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Geomorphic evidence for ancient seas on MarsGeomorphic evidence is presented for ancient seas on Mars. Several features, similar to terrestrial lacustrine and coastal features, were identified along the northern plains periphery from Viking images. The nature of these features argues for formation in a predominantly liquid, shallow body of standing water. Such a shallow sea would require either relatively rapid development of shoreline morphologies or a warmer than present climate at the time of outflow channel formation.
Document ID
19890001442
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Parker, Timothy J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Schneeberger, Dale M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Pieri, David C.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Saunders, R. Stephen
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 5, 2013
Publication Date
January 1, 1987
Publication Information
Publication: Lunar and Planetary Inst., MECA Symposium on Mars: Evolution of its Climate and Atmosphere
Subject Category
Lunar And Planetary Exploration
Accession Number
89N10813
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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