Several fundamental problems were addressed in the early impact, tectonic, and volcanic evolution of the martian lithosphere: (1) origin and evolution of the fundamental crustal dichotomy, including development of the highland/lowland transition zone; (2) growth and evolution of the Valles Marineris; and (3) nature and role of major resurfacing events in early martian history. The results in these areas are briefly summarized
Geomorphic mapping, crater counts on selected surfaces, and a detailed study of drainage basins, wer...
The Terra Cimmeria-Nepenthes Mensae Transitional Zone comprises two highly contrasting geologic-geom...
One of the fundamental questions of Martian crustal history is the origin of the crustal dichotomy b...
Four sessions were held: crustal dichotomy; crustal differentiation/volcanism; Tharsis, Elysium, and...
Although not ignored, the problems of the early tectonic and volcanic evolution of Mars have general...
The ancient crust of Mars contains a remarkable record of the planet's early history. With 45% of th...
MOLA data have revealed a large population of "Quasi-Circular Depressions" (QCDs) with little or no ...
The global-scale crustal structure of Mars is shaped by impact basins, volcanic provinces, and a hem...
MOLA data have revealed a large population of "Quasi-Circular Depressions" (QCDs) with little or no ...
This study has provided a more detailed chronology than currently exists in the literature and has c...
Despite research by numerous geologists and geo- physicists, the age and origin of the martian crust...
It is concluded that Mars was dominated by vertical tectonism more than any of the other terrestrial...
Summary: The Martian crustal dichotomy (MCD) between the southern highlands and the northern lowland...
The state of knowledge of tectonic features on Mars was determined and kinematic and mechanical mode...
The role of major impact basins (such as those which formed on the moon before 4 billion years ago) ...
Geomorphic mapping, crater counts on selected surfaces, and a detailed study of drainage basins, wer...
The Terra Cimmeria-Nepenthes Mensae Transitional Zone comprises two highly contrasting geologic-geom...
One of the fundamental questions of Martian crustal history is the origin of the crustal dichotomy b...
Four sessions were held: crustal dichotomy; crustal differentiation/volcanism; Tharsis, Elysium, and...
Although not ignored, the problems of the early tectonic and volcanic evolution of Mars have general...
The ancient crust of Mars contains a remarkable record of the planet's early history. With 45% of th...
MOLA data have revealed a large population of "Quasi-Circular Depressions" (QCDs) with little or no ...
The global-scale crustal structure of Mars is shaped by impact basins, volcanic provinces, and a hem...
MOLA data have revealed a large population of "Quasi-Circular Depressions" (QCDs) with little or no ...
This study has provided a more detailed chronology than currently exists in the literature and has c...
Despite research by numerous geologists and geo- physicists, the age and origin of the martian crust...
It is concluded that Mars was dominated by vertical tectonism more than any of the other terrestrial...
Summary: The Martian crustal dichotomy (MCD) between the southern highlands and the northern lowland...
The state of knowledge of tectonic features on Mars was determined and kinematic and mechanical mode...
The role of major impact basins (such as those which formed on the moon before 4 billion years ago) ...
Geomorphic mapping, crater counts on selected surfaces, and a detailed study of drainage basins, wer...
The Terra Cimmeria-Nepenthes Mensae Transitional Zone comprises two highly contrasting geologic-geom...
One of the fundamental questions of Martian crustal history is the origin of the crustal dichotomy b...