Lyell Collection

Journal of the Geological Society

Lyell Centre  |   Lyell Collection  |   Subscriptions   |   Geological Society  |   Email alerts  |   Online bookshop  |   Help


Keywords:
Author:
Advanced search>>
This Article
Right arrow Figures Only
Right arrow Full Text
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Right arrow Citation Map
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow Request Permissions
Citing Articles
Right arrow Citing Articles via ISI Web of Science (1)
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Eccles, J.D.
Right arrow Articles by Spörli, K.B.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation
Journal of the Geological Society; 2005; v. 162; issue.4; p. 723-735;
DOI: 10.1144/0016-764904-060
© 2005 Geological Society of London

Original Article

Aeromagnetic imaging of the Dun Mountain Ophiolite Belt in northern New Zealand: insight into the fine structure of a major SW Pacific terrane suture

J.D. Eccles, J. Cassidy, C.A. Locke & K.B. Spörli

Department of Geology, The University of Auckland, Private Bag 92019, Auckland, New Zealand (e-mail: j.cassidy@auckland.ac.nz)

A new aeromagnetic survey of the Junction Magnetic Anomaly in northern New Zealand reveals that it is associated with up to 10 subparallel lineaments. The Junction Magnetic Anomaly delineates the Dun Mountain Ophiolite Belt, a remarkably linear though sigmoidally bent major boundary zone traceable through most of New Zealand, which separates terranes sutured onto the New Zealand Gondwana margin in late Mesozoic time. Modelling of the lineaments, in conjunction with a new review of structures along the Dun Mountain Ophiolite Belt throughout New Zealand, indicates that the Dun Mountain Ophiolite Belt in Auckland consists of a number of imbricate slices, most of which are likely to dip steeply to the east (i.e. overturned away from the former trench) and extend to considerable depth in the crust. The source bodies for the central high-amplitude magnetic lineaments are interpreted to be serpentinite shear or mélange zones, cutting a large lensoid body of ultramafic rocks, similar to those occurring elsewhere along the length of the Dun Mountain Ophiolite Belt. Our data have revealed that a formerly postulated offset of the Dun Mountain Ophiolite Belt in the region instead resembles a duplex or thrust imbricate-like bundling of shear zones. These shear zones were probably initiated as accretion thrusts, but complexities in their pattern indicate subsequent shearing, including ‘backfolding’ to an overturned attitude and possibly strike slip to produce the linear nature of the Dun Mountain Ophiolite Belt. The outer lineaments mostly mark accretion thrusts in the adjacent terranes. This study demonstrates that detailed aeromagnetic surveys can delineate the fine structure in ophiolite complexes and thereby give valuable insights into the effects of micro-continental collision on an accretionary margin.

Key Words: Dun Mountain Ophiolite Belt • aeromagnetic surveys • serpentinite • accretion • shear zones