冷酷的棕矮星 Gl 229B 的红外光谱
B R Oppenheimer1, S R Kulkarni, K Matthews
1Palomar Observatory, California Institute of Technology, Pasadena 91125, USA.
概括
对棕矮星Gl 229B的光谱分析显示了甲,类似于木星,但不是恒星. 这表明表面温度低于1000K,确认它比任何已知的恒星都冷.
科学领域:
- 天文学和天体物理学
- 外系行星科学 外系行星科学
背景情况:
- 棕矮星是星下物体,对其分类构成了挑战.
- 之前的观测缺乏冷棕矮星的大气特征的详细描述.
研究的目的:
- 用光谱分析冷酷的棕矮星 Gl 229B. 的大气层.
- 为了确定 Gl 229B. 的大气组成和温度.
主要方法:
- 使用近红外光谱测量吸收特征.
- 将光谱数据与已知的天体进行比较,包括木星和恒星.
主要成果:
- 在Gl 229B的光谱中检测到归因于甲的吸收特征.
- 这些甲特征与在木星观察到的相似,而不是典型的恒星.
- 水蒸气标志也表明表面温度显著低.
结论:
- Gl 229B 含有甲,证实了它的凉爽性质.
- 据估计,Gl 229B的表面温度低于1000凯尔文.
- Gl 229B代表了一个天体,比以前任何已知的恒星都更冷.
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