V038-0002
Consequences of CO2-magma interaction for explosive volcanism at Colli Albani (Italy)

Wednesday, 16 December 2020
Poster
Corin Jorgenson, University of Geneva, Geneva, Switzerland, Luca Caricchi, University of Geneve, Earth Sciences, Geneve, Switzerland, Anne-Sophie Bouvier, University of Lausanne, Lausanne, Switzerland, Guido Giordano, Università Roma Tre, Science, Rome, Italy, Gregor Weber, University of Oxford, Oxford, United Kingdom and Felix Marxer, ETH Swiss Federal Institute of Technology Zurich, Department of Earth Sciences, Zurich, Switzerland
Abstract:
Colli Albani is a mafic-alkaline volcanic complex that repeatedly produced large caldera forming eruption of up to 63 km3 (DRE). The volcano is located just 30 km from the densely populated city of Rome. Mafic and alkaline magmas are rarely associated with such large volume explosive events. The cause of this unusual explosivity is thought to be related to the addition of CO2 resulting from the interaction with carbonates. However, whether the CO2 is supplied by shallow crustal carbonates or by carbonatic material at the top of the subducted Adriatic plate remains controversial. We measured the volatile content of melt inclusions hosted in clinopyroxene and find that several contain >2 wt. % CO2 with values as high as to 3.5 wt. % CO2 and 3.9 wt. % H2O. CO2 solubility studies indicate that such values are not compatible with shallow magma storage. Additionally, clinopyroxene phenocrysts have high magnesium number (up to 0.93) and Cr2O3 content, which suggest equilibrium with the mantle. We performed thermo-barometry of the clinopyroxene phenocrysts using a random forest machine learning approach and found pressures and temperatures of up to 16 kbar and 1250 °C. Such high pressure and temperature clinopyroxenes are particularly abundant at the base of the ignimbrite outcrop. We suggest that mafic and CO2-rich magma rapidly ascends from the mantle, destabilizing a shallow crustal magma reservoir and triggering an eruption. Magma in the shallow crust surely interacts with the host carbonates, however, we suggest that the high explosivity of this system is better explained by the addition of large amounts of CO2 to the magma in the mantle, which allow for its fast ascent through the lithosphere.