pre-main-sequence star oor Koreaans

pre-main-sequence star

Vertalings in die woordeboek Engels - Koreaans

전주계열성

en
star in the stage when it has not yet reached the main sequence
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Geskatte vertalings

Vertoon algoritmies gegenereerde vertalings

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The astronomer Louis G. Henyey and his colleagues in the 1950s, showed that the pre-main-sequence star can remain in radiative equilibrium throughout some period of its contraction to the main sequence.
1950년대에 천문학자 루이스 G. 헤니에이와 그의 동료들은 어떤 별이 압축하여 주계열성으로 진화하기 전까지 일정 기간 동안 복사적 균형 상태를 유지한다는 것을 입증했다.WikiMatrix WikiMatrix
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