来自太阳系外行星的红外辐射
Drake Deming1, Sara Seager, L Jeremy Richardson
1Planetary Systems Laboratory and Goddard Center for Astrobiology, Code 693, NASA's Goddard Space Flight Center, Greenbelt, Maryland 20771, USA. Leo.D.Deming@nasa.gov
Nature
|March 24, 2005
概括
天文学家检测到来自热木星HD 209458b的红外辐射,证实它是由它的恒星加热的. 这一发现表明,这颗行星可能具有圆形轨道,挑战了以前关于其大尺寸的理论.
科学领域:
- 天文学和天体物理学
- 外系行星科学 外系行星科学
背景情况:
- 热木星是气态巨星系外行星,它们的轨道非常靠近它们的恒星.
- 预计这些行星很热,会发出红外辐射.
- HD 209458b是一个异常大半径的系外行星,可能是由于潮消散需要轨道偏心.
研究的目的:
- 为了检测和描述来自系外行星HD 209458b的红外辐射.
- 研究HD 209458b的热辐射及其对轨道动态的影响.
主要方法:
- 在HD 209458b的次日食期间观察红外流量 (24微米) 的减少.
- 分析二次日食相对于行星过境的时间.
主要成果:
- 直接检测来自HD 209458b (55 +/- 10 microJy) 的24微米红外辐射.
- 测量的亮度温度为1.130 +/- 150 K,与恒星辐射相一致.
- 二次日食的时间表明近圆轨道,这与需要显著轨道偏心的理论相矛盾.
结论:
- 检测到的红外辐射证实了HD 209458b显著的恒星升温.
- 二次日食的精确时间表明HD 209458b的轨道偏心在动态上是微不足道的.
- 这挑战了对行星大半径的解释,这些解释依赖于由轨道偏心驱动的潮消散.
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