The process of losing their outer layers in stars is primarily driven by stellar winds and the nuclear fusion reactions occurring in their cores. As a star ages, it expands into a red giant and begins to shed its outer layers due to increased radiation pressure and thermal pulsations. This mass loss can lead to the formation of planetary nebulae in lower-mass stars or supernova explosions in more massive stars, ultimately influencing the star's evolution and the chemical enrichment of the surrounding space.
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