Press Release
Cassini Maps Global Pattern of Titan’s Dunes
Scientists have used data from the Cassini radar mapper to map the global wind pattern on Saturn's moon Titan using data collected over a four-year period, as depicted in this image.
The arrows indicate the direction in which sand is inferred to be transported along dunes observed in Titan radar data. Underlying the arrows is a base map from Cassini's imaging science subsystem. Many of the equatorial dark areas without arrows might have dunes but have not yet been imaged with radar. The dune orientations represent only the net effect of winds. It could be that sand transport only occurs on rare occasions, and winds from different directions can combine to yield the observed dune orientations.
For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov/home/index.cfm. The Cassini imaging team homepage is at http://ciclops.org.
Credit: NASA/JPL/Space Science Institute
Thu, 02/26/2009 - 09:21
Titan’s vast dune fields, which may act like weather vanes to determine general wind direction on Saturn’s biggest moon, have been mapped by scientists who compiled four years of radar data collected by the Cassini spacecraft.
Titan’s rippled dunes are generally oriented east-west. Surprisingly, their orientation and characteristics indicate that near the surface, Titan’s winds blow toward the east instead of toward the west. This means that Titan’s surface winds blow opposite the direction suggested by previous global circulation models of Titan.
“At Titan there are very few clouds, so determining which way the wind blows is not an easy thing, but by tracking the direction in which Titan’s sand dunes form, we get some insight into the global wind pattern,” says Ralph Lorenz, Cassini radar scientist at The Johns Hopkins University Applied Physics Laboratory in Laurel, Md. “Think of the dunes sort of like a weather vane, pointing us to the direction the winds are blowing.” A paper based on these findings appeared in the Feb. 11 issue of Geophysical Research Letters.
“Titan’s dunes are young, dynamic features that interact with topographic obstacles and give us clues about the wind regimes,” said Jani Radebaugh, Brigham Young University, Provo, Utah. “Winds come at these dunes from at least a couple of different directions, but then combine to create the overall dune orientation.”
The new map, based on all the high-resolution radar data collected during a four-year period, is now available at: http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini.
The wind pattern is important for planning future Titan explorations that might involve balloon-borne experiments.
Some 16,000 dune segments were mapped out from about 20 radar images, digitized and combined to produce the new map.
Titan’s dunes are believed to be made up of hydrocarbon sand grains likely derived from organic chemicals in Titan’s smoggy skies. The dunes wrap around high terrain, which provides some idea of their height. They accumulate near the equator, and may pile up there because drier conditions allow for easy transport of the particles by the wind. Titan’s higher latitudes contain lakes and may be “wetter” with more liquid hydrocarbons, not ideal conditions for creating dunes.
At the Edge of Titan's Dunes
This is a portion of a Cassini radar mapper image obtained by the Cassini spacecraft on its Dec. 21, 2008, flyby of Saturn's moon Titan.
The area shown covers the southern boundary of an equatorial band where longitudinal dunes (dunes that form along the wind direction) are pervasive. Here the dunes are apparently created by winds locally coming from the west and north-west, and generally blowing toward the east. The dunes are interspersed with radar-bright features that are inferred to rise above the surrounding terrain.
In the lower part of the image there are no dunes at all, and the texture is more typical of featureless plains observed in many other areas of Titan that lack dunes. In this transition zone, the sand-sized particles that make up the dunes might not be sWo plentiful. In this case, insufficient sand to replenish the dunes makes them gradually disappear. Compare the nature of these dunes to those seen at the northern boundary of the dune fields observed in radar images obtained during the T3 flyby on Feb. 15, 2005.
The image is centered near 19.2 degrees south and 257.4 degrees west. It covers an area of 220 kilometers (137 miles) by 170 kilometers (106 miles). North is approximately toward the top of the image, the radar illumination is from the right, and the incidence angle is about 25 degrees. The vertical stripe across the image at its center is an artifact in this preliminary version.
Credit: NASA/JPL
Cassini, which launched in 1997 and is now in extended mission operations, continues to blaze its trail around the Saturn system and will visit Titan again on March 27. Seventeen Titan flybys are planned this year.
The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL manages the Cassini-Huygens mission for NASA’s Science Mission Directorate. The Cassini orbiter was designed, developed and assembled at JPL. The radar instrument was built by JPL and the Italian Space Agency, working with team members from the United States and several European countries.