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Experimental constraints on ureilite petrogenesis

机译:实验中对绢云母成岩作用的限制

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This experimental study explores the petrogenesis of ureilites by a partial melting/smelting process. Experiments have been performed over temperature (1150-1280 degrees C), pressure (5-12.5 MPa), and low oxygen fugacity (graphite-CO gas) conditions appropriate for a hypothetical ureilite parent body similar to 200 km in size. Experimental and modeling results indicate that a partial melting/smelting model of ureilite petrogenesis can explain many of the unique characteristics displayed by this meteorite group. Compositional information preserved in the pigeonite-olivine ureilites was used to estimate the composition of melts in equilibrium with the ureilites. The results of 20 experiments saturated with olivin,, pyroxene, metal, and liquid with appropriate ureilite compositions are used to calibrate the phase coefficients and pressure-temperature dependence of the smelting reaction. The calibrated coefficients are used to model the behavior of a hypothetical residue that is, experiencing fractional smelting. The residue is initially olivine-rich and smelting progressively depletes the olivine content and enriches the pyroxene and metal contents of the residues. The modeled residue composition at 1260 degrees C best reproduces the trend of ureilite bulk compositions. The model results also indicate that as a ureilite residue undergoes isothermal decompression smelting over a range of temperatures, Ca/Al values and Cr2O3 contents are enriched at lower temperatures (below similar to 1240 degrees C) and tend to decrease at higher temperatures. Therefore, fractional smelting can account for the high Ca/Al and Cr2O3 wt% values observed in ureilites. We propose that ureilites were generated from an olivine-rich, cpx-bearing residue. Smelting began when the residue was partially melted and contained liquid, olivine, and carbon. These residues experienced varying degrees of fractional smelting to produce the compositional variability observed within the pigeonite-bearing ureilites. Variations in mineral composition, modal proportions, and isotopic signatures are best described by heterogeneous accretion of the ureilite parent body followed by minimal and variable degrees of igneous processing. (c) 2005 Elsevier Inc. All rights reserved.
机译:这项实验研究通过部分熔融/熔融过程探索了尿素岩的成岩作用。已经在温度(1150-1280摄氏度),压力(5-12.5 MPa)和低氧逸度(石墨-CO气体)条件下进行了实验,该条件适用于大小约为200 km的假想的尿素石母体。实验和模型结果表明,部分陨石成岩的熔融/熔融模型可以解释该陨石群显示的许多独特特征。保留在皂石-橄榄石滑石中的组成信息用于估计与滑石平衡的熔体组成。 20个实验的结果用饱和的橄榄石,辉石,金属和液体以及适当的硅藻土组成饱和,用于校准熔炼反应的相系数和压力-温度依赖性。校准的系数用于对假设的残渣的行为进行建模,该残渣正在经历部分熔炼。残留物最初富含橄榄石,冶炼逐渐消耗掉橄榄石含量,并富集残留物中的辉石和金属含量。在1260摄氏度下建模的残留物成分最好地再现了尿素块状成分的趋势。该模型结果还表明,随着苏莱石残余物在一定温度范围内进行等温减压熔炼,Ca / Al值和Cr2O3含量在较低温度(低于1240摄氏度)下富集,并在较高温度下趋于降低。因此,分步熔炼可说明在尿素石中观察到的高Ca / Al和Cr2O3重量%值。我们建议从富含橄榄石的,含cpx的残留物中产生尿素。当残余物部分熔融并包含液体,橄榄石和碳时,开始熔融。这些残留物经历了不同程度的分级熔炼,从而产生了在带皂石的尿素石中观察到的成分变异性。矿物组成,模态比例和同位素特征的变化最好通过将尿素石母体异质积聚,然后进行最小程度和可变程度的火成岩来描述。 (c)2005 Elsevier Inc.保留所有权利。

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