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Volatile history of Mangala Valles, MarsThe Mangala Valles channel system differs from other Mars outflow channels as they emanate from a point source determined by the local interplay of tectonism, volcanism, and volatiles that led directly to the release of groundwater. Water discharge rates through the southern reaches of Mangala Valles may have been substantially lower than estimates determined fron the canyon system as a whole, suggesting that the accumulation and release of water may have lasted longer than previously envisioned. The sequence of events determined from mapping of units along the southern reaches of Mangala Valles is closely related to the area structures.
Document ID
19930034751
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Zimbelman, James R.
(NASA Headquarters Washington, DC United States)
Craddock, Robert A.
(National Air and Space Museum Washington, United States)
Greeley, Ronald
(Arizona State Univ. Tempe, United States)
Kuzmin, Ruslan O.
(Russian Academy of Sciences Inst. of Geochemistry and Analytical Chemistry, Moscow, Russia)
Date Acquired
August 15, 2013
Publication Date
November 25, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: E11
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
93A18748
Funding Number(s)
CONTRACT_GRANT: NASW-4574
CONTRACT_GRANT: NAGW-1390
Distribution Limits
Public
Copyright
Other

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