The Trappist-1 planets provide a unique opportunity to test the current understanding of
rocky planet evolution. The James Webb Space Telescope is expected to characterize the …

JWST secondary eclipse observations of Trappist-1b seemingly disfavor atmospheres>∼ 1
bar since heat redistribution is expected to yield dayside emission temperature below the∼ …

Abstract The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI) project was
initiated to compare 3D climate models that are commonly used for predicting theoretical …

The era of atmospheric characterization of terrestrial exoplanets is just around the corner.
Modeling prior to observations is crucial in order to predict the observational challenges and …

Determining the habitability and interpreting atmospheric spectra of exoplanets requires
understanding their atmospheric physics and chemistry. We use a 3-D coupled climate …

M and K dwarf stars make up 86% of the stellar population and host many promising
astronomical targets for detecting habitable climates in the near future. Of the two, M dwarfs …

We have shown in a recent study, using 3D climate simulations, that dayside land cover has
a substantial impact on the climate of a synchronously rotating temperate rocky planet such …

Planets in synchronous rotation around low-mass stars are the most salient targets for
current ground-and space-based missions to observe and characterize. Such model …

ABSTRACT A planet's surface conditions can significantly impact its climate and habitability.
In this study, we use the 3D general circulation model exoplasim to systematically vary …

Rocky exoplanets orbiting in the habitable zone (HZ) of nearby M dwarfs provide unique
opportunities for characterizing their atmospheres and searching for biosignature gases …