Cassini observations of flow-like features in western Tui Regio, Titan

Details Cassini observations of flow-like features in western Tui Regio, Titan Cassini observations of flow-like features in western Tui Regio, Titan

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006georl..3316204b&link_type=abstract

Geophysical Research Letters, Volume 33, Issue 16, CiteID L16204

Physics

36

Planetary Sciences: Solid Surface Planets: Origin And Evolution, Planetary Sciences: Solid Surface Planets: Surface Materials And Properties, Planetary Sciences: Solid Surface Planets: Volcanism (6063, 8148, 8450), Planetary Sciences: Solar System Objects: Titan

Scientific paper

A large (>3 × 104 km2), lobate, 5-μm-bright region seen by Cassini on Titan's leading equatorial region is best explained as a flow field. We discuss observations from the Visual and Infrared Mapping Spectrometer and Imaging Science Subsystem of the feature and present a map of the field. We establish relative ages of flow features and discuss possible formation mechanisms and the implications of this finding for the evolution of Titan's surface.

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