Calculate the wavelengths of the Balmer series lines for hydrogen.

The Balmer series is formed by the set of lines obtained when electrons fall from orbits higher than the second orbit (n1 = 2; n2 = 3, 4, 5 ...).
The lines of this series are located in the visible spectrum.
The formula used to calculate the wavelengths of the Balmer series lines is shown in the text.
The Rydberg constant for hydrogen is 1.0967757 x 10^7 m^-1.