Abstract
Here, we characterize the temporal evolution of volatiles during the Tajogaite eruption by analyzing the elemental (He-Ar-CO2-N2) and isotopic (He-Ar-Ne) composition of fluid inclusions (FI) in phenocrysts (olivine+pyroxene) identified in erupted lavas. Our 2021 lava samples identify substantial temporal variations in volatile composition. We show that, during the 2021 Tajogaite eruption, the He-CO2-N2 concentrations in FI increased since October 15th; this increase was accompanied by increasing 40Ar/36Ar ratios (from ∼300 to >500), and paralleled a major shift in bulk lava chemistry, with increasing Mg contents (Mg#, from 47 to 52 to 55–59), CaO/Al2O3 (from 0.65 to 0.74 to 0.75–0.90), Ni and Cr, and decreasing TiO2, P2O5 and incompatible elements. The olivine core composition also became more forsteritic (from Mg# = 80–81 to Mg# = 84–86). Mineral thermobarometry and FI barometry results indicate that the eruption was sustained by magmas previously stored in at least two magma accumulation zones, at respectively ∼6–12 km and 15–30 km, corroborating previous seismic and FI evidence. We therefore propose that the compositional changes seen throughout the eruption can be explained by an increased contribution - since early/mid-October - of more primitive, less-degassed magma from the deeper (mantle) reservoir. Conversely, Rc/Ra values (3He/4He ratios corrected for atmospheric contamination) remained constant throughout the whole eruption at MORB-like values (7.38 ± 0.22 Ra, 1σ), suggesting an isotopically homogeneous magma feeding source. The Tajogaite He isotope signature is within the range of values observed for the 1677 San Antonio lavas (7.37 ± 0.17Ra, 1σ), but is more radiogenic than the 3He/4He values (>9 Rc/Ra) observed in the Caldera de Taburiente to the north. The 3He/4He ratios (6.75 ± 0.20 Ra, 1σ) measured in mantle xenoliths from the San Antonio volcano indicate a relatively radiogenic nature of the mantle beneath the Cumbre Vieja ridge. Based on these results and mixing modeling calculations, we propose that the homogeneous He isotopic signatures observed in volatiles from the Tajogaite/San Antonio lavas reflect three component mixing between a MORB-like source, a radiogenic component and small additions (6–15%) of a high 3He/4He reservoir-derived (>9Ra) fluid components. The simultaneous occurrence of high 3He/4He (>9Ra)- and MORB-like He signatures in northern and southern La Palma is interpreted to reflect small-scale heterogeneities in the local mantle, arising from spatially variable proportions of MORB, radiogenic, and high 3He/4He components.
| Originalsprache | Englisch |
|---|---|
| Aufsatznummer | 107928 |
| Fachzeitschrift | Journal of Volcanology and Geothermal Research |
| Jahrgang | 443 |
| DOIs | |
| Publikationsstatus | Veröffentlicht - Nov. 2023 |
Fördermittel
This research was funded by the Italian Minister (PRIN2017LMNLAW and 2022HA8XCS), by the Deep Carbon Observatory, by the Project MAGAT (Ref. CIRCNA/OCT/2016/2019), funded by the Fundação para a Ciência e Tecnologia (FCT), Portugal, by the RETURN Extended Partnership funded by the European Union Next-GenerationEU (National Recovery and Resilience Plan – NRRP, Mission 4, Component 2, Investment 1.3 – D.D. 1243 2/8/2022, PE0000005), by the National Biodiversity Future Center (National Recovery and Resilience Plan – NRRP, Mission 4, Component 2, Investment 1.4, CN00000033) and by the projects VOLRISKMAC II (MAC2/3.5b/328), co-financed by the EC Cooperation Transnational Program MAC 2014-2020, and “Cumbre Vieja Emergencia”, financed by the Spanish Ministry of Science and Innovation. AM-P acknowledges funding from FWF grant V659-N29. The Authors thank Dr. Joao Lages and Marcello Bitetto for helping with sample collection of the early lavas. We thank Ilka Wünsche for thin sections preparation and Franz Kiraly for support during EPMA analyses. We are grateful to Monika Horschinegg for Sr–Nd isotope analyses. We also thank Mariano Tantillo and Mariagrazia Misseri for helping in sample preparation and during the isotope analysis of noble gases performed in the noble gas laboratory of INGV-Palermo. We are also grateful to Federica Schiavi Laboratoire Magma et Volcans, Université Clermont Auvergne, France for providing Raman measurements. Finally, we thank Prof. James Day and Dr. Samantha Tramontano for their valuable comments which improved our manuscript. This research was funded by the Italian Minister ( PRIN2017LMNLAW and 2022HA8XCS ), by the Deep Carbon Observatory , by the Project MAGAT (Ref. CIRCNA/OCT/2016/2019 ), funded by the Fundação para a Ciência e Tecnologia (FCT), Portugal, by the RETURN Extended Partnership funded by the European Union Next-GenerationEU (National Recovery and Resilience Plan – NRRP, Mission 4, Component 2, Investment 1.3 – D.D. 1243 2/8/2022, PE0000005 ), by the National Biodiversity Future Center (National Recovery and Resilience Plan – NRRP, Mission 4, Component 2, Investment 1.4, CN00000033 ) and by the projects VOLRISKMAC II (MAC2/3.5b/328), co-financed by the EC Cooperation Transnational Program MAC 2014-2020, and “Cumbre Vieja Emergencia”, financed by the Spanish Ministry of Science and Innovation. AM-P acknowledges funding from FWF grant V659-N29 . The Authors thank Dr. Joao Lages and Marcello Bitetto for helping with sample collection of the early lavas. We thank Ilka Wünsche for thin sections preparation and Franz Kiraly for support during EPMA analyses. We are grateful to Monika Horschinegg for Sr Nd isotope analyses. We also thank Mariano Tantillo and Mariagrazia Misseri for helping in sample preparation and during the isotope analysis of noble gases performed in the noble gas laboratory of INGV-Palermo. We are also grateful to Federica Schiavi Laboratoire Magma et Volcans, Université Clermont Auvergne, France for providing Raman measurements.
ÖFOS 2012
- 105105 Geochemie
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