gtcrustГеодинамика и тектонофизикаGeodynamics & Tectonophysics2078-502XInstitute of the Earth's crust of the Russian Academy of Sciences, Siberian Branch10.5800/GT-2024-15-5-0783ZRBDWLgtcrust-1919Research ArticleПАЛЕОГЕОДИНАМИКАPALEOGEODYNAMICSМАГМАТИЧЕСКИЕ ИСТОЧНИКИ ЭВОЛЮЦИОНИРУЮЩЕЙ КОНТИНЕНТАЛЬНОЙ ТЕКТОНОСФЕРЫ ИНДИИ: ГЕНЕРАЦИЯ ЩЕЛОЧНЫХ МАГМАТИЧЕСКИХ КОМПЛЕКСОВ С КАРБОНАТИТАМИ В МАССИВАХ САМАЛПАТТИ (ЮЖНАЯ ИНДИЯ) И АМБА ДОНГАР (ЗАПАДНАЯ ИНДИЯ)MAGMATIC SOURCES OF THE EVOLVING CONTINENTAL TECTONOSPHERE IN INDIA: GENERATION OF ALKALINE IGNEOUS COMPLEXES WITH CARBONATITES IN THE SAMALPATTI (SOUTHERN INDIA) AND AMBA DONGAR (WESTERN INDIA) MASSIFShttps://orcid.org/0000-0001-9084-1652РассказовС. В.RasskazovS. V.

664033, Иркутск, ул. Лермонтова, 128

664011, Иркутск, ул. Ленина, 3

128 Lermontov St, Irkutsk 664033

3 Lenin St, Irkutsk 664011

rassk@crust.irk.ruhttps://orcid.org/0000-0003-1696-5539ЯсныгинаТ. А.YasnyginaT. A.

664033, Иркутск, ул. Лермонтова, 128

128 Lermontov St, Irkutsk 664033

ХариК. Р.HariK. R.

492010, Райпур

Raipur 492010

https://orcid.org/0000-0002-1582-4753ЧувашоваИ. С.ChuvashovaI. S.

664033, Иркутск, ул. Лермонтова, 128

664011, Иркутск, ул. Ленина, 3

128 Lermontov St, Irkutsk 664033

3 Lenin St, Irkutsk 664011

https://orcid.org/0000-0002-1842-1239СаранинаЕ. В.SaraninaE. V.

664033, Иркутск, ул. Лермонтова, 128

664033, Иркутск, ул. Фаворского, 1а

128 Lermontov St, Irkutsk 664033

1а Favorsky St, Irkutsk664033

Институт земной коры СО РАН ; Иркутский государственный университетРоссияInstitute of the Earth’s Crust, Siberian Branch of the Russian Academy of Sciences ; Irkutsk State UniversityRussian FederationИнститут земной коры СО РАНРоссияInstitute of the Earth’s Crust, Siberian Branch of the Russian Academy of SciencesRussian FederationУниверситет им. Пандита Равишанкара ШуклыИндияPt. Ravishankar Shukla UniversityIndiaИнститут земной коры СО РАН ; Институт геохимии им. А.П. Виноградова СО РАНРоссияInstitute of the Earth’s Crust, Siberian Branch of the Russian Academy of Sciences ; Vinogradov Institute of Geochemistry, Siberian Branch of the Russian Academy of SciencesRussian Federation202418102024155783783Copyright © Рассказов С.В., Ясныгина Т.А., Хари К.Р., Чувашова И.С., Саранина Е.В., 20242024Рассказов С.В., Ясныгина Т.А., Хари К.Р., Чувашова И.С., Саранина Е.В.Rasskazov S.V., Yasnygina T.A., Hari K.R., Chuvashova I.S., Saranina E.V.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/1919

Смена источников карбонатитового магматизма Индии в эволюционирующей тектоносфере рассматривается на примере неопротерозойского массива Самалпатти и мел-палеогенового массива Амба Донгар. Выявляется унаследованный характер компонентов в распределении Ba и Sr разновозрастных карбонатитов Индии, тогда как в карбонатитах Северной Азии обозначаются самостоятельные тренды обогащения Ва и Sr. Предполагается, что в процессе активности тектоносферы Индийского субконтинента около 800 млн лет назад генерировались карбонатитовые расплавы протомантийного резервуара с возрастной оценкой протолита около 4.26 млрд лет. Этот резервуар резко отличается от резервуара первичной мантии застывшего магматического океана по низкому μ и высокому начальному отношению изотопов Nd. После того как в интервале 130–100 млн лет назад Индийский субконтинент отделился от Гондваны и около 66 млн лет назад начал соединяться с Азией, в тектоносфере активизировался источник ELMU. В качестве источника карбонатитов Амба Донгара мог служить протолит гадейской мантии с возрастом около 4.40 млрд лет. Одновременно в крупной магматической провинции Декан генерировались силикатные расплавы, протолиты которых соответствовали Pb-Pb возрасту около 2 млрд лет.

Neoproterozoic Samalpatti and Cretaceous-Paleogene Amba Dongar massifs are considered to evaluate the change of sources of carbonatite magmatism in evolving tectonosphere of India. The inherited character of Ba and Sr distribution components is traced in heterogeneous carbonatites of India, whereas the independent trends in Ba and Sr enrichment are traced in carbonatites of North Asia. It is inferred that in the process of activity in the tectonosphere of the Indian subcontinent ~800 Ma ago, carbonatite melts were generated in the mantle whose photolith has an age of 4.26 Ga. This protomantle reservoir was remarkably different from the primordial mantle reservoir in the solidified magma ocean in terms of low initial μ and high initial Nd isotope ratio. After the Indian subcontinent had separated from Gondwana 130–100 Ma ago and began to join Asia ~66 Ma ago, ELMU source was activiated in the tectonosphere. The Amba Dongar carbonatites might have been derived from the 4.40 Ga mantle protoliths. Silicate melts of the Deccan LIP were simultaneously generated from the protoliths with Pb-Pb age of ~2 Ga.

карбонатитынефелиновые сиенитынеопротерозоймелпалеогенBaSrмикроэлементы207Pb/204Pb143Nd/144Nd87Sr/86Srcarbonatitesnepheline syenitesNeoproterozoicCretaceousPaleogeneBaSrtrace elements207Pb/204Pb143Nd/144Nd87Sr/86SrИсследования выполнены по базовым проектам НИР ИЗК СО РАН (FWEF-2021-0009) «Современная геодинамика, механизмы деструкции литосферы и опасные геологические процессы в Центральной Азии» и геологического факультета ИГУ «Изучение процессов мантийно-корового взаимодействия и формирования месторождений полезных ископаемых».The research was done under the basic research projects of the Institute of the Earth Crust SB RAS (FWEF-2021-0009) "Modern geodynamics, mechanisms of the lithosphere destruction and hazardous geological processes in Central Asia" and the Faculty of Geology of ISU "Study of mantle-crust interaction processes and formation of mineral deposits".ReferencesAckerman L., Magna T., Rapprich V., Upadhyay D., Krátký O., Čejková B., Erban V., Kochergina Y.V., Hrstka T., 2017. 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The authors declare that there are no conflicts of interest present.