Results 21 to 30 of about 2,964,883 (268)

Atmospheric Dynamics of Hot Exoplanets [PDF]

open access: bronzeAnnual Review of Earth and Planetary Sciences, 2015
The characterization of exoplanetary atmospheres has come of age in the past decade, as astronomical techniques now allow for albedos, chemical abundances, temperature profiles and maps, rotation periods, and even wind speeds to be measured. Atmospheric dynamics sets the background state of density, temperature, and velocity that determines or ...
Kevin Heng, Adam P. Showman
openalex   +4 more sources

Impact of Lorentz Violation Models on Exoplanets’ Dynamics

open access: greenUniverse, 2022
Many exoplanets have been detected by the radial velocity method, according to which the motion of a binary system around its center of mass can produce a periodical variation of the Doppler effect of the light emitted by the host star. These variations are influenced by both Newtonian and non-Newtonian perturbations to the dominant inverse-square ...
Antonio Gallerati   +2 more
openalex   +4 more sources

Coupled atmospheric chemistry, radiation, and dynamics of an exoplanet generate self-sustained oscillations

open access: yesProceedings of the National Academy of Sciences of the United States of America, 2023
Significance Using a fully coupled, three-dimensional atmospheric chemistry-radiation-dynamics model, we demonstrate that the atmospheric composition of terrestrial exoplanets can be self-oscillatory under nonvarying external forcings. This finding could
Yangcheng Luo   +4 more
semanticscholar   +1 more source

Evolution of Planetary Obliquity: The Eccentric Kozai–Lidov Mechanism Coupled with Tide

open access: yesThe Astrophysical Journal, 2023
Planetary obliquity plays a significant role in determining the physical properties of planetary surfaces and climate. As direct detection is constrained due to the present observation accuracy, kinetic theories are helpful for predicting the evolution ...
Xiumin Huang   +4 more
doaj   +1 more source

Exoplanet atmospheres at high resolution through a modest-size telescope. Fe II in MASCARA-2b and KELT-9b with FIES on the Nordic Optical Telescope [PDF]

open access: yesAstronomy & Astrophysics, 2022
Ground-based, high-resolution spectrographs are providing us with an unprecedented view of the dynamics and chemistry of the atmospheres of planets outside the Solar System.
A. Bello-Arufe   +6 more
semanticscholar   +1 more source

High-contrast, high-angular resolution view of the GJ 367 exoplanet system [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2022
We search for additional companions in the GJ 367 exoplanet system, and aim at better constraining its age and evolutionary status. We analyse high contrast direct imaging observations obtained with HST/NICMOS, VLT/NACO, and VLT/SPHERE.
W. Brandner   +3 more
semanticscholar   +1 more source

Dynamical Constraints on Exoplanets [PDF]

open access: yesProceedings of the International Astronomical Union, 2013
AbstractDynamical studies of new exoplanet systems are a critical component of the discovery and characterisation process. Such studies can provide firmer constraints on the parameters of the newly discovered planets, and may even reveal that the proposed planets do not stand up to dynamical scrutiny.
Horner, Jonti   +4 more
openaire   +2 more sources

DYNAMICAL MEASUREMENTS OF THE INTERIOR STRUCTURE OF EXOPLANETS [PDF]

open access: yesThe Astrophysical Journal, 2013
Giant gaseous planets often reside on orbits in sufficient proximity to their host stars for the planetary quadrupole gravitational field to become non-negligible. In presence of an additional planetary companion, a precise characterization of the system's orbital state can yield meaningful constraints on the transiting planet's interior structure ...
Becker, Juliette C., Batygin, Konstantin
openaire   +3 more sources

The Sensitivity of Eclipse Mapping to Planetary Rotation

open access: yesThe Astronomical Journal, 2022
Mapping exoplanets across phases and during secondary eclipse is a powerful technique for characterizing Hot Jupiters in emission. Since these planets are expected to rotate about axes normal to their orbital planes, with rotation periods synchronized ...
Arthur D. Adams, Emily Rauscher
doaj   +1 more source

Home - About - Disclaimer - Privacy