Javascript must be enabled to continue!
Late Palaeozoic to Late Triassic northward accretion and incorporation of seamounts along the northern South Pamir: Insights from the anatomy of the Pshart accretionary complex
View through CrossRef
Late Palaeozoic–Mesozoic volcano‐sedimentary rocks within the Rushan–Pshart Suture zone in the Pamir contain critical information on the subduction–accretion history of the Rushan–Pshart Ocean (Meso‐Tethys) prior to the Central–South Pamir collision. In this article, we report new field, petrographic, geochronological, and geochemical data of the Permian to Triassic basic volcanic and sedimentary rocks from the Pshart area. Our field study unravels block‐in‐matrix components within some sedimentary mélanges, which, together with some previously defined ophiolitic mélanges, enables us to define the Pshart accretionary complex (AC), and thus for the first time to discuss the subduction–accretion history of the Rushan–Pshart Ocean and the growth of the Pshart AC. The youngest detrital U–Pb zircons suggest that deposition of sediments was in the Late Triassic (212 Ma). Detritus of Triassic age was primarily derived from the Triassic Karakul‐Mazar Arc‐AC (Northern Pamir) and the Bashgumbaz Magmatic Arc, which developed along the northern margin of South Pamir. The evidence of north‐directed thrusts along the Kara Djilga‐2 and Ken Djilga transverses confirms previous interpretations of southward subduction of the Rushan–Pshart oceanic lithosphere beneath the South Pamir. Geochemical OIB‐type data of the Pshart alkaline basaltic rocks suggest formation in seamounts incorporated into the Pshart AC during the southward subduction of the Rushan–Pshart Ocean. The youngest Late Triassic deposition age is consistent with the coeval time of closure of the Palaeo‐Tethys and Meso‐Tethys oceans in the Pamir. The Pshart AC formed by subduction–accretion processes during the southward subduction of the Meso‐Tethys Ocean along the northern South Pamir and the final docking of the Central and South Pamir (Cimmerian Blocks) may have occurred after the Late Triassic.
Title: Late Palaeozoic to Late Triassic northward accretion and incorporation of seamounts along the northern South Pamir: Insights from the anatomy of the Pshart accretionary complex
Description:
Late Palaeozoic–Mesozoic volcano‐sedimentary rocks within the Rushan–Pshart Suture zone in the Pamir contain critical information on the subduction–accretion history of the Rushan–Pshart Ocean (Meso‐Tethys) prior to the Central–South Pamir collision.
In this article, we report new field, petrographic, geochronological, and geochemical data of the Permian to Triassic basic volcanic and sedimentary rocks from the Pshart area.
Our field study unravels block‐in‐matrix components within some sedimentary mélanges, which, together with some previously defined ophiolitic mélanges, enables us to define the Pshart accretionary complex (AC), and thus for the first time to discuss the subduction–accretion history of the Rushan–Pshart Ocean and the growth of the Pshart AC.
The youngest detrital U–Pb zircons suggest that deposition of sediments was in the Late Triassic (212 Ma).
Detritus of Triassic age was primarily derived from the Triassic Karakul‐Mazar Arc‐AC (Northern Pamir) and the Bashgumbaz Magmatic Arc, which developed along the northern margin of South Pamir.
The evidence of north‐directed thrusts along the Kara Djilga‐2 and Ken Djilga transverses confirms previous interpretations of southward subduction of the Rushan–Pshart oceanic lithosphere beneath the South Pamir.
Geochemical OIB‐type data of the Pshart alkaline basaltic rocks suggest formation in seamounts incorporated into the Pshart AC during the southward subduction of the Rushan–Pshart Ocean.
The youngest Late Triassic deposition age is consistent with the coeval time of closure of the Palaeo‐Tethys and Meso‐Tethys oceans in the Pamir.
The Pshart AC formed by subduction–accretion processes during the southward subduction of the Meso‐Tethys Ocean along the northern South Pamir and the final docking of the Central and South Pamir (Cimmerian Blocks) may have occurred after the Late Triassic.
Related Results
Post-collisional magmatism associated with the final closure of the Rushan-Pshart Meso-Tethys Ocean in Pamir, Tajikistan: Inference from Cretaceous igneous rocks of the Pshart accretionary complex
Post-collisional magmatism associated with the final closure of the Rushan-Pshart Meso-Tethys Ocean in Pamir, Tajikistan: Inference from Cretaceous igneous rocks of the Pshart accretionary complex
The Pamir orogen was formed by the subducted accretion and amalgamation of Cimmerian terranes from the northern margin of Gondwana with the southern margin of Eurasia. The Mesozoic...
Geophysical Mapping of Seamounts and Tectonic Elements over the Extinct Aegir Ridge
Geophysical Mapping of Seamounts and Tectonic Elements over the Extinct Aegir Ridge
The Aegir Ridge was active in the northeastern Atlantic between Norway and Greenland from early Eocene (~55 Ma) until its cessation in late Oligocene (~26–24 Ma). The ridge remains...
Kinematics of the Pamir orogeny on a lithospheric scale
Kinematics of the Pamir orogeny on a lithospheric scale
The south-dipping Benioff zone beneath the Pamir mountains marks the youngest, active slab accommodating India-Asia convergence near the western edge of the Indian indenter (75&...
The birth of the Mesotethys ocean recorded in the Southern Pamir Triassic basalts
The birth of the Mesotethys ocean recorded in the Southern Pamir Triassic basalts
The Pamir orogen, the western extension of the Tibetan plateau, formed and uplifted due to Mesozoic terrane amalgamation and Cenozoic India-Asia collision. The Mesozoic history of ...
Late accretion to Mercury: Global cratering, crust erosion, and accretion of exogenic materials
Late accretion to Mercury: Global cratering, crust erosion, and accretion of exogenic materials
Origin and dynamical evolution of Mercury during the early stage of planet formation are still poorly understood (e.g., Ebel and Stewart, 2018, and references therein). Regardless ...
No continuous suture between Kudi and Oytag: new evidence from geochronology and geochemistry data
No continuous suture between Kudi and Oytag: new evidence from geochronology and geochemistry data
<p>A lateral continuity between belts of mafic and ultramafic Paleozoic rocks found in the West Kunlun of Northern Tibet and comparable rocks, known from an outcrop i...
Foreland thrusting and slab formation in the Pamir
Foreland thrusting and slab formation in the Pamir
<p>The western and northern sectors of the northward convex Pamir arc are underlain by a steep Benioff zone dipping east to south, traced by earthquakes to depths of ...
The rise of ginkgoalean plants in the early Mesozoic: a data analysis
The rise of ginkgoalean plants in the early Mesozoic: a data analysis
AbstractIn the present article, ginkgoalean fossil records are analysed and the data are incorporated into a sketched, ‘epoch‐by‐epoch’ framework (e.g. late Triassic, early Jurassi...

