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dc.creatorMadiedo Gil, José Maríaes
dc.creatorTrigo-Rodríguez, Josep Mariaes
dc.creatorWilliams, Iwan P.es
dc.creatorKonovalova, Natalia A.es
dc.creatorOrtiz, J. L.es
dc.creatorCastro-Tirado, A. J.es
dc.creatorPastor, Sensies
dc.creatorReyes, José A. de loses
dc.creatorCabrera Caño, Jesús Maríaes
dc.date.accessioned2018-03-19T17:16:42Z
dc.date.available2018-03-19T17:16:42Z
dc.date.issued2014
dc.identifier.citationMadiedo Gil, J.M., Trigo-Rodríguez, J.M., Williams, I.P., Konovalova, N.A., Ortiz, J.L., Castro-Tirado, A.J.,...,Cabrera-Caño, J. (2014). Near-earth object 2012XJ112 as a source of bright bolides of achondritic nature. Monthly Notices of the Royal Astronomical Society, 439 (4), 3704-3711.
dc.identifier.issn0035-8711es
dc.identifier.urihttps://hdl.handle.net/11441/71103
dc.description.abstractWe analyse the likely link between the recently discovered near-Earth object 2012XJ112 and a bright fireball observed over the south of Spain on 2012 December 27. The bolide, with an absolute magnitude of -9 ± 1, was simultaneously imaged during the morning twilight from twometeor stations operated by the SPanish Meteor Network (SPMN). It was also observed by several casual witnesses. The emission spectrum produced during the ablation of the meteoroid in the atmosphere was also recorded. From its analysis, the chemical nature of this particle was inferred. Although our orbital association software identified several potential parent bodies for this meteoroid, the analysis of the evolution of the orbital elements performed with the MERCURY 6 symplectic integrator supports the idea that NEO 2012XJ112 is the source of this meteoroid. The implications of this potential association are discussed here. In particular, the meteoroid bulk chemistry is consistent with a basaltic achondrite, and this emphasizes the importance to deduce from future Earth approaches the reflectance spectrum and taxonomic nature of 2012XJ112. © 2014 The Author. Published by Oxford University Press on behalf of the Royal Astronomical Society.es
dc.description.sponsorshipMinisterio de Ciencia y Educación AYA2009-13227, AYA2011-26522, AYA2009-06330-Ees
dc.description.sponsorshipJunta de Andalucía P09-FQM- 4555es
dc.formatapplication/pdfes
dc.language.isoenges
dc.publisherBlackwell Publishing Ltdes
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society, 439 (4), 3704-3711.
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectMeteoriteses
dc.subjectMinor planets asteroids individual 2012XJ112es
dc.titleNear-earth object 2012XJ112 as a source of bright bolides of achondritic naturees
dc.typeinfo:eu-repo/semantics/articlees
dcterms.identifierhttps://ror.org/03yxnpp24
dc.type.versioninfo:eu-repo/semantics/publishedVersiones
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.contributor.affiliationUniversidad de Sevilla. Departamento de Física Atómica, Molecular y Nucleares
dc.relation.publisherversionttp://dx.doi.org/10.1093/mnras/stu222es
dc.identifier.doi10.1093/mnras/stu222es
idus.format.extent8es
dc.journaltitleMonthly Notices of the Royal Astronomical Societyes
dc.publication.volumen439es
dc.publication.issue4es
dc.publication.initialPage3704es
dc.publication.endPage3711es
dc.contributor.funderMinisterio de Ciencia e Innovación (MICIN). España
dc.contributor.funderJunta de Andalucía

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