This image set was taken at a distance of 15,000 kilometers (9,300 miles)
from Titan and shows two views of an area riddled by mountain ranges that
were probably produced by tectonic forces.
Near the bottom of the right image, a band of bright clouds is seen. These
clouds are probably produced when gaseous methane in Titan's atmosphere
cools and condenses into methane fog as Titan's winds drive air over the
mountains. It was once thought that these recurring clouds were produced
by volcanic activity on Titan, but this image calls that idea into
question.
These views were obtained during an Oct. 25 flyby designed to obtain the
highest-resolution infrared views of Titan yet. Cassini's visual and
infrared mapping spectrometer resolved surface features as small as 400
meters (1,300 feet). The images were taken at wavelengths of 1.3 microns
shown in blue, 2 microns shown in green, and 5 microns shown in red.
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 Visual
and Infrared Mapping Spectrometer team is based at the University of
Arizona where this image was produced.
For more information about the Cassini-Huygens mission visit
http://saturn.jpl.nasa.gov/. The visual and infrared mapping spectrometer
team homepage is at http://wwwvims.lpl.arizona.edu.
