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|Title:||Applications of mössbauer spectroscopy in meteoritical and planetary science, part ii: Differentiated meteorites, moon, and mars|
|Authors:||Maksimova, A. A.|
Goryunov, M. V.
Oshtrakh, M. I.
|Citation:||Maksimova A. A. Applications of mössbauer spectroscopy in meteoritical and planetary science, part ii: Differentiated meteorites, moon, and mars / A. A. Maksimova, M. V. Goryunov, M. I. Oshtrakh. — DOI 10.3390/min11060612 // Minerals. — 2021. — Vol. 11. — Iss. 6. — 612.|
|Abstract:||Mössbauer (nuclear γ-resonance) spectroscopy is a powerful technique which 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, got a Nobel Prize in physics in 1961 for this discovery.57 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 using57 Fe Mössbauer spectroscopy as an 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 a recent investigation of the Martian surface using two rovers equipped with miniaturized Mössbauer spectrometers. Part I considered the results of Mössbauer spectroscopy of undifferentiated meteorites. Part II discusses the results of Mössbauer spectroscopy of differentiated meteorites formed in asteroids and protoplanets due to matter differentiation, as well as Lunar and Martian matter. © 2021 by the authors. Licensee MDPI, Basel, Switzerland.|
|Keywords:||57 FE HYPERFINE INTERACTIONS|
57 FE MÖSSBAUER SPECTROSCOPY
FE2+ PARTITIONING IN SILICATE PHASES
IRON-BEARING PHASE COMPOSITION
TEMPERATURE OF CATION EQUILIBRIUM DISTRIBUTION IN SILICATE PHASES
|metadata.dc.description.sponsorship:||This work was supported by the Ministry of Science and Higher Education of the Russian Federation, project No. 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 No. AAAA-A19-119071090011-6 (A.A.M.).|
|Appears in Collections:||Научные публикации, проиндексированные в SCOPUS и WoS CC|
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