Date: July 31st 2008

July 30, 2008

Dwayne Brown NASA Headquarters, Washington
202-358-1726 dwayne c brown@nasa gov

Carolina Martinez Jet Propulsion Laboratory, Pasadena, Calif 818-354-9382 carolina martinez@jpl nasa gov

Lori Stiles University of Arizona, Tucson 520-360-0574 lstiles@u arizona edu
RELEASE: 08-193

NASA CONFIRMS LIQUID LAKE ON SATURN MOON

PASADENA, Calif -- NASA scientists have concluded that at least one of the large lakes observed on Saturn's moon Titan contains liquid hydrocarbons, and have positively identified the presence of ethane This makes Titan the only body in our solar system beyond Earth known to have liquid on its surface

Scientists made the discovery using data from an instrument aboard the Cassini spacecraft The instrument identified chemically different materials based on the way they absorb and reflect infrared light Before Cassini, scientists thought Titan would have global oceans of methane, ethane and other light hydrocarbons More than 40 close flybys of Titan by Cassini show no such global oceans exist, but hundreds of dark lake-like features are present Until now, it was not known whether these features were liquid or simply dark, solid material

"This is the first observation that really pins down that Titan has a surface lake filled with liquid," said Bob Brown of the University of Arizona, Tucson Brown is the team leader of Cassini's visual and mapping instrument The results will be published in the July 31 issue of the journal Nature

Ethane and several other simple hydrocarbons have been identified in Titan's atmosphere, which consists of 95 percent nitrogen, with methane making up the other 5 percent Ethane and other hydrocarbons are products from atmospheric chemistry caused by the breakdown of methane by sunlight

Some of the hydrocarbons react further and form fine aerosol particles All of these things in Titan's atmosphere make detecting and identifying materials on the surface difficult, because these particles form a ubiquitous hydrocarbon haze that hinders the view Liquid ethane was identified using a technique that removed the interference from the atmospheric hydrocarbons

The visual and mapping instrument observed a lake, Ontario Lacus, in Titan's south polar region during a close Cassini flyby in December 2007 The lake is roughly 7,800 square miles in area, slightly larger than North America's Lake Ontario

"Detection of liquid ethane confirms a long-held idea that lakes and seas filled with methane and ethane exist on Titan," said Larry Soderblom, a Cassini interdisciplinary scientist with the U S Geological Survey in Flagstaff, Ariz "The fact we could detect the ethane spectral signatures of the lake even when it was so dimly illuminated, and at a slanted viewing path through Titan's atmosphere, raises expectations for exciting future lake discoveries by our instrument "

The ethane is in a liquid solution with methane, other hydrocarbons and nitrogen At Titan's surface temperatures, approximately 300 degrees Fahrenheit below zero, these substances can exist as both liquid and gas Titan shows overwhelming evidence of evaporation, rain, and fluid-carved channels draining into what, in this case, is a liquid hydrocarbon lake

Earth has a hydrological cycle based on water and Titan has a cycle based on methane Scientists ruled out the presence of water ice, ammonia, ammonia hydrate and carbon dioxide in Ontario Lacus The observations also suggest the lake is evaporating It is ringed by a dark beach, where the black lake merges with the bright shoreline Cassini also observed a shelf and beach being exposed as the lake evaporates

"During the next few years, the vast array of lakes and seas on Titan's north pole mapped with Cassini's radar instrument will emerge from polar darkness into sunlight, giving the infrared instrument rich opportunities to watch for seasonal changes of Titan's lakes," Soderblom said

Launched in Oct 1997, Cassini's 12 instruments have returned a daily stream of data from Saturn's system The mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency

For information on Cassini, visit:

http://www nasa gov/cassini

-end-

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



The following information is a reminder of your current mailing list subscription:

You are subscribed to the following list: [list_name]

using the following email: example@example.com

You may automatically unsubscribe from this list at any time by visiting the following URL:

http://www aus-city com/cgi-bin/dada/plugins/dada_bridge pl/u/[list]/

If the above URL is inoperable, make sure that you have copied the entire address Some mail readers will wrap a long URL and thus break this automatic unsubscribe mechanism

You may also change your subscription by visiting this list's main screen:

<[program_url]/list/[list]>

If you're still having trouble, please contact the list owner at:

<mailto:[list_owner_email]>

The following physical address is associated with this mailing list:

[physical_address]

Forward to a Friend
 
  • This mailing list is a public mailing list - anyone may join or leave, at any time.
  • This mailing list is announce-only.

NASA Reports list

Privacy Policy:

Private list