Nucleosynthesis in Supernovae

Nucleosynthesis in supernovae is the process where new, heavier elements are created during the explosion of a dying star. When a massive star exhausts its fuel, it collapses and triggers a supernova, releasing enormous energy. The intense heat and pressure cause nuclei of lighter elements, like hydrogen and helium, to fuse into heavier elements such as iron, nickel, and other metals. These newly formed elements are then scattered into space, enriching the universe and providing the building blocks for planets, life, and future stars. This process is a key contributor to the chemical diversity observed in the cosmos.