2003 Seattle Annual Meeting (November 2–5, 2003)
Paper No. 258-12
Presentation Time: 1:30 PM-5:30 PM

HYDROCARBON-DERIVED LIMESTONES INTERBEDDED WITH LOWER MESSINIAN EUXINIC SHALES (NORTHERN APENNINES, ITALY)

BORDOLOI, Sandip, Department of Geological Sciences, Univ of Alabama, 202, Bevill Building, Tuscaloosa, AL 35487, bordo001@bama.ua.edu, AHARON, Paul, Department of Geological Sciences, Univ of Alabama, Box 870338, Tuscaloosa, AL 35487, TAVIANI, Marco, ISMAR-Marine Geology Division, Consiglio Nazionale delle Ricerche, via Gobetti 101, Bologna, 40129, Italy, and VAI, Gian Battista, Dipartimento di Science Geologiche e Ambientali, Universita di Bologna, via Zamboni 67, Bologna, I-40127, Italy

A 10.3 m section of laminated, grey-dark, organic-rich pelites (euxinic shales) of Lower Messinian age in the Vena del Gesso basin (Monticino quarry at Brisighella, Northern Apennines of Italy) are cyclically interbedded with up to eleven layers of marls and limestones. Massive gypsum beds of the Gessoso-solfifera Formation, considered equivalent to the Lower Evaporites of Sicily and Spain, cap the marine Messinian section. The limestones consist of highly indurated light yellowish to grey beds, about 30 cm in thickness. Interbedded marls are fossiliferous and show a remarkable faunal change from bottom to top of section. Grey marls contain a diverse benthic fauna dominated by bivalves (e.g., Nuculana, Propeamussium, Cardiomya), gastropods (e.g., Aporrhais, Nassarius), decapods, echinoids and foraminifera. The abundant pelagic component includes foraminifera (e.g. Orbulina) and thecosomatous pteropods, together with necktic remains (fish otoliths). The uppermost dark euxinic shales are characterized by quasi-monospecific assemblages of chemosynthetic lucinid clams (?Myrtea). d18O values of the limestones change upsection by about 10.5 per mil (i.e., from -4 per mil PDB to +6.5 per mil PDB ) and indicate a shallowing-up of the basin under increasing evaporitic and stratified conditions. The association of abundant pyrite with fine micritic limestone that yields highly negative d13C values (down to -35 per mil PDB) suggests that the carbon in the limestones is derived from hydrocarbons through coupled BSR/AMO (bacterial sulfate reduction/anaerobic methane oxidation) processes.

The exact source of the carbon is open to debate. The possibility that the interbedded limestone layers contain imprints of gas hydrate dissociation events caused by rapid tectonic uplift that destabilized the deepwater gas hydrates is intriguing but cannot be fully answered at present. Ongoing studies of gas escape features, micro-brecciation, microbial textures and biomarkers in the limestone beds are aiming to resolve remaining ambiguities.

2003 Seattle Annual Meeting (November 2–5, 2003)
Session No. 258--Booth# 133
Gas Hydrate in the Natural Environment and Implications for Energy Resources, Seafloor Stability, Climate, and the Biology of the Deep Sea (Posters)
Washington State Convention and Trade Center: Hall 4-F
1:30 PM-5:30 PM, Wednesday, November 5, 2003

Geological Society of America Abstracts with Programs, Vol. 35, No. 6, September 2003, p. 620

© Copyright 2003 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.