• eventually the star runs out of hydrogen to fuse, this breaks the equilibrium
• if the star is massive (larger than our sun)
o star swells into a red super giant – fusion of helium begins, elements up to iron are formed in the core
o then as the amount of fusion occurring increases the star begins to glow brightly again and expand, forming elements as heavy as iron – the star then explodes in a supernova
o forming elements heavier than iron and ejecting them into the universe to form planets and stars