Cassini's climb to progressively higher elevations reveals the "negative"
side of Saturn's rings. As the Sun shines through the rings, they take on
the appearance of a photonegative: the dense B ring (at the center) blocks
much of the incoming light, while the less dense regions scatter and
transmit light.
Close inspection reveals not one, but two moons in this scene. Mimas (397
kilometers, or 247 miles across) is easily visible near the upper right,
but the shepherd moon Prometheus (102 kilometers, or 63 miles across) can
also be seen. Prometheus is a dark spot against the far side of the thin,
bright F ring. Most of Prometheus' sunlit side is turned away from Cassini
in this view.
The image was taken in visible light with the Cassini spacecraft
wide-angle camera on April 15, 2005, at a distance of approximately
570,000 kilometers (350,000 miles) from Saturn. The image scale is 30
kilometers (19 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 team is based at the Space Science
Institute, Boulder, Colo.
For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov.
For additional images visit the Cassini imaging team homepage http://ciclops.org.
