Geologic map of the Phaethontis Quadrangle of Mars
January 1, 1979
The Phaethontis quadrangle of Mars is dominated by densely cratered uplands and plateaus which form some of the oldest surfaces on the planet. Extensive low-lying areas within the cratered terrains, including the floors of the large craters, are covered to different degrees by plains-forming material. The youngest plains unit surround Tharsis Montes to the north. Various erosional processes, including eolian scour and possibly scarp retreat through volatile-release sapping and mass wasting, producing several distinctive physiographic features: knob and mesa terrains, plains and small knobs, and plateaus dissected by furrows, steep walled gorges, and pits.
Citation Information
Publication Year | 1979 |
---|---|
Title | Geologic map of the Phaethontis Quadrangle of Mars |
DOI | 10.3133/i1145 |
Authors | J. H. Howard |
Publication Type | Report |
Publication Subtype | USGS Numbered Series |
Series Title | IMAP |
Series Number | 1145 |
Index ID | i1145 |
Record Source | USGS Publications Warehouse |
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Geologic map of the Phaethontis Quadrangle of Mars
The Phaethontis quadrangle of Mars is dominated by densely cratered uplands and plateaus which form some of the oldest surfaces on the planet. Extensive low-lying areas within the cratered terrains, including the floors of large craters, are covered to different degrees by plains-forming material. The youngest plains units surround Tharsis Montes to the north. Various erosional processes, includin
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Geologic map of the Phaethontis Quadrangle of Mars
The Phaethontis quadrangle of Mars is dominated by densely cratered uplands and plateaus which form some of the oldest surfaces on the planet. Extensive low-lying areas within the cratered terrains, including the floors of large craters, are covered to different degrees by plains-forming material. The youngest plains units surround Tharsis Montes to the north. Various erosional processes, includin