Media Information

 
 
 
Collection:
NASA Cassini-Huygens Collection
Title:
Rippled Rings
Description:
Rippled Rings
Full Description:
Variations in ring particle concentration give Saturn's brilliant rings the appearance of ripples in a pond in this close-up view. Many of the gaps and wavelike patterns elsewhere in the rings are due to the gravitational influence of Saturn¿s moons, but the origin of much of the structure in the B ring seen here is still unexplained.

The image was taken with the Cassini spacecraft narrow angle camera on Oct. 29, 2004, at a distance of approximately 824,000 kilometers (512,000 miles) from Saturn. The image scale is 4.5 kilometers (2.8 miles) per pixel. The image has been slightly contrast-enhanced to aid visibility.

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.n…and the Cassini imaging team home page, http://ciclops.org.

Credit: NASA/JPL/Space Science Institute
Date:
December 21, 2004
Keywords:
images
Keywords:
cassini
Keywords:
rings
facet_what:
Saturn
facet_what:
Cassini
facet_what:
Cassini-Huygens
facet_what:
Huygens Probe
facet_what:
Cassini Orbiter
facet_what:
rings
facet_where:
Saturn
facet_where:
Jet Propulsion Laboratory
facet_where:
California
facet_where:
Washington
facet_where:
Jet Propulsion Laboratory (JPL)
facet_where:
Washington, D.C.
facet_when:
December 21, 2004
facet_when_year:
2004
UID:
SPD-SATRN-1238
original url:

Rippled Rings