Cryovolcanic Features on Titan's Surface as Revealed by the Cassini RADAR

Details Cryovolcanic Features on Titan's Surface as Revealed by the Cassini RADAR Cryovolcanic Features on Titan's Surface as Revealed by the Cassini RADAR

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1885l&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1885

Physics

4

Scientific paper

The Cassini RADAR obtained SAR images of about 1.1% of Titan's surface
during the spacecraft's fly-by on October 26, 2004. These revealed
surface features that are interpreted as the result of cryovolcanism,
including extensive flows. New results from the T3 fly-by will also be
discussed.

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