Distinguishing Oceans of Water from Magma on Mini-Neptune K2-18b
Mildly irradiated mini-Neptunes have densities potentially consistent with them hosting substantial liquid-water oceans (“Hycean” planets). The presence of CO _2 and simultaneous absence of ammonia (NH _3 ) in their atmospheres has been proposed as a ...
Oliver Shorttle+4 more
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Characterizing Exoplanets for Assessing Their Potential Habitability
The Statistical-likelihood Exoplanetary Habitability Index (SEPHI) serves as a valuable tool for prioritizing targets for further study and identifying potentially habitable environments.
J. M. Rodríguez-Mozos, A. Moya
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Fully fluorinated non-carbon compounds NF3 and SF6 as ideal technosignature gases. [PDF]
Seager S+5 more
europepmc +1 more source
The effect of metallicity on the atmospheres of exoplanets with fully coupled 3D hydrodynamics, equilibrium chemistry, and radiative transfer [PDF]
Ben Drummond+7 more
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First space mission dedicated to exoplanet atmospheres gets green light [PDF]
Elizabeth Gibney
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Unraveling the complex inventory of biorelevant organics in the plumes of icy moons. [PDF]
Kaiser RI.
europepmc +1 more source
Optimizing exoplanet atmosphere retrieval using unsupervised machine-learning classification [PDF]
J. J. C. Hayes+8 more
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DETECTING INDUSTRIAL POLLUTION IN THE ATMOSPHERES OF EARTH-LIKE EXOPLANETS
Henry W. Lin+2 more
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Observing Isotopologue Bands in Terrestrial Exoplanet Atmospheres with the James Webb Space Telescope: Implications for Identifying Past Atmospheric and Ocean Loss [PDF]
Andrew Lincowski+2 more
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