Chapter 10: The Deaths of Stars
-- Evolution off the main sequence (=> giant)
Degenerate Matter
Planetary Nebulae and White Dwarfs
Binary Star Evolution (Disks, Novae, etc.)
Massive Star Evolution and Supernovae
Q. Massive stars cannot generate energy through iron fusion because:
iron fusion requires very high densities.
stars contain very little iron.
no star can get high enough for iron fusion.
iron is the most tightly bound of all nuclei.
massive stars go supernova before they create an iron core