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A medium-sized main sequence star, like our Sun, goes through several stages in its life cycle. It starts as a protostar, forming from a cloud of gas and dust, and then enters the main sequence phase where it fuses hydrogen into helium in its core, maintaining stability for billions of years. Once it exhausts its hydrogen supply, it evolves into a red giant, eventually shedding its outer layers to create a planetary nebula. The remaining core then becomes a white dwarf, which will gradually cool and fade over time.

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