CICLOPS: Cassini Imaging Central Laboratory for OPerationS

F Ring Edge
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Structure in Saturn's narrow and complex F ring is seen here, including one of the faint strands (at left) that Cassini has shown to curl around the planet in a tight, rotating spiral. Scientists think the spiral structure might be due to perturbations of micron-sized F ring particles by a tiny satellite (or satellites).

The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Jan. 19, 2006, at a distance of approximately 1.2 million kilometers (700,000 miles) from Saturn and from just above the ringplane. The image scale is 7 kilometers (4 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.

For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org.

Credit: NASA/JPL/Space Science Institute
Released: February 28, 2006 (PIA 08123)
Image/Caption Information
  F Ring Edge
PIA 08123

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