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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">litosphere</journal-id><journal-title-group><journal-title xml:lang="ru">Литосфера</journal-title><trans-title-group xml:lang="en"><trans-title>LITHOSPHERE (Russia)</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">1681-9004</issn><issn pub-type="epub">2500-302X</issn><publisher><publisher-name>A.N. Zavaritsky Institute of Geology and Geochemistry</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.24930/1681-9004-2021-21-3-409-430</article-id><article-id custom-type="elpub" pub-id-type="custom">litosphere-1449</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>Статьи</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>Articles</subject></subj-group></article-categories><title-group><article-title>Уточнение классификации и характеристика включений в метеорите Северный Колчим (H3.4)</article-title><trans-title-group xml:lang="en"><trans-title>Сlassification and characteristic of inclusions in the Severny Kolchim meteorite (H3.4)</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>Берзин</surname><given-names>С. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Berzin</surname><given-names>S. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>620016, г. Екатеринбург, ул. Акад. Вонсовского, 15</p></bio><bio xml:lang="en"><p>15 Acad. Vonsovsky st., Ekaterinburg, 620016 Russia</p></bio><email xlink:type="simple">sbersin@yandex.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>Дугушкина</surname><given-names>К. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Dugushkina</surname><given-names>K. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>620016, г. Екатеринбург, ул. Акад. Вонсовского, 15</p></bio><bio xml:lang="en"><p>15 Acad. Vonsovsky st., Ekaterinburg, 620016 Russia</p></bio><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Червяковская</surname><given-names>М. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Chervyakovskaya</surname><given-names>M. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>620016, г. Екатеринбург, ул. Акад. Вонсовского, 15</p></bio><bio xml:lang="en"><p>15 Acad. Vonsovsky st., Ekaterinburg, 620016 Russia</p></bio><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Червяковский</surname><given-names>В. С.</given-names></name><name name-style="western" xml:lang="en"><surname>Chervyakovskiy</surname><given-names>V. S.</given-names></name></name-alternatives><bio xml:lang="ru"><p>620016, г. Екатеринбург, ул. Акад. Вонсовского, 15</p></bio><bio xml:lang="en"><p>15 Acad. Vonsovsky st., Ekaterinburg, 620016 Russia</p></bio><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Панкрушина</surname><given-names>Е. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Pankrushina</surname><given-names>E. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>620016, г. Екатеринбург, ул. Акад. Вонсовского, 15</p></bio><bio xml:lang="en"><p>15 Acad. Vonsovsky st., Ekaterinburg, 620016 Russia</p></bio><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Бурлаков</surname><given-names>Е. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Burlakov</surname><given-names>E. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>620016, г. Екатеринбург, ул. Акад. Вонсовского, 15</p></bio><bio xml:lang="en"><p>15 Acad. Vonsovsky st., Ekaterinburg, 620016 Russia</p></bio><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт геологии и геохимии УрО РАН</institution><country>Россия</country></aff><aff xml:lang="en"><institution>A.N. Zavaritsky Institute of Geology and Geochemistry, Uralian Branch of RAS</institution><country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2021</year></pub-date><pub-date pub-type="epub"><day>08</day><month>07</month><year>2021</year></pub-date><volume>21</volume><issue>3</issue><fpage>409</fpage><lpage>430</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Берзин С.В., Дугушкина К.А., Червяковская М.В., Червяковский В.С., Панкрушина Е.А., Бурлаков Е.В., 2021</copyright-statement><copyright-year>2021</copyright-year><copyright-holder xml:lang="ru">Берзин С.В., Дугушкина К.А., Червяковская М.В., Червяковский В.С., Панкрушина Е.А., Бурлаков Е.В.</copyright-holder><copyright-holder xml:lang="en">Berzin S.V., Dugushkina K.A., Chervyakovskaya M.V., Chervyakovskiy V.S., Pankrushina E.A., Burlakov E.V.</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.lithosphere.ru/jour/article/view/1449">https://www.lithosphere.ru/jour/article/view/1449</self-uri><abstract><sec><title>Объект исследования</title><p>Объект исследования. Фрагменты метеорита Северный Колчим.</p></sec><sec><title>Материалы и методы</title><p>Материалы и методы. Изучение метеорита Северный Колчим выполнено в ЦКП “Геоаналитик” ИГГ УрО РАН. Изучение класта и включений производилось на сканирующем электронном микроскопе JSM-6390LV фирмы JEOL с энергодисперсионной приставкой INCA Energy 450 X-Max 80 фирмы Oxford Instruments. Валовый состав анализировался при съемке ЭДС спектров с площади хондры на срезе. Состав минералов изучался на электронно-зондовом микроанализаторе Cameca SX-100. Измерение содержаний редких элементов в оливине осуществлялось на масс-спектрометре с индуктивно-связанной плазмой NexION 300S (PerkinElmer) с приставкой для лазерной абляции NWR 213 (ESI) при диаметре кратера 25 мкм.</p></sec><sec><title>Результаты</title><p>Результаты. По совокупности петрографических и минералогических признаков классификация метеорита Северный Колчим была уточнена как H3.4. Кроме того, данный метеорит может быть также дополнительно классифицирован как геномиктовая брекчия (Genomict breccia). В метеорите Северный Колчим был изучен класт размером 6 × 6 мм, сложенный хондритом H3.9. Он имеет несколько более высокую степень ударных преобразований S2, чем вмещающий хондрит. В метеорите были найдены и изучены тугоплавкие богатые форстеритом включения (англ. refractory forsterite rich objects). Включения сложены низкожелезистым форстеритом (f = 0.004–0.2, где f – отношение Fe/(Fe + Mg)мол).</p></sec><sec><title>Заключение</title><p>Заключение. Предполагается, что порфировые оливиновые хондры, состоящие из тугоплавкого форстерита и высококальциевого стекла в мезостазисе, скорее всего, являются родительскими для тугоплавких богатых форстеритом включений. Найденные в матрице хондрита обогащенные Al хондры и пироксеновые хондры с тридимитом, вероятнее всего, являются ксеногенными и происходят из области формирования энстатитовых хондритов.</p></sec></abstract><trans-abstract xml:lang="en"><sec><title>Research subject</title><p>Research subject. Fragments of the Severny Kolchim meteorite.</p></sec><sec><title>Materials and methods</title><p>Materials and methods. The study was performed in the Geoanalyst Centre for Collective Use, Institute of Geology and Geochemistry, UB RAS. The clast and inclusions were studied using a scanning electron microscope JSM-6390LV from JEOL with an energy dispersing attachment INCA Energy 450 X-Max 80. The bulk chondrule compositions were obtained by EDS analysis of whole chondrule areas in thin sections. The composition of minerals was studied using an electron microprobe analyser Cameca SX100 equipped with five wavelength spectrometers. The concentrations of trace elements in olivine were measured using a mass spectrometer with inductively coupled plasma NexION 300S (PerkinElmer) with a laser ablation attachment NWR 213 (ESI) at a crater diameter of 25 microns.</p></sec><sec><title>Results</title><p>Results. According to the revealed set of petrographic and mineralogical features, the meteorite was clarified as H3.4. In addition, this meteorite can be further classified as genomict breccia. In the Severny Kolchim meteorite, a 6×6 mm clast fragment composed of chondrite H3.9 was studied. This inclusion has a slightly higher degree of S2 shock transformations compared to the host rock. Refractory forsterite-rich objects were found and studied. These inclusions are composed of low-ferroan forsterite (f = 0.004–0.2, f – ratio Fe/(Fe + Mg)mol).</p></sec><sec><title>Conclusion</title><p>Conclusion. The porphyry olivine chondrules consisting of refractory forsterite and high-calcium glass in mesostasis are likely to be parental to the refractory forsterite-rich inclusions. Al-rich chondrules and pyroxene chondrule with tridymite identified in the matrix of the chondrite are likely to be xenogenic, originating from the formation area of enstatite chondrites.</p></sec></trans-abstract><kwd-group xml:lang="ru"><kwd>метеорит</kwd><kwd>хондрит</kwd><kwd>класт</kwd><kwd>брекчия</kwd><kwd>микроксенолиты</kwd><kwd>тугоплавкие богатые форстеритом включения</kwd><kwd>Al-хондры</kwd><kwd>высокомагнезиальные хондры</kwd></kwd-group><kwd-group xml:lang="en"><kwd>meteorite</kwd><kwd>chondrite</kwd><kwd>xenolith</kwd><kwd>breccia</kwd><kwd>microxenoliths</kwd><kwd>refractory forsterite rich objects</kwd><kwd>Al-chondrule</kwd><kwd>high-magnesian chondrule</kwd></kwd-group><funding-group><funding-statement xml:lang="ru">Исследование выполнено при финансовой поддержке РФФИ в рамках научного проекта № 19-35-90059, изучение методом лазерной абляции проведено в ЦКП УрО РАН “Геоаналитик” в рамках темы № АААА-А18-118053090045-8 государственного задания ИГГ УрО РАН</funding-statement><funding-statement xml:lang="en">The study was funded by the Russian Foundation for Basic Research, project No. 19-35-90059, a study using laser ablation was performed in Centre for Collective Use “Geoanalyst” under No. AAAA A18-118053090045-8 state project IGG UB RAS</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">Берзин С.В. 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