首页> 外文OA文献 >THE EXPERIMENTAL PARTITIONING BEHAVIOR OF TUNGSTEN AND PHOSPHORUS: IMPLICATIONS FOR THE COMPOSITION AND FORMATION OF THE EARTH, MOON AND EUCRITE PARENT BODY.
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THE EXPERIMENTAL PARTITIONING BEHAVIOR OF TUNGSTEN AND PHOSPHORUS: IMPLICATIONS FOR THE COMPOSITION AND FORMATION OF THE EARTH, MOON AND EUCRITE PARENT BODY.

机译:钨和磷的实验分配行为:对地球,月球和奥氏体母体的组成和形成的影响。

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摘要

The solid-metal/silicate-melt partition coefficient for W has been determined experimentally for the temperature and oxygen fugacity conditions at which eucritic basalts formed. The partition coefficient for W is 25 ± 5 at 1190°C and an oxygen fugacity of 10⁻¹³∙⁴. The solid-metal/silicate-melt partition coefficient for P, D(P), has been determined experimentally at 1190°C and 1300°C. The dependence of the partition coefficient on oxygen fugacity is consistent with a valence state of 5 for P in the silicate melt. The experimental partition coefficients are given by: (1) log D(P) = -1.21 log fO₂ -15.95 at 1190°C (2) log D(P) = -1.53 log fO₂ -17.73 at 1300°C The partition coefficients may be used to interpret the depletion of W/La and P/La ratios in the Earth, Moon, and eucrites relative to Cl chondrites. The depletion of the W/La ratios in the eucrites may be explained by partitioning of W into 2% to 10% solid metal assuming equilibration and separation of the metal from the silicates at low degrees of partial melting of the silicates. The depletion of P/La ratios requires an additional 5% to 25% sulfur-bearing metallic liquid. The depletion of both P/La and W/La ratios in the Moon can be explained by partitioning of P and W into liquid metal during formation of a small lunar core by metal-silicate separation at low degrees of partial melting of the silicates. The W/La ratios in the Earth and Moon are virtually indistinguishable, while P/La ratios differ by a factor of two. The concentrations of FeO also appear to be different. These observations are difficult to reconcile with the hypothesis of a terrestrial origin of the Moon following formation of the Earth's core, but are consistent with an independent formation of the Earth and Moon. In contrast to the Moon and eucrites, the depletion of P/La and W/La ratios in the Earth cannot be explained by an internally consistent model involving equilibrium between metal and silicate at low pressures.
机译:钨的固-金属/硅酸盐-熔体分配系数已通过实验确定了共沸玄武岩形成的温度和氧逸度条件。 W在1190℃的分配系数为25±5,氧逸度为10 13∙∙⁴。 P的固-金属/硅酸盐熔体分配系数D(P)已在1190°C和1300°C下通过实验确定。分配系数对氧逸度的依赖性与硅酸盐熔体中P的价态5一致。实验分配系数由下式给出:(1)在1190°C时log D(P)= -1.21 log fO 2 -15.95(2)在1300°C时log D(P)= -1.53​​ log fO 2 -17.73用来解释相对于Cl球粒陨石,地球,月球和纤锌矿中W / La和P / La比的消耗。假定在硅酸盐的部分熔融程度低的情况下将金属与硅酸盐进行平衡和分离,则可以通过将W分配到2%至10%的固态金属中来解释珠光体中W / La比的减少。 P / La比的消耗需要额外的5%至25%的含硫金属液体。月亮中P / La和W / La比值的减少可以通过在低硅酸盐部分熔融程度下通过金属-硅酸盐分离形成小月球芯期间将P和W分配到液态金属中来解释。实际上,地球和月球的W / La比几乎无法区分,而P / La比相差两倍。 FeO的浓度似乎也不同。这些观察很难与地球核心形成后的月球地球起源的假设相吻合,但与地球和月球的独立形成是一致的。与月球和珠光体相反,地球上P / La和W / La比的减少无法通过内部一致的模型来解释,该模型涉及低压下金属和硅酸盐之间的平衡。

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    NEWSOM HORTON ELWOOD.;

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  • 年度 1982
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