EGU21-15199
https://doi.org/10.5194/egusphere-egu21-15199
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Chemical-physical constraints of the 2015 eruptive activity of Mt. Etna: new insights from thermo-barometry and geochemistry of olivine-hosted melt inclusions

Pier Paolo Giacomoni1, Federico Casetta1, Virginia Valenti1, Carmelo Ferlito2, Gabriele Lanzafame2, and Manuela Nazzari3
Pier Paolo Giacomoni et al.
  • 1University of Ferrara, University of Ferrara, Deparment of Physiscs and Earth Sciences, Italy (gcmppl@unife.it) University of Ferrara, Deparment of Physiscs and Earth Sciences, Italy (gcmppl@unife.it)
  • 2University of Catania, Department of Biological, Environmental and Geological Sciences
  • 3Institute of Geophysics and Volcanology, INGV

The concomitant activation off all four summit craters of Mt. Etna during the December 2015 eruptive event allow us to investigate the chemical-physical crystallization conditions and magma dynamics in the shallower portion of the open-conduit feeding system. In this study, we discuss new petrological, geochemical and thermo-barometric data as well as the composition of major element and volatile content (H2O, CO2, F, Cl and S) of olivine-hosted melt inclusions from the explosive and effusive products emitted during the December 2015 eruptive event.

Results and rhyolite-MELTS thermodynamic modelling of mineral phase stability highlight the relatively shallow crystal equilibrium depth prior to the eruption ranging from 400-500 MPa for Central Crater and North East Crater, up to 200 MPa below the New South East Crater. The study of high-pressure and high-temperature homogenized olivine-hosted melt inclusions allowed us to identify the composition of the almost primary alkali-basalt magma (11.8 wt% MgO) containing up to 4.9 wt% and 8151 ppm of H2O and CO2 respectively. The results, together with those already reported for the previous paroxystic events of the 2011-2012 (Giacomoni et al., 2018), reinforce the model of a vertically extended feeding system and highlight that the activity at the New South East Crater was fed by a magma residing at significant shallower depth with respect to Central Craters and North East Crater, although all conduits are fed by a common deep (P = 530-440 MPa) basic magmatic refilling. Plagioclase stability model and dissolution and resorption textures confirm its dependence on H2O content, thus suggesting that further studies on the effect that flushing from fluids with different H2O/CO2 ratio are needed in order to understand the eruption triggering mechanisms of paroxystic fountaining.

 

References

Giacomoni P., Coltorti M., Mollo S., Ferlito C., Braiato M., Scarlato P. 2018. The 2011-2012 paroxysmal eruptions at Mt. Etna volcano: Insights on the vertically zoned plumbing system. JVGR 349, 370-391.

How to cite: Giacomoni, P. P., Casetta, F., Valenti, V., Ferlito, C., Lanzafame, G., and Nazzari, M.: Chemical-physical constraints of the 2015 eruptive activity of Mt. Etna: new insights from thermo-barometry and geochemistry of olivine-hosted melt inclusions, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-15199, https://doi.org/10.5194/egusphere-egu21-15199, 2021.