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<article article-type="research-article" dtd-version="1.3" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xml:lang="ru"><front><journal-meta><journal-id journal-id-type="publisher-id">gtcrust</journal-id><journal-title-group><journal-title xml:lang="ru">Геодинамика и тектонофизика</journal-title><trans-title-group xml:lang="en"><trans-title>Geodynamics &amp; Tectonophysics</trans-title></trans-title-group></journal-title-group><issn pub-type="epub">2078-502X</issn><publisher><publisher-name>Institute of the Earth's crust of the Russian Academy of Sciences, Siberian Branch</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.5800/GT-2018-9-1-0335</article-id><article-id custom-type="elpub" pub-id-type="custom">gtcrust-518</article-id><article-categories><subj-group subj-group-type="heading"><subject>Research Article</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="ru"><subject>ПАЛЕОГЕОДИНАМИКА</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>PALEOGEODYNAMICS</subject></subj-group></article-categories><title-group><article-title>ПАЛЕОТЕКТОНИЧЕСКИЕ И ПАЛЕОГЕОГРАФИЧЕСКИЕ ОБСТАНОВКИ НАКОПЛЕНИЯ НИЖНЕРИФЕЙСКОЙ АЙСКОЙ СВИТЫ БАШКИРСКОГО ПОДНЯТИЯ (ЮЖНЫЙ УРАЛ) НА ОСНОВЕ ИЗУЧЕНИЯ ДЕТРИТОВЫХ ЦИРКОНОВ МЕТОДОМ «TERRANECHRONE®»</article-title><trans-title-group xml:lang="en"><trans-title>PALEOTECTONIC AND PALEOGEOGRAPHIC CONDITIONS FOR THE ACCUMULATION OF THE LOWER RIPHEAN AI FORMATION IN THE BASHKIR UPLIFT (SOUTHERN URALS): THE TERRANECHRONE® DETRITAL ZIRCON STUDY</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Романюк</surname><given-names>Т. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Romanyuk</surname><given-names>T. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Татьяна Валентиновна Романюк, докт. физ.-мат. наук, г.н.с. </p><p>Москва.</p></bio><bio xml:lang="en"><p>Tatiana V. Romanyuk, Doctor of Physics and Mathematics, Chief Researcher.</p><p>Moscow. </p></bio><email xlink:type="simple">t.romanyuk@mail.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Кузнецов</surname><given-names>Н. Б.</given-names></name><name name-style="western" xml:lang="en"><surname>Kuznetsov</surname><given-names>N. B.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Николай Борисович Кузнецов, докт. геол.-мин. наук, заместитель директора Геологический институт РАН.</p><p> </p></bio><bio xml:lang="en"><p>Nikolai B. Kuznetsov, Doctor of Geology and Mineralogy, Deputy Director Geological Institute of RAS.</p><p>Moscow. </p></bio><email xlink:type="simple">kouznikbor@mail.ru</email><xref ref-type="aff" rid="aff-2"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Белоусова</surname><given-names>Е. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Belousova</surname><given-names>E. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Елена Алимовна Белоусова, PhD.</p><p> </p></bio><bio xml:lang="en"><p> Elena A. Belousova, PhD.</p><p>Sydnei.</p></bio><email xlink:type="simple">elena.belousova@mq.edu.au</email><xref ref-type="aff" rid="aff-3"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Горожанин</surname><given-names>В. М.</given-names></name><name name-style="western" xml:lang="en"><surname>Gorozhanin</surname><given-names>V. M.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Валерий Михайлович Горожанин, канд. геол.-мин. наук, заведующий лабораторией.</p><p> </p></bio><bio xml:lang="en"><p>Valery M. Gorozhanin, Candidate of Geology and Mineralogy, Head of Laboratory.</p><p>Ufa.</p></bio><email xlink:type="simple">gorozhanin@ufaras.ru</email><xref ref-type="aff" rid="aff-4"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Горожанина</surname><given-names>Е. Н.</given-names></name><name name-style="western" xml:lang="en"><surname>Gorozhanina</surname><given-names>E. N.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Елена Николаевна Горожанина, канд. геол.-мин. наук, с.н.с. </p><p> </p></bio><bio xml:lang="en"><p>Elena N. Gorozhanina, Candidate of Geology and Mineralogy, Senior Researcher.</p><p> </p><p>Ufa.</p><p> </p></bio><email xlink:type="simple">ygorozhanina@yandex.ru</email><xref ref-type="aff" rid="aff-5"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт физики Земли им. О.Ю. Шмидта РАН; Российский государственный университет нефти и газа (национальный исследовательский университет) им. И.М. Губкина; Университет Маквори / центр CCFS/GEMOK.</institution><country>Россия</country></aff><aff xml:lang="en"><institution>O.Yu. Schmidt Institute of Physics of the Earth of RAS;  I.M. Gubkin Russian State University of Oil and Gas (National Research University);  Australian Research Council Centre of Excellence for Core to Crust Fluid Systems/GEMOC, Department of Earth and Planetary Sciences.</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru"><institution>Геологический институт РАН;  Институт физики Земли им. О.Ю. Шмидта РАН; Российский государственный университет нефти и газа (национальный исследовательский университет) им. И.М. Губкина; Университет Маквори / центр CCFS/GEMOK.</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Geological Institute of RAS; O.Yu. Schmidt Institute of Physics of the Earth of RAS;  I.M. Gubkin Russian State University of Oil and Gas (National Research University);  Australian Research Council Centre of Excellence for Core to Crust Fluid Systems/GEMOC, Department of Earth and Planetary Sciences.</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-3"><aff xml:lang="ru"><institution>Университет Маквори / центр CCFS/GEMOK.</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Australian Research Council Centre of Excellence for Core to Crust Fluid Systems/GEMOC, Department of Earth and Planetary Sciences, Macquarie University.</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-4"><aff xml:lang="ru"><institution>Институт геологии Уфимского научного центра РАН;  Башкирский государственный университет.</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Institute of Geology of the Ufa Federal Research Centre of RAS;  Bashkir State University.</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-5"><aff xml:lang="ru"><institution>Институт геологии Уфимского научного центра РАН.</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Institute of Geology of the Ufa Federal Research Centre of RAS</institution><country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2018</year></pub-date><pub-date pub-type="epub"><day>21</day><month>03</month><year>2018</year></pub-date><volume>9</volume><issue>1</issue><fpage>1</fpage><lpage>37</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Романюк Т.В., Кузнецов Н.Б., Белоусова Е.А., Горожанин В.М., Горожанина Е.Н., 2018</copyright-statement><copyright-year>2018</copyright-year><copyright-holder xml:lang="ru">Романюк Т.В., Кузнецов Н.Б., Белоусова Е.А., Горожанин В.М., Горожанина Е.Н.</copyright-holder><copyright-holder xml:lang="en">Romanyuk T.V., Kuznetsov N.B., Belousova E.A., Gorozhanin V.M., Gorozhanina E.N.</copyright-holder><license xml:lang="ru" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>Данная работа распространяется под лицензией Creative Commons Attribution 4.0.</license-p></license><license xml:lang="en" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>This work is licensed under a Creative Commons Attribution 4.0 License.</license-p></license></permissions><self-uri xlink:href="https://www.gt-crust.ru/jour/article/view/518">https://www.gt-crust.ru/jour/article/view/518</self-uri><abstract><p> В статье представлены результаты комплексного изучения по методике «TerraneChrone®» (LA-ICP-MS) детритных цирконов, выделенных из песчаников, слагающих базальные горизонты (навышская и чудинская подсвиты айской свиты бурзянской серии Башкирского поднятия) стратотипического разреза рифея на Южном Урале. Зафиксированные в цирконах содержания элементов-примесей свидетельствуют о малой роли комплексов океанического или окраинно-морского генезиса среди первичных источников цирконов и лучше согласуются с внутриконтинентальным, а не окраинно-континентальным расположением рифейского бассейна, базальные уровни которого выполнены айской свитой. U/Pb возрастные характеристики изученных цирконов в обеих пробах в общем схожи: преобладают палеопротерозойские цирконы (доминирующие пики фактически совпали – 2063 и 2055 млн лет), а архей представлен только немногочисленными зернами. При схожести U/Pb возрастных параметров детритных цирконов по Hf-изотопным признакам этих цирконов и содержаниям в них элементов-примесей зафиксированы существенные различия между пробами, свидетельствующие о том, что источниками цирконов для изученных песчаников были различные по геодинамической природе комплексы. Особенности характеристик цирконов в изученных пробах могут быть объяснены в рамках модели формирования айской свиты в рифтовой структуре – Навышском грабене – предшественнике Камско-Бельского авлакогена во внутренней волго-уральской части палеопротерозойского суперконтинента Колумбия. На начальной стадии рифтогенеза в Навышском грабене накапливались грубообломочные породы (навышская подсвита), представляющие собой продукты размыва слагающих борта этого грабена гранитоидных комплексов пониженной валовой кремнекислотности. В размыв попал также комплекс, содержащий специфические «карбонатитовые» цирконы с возрастом около 2.0, 2.5, 2.85 и 3.6 млрд лет и с участием палеоархейского корового материала в субстрате материнских по отношению к ним пород. В завершающую стадию рифтогенеза, уже на начальных стадиях развития Камско-Бельского авлакогена (чудинская подсвита), в грабен стали попадать эрозионные продукты с палеоводосборов, занимающих более обширные площади, первичными источниками кластики для которых были гранитоиды как пониженной, так и нормальной кремнекислотности. В размыв попал также комплекс, содержащий специфические ювенильные «карбонатитовые» цирконы с возрастом около 2.05 млрд лет. Однако к этому времени значительные площади архейского фундамента Волго-Уралии, вероятно, были покрыты проточехлом и не дренировались, поэтому архейский детрит в навышской подсвите представлен скуднее по сравнению с чудинской подсвитой и по количеству, и по возрастным группам. До сих пор докембрийские карбонатитовые породы ни в тараташском комплексе, слагающем фундамент Навышского грабена, ни в юго-восточной части Восточно-Европейской платформы не описаны, и вопрос об источнике этих «карбонатитовых» цирконов остается открытым, но имеет перспективу быть решенным по мере накопления данных о фундаменте.</p></abstract><trans-abstract xml:lang="en"><p>The TerraneChrone® (LA-ICP-MS) technique has been applied to carry out an integrated study of detrital zircons in sandstones sampled from the basal horizons of the stratotypical Riphean sequence in the Southern Urals, specifically the Navysh and Chudin suites of the Ai Formation of the Burzyan Group in the Bashkir Uplift. The concentrations of trace elements in the detrital zircons suggest that the role of oceanic or marginal-marine complexes among the primary sources of zircons was insignificant, and show a better agreement with the intra-continental rather than passive-margin origin of the Riphean basin, whose basal levels are composed by the Ai Formation. The U/Pb ages of zircons from samples K13-206 and M08-16-1 are generally similar: the Paleoproterozoic zircons predominate (the dominant peaks are actually coincident, 2063 and 2055 Ma), and only a few grains of the Archean age are present. Despite the similar U/Pb ages of the detrital zircons, these two samples considerably differ in their Hf isotopic features and the concentrations of trace elements, which means that the zircons in the studied sandstones are of different geodynamic origin. The characteristics of these zircons can be explained by a model showing the Ai Formation in the Navysh graben that is a rift structure and a predecessor of the Kama-Belaya aulacogene in the inner Volga-Ural region of the Paleoproterozoic supercontinent Columbia. At the initial stage of rifting, the granitoid complexes with a lower total silicic acidity, which composed the graben walls, had been eroded; as a result of erosion, coarse clastic rocks accumulated within the Navysh graben and formed the Navysh suite. A specific “carbonatitic” complex containing zircons (about 2.0, 2.5, 2.85 and 3.6 Ga) and the Palaeoarchean crustal material in the substrate of their parent rocks was also eroded. In the final stage of rifting, already at the initial stages of the development of the Kama-Belaya aulacogen (Chudin suite), the erosion products from the paleo-aquifers occupying vast areas began to be transported into the rift. The primary sources of clastics for the Chudin suite were both granitoids of the lower and normal silicic acidity. Besides, a specific “carbonatitic” complex containing juvenile zircons (about 2.05 Ga) was eroded. However, by that time, significant areas of the Archaean basement of the Volga-Ural region might have become hidden underneath a proto-cover and thus not eroded, so the Archean detritus in the Chudin suite is poorly represented in comparison with the Navysh suite, considering both the amounts and ages of detrital zircons. As of today, the Precambrian carbonatite rocks within both the Taratash complex (composing the basement of the Navysh graben) and the southeastern segment of the East-European Platform have not yet been described. The source of the “carbonatite” zircons remains unknown and can be discovered as more and more data on the basement rocks is accumulated.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>Башкирское поднятие</kwd><kwd>нижний рифей</kwd><kwd>детритовые цирконы</kwd><kwd>методика «TerraneChrone®»</kwd><kwd>Навышский грабен</kwd><kwd>Камско-Бельский авлакоген</kwd><kwd>карбонатиты</kwd><kwd>суперконтинент Колумбия</kwd></kwd-group><kwd-group xml:lang="en"><kwd>Bashkir uplift</kwd><kwd>Lower Riphean</kwd><kwd>detrital zircons</kwd><kwd>TerraneChrone® technique</kwd><kwd>Navysh graben</kwd><kwd>Kama-Belaya aulacogen</kwd><kwd>carbonatites</kwd><kwd>supercontinent Columbia</kwd></kwd-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Andersen T., 2005. Detrital zircons as tracers of sedimentary provenance: limiting conditions from statistics and numerical simulation. 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