To calculate the wavelength of the second spectral line in the Lyman series, we employ the Rydberg formula for hydrogen. The Lyman series involves electron transitions to the n=1 energy level from higher levels (n=2, n=3, etc.).
The Rydberg formula for spectral line wavelength \( \lambda \) in hydrogen is:
\(\frac{1}{\lambda} = R \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)\)
Where:
The first line of the Lyman series results from a transition from \(n_2 = 2\) to \(n_1 = 1\). Its wavelength \( \lambda \) is calculated as:
\(\frac{1}{\lambda} = R \left( \frac{1}{1^2} - \frac{1}{2^2} \right) = R \left( 1 - \frac{1}{4} \right) = R \cdot \frac{3}{4}\)
The second line of the Lyman series originates from a transition from \(n_2 = 3\) to \(n_1 = 1\). Its wavelength is denoted \( \lambda_2 \) and given by:
\(\frac{1}{\lambda_2} = R \left( \frac{1}{1^2} - \frac{1}{3^2} \right) = R \left( 1 - \frac{1}{9} \right) = R \cdot \frac{8}{9}\)
To relate \( \lambda \) and \( \lambda_2 \), we divide the equation for \( \lambda \) by the equation for \( \lambda_2 \):
\(\frac{\frac{1}{\lambda}}{\frac{1}{\lambda_2}} = \frac{R \cdot \frac{3}{4}}{R \cdot \frac{8}{9}}\)
This simplifies to:
\(\frac{\lambda_2}{\lambda} = \frac{\frac{8}{9}}{\frac{3}{4}} = \frac{8}{9} \times \frac{4}{3} = \frac{32}{27}\)
Therefore, the wavelength of the second member, \( \lambda_2 \), is:
\(\lambda_2 = \frac{27}{32} \lambda\)
The result is: \( \frac{27}{32} \lambda \).