Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/11129
DC FieldValueLanguage
dc.date.accessioned2018-03-12T10:56:52Zen
dc.date.available2018-03-12T10:56:52Zen
dc.date.issued2017-11-15en
dc.identifier.urihttp://hdl.handle.net/2122/11129en
dc.description.abstractWe determine the depth of fracture penetration in multiple regions of Enceladus by performing self-similar clustering and length distribution analysis of fractures. The statistical characterization of fault-population attribute, such as length and clustering, provide a productive avenue for exploring deformation rate, stress transmission mode, rheology of the medium, and mechanical stratification of the ice satellite. Through this analysis, we estimate the depth of the mechanical discontinuity of Enceladus’ ice shell that is the depth to which fractures penetrate the brittle ice layer above the ductile one. In this work, we find that for the South Polar Terrain (SPT), the brittle ice shell interested by fracture penetration is about 30 km and corresponds to the total depth of the ice shell because the SPT has a very high thermal gradient and, hence, fractures likely reach the ocean-ice interface. In the other regions analyzed, the depth of fracture penetration increases from 31 to 70 km from the South Pole to northern regions up to 75°.en
dc.language.isoEnglishen
dc.relation.ispartofIcarusen
dc.relation.ispartofseries/297 (2017)en
dc.subjectPlanetary Geology, faulting, brittle thicknessen
dc.titleBrittle ice shell thickness of Enceladus from fracture distribution analysisen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber252-264en
dc.identifier.URLhttps://www.sciencedirect.com/science/article/pii/S001910351630416X?via%3Dihuben
dc.subject.INGVfault system analysis in ici satellite (Enceladus)en
dc.identifier.doi10.1016/j.icarus.2017.07.009en
dc.description.obiettivoSpecifico7T. Struttura della Terra e geodinamicaen
dc.description.journalTypeJCR Journalen
dc.contributor.authorLucchetti, A.en
dc.contributor.authorPozzobon, R.en
dc.contributor.authorMazzarini, Francescoen
dc.contributor.authorCremonese, G.en
dc.contributor.authorMassironi, M.en
dc.contributor.departmentINAF-Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35131 Padova, Italyen
dc.contributor.departmentDipartimento di Geoscienze, Università di Padova, Padova, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italiaen
dc.contributor.departmentINAF-Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35131 Padova, Italyen
dc.contributor.departmentDipartimento di Geoscienze, Università di Padova, Padova, Italyen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptINAF-Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35131 Padova, Italy-
crisitem.author.deptDepartment of Geosciences, University of Padova-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italia-
crisitem.author.deptINAF, Osservatorio Astronomico di Padova-
crisitem.author.deptDepartment of Geosciences, University of Padova-
crisitem.author.orcid0000-0001-9183-645X-
crisitem.author.orcid0000-0002-3864-6558-
crisitem.author.orcid0000-0001-9021-1140-
crisitem.author.orcid0000-0002-7757-8818-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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