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Atmospheric carbon depletion as a tracer of water oceans and biomass on temperate terrestrial exoplanets
The conventional observables to identify a habitable or inhabited environment in
exoplanets, such as an ocean glint or abundant atmospheric O2, will be challenging to …
exoplanets, such as an ocean glint or abundant atmospheric O2, will be challenging to …
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 …
The TRAPPIST-1 habitable atmosphere intercomparison (THAI). II. Moist cases—The two waterworlds
To identify promising exoplanets for atmospheric characterization and to make the best use
of observational data, a thorough understanding of their atmospheres is needed. Three …
of observational data, a thorough understanding of their atmospheres is needed. Three …
3D modelling of the impact of stellar activity on tidally locked terrestrial exoplanets: atmospheric composition and habitability
Stellar flares present challenges to the potential habitability of terrestrial planets orbiting M
dwarf stars through inducing changes in the atmospheric composition and irradiating the …
dwarf stars through inducing changes in the atmospheric composition and irradiating the …
The TRAPPIST-1 habitable atmosphere intercomparison (THAI). III. Simulated observables—the return of the spectrum
Abstract The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI) is a community
project that aims to quantify how differences in general circulation models (GCMs) could …
project that aims to quantify how differences in general circulation models (GCMs) could …
The CARMENES search for exoplanets around M dwarfs-Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star
D Kossakowski, M Kürster, T Trifonov… - Astronomy & …, 2023 - aanda.org
We present the discovery of an Earth-mass planet (M b sin i= 1.26±0.21 M⊕) on a 15.6 d
orbit of a relatively nearby (d~ 9.6 pc) and low-mass (0.167±0.011 M⊙) M5. 0 V star, Wolf …
orbit of a relatively nearby (d~ 9.6 pc) and low-mass (0.167±0.011 M⊙) M5. 0 V star, Wolf …
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 …
Airy worlds or barren rocks? On the survivability of secondary atmospheres around the TRAPPIST-1 planets
G Van Looveren, M Güdel, SB Saikia… - Astronomy & …, 2024 - aanda.org
Context. The James Webb Space Telescope is currently at the forefront of the search for
atmospheres of exoplanets. However, the observation of atmospheres of Earth-like planets …
atmospheres of exoplanets. However, the observation of atmospheres of Earth-like planets …
Bistability of the atmospheric circulation on TRAPPIST-1e
Using a 3D general circulation model, we demonstrate that a confirmed rocky exoplanet and
a primary observational target, TRAPPIST-1e presents an interesting case of climate …
a primary observational target, TRAPPIST-1e presents an interesting case of climate …
Novel Atmospheric Dynamics Shape the Inner Edge of the Habitable Zone around White Dwarfs
White dwarfs offer a unique opportunity to search nearby stellar systems for signs of life, but
the habitable zone around these stars is still poorly understood. Since white dwarfs are …
the habitable zone around these stars is still poorly understood. Since white dwarfs are …