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单词 post-main sequence
释义

post-main sequence

Astronomy
adjective
Designating a star which is too old to lie within the main sequence on a Hertzsprung-Russell diagram, i.e. one which no longer has hydrogen fusion at its core and is relatively cool or dim, such as red giant.

Origin

1960s; earliest use found in Science.

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更新时间:2024/11/14 4:34:47