Results 131 to 140 of about 16,797 (229)
We report the discovery of a hot Jupiter candidate orbiting HS Psc, a K7 (≈0.7 M _⊙ ) member of the ≈130 Myr AB Doradus moving group. Using radial velocities over 4 yr from the Habitable-zone Planet Finder spectrograph at the Hobby–Eberly Telescope, we ...
Quang H. Tran +8 more
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Planet formation models suggest that the small exoplanets that migrate from beyond the snowline of the protoplanetary disk likely contain water-ice-rich cores (∼50% by mass), also known as water worlds.
Aritra Chakrabarty, Gijs D. Mulders
doaj +1 more source
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
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
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
The evolution of hot Jupiters revealed by the age distribution of their host stars. [PDF]
Chen DC +13 more
europepmc +1 more source
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
doaj +1 more source
Evolution of the Exoplanet Size Distribution: Forming Large Super-Earths Over Billions of Years [PDF]
Trevor J. David +10 more
openalex +1 more source
Modelling the effect of stellar metallicity on the XUV evolution of low-mass stars and its impact on exoplanet atmospheres/habitability [PDF]
Victor See +3 more
openalex +2 more sources
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

