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The life cycle of a Sun-like star differs from that of massive and supermassive stars primarily in its lifespan and end state. A Sun-like star, like our Sun, has a stable life of about 10 billion years, eventually evolving into a red giant and shedding its outer layers to form a planetary nebula, leaving behind a white dwarf. In contrast, massive stars burn through their nuclear fuel much more quickly, leading to shorter lifespans of a few million years, and they end their lives in dramatic supernova explosions, potentially leaving behind neutron stars or black holes. Supermassive stars, which can be several times more massive than typical massive stars, also undergo supernova events but can create black holes with significantly larger masses, influencing their surrounding environments more profoundly.

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5d ago

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