The plots of spectral radiancy Rλ versus wave length λ for three black bodies at temperatures T1, T2 and T3 respectively are shown. Their temperatures are such that
T1 > T2 > T3
T1 > T3 > T2
T2 > T3 > T1
T3 > T2 > T1
By Wien’s displacement Law, at maximum intensity λT= constant. Since λ1 < λ3 < λ2, we can conclude, T1 > T3 > T2.