The sun is hugely important for life on Earth. It has total power output of around 3.8 Ă— 1026 W. The fact that the Earth's temperature is not constantly increasing (barring current global warming) means that the energy arriving from the sun is radiated back into space - it is at thermal equilibrium.
It can be calculated that the total power transferred to the Earth from the sun is 1.68 x 1017 W
Given the surface area of the Earth is 510.1 million km2, and its emissivity is 1, the average global temperature of the Earth, that corresponds to this amount of radiation being emitted is: T = 276 C
T = 276 K
T = 376 K
T = 245 K