Dying Stars and the Birth of the Elements 2025

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After the hydrogen in a stars core is exhausted, the star fuses helium to form progressively heavier elements, such as carbon and iron. As this fuel runs out, the star either explodes into a supernova, seeding the universe with those elements, or violently collapses, creating neutron stars and black holes.
When the core runs out of hydrogen, these stars fuse helium into carbon just like the sun. However, after the helium is gone, their mass is enough to fuse carbon into heavier elements such as oxygen, neon, silicon, magnesium, sulfur and iron.
The expanding supernova remnant, rich with heavy elements, including mass injected by the now-dead stars giant and supergiant winds, finds its way back to the interstellar clouds. Its detritus becomes the material that will ultimately make new stars, thus completing the cycle.
But once their core has turned entirely to iron, no more fusion will happen there. The outward pressure drops and the tremendous gravity of these enormous stars takes over. Everything collapses inwards toward the core.
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