
The environmental settings during the deposition of hypogene-sourced terrestrial carbonates of the middle Pleistocene in Vedi, Ararat Basin
Shlomy Vainer(1), Alex Brittingham(2), Theodoros Karampaglidis(3), Boris Gasparyan(4), Yael Kiro(5), Yonaton Goldsmith(6), and Ariel Malinsky-Buller(2)
(1) Department of Earth and Environmental Sciences, Ben Gurion University of the Negev, Beer Sheva 84105
(4) Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 7610001, Israel
(5) Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 7610001, Israel
(6)Institute of Earth Science, The Hebrew University of Jerusalem, Jerusalem, Israel
Characterizing the genesis of terrestrial carbonates is fundamental for deciphering their role as archives of tectonic, climatic, and hydrochemical processes. However, differentiating between cold/warm, hypogene/epigean, and biotic/abiotic processes is not straightforward. Here, we study ~30 m thick carbonate deposits in Vedi Valley, the Ararat Basin, Armenia, formed in a tectonically active fault-controlled spring system. The study investigates their genesis and environmental context by applying geological mapping, petrographic, isotopic, geochemical, and U-series dating methods to unravel the depositional and diagenetic history of these deposits.
Two distinct facies are identified: (1) microbial carbonate facies associated with low-temperature palustrine settings, characterized by micritic and peloidal biotic textures, and (2) sparitic calcite facies linked to CO₂ degassing from saturated hypogene solutions, filling fractures. δ¹³CVPDB values range from +7.5‰ to +10‰ and δ¹⁸OVPDB values range between -9.6‰ and -11.6‰, indicating deeply sourced fluids. Sr and Ba concentrations suggest the interaction with buried marine carbonates, most likely those comprising the Erakh Anticline.
Co-variations in the isotopic ratios alongside Mg, Ca, and Sr concentrations point to a pristine closed degassing system at earlier stages and the incorporation of meteoric influx above 19 m depth. This upper part also shows three phases of enhanced detrital accumulation during increased runoff, possibly related to interglacials. The established chronological framework through U-Th constrains the deposition to between 319 ± 84 ka and 198 ± 14 ka, corresponding to MIS 9–7. This period coincided with profound global and regional environmental shifts triggered by changes in climate and tectonic activity. This chronostratigraphy highlights the potential of fault-controlled spring deposits, such as those in Vedi, as regional paleoenvironmental archive.