CICLOPS: Cassini Imaging Central Laboratory for OPerationS
Tethys Mysteries

Tethys Mysteries
PIA 07536

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  The sea goddess Tethys (1,062 kilometers, 660 miles across) shows off two of her more puzzling features in this Cassini image. Ithaca Chasma, near lower right, stretches for more than 1,000 kilometers (620 miles) across the moon's surface. The origin of this canyon system, which is 100 kilometers (60 miles) across on average, is not completely understood, but has been theorized to have resulted from the impact that created the giant crater Odysseus.

Also notable in this view is the dark band that girdles the moon's equator. The nature of this feature may be better understood following Cassini's planned close flyby in September, 2005.

The lit surface visible here is on the moon's Saturn-facing hemisphere; north on Tethys is straight up.

The image was taken in visible light with the narrow angle camera on May 22, 2005, from a distance of approximately 884,000 kilometers (550,000 miles) from Tethys and at a Sun-Tethys-spacecraft, or phase, angle of 97 degrees. Resolution in the original image was 5 kilometers (3 miles) per pixel. The image has been contrast-enhanced and magnified by a factor of two 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 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 Institute
Released: July 6, 2005 (PIA 07536)
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