THE AGE OF THE BARABA FORMATION INFERRED FROM THE U/PB (SHRIMP) DATING (SREDINNYI RANGE, KAMCHATKA): GEOLOGICAL CONSEQUENCES

dc.contributor.authorSoloviev A.V.
dc.contributor.authorGrigorenko E.S.
dc.contributor.authorHourigan J.K.
dc.contributor.authorBrandon M.T.
dc.contributor.authorGarver J.I.
dc.date.accessioned2022-03-30T02:31:57Z
dc.date.available2022-03-30T02:31:57Z
dc.date.issued2004
dc.description.abstractThe Baraba Formation exposed in the Sredinnyi Range (Kamchatka), where it is composed of ter- restrial conglomerates, was considered for a long time as the late Campanian-lower Maastrichtian in age based on the fossil flora evidence. Zircons from the tuff layer in the lower part of the formation are dated at 50.5 ± 1.2 Ma using the U/Pb (SHRIMP) method, i.e., the accumulation of their host deposits commenced in the ter- minal early Eocene. The Baraba Formation overlies unconformably schists and phyllites of the Malka Group, which were metamorphosed during the pre-middle Eocene time, and the Irunei marginal-sea sediments thrust over metamorphic complexes and thus suggesting the pre-middle Eocene thrusting stage.
dc.identifierhttps://www.elibrary.ru/item.asp?id=13461653
dc.identifier.citationStratigraphy and Geological Correlation, 2004, 12, 4, 418-424
dc.identifier.issn0869-5938
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/36770
dc.titleTHE AGE OF THE BARABA FORMATION INFERRED FROM THE U/PB (SHRIMP) DATING (SREDINNYI RANGE, KAMCHATKA): GEOLOGICAL CONSEQUENCES
dc.typeСтатья

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