Noble gas signatures of fluids at Santorini and Milos (Greece). - Université de Pau et des Pays de l'Adour Accéder directement au contenu
Poster De Conférence Année : 2023

Noble gas signatures of fluids at Santorini and Milos (Greece).

Résumé

The Cenozoic subduction of the African plate beneath Aegean continental microplate is responsible for the development of the Hellenic volcanic arc and back arc extension zone in the Aegean Sea (Greece). The study of the isotopic content of leaking gases in the volcanic arc enables to investigate magmatic and geodynamic processes. This study allows revealing the motion of the slab such as its tearing, as expected in the eastern part of the arc, as highlighted by the seismic tomography studies [1]. Thirty gas samples of fumaroles and bubbling springs from the Santorini and Milos volcanoes were collected and analyzed to determine the concentration of major species (CO2, N2, H2,CH4, etc.), as well as their isotopic ratio (δ13C-CO2, δ13C-CH4, δ15N-N2 and δD-H2). In addition, fifteen gas samples were analysed for noble gas concentrations (He, Ne, Ar, Kr and Xe) and their isotopic ratio (3He/4He, 20Ne/22Ne, 21Ne/22Ne, 38Ar/36Ar and 40Ar/36Ar). On both islands CO2 is the major non-atmospheric gas (>70%). In Santorini island CO2 (85-100%), CH4 (470-720ppm), and H2 (0.19-1.2%) concentrations and δ13C-CO2 values (+0.5 to +0.8‰) indicate volcanic stability since the 2011-2012 unrest [2]. The 3He/4He of gases from both Santorini and Milos islands range from 1.4 to 3.7 Ra and reflect a mixing between air and deep gas that is a mix of mantle and crust-derived Helium. One sample from Milos island might be indicative of a small amount of MORB-type mantle. The combination of CO2/3He ratio with the δ13C-CO2 (-10.7 to +0.8‰) suggests a mixing between mantle, crustal limestone, and superficial fluids. The δ15N-N2 values (-0.2 to +0.5‰) coupled with the N2/3He ratio require contributions from mantle and slab-derived sediments. Given the geological context, this mantle signature could be explained by the presence of a slab tear or a MORB-type mantle under Milos island. [1] Piromallo and Morelli (2003), J. Geophys. Res. 108, B2, 2065. [2] Tassi et al. (2013), Bull. Volcanol. 75, 4: 711.
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Dates et versions

hal-04424109 , version 1 (29-01-2024)

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Paternité

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  • HAL Id : hal-04424109 , version 1

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Alexis Bernard, Anne Battani, Jean-Paul Callot, Finlay M Stuart, Uğur Balci, et al.. Noble gas signatures of fluids at Santorini and Milos (Greece).. Goldschmidt 2023, Jul 2023, Lyon, France. ⟨hal-04424109⟩

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