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Radar-bright channels on Titan |
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| Authors: | A Le Gall MA Janssen RD Lorenz the Cassini Radar Team |
| Institution: | a Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, United States b Observatoire Aquitain des Sciences de l’Univers, University of Bordeaux I, 33271 Floirac, France c Space Department, Planetary Exploration Group, Johns Hopkins University Applied Physics Lab, Laurel, MD 20723, United States |
| Abstract: | During Cassini’s T44 flyby of Titan (May 28, 2008), the Cassini SAR (synthetic aperture radar) revealed sinuous channels in the Southwest of Xanadu. These channels feature very large radar cross-sections, up to 5 dB, whereas the angle of incidence was relatively high, ∼20°. This backscatter is larger than allowed by the coherent backscatter model considered to explain the unusual reflective and polarization properties of the icy satellites and only a few radar scattering mechanisms can be responsible for such high radar returns. The presence of rounded (icy) pebbles with size larger than the radar wavelength (2.18 cm) is proposed to explain the large radar cross-sections measured in these units. The radar-bright channels are thus interpreted as riverbeds, where debris, likely shaped and transported by fluvial activity, have been deposited. Similar debris were observed in the landing site of the Huygens probe. This work may point the way to an explanation for the enhanced brightness of other fluvial regions of Titan. |
| Keywords: | Titan Radar observations Radio observations Satellites Surfaces Geological processes |
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