1School of Environmental and Life Sciences, University of Newcastle,
University Drive, Callaghan, 2308, Australia
2Research School of Earth Sciences, Australian National University,
Bldg. 61, Mills Road, Canberra, 0200, Australia
anow at: Analytical, Environmental and Geo-Chemistry, Vrije Universiteit
Brussel, Pleinlaan 2, Brussels 1050, Belgium
Received: 20 Aug 2016 – Discussion started: 31 Aug 2016
Abstract. The New England Orogen, eastern Australia, was established as an outboard extension of the Lachlan Orogen through the migration of magmatism into forearc basin and accretionary prism sediments. Widespread S-type granitic rocks of the Hillgrove and Bundarra supersuites represent the first pulse of magmatism, followed by I- and A-types typical of circum-Pacific extensional accretionary orogens. Associated with the former are a number of small tholeiite–gabbroic to intermediate bodies of the Bakers Creek Suite, which sample the heat source for production of granitic magmas and are potential tectonic markers indicating why magmatism moved into the forearc and accretionary complexes rather than rifting the old Lachlan Orogen arc. The Bakers Creek Suite gabbros capture an early ( ∼ 305 Ma) forearc basalt-like component with low Th ∕ Nb and with high Y ∕ Zr and Ba ∕ La, recording melting in the mantle wedge with little involvement of a slab flux and indicating forearc rifting. Subsequently, arc–back-arc like gabbroic magmas (305–304 Ma) were emplaced, followed by compositionally diverse magmatism leading up to the main S-type granitic intrusion ( ∼ 290 Ma). This trend in magmatic evolution implicates forearc and other mantle wedge melts in the heating and melting of fertile accretion complex sediments and relatively long ( ∼ 10 Myr) timescales for such melting.
Revised: 28 Feb 2017 – Accepted: 08 Mar 2017 – Published: 05 Apr 2017
McKibbin, S. J., Landenberger, B., and Fanning, C. M.: First magmatism in the New England Batholith, Australia: forearc and arc–back-arc components in the Bakers Creek Suite gabbros, Solid Earth, 8, 421-434, doi:10.5194/se-8-421-2017, 2017.