(a) Find the total power radiated into space
f o6,vo hr+br )ol(,prby the Sun, assuming it to be a perfect emitter
(6+ro ) bl,hv,pfoorrat $T\,=\,5500K$ The Sun’s radius is $7.0 \times10^{ 8}\,m$
$ \times10^{ 26}\,W$
(b) From this, determine the power per unit area arriving at the Earth, $1.5 \times10^{ 11}\,m$ away (Fig. 14–21).
$ \times10^{ 3}\,W/m^2$