Dao, Harmakhis, and Reull Valles - The role of outflow channels in the degradation of the circum-Hellas highlands of Mars

Mathematics – Logic

Scientific paper

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Mars Surface, Highlands, Planetary Geology, Mars Craters, Planetary Mapping, Mineral Deposits, Structural Basins, Tectonics, Mars Volcanoes

Scientific paper

Geologic deposits and landforms representative of much of the planet's history are preserved in the southern cratered highlands of Mars. The circum-Hellas highlands to the east of the basin record the effects of volcanism, tectonism, fluvial erosion and deposition, aeolian activity, and masswasting. Mapping studies and geomorphic analyses have provided a general understanding of the evolution of the Hellas region, placed constraints on the styles and timing of volcanic activity associated with Hadriaca and Tyrrhena Paterae, and investigated Dao and Harmakhis Valles and the terminus of Reull Vallis. The present study provides a detailed comparison of Dao, Harmakhis, and Reull Valles, and examines the role of highland outflow channels in the degradation of the region.

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