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In the cores of red giants, helium burning begins once temperatures exceed 108 K, converting helium into carbon and subsequently into oxygen, neon, and magnesium.
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In the cores of red giants, helium burning begins once temperatures exceed 108 K, converting helium into carbon and subsequently into oxygen, neon, and magnesium.
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Related words
helium burning
Noun
uncountable
Japanese Meaning
ヘリウム燃焼:物理学・天文学において、10⁸Kを超える温度の星内で、ヘリウムが核融合によりまず炭素に変換され、その後酸素、ネオン、マグネシウムへと変わる核合成プロセスを指す。
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