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