Abstract
Various xenoliths have been found in lavas of the 1763 (“La Montagnola”), 2001, and 2002–03 eruptions at Mt. Etna whose petrographic evidence and mineral chemistry exclude a mantle origin and clearly point to a cognate nature. Consequently, cognate xenoliths might represent a proxy to infer the nature of the high-velocity body (HVB) imaged beneath the volcano by seismic tomography. Petrography allows us to group the cognate xenoliths as follows: i) gabbros with amphibole and amphibole-bearing mela-gabbros, ii) olivine-bearing leuco-gabbros, iii) leuco-gabbros with amphibole, and iv) Plg-rich leuco gabbros. Geobarometry estimates the crystallization pressure of the cognate xenoliths between 1.9 and 4.1 kbar. The bulk density of the cognate xenoliths varies from 2.6 to 3.0 g/cm3. P wave velocities (V P ), calculated in relation to xenolith density, range from 4.9 to 6.1 km/s. The integration of mineralogical, compositional, geobarometric data, and density-dependent V P with recent literature data on 3D V P seismic tomography enabled us to formulate the first hypothesis about the nature of the HVB which, in the depth range of 3–13 km b.s.l., is likely made of intrusive gabbroic rocks. These are believed to have formed at the “solidification front”, a marginal zone that encompasses a deep region (>5 km b.s.l.) of Mt. Etna’s plumbing system, within which magma crystallization takes place. The intrusive rocks were afterwards fragmented and transported as cognate xenoliths by the volatile-rich and fast-ascending magmas of the 1763 “La Montagnola”, 2001 and 2002–03 eruptions.
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Acknowledgments
This study was initiated thanks to G. Amendolia, geologist and volcanological guide, who collected many of the samples. We are also greatly indebted to V. Scribano for fruitful discussion and for having provided the sample XET. M. Viccaro and an anonymous reviewer greatly improved the clarity of this paper with helpful and thoughtful suggestions. We also wish to thank M.A. Clynne and two anonymous reviewers for their helpful comments on an early version of this manuscript. We are grateful to Graziella Barberi for the elaboration of the tomograms and to A. Cavallo for the assistance during EMPA measurements. Lucia Messina is thanked for rock powder preparations.
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Table A (supplementary material)
Selected amphibole (Mg-Hastingsite) analyses in cognate xenoliths of AMGB, AMMG and AMLG groups. Mineral formulae (apfu=atoms per formula unit) were calculated by normalizing the sum of tetrahedral (Si, Ti, Al) plus octahedral (Al, Ti, Cr, Fe, Mn, Mg) cations to 13 (Leake et al. 1997). (DOC 57 kb)
Table B (supplementary material)
Mean rhonite analyses (n=3 analyses) in amphibole breakdown coronas. (DOCX 14 kb)
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Corsaro, R.A., Rotolo, S.G., Cocina, O. et al. Cognate xenoliths in Mt. Etna lavas: witnesses of the high-velocity body beneath the volcano. Bull Volcanol 76, 772 (2014). https://doi.org/10.1007/s00445-013-0772-8
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DOI: https://doi.org/10.1007/s00445-013-0772-8