Basement and cover relations on the northern margin of the Amadeus Basin, central Australia

A major, linear, west-trending deformed zone (The Redbank Zone), 350 km long and up to 20 km wide, can be identified in the Arunta Block immediately north of the Amadeus Basin. The marked linearity of this zone and of the coincident gravity anomaly probably result from thrust-fault movement during the Carboniferous Alice Springs Orogeny. However, in the Ormiston area, there is evidence that the zone originated prior to 1070 m.y. and acted as a major crustal feature controlling the later orogenic event.The Alice Springs Orogeny affected the overlying Proterozoic and Lower Palaeozoic cover rocks as well as the Arunta Block basement. During the orogeny, steep north-dipping thrusts within the Redbank Zone were reactivated causing uplift to the north. These faults penetrated the Heavitree Quartzite—the basal unit of the cover sequence—to drive wedges of basement, with attached veneers of Heavitree Quartzite, for up to 20 km southward within the overlying Bitter Springs Formation. The nappes did not reach the surface or penetrate formations above the Bitter Springs. Accompanying nappe emplacement the Basin to the south rapidly deepened to receive a thick wedge of synorogenic molasse sediments.Gravity, sedimentary and structural features combine to suggest that the Alice Springs orogeny movements reached their maximum on the central part of the northern margin of the Amadeus Basin, in the Ormiston area.     

Geology and geochronology of the Arunta complex north of Ormiston Gorge,Central Australia

A major west‐trending lineament marked by a wide belt of highly deformed rocks (the Redbank Zone), lies in the Arunta Complex, north of the Amadeus Basin. Along its southern margin the Zone has been progressively affected by, and is hence older than, migmatization and granite intrusion. The migmatization event yields a Rb‐Sr isochron age of 1076 ± 50 m.y. Within the migmatite complex, relicts of a pre‐migmatite metasedimentary sequence around the Chewings Range yield a Rb‐Sr isochron age of 1620 ± 70 m.y. The migmatites are unconformably overlain by the basal unit of the Amadeus Basin sequence, the Heavitree Quartzite. The 1076 ± 50 m.y. date thus provides a maximum age for the start of sedimentation along the northern margin of the Basin. The existence of a major zone of weakness in the basement probably exerted a strong control on basement and cover deformation during the Palaeozoic Alice Springs Orogeny.     

The age of the Stuart Dyke Swarm and its bearing on the onset of late Precambrian sedimentation in central Australia

A Rb‐Sr age of 897 ± 9 m.y. is obtained for dolerite from the Stuart Dyke Swarm in the southern part of the Arunta Block, Northern Territory. The dyke swarm presents an older age limit for the unconformably overlying Heavitree Quartzite, basal formation of the Amadeus Basin sequence. This limit is consistent with all isotopic data with the exception of previously determined glauconite ages from the Vaughan Springs Quartzite, a correlative of the Heavitree Quartzite in the Ngalia Basin.     

The Undoolya sequence: Late Proterozoic salt influenced deposition,Amadeus Basin,central Australia

Parts of the Late Proterozoic to Cambrian sequence along the northeastern margin of the Amadeus Basin were deposited under the influence of salt movement within the underlying Bitter Springs Formation. Later folding during the Devonian Alice Springs Orogeny and subsequent erosion has exposed salt‐influenced structures to provide a rare opportunity to observe the effects of diapiric growth on local facies and structure. Such effects are commonly only seen in seismic section. Salt withdrawal led to normal faulting and syn‐sedimentary thickening of adjacent units. The Undoolya Sequence, a previously undescribed 710 m section, was deposited within a salt‐withdrawal basin adjacent to a proposed diapiric structure. Periods of salt mobilization are recorded by syn‐depositional thickening and localized unconformities within units flanking the diapiric structure. This structure is representative of the influence salt movement had on deposition in the northeastern Amadeus Basin during the Late Proterozoic.     

Potassium‐argon dates from the Arltunga Nappe complex,northern territory

Twenty‐four mineral separates from the Arunta Complex, four from the metamorphosed Heavitree Quartzite (White Range Quartzite), and one whole rock sample of metamorphosed Bitter Springs Formation, all from the western part of the White Range Nappe of the Arltunga Nappe Complex, and two samples from the autochthonous basement west of the nappe have been dated by the K‐Ar method. The samples from the basement rocks form two groups. Those in the southern or frontal part of the nappe are of Middle Proterozoic (Carpentarian) age (1660–1368 m.y.), determined on hornblende, biotite, and muscovite. In the northern or rear part of the nappe, all but one of the muscovite samples and two biotites are of Middle Silurian to Early Carboniferous age (431–345 m.y.); the remainder of the biotite dates range from 1775 to 548 m.y. (including the two samples from the autochthon), and two hornblendes gave dates of 1639 and 2132 m.y. respectively. All the muscovite samples from the Heavitree Quartzite, and the whole rock sample from the Bitter Springs Formation gave Early to Middle Carboniferous dates (358–322 m.y.). The findings support the identification of the White Range Quartzite as the metamorphosed part of the Heavitree Quartzite, which in turn supports the interpretation of the structure of the area as a large, basement‐cored fold nappe. In addition, they date the time of the Alice Springs Orogeny as pre‐Late Carboniferous, which agrees with fossil evidence from elsewhere in the area. The Alice Springs Orogeny was accompanied by widespread greenschist facies meta‐morphism that progressively metamorphosed the Heavitree Quartzite and Bitter Springs Formation, and retrogressively metamorphosed the Arunta Complex. However, the basement rocks in the southern part of the nappe escaped this metamorphism and retain a Middle Proterozoic age, thus dating the time of the Arunta Orogeny in this region as Carpentarian or older.     

Faults and associated fault rocks of the Southern Arunta block, Alice Springs, Central Australia

The Southern Arunta block within the Alice Springs region is dissected by an E-W-trending network of high-angle reverse faults. Microstructural evidence indicates that there is a change from dominantly ductile to brittle faulting southwards across the block towards the Amadeus Basin, and this suggests that the faults in the north were progressively uplifted by the more southern faults. The generation of ultramylonite has been particularly extensive in the Alice Springs region. TEM and SEM observations have allowed an appraisal of the deformation mechanisms at ultrafine grainsizes and suggest complex interactions between dislocation processes, diffusion and grain-boundary sliding.     

Proterozoic evolution and tectonic setting of the northwest Paterson Orogen,Western Australia

The Proterozoic igneous, deformation and metamorphic histories of the Palaeoproterozoic Rudall Complex in the northwestern Paterson Orogen can be linked to those of the Arunta Inlier in central Australia, and in part with the Capricorn Orogen in central Western Australia. The similarities in deformation and metamorphic histories for these widely separated regions indicate a Palaeoproterozoic continent–continent collisional event between the Palaeoproterozoic West Australian and North Australian cratons between c. 1830 and 1765 Ma. In the Paterson Orogen this Palaeoproterozoic collisional event resulted in the Yapungku Orogeny, which included thrust stacking of clastic sedimentary and volcanic rocks, deposition of the protoliths for the c. 1790 Ma siliciclastic paragneiss succession contemporaneous with granitic intrusion, and metamorphism up to granulite facies. During this 65-million-year period, the Arunta Inlier and Capricorn Orogen were deformed, metamorphosed at medium to high grades and intruded by granitoids during the Strangways Orogeny in the Arunta Inlier and the Capricorn Orogeny in the Capricorn Orogen.The Neoproterozoic Tarcunyah, Throssell and Lamil groups are clastic sedimentary sequences that were deposited after 1070 Ma in the northwestern Paterson Orogen, and deformed by the Miles Orogeny before 678 Ma. The Miles Orogeny produced a northwesterly trending fold and fault system of tight to isoclinal upright and overturned folds and thrust faults. The orogeny may have been coincident with the c. 750–720 Ma Areyonga tectonic movement affecting the Arunta Inlier and the lower Neoproterozoic part of the Amadeus Basin in central Australia. At c. 550 Ma the Paterson Orogeny, which is most likely equivalent to the Petermann Orogeny in the Musgrave Complex of central Australia, deformed the northwestern Paterson Orogen and was preceded by local intrusion of granites.The similarities of styles and timing of deformation in the northwestern Paterson Orogen, Arunta Inlier and Capricorn Orogen indicate that these three regions were probably linked during most of the Proterozoic.     

Implications of pre-mesozoic orogeny in the geological evolution of the Himalaya and Indo-Gangetic Plains

An integrated geological analysis of the Himalaya and Indo-Gangetic Plains demonstrates that the Great Vindhyan Basin incorporating large parts of these morphotectonic units were uplifted into an uneven landmass due to the Pre-Mesozoic orogenic cycle. This uneven landmass was eroded off largely during a considerable part of the Devonian and Carboniferous thereby causing partial absence of sedimentary sequences of these periods except in parts of the Tethys Himalaya. The Late Paleozoic epeirogenic movements brought about renewed sedimentation in the Lesser and Tethys Himalayas in the Krol and Tethys Basins, respectively, which was terminated by the Himalayan Orogeny during Late Cretaceous—Early Eocene.     

Neoproterozoic (Cryogenian) stromatolites from the Wolfe Basin,east Kimberley,Western Australia: Correlation with the Centralian Superbasin

Linella avis, an early to middle Neoproterozoic (Tonian to Cryogenian) stromatolite, occurs in the Eliot Range Dolomite, part of the Ruby Plains Group in the Wolfe Basin, east Kimberley. Previously, this dolomite was assigned to the Mesoproterozoic Bungle Bungle Dolomite in the Osmond Basin, which contains a different suite of stromatolites. Linella avis, which also occurs in the Neoproterozoic Bitter Springs Formation of the Amadeus Basin, central Australia, appears to be restricted to rocks aged around 850 to 800 Ma. The presence of L. avis indicates that the Ruby Plains Group is a probable correlative of the Heavitree Quartzite and Bitter Springs Formation, and is probably much younger than the Bungle Bungle Dolomite. If the correlation suggested here is correct, the Wolfe Basin, together with the Amadeus and Ngalia Basins, formed part of the Centralian Superbasin.     

Dating of glauconite from the Ngalia Basin,Northern Territory,Australia∗

Rb‐Sr and K‐Ar measurements have been made on five glauconite samples from the near basal Treuer Member of the Vaughan Springs Quartzite of the Ngalia Basin, Northern Territory, Australia. Comparison of results between and within the two groups of data demonstrates that variable losses of radiogenic strontium and argon have occurred, but allows a minimum age of 1280 m.y. to be calculated for the member. Sedimentation began in the Ngalia Basin shortly before the time of deposition of this member.

Regional correlations suggest that this minimum age applies to the adjacent Amadeus Basin as well.

Measurements were also made on glauconite from a single sample of the Lower Palaeozoic Djagamara Formation which is in the same sequence. It yields a mid‐Ordovician K‐Ar age which generally agrees with the broad range of post‐Lower Cambrian to pre‐Carboniferous age determined from fossil evidence in bounding formations. A low Rb/Sr ratio prevented calculation of a Rb‐Sr age, but the combination of K‐Ar age and Rb‐Sr measurements allowed an accurate initial ⁸⁷Sr/⁸⁶Sr ratio of .739 to be determined. This is much greater than ocean water values, and it appears that such information on young samples and/or those of low Rb/Sr ratio could help define the source material for glauconite formation.     

Sm–Nd evidence for high-grade Ordovician metamorphism in the Arunta Block, central Australia

Sm–Nd ages from the Harts Range in the south-eastern Arunta Inlier in central Australia indicate that regional metamorphism up to granulite facies occurred in the Early Ordovician (c. 475 Ma). This represents a radical departure from previous tectonic models for the region and identifies a previously unrecognized intraplate event in central Australia. Peak metamorphic assemblages (800 °C and 10.5 kbar) formed at around 476±14 Ma and underwent approximately 4 kbar of near-isothermal decompression at 475±4 Ma. A coarse-grained unfoliated garnet–clinopyroxene-bearing marble inferred to have recrystallized late in the decompressional evolution, gives an age of 469±7 Ma. Two lines of evidence suggest the Early Ordovician tectonism occurred in an extensional setting. First, the timing of the high-grade lower crustal deformation coincides with a period of marine sedimentation in the Amadeus and Georgina basins that was associated with a seaway that developed across central Australia. Second, isothermal decompression of lower crustal rocks was associated with the formation of a regional, sub-horizontal mid-crustal foliation. In the Entia Gneiss Complex, which forms the structurally lowest part of the Harts Range, upper-amphibolite facies metamorphism (c. 700 °C, 8–9 kbar) occurred at 479±15 Ma. There is no evidence that P–T conditions in the Entia Gneiss Complex were as high as in the overlying units. This implies that the extensional system was reworked during a later compressional event. Sm–Nd data from the mid-amphibolite facies (c. 650 °C and 6 kbar) detachment zone that separates the Irindina Supracrustal Assemblage and Entia Gneiss Complex give an age of 449±10 Ma. This age corresponds to the timing of a change in the pattern and style of sedimentation in the Amadeus and Georgina basins, and indicates that the change in basin dynamics was associated with mid-crustal deformation. It also suggests that compressional deformation culminating in the Devonian to Carboniferous (400–300 Ma) Alice Springs Orogeny may have begun as early as c. 450 Ma. At present, the extent of Early Ordovician tectonism in central Australia is unknown. However, granulite facies metamorphism and associated intense deformation imply an event of regional extent. An implication of this work is that high-grade lower crustal metamorphism and intense deformation occurred during the development of a broad, shallow, slowly subsiding intraplate basin.     

Timing relationships between pegmatite emplacement,metamorphism and deformation during the intra‐plate Alice Springs Orogeny,central Australia

In the Harts Range (central Australia), the upper amphibolite facies to lower granulite facies, c. 480–460 Ma Harts Range Metamorphic Complex (HRMC), and the upper amphibolite facies, c. 340–320 Ma Entia Gneiss Complex are cut by numerous, generally peraluminous pegmatites and their deformed equivalents. The pegmatites have previously been interpreted as locally derived partial melts. However, SHRIMP U–Pb monazite and zircon dating of 29 pegmatites or their deformed equivalents, predominantly from the HRMC, reveal that they were emplaced episodically throughout almost the entire duration of the polyphase, c. 450–300 Ma intra‐plate Alice Springs Orogeny. Episodes of pegmatite intrusion correlate with the age of major Alice Springs‐age structures and with deposition of syn‐orogenic sedimentary rocks in the adjacent Centralian Superbasin. Similar Alice Springs ages have not been obtained from anatectic country rocks in the HRMC, suggesting that the pegmatites were not locally derived. Instead, they are interpreted as highly fractionated granites, and imply that much larger parental Alice Springs‐age granites exist at depth. The mechanism to allow repeated felsic magmatism in an intraplate setting, where all exposed rock types had a previous high‐temperature history, is enigmatic. However, we suggest that episodic underthrusting and dehydration of unmetamorphosed Centralian Superbasin sedimentary rocks allowed crustal fertility to maintained over a c. 140 Ma interval during the intra‐plate Alice Springs Orogeny.     

Three Palaeoproterozoic basins—Yerrida,Bryah and Padbury—Capricorn Orogen,Western Australia

The Palaeoproterozoic Yerrida, Bryah and Padbury Basins record periods of sedimentation and magmatism along the northern margin of the Archaean Yilgarn Craton. Each basin is characterised by distinct stratigraphy, igneous activity, structural and metamorphic history and mineral deposit types. The oldest of these basins, the Yerrida Basin (ca 2200 Ma) is floored by rocks of the Archaean Yilgarn Craton. Important features of this basin are the presence of evaporites and continental flood basalts. The ca 2000 Ma Bryah Basin developed on the northern margin of the Yilgarn Craton during backarc sea‐floor spreading and rifting, the result of which was the emplacement of voluminous mafic and ultramafic volcanic rocks. During the waning stages of the Bryah Basin this mafic to ultramafic volcanism gave way to deposition of clastic and chemical sedimentary rocks. At a later stage, the Padbury Basin developed as a retroarc foreland basin on top of the Bryah Basin in a fold‐and‐thrust belt. This resulted from either the collision of the Pilbara and Yilgarn Cratons (Capricorn Orogeny) or the ca 2000 Ma westward collision of the southern part of the Gascoyne Complex and the Yilgarn Craton (Glenburgh Orogeny). During the Capricorn Orogeny the Bryah Group was thrust to the southeast, over the Yerrida Group. Important mineral deposits are contained in the Yerrida, Bryah and Padbury Basins. In the Yerrida Basin a large Pb–carbonate deposit (Magellan) and black shale‐hosted gossans containing anomalous abundances of Ba, Cu, Zn and Pd are present. The Pb–carbonate deposit is hosted by the upper units of the Juderina Formation, and the lower unit of the unconformably overlying Earaheedy Group. The Bryah and Padbury Basins contain orogenic gold, copper‐gold volcanogenic massive sulfides, manganese and iron ore. The origin of the gold mineralisation is probably related to tectonothermal activity during the Capricorn Orogeny at ca 1800 Ma.     

TECTONIC STRUCTURE OF THE WESTERN BLACK SEA REGION

The lack of preserved Phanerozoic units within the Proterozoic Mount Isa Inlier of northern Australia renders it difficult to determine its Phanerozoic tectonic history. However, thermo-chronological methods provide a means for assessing this problem. Apatite fission-track data from the central and southern parts of the Inlier reveal periods of post-early Carboniferous accelerated cooling. Apatite fission-track ages vary from 235 to 390 Ma and corresponding mean track lengths range from 11.76 to 13.55 microns. These results record a protracted cooling history below about 110 ± 10° C. The earlier period of cooling revealed by the data occurred during middle Carboniferous time. The event resulted in >2 km of exhumation across the Inlier and probably was in response to intra-continental deformation associated with the Alice Springs Orogeny and tectonics in the adjacent Tasman Orogen.

A high proportion of partly annealed fission tracks in the samples suggests that rocks now exposed across the Inlier resided at the top of the apatite partial annealing zone (approximately 60° C to 70° C) following the mid-Carboniferous cooling. Modeling of the fission-track age and length parameters suggests that approximately 30° C to 50° C of cooling occurred over the past 100 Ma. Assuming a geothermal gradient of 25° C/km, this corresponds to 1.2-2.0 km of exhumation. The post-Middle Cretaceous cooling possibly is related to extensional tectonics at the southern and eastern margins of the Australian plate during the Mesozoic and Tertiary periods and to the more recent collision at the northern margin of the plate.

The spatial variation of apatite fission-track data within the Inlier indicates that the three major structural belts-the Western fold belt, Kalkadoon-Leichhardt belt, and the Eastern fold belt-exhibit similar thermal histories on a regional scale. It also indicates that the main N-S fault zones bounding the belts have not been reactivated in a vertical sense along their entire length since ～350 Ma. However, adjacent smaller-scale fault-bounded blocks within the belts demonstrate variable cooling histories, suggesting that reactivation of favorably oriented minor faults within the Inlier, including segments of the major faults, probably occurred during this time interval. Variations in apatite fission-track data along the 1994 Australian Geological Survey Organization/Australian Geodynamics Co-operation Research Center (AGSO/AGCRC) Mount Isa seismic traverse indicate that up to 1 km of vertical displacement has occurred between two major intrabelt fault zones since middle Carboniferous time.     

The Harry Creek Deformed Zone,a retrograde schist zone of the Arunta Block,central Australia

The Harry Creek Deformed Zone, a retrograde schist zone of epidote amphibolite facies grade, which separates the granulite facies Utralanama Block from the amphibolite facies Ankala Block in the southeastern Strangways Range, N.T., is typical of the retrograde schist zones transecting the Arunta Block. Associated with the deformed zone is a small deformed granitic pluton and its various offshoots—the Gumtree Granite Suite—which provides structural and geochrono‐logical evidence that the Harry Creek Deformed Zone has had a polyphase deforma‐tional history. Early movements within the deformed zone pre‐dated intrusion of the Gumtree Granite Suite and resulted in the movement of the Utralanama and Ankala Blocks into their present juxtaposition. Reactivation of much of the zone during the Alice Springs Orogeny brought about the schistose character of the zone and the deformation of the granitic rocks. Further minor reactivation of the zone, subsequent to the main phase of the Alice Springs Orogeny, resulted in limited development of pseudotachylytes.

The age of the granite (990 ± 13 m.y.) gives a minimum age for initiation of the zone, and evidence for the nature of the structures associated with the early movements is presented. It is suggested that the Harry Creek Deformed Zone represents a post‐orogenic wrench fault which has been reactivated. Early movements, which were of a brittle transcurrent nature, brought about major uplift (up to 10 km) to the north, and lateral movements may have been of the order of 60 km in a sinistral sense. Comparison with the Redbank Zone indicates many similarities, suggestive of a similar history.     

Tracking sediment dispersal during orogenesis: A zircon age and Hf isotope study from the western Amadeus Basin,Australia

The c. 570–530 Ma intraplate Petermann Orogeny of central Australia involved high temperature and pressure metamorphism, deformation, and uplift of the Mesoproterozoic Musgrave region and associated components of the Neoproterozoic Centralian Superbasin. Orogenesis was accompanied by deposition of a syn-tectonic siliciclastic sedimentary package (Supersequence 4) in adjacent depocentres such as the Amadeus Basin. Here we investigate the provenance of Supersequence 4 within the western Amadeus Basin using U–Pb age and Hf isotope data for detrital zircons. The data from eight samples are dominated by Mesoproterozoic zircons (peak at c. 1.18 Ga) matched by age and Hf isotopes to the Musgrave region. Smaller Palaeoproterozoic components match best with the Arunta region north of the Amadeus Basin. The latter zircons are likely reworked from older Amadeus Basin sediments uplifted and eroded during the Petermann Orogeny. The combined detrital zircon age signature from Supersequence 4 in the western Amadeus Basin is strongly similar to previously published data from successions of similar age in the eastern Amadeus Basin and from two metasedimentary units in the Charters Towers Province of Queensland; a K–S test indicates that these datasets are statistically identical at > 95% confidence. This suggests a sediment pathway from the Petermann Orogen to the palaeo-Pacific margin of East Gondwana via the Amadeus Basin. From existing data, a similar pathway can be inferred from the Officer Basin to the Adelaide Rift Complex on the southern side of the Petermann Orogen, although these zircon age spectra show differences in pre- and post-Mesoproterozoic components compared to the Amadeus Basin. Differences in detrital zircon age spectra and lithology between confirmed Supersequence 4 and previously inferred components of Supersequence 4 at Uluṟu (Mutitjulu Arkose) and Kata Tjuṯa (Mount Currie Conglomerate) on the southern Amadeus Basin margin raise questions about the stratigraphic position of these latter units.     

Stratigraphy of the Neoproterozoic to early Palaeozoic Savory Basin,Western Australia,and correlation with the Amadeus and Officer Basins

The Savory Basin in central Western Australia was recognized in the mid‐1980s during regional mapping of very poorly exposed Proterozoic rocks previously assigned to the Bangemall Basin. All of the sedimentary rock units in the Savory Basin have been included in the Savory Group, which unconformably overlies the Mesoproterozoic Yeneena and Bangemall Groups. Correlation with adjacent basins is impeded by poor outcrop and the lack of subsurface information. Possible correlations have been investigated with the much better known Amadeus Basin to the east, and with the Officer Basin. Two correlations now clarify the age and relationships of the Savory Group. First, the Skates Hills Formation contains distinctive stromatolites previously recorded from the Bitter Springs Formation of the Amadeus Basin. In addition, the Skates Hills and Bitter Springs Formations have many lithological features in common. This correlation is strengthened by comparison with surface and subsurface units in the northern Officer Basin. Second, the intergrading sandstone‐diamictite of the Boondawari Formation is very similar to the intergrading Pioneer Sandstone‐Olympic Formation of the Amadeus Basin, and the overlying siltstone closely resembles the Pertatataka Formation and its correlative the Winnall beds. The stromatolitic and oolitic carbonates at the top of the Boondawari Formation are broadly comparable with those of the Julie Formation (which grades down into the Pertatataka Formation). Support for this set of correlations comes from carbon isotope chemostratigraphy. The stromatolites include two new forms described herein, Eleonora boondawarica and Acaciella savoryensis, together with a third form too poorly preserved to be formally defined. The age of the upper sandstones is unknown. The McFadden Formation seems to have its provenance in the Paterson Orogen. The southeastern extension of this orogen is the Musgrave Block, where compression followed by uplift at about 560–530 Ma (Peterman Ranges Orogeny) led to the formation of large amounts of conglomerate (Mt Currie Conglomerate) and sandstone (Arumbera Sandstone). If tectonic events in the Paterson Orogen were contemporaneous with those in the Musgrave Block, the McFadden Formation would correlate with the Arumbera Sandstone.     

Exhumation history of the Peake and Denison Inliers: insights from low-temperature thermochronology

Multi-method thermochronology applied to the Peake and Denison Inliers (northern South Australia) reveals multiple low-temperature thermal events. Apatite fission track (AFT) data suggest two main time periods of basement cooling and/or reheating into AFT closure temperatures (～60–120°C); at ca 470–440 Ma and ca 340–300 Ma. We interpret the Ordovician pulse of rapid basement cooling as a result of post-orogenic cooling after the Delamerian Orogeny, followed by deformation related to the start of the Alice Springs Orogeny and orocline formation relating to the Benambran Orogeny. This is supported by a titanite U/Pb age of 479 ± 7 Ma. Our thermal history models indicate that subsequent denudation and sedimentary burial during the Devonian brought the basement rocks back to zircon U–Th–Sm/He (ZHe) closure temperatures (～200–150°C). This period was followed by a renewal of rapid cooling during the Carboniferous, likely as the result of the final pulses of the Alice Springs Orogeny, which exhumed the inlier to ambient surface temperatures. This thermal event is supported by the presence of the Mount Margaret erosion surface, which indicates that the inlier was exposed at the surface during the early Permian. During the Late Triassic–Early Jurassic, the inlier was subjected to minor reheating to AFT closure temperatures; however, the exact timing cannot be deduced from our dataset. Cretaceous apatite U–Th–Sm/He (AHe) ages coupled with the presence of contemporaneous coarse-grained terrigenous rocks suggest a temporally thermal perturbation related with shallow burial during this time, before late Cretaceous exhumation cooled the inliers back to ambient surface temperatures.     

Low‐temperature thermochronology of the Mt Painter Province,South Australia

Apatite fission track results are reported for 26 outcrop samples from the Mt Painter Inlier, Mt Babbage Inlier and adjacent Neoproterozoic rocks of the northwestern Curnamona Craton of South Australia. Forward modelling of the data indicates that the province experienced variable regional cooling from temperatures >110°C during the Late Palaeozoic (Late Carboniferous to Early Permian). The timing of this cooling is similar to that previously reported from elsewhere in the Adelaide Fold Belt and the Curnamona Craton, suggesting that the entire region underwent extensive Late Palaeozoic cooling most likely related to the waning stages of the Alice Springs or Kanimblan Orogenies. Results from the Paralana Fault Zone indicate that the eastern margin of the Mt Painter Inlier experienced a second episode of cooling (～40–60°C) during the Paleocene to Eocene. The entire region also experienced significant cooling (less than ～40°C) during the Late Cretaceous to Palaeogene in response to unroofing and/or a decrease in geothermal gradient. Regional cooling/erosion during this time is supported by: geomorphological and geophysical evidence indicating Tertiary exhumation of at least 1 km; Eocene sedimentation initiated in basins adjacent to the Flinders and Mt Lofty Ranges sections of the Adelaide Fold Belt; and Late Cretaceous ‐ Early Tertiary cooling previously reported from apatite fission track studies in the Willyama Inliers and the southern Adelaide Fold Belt. Late Cretaceous to Palaeogene cooling is probably related to a change in stress field propagated throughout the Australian Plate, and driven by the initiation of sea‐floor spreading in the Tasman Sea in the Late Cretaceous and the Eocene global plate reorganisation.     

Pleistocene stratigraphy of the Boco Plain,western Tasmania

The Late Devonian‐Early Carboniferous Mansfield Basin is the northernmost structural sub‐basin of the Mt Howitt Province of east‐central Victoria. It is comprised predominantly of continental clastic sedimentary rocks, and is superimposed upon deformed Cambrian to Early Devonian marine sequences of the Palaeozoic Lachlan Fold Belt. This paper documents evidence for synsedimentary deformation during the early history of the Mansfield Basin, via sedimentological, structural and stratigraphic investigations. Repeating episodes of folding, erosion and sedimentation are demonstrated along the preserved western margins of Mansfield Basin, where fold structures within the lower sequences are truncated by intrabasinal syntectonic unconformities. A convergent successor basin setting (an intermontane setting adjacent to, or between major fault zones) is suggested for initial phases of basin deposition, with synsedimentary reverse faulting being responsible for source uplift and subsequent basin deformation. Palaeocurrents within conglomerate units indicate derivation from the west and are consistent with episodic thrusting along basin margin faults providing elevated source regions. Periods of tectonic quiescence are represented by finer grained meandering fluvial facies (indicative of lower regional topographic gradients) which display drainage patterns that appear not to have been influenced by bounding faults to the west. An up‐sequence increase in the textural and compositional maturity of basin sandstones and conglomerates is proposed to be a result of the incorporation of basin fill into ongoing basin deformation, with unstable metapelitic rocks being progressively winnowed from clast populations. Rather than resulting from Carboniferous (Kanimblan) reactivation of extensional structures, as is generally assumed, the deformation observed within the lower units of the Mansfield Basin is suggested here to be essentially syndepositional and at least Late Devonian in age.