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A star's daily life commences with the gravitational collapse of a gaseous nebula of material mainly comprising hydrogen, helium, and traces of heavier factors. Its full mass primarily decides its evolution and eventual fate. A star shines for many of its active lifestyle due to the thermonuclear fusion of hydrogen https://bangkokwax57913.popup-blog.com/36612198/hotel-engine-things-to-know-before-you-buy

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