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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 custom-type="elpub" pub-id-type="custom">litosphere-701</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>ДИФФЕРЕНЦИАЦИЯ ВЕЩЕСТВА МАНТИИ В ПРОЦЕССЕ АККУМУЛЯЦИИ ЗЕМЛИ И ФОРМИРОВАНИЕ ПЕРВИЧНОЙ ЗЕМНОЙ КОРЫ</article-title><trans-title-group xml:lang="en"><trans-title></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>Анфилогов</surname><given-names>Всеволод Николаевич</given-names></name></name-alternatives><email xlink:type="simple">anfilogov@mineralogy.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>Хачай</surname><given-names>Юрий Васильевич</given-names></name></name-alternatives><email xlink:type="simple">yukhachay@yandex.ru</email><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff xml:lang="ru" id="aff-1"><institution>Институт минералогии УрО РАН</institution><country>Russian Federation</country></aff><aff xml:lang="ru" id="aff-2"><institution>Институт геофизики УрО РАН</institution><country>Russian Federation</country></aff><pub-date pub-type="collection"><year>2012</year></pub-date><pub-date pub-type="epub"><day>15</day><month>02</month><year>2019</year></pub-date><volume>0</volume><issue>6</issue><fpage>3</fpage><lpage>13</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Анфилогов В.Н., Хачай Ю.В., 2019</copyright-statement><copyright-year>2019</copyright-year><copyright-holder xml:lang="ru">Анфилогов В.Н., Хачай Ю.В.</copyright-holder><copyright-holder xml:lang="en">Анфилогов В.Н., Хачай Ю.В.</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/701">https://www.lithosphere.ru/jour/article/view/701</self-uri><abstract><p>На основе численного моделирования исследуется динамика Р-Т условий во внутренних областях Земли в процессе ее аккмуляции. Основное внимание уделено условиям формирования мантии и первичной коры. Более подробно прослеживаются варианты, в которых преимущественно силикатное вещество первичной мантии отлагается на разогретой поверхность ядра, температура которой выше температуры ликвидуса силикатного вещества мантии. В результате прогрева на границе ядро–мантия образуется слой силикатного расплава. При достижении слоем критической мощности расплав начинает кристаллизоваться и на границе ядро–мантия формируется слой кристаллического материала, преимущественно Mg-перовскитового и магнезиовюститового состава. По мере увеличения мощности мантии, слой расплава перемещается к поверхности. На завершающей стадии аккумуляции Земли расплав дифференцируется, обогащаясь FeO и Al2O3 и из него формируется древняя анортозитовая кора. Одновременно происходит образование океана с высокой температурой воды, и анортозитовая кора трансформируется в хемогенные осадочные кварциты с прослоями корундовых и силлиманитовых гнейсов.</p></abstract><kwd-group xml:lang="ru"><kwd>Земля</kwd><kwd>гетерогенная аккумуляция</kwd><kwd>ядро</kwd><kwd>мантия</kwd><kwd>древняя кора</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">Анфилогов В.Н., Хачай Ю.В. Возможный вариант дифференциации вещества на начальном этапе формирования Земли // Докл. АН. 2005. Т. 405, № 6. С. 803–806.</mixed-citation><mixed-citation xml:lang="en">Анфилогов В.Н., Хачай Ю.В. Возможный вариант дифференциации вещества на начальном этапе формирования Земли // Докл. АН. 2005. Т. 405, № 6. С. 803–806.</mixed-citation></citation-alternatives></ref><ref id="cit2"><label>2</label><citation-alternatives><mixed-citation xml:lang="ru">Вдовыкин Г.П. Метеориты. 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