Spectra and Bohr's Atom

The emission spectra of hydrogen could be explained through the Bohr atomic model. Emission means that energy must be emitted or lost. Bohr proposed the spectral lines of elements were observed as a result of the electrons moving from higher energy states to lower energy states

The same spectral lines are always observed because the electrons are forced to these energy states that have fixed energies. Therefore, when an electron falls from a higher energy state to a lower energy state, there are a limited number of options to which the electron can fall . Each electron transition between different electron shells will cause a different wavelength of light to be emitted.

Notice in the diagram above that as the difference between electron shells becomes larger, more energy needs to be released in order for the electron to return to a lower energy state. This results in a more energetic wavelength of light to be released as the difference between the two shells increases. The total combination of all these different transitions will result in a unique emission spectrum for each element found in nature. 

Using his model and its corresponding equation to represent the energy of each shell, Bohr was able to predict the exact wavelengths of light observed in the hydrogen emission spectrum.