Small solar system bodies as granular systems

Please use this identifier to cite or link to this item: http://hdl.handle.net/10045/68227
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dc.contributorAstronomía y Astrofísicaes_ES
dc.contributor.authorHestroffer, Daniel-
dc.contributor.authorCampo Bagatin, Adriano-
dc.contributor.authorLosert, Wolfgang-
dc.contributor.authorOpsomer, Eric-
dc.contributor.authorSánchez, Paul-
dc.contributor.authorScheeres, Daniel J.-
dc.contributor.authorStaron, Lydie-
dc.contributor.authorTaberlet, Nicolas-
dc.contributor.authorYano, Hajime-
dc.contributor.authorEggl, Siegfried-
dc.contributor.authorLecomte, Charles-Edouard-
dc.contributor.authorMurdoch, Naomi-
dc.contributor.authorRadjai, Fahrang-
dc.contributor.authorRichardson, Derek C.-
dc.contributor.authorSalazar, Marcos-
dc.contributor.authorSchwartz, Stephen R.-
dc.contributor.authorTanga, Paolo-
dc.contributor.otherUniversidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señales_ES
dc.contributor.otherUniversidad de Alicante. Instituto Universitario de Física Aplicada a las Ciencias y las Tecnologíases_ES
dc.date.accessioned2017-07-17T10:16:41Z-
dc.date.available2017-07-17T10:16:41Z-
dc.date.issued2017-06-30-
dc.identifier.citationEPJ Web of Conferences. 2017, 140: 14011. doi:10.1051/epjconf/201714014011es_ES
dc.identifier.issn2101-6275 (Print)-
dc.identifier.issn2100-014X (Online)-
dc.identifier.urihttp://hdl.handle.net/10045/68227-
dc.description.abstractAsteroids and other Small Solar System Bodies (SSSBs) are currently of great scientific and even industrial interest. Asteroids exist as the permanent record of the formation of the Solar System and therefore hold many clues to its understanding as a whole, as well as insights into the formation of planetary bodies. Additionally, SSSBs are being investigated in the context of impact risks for the Earth, space situational awareness and their possible industrial exploitation (asteroid mining). In all these aspects, the knowledge of the geophysical characteristics of SSSB surface and internal structure are of great importance. Given their size, constitution, and the evidence that many SSSBs are not simple monoliths, these bodies should be studied and modelled as self-gravitating granular systems in general, or as granular systems in micro-gravity environments in particular contexts. As such, the study of the geophysical characteristics of SSSBs is a multi-disciplinary effort that lies at the crossroads between Granular Mechanics, Celestial Mechanics, Soil Mechanics, Aerospace Engineering and Computer Sciences.es_ES
dc.description.sponsorshipThe authors acknowledge support by the International Space Science Institute (ISSI, Bern, Switzerland) and Paris observatory (France) to the international team «Asteroids & Self-Gravitating Bodies as Granular Systemsa». EO acknowledges European Space Agency program SpaceGrains and Prodex (Belspo, Brussels, Belgium) for financial support.es_ES
dc.languageenges_ES
dc.publisherEDP Scienceses_ES
dc.rights© The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).es_ES
dc.subjectSmall solar system bodieses_ES
dc.subjectGranular systemses_ES
dc.subject.otherFísica Aplicadaes_ES
dc.titleSmall solar system bodies as granular systemses_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.peerreviewedsies_ES
dc.identifier.doi10.1051/epjconf/201714014011-
dc.relation.publisherversionhttp://dx.doi.org/10.1051/epjconf/201714014011es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
Appears in Collections:INV - Astronomía y Astrofísica - Comunicaciones a Congresos, Conferencias, etc.

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