EGU2020-1336
https://doi.org/10.5194/egusphere-egu2020-1336
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

A shallow mud volcano in the sedimentary basin off the Island of Elba

Alessandra Sciarra1, Anna Saroni2, Fausto Grassa3, Roberta Ivaldi4, Maurizio Demarte4, Christian Lott5,6, Miriam Weber5,6, Andi Eich6, Ettore Cimenti4, Francesco Mazzarini7, and Massimo Coltorti2
Alessandra Sciarra et al.
  • 1Istituto Nazionale di Geofisica e Vulcanologia, Rome 1, Rome, Italy (alessandra.sciarra@ingv.it)
  • 2Department of Physics and Earth Sciences, University of Ferrara, Italy.
  • 3Istituto Nazionale di Geofisica e Vulcanologia, Palermo, Italy
  • 4ISTITUTO IDROGRAFICO DELLA MARINA, Italy
  • 5HYDRA Field Station, Loc. Fetovaia, 57034, Campo nell’Elba, Italy
  • 6HYDRA Marine Sciences GmbH, Burgweg 4, 76547, Sinzheim, Germany
  • 7Istituto Nazionale di Geofisica e Vulcanologia, Pisa, Italy

The Island of Elba, located in the westernmost portion of the northern Cenozoic Apennine belt, is formed by metamorphic and non-metamorphic units derived from oceanic (i.e. Ligurian Domain) and continental (i.e. the Tuscan Domain) domains stacked toward NE during the Miocene.

Offshore, west of the Island of Elba, magnetic and gravimetric data suggest the occurrence of N-S trending ridges that, for the very high magnetic susceptibility, have been interpreted as serpentinites, associated with other ophiolitic rocks. Moving towards south in Tuscan domain, along N-S fault, there is clear evidence of off-shore gas seepage (mainly CH4), which can be related to recent extensional activity.

In this contest, a cold methane seep was discovered in the sedimentary basin off Elba Island, characterized by typical mud volcanoes conditions. Generally, mud volcanoes are the shallow expression of subsurface processes characterized by movements of large masses of sediments and fluids. A marine mud volcanoes is a window into different depth levels of the submerged geosphere where hydrogen sulfide, methane and other hydrocarbon-rich fluid seepage occurs caused by tectonic activity. Indeed, vertical migration of geogas, especially CH4 from the reservoir strata to the sea floor occurs along focused, permeable migration pathways, often created by faults and fractures.

The sampled gas chemistry is typical of mud volcanoes, with methane as the prevalent gas component (>95 vol%) and minor gases that include carbon dioxide, nitrogen and trace amounts of helium. The combined stable C and H isotope composition of CH413C and δ2H) highlights a thermogenic origin of fluids discharged from mud volcano, contrary to likely abiotic origin gas found in the Pomonte seep and linked to serpentinized ultramafic rock systems.

The samples collected on this mud volcano are extremely depleted in 3He and their 3He/4He ratios are typical for a geological setting in which radiogenic crustal helium is strongly predominant. On the contrary, the Pomonte ophiolitic gas seeps show a mantle-derived 3He-rich component estimated in the range between 10 and 15%.

Petrological data highlight the presence of siltites and marly mudstones characterized by different origin than those found on neighboring islets (shallow marine organogenic limestones); therefore, the possibility that the fragments of rock blocks, found in the mud volcano area, derive form erosional processes of the islet is discarded. The conical shapes highlighted by the multibeam echosounder are very similar to the typical backscatter signature of other mud volcanoes, thus confirming the possibilities of classify this site as mud volcano. Indeed, already during the scuba diving survey that allowed sampling gas and sediment, it was clearly observed and documented as a mud volcano.

How to cite: Sciarra, A., Saroni, A., Grassa, F., Ivaldi, R., Demarte, M., Lott, C., Weber, M., Eich, A., Cimenti, E., Mazzarini, F., and Coltorti, M.: A shallow mud volcano in the sedimentary basin off the Island of Elba, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-1336, https://doi.org/10.5194/egusphere-egu2020-1336, 2019

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