Quick
Search: 
 
advanced search
 GSW Home    GeoRef Home    My GSW Alerts    Contact GSW    About GSW    Journals List    Help 
  Journal of the Geological Society   Don't get GSW? Talk to your librarian.
JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS

Journal of the Geological Society; September 2007; v. 164; no. 5; p. 937-940; DOI: 10.1144/0016-76492006-175
© 2007 Geological Society of London
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
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Similar articles in Web of Science
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow reprints & permissions
Citing Articles
Right arrow Citing Articles via Web of Science (4)
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Clark, C.
Right arrow Articles by Goscombe, B.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

Short Communication

Linking crustal reworking to terrane accretion

C. Clark1, M. Hand2, D.E. Kelsey2 and B. Goscombe2

1 1The Institute for Geoscience Research (TIGeR), Department of Applied Geology, Curtin University of Technology, WA 6845, Australia (e-mail: c.clark{at}curtin.edu.au)
2 2Continental Evolution Research Group, School of Earth and Environmental Sciences, University of Adelaide, SA 5005, Australia

The Strangways Metamorphic Complex in central Australia is a key terrane in models for the evolution of the Australian continent. The Arunta Complex preserves a long-lived (c. 1700–320 Ma) record of crustal reworking, the drivers of which are the subject of considerable debate. Pressure–temperature data and in situ monazite geochronology constrain the reworking to be coincident with the c.1645 Ma Liebig Orogeny. This suggests that reworking in the Strangways Metamorphic Complex is related to terrane accretion rather than other factors such as anomalous enrichment in high-heat-producing elements or within-plate processes.







JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2010 by Geological Society of London