'Degenerate matter' diaporamas de présentation

Announcements

393 views • 31 slides

Stellar Evolution

Stellar Evolution. Chapter 12. Think, Pair, Share. Our sun started out as a: Protostar Class G star Neutron star Red giant star. Which stars are the most prevalent in the universe? Which are the least? How do stars sustain their fusion?

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Summary of Post-Main-Sequence Evolution of Sun-Like Stars

0. Summary of Post-Main-Sequence Evolution of Sun-Like Stars. Core collapses; outer shells bounce off the hard surface of the degenerate C,O core. Formation of a Planetary Nebula. Fusion stops at formation of C,O core. C,O core becomes degenerate. M < 4 M sun. 0.

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Neutron Star

183 views • 8 slides