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Morphology of Wrinkle Ridges on Lunae and Solis Plana, Mars from MOLA Topography: Implications for Their Kinematic DevelopmentMars Orbiter Laser Altimeter (MOLA) topography is used to define the detailed morphology and kinematic development of martian wrinkle ridges on Lunae and Solis Plana. Changes in ridge morphology suggest they form as fault-propagation folds, often with significant backthrusts. Additional information is contained in the original extended abstract.
Document ID
Document Type
Conference Paper
Tate, A.
(Colorado Univ. Boulder, CO United States)
Golombek, M. P.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Mueller, K. J.
(Colorado Univ. Boulder, CO United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20010044353Analytic PrimaryLunar and Planetary Science XXXII
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