gtcrustГеодинамика и тектонофизикаGeodynamics & Tectonophysics2078-502XInstitute of the Earth's crust of the Russian Academy of Sciences, Siberian Branch10.5800/GT-2023-14-1-0685gtcrust-1629Research ArticleПАЛЕОГЕОДИНАМИКАPALEOGEODYNAMICSО ВРЕМЕНИ И УСЛОВИЯХ ФОРМИРОВАНИЯ ШОКШИНСКИХ КВАРЦИТОПЕСЧАНИКОВ ЮЖНО-ОНЕЖСКОЙ ВПАДИНЫ В СВЕТЕ НОВЫХ ДАННЫХ ИЗОТОПНОЙ ГЕОХРОНОЛОГИИON THE TIME AND CONDITIONS OF FORMATION OF THE SHOKSHA QUARTZITE-SANDSTONES OF THE SOUTH ONEGA DEPRESSION BASED ON THE NEW DATA FROM ISOTOPE GEOCHRONOLOGYКузнецовН. Б.KuznetsovN. B.

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

664033, Иркутск, ул. Лермонтова, 128

 

7-1 Pyzhevsky Ln, Moscow 119017,

128 Lermontov St, Irkutsk 664033

kouznikbor@mail.ruКолодяжныйС. Ю.KolodyazhnyiS. Yu.

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

7-1 Pyzhevsky Ln, Moscow 119017

РоманюкТ. В.RomanyukT. V.

123242, Москва, ул. Большая Грузинская, 10, стр. 1

10-1 Bolshaya Gruzinskaya St, Moscow 123242

СтрашкоА. В.StrashkoA. V.

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

119991, Москва, Ленинские горы, 1

7-1 Pyzhevsky Ln, Moscow 119017,

1 Leninskie Gory, Moscow 119991

БалуевА. С.BaluevA. S.

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

7-1 Pyzhevsky Ln, Moscow 119017

ТереховЕ. Н.TerekhovE. N.

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

7-1 Pyzhevsky Ln, Moscow 119017

МежеловскаяС. В.MezhelovskayaS. V.

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

117997, Москва, ул. Миклухо-Маклая, 23

7-1 Pyzhevsky Ln, Moscow 119017,

23 Miklukho-Maklay St, Moscow 117997

ДубенскийА. С.DubenskyA. S.

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

119991, Москва, Ленинские горы, 1

7-1 Pyzhevsky Ln, Moscow 119017,

1 Leninskie Gory, Moscow 119991

ШешуковВ. С.SheshukovV. S.

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

7-1 Pyzhevsky Ln, Moscow 119017

Геологический институт РАН; Институт земной коры СО РАНРоссияGeological Institute, Russian Academy of Sciences; Institute of the Earth’s Crust, Siberian Branch of the Russian Academy of SciencesRussian FederationГеологический институт РАНРоссияGeological Institute, Russian Academy of SciencesRussian FederationИнститут физики Земли им. О.Ю. Шмидта РАНРоссияSchmidt Institute of Physics of the Earth, Russian Academy of SciencesRussian FederationГеологический институт РАН; Московский государственный университет им. М.В. ЛомоносоваРоссияGeological Institute, Russian Academy of Sciences; Lomonosov Moscow State UniversityRussian FederationГеологический институт РАН; Российский государственный геологоразведочный университет им. Серго ОрджоникидзеРоссияGeological Institute, Russian Academy of Sciences; Sergo Ordzhonikidze Russian State University for Geological ProspectingRussian Federation202317022023141685685Copyright © Кузнецов Н.Б., Колодяжный С.Ю., Романюк Т.В., Страшко А.В., Балуев А.С., Терехов Е.Н., Межеловская С.В., Дубенский А.С., Шешуков В.С., 20232023Кузнецов Н.Б., Колодяжный С.Ю., Романюк Т.В., Страшко А.В., Балуев А.С., Терехов Е.Н., Межеловская С.В., Дубенский А.С., Шешуков В.С.Kuznetsov N.B., Kolodyazhnyi S.Y., Romanyuk T.V., Strashko A.V., Baluev A.S., Terekhov E.N., Mezhelovskaya S.V., Dubensky A.S., Sheshukov V.S.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/1629

Представлены первые результаты U-Pb изотопного датирования зерен детритового циркона (dZr) из красноцветных кварцитопесчаников шокшинской свиты (шокшинского горизонта). Шокшинская свита завершает разрез вепсийского надгоризонта (вепсия) нижнего протерозоя Карелии и распространена в Южно-Онежском прогибе (мульде). Проба (KL-555) красноцветных кварцитопесчаников отобрана из нижней части разреза шокшинской свиты на одноименном месторождении, расположенном в Юго-Западном Прионежье. Выделенные из этой пробы 79 зерен dZr проанализированы сотрудниками лаборатории химико-аналитических исследований ГИН РАН с использованием оборудования ЦКП ГИН РАН. Средневзвешенное значение трех наиболее молодых датировок зерен dZr – 1906±13 млн лет. С учетом известных изотопных датировок габбро-долеритов Ропручейского силла, прорывающего шокшинскую свиту, это дает возможность ограничить время формирования шокшинской свиты ~1.90–1.75 млрд лет. Значительная часть выполненных U-Pb анализов имеет высокую степень дискордантности вычисленных по ним датировок. Особенности распределения фигуративных точек анализов на диаграмме с конкордией позволяют предположить, что в фанерозое породы изученного разреза шокшинской свиты были подвержены воздействию, нарушившему U-Pb изотопную систему цирконовых зерен.

Набор полученных датировок зерен dZr сопоставлен с известными значениями возраста кристаллических комплексов фундамента Восточно-Европейской платформы. Наборы возрастов зерен dZr из пробы KL-555 и пород ладожской серии, развитой вдоль окраины Свекофеннского аккреционного орогена, очень сходны (р-коэффициент сходства теста Колмогорова – Смирнова – 0.27) и характеризуют главным образом тектономагматические события, непосредственно предшествовавшие проявлению главного этапа свекофеннского тектогенеза (1.90–1.87 млрд лет), поэтому образования ладожской серии с высокой степенью вероятности могли быть вторичным источником для шокшинских кварцитов. На основании сравнительного анализа возрастов и торий-урановых отношений (Th/U) в зернах dZr из пробы KL-555 сделан вывод о том, что часть изученных зерен dZr с высокими Th/U(>1.5) происходят из базитов людиковия, а с низкими (<0.1) – из ультравысокобарических образований (таких, как эклогиты), развитых в районах Салма, Куру-Ваара и Гридино.

Разработана палеогеографическая схема для поздневепсийского времени, показывающая, что высокозрелые шокшинские песчаники формировались в континентальных условиях в локальном бассейне за счет накопления обломочного материала, переносимого обширным и разветвленным седиментационным потоком в направлении с севера и северо-запада на юг и юг-юго-восток.

 

The first results of U-Pb isotope dating of detrital zircons (dZr) from red-colored quartzitic-sandstones of the Shoksha formation (Shoksha horizon) are presented. The Shoksha formation completes the Vepsian sub-horizon (Vepsian) of the Lower Proterozoic of Karelia and is distributed within the South Onega trough. A sample (KL-555) of red-colored quartzitic sandstones was taken from the lower part of the section of the Shoksha formation in the same name deposit within the southwestern Cis-Onega Lake region. The 79 dZr grains isolated from this sample were analyzed by the staff of the Chemistry-Isotopic Analytic Laboratory of the GIN RAS using the equipment of the Shared Research Facilities of the GIN RAS. The weighted average of the three youngest U-Pb isotope dates for dZr grains is 1906±13 Ma. Taking into account the known isotopic dates of gabbro-dolerites from the Ropruchei sill, that cuts through the Shoksha formation, it makes possible to constrain the time of the Shoksha formation accumulation by ~1.90–1.75 Ga. A significant part of the carried out analyzes has yielded a high degree of discordance of the dates. The features of the distribution of the figurative points of these analyzes in the diagram with concordia suggest that the rocks of the studied section of the Shoksha formation were subjected to the alteration that disturbed the U-Pb isotope system of these zircon grains in the Phanerozoic.

The set of obtained dates for dZr grains has been compared with the known ages of the crystalline complexes of the basement of the East European Platform. The age sets of dZr grains from sample KL-555 and rocks of the Ladoga group, developed along the margin of the Svecofennian accretionary orogen, are very similar (p similarity coefficient in Kolmogorov – Smirnov test is 0.27) and characterize mainly tectonic–magmatic events that had immediately preceded the manifestation of the Svecofennian orogeny (1.9–1.87 Ga). Therefore, the rocks of the Ladoga group could highly probably be a secondary source for the Shoksha quartzites. Based on a comparative analysis of ages and thorium-uranium ratios (Th/U) in dZr grains from sample KL-555, it was concluded that some of the studied dZr grains with high Th/U>1.5 originate from Ludicovian mafic rocks, but those with low Th/U<0.1 originate from ultra-high-pressure formations, such as eclogites known in the Salma, Kuru-Vaara and Gridino.

A paleo-geographic scheme for the Late Vepsian is proposed, showing that the highly mature Shoksha sandstones were generated under continental conditions in a local basin due to the accumulation of clastic material carried by an extensive and branched 

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The authors declare that there are no conflicts of interest present.