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Ice in the northern lowlands and southern highlands of Mars and its enrichment beneath the Elysium LavasThe simultaneously examination of ejecta mobility, crater morphology, and surface features has enabled several conclusions to be drawn regarding the location of subsurface ice in the region. The ice distribution is shown to be highly dependent upon latitude and geological situation; in particular, pronounced differences in the distribution between the highland and lowlands are seen, and concentrations of ice were detected beneath the Elysium lavas.
Document ID
19920019758
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cave, Julie A. (University Coll. London, United Kingdom)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., Workshop on the Martian Surface and Atmosphere Through Time
Subject Category
Lunar And Planetary Exploration
Accession Number
92N29001
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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