Results 121 to 130 of about 10,220 (206)
The Solubility of N2 in High-pressure Ice and Its Consequent Outgassing Limitations in Water Worlds
Exoplanets with a few percent water mass fraction may host a high-pressure ice layer that separates the atmosphere from the interior. We investigate the role played by this layer in the transport of N _2 between the interior and the atmosphere.
Amit Levi +3 more
doaj +1 more source
Next-generation Improvements in Giant-exoplanet Evolutionary and Structural Models
Many evolutionary models of giant exoplanets still rely on simplifying assumptions that are no longer adequate, given detailed constraints from Jupiter, Saturn, and modern exoplanet observations.
Ankan Sur +3 more
doaj +1 more source
More than a thousand exoplanets have been discovered over the last decade. Perhaps more excitingly, probing their atmospheres has become possible. We now have spectra of hot Jupiters like HD 189733b and HD 209458b, of Neptune-like planets like GJ1214b and even smaller planets are within reach.
openaire +1 more source
The First Dedicated Survey of Atmospheric Escape from Planets Orbiting F Stars
Hydrodynamic escape can strip the envelopes of close-in exoplanets, but most observations of atmospheric mass loss to date have been confined to planets orbiting K and M dwarfs.
Morgan Saidel +11 more
doaj +1 more source
Terrestrial planets currently in the habitable zone around M dwarfs are estimated to have been in runaway greenhouse conditions for up to ∼1 Gyr due to the long-term pre-main-sequence phase of M dwarfs.
Yo Kawamura +7 more
doaj +1 more source
Exo-Geoscience Perspectives Beyond Habitability. [PDF]
Spohn T +7 more
europepmc +1 more source
A young progenitor for the most common planetary systems in the Galaxy. [PDF]
Livingston JH +41 more
europepmc +1 more source
A Stellar magnesium to silicon ratio in the atmosphere of an exoplanet. [PDF]
Sanchez JA +19 more
europepmc +1 more source
Prospects for detecting signs of life on exoplanets in the JWST era. [PDF]
Seager S +4 more
europepmc +1 more source
identifier:oai:t2r2.star.titech.ac.jp ...
+3 more sources

