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- Publisher Website: 10.1126/science.1076557
- Scopus: eid_2-s2.0-0037131225
- PMID: 12386333
- WOS: WOS:000178634800039
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Article: A primordial origin of the laplace relation among the Galilean satellites
Title | A primordial origin of the laplace relation among the Galilean satellites |
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Authors | |
Issue Date | 2002 |
Publisher | American 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? |
Abstract | Understanding 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 Identifier | http://hdl.handle.net/10722/151089 |
ISSN | 2023 Impact Factor: 44.7 2023 SCImago Journal Rankings: 11.902 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
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dc.contributor.author | Peale, SJ | en_US |
dc.contributor.author | Lee, MH | en_US |
dc.date.accessioned | 2012-06-26T06:16:57Z | - |
dc.date.available | 2012-06-26T06:16:57Z | - |
dc.date.issued | 2002 | en_US |
dc.identifier.citation | Science, 2002, v. 298 n. 5593, p. 593-597 | en_US |
dc.identifier.issn | 0036-8075 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/151089 | - |
dc.description.abstract | Understanding 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.language | eng | en_US |
dc.publisher | American Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org | en_US |
dc.relation.ispartof | Science | en_US |
dc.title | A primordial origin of the laplace relation among the Galilean satellites | en_US |
dc.type | Article | en_US |
dc.identifier.email | Lee, MH:mhlee@hku.hk | en_US |
dc.identifier.authority | Lee, MH=rp00724 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.doi | 10.1126/science.1076557 | en_US |
dc.identifier.pmid | 12386333 | - |
dc.identifier.scopus | eid_2-s2.0-0037131225 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-0037131225&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 298 | en_US |
dc.identifier.issue | 5593 | en_US |
dc.identifier.spage | 593 | en_US |
dc.identifier.epage | 597 | en_US |
dc.identifier.isi | WOS:000178634800039 | - |
dc.publisher.place | United States | en_US |
dc.identifier.scopusauthorid | Peale, SJ=6602697819 | en_US |
dc.identifier.scopusauthorid | Lee, MH=7409119699 | en_US |
dc.identifier.issnl | 0036-8075 | - |