17 Ultramafic and Mafic Magmatism
Tuesday, 20 April 2021
8:00 AM - 12:00 PM
Missouri State University- Geography and Geology MS Program Room
VARIATION IN OLIVINE TRACE ELEMENT CONTENTS REVEAL THE SIGNATURE OF DEEP MANTLE MELTING DURING THE ERUPTION OF THE MCCARTYS FLOW, ZUNI-BANDERA VOLCANIC FIELD, NEW MEXICO
Paper number: 17-13
Program: Theme Sessions
Time: 11:00 AM – 11:10 AM
Authors
-
Gary MichelfelderMissouri State University, Springfield, MO
-
Clayton ReinierMissouri State University, Springfield, MO
-
L. Kenneth HorkleyUniversity of Iowa, Iowa City, IA
Abstract
Here, we present electron microprobe olivine mineral chemistry from the 3200-year-old McCartys flow, the youngest tholeiite basalt in the volcanic field. Olivine displays three populations with unique textures and/or major and minor element compositions. Type 1 crystals are euhedral, and contain cores with Fo72-86, moderate CaO (0.23-0.31 wt%) and Ni (380-2150 ppm) contents. Crystals contain a rim with lower forsterite, Ni and CaO content. Crystals contain only a single rim with lower forsterite contents. Type 2 crystals are anhedral to skeletal with identifiable cores, mantles and rims. Cores range in forsterite from Fo67-82, and Ni from 740-3220 ppm. Mantles and rims are more variable ranging from Fo31-80. In each crystal, there is a general decrease in forsterite and Ni from core to rim. Type 3 olivine are euhedral. Forsterite (Fo73-90) and Ni (860-3760 ppm) contents vary widely between crystals but lack variation within a single grain. A poorly developed plumbing system can be inferred by three unique olivine populations, suggesting they were in contact with different local magma bodies, with unique chemical environments. Long residence times can be inferred by the extensive time required for olivine to re-equilibrate in the three different chemical environments. Three different zoned olivine populations, if from the same source, must have been stored in magma bodies influenced by magma mixing to be able to develop different local chemical environments.
Geological Society of America Abstracts with Programs. Vol. 53, No. 3
doi: 10.1130/abs/2021NC-362759
© Copyright 2021 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.