This composite of 24 images from the Cassini spacecraft shows multiple
layers in Titan's stratospheric haze. The most prominent layer is located
about 500 kilometers (300 miles) above the surface and is seen at all
latitudes, encircling the moon. The material in this layer is probably a
condensed substance, possibly water ice.
Several other layers are most apparent in the north polar hood (at top),
but this view also shows some at other latitudes. The mechanisms that
produce these layers are not understood, but waves in the atmosphere are
thought to play a significant role.
The images in this composite were taken over a period of 23 minutes. The
images were processed to enhance fine detail and then were combined to
create this view. North on Titan (5,150 kilometers, or 3,200 miles across)
is up.
The images were taken in visible light with the narrow-angle camera on
Jan. 27, 2006 at a distance of approximately 2.3 million kilometers (1.4
million miles) from Titan and at a Sun-Titan-spacecraft, or phase, angle
of 155 degrees. Image scale is 13 kilometers (8 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/home/index.cfm. The Cassini imaging team
homepage is at http://ciclops.org.
