Marinoan glaciation: Difference between revisions

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{{short description|A periodPeriod of worldwide glaciation during the Cryogenian period.}}
{{Graphical timeline
| title=Neoproterozoic Snowball Periods
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| period4-border-width = 1
| period4-colour = #FFFFB3
| bar1-from=-717 | bar1-to=-663662
| bar1-left=0.1 | bar1-right=0.9
| bar1-text = [[Sturtian glaciation|Sturtian]] | bar1-colour = #77bb77
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| bar2-left=0.1 | bar2-right=0.9
| bar2-text = Marinoan | bar2-colour = #77bb77
| bar3-from=-583579.79| bar3-to=-582579.46
| bar3-left=0.1 | bar3-right=0.9
| bar3-text = [[Gaskiers glaciation|Gaskiers]] | bar3-colour = #77bb77
| bar4-from = -850540 | bar4-to = -735530
| bar5bar4-text = <small>(millions of years ago)</small>
| bar4-left=0.1 | bar4-right=0.9
| bar4-text = [[Kaigas]]? | bar4-colour = #77bb77transparent
| bar5-from = -540 | bar5-to = -530
| bar5-text = <small>(millions of years ago)</small>
| bar5-colour = transparent
| legend1= [[Neoproterozoic]] era
| legend1-colour=#FFFFB3
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| issue = 1
| pages= 27–54
| doi = 10.1144/SP326.2|bibcode = 2009GSLSP.326...27S | s2cid = 129706604
}}</ref> An earlier and longer possible snowball phase, the [[Huronian glaciation]], is not shown here.
}}
<!-- End infobox, article starts here -->
The '''Marinoan glaciation''', sometimes also known as the '''Varanger glaciation''',<ref name="PazosEtAl2003">{{cite journal |last1=Pazos |first1=Pablo J. |last2=Sánchez-Bettucci |first2=Leda |last3=Tofalo |first3=Ofelia R. |date=January 2003 |title=The Record of the Varanger Glaciation at the Río De La Plata Craton, Vendian-Cambrian of Uruguay |url=https://www.sciencedirect.com/science/article/abs/pii/S1342937X05706444 |journal=[[Gondwana Research]] |volume=6 |issue=1 |pages=65–77 |doi=10.1016/S1342-937X(05)70644-4 |bibcode=2003GondR...6...65P |access-date=16 October 2022}}</ref> was a period of worldwide [[glaciation]].<ref name="RooneyEtAl2015" />
The '''Marinoan glaciation''' was a period of worldwide [[glaciation]] that lasted from approximately 650 to 635 [[Megaannum|Ma]] (million years ago) during the [[Cryogenian]] [[geologic period|period]]. The glaciation may have covered the entire planet, in an event called the [[Snowball Earth]]. The end of the glaciation may have been sped by the release of [[methane]] from equatorial [[permafrost]].<ref>{{Cite journal | last1 = Shields | first1 = G. A. | title = Palaeoclimate: Marinoan meltdown | doi = 10.1038/ngeo214 | journal = Nature Geoscience | volume = 1 | issue = 6 | pages = 351–353 | year = 2008 | pmid = | pmc = | bibcode = 2008NatGe...1..351S }}</ref><ref>{{Cite journal | doi = 10.1038/nature06961| title = Snowball Earth termination by destabilization of equatorial permafrost methane clathrate| journal = Nature| volume = 453| issue = 7195| pages = 642–5| year = 2008| last1 = Kennedy | first1 = M. | last2 = Mrofka | first2 = D. | last3 = von Der Borch | first3 = C. | pmid=18509441| bibcode = 2008Natur.453..642K}}</ref>
Its beginning is poorly constrained, but occurred no earlier than 654.5 [[Megaannum|Ma]] (million years ago).<ref>{{cite journal |last1=Ma |first1=Xiaochen |last2=Wang |first2=Jiasheng |last3=Wang |first3=Zhou |last4=Algeo |first4=Thomas J. |last5=Chen |first5=Can |last6=Cen |first6=Yue |last7=Yin |first7=Qing-Zhu |last8=Huang |first8=Chang |last9=Xu |first9=Liyuan |last10=Huang |first10=Chao |last11=Chen |first11=Dahe |date=March 2023 |title=Geochronological constraints on Cryogenian ice ages: Zircon Usingle bondPb ages from a shelf section in South China |url=https://www.sciencedirect.com/science/article/abs/pii/S0921818123000449 |journal=[[Global and Planetary Change]] |volume=222 |doi=10.1016/j.gloplacha.2023.104071 |access-date=1 June 2023|url-access=subscription }}</ref>
It ended approximately 632.3 ± 5.9 Ma<ref name="RooneyEtAl2015">{{cite journal|last1=Rooney|first1=Alan D.|last2=Strauss|first2=Justin V.|last3=Brandon|first3=Alan D.|last4=Macdonald|first4=Francis A.|year=2015|title=A Cryogenian chronology: Two long-lasting synchronous Neoproterozoic glaciations|journal=[[Geology (journal)|Geology]]|volume=43|issue=5|pages=459–462|bibcode=2015Geo....43..459R|doi=10.1130/G36511.1}}</ref>
during the [[Cryogenian]] [[geologic period|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]]<ref>{{cite journal |last1=Sun |first1=Ruiyang |last2=Shen |first2=Jun |last3=Grasby |first3=Stephen E. |last4=Zhang |first4=Jiawei |last5=Chen |first5=Jianshu |last6=Yang |first6=Chuang |last7=Yin |first7=Runsheng |date=December 2022 |title=CO2 buildup drove global warming, the Marinoan deglaciation, and the genesis of the Ediacaran cap carbonates |url=https://www.sciencedirect.com/science/article/abs/pii/S0301926822003357 |journal=[[Precambrian Research]] |volume=383 |page=106891 |doi=10.1016/j.precamres.2022.106891 |bibcode=2022PreR..38306891S |s2cid=253430013 |access-date=17 December 2022}}</ref>
The '''Marinoan glaciation''' was a period of worldwide [[glaciation]] that lasted from approximately 650 to 635 [[Megaannum|Ma]] (million years ago) during the [[Cryogenian]] [[geologic period|period]]. The glaciation may have covered the entire planet, in an event called the [[Snowball Earth]]. The end of the glaciationand may have been spedhastened by the release of [[methane]] from equatorial [[permafrost]].<ref>{{Cite journal | last1 = Shields | first1 = G. A. | title = Palaeoclimate: Marinoan meltdown | doi = 10.1038/ngeo214 | journal = Nature Geoscience | volume = 1 | issue = 6 | pages = 351–353 | year = 2008 | pmid = | pmc = | bibcode = 2008NatGe...1..351S }}</ref><ref>{{Cite journal | doi = 10.1038/nature06961| title = Snowball Earth termination by destabilization of equatorial permafrost methane clathrate| journal = [[Nature (journal)|Nature]]| volume = 453| issue = 7195| pages = 642–5| year = 2008| last1 = Kennedy | first1 = M. | last2 = Mrofka | first2 = D. | last3 = von Der Borch | first3 = C. | pmid=18509441| bibcode = 2008Natur.453..642K| s2cid = 4416812}}</ref>
 
== Origin of name and history of terminology ==
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| volume = 13
| pages = 69–72
| doi = }}</ref> The corresponding time period, referred to as the Marinoan Epoch, spanned from the middle Cryogenian to the top of the [[Ediacaran]] in modern terminology. Mawson recognised a glacial episode within the Marinoan Epoch which he referred to as the Elatina glaciation after the 'Elatina Tillite' (now [[Elatina Formation]]) where he found the evidence.<ref name=Mawson1949>{{cite journal
| author = Mawson, D.
| year = 1949
| title = A third occurrence of glaciation evidenced in the Adelaide System
| journal = [[Transactions of the Royal Society of South Australia]]
| volume = 73
| pages = 117–121
| doi = }}</ref> However, the term Marinoan glaciation came into common usage because it was the glaciation that occurred during the Marinoan Epoch, as distinct from the earlier glaciation during the Sturtian Epoch (the time period of deposition of the older Sturtian Series<ref name=Mawson1950 />).
 
The term Marinoan glaciation was later applied globally to any glaciogenic formations assumed (directly or indirectly) to correlate with Mawson's original Elatina glaciation in South Australia.<ref>{{Cite journal|lastlast1=Wen|firstfirst1=Bin|last2=Evans|first2=David A. D.|last3=Li|first3=Yong-Xiang|last4=Wang|first4=Zhengrong|last5=Liu|first5=Chao|date=2015-12-01|title=Newly discovered Neoproterozoic diamictite and cap carbonate (DCC) couplet in Tarim Craton, NW China: Stratigraphy, geochemistry, and paleoenvironment|journal=[[Precambrian Research]]|volume=271|pages=278–294|doi=10.1016/j.precamres.2015.10.006|bibcode=2015PreR..271..278W}}</ref> Recently, there has been a move to return to the term Elatina glaciation in South Australia because of uncertainties regarding global correlation and because an Ediacaran glacial episode (Gaskiers) also occurs within the wide-ranging Marinoan Epoch.<ref name=Williams2008>{{cite journal
| author = Williams, G.E. |author2=Gostin, V.A. |author3=McKirdy, D.M. |author4=Preiss, W.V.
| year = 2008
| title = The Elatina glaciation, late Cryogenian (Marinoan Epoch), South Australia: Sedimentary facies and palaeoenvironments
| journal = [[Precambrian Research]]
| volume = 163
| pages = 307–331
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| doi = 10.1038/ngeo355
| title = Sedimentary challenge to Snowball Earth
| journal = [[Nature Geoscience]]
| volume = 1
| pages = 817–825
| last2 = Etienne
| first2 = James L.
| issue=12|bibcode = 2008NatGe...1..817A }}</ref> There were three (or possibly four) significant ice ages during the late Neoproterozoic. These periods of nearly complete glaciation of Earth are often referred to as "Snowball Earth", where it is hypothesized that at times the planet was covered by ice {{convert|1|-|2|km|mi|abbr=on}} thick.<ref name="SciDaily2004">{{cite web|title=New Evidence Supports Three Major Glaciation Events In The Distant Past|url=https://www.sciencedaily.com/releases/2004/04/040421234349.htm|publisher=ScienceDaily|date=2004-04-22|accessdateaccess-date=2011-06-18}}</ref> Of these glaciations, the [[Sturtian glaciation]] was the most significant, whereas the Marinoan was a shorter, but still worldwide glaciation. Other Cryogenian glaciations were probably small and not global as compared to the Marinoan or Sturtian glaciations.
 
During the Marinoan glaciation, characteristic glacial deposits indicate that [[Earth]] suffered one of the most severe ice ages in its history. [[Glacier]]s extended and contracted in a series of rhythmic pulses, possibly reaching as far as the equator.<ref>{{cite web |title = Microfossil lineages support sloshy snowball Earth |author = Dave Lawrence |year = 2003 |publisher = Geotimes |url = http://www.agiweb.org/geotimes/apr03/WebExtra041803.html|accessdateaccess-date=2011-06-18}}</ref><ref>{{cite web|title=Global Glaciation Snowballed Into Giant Change in Carbon Cycle|url=https://www.sciencedaily.com/releases/2010/05/100501013533.htm|publisher=ScienceDaily|date=2010-05-02|accessdateaccess-date=2011-06-18}}</ref>
 
The Earth may not have been fully covered in ice, as some computer simulations show an extreme slowdown of the hydrological cycle that inhibited new glacial formation before the Earth was fully ice-covered.<ref>{{cite journal |last1=Chandler |first1=Mark A. |last2=Sohl |first2=Linda E. |date=1 August 2000 |title=Climate forcings and the initiation of low-latitude ice sheets during the Neoproterozoic Varanger glacial interval |journal=[[Journal of Geophysical Research]] |volume=105 |issue=D16 |pages=20737–20756 |doi=10.1029/2000JD900221 |doi-access=free |bibcode=2000JGR...10520737C }}</ref>
 
The melting of the Snowball Earth is associated with greenhouse warming due to the accumulation of high levels of carbon dioxide in the atmosphere.<ref name=Pierrehumbert2004>{{cite journal
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| year = 2004
| title = High levels of atmospheric carbon dioxide necessary for the termination of global glaciation
| journal = [[Nature (journal)|Nature]]
| volume = 429
| pages = 646–9
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| pmid = 15190348
| issue = 6992
|bibcode = 2004Natur.429..646P }}</ref>| s2cid = 2205883
}}</ref> Deglaciation likely started in the mid-latitudes, as in the tropics, the intense hydrological cycle replenished snow rapidly. As the mid-latitudes became ice free, dust was blown from them into other regions, lowering albedo and speeding up deglaciation.<ref>{{cite journal |last1=De Vrese |first1=Philipp |last2=Stacke |first2=Tobias |last3=Rugenstein |first3=Jeremy Caves |last4=Goodman |first4=Jason |last5=Brovkin |first5=Victor |date=14 May 2021 |title=Snowfall-albedo feedbacks could have led to deglaciation of snowball Earth starting from mid-latitudes |journal=[[Communications Earth & Environment]] |volume=2 |issue=1 |page=91 |doi=10.1038/s43247-021-00160-4 |doi-access=free |bibcode=2021ComEE...2...91D }}</ref>
 
== Evidence ==
[[File:Elatina Fm diamictite.JPG|thumb|Elatina Fm diamictite below [[Ediacaran]] [[Global Boundary Stratotype Section and Point|GSSP]] site in the [[Flinders Ranges National Park|Flinders Ranges NP]], South Australia. A$1 coin for scale.]]
[[File:PocatelloFm.JPG|thumb|[[Diamictite]] of the [[Neoproterozoic]] Pocatello Formation, a 'Snowball Earth'—type deposit]]
Even though much evidence has been lost through geological changes, field investigations show evidence of the Marinoan glaciation in China, [[Svalbard]] archipelago and South Australia. In [[Guizhou Province]], China, glacial rocks were found to be underlying and overlying a layer of [[volcanic ash]]es which contained [[zircon]] minerals, which could be dated through [[radioisotopes]]. Glacial deposits in South Australia are approximately the same age (about 630&nbsp;Ma), confirmed by similar stable [[carbon isotope]]s, mineral deposits (including sedimentary [[barite]]), and other unusual sedimentary structures.<ref name="SciDaily2004" /> Two [[diamictite]]-rich layers in the top {{convert|1|km|mi|abbr=on}} of the {{convert|7|km|mi|abbr=on}} Neoproterozoic strata of the northeastern Svalbard archipelago represent the first and final phases of the Marinoan glaciation.<ref>{{cite journal|url=http://geoweb.princeton.edu/people/maloof/downloads/marinoan.pdf|doi=10.1111/j.1365-2117.2004.00234.x|title=The Marinoan glaciation (Neoproterozoic) in northeast Svalbard|vauthors=Halverson GP, Maloof AC, Hoffman PF |journal=Basin Research|year=2004|volume=16|issue=3|pages=297–324|accessdateaccess-date=2011-06-18|bibcode=2004BasR...16..297H|citeseerx=10.1.1.368.2815|s2cid=53588955 |archive-date=2012-03-20|archive-url=https://web.archive.org/web/20120320222653/http://geoweb.princeton.edu/people/maloof/downloads/marinoan.pdf|url-status=dead}}</ref> In Uruguay, evidence of the Marinoan glaciation is known from dropstones, diamictites, rhythmites, clast layers, and varve-like deposits.<ref name="PazosEtAl2003" />
 
According to Eyles and Young, the Marinoan is a second episode of [[Neoproterozoic]] glaciation (680–690 [[Myr|Ma]]) occurring in the [[Adelaide Geosyncline]]. According to them, "It is separated from the Sturtian by a thick succession of sedimentary rocks containing no evidence of glaciation. This glacial phase could correspond to the recently described Ice Brooke [[Geological formation|formation]] in the northern [[Canadian Cordillera|Cordillera]]."<ref name=Eyles>{{cite book|last1=Eyles|first1=Nicholas|last2=Young|first2=Grant|editor1-last=Deynoux|editor1-first=M.|editor2-last=Miller|editor2-first=J.M.G.|editor3-last=Domack|editor3-first=E.W.|editor4-last=Eyles|editor4-first=N.|editor5-last=Fairchild|editor5-first=I.J.|editor6-last=Young|editor6-first=G.M.|editorlink3editor-link3=Eugene Domack|title=Geodynamic controls on glaciation in Earth history, in Earth's Glacial Record|date=1994|publisher=Cambridge University Press|location=Cambridge|isbn=978-0521548038|pages=[https://archive.org/details/earthsglacialrec0000unse/page/5 5–10]|url=https://archive.org/details/earthsglacialrec0000unse/page/5}}</ref>
 
== Effects on life ==
According to Eyles and Young, the Marinoan is a second episode of [[Neoproterozoic]] glaciation (680–690 [[Myr|Ma]]) occurring in the [[Adelaide Geosyncline]]. According to them, "It is separated from the Sturtian by a thick succession of sedimentary rocks containing no evidence of glaciation. This glacial phase could correspond to the recently described Ice Brooke [[Geological formation|formation]] in the northern [[Canadian Cordillera|Cordillera]]."<ref name=Eyles>{{cite book|last1=Eyles|first1=Nicholas|last2=Young|first2=Grant|editor1-last=Deynoux|editor1-first=M.|editor2-last=Miller|editor2-first=J.M.G.|editor3-last=Domack|editor3-first=E.W.|editor4-last=Eyles|editor4-first=N.|editor5-last=Fairchild|editor5-first=I.J.|editor6-last=Young|editor6-first=G.M.|editorlink3=Eugene Domack|title=Geodynamic controls on glaciation in Earth history, in Earth's Glacial Record|date=1994|publisher=Cambridge University Press|location=Cambridge|isbn=978-0521548038|pages=5–10}}</ref>
The survival of benthic macroalgae indicates that there remained areas of suitable habitat for them in the photic zone along the coasts of mid-latitude continents during the Marinoan glaciation.<ref>{{Cite journal |last=Ye |first=Qin |last2=Tong |first2=Jinnan |last3=Xiao |first3=Shuhai |last4=Zhu |first4=Shixing |last5=An |first5=Zhihui |last6=Tian |first6=Li |last7=Hu |first7=Jun |date=1 June 2015 |title=The survival of benthic macroscopic phototrophs on a Neoproterozoic snowball Earth |url=https://pubs.geoscienceworld.org/gsa/geology/article/43/6/507/131885/The-survival-of-benthic-macroscopic-phototrophs-on |journal=[[Geology (journal)|Geology]] |language=en |volume=43 |issue=6 |pages=507–510 |doi=10.1130/G36640.1 |issn=1943-2682 |access-date=7 October 2024 |via=GeoScienceWorld}}</ref>
 
== See also ==
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[[Category:Cryogenian]]
[[Category:Glaciology]]
[[Category:Climate history]]
[[Category:Extinction events]]
[[Category:Climate1950s historyneologisms]]