EVIDENCES OF WEATHERING OF IRON-NICKEL AND TROILITE IN THE GRUZ'KE Н4-TYPE CHONDRITE

IF 0.5 Q4 MINERALOGY
S. Shyrinbekova
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Abstract

Terrestrial weathering of the Gruz'ke chondrite was investigated by considering its initial chemical, structural, and mineralogical characteristics. The spread of corrosion and degree of alteration were related to the high content of Fe-Ni metal, the phase inhomogeneity and the different concentration of Ni in the metal, as well as, the shock metamorphism features, and the residence time of the meteorite sample in a soil environment. The formation of secondary oxide veins and oxide rims, consisting of iron hydroxide pseudomorphs was caused by the selective corrosion of kamacite α-(Fe,Ni), compared to taenite γ-(Fe,Ni) and troilite FeS. A spatial relationship between shock metamorphism features, namely areas of plastic deformation, shock heating and weathering of the meteorite matter, has been confirmed. A secondary Ni-enriched phase, which contains 71.34 to 72.94 wt.% Ni, probably corresponds to awaruite (Ni2Fe to Ni3Fe) or native nickel. This phase is described for the first time as corrosion product of Fe-Ni grains in the Gruz'ke chondrite. We assume that this phase was formed during the alteration of Fe-Ni metal. Fe was removed from the meteorite metal during the corrosion process, while sulfur was introduced. The formation of iron hydroxide pseudomorphs caused changes in primary chemical and structural properties of some crystals of nickel-iron metal and troilite. Thus, the use of weathered mineral grains to interpret the pre-terrestrial conditions of the chondrite matter formation and evolution is limited. In spite of the changes in chemical and mineral composition, the corrosion products of nickel iron and troilite have consistent low chlorine content.Therefore we assume that the akaganeite β-FeO(OH,Cl) secondary phase is unlikely to form. It will prevent further alteration of the Fe-Ni metal and ensure long-term storage and preservation of the meteorite sample for further laboratory research and storage in the museum collection.
gruz 'ke Н4-type球粒陨石中铁镍和三铁风化的证据
综合考虑格鲁兹克球粒陨石的初始化学、结构和矿物学特征,对其陆地风化进行了研究。腐蚀的范围和蚀变程度与铁镍金属含量高、物相不均匀性和金属中镍的浓度不同、冲击变质特征以及陨石样品在土壤环境中的停留时间有关。相对于带状长石γ-(Fe,Ni)和三亚硝石fees,镰状长石α-(Fe,Ni)的选择性腐蚀导致了由氢氧化铁伪晶组成的二次氧化脉和氧化环的形成。证实了冲击变质作用特征,即陨石物质的塑性变形区域、冲击加热区域和风化区域之间的空间关系。二次富镍相的Ni含量为71.34 ~ 72.94 wt.%,可能是原生镍(Ni2Fe ~ Ni3Fe)或原生镍。该相首次被描述为格鲁兹克球粒陨石中Fe-Ni晶粒的腐蚀产物。我们认为这一相是在Fe-Ni金属蚀变过程中形成的。在腐蚀过程中,铁从陨石金属中被去除,而硫被引入。氢氧化铁伪晶的形成引起了部分镍铁金属和三亚硝石晶体的主要化学性质和结构性质的变化。因此,利用风化矿物颗粒来解释球粒陨石物质形成和演化的陆前条件是有限的。尽管化学成分和矿物成分发生了变化,但镍铁和三亚硝石的腐蚀产物始终具有低氯含量。因此,我们认为赤线石β-FeO(OH,Cl)次级相不太可能形成。它将防止铁镍金属的进一步改变,并确保陨石样本的长期储存和保存,以供进一步的实验室研究和博物馆收藏。
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CiteScore
0.70
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0.00%
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18
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