The Balmer series and the Lyman series are two of the spectral line series for the hydrogen atom, described by the Rydberg formula:
\(\frac{1}{\lambda} = R \left(\frac{1}{n_1^2} - \frac{1}{n_2^2}\right)\)
where:
For the Lyman series, \(n_1 = 1\) and for the Balmer series, \(n_1 = 2\).
The "last line" refers to the transition approaching the shortest wavelength (highest energy transition possible). For the Balmer series, this is when \(n_2 = \infty\), and for the Lyman series, \(n_2 = \infty\).
1. Last line of Balmer series:
Using \(n_1 = 2\) and \(n_2 = \infty\),
\(\frac{1}{\lambda_{\text{Balmer}}} = R \left(\frac{1}{2^2} - \frac{1}{\infty}\right) = R \left(\frac{1}{4}\right)\)
Thus, \(\lambda_{\text{Balmer}} = \frac{4}{R}\)
2. Last line of Lyman series:
Using \(n_1 = 1\) and \(n_2 = \infty\),
\(\frac{1}{\lambda_{\text{Lyman}}} = R \left(\frac{1}{1^2} - \frac{1}{\infty}\right) = R\)
Thus, \(\lambda_{\text{Lyman}} = \frac{1}{R}\)
The ratio of the wavelengths of the last line of Balmer series to the last line of Lyman series can be calculated as:
\(\frac{\lambda_{\text{Balmer}}}{\lambda_{\text{Lyman}}} = \frac{\frac{4}{R}}{\frac{1}{R}} = 4\)
Thus, the correct answer is 4.