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1.
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
2.
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
3.
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
4.
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
5.
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
6.
The Re–Os (rhenium–osmium) chronometer applied to molybdenite (MoS2) is now demonstrated to be remarkably robust, surviving intense deformation and high‐grade thermal metamorphism. Successful dating of molybdenite is dependent on proper preparation of the mineral separate and analysis of a critical quantity of molybdenite, unique to each sample, such that recognized spatial decoupling of 187Re parent and 187Os daughter within individual molybdenite crystals is overcome. Highly precise, accurate and reproducible age results are derived through isotope dilution and negative thermal ion mass spectrometry (ID‐NTIMS). Spatial decoupling of parent–daughter precludes use of the laser ablation ICP‐MS microanalytical technique for Re–Os dating of molybdenite. The use of a reference or control sample is necessary to establish laboratory credibility and for interlaboratory comparisons. The Rb–Sr, K–Ar and 40Ar/39Ar chronometers are susceptible to chemical and thermal disturbance, particularly in terranes that have experienced subsequent episodes of hydrothermal/magmatic activity, and therefore should not be used as a basis for establishing accuracy in Re–Os dating of molybdenite, as has been done in the past. Re–Os ages for molybdenite are almost always in agreement with observed geological relationships and, when available, with zircon and titanite U–Pb ages. For terranes experiencing multiple episodes of metamorphism and deformation, molybdenite is not complicated by overgrowths as is common for some minerals used in U–Pb dating (e.g. zircon, monazite, xenotime), nor are Re and Os mobilized beyond the margins of individual crystals during solid‐state recrystallization. Moreover, inheritance of older molybdenite cores, incorporation of common Os, and radiogenic Os loss are exceedingly rare, whereas inheritance, common Pb and Pb loss are common complications in U–Pb dating techniques. Therefore, molybdenite ages may serve as point‐in‐time markers for age comparisons. 相似文献
7.
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
8.
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
9.
Svetlana G. Tessalina Marina A. Yudovskaya Ilya V. Chaplygin Françoise Capmas 《Geochimica et cosmochimica acta》2008,72(3):889-909
Rhenium (Re) is one of the least abundant elements in Earth, averaging 0.28 ppb in the primitive mantle. The unique occurrence of rheniite ReS2 (74.5 wt% of Re) in Kudryavy volcano precipitates raises questions about recycling of Re-rich reservoirs within the Kurile-Kamchatka volcanic Island arc setting. The sources of this unique Re enrichment have been inferred from studies of Re-Os isotope systematic and trace elements in volcanic gases, sulphide precipitates and host volcanic rocks. The fumarolic gas condensates are enriched in hydrophile trace elements relative to fluid-immobile elements and exhibit high Ba/Nb (133-204), Rb/Y (16-406) and Th/Zr (0.01-0.25) ratios. They are characterised by high Re (7-210 ppb) and Os abundances (0.4-0.9 ppb), with 187Os/188Os ratios in a range 0.122-0.152. This Os isotopic compositional range is similar to that of the peridotite xenoliths from the metasomatised mantle wedge above the subducted Pacific plate, the radiogenic isotopic signature of which is probably due to radiogenic addition from a slab-derived fluid.Re- and Os-rich sulphide and oxide minerals precipitate from volcanic gases within fumarolic fields. Molybdenite (MoS2), powellite (CaMoO4) and cannizzarite (Pb4Bi6S13) contain 1.5-1.7 wt%, 10 ppm, and 65-252 ppb of Re, respectively. Both molybdenite and rheniite contain normal Os concentrations, with total Os abundances in a range from 0.6 to 3.1 ppm for molybdenite, and 2.3-24.3 ppb for the rheniite samples. Repeated analyses of osmium isotope ratios for two rheniite samples form a best-fit line with an initial 187Os/188Os ratio of 0.32 ± 0.15 and an age of 79 ± 11 yr, which is the youngest age ever measured in natural samples. The high Re contents in molybdenite and rheniite led to high radiogenic 187Os values, even in the limited period of time, with 187Os/188Os ratios up to 3.3 for molybdenite and up to 4.4 for rheniite.The Os isotopic compositions of andesite-basaltic rocks from the Kudryavy volcano (187Os/188Os up to 0.326) are more radiogenic than those of residual peridotites and fumarolic gas condensates that are mainly constituted from magmatic vapor. Such radiogenic values can be attributed either to the addition of a radiogenic Os-rich subduction component to the depleted mantle, or to the assimilation of older dacitic caldera walls (187Os/188Os = 0.6) during arc magma ascent and emplacement. The latter hypothesis is supported by the correlation between 187Os/188Os ratio and indicators of fractionation such as MgO or Ni, and by low contents of potentially hydrophile trace elements such as Ba, Rb and Th relative to fluid-immobile elements such as Nb, Zr and Y. The high Re flux in the Kudryavy volcano (estimated at ∼46 kg/yr) can be explained by remobilisation of Re by Cl-rich water from an underplated mantle wedge and subducted organic-rich sediments of the Pacific plate. 相似文献
10.
The applications of the187Re-187Os isotope pair as a petrogenetic and geologic tracer are increasing in recent years due to several advances in the chemical
extraction and purification of Re and Os, occurring at ppb levels in environmental samples, and in the precise determination
of the Os isotope composition. We have established in our laboratory; based on available methods, chemical procedures and
Negative Thermal Ionisation Mass Spectrometric techniques for the measurement of Re-Os concentrations in environmental samples
and the Os isotope composition in them. Using these techniques, we are able to determine187Os/186Os ratios with a precision of ∼ 1% (±2σμ; twice the standard error of the mean) in several tens of picogram of Os. Preliminary analysis of black shales from the Lower
Tal section of the Maldeota phosphorite mine yields a mean187Re-187Os model age of 597 ± 30 Ma. The187Os/186Os and Os concentration in black shales of the Lesser Himalaya range from 8 to 96 and 0.02 to 13 ng g-1 respectively. The mean187Os/186Os in these samples is ∼ 25, significantly higher than the crustal value of ∼ 10.5, suggesting that these black shales could
be an important source of radiogenic Os to the rivers draining the Himalaya and to the steady increase in187Os/186Os of the oceans through the Cenozoic. 相似文献
11.
陕西洛南县石家湾钼矿Re-Os同位素年龄及地质意义 总被引：1，自引：0，他引：1
陕西石家湾钼矿床位于东秦岭成矿带西段黄龙铺地区,钼矿化呈细脉-网脉状分布于花岗斑岩体及其围岩中,与矿化有关的围岩蚀变有钾长石化、硅化、绢云母化,属斑岩型矿床.在矿床中选取不同矿化类型的辉钼矿样品,进行了Re～Os同位素定年,获得模式年龄变化范围为143.1±2.1～145.1±2.2 Ma之间,其加权平均年龄(144.0±1.1 Ma,MSWD=0.91)、等时线年龄(145.4±2.1 Ma,MSWD=0.83)与石家湾斑岩体的成岩年龄(141.4±0.6Ma)相近,说明成岩成矿作用发生在晚侏罗世一早白垩世.综合辉钼矿中Re的含量、硫同位素以及相关岩体的源区特征等多方面证据认为,石家湾斑岩型钼矿的成矿物质主要来自于下地壳,并混有少量幔源成分. 相似文献
12.
辉钼矿Re-Os同位素定年方法的改进与应用 总被引：13，自引：9，他引：4
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。 相似文献
13.
大颗粒辉钼矿Re-Os同位素失耦现象及187Os迁移模式研究 总被引：10，自引：4，他引：6
对采自西华山钨矿的大颗粒辉钼矿样品的不同部位进行了取样,并对其年龄分别进行精确厘定,得到了不同的Re-Os模式年龄值,验证了失耦现象的存在.从原理上对失耦现象及其成因进行了解释,并在前人成果的基础上,探索性地提出了187Os可能的迁移模型.取样方式的不同会对辉钼矿的模式年龄产生很大影响,因此,在实际应用中一定要严格遵循"多取样,细磨碎"的原则,这对于能获得科学真实的与地质背景相符的Re-Os同位素地质年龄,从而深入探讨矿床成矿作用具有重要意义. 相似文献
14.
Norman J. Pearson Olivier AlardWilliam L. Griffin Simon E. JacksonSuzanne Y. O’Reilly 《Geochimica et cosmochimica acta》2002,66(6):1037-1050
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.” 相似文献
15.
湘西大溶溪钨矿床中辉钼矿Re-Os同位素定年及其地质意义 总被引：9，自引：2，他引：7
湘西大溶溪钨矿床,为雪峰隆起区内的一个中型白钨矿矿床。文章对该矿床中穿插钨矿体的含辉钼矿石英脉进行了Re-Os同位素年代学研究。分析结果显示,该矿中辉钼矿的Re-Os同位素模式年龄为217.0~221.1 Ma,平均为（219.0±1.2） Ma,其对应的等时线年龄为（223.3±3.9） Ma,揭示其形成于晚三叠世。这些年龄数据与矿区内大神山花岗岩的侵位时间〔（224.3±1.0） Ma〕基本吻合,表明该区含辉钼矿石英脉的形成与花岗岩的侵位具有密切的时、空联系。考虑到该区钨矿体的形成时间介于花岗岩和含辉钼矿石英脉之间,因此,推断大溶溪钨矿床形成于223 Ma左右。该研究成果,不仅为湘西雪峰隆起区存在多期次的钨成矿事件提供了可靠证据,同时又进一步证实了华南地区确实存在一次区域性的与印支期花岗岩有关的成矿作用。 相似文献
16.
汉诺坝玄武岩Re-Os同位素地球化学——Re的挥发性丢失和壳-幔相互作用的证据 总被引：1，自引：0，他引：1
本文报道了采自汉诺坝玄武岩区周坝和白龙硐剖面以及白布洛张20井等地29个玄武岩样品的Re、Os含量和~(187)Os/~(188)Os比值。Os含量为11×10~(-12)～314×10~(-12),Re含量为40×10~(-12)～238×10~(-12),Re和Os含量有正相关趋势。碱性玄武岩(AK)的Re、Os含量高于拉斑玄武岩(TH)和过渡玄武岩(TR),玄武岩Os含量变化与分离结晶作用有关,玄武岩的低Re含量与地面喷发的火山岩浆脱气过程中Re的挥发性丢失作用有关。玄武岩的~(187)Os/~(188)Os比值为0.14735～0.61136,AK的~(187)Os/~(188)Os比值比TH和TR低且变化小。玄武岩的~(187)Os/~(188)Os比值与Os含量有负相关性。随着Os含量降低到小于75×10~(-12),~(187)Os/~(188)Os比值迅速升高,反映了地壳混染在TH和TR成因中的贡献。在以往的研究中没有观察到类似的地壳混染作用,说明了Re-Os同位素体系在示踪壳源物质上的优势。一些Os含量较高的TH的~(187)Os/~(188)Os比值表明其地幔源区既非亏损的又非经交代富集的SCLM,可能是混入了地壳俯冲物质的"Marble cake"型地幔。总之,汉诺坝玄武岩的Re-Os同位素地球化学研究支持了以往研究的主要成果,两类玄武岩地球化学差异性和异源成因论;分离结晶和部分熔融过程在玄武岩成因中的重要作用;碱性玄武岩的成因与地幔柱的关系等。同时揭示了一些新的现象:汉诺坝玄武岩形成中存在少量的地壳混染作用;地面喷发的火山熔岩在脱气过程中Re的挥发性丢失;拉斑玄武岩的源区更有可能为"Marble cake"型地幔。 相似文献
17.
Re-Os isotopes were used to constrain the source of the ore-forming elements of the Tharsis and Rio Tinto mines of the Iberian
Pyrite Belt, and the timing of mineralization. The pyrite from both mines has simila]r Os and Re concentrations, ranging between
0.05–0.7 and 0.6–66 ppb, respectively. 187Re/188Os ratios range from about 14 to 5161. Pyrite-rich ore samples from the massive ore of Tharsis and two samples of stockwork
ore from Rio Tinto yield an isochron with an age of 346 ± 26 Ma, and an initial 187Os/188Os ratio of about 0.69. Five samples from Tharsis yield an age of 353 ± 44 Ma with an initial 187Os/188Os ratio of about 0.37. A sample of massive sulfide ore from Tharsis and one from Rio Tinto lie well above both isochrons
and could represent Re mobilization after mineralization. The pyrite Re-Os ages agree with the paleontological age of 350 Ma
of the black shales in which the ores are disseminated. Our data do not permit us to determine whether the Re-Os isochron
yields the original age of ore deposition or the age of the Hercynian metamorphism that affected the ores. However, the reasonable
Re-Os age reported here indicates that the complex history of the ores that occurred after the severe metamorphic event that
affected the Iberian Pyrite Belt massive sulfide deposits did not fundamentally disturb the Re-Os geochronologic system. The
highly radiogenic initial Os isotopic ratio agrees with previous Pb isotopic studies. If the initial ratio is recording the
initial and not the metamorphic conditions, then the data indicate that the source of the metals was largely crustal. The
continental margin sediments that underlie the deposits (phyllite-quartzite group) or the volcanic rocks (volcanogenic-sedimentary
complex) in which the ores occur are plausible sources for the ore-forming metals and should constrain the models for the
genesis of these deposits.
Received: 15 March 1999 / Accepted: 26 July 1999 相似文献
18.
Re-Os同位素定年对岩浆型Cu-Ni硫化物矿床成矿时代的制约 总被引：3，自引：1，他引：2
Re-Os同位素体系被认为是岩浆Cu-Ni硫化物矿床直接定年的有力工具。通过研究世界级典型岩浆Cu-Ni硫化物矿床的Re-Os等时线表面年龄,发现有时能得到成矿年龄,有时得到与成矿年龄不一致的表面年龄或根本得不到Re-Os等时线,还有时同一矿床的不同类型矿石给出不同的Re-Os等时线表面年龄。文章介绍了能够解释上述现象的理论模型。模型预测对与基性-超基性岩共生的Cu-Ni硫化物矿床,除一些特殊情况外,块状矿石可得到有地质意义的Re-Os等时线年龄,浸染状矿石常得到没有地质意义的假等时线;而浸染状矿石常得到有地质意义的Os同位素初始比值,而块状矿石给出的"Os同位素表面初始比值"往往没有地质意义。因此,建议在应用Re-Os同位素体系定年时要结合矿床类型、矿石类型以及成矿过程等因素综合考虑;对Re-Os数据的科学合理解释同样需要从矿床学和同位素地球化学的基本原理出发,结合矿床的实际情况,进行深入分析研究。 相似文献
19.
Re-Os同位素定年方法进展及ICP-MS精确定年测试关键技术 总被引：8，自引：0，他引：8
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。 相似文献
20.
Robert A Creaser Poulomi Sannigrahi Thomas ChackoDavid Selby 《Geochimica et cosmochimica acta》2002,66(19):3441-3452
Re-Os isotopic analyses of a single organic-rich sedimentary rock unit (ORS) of known depositional age, and at three levels of regional hydrocarbon maturity, show that hydrocarbon maturation does not affect the ability the 187Re-187Os chronometer to yield a depositional age for such rocks. We present Re-Os isotope analyses from the Late Devonian Exshaw Formation in the subsurface of the Western Canada Sedimentary Basin, Alberta, and obtain a Re-Os isochron age of 358 ± 10 Ma (2σ, Model 3, λ = 1.666 × 10−11.a−1) for samples ranging from hydrocarbon immature to overmature. This age is within uncertainty of the established absolute age for the Exshaw Formation. Hydrocarbon immature, and mature plus overmature samples show no significant age differences if regressed individually, indicating that hydrocarbon maturation did not greatly disturb the Re-Os isotope system in the Exshaw Formation. As such, we propose that the Re-Os geochronometer may be used as a reliable tool for measuring the depositional ages of ORS regardless of their level of hydrocarbon maturity. We find that minimizing natural variation in the initial 187Os/188Os ratio is more important than avoiding hydrocarbon maturation in obtaining precise Re-Os ages. In particular, the Exshaw Formation appears to contain a nonhydrogenous component of unradiogenic Os, in addition to the hydrogenous Os load. A subset of Exshaw Formation samples with >5% total organic carbon (TOC), which should best reflect the hydrogenous Os load alone, yields a very well-fitted isochron having a depositional age of 358 ± 9 Ma (2σ, λ = 1.666 × 10−11.a−1) with an initial 187Os/188Os ratio of 0.59 ± 0.05 (Model 3, Mean Square of Weighted Deviates (MSWD) = 1.8). The initial 187Os/188Os ratio of this regression may provide an estimate of the Os isotopic composition of local seawater at the time of deposition. 相似文献