Understanding the climate dynamics at the inner edge of the habitable zone is crucial for predicting the habitability of rocky exoplanets. Previous studies using global climate models (GCMs) have indicated that planets receiving high stellar flux can ...
Bowen Fan, Da Yang, Dorian S. Abbot
doaj +1 more source
The Nature and Origins of Sub-Neptune Size Planets. [PDF]
Bean JL, Raymond SN, Owen JE.
europepmc +1 more source
Introduction-First Billion Years: Habitability. [PDF]
Rivera-Valentín EG +6 more
europepmc +1 more source
Planet population synthesis: the role of stellar encounters. [PDF]
Ndugu N, Abedigamba OP, Andama G.
europepmc +1 more source
Igneous processes in the small bodies of the Solar System I. Asteroids and comets. [PDF]
Leone G, Tanaka HKM.
europepmc +1 more source
Fundamentals of Interior Modelling and Challenges in the Interpretation of Observed Rocky Exoplanets. [PDF]
Baumeister P +9 more
europepmc +1 more source
In Search for a Planet Better than Earth: Top Contenders for a Superhabitable World. [PDF]
Schulze-Makuch D, Heller R, Guinan E.
europepmc +1 more source
Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity. [PDF]
Quanz SP +30 more
europepmc +1 more source
Characterization of exoplanets in the James Webb Space Telescope era. [PDF]
Lunine JI, Bahcall N.
europepmc +1 more source
Mantle redox state drives outgassing chemistry and atmospheric composition of rocky planets. [PDF]
Ortenzi G +10 more
europepmc +1 more source

