Abstract

Eclogites, metagabbros, and paragneisses from the Variscan Münchberg Massif record a complex succession of igneous, hydrothermal and metamorphic processes. The geodynamic setting related to the protolith formation and the impact of different types of fluid-rock interactions have been uncertain up to now. We use major and trace element chemistry as well as oxygen isotopes to disentangle the geochemical signatures related to the different stages of the rocks' history.In the Münchberg Massif, dark eclogites (kyanite-free; Fe-Ti-MORB signature) are distinguished from light eclogites (kyanite-bearing; higher Mg#, Al2O3, and Cr; lower incompatible element contents; positive Eu anomalies; MORB to arc basalt signature). The δ18O values for both types (+5.0 to +10.8‰) are equal to, or higher than those of MORB. Amphibolite facies metagabbros have a more enriched, almost OIB-like trace element signature and high δ18O values (+9.4 to +10.3‰).Good linear correlations between fluid-immobile elements throughout the eclogite types confirm their derivation from a common, N-MORB to E-MORB-like parental magma. We interpret the light eclogites as former plagioclase-rich cumulates and the dark eclogites as their complementary differentiates. This relationship is partly obscured by variable degrees of magma contamination by sediments, which also affected the metagabbros. However, the metagabbros originated from a more enriched mantle source than the eclogites. Following intrusion, the eclogites were subjected to hydrothermal alteration under the influence of seawater, as indicated by positive correlations between Li, B, Sb, and δ18O. Metamorphic fluid-rock interactions appear to be mostly of limited extent, probably due to the lack of lawsonite dehydration as a fluid source. Nevertheless, the contents at least of some fluid-mobile elements, such as LILE, Li, and Pb, were probably modified during the subduction-exhumation cycle of the eclogites.The crustal contamination of the protolith magmas argues against derivation of the eclogites and metagabbros from typical oceanic crust. Instead, a rift-drift transition setting related to the opening of the Rheic or Saxothuringian Ocean seems most likely. The eclogites and metagabbros, alongside with similar rocks in the Mariánské Lázně complex and other resembling high-pressure massifs, may record different stages of this rift-drift transition.

Highlights

  • Eclogite facies massifs are the only parts of the accessible Earth that directly sample rocks from ancient subduction zones at depths >60 km

  • This study presents a large dataset of major and trace elements, and oxygen isotope compositions, for eclogites, meta­ gabbros and paragneisses sampled throughout the Münchberg Massif

  • Dark eclogites Major and trace element compositions of the dark eclogites are in the usual range of mafic rocks, generally subalkaline and mostly tholeiitic (Fig. S1)

Read more

Summary

Introduction

Eclogite facies massifs are the only parts of the accessible Earth that directly sample rocks from ancient subduction zones at depths >60 km. Geochemical data of metabasic rocks provide a wealth of information about subduction- and exhumation-related processes, and about the mantle source, tectonic setting, and igneous and hydrothermal processes that shaped the protolith (e.g., Cann, 1970; Jochum and Verma, 1996; Spandler et al, 2004; Pearce, 2014). 400 ◦C) whereas high-temperature alteration causes the opposite (Gregory and Taylor Jr, 1981) Both oxygen isotopes and fluid-mobile trace elements are commonly metasomatized during later subduction-related fluid-rock interactions, and by retro­ gression during exhumation, requiring careful interpretation (e.g., Miller and Cartwright, 2000; Spandler et al, 2004; Bebout, 2007)

Methods
Results
Discussion
Conclusion
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call