Late Jurassic to Cretaceous evolution of the eastern Tethyan Hawasina Basin (Oman Mountains). Issue 1 (30th November 2016)

• Record Type: Journal Article
• Authors: Wohlwend, Stephan; Celestino, Ricardo; Reháková, Daniela; Huck, Stefan; Weissert, Helmut
• Editors: Petrizzo, Maria Rose
• Is Part Of: Sedimentology. Volume 64:Issue 1(2017)
• Page Start: 87
• Page End: 110
• Publication Date: 2016-11-30
• Subjects: Carbon cycle -- Cretaceous -- eastern equatorial Tethys -- Hawasina Basin -- OAEs -- Oman Mountains -- palaeoceanography -- Sumeini and Hamrat Duru Group; Sedimentology -- Periodicals; 552.5
• DOI: 10.1111/sed.12326
• Languages: English
• ISSNs: 0037-0746

Abstract

Abstract: Remnants of a Mesozoic continental margin can be studied today in the nappe pile of the Oman Mountains. Successions of the Arabian carbonate platform and the adjacent deep Hawasina Basin are preserved in the nappe pile and in the foothills of this Mountain range. The Jurassic–Cretaceous sediment successions of the Hawasina Basin (Sumeini and Hamrat Duru Group) are focus of this study. These basinal archives contain information on the response of an eastern Tethyan equatorial ocean system to multiple perturbations of the carbon cycle and of climate during the Cretaceous. Turbiditic continental slope and basinal successions formed near the Calcite Compensation Depth are difficult to date with biostratigraphy and sequence stratigraphy. The available stratigraphic framework for the Hawasina successions was not sufficient for tracing palaeoceanography through the time window of interest in this study. Therefore, existing sequence stratigraphy and biostratigraphy are complemented by additional biostratigraphic data and with a newly established carbon and strontium isotope chemostratigraphy. The Hawasina Basin was affected by sea‐level variations, by changes in oceanography and also by regional tectonics. A first major modification of oceanography occurred at the end of the Jurassic when pelagic Maiolica‐type sediments were accumulated in the deep basin and on adjacent submarine highs (Lower Member of Huwar and Sid'r formations). Pelagic to hemipelagic conditions existed until the Valanginian, marked by a major carbon isotope excursion. Pelagic sediments were replaced afterwards by a succession of fine to coarse‐grained turbidites of Hauterivian to Aptian age. The transition into the mid‐Cretaceous is marked by a sudden shift to fine‐grained siliceous or chert deposits, at a time when sediments enriched in organic carbon were accumulated in the western Tethys and Atlantic Oceans. The continental slope as well as the Hawasina Basin seemed to have been well‐ventilated during Early and mid‐Cretaceous time. Siliceous limestones and chert are indicators of well‐mixed and nutrient‐rich surface water, while the absence of black shales suggests young and oxygenated deep water with a possible source on the vast Arabian platform. These peculiar oceanographic conditions were most pronounced during the onset of the extreme greenhouse episodes of the Oceanic Anoxic Event 1a.