Question:medium

A black sphere has radius R whose rate of radiation is E at temperature T. If radius is made $R/2$ and temperature $3T$, the rate of radiation will be

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Radiation power is highly sensitive to temperature changes ($\text{Power} \propto T^4$).
Updated On: Jun 19, 2026
  • $3E/2$
  • $27E/8$
  • $81E/4$
  • $9E/4$
Show Solution

The Correct Option is C

Solution and Explanation

Step 1: Understanding the Question:
We need to find the new rate of radiation for a sphere when its dimensions and temperature change, based on Stefan-Boltzmann law.

Step 2: Key Formula or Approach:

According to Stefan-Boltzmann law, the rate of radiation \( E \) is:
\[ E = \sigma A T^4 \] For a sphere, Surface Area \( A = 4\pi R^2 \), so:
\[ E \propto R^2 T^4 \]

Step 3: Detailed Explanation:

Let initial rate be \( E_1 = k R^2 T^4 \).
Final radius \( R_2 = \frac{R}{2} \).
Final temperature \( T_2 = 3T \).
The new rate of radiation \( E_2 \) is:
\[ E_2 \propto R_2^2 T_2^4 \] \[ E_2 \propto \left( \frac{R}{2} \right)^2 (3T)^4 \] \[ E_2 \propto \frac{R^2}{4} \times 81 T^4 \] \[ E_2 = \frac{81}{4} (k R^2 T^4) \] \[ E_2 = \frac{81E}{4} \]

Step 4: Final Answer:

The new rate of radiation will be \( \frac{81E}{4} \).
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