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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Diffusion kinetics of Cr in spinel: Experimental studies and implications for Mn-53-Cr-53 cosmochronology
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Diffusion kinetics of Cr in spinel: Experimental studies and implications for Mn-53-Cr-53 cosmochronology

机译:Cr在尖晶石中的扩散动力学:实验研究及其对Mn-53-Cr-53天文学的意义

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The Mn-53-Cr-53 decay system, in which Mn-53 decays to Cr-53 (t(1/2) = 3.7 Ma) has been widely used to construct Cr-53/Cr-52 vs. Mn-55/Cr-52 isochrons and thus determine relative ages of early solar system objects or events, assuming that the initial Cr isotopic ratio, (Cr-53/Cr-52)(o), equals (Mn-55/Cr-52)(o). With the primary objective of interpretation of these ages within a diffusion kinetic framework, we have determined the tracer diffusion coefficient of Cr in natural spinels, which are very close to the MgAl2O4 end-member composition, as a function of temperature and oxygen fugacity (f(O-2)). It is found that the diffusion coefficient of Cr, D(Cr), in two stocks of spinels (referred to as cut-gems and gem-gravels) with very similar major element chemistry is consistently different, but the data in each stock yield well defined Arrhenius relations that show a difference of log D of 0.6-1.0, depending on temperature, with the D(Cr) in gem-gravel being higher than that in the cut-gem stock. The D(Cr) was found to have a positive dependence on f(O-2) in the range of f(O-2) of around +/- 2 log units relative to that of the wustite-magnetite buffer. The difference in the D(Cr) between the two stocks and the observed D(Cr) vs. f(O2) relation has been explained in terms of a change of point defect concentration resulting from heterovalent substitution of trace elements and equilibration with the imposed f(O-2) conditions, respectively. Assuming a homogeneous semi-infinite matrix, the closure temperature (T-c) of Cr diffusion in spinel has been calculated as a function of grain size, cooling rate, peak temperature (To) and f(O-2). Also the dependence of D(Cr) and T-c(Cr) on the Cr# (i.e. Cr/(Cr + Al) ratio) has been accounted for using available D(Cr) vs. Cr# data in Suzuki et al. (2008). We argue, on the basis of crystal chemical considerations and available diffusion kinetic data for minerals, that the T-c for Mn should be much lower than that for Cr in spinel, olivine and orthopyroxene, and discuss the potential implications of the anticipated disparity between T-c(Cr) and T-c(Mn) for the estimation of the (Mn-53/Mn-55)(o) ratio from an internal isochron defined by these minerals. Finally, we discuss the problem of determining the Tc for an internal isochron in relation to the individual Tc(Cr) for spinel, olivine and orthopyroxene. (C) 2016 The Authors. Published by Elsevier Ltd.
机译:Mn-53-Cr-53衰变系统,其中Mn-53衰变成Cr-53(t(1/2)= 3.7 Ma)已被广泛用于构造Cr-53 / Cr-52与Mn-55 / Cr-52等时线,并由此确定早期太阳系物体或事件的相对年龄,假设初始Cr同位素比(Cr-53 / Cr-52)(o)等于(Mn-55 / Cr-52)( o)。出于在扩散动力学框架内解释这些年龄的主要目的,我们确定了在自然尖晶石中Cr的示踪剂扩散系数,其与MgAl2O4末端成员组成非常接近,是温度和氧逸度(f (O-2))。发现在具有非常相似的主要元素化学特征的两种尖晶石储备中的Cr,D(Cr)扩散系数始终是不同的,但是每种储备中的数据都很好定义的阿伦尼乌斯关系,根据温度,log D的对数D差异为0.6-1.0,宝石砾石中的D(Cr)高于切工坯料中的D(Cr)。发现D(Cr)在f(O-2)范围内相对于f-O-磁铁矿缓冲中的f(O-2)具有正相关性,该范围约为+/- 2 log单位。两种储量之间的D(Cr)差异以及观察到的D(Cr)与f(O2)的关系已根据痕量元素的异价取代和施加的平衡导致的点缺陷浓度变化进行了解释。 f(O-2)条件。假设均质的半无限基体,则计算出尖晶石中Cr扩散的闭合温度(T-c)是晶粒尺寸,冷却速率,峰值温度(To)和f(O-2)的函数。 Suzuki等人还利用可用的D(Cr)与Cr#数据来说明D(Cr)和T-c(Cr)对Cr#的依赖性(即Cr /(Cr + Al)比)。 (2008)。我们基于晶体化学考虑因素和可用的矿物扩散动力学数据,认为尖晶石,橄榄石和邻二甲苯中Mn的Tc应该远低于Cr的Tc,并讨论预期的Tc之间的差异的潜在影响( Cr)和Tc(Mn),以便根据这些矿物定义的内部等时线估算(Mn-53 / Mn-55)(o)比。最后,我们讨论了确定内部等时线的Tc与尖晶石,橄榄石和邻二甲苯的单个Tc(Cr)有关的问题。 (C)2016作者。由Elsevier Ltd.发布

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