Characterization of iron meteorites by scanning electron microscopy, X‐ray diffraction, magnetization measurements, and Mössbauer spectroscopy: Kayakent <scp>IIIAB</scp>

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 α 2 ‐Fe(Ni, Co) grains, (ii) the γ‐Fe(Ni, Co) phase grains, (iii) the γ‐Fe(Ni, Co) rims around the α 2 ‐Fe(Ni, Co) phase areas, (iv) the cloudy zone (a mixture of the γ‐FeNi(Co) and α 2 ‐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 α ε ‐Fe(Ni, Co) with the presence of at least three different orientations of the α ε ‐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 α 2 ‐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 α 2 ‐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 57 Fe 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 α 2 ‐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.

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Publication Details

Journal
Meteoritics and Planetary Science
Published
2025-05-29
DOI
https://doi.org/10.1111/maps.14363
Citations
2
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
2.31

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article

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

I. Felner, Р. Ф. Муфтахетдинова, M. V. Goryunov, М. И. Оштрах et al.
2 citations
Meteoritics and Planetary Science
Astro and Planetary Science
2.31
article

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

I. Felner, Р. Ф. Муфтахетдинова, M. V. Goryunov, М. И. Оштрах, Gábor Varga, А. В. Чукин, Zoltán Dankházi, V. I. Grokhovsky, Z. Homonnay, Э. Кузманн
article en
2 citations

Abstract

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 α 2 ‐Fe(Ni, Co) grains, (ii) the γ‐Fe(Ni, Co) phase grains, (iii) the γ‐Fe(Ni, Co) rims around the α 2 ‐Fe(Ni, Co) phase areas, (iv) the cloudy zone (a mixture of the γ‐FeNi(Co) and α 2 ‐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 α ε ‐Fe(Ni, Co) with the presence of at least three different orientations of the α ε ‐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 α 2 ‐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 α 2 ‐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 57 Fe 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 α 2 ‐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.

Meteoritics and Planetary ScienceVol. 60(6)
Eötvös Loránd University (HU), Ural Federal University (RU), Hebrew University of Jerusalem (IL), Institute of Physics and Technology (RU)
Ministry of Science and Higher Education of the Russian Federation
Openalex Percentile: Top 12%
Astro and Planetary Science
2.31
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