Balmer spectral lines of hydrogen


Assignment:

Calculate the visible lines that should be seen with a spectroscope. This must correspond to lines in which the final bound energy level is N = 2.

Then, compare the observed lines to the ones that I calculate. 
The observed, recorded wave length lines were:

RED = 650 nanometers
TURQUOISE = 490 nanometers
VIOLET 1  = 435 nanometers
VIOLET 2  = 405 nanometers

(The lines above were observed by looking at the line spectra from hydrogen gas being placed in an electrical discharge tube.)

The energy of an electron bound to a proton for the Hydrogen atom as a function of energy level number N is given by:
E (N) = -13.6 / N2

Where E(N) is given in electron volts (eV).  And that one eV = 1.6 * 10-19 Joules.  This energy is negative indicating that the electron is bound to the proton by at least 13.6 eV when N = 1, and that this is the most the electron can be bound by.

Einstein proved that the energy of the photon is related to it’s frequency with:
E = h f

Where h = Planck’s constant of (6.63 * 10-34 J.sec) or (4.135 * 10-15 eV) and f is the frequency of the light being given off.

The first excited state (n=2) of the hydrogen atom has an energy of –(13.6/22) eV, or -3.40 eV.

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Physics: Balmer spectral lines of hydrogen
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