The Noachis-Sabaea region in the southern highlands preserves some of the oldest Martian crust. It records deformation by both endogenic and exogenic processes. This deformation includes giant impacts and their impact stresses, which could have resulted in both the reactivation and modification of pre-impact tectonic structures, in addition to impact-generated tectonic structures. There are also widespread extensional and compressional tectonic structures, which were formed due to endogenic processes. We have produced the first detailed morphostructural map of the Noachis-Sabaea region, which details the characteristics and spatial arrangements of structures in the region, forms the basis for making inferences about Noachian-Hesperian crust...
[1] Definitive exposures of pristine, ancient crust on Mars are rare, and the finding that much of t...
Abstract. Recently obtained Mars Orbiter Laser Altimeter (MOLA) topography has permitted a new asses...
Gusev Crater lies within the Aeolis Quadrangle of Mars at the boundary between the northern lowlands...
Extensional and compressional structures are globally abundant on Mars. Distribution of these struct...
A number of tectonic structures have been located at the Thaumasia Plateau, Daedalia Planum and Aoni...
The global-scale crustal structure of Mars is shaped by impact basins, volcanic provinces, and a hem...
Noctis Labyrinthus (Mars) is characterized by many tectonic features, which represent brittle deform...
The primary goal of this dissertation is to understand the geologic history of Mars through the use ...
MOLA data have revealed a large population of "Quasi-Circular Depressions" (QCDs) with little or no ...
As part of a continuing study to understand the relationship between valleys and highland resurfacin...
The Terra Cimmeria-Nepenthes Mensae Transitional Zone comprises two highly contrasting geologic-geom...
International audienceMartian valley networks have been identified mainly in the Noachian heavily cr...
MOLA data have revealed a large population of "Quasi-Circular Depressions" (QCDs) with little or no ...
Detailed photogeologic mapping documents for the first time the deformation sequence of the Coprates...
A detailed planetwide stratigraphy for Mars has been developed from global mapping based on Viking i...
[1] Definitive exposures of pristine, ancient crust on Mars are rare, and the finding that much of t...
Abstract. Recently obtained Mars Orbiter Laser Altimeter (MOLA) topography has permitted a new asses...
Gusev Crater lies within the Aeolis Quadrangle of Mars at the boundary between the northern lowlands...
Extensional and compressional structures are globally abundant on Mars. Distribution of these struct...
A number of tectonic structures have been located at the Thaumasia Plateau, Daedalia Planum and Aoni...
The global-scale crustal structure of Mars is shaped by impact basins, volcanic provinces, and a hem...
Noctis Labyrinthus (Mars) is characterized by many tectonic features, which represent brittle deform...
The primary goal of this dissertation is to understand the geologic history of Mars through the use ...
MOLA data have revealed a large population of "Quasi-Circular Depressions" (QCDs) with little or no ...
As part of a continuing study to understand the relationship between valleys and highland resurfacin...
The Terra Cimmeria-Nepenthes Mensae Transitional Zone comprises two highly contrasting geologic-geom...
International audienceMartian valley networks have been identified mainly in the Noachian heavily cr...
MOLA data have revealed a large population of "Quasi-Circular Depressions" (QCDs) with little or no ...
Detailed photogeologic mapping documents for the first time the deformation sequence of the Coprates...
A detailed planetwide stratigraphy for Mars has been developed from global mapping based on Viking i...
[1] Definitive exposures of pristine, ancient crust on Mars are rare, and the finding that much of t...
Abstract. Recently obtained Mars Orbiter Laser Altimeter (MOLA) topography has permitted a new asses...
Gusev Crater lies within the Aeolis Quadrangle of Mars at the boundary between the northern lowlands...