The southern Utopia highland-lowland boundary (HLB) extends >1500 km westward from northern Nepenthes Mensae to the topographic saddle that separates Isidis and Utopia Planitiae. It contains bench-like platforms that contain depressions, pitted cones (some organized into arcuate chains and thumbprint terrain), isolated domes, lineated depressions, buried circular depressions, ring fractures, polygonal fractures, and other locally- to regionally-dispersed landforms [1]. The objective of our mapping project is to clarify the geologic evolution of the southern Utopia Planitia HLB by identifying the geologic, structural, and stratigraphic relationships of surface materials in MTMs 10237, 15237, 20237, 10242, 15242, 20242, 10247, 15247, and 2024...
A geologic map of the Sedna Planitia (V-19) quadrangle is being completed at the 1:5,000,000 scale a...
The Hellas impact basin, spanning 2000+ km in the cratered highlands, is the largest well-preserved ...
Abstract. Recently obtained Mars Orbiter Laser Altimeter (MOLA) topography has permitted a new asses...
The southern Utopia highland-lowland boundary (HLB) extends >1500 km westward from Hyblaeus Dorsa to...
The southern Utopia highland-lowland transitional zone extends from northern Terra Cimmeria to south...
Geologic mapping at 1:500,000 scale of the Mars transverse Mercator (MTM) quads 40292 and 40297 is b...
We are approaching the end of the third year of mapping the Athabasca Valles region of Mars. The lin...
As part of a continuing study to understand the relationship between valleys and highland resurfacin...
Geologic mapping of Snegurochka Planitia (V-1) reveals a complex stratigraphy of tectonic and volcan...
Mawrth Vallis is a 15-25 km wide, 500 km long sinuous channel that winds through the highlands of Ar...
The highland-lowland boundary (HLB) of Mars is interpreted to be a complex tectonic and erosional tr...
The primary objective of the mapping effort is to produce a geologic map of the Argyre basin and sur...
Virtually the entire map area is mantled by an irregular deposit of material that is apparently fine...
As part of a continuing study to understand the relationship between valleys and highland resurfacin...
Geologic mapping of MTM -30247, -35247, and -40247 quadrangles is being used to characterize Reull V...
A geologic map of the Sedna Planitia (V-19) quadrangle is being completed at the 1:5,000,000 scale a...
The Hellas impact basin, spanning 2000+ km in the cratered highlands, is the largest well-preserved ...
Abstract. Recently obtained Mars Orbiter Laser Altimeter (MOLA) topography has permitted a new asses...
The southern Utopia highland-lowland boundary (HLB) extends >1500 km westward from Hyblaeus Dorsa to...
The southern Utopia highland-lowland transitional zone extends from northern Terra Cimmeria to south...
Geologic mapping at 1:500,000 scale of the Mars transverse Mercator (MTM) quads 40292 and 40297 is b...
We are approaching the end of the third year of mapping the Athabasca Valles region of Mars. The lin...
As part of a continuing study to understand the relationship between valleys and highland resurfacin...
Geologic mapping of Snegurochka Planitia (V-1) reveals a complex stratigraphy of tectonic and volcan...
Mawrth Vallis is a 15-25 km wide, 500 km long sinuous channel that winds through the highlands of Ar...
The highland-lowland boundary (HLB) of Mars is interpreted to be a complex tectonic and erosional tr...
The primary objective of the mapping effort is to produce a geologic map of the Argyre basin and sur...
Virtually the entire map area is mantled by an irregular deposit of material that is apparently fine...
As part of a continuing study to understand the relationship between valleys and highland resurfacin...
Geologic mapping of MTM -30247, -35247, and -40247 quadrangles is being used to characterize Reull V...
A geologic map of the Sedna Planitia (V-19) quadrangle is being completed at the 1:5,000,000 scale a...
The Hellas impact basin, spanning 2000+ km in the cratered highlands, is the largest well-preserved ...
Abstract. Recently obtained Mars Orbiter Laser Altimeter (MOLA) topography has permitted a new asses...