Results 91 to 100 of about 581 (180)

Next-generation Improvements in Giant-exoplanet Evolutionary and Structural Models

open access: yesThe Astrophysical Journal
Many evolutionary models of giant exoplanets still rely on simplifying assumptions that are no longer adequate, given detailed constraints from Jupiter, Saturn, and modern exoplanet observations.
Ankan Sur   +3 more
doaj   +1 more source

The First Dedicated Survey of Atmospheric Escape from Planets Orbiting F Stars

open access: yesThe Astronomical Journal
Hydrodynamic escape can strip the envelopes of close-in exoplanets, but most observations of atmospheric mass loss to date have been confined to planets orbiting K and M dwarfs.
Morgan Saidel   +11 more
doaj   +1 more source

The Orbital Imperative: Charting Cosmic Evolution from Gamma-Ray Bursts to Exoplanet Atmospheres

open access: yes
This paper explores the intricate connection between early universe energetic phenomena, specifically Gamma-Ray Bursts (GRBs), and the later-stage evolution of planetary systems, as evidenced by exoplanet atmospheres. We propose an "orbital imperative" framework, suggesting that gravitational dynamics and the resulting distribution of matter play a ...
Revista, Zen, ASTRO, 10
openaire   +1 more source

Evolution of Atmospheric Composition in Giant Exoplanets with Diluted Cores

open access: yes
Transmission spectroscopy has reported sub-solar C/O ratios (<0.55) for atmospheres of some transiting gas giants/dwarfs (e.g., Sing et al. 2024; Welbanks et al. 2024). However, static disk chemistry models (e.g., Öberg et al. 2011) predict super-solar C/O ratios for protoplanetary disk gas and, consequently, for planetary envelopes.
Matsuo, Hiroki   +2 more
openaire   +1 more source

Reduced Water Loss due to Photochemistry on Terrestrial Planets in the Runaway Greenhouse Phase around Pre-main-sequence M Dwarfs

open access: yesThe Astrophysical Journal
Terrestrial planets currently in the habitable zone around M dwarfs are estimated to have been in runaway greenhouse conditions for up to ∼1 Gyr due to the long-term pre-main-sequence phase of M dwarfs.
Yo Kawamura   +7 more
doaj   +1 more source

Thermal structure, composition, atmospheric dynamics and long-terme evolution of irradiated exoplanets

open access: yes
Structure thermique, composition, dynamique de l’atmosphère et évolution à long-terme des exoplanètes irradiées Plus d’un millier d’exoplanètes ont été découvertes depuis une dizaine d’années. Plus incroyable encore, nous pouvons maintenant caractériser les atmosphères de ces mondes lointains.
openaire   +2 more sources

The evolution and diversity of rocky planets: From the core to the atmosphere, from the Earth to exoplanets

open access: yesThe evolution and diversity of rocky planets: From the core to the atmosphere, from the Earth to exoplanets
identifier:oai:t2r2.star.titech.ac.jp ...
  +3 more sources

Exo-Geoscience Perspectives Beyond Habitability. [PDF]

open access: yesSpace Sci Rev
Spohn T   +7 more
europepmc   +1 more source

A young progenitor for the most common planetary systems in the Galaxy. [PDF]

open access: yesNature
Livingston JH   +41 more
europepmc   +1 more source

A Stellar magnesium to silicon ratio in the atmosphere of an exoplanet. [PDF]

open access: yesNat Commun
Sanchez JA   +19 more
europepmc   +1 more source

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