JWST 时代的凌日系外行星大气层

Eliza M.-R. Kempton, Heather A. Knutson
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引用次数: 0

摘要

随着大型地面望远镜高分辨率光谱技术的出现和詹姆斯-韦伯太空望远镜(JWST)的投入使用,系外行星大气表征领域最近取得了长足的进步。我们已经进入了一个可以对大气成分、气溶胶特性、热结构、质量损失和三维效应进行可靠约束的时代。虽然遥感技术所面临的挑战意味着单个系外行星大气的特征可能永远无法达到太阳系天体所能达到的详细程度,但系外行星提供了一个令人兴奋的机会,可以对具有太阳系天体所没有的特性的各种世界进行特征描述...
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Transiting Exoplanet Atmospheres in the Era of JWST
The field of exoplanet atmospheric characterization has recently made considerable advances with the advent of high-resolution spectroscopy from large ground-based telescopes and the commissioning of the James Webb Space Telescope (JWST). We have entered an era in which atmospheric compositions, aerosol properties, thermal structures, mass loss, and three-dimensional effects can be reliably constrained. While the challenges of remote sensing techniques imply that individual exoplanet atmospheres will likely never be characterized to the degree of detail that is possible for solar system bodies, exoplanets present an exciting opportunity to characterize a diverse array of worlds with properties that are not represented...
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