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Plate Tectonism on Early Mars: Diverse Geological and Geophysical EvidenceMars has been modified by endogenic and exogenic processes similar in many ways to Earth. However, evidence of Mars embryonic development is preserved because of low erosion rates and stagnant lid convective conditions since the Late Noachian. Early plate tectonism can explain such evidence. Additional information is contained in the original extended abstract.
Document ID
20020046170
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Dohm, J. M.
(Arizona Univ. Tucson, AZ United States)
Maruyama, S.
(Tokyo Inst. of Tech. Japan)
Baker, V. R.
(Arizona Univ. Tucson, AZ United States)
Anderson, R. C.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Ferris, Justin C.
(Arizona Univ. Tucson, AZ United States)
Hare, Trent M.
(Geological Survey Flagstaff, AZ United States)
Date Acquired
August 20, 2013
Publication Date
April 1, 2002
Publication Information
Publication: Lunar and Planetary Science XXXIII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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