Results 1 to 10 of about 14,343 (306)
Untrackable distal ejecta on planetary surfaces [PDF]
Heterogeneous shock impedances of planetary materials cause abrupt changes of ejection angles, forming non-radial ejecta. Interpretations for provenances of surface deposits and ages derived from crater counts are affected by such untrackable ejecta.
Rui Xu +4 more
doaj +4 more sources
The study of planetary environments of astrobiological interest has become a major challenge. Because of the obvious technical and economical limitations on in situ planetary exploration, laboratory simulations are one of the most feasible research ...
Eva Mateo-Marti
doaj +4 more sources
Decoding planetary surfaces by counting cracks. [PDF]
Planets are often covered with thin cracked shells. From mud films to lithospheres of rock or ice, fracture networks form two-dimensional (2D) tessellations of convex polygons whose geometry encodes their genesis. Here, we chart the geometry of 2D fracture mosaics across the solar system, and decode their formative conditions using a new dynamical ...
Silver S +3 more
europepmc +4 more sources
Electrostatic Repulsion of Dust from Planetary Surfaces
Surfaces of planetary bodies can have strong electric fields, subjecting conductive grains to repulsive electrostatic forces. This has been proposed as a mechanism to eject grains from the ground.
F. Chioma Onyeagusi +3 more
doaj +2 more sources
Exploring the solar system: the view of planetary surfaces with VIS/IR remote sensing methods
The structure of planetary surfaces unveils basic formation processes and evolution lines of different objects in the solar system, and often the view on the top of a planet is the only available information about it. Advanced remote sensing technologies
Gabriele E Arnold
exaly +2 more sources
Fluvial geomorphology on Earth-like planetary surfaces: A review [PDF]
VÍCTOR R Baker +2 more
exaly +2 more sources
We describe a model of the fluid mechanics and thermodynamics of turbulent lava flows capable of thermally eroding sinuous rille channels on bodies without atmospheres.
Lionel Wilson, James W. Head
doaj +1 more source
The surfaces of airless planetary bodies, such as the Moon or Mercury, are covered with regoliths, which interact with the solar wind. The solar protons can either be absorbed by the surface or neutralized and reflected as hydrogen energetic neutral ...
S. Verkercke +6 more
doaj +1 more source
Main Results from the ISSI International Team “Characterization of 67P Cometary Activity”
The ESA/Rosetta mission accompanied the Jupiter Family Comet 67P/Churyumov-Gerasimenko and provided a huge amount of data which are providing important results about cometary activity mechanisms.
Andrea Longobardo +10 more
doaj +1 more source
Planetary-Code-Collection: Thermal, Ice Evolution, and Exosphere Models for Planetary Surfaces
PCC without MSIM: The major change is that MSIM (Mars Subsurface Ice Model) now has its own repository, and is no longer part of the Planetary-Code-Collection.
Schorghofer, Norbert
core +1 more source

