Results 11 to 20 of about 2,690,574 (274)

Mapping out the time-evolution of exoplanet processes [PDF]

open access: yesarXiv, 2019
There are many competing theories and models describing the formation, migration and evolution of exoplanet systems. As both the precision with which we can characterize exoplanets and their host stars, and the number of systems for which we can make ...
Beichman, Charles   +4 more
core   +4 more sources

The timescale for giant planet formation : constraints from the rotational evolution of exoplanet host stars [PDF]

open access: greenarXiv, 2008
The timescale over which planets may form in the circumstellar disks of young stars is one of the main issues of current planetary formation models. We present here new constraints on planet formation timescales derived from the rotational evolution of ...
J. Bouvier
core   +6 more sources

The Orbital Geometries and Stellar Obliquities of Exoplanet-hosting Multistar Systems [PDF]

open access: yesThe Astronomical Journal
The current orbital geometries of exoplanet systems offer a fossilized record of the systems’ dynamical histories. A particularly rich set of dynamical mechanisms is available to exoplanets residing in multistar systems, which may have their evolution ...
Malena Rice   +2 more
doaj   +3 more sources

Exoplanet atmosphere evolution: emulation with neural networks [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
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
openaire   +5 more sources

Haze evolution in temperate exoplanet atmospheres through surface energy measurements [PDF]

open access: yesNature Astronomy, 2021
6 figures, 2 tables, 23 ...
Xinting Yu   +15 more
openaire   +9 more sources

Transiting Exoplanet Atmospheres in the Era of JWST [PDF]

open access: yesarXiv
The field of exoplanet atmospheric characterization has recently made considerable advances with the advent of high-resolution spectroscopy from large ground-based telescopes and the commissioning of the James Webb Space Telescope (JWST). We have entered
E. Kempton, H. Knutson
semanticscholar   +2 more sources

Variability of Known Exoplanet Host Stars Observed by TESS [PDF]

open access: yesThe Astronomical Journal, 2023
Both direct and indirect methods of exoplanet detection rely upon detailed knowledge of the potential host stars. Such stellar characterization allows for accurate extraction of planetary properties, as well as contributing to our overall understanding ...
Emilie R. Simpson   +5 more
doaj   +2 more sources

The transiting exoplanet CoRoT-11b and its peculiar tidal evolution [PDF]

open access: diamondEPJ Web of Conferences, 2011
CoRoT-11b is a fairly massive hot-Jupiter (Mp = 2.33 ± 0.34 MJup ) in a 3 days orbit around a F6 V star with an age of 2 ± 1 Gyr. The relatively high projected rotational velocity of the star (v sin i⋆ = 40 ± 5 km/s) places CoRoT-11 among the most rapidly rotating planet hosting stars discovered so far.
D. Gandolfi, A. F. Lanza, C. Damiani
openalex   +4 more sources

Early evolution of purple retinal pigments on Earth and implications for exoplanet biosignatures [PDF]

open access: yesInternational Journal of Astrobiology, 2018
AbstractWe propose that retinal-based phototrophy arose early in the evolution of life on Earth, profoundly impacting the development of photosynthesis and creating implications for the search for life beyond our planet. While the early evolutionary history of phototrophy is largely in the realm of the unknown, the onset of oxygenic photosynthesis in ...
DasSarma, Shiladitya   +1 more
openaire   +9 more sources

Tidal Evolution of Exoplanets [PDF]

open access: green, 2010
Tidal effects arise from differential and inelastic deformation of a planet by a perturbing body. The continuous action of tides modify the rotation of the planet 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 ...
A. C. M. Correia, J. Laskar
openalex   +5 more sources

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