Redox evolution of western Tianshan subduction zone and its effect on deep carbon cycle     

《地学前缘(英文版)》2020,11(3):915-924

Knowing the phase relations of carbon-bearing phases at high-pressure(HP) and high-temperature(HT) condition is essential for understanding the deep carbon cycle in the subduction zones.In particular,the phase relation of carbon-bearing phases is also strongly influenced by redox condition of subduction zones,which is poorly explored.Here we summarized the phase relations of carbon-bearing phases(calcite,aragonite,dolomite,magnesite,graphite,hydrocarbon) in HP metamorphic rocks(marble,metapelite,eclogite) from the Western Tianshan subduction zone and high-pressure experiments.During prograde progress of subduction,carbonates in altered oceanic crust change from Ca-carbonate(calcite) to Ca,Mg-carbonate(dolomite),then finally to Mgcarbonate(magnesite) via Mg-Ca cation exchange reaction between silicate and carbonate,while calcite in sedimentary calcareous ooze on oceanic crust directly transfers to high-pressure aragonite in marble or amorphous CaCO3 in subduction zones.Redox evolution also plays a significant effect on the carbon speciation in the Western Tianshan subduction zone.The prograde oxygen fugacity of the Western Tianshan subduction zone was constrained by mineral assemblage of garnet-omphacite from FMQ-1.9 to FMQ-2.5 at its metamorphic peak(maximum P-T) conditions.In comparison with redox conditions of other subduction zones,Western Tianshan has the lowest oxygen fugacity.Graphite and light hydrocarbon inclusions were ubiqutously identified in Western Tianshan HP metamorphic rocks and speculated to be formed from reduction of Fe-carbonate at low redox condition,which is also confirmed by high-pressure experimental simulation.Based on petrological observation and high-pressure simulation,a polarized redox model of reducing slab but oxidizing mantle wedge in subduction zone is proposed,and its effect on deep carbon cycle in subduction zones is further discussed.  相似文献   

贵州夜郎湖表层水体地球化学昼夜变化及其影响因素     

王家录  任娟  王勇  李维杰  娄昭  陈佳 《热带地理》2020,40(2):335-345

为探究岩溶水库水文地球化学行为过程,对贵州普定夜郎湖表层水体进行了为期3 d的高分辨率昼夜监测。结果表明：1）多变的天气和水文条件叠加导致水体离子指标昼夜变化不显著,规律性较差。而水温、DO、pH值、SpC、SIc、pCO₂等常规理化指标受水温变化和生物作用表现出明显的昼夜波动。2）利用亨利常数和主成分分析,得到温度变化、生物作用、人类活动、水库的蓄水与放水对夜郎湖水库水文地球化学特征变化的贡献率分别为21.66%、17.28%、14.08%和10.22%,说明作用于水库水文地球化学行为的因子具有多元性。3）δ ¹⁸O表现出与DO一致的波动趋势,即白天上升,晚上下降,反映在短时间尺度上,氢氧稳定同位素变化受控于生物过程（主要是呼吸作用过程）;而对比水库水体和大气降水的d-excess（d值）发现,水库水体的d值（8.21‰）显著偏低于当地大气降水的d值（9.64‰）,说明在长时间尺度上,主要受蒸发效应引起的不平衡分馏影响。  相似文献   

西秦岭太阳山斑岩铜-钼矿床岩体氧逸度及成矿意义     

勾宗洋  于皓丞  邱昆峰  吴鸣谦  周春生  朱锐  李俊  温依瞳 《地学前缘》2019,26(5):243-254

甘肃天水三叠纪太阳山斑岩铜钼矿床位于西秦岭造山带东段。矿体主要赋存于石英闪长斑岩、二长斑岩、石英二长斑岩和泥盆系大草滩群。氧逸度是表征岩石物理化学性质的重要参数，对岩浆热液成矿具有明显的控制作用。在综合评述常用氧逸度计算方法及适用性的前提下，文中应用激光剥蚀等离子质谱分析方法对太阳山矿床含矿岩体锆石微量元素进行测定，选用含量较高的Sm、Nd进行Ce异常计算，查明含矿斑岩岩浆氧逸度，探讨其成矿意义。太阳山矿床岩浆氧逸度计算结果表明，太阳山成矿二长斑岩和石英二长斑岩相对氧逸度ΔFMQ分别为+3.04和+3.15，成矿前石英闪长斑岩相对氧逸度ΔFMQ为-1.83，成矿岩体氧逸度明显高于成矿前岩体。成矿岩体岩浆氧逸度高于成矿前岩体的原因可能与富集地幔有关。富集岩石圈地幔的加入，带来了大量的硫和金属铜，并提高了岩浆氧逸度。  相似文献   

西藏雄村斑岩型铜(金)矿床Ⅰ、Ⅱ号矿体热液黑云母特征及地质意义     

肖鸿天  谢富伟  郎兴海  冉凤琴 《岩石矿物学杂志》2020,39(4):469-480

雄村铜(金)矿区位于西藏冈底斯成矿带中段南缘,由Ⅰ、Ⅱ、Ⅲ号矿体和多个矿化体组成。本文以Ⅰ、Ⅱ号矿体钾硅酸盐化蚀变带内的热液黑云母为研究对象,采用光薄片镜下鉴定、电子探针等分析方法,系统研究了热液黑云母的产状和成分特征。结果显示,雄村矿区Ⅰ号矿体黑云母类型主要为金云母和镁质黑云母;Ⅱ号矿体黑云母类型为镁质黑云母。两个矿体黑云母都具有低Ti(TiO_2 3%)、高Al(Al_2O_315%)的特点,且具有较高的MgO含量,Mg/Fe0.5,K/Na10,显示了与矿化良好的相关性。Ⅰ号矿体热液黑云母平均结晶温度470℃,氧逸度位于镍-氧化镍缓冲剂与磁铁矿-钛铁矿缓冲剂之间(NNO—HM);Ⅱ号矿体热液黑云母平均结晶温度234℃,氧逸度位于镍-氧化镍缓冲剂与铁橄榄石-石英-磁铁矿缓冲剂之间(NNO—FQM),说明Ⅰ号矿体形成于较高温、高氧逸度的热液系统,Ⅱ号矿体形成于相对较低温、低氧逸度的热液系统。此外,Ⅰ号矿体热液黑云母Ⅳ(F)值介于0.61～2.72之间,平均值1.26,Ⅳ(Cl)值介于-5.49～-4.53之间,平均值-5.03,Ⅳ(F/Cl)值介于5.63～7.89之间,平均值6.29;Ⅱ号矿体热液黑云母Ⅳ(F)值介于1.83～3.32之间,平均值2.66,Ⅳ(Cl)值介于-5.64～-4.89之间,平均值-5.31,Ⅳ(F/Cl)值介于7.14～8.68之间,平均值7.97,说明Ⅰ、Ⅱ号矿体都形成于富Cl的热液系统,且Ⅱ号矿体热液较Ⅰ号矿体更富Cl,贫F。富Cl流体易萃取流体中的Cu和Au等金属元素并以Cl的络合物形式运移,在沿构造裂隙向上运移的过程中,物理化学条件发生改变,使得流体中金属元素络合物溶解度降低,促使硫化物沉淀成矿。  相似文献   

Kainsaz(CO3)陨石中两个富Al球粒的氧同位素组成特征与形成演化     

戴德求  包海梅  刘爽  尹锋 《岩石学报》2020,36(6):1850-1856

富Al球粒是原始球粒陨石中一种矿物岩石学特征介于富钙铝包体(CAIs)和镁铁质硅酸盐球粒之间的特殊集合体,所以常常认为富Al球粒在认识CAIs和镁铁质硅酸盐球粒形成演化过程中的相互联系具有特殊意义。然而,对富Al球粒的初始物质组成以及形成演化过程一直存在较多争议,而氧同位素组成研究能够对球粒演化和早期星云环境等提供重要的信息。在本文中我们报导了来自Kainsaz(1937年降落于俄罗斯,CO3型)碳质球粒陨石中的2个富Al球粒(编号K1-CH1和K2-CH2)的矿物岩石学和氧同位素组成特征。K1-CH1的矿物组成主要为橄榄石、低钙辉石和富钙长石,K2-CH2为橄榄石和富钙长石。2个球粒中的矿物均具有贫~(16)O同位素组成特征。K1-CH1中矿物的△~(17)O组成基本上位于2个区间:-11.1‰～-8.7‰和-3.9‰～0.4‰;而K2-CH2的△~(17)O介于-6.6‰～-0.6‰之间,且具有从中部至边部升高的趋势。矿物岩石学和氧同位素特征表明,这2个富Al球粒的初始物质组成为富CAIs和镁铁质硅酸盐。在球粒熔融结晶过程中,与贫~(16)O同位素组成(△~(17)O:-8.7‰～-7.8‰)的星云发生了氧同位素交换。球粒形成后,发生迁移进入陨石母体,在相对更贫~(16)O同位素组成(△~(17)O:-0.6‰～0.4‰)的母体中(流体参与)发生变质作用,并再次发生了氧同位素交换。  相似文献   

邯邢地区中生代侵入岩中磷灰石的成因矿物学研究     

梁贤 《地质与勘探》2020,56(5):969-984

氧逸度为有效的氧分压，是实验岩石学中重要的研究课题，岩浆的氧逸度是继温度、压力、浓度等影响成岩成矿过程的关键性物理化学参数。本文利用磷灰石的氧逸度计，对邯邢地区六大主要岩体的岩浆氧逸度进行了计算。研究结果显示，样品中的磷灰石主要为羟-氟磷灰石，磷灰石的形态、成分和结构特征指示其为岩浆成因。磷灰石中的Mn元素在晶格中有两种方式，多以Mn3＋和Mn5＋的方式进入晶格。磷灰石氧逸度计计算的logfo2为-12.31~-9.75，均值-11.02。参考与磷灰石共生角闪石的形成温度，认为邯邢地区岩浆岩普遍具有较高的氧逸度。根据磷灰石氧逸度值与矿床规模的填图结果，认为并非氧逸度越高越有利于邯邢式铁矿的形成。结合矿物学填图等值线闭合的趋势，进而推断邯邢地区中部的符山和武安岩体深部可能仍存在较好的找矿远景。  相似文献   

Heating duration of igneous rim formation on a chondrule in the Northwest Africa 3118 CV3oxA carbonaceous chondrite inferred from micro-scale migration of the oxygen isotopes     

《Chemie der Erde / Geochemistry》2019,79(4):125524

Due to their common occurrence in various types of chondrites, igneous rims formed on pre-existing chondrules throughout chondrule-forming regions of the solar nebula. Although the peak temperatures are thought to reach similar values to those achieved during chondrule formation events, the heating duration in chondrule rim formation has not been well defined. We determined the two-dimensional chemical and oxygen isotopic distributions in an igneous rim of a chondrule within the Northwest Africa 3118 CV3_oxA chondrite with sub-micrometer resolution using secondary ion mass spectrometry and scanning electron microscopy. The igneous rim experienced aqueous alteration on the CV parent body. The aqueous alteration resulted in precipitation of the secondary FeO-rich olivine (Fa_40–49) and slightly disturbed the Fe-Mg distribution in the MgO-rich olivine phenocrysts (Fa_11–22) at about a 1 μm scale. However, no oxygen isotopic disturbances were observed at a scale greater than 100 nm. The MgO-rich olivine, a primary phase of igneous rim formation, has δ¹⁷O = −6 ± 3‰ and δ¹⁸O = −1 ± 4‰, and some grains contain extreme ¹⁶O-rich areas (δ¹⁷O, δ¹⁸O = ∼−30‰) nearly 10 μm across. We detected oxygen isotopic migration of approximately 1 μm at the boundaries of the extreme ¹⁶O-rich areas. Using oxygen self-diffusivity in olivine, the heating time of the igneous rim formation could have continued from several hours to several days at near liquidus temperatures (∼2000 K) in the solar nebula suggesting that the rim formed by a similar flash heating event that formed the chondrules.  相似文献   

滇西姚安金矿床磷灰石化学特征及指示意义     

郑瑜林  张长青  刘欢  孙嘉  张盼盼 《矿床地质》2021,40(1):156-168

姚安金矿床位于金沙江-哀牢山富碱斑岩带中段,大地构造位置处于扬子板块西缘与三江特提斯造山带结合部位,其成矿与新生代富碱岩浆-岩浆热液密切相关。野外调查发现矿化仅存在于黑云母正长斑岩体内,而与黑云母正长斑岩空间关系密切的石英正长斑岩却未发现矿化。为探讨黑云母正长斑岩与石英正长斑岩岩体含矿性差异,运用电子探针、LA-ICP-MS分析方法,以富矿黑云母正长斑岩和贫矿石英正长斑岩岩体内的磷灰石作为研究对象,对比磷灰石之间的差异,探讨磷灰石记录的岩浆演化以及反映岩浆氧化还原条件和流体活动性相关信息。测试结果表明,姚安矿区富矿岩体与贫矿岩体磷灰石均为岩浆磷灰石且富F、低Cl;富矿岩体磷灰石相比于贫矿岩体磷灰石具有较大的δEu变化范围与较低的δCe,指示富矿岩体具有较高的氧逸度,高的氧逸度会抑制金以硫化物形式沉淀,从而增强了岩体的成矿潜力。富矿岩体磷灰石具有较高的Ce/Pb比值与低的Th/U比值,表明岩浆形成过程中成矿岩体流体活动性较强,岩浆分异较强。富矿岩体角闪石和黑云母的发育表明岩浆具有较高的水含量,高水含量可以增加金属元素在熔体中的溶解度,并且高水含量的岩浆在演化过程中水也较易达到饱和,发生对成矿有重要意义的流体出溶。总之,在姚安地区,高氧逸度,高水含量以及强流体活动性是成矿的关键。  相似文献   

班公湖-怒江缝合带东段丁青地幔橄榄岩成因:来自钻孔ZK02地幔橄榄岩矿物学及地球化学特征约束     

徐向珍  熊发挥  张承杰  陈建  张然  闫金禹  杨经绥 《岩石学报》2021,37(10):2944-2970

丁青蛇绿岩位于班公湖-怒江缝合带东段,是该缝合带出露面积最大的蛇绿岩。为查明岩体成因,在丁青东岩体中实施了一口165.19m的钻孔。除最顶部有约0.5m厚的第四系残坡积物外,其余均为地幔橄榄岩。结合显微镜鉴定将岩心划分出17个岩性单元层,岩性主要以方辉橄榄岩为主,夹少量纯橄岩和含铬铁矿纯橄岩。地幔橄榄岩中橄榄石的Fo变化于88.79~93.73,铬尖晶石的Cr^#变化于44.33~81.66,揭示丁青地幔橄榄岩可能经历过约20%~40%的中高度部分熔融作用;全岩地球化学分析表明其具有富镁（MgO=45.98%~49.45%）、贫铝（Al₂O₃=0.19%~1.37%）和贫钙（CaO=0.28%~0.70%）的特点,属于熔融程度较高的地幔残余物质。岩石具有明显不同于阿尔卑斯蛇绿岩的轻稀土元素富集特征,指示区内地幔橄榄岩先经历了较强程度的部分熔融,后经历了俯冲消减过程中的流体交代。利用地幔橄榄岩中的铬尖晶石成分计算母熔体Al₂O₃含量对应的FeO/MgO值,与不同构造环境原始岩浆成分相比较,发现丁青地幔橄榄岩母熔体大多处于玻安岩中。纯橄岩氧逸度估算FMQ=-3.05~-0.71,方辉橄榄岩氧逸度FMQ=-3.89~+1.47,显示丁青地幔橄榄岩有俯冲作用的参与。通过丁青钻孔岩心的研究,提出丁青东岩体可能形成于俯冲带之上的弧前环境这一观点。  相似文献   

Composition and origin of the volatile components released from the Pesyanoe aubrite by stepwise crushing and heating     

《Chemie der Erde / Geochemistry》2021,81(1):125686

Aubrites are achondritic meteorites (enstatite pyroxenites) that were formed in highly reduced magmatic environments on a differentiated parent body sharing a common oxygen isotope reservoir with enstatite chondrites (EC), Earth and Moon, and could be considered as a geochemical model of the early proto-Earth. Some pyroxenes of the Pesyanoe aubrite have high abundance of gaseous inclusions, captured during the crystallization of the rocks. Investigation of the inclusions by IR spectroscopy reveals presence of OH⁻ groups and C–H bonds. The former are assigned to protonated point defects in enstatite lattice and the latter to compounds occupying void walls. Molecular water and CO₂ were not observed. Volatile components released from the samples of the Pesyanoe enstatite by stepwise crushing and heating are composed of CO₂, H₂O and a non-condensable phase. Hydrogen isotopic composition of volatiles extracted in form of molecular water in Px-separates varies in the range δD = −61 – −84‰ with mean value of δD = −73 ± 16‰ VSMOW and is within the ranges of ECs and Earth’s mantle. The total abundance of H₂ in the pyroxene of Pesyanoe were estimated as at least 0.047 ppm that is too low in comparison with that of enstatite chondrites (≥30 ppm H₂) and could indicate nearly complete degassing of the Pesyanoe primitive precursor material during the Pesyanoe parent body accretion or a mantle degassing in igneous differentiation process. In a last case a primitive precursor could have D/H ratio different from that of enstatite chondrites.  相似文献