太阳系外行星大气的快速升温
Gregory Laughlin1, Drake Deming, Jonathan Langton
1UCO/Lick Observatory, University of California, Santa Cruz, California 95064, USA. laughlin@ucolick.org
Nature
|January 30, 2009
概括
天文学家观察到热木星系外行星HD 80606b在其最接近其恒星的过程中. 这个星球,这个星球的行星.
科学领域:
- 外系行星科学 外系行星科学
- 红外天文学 红外天文学
- 行星大气层的行星大气层
背景情况:
- 热木星系外行星是潮同步的,拥有面向恒星的永久半球.
- 具有离心轨道的行星允许直接测量全球变暖.
- HD 80606b的轨道极为偏离中心,因此非常适合研究潮加热效应.
研究的目的:
- 为了测量HD 80606b在周围恒星穿越期间的热辐射.
- 为了限制地球的大气特性和潮加热速度.
- 为了研究在极端辐射下系外行星大气的动态.
主要方法:
- 在周围的30小时间隔内进行8微米光度观测.
- 对亮度温度变化的分析.
- 检测二次日食以确定轨道倾斜和行星质量.
主要成果:
- 观察到亮度温度在六小时内从~800K快速增加到~1500K.
- 检测到一次次日食,暗示轨道倾斜接近90度.
- 在8微米光圈测量了4.5小时的辐射时间常数.
结论:
- HD 80606b由于其离心轨道而经历了显著的全球变暖.
- 这个星球的辐射时间常数比地球的平流层值要短得多.
- 这些发现提供了对高辐射系外行星大气动态的洞察.
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