Volume: 02, Issue: 19 11/17/2004 
Radar image of Titan. Comparisons with other features and data from other instruments will help to determine whether this is a cryovolcanic flow, where water-rich liquid has welled up from Titan's warm interior. Image courtesy NASA/JPL.
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Other Articles in This Issue:
Spitzer Spies Starless Cores and Icy Planetary Origins
Scientists Map Human Genome Activity
Reduce, Reuse, Recycle… Water
Chat Live With NASA Flight Systems Engineer
 

Cassini Glimpses Possible Ice Volcano on Titan

The Cassini spacecraft has found a strikingly bright feature on Saturn’s moon Titan that could be a sign of volcanic flow. The evidence was seen in one of Cassini's first radar images of Titan. There are many possible explanations for what this feature is, but one of the leading candidates is that it may be a cryovolcanic flow, or “ice volcano.”

"It's too early to say, but it looks very much like it's something that oozed across the surface,” said Dr. Ralph Lorenz of the University of Arizona, Tucson. “It may be some sort of cryovolcanic flow, an analog to volcanism on Earth that is not molten rock but, at Titan's very cold temperatures, molten ice."

Cassini's radar mapped about one percent of Titan's surface during the spacecraft's first close Titan flyby on Oct. 26, 2004. The radar survey covered a strip 120 kilometers (75 miles) wide and 1,960 kilometers (1,200 miles) long in Titan's northern hemisphere.

Cassini was flying about 2,494 (1,550 miles) above Titan's surface, when it mapped the 230-square-kilometer (90-square-mile) area shown in the new radar image. The Cassini radar team presented the image at the 36th annual meeting of the American Astronomical Society's Division for Planetary Sciences in Louisville, Ky.

The radar instrument on board Cassini works by bouncing radio signals off Titan's surface and timing their return. The more signal reflected back to the spacecraft, the brighter the imaged area. Turning radio signals into radar images is time consuming because so many numerical calculations must be made.

"There's no such thing as a 'raw' radar image," Lorenz said.

Just two days after the Oct. 26 flyby, Cassini scientists knew that Titan is not a crater-pocked dead world, but a much more interesting place. Titan's surface is young. It might have been altered by ongoing dynamic geologic processes that cover and obscure old impact craters. Lorenz, along with Cassini interdisciplinary scientist Dr. Jonathan Lunine (also of the University of Arizona) and other Cassini scientists, agree in this interpretation.

Given this newest image, Lunine said, "Cassini's radar has provided the first evidence for possible young cryovolcanism on Titan's surface. Now our challenge is to find out what is flowing, how it works, and the implications for Titan's evolution."

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory (JPL), 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 Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The radar instrument team is based at JPL working with team members from the United States and several European countries.

More information on the Cassini-Huygens mission is available at the following websites:
http://saturn.jpl.nasa.gov
http://www.nasa.gov/cassini
http://www.esa.int

    
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