Results 91 to 100 of about 1,144 (201)
The effects of terrestrial exoplanet bulk composition on long-term planetary evolution 
Rob Spaargaren +3 more
openalex +1 more source
The evolution of stellar surface activity and possible effects on exoplanets [PDF]
M. S. Giampapa
openalex +1 more source
Unexpected Near-Resonant and Metastable States of Young Multiplanet Systems
Recent observations suggest that the incidence of near-resonant planets declines as planetary systems age, making young planetary systems key signposts of early dynamical evolution.
Zhecheng Hu +6 more
doaj +1 more source
Atmospheric escape’s potential to shape the exoplanet population motivates detailed observations of systems actively undergoing escape. AU Mic is a young and active M dwarf hosting two close-in transiting sub- to Neptune-sized planets. Atmospheric escape
Keighley E. Rockcliffe +10 more
doaj +1 more source
Not All Sub-Neptune Exoplanets Have Magma Oceans
The evolution and structure of sub-Neptunes may be strongly influenced by interactions between the outer gaseous envelope of the planet and a surface magma ocean.
Bodie Breza +2 more
doaj +1 more source
Interior and Climate Modeling of the Venus Zone Planet TOI-2285 b
As the discovery of exoplanets progresses at a rapid pace, the large number of known planets provides a pathway to assess the stellar and planetary properties that govern the climate evolution of terrestrial planets.
Emma L. Miles +7 more
doaj +1 more source
Formation and evolution of exoplanets in different environments
Invited Review. To appear in Astronomical Society of the Pacific (ASP) Conference Series "Non-Stable Universe: Energetic Resources, Activity Phenomena and Evolutionary Processes" dedicated to the 70th anniversary of Byurakan Astrophysical ...
openaire +2 more sources
Water Evolution and Inventories of Super-Earths Orbiting Late M Dwarfs
Super-Earths orbiting M dwarf stars may be the most common habitable planets in the Universe. However, their habitability is threatened by intense irradiation from their host stars, which drives the escape of water to space and can lead to surface ...
Keavin Moore +3 more
doaj +1 more source
Understanding the Planetary Formation and Evolution in Star Clusters (UPiC). I. Evidence of Hot Giant Exoplanets Formation Timescales [PDF]
Yuan-Zhe Dai +3 more
openalex +1 more source
The distribution of period ratios for 580 known two-planet systems is apparently nonuniform, with several sharp peaks and troughs. In particular, the vicinity of the 2:1 commensurability seems to have a deficit of systems.
Valeri Makarov +2 more
doaj +1 more source

