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Terrestrial Plagioclase Olivine Clinopyroxenite as a Possible Analogue of Lunar Rocks

Received: 10 December 2018    Accepted: 19 March 2019    Published: 29 April 2019
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Abstract

The article describes the mineral composition and petrochemistry of a unique ancient (more than 1848–2011 MA) igneous rock of the Urals – plagioclase olivine clinopyroxenite. These rocks are considered the oldest in the Urals. In the literature they are described under the name izrandites. They are part of the foundation of the basement of the East European platform. These rocks are highly aluminous and calcic. They are characterized by a low amount of alkalis and magnesium oxide and a comparable amount of silicon and iron. A certain petrochemical similarity is found between the izrandites and the anorthite leucogabbro, troctolite, and noritic anorthosites of lunar highlands. This similarity enhances the closeness of distribution of the minor elements, the leading role among which belongs to Sr and Ba. In those and others rocks plagioclase is represented by anorthite or labrador, its amount makes up from 5–8 to 50–70%. The izrandites are representatives of the rocks of the lower part of the Earth's crust, which in composition and absolute age can be compared with the youngest leucogabbros and troctolites of the Moon.

Published in Earth Sciences (Volume 8, Issue 2)
DOI 10.11648/j.earth.20190802.13
Page(s) 94-101
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Olivine Clinopyroxenite, Izrandite, Anorthosite, Leucogabbro, Urals, Earth, Moon

References
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    Victor Grigorievich Korinevsky, Eugeny Victorovich Korinevsky. (2019). Terrestrial Plagioclase Olivine Clinopyroxenite as a Possible Analogue of Lunar Rocks. Earth Sciences, 8(2), 94-101. https://doi.org/10.11648/j.earth.20190802.13

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    ACS Style

    Victor Grigorievich Korinevsky; Eugeny Victorovich Korinevsky. Terrestrial Plagioclase Olivine Clinopyroxenite as a Possible Analogue of Lunar Rocks. Earth Sci. 2019, 8(2), 94-101. doi: 10.11648/j.earth.20190802.13

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    AMA Style

    Victor Grigorievich Korinevsky, Eugeny Victorovich Korinevsky. Terrestrial Plagioclase Olivine Clinopyroxenite as a Possible Analogue of Lunar Rocks. Earth Sci. 2019;8(2):94-101. doi: 10.11648/j.earth.20190802.13

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  • @article{10.11648/j.earth.20190802.13,
      author = {Victor Grigorievich Korinevsky and Eugeny Victorovich Korinevsky},
      title = {Terrestrial Plagioclase Olivine Clinopyroxenite as a Possible Analogue of Lunar Rocks},
      journal = {Earth Sciences},
      volume = {8},
      number = {2},
      pages = {94-101},
      doi = {10.11648/j.earth.20190802.13},
      url = {https://doi.org/10.11648/j.earth.20190802.13},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.earth.20190802.13},
      abstract = {The article describes the mineral composition and petrochemistry of a unique ancient (more than 1848–2011 MA) igneous rock of the Urals – plagioclase olivine clinopyroxenite. These rocks are considered the oldest in the Urals. In the literature they are described under the name izrandites. They are part of the foundation of the basement of the East European platform. These rocks are highly aluminous and calcic. They are characterized by a low amount of alkalis and magnesium oxide and a comparable amount of silicon and iron. A certain petrochemical similarity is found between the izrandites and the anorthite leucogabbro, troctolite, and noritic anorthosites of lunar highlands. This similarity enhances the closeness of distribution of the minor elements, the leading role among which belongs to Sr and Ba. In those and others rocks plagioclase is represented by anorthite or labrador, its amount makes up from 5–8 to 50–70%. The izrandites are representatives of the rocks of the lower part of the Earth's crust, which in composition and absolute age can be compared with the youngest leucogabbros and troctolites of the Moon.},
     year = {2019}
    }
    

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    T1  - Terrestrial Plagioclase Olivine Clinopyroxenite as a Possible Analogue of Lunar Rocks
    AU  - Victor Grigorievich Korinevsky
    AU  - Eugeny Victorovich Korinevsky
    Y1  - 2019/04/29
    PY  - 2019
    N1  - https://doi.org/10.11648/j.earth.20190802.13
    DO  - 10.11648/j.earth.20190802.13
    T2  - Earth Sciences
    JF  - Earth Sciences
    JO  - Earth Sciences
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    EP  - 101
    PB  - Science Publishing Group
    SN  - 2328-5982
    UR  - https://doi.org/10.11648/j.earth.20190802.13
    AB  - The article describes the mineral composition and petrochemistry of a unique ancient (more than 1848–2011 MA) igneous rock of the Urals – plagioclase olivine clinopyroxenite. These rocks are considered the oldest in the Urals. In the literature they are described under the name izrandites. They are part of the foundation of the basement of the East European platform. These rocks are highly aluminous and calcic. They are characterized by a low amount of alkalis and magnesium oxide and a comparable amount of silicon and iron. A certain petrochemical similarity is found between the izrandites and the anorthite leucogabbro, troctolite, and noritic anorthosites of lunar highlands. This similarity enhances the closeness of distribution of the minor elements, the leading role among which belongs to Sr and Ba. In those and others rocks plagioclase is represented by anorthite or labrador, its amount makes up from 5–8 to 50–70%. The izrandites are representatives of the rocks of the lower part of the Earth's crust, which in composition and absolute age can be compared with the youngest leucogabbros and troctolites of the Moon.
    VL  - 8
    IS  - 2
    ER  - 

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Author Information
  • Institute of Mineralogy of the Uralian Branch of the Russian Academy of Sciences, Miass, Russia

  • Institute of Mineralogy of the Uralian Branch of the Russian Academy of Sciences, Miass, Russia

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