gtcrustГеодинамика и тектонофизикаGeodynamics & Tectonophysics2078-502XInstitute of the Earth's crust of the Russian Academy of Sciences, Siberian Branch10.5800/GT-2023-14-2-0692gtcrust-1663Research ArticleПАЛЕОГЕОДИНАМИКАPALEOGEODYNAMICSВОЛГО-ДОНСКОЙ КОЛЛИЗИОННЫЙ ОРОГЕН ВОСТОЧНО-ЕВРОПЕЙСКОГО КРАТОНА КАК ПАЛЕОПРОТЕРОЗОЙСКИЙ АНАЛОГ ГИМАЛАЙ-ТИБЕТСКОГО ОРОГЕНАTHE VOLGA-DON COLLISIONAL OROGEN IN THE EAST EUROPEAN CRATON AS THE PALEOPROTEROZOIC ANALOGUE OF THE HIMALAYAN-TIBETAN OROGENhttps://orcid.org/0000-0003-4426-1176ЩипанскийА. А.ShchipanskyA. A.

119017, Москва, Пыжевский пер., 7, стр. 1

7-1 Pyzhevsky Ln, Moscow 119017

ХерасковаТ. Н.KheraskovaT. N.

119017, Москва, Пыжевский пер., 7, стр. 1

7-1 Pyzhevsky Ln, Moscow 119017

Геологический институт РАНРоссияGeological Institute, Russian Academy of SciencesRussian Federation202319042023142692692Copyright © Щипанский А.А., Хераскова Т.Н., 20232023Щипанский А.А., Хераскова Т.Н.Shchipansky A.A., Kheraskova T.N.Данная работа распространяется под лицензией Creative Commons Attribution 4.0.This work is licensed under a Creative Commons Attribution 4.0 License.https://www.gt-crust.ru/jour/article/view/1663

Волго-Донской складчато-надвиговый пояс, возникший около 2.0 млрд лет тому назад, занимает площадь около 300000 км2 (~500 км в ширину и ~600 км в длину) и располагается между архейскими протократонными Сарматским и Волго-Уральским блоками Восточно-Европейского кратона, которые подстилаются мощными, 200‒300 км, сублитосферными мантийными килями. Целью настоящей статьи является выяснение природы его происхождения, для того чтобы ответить на фундаментальный вопрос о том, как этот и другие складчато-надвиговые пояса могли формироваться в палеопротерозое и был ли стиль орогенеза того времени схожим с таковым современных коллизионных орогенов или отличным от него. В качестве тектонотипа коллизионной геодинамики принято рассматривать хорошо изученный дивергентный Гималайско-Тибетский орогенический пояс, особенности развития которого, как правило, служат основой для расшифровки орогенических процессов в геологической истории Земли. Однако для раннего докембрия широко распространены представления о том, что орогенические процессы того времени должны были сильно отличаться от современного орогенеза вследствие высокого геотермического градиента в коре, обусловленного повышенной радиоактивной теплогенерацией.

В статье авторы детально рассматривают глубинную тектонику палеопротерозойского Волго-Донского орогена, реконструкция которого свидетельствует о том, что он представляет собой слабо эродированную орогеническую постройку дивергентной архитектуры; она сложена преимущественно ювенильными метаосадками, фазы ее развития сопоставляются с историей становления Гималайско-Тибетского коллизионного орогена, но не согласуются с представлениями о «горячем/ультрагорячем» стиле орогенеза в раннем докембрии, базирующимися, прежде всего, на результатах численного моделирования.

The ca 2.0 Ga Volgo-Don fold-and-thrust belt, about 500 km in width and at least 600 km in length, covering an area of about 300000 square kilometers intervenes between the Archean Sarmatian and Volgo-Uralian proto-cratonic blocks of the East European Craton, both of which are coupled with 200–300 km thick sub-continental lithospheric mantle keels. The focus of this paper is the elucidation of its nature in order to answer the basic question how this and other thrust-and-fold belts could be formed in the Paleoproterozoic, and whether they are the same as or different from modern collision orogens. The active Himalayan-Tibet orogen is commonly thought of as the most extensively studied large, bi-verging fold-and thrust belt continental collision zone which may provide insight into key tectonic mechanisms for an understanding of orogenic processes in the Earth’s geological past. Precambrian orogens are tentatively perceived yet as something that was distinct from recent orogenic styles and was due to the initial elevated geotherm and higher radio-genic heat production in the early Earth.

In this paper we report for the first time the revealation of the large, slightly eroded divergent Paleoproterozoic Volgo-Don orogen which is mostly composed of juvenile metasediments and comprises well-preserved patterns of the crustal orogenic architecture which are characteristic of the archetypal Himalayan-Tibet collisional orogen rather than of hot/ultra-hot Precambrian orogens based on numerical modeling.

ранний докембрийлитосфератермальная модель ТС1орогенглубинная структура земной корыколлизияEarly Precambrianlithospherethermal model TC1orogencrustal architecturecollisionРабота выполнена при поддержке Минобрнауки РФ в рамках Соглашений о сотрудничестве АААА-А20-120030690018-2 и АААА-А20-120030490104-4.The material is based upon works supported by the Ministry of Science and Higher Education of the Russian Federation under Cooperative Agreements АААА-А20-120030690018-2, and АААА-А20-120030490104-4. This article is devoted to the memory of S. Bogdanova and E. Bibikova who made the valuable contribution to the study on tectonics of EEC and with whom we had fruitful discussions for many years. We thank S. Pisarevsky and an anonymous reviewer for constructive and thorough comments that improved the text considerably. V. Balagansky is warmly thanked for his editorial comments for an early version of the manuscript.ReferencesArtemieva I.M., 2003. 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The authors declare that there are no conflicts of interest present.