太阳系外行星HD 189733b的地面近红外辐射频谱
Mark R Swain1, Pieter Deroo, Caitlin A Griffith
1Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109-8099, USA. mark.r.swain@jpl.nasa.gov
Nature
|February 5, 2010
概括
基于地面的红外光谱检测了系外行星HD 189733b中的甲 (CH(4) 排放. 这表明非局部热力学平衡 (非LTE) 效应对于理解热木星大气至关重要.
科学领域:
- 外行星科学是外行星的科学.
- 大气光谱学是大气光谱学.
- 天体化学是天体化学.
背景情况:
- 红外光谱是分析系外行星大气层的关键.
- 之前的研究已经在热木星中检测到水,甲,二氧化碳和二氧化碳.
- 空间望远镜所覆盖的光谱区域存在限制.
研究的目的:
- 报告从地面观测HD 189733b系外行星的日光辐射频谱.
- 为了研究以前基于太空的观测中未涵盖的光谱区域.
- 为了识别分子特征和大气条件.
主要方法:
- 使用地面望远镜进行红外观测.
- 收集了HD 189733b在2.0-2.4和3.1-4.1微米之间的辐射频谱数据.
- 结果与现有的基于空间的测量结果进行了比较.
主要成果:
- 在观察到的光谱中检测到一个明亮的发射特征.
- 确认了在重叠区域进行空间测量的协议.
- 在3.25微米左右观察到一个意想不到的特征.
结论:
- 3.25微米的特征很可能是由于非局部热力学平衡 (非LTE) 甲 (CH4) 排放.
- 这一发现挑战了假设外行星大气层局部热力学平衡 (LTE) 的模型.
- 在解释来自强烈辐射系外行星的数据时,必须考虑非LTE效应.
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