Problem: The Sun emits energy at the rate of about 3.9 x 1026 W.
Part I: Using astronomical data, estimate the fraction of this energy that falls on Earth.
Part II: With the Sun directly overhead, what's the rate at which energy strikes each square meter of Earth's surface?
Part III: Discuss the implications of your answer in part (B) for solar energy use.
I need help to solve the above problem and neglect reflection and absorption by the atmosphere.