CICLOPS: Cassini Imaging Central Laboratory for OPerationS
Hiding Rhea

The moon Rhea moves behind Saturn's largest moon, Titan, in this "mutual event" imaged by Cassini.

Mutual event sequences, in which one moon passes close to or in front of another, help scientists refine their understanding of the orbits of Saturn's moons. Part of Rhea's southern hemisphere is also visible here through the haze of Titan's atmosphere. See PIA11692 to watch a movie of a mutual event.

Titan has been brightened by a factor of 1.5 relative to Rhea. This view looks toward the anti-Saturn side of Titan (5150 kilometers, 3200 miles across) and the trailing hemisphere of Rhea (1528 kilometers, 949 miles across).

The image was taken in visible green light with the Cassini spacecraft narrow-angle camera on Nov. 27, 2009. The view was obtained at a distance of approximately 1.2 million kilometers (746,000 miles) from Titan and from 2.3 million kilometers (1.4 million miles) from Rhea. Image scale in the original image was 14 kilometers (9 miles) per pixel on Titan and 27 kilometers (17 miles) per pixel on Rhea. The image has been magnified by a factor of two and contrast-enhanced to aid visibility.

The Cassini Equinox Mission is a joint United States and European endeavor. 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 was designed, developed and assembled at JPL. 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 Equinox Mission visit, and

Credit: NASA/JPL/Space Science Institute
Released: March 29, 2010 (PIA 12599)
Image/Caption Information
  Hiding Rhea
PIA 12599

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