CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Color Maps of Tethys - November 2014
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Color Maps of Tethys - November 2014
PIA 18439

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Color Maps of Tethys - November 2014
PIA 18439

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Color Maps of Tethys - November 2014
PIA 18439

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Color Maps of Tethys - November 2014
PIA 18439

Full Size Polar 9692x6624:
JPEG 13.1 MB
PNG 48.3 MB
TIFF 95.6 MB

Quarter Size Polar 2423x1656:
PNG 4.3 MB
  This set of global, color mosaics of Saturn's moon Tethys was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system. These are the first global color maps of these moons produced from the Cassini data.

The most obvious feature on the maps is the difference in color and brightness between the two hemispheres. The darker colors on the trailing hemispheres are thought to be due to alteration by magnetospheric particles and radiation striking those surfaces. The lighter-colored leading hemisphere is coated with icy dust from Saturn’s E-ring, formed from tiny particles ejected from Enceladus’ south pole. These satellites are all being painted by material erupted by neighboring Enceladus.

Another dramatic feature is the moon's equatorial band. First observed on Tethys by Voyager, Cassini’s color mapping also revealed a similar type of feature on Mimas. Cassini showed these areas on both moons to be significantly brighter in the ultraviolet than surrounding terrains. This pattern, localized on the leading hemispheres, was discovered to correlate with the predicted pattern of bombardment of high-energy electrons trapped in Saturn’s magnetic field. This bombardment alters the surface ices on a crystalline scale and changes their color. Later, thermal observations by Cassini's Composite Infrared Spectrometer (CIRS) instrument showed that these features also form thermal anomalies on the surface, giving rise to the nickname "Pac-Man" features (See PIA16198).

The colors shown in these global mosaics are enhanced, or broader, relative to human vision, extending into the ultraviolet and infrared range.

Resolution on Tethys in the maps is 250 meters per pixel.

Image selection, radiometric calibration, geographic registration and photometric correction, as well as mosaic selection and assembly were performed by Paul Schenk at the Lunar and Planetary Institute. Original image planning and targeting for Saturn’s icy moons were performed by Tilman Denk (Frei Universitat, Berlin) and Paul Helfenstein (Cornell University, Ithaca, New York).

The Cassini Solstice 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 Solstice Mission visit, and

Credit: NASA/JPL-Caltech/SSI/Lunar and Planetary Institute
Released: November 4, 2014 (PIA 18439)
Image/Caption Information

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