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Cryogenian

From Wikipedia, the free encyclopedia
Second period of the Neoproterozoic Era, with major glaciation

Cryogenian
~720 – ~635Ma
A map of Earth as it appeared during the early Cryogenian,c. 690 Ma
Chronology
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Transition fromcyanobacterial toalgal dominated world.[3]
Events of the Cryogenian Period
Vertical axis scale:Millions of years ago
Etymology
Name formalityFormal
Name ratified1990
Usage information
Celestial bodyEarth
Regional usageGlobal (ICS)
Time scale(s) usedICS Time Scale
Definition
Chronological unitPeriod
Stratigraphic unitSystem
Time span formalityFormal
Lower boundary definitionDefined chronometrically with an interim calibrated age of c. 720 Ma. GSSP is in progress.
Lower boundary definition candidatesThe first appearance of widespread glaciation.[6]
Lower boundary GSSP candidate section(s)To be determined
Lower GSSP ratifiedNot formally defined
Upper boundary definition
  • Worldwide distinct cap carbonates.
  • Beginning of a distinctive pattern of secular changes incarbon isotopes.
Upper boundary GSSPEnorama Creek section,Flinders Ranges,South Australia
[https://geohack.toolforge.org/geohack.php?pagename=Cryogenian&params=31.3314_S_138.6334_E_type:landmark_region:AU–SA31°19′53″S138°38′00″E / 31.3314°S 138.6334°E /-31.3314; 138.6334]
Upper GSSP ratifiedMarch 12, 2004[7]: 30 
Atmospheric and climatic data
Mean atmosphericO2 contentc. 12 vol %
(55% of modern)
Mean atmosphericCO2 contentc. 1300ppm
(5 times pre-industrial)
Mean surface temperaturec. 5 °C
(8.5 °C below pre-industrial)
This box:
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TheCryogenian (fromAncient Greek:κρύος,romanizedkrýos, meaning "cold" andγένεσις,romanized:génesis, meaning "birth") is ageologic period that lasted from720 to 635 million years ago.[8] It is the second of the three periods of theNeoproterozoic era, preceded by theTonian and followed by theEdiacaran.

The Cryogenian was a time of drasticclimate changes. After the long environmental stability/stagnation during theBoring Billion, theSturtian glaciation began at the beginning of Cryogenian, freezing the entire planet in a state of severeicehouse climate known as asnowball Earth. After 70 million years it ended, but was quickly followed by another globalice age, theMarinoan glaciation. There is controversy over whether these glaciations indeed covered the entire planet, or whether a band of open sea survived near theequator (i.e. "slushball Earth"), but the extreme climates with massive expanse ofice sheets blocking offsunlight would nevertheless have significantly hinderedprimary production in theshallow seas and caused majormass extinctions andbiosphere turnovers.[citation needed]

Ratification

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The Cryogenian Period was ratified in 1990 by theInternational Commission on Stratigraphy.[9] In contrast to most other time periods, the beginning of the Cryogenian is not linked to a globally observable and documented event. Instead, the base of the period is defined by a fixed rock age, that was originally set at 850 million years,[10] but changed in 2015 to 720 million years.[8]

This could cause ambiguity because estimates of rock age are subject to variable interpretation and laboratory error. For instance, the time scale of theCambrian Period is not reckoned by rock younger than a given age (538.8 million years), but by the appearance of the worldwideTreptichnus pedum diagnostictrace fossil assemblages, which can be recognized in the field without extensive lab testing.[11]

Currently, there is no consensus on what global event is a suitable candidate to mark the start of the Cryogenian Period, but aglobal glaciation would be a likely candidate.[10]

Climate

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Characteristic glacial deposits indicate thatEarth suffered the most severe ice ages in its history during this period (Sturtian and Marinoan). According to Eyles and Young, "Late Proterozoic glaciogenic deposits are known from all the continents. They provide evidence of the most widespread and long-ranging glaciation on Earth." Several glacial periods are evident, interspersed with periods of relatively warm climate, with glaciers reaching sea level in low paleolatitudes.[12]

Glaciers extended and contracted in a series of rhythmic pulses, possibly reaching as far as the equator.[13]

Diamictite of the Elatina Formation in South Australia, formed during the Marinoan glaciation of the late Cryogenian

The Cryogenian is generally considered to be divisible into at least two major worldwide glaciations. TheSturtian glaciation persisted from 720 to 660 million years ago, and theMarinoan glaciation which ended approximately 635 Ma, at the end of the Cryogenian.[14] The deposits of glacialtillite also occur in places that were at low latitudes during the Cryogenian, a phenomenon which led to the hypothesis of deeply frozen planetary oceans called "Snowball Earth".[15] Between the Sturtian and Marinoan glaciations was a so-called "Cryogenian interglacial period" marked by relatively warm climate andanoxic oceans,[16] along with marine transgression.[17]

Paleogeography

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Main article:Rodinia § Geodynamics

Before the start of the Cryogenian, around 750 Ma, thecratons that made up the supercontinentRodinia started to rift apart. The superoceanMirovia began to close while the superoceanPanthalassa began to form. The cratons (possibly) later assembled into another supercontinent calledPannotia, in theEdiacaran.[18]

Eyles and Young state, "Most Neoproterozoic glacial deposits accumulated as glacially influenced marine strata along rifted continental margins or interiors." Worldwide deposition of dolomite might have reduced atmospheric carbon dioxide. The break up along the margins ofLaurentia at about 750Ma occurs at about the same time as the deposition of the Rapitan Group in North America, contemporaneously with the Sturtian in Australia. A similar period of rifting at about 650 Ma occurred with the deposition of the Ice Brook Formation in North America, contemporaneously with the Marinoan in Australia.[12] The Sturtian and Marinoan are local divisions within theAdelaide Rift Complex.[19]

Cryogenian biota and fossils

[edit]

Between the Sturtian and Marinoan glaciations, global biodiversity was very low.[16]

Fossils oftestate amoeba (orArcellinida) first appear during the Cryogenian Period.[20] Since 2009, some researchers have argued that during the Cryogenian Period, potentially the oldest known fossils ofsponges, and thereforeanimals, were formed.[21][22][23] However, it is unclear whether these fossils actually belong to sponges, though the authors do not rule out the possibility of such fossils to represent proto-sponges or complex microbial precursors to sponge-grade organisms.[24] The issue of whether or not biology was impacted by this event has not been settled, for example Porter (2000) suggests that new groups of life evolved during this period, including thered algae andgreen algae,stramenopiles,ciliates,dinoflagellates, and testate amoeba.[25]

The end of the period also saw the origin ofheterotrophicplankton, which would feed onunicellularalgae andprokaryotes, ending thebacterial dominance of the oceans.[26] The unicellular algae (Archaeplastida) went through a big bang of diversification, and their population went up by a factor of a hundred to a thousand.[27][28]

See also

[edit]

References

[edit]
  1. ^Ma, Xiaochen; Wang, Jiasheng; Wang, Zhou; et al. (March 2023)."Geochronological constraints on Cryogenian ice ages: Zircon Usingle bondPb ages from a shelf section in South China".Global and Planetary Change.222 104071.doi:10.1016/j.gloplacha.2023.104071. Retrieved27 October 2025.
  2. ^Rooney, Alan D.; Strauss, Justin V.; Brandon, Alan D.; Macdonald, Francis A. (May 2015)."A Cryogenian chronology: Two long-lasting synchronous Neoproterozoic glaciations".Geology.43 (5):459–462.Bibcode:2015Geo....43..459R.doi:10.1130/G36511.1.
  3. ^Brocks, Jochen J. (September 2018). Lyons, Timothy W.; Droser, Mary L.; Lau, Kimberly V.; Porter, Susannah M. (eds.)."The transition from a cyanobacterial to algal world and the emergence of animals".Emerging Topics in Life Sciences.2 (2):181–190.doi:10.1042/ETLS20180039.eISSN 2397-8562.ISSN 2397-8554.PMID 32412625.
  4. ^Arnaud, Emmanuelle; Halverson, Galen P.; Shields-Zhou, Graham Anthony (November 2011)."Chapter 1: The geological record of Neoproterozoic ice ages".Geological Society, London, Memoirs.36:1–16.doi:10.1144/M36.1. Retrieved27 October 2025.
  5. ^Hoffman, Paul F.; Abbot, Dorian S.; Ashkenazy, Yosef; et al. (November 2017)."Snowball Earth climate dynamics and Cryogenian geology-geobiology".Science Advances.3 (11) e1600983.Bibcode:2017SciA....3E0983H.doi:10.1126/sciadv.1600983.ISSN 2375-2548.PMC 5677351.PMID 29134193.Open access icon
  6. ^Shields-Zhou, Graham A.; Porter, Susannah; Halverson, Galen P. (2016)."A new rock-based definition for the Cryogenian Period (circa 720 – 635 Ma)"(PDF).Episodes.39 (1):3–8.doi:10.18814/epiiugs/2016/v39i1/89231.ISSN 0705-3797.
  7. ^Knoll, Andrew H.; Walter, Malcolm R.; Narbonne, Guy M.; Christie-Blick, Nicholas (March 2006)."The Ediacaran Period: a new addition to the geologic time scale"(PDF).Lethaia.39 (1).Taylor & Francis:13–30.doi:10.1080/00241160500409223.eISSN 1502-3931.ISSN 0024-1164.LCCN 72456902.OCLC 2277593. Retrieved9 October 2025.
  8. ^ab"Chart". International Commission on Stratigraphy. Archived fromthe original on 13 January 2017. Retrieved14 February 2017.
  9. ^Plumb, Kenneth A. (1991)."New Precambrian time scale"(PDF).Episodes. 2.14 (2):134–140.doi:10.18814/epiiugs/1991/v14i2/005. Retrieved7 September 2013.
  10. ^ab"GSSP Table - Precambrian". Geologic Timescale Foundation. Retrieved7 September 2013.
  11. ^Sanchez, Evelyn A. M.; Uhlein, Alexandre; Fairchild, Thomas R. (1 January 2021)."Treptichnus pedum in the Três Marias Formation, south-central Brazil, and its implications for the Ediacaran-Cambrian transition in South America".Journal of South American Earth Sciences.105 102983.Bibcode:2021JSAES.10502983S.doi:10.1016/j.jsames.2020.102983.ISSN 0895-9811.
  12. ^abEyles, Nicholas; Young, Grant (1994). Deynoux, M.; Miller, J.M.G.;Domack, E.W.; Eyles, N.; Fairchild, I.J.; Young, G.M. (eds.).Geodynamic controls on glaciation in Earth history, in Earth's Glacial Record. Cambridge: Cambridge University Press. pp. 5–10.ISBN 0-521-54803-9.
  13. ^Dave Lawrence (2003)."Microfossil lineages support sloshy snowball Earth". Geotimes.
  14. ^Shields, G. A. (2008). "Palaeoclimate: Marinoan meltdown".Nature Geoscience.1 (6):351–353.Bibcode:2008NatGe...1..351S.doi:10.1038/ngeo214.
  15. ^Hoffman, P.F. 2001.Snowball Earth theory
  16. ^abXu, Lingang; Frank, Anja B.; Lehmann, Bernd; Zhu, Jianming; Mao, Jingwen; Ju, Yongze; Frei, Robert (21 October 2019)."Subtle Cr isotope signals track the variably anoxic Cryogenian interglacial period with voluminous manganese accumulation and decrease in biodiversity".Scientific Reports.9 (1): 15056.Bibcode:2019NatSR...915056X.doi:10.1038/s41598-019-51495-0.ISSN 2045-2322.PMC 6803686.PMID 31636318.
  17. ^Freitas, B.T.; Rudnitzki, I.D.; Morais, L.; Campos, M.D.R.; Almeida, R.P.; Warren, L.V.; Boggiani, P.C.; Caetano-Filho, S.; Bedoya-Rueda, C.; Babinski, M.; Fairchild, T.R.; Trindade, R.I.F. (30 August 2021)."Cryogenian glaciostatic and eustatic fluctuations and massive Marinoan-related deposition of Fe and Mn in the Urucum District, Brazil".Geology.49 (12):1478–1483.Bibcode:2021Geo....49.1478F.doi:10.1130/G49134.1.hdl:11449/222880.ISSN 0091-7613.S2CID 239629114. Retrieved11 September 2023.
  18. ^Nance, R. Damian; Evans, David A. D.; Murphy, J. Brendan (1 September 2022)."Pannotia: To be or not to be?".Earth-Science Reviews.232 104128.Bibcode:2022ESRv..23204128N.doi:10.1016/j.earscirev.2022.104128.ISSN 0012-8252.
  19. ^Haines, Peter W.; Turner, Simon P.; Kelley, Simon P.; Wartho, Jo-Anne; Sherlock, Sarah C. (15 November 2004)."40Ar–39Ar dating of detrital muscovite in provenance investigations: a case study from the Adelaide Rift Complex, South Australia".Earth and Planetary Science Letters.227 (3):297–311.doi:10.1016/j.epsl.2004.08.020.ISSN 0012-821X.
  20. ^Porter, S.A. & Knoll, A.H. (2000)."Testate amoeba in the Neoproterozoic Era: evidence from vase-shaped microfossils in the Chuar Group, Grand Canyon".Paleobiology.26 (3):360–385.Bibcode:2000Pbio...26..360P.doi:10.1666/0094-8373(2000)026<0360:TAITNE>2.0.CO;2.ISSN 0094-8373.S2CID 54636062.
  21. ^Love; Grosjean, Emmanuelle; Stalvies, Charlotte; Fike, David A.; Grotzinger, John P.; Bradley, Alexander S.; Kelly, Amy E.; Bhatia, Maya; Meredith, William; et al. (2009)."Fossil steroids record the appearance of Demospongiae during the Cryogenian period"(PDF).Nature.457 (7230):718–721.Bibcode:2009Natur.457..718L.doi:10.1038/nature07673.PMID 19194449.S2CID 4314662. Archived fromthe original(PDF) on 8 May 2018. Retrieved15 April 2009.
  22. ^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. (17 August 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.
  23. ^"Discovery of possible earliest animal life pushes back fossil record". 17 August 2010.
  24. ^Wallace, M.W.; Hood, A.v.S.; Woon, E.M.S.; Hoffman, K.-H.; Reed, C.P. (2014). "Enigmatic chambered structures in Cryogenian reefs: The oldest sponge-grade organisms?".Precambrian Research.255:653–659.Bibcode:2014PreR..255..109W.doi:10.1016/j.precamres.2014.09.020.hdl:11343/52679.
  25. ^"Palaeos Proterozoic: Neoproterozoic: Cryogenian".
  26. ^Fossil fats reveal how complex life kicked off after Snowball Earth phase
  27. ^We Finally Know Which Groundbreaking Period in Earth's History Gave Rise to The First Animals
  28. ^The algae that terraformed Earth

Further reading

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External links

[edit]
Quaternary /
Late Cenozoic
Quaternary
Pliocene
Miocene
Oligocene
Paleozoic
Ediacaran
Cryogenian-Snowball Earth
Paleoproterozoic
Mesoarchean
Related topics
Cenozoic Era
(present–66.0 Ma)
Quaternary(present–2.58 Ma)
Neogene(2.58–23.0 Ma)
Paleogene(23.0–66.0 Ma)
Example of stratigraphic column
Mesozoic Era
(66.0–252 Ma)
Cretaceous(66.0–145 Ma)
Jurassic(145–201 Ma)
Triassic(201–252 Ma)
Paleozoic Era
(252–539 Ma)
Permian(252–299 Ma)
Carboniferous(299–359 Ma)
Devonian(359–419 Ma)
Silurian(419–444 Ma)
Ordovician(444–485 Ma)
Cambrian(485–539 Ma)
Proterozoic Eon
(539 Ma–2.5 Ga)
Neoproterozoic(539 Ma–1 Ga)
Mesoproterozoic(1–1.6 Ga)
Paleoproterozoic(1.6–2.5 Ga)
Archean Eon(2.5–4 Ga)
Hadean Eon(4–4.6 Ga)
 
ka = kiloannum (thousand years ago);Ma = megaannum (million years ago);Ga = gigaannum (billion years ago).
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