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Measured Fluid Flow in an Active H2O-CO2 Geothermal Well as an Analog to Fluid Flow in Fractures on Mars: Preliminary ReportWater in the Earth's crust generally contains dissolved gases such as CO2. Models for both 'Blue Mars' (H2O-driven processes) and 'White Mars' (CO2-driven processes) predict liquid H2O with dissolved CO2 at depth. The fate of dissolved CO2 as this mixture rises toward the surface has not been quantitatively explored. Our approach is a variation on NASA's 'Follow the Water' as we 'Follow the Fluid' from depth to the surface in hydrothermal areas on Earth and extrapolate our results to Mars. This is a preliminary report on a field study of fluid flow in a producing geothermal well. For proprietary reasons, the name and location of this well cannot be revealed, so we have named it 'Earth1' for this study.
Document ID
20040062145
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Kieffer, Susan W.
(Illinois Univ. Urbana, IL, United States)
Brown, K. L.
(Auckland Univ. New Zealand)
Simmons, Stuart F.
(Auckland Univ. New Zealand)
Watson, Arnold
(Auckland Univ. New Zealand)
Date Acquired
August 21, 2013
Publication Date
January 1, 2004
Publication Information
Publication: Lunar and Planetary Science XXXV: Mars: Gullies, Fluids, and Rocks
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
CONTRACT_GRANT: NAG5-12747
Distribution Limits
Public
Copyright
Public Use Permitted.
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