NASA'S Cassini reveals lake-like feature on Titan

NASA'S Cassini reveals lake-like feature on Titan

Scientists are fascinated by a dark, lake-like feature recently observed on Saturn's moon Titan.

NASA's Cassini spacecraft captured a series of images, released today, showing a marking, darker than anything else around it. It is remarkably lake-like, with smooth, shore-like boundaries unlike any seen previously on Titan.

"I'd say this is definitely the best candidate we've seen so far for a liquid hydrocarbon lake on Titan," said Dr. Alfred McEwen, imaging team member and a professor at the University of Arizona, Tucson. The putative lake measures 230 kilometers by 70 kilometers (145 miles long by 45 miles) wide, about the size of Lake Ontario, on the U.S. Canadian border.

The feature lies in Titan's cloudiest region, which is presumably the most likely site of recent methane rainfall. This, coupled with the shore-like smoothness of the feature's perimeter makes it hard for imaging scientists to resist some speculation about what might be filling the lake, if it indeed is one.

Cassini imaging team member Dr. Tony DelGenio of NASA's Goddard Institute for Space Studies in New York, said, "It's possible that some of the storms in this region are strong enough to make methane rain that reaches the surface. Given Titan's cold temperatures, it might take a long time for any liquid methane collecting on the surface to evaporate. So it might not be surprising for a methane-filled lake to persist for a long time."

A computer-enhanced image of the feature and a three-frame movie showing the evolution of nearby clouds can be seen at: ciclops.org, or saturn.jpl.nasa.gov and nasa.gov/cassini.

Despite earlier predictions, no definitive evidence for open bodies of liquid has yet been found on Titan. Cassini has not yet been in a favorable position for using the camera to check for glints from possible surface liquids in the south polar region.

"This feature is unique in our xploration of Titan so far," said Dr. Elizabeth Turtle, Cassini imaging team associate at the University of Arizona. "Its perimeter is intriguingly reminiscent of the shorelines of lakes on Earth, which are smoothed by water erosion and deposition."

An alternate explanation is that this feature was once a lake, but has since dried up, leaving behind dark deposits, Turtle said. Yet another possibility is that the lake is simply a broad depression filled by dark, solid hydrocarbons falling from the atmosphere onto Titan's surface. In this case, the smooth outline might be the result of a process unrelated to rainfall, such as a sinkhole or a volcanic caldera.

Dr. Torrence Johnson, an imaging team member at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif., said, "It reminds me of the lava lakes seen on Jupiter's moon, Io."

"Eventually, as the seasons change over a few years, the convective clouds may migrate northward to lower latitudes," said DelGenio, "If so, it will be interesting to see whether the Cassini cameras record changes in the appearance of the surface as well."

"It is already clear that whatever this lake-like feature turns out to be, it is only one of many puzzles that Titan will throw at us as we continue our reconnaissance of the surface over the next few years," said Dr. Carolyn Porco, imaging team leader at the Space Science Institute in Boulder, Colo.

Thirty-nine more Titan flybys are planned for Cassini's prime mission. In future flybys the science teams will search for opportunities to observe the lake feature again and to look for mirror-like reflections from smooth surfaces elsewhere on Titan. Such reflections would strongly support the presence of liquids.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL, a division of the California Institute of Technology in Pasadena, manages the Cassini mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute in Boulder, Colo.

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Public release date: 28-Jun-2005

Preston Dyches, 720-974-5859, Cassini Imaging Central Laboratory for Operations, Space Science Institute, Boulder, Colo.,

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

Erica Hupp or Dolores Beasley, 202-358-1237/1753, NASA Headquarters, Washington

more at Cassini spacecraft or Titan and Huygens

Statement from NASA Administrator Michael Griffin

Statement from NASA Administrator

The following is a statement from NASA Administrator Michael Griffin on today's final public meeting of the Stafford-Covey Task Group.

"The independent Return to Flight Task Group, led by veteran astronauts Thomas Stafford and Richard Covey, has performed a valuable public service. Given the level of complexity of the issues involved, I would certainly expect to hear, and I welcome different points of view. As an engineer, I know that a vigorous discussion of these complex issues can make us smarter. I anticipate, and expect, a healthy debate in our upcoming Flight Readiness Review for the Space Shuttle Return to Flight mission, STS-114. We appreciate this input."

Managers from the Space Shuttle program will speak to reporters following this week's Flight Readiness Review at the NASA Kennedy Space Center in Florida.

For more information about the Stafford-Covey Task Group and the flight of STS-114, visit the Internet at: www.returntoflight.org and nasa.gov/returntoflight - end -

Dean Acosta/Bob Jacobs Headquarters, Washington, (Phone: 202/358-1400/1600), June 27, 2005, RELEASE: 05-165 more at NASA and Michael Griffin