Q.

Two spherical stars A and B emit blackbody radiation. The radius of A is 400 times that of B and A emits 104 times the power emitted from B. The ratio (λAλB) of their wavelengths λA and λB at which the peaks occur in their respective radiation curves is                       [2015]


Ans.

(2)

 From (i) Stefan-Boltzmann law,  P=σAT4  and (ii) Wien's displacement law, λm×T=constant

PAPB=AAABTA4TB4=AAAB×λB4λA4

  λAλB=[AAAB×PBPA]14=[RA2RB2×PBPA]14=[400×400104]14

  λAλB=2