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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">geores</journal-id><journal-title-group><journal-title xml:lang="ru">Георесурсы</journal-title><trans-title-group xml:lang="en"><trans-title>Georesources</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">1608-5043</issn><issn pub-type="epub">1608-5078</issn><publisher><publisher-name>Georesursy LLC</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.18599/grs.2021.1.10</article-id><article-id custom-type="elpub" pub-id-type="custom">geores-220</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>ГЕОФИЗИЧЕСКИЕ ИССЛЕДОВАНИЯ И ГЕОИНФОРМАЦИОННЫЕ ТЕХНОЛОГИИ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>GEOPHYSICAL SURVEYS AND GEO-INFORMATION TECHNOLOGIES</subject></subj-group></article-categories><title-group><article-title>Типоморфизм породообразующих минералов лунного реголита, станций Луна-16, -20, -24, сравнение море-континент-море</article-title><trans-title-group xml:lang="en"><trans-title>Typomorphism of rock-forming minerals of Lunar regolith, Luna-16, -20, -24: comparision of sea vs continent vs sea</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>Макеев</surname><given-names>А. Б.</given-names></name><name name-style="western" xml:lang="en"><surname>Makeyev</surname><given-names>A. B.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Александр Борисович Макеев – доктор геол.-мин. наук, профессор, ведущий научный сотрудник Лаборатории геологии рудных месторождений</p><p>119017, Москва, Старомонетный пер., д. 35</p></bio><bio xml:lang="en"><p>Alexander B. Makeyev – Dr. Sci. (Geology and Mineralogy), Professor, Leading Researcher, Laboratory of Ore Deposits Geology</p><p>35, Staromonetny Lane, Moscow, 119017</p></bio><email xlink:type="simple">abmakeev@igem.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>Брянчанинова</surname><given-names>Н. И.</given-names></name><name name-style="western" xml:lang="en"><surname>Bryanchaninova</surname><given-names>N. I.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Наталия Игоревна Брянчанинова – доктор геол.-мин. наук, ведущий научный сотрудник</p><p>119017, Москва, Пыжевский пер, д. 7, стр.1</p></bio><bio xml:lang="en"><p>Nataliya I. Bryanchaninova – Dr. Sci. (Geology and Mineralogy), Leading Researcher</p><p>7, Pyzhevsky lane, Moscow, 119017</p></bio><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт геологии рудных месторождений, петрографии, минералогии и геохимии РАН</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Institute of Ore Geology, Petrography, Mineralogy and Geochemistry of the Russian Academy of Sciences</institution><country>Russian Federation</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru"><institution>Геологический институт РАН</institution><country>Россия</country></aff><aff xml:lang="en"><institution>Geological Institute of the Russian Academy of Sciences</institution><country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2021</year></pub-date><pub-date pub-type="epub"><day>20</day><month>04</month><year>2024</year></pub-date><volume>23</volume><issue>1</issue><fpage>94</fpage><lpage>105</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Макеев А.Б., Брянчанинова Н.И., 2024</copyright-statement><copyright-year>2024</copyright-year><copyright-holder xml:lang="ru">Макеев А.Б., Брянчанинова Н.И.</copyright-holder><copyright-holder xml:lang="en">Makeyev A.B., Bryanchaninova N.I.</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.geors.ru/jour/article/view/220">https://www.geors.ru/jour/article/view/220</self-uri><abstract><p>Изучены химические и минералогические особенности лунного реголита (электронные микроскопы JXA8200 и JSM-5610LV, 400 анализов, 50 BSE изображений, 9 фрагментов послойных проб керна) в местах посадок станций Луна-16, -20, -24 для сравнения обстановок море-континент. Диагностировано 18 минеральных фаз и 12 их разновидностей. Наиболее широко распространены железо-магниевые и кальциевые силикаты: анортит, клинопироксены и оливин. Обсуждаются типоморфные особенности породообразующих минералов в двух типах лунной поверхности. Для отображения составов лунных хромшпинелидов предложена диаграмма в виде развертки треугольной призмы.</p></abstract><trans-abstract xml:lang="en"><p>The study focuses on the comparison of the chemical and mineral composition of Lunar regolith probes from Luna-16, -20, -24 stations and their the seacontinent environments. Using microprobe JXA-8200 and JSM-5610LV (400 analyses, 50 images, 9 fragments of layer-by-layer core samples) 18 mineral phases and their 12 varieties were diagnosed. The most common are ironmagnesium and calcium-bearing varieties of silicates – anortite, clinopyroxenes and olivine. The typomorphic features of rock-forming minerals in two types of the lunar surface are discussed. The composition of chromespinelids is demonstrated on a triangular prism diagram.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>Луна</kwd><kwd>советские автоматические станции</kwd><kwd>лунный реголит</kwd><kwd>море Изобилия</kwd><kwd>Кризисов</kwd><kwd>анортит</kwd><kwd>клинопироксен</kwd><kwd>оливин</kwd><kwd>ильменит</kwd><kwd>морские базальты</kwd><kwd>оливиновое габбро</kwd></kwd-group><kwd-group xml:lang="en"><kwd>Moon</kwd><kwd>Soviet automatic stations</kwd><kwd>Lunar regolith</kwd><kwd>Mare Fecunditatis</kwd><kwd>sea of Crises</kwd><kwd>anorthite</kwd><kwd>clinopyroxen</kwd><kwd>olivine</kwd><kwd>ilmenite</kwd><kwd>olivine gabbro</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">Барсуков В.Л. (1977). Предварительные данные по керну реголита, доставленному на Землю автоматической лунной станцией «Луна-24». 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