T275 The Dance of Arcs: Causes of Arc Migrations, Flare-Ups, and Magmatic Focusing (Posters)
Tuesday, 24 October 2017
9:00 AM - 6:30 PM
Halls 4EF
PETROLOGY AND GEOCHEMISTRY OF ADAK ISLAND PLUTONIC XENOLITHS: IMPLICATIONS FOR CRUSTAL DIFFERENTIATION IN THE ALEUTIAN ISLAND ARC
Paper number: T275-17
Program: Technical Sessions
Time: 9:00 AM – 6:30 PM
Authors
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Claire E. BucholzCalifornia Institute of Technology, Pasadena, CA
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Suzanne KayCornell University, Ithaca, NY
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Robert W. KayCornell University, Ithaca, NY
Abstract
The expanded sample suite of Adagdak xenoliths comprise dunite, wehrlite, amphibole + olivine clinopyroxenite, amphibolite, & amphibole gabbro cumulates, similar to previously documented lithologies. Olivine Mg#s in dunites, wehrlites, & clinopyroxenites vary from 85-87, 84-86, & 86, respectively, corresponding to equilibrium melts with Mg#s of 63-68. Calculated equilibrium melt Mg#s from clinopyroxene compositions in the amphibolites & amphibole gabbros vary from 59-46. Dunites contain spinel as the sole oxide phase (Cr# 0.33-0.40) whereas, in the amphibole gabbros, titanomagnetite occurs as abundant (5-7 modal %), large (up to 500μm) crystals. Plagioclase first appears as an interstitial phase (8 modal %) in the wehrlites (An = 84-85%) and becomes a dominant phase (35-50 modal %) in the amphibole gabbros (An = 91-96%).
Thermobarometry & oxygenbarometry place dunite crystallization at 950-970oC (Li et. al., 1995), 0.79-0.95 GPa (Köhler & Brey, 1990), and +2.2-2.4 ΔQFM (Ballhaus, 1991), indicating lower crustal, relatively oxidizing conditions. Plagioclase-amphibole thermometry for the amphibole gabbros suggest formation at 940-1000oC (Holland & Blundy, 1994). These updated constraints on chemistry & conditions of crystallization are in agreement with the original interpretation of DeBari et al. (1987), amplified by Kay & Kay (1994), that the xenoliths represent crystallization products of near primary magmas at the base of the Aleutian Arc crust. Forthcoming data for the Mt. Moffett xenolith suite will be presented.
Geological Society of America Abstracts with Programs. Vol. 49, No. 6
doi: 10.1130/abs/2017AM-302537
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