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Phosphate and feldspar mineralogy of equilibrated L chondrites: The record of metasomatism during metamorphism in ordinary chondrite parent bodies

机译:L平衡球粒陨石的磷酸盐和长石矿物学:普通球粒陨石母体变质过程中的交代作用记录

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In ordinary chondrites (OCs), phosphates and feldspar are secondary minerals known to be the products of parent-body metamorphism. Both minerals provide evidence that metasomatic fluids played a role during metamorphism. We studied the petrology and chemistry of phosphates and feldspar in petrologic type 4-6 L chondrites, to examine the role of metasomatic fluids, and to compare metamorphic conditions across all three OC groups. Apatite in L chondrites is Cl-rich, similar to H chondrites, whereas apatite in LL chondrites has lower Cl/F ratios. Merrillite has similar compositions among the three chondrite groups. Feldspar in L chondrites shows a similar equilibration trend to LL chondrites, from a wide range of plagioclase compositions in petrologic type 4 to a homogeneous albitic composition in type 6. This contrasts with H chondrites which have homogeneous albitic plagioclase in petrologic types 4-6. Alkali- and halogen-rich and likely hydrous metasomatic fluids acted during prograde metamorphism on OC parent bodies, resulting in albitization reactions and development of phosphate minerals. Fluid compositions transitioned to a more anhydrous, Cl-rich composition after the asteroid began to cool. Differences in secondary minerals between H and L, LL chondrites can be explained by differences in fluid abundance, duration, or timing of fluid release. Phosphate minerals in the regolith breccia, Kendleton, show lithology-dependent apatite compositions. Bulk Cl/F ratios for OCs inferred from apatite compositions are higher than measured bulk chondrite values, suggesting that bulk F abundances are overestimated and that bulk Cl/F ratios in OCs are similar to CI.
机译:在普通球粒陨石(OCs)中,磷酸盐和长石是次生矿物,已知是母体变质的产物。两种矿物都提供了变质作用在变质过程中起作用的证据。我们研究了岩石学类型为4-6 L的球粒陨石中磷酸盐和长石的岩石学和化学性质,研究了交代液的作用,并比较了所有三个OC组的变质条件。 L球粒陨石中的磷灰石富含Cl,类似于H球粒陨石,而LL球粒陨石中的磷灰石具有较低的Cl / F比。在三个球粒陨石组中,美林石具有相似的组成。 L球粒长石显示出与LL球粒相似的平衡趋势,从岩石类型4的斜长石组成广泛到类型6的均质任意长石组成。这与在岩石学类型4-6中具有均质任意斜长石的H球粒形成对比。富含碱和卤素以及可能为水的交代液在OC母体的前驱变质过程中起作用,导致了碱化反应和磷酸盐矿物质的发展。小行星开始冷却后,流体成分转变为更无水的富含Cl的成分。 H和L,LL球粒陨石之间次生矿物的差异可以通过流体丰度,持续时间或流体释放时间的差异来解释。坚石角砾岩角砾岩中的磷酸盐矿物显示出与岩性有关的磷灰石成分。由磷灰石组成推断出的OC的体Cl / F比值高于测得的球粒陨石值,这表明高估了F体的丰度,并且OC中的体Cl / F比值与CI相似。

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