“…These studies point out that the early evolution of the Albany-Fraser Orogeny (Stage I) coincided with the Mount West Orogeny in the Musgrave Province, and the later evolution (Stage II) with the Musgrave Orogeny. Both sets of coincided events have been linked to the final convergence of the South Australian Craton towards the combined North and West Australian Cratons (Stage I/Mount West Orogeny; Giles et al, 2004;Betts and Giles, 2006;Cawood and Korsch, 2008; Stage II/Musgrave Orogeny; Myers et al, 1996;Smits et al, 2014). These conflicting views demonstrate the importance of understanding not only the individual provinces, but also the relationships between them.…”
Section: Significance Of the Musgrave Province In The Final Amalgamatmentioning
confidence: 91%
“…Most models propose amalgamation of the West and North Australian Cratons prior to connecting with the South Australian Craton, and all major cratonic components being in place by at least c. 1290 Ma (e.g. Giles et al, 2004;Betts and Giles, 2006;Cawood and Korsch, 2008) or by c. 1100 Ma (Myers et al, 1996;Smits et al, 2014). These studies point out that the early evolution of the Albany-Fraser Orogeny (Stage I) coincided with the Mount West Orogeny in the Musgrave Province, and the later evolution (Stage II) with the Musgrave Orogeny.…”
Section: Significance Of the Musgrave Province In The Final Amalgamatmentioning
“…These studies point out that the early evolution of the Albany-Fraser Orogeny (Stage I) coincided with the Mount West Orogeny in the Musgrave Province, and the later evolution (Stage II) with the Musgrave Orogeny. Both sets of coincided events have been linked to the final convergence of the South Australian Craton towards the combined North and West Australian Cratons (Stage I/Mount West Orogeny; Giles et al, 2004;Betts and Giles, 2006;Cawood and Korsch, 2008; Stage II/Musgrave Orogeny; Myers et al, 1996;Smits et al, 2014). These conflicting views demonstrate the importance of understanding not only the individual provinces, but also the relationships between them.…”
Section: Significance Of the Musgrave Province In The Final Amalgamatmentioning
confidence: 91%
“…Most models propose amalgamation of the West and North Australian Cratons prior to connecting with the South Australian Craton, and all major cratonic components being in place by at least c. 1290 Ma (e.g. Giles et al, 2004;Betts and Giles, 2006;Cawood and Korsch, 2008) or by c. 1100 Ma (Myers et al, 1996;Smits et al, 2014). These studies point out that the early evolution of the Albany-Fraser Orogeny (Stage I) coincided with the Mount West Orogeny in the Musgrave Province, and the later evolution (Stage II) with the Musgrave Orogeny.…”
Section: Significance Of the Musgrave Province In The Final Amalgamatmentioning
“…9 and 10). A proposed eastward extension of the central Australian Musgrave Province is consistent with the AUSMEX reconstruction of Rodinia with a link to the Grenville Orogen of eastern Laurentia (Wingate et al, 2002;Pisarevsky et al, 2003;Smits et al, 2014) but not considered in other syntheses of the Rodinia reconstruction (Li et al, 2008).…”
Section: E Implications For Nac-wac-sac Connections and Rodiniamentioning
confidence: 58%
“…This suggestion was subsequently overlooked with emphasis placed on Paleoproterozoic connections between the North and South Australian cratons (Betts and Giles, 2006;Cawood and Korsch, 2008). However new isotopic data supports the interpretation of the Musgrave-Albany-Fraser belt as a collisional suture formed in the final assembly of the Australian continent in Grenville time (Smits et al, 2014). This interpretation is also supported by a contemporary review of the Musgrave Province (Howard et al, 2015) which describes a complex orogenic history, with major episodes of igneous activity between 1345 and 1150 Ma followed by rift-related bimodal magmatism at ~1090-1040 Ma.…”
Section: E Implications For Nac-wac-sac Connections and Rodiniamentioning
confidence: 89%
“…The Grenville Orogeny is regarded as perhaps the most significant event of crustal reorganisation in Earth history (Van Kranendonk and Kirkland, 2013) with global effects which embraced the Albany-FraserMusgrave belt which extends obliquely across Australia (Smits et al, 2014). The age diversity apparent for Australian Precambrian terrains lying to the west of the Tasmanides coupled with the tight, unimodal Grenville age distributions shown by zircon age spectra from some Thomson Orogen samples (Fig.…”
Section: Detrital Zircon Ages Have Shown That the Metasedimentary Sucmentioning
The U-Pb and Lu-Hf isotopic research of detrital zircons was carried out in southern modern rivers of the South Tianshan (STS) orogenic belt to understand the accretionary processes and crustal evolution in this region. Detrital zircons from river sands yield two dominant age populations at 460-390 Ma and 310-260 Ma with several Precambrian age groups. Such age patterns imply that the significant magmatic events occurred during the Palaeozoic in the STS. Comparative studies on U-Pb age of the detrital zircons from northern and southern river sands in the STS belt provide constraints on the tectonic evolution of the STS belt and its surrounding blocks. Abundant 500-460 Ma detrital zircons in northern river sands probably reflect a bidirectional subduction of the Palaeozoic Central Tianshan Ocean under the Yili Block and the Central Tianshan Block. The 460-390 Ma zircon population in both northern and southern river sands likely implies a bidirectional subduction of the South Tianshan Ocean. A lack of the 380-320 Ma zircon grains in the southern river sands may indicates the northward subduction of the South Tianshan Ocean. A final collision between the Tarim Craton and the southwestern Central Asian Orogenic Belt possibly took place in the Late Carboniferous; the 310-260 Ma zircon population in both northern and southern river sands suggests syn-and post-collisional magmatism. Based on the Hf isotopic signatures in the detrital zircon and magmatic zircons, we propose new constraints on the Palaeozoic crustal evolution of the STS. The continent formation in the STS belt was characterised by reworking of the ancient crust in a compressional environment during the Ordovician (ca. 460-440 Ma). Abundant significant juvenile materials progressively added to the crust through time in an extensional tectonic regime since Late Ordovician to Devonian (ca. 440-390 Ma). The crustal formation is mainly dominated by reworking of the Precambrian basement rocks with limited contribution of juvenile components input into magma formation during Late Carboniferous to Early Permian (ca. 310-260 Ma).
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