Step 1: Recall the Balmer series formula.
The Balmer series describes electron transitions to the \(n = 2\) energy level from higher levels, specifically \(n \geq 3\). The formula for the reciprocal of the wavelength is: \[ \frac{1}{\lambda} = R_H \left( \frac{1}{2^2} - \frac{1}{n^2} \right) \] where \(R_H = 1.097 \times 10^7\, \text{m}^{-1}\) is the Rydberg constant.
Step 2: First line in Balmer series.
This transition is from \(n = 3\) to \(n = 2\). The reciprocal of the wavelength (\(\lambda_1\)) is: \[ \frac{1}{\lambda_1} = R_H \left( \frac{1}{4} - \frac{1}{9} \right) = R_H \left( \frac{5}{36} \right) \]
Step 3: Second line in Balmer series.
This transition is from \(n = 4\) to \(n = 2\). The reciprocal of the wavelength (\(\lambda_2\)) is: \[ \frac{1}{\lambda_2} = R_H \left( \frac{1}{4} - \frac{1}{16} \right) = R_H \left( \frac{3}{16} \right) \] The ratio of wavelengths is calculated as: \[ \frac{\lambda_2}{\lambda_1} = \frac{5/36}{3/16} = \frac{5 \cdot 16}{36 \cdot 3} = \frac{80}{108} = \frac{20}{27} \] Therefore, \(\lambda_2 = \frac{20}{27} \cdot 656 \approx 486\, \text{nm}\).