Results 41 to 50 of about 1,751 (120)
Europa’s H2O2: Temperature Insensitivity and a Correlation with CO2
H _2 O _2 is part of Europa’s water-ice radiolytic cycle and a potential source of oxidants to Europa’s subsurface ocean. However, factors controlling the concentration of this critical surface species remain unclear.
Peiyu Wu +3 more
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Some sub-Neptune planets may host habitable conditions; for example “Hycean” worlds with H _2 envelopes over liquid water oceans can maintain potentially hospitable pressures and temperatures at their surface.
Michaela Leung +4 more
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Two-dimensional Models of Microphysical Clouds on Hot Jupiters. I. Cloud Properties
We present a new two-dimensional, bin-scheme microphysical model of cloud formation in the atmospheres of hot Jupiters that includes the effects of longitudinal gas and cloud transport.
Diana Powell, Xi Zhang
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The Detection-versus-retrieval Challenge: Titan as an Exoplanet
Cassini observations of Titan’s atmosphere are exemplary benchmarks for exoplanet atmospheric studies owing to their precision, their spectral coverage, and our independent knowledge of Titan.
Prajwal Niraula +4 more
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The Resonant Remains of Broken Chains from Major and Minor Mergers
TESS and Kepler have revealed that practically all close-in sub-Neptunes form in mean-motion resonant chains, most of which unravel on timescales of 100 Myr.
Rixin Li +3 more
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Strong Fractionation of Deuterium and Helium in Sub-Neptune Atmospheres along the Radius Valley
We simulate atmospheric fractionation in escaping planetary atmospheres using IsoFATE , a new open-source numerical model. We expand the parameter space studied previously to planets with tenuous atmospheres that exhibit the greatest helium and deuterium
Collin Cherubim +3 more
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Differentiation, the Exception, Not the Rule: Evidence for Full Miscibility in Sub-Neptune Interiors
We investigate the consequences of nonideal mixing between silicate, iron metal, and hydrogen for the structures of the cores of sub-Neptunes with implications for super-Earths and perhaps other planets formed by mixtures of silicate melt, iron metal ...
Edward D. Young +4 more
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Nightside Clouds on Tidally Locked Terrestrial Planets Mimic Atmosphere-free Scenarios
We investigate the impact of nightside cloud formation on the observable day/night contrast of tidally locked terrestrial planet atmospheres. We demonstrate that, in the case where the planetary dayside is only 10 s of Kelvin hotter than the planetary ...
Diana Powell +2 more
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Eccentricity Distribution beyond the Snow Line and Implications for Planetary Habitability
A fundamental question in the study of planetary system demographics is: how common is the solar system architecture? The primary importance of this question lies in the potential of planetary systems to create habitable environments, and dissecting the ...
Stephen R. Kane, Robert A. Wittenmyer
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The detection and atmospheric characterization of potentially habitable, temperate terrestrial exoplanets using a space-based mid-infrared nulling interferometer is a major goal of contemporary astrophysics.
Philipp A. Huber +7 more
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