T176 Petrochronology: Advances and Applications to Petrogenesis and Tectonics (Posters)
Monday, 23 October 2017
9:00 AM - 6:30 PM
Halls 4EF
WHEN CRUST MEETS CHONDRULES; ZIRCON RESPONSE WITHIN A SMALL-SCALE IMPACTOR IN THE METEORITE NORTHWEST AFRICA 869
Paper number: T176-5
Program: Technical Sessions
Time: 9:00 AM – 6:30 PM
Authors
-
Desmond E. MoserUniversity of Western Ontario, London, ON
-
Kimberly TaitRoyal Ontario Museum, Toronto, ON
-
Ivan BarkerUniversity of Western Ontario, London, ON
Abstract
The zircon morphology, chemical zoning and orientation microstructure in the quartz gabbro impactor were analyzed at the Zircon and Accessory Phase Laboratory (ZAPLab) at the University of Western Ontario. This study utilized cathodoluminescence (CL), low kV backscatter electron (BSE) imaging and electron backscatter diffraction (EBSD) mapping.
Zircon grains within, and associated with, ilmenite are fractured and consist of crystalline domains exhibiting crystal plastic deformation as well as areas that appear to have been amorphized by shock. Some of these grains have randomly oriented granules around their edges suggesting local impact heating/recrystallization. A zircon in the breccia/melt rim partially shielded by ilmenite has even retained apparent igneous zonation. As seen in some eucrites (Roszjar et al. in press), zircon in or near SiO2-rich zones occur as aggregates of rounded concentrically CL-zoned regions suggesting a pre-impact, metamorphic origin. In this case, misorientations of up to 43° are seen between the regions. Zircon grains show the most significant impact modification near the edge of the impactor. In this region whole grains are replaced by granular (submicron) zircon. High pressure zircon polymorphs and the high temperature breakdown of zircon to baddeleyite+SiO2 have not been observed. The data provided in this study allow us to distinguish pre-impact zircons and shock recrystallized zircons from grains that might have grown in the melt rim. Coupled U-Pb dating and mineral chemistry will enable us to obtain a more accurate petrogenetic reconstruction of this primordial crust.
Geological Society of America Abstracts with Programs. Vol. 49, No. 6
doi: 10.1130/abs/2017AM-308066
© Copyright 2017 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.