Step 1: Establish the inverse relationship between wavelength and energy. When an electron in a hydrogen atom transitions from a higher energy level ($n_2$) to a lower one ($n_1$), it emits a photon with energy $E = hf = \frac{hc}{\lambda}$. Consequently, $\lambda = \frac{hc}{E}$. This indicates that a longer wavelength ($\lambda$) corresponds to a smaller energy difference ($E$). Therefore, the transition with the least energy difference will yield the longest wavelength.
Step 2: Apply the energy level formula for a hydrogen atom. The energy of an electron at level $n$ in a hydrogen atom is given by $E_n = -\frac{13.6}{n^2} \, \text{eV}$. The energy difference for a transition from $n_2$ to $n_1$ (where $n_2>n_1$) is calculated as $\Delta E = E_{n_2} - E_{n_1} = -\frac{13.6}{n_2^2} - \left(-\frac{13.6}{n_1^2}\right) = 13.6 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)$.
Step 3: Compute the energy difference for each transition.
- (A) Transition from $n = 4$ to $n = 3$: $\Delta E = 13.6 \left( \frac{1}{3^2} - \frac{1}{4^2} \right) = 13.6 \left( \frac{1}{9} - \frac{1}{16} \right) = 13.6 \left( \frac{16 - 9}{144} \right) = 13.6 \times \frac{7}{144} \approx 0.661 \, \text{eV}$
- (B) Transition from $n = 3$ to $n = 2$: $\Delta E = 13.6 \left( \frac{1}{2^2} - \frac{1}{3^2} \right) = 13.6 \left( \frac{1}{4} - \frac{1}{9} \right) = 13.6 \left( \frac{9 - 4}{36} \right) = 13.6 \times \frac{5}{36} \approx 1.889 \, \text{eV}$
- (C) Transition from $n = 2$ to $n = 1$: $\Delta E = 13.6 \left( \frac{1}{1^2} - \frac{1}{2^2} \right) = 13.6 \left( \frac{1}{1} - \frac{1}{4} \right) = 13.6 \times \frac{3}{4} = 10.2 \, \text{eV}$
- (D) Transition from $n = 3$ to $n = 1$: $\Delta E = 13.6 \left( \frac{1}{1^2} - \frac{1}{3^2} \right) = 13.6 \left( \frac{1}{1} - \frac{1}{9} \right) = 13.6 \times \frac{8}{9} \approx 12.089 \, \text{eV}$
Step 4: Compare the calculated energy differences.
- (A) $\Delta E \approx 0.661 \, \text{eV}$
- (B) $\Delta E \approx 1.889 \, \text{eV}$
- (C) $\Delta E = 10.2 \, \text{eV}$
- (D) $\Delta E \approx 12.089 \, \text{eV}$
The smallest energy difference is observed for transition (A) from $n = 4$ to $n = 3$. This transition will therefore have the largest wavelength.
Step 5: Verify with the Rydberg formula (optional). The Rydberg formula for wavenumber is $\frac{1}{\lambda} = R \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)$. A smaller value of $\frac{1}{\lambda}$ implies a larger $\lambda$. The term $\frac{1}{n_1^2} - \frac{1}{n_2^2}$ is minimized for transition (A), confirming the result obtained earlier.