The Balmer series in a hydrogen atom relates the possible electron transitions down to the n = 2 position to the wavelength of the emission that scientists observe. In quantum physics, when electrons transition between different energy levels around the atom (described by the principal quantum number, n) they either release or absorb a photon. The Balmer series describes the transitions from higher energy levels to the second energy level and the wavelengths of the emitted photons. You can calculate this using the Rydberg formula.
The Rydberg Formula and Balmer’s Formula
The Rydberg formula relates the wavelength of the observed emissions to the principle quantum numbers involved in the transition:
The λ symbol represents the wavelength, and RH is the Rydberg constant for hydrogen, with RH = 1.0968 × 107 m−1. You can use this formula for any transitions, not just the ones involving the second energy level.
The Balmer series just sets n1 = 2, which means the value of the principal quantum number (n) is two for the transitions being considered. Balmer’s formula can therefore be written:
Calculating a Balmer Series Wavelength
The first step in the calculation is to find the principle quantum number for the transition you’re considering. This simply means putting a numerical value on the “energy level” you’re considering. So the third energy level has n = 3, the fourth has n = 4 and so on. These go in the spot for n2 in the equations above.
Start by calculating the part of the equation in brackets:
All you need is the value for n2 you found in the previous section. For n2 = 4, you get:
Multiply the result from the previous section by the Rydberg constant, RH = 1.0968 × 107 m−1, to find a value for 1/λ. The formula and the example calculation gives:
Find the wavelength for the transition by dividing 1 by the result from the previous section. Because the Rydberg formula gives the reciprocal wavelength, you need to take the reciprocal of the result to find the wavelength.
So, continuing the example:
This matches the established wavelength emitted in this transition based on experiments.
About the Author
Lee Johnson is a freelance writer and science enthusiast, with a passion for distilling complex concepts into simple, digestible language. He's written about science for several websites including eHow UK and WiseGeek, mainly covering physics and astronomy. He was also a science blogger for Elements Behavioral Health's blog network for five years. He studied physics at the Open University and graduated in 2018.