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Dwarf stars, particularly red dwarfs, have long lifespans, often lasting tens to hundreds of billions of years due to their slow fusion rates. In contrast, larger stars, such as massive blue giants, burn through their nuclear fuel much more quickly, typically living only a few million years before exhausting their hydrogen and undergoing dramatic transformations, such as supernova explosions. The end stages for dwarf stars often lead to a stable white dwarf, while larger stars may end as neutron stars or black holes, depending on their mass. Overall, the life cycle of dwarf stars is characterized by stability and longevity, while larger stars experience rapid evolution and violent deaths.

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1mo ago

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