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The solar luminosity is a unit of luminosity ( power emitted in the form of photons) conventionally used by astronomers to give the luminosities of stars.It is equal to the luminosity of the Sun, which is 3.9 × 1026 W.
Calculating with this constant
You can calculate how much solar power hits the Earth by comparing a cross sectional area of the Earth and the total surface area of a sphere with a radius equal to the distance of the earth from the sun.
- The Earth's radius is 3963 miles (6,378 km).
- The Earth's cross sectional area = π×radius2 = 49.3 million square miles (128,000,000 km˛).
- The Sun's average distance is about 93 million miles (150,000,000 km).
- The surface area of a sphere = 4×π×radius2 = 1.09×1017 square miles (2.82×1017 km˛).
- Power reaching the Earth = P(total) × Area(earth)/Area(sphere) = 1.77×1017 W.
- The power hitting a square meter of area on Earth: (square meter = 1/16092 square miles)
- Power over square meter = P(total)(1/16092)/area(sphere) = 1387 W (the solar constant)
- Estimates have been made that humans use about 12×1012 W.
- How much land area would be needed to power that?
- The best solar cells can produce about 33% efficiency.
- Area needed = 12×1012/1387/0.33 = 26×19 m2 = 10122 square miles ~100×100 mile square. (More needed since Sun not always straight over head nor always sunny skies, and also some fraction radiation does not reach the surface.)
Luminosity
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