Results 161 to 170 of about 2,811,519 (263)
Earth-like exoplanets in spin-orbit resonances: climate dynamics, 3D atmospheric chemistry, and observational signatures [PDF]
Marrick Braam+5 more
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Clouds and Hazes in GJ 1214 b’s Metal-rich Atmosphere
The sub-Neptune GJ 1214 b has an infamously flat transmission spectrum, likely due to thick aerosols in its atmosphere. A recent JWST/MIRI spectroscopic phase curve of GJ 1214 b added to this picture, suggesting a highly reflective and metal-rich ...
Isaac Malsky+12 more
doaj +1 more source
Dynamics of exoplanets and exosatellites in binaries
This dissertation is the result of the work made under the supervision of J.A. Docobo, Full Professor in Astronomy and Director of the Ramon María Aller Astronomical Observatory of the University of Santiago de Compostela. The core of the dissertation is a compendium of articles published in peer review publications indexed in the Journal Citation ...
openaire +1 more source
Early Time Small-scale Structures in Hot Exoplanet Atmosphere Simulations
We report on the critical influence of small-scale flow structures (e.g., fronts, vortices, and waves) that immediately arise in hot exoplanet atmosphere simulations initialized with a resting state.
J. W. Skinner, J. Y-K. Cho
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How Landmass Distribution Influences the Atmospheric Dynamics of Tidally Locked Terrestrial Exoplanets [PDF]
Félix Sainsbury-Martinez+3 more
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A white paper submitted in response to the National Academy of Sciences 2018 Exoplanet Science Strategy solicitation, from the NASA Sellers Exoplanet Environments Collaboration (SEEC) of the Goddard Space Flight Center.
Henning, Wade G.+41 more
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Stability of hydrides in sub-Neptune exoplanets with thick hydrogen-rich atmospheres. [PDF]
Kim T+6 more
europepmc +1 more source
Due to the unprecedented signal strengths offered by the newest high-resolution spectrographs on 10 m class telescopes, exploring the 3D nature of exoplanets is possible with an unprecedented level of precision.
Aurora Y. Kesseli+3 more
doaj +1 more source
Before the launch of the Kepler Space Telescope, models of low-mass planet formation predicted that convergent type I migration would often produce systems of low-mass planets in low-order mean-motion resonances.
Jacob H. Hamer, Kevin C. Schlaufman
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Observational Signatures of a Previous Dynamical Instability in Multi-planet M-dwarf Systems
We identify observational signatures suggesting a history of dynamical instability in 26 out of 34 M-dwarf multi-planet systems containing no large planets.
Anna C. Childs+4 more
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