For the moon, the wavelength corresponding to the maximum specral emissive power is 14 microns. If the Wien's constant `b=2.884 xx10^(-3)mK`, then the temperature of the moon is close to

For the moon, the wavelength corresponding to the maximum spectral emissive power is 14 microns. If the Wien's constant b=2.884 xx10^(-3)mK , then the temperature of the moon is close to

If the wavelength corresponding to maximum energy radiated from the moon is 14 micron , and Wien 's constant is 2.8 xx 10^(-3) m K , then temperature of moon is

If the wavelength corresponding to maximum energy radiated from the moon is 14 micron, and wien's constant is 2.8xx10^(-3)mK , then temperature of moon is

If the wavelength corresponding to maximum energy radiated from the moon is 14 micron, and wien's constant is 2.8xx10^(-3)mK , then temperature of moon is

Light from the moon, is found to have a peak (or wevelenght of maximum emission) at lambda = 14 mu m . Given that the Wien's constant b equals 2.8988 xx 10^(-3) mK , estimate the temperature of the moon.

Wave length corresponding E_(max) for the moon in 14 micron. Estimate the temperature of the moon ( Take wien's constant = 2.884 xx 10^(-3) mK ).

The wavelength of the radiation emitted by a black body is 1 mm and Wien's constant is 3xx10^(-3) mK. Then the temperature of the black body will be

Find the wavelength at which a black body radiates maximum energy, if its temperature is 427^(@) C. (Wein's constant b=2.898 xx 10^(-3) mK )