Energy Emitted from Earth
						§   The Stefan-Boltzmann Law     The energy flux emitted by a blackbody     is related to the fourth power of the body’s     absolute temperature     F = sT4   where s is 5.67x10-8 W/m2/K §   Energy emitted from the Earth     = (blackbody emission) x (total area of Earth)     = (sTe4 )  x  (4p R2Earth )