Geologic evolution of the east rim of the Hellas basin, Mars

Details Geologic evolution of the east rim of the Hellas basin, Mars Geologic evolution of the east rim of the Hellas basin, Mars

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar..100....1c&link_type=abstract

Icarus (ISSN 0019-1035), vol. 100, no. 1, p. 1-25.

Mathematics

Logic

104

Geochronology, Mars Craters, Mars Surface, Planetary Geology, Structural Basins, Frequency Distribution, Highlands, Rims, Structural Properties (Geology), Tectonics, Volcanology

Scientific paper

The east rim of the Hellas basin, one of the largest obvious impact features on Mars, is studied. The distribution of geologic materials in the region is documented, and their modes of origin are constrained based on their geomorphologic characteristics. Superposition relationship and crater size-frequency distributions allow the relative ages of the geologic units to be determined and provide information regarding the timing and extent of the geologic processes emplacing and modifying the surface materials. Systematic analysis of the degradation of the Hellas basin is used to illustrate the sequence of events and interplay of geologic processes which control the evolution of many regions on Mars.

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