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Glossary term: G 型星

Description: 光谱类型为"G"的恒星。天文学家通过识别电离钙的强吸收线来确定G型恒星;更广泛地说,G型恒星中的金属吸收线比更热的恒星(如F型恒星)更强,而比更冷的恒星(如K型恒星)更弱。G型恒星的典型(有效)温度在5200开尔文(K)到6000 K之间。与其他恒星相比,它们对人类肉眼呈现出黄色,除非存在显著的星际或大气层红化现象。处于主序阶段的G型恒星,即通过核聚变在核心区域将氢转化为氦的恒星,被称为黄矮星。太阳就是一个典型的G型黄矮星例子。

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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

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Related Diagrams

一颗 G 型恒星的光谱

Caption: G 型恒星 UCAC4 700-069569 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。在 400 纳米以下和 700 纳米以上,人眼几乎看不到光,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 G 型恒星中,氢原子的光谱线比 F 型恒星弱,而电离钙的光谱线则比 F 型恒星强。铁、钠和钙等金属原子的谱线也开始变得突出。
Credit: IAU OAE/SDSS/Niall Deacon

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