卡拉马009 L6普通软玉体内部和熔融结壳的特征描述

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Meteoritics & Planetary Science Pub Date : 2024-07-30 DOI:10.1111/maps.14249
E. V. Petrova, A. V. Chukin, G. Varga, Z. Dankházi, G. Leitus, I. Felner, E. Kuzmann, Z. Homonnay, V. I. Grokhovsky, M. I. Oshtrakh
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引用次数: 0

摘要

我们选择了在阿塔卡马沙漠发现的卡拉马 009 L6 普通软玉碎片,通过扫描电子显微镜(SEM)、能量色散光谱(EDS)、X 射线衍射(XRD)、磁化测量和莫斯鲍尔光谱,对其内部和熔融结壳进行了复杂的研究。扫描电子显微镜显示了铁-镍-钴晶粒、块状内部和熔融结壳中的铁锂石、铬铁矿包裹体以及许多含铁化合物的矿脉。EDS 显示,金属晶粒内部和晶粒中某一金属相内的镍浓度存在差异。X 射线衍射显示,内部和熔融结壳中各种相的含量存在一些差异。XRD 显示熔壳中存在菱镁铁,并且在主体内部和熔壳中都形成了平均尺寸为 9 纳米的网纹石纳米颗粒。磁化测量结果表明,铬铁矿在 44 K 时发生了铁磁-顺磁相变,由于风化导致铁-镍-钴合金缺乏,主体内部和熔壳的饱和磁化矩值较低(100 K 时分别为 6.46 和 3.26 emu g-1)。块体内部和熔融结壳的莫斯鲍尔光谱在光谱成分的数量和相对面积上存在一些差异。通过揭示橄榄石和正辉石 M1 和 M2 位点中与 57Fe 有关的莫斯鲍尔光谱成分,并通过 XRD 确定这些位点的 Fe2+ 占有率,我们可以估算出这些硅酸盐的平衡阳离子分布温度:(i) 橄榄石为 662 K(XRD)和 706 K(莫斯鲍尔光谱);(ii) 正辉石为 893 K(XRD)和 910 K(莫斯鲍尔光谱)。
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Characterization of bulk interior and fusion crust of Calama 009 L6 ordinary chondrite

Fragment of Calama 009 L6 ordinary chondrite recovered in the Atacama Desert was chosen for a complex study of the bulk interior and the fusion crust by scanning electron microscopy (SEM) with energy-dispersive spectroscopy (EDS), X-ray diffraction (XRD), magnetization measurements, and Mössbauer spectroscopy. SEM demonstrated the presence of Fe-Ni-Co grains, troilite and chromite inclusions in both the bulk interior and the fusion crust as well as many veins with ferric compound. EDS showed variations in the Ni concentration within the metal grains and within one metal phase in the grain. XRD revealed some differences in the contents of various phases in the bulk interior and in the fusion crust. XRD indicated the presence of magnesioferrite in the fusion crust as well as the formation of goethite nanoparticles with the mean size of 9 nm in both the bulk interior and the fusion crust. Magnetization measurements demonstrated the ferrimagnetic–paramagnetic phase transition in chromite at 44 K and low values of the saturation magnetization moments (6.46 and 3.26 emu g−1 at 100 K) for the bulk interior and the fusion crust, respectively, due to the lack of Fe-Ni-Co alloy as a result of weathering. The Mössbauer spectra of the bulk interior and the fusion crust showed some differences in the number and relative areas of spectral components. The revealing of the Mössbauer spectral components related to 57Fe in the M1 and M2 sites in olivine and orthopyroxene as well as determining the Fe2+ occupations of these sites from XRD permitted us to estimate the temperature of equilibrium cation distribution for these silicates which are (i) 662 K (XRD) and 706 K (Mössbauer spectroscopy) for olivine and (ii) 893 K (XRD) and 910 K (Mössbauer spectroscopy) for orthopyroxene.

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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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Issue Information Cover Constraints on the impact history of the Apollo 16 landing site: Implications of soil-like breccia noble gas records Issue Information Cover
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