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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-2024-15-5-0780</article-id><article-id custom-type="edn" pub-id-type="custom">XESWVT</article-id><article-id custom-type="elpub" pub-id-type="custom">gtcrust-1916</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>ТЕРМОБАРОМЕТРИЯ ДЕПЛЕТИРОВАННЫХ ПЕРИДОТИТОВ</article-title><trans-title-group xml:lang="en"><trans-title>THERMOBAROMETRY OF DEPLETED PERIDOTITES</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-2216-0553</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Похиленко</surname><given-names>Л. Н.</given-names></name><name name-style="western" xml:lang="en"><surname>Pokhilenko</surname><given-names>L. N.</given-names></name></name-alternatives><bio xml:lang="ru"><p>630090, Новосибирск, пр-т Академика Коптюга, 3</p></bio><bio xml:lang="en"><p>3 Academician Koptyug Ave, Novosibirsk 630090 </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/0009-0007-5717-4422</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Королюк</surname><given-names>В. Н.</given-names></name><name name-style="western" xml:lang="en"><surname>Korolyuk</surname><given-names>V. N.</given-names></name></name-alternatives><bio xml:lang="ru"><p>630090, Новосибирск, пр-т Академика Коптюга, 3</p></bio><bio xml:lang="en"><p>3 Academician Koptyug Ave, Novosibirsk 630090 </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/0000-0002-3207-1458</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Похиленко</surname><given-names>Н. П.</given-names></name><name name-style="western" xml:lang="en"><surname>Pokhilenko</surname><given-names>N. P.</given-names></name></name-alternatives><bio xml:lang="ru"><p>630090, Новосибирск, пр-т Академика Коптюга, 3</p><p>630090, Новосибирск, ул. Пирогова, 1 </p></bio><bio xml:lang="en"><p>3 Academician Koptyug Ave, Novosibirsk 630090 </p><p>1 Pirogov St, Novosibirsk 630090 </p></bio><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт геологии и минералогии им. В.С. Соболева СО РАН</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Sobolev Institute of Geology and Mineralogy, Siberian Branch of the Russian Academy of Sciences</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru"><institution>Институт геологии и минералогии им. В.С. Соболева СО РАН ; Новосибирский государственный университет</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Sobolev Institute of Geology and Mineralogy, Siberian Branch of the Russian Academy of Sciences ; Novosibirsk State University</institution><country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2024</year></pub-date><pub-date pub-type="epub"><day>18</day><month>10</month><year>2024</year></pub-date><volume>15</volume><issue>5</issue><fpage>780</fpage><lpage>780</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Похиленко Л.Н., Королюк В.Н., Похиленко Н.П., 2024</copyright-statement><copyright-year>2024</copyright-year><copyright-holder xml:lang="ru">Похиленко Л.Н., Королюк В.Н., Похиленко Н.П.</copyright-holder><copyright-holder xml:lang="en">Pokhilenko L.N., Korolyuk V.N., Pokhilenko N.P.</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/1916">https://www.gt-crust.ru/jour/article/view/1916</self-uri><abstract><p>Проведена оценка возможности использования оливиновой термобарометрии для ксенолитов деплетированных перидотитов из трубки Удачной (Якутия), представленных 76 мегакристаллическими дунитами и 5 мегакристаллическими гарцбургитами. По специально разработанной и проверенной методике с помощью микрозондового анализа определены микропримеси Al и Ca в оливинах исследуемых образцов. РТ-параметры ксенолитов мегакристаллических дунитов рассчитаны по уравнениям оливиновых, гранатовых, оливин-гранатовых термобарометров. Для нескольких мегакристаллических гарцбургитов дополнительно использовались энстатитовые геобарометры. Произведенное сравнение полученных данных показало, что наиболее подходящей для оценки РТ-параметров изученной коллекции мегакристаллических дунитов оказывается геотермобарометрическая пара барометр Финнерти-Риджена (Са в оливине) для перидотитов широкого диапазона РТ и термометр [Bussweiler et al., 2017] (Al в оливине) для гранатовых перидотитов, хотя небольшая часть данных из области высоких РТ (&gt;60 кбар и 1200 °С) вызывает сомнение. Гранатовый барометр [Grütter et al., 2006] (соотношение СаО – Cr2O3 в пиропе) не всегда согласуется с оливиновыми геотермометрами. Это может быть связано с необходимостью корректировки уравнений барометра для более широкого спектра составов, а также с возможным нарушением равновесия между гранатом и оливином. Авторы допускают, что более точные результаты могут быть получены при использовании этого барометра в сочетании с гранатовыми термометрами, основанными на определении Ni в гранате. Для серьезных выводов данных по гарцбургитам недостаточно. Однако следует признать, что традиционная пара энстатитового барометра Макгрегора и гранат-оливинового термометра O’Нейл-Вуда пока остается наиболее приемлемой для оценки РТ-параметров мегакристаллических гарцбургитов, хотя и с некоторым занижением температур.</p></abstract><trans-abstract xml:lang="en"><p>An assessment was made of the possibility of using olivine thermobarometry for xenoliths of depleted peridotites from the Udachnaya pipe (Yakutia), represented by 76 megacrystalline dunites and 5 megacrystalline harzburgites. Specially developed and tested method of microprobe analysis was used to determine Al and Ca microimpurities in the olivine samples studied. PT-parameters of megacrystalline dunite xenoliths were calculated using the equations of olivine, garnet, and olivine-garnet thermobarometers. Enstatite geobarometers were additionally used for some megacrystalline harzburgites. Comparison of the obtained data showed that the geothermobarometric pair of FinnertyRigden barometer (Ca in olivine) for wide PT-range peridotites and thermometer [Bussweiler et al., 2017] (Al in olivine) for garnet peridotites is most suitable for assessing the PT-parameters of the megacrystalline dunite collection studied, though some of the high PT-parameters (&gt;60 kbar and 1200 °C) are questionable. Garnet barometer [Grütter et al., 2006] (CaO – Cr2O3 ratio in pyrope) does not always agree with olivine geothermometers. This may be caused by the necessity to adjust the barometer equations for a wider range of compositions, as well as by the possible imbalance between garnet and olivine. We admit that more accurate results can be obtained by using this barometer in combination with garnet thermometers based on the determination of Ni in garnet. There is not enough data on harzburgites to draw certain conclusions. However, it should be recognized that the traditional pair of McGregor enstatite barometer and O’Neill-Wood garnet-olivine thermometer still remains the most acceptable for estimating the PT-parameters of megacrystalline harzburgites, though with some temperature underestimation.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>геобарометр</kwd><kwd>геотермометр</kwd><kwd>оливин</kwd><kwd>мегакристаллические дуниты</kwd><kwd>мегакристаллические гарцбургиты</kwd><kwd>микропримеси</kwd><kwd>трубка Удачная</kwd></kwd-group><kwd-group xml:lang="en"><kwd>geobarometer</kwd><kwd>geothermometer</kwd><kwd>olivine</kwd><kwd>megacrystalline dunites</kwd><kwd>megacrystalline harzburgites</kwd><kwd>microimpurities</kwd><kwd>Udachnaya pipe</kwd></kwd-group><funding-group><funding-statement xml:lang="ru">Работа выполнена по государственному заданию ИГМ СО РАН (№ 122041400157-9).</funding-statement><funding-statement xml:lang="en">The work was carried as part of the state assignment of the IGM SB RAS (122041400157-9).</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">Bussweiler Y., Brey G.P., Pearson D.G., Stachel T., Stern R.A., Hardman M.F., Kjarsgaard B.A., Jackson S.E., 2017. 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