Mathematics – Logic
Scientific paper
Dec 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980amsci..68..626c&link_type=abstract
American Scientist, vol. 68, Nov.-Dec. 1980, p. 626-635.
Mathematics
Logic
1
Geology, Mars Surface, Space Exploration, Mars Craters, Spaceborne Photography, Tectonics, Mars, Geology, Volcanism, Tectonism, Features, Surface, Maps, Wind, Terrain, Craters, Plains, Photographs, Eolian Processes, Polar Regions, Comparisons, Review, Water, Ice, Weathering, Lithosphere, Topography, Atmosphere, History
Scientific paper
The geology of Mars is reviewed on the basis of recent spacecraft imagery of the Martian surface. Following a brief survey of physical properties which may affect Martian geology, the distribution and appearance of the Martian plains, heavily cratered regions and cratered uplands are discussed, with attention given to the volcanic, eolian, fluvial and impact origin and history of these features. Consideration is given to the Martian volcanoes, particularly in the Tharsis and Elysium regions, and to the tectonic features observed as canyons. The apparently fluvial and eolian features on Mars are discussed, with attention given to the three main types of channels and the effects of the wind in redistributing particle debris, and the young, layered deposits in the polar regions are considered. It is concluded that although Mars, like earth, is a volcanically and tectonically active planet, whose surface has been affected by wind, water and ice, the surface is relatively inactive and geological features survive almost unchanged.
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