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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/116872
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dc.contributor.authorPerna, D.-
dc.contributor.authorAlvarez-Candal, A.-
dc.contributor.authorFornasier, S.-
dc.contributor.authorKanuchova, Z.-
dc.contributor.authorGiuliatti Winter, S. M.-
dc.contributor.authorVieira Neto, E.-
dc.contributor.authorWinter, O. C.-
dc.date.accessioned2015-03-18T15:54:18Z-
dc.date.accessioned2016-10-25T20:28:15Z-
dc.date.available2015-03-18T15:54:18Z-
dc.date.available2016-10-25T20:28:15Z-
dc.date.issued2014-08-01-
dc.identifierhttp://dx.doi.org/10.1051/0004-6361/201424447-
dc.identifier.citationAstronomy & Astrophysics. Les Ulis Cedex A: Edp Sciences S A, v. 568, 4 p., 2014.-
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/11449/116872-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/116872-
dc.description.abstractContext. The Brazilian Aster project plans a space mission to rendezvous and characterize (153591) 2001 SN263, one of the only two known triple near-Earth asteroids (NEAs). Improving the knowledge of its physical properties is necessary to optimize the mission planning and science return.Aims. We study the surface composition and physical nature of 2001 SN263 by analyzing and comparing its reflectance spectra with laboratory spectra of minerals and meteorites.Methods. We performed spectroscopic observations of 2001 SN263 using the UV-to-NIR X-Shooter spectrograph at the ESO Very Large Telescope (VLT). Complementary photometric observations of the target were acquired with the FORS2 instrument.Results. We find B-type, featureless convex spectra (Themis-or Polana-like). 2001 SN263 presents the bluest visible spectrum ever observed for small bodies in the solar system, even bluer than NEAs Phaethon and Bennu. The spectra suggest that the surface composition is organic-and magnetite-rich, similar to that of heated CI carbonaceous chondrites. Phyllosilicates may be abundant as well. We find hints of a coarse-grained surface and composition variety within the triple system.Conclusions. Both the large grain size and surface variability might be connected to the formation of the triple system. The Aster mission will have the intriguing possibility of checking current models of asteroid binary formation.en
dc.description.sponsorshipNEOShield project - European Commission's Seventh Framework Programme-
dc.description.sponsorshipVEGA - The Slovack Agency for Science-
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ)-
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
dc.description.sponsorshipINCT Estudos do Espaco-
dc.description.sponsorshipFrench INSU-PNP program-
dc.format.extent4-
dc.language.isoeng-
dc.publisherEdp Sciences S A-
dc.sourceWeb of Science-
dc.subjectminor planetsen
dc.subjectasteroids: individual: (153591) 2001 SN263en
dc.subjecttechniques: spectroscopicen
dc.subjecttechniques: photometricen
dc.titleThe triple near-Earth asteroid (153591) 2001 SN263: an ultra-blue, primitive target for the Aster space missionen
dc.typeoutro-
dc.contributor.institutionUniv Paris Diderot-
dc.contributor.institutionObserv Nacl-
dc.contributor.institutionUniv Paris 07-
dc.contributor.institutionSlovak Acad Sci-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Paris Diderot, Univ Paris 06, CNRS, LESIA Observ Paris, F-92195 Meudon, France-
dc.description.affiliationObserv Nacl, BR-20921400 Rio De Janeiro, Brazil-
dc.description.affiliationUniv Paris 07, F-75013 Paris, France-
dc.description.affiliationSlovak Acad Sci, Astron Inst, Tatranska Lomnica 05960, Slovakia-
dc.description.affiliationUniv Estadual Paulista, Grp Dinam Orbital & Planetol, BR-12516410 Sp Guaratingueta, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Grp Dinam Orbital & Planetol, BR-12516410 Sp Guaratingueta, Brazil-
dc.description.sponsorshipIdNEOShield project - European Commission's Seventh Framework ProgrammeFP7-SPACE-2011-282703-
dc.description.sponsorshipIdVEGA - The Slovack Agency for Science2/0032/14-
dc.description.sponsorshipIdFAPESP: 11/08171-3-
dc.identifier.doi10.1051/0004-6361/201424447-
dc.identifier.wosWOS:000341185900138-
dc.rights.accessRightsAcesso aberto-
dc.identifier.fileWOS000341185900138.pdf-
dc.relation.ispartofAstronomy & Astrophysics-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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