Why does the Sun keep shining for billions of years?
Nuclear fusion powers the Sun: follow hydrogen turning into helium, the slow reaction rate, stellar self-regulation and the finite fuel supply in the core.
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Nuclear fusion powers the Sun: follow hydrogen turning into helium, the slow reaction rate, stellar self-regulation and the finite fuel supply in the core.
A pendulum has stopped. Where did its energy go? Follow motion turning into internal energy, distinguish heat from stored energy and account for the whole system.