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1.
《地球化学》2016,(1)
报道了山东昌乐地区新生代王家大山玄武岩的全岩主元素、微量元素,橄榄石斑晶及被其捕获的熔体包裹体主元素和铅同位素组成。王家大山玄武岩为弱碱性-拉斑玄武岩。全岩主元素成分和熔体包裹体的SiO_2、TiO_2、Al_2O_3、CaO、Na_2O、K_2O和P_2O_5含量均与MgO含量呈负相关关系,CaO/Al_2O_3值基本不变;在微量元素原始地幔标准化蛛网图上与EMI洋岛玄武岩(OIB)相似,表现为明显的Ba、K和Sr正异常,Th和Pb负异常,无Nb-Ta和Ti异常。熔体包裹体铅同位素组成为208Pb/206Pb=2.091~2.166和207Pb/206Pb=0.846~0.899,其变化范围覆盖了山东地区新生代强碱性玄武岩到弱碱性-拉斑玄武岩的铅同位素范围;根据铅同位素组成,熔体包裹体可以分为低铅同位素组(207Pb/206Pb0.86)和高Pb同位素组(207Pb/206Pb0.87)。橄榄石斑晶Ni、Fe/Mn和Ca分别为1312~2417μg/g、71~92和745~2068μg/g,与典型辉石岩熔体结晶的橄榄石斑晶成分相当,但是,比橄榄岩熔体结晶的橄榄石成分高Ni和Fe/Mn,低Ca。全岩和熔体包裹体主元素的成分变化,结合岩相学和MELTS软件模拟结果,指示王家大山玄武岩主要经历了橄榄石结晶分离作用。橄榄石斑晶高Ni和Fe/Mn,低Ca,结合全岩高Fe/MnO值和低CaO,说明其源区岩石为辉石岩。全岩微量元素和熔体包裹体铅同位素指示源区有EMI组分,可能和再循环洋壳辉长岩有关。熔体包裹体两组铅同位素组成指示王家大山玄武岩源区是不均一的,暗示山东地区新生代玄武岩的源区是高度不均一的。 相似文献
2.
南海及其周边(包括雷州半岛、海南岛、印支半岛)广泛分布新生代以来形成的板内玄武岩(弥散火成岩省),本文搜集了该区已发表的新生代玄武岩的地球化学数据并据此进行了总结分析。结果显示,该区板内火山岩主要分为拉斑玄武岩和碱性玄武岩两个系列,其微量元素组成为典型的洋岛玄武岩(OIB)特征。Sr-Nd-Pb-Hf同位素结果指示其源区为亏损地幔端元(DMM)与富集端元(EM2)二端元混合。总体上,相对橄榄岩源区形成的熔体而言,这些玄武岩具有低的CaO、较高的Fe/Mn、Zn/Mn及Zn/Fe值;同时,南海海盆玄武岩、海南岛和印支半岛玄武岩中的橄榄石斑晶相对典型地幔橄榄岩部分熔融形成的玄武岩橄榄石斑晶具有低的Ca和Mn含量,以及高的Ni含量和Fe/Mn值,显示其源区辉石岩组分含量较高。南海停止扩张后出现碳酸盐化火山岩并在地球化学上表现为向碱性玄武岩连续转化,同时海南岛和印支半岛的新生代玄武岩整体具有低于亏损橄榄岩地幔的Mg同位素组成,这些都表明南海及周缘地区的地幔源区中有俯冲板块带入的沉积碳酸盐混入。综上认为,该弥散火成岩省在地幔源区组成上均体现有"俯冲-再循环"组分的加入,该再循环地幔组分可能与该地区长期俯冲滞留板块的重熔有关。 相似文献
3.
以短时间内巨量喷发为特征的大火成岩省一般被解释为是地幔柱作用的产物,但是关于小规模大陆溢流玄武岩的源区和形成机制上仍然存在较大的争论。本文选择吉尔吉斯北天山造山带中小规模大陆溢流玄武岩为研究对象,通过~(40)Ar/~(39)Ar同位素定年精确厘定这些玄武岩的形成时代,并利用全岩地球化学以及单矿物成分分析揭示其岩石成因和深部地球动力学过程。吉尔吉斯北天山中Uchkuduk小规模大陆溢流玄武岩的喷发年龄为81.5～84.0 Ma,明显早于吉尔吉斯天山造山带中其它地区玄武岩(58～76 Ma)。其主要斑晶矿物为橄榄石(Fo_(72.5～91.4))、铬尖晶石(Cr#=13.2～50.1,58.0%～76.2%FeO_T和12.5%～20.4%TiO_2)和单斜辉石(Wo_(47.3-51.3)En_(35.5-43.2)Fs_(9.37-14.2))。Uchkuduk玄武岩微量元素特征与OIB极其相似,富集大离子亲石元素和高场强元素,显示Pb、Sr、Nb-Ta的正异常以及K的负异常,并且具有正的ε_(Nd)(t)值(+5.28～+5.42)、适度高的(~(87)Sr/~(86)Sr)i(0.7038～0.7047)和(~(206)Pb/~(204)Pb)i(18.231～18.339),暗示其来源于一个富集的软流圈地幔源区。橄榄石斑晶中高的NiO含量和Fe/Mn比值、低的CaO含量,与典型的来源于辉石岩熔体所结晶的橄榄石特征一致。此外,计算的原始岩浆成分落在L+Ol+Cpx+Grt共结线附近,同时具有高的FeO_T(11.2%～11.7%),TiO_2(2.01%～2.12%)含量,表明Uchkuduk玄武岩来源于石榴石辉石岩为主的地幔源区。该石榴石辉石岩源区可能与早期的地幔交代事件有关,通过俯冲再循环洋壳物质与周围橄榄岩的固相相互作用形成。Uchkuduk玄武岩原始岩浆形成所对应地幔潜能温度1574～1598℃,与地幔柱边部的热异常相当。因此,我们提出吉尔吉斯天山造山带及其邻区的晚白垩世-古新世小规模大陆溢流玄武岩可能是地幔柱活动的产物,地幔柱在上升过程中发生低程度(10%)的部分熔融产生—系列的碱性玄武质岩浆。 相似文献
4.
雷琼地区晚新生代玄武岩地球化学：EM2成分来源及大陆岩石圈地幔的贡献 总被引：1，自引：1，他引：0
对雷琼地区21个晚新生代玄武岩样品的主量、微量元素和Sr、Nd、Pb同位素分别用湿化学法、ICP-MS和MC-ICPMS进行了测定.这些玄武岩主要为石英拉斑玄武岩,其次为橄榄拉斑玄武岩和碱性玄武岩.大多数样品的微量元素和同位素成分与洋岛玄武岩(OIBs)相似,而且随着SiO_2不饱和度增加,不相容元素含量也增加.除R4-1可能受到地壳混染外,其他样品相对均一的Nd同位素(ε_(Nd)=2.5-6.0)以及变化明显但范围有限的Sr同位素(0.703106～0.704481),可能继承了地幔源区的特征.~(87)Sr/~(86)Sr与~(206)Pb/~(204)Pb的正相关和~(143)Nd/~(144)Nd与~(206)Pb/~(204)Pb的负相关特征暗示DM(软流圈地幔)与EM2(岩石圈地幔)的混合.地幔捕虏体的同位素特征暗示EM2成分不可能存在于尖晶石橄榄岩地幔,而La/Yb和Sm/Yb系统表明岩浆由石榴石橄榄岩部分熔融产生,这意味着EM2成分可能存在于石榴石橄榄岩地幔.雷琼地区玄武岩的地球化学变化可以用软流圈地幔为主的熔体加入不同比例石榴石橄榄岩地幔不同程度熔融产生的熔体来解释:碱性玄武岩和橄榄拉斑玄武岩是软流圈熔体与石榴石橄榄岩地幔较低程度(7%～9%)熔融体混合,而石英拉斑玄武岩是软流圈熔体与石榴石橄榄岩地幔较高程度(10%～20%)熔融体的混合. 相似文献
5.
南海北部边缘新生代玄武岩广泛分布，分布于海南岛北部的全新世早期石山组玄武岩，岩石组成为碱性橄榄玄武岩，其中可见较大颗粒的橄榄石斑晶，橄榄石斑晶具有较高的Fo值（82. 8～83. 5）和Ni含量（0. 14%～0. 20%）。橄榄玄武岩的微量元素及同位素组成与洋岛玄武岩（OIB）高度吻合，富集大离子亲石元素Rb、Ba和轻稀土元素，同时富集高场强元素Nb、Ta、Zr和Hf。矿物组成及主微量元素特征指示其源区为含石榴子石辉石岩源区，经历了较低程度的部分熔融（约5%）。此外，石山组橄榄玄武岩具有基本一致的Sr- Nd- Pb同位素组成，表明岩浆在上升过程中没有明显的地壳物质的混染，但是相比正常洋中脊玄武岩（MORB），石山组橄榄玄武岩具有较高的87 Sr/86 Sr比值，较低的ε Nd ( t )值，以及较高的207 Pb/204 Pb（15. 639～15. 643）和208 Pb/204 Pb（38. 977～38. 996）比值，说明其源区为亏损地幔（DM）和富集地幔端元（EMII）的混合。结合地球物理学证据，我们认为亏损地幔来源于软流圈，而EMII端元为含再循环古洋壳及俯冲沉积物的地幔柱，随着海南地幔柱上升，再循环物质熔融并与周围软流圈地幔橄榄岩反应形成含石榴子石辉石岩，随着地幔柱的不断上升，辉石岩首先发生部分熔融，形成的岩浆经历了橄榄石和微弱单斜辉石的分离结晶作用后形成了石山组橄榄玄武岩。华南新生代玄武岩同石山组橄榄玄武岩具有相似的地球化学特征，反映二者具有相同的物质端元组成，但两者岩浆演化上升的动力学机制不同，同时不同端元混合的比例及部分熔融程度也有差异。 相似文献
6.
橄榄石微量元素原位分析的现状及其应用 总被引：4，自引：1，他引：3
随着高精度EMPA和LA-ICP-MS分析技术的发展和矿物微量元素测试精度的提高,利用橄榄石中的微量元素示踪地幔部分熔融、地幔交代作用、岩浆早期结晶过程等地质问题成为近年来一个新兴的研究方向。一系列开拓性的研究发现也被陆续的发表,主要涉及橄榄石中Ni、Co、Al、Cr、Zn、Ti、Li、V、Sc、Mn、Ca和P等元素的示踪使用。一些卓有成效的示踪方法为:Ca、Al、Ti、Ni及Mn能够很好的用于区分橄榄石捕掳晶和斑晶;橄榄石-尖晶石地幔演化趋势线(OSMA:olivine-spinel mantle array)图解可以用于表征岩浆源区的亏损程度;玄武岩中橄榄石斑晶的Li同位素及Li含量可以很有效地指示岩浆源区是否存在地壳物质再循环及地幔交代作用;橄榄石斑晶中Ni、Ca、Mn、Cr和Al协变关系图解可以识别岩浆的辉石岩源区;利用橄榄石捕掳晶中Zr和Sc的含量差异特征可将橄榄岩中三种最主要的类型(尖晶石橄榄岩、石榴石橄榄岩以及尖晶石-石榴石橄榄岩)区分开来;一些元素的比值或组合(例如Ni/Co、Fe/Mn、V/Sc、Zr和Sc、Ca和Ti)可以指示源区交代作用、岩浆作用过程及氧化状态;基于橄榄石中Al、Cr及Ca的地质温度计可以为推算地幔热状态提供新方法;基于橄榄石分离结晶Fo-NiO演化线的原始岩浆计算模型可以较好的推算原始岩浆成分;利用橄榄石的环带及微量元素的扩散机制可以判别更多岩石成因信息,如识别交代介质、熔体类型以及地质构造背景等。基于上述最新研究的相关资料和已有成果,本文对橄榄石微量元素的地球化学示踪方法做系统性的归纳整理,并对橄榄石微量元素赋存状况、橄榄石微量元素测试方法、橄榄石微量元素的使用条件及需注意的问题等进行讨论,为读者在做相关研究时提供参考。 相似文献
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四合屯玄武岩斑晶中单个熔体包裹体元素组成及其对岩浆演化的指示 总被引：7，自引：0，他引：7
玄武岩斑晶中熔体包裹体成分特征可以推断玄武岩源区物质组成,反映岩浆形成演化过程。利用LA—ICPMS对四合屯义县组玄武岩橄榄石、单斜辉石斑晶中单个熔体包裹体的元素组成进行了分析测试。研究结果表明,橄榄石、单斜辉石斑晶中的熔体包裹体在主、微量元素含量上表现出了比全岩更大的变化范围,但微量元素分配特征总体和全岩一致。单斜辉石斑晶中包裹体的CaO含量、CaO／Al2O3比值和Cr2O3含量随着单斜辉石Mg#值的降低而降低,反映了单斜辉石结晶分离的影响,Al2O3与Sr之间的显著相关关系则记录了斜长石结晶分离作用的影响,MgO—Ni和MgO—CaO／Al2O3的变化则反映了橄榄石的分离结晶作用。包裹体元素组成变化总体受橄榄石、单斜辉石和斜长石的结晶分离作用控制。结合前人研究成果,认为四合屯玄武岩在微量元素和同位素组成上的壳源组分特征可能部分地继承自原岩（即橄榄岩＋榴辉岩部分熔融体反应形成的（橄榄）辉石岩）,而不是岩浆上升过程中受地壳岩石混染的结果。高Mg#值单斜辉石斑晶中少量高Mg馆、高Si含量,低CaO、TiO2、Al2O3和微量元素含量的熔体包裹体反映玄武岩浆上升过程中受到了S1质岩石的混染,这与义县组玄武岩下伏地层为长城系大红裕组石英岩、石英砂岩的地质特征一致。因此,高Fo橄榄石斑晶中的熔体包裹体比采用向全岩中简单添加橄榄石方式计算出的原始熔体可能更能真实反映原始熔体组成。 相似文献
8.
为了进一步了解中国东北新生代玄武岩地幔源区的物质属性,报道了大兴安岭哈拉哈河-柴河地区新生代玄武岩的全岩主量、微量元素和Sr、Nd、Pb、Hf同位素组成.哈拉哈河-柴河玄武岩属钠质碱性系列,具有与洋岛玄武岩相似的微量元素特征,如富集大离子亲石元素（LILEs）、明显的Nb、Ta正异常等.它们具有中等亏损的Sr-Nd-Hf同位素组成（87Sr/86Sr=0.703 5~0.703 9、εNd=5.21~6.55、εHf=10.00~11.25）,接近中国东部新生代玄武岩的亏损端元.这些玄武岩具有中等的放射成因Pb同位素组成（206Pb/204Pb=18.37~18.57、207Pb/204Pb=15.52~15.54和208Pb/204Pb=38.24~38.43）,在206Pb/204Pb-207Pb/204Pb相关图上位于4.42~4.45 Ga的地球等时线之间.它们在Sr-Nd-Pb同位素相关图中均落入地幔柱来源的、高3He/4He比（>30Ra）的洋岛玄武岩范围内,暗示其源区可能存在来自深部地幔的古老原始地幔物质.此外,这些玄武岩具有高MgO（8.49%~11.58%）、高Ni（174×10-6~362×10-6）和高Mg#（59.1~66.9）的特征,表明它们接近于原始岩浆的成分.反演的哈拉哈河-柴河玄武岩的原始岩浆组成具有中等的SiO2、低Al2O3以及高CaO/Al2O3比的特征,与石榴子石橄榄岩高压（>2.5 GPa）实验熔体的成分相当,暗示玄武岩的源区岩性最可能为橄榄岩.对以原始地幔（而不是亏损地幔）的微量元素为初始成分的饱满石榴子石二辉橄榄岩进行低程度（1%~2%）部分熔融的模拟计算,产生的熔体与哈拉哈河-柴河玄武岩具有一致的微量元素特征,这进一步支持了上述推断.综上所述,认为大兴安岭地区哈拉哈河-柴河玄武岩的源区含有来自深部地幔的古老的橄榄岩质原始地幔组分. 相似文献
9.
华北克拉通东部岩石圈地幔性质在中—新生代时期发生了重大转变，但细节还不清楚。本文对辽东半岛早白垩世(克拉通破坏峰期)小岭组玄武岩和第四纪(克拉通破坏后)宽甸玄武岩中橄榄石斑晶/捕虏晶进行了主量元素和氧同位素组成研究。早白垩世小岭组玄武岩斑晶橄榄石Fo为 79~88，CaO＞0. 1%，具有高Ni/Mg(0. 4~1. 2)、低Mn/Fe(1. 3~1. 6)和低Ca/Fe比值(0. 2~1. 5)的特征，指示岩浆源区是辉石岩和橄榄岩混合的岩石圈地幔；高于正常地幔橄榄石的δ18O(4. 77‰~5. 96‰，平均值5. 4‰)显示低温热液蚀变洋壳熔体/流体组分对地幔源区的影响。第四纪宽甸玄武岩捕虏晶橄榄石Fo值为88~92(平均值90)，具有高NiO(0. 3%~0. 4%)和低CaO(<0. 1%)、MnO(0. 1%~0. 2%)含量，显示主体饱满、与少量过渡型和难熔型并存的地幔组成特征；其δ18O(4. 58‰~5. 38‰，平均值5. 3‰)与正常地幔值接近。结合华北其他地区地幔橄榄石氧同位素数据，发现早白垩世破坏峰期有较多俯冲洋壳来源的熔/流体交代岩石圈地幔，而新生代岩石圈地幔则为破坏后的残余和新增生产物，我们认为古太平洋板块俯冲和后撤—撕裂引起的熔体/流体交代作用对华北克拉通岩石圈地幔的弱化、侵蚀和最终置换起了重要作用。 相似文献
10.
广西涠洲岛晚新生代玄武岩地幔源区及岩浆成因 总被引：1，自引：0，他引：1
涠洲岛作为我国最年轻的第四纪火山岩岛,其火山活动表现出多期、多旋回和多喷发中心的特征,但其地幔源区特征和岩浆成因依然存在争议。本文对涠洲岛玄武岩开展了详细的矿物学和全岩主、微量元素及Sr-Nd-Pb同位素研究,以揭示其地幔源区特征和岩浆成因。涠洲岛玄武岩主要为碱性玄武岩,在岩浆上升过程,几乎未受到地壳物质的混染,经历了橄榄石和单斜辉石的分离结晶作用。轻稀土(LREE)富集、重稀土(HREE)亏损,轻、重稀土强烈分馏((La/Yb)N=14.42～28.64),Nb、Ta明显正异常,显示出与洋岛玄武岩(OIB)相似的微量元素和Sr-Nd-Pb同位素特征。Sr-Nd-Pb同位素比值变化较均一,且呈现出亏损地幔端元(DM)与富集地幔端元(EM2)的二元混合趋势。其中,EM2端元可能源于海南地幔柱。Sr/Sr*(1.21～2.36)和Eu/Eu*(1.01～1.11)正异常,指示源区存在再循环辉长岩洋壳组分。结合已有的地震层析成像结果和岩石地球化学数据,得出南海及周缘地区的晚新生代玄武岩的形成受控于海南地幔柱。伴随着海南地幔柱的上升,再循环的辉长岩洋壳经部分熔融与地幔橄榄岩反应生成石榴石辉石岩(贫硅辉石岩),石榴石辉石岩和未反应的地幔橄榄岩混合部分熔融形成涠洲岛玄武岩。 相似文献
11.
本研究首次报道了早白垩世济南辉长岩中橄榄石斑晶捕获的熔体包裹体的研究结果。济南辉长岩中橄榄石的Fo(60.3~74.6),Mn(2500~3500μg/g),Ni(70~1349μg/g),Fe/Mn比值(61.2~83.5),与源区母岩为纯的橄榄岩形成的熔体结晶出的橄榄石性质不同,可能与源区存在辉石岩的贡献有关。橄榄石中熔体包裹体主量元素具有较大的变化范围。熔体包裹体成分的标准矿物计算(CIPW)表明,MgO10%的熔体包裹体为含有霞石和橄榄石标准矿物分子的硅不饱和熔体,Mg O10%时为含石英标准矿物分子的硅饱和熔体。橄榄石中包裹有辉石和斜长石,说明岩浆演化过程应该处于开放环境。熔体包裹体的(~208Pb/~206Pb)i和(~207Pb/~206Pb)i与MgO具有良好的负相关关系,与SiO_2具有良好的正相关关系,以及熔体包裹体具有较高的SiO_2特征表明岩浆演化过程中可能有下地壳长英质组分的加入。熔体包裹体的Pb同位素落在EMI附近并向EMII延伸,其源区可能有EMI和EMII的贡献,熔体包裹体的主量元素成分说明其源区母岩可能有橄榄岩和辉石岩的贡献。 相似文献
12.
橄榄石是基性岩浆中最早期结晶的硅酸盐矿物之一,其主量、微量元素特征可以反映出岩浆演化环境、岩浆源区岩性和再循环组分性质等重要信息.本次研究通过对峨眉山大火成岩省平川苦橄岩中橄榄石主量和微量元素分析,以及橄榄石内尖晶石包裹体分析,并与大理苦橄岩中橄榄石和尖晶石成分进行对比,来探讨不同苦橄岩母岩浆氧逸度及源区性质的异同.橄... 相似文献
13.
地壳再循环与大陆碱性玄武岩的成因：以山东新生代碱性玄武岩为例 总被引：6，自引：0，他引：6
大陆碱性玄武岩在地球化学特征上与洋岛玄武岩高度相似,被看做是板内玄武岩在大陆上的典型代表。本文以山东
新生代碱性玄武岩为例,探讨大陆碱性玄武岩的成因。山东新生代碱性玄武岩按时空分布特征可以分为两类：早期定向分
布、相互平行的三个火山群（包括鲁西的潍坊火山群、沂水火山群和胶东的蓬莱火山群）和晚期杂乱分布的孤立小火山。
早期火山群碱性较弱,以碱性橄榄玄武岩和碧玄岩为主,微量元素特征和同位素组成变化大;晚期孤立小火山碱性强,以
碧玄岩和霞石岩为主,微量元素特征和同位素组成较均一。因此,从岩性组成和时空分布特征看,山东的火山群相当于洋
岛/海山的造盾期玄武岩,而孤立小火山接近于洋岛/海山上的复苏期玄武岩。潍坊火山群和沂水火山群在Sr-Nd,Nd-Hf同位
素相关图上都存在从亏损到富集的两端元混合排列趋势,但两者的排列趋势有一点区别。其中同位素富集的端元相对于原
始地幔具有偏低的Ce/Pb比和偏高的Ba/Th比,指示其为大陆下地壳物质。同时,这种富集端元的Th/La比值明显低于大陆下
地壳的平均值,其放射成因Hf相对于放射成因Nd过剩（即Nd-Hf同位素解耦）,说明这种富集端元不是岩浆上升过程中混染
的下地壳物质,而是经历过早期熔融的再循环大陆下地壳（榴辉岩或者石榴辉石岩）。鲁西两个平行火山群在同位素排列上
的区别类似于夏威夷玄武岩中的KEA链和LOA链,因此,山东的平行火山群的深部动力学背景可能是地幔柱,再循环大陆
下地壳物质可能是这种地幔柱的重要组成物质。晚期的孤立小火山在地球化学特征上与火成碳酸岩非常相似,如在原始地
幔标准化图上都具有K,Pb,Zr,Hf,Ti的负异常等特征,因此我们认为其地幔源区为碳酸盐化的橄榄岩。孤立小火山中等亏损
的Sr,Nd,Hf同位素特征支持碳酸岩熔体来自年轻的（中生代？）再循环洋壳。 相似文献
14.
Calc-alkaline olivine andesite and two-pyroxene dacite of theTaos Plateau volcanic field evolved in an open magmatic system.mg-numbers of spatially and temporally associated ServilletaBasalt (54–61) and ohvine andesite (49–59) are comparableand preclude fractional crystallization of ferromagnesian mineralsas the major differentiation process. If Servilleta olivinetholeiite is assumed to be the parental magma type, enrichmentsof highly incompatible trace elements (up to 17 ?) oVer concentrationsin the basalts require that andesitic and dacitic magmas containa substantial proportion of assimilated crust. Isotopic compositionsof andesite and dacite, which have slightly higher 87Sr/86Srratios than the basalts but lower 143Nd/144Nd, 206Pb/204Pb,207Pb/204Pb, and 208Pb/204Pb ratios, are consistent with contaminationof parental basalt by old, low Rb/Sr, low U/Pb, and low Th/Pbcontinental crust. Concentrations of highly incompatible traceelements in andesite and dacite lavas are decoupled from majorelement compositions; the highest concentrat ions of these elementsoccur in andesitic, rather than dacitic compositions, and andesitelavas are more variable in trace element contents. Assimilationof heterogeneous crust concurrent with fractional crystallizationof varying mineral assemblages could cause this decoupled behavior.High mg-numbers in andesite and dacite, skeletal olivine phenocrysts,and reversely zoned pyroxene phenocrysts are manifestationsof mafic replenishment and magma mixing in the Taos Plateaumagmatic system. Taos Plateau volcanoes are monolithologic and are distributedin a semi-concentric zoned pattern that is a reflection of thecomplex subvolcanic magmatic system. A central focus of basaltshields developed above the main basaltic conduit system; thesemagmas contain 10–35% admixed andesitic and dacitic magma.Basalt shields are surrounded by a partial ring of olivine andesiteshield volcanoes, where replenishment of basaltic magma providedthe heat necessary for prolonged assimilation of crust, resultingin intermediate-composition lavas. Dacite shields are locatedaround the periphery of the more mafic volcanoes and reflecta decrease in mafic input on the fringes of the magmatic system. 相似文献
15.
Leonid V. Danyushevsky Michael R. Perfit Stephen M. Eggins Trevor J. Falloon 《Contributions to Mineralogy and Petrology》2003,144(5):619-637
Geochemical data from melt inclusions in olivine phenocrysts in a picritic basalt from the Siqueiros Transform Fault on the northern East Pacific Rise provide insights into the petrogenesis of mid-ocean ridge basalts (MORB). The fresh lava contains ~10% of olivine phenocrysts (Fo89.3-91.2) and rare, small (<1 mm) plagioclase phenocrysts with subhedral to irregular shapes with a range of compositions (An80-90, An57-63). Melt inclusions in olivine phenocrysts are glassy, generally rounded in shape and vary in size from a few to ~200 µm. Although most of the inclusions have compositions that are generally consistent with being representative of parental melts for the pillow-rim glasses, several inclusions are clearly different. One inclusion, which contains a euhedral grain of high-Al, low-Ti spinel, has a composition unlike any melt inclusions previously described from primitive phenocrysts in MORB. It has a very high Al2O3 (~20 wt%), very low TiO2 (~0.04 wt%) and Na2O (~1 wt%) contents, and a very high CaO/Na2O value (~14). The glass inclusion is strongly depleted in all incompatible elements (La =0.052 ppm; Yb =0.34; La/Sm(n) ~0.27), but it has large positive Sr and Eu anomalies (Sr/Sr* ~30; Eu/Eu* ~3) and a negative Zr anomaly. It also has low S (0.015 wt%) and relatively high Cl (180 ppm). We suggest that this unusual composition is a consequence of olivine trapping plagioclase in a hot, strongly plagioclase-undersaturated magma and subsequent reaction between plagioclase and the host olivine producing melt and residual spinel. Two other melt inclusions in a different olivine phenocryst have compositions that are generally intermediate between 'normal' inclusions and the aluminous inclusion, but have even higher CaO and Sr contents. They are also depleted in incompatible elements, but to a lesser degree than the aluminous inclusion, and have smaller Sr and Eu anomalies. Similar inclusions have also been described in high-Fo olivine phenocrysts from Iceland and northern Mid-Atlantic Ridge. We suggest that the compositions of these inclusions represent assimilation of gabbroic material into the hot primitive magma. The localised nature of this assimilation is consistent with it occurring within a crystal mush zone where the porosity is high as primitive magmas pass through earlier formed gabbroic 'cumulates'. In such an environment the contaminants are expected to have quite diverse compositions. Although the interaction of primitive melts with gabbroic material may not affect the compositions of erupted MORB melts on a large scale, this process may be important in some MORB suites and should be accounted for in petrogenetic models. Another important implication is that the observed variability in melt inclusion compositions in primitive MORB phenocrysts need not always to reflect processes occurring in the mantle. In particular, inferences on fractional melting processes based on geochemistry of ultra-depleted melt inclusions may not always be valid. 相似文献
16.
New high-precision minor element analysis of the most magnesian olivine cores (Fo85–88) in fifteen high-MgO (Mg#66–74) alkali basalts or trachybasalts from the Quaternary backarc volcanic province, Payenia, of the Andean Southern Volcanic Zone in Argentina displays a clear north-to-south decrease in Mn/Feol. This is interpreted as the transition from mainly peridotite-derived melts in the north to mainly pyroxenite-derived melts in the south. The peridotite–pyroxenite source variation correlates with a transition of rock compositions from arc-type to OIB-type trace element signatures, where samples from the central part of the province are intermediate. The southernmost rocks have, e.g., relatively low La/Nb, Th/Nb and Th/La ratios as well as high Nb/U, Ce/Pb, Ba/Th and Eu/Eu* = 1.08. The northern samples are characterized by the opposite and have Eu/Eu* down to 0.86. Several incompatible trace element ratios in the rocks correlate with Mn/Feol and also reflect mixing of two geochemically distinct mantle sources. The peridotite melt end-member carries an arc signature that cannot solely be explained by fluid enrichment since these melts have relatively low Eu/Eu*, Ba/Th and high Th/La ratios, which suggest a component of upper continental crust (UCC) in the metasomatizing agent of the northern mantle. However, the addition to the mantle source of crustal materials or varying oxidation state cannot explain the variation in Mn and Mn/Fe of the melts and olivines along Payenia. Instead, the correlation between Mn/Feol and whole-rock (wr) trace element compositions is evidence of two-component mixing of melts derived from peridotite mantle source enriched by slab fluids and UCC melts and a pyroxenite mantle source with an EM1-type trace element signature. Very low Ca/Fe ratios (~1.1) in the olivines of the peridotite melt component and lower calculated partition coefficients for Ca in olivine for these samples are suggested to be caused by higher H2O contents in the magmas derived from subduction zone enriched mantle. Well-correlated Mn/Fe ratios in the wr and primitive olivines demonstrate that the Mn/Fewr of these basalts that only fractionated olivine and chromite reflects the Mn/Fe of the primitive melts and can be used as a proxy for the amount of pyroxenite melt in the magmas. Using Mn/Fewr for a large dataset of primitive Payenia rocks, we show that decreasing Mn/Fewr is correlated with decreasing Mn and increasing Zn/Mn as expected for pyroxenite melts. 相似文献
17.
Based on the investigation of olivine phenocrysts and melt and spinel inclusions in them from the picrites of the Gudchikhinsky Formation and olivine phenocrysts and the whole-rock geochemistry from the Tuklonsky and Nadezhdinsky formations of the Noril’sk region, the compositions and conditions of formation and evolution of the parental melts and mantle sources of Siberian trap magmatism were evaluated. Olivine phenocrysts from the samples studied are enriched in Ni and depleted in Mn compared with olivines equilibrated with the products of peridotite melting, which suggests a considerable role of a nonperidotitic component (olivine-free pyroxenite) in their mantle source. The onset of Siberian trap magmatism (Gudchikhinsky Formation) was related to the melting of pyroxenite produced by the interaction of ancient recycled oceanic crust with mantle peridotite. During the subsequent evolution of the magmatic system (development of the Tuklonsky and Nadezhdinsky formations), the fraction of the pyroxenite component in the source region decreased rapidly (to 40 and 60%, respectively) owing to the entrainment of peridotite material into the melting zone. The formation of magmas was significantly affected by the contamination by continental crustal material. The primitive magmas of the Gudchikhinsky Formation crystallized under near-surface conditions at temperatures of 1250–1170°C and oxygen fugacities 2.5–3.0 orders of magnitude below the Ni-NiO buffer. Simultaneously, the magmas were contaminated by continental silicic rocks and evaporites. The parental magmas of the Gudchikhinsky rocks corresponded to tholeiitic picrites with 11–14 wt % MgO. They were strongly undersaturated in sulfur, contained less than 0.25 wt % water and carbon dioxide, and were chemically similar to the Hawaiian tholeiites. They were produced by melting of a pyroxenite source at depths of 130–180 km in a mantle plume with a potential temperature of 1500–1580°C. The presence of low melting temperature pyroxenite material in the source of Siberian trap magmas promoted the formation of considerable volumes of melt under the thick continental lithosphere, which could trigger its catastrophic collapse. The contribution of pyroxenite-derived melt to the magmas of the Siberian trap province was no less than 40–50%. This component, whose solid residue was free of sulfides and olivine, played a key role in the origin of high contents of Ni, Cu, and Pt-group elements and low sulfur contents in the parental trap magmas and prevented the early dispersion of these elements at the expense of sulfide melt fractionation. The high contents of Cl in the magmas resulted in considerable HCl emission into the atmosphere and could be responsible for the mass extinction at the Paleozoic-Mesozoic boundary. 相似文献
18.
L.-B. Hong Y.-H. Zhang S.-P. Qian J.-Q. Liu Z.-Y. Ren Y.-G. Xu 《Contributions to Mineralogy and Petrology》2013,165(2):305-326
The geochemical characteristics of melt inclusions and their host olivines provide important information on the processes that create magmas and the nature of their mantle and crustal source regions. We report chemical compositions of melt inclusions, their host olivines and bulk rocks of Xindian basalts in Chifeng area, North China Craton. Compositions of both bulk rocks and melt inclusions are tholeiitic. Based on petrographic observations and compositional variation of melt inclusions, the crystallizing sequence of Xindian basalts is as follows: olivine (at MgO > ~5.5 wt%), plagioclase (beginning at MgO = ~5.5 wt%), clinopyroxene and ilmenite (at MgO < 5.0 wt%). High Ni contents and Fe/Mn ratios, and low Ca and Mn contents in olivine phenocrysts, combining with low CaO contents of relatively high MgO melt inclusions (MgO > 6 wt%), indicate that Xindian basalts are possibly derived from a pyroxenite source rather than a peridotite source. In the CS-MS-A diagram, all the high MgO melt inclusions (MgO > 6.0 wt%) project in the field between garnet + clinopyroxene + liquid and garnet + clinopyroxene + orthopyroxene + liquid near 3.0 GPa, further suggesting that residual minerals are mainly garnet and clinopyroxene, with possible presence of orthopyroxene, but without olivine. Modeling calculations using MELTS show that the water content of Xindian basalts is 0.3–0.7 wt% at MgO = 8.13 wt%. Using 20–25 % of partial melting estimated by moderately incompatible element ratios, the water content in the source of Xindian basalts is inferred to be ≥450 ppm, much higher than 6–85 ppm in dry lithospheric mantle. The melting depth is inferred to be ~3.0 GPa, much deeper than that of tholeiitic lavas (<2.0 GPa), assuming a peridotite source with a normal mantle potential temperature. Such melting depth is virtually equal to the thickness of lithosphere beneath Chifeng area (~100 km), suggesting that Xindian basalts are derived from the asthenospheric mantle, if the lithospheric lid effect model is assumed. 相似文献
19.
Amiya K. Samal Srinjoy Datta Jiten Pattnaik Deepak Kumar Rajesh K. Srivastava 《Chemie der Erde / Geochemistry》2022,82(1):125839
The presence of recycled crust in the lithospheric mantle of the Dharwar craton has been investigated using trace element geochemistry of olivine grains from an ENE-trending Paleoproterozoic picrite dyke (associated with the ca. 1.89–1.88 Ga Hampi dyke swarm) emplaced in the western Dharwar craton. Olivine grains are purely magmatic, formed as early phenocrysts in a fractionated basaltic melt. They exhibit enrichment in NiO contents (0.32–0.43 wt%) and depletion in Ca (1366–2105 ppm), Mn (1578–2663 ppm) and 100 1 Mn/Fe (1.28–1.48). Further, the compiled whole-rock geochemical data of the picrite dyke and associated dyke swarm illustrates relatively low CaO/MgO (0.55–1.78), intermediate FeO/MnO (47–54), negative to positive PX# (?0.34 to +1.86), and high values of FC3MS (0.24–0.90) and FCKANTMS (0.19–1.11). These chemical markers are not consistent with the derivation of the primary melt from a pure peridotite or a pyroxenite source; therefore, contribution from a mixed type of source having both peridotite and pyroxenite end members (pyroxene rich and olivine poor lithology) is suggested. The amount of pyroxenite and recycled crust varies from 46% to 86% and 14% to 44%, respectively. The Al-in-olivine based thermometer estimates the maximum crystallization temperature as 1407 °C, which is 137 °C higher than the average temperature of MORB and accordant with several well-established plume-induced large igneous provinces (LIPs) worldwide. Therefore, it is suggested that the studied picrite dyke is derived from a primary melt generated by plume-induced melting of a peridotite-pyroxenite mixed source. The ca. 1.89–1.88 Ga Hampi dyke swarm, being genetically linked with the studied dyke, could also be derived from this same source. Further, the recycled crust in the subcontinental lithospheric mantle of the western Dharwar craton may have generated the pyroxene rich mafic source during the Neoarchean convergence between eastern and western Dharwar craton. 相似文献
20.
Compositional relations among natural glasses in basalts recovered by Legs 45 and 46 (DSDP) provide powerful constraints on their differentiation histories. Residual glass compositions in the moderately evolved aphyric and abundantly phyric basalts within each site demonstrate that none of the units is mutually related to any other or to a common parent by simple fractional crystallization. At Site 396, where clinopyroxene phenocrysts are absent, progressively more evolved liquids (lower Mg/ (Mg+Fe) and higher TiO2) are characterized by lower calcium-aluminum ratios, which can only be generated by clinopyroxene fractionation. This paradox is amplified by some melt inclusions in olivine phenocrysts that have higher CaO/Al2O3 and lower TiO2 than any residual glasses. The occurrences of these distinctive compositions are correlated with the highly magnesian character of the host olivines (Fo90–89), and the melts are interpreted as trapped primitive liquids, parental to the more fractionated derivatives.Melt inclusions intermediate in composition between the residual glasses and the most primitive olivine melt inclusions are present in the cores of some plagioclase phenocrysts that have had a history of resorption. On the basis of a petrographic and microprobe analysis of the zoning relations in these phenocrysts, the inclusions are inferred to be melts entrapped at the time of extensive corrosion of the host crystals.Interpreted in conjunction with other mineral and geochemical data, the compositional trends in the glasses indicate that magma mixing has played a major role in the genesis of the Leg 45 and 46 basalts. The reality of mixing is demonstrated by extensive disequilibrium textures in the plagioclase phenocrysts and the presence in evolved lavas of refractory plagioclase and olivine phenocrysts bearing primitive melt inclusions. The chemical imprint of clinopyroxene fractionation despite the absence of clinopyroxene phenocrysts is believed to be accomplished by plating of gabbro on to the upper walls of the subvolcanic magma chamber as it evolves between mixing events. Repeated influxes of primitive magma batches will move the resultant hybrids alway from clinopyroxene saturation and generate olivine-plagioclase cotectic magmas. This model provides a physical buffering mechanism that accounts for the volumetric dominance of moderately evolved basalts among ocean floor tholeiites. Major and trace element models based on the combination of mixing and fractional crystallization also explain heretofore enigmatic geochemical characteristics of MORB.Lunar and Planetary Institute Contribution no. 326After August 1, 1978: Department of Geological Sciences, Southern Methodist University, Dallas, TX 75275, USAThe Lunar and Planetary Institute is operated by the Universities Space Research Association under Contract No. NSR 09-051-001 with the National Aeronautics and Space Administration 相似文献