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The energy produced, which eventually works its way to the surface and gets emitted as light, balances the inward pull of gravity to keep the star stable. Eventually the star runs out of hydrogen fuel, however, and gravity starts to crush the core, raising the star’s internal temperature. After a while, this triggers new fusion reactions, creating carbon, oxygen, and the other elements essential to life. For the largest stars, this process continues until iron forms in the core. But fusing iron requires more energy than it produces, so the reactions can no longer hold off the inward pull of gravity. The core then collapses, causing the star to explode and spew its heavy elements back into the galaxy, where they can be incorporated into future generations of stars, planets, and perhaps even life. |
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