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Название: | Applications of mössbauer spectroscopy in meteoritical and planetary science, part i: Undifferentiated meteorites |
Авторы: | Maksimova, A. A. Oshtrakh, M. I. |
Дата публикации: | 2021 |
Издатель: | MDPI AG |
Библиографическое описание: | 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. |
Аннотация: | 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. |
Ключевые слова: | 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://elar.urfu.ru/handle/10995/102874 |
Условия доступа: | info:eu-repo/semantics/openAccess |
Идентификатор РИНЦ: | 46829372 |
Идентификатор SCOPUS: | 85107268173 |
Идентификатор WOS: | 000666567300001 |
Идентификатор PURE: | 22106919 94b5375c-e43a-4907-8b00-2bd486e4bd40 |
ISSN: | 2075163X |
DOI: | 10.3390/min11060614 |
Сведения о поддержке: | 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.). |
Располагается в коллекциях: | Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC |
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Файл | Описание | Размер | Формат | |
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2-s2.0-85107268173.pdf | 24,05 MB | Adobe PDF | Просмотреть/Открыть |
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