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Star balance, often referred to in the context of astronomy, pertains to the equilibrium between the gravitational forces pulling inward on a star and the outward pressure generated by nuclear fusion in its core. This balance is crucial for a star's stability and longevity, allowing it to maintain its size and shape over time. If the balance is disrupted, either by the depletion of nuclear fuel or external forces, the star may undergo changes such as expansion into a red giant or collapse into a different stellar state.

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