Magmatic Storage and Volatile Fluxes of the 2021 La Palma Eruption

Author:

Dayton K.1ORCID,Gazel E.1ORCID,Wieser P. E.2ORCID,Troll V. R.345,Carracedo J. C.5,Aulinas M.67ORCID,Perez‐Torrado F. J.5

Affiliation:

1. Department of Earth and Atmospheric Sciences Cornell University Ithaca NY USA

2. Department of Earth and Planetary Sciences University of California Berkeley Berkeley CA USA

3. Department of Earth Sciences Section for Natural Resources and Sustainable Development Uppsala University Uppsala Sweden

4. Centre of Natural Hazards and Disaster Science (CNDS) Uppsala University Uppsala Sweden

5. Instituto de Estudios Ambientales y Recursos Naturales (i‐UNAT) University of Las Palmas de Gran Canaria (ULPGC) Las Palmasde Gran Canaria Spain

6. Department of Mineralogia, Petrologia, i Geologia Aplicada Facultat Ciències de la Terra Universitat de Barcelona Barcelona Spain

7. Geomodels Research Institute University of Barcelona Barcelona Spain

Abstract

AbstractThe 2021 La Palma eruption (Tajogaite) was unprecedented in magnitude, duration, and degree of monitoring compared to historical volcanism on La Palma. Here, we provide data on melt inclusions in samples from the beginning and end of the eruption to compare the utility of both melt and fluid inclusions as recorders of magma storage. We also investigated compositional heterogeneities within the magmatic plumbing system. We found two populations of olivine crystals: a low Mg# (78–82) population present at the beginning and end of eruption, recording the maximum volatile contents (2.5 wt % H2O, 1,800 ppm F, 700 ppm Cl, 3,800 ppm S) and a higher Mg# (83–86) population sampled toward the end of the eruption, with lower volatile contents. Despite their host composition, melt inclusions share the same maximum range of CO2 concentrations (1.2–1.4 wt %), indicating olivine growth and inclusion capture at similar depths. Overall, both melt and fluid inclusions record similar pressures (450–850 MPa, ∼15–30 km), and when hosted in the same olivine crystal pressures are indistinguishable within error. At these mantle pressures, CO2 is expected to be an exsolved phase explaining the similar range of CO2 between the two samples, but other volatile species (F, Cl, S) behave incompatibly, and thus, the increase between the two olivine populations can be explained by fractional crystallization prior to eruption. Finally, based on our new data, we provide estimates on the total volatile emission of the eruption.

Funder

National Science Foundation

Publisher

American Geophysical Union (AGU)

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