Please use this identifier to cite or link to this item: http://hdl.handle.net/10995/102874
Title: Applications of mössbauer spectroscopy in meteoritical and planetary science, part i: Undifferentiated meteorites
Authors: Maksimova, A. A.
Oshtrakh, M. I.
Issue Date: 2021
Publisher: MDPI AG
Citation: Maksimova A. A. Applications of mössbauer spectroscopy in meteoritical and planetary science, part i: Undifferentiated meteorites / A. A. Maksimova, M. I. Oshtrakh. — DOI 10.3390/min11060614 // Minerals. — 2021. — Vol. 11. — Iss. 6. — 614.
Abstract: Mössbauer (nuclear γ-resonance) spectroscopy is a powerful technique that is actively used in various fields, from physics and chemistry to biology and medicine. Rudolf L. Mössbauer, who observed nuclear γ-resonance and published his results in 1958, received a Nobel Prize in physics in 1961 for this discovery. The57 Fe is the most widely used nucleus in Mössbauer spectroscopy. Therefore, a large variety of compounds containing iron can be studied by Mössbauer spectroscopy. It is well known that planetary matter contains various iron-bearing phases and minerals. Therefore, the extraterrestrial material from different meteorites, asteroids, and planets can be studied using 57 Fe Mössbauer spectroscopy as additional powerful technique. Two parts of this review consider the results of more than 50 years of experience of Mössbauer spectroscopy applied for the studies of various meteorites, soils, and rocks from the Moon and recent investigation of the Mars surface using two rovers equipped with miniaturized Mössbauer spectrometers. Part I will discuss known results on Mössbauer spectroscopy of undifferentiated meteorites, which are the most primitive and formed with the solar system. © 2021 by the authors. Licensee MDPI, Basel, Switzerland.
Keywords: 57 FE HYPERFINE INTERACTIONS
57FE MÖSSBAUER SPECTROSCOPY
CHONDRITES WEATHERING
CLASSIFICATION OF H, L, AND LL ORDINARY CHONDRITES
FE2+ PARTITIONING IN SILICATE PHASES
FUSION CRUST
IRON-BEARING MINERALS
IRON-BEARING PHASE COMPOSITION
TEMPERATURE OF CATION EQUILIBRIUM DISTRIBUTION IN SILICATE PHASES
UNDIFFERENTIATED METEORITES
URI: http://hdl.handle.net/10995/102874
Access: info:eu-repo/semantics/openAccess
SCOPUS ID: 85107268173
PURE ID: 22106919
94b5375c-e43a-4907-8b00-2bd486e4bd40
ISSN: 2075163X
DOI: 10.3390/min11060614
metadata.dc.description.sponsorship: This work was supported by the Ministry of Science and Higher Education of the Russian Federation, project № FEUZ‐2020‐0060. The Zavaritsky Institute of Geology and Geochemistry of the Ural Branch of the Russian Academy of Sciences is supported by the Ministry of Science and Higher Education of the Russian Federation, project № AAAA‐A19‐119071090011‐6 (A.A.M.).
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