Results 101 to 110 of about 176,490 (172)
The bulk compositions of small planets ( R _p < 2 R _⊕ ) are directly linked to their formation histories, making reliable compositional constraints imperative for testing models of planet formation and evolution.
Joseph G. Schulze +3 more
doaj +1 more source
Vertically Resolved Magma Ocean-Protoatmosphere Evolution: H2, H2O, CO2, CH4, CO, O2, and N2 as Primary Absorbers. [PDF]
Lichtenberg T +6 more
europepmc +1 more source
Properties of transiting extrasolar planets
Includes bibliographical references (leaves 42-44)A growing number of extrasolar planets have been detected using transit photometry, and these systems are presently important, in that these planets have strongly constrained parameters, particularly ...
Lund, Michael Bryant
core
Magnetospheric Emission from Extrasolar Planets [PDF]
The magnetospheric emissions from extrasolar planets represent a science frontier for the next decade. All of the solar system giant planets and the Earth produce radio emissions as a result of interactions between their magnetic fields and the solar ...
Majid, W. +14 more
core
Haze Optical Depth in Exoplanet Atmospheres Varies with Rotation Rate: Implications for Observations
Transmission spectroscopy supports the presence of uncharacterized, light-scattering and -absorbing hazes in the atmospheres of many exoplanets. The complexity of factors influencing the formation, 3D transport, radiative impact, and removal of hazes ...
Maureen Cohen +4 more
doaj +1 more source
Observational Signatures of a Previous Dynamical Instability in Multi-planet M-dwarf Systems
We identify observational signatures suggesting a history of dynamical instability in 26 out of 34 M-dwarf multi-planet systems containing no large planets.
Anna C. Childs +4 more
doaj +1 more source
Evaluating the Microbial Habitability of Rogue Planets and Proposing Speculative Scenarios on How They Might Act as Vectors for Panspermia. [PDF]
Schulze-Makuch D, Fairén AG.
europepmc +1 more source
Temporal variation of planetary iron as a driver of evolution. [PDF]
Wade J +3 more
europepmc +1 more source
Introduction-First Billion Years: Habitability. [PDF]
Rivera-Valentín EG +6 more
europepmc +1 more source

