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