Step 1: State Wien's Displacement Law. Wien's law states that the wavelength at which a black body emits the maximum amount of radiation, \( \lambda_{\text{max}} \), is inversely proportional to its absolute temperature \(T\). \[ \lambda_{\text{max}} T = b \] where \(b\) is Wien's displacement constant (\( \approx 2.898 \times 10^{-3} \) m⋅K).
Step 2: Set up a ratio for the two bodies P and Q. Since \( \lambda_{\text{max}} T \) is constant for any black body: \[ \lambda_{P} T_{P} = \lambda_{Q} T_{Q} \]
Step 3: Rearrange the formula to solve for the unknown temperature, \(T_Q\). \[ T_Q = T_P \left( \frac{\lambda_P}{\lambda_Q} \right) \]
Step 4: Substitute the given values and calculate \(T_Q\). - \( T_P = 1000 \) K - \( \lambda_P = 3000 \) nm - \( \lambda_Q = 550 \) nm Note that since we are using a ratio, we do not need to convert nanometers to meters. \[ T_Q = 1000 \times \frac{3000}{550} = 1000 \times \frac{300}{55} = 1000 \times \frac{60}{11} \approx 1000 \times 5.4545 \] \[ T_Q \approx 5454.5 \text{ K} \]