Mediterranean isolation preconditioning the Earth System for late Miocene climate cooling

The origin of carbonate mud and implications for global climate

Carbonate mud represents one of the most important geochemical archives for reconstructing ancient climatic, environmental, and evolutionary change from the rock record. Mud also represents a major sink in the global carbon cycle. Yet, there remains no consensus about how and where carbonate mud is formed. Here, we present stable isotope and trace-element data from carbonate constituents in the Bahamas, including ooids, corals, foraminifera, and algae. We use geochemical fingerprinting to demonstrate that carbonate mud cannot be sourced from the abrasion and mixture of any combination of these macroscopic grains. Instead, an inverse Bayesian mixing model requires the presence of an additional aragonite source. We posit that this source represents a direct seawater precipitate. We use geological and geochemical data to show that "whitings" are unlikely to be the dominant source of this precipitate and, instead, present a model for mud precipitation on the bank margins that can explain the geographical distribution, clumped-isotope thermometry, and stable isotope signature of carbonate mud. Next, we address the enigma of why mud and ooids are so abundant in the Bahamas, yet so rare in the rest of the world: Mediterranean outflow feeds the Bahamas with the most alkaline waters in the modern ocean (>99.7th-percentile). Such high alkalinity appears to be a prerequisite for the nonskeletal carbonate factory because, when Mediterranean outflow was reduced in the Miocene, Bahamian carbonate export ceased for 3-million-years. Finally, we show how shutting off and turning on the shallow carbonate factory can send ripples through the global climate system.

Vegetation climate and marine environmental reconstruction in the western Mediterranean (southern Rifian corridor, Morocco) over the Tortonian-Messinian transition

The Southern Rifian Corridor was a gateway connecting the Mediterranean Sea to the Atlantic Ocean in the Late Miocene. Its rapid narrowing at the Tortonian - Messinian transition around 7.2 Ma, resulting from very intense tectonic activity, has triggered an ecological crisis well before the deposition of the Messinian Salinity crisis evaporites.

The sedimentary successions deposited in the Saïs Basin have recorded different events regarding biostratigraphic, environmental, tectonic, and eustatic that characterized the area during the late Miocene. In order to get information on the marine and continental environment during the Tortonian-Messinian Transition (TMT), a palynological and biostratigraphic study was carried out on two boreholes in the Saïs Basin.

The biostratigraphic analyses based on the planktonic foraminifera of the boreholes studied reveals the succession of several biostratigraphic events, allowing us to attribute these sedimentary deposits to the late Tortonian - early Messinian time interval including the recognition of the T/M boundary.

The abundance of continental inputs (pollen, spores, BOM, WOM, and COM in the palynofacies) and the low D/S ratio values indicated that the Saïs basin was a neritic epicontinental environment suffering a significant influence of terrigenous inputs. The temperature index shows that the thermal conditions of the surface water were warm.

In the late Tortonian, faunal and floristic assemblages indicate an open, relatively deep, outer platform type marine environment with a slight tendency towards an inner platform context. At the Tortonian-Messinian boundary, there is an increase in land inputs and relative reduction in the diversity of both microfauna and microflora. The presence of cold-water taxa probably indicates moderate cooling. In Lower Messinian the marine environment, was external platform with tendencies towards an internal area.

The cover is opened and dominated by herbaceous plants that colonize the low altitudes, while trees colonized the middle altitudes. The climate was hot and humid in the mid-altitude and dry in the lowlands.

(U-Th)/He Dating of Supergene Iron (Oxyhydr-)Oxides of the Nefza-Sejnane District (Tunisia): New Insights into Mineralization and Mammalian Biostratigraphy

The mining district of Nefza-Sejnane (Tunisia) encloses numerous ores and raw material deposits, all formed in relation with successive Fe-rich fluids of meteoric and/or hydrothermal origins. Here, for the first time in Tunisia, (U-Th)/He ages were obtained on supergene goethite from various localities/deposits of the district highlight direct dating of significant weathering episodes during late Tortonian and late Pleistocene. These weathering events are most likely associated with favorable conditions that combine (i) wet climate displaying sufficient meteoric water/fluid; and (ii) regional exhumation, due to large-scale vertical lithospheric movements enhancing the percolation of fluids. Matched with previous works, these results refine the stratigraphic frame for the polymetallic mineralization and clay deposits in the district, confirming the influence of meteoric fluids circulation during the late Cenozoic. As a consequence of the new (U-Th)/He data, we moreover propose a taxonomic and stratigraphic revision of the well-known mammalian fauna from the Fe-rich Douahria locality, suggesting an early Tortonian age for the fossils, i.e., prior to the first episode of meteoric event in the area.