Eruptive history and petrologic evolution of the Albano multiple maar (Alban Hills, Central Italy) |
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Authors: | Carmela Freda Mario Gaeta Daniel B. Karner Fabrizio Marra Paul R. Renne Jacopo Taddeucci Piergiorgio Scarlato John N. Christensen Luigi Dallai |
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Affiliation: | (1) Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Sismologia e Tettonofisica, Via di Vigna Murata, 605-00143 Roma, Italy;(2) Dipartimento di Scienze della Terra, Università degli Studi “La Sapienza”, P. Aldo Moro, 5-00185 Roma, Italy;(3) Dept of Geology, Sonoma State University, 1801 East Cotati Ave., Rohnert Park, CA 94928, USA;(4) Berkeley Geochronology Center, 2455 Ridge Road, Berkeley, CA 94709, USA;(5) Dept of Earth and Planetary Science, University of California, Berkeley, CA 94720, USA;(6) Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 70A4418 Berkeley, CA 94720, USA;(7) CNR-Istituto di Geologia Ambientale e Geoingegneria, Via Bolognola, 7-00138 Rome, Italy |
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Abstract: | A comprehensive volcanological study of the Albano multiple maar (Alban Hills, Italy) using (i) 40Ar/39Ar geochronology of the most complete stratigraphic section and other proximal and distal outcrops and (ii) petrographic observations, phase analyses of major and trace elements, and Sr and O isotopic analyses of the pyroclastic deposits shows that volcanic activity at Albano was strongly discontinuous, with a first eruptive cycle at 69±1 ka producing at least two eruptions, and a second cycle with two peaks at 39±1 and 36±1 ka producing at least four eruptions. Contrary to previous studies, we did not find evidence of magmatic or hydromagmatic eruptions younger than 36±1 ka. The activity of Albano was fed by a new batch of primary magma compositionally different from that of the older activity of the Alban Hills; moreover, the REE and 87Sr/86Sr data indicate that the Albano magma originated from an enriched metasomatized mantle. According to the modeled liquid line of descent, this magma differentiated under the influence of magma/limestone wall rock interaction. Our detailed eruptive and petrologic reconstruction of the Albano Maar evolution substantiates the dormant state of the Alban Hills Volcanic District. Electronic Supplementary Material Supplementary material is available for this article at Editorial responsibility: J. Donnelly-Nolan An erratum to this article can be found at |
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Keywords: | Eruptive cycles Geochronology Alban Hills Maar Hydromagmatic Ultrapotassic Decarbonation |
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