Chronology of continents

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A continent is a large geographical region defined by the continental shelves and the cultures on the continent. [1] In the modern day, there are seven continents. However, there have been more continents throughout history. Vaalbara was the first supercontinent. [2] Europe is the newest continent. [3] Geologists have predicted that certain continents will appear, these being Pangaea Proxima, Novopangaea, Aurica, and Amasia.

List of Continents

Name Era Time before present ImageReference
Vaalbara Eoarchean 3.6-2.7 Ga Diagram of the (conjectured) Vaalbara ancient continent.png [2]
Ur Paleoarchean 3.1 Ga Diagram of possible Ur Continent of the (conjectured) Eoarchean Era.png [4]
Kenorland Neoarchean 2.7 Ga Kenorland.jpg [5]
Arctica Neoarchean2.565 Ga 2400 Ma paleoglobe.png [6]
Columbia Paleoproterozoic 2.1-1.5 Ga Columbia1600.png [7]
Atlantica Paleoproterozoic2.0 Ga Atlantica-2Ga.svg [8]
Nena Paleoproterozoic1.9 Ga [9]
Baltica Paleoproterozoic1.8 Ga Baltica outline.png [10]
Rodinia Neoproterozoic 1100-633 Ma [11]
Avalonia Neoproterozoic750 Ma AVALONIA.svg [12]
Pannotia Neoproterozoic500-600 Ma Panotiaggg.jpg [13]
Pampia Neoproterozoic555-515 Ma [11]
Gondwana Neoproterozoic550 Ma Gondwana 420 Ma.png [14]
Cimmeria Neoproterozoic550 Ma 249 global.png [15]
Laurasia Neoproterozoic550 Ma Laurasia 200Ma.jpg [16]
Cuyania Paleozoic ~420-390 Ma [17]
Chilenia Paleozoic~420-390 Ma [18]
Pangaea Paleozoic335 Ma Pangaea 200Ma.jpg [16]
Africa Paleozoic300 Ma Africa (orthographic projection).svg [19]
South America Mesozoic 225 Ma South America (orthographic projection).svg [20]
North America Mesozoic200 Ma BK North America (orthographic projection).png [21]
Mauritia Mesozoic70-60 Ma Early Jurassic breakup of Gondwana.png [22]
Asia Mesozoic66 Ma Asia (orthographic projection).svg [23]
Australia Cenozoic 10 Ma Map of Australia and New Zealand.png [24]
Europe Cenozoic5 Ma World Association of Girl Guides and Girl Scouts-Europe Region.svg [25]
Pangaea Proxima ~250 myf PangeaUltimaRoughEstimation.png [3]
Novopangaea ~250 myf Image 200.00my (Novopangea).jpg [26]
Aurica ~250 myf [26]
Amasia ~250 myf Image 100.00MPVF Amasia.jpg [26]

Related Research Articles

The Precambrian is the earliest part of Earth's history, set before the current Phanerozoic Eon. The Precambrian is so named because it preceded the Cambrian, the first period of the Phanerozoic Eon, which is named after Cambria, the Latinised name for Wales, where rocks from this age were first studied. The Precambrian accounts for 88% of the Earth's geologic time.

<span class="mw-page-title-main">Supercontinent</span> Landmass comprising more than one continental core, or craton

In geology, a supercontinent is the assembly of most or all of Earth's continental blocks or cratons to form a single large landmass. However, some geologists use a different definition, "a grouping of formerly dispersed continents", which leaves room for interpretation and is easier to apply to Precambrian times. To separate supercontinents from other groupings, a limit has been proposed in which a continent must include at least about 75% of the continental crust then in existence in order to qualify as a supercontinent.

Rodinia was a Mesoproterozoic and Neoproterozoic supercontinent that assembled 1.26–0.90 billion years ago and broke up 750–633 million years ago. 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">Proterozoic</span> Geologic eon, 2500–539 million years ago

The Proterozoic is the third of the four geologic eons of Earth's history, spanning the time interval from 2500 to 538.8 Mya, the longest eon of the Earth's geologic time scale. It is preceded by the Archean and followed by the Phanerozoic, and is the most recent part of the Precambrian "supereon".

<span class="mw-page-title-main">Laurasia</span> Northern landmass that formed part of the Pangaea supercontinent

Laurasia was the more northern of two large landmasses that formed part of the Pangaea supercontinent from around 335 to 175 million years ago (Mya), the other being Gondwana. It separated from Gondwana 215 to 175 Mya during the breakup of Pangaea, drifting farther north after the split and finally broke apart with the opening of the North Atlantic Ocean c. 56 Mya. The name is a portmanteau of Laurentia and Asia.

<span class="mw-page-title-main">Mesoproterozoic</span> Second era of the Proterozoic Eon

The Mesoproterozoic Era is a geologic era that occurred from 1,600 to 1,000 million years ago. The Mesoproterozoic was the first era of Earth's history for which a fairly definitive geological record survives. Continents existed during the preceding era, but little is known about them. The continental masses of the Mesoproterozoic were more or less the same ones that exist today, although their arrangement on the Earth's surface was different.

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

The Iapetus Ocean was an ocean that existed in the late Neoproterozoic and early Paleozoic eras of the geologic timescale. The Iapetus Ocean was situated 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">Arctica</span> Ancient continent in the Neoarchean era

Arctica, or Arctida was an ancient continent which formed approximately 2.565 billion years ago in the Neoarchean era. It was made of Archaean cratons, including the Siberian Craton, with its Anabar/Aldan shields in Siberia, and the Slave, Wyoming, Superior, and North Atlantic cratons in North America. Arctica was named by Rogers 1996 because the Arctic Ocean formed by the separation of the North American and Siberian cratons. Russian geologists writing in English call the continent "Arctida" since it was given that name in 1987, alternatively the Hyperborean craton, in reference to the hyperboreans in Greek mythology.

<span class="mw-page-title-main">Pannotia</span> Hypothesized Neoproterozoic supercontinent from the end of the Precambrian

Pannotia, also known as the Vendian supercontinent, Greater Gondwana, and the Pan-African supercontinent, was a relatively short-lived Neoproterozoic supercontinent that formed at the end of the Precambrian during the Pan-African orogeny, during the Cryogenian period and broke apart 560 Ma with the opening of the Iapetus Ocean, in the late Ediacaran and early Cambrian. Pannotia formed when Laurentia was located adjacent to the two major South American cratons, Amazonia and Río de la Plata. The opening of the Iapetus Ocean separated Laurentia from Baltica, Amazonia, and Río de la Plata. In 2022 the whole concept of Pannotia has been put into question by scientists who argue its existence is not supported by geochronology, "the supposed landmass had begun to break up well before it was fully assembled".

<span class="mw-page-title-main">Baltica</span> Late-Proterozoic to early-Palaeozoic continent

Baltica is a paleocontinent that formed in the Paleoproterozoic and now constitutes northwestern Eurasia, or Europe north of the Trans-European Suture Zone and west of the Ural Mountains. The thick core of Baltica, the East European Craton, is more than three billion years old and formed part of the Rodinia supercontinent at c.Ga.

<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">Supercontinent cycle</span> Quasi-periodic aggregation and dispersal of Earths continental crust

The supercontinent cycle is the quasi-periodic aggregation and dispersal of Earth's continental crust. There are varying opinions as to whether the amount of continental crust is increasing, decreasing, or staying about the same, but it is agreed that the Earth's crust is constantly being reconfigured. One complete supercontinent cycle is said to take 300 to 500 million years. Continental collision makes fewer and larger continents while rifting makes more and smaller continents.

<span class="mw-page-title-main">Vaalbara</span> Archaean supercontinent from about 3.6 to 2.7 billion years ago

Vaalbara is a hypothetical Archean supercontinent consisting of the Kaapvaal Craton and the Pilbara Craton. E. S. Cheney derived the name from the last four letters of each craton's name. The two cratons consist of crust dating from 2.7 to 3.6 Gya, which would make Vaalbara one of Earth's earliest supercontinents.

<span class="mw-page-title-main">Gondwana</span> Neoproterozoic to Cretaceous landmass

Gondwana was a large landmass, sometimes referred to as a supercontinent. It was formed by the accretion of several cratons, beginning c. 800 to 650Ma with the East African Orogeny, the collision of India and Madagascar with East Africa, and was completed c.600 to 530 Ma with the overlapping Brasiliano and Kuunga orogenies, the collision of South America with Africa, and the addition of Australia and Antarctica, respectively. Eventually, Gondwana became the largest piece of continental crust of the Palaeozoic Era, covering an area of about 100,000,000 km2 (39,000,000 sq mi), about one-fifth of the Earth's surface. It fused with Euramerica during the Carboniferous to form Pangea. It began to separate from northern Pangea (Laurasia) during the Triassic, and started to fragment during the Early Jurassic. The final stages of break-up, involving the separation of Antarctica from South America and Australia, occurred during the Paleogene (from around 66 to 23 million years ago. Gondwana was not considered a supercontinent by the earliest definition, since the landmasses of Baltica, Laurentia, and Siberia were separated from it. To differentiate it from the Indian region of the same name, it is also commonly called Gondwanaland.

<span class="mw-page-title-main">Laurentia</span> A large continental craton that forms the ancient geological core of the North American continent

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 also the northwestern part of Scotland, known as the Hebridean Terrane. During other times in its past, Laurentia has been part of larger continents and supercontinents and itself 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.

<span class="mw-page-title-main">Pangaea</span> Supercontinent from the late Paleozoic to early Mesozoic eras

Pangaea or Pangea was a supercontinent that existed during the late Paleozoic and early Mesozoic eras. It assembled from the earlier continental units of Gondwana, Euramerica and Siberia during the Carboniferous approximately 335 million years ago, and began to break apart about 200 million years ago, at the end of the Triassic and beginning of the Jurassic. In contrast to the present Earth and its distribution of continental mass, Pangaea was centred on the equator and surrounded by the superocean Panthalassa and the Paleo-Tethys and subsequent Tethys Oceans. Pangaea is the most recent supercontinent to have existed and the first to be reconstructed by geologists.

The Precordillera Terrane or Cuyania was an ancient microcontinent or terrane whose history affected many of the older rocks of Cuyo in Argentina. It was separated by oceanic crust from the Chilenia terrane which accreted into it at ~420-390 Ma when Cuyania was already amalgamated with Gondwana. The hypothesized Mejillonia Terrane in the coast of northern Chile is considered by some geologists to be a single block with Cuyania.

A paleocontinent or palaeocontinent is a distinct area of continental crust that existed as a major landmass in the geological past. There have been many different landmasses throughout Earth's time. They range in sizes, some are just a collection of small microcontinents while others are large conglomerates of crust. As time progresses and sea levels rise and fall more crust can be exposed making way for larger landmasses. The continents of the past shaped the evolution of organisms on Earth and contributed to the climate of the globe as well. As landmasses break apart, species are separated and those that were once the same now have evolved to their new climate. The constant movement of these landmasses greatly determines the distribution of organisms on Earth's surface. This is evident with how similar fossils are found on completely separate continents. Also, as continents move, mountain building events (orogenies) occur, causing a shift in the global climate as new rock is exposed and then there is more exposed rock at higher elevations. This causes glacial ice expansion and an overall cooler global climate. The movement of the continents greatly affects the overall dispersal of organisms throughout the world and the trend in climate throughout Earth's history. Examples include Laurentia, Baltica and Avalonia, which collided together during the Caledonian orogeny to form the Old Red Sandstone paleocontinent of Laurussia. Another example includes a collision that occurred during the late Pennsylvanian and early Permian time when there was a collision between the two continents of Tarimsky and Kirghiz-Kazakh. This collision was caused because of their askew convergence when the paleoceanic basin closed.

<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.

References

  1. "Continent". National Geographic Society. 2011-09-20. Archived from the original on 2021-03-03. Retrieved 2021-02-01.
  2. 1 2 Zegers, T. E.; de Wit, M. J.; White, S. H. (1998). "Vaalbara, Earth's oldest assembled continent? A combined. structural, geochronological, and palaeomagnetic test" (PDF). Terra Nova. 10(5): 250–259.
  3. 1 2 Willams, Caroline; Nield, Ted (2007). "Earth's next supercontinent". New Scientist. 196 (2626): 36–40. doi:10.1016/S0262-4079(07)62661-X.
  4. Rogers & Santosh 2003, Rodinia, pp. 363–364
  5. Pesonen, L. J.; Elming, S.-Å.; Mertanen, S.; Pisarevsky, S.; D’Agrella-Filho, M. S.; Meert, J. G.; Schmidt, P. W.; Abrahamsen, N.; Bylund, G. (2003). "Palaeomagnetic configuration of continents during the Proterozoic". Tectonophysics. 375 (1–4): 289–324
  6. Vernikovsky, V. A.; Dobretsov, N. L. (2015). "Geodynamic evolution of the Arctic Ocean and modern problems in geological studies of the Arctic region". Herald of the Russian Academy of Sciences. 85 (3): 206–212.
  7. Zhao, G.; Cawood, P. A.; Wilde, S. A.; Sun, M. (2002). "Review of global 2.1–1.8 Ga orogens: implications for a pre-Rodinia supercontinent". Earth-Science Reviews. 59 (1): 125–162.
  8. Rogers, John J. W. (1996). "A History of Continents in the past Three Billion Years". The Journal of Geology. 104 (1): 91–107. Bibcode:1996JG....104...91R. doi:10.1086/629803. ISSN   0022-1376. S2CID   128776432. Archived from the original on 2021-03-03. Retrieved 2021-02-01.
  9. Gower, Ryan & Rivers 1990, Introduction, p. 2
  10. Cocks, L. R. M.; Torsvik, T. H. (2005). "Baltica from the late Precambrian to mid-Palaeozoic times: the gain and loss of a terrane's identity" (PDF). Earth-Science Reviews. 72 (1–2): 39–66.
  11. 1 2 Gaucher, Claudio; Bossi, Jorge; Blanco, Gonzalo (2009). "Palaeogeography". Neoproterozoic-Cambrian Tectonics, Global Change and Evolution: A Focus on South Western Gondwana. Developments in Precambrian Geology. 16. pp. 131–41. doi:10.1016/S0166-2635(09)01609-0. ISBN   978-0-444-53249-7.
  12. Murphy, J. B.; Pisarevsky, S. A.; Nance, R. D.; Keppie, J. D. (2001). Jessell, M. J. (ed.). "Animated history of Avalonia in Neoproterozoic - Early Proterozoic". General Contributions. Journal of the Virtual Explorer. 3: 45–58. doi:10.3809/jvirtex.2001.00026. Retrieved 28 November 2015.
  13. Scotese 2009, Reconstruction of Rodinia and Pannotia, p. 68
  14. Bradley, D.C. (2011). "Secular Trends in the Geologic Record and the Supercontinent Cycle". Earth-Science Reviews. 108 (1–2): 16–33. CiteSeerX 10.1.1.715.6618. doi:10.1016/j.earscirev.2011.05.003.
  15. Buchs, D. M.; Bagheri, S.; Martin, L.; Hermann, J.; Arculus, R. (2013). "Paleozoic to Triassic ocean opening and closure preserved in Central Iran: Constraints from the geochemistry of meta-igneous rocks of the Anarak area". Lithos . 172: 267–287.
  16. 1 2 Blakey 2003, Assembly of Western Pangaea: Carboniferous–Permian, pp. 453–454; Assembly of Eastern Pangaea: Late Permian–Jurassic, p. 454; Fig. 10, p. 454
  17. Rapalini 2005
  18. Rapalini, A.E. 2005. The accretionary history of southern South America from the latest Proterozoic to the Late Palaeozoic: some palaeomagnetic constraints. From: Vaughan, A. R M., Leat, P. T. & Pankhurst, R. J, (eds). Terrane Processes at the Margins of Gondwana. Geological Society, London, Special Publications, 246, 305-328.
  19. "Africa - Geologic history". Encyclopedia Britannica. Archived from the original on 2021-01-25. Retrieved 2021-02-01.
  20. "South America - Geologic history". Encyclopedia Britannica. Archived from the original on 2020-05-07. Retrieved 2021-02-04.
  21. "North America - Tectonic evolution". Encyclopedia Britannica. Archived from the original on 2015-05-03. Retrieved 2021-02-01.
  22. Torsvik, Trond H.; Amundsen, Hans; Hartz, Ebbe H.; Corfu, Fernando; Kusznir, Nick; Gaina, Carmen; Doubrovine, Pavel V.; Steinberger, Bernhard; Ashwal, Lewis D.; Jamtveit, Bjørn (24 February 2013). "A Precambrian microcontinent in the Indian Ocean" (PDF). Nature Geoscience . 6 (3): 223–227. doi:10.1038/ngeo1736. hdl:10852/62002. ISSN 1752-0894. Retrieved 5 December 2015.
  23. "Asia - Geologic history". Encyclopedia Britannica. Archived from the original on 2008-11-18. Retrieved 2021-02-01.
  24. "Australia - Geologic history". Encyclopedia Britannica. Archived from the original on 2015-05-02. Retrieved 2021-02-01.
  25. "Europe - Geologic history". Encyclopedia Britannica. Archived from the original on 2014-12-12. Retrieved 2021-02-01.
  26. 1 2 3 Wilkins, Alasdair. "A Geological History of Supercontinents on Planet Earth" at io9. 27 Jan 2011. Accessed 22 July 2014.