Loading...

Glossary term: F 型星

Description: 光谱类型为“F”的恒星。天文学家通过光谱中存在的中等强度的电离钙线和其他一些原子金属线以及微弱的氢吸收线来识别 F 型恒星。它们的典型(有效)温度大约在6000开尔文(K)到7400开尔文之间。与其他恒星相比,它们在人眼中呈现白色或黄白色,除非受到星际或大气的影响导致发红。北极星就是 F 型星的一个例子。

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

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

一颗 F 型恒星的光谱

Caption: F 型恒星 2MASS J22243289+4937443 的光谱。波长在 400 纳米到 700 纳米之间的光谱线的颜色大致与人眼看到的该波长光线的颜色一致。波长低于 400 纳米和高于 700 纳米时,人眼几乎看不到光,这两条光谱线分别被染成蓝色和红色。 黑线表示恒星大气中不同元素的原子和离子造成的光谱吸收线。这些原子和离子会吸收特定波长的光,从而在光谱中形成尖锐的暗线。这些线条的强度取决于恒星大气层的温度。如果两颗恒星的大气层温度不同,那么由相同元素混合而成的两颗恒星的光谱中可能会出现截然不同的光谱线。在 A 型恒星中最强的氢原子谱线在 F 型恒星中仍然相对较强,但金属(尤其是电离钙)谱线在这一光谱类型开始变得较强。
Credit: IAU OAE/SDSS/Niall Deacon

License: CC-BY-4.0 Creative Commons 署名 4.0 国际 (CC BY 4.0) icons