2. 地质过程与矿产资源国家重点实验室,武汉 430074;
3. 中国地质大学地球科学学院,武汉 430074
2. State Key Laboratory of Geological Processes and Mineral Resources,Wuhan 430074,China;
3. Faculty of Earth Sciences,China University of Geosciences,Wuhan 430074,China
华北克拉通是世界上最古老的克拉通之一,其组分可以追溯到3.8Ga以前(Liu et al., 1992,2008; Song et al., 1996; Zheng et al., 2004a,2012; Wan et al., 2005,2012; 吴福元等,2008),并经历了复杂的演化过程(刘敦一等,1997; Wu et al., 2005; Kusky et al., 2007; Jiang et al., 2010; Zhai et al., 2010; Kusky,2011; Geng et al., 2012; Zhang et al., 2012a; Zhao and Zhai, 2013)。岩浆岩的全岩Nd同位素和锆石Hf同位素研究表明,2.8~2.6Ga可能是华北大陆地壳生长的重要时期(Zheng et al., 2004b,2009,2012; Wu et al., 2005; Geng et al., 2012; Zhang et al., 2013)。华北中部广泛分布的岩石,其时代主要集中在新太古代晚期-古元古代末,新太古代早期的岩石仅在少数地区以包体的形式存在(Guan et al., 2002; Kröner et al., 2005),或者在古元古代岩石中残留少量新太古代早期的继承锆石(刘敦一等,1997; Wilde et al., 1997,2002,2003)。这些新太古代-古元古代的岩石及其中的锆石Hf同位素组成暗示华北克拉通在~2.5Ga也经历了强烈的增生和再造事件(Wan et al., 2005,2012; 刘富等,2009; Diwu et al., 2011; Liu et al., 2011,2012; Zhang et al., 2012b)。翟明国(2011)和Kusky(2011)指出2.5Ga左右华北克拉通有广泛的麻粒岩相和角闪岩相变质作用;郭敬辉等(2002)、Guo et al.(2005)和Zhao et al.(2010)通过华北中北部麻粒岩锆石U-Pb年代学研究发现~1.85Ga的变质作用可能更为显著。经历了3.0~2.5Ga复杂的地壳形成与演化,2.45~1.9Ga华北进入构造相对宁静的时期(Du et al., 2013)。随着研究的深入,2.3~2.0Ga的岩浆事件越来越多的被报道(第五春荣等,2007; 郭素淑和李曙光,2009; 黄道袤等,2012),其地质意义日渐突显。麻粒岩是大陆下地壳的主要组成岩石,对华北中北部麻粒岩地质体的研究不仅可以反演华北太古代-古元古代的下地壳增生和再造历史,而且可能约束华北中部的变质时间。
位于华北中北部的怀安杂岩体,出露晚太古代至古元古代的角闪岩相-麻粒岩相高级变质岩,包括TTG片麻岩、(高压)镁铁质麻粒岩、片麻状花岗岩、紫苏花岗岩、S型花岗岩等(Zhao et al., 2006),翟明国和刘文军(2001)还根据蔓菁沟-瓦窑口-马市口-下白窑-尚义等地代表性岩石的研究建立了下地壳剖面结构。怀安杂岩体可视为探索华北大陆下地壳形成与演化的重要窗口之一,本文选择镁铁质麻粒岩及其中的条带状分布的长英质麻粒岩,展开岩石学、锆石U-Pb年代学及原位Hf同位素研究,以探讨华北北部深部地壳的早期演化过程。
2 地质背景华北克拉通的构造划分存在一定的争议性,Zhao et al.(2001,2005)根据华北克拉通基底岩石特征将其划分为东部陆块、西部陆块和中部造山带三个主要构造单元。Zhai and Santosh(2011)根据古老花岗岩-绿岩带将华北克拉通划分为胶辽、迁怀、集宁、鄂尔多斯、阿拉善、许昌和徐淮7个不同的陆块。按照Zhai and Santosh(2011)的划分,怀安杂岩体位于集宁陆块中核与鄂尔多斯陆块交汇部位(图 1),也相当于中部带(Zhao et al., 2005)的北缘。
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图 1 华北克拉通构造划分简图(据Zhai and Santosh, 2011) Fig. 1 Distribution of tectonic subdivision of the North China Craton(after Zhai and Santosh, 2011) |
怀安杂岩体以南是恒山、五台、阜平等地块,北部以尚义-赤城大断裂为界与角闪岩相的红旗营子群变质表壳岩组合相接。怀安杂岩体西边出露典型的孔兹岩系,其岩石组合为石墨-含矽线石-石榴子石片麻岩、石榴子石石英岩、长英质副片麻岩、钙质硅酸盐和大理岩(Yin et al., 2009; Zhao et al., 2010)。孔兹岩系原岩形成时间为2.3~1.9Ga,2.0~1.9Ga发生变质作用。伴随孔兹岩系出露零星的紫苏花岗岩和S型花岗岩,形成于~1930Ma(Peng et al., 2012)。
怀安杂岩体的内部构造略呈穹窿状,穹窿的中心大致在该地体的中心瓦窑堡-新平堡一带(刘富等,2009),它主要由TTG片麻岩系列、(高压)镁铁质麻粒岩、片麻状花岗岩、紫苏花岗岩和S型花岗岩组成,局部含有孔兹岩带的变表壳岩成分(Zhao et al., 2006,2010)。本文研究样品取自怀安杂岩体北部的尚义地上村(N40°43′33.13″,E114°18′7.86″)和兴和马市口国道边(N40°43′57.32″,E114°08′19.52″,图 2),毗邻高压麻粒岩出露点。尚义地上的镁铁质麻粒岩露头较小,岩石组合多变,周围产出大量的肉红色钾质花岗岩。马市口的基性麻粒岩露头长约15m,宽3~4m,其中夹有长英质的麻粒岩条带。
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图 2 怀安杂岩体地质简图(据Peng et al., 2012)及采样点 Fig. 2 Simplified geological map of Huai’an complexes in the North China Craton(after Peng et al., 2012),showing sample locations |
尚义地上地区麻粒岩呈块状构造,粒状变晶结构,主要组成矿物有单斜辉石(10%~55%)、斜长石(30%~40%)、石英(5%~10%)、斜方辉石(0~15%)和角闪石(0~50%),副矿物为石榴子石、磷灰石和锆石。根据辉石和角闪石含量,进一步可以分为二辉石麻粒岩(如样品DS-2、DS-3、DS-4)、单斜辉石麻粒岩(DS-5)和二辉角闪石麻粒岩(DS-9)。单斜辉石麻粒岩矿物组成为单斜辉石、斜长石和少量石英,不发育斜方辉石(图 3)。二辉石麻粒岩中石榴子石发育有斜长石(部分蚀变为绢云母)和斜方辉石组成的后成合晶(图 3),另有斜方辉石包裹单斜辉石(图 3c),指示二辉石麻粒岩可能经历了近等温降压的退变过程(Guo et al., 2002; 翟明国,2009)。二辉角闪石麻粒岩中角闪石环绕单斜辉石和斜方辉石生长,并将早期的石榴石和辉石隔开(图 3),反映了二辉石麻粒岩的进一步降温退变质(O’Brien and RöTzler,2003; 翟明国,2009)。
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图 3 怀安麻粒岩镜下特征 (DS-2)二辉石麻粒岩:“白眼圈”结构;(DS-3,DS-4)二辉石麻粒岩:斜方辉石包裹单斜辉石;(DS-5)单斜辉石麻粒岩:单斜辉石+斜长石+石英;(DS-9)二辉角闪石麻粒岩:角闪石交代斜方辉石;(XH-1)长英质麻粒岩:单斜辉石+斜方辉石+条纹长石+斜长石+石英.Grt-石榴子石;Opx-斜方辉石;Cpx-单斜辉石;Pl-斜长石;Am-角闪石;Qz-石英;Kfs-钾长石 Fig. 3 Selected photographs showing Huai’an granulites |
马市口地区基性麻粒岩呈块状构造,其中的长英质麻粒岩条带发育弱片麻理。基性麻粒岩为粒状变晶结构,主要矿物组成有单斜辉石(5%~60%)、斜方辉石(5%~25%)、斜长石(10%~40%)和角闪石(0~35%),次要矿物有石英(5%)、条纹长石(0~10%)和黑云母(0~10%),副矿物为磷灰石和锆石。根据暗色矿物含量可分为二辉石麻粒岩(如样品XH-2、XH-9)和二辉角闪斜长石麻粒岩(XH-5)。二辉石麻粒岩中含少量黑云母,不含碱性长石;二辉角闪斜长石麻粒岩中不含黑云母,含约10%条纹长石,单斜辉石和斜方辉石含量约为5%。长英质麻粒岩条带(XH-1)(图 3)为粒状变晶结构,矿物组成为斜长石(55%)、条纹长石(20%)、单斜辉石(10%)、石英(10%)和斜方辉石(5%),副矿物为磷灰石和锆石。
4 分析方法选择尚义地上单斜辉石麻粒岩(DS-5)和马市口长英质麻粒岩条带(XH-1)进行锆石U-Pb年龄、微量元素分析及原位Hf同位素分析。这些分析都在中国地质大学(武汉)地质过程与矿产资源国家重点实验室完成。U-Pb定年利用LA-ICP-MS完成,激光剥蚀系统为GeoLas 2005,ICP-MS为Agilent 7500a。激光剥蚀过程中采用氦气作载气、氩气为补偿气以调节灵敏度。每个时间分辨分析数据包括大约20~30s的空白信号和50s的样品信号。对分析数据的离线处理采用软件ICPMSDataCal完成(Liu et al., 2008,2010a)。详细的仪器操作条件和数据处理方法同(Liu et al., 2008,2010a,b)。 U-Pb同位素定年中采用锆石标准91500作外标进行同位素分馏校正,每分析5个样品点,分析2次91500。锆石标准91500的U-Th-Pb同位素比值推荐值据Wiedenbeck et al.(1995)。锆石样品的U-Pb年龄谐和图绘制和年龄权重平均计算均采用Isoplot/Ex_ver3完成(Ludwig,2003)。 锆石原位Hf同位素分析利用Neptune MC-ICP-MS和193nm激光取样系统完成。分析时激光束直径为64μm,激光剥蚀时间约为50s。仪器的运行条件及详细的分析过程参见文献Hu et al.(2012)。数据的离线处理采用ICPMSDataCal完成(Liu et al., 2010b)。
5 分析结果 5.1 锆石U-Pb年龄DS-5和XH-1样品的锆石稀土元素组成见表 1,U-Pb年龄结果见表 2。
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表 1 怀安麻粒岩锆石稀土元素组成(×10-6) Table 1 LA-ICP-MS zircon rare earth elements results for the Huai’an granulites(×10-6) |
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表 2 怀安麻粒岩锆石U-Pb年龄结果 Table 2 LA-ICP-MS zircon U-Pb results for the Huai’an granulites |
尚义地上单斜辉石麻粒岩(DS-5)中锆石为椭圆形-圆形,大小为50~100μm,根据其内部结构(图 4)可分为两种类型:一类具有核边结构,核部显示弱振荡环带,阴极发光为灰黑色,边部小于10μm,阴极发光呈白色;另一类成分较均一,无内部结构,阴极发光呈白色。第一类锆石具有强烈的正Ce异常,重稀土元素富集(图 5),(Gd/Lu)N在0.01~0.06之间,Th、U含量分别为121×10-6~659×10-6和317×10-6~1402×10-6,Th/U比值为0.32~0.60,是岩浆锆石。第二类锆石具有强的正Ce异常,重稀土平坦且轻重稀土分异较弱,(Gd/Lu)N分别为0.20、0.05、0.29,Th含量分别为4×10-6、1×10-6和1×10-6,U含量分别为14×10-6、30×10-6和24×10-6,Th/U比为0.31、0.03和0.04,为变质锆石。对27颗岩浆锆石和3颗变质锆石核部进行LA-ICP-MS定年分析。3颗变质锆石207Pb/206Pb年龄分别为2643±171Ma、2029±135Ma和2270±172Ma;27颗岩浆锆石207Pb/206Pb年龄分布在2387~2559Ma之间,在U-Pb谐和图(图 6)中获得2463±53Ma(MSWD=1.9)的上交点年龄,其中20颗谐和锆石的207Pb/206Pb加权平均年龄为2461±20Ma(MSWD=0.97),另外三颗谐和锆石的207Pb/206Pb年龄分别为2410±55Ma、2418±42Ma和2387±36Ma。
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图 4 尚义地上麻粒岩(DS-5)和马市口麻粒岩(XH-1)锆石CL图像 虚线圆圈为锆石U-Pb分析的激光剥蚀点位,实线圆圈为Hf分析位置,锆石年龄值为207Pb/206Pb年龄,括弧内数据为Th/U比值 Fig. 4 Representative CL images of zircons from Dishang(DS-5)and Mashikou granulites(XH-1) |
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图 5 尚义地上麻粒岩(DS-5)和马市口麻粒岩(XH-1)锆石稀土配分图 Fig. 5 Chondrite-normalized REE patterns of zircons from Dishang(DS-5)and Mashikou granulites(XH-1) |
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图 6 尚义地上麻粒岩(DS-5)和马市口麻粒岩(XH-1)锆石U-Pb年龄谐和图 Fig. 6 Concordia diagrams of zircon U-Pb dating for Dishang(DS-5)and Mashikou granulites(XH-1) |
马市口长英质麻粒岩(XH-1)中锆石为椭圆形或棱镜状,大小为150~200μm,具有核边结构(图 4),核部发育规则的振荡环带,阴极发光为灰黑色,边部小于10μm,阴极发光为白色。它们的稀土元素模式均一(图 5),具有强烈的正Ce异常以及不同程度的负Eu异常(δEu=0.10~0.97),富集重稀土元素,(Gd/Lu)N在0.01~0.07之间。Th、U含量分别为161×10-6~1946×10-6和346×10-6~1628×10-6,Th/U比在0.28~3.19之间,都显示了岩浆锆石的特征。对30颗锆石核部进行LA-ICP-MS定年分析,4个谐和点的207Pb/206Pb年龄分别为2114±47Ma、2165±44Ma、2271±43Ma和2316±39Ma,其余26颗锆石在U-Pb谐和图(图 6)中给出2458±46Ma(MSWD=4.1)的上交点年龄。
5.2 锆石Hf同位素组成DS-5和XH-1样品的锆石Hf同位素组成见表 3。
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表 3 怀安麻粒岩锆石Hf同位素结果 Table 3 In situ zircon Hf isotope composition for the Huai’an granulites |
单斜辉石麻粒岩(DS-5)在U-Pb测试的基础上对28颗锆石进行原位Hf同位素分析,锆石176Hf/177Hf比值为0.281284~0.281647,εHf(t)值分布范围为+2.1~+11.0,Hf亏损地幔模式年龄集中在2.6~2.7Ga,两个较年轻的tDM为2.4Ga和2.5Ga。207Pb/206Pb年龄为2029Ma和2270Ma的2颗变质锆石的εHf(t)分别为+4.4和+11.0,tDM均为2.2Ga。
长英质麻粒岩(XH-1)在U-Pb测试的基础上对27颗锆石进行原位Hf同位素分析,锆石Hf同位素分布比较均一,176Hf/177Hf比值在0.281325~0.281410之间,锆石εHf(t)值分布于-4.4~+5.3,tDM分布范围为2.6~2.7Ga,tcrust变化范围为2.7~3.0Ga。207Pb/206Pb年龄为2114±47Ma、2165±44Ma、2271±43Ma和2316±39Ma的锆石εHf(t)值分别为-4.4、-3.1、+0.5和+0.6,这四颗锆石的tcrust变化范围为2.8~3.0Ga,其余23颗锆石的εHf(t)值为+2.9~+5.3,tcrust分布于2.7~2.8Ga之间。
6 讨论 6.1 怀安地区2.7~2.8Ga的地壳物质大陆地壳来源于原始地幔的分异作用,经历了复杂演化历史,并具有幕式生长的特点(Condie,1998; Condie et al., 2009)。全球大陆地壳的主要生长时期为3.0~2.5Ga,该时期的增生陆壳占现在大陆的36%(Condie,1998),广泛分布的2.7~2.8Ga的构造热事件对全球陆壳生长的影响尤为重要(Zheng et al., 2009,2012; Geng et al., 2012)。华北火成岩具有3.0~2.6Ga(峰期为2.8Ga)的Nd模式年龄值(Wu et al., 2005),岩浆锆石的Hf模式年龄也显示了~2.7Ga的峰期(Zhang et al., 2012a),这些表明2.6~2.8Ga可能是华北大陆地壳生长的重要时期(Zheng et al., 2004a,2009,2012; Wu et al., 2005; Geng et al., 2012; Zhang et al., 2013)。在华北克拉通中北部已有的锆石U-Pb年代学数据也记录了~2.7Ga的热事件:Zheng et al.(2004c)和Jiang et al.(2010)报道了汉诺坝辉石岩捕掳体中2.7Ga的锆石和条带状麻粒岩捕掳体中2.8Ga的锆石;刘敦一等(1997)在怀安2500Ma的英云闪长质片麻岩中发现2761~2613Ma的锆石捕掳晶;Kröner et al.(2005)、Wilde et al.(2005)和陈斌等(2006)在吕梁-五台地区晚太古代花岗岩中发现2.7Ga的古老残留锆石;孙敏和关鸿(2001)在阜平群角闪片麻岩中获得2708±8Ma的古老地壳信息;恒山和阜平地区零星存在2.7Ga的片麻岩(Kröner et al., 2005);Liu et al.(2009)报道了太华2829Ma和2832Ma的英云闪长质片麻岩。
本文所研究的长英质麻粒岩(XH-1)的锆石Hf同位素组成与上述有相似的特征。长英质麻粒岩中~2.5Ga的锆石Hf两阶段模式年龄为2.7~2.8Ga,~2.1Ga锆石的Hf tcrust为3.0Ga,显示怀安地区存在≥2.7Ga的古老地壳物质,可能追溯到3.0Ga。因为数据有限,这一认识尚需进一步研究。其锆石εHf(t)值均较低,分布在-4.4~+5.9之间,长英质麻粒岩原岩主体可能来自~2.7Ga的新生地壳。
6.2 怀安地区2.5Ga的地壳增生与再造近年来,刘富等(2009)和Liu et al.(2012)通过怀安TTG片麻岩和闪长质片麻岩地体的锆石U-Pb年龄、Hf同位素以及全岩Sm-Nd同位素研究认为怀安地区在2.5Ga也发生了重要的地壳增生事件,其TTG片麻岩的εNd(t)值和大部分岩浆锆石的εHf(t)值分别与同期的亏损地幔εNd(t)值和εHf(t)值相近,TTG片麻岩和闪长质片麻岩较年轻的Hf亏损地幔模式年龄(2.44~2.73Ga和2.49~2.75Ga)与锆石U-Pb年龄一致。
2.5Ga的热事件在华北中部的分布十分广泛:怀安TTG片麻岩和闪长质片麻岩原岩形成于2500~2550Ma(Zhao et al., 2006,2008; 刘富等,2009; Wang et al., 2010; Liu et al., 2012; Zhang et al., 2012b),并发现2437~2493Ma的花岗岩(Zhang et al., 2011)及2477Ma的紫苏花岗岩(Santosh et al., 2013);承德地区正片麻岩原岩主要形成于2540~2470Ma(耿元生等,2010);恒山条带状片麻岩、花岗闪长质片麻岩及与深熔有关的花岗质片麻岩都形成于2530~2500Ma期间,一些闪长质片麻岩在2470Ma左右形成(Kröner et al., 2005; Wang,2009; 耿元生等,2010; Diwu et al., 2011);五台地块的灰色花岗岩类主要形成于2570~2510Ma(Liu et al., 2004; Kröner et al., 2005; Wilde et al., 2005; 耿元生等,2010);阜平的TTG系列和花岗质片麻岩主要形成于2540~2500Ma,部分花岗闪长质岩浆活动可以持续到2470Ma(Guan et al., 2002; Zhao et al., 2002; Liu et al., 2004; 耿元生等,2010);中条山奥长花岗质片麻岩和二长花岗质片麻岩形成时间为2560~2470Ma(郭丽爽等,2008; 耿元生等,2010; 张瑞英等,2012);登封地区的岩浆活动主要发生在2530~2500Ma之间,一些奥长花岗质岩形成于2560Ma左右,而闪长岩则形成于2490Ma(耿元生等,2010; Diwu et al., 2011)。
本文所研究麻粒岩记录的2458Ma和2461Ma的岩浆事件与上述事件可能反映了同一期次的地质作用。单斜辉石麻粒岩(DS-5)中岩浆锆石εHf(t)为+2.1~+9.7,分布在亏损地幔演化线和球粒陨石之间,少数高εHf(t)值接近当时的亏损地幔值,其锆石U-Pb年龄与亏损地幔模式年龄相近,显示单斜辉石麻粒岩原岩可能来自亏损地幔的部分熔融,反映怀安地区~2.5Ga重要的地壳增生事件。长英质麻粒岩(XH-1)的锆石εHf(t)值较低,多数在球粒陨石线附近,表明源区物质为古老(≥2.7Ga)的先存地壳,暗示了~2.5Ga怀安地区同时发生了大陆地壳再造。可能亏损地幔部分熔融的物质底侵,为陆壳熔融提供热量,并在一定程度对其进行混染。
对比怀安杂岩体中TTG片麻岩及其以南五台-阜平杂岩体、太华片麻岩地体、中条片麻岩地体、登封杂岩体、嵩山花岗岩等中酸性岩中岩浆锆石的Hf同位素组成(陈斌等,2006; Xia et al., 2006; 第五春荣等, 2007,2010; 郭丽爽等,2008; Wang et al., 2010; 刘富,2010; Diwu et al., 2011; Jiang et al., 2011; Zhang et al., 2011; Zhou et al., 2011; Geng et al., 2012; 李创举等,2012),发现:从εHf(t)与U-Pb年龄关系图解(图 7)中可知怀安地区以~2.5Ga的新生地壳为主,同时存在先存地壳重熔。
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图 7 华北中部带主要杂岩体锆石εHf(t)和年龄关系图 其他数据来源:怀安杂岩体(刘富,2010; Jiang et al., 2011; Zhang et al., 2011; 李创举等,2012); 嵩山花岗岩(Zhou et al., 2011); 登封杂岩(第五春荣等,2007; Diwu et al., 2011); 中条片麻岩(郭丽爽等,2008); 太华片麻岩(第五春荣等,2010; Huang et al., 2010);五台-阜平杂岩体(Xia et al., 2006; 陈斌等,2006; Geng et al., 2012) Fig. 7 Plot of zircon εHf(t)versus age for important complexes in the Trans-North China Craton |
本文所研究的长英质麻粒岩(XH-1)中有4颗谐和的岩浆锆石207Pb/206Pb年龄分别为2114±47Ma、2165±44Ma、2271±43Ma和2316±39Ma,这期热事件在华北中部、孔兹岩带和南缘都有记录,如:中部恒山-五台-阜平等广泛分布2.2~2.0Ga的花岗岩和变火山岩(Du et al., 2013);孔兹岩带变表壳岩系中碎屑锆石普遍记录了2.3~2.0Ga的年龄(董春艳等,2007; Yin et al., 2009);南缘蚌埠地区出露变形花岗岩岩浆结晶年龄为2054Ma(郭素淑和李曙光,2009),豫西也存在2.3Ga的岩浆作用(第五春荣等,2007; 黄道袤等,2012)及2.2~2.0Ga的变表壳岩(第五春荣等,2010)。本文认为2.3~2.1Ga的热事件的研究在怀安地区应进一步受到重视。
单斜辉石麻粒岩(DS-5)的3颗变质锆石分别获得2643±171Ma、2270±172Ma、2029±135Ma,谐和度>92%,在U-Pb谐和图中分别落在不一致线上与谐和线附近,可能是锆石在~1.85Ga麻粒岩相变质(郭敬辉等2001; Guo et al., 2005)发生了Pb丢失造成的。
7 主要认识(1) 单斜辉石麻粒岩原岩形成于~2.5Ga,其锆石高εHf(t)值在亏损地幔线附近,Hf单阶段模式年龄接近形成年龄,指示怀安地区在2.5Ga左右发生了亏损地幔的部分熔融。
(2) 长英质麻粒岩原岩形成于~2.5Ga,其锆石εHf(t)值较低,Hf两阶段模式年龄在2.7~2.8Ga之间,指示怀安地区可能存在≥2.7Ga的古老地壳物质。怀安地区在~2.5Ga发生亏损地幔的部分熔融,为单斜辉石麻粒岩提供原岩物质的同时,可能引起了先存地壳的重熔,即同时存在地壳再造,进一步为长英质麻粒岩提供了原岩物质。
(3) 怀安地区的最古老地壳物质可能可以追溯到3.0Ga,同时可能存在2.3~2.1Ga的热事件。由于数据有限,这些认识尚需进一步研究和积累。
致谢 感谢中国地质大学(武汉)陈明和林向洋在实验分析方面给予的帮助。感谢审稿人刘福来研究员、董春艳博士和刘富博士所提出的宝贵意见。| [] | Chen B, Liu SW, Geng YS, Liu CQ. 2006. Zircon U-Pb ages, Hf isotopes and significance of the Late Archean-Paleoproterozoic granitoids from the Wutai-Lvliang terrain, North China. Acta Petrologica Sinica, 22(2): 296–304. |
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