Abstract
GEOPHYSICAL RESEARCH LETTERS,
VOL. 37,
L06203,
7 PP., 2010
doi:10.1029/2009GL042192
Evidence for present day gully activity on the Russell crater dune field, Mars
Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Münster, Germany
Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Münster, Germany
Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Münster, Germany
Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Münster, Germany
On the basis of High Resolution Imaging Science Experiment (HiRISE) images of two successive years we observed changes of a gully on the Russell crater dune field. Within the first year the length of a ∼2 m wide incised gully channel grew about 50 m downslope, and ∼120 m within in the second year. Gully activity occurred in early spring between LS ∼198° and ∼218° in the first year and between LS ∼192° and ∼221° in the second year. Based on the channel morphology, spectral data and modeled surface temperatures, the changes can be best explained with transient melting of small amounts of H2O-ice triggering slurry flows consisting of sand mixed with liquid water.
Received 15 December 2009; accepted 22 February 2010; published 26 March 2010.
Citation: (2010), Evidence for present day gully activity on the Russell crater dune field, Mars, Geophys. Res. Lett., 37, L06203, doi:10.1029/2009GL042192.
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