Interpreting exoplanet biosignatures with a coupled atmosphere-interior-geochemical evolution model
, 2021The atmospheric evolution of rocky planets is shaped by a range of astrophysical, geophysical, and geochemical processes. Interpreting observations of potentially habitable exoplanets will require an improved understanding of how these competing ...
J. Krissansen‐Totton+3 more
semanticscholar +3 more sources
Coupling the Atmospheric and Dynamical Evolution of Close-in Exoplanets
The vast majority of the detected exoplanets orbit in less than a month around their star, in extreme conditions unmet in the Solar System. The demographics of these close-in planets exhibit a striking feature: the lack of Neptune-size worlds on very short orbits, also dubbed the "Neptunian desert", which challenges our understanding of planetary ...
O. Attia, V. Bourrier
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EXODUS: A mission to explore exoplanet evolution through understanding atmospheric escape
EXODUS is a proposed mission to study the largely unexplored range of sub-Neptune to Jupiter-sized exoplanets with orbital periods longer than 100 days. The focus of the mission lies in the detection of these planets and characterisation of atmospheric escape to constrain their evolutionary pathways.
Citlali Bruce Rosete+10 more
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Exoplanet Atmospheric Studies At High Spectral Resolution
, 2020The study of exoplanet atmospheres is essential to understand the formation, evolution and composition of exoplanets. When a planet pass between its host star and an observer, a fraction of the star-light is absorbed by its atmosphere, thus revealing its
R. Allart
semanticscholar +1 more source
Biomarkers and Tracers of Atmospheric Evolution of Exoplanets In The Spectroscopic Window of Darwin
Franck Selsis+5 more
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The effects of terrestrial exoplanet bulk composition on long-term planetary evolution
, 2020With more observations of terrestrial exoplanets becoming available every year, the importance of geodynamical studies focusing on exoplanets is increasing. We know from observations that stellar chemical abundances vary in the Solar neighbourhood, which
R. Spaargaren+4 more
semanticscholar +1 more source
Grid-based exoplanet atmospheric mass-loss predictions via neural networks
Astronomy & AstrophysicsThe fast and accurate estimation of planetary mass-loss rates is critical for planet population and evolution modelling. We used machine learning (ML) for fast interpolation across an existing large grid of hydrodynamic upper atmosphere models, providing
Amit Reza+3 more
semanticscholar +1 more source
Grid-based exoplanet atmospheric mass loss predictions through neural network
arXiv.orgThe fast and accurate estimation of planetary mass-loss rates is critical for planet population and evolution modelling. We use machine learning (ML) for fast interpolation across an existing large grid of hydrodynamic upper atmosphere models, providing ...
Amit Reza+3 more
semanticscholar +1 more source
Investigating the Interplay of Stellar Evolution and Exoplanet Habitability Through Spectroscopy
International Journal of Current Research in Science, Engineering & TechnologyThe study of stellar evolution and exoplanet habitability is a cornerstone of modern astrophysics, with spectroscopy serving as a vital tool in unraveling the complexities of these phenomena.
D. Tolasa
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Transiting Exoplanet Atmospheres in the Era of JWST
Reviews in Mineralogy & GeochemistryThe field of exoplanet atmospheric characterization has recently made considerable advances with the advent of high-resolution spectroscopy from large ground-based telescopes and the commissioning of the James Webb Space Telescope (JWST). We have entered
E. Kempton, H. Knutson
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