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G-type stars, like the sun, will generally go through their main sequence, growing brighter all the time, until they expand to red giants, followed by a helium flash (or possibly several flashes), followed by the shedding of the outer layers of the star, at which time a slowly cooling white dwarf remains, which should, given enough time, cool enough to become a black dwarf.

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11y ago
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Q: What is the life cycle of a sunlike star?
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