Journal
JOURNAL OF PETROLOGY
Volume 51, Issue 5, Pages 973-991Publisher
OXFORD UNIV PRESS
DOI: 10.1093/petrology/egq007
Keywords
partial melting; crustal xenolith; microstructure; THERMOCALC; wall-rock interaction; magma chamber
Categories
Funding
- Spanish Government (MEC)
- Earth Sciences Department of the Oxford University
- Department of Geology at Huelva University
- Department of Mineralogy and Petrology of the University of Padova
- European Commission [ERAS-CT-2003-980409]
- JAE [CSIC-2007]
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Crustal xenoliths from the Neogene Volcanic Province (NVP) of the Betic Cordillera, SE Spain, constitute an unusual suite of high-grade melt-bearing metapelitic rocks derived in two stages from metasediments surrounding crustal magma chambers. Microstructures and age relationships indicate that a first stage of migmatization and melt extraction was overprinted by a sequence of melt-bearing reaction microstructures. The preservation of melt as glass requires only a short residence time before eruption of the xenoliths in the host melt. The P-T conditions of the melting processes have been constrained by metamorphic modelling of mineral assemblages, phase compositions and reaction sequences in local compositional domains in the system NCKFMASHTO using THERMOCALC software. The calculations predict that within the El Hoyazo and Mazarron volcanic suites, Grt-Bt-Sil (+/- Crd, Pl) enclaves containing a distinctive fibrolite-melt intergrowth formed over the temperature range 700-770 degrees C at 5 kbar, and that these were overprinted by corona structures around garnet containing Spl-Crd-Kfs-melt at 775 degrees C, 4 center dot 8 kbar, and newly grown spinel with melt haloes (only at El Hoyazo) at 835 degrees C and 5 center dot 8 kbar. At Mar Menor, the xenoliths show garnet replaced by Opx, Crd, Spl and melt at 810-840 degrees C, 2-2 center dot 5 kbar; aluminous xenoliths containing andalusite were replaced by Spl + Crd under the same conditions. The P-T distribution, size and relative abundance of the various xenolith types are best explained by the formation of the melt-bearing assemblages in a transiently heated wall-rock profile adjacent to a magma chamber or conduit, followed by collapse of the wall and brief residence of the resulting fragments as xenoliths in a dacitic magma at c. 850 degrees C. The difference in pressure between the locations reflects the depth of magma chambers in the crust. The predominance of smaller, hotter enclaves in the Mar Menor occurrence may reflect less favourable conditions for developing thermally softened wall-rock profiles along high thermal gradients at shallower depth.
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