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 …
[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 …
JWST-TST DREAMS: quartz clouds in the atmosphere of WASP-17b
Clouds are prevalent in many of the exoplanet atmospheres that have been observed to
date. For transiting exoplanets, we know if clouds are present because they mute spectral …
date. For transiting exoplanets, we know if clouds are present because they mute spectral …
Awesome SOSS: atmospheric characterization of WASP-96 b using the JWST early release observations
The newly operational JWST offers the potential to study the atmospheres of distant worlds
with precision that has not been achieved before. One of the first exoplanets observed by …
with precision that has not been achieved before. One of the first exoplanets observed by …
A mini-chemical scheme with net reactions for 3D general circulation models-II. 3D thermochemical modelling of WASP-39b and HD 189733b
Context. The chemical inventory of hot Jupiter (HJ) exoplanet atmospheres continues to be
observed by various ground-and space-based instruments in increasing detail and …
observed by various ground-and space-based instruments in increasing detail and …
Stratospheric dayside-to-nightside circulation drives the 3D ozone distribution on synchronously rotating rocky exoplanets
Determining the habitability and interpreting future atmospheric observations of exoplanets
requires understanding the atmospheric dynamics and chemistry from a 3D perspective …
requires understanding the atmospheric dynamics and chemistry from a 3D perspective …
Global Chemical Transport on Hot Jupiters: Insights from the 2D VULCAN Photochemical Model
The atmospheric dynamics of tidally locked hot Jupiters is characterized by strong equatorial
winds. Understanding the interaction between global circulation and chemistry is crucial in …
winds. Understanding the interaction between global circulation and chemistry is crucial in …
Modelling the day–night temperature variations of ultra-hot Jupiters: confronting non-grey general circulation models and observations
ABSTRACT Ultra-hot Jupiters (UHJs) are natural laboratories to study extreme physics in
planetary atmospheres and their rich observational data sets are yet to be confronted with …
planetary atmospheres and their rich observational data sets are yet to be confronted with …
An extensively validated C/H/O/N chemical network for hot exoplanet disequilibrium chemistry
R Veillet, O Venot, B Sirjean, R Bounaceur… - Astronomy & …, 2024 - aanda.org
Context. The reliability of one-dimensional disequilibrium chemistry models in hot exoplanet
atmospheres depends on the chemical network used. To develop robust networks, we can …
atmospheres depends on the chemical network used. To develop robust networks, we can …
3D simulations of TRAPPIST-1e with varying CO2, CH4, and haze profiles
MT Mak, DE Sergeev, N Mayne, N Banks… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT Using a 3D General Circulation Model, the Unified Model, we present results
from simulations of a tidally locked TRAPPIST-1e with varying carbon dioxide CO2 and …
from simulations of a tidally locked TRAPPIST-1e with varying carbon dioxide CO2 and …