- Restrictions on Access:
- Unclassified, Unlimited, Publicly available.
- Wrinkle ridges on Mars occur almost exclusively in smooth plains material referred to as ridged plains. One of the largest contiguous units of ridged plains occurs on Lunae Planum on the eastern flank of the Tharsis rise. The eastern, western, and northern margins of the ridged plains of Lunae Planum suffered extensive erosion in early Amazonian channel-forming events. The most dramatic example of erosion in early Amazonian plains is in Kasei Valles. The nature an origin of the wrinkle ridges in the floor material of Kasei Valles are discussed.
- Document ID: 19920001737.
Accession ID: 92N10955.
NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990; p 575-577.
Lunar and Planetary Science Conference; 18-22 Mar. 1991; Houston, TX; United States.
- No Copyright.
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