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Australia: The Land Where Time Began |
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Precambrian Tectonics Archean crust, that formed some time between 4.4-2.5 Ga, is present in the relatively flat, stable regions of the continents. The transition from the molten early Earth to a condition where crust could be preserved is marked by the first appearance of the cratonic nuclei which were the original blocks around which the continents were built. Most cratons are attached to a mantle root, that is of high seismic velocity, extending down at least 200 km (King, 2005). The roots of cratons are chemically buoyant mantle material that is stiff and resistant, contributing to their survival from the Archean to the present (Carlson et al.2005). The age of rocks at the beginning of the Archean Eon, when solid rock first formed that has been preserved, is not known for certain. The oldest generally accepted dates are for the Acasta gneisses of the Slave Craton, northwest Canada (Bowring & Williams, 1999). Detrital zircons have been found at Jack Hills, on the Yilgarn Craton, Western Australia (Wilde et al., 2001) that have been dated to 4.4 Ga. This interpretation has been disputed (Harrison et al., 2005, 2006; Valley et al., 2006). Because the age of the earliest rocks is being continually pushed back it cannot be said with confidence when the first solid rocks actually formed (Gradstein, 2004). The end of the Archean - beginning of the Proterozoic Era coincides approximately with the inferred changes in tectonic style and petrologic characteristics of Precambrian rocks. The debate over the nature of tectonic activity in the Precambrian centres on these inferences. One of the issues is whether plate tectonics operated in some form in the early Earth, and when it began. Based on current evidence it is believed the mechanisms of plate tectonics, such as subduction, were occurring by at least 2.8-2.6 Ga, and possibly much earlier (van der Velden et al., 2006; Cawood et al., 2006). 3 approaches have been used when considering Precambrian tectonic processes (Kröner, 1981; Cawood, et al., 2006). These are:
Informative results have been obtained from all 3 approaches. See Source 1 for more detailed information on all aspects of plate tectonics See Australian Proterozoic Evolution - Palaeomagnetic Constraints
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Author: M.H.Monroe Email: admin@austhrutime.com Sources & Further reading |