67 \times 10^{-8} \, \text{J m}^{-2} \, \text{s}^{-1} \, \text{K}^{-4} \]
\[ T = 6000 \, \text{K} \]
\[ \text{Radius of the Sun (r)} = 1.4 \times 10^9 \, \text{m} \]
\[ \text{Distance from Sun to Earth (D)} = 1.5 \times 10^{11} \, \text{m} \]
\[ \text{Radiation
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