Characterization of iron meteorites by scanning electron microscopy, X-ray diffraction, magnetization measurements, and Mössbauer spectroscopy: Kayakent IIIAB

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
M. V. Goryunov, G. Varga, Z. Dankházi, A. V. Chukin, I. Felner, E. Kuzmann, Z. Homonnay, R. F. Muftakhetdinova, V. I. Grokhovsky, M. I. Oshtrakh
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引用次数: 0

Abstract

A fragment of the Kayakent IIIAB iron meteorite was analyzed using optical microscopy, scanning electron microscopy (SEM) with energy-dispersive spectroscopy (EDS) and electron backscatter diffraction (EBSD), X-ray diffraction (XRD), magnetization measurements, and Mössbauer spectroscopy. Optical microscopy and SEM show the presence of (i) the pure α2-Fe(Ni, Co) grains, (ii) the γ-Fe(Ni, Co) phase grains, (iii) the γ-Fe(Ni, Co) rims around the α2-Fe(Ni, Co) phase areas, (iv) the cloudy zone (a mixture of the γ-FeNi(Co) and α2-Fe(Ni, Co) phases), (v) plessite structures, and (vi) schreibersite inclusions in the α-Fe(Ni, Co) phase. The α-Fe(Ni, Co) phase demonstrates the ε-structure αε-Fe(Ni, Co) with the presence of at least three different orientations of the αε-Fe(Ni, Co) microcrystals, as shown by EBSD. EDS indicates variations in the Ni concentrations in the following ranges: (i) ~5.4–7.2 atom% in the α-Fe(Ni, Co) phase, (ii) ~15–18 atom% in the α2-Fe(Ni, Co) phase, and (iii) ~29–47 atom% in the γ-Fe(Ni, Co) phase grains. Schreibersite inclusions contain ~23.5–23.6 atom% of P, ~45.1–46.5 atom% of Fe, and ~28.8–31.4 atom% of Ni. The presence of ~98.1 wt% of the α-Fe(Ni, Co) phase and ~1.9 wt% of the γ-Fe(Ni, Co) phase is found by XRD in the powdered sample, while schreibersite is detected by XRD in the surface of the section only. Magnetization measurements show ferromagnetic multiphase material and a magnetic saturation moment of 175 emu g−1. The room temperature Mössbauer spectrum of the powdered Kayakent IIIAB sample demonstrates six magnetic sextets related to the ferromagnetic α2-Fe(Ni, Co), α-Fe(Ni, Co), and γ-Fe(Ni, Co) phases and one singlet assigned to the paramagnetic γ-Fe(Ni, Co) phase. In addition, the Mössbauer spectrum shows six minor magnetic sextets associated with 57Fe in the M1, M2, and M3 sites in schreibersite and one minor doublet shape assigned to the superparamagnetic rhabdite microcrystals. The iron fractions in the detected phases can be roughly estimated as follows: (i) ~11.9% in the α2-Fe(Ni, Co) phase, (ii) ~75.6% in the α-Fe(Ni, Co) phase, (iii) ~5.7% in the disordered γ-Fe(Ni, Co) phase with Ni content of ~34–40 atom%, (iv) ~1.5% in the more ordered γ-Fe(Ni, Co) phase with a higher Ni content (~46–47 atom%), (v) ~0.5% in the paramagnetic γ-Fe(Ni, Co) phase (~29–33 atom% of Ni), (vi) ~3% in schreibersite, and (vii) ~2% in rhabdite.

铁陨石的表征通过扫描电子显微镜,x射线衍射,磁化测量,和Mössbauer光谱:Kayakent IIIAB
对Kayakent IIIAB铁陨石的一块碎片进行了光学显微镜、扫描电子显微镜(SEM)、能量色散光谱(EDS)和电子背散射衍射(EBSD)、x射线衍射(XRD)、磁化测量和Mössbauer光谱分析。光学显微镜和扫描电镜显示:(i)纯α2-Fe(Ni, Co)晶粒,(ii) γ-Fe(Ni, Co)相晶粒,(iii) α2-Fe(Ni, Co)相周围的γ-Fe(Ni, Co)边缘,(iv)浑浊区(γ-FeNi(Co)和α2-Fe(Ni, Co)相的混合物),(v)硅质体结构,(vi) α-Fe(Ni, Co)相的晶状体包裹体。EBSD显示,α-Fe(Ni, Co)相具有α- ε- fe (Ni, Co)的ε-结构,α- ε- fe (Ni, Co)微晶至少存在三个不同取向。能谱分析结果表明:α-Fe(Ni, Co)相的Ni含量变化范围为(i) ~ 5.4-7.2原子%,α-Fe(Ni, Co)相的Ni含量变化范围为(ii) ~ 15-18原子%,γ-Fe(Ni, Co)相的Ni含量变化范围为(iii) ~ 29-47原子%。schreiberite夹杂物含有~23.5 ~ 23.6原子%的P, ~45.1 ~ 46.5原子%的Fe和~28.8 ~ 31.4原子%的Ni。粉末样品中存在~ 98.1%的α-Fe(Ni, Co)相和~1.9 wt%的γ-Fe(Ni, Co)相,而截面表面则存在~1.9 wt%的晶贝体。磁化测量显示铁磁性多相材料,磁饱和力矩为175 emu g−1。粉末Kayakent IIIAB样品的室温Mössbauer谱显示了与铁磁性α2-Fe(Ni, Co)、α-Fe(Ni, Co)和γ-Fe(Ni, Co)相相关的6个磁性六重体和与顺磁性γ-Fe(Ni, Co)相相关的1个单线态。此外,Mössbauer光谱显示,在晶氏体的M1、M2和M3位点有6个与57Fe相关的小磁六重体,而超顺磁性横纹石微晶体有一个小的双重体形状。检测相中铁的含量大致可估计为:(i) α2-Fe(Ni, Co)相中铁的含量为11.9%,(ii) α-Fe(Ni, Co)相中铁的含量为75.6%,(iii)无序的γ-Fe(Ni, Co)相中铁的含量为~ 34-40原子%,(iv)有序的γ-Fe(Ni, Co)相中铁的含量为~ 46-47原子%,(v)顺磁的γ-Fe(Ni, Co)相中铁的含量为~0.5%,顺磁的γ-Fe(Ni, Co)相中铁的含量为~ 29-33原子%,(vi) schreiberite中铁的含量为~3%,(vii) rhabite中铁的含量为~2%。
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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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