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首页> 外文期刊>The American mineralogist >An experimental study of the oxidation state of vanadium in spinel and basaltic melt with implications for the origin of planetary basalt
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An experimental study of the oxidation state of vanadium in spinel and basaltic melt with implications for the origin of planetary basalt

机译:尖晶石和玄武质熔体中钒的氧化态的实验研究对行星玄武岩的起源有影响

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The distribution of V in magmatic rocks is controlled primarily by spinel stability. Extensive previous experimental work at oxidized conditions on doped (V-rich) compositions has led to the recognition of the importance of temperature, oxygen fugacity, and spinet composition, but also left ambiguity with respect to the relative importance of these variables in controlling D-v(spinel/melt). One major uncertainty has been the valence of V in the spinet and glass. Spinel-melt pairs were equilibrated at low and variable oxygen fugacities, with a range of V and Ti contents. XANES spectra were measured on the spinet and glass products, and pre-edge peaks measured and calibrated against valence with the use of glass and oxide standards. The valence of V is always greater in the glass than in the spinels. In spinet, V is dominantly 3+ at oxygen fugacities near the FMQ (fayalite magnetite quartz) buffer, but we find evidence for mixed 3+, 4+, and 5+ at oxidized conditions (FMQ to air), and 2+ and 3+ at very reduced conditions [FMQ to IW-1 (1 log f(O2) unit below the iron wustite buffer)]. Increased V contents in spinels are correlated with increased D-v(spinel-melt), at constant temperature and oxygen fugacity. However, increased Ti content causes only a slight decrease in D-v(spinel-melt) and a shift to more reduced V (smaller pre-edge peak), which may be related to Fe-V exchange equilibria. Using the new partition coefficients, together with published results and valence information, expressions have been derived to predict D-v(spinel/melt) for basaltic systems. Application of these expressions to natural suites illustrate their utility and also the great range of D-v(spinel/melt) values relevant to natural systems. Calculation of V depletions in planetary mantles from basalt suites must take silicate, oxide, and metal fractionation into account, as is demonstrated using terrestrial, lunar, martian, and eucritic samples.
机译:V在岩浆岩中的分布主要由尖晶石稳定性控制。以前在氧化条件下对掺杂的(富V)组合物进行的大量实验工作已导致人们认识到温度,氧逸度和尖晶石成分的重要性,但这些变量在控制Dv的相对重要性方面也存在歧义。尖晶石/熔体)。一个主要的不确定因素是尖晶石和玻璃中V的价。尖晶石熔体对在低和可变氧逸度下平衡,具有一定范围的V和Ti含量。 XANES光谱是在尖晶石和玻璃制品上测量的,并且使用玻璃和氧化物标准品测量了前边缘峰并针对化合价进行了校准。在玻璃中,V的价总是比在尖晶石中大。在刺子中,V在FMQ(铁橄榄石磁铁矿石英)缓冲液附近的氧逸度下占主导地位的3+,但我们发现在氧化条件下(FMQ到空气)混合3 +,4 +和5+的证据,以及2+和3 +在非常减少的条件下[FMQ至IW-1(铁水铁矿缓冲区下方1 log f(O2)单位)]。在恒定温度和氧气逸度下,尖晶石中V含量的增加与D-v(尖晶石熔体)的增加相关。但是,增加的Ti含量只会导致D-v(尖晶石熔体)略微降低,而向V的降低趋势(较小的前边缘峰)转移,这可能与Fe-V交换平衡有关。使用新的分配系数,连同已发布的结果和化合价信息,已得出表达式来预测玄武岩系的D-v(尖晶石/熔体)。这些表达式在自然套件中的应用说明了它们的效用以及与自然系统相关的D-v(尖晶石/熔体)值的范围。如玄武岩,月球,火星和同生样本所证明的那样,从玄武岩组中计算行星地幔中的V损耗必须考虑到硅酸盐,氧化物和金属的分馏。

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