Retrograde mineral and fluid evolution in high-pressure metapelites (Schistes lustres unit, Western Alps)

Citation
P. Agard et al., Retrograde mineral and fluid evolution in high-pressure metapelites (Schistes lustres unit, Western Alps), CONTR MIN P, 140(3), 2000, pp. 296-315
Citations number
99
Categorie Soggetti
Earth Sciences
Journal title
CONTRIBUTIONS TO MINERALOGY AND PETROLOGY
ISSN journal
00107999 → ACNP
Volume
140
Issue
3
Year of publication
2000
Pages
296 - 315
Database
ISI
SICI code
0010-7999(200012)140:3<296:RMAFEI>2.0.ZU;2-C
Abstract
Fluid inclusions have been analysed in successive generations of syn-metamo rphic segregations within low-grade, high-pressure, low-temperature (HP-LT) metapelites from the Western Alps. Fluid composition was then compared to mass transfer deduced from outcrop-scale retrograde mineral reactions. Two types of quartz segregations (veins) occur in the 'Schistes lustres' unit: early blueschist-facies carpholite-bearing veins (BS) and retrograde greens chist-facies chlorite-bearing veins (GS). Fluid inclusions in both types of segregations are aqueous (no trace of dissolved gases such as CO2, CH4, N- 2), with significant differences in density and composition (salinity). BS fluids are moderately saline fluids (average 9.1 wt% eq. NaCl) characterize d by a chronological trend towards more dilute composition (from 15 down to 0 wt% eq. NaCl), whereas GS fluids have a very constant salinity of simila r to3.7 wt% eq. NaCl. Both types of inclusions were continuously reset to l ower densities along the retrograde path, until a temperature of similar to 300 degreesC. Mass-balance calculations, together with fluid inclusion dat a, suggest that GS fluids result from the mixing between two fluid sources: one initial,: early metamorphic, moderately saline HF fluid and a second n early pure water fluid provided by the breakdown of carpholite. Estimates o f the amount of water released by carpholite breakdown result in a dilution of the interstitial fluid phase (from 10 to 2.5-4 wt% eq. NaCl) consistent with the actual shift of the fluid composition. Alkali elements required f or the formation of the GS chlorite + phengite assemblage after carpholite could be locally provided by HP phengite. This is taken as an indirect evid ence that, during the generation of both BS and GS fluids, mixing with exte rnally derived fluids may have been very limited. The location, amount and constant composition of the less saline GS fluids appear to be related to a n interconnected porosity at the time of inclusion formation.