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Rydberg formula
The Rydberg formula is used in atomic, molecular, and optical physics for determining the full spectrum of light emission from hydrogen, later extended to be useful with any element.
A piece of the original document detailing the Rydberg formula in 1888.
The spectrum are the wavelengths of photons emitted when electrons jump between discrete energy levels, "shells" around the atom of a certain chemical element.
The fomula was invented by the Swedish physicist Janne Rydberg and presented on November 5, 1888.
Rydberg formula for hydrogen
Where
By setting n1 to 1 and letting n2 run from 2 to infinity, the spectral lines known as the Lyman series converging to 91nm are obtained, in the same manner:
n1
n2
Name
Converge toward
1
Lyman series
91nm
2
Balmer series
365nm
3
Paschen series
821nm
Rydberg formula for any element
The formula above can be extended for use with any chemical element.
Where
The above article is adapted from from Wikipedia All Wikipedia article text is available under the terms of the GNU Free Documentation License
Updates and comments at Essential Facts blog
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