CES 영어사전

Supercloud

발음 발음 정보 없음 · 품사 명사 (noun)

가장 먼저 보는 뜻

한국어 뜻

검증된 한국어 뜻을 준비 중입니다. 확인되지 않은 자동 번역은 표시하지 않습니다.

영어 정의

(astronomy) A very large cloud of stellar material..

예문

There is, however, a significant difference between the contraction of the stars of a cluster from the original gas cloud, and the contraction of whole galaxies from the supercloud that gives rise to a group or galaxies. While the stellar cluster cloud fragments into stars, the turbulence in the contracting supercloud fragments it into pieces which themselves are further subdivided, and galaxies are formed by the gradual attachment of smaller pieces to one another. The rotational property of the Galaxy is explained by the original relative motions of the constituent pieces, and the more compact the Galaxy became, the more marked would be the effect of its original angular momentum; the flatness of the disc is a result of this rotation.
“Regular strings of H II regions and superclouds in spiral galaxies: clues to the origin of cloudy structure.”
The molecular component of the interstellar medium is observed to be fragmented at all scales ranging from that of the supercloud complexes to that of the protostellar cores, forming a hierarchy which is not self-similar.

단어 변화형

관련 단어

Supercloud 사용 팁

supercloud의 의미, 어조와 문법이 전체 문장에 맞을 때 사용하세요. 동의어라도 모든 문장에서 바로 바꿔 쓸 수 있는 것은 아닙니다.

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자주 묻는 질문

supercloud의 뜻은 무엇인가요?

현재 검증된 한국어 뜻은 준비 중이며 영어 정의는 “(astronomy) A very large cloud of stellar material.”입니다.

supercloud의 동의어는 무엇인가요?

문장 속 의미에 따라 가까운 동의어가 달라집니다.

supercloud의 반의어는 무엇인가요?

정확한 반대말은 사용된 의미에 따라 달라집니다.

supercloud를 문장에서 어떻게 쓰나요?

There is, however, a significant difference between the contraction of the stars of a cluster from the original gas cloud, and the contraction of whole galaxies from the supercloud that gives rise to a group or galaxies. While the stellar cluster cloud fragments into stars, the turbulence in the contracting supercloud fragments it into pieces which themselves are further subdivided, and galaxies are formed by the gradual attachment of smaller pieces to one another. The rotational property of the Galaxy is explained by the original relative motions of the constituent pieces, and the more compact the Galaxy became, the more marked would be the effect of its original angular momentum; the flatness of the disc is a result of this rotation.

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