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A star's lifetime begins with the gravitational collapse of a gaseous nebula of material largely comprising hydrogen, helium, and traces of heavier factors. Its total mass primarily determines its evolution and eventual fate. A star shines for many of its active life a result of the thermonuclear fusion of hydrogen https://edwinggifj.snack-blog.com/37836350/indicators-on-hotel-transylvania-you-should-know

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