Try it on paper first. A hint, the key idea and the worked solution are here when you need them.
The Sun radiates W. Find the mass that is turned into energy each second and in one year ( s). Four hydrogen atoms of mass u each make one helium-4 atom of mass u. Find the share of the hydrogen mass that becomes energy. Use m/s.
The electric potential energy of two nuclei that touch is MeV, with in fm and . The average kinetic energy of a particle in a gas is , with eV/K. The Sun's luminosity is W, and the energy that goes with a mass is .
Have you tried it?
Work it out on paper first. It is fine to get stuck or make a mistake: that is how we learn. When you are ready, go through the solution one step at a time, and check each step against your own.
Step 1. Each second. kg.
Step 2. In a year. kg.
Step 3. The share. The mass before is u. The mass lost is u. So the share is , which is .
Answer: kg each second, kg in a year, and .
Check. The Sun has a mass of kg, so the loss in a year is a tiny part of it, about . Over its life so far the Sun has lost only about of its mass as light.
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