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A star's life starts Using the gravitational collapse of a gaseous nebula of fabric mostly comprising hydrogen, helium, and traces of heavier components. Its overall mass mainly establishes its evolution and eventual destiny. A star shines for most of its active lifetime as a result of thermonuclear fusion of hydrogen https://historyofjudo83603.blogrenanda.com/44335468/hotel-bangkok-things-to-know-before-you-buy

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