The rate of emission of radiation from a black body is given by Stefan's Law, which states that the power emitted per unit area is proportional to the fourth power of the absolute temperature:
\[ E = \sigma T^4 \]where:
Let the initial temperature be \( T_1 = 27^\circ \text{C} = 273 + 27 = 300 \, \text{K} \) and the final temperature be \( T_2 = 327^\circ \text{C} = 273 + 327 = 600 \, \text{K} \).
According to Stefan's Law, the ratio of the emissions is given by:
\[ \frac{E_2}{E_1} = \left( \frac{T_2}{T_1} \right)^4 \]Substituting the values of \( T_1 \) and \( T_2 \):
\[ \frac{E_2}{E_1} = \left( \frac{600}{300} \right)^4 = 2^4 = 16 \]Thus, \( E_2 = 16E_1 \).
So, the correct answer is Option (3), \( E_2 = 16E_1 \).
To solve the problem, we need to calculate the rate of emission of radiation at two different temperatures based on the Stefan-Boltzmann law.
1. Understanding the Stefan-Boltzmann Law:
The rate of emission of radiation (E) of a black body is proportional to the fourth power of its temperature, as per the Stefan-Boltzmann law:
\[
E \propto T^4
\]
where \( T \) is the absolute temperature of the body in Kelvin. Let the rate of emission at temperature \( T_1 \) be \( E_1 \), and at temperature \( T_2 \) be \( E_2 \).
2. Converting Temperatures to Kelvin:
We are given the temperatures in Celsius:
- \( T_1 = 27^\circ C = 27 + 273 = 300 \, \text{K} \)
- \( T_2 = 327^\circ C = 327 + 273 = 600 \, \text{K} \)
3. Applying the Stefan-Boltzmann Law:
We know:
\[
\frac{E_2}{E_1} = \left( \frac{T_2}{T_1} \right)^4
\]
Substituting the values of \( T_2 \) and \( T_1 \):
\[
\frac{E_2}{E_1} = \left( \frac{600}{300} \right)^4 = 2^4 = 16
\]
Thus, \( E_2 = 16 E_1 \).
4. Identifying the Correct Answer:
The rate of emission at 327°C is 16 times the emission at 27°C, which corresponds to Option 3.
Final Answer:
The correct answer is Option C: 16 E1.