Encircled in purple stratospheric haze, Titan appears as a softly glowing
sphere in this colorized image taken one day after Cassini's first flyby
of that moon.
This image shows two thin haze layers. The outer haze layer is detached
and appears to float high in the atmosphere. Because of its thinness, the
high haze layer is best seen at the moon's limb.
The image was taken using a spectral filter sensitive to wavelengths of
ultraviolet light centered at 338 nanometers. The image has been falsely
colored: The globe of Titan retains the pale orange hue our eyes usually
see, and both the main atmospheric haze and the thin detached layer have
been brightened and given a purple color to enhance their visibility.
The best possible observations of the detached layer are made in
ultraviolet light because the small haze particles which populate this
part of Titan's upper atmosphere scatter short wavelengths more
efficiently than longer visible or infrared wavelengths.
Images like this one reveal some of the key steps in the formation and
evolution of Titan's haze. The process is thought to begin in the high
atmosphere, at altitudes above 400 kilometers (250 miles), where
ultraviolet light breaks down methane and nitrogen molecules. The
products are believed to react to form more complex organic molecules
containing carbon, hydrogen and nitrogen that can combine to form the
very small particles seen as haze. The bottom of the detached haze layer
is a few hundred kilometers above the surface and is about 120 kilometers
(75 miles) thick.
The image was taken with the narrow angle camera on July 3, 2004, from a
distance of about 789,000 kilometers (491,000 miles) from Titan and at a
Sun-Titan-spacecraft, or phase, angle of 114 degrees. The image scale is
4.7 kilometers (2.9 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 Cassini-Huygens mission for NASA's Office of Space
Science, Washington, D.C. The Cassini orbiter and its two onboard cameras,
were designed, developed and assembled at JPL. The imaging team is based
at the Space Science Institute, Boulder, Colo.
For more information, about the Cassini-Huygens mission visit,
http://saturn.jpl.nasa.gov and the Cassini imaging team home page,
http://ciclops.org.