Transiting exoplanet atmospheres in the era of JWST
EMR Kempton, HA Knutson - Reviews in Mineralogy …, 2024 - pubs.geoscienceworld.org
The field of exoplanet atmospheric characterization has recently made considerable
advances with the advent of high-resolution spectroscopy from large ground-based …
advances with the advent of high-resolution spectroscopy from large ground-based …
No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c
Seven rocky planets orbit the nearby dwarf star TRAPPIST-1, providing a unique opportunity
to search for atmospheres on small planets outside the Solar System. Thanks to the recent …
to search for atmospheres on small planets outside the Solar System. Thanks to the recent …
From stars to diverse mantles, melts, crusts, and atmospheres of rocky exoplanets
CM Guimond, H Wang, F Seidler… - … in Mineralogy and …, 2024 - pubs.geoscienceworld.org
The advent of radial velocity (RV) and transit photometry method has resulted in the
detection of more than 5000 exoplanets since 1995. Of these detected planets, a significant …
detection of more than 5000 exoplanets since 1995. Of these detected planets, a significant …
[HTML][HTML] The 2024 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres
The ExoMol database (www. exomol. com) provides molecular data for spectroscopic
studies of hot atmospheres. These data are widely used to model atmospheres of …
studies of hot atmospheres. These data are widely used to model atmospheres of …
Potential Atmospheric Compositions of TRAPPIST-1 c Constrained by JWST/MIRI Observations at 15 μm
Abstract The first James Webb Space Telescope observations of TRAPPIST-1 c showed a
secondary eclipse depth of 421±94 ppm at 15 μm, which is consistent with a bare rock …
secondary eclipse depth of 421±94 ppm at 15 μm, which is consistent with a bare rock …
Constraining the thickness of TRAPPIST-1 b's atmosphere from its JWST secondary eclipse observation at 15 μm
J Ih, EMR Kempton, EA Whittaker… - The Astrophysical …, 2023 - iopscience.iop.org
Recently, the first JWST measurement of thermal emission from a rocky exoplanet was
reported. The inferred dayside brightness temperature of TRAPPIST-1 b at 15 μm is …
reported. The inferred dayside brightness temperature of TRAPPIST-1 b at 15 μm is …
Mapping out the parameter space for photoevaporation and core-powered mass-loss
JE Owen, HE Schlichting - Monthly Notices of the Royal …, 2024 - academic.oup.com
Understanding atmospheric escape in close-in exoplanets is critical to interpreting their
evolution. We map out the parameter space over which photoevaporation and core-powered …
evolution. We map out the parameter space over which photoevaporation and core-powered …
Observability of silicates in volatile atmospheres of super-Earths and sub-Neptunes-Exploring the edge of the evaporation desert
Many of the confirmed short-period super-Earths and smaller sub-Neptunes are sufficiently
irradiated for the surface silicates to be sustained in a long-lasting molten state. While there …
irradiated for the surface silicates to be sustained in a long-lasting molten state. While there …
TESS Hunt for Young and Maturing Exoplanets (THYME). XI. An Earth-sized Planet Orbiting a Nearby, Solar-like Host in the 400 Myr Ursa Major Moving Group
BK Capistrant, M Soares-Furtado… - The Astronomical …, 2024 - iopscience.iop.org
Young terrestrial worlds are critical test beds to constrain prevailing theories of planetary
formation and evolution. We present the discovery of HD 63433 d—a nearby (22 pc), Earth …
formation and evolution. We present the discovery of HD 63433 d—a nearby (22 pc), Earth …
The Character of M Dwarfs
TJ Henry, WC Jao - Annual Review of Astronomy and …, 2024 - annualreviews.org
M dwarfs dominate the stellar population, accounting for three of every four stars, the nearest
of which is Proxima Centauri, the closest destination beyond our Solar System. These cool …
of which is Proxima Centauri, the closest destination beyond our Solar System. These cool …