Abstract
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.
| Original language | English (US) |
|---|---|
| Article number | L16204 |
| Journal | Geophysical Research Letters |
| Volume | 33 |
| Issue number | 16 |
| DOIs | |
| State | Published - Aug 1 2006 |
ASJC Scopus subject areas
- Geophysics
- General Earth and Planetary Sciences
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