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Don Quixote Pond: A Small Scale Model of Weathering and Salt AccumulationThe formation of Don Quixote Pond in the North Fork of Wright Valley, Antarctica, is a model for unique terrestrial calcium, chlorine, and sulfate weathering, accumulation, and distribution processes. The formation of Don Quixote Pond by simple shallow and deep groundwater contrasts more complex models for Don Juan Pond in the South Fork of Wright Valley. Our study intends to understand the formation of Don Quixote Pond as unique terrestrial processes and as a model for Ca, C1, and S weathering and distribution on Mars.
Document ID
20150002983
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Englert, P.
(Hawaii Univ. Honolulu, HI, United States)
Bishop, J. L.
(Search for Extraterrestrial Intelligence Inst. Mountain View, CA, United States)
Patel, S. N.
(San Jose State Univ. San Jose, CA, United States)
Gibson, E. K.
(NASA Johnson Space Center Houston, TX, United States)
Koeberl, C.
(Naturhistorisches Museum Vienna, Austria)
Date Acquired
March 16, 2015
Publication Date
March 16, 2015
Subject Category
Geosciences (General)
Geophysics
Report/Patent Number
JSC-CN-32877
Report Number: JSC-CN-32877
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 16, 2015
End Date: March 20, 2015
Sponsors: Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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