镁铁-超镁铁岩铼-锇同位素体系分析方法

通过试验建立了镁铁-超镁铁岩Re-Os同位素体系分析方法，包括Re-Os的化学分离纯化流程，Re同位素比值的电感耦合等离子体质谱测量方法和Os同位素比值的负离子热电离质谱测量方法。化学流程包括Carius管溶样，小型蒸馏分离Os，微蒸馏纯化Os，阴离子交换法分离、纯化Re。用该流程测定了汉诺坝幔源橄榄岩、辉石岩捕虏体和大别山饶拔寨超镁铁岩样品的Re、Os含量和Os同位素比值。     

松树沟超镁铁岩主量元素及Os同位素初步研究

本文利用 N-TIMS 方法测定了松树沟超镁铁岩的Os同位素组成，初步获得的Os同位素组成数据显示：残余型超镁铁岩的Os同位素比值明显低于岩浆型，表明松树沟岩体在岩浆演化过程中发生了 Re/Os分异；187Os/188Os与Al2O3、Al2O3/MgO正相关，与MgO负相关，表明在岩浆演化过程中，微量的 Re、Os元素分别与主要元素 Al2O3和MgO的性质相似。     

云南潞西三台山超镁铁岩体Os-Nd-Pb-Sr同位素特征及地质意义

滇西地区特提斯造山带具有多块体拼合的构造特点,是东特提斯造山带的重要组成部分之一,其大地构造演化对理解全球特提斯造山带具有重要的地质意义.在腾冲和保山地块之间的龙陵-瑞丽断裂带中出露超镁铁质岩石,曾被解释为两个陆块缝合的证据.本文采用高灵敏度高精度超低本底Re-Os、Sm-Nd、Pb和Rb-Sr同位素分析技术,对采自该断裂带潞西三台山的超镁铁岩样品进行了Os-Nd-Pb-Sr同位素测定.分析结果表明,这些超镁铁岩石具有强烈富集特征.分析的5个岩石样品具有高的初始~(87)Sr/~(86)Sr值(0.71074～0.71444)、低的初始ε_(Nd)值(-6.2～-10.6)、低初始γ_(Os)值(-4.8～-8.8)和较高的初始铅同位素比值,其Os同位素模式年龄值(t_(RD))为0.97～1.71Ga.Nd-Os同位素组成特征表明,三台山超镁铁岩具有古老的富集大陆岩石圈地幔岩石的特征,不能作为腾冲和保山地块的缝合证据.     

微量地质样品铼锇含量及其同位素组成的高精度测定方法

报道了采用新型IsoProbe—T热电离质谱计测定Os含量及其同位素组成和Neptune多接收器等离子体质谱仪（MC—ICPMS）测定Re含量的分析方法。样品化学处理采用Carius管溶样、小型蒸馏法分离和微蒸馏法纯化提取Os以及阴离子树脂交换分离Re的方法。采用IsoProbe—T质谱计测定Os同位素组成具有灵敏度高和精度高的特点。对溶液标样，采用多法拉第接收器系统测定Os总量低至0．2ng的样品时，平均^192Os^16O3-离子流强度可达100mV以上并可维持约20min，其^187Os／^188Os同位素比值的测定精度可优于0．1％（1RSD）。采用所建立的化学分离流程和高精度质谱测量方法，测定了铂族元素橄榄岩标样WPR-1中Re、Os含量和Os同位素组成，测定结果与文献报道值在误差范围内吻合。     

西藏日喀则蛇绿岩镁铁质岩石Re-Os同位素特征及意义

通过对日喀则蛇绿岩的镁铁质岩石进行岩石学和地球化学研究,探讨其岩石成因及源区性质,同时根据Re-Os同位素的地球化学约束来探索雅鲁藏布蛇绿岩的形成机制。研究表明,日喀则蛇绿岩镁铁质岩石微量元素的标准化配分型式与洋中脊玄武岩类似,又具有岛弧玄武岩的地球化学特征。结合微量元素和同位素特征,均表明岩石的形成与俯冲作用有关。日喀则蛇绿岩产出于远离大陆地壳的SSZ环境,其形成过程未受到陆壳的混染;同时,Re-Os同位素体系受蚀变作用的影响也不明显。日喀则蛇绿岩镁铁质岩石的Re、Os含量低,¹⁸⁷Os/¹⁸⁸Os同位素比值较高,主要是源区性质和俯冲作用影响的结果。特提斯洋早期发生的多次俯冲作用造成地幔源区不均一。新特提斯洋壳俯冲过程中,上述不均一地幔发生部分熔融产生的镁铁质岩浆上升,经过遭受了早期熔体/岩石作用的纯橄岩通道,发生强烈的Re-Os同位素分馏,使熔体与地幔残余Os同位素组成表现出明显的解耦现象,进而形成现今的日喀则蛇绿岩。     

新疆黄山镁铁-超镁铁岩带锆石Hf同位素特征及源区性质探讨

黄山东、香山及土墩岩体均为多阶段侵入的杂岩体,岩体与围岩为侵入接触关系,显示热侵位特征。岩石组成单元主要为超镁铁质橄榄岩和镁铁质辉长岩。岩石化学组成以拉斑玄武岩系列为主,存在部分钙碱性系列和碱性系列。稀土元素具平坦的分配型式或轻稀土略富集的分配型式。锆石Hf同位素指示岩石来源于亏损型地幔源区。黄山东、香山及土墩镁铁-超镁铁岩不是俯冲洋壳的残余或者岛弧环境的阿拉斯加型岩体,而是来源于亏损型地幔源区的岩浆底侵形成。     

新疆北部镁铁-超镁铁质岩的PGE成矿问题

铂族元素(PGE)矿化主要与镁铁-超镁铁杂岩有关,成矿类型主要为岩浆型矿床,这类PGE矿床的形成主要依赖两个条件:一是岩浆中富含PGE;二是具备PGE从岩浆中分离和富集的机制,主要是在岩浆演化过程中硫达到饱和。新疆北部镁铁-超镁铁质杂岩发育,并产有喀拉通克、黄山、黄山东、图拉尔根4个大型铜镍矿床和香山、土墩、葫芦、白石泉等中、小型铜镍矿,以及香山西、尾亚等中型钒钛磁铁矿矿床,但迄今尚未发现成型的PGE矿床。文中通过对PGE矿床的形成机制与镁铁-超镁铁杂岩源区特征研究,探讨了北疆地区PGE矿床的成矿问题。综合分析认为,新疆北部后碰撞镁铁-超镁铁质岩的岩石类型为经过了分离结晶形成的铁质岩石系列,是PGE矿床的有利容矿岩石;矿床的Sr、Nd、Pb、O、Os和S同位素和含矿岩石地球化学特征表明,铜镍硫化物矿床含矿岩浆在岩浆演化和成矿过程中有地壳物质加入并可导致硫化物熔离作用,说明在成矿机制上也存在形成岩浆型PGE矿化的条件。新疆北部PGE矿化微弱的原因可能在于该区广泛发育的亏损型地幔源(具正的εNd值特征),这一亏损型地幔可能部分源于洋壳熔融,与产于后碰撞造山带环境、发育于"洋壳"或"不成熟"陆壳基底之上有关,由此决定了原始岩浆为贫PGE的源区,因此不利于PGE的富集成矿。     

龙首山岩带典型镁铁-超镁铁质岩体岩石地球化学特征

通过龙首山岩带中几个典型镁铁-超镁铁质岩体样品的岩石地球化学分析,对金川超镁铁质岩体与其外围镁铁-超镁铁质岩体的形成演化关系进行探讨,结果发现:这些岩体处于相同的构造环境,样品点整体为亚碱性拉斑玄武岩系列,随M g#值的增加,C aO,A l2O3,N a2O,K2O值具有连续减少的趋势,指示了它们存在连续的岩浆演化关系;稀土与微量元素分析,蛛网图整体具有右倾特征,龙首山岩带中段岩体有明显δEu负异常,东、西段岩体样品有δEu正异常或无异常,暗示中段岩体较外围岩体经历了更完全的分离结晶作用;结合前人对金川所做的S r-N d同位素等资料,证明金川岩体的岩浆源区为富集型地幔。     

胶东变质超镁铁—镁铁质岩石的地球化学特征及地幔源区性质

本文以地球化学方法为研究手段,结合野外宏观地质特征,论述了胶东地区前寒武纪变质建造中超镁铁—镁铁质岩石的地球化学性质及其成因。研究结果表明,该区超镁铁—镁铁质岩石为地幔不同程度熔融的产物,超镁铁质岩石相当于科马提岩类;镁铁质岩石为拉斑玄武岩类,并按橄榄质科马提岩→玄武质科马提岩→拉斑玄武岩演化系列的化学组成表现出连续的变化趋势。 拉斑玄武岩中的微量元素(主要是稀土元素)地球化学特征表明,其形成环境与现代板块构造的典型火山(岛)孤或孤后盆地环境相类似,并反映出地幔源区具有“富集型”地幔的特点,且存在着地幔不均一性。     

内蒙古乌拉特中旗克布镁铁质-超镁铁质岩体年代学、矿物学和岩石地球化学

内蒙古乌拉特中旗地处华北陆块北缘西段,大地构造分区属于狼山-白云鄂博陆缘裂谷。区域上,镁铁质-超镁铁质岩呈东西向带状分布,断续出露长约300km,宽约30km。该镁铁质-超镁铁质岩带内铜镍矿床(点)较为发育,克布为该带内一个中-小型铜镍硫化物矿床。克布镁铁质-超镁铁岩体出露面积约45km2,主要由辉长岩相和橄榄岩相组成,辉长岩相为岩体的主要岩相,橄榄岩相为主要的赋矿岩石,两个相带相伴产出,呈渐变过渡关系。本文采用LA-ICP-MS锆石U-Pb法测年,获得克布斜长方辉橄榄岩年龄为258.1±1.8Ma(MSWD=2.3),属于晚二叠世。岩石主、微量及稀土元素分析结果表明,岩石样品属铁质镁铁质-超镁铁质岩,具有拉斑玄武岩系列演化趋势,并相对富集大离子亲石元素(Rb、Sr、Ba),亏损高场强元素(Nb、Ta、Zr、Hf、Ti),以及具有轻稀土富集[(La/Yb)N=2.47~11.29]的右倾型稀土配分模式。以橄榄石-熔体平衡原理估算克布镁铁质-超镁铁质岩体母岩浆的MgO含量为10.1%,FeO为12.1%,应为高镁的拉斑玄武质岩浆。综合分析认为,克布镁铁质-超镁铁质岩体应形成于后碰撞伸展阶段,岩浆源区由被消减板片交代的地幔楔物质和软流圈物质组成。橄榄石和辉石等富镁铁矿物的分离结晶和富硅地壳物质的混染可能对硫化物熔离富集成矿起到了关键性作用。     

利用同一化学流程分析地质样品中的铂族元素含量和铼-锇同位素组成

报道了利用一次溶样和同一化学流程分离富集地质样品中铂族元素(Pt、Pd、Os、Ir和Ru)和Re的方法.该化学流程包括以下几个步骤:(1) Carius管溶样法分解岩石样品中富集铂族元素的矿物;(2)四氯化碳萃取法分离出Os;(3)微蒸馏法进一步纯化Os;(4)阳离子交换树脂法将铂族元素(Pt、Pd、Ir和Ru)以及R...     

In situ measurement of Re-Os isotopes in mantle sulfides by laser ablation multicollector-inductively coupled plasma mass spectrometry: analytical methods and preliminary results

A method has been developed for the in situ determination of Re-Os isotopes in single grains of sulfides in mantle-derived peridotites using a laser ablation microprobe attached to a multicollector-induced coupled plasma mass spectrometer (MC-ICPMS). High-precision Os isotope analysis by MC-ICPMS is demonstrated by the measurement of interlaboratory Os standards. Evaluation of mass bias correction procedures shows that the exponential law provides the best fit to the Os isotope data and that the ratio of the mass fractionation coefficients for Re and Os remains constant for the range of typical instrument operating conditions. This relationship enables the accurate and precise correction of the isobaric interference of ¹⁸⁷Re on ¹⁸⁷Os for ¹⁸⁷Re/¹⁸⁸Os values up to 1.6.Results are presented for single sulfide inclusions in olivine macrocryts from kimberlites in the Siberian and Slave Cratons, and sulfides enclosed in silicates and interstitial to silicates in peridotite xenoliths from the Slave Craton and Massif Central, France. Enclosed sulfides larger than 50 μm in diameter and with Os contents ≥40 ppm give ¹⁸⁷Os/¹⁸⁸Os ratios with a precision of 0.1% (2 SE), which is equivalent to N-TIMS whole-rock data. Interstitial sulfides typically have lower Os (10 to 30 ppm) and give analyses with lower precision (∼1 to 2%) but still provide valuable information on the movement of Os within the lithosphere. The sulfide inclusions in silicates preserve significantly less radiogenic Os isotopic compositions than interstitial sulfides and accordingly produce significantly older and more realistic Re-Os age information. Whole-rock Os isotope compositions reflect the proportions of different generations of enclosed and interstitial sulfides; this calls into question the significance of many published “depletion ages.”     

Platinum-group element geochemistry of peridotite xenoliths from the Sierra Nevada and the Basin and Range, California

The nature of PGE-Re (PGE = Pt, Pd, Os, Ir, Ru) behavior in subcontinental lithospheric mantle was investigated using new, high precision PGE-Re abundance measurements and previously published Re-Os isotopic analyses of peridotite xenoliths from the Sierra Nevada and Mojave Province, California. Ru/Ir ratios and Ir concentrations are constant over a wide range in S content and major-element fertility indices (e.g., Mg/(Mg+Fe)), indicating that Ru and Ir are not only compatible during partial melting, but also that their partitioning behaviors may not be controlled entirely by sulfide. Pt/Ir, Pd/Ir, Os/Ir, and Re/Ir ratios range from slightly superchondritic to distinctly subchondritic for all xenoliths except for one anomalous sample (1026V), which is characterized by radiogenic ¹⁸⁷Os/¹⁸⁸Os, low Re/Os ratio, and large enrichments in Cu, Os, Pt, Pd, and S relative to Ir (COPPS metasomatism). Assuming chondritic initial relative abundances, the magnitudes of some of the depletions in Pt, Pd, Os, and Re relative to Ir and Ru require incompatible behavior or substantial secondary loss. In detail, some samples, which are otherwise characterized by fertile major-element indices, exhibit low S contents and subchondritic Os/Ir and Pd/Ir ratios, indicating that depletions in Pd and Os relative to Ir are not simple functions of the degree of melting as inferred from major elements. Possible mechanisms for depleting Pt, Pd, Os, and Re relative to Ir and Ru include partitioning into chromian spinels and alloys, partitioning between sulfide and sulfide liquids, mobilization by aqueous fluids, or secondary loss associated with late-stage sulfide breakdown. However, it is not possible to explain all of the depletions in Pt, Pd, Os, and Re by any single mechanism.The preferential enrichment in Os over Re and Ir in sample 1026V is somewhat paradoxical because this sample’s radiogenic ¹⁸⁷Os/¹⁸⁸Os requires a metasomatic agent, originating from a source with a high time-integrated Re/Os ratio. The abundant garnet websterite xenoliths may be a suitable source because they have high Re/Os ratios, radiogenic Os, and abundant garnet, which may sequester Re over Os during partial melting. However, their extremely low Os contents require the processing of large amounts of garnet websterite to concentrate enough Os into the metasomatic sulfides needed to enrich sample 1026V in Os. The homogeneity in ¹⁸⁷Os/¹⁸⁸Os ratio in the remaining xenoliths suggest that their Os isotopic compositions were not significantly affected by PGE metasomatism. The singular nature of 1026V’s composition emphasizes the rarity of COPPS metasomatism.     

Re-Os同位素组成测试方法及其应用进展

Re为中等不相容元素,Os则属强相容元素,与母子体均为不相容元素的Rb Sr、Sm Nd、U Th Pb等同位素体系相比,具亲铁、亲硫性的Re Os同位素体系在定年和示踪研究中显示出特殊性,受到了地学家高度重视,其应用正走向普及。总结和对比了近年来Re Os同位素分析中样品分解的不同方法（NiS火试金法、Carius管溶样法、高压灰化消解法、浸提法、水样处理法）、Os的分离（常规蒸馏、液溴和CCl4提取、快速低本底提取、小型蒸馏）与纯化流程（微蒸馏）、Os同位素比值质谱测定法（N TIMS、ICP MS、微区原位（in situ）分析）及随测定方法的改进Re Os同位素体系在地球科学研究中的应用进展。     

Re-Os同位素定年方法进展及ICP-MS精确定年测试关键技术

本文介绍了Re-Os同位素定年的基本原理、技术发展及应用现状;综述了样品分解和Re-Os分离富集的主要方法,重点对ICP-MS法进行Re-Os同位素定年做了较详尽的介绍,包括质量分馏校正、干扰校正、含量初测、取样量的确定、稀释剂的稀释比及稀释剂加入量等,以确保高精度测试;评述了ICP-MS最常见的测定对象-辉钼矿中Re-Os的失耦现象及降低其对Re-Os同位素定年影响的对策,文中描述了由测定同位素比值计算含量时的误差传递公式并重申了最佳稀释比。最后,指出了Re-Os同位素定年方法研究中应该关注的工作方向。     

铼-锇同位素定年方法及分析测试技术的进展

铼-锇同位素定年已经成为矿床学乃至于地质学领域最重要的定年技术之一。文章简略地回顾了铼-锇同位素体系技术方法的发展过程;介绍了准确测定187Re衰变常数的发展历史,铼-锇同位素定年和同位素示踪的基本原理,铼与锇的基本化学性质、在自然界的分布、地球化学行为、赋存状态和样品采集应注意的问题。结合作者实验室10余年的铼-锇同位素体系分析经验,较系统地总结了常用的样品分解和化学分离方法;介绍了负离子热表面电离质谱和电感耦合等离子体质谱测定铼、锇同位素的方法原理、特点和应注意的技术细节,以及近年来用于准确测定锇稀释剂的锇标准参考物质的选择、化学组分测定和铼-锇标准参考物质的研究进展。     

湖南鲁塘石墨矿Re-Os同位素研究

石墨具有较高的Re、Os含量,可望成为理想的Re-Os同位素测年对象,但迄今国内外研究较少,尤其在煤层经变质作用形成石墨过程中,其中Re-Os同位素体系的变化还有待研究。湖南鲁塘石墨矿是我国典型的隐晶质石墨矿床之一,矿体产于二叠系龙潭组煤系地层中。本文采用Carius管逆王水溶解样品,直接蒸馏、微蒸馏分离纯化Os,丙酮萃取法分离富集Re,热表面电离质谱法对鲁塘矿区石墨样品以及外围原煤进行了Re-Os同位素分析。结果表明:鲁塘石墨的Re含量为0.901~9.794 ng/g,Os含量为7.3~189.5 pg/g,Re-Os同位素等时线年龄为155.6±3.6 Ma,该年龄与鲁塘石墨矿东侧骑田岭岩体第二阶段中粒黑云母花岗岩锆石U-Pb年龄153~157 Ma一致,表明了龙潭组煤层受到骑田岭岩体"烘烤"作用,发生热接触变质作用,使得靠近骑田岭岩体原煤变质为石墨,形成石墨矿床。通过对比石墨、原煤和骑田岭岩体Re、Os含量及比值,发现石墨中的Re、Os主要来源于原煤,并根据石墨Re-Os等时线初始(187Os/188Os)i值(0.686±0.032),推测骑田岭岩体在侵入煤系地层过程中,有少量具有较低187Os/188Os值的Os被碳质吸附。     

Highly siderophile element evidence for early solar system processes in components from ordinary chondrites

Separated magnetic and nonmagnetic components from the ordinary chondrites Dhajala (H3.8) and Ochansk (H4) were analyzed for their Re-Os isotopic compositions, as well as for the abundances of the highly siderophile elements (HSE) Re, Os, Ir, Ru, Pt and Pd. The Re-Os isotopic systematics of these components are used to constrain the timing of HSE fractionations, and assess the level of open-system behavior of these elements in each of the different components. The high precision, isotope dilution mass spectrometric analyses of the HSE are used to constrain the origins of, and possible relations between some of the diverse components present in these chondrites. The relative and absolute abundances of the HSE differ considerably among the components. Metal fractions have Re/Os that are factors of ∼2 (Dhajala) to ∼3 (Ochansk) higher than those of their nonmagnetic fractions. The isotopic data for both meteorites are consistent with the largest Re-Os fractionations occurring between metal and nonmagnetic components early in solar system history, although minor to moderate late stage, open-system behavior, and limited variations in Re/Os preclude a precise determination of the age for that fractionation. Open-system behavior is generally absent to minor in the metal fractions, and highly variable in nonmagnetic fractions. Re/Os ratios of nonmagnetic fractions deviate as much as 40% from a primordial isochron. Although some deviations are large for isochron applications, nearly all are negligible with respect to consideration of fractionation processes controlling the HSE.Metal from both meteorites contains about 90% of the total budget of HSE. Metal in Ochansk has ∼2 to 10 times the abundances of the bulk meteorite, while metal from the matrix of Dhajala has ∼2 to 4 times the abundances of the bulk. Fine metal in both meteorites has higher abundances than coarse metal, as has been previously observed. Nonmagnetic components, consisting of chondrules and matrix from which metal was removed in the laboratory, have highly fractionated HSE, characterized by much lower Re/Os than the bulk meteorites, as well as large relative depletions in Pd. The abundances of Re, Os, Ir, Ru and Pt in the nonmagnetic fractions are 14-120 ng/g, much higher than would be expected if they had equilibrated with the metal phases present (150-16,000 ng/g). Collectively, the data are consistent with the HSE budget in ordinary chondrites being dominated by two HSE-bearing carrier phases with distinct compositions. These phases formed separately, and never subsequently equilibrated. Metal components incorporated a HSE carrier that formed at high through moderate temperatures and relatively high pressures, such that the relatively volatile Pd behaved coherently with the more refractory HSE. Nonmagnetic fractions from both chondrules and matrix have HSE compositions that likely require at least two processes that fractionated the HSE. Depletions in Pd are consistent with the presence of HSE carriers that formed as either highly refractory condensates, or residues of high degrees of metal melting. Depletions in Re may implicate a period of relatively high f_O2 during which a volatile form of Re was separated from the other HSE.     

辉钼矿Re-Os同位素定年方法的改进与应用

公认的Re-Os同位素定年代表物辉钼矿,目前已在金属硫化物矿床年代学研究领域获得了广泛的应用。本研究采用浓HNO₃分解辉钼矿样品,大大地简化了Re和Os的化学制备过程,并根据辉钼矿中正常Os含量水平相对放射成因¹⁸⁷Os可以忽略的特点,以正常Os标准为稀释剂,实现了仪器测量过程中Os同位素质量分馏的在线校正,改善了分析数据的质量。该方法经辉钼矿国家标准物质进行验证,获得了满意的Re、Os含量及Re-Os年龄数据,并且在南岭地区与连阳复式岩体相关的姓坪夕卡岩型钼矿床成矿年龄研究中获得了成功应用。在实际应用中,为了获得有意义的能反映真实地质事件的年龄数据,辉钼矿样品不仅要有足够的取样量,而且还要保证粒度细、混合均匀。