Results 61 to 70 of about 252 (123)
The standard formation model of close-in low-mass planets involves efficient inward migration followed by growth through giant impacts after the protoplanetary gas disk disperses.
Tadahiro Kimura +4 more
doaj +1 more source
Temporal variation of planetary iron as a driver of evolution. [PDF]
Wade J +3 more
europepmc +1 more source
The Nature and Origins of Sub-Neptune Size Planets. [PDF]
Bean JL, Raymond SN, Owen JE.
europepmc +1 more source
In previous work, we demonstrated that machine-learning techniques based on mixture density networks (MDNs) are successful in inferring the interior structure of rocky exoplanets with large compositional diversity.
Yong Zhao +3 more
doaj +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
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
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
Fundamentals of Interior Modelling and Challenges in the Interpretation of Observed Rocky Exoplanets. [PDF]
Baumeister P +9 more
europepmc +1 more source

