Origins and energetics of maar volcanoes: examples from the ultrapotassic Sabatini Volcanic District (Roman Province,Central Italy) |
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| Authors: | Gianluca Sottili Danilo M Palladino Mario Gaeta Matteo Masotta |
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| Institution: | 1.Dipartimento di Scienze della Terra,Sapienza-Università di Roma,Rome,Italy;2.Istituto di Geologia Ambientale e Geoingegneria-CNR,Rome,Italy |
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| Abstract: | Maar volcanoes represent a common volcano type which is produced by the explosive interaction of magma with external water.
Here, we provide information on a number of maars in the ultrapotassic Sabatini Volcanic District (SVD, Roman Province) as
young as ∼90 ka. The SVD maars are characterised in terms of crater and ejecta ring morphologies, eruptive successions and
magma compositions, in light of the local substrate settings, with the aim of assessing magma–water interaction conditions,
eruption energetics and genetic mechanisms. Feeder magmas spanned the whole SVD differentiation trend from trachybasalts–shoshonites
to phonolites. From the ejected lithic fragments from aquifer rocks, the range of depth of magma–water explosive interaction
is estimated to have been mostly at ∼400–600 m below ground level, with a single occurrence of surficial interaction in palustrine–lacustrine
environment. In particular, the interaction with external water may have triggered the explosive behaviour of poorly differentiated
magmas, whereas it may have acted only as a late controlling factor of the degree of fragmentation and eruption style for
the most differentiated magma batches during low-flux ascent in an incipiently fragmented state. Crater sizes, ejecta volumes
and ballistic data allow a reconstruction of the energy budget of SVD maar-forming eruptions. Erupted tephra volumes from
either monogenetic or polygenetic maars ranged 0.004–0.07 km3 during individual maar-forming eruptions, with corresponding total magma thermal energies of 8 × 1015–4 × 1017 J. Based on energy partitioning and volume balance of erupted magmas and lithic fractions vs. crater holes, we consider the
different contributions of explosive excavation of the substrate vs. subsidence in forming the SVD maar craters. Following
available models based on crater sizes, highly variable fractions (5–50%) of the magma thermal energies would have been required
for crater excavation. It appears that subsidence may have played a major role in some SVD maars characterised by low lithic
contents, whilst substrate excavation became increasingly significant with increasing degrees of aquifer fragmentation. |
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