Results 101 to 110 of about 8,820 (196)
Observations of Exoplanet Atmospheres
Detailed characterization of an extrasolar planet's atmosphere provides the best hope for distinguishing the makeup of its outer layers, and the only hope for understanding the interplay between initial composition, chemistry, dynamics & circulation, and
Crossfield, Ian J. M.
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Three-dimensional Orbital Architectures and Detectability of Adjacent Companions to Hot Jupiters
The orbital properties of the (as yet) small population of hot Jupiters with nearby planetary companions provide valuable constraints on the past migration processes of these systems.
Thomas MacLean, Juliette Becker
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Role of Dynamical Research in the Detection and Characterization of Exoplanets
9 pages, White Paper Submitted to the ExoPlanet Task ...
Ford, Eric B. +8 more
openaire +2 more sources
The Dynamics-Based Approach to Studying Terrestrial Exoplanets
One of the great quests of astronomy is to obtain the spectrum of a terrestrial planet orbiting within the habitable zone of its star, and the dominant challenge in doing so is to isolate the light of the planet from that of the star. Dynamics-based methods separate these signals temporally, whereas imaging techniques do so spatially.
Charbonneau, David, Deming, Drake
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On the Stability of Super-Earth Atmospheres
We investigate the stability of super Earth atmospheres around M stars using a 7-parameter, analytical framework. We construct stability diagrams in the parameter space of exoplanetary radius versus semi-major axis and elucidate the regions in which the ...
Heng, Kevin, Kopparla, Pushkar
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Evidence for a Peak at ∼0.3 in the Eccentricity Distribution of Typical Super-Jovian Exoplanets
In this study, we compute completeness-corrected occurrence rates of giant exoplanets as a function of mass, semimajor axis, and eccentricity, using the approximately uniform California Legacy Survey sample of radial velocity-discovered planets published
Sarah Blunt +5 more
doaj +1 more source
Free Floating or Merely Detached?
Microlensing surveys suggest the presence of a surprisingly large population of free-floating planets, with a rate of about two Neptunes per star.
Sam Hadden, Yanqin Wu
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A Comprehensive Analysis of Spitzer 4.5 μm Phase Curves of Hot Jupiters
Although exoplanetary science was not initially projected to be a substantial part of the Spitzer mission, its exoplanet observations set the stage for current and future surveys with JWST and Ariel.
Lisa Dang +21 more
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Inhomogeneous cloud formation and wavelength-dependent phenomena are expected to shape hot Jupiter atmospheres. We present a general circulation model with multiwavelength “picket fence” radiative transfer and radiatively active, temperature-dependent ...
Isaac Malsky +7 more
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Eccentricity Evolution of Warm Jupiters: The Role of Distant Perturbers and nearby Companions
Warm Jupiters (WJs)—giant exoplanets with orbital periods between 10 and 200 days—exhibit a broad range of eccentricities and are often accompanied by nearby low-mass planets.
Ying He, Dong-Hong Wu, Sheng Jin
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