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Calculate the radiative equilibrium temperature of the satellite immedi-ately after it emerges from the earth’s shadow (i.e., when the satelliteis sunlit but the earth, as viewed from the satellite, is still entirely inshadow). Givens: the Earth radiates as a blackbody at an equivalent blackbody temperature TE 255 K, the subtended angle is 2.21 steradians, and the radiative equilibrium temperature of the satellite is 166 K when it is in the Earth's shadow

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The diagram below shows two successive scatterings at locations A and B. In the first scattering, a photon of wavelength 1, hits a free electron at A resulting in a photon of wavelength 1, that moves at an angle 0, to the incident direction. The second photon hits an electron at B and scatters at an angle 0, to the direction of the second photon resulting in a photon of wavelength 12. Determine th angle 0, (in degrees) if 0, = 47.0° and the total shift in wavelength of the combined scattering is 4.08 x 10 -3 nm. 1 A B ° relative to the incident direction
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