Iron is the most tightly bound nucleus in nature, and unlike fusion reactions up to iron which release energy, fusing iron absorbs energy. When a star's core reaches iron, it loses all outward pressure support and collapses catastrophically in less than a second, forming a neutron star about 20 km in diameter from a core of 1.4 solar masses, while the outer layers bounce off this rigid surface and create a shockwave that triggers a supernova explosion.
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Iron Kills the Star That Made ItAñadido:
Iron is the most tightly bound nucleus in nature. Every reaction up to iron releases energy, and that energy is what holds the star up against gravity.
Fusing iron doesn't release energy, it absorbs it. The furnace doesn't slow down, it reverses. What follows takes less than a second. The iron core, about 1.4 solar masses packed into a volume the size of Earth, loses all outward pressure support. It collapses. In under a quarter of a second, that core crushes down to a sphere roughly 20 km across, a neutron star. Protons and electrons smash together into neutrons by raw gravitational compression.
The outer layers, still falling inward, slam into this suddenly rigid surface.
They bounce. A shockwave rips outward through every layer of the onion at tens of thousands of kilometers per second.
For a limited time only, we are giving out the first three chapters of our complete introduction to stargazing, completely free. Check our channel profile for the link.
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