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The Origin of Carbon-Bearing Volatiles in a Continental Hydrothermal System in the Great Basin: Water Chemistry and Isotope CharacterizationsHydrothermal systems on Earth are active centers in the crust where organic molecules can be synthesized biotically or abiotically under a wide range of physical and chemical conditions [1-3]. Not only are volatile species (CO, CO2, H2, and hydrocarbons) a reflection of deep-seated hydrothermal alteration processes, but they also form an important component of biological systems. Studying carbon-bearing fluids from hydrothermal systems is of specific importance to understanding (bio-)geochemical processes within these systems. With recent detection of methane in the martian atmosphere [4-7] and the possibility of its hydrothermal origin [8, 9], understanding the formation mechanisms of methane may provide constraints on the history of the martian aqueous environments and climate.
Document ID
20120003011
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Fu, Qi
(Lunar and Planetary Inst. Houston, TX, United States)
Socki, Richard A.
(Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Niles, Paul B.
(NASA Johnson Space Center Houston, TX, United States)
Romanek, Christopher
(Kentucky Univ. Lexington, KY, United States)
Datta, Saugata
(Kansas State Univ. Manhattan, KS, United States)
Darnell, Mike
(Houston Univ. Houston, TX, United States)
Date Acquired
August 25, 2013
Publication Date
March 19, 2012
Subject Category
Geophysics
Report/Patent Number
JSC-CN-25782
Meeting Information
Meeting: 43rd Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 19, 2012
End Date: March 23, 2012
Sponsors: Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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