The spectral emissive power E? for a body at temperature T1 is plotted against the wavelength and area under the curve is found to be A. At a different temperature T2, the area is found to be 9A. Then ?1/?2
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For a radioactive body the ratio of T1/T2 will be (9)^1/4.
The relation between emissive power E, temperature T and area A of a radioactive body can be determined by Stefan's law.
According to Stefan's law,
Spectral emissive power can be determined by,
E=sigma**A*T^4
Where,E=Spectral emissive power
T=temperature of the body
A=Area of the body
Sigma=Stefan's constant
For a body of constant temperature E,
T^4 will be inversely proportional to A.
Hence,
A1/A2=T1^4/T2^4
Or,9A/A=T1^4/T2^4
Or,T1/T2=(9)^1/4
Hence for the body the ratio will be (9)^1/4.
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