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As time passed, the region would have cooled down considerably and contracted--thus pulling away from its surroundings and forming fractures akin to the cracks that form in mud as it becomes dry--but on a considerably larger scale.



The nitrogen that exists in Titan's atmosphere indicates that it likely formed early in our Solar System's 4.56 billion-year-old history. This means that Titan probably was born within the same cold disk of gas and dust that gave birth to our Sun (protostellar nebula), instead of forming in the warmer disk that eventually created Saturn.



"We believe that the Huygens Probe, which landed on Titan in January 2005, raised a small amount of organic dust upon arrival due to its powerful aerodynamic wake. But what we spotted here with Cassini is at a much larger scale. The near surface wind speeds required to raise such an amount of dust as we see in these dust storms would have to be very strong--about five times as strong as the average wind speeds estimated by the Huygens measurements near the surface and with climate models," Dr. Rodriguez added.