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<strong>Cosmic</strong> <strong>Game</strong> © Douglass A. White, 2012 v151207 162<br />
Since the sacred fire was kindled in the dark and hidden depths of the temple by the<br />
magical power of the Crystal Water Eye, it might also occur to the priest to repeat the<br />
process on a smaller scale. Once the sunbeam had passed and the fire was lit in the dark<br />
room, he might then place a canopy over the sacred glow of the natron and use the<br />
Crystal Eye to focus the captured light of Amen Ra a second time.<br />
This time he would not get a perfect rainbow. He might notice that within the rainbow<br />
some bars of various colors stood out more brightly, particularly a yellow bar. He would<br />
have discovered in a very limited way what we today call an optical spectrum. Unless he<br />
could view the spectrum of the burning natron in the state of a thin gas, he would not<br />
merely see the spectral lines, but would have a more spread out spectrum. However<br />
there would be a bright yellow bar part way across the spectrum.<br />
<strong>The</strong> sodium spectrum has bright lines at 589 nm. <strong>The</strong>re are actually two lines, one at<br />
588.995 nm and another at 589.5924 nm. <strong>The</strong> one closest to 589 nm is much brighter,<br />
and so the secondary line probably would not be noticed by the ancient Egyptians, or they<br />
may have seen them as one thicker line.<br />
Gustav Kirchhoff and Robert Bunsen identified many elements using optical<br />
spectroscopy aided by a specially designed burner developed by Bunsen.<br />
<strong>The</strong> Three Laws of Spectroscopy (from Wikipedia, "Kirchhoff" article)<br />
1. A hot solid object produces light with a continuous spectrum.<br />
2. A hot tenuous gas produces light with spectral lines at discrete wavelengths (i.e.<br />
specific colors) which depend on the energy levels of the atoms in the gas.<br />
3. A hot solid object surrounded by a cool tenuous gas (i.e. cooler than the hot<br />
object) produces light with an almost continuous spectrum which has gaps at discrete<br />
wavelengths depending on the energy levels of the atoms in the gas.<br />
Above is a drawing of the Kirchhoff-Bunsen spectroscope. <strong>The</strong> device does not make<br />
use of anything unknown to the Egyptians. It includes a box with a blackened interior, a<br />
triangular prism, tubes with lenses for directing and observing the light, a flame, and a<br />
material to study -- e.g., natron.