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Pressurized groundwater outflow experiments and numerical modeling for outflow channels on Mars

Marra, Wouter A.; Hauber, Ernst; McLelland, Stuart J.; Murphy, Brendan J.; Parsons, Daniel R.; Conway, Susan J.; Roda, Manuel; Govers, Rob; Kleinhans, Maarten G.

Authors

Wouter A. Marra

Ernst Hauber

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Dr Stuart McLelland S.J.McLelland@hull.ac.uk
Deputy Director of the Energy and Environment Institute

Brendan J. Murphy

Susan J. Conway

Manuel Roda

Rob Govers

Maarten G. Kleinhans



Abstract

© 2014. American Geophysical Union. All Rights Reserved. The landscape of Mars shows incised channels that often appear abruptly in the landscape, suggesting a groundwater source. However, groundwater outflow processes are unable to explain the reconstructed peak discharges of the largest outflow channels based on their morphology. Therefore, there is a disconnect between groundwater outflow processes and the resulting morphology. Using a combined approach with experiments and numerical modeling, we examine outflow processes that result from pressurized groundwater. We use a large sandbox flume, where we apply a range of groundwater pressures at the base of a layer of sediment. Our experiments show that different pressures result in distinct outflow processes and resulting morphologies. Low groundwater pressure results in seepage, forming a shallow surface lake and a channel when the lake overflows. At intermediate groundwater pressures, fissures form and groundwater flows out more rapidly. At even higher pressures, the groundwater initially collects in a subsurface reservoir that grows due to flexural deformation of the surface. When this reservoir collapses, a large volume of water is released to the surface. We numerically model the ability of these processes to produce floods on Mars and compare the results to discharge estimates based on previous morphological studies. We show that groundwater seepage and fissure outflow are insufficient to explain the formation of large outflow channels from a single event. Instead, formation of a flexure-induced subsurface reservoir and subsequent collapse generates large floods that can explain the observed morphologies of the largest outflow channels on Mars and their source areas.

Citation

Marra, W. A., Hauber, E., McLelland, S. J., Murphy, B. J., Parsons, D. R., Conway, S. J., …Kleinhans, M. G. (2014). Pressurized groundwater outflow experiments and numerical modeling for outflow channels on Mars. Journal of Geophysical Research: Planets, 119(12), 2668-2693. https://doi.org/10.1002/2014JE004701

Acceptance Date Nov 21, 2014
Online Publication Date Nov 26, 2014
Publication Date 2014-12
Deposit Date Dec 22, 2016
Publicly Available Date Dec 22, 2016
Journal Journal of geophysical research : planets
Print ISSN 2169-9097
Electronic ISSN 2169-9100
Publisher American Geophysical Union
Peer Reviewed Peer Reviewed
Volume 119
Issue 12
Pages 2668-2693
DOI https://doi.org/10.1002/2014JE004701
Keywords Mars; Fluvial processes; Groundwater; Hydrology; Experiments; Outflow channels
Public URL https://hull-repository.worktribe.com/output/446666
Publisher URL http://onlinelibrary.wiley.com/doi/10.1002/2014JE004701/abstract
Additional Information This is the author's accepted manuscript of an article published in: Journal of geophysical research : planets, 2014, v.119 issue 12.

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