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1.
含辉钼矿全岩样品Re-Os同位素定年研究:在北京大庄科钼矿床中的应用 总被引：1，自引：1，他引：0
采用硝酸在比色管中对辉钼矿样品中Re含量进行初测的方法,测得辉钼矿标准样品JDC Re含量与推荐值在误差范围内基本一致,与传统的Carius管法相比,该方法具有简便快速的特点。传统的辉钼矿Re-Os同位素定年分析对象为辉钼矿单矿物,根据所测得的187Re/187Os值获得辉钼矿的Re-Os年龄,Re、Os在辉钼矿中大量富集,而在硅酸盐矿物中几乎没有,探索性地对含有辉钼矿的全岩样品进行Re-Os同位素定年,虽然所得Re、Os含量偏低,但187Re/187Os值不会变。该方法省去了选样过程花费的大量时间,避免了选样过程中可能造成的交叉污染。采用同位素稀释Carius管逆王水法探索性地对北京大庄科钼矿床中含辉钼矿全岩样品进行Re-Os同位素年龄测定,获得了(137.6±3.7)Ma精确的等时线年龄,与挑选出辉钼矿单矿物样品的Re-Os同位素等时线年龄(136.8±2.6)Ma吻合较好,直接厘定了大庄科钼矿的成矿时代。该年龄与矿区汉家川石英二长岩锆石U-Pb年龄一致,表明大庄科钼矿的形成与汉家川石英二长岩关系较为密切,为中国东部第二期大规模成矿作用的产物,形成于中国东部岩石圈伸展环境。 相似文献
2.
云南马关地区岩石圈地幔组成和年龄:地幔橄榄岩包体的Re-Os同位素限制 总被引：3，自引：2，他引：1
本文对马关地区新生代碱性玄武岩中的地幔包体进行了系统的岩石学和地球化学研究,并首次进行了包体的Re-Os同位素测试。马关地区的橄榄岩包体主量成分上表现为饱满肥沃的特征;具有不同程度的轻稀土亏损特征,亏损Nb、Ti和Zr等高场强元素(HFSE)以及Ba等大离子亲石元素(LILE);橄榄岩包体的Nd同位素特征表明橄榄岩包体代表的是不均一的亏损地幔。5个橄榄岩全岩样品的Re-Os同位素分析结果表明,样品的Os含量总体较高(3.29×10-9~3.78×10-9),接近于造山带橄榄岩体的Os含量,Re含量变化范围较大(0.24×10-9~0.54×10-9),与Re的迁移能力较强有关。样品的187Os/188Os值在0.12295~0.12530之间变化,与187Re/188Os值和Al2O3含量之间都不存在较好的相关性,说明Re-Os体系不单纯由熔体抽取过程所控制。橄榄岩包体的Re亏损年龄tRD为254~604Ma,说明马关地区岩石圈地幔形成的时代应该在新元古代之前。马关地区岩石圈地幔并非是由软流圈上涌新增生的地幔,而是经历了如下演化历史:在新元古代之前,由原始地幔的部分熔融和熔体抽取作用形成了岩石圈地幔,之后经历了熔/流体交代和改造而发生了再富集作用,导致部分地幔橄榄岩逐渐从亏损难熔的特征向饱满肥沃转变,而未遭受熔/流体的改造的橄榄岩仍然保持了难熔亏损的特征。这种熔/流体交代和改造作用很可能与晚二叠纪峨眉山地幔柱的活动有关,而新生代以来印度-亚洲大陆碰撞导致地幔物质向东南方向的侧向流动,诱发软流圈上涌和马关地区的钾质岩浆的活动,也对马关地区岩石圈地幔的改造具有重要的影响,但由于喷发时间较新对Os同位素组成的影响还未显现出来。 相似文献
3.
橄榄岩—熔体相互作用过程中Re-Os体系的变化趋势: 对华北新生代地幔橄榄岩Re-Os年龄含义的启示 总被引：1，自引：0，他引：1
橄榄岩的Re-Os同位素体系作为探讨岩石圈地幔形成年龄的重要手段已受到人们越来越多的重视。然而,Re-Os体系是否会受到橄榄岩的低温蚀变如蛇纹石化和地幔交代作用或橄榄岩—熔体相互作用的影响并不十分清楚。本文在总结国际上典型造山带橄榄岩剖面研究和地幔橄榄岩捕虏体研究的基础上,发现橄榄岩的Re-Os同位素体系基本不受蛇纹石化等低温蚀变作用的影响; 但橄榄岩—熔体相互作用会造成橄榄岩的Re-Os体系的变化即Re或Os的带入。当熔体/岩石比例较小时(≤1),橄榄岩—熔体相互作用会造成橄榄岩的Re含量显著增加,而放射成因的Os同位素即187Os增量有限。但当熔体/岩石比例很大时(≥1),会造成187Os同位素显著增加。同时,橄榄岩的Re含量与中等程度不相容主、微量元素如Al、Ti、Yb的正相关关系可以通过橄榄岩的两阶段演化模式来解释,即早期的部分熔融残留和后期的橄榄岩—熔体相互作用共同影响的结果。橄榄岩的Re含量与Cr含量的正相关关系进一步说明了这一问题。上述结果对华北东部岩石圈地幔的演化过程有重要的启示作用。因为华北东部古生代时期的确存在太古宙岩石圈地幔,然而新生代时期地幔橄榄岩捕虏体普遍具有元古宙而非太古宙的事实证明橄榄岩—熔体的相互作用的确广泛存在,从而造成岩石圈地幔橄榄岩变年轻。因此,新生代地幔捕虏体的Re-Os同位素年龄并不是岩石圈地幔的形成年龄,而是混合作用的结果。汉诺坝地幔橄榄岩的Re含量和Sr、Nd同位素组成符合橄榄岩—多元熔体相互作用的混合趋势,其橄榄岩的全岩Al2O3含量和橄榄石Fo的反相关性能够通过橄榄岩—熔体相互作用来解释。 相似文献
4.
含有普通锇的辉钼矿Re-Os同位素定年研究 总被引：14，自引：3，他引：11
通过大量数据统计,表明较高比例的辉钼矿中存在普通锇。普通锇可能以类质同像形式存在于辉钼矿样品中,理论上辉钼矿中可能含有较高含量普通锇。辉钼矿样品含有较高含量普通锇可能对Re-Os定年结果产生很大影响,从原理上并结合实例证实了普通锇含量对辉钼矿Re-Os年龄影响程度。对于一般辉钼矿样品来讲,如果187Os总量(放射成因187Os与非放射成因187Os之和)与普通锇比值小于20,需要考虑普通锇对Re-Os模式年龄的影响,并提出了对于含有普通锇辉钼矿模式年龄的计算方法。先做出187Os/188Os-187Re/188Os等时线,求得初始187Os/188Os值,再根据初始187Os/188Os值和单个样品的普Os含量求得非放射成因的普Os中187Os的量。最后根据Re含量以及放射成因187Os含量得到模式年龄。 相似文献
5.
福建德化邱埕钼矿床是德化-尤溪-永泰矿集区唯一一处规模较大的钼矿床。辉钼矿体分布在花岗斑岩外接触带,辉钼矿多沿中新元古代变质岩和晚侏罗世花岗岩裂隙分布,多呈浸染状、脉状和团块状。本次测得该矿床6件辉钼矿样品Re-Os模式年龄为150.1~152.8 Ma,187Re-187Os等时线年龄为（150.8±1.6）Ma,加权平均年龄为（151.8±0.9）Ma,表明成矿时代为晚侏罗世晚期,与该地区大规模的火山-侵入体活动相关;Re/Os比值远大于4,Re同位素含量14.31×10-6~45.8×10-6（最高达174.7×10-6）,指示成矿物质主要来源于壳源,可能还有少量幔源物质的加入。邱埕钼矿床的形成可能为古太平洋板块朝东亚陆缘碰撞挤压作用结束向伸展作用转化过程的产物。 相似文献
6.
铼-锇同位素的等离子体质谱法测定及其在辉钼矿测年中的应用 总被引：10，自引：12，他引：10
研究了用ICPMS法测定地质样品Re-Os同位素的条件。通过选用Meinhard同心雾化器进样对Os(Ⅷ)水溶液进行测定,可使Os的测定灵敏度提高50倍。讨论了质量歧视效应校正中的有关问题。采用氧化剂清洗,克服了Os在进样系统中的严重记忆效应。用同位素稀释法测定了辉钼矿中Re和~(187)Os的含量,计算了成矿年龄。 相似文献
7.
<正>Re-Os同位素定年法是金属矿床年代学中不可或缺的技术手段之一。辉钼矿由于具有极高含量的Re以及极低含量的初始Os,被地质学家公认为是Re-Os同位素定年的最佳对象之一,Re-Os法在钼矿、铜矿、钨矿等金属矿床年代学研究中得到了广 相似文献
8.
Re-Os法能够直接厘定内生金属矿床成矿时代,但是封闭Carius管法化学流程复杂,且有一定的危险性。本文建立了一种简便快速测定辉钼矿Re-Os年龄及其Re含量的方法。用3 mL浓硝酸在10 mL比色管中溶解5~15 mg辉钼矿样品,将溶液中的钼酸沉淀分离后稀释定容,直接采用质谱测量187和185质量数比值(M187/M185)。利用辉钼矿Re-Os年龄标准物质JDC和HLP的M187/M185值与其年龄的正相关线性关系计算未知辉钼矿样品的Re-Os年龄,并通过185Re计数利用相对法计算Re含量。本方法应用于测量13.26~2130 Ma的辉钼矿,Re-Os年龄的测定值与推荐值的相对偏差多数在0.36%~7.42%之间,由于放射性积累较多,长年龄样品测量的准确度较高。与传统Carius管法相比,该方法不需要加入稀释剂,省去了封闭和打开Carius管环节以及Re-Os分离纯化流程,适合于辉钼矿Re-Os年龄的初步分析。 相似文献
9.
江西省都昌县阳储岭钨钼矿床位于江南造山带东段,为准确厘定阳储岭钨钼矿床的成岩成矿时代,本次在详实的野外地质调查基础上,对阳储岭成矿花岗闪长斑进行锆石U-Pb定年工作,同时开展辉钼矿Re-Os同位素定年研究。LA-ICP-MS锆石U-Pb年龄为（145.08±0.35）Ma（MSWD=0.51,n=7）;辉钼矿Re-Os模式年龄为（143.3±2.0）Ma~（145.5±2.2）Ma,等时线年龄为（145.4±1.0）Ma。阳储岭成矿花岗闪长斑岩锆石U-Pb年龄与辉钼矿Re-Os等时线年龄基本一致,表明阳储岭钨钼矿床成岩成矿时代约为145 Ma。辉钼矿中Re含量为16.62×10-6~87.76×10-6,平均值为44.68×10-6,与壳幔混源岩浆热液矿床中Re的含量相似,指示阳储岭钨钼矿床成矿物质来源于壳幔混源。 相似文献
10.
11.
Reproducibility of Re-Os molybdenite ages depends on sample size and homogeneity, suggesting that Re and Os are decoupled within individual molybdenite crystals and do not remain spatially linked over time. In order to investigate the Re-Os systematics of molybdenite at the subgrain (micron) scale, we report LA-ICP-MS Re-Os ages for an Archean molybdenite crystal from Aittojärvi, Finland, analyzed in situ in a white aplite matrix. A related Aittojärvi molybdenite (A996D), in the form of a very fine-grained mineral separate, is used as one of our in-house NTIMS standards, and thus its age of 2760 ± 9 Ma is well established. Measurements of (187Re + 187Os)/185Re on micron scale spots along 200 μm traverses across the crystal yield a wide range of ages demonstrating that, in this case, microsampling of molybdenite does not produce geologically meaningful ages. Experimentation with mineral separations and sample size over a 7-yr period predicted that this would be the outcome. We suggest that 187Os is more likely to be the mobile species, based on its charge and ionic radius, and that 187Os becomes decoupled from parent 187Re with time on the micron and larger scale. Incompatible charge and ionic radius for Os ions formed during reduction of molybdenite-forming fluids may explain the widely observed absence of common (initial) Os in molybdenite. Geologically accurate ages for molybdenite can only be obtained for fully homogenized crystals (or crystal aggregates) so that any post-crystallization 187Re-187Os decoupling is overcome.A growing number of geologically accurate ID-NTIMS 187Re-187Os ages for homogenized molybdenite suggest that postcrystallization mobility of radiogenic 187Os must be limited to within the molybdenite mineral phase. We suggest that radiogenic 187Os may be stored in micron scale dislocations, kink bands, and delamination cracks produced by deformation, and that the unusual structure and deformation response of molybdenite results in an increased chemical stability in this mineral. Migration of 187Os into adjacent silicate phases is highly unlikely, but other contacting sulfides may take in Os. In an example from a Proterozoic skarn deposit at Pitkäranta (western Russia), we demonstrate minor loss of radiogenic 187Os from molybdenite and a corresponding gain in adjacent chalcopyrite such that the molybdenite age is not perceptibly disturbed, whereas the resulting chalcopyrite ages are impossibly old. Therefore, it is unadvisable to perform Re-Os analytical work on any sulfide in contact or intimate association with molybdenite. In addition to large errors in the age, if the isochron method is employed, initial 187Os/188Os ratios could be erroneously high, leading to seriously errant genetic interpretations. 相似文献
12.
We present a detailed study of Re-Os age determinations for eight natural molybdenite samples of like polytype (2H), spanning a range of age, natural grain size and deposit type. The focus of the study is to critically evaluate the effects of sampling, sample preparation and aliquant size on the accuracy and reproducibility of Re-Os ages for these molybdenite samples. We find that for some molybdenite samples, analysis of small sample aliquants (<20 mg) may not yield accurate or reproducible Re-Os ages, whereas analysis of larger aliquants from the same mineral separate do yield reproducible Re-Os dates. Such an observation is best explained if Re and 187Os are internally decoupled within molybdenite grains. This finding is supported from spot analyses by laser ablation MC-ICP-MS analyses presented here and is consistent with previously published observations.The degree of decoupling between Re and 187Os appears to increase both as a function of increasing grain size, and increasing age of molybdenite. From detailed dating of individual molybdenite mineral separates, we provide approximate minimum aliquant amounts required for reproducible Re-Os age dating, as a function of molybdenite age and grain size. Geologically younger, naturally fine-grained molybdenite samples appear to show little Re and 187Os decoupling, and reproducible ages can be determined from some samples with as little as 1 mg of aliquant. Geologically old, and coarse-grained molybdenite samples may require as much as 40 mg of aliquant from a much larger mineral separate to overcome Re and 187Os decoupling. The mechanism(s) of Re and 187Os decoupling within molybdenite is not constrained by this results of this study, but the observation that the degree of decoupling increases with grain size (distance) and age (time/geologic history) may suggest primary diffusive control. Assuming that Re and 187Os decoupling in molybdenite results primarily from diffusion of 187Os, apparent diffusion coefficients are calculated (D = x2/t). Estimates of D for Os made in this way range from 2.8 × 10−26 to 2.1 × 10−21 m2/s, which are broadly similar to experimentally derived diffusion coefficients for Os in Fe-sulfide minerals and for Re in molybdenite at temperatures <500°C. 相似文献
13.
Preparation and Certification of Re-Os Dating Reference Materials: Molybdenites HLP and JDC 总被引：27，自引：1，他引：27
Andao Du Shuqi Wu Dezhong Sun Shuxian Wang Wenjun Qu Richard Markey Holly Stain John Morgan Dmitry Malinovskiy 《Geostandards and Geoanalytical Research》2004,28(1):41-52
Two Re-Os dating reference material molybdenites were prepared. Molybdenite JDC and molybdenite HLP are from a carbonate vein-type molybdenum-(lead)-uranium deposit in the Jinduicheng-Huanglongpu area of Shaanxi province, China. The samples proved to be homogeneous, based on the coefficient of variation of analytical results and an analysis of variance test. The sampling weight was 0.1 g for JDC and 0.025 g for HLP. An isotope dilution method was used for the determination of Re and Os. Sample decomposition and pre-concentration of Re and Os prior to measurement were accomplished using a variety of methods: acid digestion, alkali fusion, ion exchange and solvent extraction. Negative thermal ionisation mass spectrometry and inductively coupled plasma-mass spectrometry were used for the determination of Re and 187 Os concentration and isotope ratios. The certified values include the contents of Re and Os and the model ages. For HLP, the Re content was 283.8 ± 6.2 μg g−1 , 187 Os was 659 ± 14 ng g−1 and the Re-Os model age was 221.4 ± 5.6 Ma. For JDC, the Re content was 17.39 ± 0.32 μg g−1 , 187 Os was 25.46 ± 0.60 ng g−1 and the Re-Os model age was 139.6 ± 3.8 Ma. Uncertainties for both certified reference materials are stated at the 95% level of confidence. Three laboratories (from three countries: PR. China, USA, Sweden) joined in the certification programme. These certified reference materials are primarily useful for Re-Os dating of molybdenite, sulfides, black shale, etc. 相似文献
14.
Yoshio Takahashi Tomoya Uruga Hajime Tanida Keiko H. Hattori 《Geochimica et cosmochimica acta》2007,71(21):5180-5190
Local atomic structures of Re and radiogenic Os in molybdenite from the Onganja mine, Namibia, were examined using X-ray absorption fine structure (XAFS). Rhenium LIII-edge X-ray absorption near-edge structure (XANES) and extended X-ray absorption fine structure (EXAFS) show that the oxidation state of Re, the interatomic distances between Re and the neighboring atoms, and the coordination number of Re to S are very similar to those of Mo in molybdenite. The results confirm that Re is present as Re(IV) in the Mo site in molybdenite.Measurement of LIII-edge XANES and EXAFS of a minor concentration (8.55 ppm) of radiogenic Os was accomplished in fluorescence mode by removing the interfering X-rays from Re and other elements using a crystal analyzer system. The data indicate that the oxidation state of radiogenic Os is Os(III) and Os(IV) and clearly different from Os(II) in natural sulfide minerals, such as OsS2 (erlichmanite). XANES data also suggest that radiogenic Os does not form a secondary Os phase, such as OsS2 or Os metal, in molybdenite.EXAFS of radiogenic Os was successfully simulated assuming that Os is present in the Mo site in molybdenite. The data are consistent with the XANES data; Os does not form Os phases in molybdenite. The EXAFS simulation showed that the interatomic distance between Os and S is 2.27 Å, which is 0.12 Å smaller than the distances of Re-S and Mo-S (2.39 Å) in molybdenite. Similar valences and ionic sizes of Re and Mo in molybdenite support the fact that large amounts of Re can be incorporated into the Mo site as has been observed in previous studies, whereas the different properties of Os compared to Mo and Re suggested here support much lower abundance of common Os in molybdenite. This makes molybdenite an ideal mineral for the Re-Os geochronometer as shown in many studies. However, the shorter distance between radiogenic Os and S compared to those of Re-S and Mo-S in molybdenite suggests that the radiogenic Os has a smaller ionic size than Re(IV) and Mo(IV). Furthermore, Os may be partly present as Os(III). Smaller and lower charge Os can diffuse faster than larger and higher charge Re in molybdenite at a given set of conditions. Hence, our study provides an atomic-level explanation for the high mobility of Os compared to Re, which has been suggested by earlier workers using laser ablation ICP-MS. 相似文献
15.
Seven 187Re-187Os ages were determined for molybdenite and pyrite samples from two well-dated Precambrian intrusions in Fennoscandia to examine
the sustainability of the Re-Os chronometer in a metamorphic and metasomatic setting. Using a new 187Re decay constant (1.666 × 10−11y−1) with a much improved uncertainty (±0.31%), we determined replicate Re-Os ages for molybdenite and pyrite from the Kuittila
and Kivisuo prospects in easternmost Finland and for molybdenite from the Kabeliai prospect in southernmost Lithuania. These
two localities contain some of the oldest and youngest plutonic activity in Fennoscandia and are associated with newly discovered
economic Au mineralization (Ilomantsi, Finland) and a Cu-Mo prospect (Kabeliai, Lithuania). Two Re-Os ages for vein-hosted
Kabeliai molybdenite average 1486 ± 5 Ma, in excellent agreement with a 1505 ± 11 Ma U-Pb zircon age for the hosting Kabeliai
granite pluton. The slightly younger age suggests the introduction of Cu-Mo mineralization by a later phase of the Kabeliai
magmatic system. Mean Re-Os ages of 2778 ± 8 Ma and 2781 ± 8 Ma for Kuittila and Kivisuo molybdenites, respectively, are in
reasonable agreement with a 2753 ± 5 Ma weighted mean U-Pb zircon age for hosting Kuittila tonalite. These Re-Os ages agree
well with less precise ages of 2789 ± 290 Ma for a Rb-Sr whole-rock isochron and 2771 ± 75 Ma for the average of six Sm-Nd
TDM model ages for Kuittila tonalite. Three Re-Os analyses of a single pyrite mineral separate, from the same sample of Kuittila
pluton that yielded a molybdenite separate, provide individual model ages of 2710 ± 27, 2777 ± 28, and 2830 ± 28 Ma (Re = 17.4,
12.1, and 8.4 ppb, respectively), with a mean value of 2770 ± 120 Ma in agreement with the Kuittila molybdenite age. The Re
and 187Os abundances in these three pyrite splits are highly correlated (r = 0.9994), and provide a 187Re-187Os isochron age of 2607 ± 47 Ma with an intercept of 21 ppt 187Os (MSWD = 1.1). It appears that the Re-Os isotopic system in pyrite has been reset on the millimeter scale and that the 21 ppt 187Os intercept reflects the in situ decay of 187Re during the ∼160 to 170 m.y. interval from ∼2778 Ma (time of molybdenite ± pyrite deposition) to ∼2607 Ma (time of pyrite
resetting). When the Re-Os data for molybdenites from the nearby Kivisuo prospect are plotted together with the Kuittila molybdenite
and pyrite data, a well-constrained five-point isochron with an age of 2780 ± 8 Ma and a 187Os intercept (−2.4 ± 3.8 ppt) of essentially zero results (MSWD = 1.5). We suggest that the pyrite isochron age records a
regional metamorphic and/or hydrothermal event, possibly the time of Au mineralization. A proposed Re-Os age of ∼2607 Ma for
Au mineralization is in good agreement with radiometric ages by other methods that address the timing of Archean Au mineralization
in deposits worldwide (so-called “late Au model”). Molybdenite, in contrast, provides a robust Re-Os chronometer, retaining
its original formation age of ∼2780 Ma, despite subsequent metamorphic disturbances in Archean and Proterozoic time.
Received: 25 September 1996 / Accepted: 27 August 1997 相似文献
16.
辉钼矿中Re、Os含量高且几乎不含普通Os,通常被认为是开展金属矿床定年的理想对象。然而,在一些矿床中辉钼矿常以浸染状产出,矿物颗粒微小,挑纯难度较大,本文尝试使用含辉钼矿的岩石样品进行测年实验。选择研究程度较高、年龄数据较多的德兴斑岩铜矿田朱砂红矿床的4件含辉钼矿岩石样品进行了Re_Os同位素定年,结果获得等时线年龄为172.6±2.6 Ma,与前人已获得的年龄数据基本一致,说明该年龄数据可靠,样品中的硅酸盐矿物对定年结果没有影响。德兴斑岩铜矿田中3个矿床的辉钼矿Re_Os年龄与花岗闪长斑岩的锆石U_Pb年龄相一致,表明其矿化与斑岩侵入体直接相关。而前人获得的Rb_Sr年龄及K_Ar年龄与近年得到的Re_Os、U_Pb年龄数据存在差别的原因可能是后期热液蚀变及热事件破坏或重置了Rb_Sr和K_Ar同位素体系。 相似文献
17.
Dating of metallic ore deposits has been one of the problems concerned with by ore geologists for many years.The establishment of the Re-Os Isotope Laboratory at the Institute of Rock and Mineral Analysis,Chinese Academy of Geological Sciences, has provided us with a new technique to carry out geochronological studies of molybdenum ores.As one of the most important Re-bearing minerals, molybdenite contains almost no common osmium, but ^187Os was derived completely from decay of ^187Re, with ^187Os content as the function of Re content in the mineral .An ID-ICP-MS technique has been used in this study,and Re-Os isotopic ages of several large molybdenum deposits of differ-ent types from the East Qinling molybdenum belt have been determined.It is indicated that the Huanglongpu carbonatite vein-type molybdenum-(lead) deposit has a Re-Os age corresponding to Indosinian,while the rest porphyry-type molybdenum deposits and porphyry-skarn-type molybdenum-(tungsten) deposits have Re-Os ages corresponding to Yenshanian. 相似文献