Matches in DBpedia 2014 for { ?s ?p Iapetus (/aɪˈæpɨtəs/; Greek: Ιαπετός), or occasionally Japetus /ˈdʒæpɨtəs/, is the third-largest natural satellite of Saturn, eleventh-largest in the Solar System, and the largest body in the Solar System known to not be in hydrostatic equilibrium. Iapetus is best known for its dramatic 'two-tone' coloration, but discoveries by the Cassini mission in 2007 have revealed several other unusual features, such as a massive equatorial ridge that runs three quarters of the way around Iapetus.. }
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- Iapetus_(moon) abstract "Iapetus (/aɪˈæpɨtəs/; Greek: Ιαπετός), or occasionally Japetus /ˈdʒæpɨtəs/, is the third-largest natural satellite of Saturn, eleventh-largest in the Solar System, and the largest body in the Solar System known to not be in hydrostatic equilibrium. Iapetus is best known for its dramatic 'two-tone' coloration, but discoveries by the Cassini mission in 2007 have revealed several other unusual features, such as a massive equatorial ridge that runs three quarters of the way around Iapetus.".
- Iapetus_(moon) comment "Iapetus (/aɪˈæpɨtəs/; Greek: Ιαπετός), or occasionally Japetus /ˈdʒæpɨtəs/, is the third-largest natural satellite of Saturn, eleventh-largest in the Solar System, and the largest body in the Solar System known to not be in hydrostatic equilibrium. Iapetus is best known for its dramatic 'two-tone' coloration, but discoveries by the Cassini mission in 2007 have revealed several other unusual features, such as a massive equatorial ridge that runs three quarters of the way around Iapetus.".