CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Closing in on Phoebe
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Closing in on Phoebe
PIA 06062

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  The Cassini spacecraft is closing in fast on its first target of observation in the Saturn system: the small, mysterious moon Phoebe, only 214 kilometers (133 miles) across.

The three images shown here, the latest of which is twice as good as any image returned by the Voyager 2 spacecraft in 1981, were captured in the past week on approach to this outer moon of Saturn. Phoebe's surface is already showing a great deal of contrast, most likely indicative of topography, such as tall sunlit peaks and deep shadowy craters, as well as genuine variation in the reflectivity of its surface materials. Left to right, the three views were captured at a Sun-Saturn-spacecraft, or phase, angle of 87 degrees between June 4 and June 7, from distances ranging from 4.1 million km (2.6 million miles) to 2.5 million km (1.5 million miles). The image scale ranges from 25 to 15 km (16 to 9 miles) per pixel.

The images have been magnified eight times using a linear interpolation scheme; the contrast has been untouched. Phoebe rotates once every 9 hours and 16 minutes; each of these images shows a different region on Phoebe.

Cassini's powerful cameras will provide the best-ever look at this moon on Friday, June 11, when the spacecraft will streak past Phoebe at a distance of only about 2,000 kilometers (1,240 miles) from the moon's surface. The current images, and the presence of large craters, promise a heavily cratered surface which will come into sharp view over the next few days when image scales should shrink to a few 10's of meters...the size of office buildings.

Because of its small size and retrograde orbit - Phoebe orbits Saturn in a direction opposite to that of the larger inner Saturnian moons - and because of the presence of water ice on its surface, Phoebe is believed to be a body from the distant outer solar system, one of the building blocks of the outer planets that was captured into orbit around Saturn. If true, the little moon will provide a windfall of precious information about a primitive piece of the solar system that has never before been explored up close.

Phoebe was the first moon discovered using photography in 1898 and has a very dark surface. It has long been believed that material coming from Phoebe's surface and impacting the very dark leading hemisphere of Iapetus may play some role in the latter's extreme albedo asymmetry, though the precise relationship is unclear. Cassini should help solve this and other mysteries during its exciting encounter with Phoebe.

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 Office of Space Science, 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: June 9, 2004 (PIA 06062)
Image/Caption Information

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