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If the absolute temperature of a black b...

If the absolute temperature of a black body is doubled the percentage increase in the rate of loss of heat by radiation is .

A

`15%`

B

`16%`

C

`1600%`

D

`1500%`

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AI Generated Solution

The correct Answer is:
To solve the problem of finding the percentage increase in the rate of loss of heat by radiation when the absolute temperature of a black body is doubled, we can follow these steps: ### Step-by-Step Solution: 1. **Understanding the Stefan-Boltzmann Law**: The power radiated by a black body is given by the formula: \[ P = E \sigma A T^4 \] where: - \( P \) is the power (rate of heat loss), - \( E \) is the emissivity (for a black body, \( E = 1 \)), - \( \sigma \) is the Stefan-Boltzmann constant, - \( A \) is the surface area, - \( T \) is the absolute temperature in Kelvin. 2. **Define Initial and Final Temperatures**: Let the initial absolute temperature be \( T_1 \) and the final temperature be \( T_2 \). According to the problem, if the absolute temperature is doubled: \[ T_2 = 2T_1 \] 3. **Calculate Initial and Final Power**: - The initial power \( P_1 \) at temperature \( T_1 \): \[ P_1 = E \sigma A T_1^4 \] - The final power \( P_2 \) at temperature \( T_2 \): \[ P_2 = E \sigma A (2T_1)^4 = E \sigma A \cdot 16 T_1^4 \] 4. **Finding the Ratio of Powers**: To find the ratio of the final power to the initial power: \[ \frac{P_2}{P_1} = \frac{E \sigma A \cdot 16 T_1^4}{E \sigma A T_1^4} = 16 \] 5. **Calculate the Increase in Power**: The increase in power can be calculated as: \[ P_2 - P_1 = P_2 - P_1 = 16P_1 - P_1 = 15P_1 \] 6. **Percentage Increase in Power**: To find the percentage increase: \[ \text{Percentage Increase} = \left(\frac{P_2 - P_1}{P_1}\right) \times 100 = \left(\frac{15P_1}{P_1}\right) \times 100 = 1500\% \] ### Final Answer: The percentage increase in the rate of loss of heat by radiation when the absolute temperature of a black body is doubled is **1500%**. ---

To solve the problem of finding the percentage increase in the rate of loss of heat by radiation when the absolute temperature of a black body is doubled, we can follow these steps: ### Step-by-Step Solution: 1. **Understanding the Stefan-Boltzmann Law**: The power radiated by a black body is given by the formula: \[ P = E \sigma A T^4 ...
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