
The wavelength of a spectral line in the hydrogen spectrum is given by:
\[ \frac{1}{\lambda} = RZ^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right), \]
where \( R \) is the Rydberg constant, \( Z \) is the atomic number, \( n_1 \) is the lower energy level, and \( n_2 \) is the higher energy level.
For the shortest wavelength in the Balmer series:
\[ n_1 = 2, \quad n_2 = \infty \]
\[ \frac{1}{\lambda_B} = RZ^2 \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right) = RZ^2 \left( \frac{1}{4} \right). \]
For the shortest wavelength in the Lyman series:
\[ n_1 = 1, \quad n_2 = \infty \]
\[ \frac{1}{\lambda_L} = RZ^2 \left( \frac{1}{1^2} - \frac{1}{\infty^2} \right) = RZ^2 (1). \]
Taking the ratio of wavelengths:
\[ \frac{\lambda_B}{\lambda_L} = \frac{\frac{1}{RZ^2 \frac{1}{4}}}{\frac{1}{RZ^2 (1)}} = 4 : 1. \]
Thus, the ratio is:
\[ \lambda_B : \lambda_L = 4 : 1. \]
Final Answer: 4:1 (Option 1)
The problem asks for the ratio of the shortest wavelength of the Balmer series to the shortest wavelength of the Lyman series for a hydrogen atom.
1. Rydberg's Formula: The wavelength \( \lambda \) of the radiation emitted when an electron in a hydrogen-like atom makes a transition from a higher energy level \( n_i \) to a lower energy level \( n_f \) is given by Rydberg's formula:
\[ \frac{1}{\lambda} = R Z^2 \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right) \]where \( R \) is the Rydberg constant and \( Z \) is the atomic number. For a hydrogen atom, \( Z = 1 \).
2. Lyman and Balmer Series:
3. Shortest Wavelength (Series Limit): The energy of the emitted photon is \( E = \frac{hc}{\lambda} \). To have the shortest wavelength (\( \lambda_{\text{min}} \)), the energy of the transition must be maximum. This occurs when the electron transitions from the highest possible energy level, which is \( n_i = \infty \).
Step 1: Determine the shortest wavelength of the Lyman series (\( \lambda_{\text{Lyman, min}} \)).
For the Lyman series, the final state is \( n_f = 1 \). For the shortest wavelength, the initial state is \( n_i = \infty \). For hydrogen, \( Z=1 \). Substituting these values into Rydberg's formula:
\[ \frac{1}{\lambda_{\text{Lyman, min}}} = R (1)^2 \left( \frac{1}{1^2} - \frac{1}{\infty^2} \right) \]Since \( \frac{1}{\infty^2} = 0 \), the equation simplifies to:
\[ \frac{1}{\lambda_{\text{Lyman, min}}} = R (1 - 0) = R \]Therefore, the shortest wavelength for the Lyman series is:
\[ \lambda_{\text{Lyman, min}} = \frac{1}{R} \]Step 2: Determine the shortest wavelength of the Balmer series (\( \lambda_{\text{Balmer, min}} \)).
For the Balmer series, the final state is \( n_f = 2 \). For the shortest wavelength, the initial state is \( n_i = \infty \). Again, for hydrogen, \( Z=1 \). Substituting these values into Rydberg's formula:
\[ \frac{1}{\lambda_{\text{Balmer, min}}} = R (1)^2 \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right) \]This simplifies to:
\[ \frac{1}{\lambda_{\text{Balmer, min}}} = R \left( \frac{1}{4} - 0 \right) = \frac{R}{4} \]Therefore, the shortest wavelength for the Balmer series is:
\[ \lambda_{\text{Balmer, min}} = \frac{4}{R} \]Step 3: Calculate the ratio of the shortest wavelength of the Balmer series to that of the Lyman series.
\[ \frac{\lambda_{\text{Balmer, min}}}{\lambda_{\text{Lyman, min}}} = \frac{4/R}{1/R} \] \[ \frac{\lambda_{\text{Balmer, min}}}{\lambda_{\text{Lyman, min}}} = 4 \]Thus, the ratio of the shortest wavelength of the Balmer series to the shortest wavelength of the Lyman series is 4:1.
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 : \(A_2 \rightleftharpoons 2A\)