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Revised three-dimensional geometry of the platiniferous Hekeia Gabbro, Longwood Range, Southland.

Authors :
Mortimer N.
Martin C.E.
Tontini F.C.
Mortimer N.
Martin C.E.
Tontini F.C.
Publication Year :
2016

Abstract

The Hekeia Gabbro in the Longwood Range of Southland, New Zealand, is prospective for platinum group element mineralisation. Recently acquired geological and isotopic data, combined with reinterpreted aeromagnetic data, provide new constraints on the three-dimensional extent and internal structure of the gabbro. Direct observations of in situ subvertical igneous layering give confidence that most curvilinear aeromagnetic patterns are largely caused by macroscopic primary igneous layering. Steep magnetic gradients can be used to reliably define the areal limits of the Hekeia Gabbro and show that it extends to depths of over 1 km. Neodymium isotope ratios distinguish Hekeia Gabbro from younger gabbros and confirm the presence of at least two surface outcrops of Hekeia Gabbro a few kilometres west of the main body. Hekeia Gabbro is interpreted to be part of a 5 km thick Late Permian lopolith that was subsequently deformed and intruded by Triassic plutons. (Authors.)<br />The Hekeia Gabbro in the Longwood Range of Southland, New Zealand, is prospective for platinum group element mineralisation. Recently acquired geological and isotopic data, combined with reinterpreted aeromagnetic data, provide new constraints on the three-dimensional extent and internal structure of the gabbro. Direct observations of in situ subvertical igneous layering give confidence that most curvilinear aeromagnetic patterns are largely caused by macroscopic primary igneous layering. Steep magnetic gradients can be used to reliably define the areal limits of the Hekeia Gabbro and show that it extends to depths of over 1 km. Neodymium isotope ratios distinguish Hekeia Gabbro from younger gabbros and confirm the presence of at least two surface outcrops of Hekeia Gabbro a few kilometres west of the main body. Hekeia Gabbro is interpreted to be part of a 5 km thick Late Permian lopolith that was subsequently deformed and intruded by Triassic plutons. (Authors.)

Details

Database :
OAIster
Notes :
und
Publication Type :
Electronic Resource
Accession number :
edsoai.on1309246897
Document Type :
Electronic Resource