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- j.icarus.2012.03.025 bibcode "2012Icar..219..737M".
- j.icarus.2012.03.025 doi "10.1016/j.icarus.2012.03.025".
- j.icarus.2012.03.025 first1 "A.".
- j.icarus.2012.03.025 first2 "K.".
- j.icarus.2012.03.025 first3 "K.".
- j.icarus.2012.03.025 first4 "A.".
- j.icarus.2012.03.025 first5 "R.".
- j.icarus.2012.03.025 isCitedBy Satellite_system_(astronomy).
- j.icarus.2012.03.025 issn "00191035".
- j.icarus.2012.03.025 issue "2".
- j.icarus.2012.03.025 journal "Icarus".
- j.icarus.2012.03.025 last1 "Morbidelli".
- j.icarus.2012.03.025 last2 "Tsiganis".
- j.icarus.2012.03.025 last3 "Batygin".
- j.icarus.2012.03.025 last4 "Crida".
- j.icarus.2012.03.025 last5 "Gomes".
- j.icarus.2012.03.025 pages "737–740".
- j.icarus.2012.03.025 title "Explaining why the uranian satellites have equatorial prograde orbits despite the large planetary obliquity".
- j.icarus.2012.03.025 volume "219".
- j.icarus.2012.03.025 year "2012".