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Question: Two spheres of the same material have radii \( 1m \) and \( 4m \) and temperature \( 4000K \) and \(...

Two spheres of the same material have radii 1m1m and 4m4m and temperature 4000K4000K and 2000K2000K respectively. Which of the following is the energy radiated per second by the first sphere?
A. Greater than of the second sphere
B. Less than of the second sphere
C. Equal to that of the second sphere
D. The information is incomplete to draw any conclusion.

Explanation

Solution

Hint : Calculate the radiated energy by using Stefan’s law of radiation. The formula for total energy radiated from a body with surface area AA at absolute temperature TT is,
E=eσT4AE = e\sigma {T^4}A , Where ee is the emissivity of that body and σ\sigma is the Stefan’s constant.

Complete Step By Step Answer:
We know that Stefan's law of blackbody radiation states that the energy radiated by a black body from per unit area per second is proportional to the fourth power of it’s absolute temperature.
That means, energy radiated per second per unit area from a blackbody, EαT4E\alpha {T^4}
EE is energy radiated per unit area per second from the blackbody,
TT is the absolute temperature of the blackbody.
Now, Equating this equation we know,
E=σT4E = \sigma {T^4}
where, σ\sigma is a constant and is called Stefan’s constant. It’s value is σ=5.672×105Wm2K4\sigma = 5.672 \times {10^{ - 5}}W \cdot {m^{ - 2}} \cdot {K^{ - 4}}
Now, If the body is a normal one rather than a blackbody then, energy radiated from the body per second per unit area becomes,
E=eσT4E = e\sigma {T^4} Where ee is the emissivity of that body.
It is defined as, the ratio of the energy radiated from a material's surface to that radiated from a perfect emitter or known as a blackbody, at the same temperature and wavelength and under the same conditions. That means the geometry of the blackbody and the material must be the same.
So that means, emissivity e=EEBe = \dfrac{E}{{{E_B}}} where, EE is the radiated energy of a body with surface area AA and EB{E_B} is the radiated energy per second from a blackbody of same surface area AA at absolute temperature TT .
\therefore Total energy radiated from a body with surface area AA at absolute temperature TT is,
E=eσT4AE = e\sigma {T^4}A
Here, we have two spheres built from same material of radius r1=1m{r_1} = 1m and r2=4m{r_2} = 4m
Also, we have the two spheres are made of the same material, hence emissivity ee is the same for both the bodies.
\therefore Energy radiated by the first sphere E1=eσT14A1{E_1} = e\sigma {T_1}^4{A_1} where, A1=4πr12=4π12{A_1} = 4\pi {r_1}^2 = 4\pi \cdot {1^2} , T1=4000K{T_1} = 4000K
\therefore Energy radiated by the second sphere E2=eσT24A2{E_2} = e\sigma T_2^4{A_2} Where, A2=4πr22=4π42{A_2} = 4\pi {r_2}^2 = 4\pi \cdot {4^2} and T2=2000K{T_2} = 2000K
\therefore E1E2=eσT14A1eσT24A2=T14A1T24A2\therefore \dfrac{{{E_1}}}{{{E_2}}} = \dfrac{{e\sigma T_1^4{A_1}}}{{e\sigma T_2^4{A_2}}} = \dfrac{{T_1^4{A_1}}}{{T_2^4{A_2}}}
That becomes,
=T144πr12T244πr22=T14r12T24r22= \dfrac{{T_1^44\pi r_1^2}}{{T_2^44\pi r_2^2}} = \dfrac{{T_1^4r_1^2}}{{T_2^4r_2^2}}
Putting the values, r1=1{r_1} = 1 , T1=4000K{T_1} = 4000K , r2=4{r_2} = 4 and T2=2000K{T_2} = 2000K we get,
=(40000)4×12(2000)4×42=11= \dfrac{{{{\left( {40000} \right)}^4} \times {1^2}}}{{{{\left( {2000} \right)}^4} \times {4^2}}} = \dfrac{1}{1}
=1= 1
Hence, energy radiated by the spheres is equal
Hence, correct option is option (C).

Note :
\bullet Stefan’s law of radiation states that the energy radiated per second per unit area from a blackbody is which is basically the power radiated by that body per unit area.
\bullet Ratio of the energy radiated from two bodies with the same material does not depend on the emissivity.