CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Discovery of the Wavemaker
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Discovery of the Wavemaker
PIA 06238

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Discovery of the Wavemaker
PIA 06239

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  Cassiniís celestial sleuthing has paid off with this time-lapse series of images which confirmed earlier suspicions that a small moon was orbiting within the narrow Keeler gap.

The movie sequence (which consists of 12 images taken over 16 minutes while Cassini gazed down upon the sunlit side of the A ring) shows a tiny moon orbiting in the center of the Keeler Gap, churning up waves in the gap edges as it goes. Note that the pattern of waves travels with the moon in its orbit.

The Keeler gap is located about 250 kilometers (155 miles) interior to the outer edge of the A ring, which is also the outer edge of the bright main rings. The new object is about 7 kilometers (4 miles) across and reflects about 50 percent of the sunlight light that falls upon it Ė a brightness that is typical of particles in the nearby rings.

The new body has been provisionally named S/2005 S1.

Imaging scientists predicted the moonís presence and its orbital distance from Saturn after sighting in July, 2004 a set of peculiar spiky and wispy features in the Keeler gapís outer edge. The similarities of the Keeler gap features to those noted in Saturnís F ring and the Encke gap led the scientists to conclude that a small body, a few kilometers across, was lurking in the center of the Keeler gap, awaiting discovery.

Also included here is a view of the same scene created by combining six individual, unmagnified frames used in the movie sequence. This digital composite view improves the overall resolution of the scene compared to that available in any of the single images.

The images in this movie sequence were obtained with the narrow angle camera on May 1, 2005 from a distance of approximately 1.1 million kilometers (708,000 miles) from Saturn. Resolution in the original image was 8 kilometers (5 miles) per pixel. The images in the movie sequence have been magnified in (the vertical direction only) by a factor of two to aid visibility of features caused within the gap by the moonlet.

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: May 10, 2005 (PIA 06238, 06239)
Image/Caption Information



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