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Article: A primordial origin of the laplace relation among the Galilean satellites

TitleA primordial origin of the laplace relation among the Galilean satellites
Authors
Issue Date2002
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2002, v. 298 n. 5593, p. 593-597 How to Cite?
AbstractUnderstanding the origin of the orbital resonances of the Galilean satellites of Jupiter will constrain the longevity of the extensive voicanism on lo, may explain a liquid ocean on Europa, and may guide studies of the dissipative properties of stars and Jupiter-like planets. The differential migration of the newly formed Galilean satellites due to interactions with a circumjovian disk can lead to the primordial formation of the Laplace relation n1-3n2 + 2n3 = 0, where the ni are the mean orbital angular velocities of lo, Europa, and Ganymede, respectively. This contrasts with the formation of the resonances by differential expansion of the orbits from tidal torques from Jupiter.
Persistent Identifierhttp://hdl.handle.net/10722/151089
ISSN
2015 Impact Factor: 34.661
2015 SCImago Journal Rankings: 13.217
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorPeale, SJen_US
dc.contributor.authorLee, MHen_US
dc.date.accessioned2012-06-26T06:16:57Z-
dc.date.available2012-06-26T06:16:57Z-
dc.date.issued2002en_US
dc.identifier.citationScience, 2002, v. 298 n. 5593, p. 593-597en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/151089-
dc.description.abstractUnderstanding the origin of the orbital resonances of the Galilean satellites of Jupiter will constrain the longevity of the extensive voicanism on lo, may explain a liquid ocean on Europa, and may guide studies of the dissipative properties of stars and Jupiter-like planets. The differential migration of the newly formed Galilean satellites due to interactions with a circumjovian disk can lead to the primordial formation of the Laplace relation n1-3n2 + 2n3 = 0, where the ni are the mean orbital angular velocities of lo, Europa, and Ganymede, respectively. This contrasts with the formation of the resonances by differential expansion of the orbits from tidal torques from Jupiter.en_US
dc.languageengen_US
dc.publisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.orgen_US
dc.relation.ispartofScienceen_US
dc.titleA primordial origin of the laplace relation among the Galilean satellitesen_US
dc.typeArticleen_US
dc.identifier.emailLee, MH:mhlee@hku.hken_US
dc.identifier.authorityLee, MH=rp00724en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1126/science.1076557en_US
dc.identifier.pmid12386333-
dc.identifier.scopuseid_2-s2.0-0037131225en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0037131225&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume298en_US
dc.identifier.issue5593en_US
dc.identifier.spage593en_US
dc.identifier.epage597en_US
dc.identifier.isiWOS:000178634800039-
dc.publisher.placeUnited Statesen_US
dc.identifier.scopusauthoridPeale, SJ=6602697819en_US
dc.identifier.scopusauthoridLee, MH=7409119699en_US

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