“…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).…”