Results 191 to 200 of about 2,563,330 (219)
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Spin-Orbital Evolution of Exoplanets
EAS Publications Series, 2003We investigated the equation describing the evolution of the kinetic momentum vector of planets by the action of gravitational and magnetic interaction. The obtained gallery of portraits of the kinetic momentum evolution illustrates the various regimes of planetary system evolution.
A. Gusev, I. Kitiashvili
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Modelling the effect of stellar metallicity on the XUV evolution of low-mass stars and its impact on exoplanet atmospheres/habitability [PDF]
Monthly Notices of the Royal Astronomical SocietyUnderstanding how exoplanet atmospheres evolve is a key question in the context of habitability. One key process governing this evolution is atmospheric evaporation by stellar X-ray and EUV emission (collectively, XUV).
Víctor See, O J Hall, Louis Amard
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Formation and Evolution of Exoplanets
2010Introduction Exoplanet Observations Pinpointing Planets in Circumstellar Disks Planet-Planet Interactions Formation via Disk Instability Core Accretion Model Formation of Terrestrial Planets Brown Dwarfs Exoplanet Chemistry Migration and Multiplicity Effects During Giant Planet formation Planets in mean motion resonance Planet-Planet Gravitational ...
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Pushing the envelope of exoplanet evolution modelling [PDF]
, 2021 Propelled by the discovery of the first exoplanet thirty years ago, the scientific community has rallied and made tremendous strides towards a full understand of the formation and evolution of planetary systems. During this period, over 4, 300 confirmed exoplanets have been detected, and the resulting dataset has driven a revolution by allowing for new
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The Irradiation-Driven Evolution of Gas-Giant Exoplanets
2022Nearly thirty years after their initial discovery, we now know of over five thousand extrasolar planets. Intensive efforts have been made to characterize the sizes, masses, orbits, and compositions of these new worlds, and the resulting population challenges our intuition from the Solar System.
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Evolution of Angular Momentum Distribution in Exoplanet Systems
Astrophysics, 2015The distribution of angular momentum is investigated in “star–planet systems, taking due account of stellar evolution effects. Numerical simulation is carried out for 15 systems for which stellar rotation data are available. Consideration of changes in stellar structure is confirmed to be significant for the evolution of momentum distribution.
P. A. Tarakanov, A. S. Artamonov
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Tidal evolution of close-in exoplanets
2014The continuous action of tides modify the rotation of close-in planets together with its orbit until an equilibrium situation is reached. It is often believed that synchronous motion is the most probable outcome of the tidal evolution process, since synchronous rotation is observed for the majority of the satellites in the solar system. However, in the
Correia, Alexandre C. M. +3 more
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Coupling the Atmospheric and Dynamical Evolution of Close-in Exoplanets
The vast majority of the detected exoplanets orbit in less than a month around their star, in extreme conditions unmet in the Solar System. The demographics of these close-in planets exhibit a striking feature: the lack of Neptune-size worlds on very short orbits, also dubbed the "Neptunian desert", which challenges our understanding of planetary ...Omar Attia, Vincent Bourrier
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Exoplanet Statistics and Theoretical Implications
Annual Review of Astronomy and Astrophysics, 2021Subo Dong
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