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Reactive thermodynamics of crustal eclogitization and foundering

delete2025-05-01
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M
Mitchell McMillan *
S
Shi J. Sim
C
C. R. Wilson
DOI:10.1016/j.epsl.2025.119302delete
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Abstract

Abstract

En 中文
Regional metamorphism and densification (eclogitization) of the lower crust can affect the lithospheric dynamics of mountain belts, but the coupled effects of reaction rate, temperature, and composition on metamorphism are poorly understood. We present a reactive thermodynamic model of the granulite-eclogite transition to investigate the long-term buoyancy and gravitational stability of the lower crust. First, we characterize the conditions for which orogenic crust attains negative buoyancy by determining its reactive mineral assemblage and density under prescribed pressure-temperature-time paths. Using existing metamorphic rate data, we calibrate a Damkohler number (a relative reaction rate) to parameterize the catalytic effect of aqueous fluids. The depth necessary for negative buoyancy is sensitive to temperature and Da, ranging from similar to 45 to 70 km for a basaltic-andesite composition (54 wt.% SiO2). Second, using a Rayleigh-Taylor instability analysis, we suggest that, while cold eclogitic crusts <850 C-degrees would be strong enough to resist foundering within 50 Myr, warm crusts >850 C-degrees could obtain large thicknesses of similar to 10 to 30 km and would founder within 50 Myr. We hypothesize that such foundering events are a natural consequence of convergent tectonics, where the aqueous fluids and high pressures required for metamorphism are known to exist. The Pampean flat slab in the Central Andes provides geophysical evidence linking slab fluids to eclogitization and densification of the thickened continental crust. Lithospheric foundering coupled to convergent tectonics through eclogitization could explain many observations of orogenic hinterland deformation and magmatism.
Keywords:
Eclogite
Granulite
Orogeny
Geodynamics
High pressure metamorphism
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Journal

Earth and Planetary Science Letters cover
Earth and Planetary Science Letters
IF:
5.1
Papers:
774
Citations:
6.9W

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C
carnegie sci
Scholars:
8
Papers: 6
Citations: 0
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