共查询到18条相似文献，搜索用时 109 毫秒
1.
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 总被引：4，自引：2，他引：4
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。 相似文献
2.
Re-Os同位素体系在蛇绿岩应用研究中的进展 总被引：2，自引：1，他引：2
Re-Os不同于由亲石元素构成的同位素体系，在原始上地幔（PUN）部分熔融过程中，母体Re是中等不相容元素，优先进入熔体相，子体Os是强相容元素，富集在残留相中，是研究蛇绿岩的极好示踪剂。在蛇绿岩应用研究中已经取得了4个方面的进展：（1）明确了熔体相的Re／Os和^187Os／^188Os比值高，而残留相的低；（2）铬铁矿中铂族元素矿物（PGM）的Re亏损年龄（TRD）证实了蛇绿岩中复杂的超镁铁岩体是多阶段部分熔融的产物；（3）现代大洋橄榄岩和玄武岩的Re-Os同位素研究表明熔体相和残留相的^187Os／^188Os比值在高于亏损地幔值（DMM）的部分是一致的，而低于DMM的存在不一致性，为研究蛇绿岩中熔体相与残留相是否存在“耦合”关系提供了新的制约因素；（4）揭示了蛇绿岩地幔橄榄岩中含有古大陆岩石圈地幔，这是前所未知的。虽然取得了不少进展，但是由于Re-Os同位素体系用于蛇绿岩研究的时间较短，尚存在一些问题，如显生宙蛇绿岩地幔橄榄岩的定年问题，有待进一步深化研究。 相似文献
3.
从浙东、闽东南的早白垩世“双峰式火山岩”和“复合岩体”中选择了有代表性的玄武岩和角闪辉长岩，分离出钛-磁铁矿，进行Re—Os同位素分析。角闪辉长岩的γos（130Ma）为-83．7～ -47．1，其（^187 Os／^188 Os）。过低，为0．0667和0．0205。这低得不合理的（^187 Os／^188 Os）i表明成岩之后Re-Os体系可能受到扰动，某些地质过程导致外加Re的进入，使岩石的^187 Re／^188 Os比值偏高、（^187 Os／^188 Os）;及γOs（t）值偏低。玄武岩的γOs（130Ma）=21．4—267．8，其（^187 Os／^188 Os）。为0．1531～0．4639。Re—Os、Sm—Nd同位素及微量元素地球化学研究表明，早白垩世玄武岩浆不是来自富集地幔，而是来自亏损的地幔源区，在其演化过程中经受了地壳岩石和熔体的混染。晚中生代时期，东南沿海“大陆弧”下的地幔可能不是富集的岩石圈地幔，具有亏损特性，因而是软流圈地幔。 相似文献
4.
Re-Os同位素对峨眉山大火成岩省成因制约的探讨 总被引：6，自引：3，他引：3
峨眉山大火成岩省（ELIP）主要由玄武岩、玄武质火山碎屑岩及少量的苦橄岩（包括越南的科马提岩）、长英质岩石以及层状岩体和岩墙组成,其物质来源直接关系到其成因是否与地幔柱活动有关。Re-Os同位素体系是地核、地幔和地壳物质的最佳示踪剂。前人对ELIP内的Re-Os同位素研究表明,低Ti玄武岩的Os含量为0．006×10^-9-0．40010^-9,^187Os／^188Os初始值为0．1371～1．403,并提出其与地幔柱活动有关;而高Ti玄武岩的Os含量为0．00410^-9～0．56010^-9,^187Os／^188Os初始值为0．1271～5．19,认为起源于大陆岩石圈地幔或地幔柱上升过程中受到大量岩石圈地幔“混染”（xu JF et al．,2007）;科马提岩的0s含量为1．2410^-9～7．0010^-9,^187Os／^188Os初始值为0．1251～0．1261,苦橄岩的Os含量为0．3210^-9～2．32910^-9,^187Os／^188Os初始值为0．1233～0．1266,指示苦橄岩和科马提岩均来自亏损地幔源区（Hanski et al．,2004;陈雷等,2007）。本文利用Os含量最低、^187Os／^188Os最高的高Ti玄武岩作为地壳端员,用铁质陨石、原始上地幔（PUM）和亏损地幔（DMM）作为地核和各种地幔端员,分别做二元混合计算,结果显示绝大多数玄武岩和所有苦橄岩及科马提岩均落在地壳和DMM混合曲线附近,并且邻区特提斯洋地幔岩与DMM具有相近的Os含量和^187Os／^188Os组成,据此推测峨眉山火成岩的形成与特提斯洋的活动有关,主要受控于地壳和亏损地幔的相互作用。 相似文献
5.
黑矿型矿床成矿物质来源：日本上向黑矿铼—锇和氦同位素证据 总被引：5，自引：1，他引：5
上向黑矿（Uwamuki Kuroko)是日本最典型的黑矿型矿床，它形成于日本岛弧中新世矢折岛弧裂谷环境，产于双峰式岩石组合的长英质火山岩系中。矿床由下部筒状硅矿带和上部块状黑矿带构成，后者显示典型的上黑（黑矿）下黄（黄矿）金属分带。为探索研究长期争议的成矿物质来源，系统测定了矿石和主岩的Os,He同位素组成。含矿流纹岩系的R／RA值介于0．93－1．14间，证实该岩浆可能主要来源于陆壳重熔。上向黑矿的上部块状黑矿矿石具较高的^187Os/^188Os值（2．246－7．608），反映矿石Os主体来源于壳源沉积物或矿区基底岩系；下部脉状－网脉状硅矿、块状黄矿和少量黑矿则具低^187Os/^188Os值（0．423－0．793），证实矿石Os具两源性，估计幔源物质贡献约57％－89％，壳源物质贡献约11％－43％。此外，在上部块状黑矿带内部，矿石 ^187Os/^188O显示清楚的垂向韵律性变化，揭示了成矿流体及成矿物质的周期性混合，据此，本文提出了一个新的两阶段成矿模式。 相似文献
6.
汉诺坝幔源橄榄岩包体的微量元素和Re-Os同位素地球化学：SCLM的性质和形成时代 总被引：11，自引：6，他引：11
本文报道了汉诺坝新生代碱性玄武岩中地幔橄榄岩包体的主量、微量元素和Re-Os同位素。14个尖晶石橄榄岩Re、Os含量分别为0.022～0.193ng/g和1.237～4.304ng/g，^187Os/^188Os比值为0.1183～0.1244，与^187Os/^188Os比值相关性不好，但与熔体亏损指标如重稀土元素Yb的含量、全岩Al2O3的百分含量有很好的线性关系，可能反映了地幔熔融后的Re或/和Os的活动。全岩Al2O3、CaO、TiO2含量均与MgO有很好的负相关性，全岩原始地幔标准化REE丰度模式呈现了LREE亏损，表明该区橄榄岩包体是由软流圈地幔经过部分熔融，亏损了玄武质组分后形成的。由Os同位素代理等时线得到该区陆下岩石圈地幔的形成年龄为1.7～2.0Ga，表明尖晶石相橄榄岩所代表的岩石圈地幔是中元古代的陆下岩石圈地幔减薄后的残留体。 相似文献
7.
铼-锇同位素地球化学进展 总被引：4，自引：0，他引：4
蒋少湧 《矿物岩石地球化学通报》2000,19(4):421-422
Re和Os是强亲铁元素。Re同位素有：^185Re(37．07％)和^187Re(62．93％)。Os有7个同位素：^184Os(0．018％)、^186Os(1．59％)、^187Os(1．64％)、^188Os(13．20％)、^189Os(16．10％)、^180Os(26．40％)和^192Os(41．0％)。^186Os和^187Os为放射性衰变产物。^186Os由^190Pt通过α衰变而成,^187Os由^187Re通过β衰变而成。 相似文献
8.
云南丽江苦橄岩Re-Os同位素地球化学初步研究 总被引：5，自引：0，他引：5
报导了云南丽江地区大具和仕满剖面12个苦橄岩和6个玄武岩的Re，Os含量和Os同位素组成。苦橄岩和玄武岩具有明显不同的Re-Os体系的特征。苦橄岩具有高的Os元素丰度［(1.5~3)×10-9］和低的Re元素丰度（<0.05×10-9）；共生的玄武岩具有低的Os元素丰度（<0.5×10-9）和相对高的Re元素丰度（<0.8×10-9）；苦橄岩具有低放射成因的 187Os/188Os 比值（0.123 3~0.126 6），而玄武岩具有高放射成因的187Os/188Os比值（0.133 8~0.157 7）。苦橄岩的Re-Os同位素特征与越南西北部二叠—三叠纪科马提岩具有低放射成因Os同位素特征相似，而玄武岩的Re-Os同位素特征与峨眉山大火成岩省（LIP）其他地区玄武岩的高放射成因的Os同位素特征相似。苦橄岩的Re-Os同位素特征表明，形成峨眉山LIP的地幔柱可能来自对流上地幔而不是深部的核-幔界面。换言之，峨眉山LIP的形成受控于岩石圈地幔过程而不是地幔柱过程。 相似文献
9.
苏皖地区幔源橄榄岩捕瞄虏体的锇同位素组成、模式年龄及其意义 总被引：9，自引：5，他引：9
苏皖地区发育的新生代玄武岩中富含地幔橄榄岩捕虏体，测定了25个橄榄岩全岩的锇同位素组成。结果表明大部分样品呈亏损特征,187Os/188Os=0.119～0.129.Os同位素比值与主量成分之间有显著的相关性.采用187Os/188Os-Al2O3代用等时线方法,由截距得到初始值(187Os/188Os)0=0.109,在对流地幔的187Os/188Os比值演化线上获得模式年龄t=2.5(±0.1)Ga,为晚太古-早元古代。用样品组中最低的锇同位素组成,即187Os/188Os=0.119,计算Re亏损模式年龄,t=1.2Ga,为中元古代。表明苏皖地区新生代玄武岩中的地幔橄榄岩捕虏体具有古老的形成年龄,它们是经过显生宙减薄作用后的残余地幔的碎片。大陆岩石圈地幔的古老形成年龄与上覆地壳克拉通的古老稳定年龄相耦合。 相似文献
10.
Re-Os同位素组成测试方法及其应用进展 总被引：1，自引：0，他引：1
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CCl4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。 相似文献
11.
12.
Geological reference materials (RMs) with variable compositions and NIST SRM 612 were analysed by isotope dilution mass spectrometry for bulk rock concentrations of chalcogen elements (sulfur, selenium and tellurium), rhenium and platinum‐group elements (PGEs: Ru, Pd, Os, Ir and Pt), including the isotope amount ratios of 187Os/188Os. All concentrations were obtained from the same aliquot after HCl‐HNO3 digestion in a high pressure asher at 320 °C. Concentrations were determined after chemical separation by negative TIMS, ICP‐MS and hydride generation ICP‐MS (Se, Te). As in previous studies, concentrations of the PGEs in most RMs were found to be highly variable, which may be ascribed to sample heterogeneity at the < 1 g level. In contrast, S, Se and Te displayed good precision (RSD < 5%) in most RMs, suggesting that part of the PGE budget is controlled by different phases, compared with the chalcogen budget. The method may minimise losses of volatile chalcogens during the closed‐system digestion and indicates the different extent of heterogeneity of chalcogens, Re and PGEs in the same sample aliquot. OKUM, SCo‐1, MRG‐1, DR‐N and MAG‐1 are useful RMs for the chalcogens. NIST SRM 612 displays homogenous distribution of S, Se, Te, Pt and Pd in 30 mg aliquots, in contrast with micro‐scale heterogeneity of Se, Pd and Pt. 相似文献
13.
Osmium isotopic compositions, and Re and Os concentrations have been examined in one komatiite unit and two komatiitic basalt units at Dundonald Beach, part of the 2.7 Ga Kidd-Munro volcanic assemblage in the Abitibi greenstone belt, Ontario, Canada. The komatiitic rocks in this locality record at least three episodes of alteration of Re-Os elemental and isotope systematics. First, an average of 40% and as much as 75% Re may have been lost due to shallow degassing during eruption and/or hydrothermal leaching during or immediately after emplacement. Second, the Re-Os isotope systematics of whole rock samples with 187Re/188Os ratios >1 were reset at ∼2.5 Ga, possibly due to a regional metamorphic event. Third, there is evidence for relatively recent gain and loss of Re in some rocks.Despite the open-system behavior, some aspects of the Re-Os systematics of these rocks can be deciphered. The bulk distribution coefficient for Os (DOssolid/liquid) for the Dundonald rocks is ∼3 ± 1 and is well within the estimated D values obtained for komatiites from the nearby Alexo area and stratigraphically-equivalent komatiites from Munro Township. This suggests that Os was moderately compatible during crystal-liquid fractionation of the magmas parental to the Kidd-Munro komatiitic rocks. Whole-rock samples and chromite separates with low 187Re/188Os ratios (<1) yield a precise chondritic average initial 187Os/188Os ratio of 0.1083 ± 0.0006 (γOs = 0.0 ± 0.6) for their well-constrained ∼2715 Ma crystallization age. The chondritic initial Os isotopic composition of the mantle source for the Dundonald rocks is consistent with that determined for komatiites in the Alexo area and in Munro Township, suggesting that the mantle source region for the Kidd-Munro volcanic assemblage had evolved with a long-term chondritic Re/Os before eruption. The chondritic initial Os isotopic composition of the Kidd-Munro komatiites is indistinguishable from that of the projected contemporaneous convective upper mantle. The uniform chondritic Os isotopic composition of the Kidd-Munro komatiites contrasts with the typical large-scale Os isotopic heterogeneity in the mantle sources for ca. 89 Ma komatiites from the Gorgona Island, arc-related rocks and present-day ocean island basalts. This suggests that the Kidd-Munro komatiites sampled a late-Archean mantle source region that was significantly more homogeneous with respect to Re/Os relative to most modern mantle-derived rocks. 相似文献
14.
Os同位素在花岗岩物质来源示踪中的初步研究:以湖南骑田岭岩体为例 总被引：3，自引：0，他引：3
Re-Os同位素在基性-超基性岩物质来源示踪方面已得到较广泛应用,但在酸性岩方面尚属少见。与其它同位素体系不同,Re、Os均为高亲铁元素,在岩浆分异演化过程中,Re属于中等不相容元素,Os属于强相容元素,地壳和地幔两端员Os同位素组成差别较大,因此,Re-Os同位素是研究花岗岩中是否存在幔源物质贡献的灵敏示踪剂。通过采自湖南骑田岭复式岩体三个阶段15件花岗岩全岩样品Re-Os同位素的分析,这些样品中Re、Os含量极低(Re含量0.0053～0.4539ng/g,Os含量0.0011～0.0328ng/g),Os同位素初始比值为0.3543～1.728,波动较大,显示骑田岭岩体成岩物质具有壳幔混合来源的特征。其中,早阶段与新田岭钨成矿关系密切的中粗粒似斑状角闪石黑云母花岗岩中壳源物质贡献更多一些,而晚阶段与芙蓉锡矿关系密切的细粒黑云母花岗岩幔源物质相对更多一些。Re-Os同位素的研究,不仅能够为花岗岩物质来源与成因机制的研究提供新的手段,而且,对于获取南岭重点矿集区深部成矿的地球化学信息、探索南岭矿集区壳幔相互作用过程以及幔源岩浆在不同类型矿化花岗岩形成过程中的作用也具有重要意义。 相似文献
15.
Lukáš Ackerman Richard J. Walker Lynnette Pitcher Ladislav Strnad 《Geochimica et cosmochimica acta》2009,73(8):2400-5596
The effects of melt percolation on highly siderophile element (HSE) concentrations and Re-Os isotopic systematics of subcontinental lithospheric mantle are examined for a suite of spinel peridotite xenoliths from the 4 Ma Kozákov volcano, Bohemian Massif, Czech Republic. The xenoliths have previously been estimated to originate from depths ranging from ∼32 to 70 km and represent a layered upper mantle profile. Prior petrographic and lithophile trace element data for the xenoliths indicate that they were variably modified via metasomatism resulting from the percolation of basaltic melt derived from the asthenosphere. Chemical and isotopic data suggest that lower sections of the upper mantle profile interacted with melt characterized by a primitive, S-undersaturated composition at high melt/rock ratios. The middle and upper layers of the profile were modified by more evolved melt at moderate to low melt/rock ratios. This profile permits an unusual opportunity to examine the effects of variable melt percolation on HSE abundances and Os isotopes.Most HSE concentrations in the studied rocks are significantly depleted compared to estimates for the primitive upper mantle. The depletions, which are most pronounced for Os, Ir and Ru in the lower sections of the mantle profile, are coupled with strong HSE fractionations (e.g., OsN/IrN ratios ranging from 0.3 to 2.4). Platinum appears to have been removed from some rocks, and enriched in others. This enrichment is coupled with lithophile element evidence for the degree of percolating melt fractionation (i.e., Ce/Tb ratio).Osmium isotopic compositions vary considerably from subchondritic to approximately chondritic (γOs at 5 Ma from -6.9 to +2.1). The absence of correlations between 187Os/188Os and indicators of fertility, as is common in many lithospheric mantle suites, may suggest significant perturbation of the Os isotopic compositions of some of these rocks, but more likely reflect the normal range of isotopic compositions found in the modern convecting mantle. Osmium isotopic compositions correspondingly yield model Re-depletion (TRD) ages that range from essentially modern to ∼1.3 Ga.Our data provide evidence for large-scale incompatible behavior of HSE during melt percolation as a result of sulfide dissolution, consistent with observations of prior studies. The degree of incompatibility evidently depended on melt/rock ratios and the degree of S-saturation of the percolating melt. The high Pt contents of some of these rocks suggest that the Pt present in this pervasively metasomatized mantle was controlled by a phase unique to the other HSE. Further, high Os concentrations in several samples suggest deposition of Os in a minority of the samples by melt percolation. In these rocks, the mobilized Os was characterized by similar to the 187Os/188Os ratios in the ambient rocks. There is no evidence for either the addition of Os with a strongly depleted isotopic composition, or Os with suprachondritic isotopic composition, as is commonly observed under such circumstances. 相似文献
16.
The Rhön area as part of the Central European Volcanic Province (CEVP) hosts an unusual suite of Tertiary 24-Ma old hornblende-bearing alkaline basalts that provide insights into melting and fractionation processes within the lithospheric mantle. These chemically primitive to slightly evolved and isotopically (Sr, Nd, Pb) depleted basalts have slightly lower Hf isotopic compositions than respective other CEVP basalts and Os isotope compositions more radiogenic than commonly observed for continental intraplate alkaline basalts. These highly radiogenic initial 187Os/188Os ratios (0.268–0.892) together with their respective Sr–Nd–Pb isotopic compositions are unlikely to result from crustal contamination alone, although a lack of Os data for lower crustal rocks from the area and limited data for CEVP basalts or mantle xenoliths preclude a detailed evaluation. Similarly, melting of the same metasomatized subcontinental lithospheric mantle as inferred for other CEVP basalts alone is also unlikely, based on only moderately radiogenic Os isotope compositions obtained for upper mantle xenoliths from elsewhere in the province. Another explanation for the combined Nd, Sr and Os isotope data is that the lavas gained their highly radiogenic Os isotope composition through a mantle “hybridization”, metasomatism process. This model involves a mafic lithospheric component, such as an intrusion of a sublithospheric primary alkaline melt or a melt derived from subducted oceanic material, sometime in the past into the lithospheric mantle where it metasomatized the ambient mantle. Later at 24 Ma, thermal perturbations during rifting forced the isotopically evolved parts of the mantle together with the peridotitic ambient mantle to melt. This yielded a package of melts with highly correlated Re/Os ratios and radiogenic Os isotope compositions. Subsequent movement through the crust may have further altered the Os isotope composition although this effect is probably minor for the majority of the samples based on radiogenic Nd and unradiogenic Sr isotope composition of the lavas. If the radiogenic Os isotope composition can be explained by a mantle-hybridization and metasomatism model, the isotopic compositions of the hornblende basalts can be satisfied by ca. 5–25% addition of the mafic lithospheric component to an asthenospheric alkaline magma. Although a lack of isotope data for all required endmembers make this model somewhat speculative, the results show that the Re–Os isotope system in continental basalts is able to distinguish between crustal contamination and derivation of continental alkaline lavas from isotopically evolved peridotitic lithosphere that was contaminated by mafic material in the past and later remelted during rifting. The Hf isotopic compositions are slightly less radiogenic than in other alkaline basalts from the province and indicate the derivation of the lavas from low Lu–Hf parts of the lithospheric mantle. The new Os and Hf isotope data constrain a new light of the nature of such metasomatizing agents, at least for these particular rocks, which represent within the particular volcanic complex the first product of the volcanism. 相似文献
17.
Mineralogical studies of the heavy fraction from a Holocene pyrope-rich garnet placer deposit at Vestřev (Krkonoše Piedmont Basin, Bohemian Massif) have identified the presence of very rare grains of platinum group minerals (PGM). Pt–Fe alloy grains are accompanied by Os–Ir–Ru minerals (native osmium, iridium, and ruthenium) with inclusions of Pt–Fe alloy and hongshiite (PtCu). This mineral assemblage is typical for several mantle settings including ophiolites. The chemistry of the Os–Ir–Ru minerals shows an enrichment of the PGM in Ru, which is typical of ophiolites. The grain morphology of PGM and pyrope-rich garnet (mostly rounded with numerous euhedral/subhedral grains) does not exclude a common source. In-situ laser-ablation MC-ICP-MS was used to measure the Re–Os isotopic compositions of single Os-rich grains, which show heterogeneous subchondritic Os isotopic compositions (187Os/188Os = 0.12082–0.12505 ± 0.00003). This precludes their low-temperature origin and indicates derivation of platinum-group elements (PGEs) essentially from mantle-derived rocks without a significant contribution of crustal Os. The mantle model age (TMA) and Re-depletion model age (TRD) model ages range from ~ 0.4 to ~ 1.0 Ga and most likely reflect a long history of melt depletion that affected the mantle sources of PGM. 相似文献
18.
Victoria C. Bennett Allen P. NutmanTezer M. Esat 《Geochimica et cosmochimica acta》2002,66(14):2615-2630
Initial 187Os/188Os isotopic compositions for geochronologically and geologically well -constrained 3.8-Ga spinel peridotites from the Itsaq Gneiss Complex of southern West Greenland and chromite separates from 3.46-Ga komatiites from the Pilbara region of Western Australia have been determined to investigate the osmium isotopic evolution of the early terrestrial mantle. The measured compositions of 187Os/188Os(0) = 0.10262 ± 2, from an olivine separate, and 0.10329 ± 3, for a spinel separate from ∼3.8-Ga peridotite G93/42, are the lowest yet reported from any terrestrial sample. The corrections for in situ decay over 3.8 Ga for these low Re/Os phases are minimal and change the isotopic compositions by only 0.5 and 2.2% for the spinel and the olivine, respectively, resulting in 187Os/188Os(3.8 Ga) = 0.1021 ± 0.0002 and 0.1009 ± 0.0002, respectively. These data extend direct measurement of Os isotopic compositions to much earlier periods of Earth history than previously documented and provide the best constraints on the Os isotopic composition of the early Archean terrestrial mantle. Analyses of Pilbara chromites yield 3.46-Ga mantle compositions of 0.1042 ± 0.0002 and 0.1051 ± 0.0002.These new data, combined with published initial Os isotopic compositions from late Archean and early Proterozoic samples, are compatible with the mantle, or at least portions of it, evolving from a solar system initially defined by meteorites to a modern composition of 187Os/188Os(0) = 0.1296 ± 0.0008 as previously suggested from peridotite xenolith data ( Meisel et al., 2001); the associated 187Re/188Os(0) = 0.435 ± 0.005. Thus, chondritic 187Os/188Os compositions were a feature of the upper mantle for at least 3.8 billion years, requiring chondritic Re/Os ratios to have been a characteristic of the very early terrestrial mantle. In contrast, nonchondritic initial compositions of some Archean komatiites demonstrate that Os isotopic heterogeneity is an ancient feature of plume materials, reflecting the development of variable Re/Os mantle sources early in Earth history.The lower average 187Os/188Os = 0.1247 for abyssal peridotites (Snow and Reisberg, 1995) indicate that not all regions of the modern mantle have evolved with the same Re/Os ratio. The relative sizes of the various reservoirs are unknown, although mass balance considerations can provide some general constraints. For example, if the unradiogenic 187Os/188Os modern abyssal peridotite compositions reflect the prevalent upper mantle composition, then the complementary high Re/Os basaltic reservoir must represent 20 to 40% by mass of the upper mantle (taken here as 50% of the entire mantle), depending on the mean storage age. The difficulties associated with efficient long-term storage of such large volumes of subducted basalt suggest that the majority of the upper mantle is not significantly Re-depleted. Rather, abyssal peridotites sample anomalous mantle regions.The existence of 3.8-Ga mantle peridotites with chondritic 187Os/188Os compositions and with Os concentrations similar to the mean abundances measured in modern peridotites places an upper limit on the timing of a late accretionary veneer. These observations require that any highly siderophile element -rich component must have been added to the Earth and transported into and grossly homogenized within the mantle by 3.8 Ga. Either large-scale mixing of impact materials occurred on very short (0-100 myr) timescales or (the interpretation preferred here) the late veneer of highly siderophile elements is unrelated to the lunar terminal cataclysm estimated to have occurred at ∼3.8 to 3.9 Ga. 相似文献