Titan Radar Mapper observations from Cassini's T3 fly-by

Details Titan Radar Mapper observations from Cassini's T3 fly-by Titan Radar Mapper observations from Cassini's T3 fly-by

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006natur.441..709e&link_type=abstract

Nature, Volume 441, Issue 7094, pp. 709-713 (2006).

Mathematics

Logic

51

Scientific paper

Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These data provide the first definitive identification of impact craters on the surface of Titan, networks of fluvial channels and surficial dark streaks that may be longitudinal dunes. Here we describe this great diversity of landforms. We conclude that much of the surface thus far imaged by radar of the haze-shrouded Titan is very young, with persistent geologic activity.

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