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    A study of ordinary chondrites by Mossbauer spectroscopy with high-velocity resolution

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    Author
    Oshtrakh, M. I.
    Petrova, E. V.
    Grokhovsky, I.
    Semionkin, V. A.
    Issue Date
    2008-01-01
    Keywords
    L chondrites
    Mössbauer spectroscopy
    H chondrites
    
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    Citation
    Oshtrakh, M. I., Petrova, E. V., Grokhovsky, V. I., & Semionkin, V. A. (2008). A study of ordinary chondrites by Mössbauer spectroscopy with high‐velocity resolution. Meteoritics & Planetary Science, 43(5), 941-958.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656433
    DOI
    10.1111/j.1945-5100.2008.tb01091.x
    Additional Links
    https://meteoritical.org/
    Abstract
    An improvement in the velocity resolution and quality of Mössbauer spectra has been applied to a group of ordinary chondrites. This improvement permitted us to carry out a more detailed study of the iron bearing phases in these samples than has previously been possible. Mössbauer spectra of 11 ordinary chondrites of L and H chemical groups were measured using 4096 channels and presented for further analysis in 1024 channels. Subspectra of the metal grains of several chondrites demonstrated the presence of at least two magnetic sextets related to the main Fe(Ni, Co) phases. Moreover, Mössbauer study of extracted metal grains from Tsarev L5 revealed three sextets and one singlet spectral components related to various alpha-Fe(Ni, Co), alpha'-Fe(Ni, Co), alpha2-Fe(Ni, Co), and gamma-Fe(Ni, Co) phases. Each subspectrum of olivine and pyroxene in Mössbauer spectra of ordinary chondrites was fitted by superposition of two quadrupole doublets related to M1 and M2 sites in minerals for the first time. An analysis of relative areas and Mössbauer hyperfine parameters was performed and some differences for L and H chondrites as well as for M1 and M2 sites were observed. Mössbauer parameters of troilite and oxidized iron were analyzed. In contrast to a previous study with 512-channel spectra, the presence of oxidized iron was found in all chondrites.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2008.tb01091.x
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    Meteoritics & Planetary Science, Volume 43, Number 5 (2008)

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