Adelaide Superbasin

Last updated

Adelaide Superbasin
Adelaide Geosyncline; Adelaide Rift Complex
Australia relief map.jpg
Orange pog.svg
Extent map of the Adelaide Superbasin.svg
An outline of both the known and potential extent of the Adelaide Superbasin
Coordinates 33°41′S138°44′E / 33.683°S 138.733°E / -33.683; 138.733
CountryFlag of Australia (converted).svg  Australia
State(s) South Australia; New South Wales; Victoria
Cities Adelaide
Geology
Basin type Rift; Passive margin
Plate Australian
Orogeny Delamerian; Alice Springs; Spriggs
Age Neoproterozoic-Cambrian
Stratigraphy Stratigraphy
Faults Paralana; Norwest; Anabama-Redan

The Adelaide Superbasin [1] (previously known as the Adelaide Geosyncline [2] [3] [4] and Adelaide Rift Complex [5] ) is a major Neoproterozoic to middle Cambrian geological province in central and south-east South Australia, western New South Wales, and western Victoria.

Contents

The Adelaide Superbasin consists of a thick pile of sedimentary rocks and minor volcanic rocks that were deposited on the eastern margin of Australia during the time of breakup of the supercontinent Rodinia. [6] A number of authors have noted the similarity in these sedimentary rocks with rocks found in western North America and have suggested that they were formerly adjacent to each other in Rodinia. This is one major correlation in the SWEAT (south-west USA against East Antarctica) reconstruction of Rodinia. [7] [8]

Particularly notable events that are preserved in the rock record of the Adelaide Superbasin are the two Neoproterozoic Snowball Earth events (the Sturtian and Marinoan Glaciations), the Neoproterozoic Oxygenation Event, [9] the Ediacaran Acraman bollide ejecta layer [10] and the rise of Ediacaran Fauna. [11] [12]

Geography

North–south it stretches over 850 km (530 mi) from the Peake and Denison Ranges in the central-north of South Australia down through the Flinders Ranges and Mount Lofty Ranges, narrowing at the Fleurieu Peninsula and extending onto Kangaroo Island. West–east it stretches about 700 km (430 mi) from the eastern margin of Lake Gairdner across to the Barrier Ranges of New South Wales. The true northern and eastern extent of the Adelaide Superbasin is not well known [1] due to much of the basin being buried beneath younger basins, including the Murray Basin, and is the subject of current research.

It is thought that the Moyston Fault in Victoria marks the eastern boundary and the northern extension may continue underneath and potentially include the Warburton Basin; however, this remains speculative. [1] [13] Most of the outcropping rock today is within the two major mountain ranges of South Australia: the Flinders Ranges and the Mount Lofty Ranges.

Much like the partly coeval Centralian Superbasin it contains several named basins and sub-basins. The oldest and largest of these is the Adelaide Rift Complex, with the adjoining and relatively undeformed Stuart Shelf, Torrens Hinge Zone and Coombalarnie Platform making up the remaining Neoproterozoic provinces. The Stansbury Basin (including its sub-province the Kanmantoo Province/Trough) and Arrowie Basin (including its sub-province the Yalkalpo Sub-basin) are the two known Cambrian provinces within the Adelaide Superbasin. [1] [4] [14]

Geologic history

Deposition in the Adelaide Superbasin began just prior to 830 Ma as Laurentia (and possibly an intervening continent, see Rodinia for alternative reconstructions) began to rift away from Australia during the breakup of the supercontinent Rodinia. Deposition continued through to the Delamerian Orogeny c. 514–490 Ma [15] [16] at which time deposition in the Adelaide Superbasin stopped and the rocks were folded and deformed. Initially, deposition occurred from gradual subsidence of peneplained cratonic lithosphere before developing into a rift basin.

After about 725 Ma, deposition continued in a mostly passive margin setting along the western edge of the Palaeo-Pacific Ocean, [17] with renewed rifting during the Ediacaran to the east (present day) of the main depocentres until being terminated by the Delamerian Orogeny. The most abundant rock types indicate a transition from evaporitic depositional environments through to proximal marine, glacial and marine depositional environments. [1] [13] [6] [3] The thickest parts of the stratigraphy reach a total cumulative thickness of about 24,000 m.

Basin subdivision

The Adelaide Superbasin composed of several named basins and sub-basins. In total there are currently eight defined basins/sub-basins within the Adelaide Superbasin. [1] [4] [18]

Known extents of the subdivisions of the Adelaide Superbasin for both the Neoproterozoic and Cambrian Basin subdivision of the Adelaide Superbasin.svg
Known extents of the subdivisions of the Adelaide Superbasin for both the Neoproterozoic and Cambrian

Adelaide Rift Complex

The Adelaide Rift Complex is the oldest and most central part of the Adelaide Superbasin. It is a series of rift troughs and passive margins basins with protracted development from c. 840 Ma to c. 550 Ma with the top of the sedimentary sequence marked by a major basin-wide disconformity separating it from the Cambrian Arrowie and Stansbury Basins.

Torrens Hinge Zone

The Torrens Hinge Zone is a transitional area between the relatively undeformed platform deposits of the Stuart Shelf and the deformed rocks of the central Adelaide Rift Complex. It runs along the western margin of the primary rift basin.

Stuart Shelf

The Stuart Shelf is a region of platform deposits on the western rift shoulder that overlies the Gawler Craton. It experienced deposition in the late Neoproterozoic after the Sturtian Glaciation during a period of marine transgression and remains relatively undeformed to this day.

Coombalarnie Platform

The Coombalarnie Platform, like the Stuart Shelf, is a region of platform deposits; however, it overlies the Curnamona Province to the north-east of the main depocentre. Deposition occurred only after a major marine transgression event during the late Neoproterozoic after the Sturtian Glaciation.

Stansbury Basin

The Stansbury Basin is one of the two known Cambrian basins of the Adelaide Superbasin. It is exposed in the south of the superbasin, extending from Kangaroo Island and the Mount Lofty Ranges toward Victoria underneath the Murray Basin. The true eastward extent of this basin is not well understood and is a focus of current geological research in South Australia. It is likely that deposition was continuous with the Arrowie Basin to the north. [18]

Kanmantoo Province

The Kanmantoo Province (also Kanmantoo Trough) is a deeply subsident rift formed in early Cambrian. It forms the eastern and southern portion of the Stansbury Basin, extending to the Glenelg River region of Victoria. Most rocks were highly deformed and experienced moderate to high grade metamorphism during the Delamerian Orogeny. [18] [19]

Arrowie Basin

The Arrowie Basin is second of the two known Cambrian basins of the Adelaide Superbasin. It extends from the Stuart Shelf in the west across the Flinders Ranges to western New South Wales where it forms part of the Neoproterozoic–Cambrian cover on the Curnamona Province. [18]

Yalkalpo Sub-basin

The Yalkalpo Sub-basin is the easternmost part of the Arrowie Basin. Its western boundary is the basement high Benagerie Ridge of the Curnamona Province. [18]

Lithostratigraphy

The lithostratigraphy of the Adelaide Superbasin is divided into three supergroups [20] with further division into numerous groups and subgroups and over 140 formations. [1] [3] [6] [21] [22] [23] [24]

Generalised Lithostratigraphy of the Adelaide Superbasin
GeochronologySouth AustraliaNew South Wales
Eon Era Period Local Chronostratigraphy (historical – not in use) Supergroup Groups Subgroups Groups Subgroups
Phanerozoic Palaeozoic Cambrian Unconformity overlaid by Permian glacial sediments
Mid-lateMoralana SupergroupLake Frome Group / Kanmantoo Group / Yorke Group
EarlyKanmantoo Group / Yorke Group / Kangaroo Island GroupKeynes Subgroup / Bollaparudda Subgroup
Normanville Group / Hawker Group / Pavy Group / Kangaroo Island Group
Unconformity
Proterozoic Neoproterozoic Ediacaran MarinoanHeysen SupergroupWilpena GroupPound SubgroupFarnell Group
Depot Springs Subgroup
Aruhna Subgroup
Sandison Subgroup
Unconformity
Cryogenian Umberatana GroupYerelina SubgroupToorrowangee GroupTeamsters Creek Subgroup
Upalinna Subgroup
UnconformityEuriowie Subgroup
SturtianNepouie Subgroup
UnconformityUnconformity
Yudnamutana SubgroupYancowinna Subgroup
Unconformity
Tonian Warrina SupergoupBurra GroupBelair SubgroupUnconformity
TorrensianBungarider Subgroup
Mundallio Subgroup
Emeroo Subgroup
Unconformity
WillouranCallanna GroupCurdimurka SubgroupPoolamacca GroupUnconformity
Arkaroola SubgroupWendalpa Subgroup / Pintapah Subgroup
Mesoproterozoic Unconformity underlain by metamorphosed Mesoproterozoic basement (Gawler Craton, Curnamona Province)

Delamerian orogeny

Sedimentation in the Adelaide Superbasin ended in the middle Cambrian, when tectonic inversion occurred along the eastern margin of Neoproterozoic and Cambrian cratonic Australia and the margin became a subduction zone of the Palaeo-Pacific. [1] [15] After this time the region experienced an orogeny (mountain-building period) extending into the Ordovician. Foden et al. (2006) suggest that this orogeny lasted from ~514 Ma to 490 Ma. This event is called the Delamerian Orogeny, named after Delamere, a small town on the Fleurieu Peninsula where evidence was found for the event. The orogeny caused substantial folding, buckling, and faulting of the strata, and resulted in the creation of a major mountain range, the eroded stumps of which can today be seen as the Mount Lofty and Flinders Ranges. Not all of the basin experienced tectonic activity; the deposits on the Stuart Shelf and Coombalarnie Platform to the north-west and north-east remained undisturbed (and still do today).

Accompanying this folding and faulting were several intrusions: the granites at Victor Harbor were intruded at this time, as were those at Palmer in the eastern South Mount Lofty Ranges. [15] [16]

Fossil content

Fossils of the earliest Animalia are found in the Adelaide Superbasin. The first of these might be the probable sponges found in the Trezona Formation, [25] although the first confirmed [26] Animalia are the world-renowned Ediacaran fauna, named for the Ediacara Hills where they were first discovered in South Australia in 1946. [27] They occur at the end of the Neoproterozoic, and in 2004 the location gave its name to the last geological period of the era, the Ediacaran. [28]

Recent geological history

The ranges formed during the Delamerian orogeny continue to erode, and intra-plate subsidence is occurring. In the South Mount Lofty Ranges this has resulted in rifting and the formation of graben structures, creating the long parallel faults which shape the Adelaide Plains.

See also

Related Research Articles

<span class="mw-page-title-main">Neoproterozoic</span> Third and last era of the Proterozoic Eon

The Neoproterozoic Era is the unit of geologic time from 1 billion to 538.8 million years ago.

Rodinia was a Mesoproterozoic and Neoproterozoic supercontinent that assembled 1.26–0.90 billion years ago (Ga) and broke up 750–633 million years ago (Ma). Valentine & Moores 1970 were probably the first to recognise a Precambrian supercontinent, which they named "Pangaea I." It was renamed "Rodinia" by McMenamin & McMenamin 1990 who also were the first to produce a reconstruction and propose a temporal framework for the supercontinent.

<span class="mw-page-title-main">Iapetus Ocean</span> Ocean that existed in the late Neoproterozoic and early Paleozoic eras

The Iapetus Ocean existed in the late Neoproterozoic and early Paleozoic eras of the geologic timescale. It lay in the southern hemisphere, between the paleocontinents of Laurentia, Baltica and Avalonia. The ocean disappeared with the Acadian, Caledonian and Taconic orogenies, when these three continents joined to form one big landmass called Euramerica. The "southern" Iapetus Ocean has been proposed to have closed with the Famatinian and Taconic orogenies, meaning a collision between Western Gondwana and Laurentia.

<span class="mw-page-title-main">Congo Craton</span> Precambrian craton that with four others makes up the modern continent of Africa

The Congo Craton, covered by the Palaeozoic-to-recent Congo Basin, is an ancient Precambrian craton that with four others makes up the modern continent of Africa. These cratons were formed between about 3.6 and 2.0 billion years ago and have been tectonically stable since that time. All of these cratons are bounded by younger fold belts formed between 2.0 billion and 300 million years ago.

<span class="mw-page-title-main">Geology of Australia</span>

The geology of Australia includes virtually all known rock types, spanning a geological time period of over 3.8 billion years, including some of the oldest rocks on earth. Australia is a continent situated on the Indo-Australian Plate.

<span class="mw-page-title-main">Amadeus Basin</span> Intracratonic sedimentary province in Australia

The Amadeus Basin is a large (~170,000 km2) intracratonic sedimentary basin in central Australia, lying mostly within the southern Northern Territory, but extending into the state of Western Australia.

<span class="mw-page-title-main">Geology of Norway</span>

The geology of Norway encompasses the history of Earth that can be interpreted by rock types found in Norway, and the associated sedimentological history of soils and rock types.

<span class="mw-page-title-main">Laurentia</span> Craton forming the geological core of North America

Laurentia or the North American Craton is a large continental craton that forms the ancient geological core of North America. Many times in its past, Laurentia has been a separate continent, as it is now in the form of North America, although originally it also included the cratonic areas of Greenland and the Hebridean Terrane in northwest Scotland. During other times in its past, Laurentia has been part of larger continents and supercontinents and consists of many smaller terranes assembled on a network of early Proterozoic orogenic belts. Small microcontinents and oceanic islands collided with and sutured onto the ever-growing Laurentia, and together formed the stable Precambrian craton seen today.

The Marinoan glaciation, sometimes also known as the Varanger glaciation, was a period of worldwide glaciation. Its beginning is poorly constrained, but occurred no earlier than 654.5 Ma. It ended approximately 632.3 ± 5.9 Ma during the Cryogenian period. This glaciation possibly covered the entire planet, in an event called the Snowball Earth. The end of the glaciation was caused by volcanic release of carbon dioxide and dissolution of gas hydrates and might have been hastened by the release of methane from equatorial permafrost.

<span class="mw-page-title-main">Carolina terrane</span> Exotic terrane from central Georgia to central Virginia in the United States

The Carolina Terrane, also called the Carolina Superterrane or Carolinia, is an exotic terrane running ~370 miles (600 km) approximately North-South from central Georgia to central Virginia in the United States. It constitutes a major part of the eastern Piedmont Province.

<span class="mw-page-title-main">Geology of South Australia</span>

South Australia is an Australian state, situated in the southern central part of the country, and featuring some low-lying mountain ranges, the most significant being the Mount Lofty Ranges, which extend into the state's capital city, Adelaide, which comprises most of the state's population. Adelaide is situated on the eastern shores of Gulf St Vincent, on the Adelaide Plains, north of the Fleurieu Peninsula, between Gulf St Vincent and the low-lying Mount Lofty Ranges. The state of South Australia, which stretches along the coast of the continent and has boundaries with every other state in Australia, with the exception of the Australian Capital Territory and Tasmania. The Western Australia border has a history with South Australia, involving the South Australian Government Astronomer, Dodwell and the Western Australian Government Astronomer, Curlewis in the 1920s to mark the border on the ground.

The Sturtian glaciation was a worldwide glaciation during the Cryogenian Period when the Earth experienced repeated large-scale glaciations. As of January 2023, the Sturtian glaciation is thought to have lasted from c. 717 Ma to c. 660 Ma, a time span of approximately 57 million years. It is hypothesised to have been a Snowball Earth event, or contrastingly multiple regional glaciations, and is the longest and most severe known glacial event preserved in the geologic record, after the much earlier Huronian glaciation.

<span class="mw-page-title-main">East Antarctic Shield</span> Cratonic rock body which makes up most of the continent Antarctica

The East Antarctic Shield or Craton is a cratonic rock body that covers 10.2 million square kilometers or roughly 73% of the continent of Antarctica. The shield is almost entirely buried by the East Antarctic Ice Sheet that has an average thickness of 2200 meters but reaches up to 4700 meters in some locations. East Antarctica is separated from West Antarctica by the 100–300 kilometer wide Transantarctic Mountains, which span nearly 3,500 kilometers from the Weddell Sea to the Ross Sea. The East Antarctic Shield is then divided into an extensive central craton that occupies most of the continental interior and various other marginal cratons that are exposed along the coast.

<span class="mw-page-title-main">Terra Australis Orogen</span>

The Terra Australis Orogen (TAO) was a late Neoproterozoic- to Paleozoic-age accretionary orogen that ringed the ancient, active southern margin of the supercontinents Rodinia and later Pannotia. This vast orogenic belt stretched for c. 18,000 km (11,000 mi) along-strike and involved, from west to east, landmasses belonging to the modern-day Andean margin of South America, the South African Cape, West Antarctica, Victoria Land in East Antarctica, Eastern Australia, Tasmania, and New Zealand. The formation of the Terra Australis Orogen is associated with the breakup of Rodinia at the end of the Neoproterozoic Era and the creation of Panthalassa, the paleo-Pacific Ocean, and it was succeeded by the Gondwanide orogeny with the formation of the supercontinent Pangea in the middle Paleozoic Era.

<span class="mw-page-title-main">Tectonic evolution of the Aravalli Mountains</span> Overview article

The Aravalli Mountain Range is a northeast-southwest trending orogenic belt in the northwest part of India and is part of the Indian Shield that was formed from a series of cratonic collisions. The Aravalli Mountains consist of the Aravalli and Delhi fold belts, and are collectively known as the Aravalli-Delhi orogenic belt. The whole mountain range is about 700 km long. Unlike the much younger Himalayan section nearby, the Aravalli Mountains are believed much older and can be traced back to the Proterozoic Eon. They are arguably the oldest geological feature on Earth. The collision between the Bundelkhand craton and the Marwar craton is believed to be the primary mechanism for the development of the mountain range.

<span class="mw-page-title-main">Tectonic evolution of Patagonia</span>

Patagonia comprises the southernmost region of South America, portions of which lie on either side of the Argentina-Chile border. It has traditionally been described as the region south of the Rio, Colorado, although the physiographic border has more recently been moved southward to the Huincul fault. The region's geologic border to the north is composed of the Rio de la Plata craton and several accreted terranes comprising the La Pampa province. The underlying basement rocks of the Patagonian region can be subdivided into two large massifs: the North Patagonian Massif and the Deseado Massif. These massifs are surrounded by sedimentary basins formed in the Mesozoic that underwent subsequent deformation during the Andean orogeny. Patagonia is known for its vast earthquakes and the damage they cause.

The Officer Basin is an intracratonic sedimentary basin that covers roughly 320,000 km2 along the border between southern and western Australia. Exploration for hydrocarbons in this basin has been sparse, but the geology has been examined for its potential as a hydrocarbon reservoir. This basin's extensive depositional history, with sedimentary thicknesses exceeding 6 km and spanning roughly 350 Ma during the Neoproterozoic, make it an ideal candidate for hydrocarbon production.

<span class="mw-page-title-main">Geology of the Ellsworth Mountains</span> Geology of the Ellsworth Mountains, Antarctica

The geology of the Ellsworth Mountains, Antarctica, is a rock record of continuous deposition that occurred from the Cambrian to the Permian periods, with basic igneous volcanism and uplift occurring during the Middle to Late Cambrian epochs, deformation occurring in the Late Permian period or early Mesozoic era, and glacier formation occurring in the Cretaceous period and Cenozoic era. The Ellsworth Mountains are located within West Antarctica at 79°S, 85°W. In general, it is made up of mostly rugged and angular peaks such as the Vinson Massif, the highest mountain in Antarctica.

The Knoydartian Orogeny is a Tonian tectonic and metamorphic event, or group of events, that is recognised in the rocks of the Wester Ross and Loch Ness supergroups of the Scottish Highlands. It is dated to about 820–725 Ma, predating the deposition of the Cryogenian to Cambrian Dalradian Supergroup. It is named after Knoydart, one of the localities where the event was first recognised.

References

  1. 1 2 3 4 5 6 7 8 Lloyd, Jarred C.; Blades, Morgan L.; Counts, John W.; Collins, Alan S.; Amos, Kathryn J.; Wade, Benjamin P.; Hall, James W.; Hore, Stephen; Ball, Ashleigh L.; Shahin, Sameh; Drabsch, Matthew (8 July 2020). "Neoproterozoic Geochronology and Provenance of the Adelaide Superbasin". Precambrian Research. 350: 105849. Bibcode:2020PreR..35005849L. doi:10.1016/j.precamres.2020.105849. ISSN   0301-9268. S2CID   225530500.
  2. Mawson, Douglas; Sprigg, Reginald (1950). "Subdivision of the Adelaide System". Australian Journal of Science. 13 (3): 69–72.
  3. 1 2 3 Preiss, Wolfgang V., ed. (1987). The Adelaide Geosyncline : late Proterozoic stratigraphy, sedimentation, palaeontology, and tectonics. Bulletin 54. Geological Survey of South Australia. Adelaide: Dept. of Mines and Energy. ISBN   0-7243-7845-6. OCLC   27539001.
  4. 1 2 3 Preiss, Wolfgang V. (2000). "The Adelaide Geosyncline of South Australia and its significance in Neoproterozoic continental reconstruction". Precambrian Research. 100 (1–3): 21–63. Bibcode:2000PreR..100...21P. doi:10.1016/S0301-9268(99)00068-6.
  5. Veevers, J. J.; Walter, M. R.; Scheibner, E. (1997). "Neoproterozoic Tectonics of Australia-Antarctica and Laurentia and the 560 Ma Birth of the Pacific Ocean Reflect the 400 M.Y. Pangean Supercycle". The Journal of Geology. 105 (2): 225–242. Bibcode:1997JG....105..225V. doi:10.1086/515914. ISSN   0022-1376. S2CID   140652348.
  6. 1 2 3 Powell, C.McA.; Preiss, Wolfgang V.; Gatehouse, Colin G.; Krapez, B.; Li, Zheng-Xiang (1994). "South Australian record of a Rodinian epicontinental basin and its mid-neoproterozoic breakup (~700 Ma) to form the Palaeo-Pacific Ocean". Tectonophysics. 237 (3–4): 113–140. Bibcode:1994Tectp.237..113P. doi:10.1016/0040-1951(94)90250-X.
  7. Moores, E. M. (1991). "Southwest U.S.-East Antarctic (SWEAT) connection: A hypothesis". Geology. 19 (5): 425. Bibcode:1991Geo....19..425M. doi:10.1130/0091-7613(1991)019<0425:SUSEAS>2.3.CO;2.
  8. Dalziel, Ian W.D. (1991). "Pacific margins of Laurentia and East Antarctica-Australia as a conjugate rift pair: Evidence and implications for an Eocambrian supercontinent". Geology. 19 (6): 598. Bibcode:1991Geo....19..598D. doi:10.1130/0091-7613(1991)019<0598:PMOLAE>2.3.CO;2.
  9. Och, Lawrence M.; Shields-Zhou, Graham A. (2012). "The Neoproterozoic oxygenation event: Environmental perturbations and biogeochemical cycling". Earth-Science Reviews. 110 (1–4): 26–57. Bibcode:2012ESRv..110...26O. doi:10.1016/j.earscirev.2011.09.004.
  10. GOSTIN, V. A.; HAINES, P. W.; JENKINS, R. J. F.; COMPSTON, W.; WILLIAMS, I. S. (11 July 1986). "Impact Ejecta Horizon Within Late Precambrian Shales, Adelaide Geosyncline, South Australia". Science. 233 (4760): 198–200. Bibcode:1986Sci...233..198G. doi:10.1126/science.233.4760.198. ISSN   0036-8075. PMID   17737290. S2CID   11307364.
  11. Sprigg, Reginald C. (1948). "Jellyfish from the Basal Cambrian in South Australia". Nature. 161 (4093): 568–569. Bibcode:1948Natur.161..568S. doi:10.1038/161568a0. ISSN   0028-0836. S2CID   4098098.
  12. Droser, Mary L.; Gehling, James G. (21 April 2015). "The advent of animals: The view from the Ediacaran". Proceedings of the National Academy of Sciences. 112 (16): 4865–4870. Bibcode:2015PNAS..112.4865D. doi: 10.1073/pnas.1403669112 . ISSN   0027-8424. PMC   4413262 . PMID   25901306.
  13. 1 2 Counts, John W. (2017). The Adelaide Rift Complex in the Flinders Ranges: geologic history, past investigations and relevant analogues. Report Book, no. 2017/00016. Geological Survey of South Australia. Department of Premier and Cabinet. Adelaide, South Australia.https://sarigbasis.pir.sa.gov.au/WebtopEw/ws/samref/sarig1/wcir/Record?r=0&m=1&w=catno=2039731
  14. Preiss, Wolfgang V.; Alexander, Elinor M.; Cowley, Wayne M.; Schwarz, Michael P. (2002). "Towards defining South Australia's geological provinces and sedimentary basins". MESA. 27: 39–52.
  15. 1 2 3 Foden, John; Elburg, Marlina A; Dougherty-Page, Jon; Burtt, Andrew (2006). "The Timing and Duration of the Delamerian Orogeny: Correlation with the Ross Orogen and Implications for Gondwana Assembly". The Journal of Geology. 114 (2): 189–210. Bibcode:2006JG....114..189F. doi:10.1086/499570. hdl: 2440/23647 . ISSN   0022-1376. S2CID   131724740.
  16. 1 2 Foden, John; Elburg, Marlina; Turner, Simon; Clark, Chris; Blades, Morgan L.; Cox, Grant; Collins, Alan S.; Wolff, Keryn; George, Christian (2020). "Cambro-Ordovician magmatism in the Delamerian orogeny: Implications for tectonic development of the southern Gondwanan margin". Gondwana Research. 81: 490–521. Bibcode:2020GondR..81..490F. doi:10.1016/j.gr.2019.12.006. S2CID   213741512.
  17. Cawood, Peter A. (2005). "Terra Australis Orogen: Rodinia breakup and development of the Pacific and Iapetus margins of Gondwana during the Neoproterozoic and Paleozoic". Earth-Science Reviews. 69 (3–4): 249–279. Bibcode:2005ESRv...69..249C. doi:10.1016/j.earscirev.2004.09.001.
  18. 1 2 3 4 5 Preiss, Wolfgang V.; Alexander, Elinor M.; Cowley, Wayne M.; Schwarz, Michael P. (2002). "Towards defining South Australia's geological provinces and sedimentary basins". MESA Journal. 27: 39–52.
  19. Belperio, Antonio P.; Preiss, Wolfgang V.; Fairclough, Martin C.; Gatehouse, Colin G.; Gum, Justin C.; Hough, J.; Burtt, Andrew (1998). "Tectonic and metallogenic framework of the Cambrian Stansbury Basin - Kanmantoo Trough, South Australia". ASGO Journal of Australian Geology and Geophysics. 17 (3): 183–200.
  20. Preiss, Wolfgang V. (1982). "Supergroup classification in the Adelaide Geosyncline". Transactions of the Royal Society of South Australia. 106: 81–83.
  21. Drexel, John F.; Preiss, Wolfgang V.; Parker, A.J., eds. (1993). The Geology of South Australia. Geological Survey of South Australia. Adelaide: Mines and Energy South Australia. ISBN   0-7308-4147-2. OCLC   30439436.
  22. Lloyd, Jarred (2020), Lithostratigraphic Correlation Chart of the Adelaide Superbasin (Neoproterozoic), Figshare, doi:10.6084/m9.figshare.11812047 , retrieved 16 July 2020
  23. Cooper, P.F.; Tuckwell, K.D.; Gilligan, L.B.; Meares, R.M.D. (1974). "Geology of the Torrowangee and Fowlers Gap 1:100,000 Sheets". Geological Survey of New South Wales, Department of Mines, Sydney, New South Wales.
  24. Preiss, Wolfgang V.; Cowley, Wayne M. (1999). "Genetic stratigraphy and revised lithostratigraphic classification of the Burra Group in the Adelaide Geosyncline". MESA. 14: 30–40.
  25. Maloof, Adam C.; Rose, Catherine V.; Beach, Robert; Samuels, Bradley M.; Calmet, Claire C.; Erwin, Douglas H.; Poirier, Gerald R.; Yao, Nan; Simons, Frederik J. (2010). "Possible animal-body fossils in pre-Marinoan limestones from South Australia". Nature Geoscience. 3 (9): 653–659. Bibcode:2010NatGe...3..653M. doi:10.1038/ngeo934. ISSN   1752-0894.
  26. Bobrovskiy, Ilya; Hope, Janet M.; Ivantsov, Andrey; Nettersheim, Benjamin J.; Hallmann, Christian; Brocks, Jochen J. (21 September 2018). "Ancient steroids establish the Ediacaran fossil Dickinsonia as one of the earliest animals". Science. 361 (6408): 1246–1249. Bibcode:2018Sci...361.1246B. doi: 10.1126/science.aat7228 . hdl: 1885/230014 . ISSN   0036-8075. PMID   30237355. S2CID   52306108.
  27. Sprigg, Reg. C. (1948). "Jellyfish from the Basal Cambrian in South Australia". Nature. 161 (4093): 568–569. Bibcode:1948Natur.161..568S. doi:10.1038/161568a0. ISSN   0028-0836. S2CID   4098098.
  28. Knoll, Andrew; Walter, Malcolm; Narbonne, Guy; Christie-Blick, Nicholas (1 March 2006). "The Ediacaran Period: a new addition to the geologic time scale". Lethaia. 39 (1): 13–30. Bibcode:2006Letha..39...13K. doi:10.1080/00241160500409223. ISSN   0024-1164.

Further reading