Logotipo do repositório
 

Publicação:
The sailboat island and the New Horizons trajectory

dc.contributor.authorWinter, Silvia M. Giuliatti [UNESP]
dc.contributor.authorWinter, Othon C. [UNESP]
dc.contributor.authorNeto, Ernesto Vieira [UNESP]
dc.contributor.authorSfair, Rafael [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2015-10-22T07:23:09Z
dc.date.available2015-10-22T07:23:09Z
dc.date.issued2015-01-15
dc.description.abstractIn previous works we have studied the location of stable regions in the Pluto-Charon system. Among the findings, we discovered an island of stability, named sailboat island. One of the main goals of the New Horizons mission, launched in 2006, is to have a flyby close to the Pluto-Charon system in order to explore it. In the present work we analyze the relevance of the sailboat island for the New Horizons mission. Firstly, we identify the location and extent of these stable trajectories in the physical space around Pluto. They go beyond the trajectory of Charon in a way that Charon never crosses such trajectories. We verify that the nominal trajectory of the New Horizons spacecraft passes near the region of the sailboat island trajectories, reaching the closest distance at about 1650 km. Analyzing an alternative trajectory for the spacecraft, known as Deep Inner SHBOT, we found that it is not as safe as the nominal trajectory, because it crosses a region of highly inclined trajectories located at the sailboat island. We also estimate the density of particles from the sailboat island in the physical space around Pluto in comparison with the density of particles from a well-known stable region of near circular trajectories close to Pluto. Finally, we identified the location of the densest regions, which corresponds to the highest probable location of particles of the sailboat island. Such locations can be considered as spots for search and new detections of bodies by the New Horizons cameras along the flyby close to the Pluto-Charon system. (C) 2014 Elsevier Inc. All rights reserved.en
dc.description.affiliationUnespUniv. Estadual Paulista – UNESP, Grupo de Dinâmica Orbital e Planetologia, Guaratinguetá CEP 12516-410, Brazil
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipINCT-Estudos do Espaço
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipIdFAPESP: 2011/08171-3
dc.format.extent339-344
dc.identifierhttp://www.sciencedirect.com/science/article/pii/S0019103514001869
dc.identifier.citationIcarus. San Diego: Academic Press Inc Elsevier Science, v. 246, p. 339-344, 2015.
dc.identifier.doi10.1016/j.icarus.2014.04.003
dc.identifier.issn0019-1035
dc.identifier.lattes6928187292584643
dc.identifier.orcid0000-0002-4939-013X
dc.identifier.urihttp://hdl.handle.net/11449/129861
dc.identifier.wosWOS:000346693800031
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofIcarus
dc.relation.ispartofjcr2.981
dc.relation.ispartofsjr2,037
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.subjectCelestial mechanicsen
dc.subjectKuiper Belten
dc.subjectPlutoen
dc.titleThe sailboat island and the New Horizons trajectoryen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.author.lattes6928187292584643[3]
unesp.author.orcid0000-0002-7589-0998[3]
unesp.author.orcid0000-0002-3949-6045[1]
unesp.author.orcid0000-0002-4939-013X[4]
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia, Guaratinguetápt
unesp.departmentMatemática - FEGpt

Arquivos