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A very low mass star can remain fully convective for billions of years, gradually fusing its hydrogen until only helium cores remain.
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A very low mass star can remain fully convective for billions of years, gradually fusing its hydrogen until only helium cores remain.
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Related words
very low mass star
Noun
Japanese Meaning
(天文学) 水素の核融合が可能な最小限の質量を有する星。全体が対流層となっており、その内部の水素を完全に燃焼・消費できる星
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