Post-collisional potassic magmatism in the eastern Lhasa ... · Tibet: Products of partial melting...

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Post-collisional potassic magmatism in the eastern Lhasa terrane, South Tibet: Products of partial melting of mélanges in a continental subduction channel Lihong Zhang a,b , Zhengfu Guo a, , Maoliang Zhang a,b , Zhihui Cheng a,b , Yutao Sun a,b a Key Laboratory of Cenozoic Geology and Environment, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China b University of Chinese Academy of Sciences, Beijing 100049, China abstract article info Article history: Received 29 May 2015 Received in revised form 18 October 2015 Accepted 3 November 2015 Available online 23 December 2015 Post-collisional, potassic magmatic rocks widely distributed in the eastern Lhasa terrane provide signicant information for comprehensive understanding of geodynamic processes of northward subduction of the Indian lithosphere and uplift of the Tibetan Plateau. A combined dataset of whole-rock major and trace elements, SrNdPb isotopes, and in situ zircon UPb dating and HfO isotopic analyses are presented for the Yangying potassic volcanic rocks (YPVR) in the eastern part of the Lhasa terrane, South Tibet. These volcanic rocks consist of trachytes, which are characterized by high K 2 O (5.469.30 wt.%), SiO 2 (61.3468.62 wt.%) and Al 2 O 3 (15.0617.36 wt.%), and relatively low MgO (0.472.80 wt.%) and FeO t (1.704.90 wt.%). Chondrite-normalized rare earth elements (REE) patterns display clearly negative Eu anomalies. Primitive mantle-normalized incompatible trace elements diagrams exhibit strong enrichment in large ion lithophile elements (LILE) relative to high eld strength elements (HFSE) and display signicantly negative NbTaTi anomalies. Initial isotopic compositions indicate relatively radiogenic Sr [( 87 Sr/ 86 Sr) i = 0.7119780.712090)] and unradiogenic Nd [( 143 Nd/ 144 Nd) i = 0.5121210.512148]. Combined with their Pb isotopic compositions [( 206 Pb/ 204 Pb) i = 18.61518.774, ( 207 Pb/ 204 Pb) i = 15.70815.793, ( 208 Pb/ 204 Pb) i = 39.27439.355)], these data are consistent with the involve- ment of component from subducted continental crustal sediment in their source region. The whole-rock SrNdPb isotopic compositions exhibit linear trends between enriched mantle-derived mac ultrapotassic magmas and relatively depleted crustal contaminants from the Lhasa terrane. The enrichment of the upper mantle below South Tibet is considered to result from the addition of components derived from subducted Indian continental crust to depleted MORB-source mantle during northward underthrusting of the Indian continental lithosphere beneath the Lhasa terrane since IndiaAsia collision at ~55 Ma. Secondary Ion Mass Spectrometry (SIMS) UPb zircon analyses yield the eruptive ages of 10.61 ± 0.10 Ma and 10.70 ± 0.18 Ma (weighted mean ages). Zircon Hf isotope compositions [Ɛ Hf (t) = 4.79 to 0.17], combined with zircon O isotope ratios (5.517.22), imply an addition of crustal material in their petrogenesis. Clinopyroxene-liquid thermobarometer reveals pres- sure (2.54.1 kbar) and temperature (1029.41082.9 °C) of clinopyroxene crystallization, suggesting that depth of the magma chamber was 11.616.4 km. Energy-constrained assimilation and fractional crystallization (ECAFC) model calculation indicates depth of assimilation and fractional crystallization in the region of 14.4018.75 km underneath the Lhasa terrane, which is in consistent with depth of the magma chamber as suggested by clinopyroxene-liquid thermobarometer. Based on the whole-rock major and trace elements and SrNdPb isotope compositions, combined with ECAFC modeling simulations and zircon HfO isotope data, we propose that the YPVR resulted from assimilation and fractional crystallization (AFC) process of the K-rich mac primitive magmas, which were caused by partial melting of the Indian continental subduction-induced mélange rocks. © 2015 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved. Keywords: Post-collisional potassic magmatism Zircon UPb dating Assimilation and fractional crystallization (AFC) Indian mélanges South Tibet 1. Introduction During IndiaAsia collision and subsequent northward subduction of the Indian continental lithosphere, multi-stage magmatism and crustmantle interaction took place in the Lhasa terrane, South Tibet (e.g., Miller et al., 1999; Ding et al., 2003, 2006; Mo et al., 2003, 2006a, 2006b; Zhao et al., 2006, 2009; Gao et al., 2007a, 2007b, 2009, 2010; Guo et al., 2007, 2013, 2015; Wang et al., 2008, 2014, 2015; J.L. Chen et al., 2010; Chen et al., 2011, 2012; Guo and Wilson, 2012; Hou et al., 2013; Zhu et al., 2013; Jiang et al., 2014; Ma et al., 2014; Liu et al., 2015). The magmatism in continental collision settings records recycling of subducted crustal components at continental subduction zone and uplift process of the Tibetan Plateau (e.g., Chung et al., 2003, 2005, 2009; Ding et al., 2003; Hou et al., 2006, 2013; Guo et al., 2007, 2013, 2015; Zhao et al., 2009; Guo and Wilson, 2012). Post-collisional, K-rich (including ultrapotassic and potassic) magmatic rocks (25Gondwana Research 41 (2017) 928 Corresponding author at: No. 19, Beitucheng Western Road, Chaoyang District, Beijing 100029, China. Tel.: +86 10 82998393; fax: +86 10 62010846. E-mail address: [email protected] (Z. Guo). http://dx.doi.org/10.1016/j.gr.2015.11.007 1342-937X/© 2015 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved. Contents lists available at ScienceDirect Gondwana Research journal homepage: www.elsevier.com/locate/gr

Transcript of Post-collisional potassic magmatism in the eastern Lhasa ... · Tibet: Products of partial melting...

Page 1: Post-collisional potassic magmatism in the eastern Lhasa ... · Tibet: Products of partial melting of mélanges in a continental subduction channel Lihong Zhanga,b, Zhengfu Guoa,⁎,MaoliangZhanga,b,

Gondwana Research 41 (2017) 9–28

Contents lists available at ScienceDirect

Gondwana Research

j ourna l homepage: www.e lsev ie r .com/ locate /gr

Post-collisional potassic magmatism in the eastern Lhasa terrane, SouthTibet: Products of partial melting of mélanges in a continentalsubduction channel

Lihong Zhang a,b, Zhengfu Guo a,⁎, Maoliang Zhang a,b, Zhihui Cheng a,b, Yutao Sun a,b

a Key Laboratory of Cenozoic Geology and Environment, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, Chinab University of Chinese Academy of Sciences, Beijing 100049, China

⁎ Corresponding author at: No. 19, BeituchengWestern100029, China. Tel.: +86 10 82998393; fax: +86 10 6201

E-mail address: [email protected] (Z. Guo).

http://dx.doi.org/10.1016/j.gr.2015.11.0071342-937X/© 2015 International Association for Gondwa

a b s t r a c t

a r t i c l e i n f o

Article history:Received 29 May 2015Received in revised form 18 October 2015Accepted 3 November 2015Available online 23 December 2015

Post-collisional, potassic magmatic rocks widely distributed in the eastern Lhasa terrane provide significantinformation for comprehensive understanding of geodynamic processes of northward subduction of the Indianlithosphere and uplift of the Tibetan Plateau. A combined dataset of whole-rock major and trace elements,Sr–Nd–Pb isotopes, and in situ zircon U–Pb dating and Hf–O isotopic analyses are presented for the Yangyingpotassic volcanic rocks (YPVR) in the eastern part of the Lhasa terrane, South Tibet. These volcanic rocks consistof trachytes, which are characterized by high K2O (5.46–9.30 wt.%), SiO2 (61.34–68.62 wt.%) and Al2O3 (15.06–17.36 wt.%), and relatively low MgO (0.47–2.80 wt.%) and FeOt (1.70–4.90 wt.%). Chondrite-normalized rareearth elements (REE) patterns display clearly negative Eu anomalies. Primitive mantle-normalized incompatibletrace elements diagrams exhibit strong enrichment in large ion lithophile elements (LILE) relative to high fieldstrength elements (HFSE) and display significantly negative Nb–Ta–Ti anomalies. Initial isotopic compositionsindicate relatively radiogenic Sr [(87Sr/86Sr)i = 0.711978–0.712090)] and unradiogenic Nd [(143Nd/144Nd)i =0.512121–0.512148]. Combined with their Pb isotopic compositions [(206Pb/204Pb)i = 18.615–18.774,(207Pb/204Pb)i = 15.708–15.793, (208Pb/204Pb)i = 39.274–39.355)], these data are consistent with the involve-ment of component from subducted continental crustal sediment in their source region. The whole-rock Sr–Nd–Pb isotopic compositions exhibit linear trends betweenenrichedmantle-derivedmafic ultrapotassicmagmasand relatively depleted crustal contaminants from the Lhasa terrane. The enrichment of the upper mantle belowSouth Tibet is considered to result from the addition of components derived from subducted Indian continentalcrust to depleted MORB-source mantle during northward underthrusting of the Indian continental lithospherebeneath the Lhasa terrane since India–Asia collision at ~55 Ma. Secondary Ion Mass Spectrometry (SIMS) U–Pbzircon analyses yield the eruptive ages of 10.61 ± 0.10 Ma and 10.70 ± 0.18 Ma (weighted mean ages). ZirconHf isotope compositions [ƐHf(t) = −4.79 to −0.17], combined with zircon O isotope ratios (5.51–7.22‰),imply an addition of crustal material in their petrogenesis. Clinopyroxene-liquid thermobarometer reveals pres-sure (2.5–4.1 kbar) and temperature (1029.4–1082.9 °C) of clinopyroxene crystallization, suggesting that depthof the magma chamber was 11.6–16.4 km. Energy-constrained assimilation and fractional crystallization (EC–AFC) model calculation indicates depth of assimilation and fractional crystallization in the region of 14.40–18.75 km underneath the Lhasa terrane, which is in consistent with depth of the magma chamber as suggestedby clinopyroxene-liquid thermobarometer. Based on the whole-rock major and trace elements and Sr–Nd–Pbisotope compositions, combined with EC–AFC modeling simulations and zircon Hf–O isotope data, we proposethat the YPVR resulted from assimilation and fractional crystallization (AFC) process of the K-richmafic primitivemagmas, which were caused by partial melting of the Indian continental subduction-induced mélange rocks.

© 2015 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.

Keywords:Post-collisional potassic magmatismZircon U–Pb datingAssimilation and fractional crystallization (AFC)Indian mélangesSouth Tibet

1. Introduction

During India–Asia collision and subsequent northward subductionof the Indian continental lithosphere, multi-stage magmatism andcrust–mantle interaction took place in the Lhasa terrane, South Tibet(e.g., Miller et al., 1999; Ding et al., 2003, 2006; Mo et al., 2003, 2006a,

Road, ChaoyangDistrict, Beijing0846.

na Research. Published by Elsevier B.

2006b; Zhao et al., 2006, 2009; Gao et al., 2007a, 2007b, 2009, 2010;Guo et al., 2007, 2013, 2015; Wang et al., 2008, 2014, 2015; J.L. Chenet al., 2010; Chen et al., 2011, 2012; Guo and Wilson, 2012; Hou et al.,2013; Zhu et al., 2013; Jiang et al., 2014; Ma et al., 2014; Liu et al.,2015). The magmatism in continental collision settings recordsrecycling of subducted crustal components at continental subductionzone and uplift process of the Tibetan Plateau (e.g., Chung et al., 2003,2005, 2009; Ding et al., 2003; Hou et al., 2006, 2013; Guo et al., 2007,2013, 2015; Zhao et al., 2009; Guo and Wilson, 2012). Post-collisional,K-rich (including ultrapotassic and potassic) magmatic rocks (25–

V. All rights reserved.

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8 Ma) in the Lhasa terrane are thought to link to partial melting eventsassociated with deep geodynamic processes in the Himalaya–Tibetcontinent orogenic zone, such as northward subduction of the Indiancontinental lithosphere (Ding et al., 2003; Hou et al., 2006; Guo et al.,2013, 2015) and convective thinning of over-thickened Tibetan conti-nental lithosphere (e.g., Turner et al., 1996; Miller et al., 1999; Chunget al., 2003, 2005, 2009; Sun et al., 2007; Zhao et al., 2009; C.Z. Liuet al., 2011, 2014; D. Liu et al., 2014; Liu et al., 2015; Tian et al., 2012;Wang et al., 2014) and break-off of a northward subducted slab of theIndian continental lithosphere (e.g., Mahéo et al., 2002; Replumazet al., 2010, 2013, 2014). Intense controversies still remain in spite ofmany previous studies, which proposed that ultrapotassic and potassicmagmas are derived from: (1) asthenospheric mantle enriched bymaterials from subducted Indian continental lithosphere (e.g., Arnaudet al., 1992; Guo et al., 2013, 2015); and (2) enriched metasomatizedlithospheric mantle and/or mafic lower crust (e.g., Turner et al., 1996;

Fig. 1. (a) Simplified map showing distribution of the Cenozoic magmatic rocks in the Lhasa tYangying potassic volcanic field (modified from Li et al., 1992; Zhou et al., 2010).

Miller et al., 1999; Ding et al., 2003; Nomade et al., 2004; Zhao et al.,2009; J.L. Chen et al., 2010; Chen et al., 2012; Zhou et al., 2010; C.Z. Liuet al., 2011, 2014; D. Liu et al., 2011, 2014; Liu et al., 2015; Wang et al.,2014). Because these previous studies simply presented whole-rock major element, trace element and Sr–Nd–Pb isotopic data of thepotassic rocks in South Tibet, lack of detailed zircon Hf–O isotopic dataand comprehensive mineralogical and petrological data has precludedfurther understanding of the origin and evolution of these potassicmagmas.

We focus on the Yangying potassic volcanic rocks (YPVR) (Fig. 1),which have been thought to exhibit many typical outcrops ofthe post-collisional potassium-rich magmatic rocks in South Tibet (Liet al., 1992). In this study, we report new systematic dataset of whole-rock major, trace elements and Sr–Nd–Pb isotopes, in situ zircon U–Pbage and Hf–O isotopes of the YPVR, South Tibet. These data, combinedwith previously published geochemical and geophysical data, allow us

errane, South Tibet (modified from Guo et al., 2015). (b) Simplified geological map of the

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Table 1Phenocryst and groundmass mineral assemblages of the Yangying potassic volcanic rocks.

Sample no. Rock type Phenocrysts Groundmass

YY-01 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-02 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-03 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-04 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-05 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-06 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-07 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-08 Trachyte Sani + Pl + Phl Sani + Pl + Ap + Fe–TiYY-09 Trachyte Sani + Phl Sani + Pl + ApYY-10 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-11 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-12 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-13 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–TiYY-14 Trachyte Cpx + Sani + Pl + Phl Cpx + Sani + Pl + Ap + Fe–Ti

Abbreviations are as follows: Ap, apatite; Cpx, clinopyroxene; Fe–Ti, Fe–Ti oxides; Phl,phlogopite; Pl, plagioclase; Sani, sanidine.

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to develop a more robust petrogenetic model for the YPVR in SouthTibet.

2. Geological setting

Tibetan Plateau is composed of the Kunlun-Qaidam, Songpan-Ganzi,Qiangtang and Lhasa terranes fromnorth to south,whichwere integratedtogether during closure of the Tethys Oceans since the Paleozoic times(Yin and Harrison, 2000). The Lhasa and Qiangtang terranes areseparated by the Jurassic-Cretaceous Bangong-Nujiang suture (BNS),whereas the Indus-Tsangpo suture (ITS) marks the boundary betweenthe Lhasa terrane and the Himalayas (Fig. 1a; Kapp et al., 2003, 2007).Precambrian basement has been only discovered in the central andnorthern Lhasa terrane, as represented by metamorphic rocks to thewest of the Nam Lake (~750 Ma; Hu et al., 2005) and the Amdo gneiss(852Ma; Guynn et al., 2006). Paleozoic to Mesozoic sedimentary strataand Jurassic to Cretaceous volcanic rocks comprise sedimentary cover ofthe Lhasa terrane (Zhu et al., 2008).

The onset of Indian and Asian continent collision was still a contro-versial issue; estimates vary from as early as the late Cretaceous (70–65 Ma; Gnos et al., 1997; Yin and Harrison, 2000; Mo et al., 2007; Xiaet al., 2011) to the Paleocene (65–55 Ma, e.g., Ding et al., 2005; Huet al., 2012; X. Hu et al., 2015; Chung et al., 2009; J. Chen et al., 2010;Yi et al., 2011; Jiang et al., 2014; F.Y. Wu et al., 2014) or even later(55–50 Ma, e.g., Patriat and Achache, 1984; Tapponnier et al., 2001;Royden et al., 2008; Najman et al., 2010; Aitchison et al., 2011;Shellnutt et al., 2014). The India–Asia continent collision has led to exten-sivemagmatism in the Lhasa terrane, generatingwidespreadCenozoic ig-neous rocks (Fig. 1a) which are mainly classified as Gangdese batholith(e.g., Jiang et al., 1999; Dong et al., 2005, 2008; Mo et al., 2005; Wenet al., 2008; Zhu et al., 2008, 2009, 2011, 2013; Ji et al., 2009a, 2009b,2012, 2014), Linzizong volcanic rocks (e.g., Mo et al., 2005, 2006a,2006b; Lee et al., 2007, 2009, 2012), adakitic rocks (e.g., Chung et al.,2003, 2009; Hou et al., 2004, 2013; Gao et al., 2007a, 2010; Guo et al.,2007; King et al., 2007; Xu et al., 2010; Chen et al., 2011; Guan et al.,2012; Hébert et al., 2014; Jiang et al., 2014; Ma et al., 2014; L.Y. Zhanget al., 2014; Zeng et al., 2017; S. Wu et al., 2014; Y. Hu et al., 2015) andK-rich magmatic rocks (e.g., Miller et al., 1999; Williams et al., 2001,2004; Ding et al., 2003, 2006; Nomade et al., 2004; Zhao et al., 2009; J.L.Chen et al., 2010; Chen et al., 2012; Zhou et al., 2010; Guo et al., 2013,2015; C.Z. Liu et al., 2011, 2014; D. Liu et al., 2011, 2014; Liu et al., 2013,2015; Wang et al., 2008, 2014; Huang et al., 2015). Ultrapotassic and po-tassic magmatic rocks in South Tibet are found as lavas, plugs and dikeswith small volumes, which mainly crop out in near NS trending rifts tothe west of longitude 87°E while potassic lavas have only been discov-ered in two volcanic fields (Majiang and Yangying) to the east of longi-tude 87°E (Fig. 1a).

Yangying volcanic field is located at central segment of the NE–SWtrending Yadong-Gulu rift, about 80 km west of Lhasa (Fig. 1b). YPVRmainly consist of trachytes which cover an area less than 10 km2.These lavas are controlled by NS trending high-angle normal faultsand crop out as the lava flow and domewhich are cut by PujiemuValley,Nangzeng Valley and Qialagai Valley from south to north (Fig. 1b; Liet al., 1992, 1994). High-temperature hydrothermal activities (e.g., hotsprings, soil microseepage) are pervasive around the Yangying volcanicfield (Li et al., 1994). Volatiles and volcanic gases from high-temperature hydrothermal systems in the Yangying volcanic fieldmight be related with shallow magmatic heat source, similar to thosefrom Yangbajing geothermal field ~30 km north of Yangying (Zhaoet al., 1993; Brown et al., 1996; Nelson et al., 1996; Liao and Zhao,1999;Wei et al., 2001). Recent studies show that total soilmicroseepageCO2 flux (~4.43 × 104 t a−1; Guo et al., 2014b) of the Yangying volcanicfield is comparable to that (~8.59 × 104 t a−1; L.H. Zhang et al., 2014) ofthe Yangbajing geothermal field with well-developed geothermal ener-gy, suggesting considerable potentiality for geothermal power genera-tion in the Yangying volcanic field, South Tibet.

3. Petrography

Fourteen samples were collected for analyses from the Yangyingvolcanic field (Fig. 1b). The analyzed samples have porphyritic texturesand most phenocrysts with size ranging from 1 to 5 mm. Phenocrystminerals consist of clinopyroxene, alkali feldspar, plagioclase and phlog-opite scattered in the groundmass composed of feldspar, clinopyroxene,apatite and Fe–Ti oxides (Table 1 and Fig. 2). The clinopyroxene crystalsare mostly euhedral (Fig. 2a). Almost all the plagioclase phenocrystshave reaction rims of alkali feldspars (Fig. 2). Phlogopite phenocrystsare characterized by altered and oxidized dark rims of Fe–Ti oxides(Fig. 2e and f).

4. Analytical methods

4.1. Whole-rock elemental and Sr–Nd–Pb isotopic analyses

All samples from Yangying potassic volcanic field (Fig. 1b) wereanalyzed for their major and trace elements and Sr–Nd–Pb isotopiccompositions at Beijing Research Institute of Uranium Geology (BRIUG).FeO concentrations were obtained by KMnO4 titration. Sample powdersfor trace elements analyses were digested with mixed HNO3 + HF acidin steel-bomb coated Teflon beakers to assure the complete dissolutionof refractory minerals. The trace elements were measured using aFinnigan Element II ICP–MS at the BRIUG following the proceduresdescribed by Li (1997). The analytical precisions for trace elementswere between 5% and 10% depending on the concentration level ofa specific element. The major and trace element analytical data arepresented in Table S1 in the Supplementary data.

Sr–Nd–Pb isotopes were determined by an Isoprobe-T thermal ioni-zationmass spectrometry (TIMS) at the BRIUG following the proceduresof GB/T17672-1999. Powder samples were mixed for isotope dilutionand dissolved using HF + HNO3 + HClO4 in sealed Teflon capsules ona hot plate for 24 h. After the separation of the Rb, Sr and light REE ina cation-exchange column, the Sm and Nd were further purified usinga cation-exchange column, conditioned and eluted with dilute HCl.The isotopic mass fractions were normalized to 143Nd/144Nd = 0.7219and 87Sr/86Sr = 0.1194, respectively. Repeated analyses of the86Sr/88Sr ratio of the standard NBS987 and 146Nd/144Nd ratio of thestandard SHINESTU gave 0.710250 ± 0.000007 (2σ) and 0.512118 ±0.000003 (2σ), respectively. Total chemical blanks were b200 pgfor strontium and b50 pg for neodymium (X. Zhao et al., 2014). Theanalytical precision for Rb/Sr and Sm/Nd ratios were below 1%. For Pbisotope measurements, Pb was separated from the silicate matrix andpurified using AG1 × 8 anionic ion-exchange columns with dilute HBras eluant. During the period of analyses repeat analyses of the interna-tional standard NBS981 yielded 204Pb/206Pb = 0.0591107 ± 0.000002;

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Fig. 2. Representativemicrophotographs of the YPVR (cross-polarized). (a) Euhedral clinopyroxene phenocrysts. (b) Euhedral plagioclase and sanidine phenocrysts. (c) Sanidine showingthin reaction rim of alkali feldspar. (d) Plagioclase showing thin rim of alkali feldspar. (e) Altered phlogopite phenocrysts. (f) Corroded sanidine and phlogopite phenocrysts. Abbreviationsare as follows: Ap, apatite; Cpx, clinopyroxene; Phl, phlogopite; Pl, plagioclase; Sani, sanidine.

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207Pb/206Pb = 0.914338 ± 0.00007; 208Pb/206Pb = 2.164940 ±0.000015. Pb isotope fractionations were corrected using correctionfactors from the certified values of the international standard NBS981.The analytical precision for Pb isotopic ratios was below 0.05%. The Sr,Nd and Pb isotopic data are presented in Table S2 in the Supplementarydata.

4.2. Zircon U–Pb dating

Zircon U–Pb dating, together with pre-analytical prepared work,was achieved at the Institute of Geology and Geophysics, ChineseAcademy of Sciences (IGGCAS), Beijing. The pre-analytical preparationscontain the following two parts: (1) zircon grains were separated usingheavy-liquid and magnetic techniques and then they were mounted inepoxy resin and polished for analyses; (2) transmitted, reflected lightimages and cathodoluminescence (CL) images of the zircon wereobtained. Cathodoluminescence images were used to check the internalstructures of individual zircon grains and to select positions for analyses(Fig. 6a and b).

U and Pb isotopes were measured using Cameca IMS-1280 SIMS.The O2− primary ion beamwas accelerated at ~13 kV, with an intensityof ca. 10 nA and the ellipsoidal spot is about 20 μm × 30 μm. Positivesecondary ions use a 60 eV energy window and a mass resolution of~5400. Each measurement consists of 40 cycles, and the total analyticaltime is 12 min. Analytical procedures are described in details (Li et al.,2009, 2012; Balintoni et al., 2011; Dan et al., 2012, 2016; Eyal et al.,2014; Wang et al., 2015). Zircon U–Pb isotopic data are presented inTable S3 in the Supplementary data.

4.3. Zircon Hf–O isotopic analyses

Zircon oxygen isotopes were measured using Cameca IMS-1280 atthe IGGCAS. The Cs+ primary ion beam was accelerated at 10 kV withintensity of ca. 2 nA and rastered over a 10 μmareawith a spot diameterof 20 μm. Oxygen isotopes were measured in multi-collector modeusing two off axis Faraday cups. The internal precision of single analyseswas generally better than 0.2 ‰ for 18O/16O ratio. The instrumentalmass fractionation factor (IMF) was corrected using 91,500 zircon

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standard with (δ18O)VSMOW = 9.9‰ (Wiedenbeck et al., 2004). Mea-sured 18O/16O was normalized by using VSMOW (Vienna StandardMean Ocean Water) compositions, and then corrected for the instru-mentalmass fractionation factor. The working conditions and analyticalprocedures have been described in details (Li et al., 2009; Su et al., 2011;

Table 2Zircon Hf–O isotope data of the Yangying potassic volcanic rocks.

Sample t (Ma) 176Yb/177Hf 176Lu/177Hf 176Hf/177Hf ± 2σ

YY-08-01 10.0 0.005357 0.000203 0.282705 0.000015YY-08-02 62.9 0.040641 0.001667 0.282900 0.000016YY-08-03 10.6 0.007239 0.000272 0.282730 0.000017YY-08-04 10.9 0.005083 0.000194 0.282699 0.000016YY-08-05 10.9 0.007185 0.000263 0.282729 0.000022YY-08-06 63.5 0.072463 0.002993 0.282896 0.000026YY-08-07 10.3YY-08-08 10.4 0.009920 0.000394 0.282681 0.000014YY-08-09 10.5 0.014747 0.000526 0.282711 0.000020YY-08-10 10.3YY-08-11 10.3 0.028974 0.001027 0.282681 0.000018YY-08-12 10.6 0.025624 0.000929 0.282704 0.000017YY-08-13 10.5 0.032422 0.001144 0.282695 0.000019YY-08-14 59.2 0.048940 0.001882 0.282922 0.000021YY-08-15 10.9YY-08-16 10.5 0.011925 0.000489 0.282698 0.000014YY-08-17 10.9 0.008937 0.000325 0.282707 0.000015YY-08-18 10.3 0.016233 0.000594 0.282702 0.000018YY-08-19 65.4YY-08-20 62.9 0.066980 0.002635 0.282871 0.000017YY-08-21 10.1 0.008673 0.000324 0.282754 0.000025YY-08-22 9.9 0.013494 0.000490 0.282687 0.000018YY-08-23 10.9 0.019257 0.000676 0.282647 0.000015YY-08-24 11.0 0.006092 0.000226 0.282686 0.000018YY-08-25 67.0 0.040666 0.001570 0.282974 0.000304YY-08-26 10.2 0.011021 0.000405 0.282752 0.000021YY-08-27 10.8 0.015357 0.000569 0.282735 0.000019YY-08-28 10.2 0.013133 0.000483 0.282704 0.000017YY-08-29 10.5 0.009313 0.000351 0.282702 0.000015YY-12-01 10.9 0.017196 0.000618 0.282694 0.000019YY-12-02 10.8 0.004635 0.000177 0.282710 0.000016YY-12-03 61.1 0.076558 0.003048 0.282944 0.000018YY-12-04 10.6 0.049378 0.001679 0.282704 0.000017YY-12-05 10.5YY-12-06 37.5 0.059471 0.002473 0.282951 0.000016YY-12-07 63.2 0.026749 0.001078 0.282850 0.000014YY-12-08 10.5 0.008267 0.000305 0.282692 0.000015YY-12-09 63.3 0.035398 0.001460 0.282905 0.000013YY-12-10 9.6 0.016490 0.000595 0.282698 0.000018YY-12-11 10.7 0.051714 0.001778 0.282680 0.000017YY-12-12 10.5 0.037633 0.001318 0.282774 0.000022YY-12-13 10.7 0.019032 0.000681 0.282673 0.000022YY-12-14 58.7 0.034657 0.001429 0.282933 0.000015YY-12-15 10.2 0.009032 0.000328 0.282700 0.000022YY-12-16 10.2 0.011190 0.000417 0.282643 0.000016

Initial 176Lu/177Hf and 176Hf/177Hf ratios and εHf(t) (the parts in 104 deviation of initial Hf isotowith the reference to the chondritic uniform reservoir (CHUR) at the time of zircon growth froThe ratios of (176Lu/177Hf)CHUR= 0.0336 and (176Hf/177Hf)CHUR= 0.282785 (Bouvier et al., 200mantle model ages (TDM) were calculated with reference to depleted mantle at a present-day 1

hafnium isotopic “crustal”model ages (TDM C)were also calculated for each zircon grain by assum176Lu/177Hf = 0.015, that originated from the depleted mantle source (Griffin et al., 2002). The

εHf 0ð Þ ¼

176Hf

.177Hf Þ

� �Sample

176Hf.

177Hf Þ

� �CHUR

−1

26664

37775� 104; εHf tð Þ ¼

176Hf

.177Hf Þ

� �Sample

− 176Lu

.177Hf Þ

� �

176Hf.

177Hf Þ

� �CHUR

− 176 Lu�

177Hf Þ� �

C

26664

TDM ¼ 1�λ � ln 1þ

176Hf

.177Hf Þ

� �Sample

− 176Lu

.177Hf Þ

� �DM

176Hf.

177Hf Þ

� �Sample

− 176 Lu�

177Hf Þ� �

DM

8>>><>>>:

9>>>=>>>;; TC

DM ¼ TDM− TDM−tð Þ � f

f Sample ¼176Lu

.177Hf Þ

� �Sample

176 Lu�

177Hf Þ� �

CHUR

−1; f MC ¼176Lu

.177Hf Þ

� �MC

176 Lu�

177Hf Þ� �

CHUR

−1; f DM ¼176Lu

.177Hf Þ

� �DM

176 Lu�

177Hf Þ� �

CHUR

−1

t, crystallization time of zircon; 206Pb/238U ages were used for zircons younger than 1000 Ma.

Dan et al., 2012, 2016; Wang et al., 2015). Zircon oxygen isotopic dataare listed in Table 2.

Lu–Hf isotopes were measured using laser-ablation multi-collectorinductively coupled plasma mass spectrometry (LA–ICP–MS) at theIGGCAS. Lu–Hf isotopic analyseswere obtained on the same zircon grains

ƐHf(t) ƐHf(0) TDM(Ma) TDMC (Ma) fSample δ18O (‰)

−2.59 −2.81 758 1231 −0.99 6.475.41 4.08 507 761 −0.95 6.35

−1.72 −1.95 726 1176 −0.99 6.13−2.79 −3.03 767 1245 −0.99 6.19−1.76 −1.99 727 1179 −0.99 6.69

5.21 3.92 533 774 −0.91 5.656.86

−3.45 −3.68 796 1287 −0.99 7.16−2.39 −2.62 757 1219 −0.98 6.75

6.67−3.45 −3.67 809 1286 −0.97 6.51−2.63 −2.85 774 1234 −0.97 6.63−2.95 −3.17 792 1254 −0.97 6.41

6.07 4.83 480 715 −0.94 5.606.21

−2.85 −3.08 775 1248 −0.99 5.51−2.54 −2.78 759 1228 −0.99 6.61−2.73 −2.95 771 1240 −0.98 6.62

5.664.31 3.03 565 831 −0.92 5.62

−0.88 −1.10 693 1122 −0.99 6.50−3.27 −3.48 790 1274 −0.99 6.54−4.64 −4.87 849 1362 −0.98 6.66−3.26 −3.51 786 1275 −0.99 7.22

8.11 6.69 399 590 −0.95 5.82−0.94 −1.16 697 1126 −0.99 6.32−1.52 −1.76 724 1163 −0.98 6.19−2.65 −2.87 766 1235 −0.99 6.27−2.71 −2.94 766 1239 −0.99 6.18−3.00 −3.23 783 1258 −0.98 6.02−2.42 −2.65 751 1221 −0.99 6.13

6.86 5.62 462 666 −0.91 5.71−2.65 −2.87 791 1235 −0.95 5.96

6.446.65 5.87 444 661 −0.93 5.533.65 2.29 571 873 −0.97 6.27

−3.05 −3.28 779 1261 −0.99 6.595.59 4.24 498 749 −0.96 5.76

−2.85 −3.06 776 1248 −0.98 6.53−3.47 −3.70 827 1288 −0.95 6.34−0.17 −0.39 683 1077 −0.96 6.60−3.73 −3.96 813 1304 −0.98 6.15

6.47 5.23 458 689 −0.96 5.77−2.77 −2.99 768 1243 −0.99 6.41−4.79 −5.01 849 1371 −0.99 6.46

pe ratios between the zircon sample and the chondritic reservoir) values were calculatedm magmas. The 176Lu decay constant was 1.867 × 10−11 year−1 (Söderlund et al., 2004).8), (176Lu/177Hf)DM= 0.0384 (Griffin et al., 2000) were also shown. And then the depleted76Hf/177Hf ratio of 0.28325 similar to that of the average MORB (Nowell et al., 1998). Theing its parentalmagma tohave been derived fromanaverage continental crust (MC),withcalculation formulas used in Table 2 are presented below.

Sample� eλt−1� �

HUR� eλt−1ð Þ

−1

37775� 104;

MC− f Sample

f MC− f DM

;

Page 6: Post-collisional potassic magmatism in the eastern Lhasa ... · Tibet: Products of partial melting of mélanges in a continental subduction channel Lihong Zhanga,b, Zhengfu Guoa,⁎,MaoliangZhanga,b,

Fig. 3. (a) K2O+Na2O (wt.%) vs. SiO2 (wt.%) for the YPVR and other K-rich volcanic rocksof the Lhasa terrane. All data plotted have been recalculated to 100 wt.% on a volatile-freebasis. Classification boundaries are from Le Bas et al. (1986) and Le Maitre et al. (1989).Filled and open symbols represent, respectively, data from this study and the publishedliteratures of Miller et al. (1999); Williams et al. (2001, 2004); Ding et al. (2003, 2006);Jiang (2003); Jiang et al. (2003); Gao et al. (2007a, 2009); Sun et al. (2007); Wang et al.(2008, 2014); Zhao et al. (2009); Chen et al. (2012); J.L. Chen et al. (2010); Tian et al.(2012); Guo et al. (2013); D. Liu et al. (2011, 2014) and reference therein. Rock typesshown by letters are as follows: S2, basaltic trachyandesite; S3, trachyandesite; T,trachyte; R, rhyolite; U3, tephriphonolite; Ph, phonolite; O1, basaltic andesite; O2,andesite; O3, dacite. (b) K2O (wt.%) vs. SiO2 (wt.%) diagram for same samples as plottedin (a). The dividing lines show the classification boundaries from Rickwood (1989).

14 L. Zhang et al. / Gondwana Research 41 (2017) 9–28

thatwere previously analyzed forU–Pb andO isotopes,with ablation pitsof 40–80 μmindiameter, ablation time of 26 s and repetition rate of 8Hz.The detailed analytical procedures are described in Li et al. (2010) andWang et al. (2015). Zircon Hf isotopic data are presented in Table 2.

4.4. Mineral compositional analyses

The compositions of phenocryst minerals of the YPVR weredetermined using a JEOL JXA-8100 electron microprobe at the IGGCAS.Analytical conditions include an accelerating voltage of 15 kV, beamcurrent of 2 × 10−8 A, a spot diameter of 5 μm for clinopyroxene, phlog-opite and feldspar. The analytical procedures are described in details(Cheng and Kusky, 2007; Tam et al., 2011; H. Xu et al., 2015). The bulkcompositions of phenocryst minerals are presented in Tables S4, S5and S6 in the Supplementary data.

5. Results

5.1. Whole-rock major, trace elements and Sr–Nd–Pb isotopes

Samples of the YPVR are all plotted in the field of trachyte (Fig. 3a),which have relatively high SiO2 (61.34–68.62 wt.%), K2O (5.46–9.30 wt.%), Al2O3 (15.06–17.36 wt.%), low MgO (0.47–2.80 wt.%) andFeOt (1.70–4.90 wt.%) contents (Table S1 in the Supplementary data).These trachytes are potassic (K2O/Na2O N 1) according to the criteriaproposed by Nelson (1992) and mainly lie in the shoshonitic series(Fig. 3b) with the exception of sample YY-09 which might be alteredin the hydrothermal field (Li et al., 1992). MgO, FeOt, CaO decreasewith increasing SiO2 in Harker diagrams (not shown), indicatingfractional crystallization of clinopyroxene and plagioclase. Negativecorrelation between SiO2 and TiO2 (or P2O5) might be interpreted asthe fractional crystallization of Fe–Ti oxides and apatite. Al2O3 firstlyincreases and then decreases with increasing SiO2, implying removalof feldspar from magma during low-pressure fractional crystallization.

The chondrite-normalized rare earth elements (REE) patterns of theYPVR are characterized by enrichment of LREE and distinctive negativeEu anomalies (δEu = 0.55–0.68; Table S1 in the Supplementary dataand Fig. 4a), which can be explained by fractional crystallization ofplagioclase. Primitive mantle-normalized incompatible trace elementsdiagrams of the studied rocks show positive anomalies for large ionlithosphile element (LILE, e.g., K, Ba and Rb; Fig. 4b) and significantlynegative anomalies for high field strength elements (HFSE, e.g., Nb, Taand Ti; Fig. 4b).

The studied YPVR have relatively radiogenic initial Sr isotopic com-position [(87Sr/86Sr)i = (0.711978–0.712090)] and unradiogenic initialNd isotopic composition [(143Nd/144Nd)i = (0.512121–0.512148)](Table S2 in the Supplementary data), which differs from Sr–Nd isotopiccompositions of theGangdese batholith, adakites and Linzizong volcanicrocks (Fig. 5a). The YPVR are characterized by fairly radiogenic Pb isotopicsignatures [(206Pb/204Pb)i = (18.615–18.774), (207Pb/204Pb)i = (15.708–15.793), (208Pb/204Pb)i = (39.274–39.355)](Table S2 in the Supple-mentary data), which are plotted above the North HemisphereReference Line (NHRL; Hart, 1984) as shown in Fig. 5b–e, suggestingenriched source for the Yangying potassic magma.

5.2. Zircon U–Pb geochronology

As shown in cathodoluminescence (CL) images (Fig. 6a and b),zircons for U–Pb dating from samples YY-08 and YY-12 are mostlyeuhedral and display long to short prismatic shapes with crystal lengthsof about 50–250 μm,which could bedivided into twogroups: (1)Group1is composed of magmatic zircons exhibiting weak oscillatory zoning anduniform internal texture (Corfu et al., 2003; Hoskin and Schaltegger,2003). Most of these zircons have Th/U ratios higher than 1 (1.1–4.3;Table S3 in the Supplementary data), in consistent with those of mag-matic zircons (N0.5; Hoskin and Schaltegger, 2003); and (2) Group 2

represents zircon xenocrysts or inherited core with lower Th/U ratios(0.23–0.83) that were captured during evolution of the Yangyingpotassic magma, suggesting potential crustal materials involved in theYangying magma generation. In situ zircon U–Pb age of the Group 1zircons could be interpreted as crystallization age of the YPVR (Wuet al., 2007; Chiu et al., 2009).

Magmatic zircons from sample YY-08 are coeval and yield a lowerintercept age of 10.62 ± 0.10 Ma (MSWD = 0.88) and a weightedmean 206Pb/238U age of 10.61 ± 0.10 Ma (MSWD = 0.88) in the Tera-Wasserburg U–Pb concordia diagram (Fig. 6c). Five zircon grains with

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Fig. 4. (a) Chondrite-normalized rare earth element diagram of the YPVR. (b) Primitivemantle-normalized incompatible trace element patterns of the YPVR. Normalizationfactors are from Sun and McDonough (1989). Data for the average composition ofsubduction channel mélange rocks are from Marschall and Schumacher (2012) andreferences therein. Data sources of the potassic and ultrapotassic rocks in the Lhasaterrane are as in Fig. 3.

15L. Zhang et al. / Gondwana Research 41 (2017) 9–28

U–Pb ages ranging from 63 to 67.4 Ma are interpreted as xenocrysticcrystals which represent contaminants added to the Yangyingmagmas.Eleven analyses of magmatic zircons from sample YY-12 yields a lowerintercept age of 10.72 ± 0.14 Ma (MSWD= 1.3) and a weighted mean206Pb/238U age of 10.70 ± 0.18 Ma (MSWD = 1.3) (Fig. 6d), in consis-tent with crystallization age of sample YY-08. U–Pb ages of zirconxenocrysts range from 58.7 to 67 Ma (Table S3 in the Supplementarydata). In situ zircon U–Pb ages for the YPVR in this study are consistentwith previously published age data using K–Ar and Ar–Ar datingmethods (10.83 ± 0.27 Ma, 10.84 ± 0.17 Ma; Li et al., 1992; Zhouet al., 2010). Furthermore, potassicmagmatism in the Yangying volcanicfield is coeval with the late stage of the ultrapotassic magmatism in thewestern Lhasa terrane (25–8Ma; e.g., Miller et al., 1999;Williams et al.,2001, 2004; Ding et al., 2003; Zhao et al., 2009; J.L. Chen et al., 2010;Chen et al., 2012; Guo et al., 2013).

5.3. Zircon Hf–O isotopes

In situ zircon Hf–O isotopic data were analyzed for 45 zircongrains (samples YY-08 and YY-12) that have been previously dated bySIMS. Magmatic zircons exhibit relatively uniform 176Hf/177Hf ratios(0.282647–0.282774) and negative ƐHf(t) values (−4.79 to −0.17). Incontrast, xenocrystic zircons have relatively variable 176Hf/177Hf ratios(0.282850–0.282996) and positive ƐHf(t) values (3.65–8.11). The δ18Ovalues of the magmatic zircons range from 5.51‰ to 7.22‰ andxenocrystic zircons have similar δ18O value (5.62–6.57‰), which are

slightly higher than those of mantle zircons (δ18O = 5.3 ± 0.3‰;Valley, 2003).

5.4. Mineral chemistry

Clinopyroxene is ubiquitous and the most abundant phase occurredboth as phenocryst and groundmass in the YPVR (Fig. 2a), and plottedin the fields of augite and endiopside (Fig. 7a). These clinopyroxenephenocrysts are characterized by relatively low AlVI/AlIV (0.5–4), Ti/Al(0.091–0.25) ratios, and lowAl (b0.2 apfu) andNa (b0.05 apfu) contents(Table S6 in the Supplementary data), suggesting the crystallization ofthe clinopyroxene occurring at low pressure situation (b10 × 103 bar;Dobosi and Fodor, 1992; Haase et al., 1996; Seyler and Bonatti, 1994;McCarthy and PatiÑO Douce, 1998). Meanwhile, the AlVI/AlIV ratioshave relatively broad ranges, suggesting the AlVI of clinopyroxenecrystallizing much deeper than that of AlVI beneath the Lhasa terranecrust and the changing depth of clinopyroxene crystallization.

Alkali feldspar and plagioclase are themost commonminerals in theYPVR (Fig. 2). The plagioclases (An30–39) are plotted within the fields ofandesine and K-andesine in An–Ab–Or diagram (Fig. 7b), while all thealkali feldspars have relatively uniform end-member values (Or38–54Ab45–59 An3–10) (Fig. 7b), including euhedral alkali feldspar phenocrysts(Fig. 2b and f), cores and rims of overgrowth alkali feldspars (Fig. 2a, c–e).

Phlogopite phenocrysts are very common in the South Tibetanpotassic and ultrapotassic magmatic rocks. All analyzed phlogopites inthe YPVR are plotted within the field of ultrapotassic magmatic rocksin the Lhasa terrane (Fig. 7c). Moreover, the analyzed phlogopitephenocrysts are characterized by high-Ti (TiO2 = 5.55–7.93 wt.%), lowMgO (15.46–18.60 wt.%) and low K2O (7.52–8.44 wt.%) (Table S4 inthe Supplementary data), which resemble cores of phlogopite inultrapotassic rocks in the Lhasa terrane (Miller et al., 1999; Gao et al.,2007b), suggesting a genetic relation between the YPVR andultrapotassicmagmas in South Tibet.

6. Discussion

6.1. Origin of YPVR and the relationships between the ultrapotassic andpotassic magmas in the Lhasa terrane

The YPVR have different geochemical characteristics (i.e., whole-rock major elements, trace elements and Sr–Nd–Pb isotope ratios)from those of Miocene mantle-derived ultrapotassic magmatic rocksin the Lhasa terrane (e.g., Miller et al., 1999; Zhao et al., 2009; Guoet al., 2013, 2015; D. Liu et al., 2014; Liu et al., 2015) and of Mioceneadakitic rocks derived by partial melting of thickened lower crust inSouth Tibet (e.g., Chung et al., 2003, 2009; Gao et al., 2007a; Guo et al.,2007; Chen et al., 2011; Li et al., 2011; Hou et al., 2013) (Figs. 3–5).The YPVR are mainly characterized by high SiO2 (61.34–64.48 wt.%),low MgO (0.84–2.80 wt.%), FeOt (3.70–4.91 wt.%) and low contents ofCr (53.1–79.2 ppm) and Ni (27.2–36.4 ppm) and other compatibleelements (Table S1 in the Supplementary data), implying that theymight result from either partial melting of the mafic lower crust orassimilation and fractional crystallization (AFC) of mantle-derivedprimitive melts.

The negative Eu anomalies (δEu = 0.55–0.68) in Chondrite-normalized REE patterns of the YPVR (Fig. 4a) indicate fractionalcrystallization of plagioclase, which differs from lower crust-derivedadakitic rocks with positive or no Eu anomalies in the Lhasa terrane(e.g., Guo et al., 2007; Chen et al., 2011). Furthermore, the YPVR arecharacterized by relatively higher (87Sr/86Sr)i, (207Pb/204Pb)i, (208Pb/204Pb)i, (206Pb/204Pb)i and lower (143Nd/144Nd)i relative to those ofadakitic rocks in the Lhasa terrane (Fig. 5), indicating different magmasources for potassic and adakitic rocks which questions the hypothesisthat potassic magma of the Lhasa terrane originated from the maficlower crust (e.g., J.L. Chen et al., 2010; D. Liu et al., 2014).

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Fig. 5. (a) (143Nd/144Nd)i vs. (87Sr/86Sr)i. (b) (87Sr/86Sr)i vs. (206Pb/204Pb)i. (c) (143Nd/144Nd)i vs. (206Pb/204Pb)i. (d) (207Pb/204Pb)i vs. (206Pb/204Pb)i. (e) (208Pb/204Pb)i vs. (206Pb/204Pb)i.Lower continental crust (LCC) and upper continental crust (UCC) are from Zartman and Haines (1988). Data for the average composition of subduction channel mélange rocks arecalculated from Bulle et al. (2010). The GLOSS (Global Subducting Sediment; Plank and Langmuir, 1998), NHRL (Northern Hemisphere Reference Line; Hart, 1984), EMI and EMII(enriched mantle end-members; Zindler and Hart, 1986; Hofmann, 1997; Zou et al., 2000), and MORB and OIB fields (Wilson, 1989; Hofmann, 1997) are shown for comparison. Thepotassic and ultrapotassic rocks from North Tibet are from Turner et al. (1993, 1996), Deng (1998); Liu (1999); Ding et al. (2003, 2007), Guo et al. (2006) and references therein. Datafor the Higher Himalayan Crystalline Sequence (HHCS) are from Allègre and Ben Othman (1980); Vidal et al. (1982, 1984); Deniel et al. (1987); Inger and Harris (1993); Parrish andHodges (1996); Harrison et al. (1999); Whittington et al. (1999); Ahmad et al. (2000); Robinson et al. (2001); Richards et al. (2005); Guo and Wilson (2012) and references therein.Compositions of the Gangdese batholith in the Lhasa terrane are from Jiang et al. (1999); Dong et al. (2008); and Z.D. Zhao et al. (2011). Linzizong volcanic rocks in Lhasa terrane arefrom Dong (2002) and Zhang (1996) and Lee et al. (2007, 2009, 2012). Adakitic rocks in Lhasa terrane are from Guo et al. (2007); Chen et al. (2011); Hou et al. (2004, 2013) andreferences therein. Lower crust in South Tibet is from Miller et al. (1999). Data sources of the potassic and ultrapotassic rocks in the Lhasa terrane are as in Fig. 3.

16 L. Zhang et al. / Gondwana Research 41 (2017) 9–28

Compared with ultrapotassic magmatic rocks with MgO ≥ 6 wt.%from the Lhasa terrane, the bulk potassic magmatic rocks (includingthe YPVR) display slightly lower (87Sr/86Sr)i and higher (143Nd/144Nd)iratios, and moreover the potassic rocks plot in linear trends betweenmantle-derived mafic ultrapotassic magmas and relatively depletedcrustal contaminants from the Lhasa terrane (Fig. 5), suggesting closelinks with ultrapotassic magmas and the relatively depleted crustal

contaminants. The YPVR have lower contents of LILE (e.g., Rb, Ba, Sr)and LREE than those of the ultrapotassic rocks in the Lhasa terrane(Fig. 4), indicating that only fractional crystallization of the ultrapotassicmagmas could not account for geochemical characteristics of the YPVRand crustal contaminant must be involved. Additionally, the maficultrapotassic rocks (MgO ≥ 6 wt.%) in the Lhasa terrane have extremelyhigh (87Sr/86Sr)i (0.7117–0.7393), (206Pb/204Pb)i (18.284–18.965),

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17L. Zhang et al. / Gondwana Research 41 (2017) 9–28

(207Pb/204Pb)i (15.660–15.839) and (208Pb/204Pb)i (39.092–40.025)ratios and low (143Nd/144Nd)i (0.5117–0.5212) ratios (e.g., Milleret al., 1999; Williams et al., 2001, 2004; Liao et al., 2002; Jiang, 2003;Gao et al., 2007b; Zhao et al., 2009; Ding et al., 2006; Chen et al., 2012;Tian et al., 2012; Guo et al., 2013), further enriched relative to thewhole-rock continental crust (Fig. 5; Zartman and Haines, 1988).Hence, ultrapotassic and potassic magmatic rocks including the YPVRdisplay a positive correlation between (143Nd/144Nd)i and SiO2

Fig. 6.Cathodoluminescence (CL) images of zircons of theYPVR samples YY08 (a) andYY12 (b).zircons. Solid circles and dashed ellipses indicate the locations of in situ U–Pb dating (yellow–da(yellow number), Hf isotopic values (green number) and O isotopic values (white number) anspot. Tera-Wasserburg diagrams (lower intercept age) and weighted-mean age diagrams (2

(e) Zircon δ18O vs. ƐHf(t) for the YPVR. (f) Zircon ƐHf(t) vs. U–Pb age for the YPVR, GangdeseHf isotope and U–Pb ages of Gangdese batholith, adakitic rocks and Linzizong volcanic rock(2009b, 2012) and Hou et al. (2013).

(Fig. 8a), whichmight be interpreted as assimilation of the ultrapotassicmagma by crustal materials during fractional crystallization.

Albeit with broader ranges of (87Sr/86Sr)i and SiO2 for ultrapotassicand potassic magmatic rocks (Fig. 8b), their correlations might beexplained by AFC processes of ultrapotassic magma involving variablecrustal contaminants (from an enriched one to a depleted one)(DePaolo, 1981; Handley et al., 2010), giving rise to potassic magmawith higher SiO2 (51.41–76.30 wt.%) and broad (87Sr/86Sr)i (0.710749–

Cathodoluminescence (CL) images are taken for inspecting internal structures of individualshed ellipses) andHf–O isotope analyses (green—solid circles), respectively. TheU–Pb agesd the grain numbers for measured zircon (blue number) are also shown for each analyses06Pb/238U age) of zircons from the YPVR are shown for samples YY08 (c) and YY12 (d).batholith, adakitic rocks and Linzizong volcanic rocks from the Lhasa terrane. The Zircons from Lhasa terrane are from Lee et al. (2007, 2009, 2012); Wen et al. (2008); Ji et al.

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Fig. 6 (continued).

18 L. Zhang et al. / Gondwana Research 41 (2017) 9–28

0.737638). Therefore, we suggest that the YPVRmight result from assim-ilation and fractional crystallization of the mantle-derived ultrapotassicmagma involving depleted crustal contaminant with lower (87Sr/86Sr)iand higher (143Nd/144Nd)i in the Lhasa terrane. The processes responsi-ble for evolution of the Yangying potassic magmas will be discussed indetail below based on energy-constrained assimilation and fractionalcrystallization (EC–AFC) model.

6.2. Petrogenesis of the ultrapotassic magmatic rocks in the Lhasa terrane

Convective thinning of the over-thickened Tibetan lithosphere(e.g., Miller et al., 1999; Williams et al., 2001; Zhao et al., 2009; D. Liuet al., 2014) has been proposed to explain the genesis of the post-collisional K-rich magmatic rocks in South Tibet. However, this modelmight be ineffective to account for E–W trending linear distribution ofultrapotassic and potassic rocks in the Lhasa terrane and youngingtrend of the K-rich magmatism from north to south (Ding et al., 2003;Nomade et al., 2004; Guo et al., 2013). Although break-off of the north-ward subducted Indian continental lithosphere (e.g., Mahéo et al., 2002;Replumaz et al., 2010, 2013, 2014) can explain the E–W trending K-richmagmatic belt in the Lhasa terrane, it is inconsistentwith the southwardyounging trend and systematic variations onproportions ofmetasomaticcomponents added to the mantle source of the K-rich magmatic rocksfrom Xuruco lake–Dangre Yongcuo lake rift in the central Lhasa terrane(Guo et al., 2013). Considering the temporal, spatial and compositionalvariations of the post-collisional K-rich magmas in the Lhasa terrane,rollback and breakoff of northward subducted Indian slab mightbe reasonable geodynamic mechanism responsible for the post-collisional K-rich volcanism (Guo et al., 2013, 2015), which is supportedby Cenozoic plate motion reconstruction of Indian and Asian plates and

geodynamic modeling for subduction kinetics (Lee and Lawver, 1995;Mahéo et al., 2002; Husson et al., 2012). Partial melting of previouslyenriched mantle wedge induced by decompression and hot astheno-spheric corner flow during rollback of northward subducted Indianslab would gave rise to formation of the post-collisional K-richmagmas(Guo et al., 2013). However, the nature of enriched component added tomantle source of the K-rich magmas remains a matter of heated debate(Miller et al., 1999; Gao et al., 2007b; Guo et al., 2013).

Previous studies (e.g., Gao et al., 2007b) have focused on the role ofsubducted sediments from the Neo-Tethyan oceanic lithosphere inenrichment of the mantle source. However, the low (207Pb/204Pb)i and(208Pb/204Pb)i ratios of the Neo-Tethyan oceanic subducted sedimentscannot account for the extremely high (87Sr/86Sr)i, (206Pb/204Pb)i,(207Pb/204Pb)i and (208Pb/204Pb)i ratios and low (143Nd/144Nd)i ratiosof the ultrapotassic rocks in South Tibet (Fig. 5; Zhao et al., 2009).Whole-rock Sr–Nd–Pb isotopic compositions exhibit linear trendsbetween depleted MORB-sourcemantle (DMM) and Indian continentalcrust (Fig. 5). Enrichment of mantle source for the post-collisionalK-rich magmas might have close affinity with subducted Indian conti-nental crust added to depleted MORB-source mantle during northwardunderthrusting of the Indian continental lithosphere beneath the Lhasaterrane (Mahéo et al., 2002). Using Sr–Nd–Pb–O isotopes and traceelements ratios from Higher Himalayan Crystalline Sequence (HHCS),many previous studies (e.g., Ding et al., 2003; Zhao et al., 2006, 2009;Guo et al., 2013, 2015) have pointed out that the ultrapotassic lavascan be well explained by underthrusting of the Himalayan continentalmaterials into the mantle source beneath the southern Tibet. In Figs. 5and 10, the ultrapotassic samples lie along a clear linear trend betweendepleted MORB-source mantle (DMM; Workman and Hart, 2005) andthe Indian continental margin sediments (HHCS; e.g., Najman et al.,

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Fig. 7.Mineral compositions of major phenocrysts in the YPVR. (a) Pyroxenes plotted on the enstatite–ferrosilite–diopside–hedenbergite quadrilateral diagram after Morimoto (1988).(b) Feldspars plotted on ternary diagram after Smith (1974). (c) Micas plotted on the Al–Mg–Fe diagram after Sheppard and Taylor (1992). Data for phlogopite of the ultrapotassicrocks in the Lhasa terrane are from Miller et al. (1999); Zhao et al. (2009); Gao et al. (2007a) and C.Z. Liu et al. (2011). Data for the Sailipu mantle xenolith are from C.Z. Liu et al.(2011). Data for kamafugite of the West Qinling are from Yu (1994).

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2010; Robinson et al., 2001; Harris et al., 2004; Zhao et al., 2009; Guoand Wilson, 2012; Guo et al., 2013 and references therein), implyingthe involvement of the Indian plate-derivedmaterials due to northwardsubduction of the Indian lithosphere beneath the Tibetan Plateau.Therefore, we propose a two-component mixing model to accountfor the enrichment of asthenospheric mantle source of the maficultrapotassic magmas beneath the Lhasa terrane (Fig. 9b). As shownin Fig. 9b, Sr–Nd isotopic compositions of the mantle-derivedultrapotassic magmas could be explained by a simple two-componentmixing between DMM and HHCS. The HHCS are represented by themetamorphic rocks in the Higher Himalaya (e.g., Najman et al., 2010;Robinson et al., 2001; Harris et al., 2004; Richards et al., 2005; Guoand Wilson, 2012), while the composition of the DMM is taken from

Fig. 8. (a) (143Nd/144 Nd)i vs. SiO2 and (b) (87Sr/86Sr)i vs. SiO2. Data sources and the sy

Workman and Hart (2005). In addition, modeling curves 1 and 2 inFig. 9b represent upper and lower limitation of the simulation curvesbetween HHCS and DMM (Table 3).

Previous studies (e.g., Johnson and Plank, 1999; Woodhead et al.,2001) demonstrated that ratios of fluid/melt-mobile trace elements tofluid/melt-immobile trace elements can effectively reflect the impor-tance of subduction-induced fluids/melts in the mantle source ofsubduction-related magmas, and particularly these elements ratios areinsignificantly fractionated during partial melting (Class et al., 2000).The combination of incompatible element and Sr–Nd isotopic ratioshas been effectively used as a fingerprint in identifying metasomaticcomponents in the mantle source of the subduction-related magmas(e.g., Hawkesworth et al., 1997; Turner and Hawkesworth, 1997; Class

mbols of the potassic and ultrapotassic rocks in the Lhasa terrane are as in Fig. 3.

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Fig. 9. (a) (87Sr/86Sr)i vs. Sr and (b) (143Nd/144Nd) vs. (87Sr/86Sr)i plots for the potassic andultrapotassic rocks in the Lhasa terrane, showing two-component mixing line of HigherHimalayan Crystalline Sequence (HHCS) and depleted MORB-source Mantle (DMM) andthe AFC and EC–AFC processes. For two-component mixing trends with the F = 10%increment. The AFC trends are displayed as green curves with 5% increment in F = Mm/M0 (Mm, present mass of magma; M0, initial mass of magma). EC–AFC trends (redcurve) for equilibration temperatures (Teq) of 900 °C are shown. Abbreviations are asfollows: A, crustal assimilant; P, primitive magma.

Table 3Sr and Nd concentration (ppm) and initial (87Sr/86Sr)i and (144Nd/143Nd)i of the HighHimalayan Crystalline Sequence (HHCS) and depleted MORB-source mantle (DMM).

End-member parameterHHCS

DMMMin Max

Sr (ppm) 2 253.5 7.66(87Sr/86Sr)i 0.705442 1.198001 0.702626Nd (ppm) 1.1 1847 0.58(144Nd/143Nd)i 0.511591 0.512571 0.513106

Sr and Nd concentration and their initial isotopic ratios of the HHCS are taken from Vidalet al. (1982), Deniel et al. (1987), France-Lanord et al. (1993), Inger and Harris (1993),Parrish and Hodges (1996), Whittington et al. (1999), Ahmad et al. (2000); Najman et al.(2010); Robinson et al. (2001); Harris et al. (2004), Richards et al. (2005), Guo andWilson(2012). Compositions of depleted MORB-source mantle wedge (DMM) are taken fromWorkman and Hart (2005). The HHCS and DMM are age-corrected to 10 Ma based on theage of the Yangying potassic volcanic rocks.

20 L. Zhang et al. / Gondwana Research 41 (2017) 9–28

et al., 2000; Guo et al., 2005, 2006, 2013, 2014a, 2015). Therefore, weuse Ba/La, Ba/Th and Th/Nd ratios to constrain the involvement of fluidsand melts in generation of the ultrapotassic magmas. High Ba/La, Ba/Thand Th/Nd ratios in the ultrapotassic rocks in the Lhasa terrane reflectpresence of the slab-derived fluids and melts in the mantle source re-gion (Fig. 10).

Recently, subduction-derived mélange rocks, mixture of hydrousfluids and melts derived from subducted slab and mantle peridotiteformed at the slab–mantle interface, have been introduced to illustratethe physico-chemical process responsible for recycling of crustal com-ponent to the mantle-source region of arc volcanic rocks (Marschalland Schumacher, 2012; Guo et al., 2014a). The ultrapotassic magmaticrocks in the Lhasa terrane and the mélange rocks both display enrich-ment in LILE, LREE and depletion in HFSE, e.g., positive Pb anomalyand negative Nb, Ta and Ti anomalies (Fig. 4), suggesting that the mé-lange rocks might be potential source rocks for the mantle-derivedultrapotassic magmatic rocks. This inference is in good agreementwith comparable Nb/La and Ce/Pb ratios between ultrapotassic igneousrocks and mélange rocks (Fig. 11a).

Positively-correlated Ba/Th and (La/Sm)N ratios of the ultrapotassicmagmatic rocks in the Lhasa terrane suggest involvement ofsubduction-related fluids and melts in magma generation (Fig. 11b),which could be well explained by characteristics of the mélange rocks(Marschall and Schumacher, 2012; Guo et al., 2014a). Th/La and Sm/Laratios of ultrapotassic magmatic rocks in the Lhasa terrane show a pos-itive correlation (Fig. 12a), suggesting that Th and Sm enrichmentscould be linked to the involvement of the subducted Indian mélangeswhich might contain zoisite/epidote and lawsonite (Guo et al., 2014a,2015). Ultrapotassic magmatic rocks in the Lhasa terrane are character-ized by lower Dy/Dy* than those of magmas derived from oceanic platesubduction and oceanic island basalts (Fig. 12b; Davidson et al., 2013),implying the addition of the Indian continental subducted sedimentsto themantle source and the different evolution trend ofmagma at con-tinental and oceanic seduction zones.

6.3. Shallow crustal magma chamber processes

Clinopyroxene-liquid thermobarometers are key tools in under-standing processes of storage, cooling, and fractionation of magmas(Putirka et al., 1996, 2003; Putirka, 2008). There are several steps thatshould be followed before calculating temperature and pressure usingthe clinopyroxene-liquid thermobarometers.

First, choose the suitable melts which are in equilibrium withclinopyroxenes. Themost commonly usedmelts are represented by com-positions of whole rock, groundmass and glass (e.g., Shaw and Klügel,2002; Putirka and Condit, 2003; Putirka et al., 2003; Dahren et al.,2012). Considering that clinopyroxene crystallizes at the early stage dur-ingmagma evolution, whole rock components of the YPVR are chosen tobe liquid composition (Putirka et al., 1996, 2003; Putirka, 2008).

Second, check whether the clinopyroxene grains are in equilibriumwith the host melt. Clinopyroxenes of the YPVR (Fig. 2) are commonlyeuhedral, exhibiting no clear petrographic indications of disequilibriumwith their host melt (e.g., reaction rim texture, corrosion structure).Based on major elements of the clinopyroxene analyses (Table S6 inthe Supplementary data), we use the Fe–Mg exchange coefficientsKD(Fe–Mg)cpx-liq to test for the clinopyroxene-melt equilibrium(Putirka et al., 2003), as is shown by the equation below:

KD Fe−Mgð Þcpx−liq ¼ Mgliq Fecpx

Mgcpx Feliq¼ 0:27� 0:03

Third, estimate H2O content of the magma before eruption. H2Ocontent is a very influential parameter for the clinopyroxene-liquid thermobarometers (e.g., Putirka, 2008; Dahren et al., 2012).Based on the thermal model proposed by Melekhova et al. (2013), thecompositional distribution of derivative magma varies as a function

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Fig. 10. (a) Ba/Th vs. Th/Nd. (b) Ba/La vs. Th/Nd. (c) (87Sr/86Sr)i vs. Ba/La. (d) (87Sr/86Sr)i vs. Th/Nd. (e) (143Nd/144Nd)i vs. Ba/La and (f) (143Nd/144Nd)i vs. Th/Nd. The ultrapotassic rocks(MgO ≥ 6%, filled circle) in the Lhasa terrane form linear arrays, suggesting binary mixing (brown dashed-line with double-sided arrows) between DMM and HHCS-derived componentswith higher Ba/La (fluids) and Th/Nd (melts) ratios relative to the bulk HHCS (Fig. 10c–f). Data sources and symbols of the K-rich rocks are as in Figs. 3 and 5.

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of water content of themagmatic system, which is related with the fluxand duration of magma input. In order to minimize the effect of H2Ocontent, we use a new equation of clinopyroxene-liquidthermobarometers proposed by Masotta et al. (2013) for alkalinedifferentiated magmas. The pre-eruptive H2O content we used inclinopyroxene-liquid thermobarometer is estimated at 3%.

Based on the above analyses, we calculated pressure (P) andtemperature (T) conditions under which clinopyroxenes crystallize inthe magma chamber beneath the Yangying volcanic field in SouthTibet. The results of the clinopyroxene-liquid thermobarometersdisplay a relatively concentrated pressure (P = 2.5–4.1 kbar) and tem-perature (T= 1029.4–1082.9 °C) range (Table S6 in the Supplementary

data). Using the equation D (km)=4.02+ 3.03 × P (kbar) proposed byAve Lallemant et al. (1980), we calculated storage depth of the magmachamber which ranges from 11.60 km to 16.44 km, consistent withthe changing depth of the clinopyroxene crystallization due to broadrange of AlVI/AlIV ratios. Previous studies have demonstrated that pres-ence of a low-velocity anomaly zone with depth of ~15 km beneaththe Yadong-Gulu rift which was interpreted as partiallymolten middle crust (Nelson et al., 1996; Brown et al., 1996; Weiet al., 2001). Our estimations are consistent with the depth of theMiocene Yangying magma chamber, implying that the low-velocityanomaly zone might be remnant of the Late Miocene potassic magmassince eruption.

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Fig. 11. (a) Ce/Pb vs. Na/La plot for the potassic and ultrapotassic rocks in the Lhasa terrane. (b) Ba/Th vs. (La/Sm)N plot for the potassic and ultrapotassic rocks in the Lhasa terrane. Data forthe average composition of subduction channelmélange rocks are fromMarschall and Schumacher (2012) and references therein. TheGlobal Subducting Sediment (GLOSS) data are fromPlank and Langmuir (1998). Upper continental crust (UCC) data are fromZartman andHaines (1988).MORB andOIB data are from Sun andMcDonough (1989). Data sources and symbolsof the K-rich rocks are as in Figs. 3 and 5.

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6.4. Energy-constrained assimilation and fractional crystallization (EC–AFC) modeling

Crustal contamination and fractional crystallization are consideredas important processes contributing to magmatic differentiation of theevolved magma (DePaolo, 1981; Foland et al., 1993; Douce, 1999;Spera and Bohrson, 2001, 2004; Barnes et al., 2005; Guo et al., 2006;Farahat et al., 2007). Based on the available geochemical data of themafic ultrapotassic (MgO ≥ 6 wt.%) and potassic rocks in the Lhasaterrane, we present EC–AFC model to quantitatively illustrate physicaland chemical characteristics of the magma–country rock interactionsin YPVR, which could provide rigorous constraints on evolution of themantle-derived ultrapotassic magma in crustal magma chamberbeneath the Yangying volcanic field. Reasonable ranges of initialthermal and compositional parameters used in the EC–AFC model arefrom Bohrson and Spera (2007) as shown in Table 4.

Potential crustal materials involved in petrogenesis of the YPVRare characterized by low (87Sr/86Sr)i and high (143Nd/144Nd)i ratios(Figs. 5 and 8), similar to those of relatively depleted crustal materialsfrom the Lhasa terrane, e.g., adakitic rocks, Linzizong volcanic rocksand Gangdese batholith (Fig. 5a). Moreover, the best-fit lithology forcrustal contamination of the mafic ultrapotassic magmas must also be

Fig. 12. (a) Sm/La vs. Th/La plot for the YPVR and thepotassic and ultrapotassic rocks in Lhasa terPlank and Langmuir, 1998) are reported as proxies of crustal recycled components. MORB and Othe potassic–ultrapotassic rocks in Lhasa terrane. Fields forMORB and OIB and continent crust adepleted mantle (DM) is from Salters and Stracke (2004). GLOSS average are calculated from P

consistent with ƐHf(t) (3.65–8.11) and ages (67–59 Ma) of xenocrysticzircons in the YPVR. Following these considerations, the adakitic rocksshould be ruled out because their extrusive/intrusive ages (26–8 Ma;e.g., Hou et al., 2004, 2013; Guo et al., 2007) postdate the U–Pb ages(67–59 Ma) of these xenocrystic zircons (Fig. 6f). Hence, the Gangdesebatholith and/or Linzizong volcanic rocks might be the most appropri-ate crustal material mixed to mantle-derived ultrapotassic melts inthe middle crust, because (1) they have the proper Sr–Nd–Pb isotoperatios required for assimilation of the mantle-derived ultrapotassicmelts to generate YPVR magmas (Fig. 5; Zhang, 1996; Jiang et al.,1999; Dong, 2002; Guo et al., 2007; Lee et al., 2007, 2009, 2012; Donget al., 2008; Z.D. Zhao et al., 2011); (2) they have consistent intrusiveages and zircon Hf isotopic ratios (Fig. 6f) with the studied xenocrysticzircons from YPVR (Lee et al., 2007, 2009, 2012; Wen et al., 2008; Jiet al., 2009b, 2012); (3) Guo et al. (2007) have indicated that theLinzizong magmas underplate the lower crust of the Lhasa terrane,and result in the lower crustal thickening. The middle crust of Lhasaterrane also might be affected by the underplating of the Linzizongmagmas, suggesting the component of the Lhasa terrane middle crustconsistent with the Linzizong magmas. Furthermore, Mo et al. (2003)have provided evidence to demonstrate that the composition of theLinzizong magmas could be regarded as the component of middle-

rane. Continental Crust (Rudnick andGao, 2003) andGlobal Subducting Sediment (GLOSS;IB data are from Sun andMcDonough (1989). (b) Dy/Yb vs. Dy/Dy* plot for the YPVR and

re fromDavidson et al. (2013). Primitivemantle (PM) is from Sun andMcDonough (1989);lank and Langmuir (1998). Data sources and symbols of the K-rich rocks are as in Fig. 3.

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Table 4Assumed parameters and best-fit calculation results of the EC-AFC model calculations.

Modeling processesYangying potassicvolcanic fields

Thermal parametersMagma liquidus temperature (Tl,q, °C) 1200Magma initial temperature (Tm°, °C) 1200Assimilant liquidus temperature (Tl,a, °C) 1000Assimilant initial temperature (Ta°, °C) 230–300Solidus temperature (Ts, °C) 800Equilibration temperature (Teq, °C) 900Isobaric specific heat of magma (Cp,m, J/kg per K) 1200Isobaric specific heat of Assimilant (Cp,a, J/kg per K) 900Crystallization enthalpy (Δhcry, J/kg) 396,000Fusion enthalpy (Δhcry, J/kg) 354,000

Compositional parametersMagma initial Sr content (Csr,m°, ppm) 985.8Magma initial Nd content (CNd,m°, ppm) 191.2Magma Sr isotope ratio (ɛsr,m) 0.720952Magma Nd isotope ratio (ɛNd,m) 0.511982Magma bulk distribution coefficient for Sr (Dsr,m) 0.8Magma bulk distribution coefficient for Nd (DNd,m) 1.45Assimilant initial Sr content (Csr,a°, ppm) 551.32Assimilant initial Nd content (CNd,a°, ppm) 15.57Assimilant Sr isotope ratio (ɛsr,a) 0.704056Assimilant Nd isotope ratio (ɛ Nd,a) 0.512849Assimilant bulk distribution coefficient for Sr (Dsr,a) 0.1Assimilant bulk distribution coefficient for Nd (DNd,a) 0.2

The thermal parameters are taken from Bohrson and Spera (2007). The compositionalparameters of primitive magmas are from Guo et al. (2013). The assimilants are theGangdese batholith with average compositions reported by Dong et al. (2008).

23L. Zhang et al. / Gondwana Research 41 (2017) 9–28

upper crust of the Lhasa terrane. Thus, the component of the Linzizongmagmas can be used as that of the middle-upper crust beneath theLhasa terrane; and (4) the whole-rock Sr–Nd–Pb isotopic compositionsexhibit linear trends between enriched mantle-derived maficultrapotassic magmas and relatively depleted crustal contaminants(e.g., the Gangdese batholith and/or Linzizong volcanic rocks) in theLhasa terrane.

Compositions of the crustal assimilant in the Lhasa terrane are listedin Table 4. As indicated by the calculated results, the liquidus tempera-ture, solidus temperature and initial temperature of the crustalassimilant (i.e., the Gangdese batholith and/or the Linzizong volcanicrocks) are 1000 °C, 800 °C and 230–300 °C, respectively. In addition,the liquidus temperature, initial temperature of the primitive magmaand the equilibration temperature between magma and the countryrocks are 1200 °C, 1200 °C and 900 °C, respectively. In consideration ofthe ultrapotassic magmatic rocks have not been discovered in Yangyingvolcanic field, we select somemafic ultrapotassic rocks with the highestMgO, Cr and Ni content in the western Lhasa terrane as the primitivemagmas for the EC–AFC model simulation (Table 4). As shown inFig. 9, the YPVR can be explained by an EC–AFC model with a best-fitprimitive K-rich magma with Sr = 985.8 ppm, Nd = 191.2 ppm,(87Sr/86Sr)i = 0.720952, and (143Nd/144Nd)i = 0.511982.

Before the country rocks were heated up to solidus temperature(800 °C), Sr content of the mantle-derived ultrapotassic magmas firstlyincreased whereas (87Sr/86Sr)i remained constant as indicated by a flattrajectory in Fig. 9a, suggesting that fractional crystallization(e.g., clinopyroxene and phlogopite) dominated this stage before addi-tion of melts from country rocks into the mantle-derived ultrapotassicmagmas. When the temperatures reached solidus of the country rocks(800 °C), Sr content continued to increase while (87Sr/86Sr)i decreaseddramatically due to involvement of partialmelts derived from the coun-try rocks with relatively less radiogenic (87Sr/86Sr)i ratios. By the end ofthe magma evolution, Sr content of the contaminated primitiveultrapotassic magma decreased in response to the fractional crystalliza-tion of Sr-rich plagioclase (Fig. 9a). Therefore, YPVR can be well ex-plained by fractional crystallization and contamination (by partial

melts from the Gangdese batholith and/or the Linzizong volcanic rockswith depleted Sr–Nd isotopic compositions) of mantle-derivedultrapotassic magmas, which gains support from petrographic evidence(Fig. 2). For example, YPVR shows that plagioclase appears to have expe-rienced stages of growth assimilation and overgrowth (Fig. 2), implyingthat the Yangyingmagmas underwent complicated EC–AFCprocesses. Inaddition, the AFC calculation proposed by DePaolo (1981) was also per-formed, and the results (Fig. 9b) show that the YPVR have undergone avery high rate of assimilation (r =Ṁa/Ṁc = 0.6;Ṁa, the mass of assim-ilation;Ṁc, the mass of fractional crystallization) which is nearly consis-tent with the results displayed by the EC–AFC (Ma⁎/Mc = 0.675; Ma⁎, theamount of assimilant partial melt; Mc, the mass of cumulate).

The thermal and compositional parameters are generally used toexplain the site at which EC–AFC processes occurred (Guo et al.,2006). Chan et al. (2009) proposed a geothermal gradient (16 °C/km)for crust of the Lhasa terrane based on the xenolith temperatureestimations. Therefore, the depth atwhich the EC–AFC process occurredfor the YPVR ranges from 14.40 to 18.75 km, similar to depth of thecrustal magma chamber provided by the clinopyroxene-liquid thermo-barometers (Fig. 13). Based on the depth of crustalmagma chamber andcrustal thicknesses in the Lhasa terrane (Zhang and Klemperer, 2005;Searle et al., 2011), we suggest that the assimilation and fractional crys-tallization process took place in the middle crust of the Lhasa terrane(11.60–18.75 km).

6.5. Petrogenetic model of the Yangying potassic volcanic rocks

Based on the abovediscussions, we present a two-stage petrogeneticmodel for the Yangying potassic volcanic rocks (Fig. 13). The first stageof themodel involves formation of themafic ultrapotassic magmas. Thesubducted Indian continent crustal materials and mantle wedge weremechanically mixed in subduction channel forming the Indian mé-langes at the slab-mantle interface as a consequence of the northwardsubduction of Indian continental lithosphere followed the Asia–Indiacollision during 55–25 Ma (Guo et al., 2013, 2014a, 2015). Then, theenriched Indian mélanges rose buoyantly from the surface of theIndian subducting slab and underplated beneath the base of theTibetan lithosphere (Marschall and Schumacher, 2012; Guo et al.,2014a, 2015). India–Asia continent convergence rate decreased duringthe period of 25–8 Ma (Lee and Lawver, 1995; Chung et al., 2005; Guoet al., 2013), leading to rollback of the subducted Indian slab(Fig. 13a), and more importantly, decompression partial melting ofthe Indian mélanges and the generation of the post-collisionalultrapotassic mafic magmas (Fig. 13b). Moreover, age of E–Wextensionof the Yadong-Gulu rift in South Tibet has been constrained to be ~12–8Ma (Harrison et al., 1995; Edwards and Russell, 1998;Wu et al., 1998),which is in accordancewith the ages of the slab rollback (25–8Ma), im-plying that lithospheric extensional tectonics beneath the Lhasa terranemight be closely related to slab rollback process. These can also explainthe spatial correlation between the post-collisional potassic–ultrapotassic magmatism and the NS trending rifts in South Tibet (Guoet al., 2013, 2015).

The second stage of the model involves the AFC processes ofthe mantle-derived ultrapotassic magmas in middle crust (11.60–18.75 km) beneath the Lhasa terrane (Fig. 13c). During this stage,mantle-derived ultrapotassic mafic magmas were contaminated bythe Gangdese batholith and/or Linzizong volcanic rocks with depletedSr–Nd isotopic compositions (Fig. 9), accompanied by fractional crystal-lization processes, giving rise to formation of the Yangying potassicmagmas (Fig. 13c). The linear trends between mantle-derivedultrapotassic magmas and the Gangdese batholiths and/or Linzizongvolcanics in the Sr–Nd–Pb isotope diagrams are consistent with thisAFC inference (Fig. 5). Geophysical studies (e.g., Zhou and Murphy,2005; Li et al., 2008; Zhao et al., 2010; W. Zhao et al., 2011; J. Zhaoet al., 2014; Q. Xu et al., 2015; Zhang et al., 2015) have indicated thecontinuous presence of a northward dipping subducted slab of Indian

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Fig. 13. Petrogeneticmodel for post-collisional potassicmagmatism in the Yangying volcanic field of the Lhasa terrane, South Tibet. The diagram shows anNS cross section and ismodifiedafter studies of Guo et al. (2007, 2013, 2014a);Marschall and Schumacher (2012) and Cashman and Sparks (2013). Abbreviations are as follows: BNS, Bangong-Nujiang suture; ITS, Indus-Tsangpo suture; MBT, the Main Boundary thrust; MCT, the Main Central thrust; STD, South Tibetan detachment; SCLM, subcontinental lithospheric mantle; P, potassic magmatism; UP,ultrapotassic magmatism. Outcrops of ultrapotassic volcanic rocks in Yangying volcanic field have not been discovered, as shown by the question mark.

24 L. Zhang et al. / Gondwana Research 41 (2017) 9–28

continental lithosphere beneath the Lhasa terrane, and a low-velocityanomaly zone with depth of ~15 km beneath the Yadong-Gulu rift isclearly imaged which has been interpreted as partial melts in middlecrust (e.g., Nelson et al., 1996; Brown et al., 1996; Wei et al., 2001).We suggest that the residual magma beneath the Yadong-Gulu rift canprovide continuous heat for extensive hydrothermal activities atpresent (e.g. hot springs, soil microseepage; Guo et al., 2014b; L.H.Zhang et al., 2014) in Yangying and Yangbajing, which are releasingconsiderable amounts of volatiles (e.g., CO2; Guo et al., 2014b; L.H.Zhang et al., 2014). Moreover, hydrothermal gases released from theYadong-Gulu rift are characterized by “mantle signature” (3He/4He =0.1–0.14 RA; Yokoyama et al., 1999; Hoke et al., 2000; L.H. Zhang et al.,2014), suggesting that the excess 3He might have close affinities withresidual mantle-derived magmas in middle crust beneath the Yadong-Gulu rift in the Lhasa terrane.

7. Conclusions

Based on the whole-rock major and trace elements and Sr–Nd–Pbisotopic compositions of the Yangying volcanic rocks, and comprehen-sive mineralogical and petrological data, combined with in situ zirconU–Pb dating and Hf–O isotopic compositions, we conclude that:

(1) SIMS zircon U–Pb dating analyses yield ages of 10.61 ± 0.10 Maand 10.70 ± 0.18 Ma (weighted mean ages); their ƐHf(t) valuesrange from −4.79 to −0.17, combined with O isotope (5.51–7.22‰), imply an addition of crustal material in their source.

(2) Based on the EC–AFC model and the clinopyroxene-liquidthermobarometers, the assimilation and fractional crystallizationprocesses of the mantle-derived ultrapotassic magmas mighthave taken place in middle crust with the depth ranging from11.60 km to 18.75 km beneath the Lhasa terrane.

(3) A two-stage model for the petrogenesis of the YPVR wasproposed, which involves (a) formation of the ultrapotassicmafic magmas due to partial melting of the Indian mélangesbeneath base of the Tibetan lithosphere during rollback of thesubducted Indian lithosphere, and (b) occurrence of the YPVR

as a result of AFC processes of the mantle-derived primitiveultrapotassic magmas in middle crust of the Lhasa terrane.

Acknowledgments

This studywas supported by the Strategic Priority Research Program(B) of Chinese Academy of Sciences (Grant No. XDB03010600). We aregrateful to Drs. Xianhua Li, QianMao, Qiuli Li and Xiaoxiao Ling for theirassistance in laboratory. Drs.WenfengGuo and Yanan Yang are thankedfor helpful discussion.

Appendix A. Supplementary data

Supplementary data to this article can be found online at http://dx.doi.org/10.1016/j.gr.2015.11.007.

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