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DOI10.1016/j.tecto.2021.228779
Assessing the brittle crust thickness from strike-slip fault segments on Earth, Mars and Icy moons
Donzé F.-V.; Klinger Y.; Bonilla-Sierra V.; Duriez J.; Jiao L.; Scholtès L.
发表日期2021
ISSN00401951
卷号805
英文摘要Segment lengths along major strike-slip faults exhibit a size dependency related to the brittle crust thickness. These segments result in the formation of the localized “P-shear” deformation crossing and connecting the initial Riedels structures (i.e. en-echelon fault structures) which formed during the genesis stage of the fault zone. Mechanical models show that at all scales, the geometrical characteristics of the Riedels exhibit dependency on the thickness of the brittle layer. Combining the results of our mechanical discrete element model with several analogue experiments using sand, clay and gypsum, we have formulated a relationship between the orientation and spacing of Riedels and the thickness of the brittle layer. From this relationship, we derive that for a pure strike-slip mode, the maximum spacing between the Riedels is close to three times the thickness of the layer. For a transtensional mode, as the extensive component becomes predominant, the spacing distance at the surface becomes much smaller than the thickness. Applying this relationship to several well-characterized strike-slip faults on Earth, we show that the predicted brittle thickness is consistent with the seismogenic depth. Supposing the ubiquity of this phenomenon, we extented this relationship to characterize en-echelon structures observed on Mars, in the Memnonia region located West of Tharsis. Assuming that the outer ice shells of Ganymede, Enceladus and Europa, exhibit a brittle behavior, we suggest values of the corresponding apparent brittle thicknesses. © 2021 Elsevier B.V.
关键词Brittle crust thicknessDiscrete element modelEn-echelon structuresIcy moonsMarsStrike-slip faults
英文关键词Strike-slip faults; Brittle behavior; Brittle layers; Discrete element modeling; Echelon faults; Geometrical characteristics; Mechanical model; Segment lengths; Size dependency; Fault slips; brittle medium; crustal thickness; deformation; discrete element method; en echelon structure; Mars; Moon; strike-slip fault
语种英语
来源期刊Tectonophysics
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/207964
作者单位Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, IFSTTAR, ISTerre, Grenoble, 38000, France; Institut de Physique du Globe de Paris, Sorbonne Paris Cite, Université Paris Diderot, UMR 7154, CNRS, Paris, France; Inrae, UR RECOVER, Aix-en-Provence, F-13182, France; Univ. Clermont Auvergne, CNRS, IRD, OPGC, Laboratoire Magmas et Volcans, Clermont-Ferrand, 63000, France
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Donzé F.-V.,Klinger Y.,Bonilla-Sierra V.,et al. Assessing the brittle crust thickness from strike-slip fault segments on Earth, Mars and Icy moons[J],2021,805.
APA Donzé F.-V.,Klinger Y.,Bonilla-Sierra V.,Duriez J.,Jiao L.,&Scholtès L..(2021).Assessing the brittle crust thickness from strike-slip fault segments on Earth, Mars and Icy moons.Tectonophysics,805.
MLA Donzé F.-V.,et al."Assessing the brittle crust thickness from strike-slip fault segments on Earth, Mars and Icy moons".Tectonophysics 805(2021).
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