Özet
Lower crustal flow in regions of post-orogenic extension has been inferred to explain the exhumation of metamorphic core complexes and associated low-angle normal (detachment) fault systems. However, the origin of detachment faults, whether initially formed as high-angle or low-angle shear zones, and the extension is symmetric or asymmetric remains enigmatic. Here, we use numerical modeling constrained by geophysical and geological data to show that symmetric extension in the central Menderes Massif of western Anatolia is accommodated by the crustal flow. Our geodynamic model explains how opposite dipping Gediz and Büyük Menderes detachment faults are formed by ∼40° footwall rotation. Model predictions agree with seismic tomography data that suggests updoming of lower crust beneath the exhumed massifs, represented as “twin domes” and a flat Moho. Our work helps to account for the genetic relation between the exhumation of metamorphic core complexes and low-angle normal faulting in both Cordillera and Aegean orogenic regions and has important implications on crustal dynamics in extensional provinces.
Orijinal dil | İngilizce |
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Makale numarası | 118309 |
Dergi | Earth and Planetary Science Letters |
Hacim | 619 |
DOI'lar | |
Yayın durumu | Yayınlandı - 1 Eki 2023 |
Bibliyografik not
Publisher Copyright:© 2023 Elsevier B.V.
Finansman
We thank the Computational Infrastructure for Geodynamics (geodynamics.org) which is funded by the National Science Foundation under award EAR-0949446 and EAR-1550901 for supporting the development of ASPECT. The numerical experiments presented here are available through contacting the authors. Meanwhile, documentation and the details for the numerical code can be found online (at https://aspect.geodynamics.org). OHG, AF and EŞU acknowledge Anatolian Tectonics Project-ANATEC (funded by International Lithosphere Program). The authors gratefully acknowledge the computing time granted by the Resource Allocation Board and provided on the supercomputer Lise at NHR@ZIB as part of the NHR infrastructure. The calculations for this research were conducted with computing resources under the project bbp00039. We are grateful to Paul Kapp and an anonymous reviewer for their constructive comments on the manuscript. OHG acknowledges Turkish Academy of Sciences (TUBA) for GEBIP support and TUBITAK for 2219 fellowship programme. ACG is funded by a Helmholtz Recruitment Initiative. We thank the Computational Infrastructure for Geodynamics (geodynamics.org) which is funded by the National Science Foundation under award EAR-0949446 and EAR-1550901 for supporting the development of ASPECT. The numerical experiments presented here are available through contacting the authors. Meanwhile, documentation and the details for the numerical code can be found online (at https://aspect.geodynamics.org ). OHG, AF and EŞU acknowledge Anatolian Tectonics Project-ANATEC (funded by International Lithosphere Program). The authors gratefully acknowledge the computing time granted by the Resource Allocation Board and provided on the supercomputer Lise at NHR@ZIB as part of the NHR infrastructure. The calculations for this research were conducted with computing resources under the project bbp00039. We are grateful to Paul Kapp and an anonymous reviewer for their constructive comments on the manuscript. OHG acknowledges Turkish Academy of Sciences (TUBA) for GEBIP support and TUBITAK for 2219 fellowship programme. ACG is funded by a Helmholtz Recruitment Initiative .
Finansörler | Finansör numarası |
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Anatolian Tectonics Project-ANATEC | bbp00039 |
TUBA | |
National Science Foundation | EAR-0949446, EAR-1550901 |
Türkiye Bilimsel ve Teknolojik Araştırma Kurumu | |
Türkiye Bilimler Akademisi |