Results 81 to 90 of about 1,240 (223)
Abstract The Martian surface, with its diverse landforms that reflect the planet's evolution, has attracted increasing scientific interest. While extensive data is needed for interpretation, identifying landform types is crucial. This semantic information reveals underlying features and patterns, offering valuable scientific insights.
Yuan Ma, Zhaojin Li, Bo Wu, Ran Duan
wiley +1 more source
The Link Between Subsurface Rheology and Ejecta Mobility: The Case of Small New Impacts on Mars
Abstract The dynamics of crater ejecta are sensitive to the material properties of the target, much like the crater size and morphology. We isolate and quantify the effect of target properties on the ejecta mobility (EM) ‐ the maximum radial extent of ejecta scaled by the crater radius.
A. J. Sokolowska +3 more
wiley +1 more source
Episodic flood inundations of the northern plains of Mars [PDF]
Throughout the recorded history of Mars, liquid water has distinctly shaped its landscape, including the prominent circum-Chryse and the northwestern slope valleys outflow channel systems, and the extremely flat northern plains topography at the distal ...
Anderson, Robert C. +6 more
core +1 more source
Gravity and Magnetic Field Signatures in Hydrothermally Affected Regions on Mars
Abstract Multiple lines of evidence indicate that liquid water‐rock interactions occurred on ancient Mars, particularly within the crust, where hydrothermal systems have been hypothesized. Such hydrothermal circulation (HC) can significantly lower temperatures in the crust, thereby restricting the viscoelastic relaxation of impact craters. Craters with
Anna Mittelholz +3 more
wiley +1 more source
Mud Flows in the Southwestern Utopia Planitia, Mars
Vojtěch Cuřín +3 more
openalex +2 more sources
Anomalies of Density, Stresses, and the Gravitational Field in the Interior of Mars
We determined the possible compensation depths for relief harmonics of different degrees and orders. The relief is shown to be completely compensated within the depth range of 0 to 1400 km.
A. S. Konopliv +14 more
core +1 more source
Statistical Characteristics of Nighttime ULF Waves Observed on the Surface of Mars by InSight
Abstract Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) Fluxgate Magnetometer returned data from the Martian surface throughout the course of the InSight mission, between November 2018 and May 2022. Ultra‐low frequency (ULF) electromagnetic waves are commonly observed by InSight during nighttime hours.
K. Webster, Y. Ma, S. Joy, P. J. Chi
wiley +1 more source
Possible ice-wedge polygonisation in Utopia Planitia, Mars and its poleward gradient of latitude [PDF]
<p><strong>Introduction</strong></p> <p>On Mars, polygonally patterned ground is widespread at the mid to high latitudes and it is accepted to result from thermal contraction of ice-cemented soil<sup>1</sup>. Low-centered polygons (LCPs), i.e.
Richard J. Soare +6 more
openaire +2 more sources
Abstract Recent observations by instruments aboard the ExoMars Trace Gas Orbiter (TGO) have revealed the seasonal presence of hydrogen chloride (HCl $\text{HCl}$) in the Martian atmosphere. This discovery may have important implications for Martian photochemistry as chlorine species are chemically active, and it may provide a link between the ...
K. Rajendran +7 more
wiley +1 more source
Atmospheric Gravity Waves in Mars' Lower Atmosphere: Nadir Observations From OMEGA/Mars Express Data
Abstract We present the detection and characterization of mesoscale waves on the lower clouds of Mars (20–40 km) using hyperspectral images from the Observatoire pour la Minéralogie, l’Eau, les Glaces et l’Activité (OMEGA) onboard the European Mars Express space mission.
F. Brasil +8 more
wiley +1 more source

