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After the main sequence phase, a star's fate depends on its mass. Medium-sized stars, like the Sun, expand into red giants, eventually shedding their outer layers to form a planetary nebula, leaving behind a white dwarf. Massive stars, on the other hand, undergo a more dramatic transformation, leading to supernova explosions and potentially resulting in neutron stars or black holes. This post-main sequence evolution significantly influences the chemical composition of the universe and the formation of new stars.

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2w ago

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