Step 1: Wien's Displacement Law: The wavelength of maximum radiation emission (\( \lambda_{\text{max}} \)) from a black body is inversely proportional to its absolute temperature (\(T\)). Mathematically:\[ \lambda_{\text{max}} T = b \]where \(b\) is Wien's displacement constant (\( \approx 2.898 \times 10^{-3} \) m⋅K).
Step 2: Ratio Setup for Bodies P and Q: Because \( \lambda_{\text{max}} T \) is constant:\[ \lambda_{P} T_{P} = \lambda_{Q} T_{Q} \]
Step 3: Solve for Unknown Temperature \(T_Q\): Rearrange the formula:\[ T_Q = T_P \left( \frac{\lambda_P}{\lambda_Q} \right) \]
Step 4: Calculate \(T_Q\): Substitute values:- \( T_P = 1000 \) K- \( \lambda_P = 3000 \) nm- \( \lambda_Q = 550 \) nmNote: Nanometer units can be used in the ratio without conversion. Calculation:\[ T_Q = 1000 \times \frac{3000}{550} = 1000 \times \frac{300}{55} = 1000 \times \frac{60}{11} \approx 1000 \times 5.4545 \]\[ T_Q \approx 5454.5 \text{ K} \]