Question

The rate of emission of radiation of a black body at ${273^ \circ }C$ is $E$, then what will be the rate of emission of radiation of the body at ${0^ \circ }C$?
A. $\dfrac{E}{{16}}$
B. $\dfrac{E}{4}$
C. $\dfrac{E}{8}$
D. $0$

Answer 1

Hint- Stefan's law gives us the expression for total power radiated per unit surface area of a black body.
According to this law, the total power radiated per unit surface area of a black body is directly proportional to the fourth power of temperature. In mathematical form this law can be written as,
$E \propto {T^4}$
Here, $T$ is the temperature of the black body.

Step by step solution:
Stefan's law gives us the expression for total power radiated per unit surface area of a black body.
According to this law, the total power radiated per unit surface area of a black body is directly proportional to the fourth power of temperature. In mathematical form this law can be written as,
$E \propto {T^4}$
Or
$E = \sigma {T^4}$
Where, $\sigma$ is the Stefan’s constant and $T$ is the temperature.
Given,
Temperature,
${T_1} = {273^ \circ }C \\\ = 273 + 273\,K \\\ = 556\,K \\\$
Let the rate of emission of radiation of black body at ${273^ \circ }C$ be denoted as ${E_1}$.
Therefore, using Stefan’s law, we can write,
${E_1} = \sigma {T_1}^4$ ……. (1)
Temperature,
${T_2} = {0^ \circ }C \\\ = 0 + 273\,K \\\ = 273\,K \\\$
Let the rate of emission of radiation of black body at ${0^ \circ }C$ be denoted as ${E_2}$.
Therefore, using Stefan’s law, we can write,
${E_2} = \sigma {T_2}^4$ …… (2)
Divide equation (1) by (2). Then, we get

$$\dfrac{{{E_1}}}{{{E_2}}} = \dfrac{{{T_1}^4}}{{{T_2}^4}} \\\ \dfrac{{{E_1}}}{{{E_2}}} = {\left( {\dfrac{{{T_1}}}{{{T_2}}}} \right)^4} \\\$$

Now substitute the given values. Then, we get

$$\dfrac{{{E_1}}}{{{E_2}}} = {\left( {\dfrac{{556}}{{273}}} \right)^4} \\\ = {\left( 2 \right)^4} \\\ = 16 \\\$$

That is,
${E_2} = \dfrac{{{E_1}}}{{16}}$

Hence the correct answer is option A.

Note: Remember to convert the temperatures given in $^ \circ C$ into the corresponding temperature in kelvin.
Formula to remember
Stefan’s law, $E = \sigma {T^4}$
Where, $E$ is the total power radiated per unit surface area of a black body and $T$ is the temperature of black body.