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THE ATMOSPHERES OF EXTRASOLAR PLANETS

机译:外辐射行星的气氛

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The characteristics of irradiated solar system planetary at-mospheres have been studied for decades. Modern planetary science benefits from an exhaustive body of ground- and space-based data. The study of extrasolar planetary atmospheres, by contrast, is in its infancy and currently rests on a few score of datapoints, mostly of the transiting planets. As the study of exoplanetary atmospheres blossoms, it is well worth remembering lessons learned from the solar system. In this contribution, based on my Les Houches lecture on exoplanet at-mospheres, I briefly review a few of the key concepts relevant to under-standing planetary atmospheres and point to examples both in our own solar system and among the exoplanets. This short survey aims not to review the field but rather stresses the importance of understanding the structure, dynamics, cloud processes and photochemistry of plane-tary atmospheres and points the reader towards useful reference works. Here I particularly explain the importance of cloud and photochemical processes in controlling the spectra arid albedos of extrasolar planets and urge that care be taken in the interpretation of exoplanet colors.
机译:几十年来研究了辐照太阳能系统行星行星静脉内的特点。现代行星科学受益于基于空间和空间的详尽的数据。相比之下,通过对比的辐射行星氛围的研究在其初期,目前依赖于分数的DataPoints,大多是过渡行星。作为对外部化环境的研究开花,值得记载从太阳系中吸取的经验教训。在这一贡献中,根据我的Les Houches在Exoplanet at-Moplanes的讲座,简要审查了一些与常设行星大气相关的关键概念,并在我们自己的太阳系和外产上的例子中指出。这项短暂的调查旨在不审查该领域,而是强调了了解平面大气的结构,动态,云流程和光明性的重要性,并将读者指向有用的参考作品。在这里,我特别解释了云和光化学过程在控制外散行星的光谱和敦促促进外产色彩的解释中的思考的重要性。

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