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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-2020-11-4-0500</article-id><article-id custom-type="elpub" pub-id-type="custom">gtcrust-1118</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>КИМБЕРЛИТОПОДОБНЫЕ ПОРОДЫ УРИКСКО-ИЙСКОГО ГРАБЕНА, ВОСТОЧНОЕ ПРИСАЯНЬЕ: МИНЕРАЛЬНЫЙ СОСТАВ, ГЕОХИМИЯ И УСЛОВИЯ ФОРМИРОВАНИЯ</article-title><trans-title-group xml:lang="en"><trans-title>KIMBERLITE-LIKE ROCKS OF THE URIK-IYA GRABEN, EASTERN SAYAN REGION: MINERAL COMPOSITION, GEOCHEMISTRY AND FORMATION CONDITIONS</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-9238-4763</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Савельева</surname><given-names>В. Б.</given-names></name><name name-style="western" xml:lang="en"><surname>Savel'eva</surname><given-names>V. B.</given-names></name></name-alternatives><bio xml:lang="ru"><p>664033, Иркутск, ул. Лермонтова, 128</p></bio><bio xml:lang="en"><p>128 Lermontov St, Irkutsk 664033</p></bio><email xlink:type="simple">vsavel@crust.irk.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-6454-3552</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Данилова</surname><given-names>Ю. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Danilova</surname><given-names>Yu. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>664033, Иркутск, ул. Лермонтова, 128</p></bio><bio xml:lang="en"><p>128 Lermontov St, Irkutsk 664033</p></bio><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-6644-2659</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Базарова</surname><given-names>Е. П.</given-names></name><name name-style="western" xml:lang="en"><surname>Bazarova</surname><given-names>E. P.</given-names></name></name-alternatives><bio xml:lang="ru"><p>664033, Иркутск, ул. Лермонтова, 128</p></bio><bio xml:lang="en"><p>128 Lermontov St, Irkutsk 664033</p></bio><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-3262-6636</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Данилов</surname><given-names>Б. С.</given-names></name><name name-style="western" xml:lang="en"><surname>Danilov</surname><given-names>B. S.</given-names></name></name-alternatives><bio xml:lang="ru"><p>664033, Иркутск, ул. Лермонтова, 128</p></bio><bio xml:lang="en"><p>128 Lermontov St, Irkutsk 664033</p></bio><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт земной коры СО РАН</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Institute of the Earth’s Crust, Siberian Branch of the Russian Academy of Science</institution><country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2020</year></pub-date><pub-date pub-type="epub"><day>15</day><month>12</month><year>2020</year></pub-date><volume>11</volume><issue>4</issue><fpage>678</fpage><lpage>696</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Савельева В.Б., Данилова Ю.В., Базарова Е.П., Данилов Б.С., 2020</copyright-statement><copyright-year>2020</copyright-year><copyright-holder xml:lang="ru">Савельева В.Б., Данилова Ю.В., Базарова Е.П., Данилов Б.С.</copyright-holder><copyright-holder xml:lang="en">Savel'eva V.B., Danilova Y.V., Bazarova E.P., Danilov B.S.</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/1118">https://www.gt-crust.ru/jour/article/view/1118</self-uri><abstract><p>Изучен химический состав минералов, распределение петрогенных и редких элементов в беспироксеновых щелочных пикритах, образующих жилы и дайки в позднерифейском (около 645 млн лет) Большетагнинском щелочно-карбонатитовом массиве и за его пределами, выполнено их сопоставление с Бушканайской дайкой кимберлит-пикритового состава. Вкрапленники в беспироксеновых пикритах представлены оливином (замещен серпентином) и флогопитом, основная масса образована серпентином, флогопитом, монтичеллитом, кальцитом и др.; ксенокристы пиропа, хромдиопсида отсутствуют. Флогопит и Cr-шпинель из пикритов по химическому составу сходны с этими минералами в кимберлитах, но эволюция состава шпинелидов отвечает титаномагнетитовому тренду; монтичеллит обеднен форстеритовым (Mg2SiO4 ) компонентом. Породы содержат стронцианит, бурбанкит, титанистый андрадит, кальциртит, Mn-ильменит, не характерные для кимберлитов, но присущие карбонатсодержащим ультрамафическим лампрофирам ‒ айлликитам. Беспироксеновые пикриты имеют низкое содержание (мас. %) SiO2  (28.4‒33.2), Al2O3  (3.2‒5.6), Na2O (0.01‒0.05), умеренно высокое TiO2  (2.0‒3.3), К2О (0.45‒1.33), варьирующееся MgO (16.1‒24.1), СаО (12.9‒22.8), СО2 (1.1‒12.2), а также Ni (260‒850 ppm), Cr (840‒2200 ppm); Mg#=0.73‒0.80. Содержание Th, U, Nb, Ta, La, Ce в жилах повышено примерно на два порядка по сравнению с примитивной мантией; спектры микроэлементов отличаются от спектров южно-африканских и якутских кимберлитов. Отношения Nb/U, Nb/Th, Th/Ce, La/Nb, Zr/Nb в беспироксеновых пикритах и в породах Бушканайской дайки близки к таковым в OIB, что отражает ведущий вклад рециклированного компонента в источник расплавов. На основе результатов экспериментов по плавлению карбонатизированного гранатового лерцолита показано, что выплавление беспироксеновых щелочных пикритов происходило при 5–6 GРa.</p></abstract><trans-abstract xml:lang="en"><p>The study of the Bol’shaya Tagna alkaline-carbonatite massif and adjacent areas was focused on the mineral and chemical compositions of minerals, the distribution of petrogenic and trace elements in pyroxene-free alkaline picrites in veins and dikes dated at the late Riphean (circa 645 Ma), and comparison with the Bushkanai kimberlite-picrite dike. Phenocrysts in the pyroxene-free picrites are represented by olivine (replaced with serpentine) and phlogopite; the bulk is formed by serpentine, phlogopite, monticellite, calcite, etc .; xenocrysts of pyrope and chrome diopside are absent. Phlogopite and Cr-spinel from the picrites are chemically similar to these minerals in kimberlites, but the evolution of the spinel compositions corresponds to the titanomagnetite trend; monticellite is depleted in forsterite (Mg2SiO4). The rocks contain strontianite, burbankite, titanium andradite, calcirtite and Mn-ilmenite, which are not typical of kimberlites, but are inherent in carbonate-bearing ultramafic lamprophyres, ayllikites. The pyroxene-free picrites have low contents (wt %) of SiO2  (28.4‒33.2), Al2O3  (3.2‒5.6), and Na2O (0.01‒0.05); relatively high contents of TiO2  (2.0‒3.3), and К2О (0.45‒1.33); varying contents of MgO (16.1‒24.1), СаО (12.9‒22.8), СО2  (1.1‒12.2), Ni (260‒850 ppm), and Cr (840‒2200 ppm); and Mg#=0.73‒0.80. The contents of Th, U, Nb, Ta, La, and Ce in the veins are approximately two orders higher than those in the primitive mantle; the spectra of trace elements differ from the spectra of the South African and Yakuian kimberlites. In the pyroxene-free picrites and the rocks of the Bushkanai dike, the Nb/U, Nb/Th, Th/Ce, La/Nb, and Zr/Nb ratios are similar to those in ocean island basalts (OIB) and thus give evidence of the leading contribution of the recycled component into the source melt. In experiments conducted to investigate melting of carbonated garnet lherzolite, the pyroxene-free alkaline picrites melted at 5–6 GPa.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>кимберлит</kwd><kwd>беспироксеновый щелочной пикрит</kwd><kwd>флогопит</kwd><kwd>шпинель</kwd><kwd>монтичеллит</kwd><kwd>Урикско-Ийский грабен</kwd><kwd>зиминский комплекс</kwd><kwd>Большетагнинский массив</kwd><kwd>Присаянье</kwd></kwd-group><kwd-group xml:lang="en"><kwd>kimberlite</kwd><kwd>pyroxene-free alkaline picrite</kwd><kwd>phlogopite</kwd><kwd>spinel</kwd><kwd>monticellite</kwd><kwd>Urik-Iya graben</kwd><kwd>Zima complex</kwd><kwd>Bol’shaya Tagna massif</kwd><kwd>Sayan region</kwd></kwd-group><funding-group><funding-statement xml:lang="ru">Работа выполнена при финансовой поддержке РНФ (РНФ-18-17-00101) и ИНЦ СО РАН (Интеграционный проект, блок 1.4).</funding-statement><funding-statement xml:lang="en">The study was financially supported by the Russian Science Foundation (RSF-18-17-00101) and the Irkutsk Scientific Center SB RAS (Block 1.4 of the Integration Project).</funding-statement></funding-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Ashchepkov I., Zhmodik S., Belyanin D., Kiseleva O., Medvedev N., Travin A., Yudin D., Karmanov N., Downes H., 2020. 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