Dating polygenetic metamorphic assemblages along atransect across thewestern alps
Journal of Petrology, ISSN: 1460-2415, Vol: 55, Issue: 4, Page: 803-830
2014
- 80Citations
- 49Captures
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Article Description
Multichronometric analyses were performed on samples from a transect in the French-Italian Western Alps crossing nappes derived from the Briançonnais terrane and the Piemonte-Liguria Ocean, in an endeavour to date both high-pressure (HP) metamorphism and retrogression history.Twelve samples of white mica were analysed by Ar-Ar stepwise heating, complemented by two samples from the Monte Rosa nappe 100 km to the NE and also attributed to the Briançonnais terrane. One Sm-Nd and three Lu-Hf garnet ages from eclogites were also obtained.White mica ages decrease from c. 300Ma in the westernmost samples (Zone Houillère), reaching c. 300°C during Alpine metamorphism, to< 48Ma in the internal units to the east, which reached c. 500°C during the Alpine orogeny. The spatial pattern of Eocene K-Ar ages demonstrates that Si-rich HP white mica records the age of crystallization at 47-48Ma and retains Ar at temperatures of around 500°C. Paleocene-early Eocene Lu-Hf and Sm-Nd ages, recording prograde garnet growth before the HP peak, confirm eclogitization in Eocene times. Petrological and microstructural features reveal important mineralogical differences along the transect. All samples contain mixtures of detrital, syn-D and syn-D mica, and retrogression phases (D) in greatly varying proportions according to local variations in the evolution of pressure-temperature-fluid activity-deformation (P-T-a-D) conditions. Samples from the Zone Houillère mostly contain detrital mica.The abundance of white mica with Si>6̇45 atoms per formula unit increases eastward. Across the whole traverse, phengitic mica grown during HP metamorphism defines the D foliation. Syn-D mica is more Si-poor and associated with nappe stacking, exhumation, and hydrous retrogression under greenschist-facies conditions. Syn-D phengite is very often corroded, overgrown by, or intergrown with, syn-D muscovite. Most importantly, syn-D recrystallization is not limited to S schistosity domains; micrometrescale chemical fingerprinting reveals muscovite pseudomorphs after phengite crystals, which could be mistaken for syn-D mica based on microstructural arguments alone.The Cl/K ratio in white mica is a useful discriminator, as D retrogression was associated with a less saline fluid than eclogitization. As petrology exerts the main control on the isotope record, constraining the petrological and microstructural framework is necessary to correctly interpret the geochronological data, described in both the present study and the literature. Our approach, which ties geochronology to detailed geochemical, petrological and microstructural investigations, identifies 47-48Ma as the age of HP formation of syn-D mica along the studied transect and in the Monte Rosa area. Cretaceous apparent mica ages, which were proposed to date eclogitization by earlier studies based on conventional 'thermochronology', are due to Ar inheritance in incompletely recrystallized detrital mica grains. The inferred age of the probably locally diachronous, greenschist-facies, low-Si, syn-D mica ranges from 39 to 43Ma. Coexistence of D and D ages, and the constancy of non-reset D ages along the entire transect, provides strong evidence that the D white mica ages closely approximate formation ages. Volume diffusion of Ar in white mica (activation energy E=250 kJ mol; pressure-adjusted diffusion coefficient D'<0̇03 cm s) has a subordinate effect on mineral ages compared with both prograde and retrograde recrystallization in most samples. © The Author 2014. Published by Oxford University Press. All rights reserved.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84896120225&origin=inward; http://dx.doi.org/10.1093/petrology/egu007; https://academic.oup.com/petrology/article-lookup/doi/10.1093/petrology/egu007; http://academic.oup.com/petrology/article-pdf/55/4/803/16676100/egu007.pdf; https://dx.doi.org/10.1093/petrology/egu007; https://academic.oup.com/petrology/article/55/4/803/1398076
Oxford University Press (OUP)
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