Energy from the Sun received at the Earth cross section

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SUMMARY

The discussion focuses on calculating the energy received by Earth from the Sun, emphasizing the importance of understanding the geometry involved. The correct approach involves using the formula for the area of a circle, πR², where R is the radius of the Earth, to determine the cross-sectional area that the Sun "sees." This method is preferred over using half the surface area of the Earth, as the Sun emits energy uniformly in all directions and the relevant factor is the solid angle subtended by the Earth at the Sun.

PREREQUISITES
  • Understanding of basic geometry, specifically the area of a circle.
  • Familiarity with the concept of solid angles in physics.
  • Knowledge of the Earth's radius and its significance in calculations.
  • Basic principles of solar energy and its distribution.
NEXT STEPS
  • Study the concept of solid angles and how they relate to energy distribution from a point source.
  • Learn about the geometry of spheres and their projections, particularly in relation to light and shadow.
  • Explore the calculations involved in solar energy received at different distances, such as 1 AU.
  • Investigate the effects of angle of incidence on energy absorption in various contexts.
USEFUL FOR

Students in physics or astronomy, educators teaching energy concepts, and anyone interested in understanding solar energy calculations and their geometric implications.

Puchinita5
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Homework Statement



My homework involves calculating the amount of energy the Earth receives from the Sun in a given year. I actually have the answer, but what I'm confused with is that the calculation says that the Sun "sees the cross section of the Earth, a circle". So in the calculation, we multiply the energy per square meter received at 1AU by pi*R^2 (R is the radius of the Earth).

Why isn't it multiplied by half of the surface area of Earth? I picture half of the Earth facing the sun as the surface receiving the energy. So I would think to multiply by 2*pi*r^2.

Homework Equations

The Attempt at a Solution

 
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Hi.

##\pi r^2## is the area of a circle. That's what the sun 'sees'.

You seem to be thinking of half a sphere, but then
  1. a sphere has area ##{4\over 3} \pi r^2##
  2. the angle of incidence has to be corrected for -- which brings you back to ##\pi r^2##
Make a little sketch showing this angle of incidence

Or check the shadow of a sphere on a wall !
 
Puchinita5 said:
Why isn't it multiplied by half of the surface area of Earth?
Because the Sun doesn't care what shape the Earth is. It sends out the same power per unit solid angle in all directions. The power the Earth gets is proportional to the solid angle it subtends at the Sun.
 

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