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一个具有平流层的超热气体巨行星
Thomas M Evans1, David K Sing1, Tiffany Kataria2
1Astrophysics Group, School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, UK.
Nature
|August 4, 2017
概括
天文学家使用红外光谱检测到WASP-121b上的系外行星平流层. 这一发现证实了高辐射系外行星中平流层的存在,为大气组成和温度提供了洞察力.
科学领域:
- 外行星科学
- 大气物理
- 红外光谱学
背景情况:
- 星球大气层发射红外辐射, 显示化学成分和温度.
- 在高度辐射的系外行星中,温度随着高度的增加而增加的平流层可以形成.
- 由于恒星的变化和低光谱分辨率,此前有关系外行星平流层的说法面临挑战.
研究的目的:
- 在超热气体巨星WASP-121b上研究平流层的存在和特征.
- 在高辐射系外行星中提供平流层形成的观测证据.
主要方法:
- 获得了WASP-121b系外行星的近红外热辐射频谱.
- 分析光谱特征以识别分子气体并推断大气温度概况.
- 使用高准确度测量来克服之前的观察局限性.
主要成果:
- 探测到水蒸气的辐射, 证实存在一个系外行星的平流层在5-西格玛的信心.
- WASP-121b的平衡温度大约是2500克尔文.
- 这些发现表明恒星辐射在高海拔地区有显著的保留.
结论:
- 在WASP-121b上发现系外行星的平流层为这一现象提供了强有力的观测证据.
- 在高海拔地区保留的能量可能会被氧化物和氧化物等物种吸收.
- 这项研究提高了我们对极端系外行星大气动力学和化学的理解.
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