Glossary term: 主序
Description: 主序是赫羅圖上一個細長的恆星群,其上的恆星處於主要的氫聚變演化階段。除質量最小的恆星以外,其他恆星在完成核心氫聚變後都會脫離主序,開始進入巨星階段的演化。主序上的恆星通常被稱為矮星,以區別於巨星。主序上的熱恆星比主序上的冷恆星更亮。最熱的恆星消耗氫的速度很快,因此通常只在主序上停留幾百萬年。像太陽這樣的恆星在主序上的時間約為百億年,而較冷的恆星在主序上保持穩定氫聚變的時間甚至更長。
Related Terms:
See this term in other languages
Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher The translation of this term and its definition is still awaiting approval
This is an automated transliteration of the simplified Chinese translation of this term
The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".
Related Diagrams
赫羅圖
Credit: IAU OAE/Niall Deacon
License: CC-BY-4.0 Creative Commons 姓名標示 4.0 國際 (CC BY 4.0) icons