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What is Evolution of the Sun about?

The Sun was once a massive star, significantly larger and brighter than it is today, but has since lost mass and brightness due to internal processes. It is currently in a stable phase that will last for another 10 billion years, during which it will convert hydrogen into helium. Eventually, the Sun will either undergo a rapid collapse leading to new thermonuclear reactions or a slow contraction, ultimately becoming a white dwarf star.

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