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An orbital determination of Triton with the use of a revised pole model

hal.structure.identifierNational Time Service Center [Lintong, Shaanxi] [NTSC]
hal.structure.identifierGraduate School of the Chinese Academy of Sciences [GSCAS]
dc.contributor.authorZHANG, H. Y.
hal.structure.identifierNational Time Service Center [Lintong, Shaanxi] [NTSC]
dc.contributor.authorSHEN, K. X.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorDOURNEAU, G.
hal.structure.identifierThe Wellcome Trust Sanger Institute [Cambridge]
dc.contributor.authorHARPER, D.
hal.structure.identifierNational Time Service Center [Lintong, Shaanxi] [NTSC]
dc.contributor.authorQIAO, R. C.
hal.structure.identifierNational Time Service Center [Lintong, Shaanxi] [NTSC]
hal.structure.identifierGraduate School of the Chinese Academy of Sciences [GSCAS]
dc.contributor.authorXI, X. J.
hal.structure.identifierGraduate School of the Chinese Academy of Sciences [GSCAS]
dc.contributor.authorCHENG, X.
hal.structure.identifierNational Time Service Center [Lintong, Shaanxi] [NTSC]
dc.contributor.authorYAN, D.
hal.structure.identifierShanghai Astronomical Observatory [Shanghai] [SHAO]
dc.contributor.authorLI, S. N.
hal.structure.identifierShanghai Astronomical Observatory [Shanghai] [SHAO]
dc.contributor.authorWANG, S. H.
dc.date.issued2014
dc.identifier.issn0035-8711
dc.description.abstractEnIn this paper, we used the 3108 Earth-based astrometric observations from the Natural Satellite Data Center over more than 30 yr time span from 1975 to 2006 for determining the epoch state vectors of the Neptunian largest satellite Triton. These observations almost contain all modern photo and CCD observations available. In integrating perturbation equation, the barycentric frame of Neptune-Triton system is adopted, and in considering the oblateness perturbation due to Neptune, a revised pole model describing the precession of the Neptune's pole is used in our calculation.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.subject.enastrometry
dc.subject.enplanets and satellites: general
dc.title.enAn orbital determination of Triton with the use of a revised pole model
dc.typeArticle de revue
dc.identifier.doi10.1093/MNRAS/STT2304
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page1663-1668
bordeaux.volume438
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-00944312
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00944312v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society&rft.date=2014&rft.volume=438&rft.issue=2&rft.spage=1663-1668&rft.epage=1663-1668&rft.eissn=0035-8711&rft.issn=0035-8711&rft.au=ZHANG,%20H.%20Y.&SHEN,%20K.%20X.&DOURNEAU,%20G.&HARPER,%20D.&QIAO,%20R.%20C.&rft.genre=article


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