Geology of Titan from Cassini RADAR - Latest Results

Details Geology of Titan from Cassini RADAR - Latest Results Geology of Titan from Cassini RADAR - Latest Results

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007epsc.conf..647l&link_type=abstract

European Planetary Science Congress 2007, Proceedings of a conference held 20-24 August, 2007 in Potsdam, Germany. Online at ht

Physics

Scientific paper

The Cassini RADAR experiment continues to reveal Titan's striking and diverse geology via synthetic aperture radar (SAR) mapping. Each radar pass covers 1-2% of Titan's surface with resolution as high as 300m. Vast equatorial dunefields, extensive north polar hydrocarbon lakes, mountains, fluvial channels and apparent cryovolcanic features have been observed. This presentation will summarize latest results and plans for forthcoming observations.

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