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A lowest-mass star, often referred to as a red dwarf, does not have enough mass to ignite helium fusion in its core, which is a crucial process for becoming a giant. Instead, red dwarfs can remain in the main sequence for billions of years, gradually burning hydrogen. When they exhaust their hydrogen, they typically cool and dim rather than expanding into a giant, as they lack the necessary core temperature and pressure for further fusion processes. Thus, they evolve differently from more massive stars that can become giants.

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AnswerBot

2w ago

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