CICLOPS: Cassini Imaging Central Laboratory for OPerationS
Towering Peaks of Iapetus

Towering Peaks of Iapetus
PIA 08379

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Full Size Anaglyph 4082x1546:
PNG 4.1 MB
TIFF 15.2 MB

Half Size Anaglyph 2041x773:
PNG 1.5 MB


Towering Peaks of Iapetus
PIA 08379

Avg Rating: 10/10

Full Size Non-stereo 4763x1803:
PNG 2.3 MB

Half Size Non-stereo 2382x902:
GIF 684 KB
  This stereo image, or anaglyph, shows huge mountains on Iapetus, imaged by the Cassini spacecraft during its very close flyby in Sept. 2007. These mountains are located at the moon's equator in the westward-most part of the dark terrain.

Here, the brightness pattern on the surface is very complex. The mountain in the center of this view is part of the range informally named "the Voyager mountains" that were first detected on the limb of the moon in Voyager images. Interestingly, its eastern (right) flank is dark, while the other flanks are bright. This suggests that external material arriving on Iapetus from its orbital motion might play a role in the darkening process. One plausible source, the outer moons of Saturn, might provide a very thin but steady stream of very dark particles from the eastern direction as seen from this mountain.

The mosaic consists of six image footprints across the surface of Iapetus. The view is centered on terrain near 0.1 degree north latitude, 199 degrees west longitude. Image scale is approximately 46 meters (151 feet) per pixel.

The clear spectral filter images in this mosaic were obtained with the Cassini spacecraft narrow angle camera on Sept. 10, 2007. Distances for the blue portion of the image range from 7,744 to 9,135 kilometers (4,812 to 5,676 miles) from Iapetus; distances for the red portion of the image range from 20,267 to 21,595 kilometers (12,593 to 13,418 miles) from the moon.

A separate, non-stereo version of the scene is included for comparison.

Iapetus is 1,471 kilometers (914 miles) across.

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: October 8, 2007 (PIA 08379)
Image/Caption Information