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Mercury Isotope Geochemistry in Ediacaran Cap Carbonates and Cretaceous Oceanic Red Beds

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Mercury (Hg), a highly volatile metal, is capable of tracing volcanism through geological history as LIP events transiently emit large amounts of Hg. There are two indicators that make Hg a unique tool for geochemistry, the Hg to total organic carbon ratio (Hg/TOC) and mass-independent fractionation (Hg-MIF, defined as Δ199Hg). Owing to the affinity of Hg to organic matter, anomalous high Hg/TOC ratios in sediments can better reveal large volcanic eruptions. The anomaly of Hg-MIF is mainly observed in Hg photoreactions, providing a fingerprints of specific reaction pathways of Hg. Volcanic Hg usually has Δ199Hg ~ 0, but photochemical processes in the surface environment can alter this signal, resulting in positive Δ199Hg in marine systems (e.g., seawater and marine sediments) and negative Δ199Hg in terrestrial systems (e.g., soil and vegetation). Here, we examined the Hg records in Ediacaran cap carbonates in South China and Upper Cretaceous oceanic red beds (ORBs) in southern Tibet and the North Atlantic, to obtain their sedimentary material sources and the cause of the termination of Marinoan glaciation and Cretaceous oceanic anoxic events. (1) The cap carbonates show higher Hg concentrations (4.9 to 405 ppb), most of which are comparable to that observed in carbonates deposited during non-LIPs periods. The lack of Hg/TOC anomalies in these cap carbonates suggests that background volcanic activity, rather than a short-term large igneous province event, drove the Marinoan deglaciation. The cap carbonates show positive Δ199Hg values (0.18 to 0.34 ‰) in slope settings and slightly negative to slightly positive Δ199Hg values (0.16 to 0.11 ‰) in shelf settings, suggesting a binary mixing of seawater- and terrestrial-derived Hg in early Ediacaran Ocean. We infer that the accumulation of greenhouse gases, due to ongoing volcanic emissions of CO2 and enhanced release of gas hydrates, triggered global warming. This warming led to melting of sea ice cover, enhanced terrestrial inputs, and large-scale dissolution of atmospheric CO2 into seawater, driving widespread deposition of Ediacaran cap carbonates. (2) In southern Tibet and the North Atlantic, black/gray shales (typical deposition of oceanic anoxic events) show much higher Hg concentrations and Hg/TOC values than ORBs, indicating enhanced Hg flux to global oceans during time of black/gray shale deposition. Black/gray shales show lower Fe3+/Fe2+ and positive Δ199Hg, suggesting a significant input of Hg into the anoxic/dysoxic ocean via atmospheric deposition. The isotope values are consistent with a volcanic source for this excess Hg. ORBs show high Fe3+/Fe2+ and negative shifts of Δ199Hg, suggesting that the dominant source of Hg into the oxic oceans was via terrestrial runoff. These results suggest that volcanism was an important driver of the climate/ocean dynamics during the Late Cretaceous. To sum up, in addition to indicating short-strong volcanic activities, Hg can also trace the source of sedimentary materials under weak magmatism. Moreover, Hg offers a more accurate depiction of the interactions and exchanges among the Earth’s atmosphere-ocean-land system.

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The Cretaceous is an important period in which many geological events occurred, especially the OAEs (oceanic anoxic events) which are characterized by black shale, and the oxic process characterized by CORBs (Cretaceous oceanic red beds). In this paper, the causative mechanism behind the formation of black shale and the oceanic red beds are described in detail. This may explain how the oceanic environment changed from anoxic to oxic in the Cretaceous period. It is suggested that these two different events happened because of the same cause. On the one hand, the large-scale magma activities in Cretaceous caused the concentration of CO2, the release of the inner energy of the earth, superficial change in the ocean-land, and finally, the increase of atmospheric temperature. These changes implied the same tendency as the oceanic water temperature show, and caused the decrease in O2 concentration in the Cretaceous ocean, and finally resulted in the occurrence of the OAEs. On the other hand, violent and frequent volcanic eruptions in the Cretaceous produced plenty of Fe-enriched lava on the seafloor. When the seawater reacted with the lava, the element Fe became dissolved in seawater. Iron, which could help phytoplankton grow rapidly, is a micronutrient essential to the synthesis of enzymes required for photosynthesis in the oceanic environment. Phytoplankton, which grows in much of the oceans around the world, can consume carbon dioxide in the air and the ocean. Meanwhile, an equal quantity of oxygen can be produced by the phytoplankton during its growth. Finally, the oxic environment characterized by red sediment rich in Fe3+ appeared. The anoxic and oxic conditions in the Cretaceous ocean were caused by volcanic activities, but they stemmed from different causative mechanisms. The former was based on physical and chemical processes, while the latter involved more complicated bio-oceanic-geochemical processes.

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During the Late Cretaceous, Earth's climate oscillated between warm and cool states, and global oceans changed between anoxic and oxic conditions, resulting in black/gray shales and oceanic red beds (ORBs) deposition, respectively. To understand such climate/ocean dynamics, this study investigated bulk Hg and Hg isotopes, as well as Fe3+/Fe2+ in Upper Cretaceous sediments deposited in southern Tibet and the North Atlantic. In both areas, black/gray shales show much higher Hg concentrations than ORBs, indicating enhanced Hg flux to global oceans during time of black/gray shale deposition. Black/gray shales show lower Fe3+/Fe2+ and positive Δ199Hg, suggesting a significant input of Hg into the anoxic/dysoxic ocean via atmospheric deposition. The isotope values are consistent with a volcanic source for this excess Hg. ORBs show high Fe3+/Fe2+ and negative shifts of Δ199Hg, suggesting that the dominant source of Hg into the oxic oceans was via terrestrial runoff. This study suggests that volcanism was an important driver of the climate/ocean dynamics during the Late Cretaceous.

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Abstract: Cretaceous oceanic red beds (CORBs) represented by red shales and marls, were deposited during the Cretaceous and early Paleocene, predominantly in the Tethyan realm, in lower slope and abyssal basin environments. Detailed studies of CORBs are rare; therefore, we compiled CORBs data from deep sea ocean drilling cores and outcrops of Cretaceous rocks subaerially exposed in southern Europe, northwestern Germany, Asia and New Zealand. In the Tethyan realm, CORBs mainly consist of reddish or pink shales, limestones and marlstones. By contrast, marlstones and chalks are rare in deep‐ocean drilling cores. Upper Cretaceous marine sediments in cores from the Atlantic Ocean are predominantly various shades of brown, reddish brown, yellowish brown and pale brown in color. A few red, pink, yellow and orange Cretaceous sediments are also present. The commonest age of CORBs is early Campanian to Maastrichtian, with the onset mostly of oxic deposition often after Oceanic Anoxic Events (OAEs), during the early Aptian, late Albian‐early Turonian and Campanian. This suggests an indicated and previously not recognized relationship between OAEs, black shales deposition and CORBs. CORBs even though globally distributed, are most common in the North Atlantic and Tethyan realms, in low to mid latitudes of the northern hemisphere; in the South Atlantic and Indian Ocean in the mid to high latitudes of the southern hemisphere; and are less frequent in the central Pacific Ocean. Their widespread occurrence during the late Cretaceous might have been the result of establishing a connection for deep oceanic current circulation between the Pacific and the evolving connection between South and North Atlantic and changes in oceanic basins ventilation.

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The “Cretaceous oceanic red beds (CORBs)” associated with “oceanic oxic events” have become a hot topic for geologists from around the world. In southern Tibet, the CORBs are widely distributed in the Upper Cretaceous of the northern Tethys Himalayas, but they have never been reported from the southern Tethyan Himalaya (Tibet, China). A mixed Upper Cretaceous carbonate‐shale succession is well exposed in the Gyabukeqing section of Guru town, Yadong County, southern Tibet, which tectonically belongs to the southern Tethyan Himalaya. These sedimentary strata constitute the transition from the Gangbacunkou Formation shale towards the Zongshan Formation limestone through the Jiubao Formation alternations of marl and shale. The Gangbacunkou Formation is characterized by grey‐greenish shales occasionally interspersed with laminated marls, followed by the Jiubao Formation composed of marls with interbeds of shales, which is overlain by the limestones of the Zongshan Formation. A 5‐m‐thick purplish marl bed was found from the lower Jiubao Formation in the Gyabukeqing section, and these reddish marls are assignable to shallow marine red beds. Detailed foraminifer biostratigraphy established five planktic foraminifer zones: Dicarinella covcavata, D. asymetrica, Globotruncanita elevata, G. ventricosa, and Radotruncana calcarata throughout the entire Upper Cretaceous succession in the Gyabukeqing section. The reddish marl beds are constrained as middle Campanian in age as they are calibrated to the middle part of the foraminifer Radotruncana calcarata Zone. As a comparison, the typical CORBs of pelagic–hemipelagic settings are also documented from the Upper Cretaceous of the northern Tethys Himalayas in southern Tibet. A total of 10 microfacies were recognized from the entire sequence of the Upper Cretaceous outer shelf‐slope settings in the Yadong area, southern Tibet. The Yadong red marl beds represent the sedimentation of the foraminiferal biomicrite/foraminiferal wackestone and mudstone/mudrock microfacies, pointing to a shallow marine continental shelf margin setting. Global biostratigraphic correlations indicate that the Yadong red marl beds are coeval with the typical CORBs of the Gyangze and Kangmar documented from the northern Tethys Himalayas in this study or reported previously from the same region as well as elsewhere in the world. The Yadong red beds also are comparable in lithology and biostratigraphy with the shallow marine red beds documented from Europe, and they all may represent the contemporaneous deposition of the CORBs in shallow shelf. These shallow marine CORBs share similar depositional mechanisms: undergoing a phase of iron and manganese enrichment in seawater due to injection of deep sea anoxic water to shallow shelf, followed by oxidization in shallow settings or being oxidized during diagenetic process or a response to the oxygenation of coeval CORBs in deep seas.

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