In stars, fusion continues beyond H+H = He. As the star converts to a majority of He, what other particles can also be formed if He and H both exist in the star? After those two particles are formed and the He/H is running out? What other particles can form from fusing the two newer/newest particles and with H, He and the second set of particles. What "Heavy" atom signifies the dead end of solar fusion and then the star might go Nova?

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In stars, fusion continues beyond H+H = He. As the star converts to a majority of He, what other
particles can also be formed if He and H both exist in the star? After those two particles are formed
and the He/H is running out? What other particles can form from fusing the two newer/newest
particles and with H, He and the second set of particles.
What "Heavy" atom signifies the dead end of solar fusion and then the star might go Nova?
Transcribed Image Text:In stars, fusion continues beyond H+H = He. As the star converts to a majority of He, what other particles can also be formed if He and H both exist in the star? After those two particles are formed and the He/H is running out? What other particles can form from fusing the two newer/newest particles and with H, He and the second set of particles. What "Heavy" atom signifies the dead end of solar fusion and then the star might go Nova?
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