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Question: A spherical black body with a radius of \( 12\;cm \) radiates \( 450\;W \) power at \( 500\;K \) . T...

A spherical black body with a radius of 12  cm12\;cm radiates 450  W450\;W power at 500  K500\;K . The radius was halved and the temperature doubled, the power radiated in watts would be:
(A) 225  225\;
(B) 450  450\;
(C) 900  900\;
(D) 1800  1800\;

Explanation

Solution

Here we will use Stefan’s law to obtain the relation between the area, temperature and the power radiated by a body. Since it is a black body, e=1e = 1 is used. Then we find the ratios of the new temperature and are with the original values and substitute in the formula. Thus we will get the new value of the power radiation in terms of the original radiation.

Formula used:
P=σAeT4P = \sigma Ae{T^4} .

Complete step by step answer:
It is given in the question that the black body radiates a given amount of power. Any such radiation is given by Stefan’s law
P=σAeT4P = \sigma Ae{T^4}
where ee is the emissivity of the body,
σ\sigma is Stefan's constant, and
AA is the area of the body from which the radiation is taking place.
The Stefan’s constant has a value σ=5.67×108W/m2K4\sigma = 5.67 \times {10^{ - 8}}W/{m^2}{K^4} .
Now for a perfect black body, the emissivity, e=1e = 1 .
Thus we have our initial value of the power radiation as
P1=σA1T14{P_1} = \sigma {A_1}{T_1}^4
where A1{A_1} is the area of the black body and T1{T_1} is the absolute temperature of the surface of the body given as T1=500  K{T_1} = 500\;K .
It is given that the radius of the black body is r1=12  cm{r_1} = 12\;cm .
A1=4πr12\therefore {A_1} = 4\pi {r_1}^2
Now when the radius of the black body is halved, the new radius becomes r2=6  cm{r_2} = 6\;cm .
A2=4πr22\therefore {A_2} = 4\pi {r_2}^2
Upon substituting the values we get,
A2=4π(r12)2\Rightarrow {A_2} = 4\pi {(\dfrac{{{r_1}}}{2})^2}
A2=4πr124\Rightarrow {A_2} = \dfrac{{4\pi {r_1}^2}}{4}
Thus we have,
A2=A14\Rightarrow {A_2} = \dfrac{{{A_1}}}{4}
Also when the temperature of the surface of the black body is doubled, the new temperature T2{T_2} becomes, T2=1000  K{T_2} = 1000\;K .
i.e., T2=2T1{T_2} = 2{T_1}
Now applying the Stefan’s law on the changed conditions, we have,
P2=σA2T24{P_2} = \sigma {A_2}{T_2}^4
Substituting the values of the area and the temperature, we get,
P2=σA14(2T1)4\Rightarrow {P_2} = \sigma \dfrac{{{A_1}}}{4}{(2{T_1})^4}
P2=164σA1T14\Rightarrow {P_2} = \dfrac{{16}}{4}\sigma {A_1}{T_1}^4
This is related to the initial power transmitted as,
P2=4P1\Rightarrow {P_2} = 4{P_1}
Substituting the value of P1{P_1} in the above equation, we have the new power radiated as,
P2=4×450  W{P_2} = 4 \times 450\;W
Thus P2=1800  W{P_2} = 1800\;W is the power radiated after the changes in temperature and the radius.
Therefore the correct answer is option (D).

Note:
The value of emissivity is a fraction which lies between 00 and 11 . This value is unity for a perfect black body. Also, the temperature used in the formula is the absolute value of the temperature in Kelvin. The area given here is assumed to be the total area of a sphere without any minimization due to contacts of placement.