To determine the wavelength of the second member of the Lyman series, we need to understand the Lyman series and apply the Rydberg formula for hydrogen spectral lines. The Lyman series corresponds to electronic transitions where the electrons drop to the n=1 energy level from higher levels (n=2, n=3, etc.).
The Rydberg formula for calculating the wavelength \(\lambda\) of any transition in a hydrogen atom is given as:
\(\frac{1}{\lambda} = R \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)\)
Where:
The first member of the Lyman series corresponds to a transition from \(n_2 = 2\) to \(n_1 = 1\). Thus, the wavelength \(\lambda\) is given by:
\(\frac{1}{\lambda} = R \left( \frac{1}{1^2} - \frac{1}{2^2} \right) = R \left( 1 - \frac{1}{4} \right) = R \cdot \frac{3}{4}\)
The second member of the Lyman series involves a transition from \(n_2 = 3\) to \(n_1 = 1\):
\(\frac{1}{\lambda_2} = R \left( \frac{1}{1^2} - \frac{1}{3^2} \right) = R \left( 1 - \frac{1}{9} \right) = R \cdot \frac{8}{9}\)
To find the relationship between \(\lambda\) and \(\lambda_2\), we divide the first equation by the second:
\(\frac{\frac{1}{\lambda}}{\frac{1}{\lambda_2}} = \frac{R \cdot \frac{3}{4}}{R \cdot \frac{8}{9}}\)
Simplifying, we have:
\(\frac{\lambda_2}{\lambda} = \frac{\frac{8}{9}}{\frac{3}{4}} = \frac{8}{9} \times \frac{4}{3} = \frac{32}{27}\)
Thus, the wavelength of the second member \(\lambda_2\) is:
\(\lambda_2 = \frac{27}{32} \lambda\)
Therefore, the correct answer is: \(\frac{27}{32} \lambda\).
For the first member of the Lyman series:
\[ \frac{1}{\lambda} = \frac{13.6 \, z^2}{hc} \left[ \frac{1}{1^2} - \frac{1}{2^2} \right] \quad \dots \text{(i)} \]
For the second member of the Lyman series:
\[ \frac{1}{\lambda'} = \frac{13.6 \, z^2}{hc} \left[ \frac{1}{1^2} - \frac{1}{3^2} \right] \quad \dots \text{(ii)} \]
Dividing equation (i) by (ii):
\[ \lambda' = \frac{27}{32} \lambda \]
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,

What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)