Transiting Exoplanet Atmospheres in the Era of JWST
Eliza M.-R. Kempton, Heather A. Knutson

TL;DR
This review discusses recent advances in exoplanet atmospheric characterization enabled by JWST and high-resolution spectroscopy, highlighting new insights into planetary composition, structure, and diversity.
Contribution
It provides a comprehensive overview of the first year of JWST exoplanet data and recent high-resolution spectroscopy results, emphasizing their impact on understanding exoplanet atmospheres.
Findings
JWST has significantly advanced atmospheric studies of transiting exoplanets.
High-resolution spectroscopy reveals detailed atmospheric compositions.
Exoplanet diversity extends beyond solar system analogs.
Abstract
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 in our solar system. This review article summarizes the current state of exoplanet atmospheric studies for transiting planets. We focus on how observational results inform…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
