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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/116872
Title: 
The triple near-Earth asteroid (153591) 2001 SN263: an ultra-blue, primitive target for the Aster space mission
Author(s): 
Institution: 
  • Univ Paris Diderot
  • Observ Nacl
  • Univ Paris 07
  • Slovak Acad Sci
  • Universidade Estadual Paulista (UNESP)
ISSN: 
0004-6361
Sponsorship: 
  • NEOShield project - European Commission's Seventh Framework Programme
  • VEGA - The Slovack Agency for Science
  • Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
  • Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ)
  • Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
  • INCT Estudos do Espaco
  • French INSU-PNP program
Sponsorship Process Number: 
  • NEOShield project - European Commission's Seventh Framework ProgrammeFP7-SPACE-2011-282703
  • VEGA - The Slovack Agency for Science2/0032/14
  • FAPESP: 11/08171-3
Abstract: 
Context. 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.
Issue Date: 
1-Aug-2014
Citation: 
Astronomy & Astrophysics. Les Ulis Cedex A: Edp Sciences S A, v. 568, 4 p., 2014.
Time Duration: 
4
Publisher: 
Edp Sciences S A
Keywords: 
  • minor planets
  • asteroids: individual: (153591) 2001 SN263
  • techniques: spectroscopic
  • techniques: photometric
Source: 
http://dx.doi.org/10.1051/0004-6361/201424447
URI: 
Access Rights: 
Acesso aberto
Type: 
outro
Source:
http://repositorio.unesp.br/handle/11449/116872
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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