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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: March 9, 2006Pockets of liquid water may exist near the surface of Saturn's icy moon Enceladus, the apparent source of huge Yellowstone-type geysers seen erupting from the moon's south polar region by NASA's Cassini spacecraft, scientists reported today. If so, Enceladus would join a very short list of bodies in the solar system with environments that could, in theory at least, support life. Credit: NASA/JPL/Space Science InstituteDownload larger image version "What we have found on Enceladus - simple organics, excess heat and evidence for liquid water - represents the Holy Grail of modern day planetary exploration, and we've just stumbled upon it," said Cassini imaging team leader Carolyn Porco. "How cool is that?"It is not yet clear what process might be generating the energy needed to thaw ice in the ultra cold realm, but it may be a combination of natural radioactive heating and tidal flexing caused by Saturn's gravity, coupled with an era of heating in the past.While the heat source is not yet clear, the results are. High resolution images and data from other instruments aboard Cassini show towering plumes erupting from long fractures dubbed "tiger stripes" in the fractured terrain near the south pole. Based on the volume and size of the ice particles spewing out, scientists believe they may originate from near-surface reservoirs of water that have been warmed above the freezing point."This finding has substantially broadened the range of environments in the solar system that might support life," Porco said in an email. "And it doesn't get any more significant than that. I'd say that if we did nothing else at Saturn, this discovery alone and its possible biological implications would have made the Cassini mission worthwhile."Additional coverage for subscribers:VIDEO:CASSINI IMAGERY OF ENCELADUS VIDEO:INTERVIEW WITH CASSINI SCIENTIST The Cassini imaging team, led by Porco of the Space Science Institute in Boulder, Colo., reported the findings in the current issue of Science magazine.Carrying a suite of sophisticated instruments, Cassini braked into orbit around Saturn in July 2004 after a seven-year voyage from Earth. Since then, it's been looping around the planet in a series of ever-changing orbits, studying its spectacular ring system, its atmosphere, the space environment near Saturn and many of the planet's more interesting moons. Much of the early attention has been focused on Titan, a moon larger than Mercury that is shrouded in a thick atmosphere.The much smaller Enceladus, just 300 miles or so across but one of the brightest moons in the solar system, has long been a target of interest because of earlier observations that hinted at an unusual surface. Cassini's observations have raised that interest to a new level. Plumes of icy material extend above the southern polar region of Saturn's moon Enceladus as imaged by the Cassini spacecraft in February 2005. The monochrome view is presented along with a color-coded version on the right. The latter reveals a fainter and much more extended plume component. Credit: NASA/JPL/Space Science InstituteDownload larger image version "Images taken as early as 16 January 2005, images acquired during the February and July 2005 flybys, and those taken in late November 2005 have yielded striking visual evidence of many narrow jets of fine icy particles emanating from the south polar terrain," the imaging team wrote in Science."They also have yielded indications of extreme geologic youth in the SPT, morphological evidence of a change over time in surface stresses in the southern hemisphere, and possible evidence of an epoch of intense heating in the past."During the November 2005 flyby, Cassini images revealed "many distinct near-surface jets, emanating from the surface in a variety of directions and supplying a much bigger, fainter plume towering over the south polar region by at least 435 km (270 miles)," the team wrote.The source of the jets appears to be the so-called tiger stripes, a family of long, roughly parallel f
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