Frigid Titan continues to prove itself a remarkably complex and dynamic
world. Here, bright clouds are seen encircling the moon's north polar
region.
The Cassini spacecraft has revealed the presence of great lakes and seas
of liquid hydrocarbons on this part of Titan's surface (see PIA08365 and
PIA08930). An extended, high-altitude haze
hovers above the limb of Titan (5,150 kilometers, or 3,200 miles across)
at top of the image.
The image was taken with the Cassini spacecraft narrow-angle camera on
April 26, 2008 using a spectral filter sensitive to wavelengths of
infrared light centered at 938 nanometers. The view was acquired at a
distance of approximately 786,000 kilometers (488,000 miles) from Titan.
Image scale is 5 kilometers (3 miles) per pixel.
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 and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
http://saturn.jpl.nasa.gov/. The Cassini imaging team
homepage is at http://ciclops.org.
