Publicação:
The triple near-Earth asteroid (153591) 2001 SN263: an ultra-blue, primitive target for the Aster space mission

dc.contributor.authorPerna, D.
dc.contributor.authorAlvarez-Candal, A.
dc.contributor.authorFornasier, S.
dc.contributor.authorKanuchova, Z.
dc.contributor.authorGiuliatti Winter, S. M. [UNESP]
dc.contributor.authorVieira Neto, E. [UNESP]
dc.contributor.authorWinter, O. C. [UNESP]
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.date.accessioned2015-03-18T15:54:18Z
dc.date.available2015-03-18T15:54:18Z
dc.date.issued2014-08-01
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.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.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.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.format.extent4
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.doi10.1051/0004-6361/201424447
dc.identifier.fileWOS000341185900138.pdf
dc.identifier.issn0004-6361
dc.identifier.lattes9224861533404236
dc.identifier.lattes7161963144100182
dc.identifier.lattes0960024575647258
dc.identifier.urihttp://hdl.handle.net/11449/116872
dc.identifier.wosWOS:000341185900138
dc.language.isoeng
dc.publisherEdp Sciences S A
dc.relation.ispartofAstronomy & Astrophysics
dc.relation.ispartofsjr2,265
dc.rights.accessRightsAcesso aberto
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.typeArtigo
dcterms.rightsHolderEdp Sciences S A
dspace.entity.typePublication
unesp.author.lattes9224861533404236
unesp.author.lattes7161963144100182
unesp.author.lattes0960024575647258
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia, Guaratinguetápt
unesp.departmentMatemática - FEGpt

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