Wavy bands in Saturn's high atmosphere lazily circle the south polar
region in this Cassini image, taken through a filter sensitive to
ultraviolet light.
At these wavelengths, gas in the atmosphere scatters sunlight more than
the particles that make up the clouds, so the clouds look dark. This
scattering of short-wavelength light by gas molecules is called Rayleigh
scattering, and is the phenomenon that makes Earth's sky look blue.
The bright wedge near the lower-left limb of the planet falls in a
latitude band just south of the dark `polar collar'. Imaging scientists
can discern from this image that the stratosphere in this more southerly
latitude band is relatively pure hydrogen and helium and contains very
little of the stratospheric haze that causes darkening closer to the pole.
This image was taken with the Cassini spacecraft narrow angle camera on
Aug. 27, 2004, at a distance of 9 million kilometers (5.6 million miles)
from Saturn. The image scale is 108 kilometers (67 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.
