Zircon O and Lu-Hf isotope evidence of mantle and supracrustal origins of Tasmanian Devonian granites

The Tasmanian Devonian granites were emplaced during the Tabberabberan Orogeny when the East and West Tasmania Terranes were sutured. The primary aim of this study is to determine zircon O and Lu-Hf isotope constraints on, and relationships between, the magmas forming these granites. A second aim is to determine if these zircon isotopic compositions can be used to inform granite-related ore endowment. Several granites (n = 11 in East Tasmania Terrane, n = 1 West Tasmania Terrane) were previously dated by U-Pb geochronology using SHRIMP, and the zircon pits from the dating analyses were targeted firstly in O and later in Lu-Hf isotope analyses. The magmatic zircon delta O-18(VSMOW) results ranged from mantle-like values (< 5.7 parts per thousand) to values like supracrustal rocks (similar to 12 parts per thousand). The granites with the lowest most mantle-like zircon delta O-18 are all I-types, and these include the relatively mafic Lisle to the very felsic and highly fractionated Mt Stronach and Tombstone Creek plutons. The Tombstone Creek zircon epsilon Hf-i results are significantly lower than those of Lisle and Mt Stronach, indicating distinct melt sources from which the zircons crystallized. The magmatic zircon delta O-18 and epsilon Hf-i results revealed two distinct paths of infracrustal to upper crustal rock epsilon Hf-i- delta O-18 melt evolution: one "high epsilon Hf" path linking the results from the Lisle, Mt Stronach, Hazards, Henbury, Lottah, Gipps Creek and Royal George granites, and the other "low epsilon Hf" path linking those from Tombstone Creek, Meredith, Poimena, Bicheno and Ansons Bay granites. The paths are statistically different and modeled results are consistent with mixing of Mathinna Supergroup rocks with different isotopically defined infracrustal/mantle-like components. The high epsilon Hf group of granites are strongly associated with granite-related Au, Sn, and Sn-W ore deposits. (C) 2022 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.