A-type magmatism in a syn-collisional setting: The case of the Pan-African Hook Batholith in Central Zambia

作者:Milani Lorenzo*; Lehmann Jeremie; Naydenov Kalin V; Saalmann Kerstin; Kinnaird Judith A; Daly J Stephen; Frei Dirk; Lobo Guerrero Sanz Alberto
来源:Lithos, 2015, 216: 48-72.
DOI:10.1016/j.lithos.2014.11.029

摘要

The Pan-African Hook Batholith formed during the assembly of the Gondwana supercontinent as a result of syncollisional stage interaction between the Congo and Kalahari Cratons. The bimodal magmatism (mafic to predominantly felsic) is characterized by both an alkali-calcic and an alkalic suite, with typical A-type, metaluminous, high Fe/Mg and K/Na geochemical signature. Occasionally, sodic granitoids have been documented. Compositions were driven to more differentiated products by fractional crystallization, while Sr-Nd isotopes exclude crustal assimilation during crystallization. Recent new U-Pb age data constrain most of the felsic magmatism between 550 and 540 Ma. Scattered outcrops of gabbroic rocks, both tholeiitic and alkaline, testify to periodic input of mantle material, and, in some cases, to interaction with metasomatizing fluids. Crystallization ages on mafic rocks span from 570 to 520 Ma, thus indicating that they were contemporaneous with the major granitic intrusion, which was the result of a number of successive felsic batches, eventually forming a coalescing batholith. Highly radiogenic Pb isotopic values attest to the radiogenic character of the rocks. Such an anomalous signature was acquired during, or soon after, magma emplacement, perhaps as result of metasomatizing fluids. Enrichment in Th-U of large portions of the crust along this part of the margin of the Congo Craton is suggested. Geochemical and isotopic evidence support the interaction between mantle components and portions of the deep crust at pressure of < 10 kbar, while decompression melting of rising asthenospheric mantle ponding at the base of the crust heated, and ultimately melted, crustal material. An additional and crucial contribution to the crustal melting was likely provided by internal radiogenic heat production of the thickened crust, and is in agreethent with the high radioactivity of the pluton. A tectono-thermal model, implying crustal accretion accompanied by slab retreat and lithospheric mantle thinning, is proposed to reconcile coeval orogenic contraction in the crust and A-type magmatism. Low-pressure mineral phases in metasedimentaty wall rocks along the eastern margin of the pluton indicate that the magma was emplaced at shallow crustal depths. This study further supports the idea that A-type granites, commonly considered to be restricted to anorogenic or extension-related environments, can also occur in compressional regimes.

  • 出版日期2015-2