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dc.contributor.authorMaksimova, A. A.en
dc.contributor.authorGoryunov, M. V.en
dc.contributor.authorOshtrakh, M. I.en
dc.date.accessioned2021-08-31T15:05:48Z-
dc.date.available2021-08-31T15:05:48Z-
dc.date.issued2021-
dc.identifier.citationMaksimova 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.en
dc.identifier.issn2075163X-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Gold3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85107307383&doi=10.3390%2fmin11060612&partnerID=40&md5=724edd961fe4c110f5887b7b1bbc93b9
dc.identifier.otherhttps://www.mdpi.com/2075-163X/11/6/612/pdfm
dc.identifier.urihttp://elar.urfu.ru/handle/10995/102867-
dc.description.abstractMössbauer (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.en
dc.description.sponsorshipThis 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.).en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherMDPI AGen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceMinerals2
dc.sourceMineralsen
dc.subject57 FE HYPERFINE INTERACTIONSen
dc.subject57 FE MÖSSBAUER SPECTROSCOPYen
dc.subjectDIFFERENTIATED METEORITESen
dc.subjectFE2+ PARTITIONING IN SILICATE PHASESen
dc.subjectFUSION CRUSTen
dc.subjectIRON-BEARING MINERALSen
dc.subjectIRON-BEARING PHASE COMPOSITIONen
dc.subjectMARSen
dc.subjectMETEORITE WEATHERINGen
dc.subjectMOONen
dc.subjectTEMPERATURE OF CATION EQUILIBRIUM DISTRIBUTION IN SILICATE PHASESen
dc.titleApplications of mössbauer spectroscopy in meteoritical and planetary science, part ii: Differentiated meteorites, moon, and marsen
dc.typeReviewen
dc.typeinfo:eu-repo/semantics/reviewen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.rsi46827703-
dc.identifier.doi10.3390/min11060612-
dc.identifier.scopus85107307383-
local.contributor.employeeMaksimova, A.A., Department of Experimental Physics, Institute of Physics and Technology, Ural Federal University, Ekaterinburg, 620002, Russian Federation, The Zavaritsky Institute of Geology and Geochemistry of the Ural Branch of the Russian Academy of Sciences, Ekaterinburg, 620016, Russian Federation
local.contributor.employeeGoryunov, M.V., Department of Experimental Physics, Institute of Physics and Technology, Ural Federal University, Ekaterinburg, 620002, Russian Federation
local.contributor.employeeOshtrakh, M.I., Department of Experimental Physics, Institute of Physics and Technology, Ural Federal University, Ekaterinburg, 620002, Russian Federation
local.issue6-
local.volume11-
dc.identifier.wos000666243000001-
local.contributor.departmentDepartment of Experimental Physics, Institute of Physics and Technology, Ural Federal University, Ekaterinburg, 620002, Russian Federation
local.contributor.departmentThe Zavaritsky Institute of Geology and Geochemistry of the Ural Branch of the Russian Academy of Sciences, Ekaterinburg, 620016, Russian Federation
local.identifier.pure22106855-
local.identifier.purec0834b97-6b70-4969-a9f0-c963bba08089uuid
local.description.order612-
local.identifier.eid2-s2.0-85107307383-
local.identifier.wosWOS:000666243000001-
local.fund.feuzFEUZ-2020-0060-
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