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

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 α 2 ‐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 Fe 2+ 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.

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Publication Details

Journal
Meteoritics and Planetary Science
Published
2025-05-24
DOI
https://doi.org/10.1111/maps.14368
Citations
2
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
2.31

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article

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

I. Felner, Gregory Leitus, Maria Gritsevich, T. Kohout et al.
2 citations
Meteoritics and Planetary Science
Astro and Planetary Science
2.31
article

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

I. Felner, Gregory Leitus, Maria Gritsevich, T. Kohout, E. V. Petrova, M. V. Goryunov, М. И. Оштрах, Gábor Varga, А. В. Чукин, Zoltán Dankházi, A. A. Maksimova, Z. Homonnay, Э. Кузманн
article en
2 citations

Abstract

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 α 2 ‐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 Fe 2+ 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.

Meteoritics and Planetary ScienceVol. 60(7)
Eötvös Loránd University (HU), Ural Federal University (RU), Swedish Institute of Space Physics (SE), University of Helsinki (FI), University of South Carolina (US), Hebrew University of Jerusalem (IL), Institute of Physics and Technology (RU), Czech Academy of Sciences, Institute of Geology (CZ), Weizmann Institute of Science (IL), Aalto University (FI)
Academy of Finland, Ministry of Science and Higher Education of the Russian Federation
Openalex Percentile: Top 12%
Astro and Planetary Science
2.31
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