Comparison of the iron-bearing crystals and phases from Tamdakht H5 and Annama H5 ordinary chondrites by X-ray diffraction, magnetization measurements and Mössbauer spectroscopy

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
M. V. Goryunov, E. V. Petrova, A. V. Chukin, A. A. Maksimova, G. Varga, Z. Dankházi, I. Felner, G. Leitus, M. Gritsevich, E. Kuzmann, Z. Homonnay, T. Kohout, M. I. Oshtrakh
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Abstract

The iron-bearing phases and crystals within (i) the bulk interior and the fusion crust from Tamdakht H5 and (ii) the bulk interior from Annama H5 ordinary chondrites were studied by optical microscopy, scanning electron microscopy with energy dispersive spectroscopy, X-ray diffraction (XRD), magnetization measurements, and Mössbauer spectroscopy. The main iron-bearing phases/crystals such as olivine, orthopyroxene, clinopyroxene, troilite, chromite, and hercynite, as well as Fe-Ni-Co alloy with the α2-Fe(Ni, Co), α-Fe(Ni, Co) and γ-Fe(Ni, Co) phases were identified in both meteorites. XRD and Mössbauer spectroscopy showed high contents of Fe-Ni-Co alloy in the bulk interiors from Tamdakht H5 and Annama H5 ordinary chondrites. The fusion crust from Tamdakht H5 contains a new phase of magnesioferrite. A classification scheme for H, L, and LL ordinary chondrites using the relative areas of Mössbauer spectral components was applied to these meteorites' classification. The ratios of the M1 and M2 site occupations by Fe2+ in olivine and orthopyroxene were determined using XRD and Mössbauer spectroscopy, showing consistent results. The equilibrium cation distribution temperatures for olivine and orthopyroxene in Tamdakht H5 and Annama H5 were determined using XRD and Mössbauer spectroscopy.

Tamdakht H5和Annama H5普通球粒陨石含铁晶体和相的x射线衍射、磁化测量和Mössbauer光谱比较
采用光学显微镜、扫描电子显微镜、能谱、x射线衍射(XRD)、磁化测量和Mössbauer光谱等方法研究了Tamdakht H5球粒陨石(i)内部块状和熔合壳和(ii) Annama H5普通球粒陨石内部块状的含铁相和晶体。主要含铁相/晶为橄榄石、正辉石、斜辉石、三辉石、铬铁矿和海绢石,以及α2-Fe(Ni, Co)、α-Fe(Ni, Co)和γ-Fe(Ni, Co)相的Fe-Ni-Co合金。XRD和Mössbauer光谱分析表明,Tamdakht H5和Annama H5普通球粒陨石内部的Fe-Ni-Co合金含量较高。Tamdakht H5熔合壳含有一个新相的镁铁素体。利用Mössbauer光谱分量的相对面积对H、L、LL三种普通球粒陨石进行分类。利用XRD和Mössbauer光谱法测定了Fe2+在橄榄石和正辉石中M1和M2位点的占比,结果一致。采用XRD和Mössbauer光谱法测定了Tamdakht H5和Annama H5中橄榄石和正辉石的平衡阳离子分布温度。
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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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