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A black body is at a temperature of 2880 K. The energy of radiation emitted by this object with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. Wien's constant b = 2.88 x 106 nm - K, then
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U2 > U1
From Wien's law, constant, where T is the temperature of black body and is the wavelength corresponding to maximum energy of emission. Energy distribution of black body radiation is given below :
i. U1 and U2 are not zero because a black body emits radiations of nearly all wavelengths.
ii. Since U1 corresponding to lower wavelength, U3 corresponds to higher wavelength and U2 corresponds to medium wave length hence U2 > U1.
i. U1 and U2 are not zero because a black body emits radiations of nearly all wavelengths.
ii. Since U1 corresponding to lower wavelength, U3 corresponds to higher wavelength and U2 corresponds to medium wave length hence U2 > U1.
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