T20 Glacial Mars
Sunday, 18 October 2009
8:00 AM - 12:00 PM
A106
WHAT CAUSES RADAR REFLECTIONS INSIDE MARTIAN POLAR DEPOSITS?
Paper number: T20-2
Program: Technical Sessions
Time: 8:15 AM – 8:30 AM
Authors
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Kathryn E. FishbaughSmithsonian Institution, Washington, DC
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John HoltUniversity of Texas at Austin, Austin, TX
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Ken HerkenhoffUS Geological Survey, Flagstaff, AZ
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Sarah MilkovichCalifornia Institute of Technology, Pasadena, CA
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Shane ByrneUniversity of Arizona, Tucson, AZ
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Nathaniel E. PutzigSouthwest Research Institute, Boulder, CO
Abstract
We examine an area of the North Polar Layered Deposits (NPLD) that was observed numerous times by the SHAllow RADar (SHARAD) on MRO, and for which an adjacent trough was imaged in stereo by HiRISE and studied in detail for stratigraphic information [Fishbaugh et al., 2009]. These datasets allow absolute 3D positioning to be obtained for reflecting horizons in the radar data and for the associated nearby outcrop. While the radar reflectors cannot be traced all the way to the sloping exposure, an extrapolation of the flat lying layers of several km does not introduce large errors in elevation position. The upper ~500 m of layers are well-imaged by SHARAD, consisting of individual reflecting horizons, groups of closely spaced reflectors, and regions of low return between reflectors. Preliminary results indicate that radar reflectors may be correlated with so-called “marker beds”, layers with a hummocky, protruding appearance in images of sloping exposures. This suggests that the compositional and/or textural character of these layers provides both a dielectric contrast with adjacent layers, and a mechanical contrast that results in a distinctive weathering style.