KentuckyFC writes: Iapetus, Saturn’s third largest moon, was first photographed by the Cassini spacecraft on 31 December 2004. The images created something of a stir. Clearly visible was a narrow, steep ridge of mountains that stretch almost halfway around the moon’s equator. The question that has since puzzled astronomers is how this mountain range got there. Now evidence is mounting that this mountain range is not the result of tectonic or volcanic activity, like mountain ranges on other planets. Instead, astronomers are increasingly convinced that this mountain range fell from space. The latest evidence is a study of the shape of the mountains using 3-D images generated from Cassini data. They show that the angle of the mountainsides is close to the angle of repose, that’s the greatest angle that a granular material can form before it landslides. That’s not proof but it certainly consistent with this exotic formation theory. So how might this have happened? Astronomers think that early in its life, Iapetus must have been hit by another moon, sending huge volumes of ejecta into orbit. Some of this condensed into a new moon that escaped into space. However, the rest formed an unstable ring that gradually spiralled in towards the moon, eventually depositing the material in a narrow ridge around the equator. Cassini’s next encounter with Iapetus will be in 2015 which should give astronomers another chance to study the strangest mountain range in the Solar System.