Large-Scale Fault-controlled Paleo-Fluid Flow in the Valles Marineris: Fault-Continuation Ridges

Details Large-Scale Fault-controlled Paleo-Fluid Flow in the Valles Marineris: Fault-Continuation Ridges Large-Scale Fault-controlled Paleo-Fluid Flow in the Valles Marineris: Fault-Continuation Ridges

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3187t&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3187

Physics

Scientific paper

Traces of some graben-bounding faults adjacent to the Valles Marinis can
be followed as ridges, to >100 km long, on the VM walls. As with the
much smaller ridges in VM interior deposits, these ridges are likely to
be fault planes hardened and bleached by flowing groundwater.

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