Evolving Marginal Terranes During Neoproterozoic Supercontinent Reorganization: Constraints From the Bemarivo Domain in Northern Madagascar

被引:29
作者
Armistead, Sheree E. [1 ]
Collins, Alan S. [1 ]
Merdith, Andrew S. [2 ]
Payne, Justin L. [3 ]
Cox, Grant M. [1 ]
Foden, John D. [1 ]
Razakamanana, Theodore [4 ]
De Waele, Bert [5 ,6 ]
机构
[1] Univ Adelaide, Dept Earth Sci, Ctr Tecton Resources & Explorat TRaX, Adelaide, SA, Australia
[2] Univ Lyon 1, LGL TPE, Villeurbanne, France
[3] Univ South Australia, Sch Built & Nat Environm, Ctr Tecton Resources & Explorat TraX, Adelaide, SA, Australia
[4] Univ Toliara, Dept Sci Terre, Toliara, Madagascar
[5] SRK Consulting, Perth, WA, Australia
[6] Curtin Univ, Dept Appl Geol, Perth, WA, Australia
基金
澳大利亚研究理事会;
关键词
Rodinia; Gondwana; supercontinent; Neoproterozoic; Lu-Hf; zircon; ZIRCON U-PB; EAST-AFRICAN OROGEN; TONIAN ARC MAGMATISM; TECTONIC EVOLUTION; IN-SITU; SOUTH CHINA; LU-HF; PASSIVE MARGIN; GEOCHRONOLOGY; GRANITOIDS;
D O I
10.1029/2018TC005384
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Madagascar is a key area for unraveling the geodynamic evolution of the transition between the Rodinia and Gondwana supercontinents as it contains several suites of c. 850-700 Ma magmatic rocks that have been postulated to correlate with other Rodinian terranes. The Bemarivo Domain of northern Madagascar contains the youngest of these units that date to c. 750-700 Ma. We present zircon Hf and O isotope data to understand northern Madagascar's place in the Neoproterozoic plate tectonic reconfiguration. We demonstrate that the northern component of the Bemarivo Domain is distinct from the southern part of the Bemarivo Domain and have therefore assigned new names-the Bobakindro Terrane and Marojejy Terrane, respectively. Magmatic rocks of the Marojejy Terrane and Anaboriana Belt are characterized by evolved epsilon(Hf)(t) signatures and a range of delta O-18 values, similar to the Imorona-Itsindro Suite of central Madagascar. These magmatic suites likely formed together in the same long-lived volcanic arc. In contrast, the Bobakindro Terrane contains juvenile epsilon(Hf)(t) and mantle-like delta O-18 values, with no probable link to the rest of Madagascar. We propose that the Bobakindro Terrane formed in a juvenile arc system that included the Seychelles, the Malani Igneous Suite of northwest India, Oman, and the Yangtze Belt of south China, which at the time were all outboard from continental India and south China. The final assembly of northern Madagascar and amalgamation of the Bobakindro Terrane and Marojejy Terrane occurred along the Antsaba subduction zone, with collision occurring at c. 540 Ma.
引用
收藏
页码:2019 / 2035
页数:17
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