Results 91 to 100 of about 581 (180)
Next-generation Improvements in Giant-exoplanet Evolutionary and Structural Models
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
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
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
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
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
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
identifier:oai:t2r2.star.titech.ac.jp ...
+3 more sources
Exo-Geoscience Perspectives Beyond Habitability. [PDF]
Spohn T +7 more
europepmc +1 more source
A young progenitor for the most common planetary systems in the Galaxy. [PDF]
Livingston JH +41 more
europepmc +1 more source
A Stellar magnesium to silicon ratio in the atmosphere of an exoplanet. [PDF]
Sanchez JA +19 more
europepmc +1 more source

