To determine the factor by which the rate of emission of a black body increases when its temperature increases from \( T \) to \( 2T \), we use the Stefan-Boltzmann Law. This law states that the power radiated per unit area of a black body is directly proportional to the fourth power of the temperature. Mathematically, it is expressed as:
\(P = \sigma \cdot A \cdot T^4\)
where:
For the initial temperature \( T \), the power emitted is:
\(P_1 = \sigma \cdot A \cdot T^4\)
When the temperature is increased to \( 2T \), the power emitted becomes:
\(P_2 = \sigma \cdot A \cdot (2T)^4 = \sigma \cdot A \cdot 16T^4\)
Hence, the rate of emission increases by a factor:
\(\frac{P_2}{P_1} = \frac{16 \sigma \cdot A \cdot T^4}{\sigma \cdot A \cdot T^4} = 16\)
Therefore, the correct answer is that the rate of emission increases by a factor of 16 when the temperature of the black body is doubled.
