Results 11 to 20 of about 2,912,496 (265)

Impact of Lorentz violation models on exoplanets dynamics [PDF]

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
  +7 more sources

Secular spin-axis dynamics of exoplanets (Corrigendum) [PDF]

open access: hybridAstronomy & Astrophysics, 2019
International ...
Melaine Saillenfest   +2 more
openalex   +5 more sources

Evidence for Low-level Dynamical Excitation in Near-resonant Exoplanet Systems

open access: yesThe Astronomical Journal, 2023
The geometries of near-resonant planetary systems offer a relatively pristine window into the initial conditions of exoplanet systems. Given that near-resonant systems have likely experienced minimal dynamical disruptions, the spin–orbit orientations of ...
Malena Rice   +20 more
doaj   +3 more sources

The Diversity of Exoplanets: From Interior Dynamics to Surface Expressions [PDF]

open access: greenElements, 2021
The coupled interior–atmosphere system of terrestrial exoplanets remains poorly understood. Exoplanets show a wide variety of sizes, densities, surface temperatures, and interior structures, with important knock-on effects for this coupled system. Many exoplanets are predicted to have a “stagnant lid” at the surface, with a rigid stationary crust ...
Maxim Ballmer, Lena Noack
  +9 more sources

Tidal dynamics of transiting exoplanets [PDF]

open access: bronzeProceedings of the International Astronomical Union, 2010
AbstractTransits give us the mass, radius, and orbital properties of the planet, all of which inform dynamical theories. Two properties of the hot Jupiters suggest they had a dramatic origin via tidal damping from high eccentricity. First, the tidally circularized planets (in the 1-4 day pile-up) lie along a relation or boundary in the mass-period ...
Daniel C. Fabrycky
openalex   +3 more sources

Secular spin-axis dynamics of exoplanets [PDF]

open access: hybridAstronomy & Astrophysics, 2019
Context. Seasonal variations and climate stability of a planet are very sensitive to the planet obliquity and its evolution. This is of particular interest for the emergence and sustainability of land-based life, but orbital and rotational parameters of exoplanets are still poorly constrained.
Melaine Saillenfest   +2 more
openalex   +6 more sources

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   +5 more sources

DYNAMICS AND TRANSIT VARIATIONS OF RESONANT EXOPLANETS [PDF]

open access: greenThe Astrophysical Journal, 2016
ABSTRACT Transit timing variations (TTVs) are deviations of the measured midtransit times from the exact periodicity. One of the most interesting causes of TTVs is the gravitational interaction between planets. Here we consider a case of two planets in a mean motion resonance (orbital periods in a ratio of small integers).
David Nesvorný, David Vokrouhlický
openalex   +4 more sources

Keplerian Orbits and Dynamics of Exoplanets

open access: green, 2010
8 pages, 9 figures, Chapter in "Exoplanets"; ISBN 978-0-8165-2945 ...
C. D. Murray, A. C. M. Correia
openalex   +4 more sources

Aerosol dynamics on hot exoplanets: the role of radiation pressure [PDF]

open access: hybridMonthly Notices of the Royal Astronomical Society
Abstract Aerosols appear to be ubiquitous in exoplanetary atmospheres. However because our understanding of the physical processes that govern aerosols is incomplete, their presence makes the measurement of atmospheric properties, such as molecular abundance ratios, difficult.
James E. Owen, Ruth Murray‐Clay
  +4 more sources

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