Observation based climatology Martian atmospheric waves perturbation Datasets. [PDF]
Sci Data, 2023 Zhang J +8 more
europepmc +1 more source
Chemical evolution of the early Martian hydrosphere [PDF]
The chemical evolution of the early Martian hydrosphere is discussed. The early Martian ocean can be modeled as a body of relatively pure water in equilibrium with a dense carbon dioxide atmosphere. The chemical weathering of lavas, pyroclastic deposits,
Schaefer, M. W.
core +1 more source
Deep impact craters in the Isidis and southwestern Utopia Planitia regions of Mars: High target material strength as a possible cause [PDF]
, 2006 J. M. Boyce +3 more
openalex +1 more source
Modern water at low latitudes on Mars: Potential evidence from dune surfaces. [PDF]
Sci Adv, 2023 Qin X +21 more
europepmc +1 more source
Eolian erosion of polygons in the Atacama Desert as a proxy for hyper-arid environments on Earth and beyond. [PDF]
Sci Rep, 2022 Sager C +3 more
europepmc +1 more source
Formation of double‐ring circular grabens due to volumetric compaction over buried impact craters: Implications for thickness and nature of cover material in Utopia Planitia, Mars [PDF]
, 2004 D. L. Buczkowski, Michele L. Cooke
openalex +1 more source
Sheeting joints and polygonal patterns in the Navajo Sandstone, southern Utah: Controlled by rock fabric, tectonic joints, buckling, and gullying [PDF]
, 2018 Sheeting joints are ubiquitous in outcrops of the Navajo Sandstone on the west-central Colorado Plateau, USA. As in granitic terrains, these are opening- mode fractures and form parallel to land surfaces.
Burberry, Caroline M., Loope, David B.
core +1 more source
Evidence for glaciation in Elysium [PDF]
It is suggested that certain landforms in the Elysium region of Mars provide strong evidence for glaciation. Landscapes related to subglacial volcanism suggest that ice was a primary agent in the development of ...
Anderson, Duwayne M. +1 more
core +1 more source
Characterizing Ice-wedge Polygon Geomorphology in the Haughton Impact Structure, Devon Island [PDF]
, 2018 Ice-wedge polygon networks are a common feature in periglacial environments formed through thermal contraction cracking and snowmelt infiltration. Polygons of similar morphology are ubiquitous throughout the mid-latitudes of Mars and are believed to have
Hawkswell, Jordan
core +1 more source
Three New Missions Head for Mars. [PDF]
Engineering (Beijing), 2020 Leslie M.
europepmc +1 more source