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Microstructural evidence for a disequilibrium condensation origin for hibonite-spinel inclusions in the ALHA77307 CO3.0 chondrite

机译:微观结构证据表明ALHA77307 CO3.0球粒陨石中辉石-尖晶石夹杂物的不平衡凝结起源

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摘要

Two hibonite-spinel inclusions (CAIs 03 and 08) in the ALHA77307 CO3.0 chondrite have been characterized in detail using the focused ion beam sample preparation technique combined with transmission electron microscopy. These hibonite-spinel inclusions are irregularly shaped and porous objects and consist of randomly oriented hibonite laths enclosed by aggregates of spinel with fine-grained perovskite inclusions finally surrounded by a partial rim of diopside. Melilite is an extremely rare phase in this type of CAI and occurs only in one inclusion (CAI 03) as interstitial grains between hibonite laths and on the exterior of the inclusion. The overall petrologic and mineralogical observations suggest that the hibonite-spinel inclusions represent high-temperature condensates from a cooling nebular gas. The textural relationships indicate that hibonite is the first phase to condense, followed by perovskite, spinel, and diopside. Texturally, melilite condensation appears to have occurred after spinel, suggesting that the condensation conditions were far from equilibrium. The crystallographic orientation relationships between hibonite and spinel provide evidence of epitaxial nucleation and growth of spinel on hibonite surfaces, which may have lowered the activation energy for spinel nucleation compared with that of melilite and consequently inhibited melilite condensation. Hibonite contains abundant stacking defects along the (001) plane consisting of different ratios of the spinel and Ca-containing blocks within the ideal hexagonal hibonite structure. This modification of the stacking sequence is likely the result of accommodation of excess Al in the gas into hibonite due to incomplete condensation of corundum from a cooling gas under disequilibrium conditions. We therefore conclude that these two hibonite-spinel inclusions in ALHA77307 formed by high-temperature condensation under disequilibrium conditions.
机译:使用聚焦离子束样品制备技术与透射电子显微镜相结合,详细描述了ALHA77307 CO3.0球粒陨石中的两个辉石-尖晶石夹杂物(CAI 03和08)。这些辉石-尖晶石包裹体是不规则形状的多孔物体,由随机取向的辉石板条组成,它们被尖晶石的聚集体所包围,而钙钛矿包裹体的细粒最终被透辉石的部分边缘包围。堇青石是这种类型的CAI中极为稀少的相,仅在一个夹杂物(CAI 03)中出现,作为菱形板条之间和夹杂物外部的间隙晶粒。总体岩石学和矿物学观察结果表明,辉石-尖晶石包裹体代表了来自冷却星云气体的高温冷凝物。织构关系表明,菱铁矿是冷凝的第一阶段,其次是钙钛矿,尖晶石和透辉石。从质地上看,在尖晶石之后似乎发生了莫来石缩合,这表明缩合条件远非平衡。锂铁矿与尖晶石之间的晶体取向关系提供了证据,表明在锂铁矿表面上尖晶石的外延成核和生长,与硅镁石相比,可能降低了尖晶石成核的活化能,从而抑制了硅铁矿的凝结。在理想的六角形菱形组织中,菱形组织沿(001)平面包含大量堆积缺陷,该缺陷由尖晶石和含Ca嵌段的不同比例组成。堆积顺序的这种改变很可能是由于在不平衡条件下刚玉从冷却气体中不完全凝结而使气体中过量的Al容纳在菱铁矿中的结果。因此,我们得出的结论是,ALHA77307中的这两个hi石-尖晶石夹杂物是在不平衡条件下通过高温冷凝形成的。

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