Large areas of this Cassini synthetic aperture radar image of Titan are
covered by long, dark ridges. They resemble the "cat scratches" seen in
other places on Titan, but here they are longer and straighter. Spaced
about 1 to 2 kilometers (0.6 to 1 miles) apart, they curve slightly around
teardrop-shaped bright terrain, giving the impression of a Japanese garden
of sand raked around boulders. The bright material appears to be
high-standing rough material that the ridges bend around. This suggests
that the ridges are dunes that winds have blown across the surface of
Titan from left to right (roughly west to east).
This image was taken during the ninth Titan flyby on Oct. 28, 2005, (the
fourth flyby for Cassini's synthetic aperture radar), at a distance of
about 1300 kilometers (800 miles).
The image covers an area roughly 140 kilometers by 200 kilometers (120
miles). It is located 13 degrees south latitude and 300 degrees west
longitude.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter was designed, developed and assembled at JPL. The radar
instrument team is based at JPL, working with team members from the United
States and several European countries.
For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov.
