Hydrocarbon-bearing fluid migration produces brecciation at high pressure condition in subduction
- 1University of Bologna, Department of Biological, Geological and Environmental Sciences, Bologna, Italy (francesco.giuntoli@unibo.it)
- 2The Njord Centre, Department of Geosciences, University of Oslo, P.O. Box 1048 Blindern, Norway
- 3Department of basic and applied sciences for engineering (SBAI), Università degli Studi di Roma La Sapienza
- 4Univ. Lille, CNRS, INRAE, Centrale Lille, UMR 8207, UMET, Unité Matériaux et Transformations, F-59000 Lille, France
- 5Dipartimento di Scienze della Terra, Università degli Studi di Torino, via Valperga Caluso 35, 10100 Torino, Italy
- 6Sorbonne Université, Muséum National d’Histoire Naturelle, UMR CNRS 7590, IRD, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, IMPMC, 75005 Paris, France
- 7Institute of Geosciences and Earth Resources, National Research Council of Italy, Pisa, Italy
It has been recently proposed that high-pressure genesis of abiotic hydrocarbon can lead to strain localization in subducted carbonate rocks1. However, the mechanical effects of the migration of these hydrocarbon-bearing fluids on the infiltrated rocks still need to be constrained.
In this study, we investigate omphacitite (i.e. omphacite-rich rock) adjacent to a high-pressure methane-rich fluid source from the Western Italian Alps (Italy) using a multiscale and analytical approach including petrographic, microstructural, X-ray compositional mapping and electron backscatter diffraction analyses (EBSD). In the field, omphacitite bands are 1-5 metres thick and tens of metres long and are adjacent to carbonate rocks affected by high-pressure reduction and methane-rich fluid production.
Hand specimens and thin sections display a brecciated structure, with omphacitite fragments ranging in size from a few microns to several centimetres, surrounded by a matrix of jadeite, omphacite, grossular, titanite, and graphite. X-ray compositional maps and cathodoluminescence images highlight oscillatory zoning and skeletal textures in jadeite, omphacite and garnet in the matrix, suggesting a fast matrix precipitation under plausible disequilibrium conditions. CH4 and H2 are found in fluid inclusions in the jadeite grains. This feature suggests a potential link between the genesis of CH4 in the adjacent carbonate rocks and the brecciation event.
EBSD analysis was performed on omphacitite clasts close to their borders, where omphacite grain size varies between a few microns and a maximum of 100 microns. Those omphacite grains display no crystallographic preferred orientation, abundant low angle boundaries and low (< 5°) internal lattice distortion. We interpret these textures as formed by pervasive and diffuse micro-fracturing related to the brecciation occurring at high pore fluid pressure, reaching sub-lithostatic values. This study suggests that at high-pressure conditions in subduction zones, the genesis and migration of hydrocarbon-bearing fluids can trigger fracturing in adjacent lithotypes.
1 Giuntoli, F., Vitale Brovarone, A., Menegon, L., 2020. Feedback between high-pressure genesis of abiotic methane and strain localization in subducted carbonate rocks. Sci. Rep. 10, 9848. https://doi.org/10.1038/s41598-020-66640-3
This work is part of project that has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Grant agreement No. 864045).
How to cite: Giuntoli, F., Menegon, L., Siron, G., Cognigni, F., Leroux, H., Compagnoni, R., Rossi, M., and Vitale Brovarone, A.: Hydrocarbon-bearing fluid migration produces brecciation at high pressure condition in subduction, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-7017, https://doi.org/10.5194/egusphere-egu23-7017, 2023.
