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A sphere at temperature 600 K is placed ...

A sphere at temperature `600 K` is placed in an enviroment to temperature is `200 K`. Its cooling rate is `R`. If its temperature reduced to `400 K` then cooling rate in same enviorment will become

A

`(3)/(16)R`

B

`(16)/(3)R`

C

`(9)/(27)R`

D

None

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem, we will use Stefan-Boltzmann's law, which states that the power radiated by a black body is proportional to the fourth power of its absolute temperature. ### Step-by-Step Solution: 1. **Identify Initial Conditions**: - Initial temperature of the sphere, \( T_1 = 600 \, K \) - Temperature of the environment, \( T = 200 \, K \) 2. **Calculate Initial Cooling Rate (R)**: According to Stefan-Boltzmann's law, the cooling rate \( R \) can be expressed as: \[ R = \sigma (T_1^4 - T^4) \] where \( \sigma \) is the Stefan-Boltzmann constant. 3. **Substitute Values for Initial Cooling Rate**: Plugging in the values: \[ R = \sigma (600^4 - 200^4) \] 4. **Identify New Conditions**: - New temperature of the sphere, \( T_2 = 400 \, K \) 5. **Calculate New Cooling Rate (R1)**: The new cooling rate \( R_1 \) is given by: \[ R_1 = \sigma (T_2^4 - T^4) \] Substituting the new temperature: \[ R_1 = \sigma (400^4 - 200^4) \] 6. **Set Up the Ratio of Cooling Rates**: We can find the ratio of the new cooling rate to the initial cooling rate: \[ \frac{R_1}{R} = \frac{T_2^4 - T^4}{T_1^4 - T^4} \] 7. **Substitute the Values into the Ratio**: \[ \frac{R_1}{R} = \frac{400^4 - 200^4}{600^4 - 200^4} \] 8. **Calculate the Fourth Powers**: - \( 400^4 = 256 \times 10^4 \) - \( 200^4 = 16 \times 10^4 \) - \( 600^4 = 1296 \times 10^4 \) 9. **Substitute the Fourth Powers into the Ratio**: \[ \frac{R_1}{R} = \frac{(256 - 16) \times 10^4}{(1296 - 16) \times 10^4} = \frac{240 \times 10^4}{1280 \times 10^4} \] 10. **Simplify the Ratio**: \[ \frac{R_1}{R} = \frac{240}{1280} = \frac{3}{16} \] 11. **Calculate New Cooling Rate**: Therefore, the new cooling rate \( R_1 \) is: \[ R_1 = \frac{3}{16} R \] ### Final Answer: The cooling rate when the temperature of the sphere is reduced to \( 400 \, K \) will be \( \frac{3}{16} R \).

To solve the problem, we will use Stefan-Boltzmann's law, which states that the power radiated by a black body is proportional to the fourth power of its absolute temperature. ### Step-by-Step Solution: 1. **Identify Initial Conditions**: - Initial temperature of the sphere, \( T_1 = 600 \, K \) - Temperature of the environment, \( T = 200 \, K \) ...
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