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A star's life starts with the gravitational collapse of the gaseous nebula of fabric mainly comprising hydrogen, helium, and traces of heavier aspects. Its full mass generally establishes its evolution and eventual fate. A star shines for most of its active lifetime mainly because of the thermonuclear fusion of hydrogen https://byd-atto-3-extended-range95825.blogdemls.com/37600476/top-guidelines-of-hotels-in-bangkok

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