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

Science
By: , and 

Metrics

348
Crossref references
Web analytics dashboard Metrics definitions

Links

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
Additional publication details