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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Ancient high Pt/Os crustal contaminants can explain radiogenic Os-186 in some intraplate magmas
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Ancient high Pt/Os crustal contaminants can explain radiogenic Os-186 in some intraplate magmas

机译:古代高Pt / OS外壳污染物可以解释一些内部岩浆岩浆中的辐射性OS-186

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The origin of variations in Os-186/Os-188 ratios amongst mantle-derived basaltic and komatiitic lavas remains controversial, with opposing models arguing for deep core-mantle versus shallow mantle sources. Crustal contamination has generally not been favored due to the low Os contents of such sources, meaning that variations in Os-186/Os-188 would require involvement of extremely high proportions of crustal material. Here we re-examine crustal contamination as an effective means for generating significant Os-186/Os-188 variations in Earth materials. Using chromitites and peridotites from the Stillwater, Muskox and Rum layered intrusions, we show that radiogenic Os-186/Os-188 ratios are correlated with Os-187/Os-188 ratios and can only be explained by shallow-level mixing processes and crustal contamination. The samples have delta Os-186 ([{(Os-186/Os-188(sample[t])/Os-186/Os-188(PM(t))) - 1) x 1000], where the modern primitive mantle [PM] Os-186/Os-188 is 0.1198388) values ranging between 0.04 to 0.15 for the similar to 2.7 Ga Stillwater Igneous Complex, -0.05 to 0.17 for the similar to 1.27 Ga Muskox Intrusion, and 0.02 to 0.13 for the similar to 0.06 Ga Rum Layered Suite. The highly siderophile element (HSE: Os, IL Ru, Pt, Pd, Re) contents of the chromitites and peridotites can be modeled through high sulfide-melt partitioning (typically >8000) and emphasize the role of S-saturation and HSE scavenging. Considering the high sulfide-melt partitioning and accounting for high silicate melt to sulfide melt ratios (R-factors), it is possible to explain the variations in Os-186/Os-188 in layered intrusions using calculated Os isotope crustal evolution growth models. These calculations indicate that <4% of ancient high Pt/Os crustal contributions can explain the composition of the chromitites and peridotites that were examined. Our observations are consistent with published models for chromitite genesis that invoke either crustal melt-primitive melt mixing, or cumulate as
机译:术士源性玄武岩和柯马蒂米特拉斯山脉之间的OS-186 / OS-188比率的变异起源仍然存在争议,反对模型对深核心披风的争论与浅地幔来源。由于这种来源的低OS含量,地壳污染通常没有受到青睐,这意味着OS-186 / OS-188的变化将需要参与极高比例的地壳材料。在这里,我们将地壳污染重新检查作为在地球材料中产生显着的OS-186 / OS-188变化的有效手段。使用铬酸盐和偏见来自静止物,麝香和朗姆酒分层入侵,我们表明辐射性OS-186 / OS-188比率与OS-187 / OS-188比率相关,只能通过浅水平混合过程和地壳解释污染。样品具有Delta OS-186([{(OS-186 / OS-188(样本[T])/ OS-186 / OS-188(PM(T))) - 1)x 1000],其中现代原始Mantle [PM] OS-186 / OS-188为0.1198388)值为0.04至0.15,类似于2.7 Ga Silldwater igneous复合物,-0.05至0.17,类似于1.27 Ga Muskox侵入,类似于0.02至0.13到0.06克朗分层套房。铬酸盐和恒星的高度磷酸化元素(HSE:OS,IL Ru,Pt,Pd,Re)含量可以通过高硫化物 - 熔体分配(通常> 8000)来建模,并强调S饱和度和HSE清除的作用。考虑到高硅酸盐熔体对硫化物熔体比率(R型因子)的高硫化物 - 熔体分配和算法,可以使用计算的OS同位素地壳演进生长模型来解释OS-186 / OS-188中的OS-186 / OS-188的变化。这些计算表明,古代高Pt / OS地壳贡献的<4%可以解释检查的铬酸盐和偏见的组成。我们的观察结果与发表的铬酸盐创世模型一致,其调用地壳熔融原始熔体混合或累积为

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