The morphology of the Martian surface

Details The morphology of the Martian surface The morphology of the Martian surface

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...25..231c&link_type=abstract

Space Science Reviews, vol. 25, Mar. 1980, p. 231-284.

Physics

8

Geomorphology, Mars Surface, Topography, Viking Orbiter Spacecraft, Asymmetry, Geochronology, Impact Damage, Photographs, Planetary Craters, Surface Properties, Surface Temperature, Tectonics, Volcanology, Wind Erosion, Review, Mars, Morphology, Surface, Topography, Channels, Ages, Fractures, Volcanoes, Plains, Terrain, Tharsis Bulge, Tectonism, Chryse Planitia, Valles Marineris, Faulting, Layers, Impact Craters, Ice, Polar Regions, Volatiles, Aeolian Processes, Dunes, Dust Storms, Photographs, Features, El

Scientific paper

Data on the Martian surface are reviewed and illustrated with Viking Orbiter pictures. Various surface temperatures are discussed, including densely cratered terrains; chaotic, fretted, and knobby terrains; sparsely cratered plains; volcanic features; and channels. Tectonic features, Valles Marineris, impact craters, polar regions, and aeolian features are also discussed. It is shown that Mars is asymmetric in its topography, distribution of surface features, and physiography. Physiographic differences are discussed together with some hypotheses proposed to explain the differences.

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