Search for life signal on Titan <br /><br />Titan: An atmosphere not unlike Earth's billions of years ago<br /><br /><br />Scientists will comb data sent back from Titan by the Huygens probe for the chemical signature of life in a bid to identify the moon's source of methane. <br />Methane is constantly destroyed by UV light so there must be a source within Titan to replenish the atmosphere. <br /><br />Life is a possible - though some think unlikely - source of this hydrocarbon along with geological processes. <br /><br />The surface is too cold for biology, but microbes could survive in an ocean within Titan, a senior scientist says. <br /><br />Methane can also be released from a trapped form called clathrate and produced by a geological process called "serpentinisation". Neither of these involve biology. <br /><br />Dominated by nitrogen, methane and other organic (carbon-based) molecules, Titan is thought to resemble a deep-frozen version of Earth 4.6 billion years ago. <br /><br />Liquid methane rains down on Titan into river channels carved between hills of water ice. Reservoirs of this hydrocarbon probably lie on or just below the surface. <br /><br />But UV light would destroy all the methane on Titan within 10 million years if it were not being constantly renewed. <br /><br /> We have liquid water, organics not so far away; we have everything on Titan to make life <br /><br />Francois Raulin, University of Paris <br /><br />"We cannot say there is absolutely no chance for life," Dr Francois Raulin, one of three interdisciplinary scientists on the Huygens mission told the BBC News website. <br /><br />"There is no chance for life on the surface because it is too cold and there is no liquid water. <br /><br />"However, models of Titan's interior show there should be an ocean about 100km deep at around 300km below the surface." <br /><br />If the models are correct, this ocean would be composed mostly of liquid water with about 15% ammonia at a temperature of about -80C, said Dr Raulin