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From the Middle Triassic Cima Pape complex (Dolomites; Southern Alps) to the feeding systems beneath active volcanoes: Clues from clinopyroxene textural and compositional zoning
Language
English
Obiettivo Specifico
2V. Struttura e sistema di alimentazione dei vulcani
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Title of the book
Issue/vol(year)
/422 (2022)
ISSN
0377-0273
Publisher
Elsevier
Pages (printed)
107459
Issued date
2022
Abstract
Crystal zoning plays a fundamental role in modern volcanology as a key to unravel the geometry and the dynamics
of plumbing systems. In this study, a detailed textural and compositional study of clinopyroxene crystals
entrained in intrusive, hypabyssal and effusive products from Cima Pape (Dolomites) is coupled with
thermobarometric-hygrometricmodels to reconstruct the geometry and evolution of the feeding systembeneath
Middle Triassic volcanic edifices. Whole-rock major, trace element distribution and Sr-Nd isotopic signature
(87Sr/86Sri = 0.7045–0.7050; 143Nd/144Ndi = 0.51223–0.51228) show that the rocks from Cima Pape are SiO2-
saturated and have shoshonitic affinity, and likely belong to the acme of the Mid-Triassic magmatismthat shaped
the Southern Alps between 239 and 237.6Ma. Highly porphyritic trachybasaltic to basaltic trachyandesitic volcanic
rocks contain a large number of concentric-zoned clinopyroxene crystals. Here, high-Mg# and -Cr2O3, REEdepleted
bands (Mg# 80–91; Cr2O3 up to 1.2 wt%) with variable thickness grew between relatively low-Mg# and
-Cr2O3 (Mg# 70–77; Cr2O3 < 0.1 wt%) augitic cores and rims. In contrast, the gabbroic to monzodioritic 50- to
300-m-thick sill cropping out belowthe volcanic sequences, though to represent a relic of the shallowest portion
of the plumbing system, is mostly made up of unzoned clinopyroxene crystals.
Thermobarometric and hygrometric models allowed us to define that a small “mush-type” batchwas located beneath
the Cima Pape volcano at depths between 7 and 14 km. Here, augitic clinopyroxene formed in equilibrium
with a slightly evolved (basaltic trachyandesitic), H2O-rich melt (Mg# = 43–45; T = 1035–1075 °C; H2O =
2.6–3.8 wt%). Periodic replenishments of the magma batch by primitive (Mg# = 65–70), hotter and relatively
H2O-poor (T = 1130–1150 °C; H2O = 2.1–2.8 wt%) basaltic magmas led to the formation of diopsidic bands
mantling the already formed augitic cores. Later on, re-equilibration of clinopyroxene with the mixed melt resulted
in the formation of low-Mg#, LILE- and LREE-enriched rims. The most Mg-poor micro-phenocrystic
clinopyroxene in the volcanic rocks and in the sill records the ultimate and shallowest conditions of crystallization,
occurring at T of 975–1010 °C and P comprised between 50 and 150 MPa. Based on the presence of similar
zoning in clinopyroxene phenocrysts, a comparison between the Mid-Triassic Cima Pape and active volcanoes
was put forward to highlight the potential of studying ancient, entirely exposed volcanic systems for interpreting
the feeding systemprocesses acting beneath active volcanoes. At a regional scale, this approach represents a new,
powerful tool for investigating the evolution of the Mid-Triassic magmatism in the Southern Alps and shedding
light on the interactions between mantle-derived melts and differentiated batches ponding in the crust.
of plumbing systems. In this study, a detailed textural and compositional study of clinopyroxene crystals
entrained in intrusive, hypabyssal and effusive products from Cima Pape (Dolomites) is coupled with
thermobarometric-hygrometricmodels to reconstruct the geometry and evolution of the feeding systembeneath
Middle Triassic volcanic edifices. Whole-rock major, trace element distribution and Sr-Nd isotopic signature
(87Sr/86Sri = 0.7045–0.7050; 143Nd/144Ndi = 0.51223–0.51228) show that the rocks from Cima Pape are SiO2-
saturated and have shoshonitic affinity, and likely belong to the acme of the Mid-Triassic magmatismthat shaped
the Southern Alps between 239 and 237.6Ma. Highly porphyritic trachybasaltic to basaltic trachyandesitic volcanic
rocks contain a large number of concentric-zoned clinopyroxene crystals. Here, high-Mg# and -Cr2O3, REEdepleted
bands (Mg# 80–91; Cr2O3 up to 1.2 wt%) with variable thickness grew between relatively low-Mg# and
-Cr2O3 (Mg# 70–77; Cr2O3 < 0.1 wt%) augitic cores and rims. In contrast, the gabbroic to monzodioritic 50- to
300-m-thick sill cropping out belowthe volcanic sequences, though to represent a relic of the shallowest portion
of the plumbing system, is mostly made up of unzoned clinopyroxene crystals.
Thermobarometric and hygrometric models allowed us to define that a small “mush-type” batchwas located beneath
the Cima Pape volcano at depths between 7 and 14 km. Here, augitic clinopyroxene formed in equilibrium
with a slightly evolved (basaltic trachyandesitic), H2O-rich melt (Mg# = 43–45; T = 1035–1075 °C; H2O =
2.6–3.8 wt%). Periodic replenishments of the magma batch by primitive (Mg# = 65–70), hotter and relatively
H2O-poor (T = 1130–1150 °C; H2O = 2.1–2.8 wt%) basaltic magmas led to the formation of diopsidic bands
mantling the already formed augitic cores. Later on, re-equilibration of clinopyroxene with the mixed melt resulted
in the formation of low-Mg#, LILE- and LREE-enriched rims. The most Mg-poor micro-phenocrystic
clinopyroxene in the volcanic rocks and in the sill records the ultimate and shallowest conditions of crystallization,
occurring at T of 975–1010 °C and P comprised between 50 and 150 MPa. Based on the presence of similar
zoning in clinopyroxene phenocrysts, a comparison between the Mid-Triassic Cima Pape and active volcanoes
was put forward to highlight the potential of studying ancient, entirely exposed volcanic systems for interpreting
the feeding systemprocesses acting beneath active volcanoes. At a regional scale, this approach represents a new,
powerful tool for investigating the evolution of the Mid-Triassic magmatism in the Southern Alps and shedding
light on the interactions between mantle-derived melts and differentiated batches ponding in the crust.
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