@prefix prodottidellaricerca: . @prefix istituto: . @prefix prodotto: . istituto:CDS036 prodottidellaricerca:prodotto prodotto:ID25140 . @prefix pubblicazioni: . @prefix unitaDiPersonaleInterno: . unitaDiPersonaleInterno:MATRICOLA27916 pubblicazioni:autoreCNRDi prodotto:ID25140 . @prefix modulo: . modulo:ID7961 prodottidellaricerca:prodotto prodotto:ID25140 . @prefix rdf: . prodotto:ID25140 rdf:type prodotto:TIPO1101 . @prefix retescientifica: . prodotto:ID25140 rdf:type retescientifica:ProdottoDellaRicerca . @prefix rdfs: . prodotto:ID25140 rdfs:label "A collision in 2009 as the origin of the debris trail of asteroid P/2010 A2 (Articolo in rivista)"@en . @prefix xsd: . prodotto:ID25140 pubblicazioni:anno "2010-01-01T00:00:00+01:00"^^xsd:gYear ; pubblicazioni:doi "10.1038/nature09453"^^xsd:string . @prefix skos: . prodotto:ID25140 skos:altLabel "
C. Snodgrass; C. Tubiana; J.-B. Vincent; H. Sierks; S. Hviid; R. Moissl; H. Boehnhardt; C. Barbieri; D. Koschny; P. Lamy; H. Rickman; R. Rodrigo; B. Carry; S.C. Lowry; R.J.M. Laird; P.R. Weissman; A. Fitzsimmons; S. Marchi; and the OSIRIS team ( M. A'Hearn; F. Angrilli; A. Barucci; J.-L. Bertaux; G. Cremonese; V. Da Deppo; B. Davidsson; S. Debei; M. De Cecco; S. Fornasier; M. Fulle; O. Groussin; P. Guti\u00E9rrez; W.-H. Ip; L. Jorda; H. U. Keller; J. Knollenberg; J. R Kramm; E. Kuehrt; M. Kueppers; L. M. Lara; M. Lazzarin; J. L\u00F3pez; F. Marzari; H. Michalik; G. Naletto; L. Sabau; N. Thomas; K.-P. Wenzel) (2010)
A collision in 2009 as the origin of the debris trail of asteroid P/2010 A2
in Nature (Lond.)
"^^rdf:HTML ; pubblicazioni:autori "C. Snodgrass; C. Tubiana; J.-B. Vincent; H. Sierks; S. Hviid; R. Moissl; H. Boehnhardt; C. Barbieri; D. Koschny; P. Lamy; H. Rickman; R. Rodrigo; B. Carry; S.C. Lowry; R.J.M. Laird; P.R. Weissman; A. Fitzsimmons; S. Marchi; and the OSIRIS team ( M. A'Hearn; F. Angrilli; A. Barucci; J.-L. Bertaux; G. Cremonese; V. Da Deppo; B. Davidsson; S. Debei; M. De Cecco; S. Fornasier; M. Fulle; O. Groussin; P. Guti\u00E9rrez; W.-H. Ip; L. Jorda; H. U. Keller; J. Knollenberg; J. R Kramm; E. Kuehrt; M. Kueppers; L. M. Lara; M. Lazzarin; J. L\u00F3pez; F. Marzari; H. Michalik; G. Naletto; L. Sabau; N. Thomas; K.-P. Wenzel)"^^xsd:string ; pubblicazioni:paginaInizio "814"^^xsd:string ; pubblicazioni:paginaFine "816"^^xsd:string ; pubblicazioni:url "http://www.nature.com/nature/journal/v467/n7317/full/nature09453.html"^^xsd:string ; pubblicazioni:numeroVolume "467"^^xsd:string . @prefix ns11: . prodotto:ID25140 pubblicazioni:rivista ns11:ID372285 ; skos:note "Scopu"^^xsd:string , "ISI Web of Science (WOS)"^^xsd:string ; pubblicazioni:affiliazioni "1,2,3,4,5,6,7,33 : Max-Planck-Institut f\u00FCr Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany\n1 : European Southern Observatory, Alonso de C\u00F3rdova 3107, Casilla 19001, Santiago 19, Chile\n8,18,37 : University of Padova, Department of Astronomy, Vicolo dell'Osservatorio 3, 35122 Padova, Italy\n9,44 : Research and Scientific Support Department, European Space Agency, Keplerlaan 1, Postbus 229, 2201AZ Noordwijk ZH, Netherlands\n10 : Laboratoire d'Astrophysique de Marseille, UMR6110CNRS, Universit\u00E9 Aix-Marseille, 38 rue Fr\u00E9d\u00E9ric Joliot-Curie, 13388 Marseille cedex 13, France\n11,25 : Department of Astronomy and Space Physics, Uppsala University, Box 516, 75120 Uppsala, Sweden\n11 : PAS Space Research Center, Bartycka 18A, 00-716 Warszawa, Poland\n12,29,36,38 : Instituto de Astrof\u00EDsica de Andaluc\u00EDa, CSIC, Box 3004, 18080 Granada, Spain\n13,21,28 : LESIA, Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France\n14,15 : Centre for Astrophysics and Planetary Science, University of Kent, Canterbury CT2 7NH, United Kingdom\n16 : Jet Propulsion Laboratory, MS 183-301, 4800 Oak Grove Drive, Pasadena, CA 91101, United States\n17 : Astrophysics Research Centre, Queen's University Belfast, Belfast BT7 1NN, United Kingdom\n19 : University of Maryland, Department of Astronomy, College Park, MD 20742-2421, United States\n20,26 : Department of Mechanical Engineering, University of Padova, Via Venezia 1, 35131 Padova, Italy\n22 : LATMOS, CNRS, UVSQ/IPSL, 11 Boulevard d'Alembert, 78280 Guyancourt, France\n23 : INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy\n24 : CNR-IFN UOS Padova LUXOR, Via Trasea 7, 35131 Padova, Italy\n27 : UNITN, Universit\u00E0 di Trento, Via Mesiano 77, 38100 Trento, Italy\n30 : National Central University, Institute of Astronomy, 32054 Chung-Li, Taiwan\n31,40 : Institut f\u00FCr Datentechnik und Kommunikationsnetze der TU Braunschweig, Hans-Sommer-Strasse 66, 38106 Braunschweig, Germany\n32,34 : DLR Institute for Planetary Research, Rutherfordstrasse 2, 12489 Berlin, Germany\n35 : ESA-ESAC, Camino bajo del Castillo S/N, 28691 Villanueva de la Ca\u00F1ada, Madrid, Spain\n39 : Department of Physics, University of Padova, Via Marzolo 8, 35131 Padova, Italy\n41 : Department of Information Engineering, University of Padova, Via Gradenigo, 6/B I, 35131 Padova, Italy\n42 : Instituto Nacional de Tecnica Aeroespacial, Carretera de Ajalvir, p.k. 4, 28850 Torrejon de Ardoz, Madrid, Spain\n43 : Physikalisches Institut, Abteilung Weltraumforschung und Planetologie, Universit\u00E4t Bern, Sidlerstrasse 5, 3012 Bern, Switzerland"^^xsd:string ; pubblicazioni:titolo "A collision in 2009 as the origin of the debris trail of asteroid P/2010 A2"^^xsd:string ; prodottidellaricerca:abstract "The peculiar object P/2010 A2 was discovered(1) in January 2010 and given a cometary designation because of the presence of a trail of material, although there was no central condensation or coma. The appearance of this object, in an asteroidal orbit (small eccentricity and inclination) in the inner main asteroid belt attracted attention as a potential new member of the recently recognized(2) class of main-belt comets. If confirmed, this new object would expand the range in heliocentric distance over which main-belt comets are found. Here we report observations of P/2010 A2 by the Rosetta spacecraft. We conclude that the trail arose from a single event, rather than a period of cometary activity, in agreement with independent results(3). The trail is made up of relatively large particles of millimetre to centimetre size that remain close to the parent asteroid. The shape of the trail can be explained by an initial impact ejecting large clumps of debris that disintegrated and dispersed almost immediately. We determine that this was an asteroid collision that occurred around 10 February 2009."@en ; prodottidellaricerca:prodottoDi modulo:ID7961 , istituto:CDS036 ; pubblicazioni:autoreCNR unitaDiPersonaleInterno:MATRICOLA27916 . @prefix parolechiave: . prodotto:ID25140 parolechiave:insiemeDiParoleChiave . ns11:ID372285 pubblicazioni:rivistaDi prodotto:ID25140 . parolechiave:insiemeDiParoleChiaveDi prodotto:ID25140 .