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首页> 外文期刊>Meteoritics & planetary science >Martian meteorite Dhofar 019: A new shergottite
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Martian meteorite Dhofar 019: A new shergottite

机译:火星陨石Dhofar 019:一种新的钙锰矿

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摘要

Dhofar 019 is a new martian meteorite found in the desert of Oman. In texture, mineralogy, and major and trace element chemistry, this meteorite is classified as a basaltic shergottite. Olivine megacrysts are set within a groundmass composed of finer grained olivine, pyroxene (pigeonite and augite), and maskelynite. Minor phases are chromite-ulvospinel, ilmenite, silica, K-rich feldspar, merrillite, chlorapatite, and pyrrhotite. Secondary phases of terrestrial origin include calcite, gypsum, celestite, Fe hydroxides, and smectite. Dhofar 019 is most similar to the Elephant Moraine (EETA) 79001 lithology a and Dar al Gani (DaG) 476/489 shergottites. The main features that distinguish Dhofar 019 from other shergottites are lack of orthopyroxene; lower Ni contents of olivine; the heaviest oxygen-isotopic bulk composition; and larger compositional ranges for olivine, maskelynite, and spinel, as well as a wide range for pyroxenes. The large compositional ranges of the minerals are indicative of relatively rapid crystallization. Modeling of olivine chemical zonations yield minimum cooling rates of 0.5-0.8 ℃/h. Spinel chemistry suggests that crystallization took place under one of the most reduced conditions for martian meteorites, at an fO_2 3 log units below the quartz-fayalite-magnetite (QFM) buffer. The olivine megacrysts are heterogeneously distributed in the rock. Crystal size distribution analysis suggests that they constitute a population formed under steady-state conditions of nucleation and growth, although a few grains may be comulates. The parent melt is thought to have been derived from partial melting of a light rare earth element- and platinum group element-depleted mantle source. Shergottites, EETA79001 lithology A, DaG 476/489, and Dhofar 019, although of different ages, comprise a particular type of martian rocks. Such rocks could have formed form chemically similar source(s) and parent melt(s), with their bulk compositions affected by olivine accumulation.
机译:Dhofar 019是在阿曼沙漠中发现的一种新的火星陨石。在质地,矿物学以及主要和微量元素化学上,该陨石被归类为玄武质黑云母。橄榄石巨晶位于由细粒橄榄石,辉石(ox石和a石)和蒙砂石组成的地基中。次要相为亚铬铁矿-ulsulpinel,钛铁矿,硅石,富钾长石,锰铁矿,氯磷灰石和黄铁矿。陆源的次生相包括方解石,石膏,天青石,氢氧化铁和蒙脱石。 Dhofar 019最类似于大象冰((EETA)79001岩性a和Dar al Gani(DaG)476/489隐身岩。使Dhofar 019与其他斜方锰矿区别开的主要特征是缺少邻苯二甲醚。降低橄榄石中的镍含量;最重的氧同位素本体组成;橄榄石,蒙砂石和尖晶石的成分范围更大,辉石的范围也很大。矿物的大组成范围表明结晶相对较快。橄榄石化学区域的建模产生的最小冷却速率为0.5-0.8℃/ h。尖晶石化学表明,结晶是在火星陨石还原度最高的条件之一下,在石英-铁橄榄石-磁铁矿(QFM)缓冲液以下的fO_2 3 log单位处发生的。橄榄石巨晶在岩石中异质分布。晶体粒度分布分析表明,它们构成了在成核和生长的稳态条件下形成的总体,尽管可能会混入一些晶粒。据认为,母体熔体来自贫稀土元素和铂族元素贫化地幔源的部分熔解。角铁矿,EETA79001岩性A,DaG 476/489和Dhofar 019,尽管年龄不同,但都包含特定类型的火星岩石。这样的岩石可能形成了化学上相似的一种或多种来源和母体熔体,它们的整体组成受橄榄石堆积的影响。

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