The extreme contrast in this view of the unlit side of the rings is intentional. Contrast-enhanced views like this are used to look for spokes (the transient, ghostly lanes of dust seen in Voyager and Hubble Space Telescope images), but so far, none have been seen by Cassini.
The apparent absence of spokes is thought to be related to the Sun's elevation angle above the ringplane, which currently is rather high. As summer wanes in the southern hemisphere, the Sun's angle will drop, and spoke viewing is expected to become more favorable.
In unlit-side views, the denser ring regions (and empty gaps) appear dark, while less populated and dustier ring regions appear bright.
The image was taken in visible light with the wide angle camera on Aug. 3, 2005, from a distance of approximately 781,000 kilometers (485,000 miles) from Saturn. The image scale is 43 kilometers (27 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 Science Mission Directorate, Washington, D.C. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.