You would have to count pretty quickly to do this for light, however.
Light waves vibrate or oscillate at the rate of some 400 million million
times a second. That’s the vibration rate of waves of red light; violet
results from vibrations that are just about twice that fast.
With frequencies of this magnitude, discussion and handling of data and
dimensions are cumbersome and rather awkward. Fortunately there is
another approach. Let’s look again at our ocean waves. We see that there
is a regularity about them (before they begin to break on the shore).
The distance from one crest to the next is significant and is called the
_wavelength_. Water waves are measured in feet, and in comparable units
light waves are recorded in ten-millionths of an inch—again a very
cumbersome number. Scientists therefore use the metric system[2] and
have standardized a unit called the angstrom[3], which is equal to the
one-hundred-millionth part of a centimeter (10⁻⁸ cm). Thus we find, as
shown in Figure 3, that the visible light range runs from the violet at
about 4000 angstroms to red at about 7000 angstroms.
[Illustration: Figure 3 _The visible light spectrum ranges between
approximately 4000 and 7000 angstroms._]
Wavelength
(Angstroms)
Violet 4000-4300
Blue 4300-5000
Green 5000-5600
Yellow 5600-5800
Orange 5800-6100
Red 6100-7000
At roughly the same time that the wavelength of light was being
determined, the German-British astronomer William Herschel performed an
interesting experiment. He held a thermometer in turn in the various
colors of light that had been spread out by an optical prism. As he
moved the thermometer from the violet to the red, the temperature
reading rose—and it continued to rise as he moved the instrument
_beyond_ the red area, where no prismatic light could be seen.
Thus Herschel discovered infrared rays (the kind of heat we get from the
sun) adjoining the visible red light, and at the same time found that
they were merely a continuation of the visible spectrum. Shortly
thereafter, ultraviolet rays were found on the other end of the visible
light band.
Public-domain text, read in full here on John Shaqi.
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