36 Implications of Lithosphere-Crust interactions within the Northern Cordillera
Friday, 17 May 2024
8:00 AM - 12:00 PM
Cedar Ballroom
THE KANUTI OPHIOLITE, INTERIOR ALASKA: GEOLOGY AND TECTONIC SETTING OF (POSSIBLE) SUPRA-SUBDUCTION OCEANIC LITHOSPHERE
Paper number: 36-13
Program: Theme Sessions
Time: 11:40 AM – 12:00 PM
Authors
-
Jonathan S. CaineGeology, Geophysics, and Geochemistry Science Center, Denver, CO
-
Michael BizimisUniversity of South Carolina, Columbia, SC
-
Robert HammondUniversity of South Carolina, Columbia, SC
-
Heather LowersGeology, Geophysics, and Geochemistry Science Center, Denver, CO
-
Jay ThompsonGeology, Geophysics, and Geochemistry Science Center, Denver, CO
Abstract
Geochronology, both of melting to produce Kanuti crust, and timing of obduction, is poorly constrained. Hornblende in dikes intruding UMs, and in metamorphic sole amphibolite have K-Ar ages between ca. 160-140 Ma, though datable U-bearing phases in Kanuti gabbros are elusive; efforts are ongoing.
Kanuti gabbros are subalkaline and N-MORB-like and gabbro cpx resembles mid-ocean ridge cumulates (TiO2 ~0.8, Mg# ~80). Small Th over Nb enrichment in gabbro point to weak crustal/subduction modification, yet Ti/V is not consistent with oxidized mantle. Gabbros have Pacific MORB-like Hf-Nd isotopes, with some samples extending to more enriched Nd along the mantle array. Lherzolite and dunite olivine has Fo ~90; Fo in chromitite is higher (93-96) and is lower in pyroxenite (86). Clinopyroxenes (cpx) in UMs have high Mg# (92-99) and low Ti (<0.2wt%), transitional between depleted abyssal and suprasubduction types. Spinels have high-Mg and low-Cr in mantle rocks, but are more depleted, and likely melt-reacted, in cumulates. Studies are ongoing, but Kanuti ophiolite shows a source with weak subduction modification, possibly at a forearc setting.
Geological Society of America Abstracts with Programs. Vol. 56, No. 4
doi: 10.1130/abs/2024CD-399711
© Copyright 2024 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.