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How does a high-mass star differ from a low-mass star as both enter the final stages of their life cycle?
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The difference is that according to Chandrashekhar Limit, if the start has the mass more than 1.4 times mass of the sun, it'll blast into supernova and will eventually make a black hole but if it has less mass than that, it'll be convert into a a white dwarf and will eventually die.
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