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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >A new lunar high-Ti basalt type defined from clasts in Apollo 16 breccia 60639
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A new lunar high-Ti basalt type defined from clasts in Apollo 16 breccia 60639

机译:从阿波罗16角砾岩60639中的碎屑定义的新的月球高钛玄武岩类型

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摘要

This paper reports the detailed examination of three basalt clasts from Apollo 16 breccia 60639 that represent a new variant of high-Ti basalt returned from the Moon by the Apollo 16 mission. Mineral chemistry and whole-rock analyses were conducted on aliquots from three clasts (breccia matrix, basalt, and basalt + breccia matrix). The basalt clasts, which are not overtly porphyritic, contain compositionally zoned pyroxene, olivine, and plagioclase crystals that represent the evolution of the magma during crystallization; ilmenite does not exhibit major-element compositional zoning within individual crystals. Mineral compositions are distinct between the basalt and breccia matrix lithologies. In addition, whole-rock analyses identify clear compositional differences between the basalt and breccia matrix lithologies in both major and trace element concentrations. The composition of the mixed lithology aliquots (i.e., basalt + breccia matrix) do not indicate simple two component mixing (i.e., compositions are not intermediate to the basalt and breccia end-members); this apparent incongruity can be accounted for by adding similar to 19-40% plagioclase to an amalgamation of the average basalt and individual breccia clast compositions via impact mixing. Whole-rock analyses are consistent with previous analyses of one 60639 basalt clast, which were interpreted to indicate chemical similarity with Apollo 11 and 17 basalts. However, both major and trace elements suggest that the 60639 basalt clasts examined here have compositions that are distinct from Apollo 11 and 17 high-Ti basalts. Although the 60639 basalt clasts have similar characteristics to a variety of previously identified basalt types, the more extensive whole-rock analyses reported here indicate that they represent a type of Apollo high-Ti basalt heretofore unrecognized in the Apollo and lunar meteorite collections. By placing these new analyses in the context of other mare basalt compositions, a petrogenetic model for the basalts found in breccia 60639 is presented. (C) 2015 Elsevier Ltd. All rights reserved.
机译:本文报告了对来自阿波罗16角砾岩60639的三种玄武岩碎屑的详细检查,这三种岩石代表了由阿波罗16号任务从月球返回的高钛玄武岩的新变种。矿物化学和全岩体分析是对三种碎屑(角砾岩基质,玄武岩和玄武岩+角砾岩基质)的等分试样进行的。玄武岩碎屑不是明显的斑状,含有组成分区的辉石,橄榄石和斜长石晶体,它们代表了岩浆在结晶过程中的演化。钛铁矿在单个晶体中不显示主要元素组成区带。矿物成分在玄武岩和角砾岩基质岩性之间是不同的。此外,全岩体分析可以确定玄武岩和角砾岩基质岩性在主要元素和痕量元素浓度方面的明显成分差异。混合岩性等分试样的组成(即玄武岩+角砾岩基质)不表示简单的两组分混合(即,组成不在玄武岩和角砾岩端构件中间);这种明显的不一致性可以通过在平均玄武岩和单个角砾岩碎屑组合物的混合中添加约19-40%斜长石,通过冲击混合来解决。全岩体分析与之前对60639玄武岩碎屑的分析一致,这被解释为与Apollo 11和17玄武岩具有化学相似性。但是,主要元素和痕量元素均表明,此处检查的60639玄武岩碎屑具有与阿波罗11号和17种高钛玄武岩不同的成分。尽管60639玄武岩碎屑具有与各种先前确定的玄武岩类型相似的特征,但此处报道的更广泛的全岩分析表明,它们代表了迄今为止在阿波罗陨石和月球陨石集合中尚未发现的一种阿波罗高钛玄武岩。通过将这些新的分析放在其他母马玄武岩成分的背景下,提出了角砾岩60639中发现的玄武岩的成岩模型。 (C)2015 Elsevier Ltd.保留所有权利。

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