Hornblende- and Phlogopite-Bearing Gabbroic Xenoliths from Volcan San Pedro (36{degrees}S), Chilean Andes: Evidence for Melt and Fluid Migration and Reactions in Subduction-Related Plutons

Two groups of gabbroic xenoliths (I and II) containing largeproportions of late-crystallized hornblende (up to 50 vol. %)and Na-rich phlogopite (up to 15 vol. %), were brought to thesurface by a late Holocene eruption of Volcán San Pedro,the youngest edifice of the Tatara–San Pedro VolcanicComplex (36°S, Chilean Andes). Group I are inferred to befragments of partially solidified Holocene plutons because theycontain residual interstitial glass, whereas exsolution anddeformation textures in Group II indicate that they are fragmentsof pre-Quaternary plutonic basement. On the basis of texturalrelations plus the mineral and whole-rock compositions of bothgroups of xenoliths, we suggest that hornblende and phlogopitewith high mg-numbers and Cr contents have formed by reactionsbetween refractory cumulus minerals (olivine, Cr-spinel, pyroxenesor plagioclase) and evolved melts ± aqueous fluids thatmigrated through partly solidified crystalline frameworks. Thus,the hydrous minerals are not early-crystallized phases in thebasaltic magmas from which the cumulus minerals precipitated.The high proportions of hornblende in many subduction-relatedgabbroic plutons and xenolith suites compared with its paucityin basaltic or basaltic andesitic lavas may be partially explainedby multistage plutonic crystallization histories involving reactionand migration of evolved melt ± aqueous fluids that eithercould have originated within the cumulus pile of the mafic intrusionor were derived externally, from broadly contemporaneous felsicmagmas. KEY WORDS: Tatara–San Pedro; gabbroic xenolith; hornblende; phlogopite; melt migration