References

gtcrust

Геодинамика и тектонофизика

Geodynamics & Tectonophysics

2078-502X

Institute of the Earth's crust of the Russian Academy of Sciences, Siberian Branch

10.5800/GT-2021-12-3-0540

gtcrust-1241

Research Article

ПАЛЕОГЕОДИНАМИКА

PALEOGEODYNAMICS

О ВРЕМЕНИ ФОРМИРОВАНИЯ КАНДАЛАКШСКОГО И КЕРЕЦКОГО ГРАБЕНОВ ПАЛЕОРИФТОВОЙ СИСТЕМЫ БЕЛОГО МОРЯ В СВЕТЕ НОВЫХ ДАННЫХ ИЗОТОПНОЙ ГЕОХРОНОЛОГИИ

TIME CONSTRAINTS ON THE FORMATION OF THE KANDALAKSHA AND KERETSK GRABENS OF THE WHITE SEA PALEO-RIFT SYSTEM FROM NEW ISOTOPIC GEOCHRONOLOGICAL DATA

Кузнецов

Н. Б.

Kuznetsov

N. B.

119017, Москва, Пыжевский пер., 7

664033, Иркутск, ул. Лермонтова, 128

7 Pyzhevsky Ln, Moscow 119017

128 Lermontov St, Irkutsk 664033

kouznikbor@mail.ru

Балуев

А. С.

Baluev

A. S.

119017, Москва, Пыжевский пер., 7

7 Pyzhevsky Ln, Moscow 119017

Терехов

Е. Н.

Terekhov

E. N.

119017, Москва, Пыжевский пер., 7

7 Pyzhevsky Ln, Moscow 119017

Колодяжный

С. Ю.

Kolodyazhnyi

S. Yu.

119017, Москва, Пыжевский пер., 7

7 Pyzhevsky Ln, Moscow 119017

Пржиялговский

Е. С.

Przhiyalgovskii

E. S.

119017, Москва, Пыжевский пер., 7

7 Pyzhevsky Ln, Moscow 119017

Романюк

Т. В.

Romanyuk

T. V.

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

10-1 Bolshaya Gruzinskaya St, Moscow 123242

Дубенский

А. С.

Dubensky

A. S.

119017, Москва, Пыжевский пер., 7

119991, Москва, Ленинские горы, 3

7 Pyzhevsky Ln, Moscow 119017

3 Leninskie Gory, Moscow 119991

Шешуков

В. С.

Sheshukov

V. S.

119017, Москва, Пыжевский пер., 7

7 Pyzhevsky Ln, Moscow 119017

Ляпунов

С. М.

Lyapunov

S. M.

119017, Москва, Пыжевский пер., 7

7 Pyzhevsky Ln, Moscow 119017

Баянова

Т. Б.

Bayanova

T. B.

184209, Апатиты, ул. Ферсмана, 14

14 Fersman St, Apatity 184209

Серов

П. А.

Serov

P. A.

184209, Апатиты, ул. Ферсмана, 14

14 Fersman St, Apatity 184209

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 Federation

Геологический институт РАНРоссияGeological Institute, Russian Academy of SciencesRussian Federation

Институт физики Земли им. О.Ю. Шмидта РАНРоссияSchmidt Institute of Physics of the Earth, Russian Academy of SciencesRussian Federation

Геологический институт РАН; Московский государственный университет им. М.В. ЛомоносоваРоссияGeological Institute, Russian Academy of Sciences; Lomonosov Moscow State UniversityRussian Federation

Геологический институт КНЦ РАНРоссияGeological Institute, Kola Scientific Center of the Russian Academy of SciencesRussian Federation

2021

17092021

123570607

2021

Кузнецов Н.Б., Балуев А.С., Терехов Е.Н., Колодяжный С.Ю., Пржиялговский Е.С., Романюк Т.В., Дубенский А.С., Шешуков В.С., Ляпунов С.М., Баянова Т.Б., Серов П.А.

Kuznetsov N.B., Baluev A.S., Terekhov E.N., Kolodyazhnyi S.Y., Przhiyalgovskii E.S., Romanyuk T.V., Dubensky A.S., Sheshukov V.S., Lyapunov S.M., Bayanova T.B., Serov P.A.

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/1241

На начальном этапе исследований возраст и стратиграфическое положение терской свиты ограничивались снизу ее налеганием на раннепротерозойские гранитоиды, а сверху – тем, что породы терской свиты вмещают позднедевонские щелочные интрузии (в том числе и трубки взрыва).

В статье представлены результаты U-Pb изотопного датирования зерен детритового циркона (dZr) из песчаников терской свиты, дополненные определениями химического состава пород и результатами их изотопного Sm-Nd изучения. Полученный средневзвешенный возраст четырех наиболее молодых зерен dZr из песчаников терской свиты составил 1145±20 млн лет, что означает, что часть разреза терской свиты, залегающая выше изученного уровня, не может быть древнее конца среднего рифея. Сравнительный анализ полученного набора U-Pb изотопных датировок зерен dZr (провенанс-сигнала) из песчаников терской свиты и аналогичных данных по другим верхнедокембрийским обломочным толщам, распространенным на северо-востоке Восточно-Европейской платформы и в сопредельных регионах, выявил существенные различия. Это находится в хорошем соответствии с представлениями о том, что палеогеографическую обстановку, господствовавшую в конце среднего и в позднем рифее в области заложения и развития рифтовой системы Белого моря (РСБМ), можно рассматривать как совокупность небольших (часто бессточных) бассейнов, разделенных поднятиями. Эти бассейны могли время от времени иметь связь с Мировым океаном. Такая палеогеографическая ситуация не благоприятствовала развитию крупных рек, поэтому грабены заполнялись преимущественно материалом местного происхождения. Кандалакшский и Керецкий грабены РСБМ заполнены осадками морского генезиса, представляющими собой преимущественно продукты размыва вещественных комплексов, участвующих в строении бортов этих грабенов. Среди местных локальных источников идентифицированы эклогитовые комплексы с возрастом метаморфизма ~1.9 млрд лет и базитовового магматизма с возрастом ~2.4–2.5 и ~2.7–2.9 млрд лет. Попадание зерен dZr, для которых нет потенциальных близких первичных источников, расположенных около Керецкого грабена, произошло за счет рециклинга из вторичных источников циркона – местных древних осадочных образований.

Initially, the age and stratigraphic position of the Tersk formation were determined with respect to the fact that this formation overlaps the Early Proterozoic granitoids. Its top was marked by the rocks penetrated by the Late Devonian alkaline intrusions, including explosion pipes.

This article presents the U-Pb isotopic dating of detrital zircon grains (dZr) from sandstones of the Tersk formation. It describes the geochemical compositions of the rocks and the Sm-Nd study results. In our study, the weighted average age of four youngest dZr grains from the sandstones of the Tersk formation is 1145±20 Ma, which suggests that the rocks above the studied rock layer (see the Tersk formation cross-section) are is not older than the end of the Middle Riphean. The U-Pb isotopic ages of dZr grains (provenance signals) from the sandstones of the Tersk formation were compared to the ages of other Upper Precambrian clastic strata in the northeastern East European platform (EEP) and adjacent areas. Our comparative analysis shows that these rocks significantly differ in age. This conclusion is in good agreement with the idea that at the end of the Middle and during the Late Riphean, several small (mainly closed) basins separated by uplifts dominated in the paleogeographic setting of the area wherein the White Sea rift system (WSRS) formed and developed. Temporal connections of these basins with the ocean were possible. Such paleogeographic setting does not favour the development of large rivers; this is why the grabens are mainly filled with local rock materials. The Keretsk and Kandalaksha grabens (WSRS) are filled with marine sediments eroded from the grabens walls. The local sediment sources include eclogite complexes (~1.9 Ga), which basic magmatism is dated at ~2.4–2.5 and ~2.7–2.9 Ga. Any potential primary sources for dZr grains are lacking in the area near the Keretsk graben. We suggest that such grains occurred due to recycling of the secondary sources of zircon, i.e. originated from ancient local sedimentary formations.

рифейрифтовая система Белого моряКандалакшский и Керецкий грабенытерская свитазерна детритового цирконаU–Pb датирование

RipheanWhite Sea rift system (WSRS)Keretsk and Kandalaksha grabensTersk formationdetrital zircon grainsU-Pb dating

Работа выполнена в рамках бюджетной темы лаборатории ГИН РАН при поддержке РФФИ, проект № 18-05-00485. Сбор и систематизация геохронологических данных выполнены при финансовой поддержке МОН РФ (мегагрант 075-15-2019-1883, «Орогенез: образование и рост континентов и суперконтинентов»).

The study was budgeted by the Geological Institute RAS (Laboratory budget) and supported by the Russian Foundation for Basic Research (Project 18-05-00485). The geochronological data were consolidated and systematized with the financial support of the RF Ministry of Education and Science (Megagrant 075-15-2019-1883 – Orogenesis: Formation and Growth of Continents and Supercontinents).

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