Results 1 to 10 of about 931 (166)
True Polar Wander of Lava Worlds
As one of the most detectable types of terrestrial planets, lava worlds are highly prioritized targets for exoplanet atmosphere characterization since their atmospheres may reveal what they are made of and how.
Wanying Kang, Francis Nimmo, Feng Ding
doaj +1 more source
Thermal and Orbital Evolution of Low-mass Exoplanets [PDF]
Abstract The thermal, orbital, and rotational dynamics of tidally loaded exoplanets are interconnected by intricate feedback. The rheological structure of the planet determines its susceptibility to tidal deformation and, as a consequence, participates in shaping its orbit.
Michaela Walterová, Marie Běhounková
openaire +2 more sources
Surrounded by Giants: Habitable Zone Stability Within the HD 141399 System
The search for exoplanets has revealed a diversity of planetary system architectures, the vast majority of which diverge significantly from the template of the solar system.
Stephen R. Kane
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Evolution of exoplanets and their parent stars [PDF]
Studying exoplanets with their parent stars is crucial to understand their population, formation and history. We review some of the key questions regarding their evolution with particular emphasis on giant gaseous exoplanets orbiting close to solar-type stars.
Guillot, Tristan +4 more
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Evolution of Planetary Obliquity: The Eccentric Kozai–Lidov Mechanism Coupled with Tide
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
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Haze evolution in temperate exoplanet atmospheres through surface energy measurements [PDF]
6 figures, 2 tables, 23 ...
Xinting Yu +15 more
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Dynamical Evolution of Closely Packed Multiple Planetary Systems Subject to Atmospheric Mass Loss
A gap in exoplanets’ radius distribution has been widely attributed to the photoevaporation threshold of their progenitors’ gaseous envelope. Giant impacts can also lead to substantial mass loss.
Su Wang, D. N. C. Lin
doaj +1 more source
Exoplanet atmosphere evolution: emulation with neural networks
ABSTRACT Atmospheric mass-loss is known to play a leading role in sculpting the demographics of small, close-in exoplanets. Knowledge of how such planets evolve allows one to ‘rewind the clock’ to infer the conditions in which they formed.
James G Rogers +3 more
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Obliquity Evolution of the Potentially Habitable Exoplanet Kepler-62f [PDF]
15 pages, 17 figures, 5 tables; Revised relative to Referee Reports.
Quarles, Billy +3 more
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Tidal evolution of close-in exoplanets and host stars
ABSTRACT The evolution of exoplanetary systems with a close-in planet is ruled by the tides mutually raised on the two bodies and by the magnetic braking of the host star. This paper deals with consequences of this evolution and some features that can be observed in the distribution of the systems' two main periods: the orbital period ...
Ferraz Mello, S, Beauge, Cristian
openaire +3 more sources

