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A star's lifetime commences with the gravitational collapse of a gaseous nebula of material largely comprising hydrogen, helium, and traces of heavier components. Its total mass largely decides its evolution and eventual fate. A star shines for the majority of of its Energetic everyday living because of the thermonuclear fusion https://ota82592.blogprodesign.com/58968778/hotel-in-pattaya-things-to-know-before-you-buy

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