Results 1 to 10 of about 40,892 (232)

Signatures of Atmospheric Mass Loss and Planet Migration in the Time Evolution of Short-period Transiting Exoplanets [PDF]

open access: goldThe Astronomical Journal
Comparative studies of young and old exoplanet populations offer a glimpse into how planets may form and evolve with time. We present an occurrence rate study of short-period (
Rachel B. Fernandes   +21 more
doaj   +6 more sources

Atmospheric Escape and the Evolution of Close-In Exoplanets [PDF]

open access: greenAnnual Review of Earth and Planetary Sciences, 2018
Exoplanets with substantial hydrogen/helium atmospheres have been discovered in abundance, many residing extremely close to their parent stars.
James E. Owen
semanticscholar   +9 more sources

Biological, Equilibrium and Photochemical Signatures of C, N and S Isotopes in the Early Earth and Exoplanet Atmospheres [PDF]

open access: yesLife
The unambiguous detection of biosignatures in exoplanet atmospheres is a primary objective for astrobiologists and exoplanet astronomers. The primary methodology is the observation of combinations of gases considered unlikely to coexist in an atmosphere ...
James R. Lyons
doaj   +3 more sources

On the relative importance of AGN winds for the evolution of exoplanet atmospheres [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2022
Recent work investigating the impact of winds and outflows from active galactic nuclei (AGN) on the habitability of exoplanets suggests that such activity could be deleterious for the long-term survival of planetary atmospheres and the habitability of ...
S. Heinz
semanticscholar   +3 more sources

Exoplanet atmosphere evolution: emulation with neural networks [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
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
semanticscholar   +5 more sources

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

open access: yesNature Astronomy, 2021
Photochemical hazes are important opacity sources in temperate exoplanet atmospheres, hindering current observations from characterizing exoplanet atmospheric compositions.
Xinting Yu   +15 more
semanticscholar   +9 more sources

The Atmospheric Evolution of Small, Close-In Exoplanets [PDF]

open access: green, 2022
Submitted in part fulfilment of the requirements for the degree of Doctor of Philosophy at Imperial College London, July 2022.
James G. Rogers
openalex   +5 more sources

The role of planetary interior in the long-term evolution of atmospheric CO2on Earth-like exoplanets [PDF]

open access: bronzeAstronomy & Astrophysics, 2021
Context.The long-term carbonate silicate cycle plays an important role in the evolution of Earth’s climate and, therefore, may also be an important mechanism in the evolution of the climates of Earth-like exoplanets. However, given the large diversity in the possible interiors for Earth-like exoplanets, the ensuing evolution of the atmospheric ...
Mark Oosterloo   +3 more
openalex   +6 more sources

The Evolution of Atmospheric Escape of Highly Irradiated Gassy Exoplanets [PDF]

open access: hybridProceedings of the International Astronomical Union, 2021
AbstractAtmospheric escape has traditionally been observed using hydrogen Lyman-α transits, but more recent detections utilise the metastable helium triplet lines at 1083nm. Capable of being observed from the ground, this helium signature offers new possibilities for studying atmospheric escape.
Andrew Allan   +2 more
openalex   +2 more sources

A Coupled Analysis of Atmospheric Mass Loss and Tidal Evolution in XUV Irradiated Exoplanets: The TRAPPIST-1 Case Study [PDF]

open access: bronzeThe Astronomical Journal, 2020
Abstract Exoplanets residing close to their stars can experience evolution of both their physical structures and their orbits due to the influence of their host stars. In this work, we present a coupled analysis of dynamical tidal dissipation and atmospheric mass loss for exoplanets in X-ray and ultraviolet (XUV) irradiated environments.
Juliette Becker   +4 more
openalex   +8 more sources

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