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A star's lifetime commences with the gravitational collapse of a gaseous nebula of fabric largely comprising hydrogen, helium, and traces of heavier components. Its total mass largely establishes its evolution and eventual fate. A star shines for many of its Energetic lifetime due to the thermonuclear fusion of hydrogen into https://websitewordpress50470.humor-blog.com/36441435/how-star-can-save-you-time-stress-and-money

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