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A star is primarily affected by two opposing forces: gravitational force and radiation pressure. Gravitational force pulls the star's mass inward, trying to collapse it, while radiation pressure, generated by nuclear fusion reactions in the star's core, pushes outward. The balance between these forces determines the star's stability and lifecycle. If the balance is disrupted, it can lead to various evolutionary stages, including expansion into a red giant or collapse into a supernova.

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