Step 1: Identify the given energy levels and transitions clearly:
Three energy levels (E₁ < E₂ < E₃) of a hydrogen atom are given. Wavelengths of radiation emitted due to transitions between these levels are λ₁, λ₂, and λ₃:
Step 2: Use the energy-wavelength relationship clearly:
The energy difference (ΔE) between two levels is related to the wavelength (λ) of emitted radiation by:
\[ ΔE = \frac{hc}{λ} \]
where \(h\) = Planck’s constant, \(c\) = speed of light.
Step 3: Express the energy differences for each transition clearly:
Step 4: Relate the above energy differences:
Clearly, energy levels satisfy:
\[ (E_3 - E_1) = (E_3 - E_2) + (E_2 - E_1) \]
Substitute wavelength terms:
\[ \frac{hc}{λ_2} = \frac{hc}{λ_1} + \frac{hc}{λ_3} \]
Canceling out \(hc\), we get clearly:
\[ \frac{1}{λ_2} = \frac{1}{λ_1} + \frac{1}{λ_3} \]
Step 5: Solve this clearly to find λ₂ explicitly:
\[ λ_2 = \frac{λ_1λ_3}{λ_1 + λ_3} \]
Final Conclusion:
Thus, the correct relation is clearly:
\[ λ_2 = \frac{λ_1λ_3}{λ_1 + λ_3} \]