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Two bodies A and B have emissivities 0.5...

Two bodies A and B have emissivities 0.5 and 0.8 respectively. At some temperature the two bodies have maximum spectral emissive powers at wavelength `8000 Å` and `4000 Å` respectively. The ratio of their emissive powers at these temperatures is :

A

`(5)/(128)`

B

`10`

C

`(5)/(16)`

D

None of these

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To solve the problem, we need to find the ratio of the emissive powers of two bodies A and B, given their emissivities and the wavelengths at which they have maximum spectral emissive powers. ### Step-by-Step Solution: 1. **Identify Given Data:** - Emissivity of body A, \( E_A = 0.5 \) - Emissivity of body B, \( E_B = 0.8 \) - Wavelength for body A, \( \lambda_A = 8000 \, \text{Å} \) - Wavelength for body B, \( \lambda_B = 4000 \, \text{Å} \) 2. **Apply Wien’s Displacement Law:** - According to Wien's displacement law, the product of the wavelength at which the maximum spectral emissive power occurs and the absolute temperature is constant: \[ \lambda_1 T_1 = \lambda_2 T_2 \] - Rearranging gives us: \[ \frac{\lambda_1}{\lambda_2} = \frac{T_2}{T_1} \] 3. **Substituting the Values:** - Substitute \( \lambda_1 = 8000 \, \text{Å} \) and \( \lambda_2 = 4000 \, \text{Å} \): \[ \frac{8000}{4000} = \frac{T_2}{T_1} \] - Simplifying gives: \[ 2 = \frac{T_2}{T_1} \quad \Rightarrow \quad T_1 = \frac{T_2}{2} \] 4. **Emissive Power Formula:** - The emissive power \( E \) of a body is given by: \[ E = \epsilon \sigma T^4 \] - Where \( \epsilon \) is the emissivity, \( \sigma \) is the Stefan-Boltzmann constant, and \( T \) is the absolute temperature. 5. **Expressing the Ratio of Emissive Powers:** - The emissive powers for bodies A and B can be expressed as: \[ E_A = E_A \sigma T_1^4 \quad \text{and} \quad E_B = E_B \sigma T_2^4 \] - The ratio of emissive powers \( \frac{E_A}{E_B} \) is: \[ \frac{E_A}{E_B} = \frac{E_A \sigma T_1^4}{E_B \sigma T_2^4} = \frac{E_A}{E_B} \cdot \frac{T_1^4}{T_2^4} \] 6. **Substituting the Values:** - Substitute \( E_A = 0.5 \) and \( E_B = 0.8 \): \[ \frac{E_A}{E_B} = \frac{0.5}{0.8} \cdot \left(\frac{T_1}{T_2}\right)^4 \] - From step 3, we have \( T_1 = \frac{T_2}{2} \): \[ \frac{T_1}{T_2} = \frac{1}{2} \] - Therefore: \[ \left(\frac{T_1}{T_2}\right)^4 = \left(\frac{1}{2}\right)^4 = \frac{1}{16} \] 7. **Final Calculation:** - Now substituting back: \[ \frac{E_A}{E_B} = \frac{0.5}{0.8} \cdot \frac{1}{16} = \frac{5}{8} \cdot \frac{1}{16} = \frac{5}{128} \] ### Conclusion: The ratio of the emissive powers of bodies A and B is: \[ \frac{E_A}{E_B} = \frac{5}{128} \]

To solve the problem, we need to find the ratio of the emissive powers of two bodies A and B, given their emissivities and the wavelengths at which they have maximum spectral emissive powers. ### Step-by-Step Solution: 1. **Identify Given Data:** - Emissivity of body A, \( E_A = 0.5 \) - Emissivity of body B, \( E_B = 0.8 \) - Wavelength for body A, \( \lambda_A = 8000 \, \text{Å} \) ...
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