Genesis Directory UMM :Data Elmu:jurnal:P:Precambrian Research:Vol101.Issue1.2000:

no volcanicity to the depositional environment of the Braemar ironstone. Deposition of the Pualco Tillite diamictites during the Sturtian glacial maximum was re- stricted to the marine Baratta Trough and the main depocentre was in the Braemar area Preiss, 1987. The diamictites have been inter- preted as glaciomarine sediments, deposited from wet-based glaciers originating from the Palaeoproterozoic to Mesoproterozoic Willyama basement Curnamona Cratonic Nucleus and debouching into a marine basin Preiss et al., 1993. The lack of local detritus in the basal diamictite and the generally regionally planar de- positional surface probably imply deposition of the Pualco Tillite from an extensive floating ice- sheet Preiss, 1987. Reworking of the diamic- tites, possibly by water currents, is indicated by interbedded quartzites, or the quartzites may have been derived from a different, more mature sediment source than the associated diamictites. The Pualco Tillite rests on a slightly irregular erosional surface developed on the Burra Group, or locally on crystalline basement, over the whole Olary province Preiss, 1987. It contains basement-derived material near Olary, probably shed from the exposed Willyama Inliers. An 800-m long slide block of granite in the Pualco Tillite adjacent to the MacDonald Fault and lenticular granite conglomerates suggest an ac- tively rising fault scarp in the Olary region and it is thus interpreted that the diamictites and conglomerates may have been deposited in deep glacial valleys of a highland terrain Preiss, 1987. Faulting is less obvious at the other mar- gins of the Barratta Trough, which may have been a halfgraben. The preservation of pre- glacial regoliths in parts of the southern and central Flinders Ranges, as well as possibly on the Stuart Shelf, suggests that the lowlands to the west were not severely glaciated Preiss, 1987. These sedimentological data imply that the Braemar ironstones accumulated in a basin along the border of a continental glaciated high- land to the northeast and a low-lying weathered landmass to the west.

8. Genesis

8 . 1 . Formation of the Braemar facies The role of glaciation in the formation of Neoproterozoic ironstones has been emphasised by a number of authors Yeo, 1983; Urban et al., 1992; Klein and Beukes, 1993; Graf et al., 1994. The occurrence of ironstones in several Neoproterozoic glacial deposits inspired the hy- pothesis that during glaciation, the underlying stagnant seawater was cut off from oxygen sup- ply and was rendered anoxic by organic matter decomposition. Build-up of dissolved Fe oc- curred in the Proterozoic oceans during glacial periods and deposition of Fe followed during transgressive interglacial periods e.g. Urban et al., 1992; Klein and Beukes, 1993. In fact, the ‘snowball-type Earth’ theory suggests the pres- ence of floating pack ice over most of the ocean surface at middle to high latitudes as well as equatorial glaciation Kirschvink, 1992. Oxy- genation of ferriferous waters after glaciation would drive the precipitation of ferric oxide in oxic and highly oversaturated surface waters cf. Kaufman et al., 1991; Hoffman et al., 1998. Previous authors have assigned the origin of the Braemar ironstones to chemical precipitation in a lacustrine environment Preiss, 1987 or to physical accumulation of detrital Fe oxides Whitten, 1970; Preiss, 1987. However, our compositional data show that the Braemar facies was generated by the intermixing of chemical precipitates and terrigenous debris on a conti- nental margin. Evaporation of waters in a playa- lake complex cf. Eugster and Chou, 1973 did not produce Braemar ironstones as indicated by the palaeogeographic environment. The possibility that ferriferous exhalations have influenced the formation of the Braemar ironstone is supported for the following reason. While the rocks exhibit exceptionally low con- centrations of As, Cu, Pb and Zn compared to upper crustal abundances values Taylor and McLennan, 1981, they exhibit positive correla- tions of Fe with As, Cu, Sb, V and Zn, elements typical of ironstones formed under hydrothermal influences e.g. Dymek and Klein, 1988; Duhig et al., 1992; Lottermoser and Ashley, 1996; Ash- ley et al., 1998. Thus the Fe of the Braemar ironstone originally derived from hydrothermal exhalations. The Braemar ironstone facies consists of lentic- ular laminated and diamictic ironstones and di- amictic ironstones are interbedded with Braemar facies devoid of, and also with, dropstones Fig. 3c. Thus Fe deposition was clearly associated with ice-melting and clastic sedimentation and occurred during openwater ocean circulation and melting of icebergs. The presence of Fe oxide-rich diamictites indicates that refrigeration prevailed during Braemar facies deposition, and was proba- bly maintained throughout deposition of the Benda Siltstone as indicated by scattered drop- stones brought in by floating icebergs cf. Preiss, 1987. Thus the Braemar facies, including the dolostones, was deposited during the waning stages of the Pualco glaciation, during a climate change from deep refrigeration to slightly warmer temperatures. When the sea ice retreated, oxy- genation of the water column of ferriferous + manganiferous, carbonate and CO 2 charged waters occurred cf. Kaufman et al., 1991; Hoff- man et al., 1998. These waters precipitated car- bonate upon release of CO 2 to the atmosphere cf. Kaufman et al., 1991; Hoffman et al., 1998 and hence the dolostones of the Braemar facies are interpreted as inorganic cold water deposits. During glacial periods build-up of dissolved, reduced hydrothermal Fe occurred. A subsequent transgressive event during an interglacial period and associated melting of floating ice led to the oxidation of coastal seawater and the precipita- tion of dissolved Fe. Coprecipitation and adsorp- tion of REE from the water column caused a coastal seawater REE signature of the chemical sediments. Intercalations of Fe-poor siltstones and diamictites between the ferruginous facies Fig. 3c would indicate an episodic decrease in Fe precipitation and dominating clastic sedimenta- tion. These siliceous, aluminous sediments ob- tained a detrital REE signature. Climate controlled regressions and transgressions of the sea ice are the most likely reason for the presence of intercalated non-ferruginous clastic sediments in diamictic and laminated ironstones. Redox po- tential differences kept Mn in solution, however, increasing oxidising conditions led to the precipi- tation of Mn oxides or carbonates and their in- corporation in clastic sediments and the resulting formation of manganiferous siltstones cf. Urban et al., 1992; Manikyamba and Naqvi, 1995. 8 . 2 . Geotectonic setting The palaeolatitude of Neoproterozoic iron- stones and associated glacial sediments has been controversial. Meert and Van der Voo 1994 argued, using palaeomagnetic data, that Neoproterozoic glaciations did not occur below 25° latitude. However, recent palaeomagnetic data indicate that the formation of Neoproterozoic ironstones and associated glacial sediments oc- curred in low-latitude environments. The Mari- noan glaciation in South Australia 650 – 600 Ma, including permafrost, grounded glaciers and marine glacial deposition, occurred near the palaeoequator Schmidt and Williams, 1995. Similarly, the formation of the Rapitan ironstone and associated glacial sediments ca. 725 Ma of northwestern Canada occurred in a low-latitude environment Park, 1997. Young 1992, 1995 proposed that the Sturtian glaciation in the Ade- laide Geosyncline corresponds to the Rapitan glaciation in northwestern Canada. Such strati- graphic correlations would imply that the iron- stones of the Sturtian Braemar facies ca. 750 – 700 Ma were deposited in a low-latitude environment. However, further geochronological and palaeomagnetic studies will be required to establish whether the Sturtian and Rapitan glacia- tions are diachronous or synchronous. In addi- tion, Rui and Piper 1997 stated that the sedimentary cycles recognised in the Neoprotero- zoic successions of Australia and Canada were probably driven by global eustatic changes and do not imply close proximity of the two regions.

9. Conclusions