For more information, please contact:
Public Services Office
Mail Stop 186-113
Jet Propulsion Laboratory
4800 Oak Grove Drive
Pasadena, CA 91109
Phone: (818) 354-0112
Fax: (818) 393-4641
Click here for directions. |
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This month’s lecture: |
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Saturn's Moon Enceladus: A Small, Cold Moon with a Warm Spot
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Summary : |
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Active volcanism has been known to exist on just three solar system bodies — Earth, Jupiter’s moon Io, and possibly Neptune’s moon Triton. Now Cassini scientists have proposed another member of this exclusive club. The Cassini spacecraft may have found evidence of liquid water reservoirs that erupt in Yellowstone-like geyers on Saturn’s moon Enceladus. High-resolution images of the warm south polar region show icy jets and towering plumes ejecting large quantities of particles at high speed. Why is Enceladus so active? And why is the south pole so hot? The answer might be the effects of tidal forces that squeeze and stretch the moon as it orbits Saturn. Warm, low-density material rising to the surface could have literally caused Enceladus to roll over, putting the mass of warm material at the south pole. |
Speaker : |
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Tom Spilker JPL, Scientist, Mission Architect |
Location: |
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Thursday, August 16, 2007, 7p.m.
The von Kármán Auditorium at JPL
4800 Oak Grove Drive
Pasadena, CA
+Directions
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Friday, August 17, 2007, 7p.m.
The Vosloh Forum at Pasadena City College
1570 East Colorado Blvd.
Pasadena, CA
+Directions |
Webcast: |
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"Saturn's Moon Enceladus: A Small, Cold Moon with a Warm Spot" Archived Webcasts:
RealPlayer (with captions): "Saturn's Moon Enceladus" Webcast
RealPlayer (w/out captions): "Saturn's Moon Enceladus" Webcast
If you don't have RealPlayer, you can download the free RealPlayer 8 Basic.
Click here to return to the 2007 von Kármán Lecture Schedule.
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