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Question: A blackbody emits heat at the rate of 20W. When its temperature is \({227^ \circ }C\). Another black...

A blackbody emits heat at the rate of 20W. When its temperature is 227C{227^ \circ }C. Another black body emits heat at the rate of 15W15W when its temperature is 277C{277^ \circ }C. Compare the area of the surface of the two bodies, if the surrounding is at NTP:
(A) 16:116:1
(B) 1:41:4
(C) 12:112:1
(D) 1:121:12

Explanation

Solution

Here we are given two black bodies that emit different powers at different temperatures. We have to compare the surface area of the two black bodies when the surrounding of the black bodies is at normal temperature and pressure. We have to consider one of the laws for black body radiation to solve this problem.
Formula used
W=eσAT4W = e\sigma A{T^4}
Where, WW stands for the power emitted by the black body, ee stands for the emissivity of the black body, σ\sigma stands for the Stefan’s constant, AA stands for the surface area of the black body, and TT stands for the temperature of the black body.

Complete step by step solution:
According to the Stefan-Boltzmann law, the amount of power radiated per unit time for a unit area of the black body is directly proportional to the fourth power of the temperature.
It can be expressed as,
W=eσAT4W = e\sigma A{T^4}
The radiation emitted by the first black body can be written as,
W1=eσA1T14{W_1} = e\sigma {A_1}T_1^4
Where T0{T_0}is the temperature of the surrounding.
The radiation emitted by the second black body can be written as,
W2=eσA2T24{W_2} = e\sigma {A_2}T_2^4
Comparing the powers of the two black bodies,
W1W2=eσA1T14eσA2T24\dfrac{{{W_1}}}{{{W_2}}} = \dfrac{{e\sigma {A_1}T_1^4}}{{e\sigma {A_2}T_2^4}}
Cancelling out the same values, we get
W1W2=A1T14A2T24\dfrac{{{W_1}}}{{{W_2}}} = \dfrac{{{A_1}T_1^4}}{{{A_2}T_2^4}}
From this we can write the comparison of the areas as,
A1A2=W1T24W2T14\dfrac{{{A_1}}}{{{A_2}}} = \dfrac{{{W_1}T_2^4}}{{{W_2}T_1^4}}
From the question, we know that
W1=20W{W_1} = 20W
W2=15W{W_2} = 15W
T1=227C=500K{T_1} = {227^ \circ }C = 500K
T2=277C=550K{T_2} = {277^ \circ }C = 550K
(To convert degree Celsius to Kelvin we have to add the273K273Kwith the given temperature.)
Substituting the values in the above equation, we get that,
A1A2=20×550415×5004\dfrac{{{A_1}}}{{{A_2}}} = \dfrac{{20 \times {{550}^4}}}{{15 \times {{500}^4}}}
After solving, we get the ratio as, 2:12:1

The correct answer is not given in the option.

Note:
A blackbody will absorb all radiation incident on it without considering the frequency or the wavelength of the incident radiation. Since it absorbs all the radiations, it will appear black in color hence it is called a black body. The black body will also emit radiations of a certain frequency which are called blackbody radiations.