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20212026
most citedDay-night cloud asymmetry prevents early oceans on Venus but not on Earth

145 citations · 375 across the 19 of their papers we have counts for

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21 papers · 1 filter

astro-ph.EP2026

A broad exploration of climate and observability of close-in rocky exoplanets: applications to Ross 128 b

Mathilde Houelle, Emeline Bolmont, Christophe Lovis +4

VLT/RISTRETTO, ELT/ANDES and ELT/PCS will soon enable atmospheric characterization of non-transiting, small rocky exoplanets orbiting closer than the inner edge of the Habitable Zo…

astro-ph.EP2026

A Fast and Physically Grounded Ocean Model for GCMs: The Dynamical Slab Ocean Model of the Generic-PCM (rev. 3423)

Siddharth Bhatnagar, Francis Codron, Ehouarn Millour +5

Ocean dynamics are often sidelined in exoplanet climate studies due to the high computational cost of fully coupled atmosphere-ocean general circulation models (GCMs). However, oce…

astro-ph.EP2026

Atmospheric Collapse and Habitability on Tidally-Locked Exoplanets

Keigo Taniguchi, Takanori Kodama, Martin Turbet +3

The habitability of terrestrial exoplanets orbiting M dwarfs is a key topic in the search for extraterrestrial life. The climates of these planets differ significantly from the Ear…

astro-ph.EP2026

Climates of Terrestrial Exoplanets and Biosignatures

Siddharth Bhatnagar, Emeline Bolmont, Nikita J. Boeren +18

Understanding the climates of terrestrial exoplanets and the detectability of biosignatures is an inherently interdisciplinary challenge, requiring the integration of insights from…

astro-ph.EP2025

Constraints on the possible atmospheres on TRAPPIST-1 b: insights from 3D climate modeling

Alice Maurel, Martin Turbet, Elsa Ducrot +13

JWST observations of the secondary eclipse of TRAPPIST-1 b at 12.8 and 15 microns revealed a very bright dayside. These measurements are consistent with an absence of atmosphere. P…

astro-ph.EP2025★ 1 cited

SpeCT: A state-of-the-art tool to calculate correlated-k tables and continua of CO-HO-N gas mixtures

G. Chaverot, M. Turbet, H. Tran +4

A key challenge in modeling (exo)planetary atmospheres lies in generating extensive opacity datasets that cover the wide variety of possible atmospheric composition, pressure, and…