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一个系外行星侵蚀大气中的
J J Spake1, D K Sing2,3, T M Evans2
1Department of Physics and Astronomy, University of Exeter, Exeter, UK. jspake@astro.ex.ac.uk.
Nature
|May 4, 2018
概括
科学家在一个系外行星上发现了
科学领域:
- 外行星科学
- 大气物理
- 光谱学
背景情况:
- 是宇宙中第二大元素.
- 理论模型预测可以在系外行星大气层中检测到.
- 之前对外行星的搜索一直没有成功.
研究的目的:
- 探测系外行星大气中的.
- 描述温暖的气体巨星WASP-107b的大气层.
主要方法:
- 测量了WASP-107b的近红外传输频谱.
- 确定了10833安格斯特罗姆激发转移稳定的的吸收特性.
主要成果:
- 报告了在系外行星上首次发现, 标准偏差值为4.5.
- 观察到一个显著的吸收特征 (0.049 ± 0.011%在98安格斯特罗姆带通过).
- 这种信号比恒星染色体活动的预期大五倍.
结论:
- WASP-107b有一个正在侵蚀的大气层.
- 太阳系外行星的大气层以每秒10^10到3x10^11克的速度逃逸.
- 逃逸的气体可能会形成由辐射压力形成的彗星状尾巴.
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