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When stars lose their outer layers, they primarily expel gas and dust, which can include hydrogen, helium, and heavier elements. This process often occurs during the later stages of a star's life, such as during a red giant phase or in supernova explosions. The ejected material contributes to the interstellar medium, enriching it with elements essential for the formation of new stars and planets. Additionally, the star may lose significant mass, affecting its gravitational pull and evolutionary path.

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1mo ago

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