2004
DOI: 10.1016/j.precamres.2003.09.002
|View full text |Cite
|
Sign up to set email alerts
|

Palaeoproterozoic crustal accretion and collision in the southern Capricorn Orogen: the Glenburgh Orogeny

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

1
40
0

Year Published

2006
2006
2020
2020

Publication Types

Select...
6
2

Relationship

0
8

Authors

Journals

citations
Cited by 110 publications
(41 citation statements)
references
References 20 publications
1
40
0
Order By: Relevance
“…2.0-1.8-Ga Proterozoic orogenic belts in the Northern Hemisphere (e.g., Hoffman 1980Hoffman , 1988Lewry 1981;Condie 1982;Park 1985;Patchett and Arndt 1986;Dickin and McNutt 1990;Snyder et al 1996;Torsvik et al 1996;Patchett and Chase 2002;Steltenpohl et al 2003). Recent geochemical and isotopic studies within Australian terrains such as the Arunta Region and the Capricorn Orogen have recognized, albeit in a somewhat cryptic way, accreted fragments along convergent plate margins (e.g., Zhao 1994;Zhao and McCulloch 1995;Cawood and Tyler 2004;Occhipinti et al 2004). These data sets have been used by a number of workers to propose that the evolution of Proterozoic Australia involved important accretionary and collisional events (e.g., Myers et al 1996;Scott et al 2000;Betts et al 2002;Giles et al , 2004Tyler 2005).…”
Section: Introductionmentioning
confidence: 99%
See 2 more Smart Citations
“…2.0-1.8-Ga Proterozoic orogenic belts in the Northern Hemisphere (e.g., Hoffman 1980Hoffman , 1988Lewry 1981;Condie 1982;Park 1985;Patchett and Arndt 1986;Dickin and McNutt 1990;Snyder et al 1996;Torsvik et al 1996;Patchett and Chase 2002;Steltenpohl et al 2003). Recent geochemical and isotopic studies within Australian terrains such as the Arunta Region and the Capricorn Orogen have recognized, albeit in a somewhat cryptic way, accreted fragments along convergent plate margins (e.g., Zhao 1994;Zhao and McCulloch 1995;Cawood and Tyler 2004;Occhipinti et al 2004). These data sets have been used by a number of workers to propose that the evolution of Proterozoic Australia involved important accretionary and collisional events (e.g., Myers et al 1996;Scott et al 2000;Betts et al 2002;Giles et al , 2004Tyler 2005).…”
Section: Introductionmentioning
confidence: 99%
“…1; e.g., Foden et al 1988;Zhao 1994;Zhao and McCulloch 1995;McDonald et al 1997;Sheppard et al 1999;Close et al 2004), and the West Australian Craton (WAC), including the Capricorn Orogen ( fig. 1; e.g., Cawood and Tyler 2004;Occhipinti et al 2004). Mafic and felsic magmatic rocks with subduction-related geochemical affinities from these regions have been viewed as a result of Paleoproterozoic arc magmatism (e.g., Foden et al 1988;Zhao 1992;Zhao and McCulloch 1995;Sheppard et al 1999Sheppard et al , 2004Cawood and Tyler 2004;Occhipinti et al 2004).…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…The next major pulse of magmatic activity is represented by the granitic gneisses and granites of the 2005-1970 Ma Dalgaringa Supersuite (Cycle 2; Fig. 2), which formed in a continental arc prior to the final collision amalgamating the West Australian Craton Occhipinti et al, 2004). The isotopic compositions of magmatic zircons indicate mixing of mantle-derived material and older continental crust similar to the Halfway Gneiss (Johnson et al, 2010(Johnson et al, , 2011a(Johnson et al, , 2011b.…”
Section: Evolution Of Radiogenic Heat Production With Timementioning
confidence: 99%
“…The Capricorn Orogen comprises rocks deformed and metamorphosed during several Palaeoproterozoic orogenic events ranging from 2.0-1.6 Ga (e.g. Occhipinti et al 2004). Together with the Archaean Pilbara and Yilgarn cratonic blocks, the Palaeoproterozoic Capricorn Orogen form the West Australian Craton (Myers 1993).…”
Section: Proterozoic Orogensmentioning
confidence: 99%