
Iapetus is the third-largest moon of Saturn, first observed by Giovanni Domenico Cassini in October 1671 on the western side of Saturn. It is named after the Titan Iapetus from the Greek mythology. Iapetus is best known for its dramatic 'two-tone' colouration. Cassini correctly surmised that Iapetus has a bright a dark hemisphere; and furthermore that it is tidally locked, always keeping the same face towards Saturn, so that the bright hemisphere is visible from Earth when Iapetus is on the western side of the planet, and the dark hemisphere on the other side. NASA's Voyager 2 flew past Iapetus on 2 August 1981. Passing at a relatively distant 966,000 km, the spacecraft's cameras could make out few details in the area of dark material. The images revealed the bright side to be icy and heavily cratered. Recent discoveries by the Cassini mission have revealed several other unusual physical characteristics, such as an equatorial ridge that runs about halfway around the moon.
Cassini is on the trail of a runaway mysteryNASA scientists are on the trail of Iapetus' mysterious dark side, which seems to be home to a bizarre 'runaway' process that is transporting vaporised water ice from the dark areas... — full story
Iapetus is the yin-yang of the solar systemCassini scientists are poring through hundreds of images returned from the 10 September fly-by of Saturn's two-toned moon Iapetus. The pictures show the moon's yin and yang - a white... — full story
Cassini gets close-up views of IapetusCassini completed its closest flyby of the odd moon Iapetus on 10 September 2007. The spacecraft flew about 1,640 kilometres (1,000 miles) from Iapetus' surface and is returning amazing... — full story
Iapetus cryogenically frozen in its teenage yearsSaturn's distinctive moon Iapetus is cryogenically frozen in the equivalent of its teenage years. The moon has retained the youthful figure and bulging waistline it sported more than... — full story