The Cassini Mission to Saturn



During Cassini's first flyby of Enceladus, a tenuous atmosphere was detected in magnetic field data, which may imply internal activity. This atmosphere may help explain the source of Saturn's outermost E ring.
The icy surface of Enceladus appears to have similarities to both Europa and Ganymede -- two prominent icy satellites of Jupiter. Both Europa and Ganymede are thought to have subsurface water layers or "oceans," so the similarities with Enceladus are intriguing.

Next up for Cassini: Titan Flyby: 1400 km (800 miles): October 28, 2005

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Image Credit: ESA/NASA/Univ. of Arizona
Full res picture of Titan S/2005 S1 image Saturn moon EnceladusSaturn's icy moon Dione


After arriving at Saturn Cassini launched the Huygens probe to the Saturn moon Titan, seen here in an artist's conception. There is a theory that liquid water may exist under Titans frozen surface.


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A short clip of Cassini and the probe Huygens
A clip of the Cassini Probe at Saturn's moon Titan MPG 4.34M
Hi res mpg of S/2005 S1
S/2005 S1 MPG CLIP Mpg 1.27M

Nasa.org.  Cassini MissionThe Nasa page on the Cassini Mission to Saturn. Opens in a new window.




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