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Tethys Atlas Index
PDF 527 KB
JPEG 482 KB
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Ste-1 North Polar Area
PDF 29.6 MB
JPEG 774 KB
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JPEG 187 KB
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Ste-2 Anticleia
PDF 31.3 MB
JPEG 1.1 MB
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Ste-3 Odysseus
PDF 31.5 MB
JPEG 1.0 MB
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JPEG 557 KB
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Ste-4 Alcinous
PDF 31.3 MB
JPEG 970 KB
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JPEG 512 KB
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Ste-5 Telemachus
PDF 31.5 MB
JPEG 1.1 MB
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Ste-6 Circe
PDF 30.2 MB
JPEG 1.1 MB
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JPEG 675 KB
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Ste-7 Polycaste
PDF 30.1 MB
JPEG 1.0 MB
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JPEG 611 KB
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Ste-8 Theoclymenus
PDF 30.1 MB
JPEG 965 KB
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JPEG 518 KB
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Ste-9 Penelope
PDF 30.1 MB
JPEG 963 KB
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JPEG 520 KB
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Ste-10 Salmoneus
PDF 30.2 MB
JPEG 1000 KB
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JPEG 558 KB
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Ste-11 Ithaca Chasma
PDF 31.5 MB
JPEG 1.0 MB
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Ste-12 Hermione
PDF 31.3 MB
JPEG 1.0 MB
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JPEG 569 KB
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Ste-13 Melanthius
PDF 31.3 MB
JPEG 999 KB
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JPEG 534 KB
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Ste-14 Antinous
PDF 31.3 MB
JPEG 1.1 MB
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Ste-15 Naubolos, South Polar Area
PDF 29.7 MB
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Presented here is a complete set of cartographic map sheets from a high-resolution Tethys atlas, a project of the Cassini Imaging Team.
The map sheets form a 15-quadrangle series covering the entire surface of Tethys at a nominal scale of 1:1,000,000. An index for the atlas is included here, along with an unlabeled version of each terrain section.
The map data was acquired by the Cassini imaging experiment. The mean radius of Tethys used for projection of the maps is 536.3 kilometers (333.2 miles).
Names for features have been approved by the International Astronomical Union (IAU).
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 http://ciclops.org, http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.
Credit: NASA/JPL/Space Science Institute/DLR
Released: August 6, 2008 (PIA 11008)
Image/Caption Information |
