(a) Find the total power radiated into
bc 7 s.* )aer*iwrbn3 kxve9;kspace by the Sun, assuming it to be a perfec
.wexvn3 *resc)7kk*rb a;b9it emitter at $T\,=\,5500K$ 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$