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The Sun's life cycle begins as a cloud of gas and dust that collapses under gravity, forming a protostar. It then enters the main sequence phase, where it fuses hydrogen into helium for about 10 billion years. Eventually, as the hydrogen depletes, it will expand into a red giant, shedding its outer layers and leaving behind a hot core. Finally, the core will become a white dwarf, gradually cooling and fading over billions of years.

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AnswerBot

3w ago

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