Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? [PDF]
C. Swastik+7 more
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The Impact-driven Atmospheric Loss of Super-Earths around Different Spectral Types of Host Stars
A planet’s mass loss is important for the its formation and evolution. The radius valley (RV) is believed to be triggered by evaporation-induced mass loss.
Wei Zhong+3 more
doaj +1 more source
Structure and evolution of super-Earth to super-Jupiter exoplanets [PDF]
I. Baraffe, G. Chabrier, Travis Barman
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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
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The Formation of Double Hot Jupiter Systems through von Zeipel–Lidov–Kozai Migration
The von Zeipel–Lidov–Kozai (ZLK) mechanism with tidal friction has been demonstrated as a promising avenue to generate hot Jupiters in stellar binary systems.
Yurou Liu, Tiger Lu, Malena Rice
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The Age and High-energy Environment of the Very Young Transiting Exoplanet TOI 1227b
The mid-M star TOI 1227 hosts among the youngest known transiting exoplanets. We have conducted new X-ray imaging and optical spectroscopic observations of TOI 1227 aimed at ascertaining its age and the influence of its high-energy radiation on the ...
Attila Varga+4 more
doaj +1 more source
LITHIUM ABUNDANCES IN NEARBY FGK DWARF AND SUBGIANT STARS: INTERNAL DESTRUCTION, GALACTIC CHEMICAL EVOLUTION, AND EXOPLANETS [PDF]
I. Ramírez+3 more
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Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres? [PDF]
Glidden A+3 more
europepmc +1 more source
Temporal Evolution of the High-energy Irradiation and Water Content of TRAPPIST-1 Exoplanets [PDF]
V. Bourrier+15 more
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Pushing the envelope of exoplanet evolution modelling
Propelled by the discovery of the first exoplanet thirty years ago, the scientific community has rallied and made tremendous strides towards a full understand of the formation and evolution of planetary systems. During this period, over 4, 300 confirmed exoplanets have been detected, and the resulting dataset has driven a revolution by allowing for new
openaire +1 more source