Question

During the helium flash a star generates a very large amount of energy and pressure over...

During the helium flash a star generates a very large amount of energy and pressure over a very small time. What does this increase in pressure accomplish within the star?

When a low mass star first develops an inert carbon core what elements (if any) are still burned within the star?

What is the final element generated in the core of high mass stars? (Hint: fusion of this element releases no energy)

Where are the heaviest elements formed? (All elements above Iron)

Type I Supernova only occur under certain conditions in a binary star system. What state must each of the two stars be in for a type I Supernova to occur?

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