New insights from plumbing system below composite mafic volcanoes: Post-glacial volatile contents and magmatic fluids from Villarrica magmas
Author(s)
Department of Geology, Facultad de Ciencias Físicas y Matem´aticas, Universidad de Chile, 8370450 Santiago, Chile
Lamont-Doherty Earth Observatory, Columbia University, New York, USA
Institut des Sciences de la Terre d’Orl´eans (ISTO), CNRS UMR 7327, Universit´e d’Orl´eans, BRGM, 1A rue de la F´erollerie, 45071 Orl´eans, Cedex 2, France
Guillaume, Georgeais
Lamont-Doherty Earth Observatory, Columbia University, New York, USA
Centro de Geociencias, UNAM Campus Juriquilla Blvd. Juriquilla 3001, Quer´etaro 76230, Mexico
Ferrando, Simona
Department of Earth Sciences, University of Torino, Via Valperga Caluso 35, 10125, Torino, Italy
Language
English
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Issue/vol(year)
/488–489 (2024)
ISSN
0024-4937
Publisher
Elsevier
Pages (printed)
107786
Date Issued
September 4, 2024
Abstract
Villarrica volcano, in the southern Andes, is a composite mafic volcano whose persistent open-vent activity is
punctuated by frequent Strombolian/Hawaiian eruptions and, more rarely, by more energetic (sub-Plinian)
events. Here, we investigate the volatile composition of the parental melts that sustain this activity, and the
conditions of pre-eruptive magma storage, by characterizing the composition of olivine-hosted melt and fluid
inclusions. We concentrate on inclusions entrapped in minerals from pyroclastic materials erupted from both
Villarrica summit and from its flank Minor Eruptive Centers (MECs) post the 14.5–13.5 kyr caldera collapse event
that formed the Lic´an ignimbrite. Our micro-FTIR and SIMS measurements indicate that the Puc´on eruption
records the highest volatile contents, with 6.0 wt% H2O, >1500 ppm CO2, 1330 ppm S, 1556 ppm Cl, and 2055
ppm F. These volatile contents imply a volatile-saturated magma originating from a depth of 14.4 to 17 km below
Villarrica. Results for other flank eruptions highlight a similarly deep (17–21 km depth) source for basaltic CO2-
rich mafic magmas erupted at regional MECs (Los Nevados, Caburgua). Melt inclusion results also reveal that
deep rising mafic magma batches, when temporarily stored at 1–5 km depth, produce the more differentiated and
degassed magma batches that sustain the decadal-old persistent effusive-explosive eruptive activity at Villarrica.
Helium isotope ratios (3He/4He; Rc/Ra when corrected for atmosphere) measured in bulk noble gases from
olivines (Fo75–88) indicate that the parental magmatic fluid signature (Rc/Ra = 6.7–7.6; CO2/3He = 4.7–7.5E+08)
is only recorded during central paroxysmal sub-Plinian eruption, and that this primitive gas signal is diluted in
lateral MECs (Rc/Ra < 6.5; CO2/3He = 1.4 × 10+9–3.1E+10).
punctuated by frequent Strombolian/Hawaiian eruptions and, more rarely, by more energetic (sub-Plinian)
events. Here, we investigate the volatile composition of the parental melts that sustain this activity, and the
conditions of pre-eruptive magma storage, by characterizing the composition of olivine-hosted melt and fluid
inclusions. We concentrate on inclusions entrapped in minerals from pyroclastic materials erupted from both
Villarrica summit and from its flank Minor Eruptive Centers (MECs) post the 14.5–13.5 kyr caldera collapse event
that formed the Lic´an ignimbrite. Our micro-FTIR and SIMS measurements indicate that the Puc´on eruption
records the highest volatile contents, with 6.0 wt% H2O, >1500 ppm CO2, 1330 ppm S, 1556 ppm Cl, and 2055
ppm F. These volatile contents imply a volatile-saturated magma originating from a depth of 14.4 to 17 km below
Villarrica. Results for other flank eruptions highlight a similarly deep (17–21 km depth) source for basaltic CO2-
rich mafic magmas erupted at regional MECs (Los Nevados, Caburgua). Melt inclusion results also reveal that
deep rising mafic magma batches, when temporarily stored at 1–5 km depth, produce the more differentiated and
degassed magma batches that sustain the decadal-old persistent effusive-explosive eruptive activity at Villarrica.
Helium isotope ratios (3He/4He; Rc/Ra when corrected for atmosphere) measured in bulk noble gases from
olivines (Fo75–88) indicate that the parental magmatic fluid signature (Rc/Ra = 6.7–7.6; CO2/3He = 4.7–7.5E+08)
is only recorded during central paroxysmal sub-Plinian eruption, and that this primitive gas signal is diluted in
lateral MECs (Rc/Ra < 6.5; CO2/3He = 1.4 × 10+9–3.1E+10).
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