最終更新日：2025/11/21
Hydrogen burning in stars under 1.2 solar masses primarily fuels the conversion of hydrogen into helium, deuterium, and traces of lithium, shaping their long-term structure and evolution.
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Hydrogen burning in stars under 1.2 solar masses primarily fuels the conversion of hydrogen into helium, deuterium, and traces of lithium, shaping their long-term structure and evolution.
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