Cassini Spots Potential Ice Volcano On Saturn Moon

[Date Prev] [Date Next] [Thread Prev] [Thread Next] [Date Index] [Thread Index]

 



Dec. 14, 2010

Dwayne C. Brown 
Headquarters, Washington      
202-358-1726 
dwayne.c.brown@xxxxxxxx 

Jia-Rui C. Cook 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-354-0850 
jccook@xxxxxxxxxxxx 

Paul Laustsen 
U.S. Geological Survey, Menlo Park, Calif. 
650-329-4046 
plaustsen@xxxxxxxx   


RELEASE: 10-335

CASSINI SPOTS POTENTIAL ICE VOLCANO ON SATURN MOON

WASHINGTON -- NASA's Cassini spacecraft has found possible ice 
volcanoes on Saturn's moon Titan that are similar in shape to those 
on Earth that spew molten rock. 

Topography and surface composition data have enabled scientists to 
make the best case yet in the outer solar system for an Earth-like 
volcano landform that erupts in ice. The results were presented today 
at the American Geophysical Union meeting in San Francisco. 

"When we look at our new 3-D map of Sotra Facula on Titan, we are 
struck by its resemblance to volcanoes like Mt. Etna in Italy, Laki 
in Iceland and even some small volcanic cones and flows near my 
hometown of Flagstaff," said Randolph Kirk, who led the 3-D mapping 
work, and is a Cassini radar team member and geophysicist at the U.S. 
Geological Survey (USGS) Astrogeology Science Center in Flagstaff, 
Ariz. 

Scientists have been debating for years whether ice volcanoes, also 
called cryovolcanoes, exist on ice-rich moons, and if they do, what 
their characteristics are. The working definition assumes some kind 
of subterranean geological activity warms the cold environment enough 
to melt part of the satellite's interior and sends slushy ice or 
other materials through an opening in the surface. Volcanoes on 
Jupiter's moon Io and Earth spew silicate lava. 

Some cryovolcanoes bear little resemblance to terrestrial volcanoes, 
such as the tiger stripes at Saturn's moon Enceladus, where long 
fissures spray jets of water and icy particles that leave little 
trace on the surface. At other sites, eruption of denser materials 
might build up volcanic peaks or finger-like flows. But when such 
flows were spotted on Titan in the past, theories explained them as 
non-volcanic processes, such as rivers depositing sediment. At Sotra, 
however, cryovolcanism is the best explanation for two peaks more 
than 3000 feet high with deep volcanic craters and finger-like flows. 


"This is the very best evidence, by far, for volcanic topography 
anywhere documented on an icy satellite," said Jeffrey Kargel, a 
planetary scientist at the University of Arizona, Tucson. "It's 
possible the mountains are tectonic in origin, but the interpretation 
of cryovolcano is a much simpler, more consistent explanation." 

Kirk and colleagues analyzed new Cassini radar images. His USGS group 
created the topographic map and 3-D flyover images of Sotra Facula. 
Data from Cassini's visual and infrared mapping spectrometer revealed 
the lobed flows had a composition different from the surrounding 
surface. Scientists have no evidence of current activity at Sotra, 
but they plan to monitor the area. 

"Cryovolcanoes help explain the geological forces sculpting some of 
these exotic places in our solar system," said Linda Spilker, Cassini 
project scientist at NASA's Jet Propulsion Laboratory in Pasadena, 
Calif. "At Titan, for instance, they explain how methane can be 
continually replenished in the atmosphere when the sun is constantly 
breaking that molecule down." 

Cassini launched Oct. 15, 1997, and began orbiting Saturn in 2004. 
Saturn has more than 60 known moons, with Titan being the largest. 
The Cassini-Huygens mission is a cooperative project of NASA, the 
European Space Agency and the Italian Space Agency (ASI). JPL manages 
the mission for NASA's Science Mission Directorate at the agency's 
Headquarters in Washington. 

The Cassini orbiter was designed, developed and assembled at JPL. The 
radar instrument was built by JPL and ASI, working with team members 
from the U.S. and several European countries. The visual and infrared 
mapping spectrometer was built by JPL, with a major contribution by 
ASI. The visual and infrared mapping spectrometer science team is 
based at the University of Arizona, Tucson. 

For more information about the Cassini mission, visit: 



http://www.nasa.gov/cassini   

	
-end-



To subscribe to the list, send a message to: 
hqnews-subscribe@xxxxxxxxxxxxxxxxxxxxxx
To remove your address from the list, send a message to:
hqnews-unsubscribe@xxxxxxxxxxxxxxxxxxxxxx

[Index of Archives]     [JPL News]     [Cassini News From Saturn]     [NASA Marshall Space Flight Center News]     [NASA Science News]     [James Web Space Telescope News]     [JPL Home]     [NASA KSC]     [NTSB]     [Deep Creek Hot Springs]     [Yosemite Discussion]     [NSF]     [Telescopes]

  Powered by Linux