CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Shear Zone
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Shear Zone
PIA 08140

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  This atmosphere close-up shows bright clouds in Saturn's northern hemisphere being sheared apart. The clouds at the bottom of the image are tilted and stretched because the wind at those lower latitudes is moving much faster to the east than the wind at the higher latitudes near the top of the image, hence the shear.

This appearance suggests that these bright eddies are passive tracers of the atmosphere's motion - they appear, probably as a result of convection from below, and then they are sheared apart.

The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Feb. 16, 2006, at a distance of approximately 3.3 million kilometers (2 million miles) from Saturn. The image scale is 19 kilometers (12 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 and the Cassini imaging team home page,

Credit: NASA/JPL/Space Science InstituteNASA/JPL/Space Science Institute
Released: March 23, 2006 (PIA 08140)
Image/Caption Information

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