Sun Losing Mass due to Energy Radiation

AI Thread Summary
The discussion focuses on calculating the mass loss of the sun due to energy radiation, given the solar constant of 1400 W/m² at Earth's distance. The initial approach involves using the formula Ei = E/r² to find the total energy output of the sun. To determine mass loss, the total energy output is then divided by c² using E=mc². The key point of confusion lies in calculating the total area over which the sun's energy spreads at Earth's distance. Understanding this area is crucial for accurately determining the sun's mass loss per second.
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Homework Statement



Energy from the sun (distance 1.496 x 10^11m from earth) arrives at the Earth at a rate of 1400W/m^2. How fast is the sun losing mass due to energy radiation?

Homework Equations





The Attempt at a Solution



Ok so i thought that Ei = E/r^2 where Ei is incident radiation and E is radiation at source..

Therefore E sun = r^2 (1400)

Then using E=mc^2..I divide the result by c^2 to give mass loss per second..

but i don't get the right answer..where am i going wrong?
thanks
 
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The solar constant specifies how much power sun light contains per square meter at our distance from the sun. To get the total power output of the sun light you would then need to know "how many" square meters there are all around the sun at our distance from it.
 
You are given the power per unit area at a certain distance from the sun. What's the total area over which the sun's energy is spread at that distance? (You're almost there.)
 
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