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地球外行星LHS 3844b没有厚厚的大气层
Laura Kreidberg1, Daniel D B Koll2, Caroline Morley3
1Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA. laura.kreidberg@cfa.harvard.edu.
Nature
|August 21, 2019
概括
围绕小恒星运行的热型地球系外行星可能缺乏厚厚的大气层. 对LHS 3844b的新观测显示了光的岩石表面,这表明由于恒星风和高温而造成的大气侵蚀.
科学领域:
- 外行星科学
- 大气物理
- 恒星天体物理学
背景情况:
- 大多数已知的地球系系外行星围绕小恒星运行, 理论上它们更容易受到大气损失的影响.
- 之前对55 Cancrie系外行星的研究表明, 基于它的热相曲线,
- 在围绕M矮星运行的系外行星上研究大气保留对于了解行星可居住性至关重要.
研究的目的:
- 测量系外行星LHS 3844b的热相曲线以评估其大气特性.
- 为了确定LHS 3844b,一个小的陆地系外行星,是否保留了大量的大气.
- 测试围绕小恒星运行的行星大气脆弱性的理论预测.
主要方法:
- 对系外行星LHS 3844b进行热相曲线观测.
- 分析了相位变化以推断白天和夜晚的温度.
- 使用大气和裸岩场景来限制大气压力和光度.
主要成果:
- 发现LHS 3844b的相变是对称的,幅度很大.
- 确定白天亮度温度为1,040±40K,夜间亮度温度接近0K.
- 排除了厚厚的大气层 (表面压力> 10 bar);数据符合低度的裸岩模型.
结论:
- LHS 3844b的表面很可能是赤裸的岩石,几乎没有大气层.
- 围绕小恒星运行的热陆地行星容易受到恒星风带来的大气侵蚀.
- 这些发现支持预测M矮星周围系外行星大气损失的理论模型.
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