Cassini Finds Lakes on Titan's Arctic Region

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July 28, 2006

Dwayne Brown/Erica Hupp 
Headquarters, Washington 
202-358-1726/1237

Carolina Martinez
Jet Propulsion Laboratory, Pasadena, Calif. 
818-354-9382 

RELEASE: 06-274

CASSINI FINDS LAKES ON TITAN'S ARCTIC REGION

NASA's Cassini spacecraft has found lakes on Saturn's moon Titan. 

The lakes are most likely the source of hydrocarbon smog in the frigid 
moon's atmosphere. Finding the source of the complex soup of 
hydrocarbons in Titan's atmosphere has been a major goal for the 
Cassini mission and is a significant accomplishment. 

Numerous well-defined dark patches resembling lakes are present in 
radar images of Titan's high latitudes taken during a July 22 flyby. 
At Titan's frigid temperatures, about minus 180 degrees Celsius, the 
liquids in the lakes are most likely methane or a combination of 
methane and ethane. 

"This is a big deal," said Steve Wall, deputy radar team leader at 
NASA's Jet Propulsion Laboratory, Pasadena, Calif. "We've now seen a 
place other than Earth where lakes are present." 

This area of Titan has been in winter's shadow since before Cassini 
arrived, and the spacecraft had not flown over it before. During the 
flyby, Cassini's radar spotted several dozen lakes as small as 0.6 
miles wide, with some nearly 20 miles wide. The biggest lake is about 
62 miles long and may be only partly wet. 

"What we see is darker than anything we've ever seen elsewhere on 
Titan. It was almost as though someone laid a bull's-eye around the 
whole north pole of Titan, and Cassini sees these regions of lakes 
just like those we see on Earth," said Larry Soderblom, Cassini 
interdisciplinary scientist at the U.S. Geological Survey, Flagstaff, 
Ariz. "Titan has turned out to be like a musical crescendo -- each 
pass is more exciting than the last." 

Titan has not yielded its secrets easily because the dense smoggy 
atmosphere makes it very difficult to obtain good visible images. 
Radar can penetrate the smog and obtain clear images. 

Dark regions in radar images generally mean smoother terrain, while 
bright regions mean a rougher surface. Some of the new radar images 
show channels leading in or out of a variety of dark patches. The 
shape of the channels also strongly implies they were carved by 
liquid. 

Some of the dark patches and connecting channels are completely black 
-- they reflect back essentially no radar signal, which means they 
must be extremely smooth and might contain liquid. In some cases rims 
can be seen around the dark patches, suggesting deposits that might 
form as liquid evaporates. 

Scientists had predicted, but had no confirmation until now, that 
pools of liquid were contributing to the high concentration of 
methane and other hydrocarbons in Titan's atmosphere. 

"We've always believed Titan's methane had to be maintained by liquid 
lakes or extensive underground 'methanofers,' the methane equivalent 
of aquifers. We can't see methanofers but we can now say we've seen 
lakes," said Jonathan Lunine, Cassini interdisciplinary scientist at 
the University of Arizona, Tucson. 

Since lakes come and go with the seasons, they wax and wane over time, 
and winds might alter the roughness of their surfaces. Repeat 
coverage of these areas is expected to provide more information on 
these lakes. By passing over a lake in a different direction, Cassini 
may see the effect of prevailing winds in the changing brightness of 
the lake surface. On later passes toward the end of its prime 
mission, Cassini might see changes in the shape or size of lakes as 
winter yields to spring in the northern hemisphere. 

Cassini's next flyby is on September 7. In October, Cassini's radar 
will look even closer to the north pole, searching for more lakes and 
mapping more of the polar region covered by these features. 

The Cassini-Huygens mission is a cooperative project between NASA, the 
European Space Agency and the Italian Space Agency. The Jet 
Propulsion Laboratory manages the Cassini-Huygens mission for NASA's 
Science Mission Directorate, Washington. 

For images on the lakes and more information, visit: 

http://www.nasa.gov/cassini

	
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