The sand seas of titan: Cassini RADAR observations of longitudinal dunes

Science
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Abstract

The most recent Cassini RADAR images of Titan show widespread regions (up to 1500 kilometers by 200 kilometers) of near-parallel radar-dark linear features that appear to be seas of longitudinal dunes similar to those seen in the Namib desert on Earth. The Ku-band (2.17-centimeter wavelength) images show ∼100-meter ridges consistent with duneforms and reveal flow interactions with underlying hills. The distribution and orientation of the dunes support a model of fluctuating surface winds of ∼0.5 meter per second resulting from the combination of an eastward flow with a variable tidal wind. The existence of dunes also requires geological processes that create sand-sized (100- to 300-micrometer) particulates and a lack of persistent equatorial surface liquids to act as sand traps.

Publication type Article
Publication Subtype Journal Article
Title The sand seas of titan: Cassini RADAR observations of longitudinal dunes
Series title Science
DOI 10.1126/science.1123257
Volume 312
Issue 5774
Year Published 2006
Language English
Publisher Nature Research
Contributing office(s) Astrogeology Science Center
Description 4 p.
Larger Work Type Article
Larger Work Subtype Journal Article
Larger Work Title Science
First page 724
Last page 727
Other Geospatial Titan
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