are full of LED lamps, some of which
blink rapidly. You can see them blinking by moving your eye
rapidly. Most car tail lights are filtered
incandescent light; others are red LED's. Can
you see the difference?
Check out sunlight and moonlight. (Starlight
is too faint without a telescope). What lights can you find around
your home? How many different spectra can you find?
Apart from its scientific interest, it’s still
thrilling to view from a distance the night lights of a city, or an
airport, or a harbor – through a diffraction grating.
References:
S.F. Jacobs “Night Spectra Quest”, The
Physics Teacher, 33, 380, (1995).
S.F. Jacobs, “Challenges of Everyday Spectra”,
J. Chem. Ed, 74, 1070, (1996).
Below is a chart that shows some spectra of night
lights.
b) Fluorescent
c) Mercury (low pressure)
d) Mercury (high pressure)
e) Metal halide
f) Sodium (high pressure)
g) Sodium (low pressure)
h) Neon sign (red)
i) Neon sign (other colors, using tinting &
phosphors)
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