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

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