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成果名称: Fluxed melting of metapelite and the formation of Miocene high-CaO two-mica granites in the Malashan gneiss dome, southern Tibet
作者: Li-E. Gao
Lingsen Zeng
首次发表日期: 2014-06
出版者: Institute of Geology Chinese Academy of Geological Sciences
摘要: Identifying the timing of formation and geochemical nature of the Cenozoic granites along the Himalayan orogen is essen- tial to test or formulate models that link crustal anatexis with tectonic transition during the evolution of large-scale collisional orogenic belts. The Malashan gneiss dome, one of the prominent domes within the Tethyan Himalaya, experienced Barro- vian-type metamorphism and partial melting of pelitic rocks at relatively deep levels during the collision between India and Eurasia. New LA-MC-ICP-MS zircon U–Pb analyses yielded that the Malashan two-mica granites formed at a time span of 17.6 ± 0.1 to 16.9 ± 0.1 Ma. The Malashan two-mica granites are characterized by: (1) high SiO 2 (>71.3 wt.%), Al 2 O 3 (>14.8 wt.%), and relatively high CaO (>1.3 wt.%); (2) relatively high Sr (>146 ppm), but low Rb/Sr ratios (<1.3) which are nearly constant relative to large variations in Ba concentrations; (3) enrichment in LREE, depletion in HREE, and no or weak negative Eu anomalies (Eu/Eu * = 0.7–0.9); (4) as compared to granites in the other Northern Himalayan Gneiss Domes and High Himalayan Belt, relatively lower initial 87 Sr/ 86 Sr ratios (0.7391–0.7484) and similar unradiogenic Nd isotope compositions (e Nd (t) = ?13.7 to ?14.4). These characteristics imply that the two-mica granites were derived from fluid-fluxing melting of metapelite, possibly triggered by the E–W extension. Our new data in combination with literature data indicate that there are three types of granites with diverse geochemical characteristics and distinct formation mechanisms along the Hima- layan orogen since the Cenozoic India–Eurasia continental collision. Conceivably, our new results will provide new insights on how the partial melting behavior of relatively deeper crustal rocks evolved as the tectonic evolution of large orogenic belts. Crown copyright ? 2014 Published by Elsevier Ltd. All rights reserved.
引用地址: http://www.igeodata.org/handle/20.500.11758/193
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