Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-04T19:26:16.893Z Has data issue: false hasContentIssue false

New U-Pb zircon ages from the Denman Glacier area, East Antarctica, and their significance for Gondwana reconstruction

Published online by Cambridge University Press:  13 May 2004

Lance P. Black
Affiliation:
Bureau of Mineral Resources, G.P.O. Box 378, Canberra, A.C.T. 2601, Australia
John W. Sheraton
Affiliation:
Bureau of Mineral Resources, G.P.O. Box 378, Canberra, A.C.T. 2601, Australia
Robert J. Tingey
Affiliation:
Bureau of Mineral Resources, G.P.O. Box 378, Canberra, A.C.T. 2601, Australia
Malcolm T. Mcculloch
Affiliation:
Research School of Earth Sciences, Australian National University, G.P.O. Box 4, Canberra, A.C.T. 2601, Australia

Abstract

Two new U-Pb zircon ages from the area immediately west of Denman Glacier in Antarctica show that its geological history differs from that of the Obruchev Hills and Bunger Hills, to the east of the glacier. A crystallization age of 516.0 ± 1.5 Ma for syenite is by far the youngest primary age reported for this region, whereas tonalitic orthogneiss from Cape Charcot, the oldest known local rock, was derived by the high-grade metamorphism and deformation at 2889 ± 9 Ma of a 3003 ± 8 Ma igneous precursor. Both major populations of zircon in this rock lost Pb at 500–600 Ma. Although the Sm-Nd characteristics of the entire region resemble those of the Albany Mobile Belt of Western Australia, the Sm-Nd systematics of the felsic gneisses and plutonics are too old to allow direct correlation with the rocks of the Naturaliste Block (Western Australia), a potential key element for Gondwana reconstruction. However, the possibility exists that there is an indirect relationship between the Naturaliste Block and the region immediately west of Denman Glacier.

Type
Papers—Earth Sciences and Glaciology
Copyright
© Antarctic Science Ltd 1992

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)