Fluxed melting of metapelite and the formation of Miocene high-CaO two-mica granites in the Malashan gneiss dome, southern Tibet

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• 作者：Li-E. Gao ; ^{liegao09@gmail.com" class="auth_mail} ; Lingsen Zeng
• 刊名：Geochimica et Cosmochimica Acta
• 出版年：1 April, 2014
• 年：2014
• 卷：130
• 期：Complete
• 页码：136-155
• 全文大小：2322 K

文摘

Identifying the timing of formation and geochemical nature of the Cenozoic granites along the Himalayan orogen is essential 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 Barrovian-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 卤 0.1 to 16.9 卤 0.1 Ma. The Malashan two-mica granites are characterized by: (1) high SiO₂ (>71.3 wt.%), Al₂O₃ (>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^{鈭?/sup> = 0.7-0.9); (4) as compared to granites in the other Northern Himalayan Gneiss Domes and High Himalayan Belt, relatively lower initial 87Sr/86Sr ratios (0.7391-0.7484) and similar unradiogenic Nd isotope compositions (蔚_Nd(t) = 鈭?3.7 to 鈭?4.4). 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 Himalayan 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.}