scholarly journals Late Paleozoic geodynamic evolution of the western North Patagonian Massif and its tectonic context along the southwestern Gondwana margin

Lithos ◽  
2020 ◽  
Vol 376-377 ◽  
pp. 105801 ◽  
Author(s):  
Paulo Marcos ◽  
Cecilia Pavón Pivetta ◽  
Leonardo Benedini ◽  
Daniel Gregori ◽  
Mauro Geraldes ◽  
...  
2018 ◽  
Author(s):  
Kathryn N. Pauls ◽  
◽  
John L. Isbell ◽  
Levi D. Moxness ◽  
C. Oscar Limarino ◽  
...  

2020 ◽  
Vol 57 (12) ◽  
pp. 1478-1491 ◽  
Author(s):  
Yong-gang Sun ◽  
Bi-le Li ◽  
Feng-yue Sun ◽  
Qing-feng Ding ◽  
Ye Qian ◽  
...  

Geodynamic evolution in the late Paleozoic is significant for understanding the final amalgamation of the Central Asian Orogenic Belt (CAOB). No consensus has yet been reached regarding the late Paleozoic geodynamic evolution of the northern Great Xing’an Range (GXR) in northeastern China, the eastern CAOB. Furthermore, late Paleozoic syenogranite–diabase dyke association is present in the Xiaokele area in northern GXR. It provides an important opportunity to understand the nature of magmatism and the geodynamic evolution during this period. This paper presents new zircon U–Pb ages, zircon Hf isotopic compositions, and geochemical data of whole rocks for Xiaokele syenogranite and diabase. Zircon U–Pb dating suggests that the Xiaokele syenogranite (292.5 ± 0.9 Ma) and diabase (298.3 ± 1.5 Ma) were emplaced during the early Permian. The Xiaokele syenogranites have high SiO2 contents, low MgO contents, and enriched zircon εHf(t) values, suggesting that their primary magma was generated by the partial melting of the juvenile crustal material. The Xiaokele diabases have low SiO2 contents, high MgO contents, are enriched in large-ion lithophile elements, depleted in high-field-strength elements, and exhibit enriched zircon εHf(t) values. They derived from a lithospheric mantle source that had previously been metasomatized by slab-derived fluids. Combined with previous research results, we believe that the continent–continent collision between the Xing’an and Songliao blocks occurred during the late early Carboniferous – early late Carboniferous (330–310 Ma), and the two blocks were transformed into a post-collisional extensional setting during the latest Carboniferous – early Permian.


Geology ◽  
1989 ◽  
Vol 17 (4) ◽  
pp. 324 ◽  
Author(s):  
Suzanne Mahlburg Kay ◽  
Victor A. Ramos ◽  
Constantino Mpodozis ◽  
Patricia Sruoga

Author(s):  
John Davidson ◽  
Constantino Mpodozis ◽  
Estanislao Godoy ◽  
Francisco Hervé ◽  
Robert Pankhurst ◽  
...  

2019 ◽  
Vol 131 (11-12) ◽  
pp. 1907-1919 ◽  
Author(s):  
Ming Wang ◽  
Cai Li ◽  
Xiao-Wen Zeng ◽  
Hang Li ◽  
Jian-Jun Fan ◽  
...  

AbstractThis study presents 13 new U-Pb zircon ages obtained by laser ablation–inductively coupled plasma–mass spectrometry (LA-ICP-MS) together with whole-rock geochemical, Sr-Nd isotopic and zircon Hf isotopic data for a mafic dike swarm in the southern Qiangtang area of Tibet. These data provide the basis for a new model of the late Paleozoic evolution of the Tethys. Combined with the results of previous zircon U-Pb dating, the magmatic zircon grains extracted from mafic dikes yield latest Carboniferous to Early Permian ages (317–279 Ma). The geochemistry of the southern Qiangtang mafic rocks indicates the presence of low-Ti (QLT) and high-Ti (QHT) suites. The magmas that formed the QLT suite underwent higher degrees of partial melting (>5%) and display evidence of crustal contamination, whereas the QHT suite was derived from magmas generated by low-degree (1%–5%) partial melting of a garnet-bearing mantle source, with a greater extent of fractional crystallization than the QLT suite, and no evidence of crustal contamination. We propose that the QHT and QLT suites may have been derived from magmas from different parts of a single mantle plume. The formation of the southern Qiangtang mafic dikes (latest Carboniferous to Early Permian; 317–279 Ma) may have been related to the northward drift of the Cimmerian continent from the northern Gondwana margin, which resulted in the opening of the Meso-Tethys Ocean.


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