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  • Why Iron Fusion Fails in Massive Stars: A Deep Dive
    Massive stars cannot generate energy through iron fusion because iron has the most stable nucleus of all elements. Here's why:

    * Nuclear Fusion Requires Energy Input: Fusion reactions release energy when lighter nuclei combine to form heavier ones. This energy release is due to the difference in binding energy per nucleon between the initial and final nuclei.

    * Iron's Binding Energy: Iron has the highest binding energy per nucleon of all elements. This means it's extremely stable, and fusing iron nuclei would actually *require* energy input, rather than releasing it.

    * Endothermic Reactions: Iron fusion reactions are endothermic – they absorb energy instead of releasing it. This makes them unfavorable in a stellar environment.

    The Implications:

    When a massive star runs out of lighter elements to fuse, it reaches the iron core. This iron core can no longer generate energy through fusion. The core collapses under its own gravity, leading to a catastrophic supernova explosion.

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