Answer:
T=270 K
Explanation:
Power absorbed by the Moon
[tex]P_{absorbed}= [1-0.12]solar\ constant\times\pi R^2[/tex]
the reason for choosing the area as π R^2 and not 4π R^2 is because the absorbed light is only from the surface facing the Sun which is a disc.
Using Stefan Boltzmann's law,
[tex]P_{emitted}= \sigma T^4(4\pi R^2)[/tex]
So, using Conservation of Energy,
[tex][1-0.12]solar\ constant\times\pi R^2=\sigma T^4(4\pi R^2)[/tex]
this gives, T = 270 K. This is the temperature of the sunlight side of the Moon.