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Siderian

From Wikipedia, the free encyclopedia
First period of the Paleoproterozoic Era

Siderian
2500 – 2300Ma
A close-up view of a canyon wall. Red streaks stretch horizontally on the wall, and a few shrubs grow from the surrounding sandstone.
A Siderian banded iron formation in Dales Gorge,Western Australia
A 3D rendered image of Earth covered with ice and snow.
Artist's impression of the Earth during theHuronian glaciation, starting from the mid-Siderian
Chronology
−2520 —
−2500 —
−2480 —
−2460 —
−2440 —
−2420 —
−2400 —
−2380 —
−2360 —
−2340 —
−2320 —
−2300 —
−2280 —
 
 
 
 
Beginning of theGreat Oxidation Event
Breakup of the supercontinentKenorland[2]
Events of the Siderian Period
Vertical axis scale:Millions of years ago
Proposed redefinition(s)2630 – 2420 Ma

Kranendonk et al., 2012
3000?[a]c. 2450 Ma

Shields et al., 2021
Proposed containerNeoarchean

Kranendonk et al., 2012
Neoarchean

Shields al., 2021
Etymology
Name formalityFormal
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
Lower GSSA ratified1990[4]
Upper boundary definitionDefined chronometrically
Upper GSSA ratified1990[4]
Atmospheric and climatic data
Mean atmosphericO2 contentc. 0.014007 vol %
(0% of modern)[5]
Mean atmosphericCO2 contentc. 11000ppm
(39 times pre-industrial)[6]

TheSiderian (/sˈdɪəri.ən,sɪ-/) is the firstgeologic period in thePaleoproterozoic Era andProterozoic Eon. It lasted from 2500 to 2300million years ago (Ma), spanning 200 million years, and is followed by theRhyacian Period. Instead of being based onstratigraphy, these dates are definedchronometrically.

Most continential activity in this period was met with the breakup of the supercontinentKenorland. While this event mainly occurred in the cratonLaurentia, volcanic intrusions anddike swarms have appeared in plates pertaining toNorthwestern Europe,South Africa, andAustralia in connection to the rifting. In the ocean, emissions fromhydrothermal vents contributed to the production andcrystallization of minerals, along with varying concentrations ofsulfur andiron. While this sedimentation circulated in the ocean, the amounts deposited on the ocean floor contributed to the development ofbanded iron formations, along with a diverse range of ores such aspyrite andmagnetite.

Cyanobacteria continued to develop their molecular structure, witheukaryotes beginning to appear near the end of the period, and they contributed to the ocean'soxidation. Their presence eventually became the partial cause for the build-up ofoxygen in Earth's atmosphere, becoming known as theGreat Oxidation Event. This led to a decrease inmethane andcarbon dioxide, which were two majorgreenhouse gases at the time, dropping the overall global temperature below 0 °C. As a result of this, the Earth experienced threesnowball events which have been collectively known as theHuronian glaciation.

Etymology and history

[edit]

The nameSiderian is derived from theGreek wordsideros, meaning "iron", and refers to thebanded iron formations formed during this period.[7] Before its use, the period was suggested to be named as theHuronian Era[b] with a boundary from 2450 to 2200 Ma, in correlation to the sedimentary record of Canada'sHuronian Supergroup. Despite the stratigraphic use of the term "Huronian" since the nineteenth century,[9][10] the Siderian period was proposed under the current nomenclature (2500 to 2300 Ma) in 1989 by the Subcommission on Precambrian Stratigraphy. It was later ratified in 1990 by theInternational Union of Geological Sciences as a subdivision of theProterozoic Eon.[4]

While the Siderian is well-defined by the lower edge of iron-deposition layers and the initial appearance of glacial deposits, alternate names have been suggested to mark the period stratigraphically. In 2012, Kranendonket al. proposed to set the Siderian Period to an earlier date range, due to the slow expansion of the period's continential plates, spanning from 2630 to 2420 Ma as the final subdivision of theNeoarchean Era.[11] They also suggested adjusting the upper half of the Siderian's preceding definition to occur from 2420 to 2250 Ma as theOxygenian Period, in response to the change in Earth's atmosphere during this time.[12] In 2021, Shieldset al. presented a similar alteration, but with the Siderian ending at about 2450 Ma, and the first period of thePaleoproterozoic Era termed theSkourian instead of the Oxygenian. The name "Skourian" would refer to the oxidation of the ocean's iron supply, and its period would span from about 2450 to 2300 Ma.[3] As of December 2024[update], the Siderian retains its 1989 definition, and is the earliest internationally recognized period on Earth'sgeologic time scale.[13]

Paleogeography

[edit]

Paleotectonics and lithology

[edit]

Tectonic activity mainly revolved around the growth ofcontinental plates during the early Siderian. Manycratons at the time, including theGawler,Superior, andPilbara cratons, experienced volcanic activity through a global plume breakout, which occurred from 2500 to 2450 Ma. During that time, depositions atbanded iron formations began occurring at theKaapvaal and Pilbara cratons.[14] Additionally, volcanic andsedimentary rocks have begun to deposit into theTransvaal Basin at 2400 Ma, lasting until 2000 Ma in theOrosirian Period.[15]

Some depositional activity in what would become present-dayAustralia involved a selection ofsupersequences, consisting of a diverse set of densely packed sediments. The Brockman Supersequence, lasting from 2500 to 2449 Ma, has been shown to at least consist ofmudrock and sediments from banded iron formations, which have been deposited during rising sea levels and times of volcanic activity.[16] Additionally, there have been traces ofsulfur isotopes found in this sequence's Brockman Iron Formation, indicating a rise in the atmosphere'soxygen at the time.[17] The Woongarra Supersequence followed, consisting of depositions mainly fromrhyolite, but with layers ofdiabase andbasalt present beforehand, dating back to 2449 Ma.[18] It was then capped by the Turee Creek Supersequence, which presents itself with a layer ofsandstone andlimestone sequences, and lasted from 2449 to 2410 Ma before a stratigraphic hiatus occurred.[16]: 982 

On theNorth American plate, sediments began to pack themselves and form theHuronian and Snowy Pass supergroups. Sandstone in the Huronian Supergroup was deposited in diverse compositions between 2450 and 2219 Ma, with some layers takingarkosic,felspathic, andquartzose structures.[19][20] While major depositions involved conglomerates ofsiltstone, limestone, andgranite,[21] there were trace amounts ofgold,uranium, andaluminium present as well.[22][23] In theWyoming Craton, the Snowy Pass Supergroup holds signs ofquartzite deposited throughout its layers, accompanied by sedimentary structures ofmarble,phyllite, andpebble conglomerates.[24] Additionally, there have been deposits ofrhythmite anddropstone in northern Canada's Hurwitz Group between 2450 and 2110 Ma.[25] The extent of theseLaurentian depositions ranges from glacial origins andice sheets torivers andshallow marine conditions.[26][27]

In northwestern Europe, evidence of deposition has been found in theBaltic Shield, within the lower portion of the Karelian Supergroup. Volcanic sediments frommafic complexes have been layered withporphyry containing bluequartz within the Sumian Group, being deposited during the first half of the Sideran.[28] In the following sequence,saprolite andpyroclastics have been found in the Sarolian Group, with traces spanning from 2400 to 2300 Ma.[29]Diamictites have also been identified in this sequence, providing evidence of glacial deposits occurring in the area.[30]

The lower half of theTransvaal Supergroup inSouth Africa has been deposited for the duration of the Siderian Period.[31] It mainly consists of a patterned sequence ofshale, sandstone, andsiltstone, and is embedded with an additional diversity of sediments.[32] Traces ofhematite,magnetite, andmarl can be found in the Eastern Transvaal Basin,[33] while the Griqualand West Basin holds instances ofgraywacke, ironlutite, andhyaloclastite deposits.[34] Some sequences have been deposited as banded iron formations, such as those presented through the Penge and Doradale formations.[35] However, different types of BIFs are also present in this supergroup, with granular,silicate, and orthochemical[c] iron formations existing in the Koegas Subgroup.[37]

In theNorth China Craton, banded iron formations,schists of various qualities, and additional layers of sedimentation have been deposited during this period, following the Fupingian orogeny which occurred 2550 Ma.[38][39] The Shuangshanzi Group in easternHebei holds layers ofamphibolite andmica-granulite.[40] In the Wutai Group found within theTaihang andWutai Mountains, conglomerates oftholeiitic basalt,rhyodacite, andtonalite have been identified.[41]

Magmatism

[edit]
A close-up view of a gray rock. It is slanted with diagonal light and dark streaks, and has a brighter, irregular marking on its surface.
GrayBadcallian gneiss (c. 2500 Ma)intruded by a dark amphiboliticScourie dike (c. 2400 Ma), both intruded by younger graniticveins

Magma in the form ofdike swarms penetrated the surface of multiple cratons during the Siderian, taking place in some of the major continental plates such as those spanningNorth America,South Africa, andAustralia. About 2470 Ma, theMistassini dike swarm penetrated theSuperior Craton.[42] With a surface area of at least 100,000 square kilometers (39,000 sq mi), it can be classified as alarge igneous province (LIP).[43] It was followed by theMatachewan dike swarm, an LIP occurring from about 2470 to 2450 Ma, and spanning a surface area of at least 300,000 square kilometers.[44] The Mistassini and Matachewan swarms can be genetically associated with each other, as the Matachewan swarm intruded into the Superior Craton in the area betweenLake Superior andJames Bay.[45] In the region pertaining to present-dayScotland, the Scourie dike swarm penetrated theLewisian Gneiss Complex from about 2418 to 2375 Ma,[46] while the Widgiemooltha dike swarm intruded into theYilgarn Craton in Australia at around 2410 Ma.[47] The Widgiemooltha swarm occurred in close proximity to the Sebanga Poort dike's intrusion into theZimbabwe Craton, which occurred about 2408 Ma.[48]

Breakup of Kenorland

[edit]
Main article:Kenorland

Tectonic rifting began separating the supercontinentKenorland at around 2450 Ma, with the breakup mainly occurring inLaurentia.[49] As a result, the Hurwitz Group innorthern Canada experienced continental stretching and depression, resulting in the depositions of the Noomut, Padlei, and Kinga Formations, along with the creation of the Hurwitz Basin.[50] Additionally, lowsulfidation deposits holding copper and nickel began to form in the Nena andKalahari cratons,[49] whilezircons formed within the Deep Lake Group in what is now theSierra Madre Range.[51][52] Despite the intrusions contributing to the rifting, Kenorland experienced little continental movement, and there have been no signs of ocean development as a result. However, sedimentation from shallow waters began to occupy the Strel'na Group in what is now theKola Peninsula.[53][54]

Climate

[edit]

Great Oxidation Event

[edit]
Main article:Great Oxidation Event
A graph of changing atmosphere levels. Oxygen experiences a sharp increase, carbon dioxide and methane steadily decrease, and nitrogen remains relatively constant.
Semi-logarithmic chart of atmospheric levels throughout Earth's history, with the surge of oxygen occurring approximately 2.4 billion years ago

Since the beginning of the Siderian, there has been an irreversible rise of oxygen in the Earth's atmosphere, which has come to be known as theGreat Oxidation Event. The partial pressure of oxygen in the air (pO2) has been shown to have increased to at least 104 times its original level, rising from 2 × 10−6bar to at least 2 × 10−3 bar between 2410 and 2320 Ma.[5][55] As a result, the rapid change came at the expense of greenhouse gases such ascarbon dioxide andmethane, indirectly leading to a series of ice ages known as theHuronian glaciation.[56]

The levels ofcarbonates and organic carbon have been relatively stagnant. The abundance of carbon-13 isotopes (δ13C), found withindolomites and formations in theMount Bruce,Transvaal, andHuronian supergroups, has maintained a steady level of 0‰ in carbonates, while organic carbon created through the activity and burial ofcyanobacteria remained stationary at approximately −28‰.[57][58] Although this may present itself as a sign of inactivity during this period, it suggests that there have been multiple sources causing an equal force of sinks and rises in the levels of oxygen.[59] This includes the influx and settlement of carbon dioxide from volcanic activity which stems from tectonic processes,[60] along with the delivery ofphosphate to oceans through cycles of chemical weathering.[61]

As a consequence of the excess oxygen, a shift began to occur in the level and activity ofgreenhouse gases. The carbon dioxide in the atmosphere maintained equilibrium at a partial pressure of 1.1 × 10−2 bar, due to the oxidation of methane in the air,silicate weathering on the surface, and emissions from volcanic activity.[62][63] However, this process depleted the amounts of methane by a significant amount, dropping from 300 to 4ppmv.[64] Despite the balance in carbon dioxide, the significant change in methane caused Earth to undergo asnowball event, dropping the average global temperatures below 0 °C.[65]

Huronian glaciation

[edit]
Main article:Huronian glaciation

Due to the loss of global temperature, the Earth entered theHuronian glaciation, which lasted from about 2450 to 2200 Ma.[66] While this event has been divided into four separate glaciations, only the first three occur in the Siderian Period, serving as a reaction to the oxidizing environment.[67] Traces of this glaciation have been found in thediamictites and sequences of six cratons,[68] including theWyoming,Kaapvaal, and Karelia-Kola cratons.[67]

The oldest glaciation correlates to quartz located in the Campbell Lake and Headquarters formations,[69] along with glacial deposits in the Polisarka Formation.[70] It lasted from about 2440 to 2420 Ma,[67] and is generally referred to after the diamictites found in the Duitschland Formation.[71] The second glaciation, known as the Makganyene glaciation after its eponymous formation, is marked bycap carbonate sequences found above the Bruce and Vagner formations,[72] occurring from about 2380 to 2360 Ma.[67] The youngest of the three glaciations occurs from about 2340 to 2310 Ma near the end of the Siderian,[67] represented in the Gowganda Formation of theHuronian Supergroup, and referred to after the Rietfontein diamictite located inSouth Africa.[73]

Life

[edit]

By the beginning of the Great Oxidation Event,cyanobacteria have developed intercelluar communication through molecular exchange, and have begun to differentiate from each other. Strands such as those in thePseudanabaena genus began chaining themselves in afilamentous structure,[74] andGiardia, one of the earliesteukaryotes, emerged at around 2309 Ma.[75][76] Additionally,flagellated microorganisms began to develop in the ocean's crust, appearing at about 2400 Ma.[77]

Traces of cyanobacteria have made marks in a few deposition sites.Microfossils embedded inblack chert have been dated back to 2450 Ma in Australia'sTuree Creek Group,[78] while bacterial remnants from theConophyton andSiphonophycus genus have been preserved in South Africa's Kuruman Iron Formation.[79] In China,stromatolites have been spotted in the Dashiling and Qingshicun formations of the Hutuo Group, existing for the duration of the Siderian Period.[80] Additionally, findings in theFennoscandian Shield show that the taxonomy of stromatolites began to diversify at around 2330 Ma.[81]

There have been signs offungus-like organisms appearing at about 2400 Ma within the cracks and vesicles of filamentous structures.[82] Open spaces and cavities below the seafloor have led to the development of root-like structures such ashyphae andmycelia, and have been preserved inbasalt andclay within the Ongeluk Formation in South Africa.[77][83] This has raised suggestions to the preexistence of a stable environment for fungal development, as evidenced by the fossil's similarities withvolcanic pillows from theDevonian Period.[84]

Marine geochemistry

[edit]

Isotopic composition of iron

[edit]

The fluctuation of iron in seawater was met with an increase in the creation and deposition of iron oxides and ferrous minerals.Hydrothermal vents served as the ocean's primary source of iron,[85] increasing its isotopic56Fe/54Fe ratio (δ56Fe) by up to 3‰, compared to values in theNeoarchean Era.[86] Some of the iron present was oxidized intoiron(II) oxide andiron(III) oxide, either through the bacterial process ofdisimilatory iron reduction, or by the presence of oxygen in its aqueous form.[85] Isotopes with a particularly heavy δ56Fe value, however, deposited in iron reservoirs before 2400 Ma, which would develop into banded iron formations holding traces of ores such assiderite,magnetite, andgreenalite.[87]

Isotopic composition of sulfur

[edit]
Further information:Sulfur cycle

Before the Great Oxidation Event, sulfur was mainly supplied as sulfide through the volcanic outgassing ofhydrogen sulfide andsulfur dioxide.[88] These molecules were then deposited into the anoxic seawater at concentrations of 1–2 mM, withsulfide minerals such aspyrite being created as a result,[89][90] and sulfate being oxidized from the aqueous solution.[91] Due to the lack of oxygen, however, there was a very minimal amount of sulfate in circulation, falling within a concentration of 5–200 μM before 2400 Ma.[92][93] At the time, most of the sulfate available converted into sulfide through processes of sulfate reduction, such as being recycled back into the mantle,[88] or by conversion via microbial activity.[94]

As oxygen began to rapidly accumulate in the atmosphere, sulfate levels began to increase in the seawater and sedimentary reservoirs, while the circulation of sulfide decreased as a result. Between 2500 and 2300 Ma, the isotopic ratio of sulfate (δ34S) increased from 10 to 12‰ as a result of aerobic weathering and precipitation, entering the sedimentary record asgypsum andanhydrite.[95] At the same time, the levels of sulfide experienced decreases as a result of the spike in oxygen, with its δ34S value reaching as low as −30‰.[96][97]

Isotopic composition of nitrogen

[edit]

The isotopic ratio of nitrogen (δ15N) was relatively constant during the Siderian, ranging from 1.1 to 7.7‰ between 2450 and 2300 Ma.[98][99] Some concentrations formed askerogen in South Africa's Timeball Hill Formation, while traces existed asshale in Australia'sTuree Creek Group.[100] Despite the stability of nitrogen carried out throughits circulation,[101] the oxidation of the ocean's surface water slowly increased the size ofnitrate reservoirs,[100] with seawater concentrations ranging from 0.35 to 3.5 μM.[102]

Composition of strontium and rubidium

[edit]

There have been fluctuations in the ocean's level ofstrontium. At the time, its87Sr/86Sr isotopic ratio was relatively balanced; while its sources involved periods of high weathering rates, its sinks were due to the input of strontium from hydrothermal ventilation,[103] along with the recrystallization ofcalcite anddolomite in the ocean's crust.[104] Nonetheless, the ratio's value began a trend of increase up until theOrosirian Period, beginning with a value of 0.7022 in 2500 Ma.[103] Traces of this strontium have been identified within the Polisarka Formation's bedding. The concentrations in carbonate rocks ranged between 560 and 1030 ppm, dating between 2441 and 2434.8 Ma, while calcites and inorganicaragonites hold values of 1000 and 9000 ppm respectively.[104]

Strontium has also been detected through thebeta decay andradiometric dating ofrubidium (Rb–Sr), and is mainly connected to the deposition of volcanic rocks. At theFennoscandian Shield, this isotopic presence has been found indacite and basalticandesite within the Pechenga–Varzuga Belt, dating back to 2324 Ma,[105][106] and indicates the creation ofpaleosols from an intense weathering period.[107] Similar Rb–Sr datings have been found in the Superior and Kaapvaal cratons; the 2330 Ma dating of volcanictuffs in North America's McKam Formation serves as one of the marks of the beginning of the Huronian glaciation,[108] while a 2300 Ma dating in South Africa represents a unconformity between the Transvaal and Ventersdrop supergroups.[109] Additionally, rubidium and strontium have been detected inmigmatite found in eastern Hebei's Qianxi Group, and are dated back to 2480 Ma.[110]

See also

[edit]
  • Sleaford orogeny – a craton forming event which occurred from 2460 to 2410 million years ago

References

[edit]

Notes

[edit]
  1. ^A lower boundary was not defined for this proposal.[3]
  2. ^The "Era" subdivision was chosen under the pretense to use aPrecambrian chronostratic scale, and does not represent the modern use defined by theInternational Commission on Stratigraphy.[8]
  3. ^In the context of iron formations, "orthochemical" refers to iron formations that are dominated by fine-grained iron-rich material, consisting of tiny rock grains that were formedin situ (i.e., formed where they were deposited, not transported to their place of deposition).[36]

Citations

[edit]
  1. ^Teitler et al. 2014, §§ 1–2.1, pp. 71-72.
  2. ^Yakubchuk 2019, p. 169.
  3. ^abShields, Graham A.; Strachan, Robin A.;Porter, Susannah M.; Halverson, Galen P.; Macdonald, Francis A.; Plumb, Kenneth A.; Alvarenga, Carlos J. de; Banerjee, Dhiraj M.; Bekker, Andrey; Bleeker, Wouter; Brasier, Alexander; Chakraborty, Partha P.; Collins, Alan S.;Condie, Kent; Das, Kaushik; Evans, David A. D.; Ernst, Richard; Fallick, Anthony E.; Frimmel, Hartwig; Fuck, Reinhardt;Hoffman, Paul F.; Kamber, Balz S.; Kuznetsov, Anton B.; Mitchell, Ross N.; Poiré, Daniel G.; Poulton, Simon W.; Riding, Robert; Sharma, Mukund; Storey, Craig; Stueeken, Eva; Tostevin, Rosalie; Turner, Elizabeth;Xiao, Shuhai; Zhang, Shuanhong; Zhou, Ying; Zhu, Maoyan (July 7, 2021)."A template for an improved rock-based subdivision of the pre-Cryogenian timescale"(PDF).Journal of the Geological Society.179 (1) jgs2020-222.Geological Society of London.Bibcode:2022JGSoc.179..222S.doi:10.1144/jgs2020-222.eISSN 2041-479X.ISSN 0016-7649.LCCN 79641612.OCLC 1934542.S2CID 236285974.Archived(PDF) from the original on January 24, 2025. RetrievedDecember 11, 2025.Open access icon
  4. ^abcPlumb, Kenneth A. (June 1991)."New Precambrian time scale".Episodes.14 (2):139–140.doi:10.18814/epiiugs/1991/v14i2/005.eISSN 2586-1298.ISSN 0705-3797.LCCN 78646808.OCLC 4130038.S2CID 126954461.Open access icon
  5. ^abCatling, David C.;Zahnle, Kevin J. (February 26, 2020)."The Archean atmosphere".Science Advances.6 (9) eaax1420.American Association for the Advancement of Science.Bibcode:2020SciA....6.1420C.doi:10.1126/sciadv.aax1420.eISSN 2375-2548.PMC 7043912.PMID 32133393.S2CID 212116079.Open access icon
  6. ^Teitler et al. 2014, §§ 4.2, 5, pp. 76–78.
  7. ^Cowie, Ziegler & Remane 1989, p. 79.
  8. ^Harland et al. 1990, §§ 3.4–3.5, pp. 21–22.
  9. ^Harland et al. 1990, §§ 3.5, 3.5.5, pp. 22, 25–26.
  10. ^Logan, William E.; Murray, Alexander; Hunt, T. Sterry; Billings, E. (1863)."Huronian Series".Report of progress from its commencement to 1863.Geological Survey of Canada. pp. 50–66.doi:10.4095/123563.LCCN 04006403.S2CID 210101061.
  11. ^Kranendonk 2012, § 16.5.2.3, pp.361362.
  12. ^Kranendonk 2012, § 16.5.4.1, pp.361,363.
  13. ^"International Chronostratigraphic Chart"(PDF).International Commission on Stratigraphy. December 2024. RetrievedOctober 23, 2025.
  14. ^Barley, Bekker & Krapež 2005, § 3, pp.163–164.
  15. ^Barley, Bekker & Krapež 2005, § 4, p.165.
  16. ^abKrapež, Bryan; Barley, Mark E.; Pickard, April L. (October 2003)."Hydrothermal and resedimented origins of the precursor sediments to banded iron formation: sedimentological evidence from the Early Palaeoproterozoic Brockman Supersequence of Western Australia"(PDF).Sedimentology.50 (5). International Association of Sedimentologists:979–1011.Bibcode:2003Sedim..50..979K.doi:10.1046/j.1365-3091.2003.00594.x.eISSN 1365-3091.ISSN 0037-0746.LCCN 67003114.OCLC 1765340.S2CID 131361021. Archived fromthe original(PDF) on August 10, 2017. RetrievedDecember 25, 2025.
  17. ^Mojzsis, S. J.; Coath, C. D.; Greenwood, J. P.; McKeegan, K. D.; Harrison, T. M. (May 2003)."Mass-independent isotope effects in Archean (2.5 to 3.8 Ga) sedimentary sulfides determined by ion microprobe analysis"(PDF).Geochimica et Cosmochimica Acta.67 (9).Elsevier:1635–1638.Bibcode:2003GeCoA..67.1635M.doi:10.1016/S0016-7037(03)00059-0.eISSN 1872-9533.ISSN 0016-7037.LCCN 53032712.OCLC 1570626.S2CID 38837378. Archived fromthe original(PDF) on May 26, 2019. RetrievedDecember 10, 2025.
  18. ^Barley, Mark E.; Pickard, April L.; Sylvester, P. J. (January 1997)."Emplacement of a large igneous province as a possible cause of banded iron formation 2.45 billion years ago".Nature.385 (6611):55–58.Bibcode:1997Natur.385...55B.doi:10.1038/385055a0.eISSN 1476-4687.ISSN 0028-0836.LCCN 12037118.OCLC 1586310.S2CID 4250877. RetrievedNovember 29, 2025.
  19. ^McLennan, Simonetti & Goldstein 2000, §§ 1–2, pp. 265–266.
  20. ^Al-hashim 2016, § 1.5, pp. 9–18.
  21. ^Al-hashim 2016, § 1.5.3, pp. 13–14.
  22. ^Ross 1981, §§ 1.2, 6, pp.3–6,79.
  23. ^Al-hashim 2016, § 1.5.4, p. 17.
  24. ^Houston & Karlstrom 1992, pp. 5–13.
  25. ^Aspler et al. 2001, p. 291.
  26. ^Al-hashim 2016, §§ 1.5.2–1.5.3, pp. 13–14.
  27. ^Houston & Karlstrom 1992, pp. 7–9.
  28. ^Ojakangas, Marmo & Heiskanen 2001, §§ 2.1–2.1.1, 2.2.1, pp. 258–260, 264.
  29. ^Ojakangas, Marmo & Heiskanen 2001, §§ 2.1, 2.2.2, pp. 258–259, 264.
  30. ^Ojakangas, Marmo & Heiskanen 2001, §§ 2.1.2, 2.2.2, pp. 261, 264–265.
  31. ^Warke 2017, § 2.1.1, p. 33.
  32. ^Warke 2017, §§ 2.1.1, 2.1.3–2.1.7, pp. 33, 38–49.
  33. ^Warke 2017, §§ 2.1.3, 2.1.5, pp. 38, 44.
  34. ^Warke 2017, §§ 2.1.6–2.1.7, pp. 45–46, 48.
  35. ^Warke 2017, §§ 2.1.1, 2.1.3, 2.1.6, pp. 33, 38, 46.
  36. ^Beukes 1983, pp. 141, 161–162.
  37. ^Warke 2017, § 2.1.6, pp. 45–47.
  38. ^Dazhong & Songnian 1985, pp. 145–150.
  39. ^Zhao 1987, p. 8.
  40. ^Dazhong & Songnian 1985, pp. 145–146.
  41. ^Dazhong & Songnian 1985, pp. 147–150.
  42. ^Heaman, L. M. (June 1994)."2.45 Ga Global Mafic Magmatism: Earth's Oldest Superplume?". In Lanphere, M. A.; Dalrymple, G. B.; Turrin, B. D. (eds.).Abstracts of the Eighth International Conference on Geochronology, Cosmochronology, and Isotope Geology.United States Geological Survey. p. 132.ISBN 978-0-7881-1349-9.LCCN 94193205.OCLC 30658967.
  43. ^Ernst & Buchan 2004, p. 105.
  44. ^Phinney & Halls 2001, p. 1542.
  45. ^Phinney & Halls 2001, p. 1543.
  46. ^Davies & Heaman 2014, pp. 180, 194.
  47. ^Smirnov et al. 2013, pp. 11–12.
  48. ^Smirnov et al. 2013, pp. 18,20.
  49. ^abYakubchuk 2019, p. 180.
  50. ^Aspler et al. 2001, p. 287.
  51. ^Bekker, Andrey; Eriksson, Kenneth A. (February 10, 2003)."A Paleoproterozoic drowned carbonate platform on the southeastern margin of the Wyoming Craton: a record of the Kenorland breakup"(PDF).Precambrian Research.120 (3–4).Elsevier:327–364.Bibcode:2003PreR..120..327B.doi:10.1016/S0301-9268(02)00165-1.eISSN 1872-7433.ISSN 0301-9268.LCCN 74642650.OCLC 1792859.S2CID 128917263. Archived fromthe original(PDF) on August 24, 2015. RetrievedDecember 10, 2025.
  52. ^Houston & Karlstrom 1992, pp. 5–7.
  53. ^Daly, J. Stephen; Balagansky, Victor V.; Timmerman, Martin J.; Whitehouse, Martin J. (2006). "The Lapland-Kola orogen: Palaeoproterozoic collision and accretion of the northern Fennoscandian lithosphere". In Gee, D. G.; Stephenson, R. A. (eds.).European Lithosphere Dynamics. Vol. 32.Geological Society of London. pp. 579–598.Bibcode:2006GSLMm..32..579D.doi:10.1144/GSL.MEM.2006.032.01.35.ISBN 978-1-86239-212-0.LCCN 2007274602.OCLC 78202548.S2CID 129511509.
  54. ^Astaf'ev, B. Yu.; Levchenkov, O. A.; Rizanova, N. G.; Voinova, O. A.; Voinov, A. S.; Levskii, L. K.; Makeev, A. F.; Lokhov, K. I. (March 2010)."Geological Structure and Isotopic–Geochronologic Study of Rocks from the Strel'na Segment of the Terskii Greenstone Belt, Kola Peninsula".Stratigraphy and Geological Correlation.18 (1). Pleiades Publishing:1–15.Bibcode:2010SGC....18....1A.doi:10.1134/S0869593810010016.eISSN 1555-6263.ISSN 0869-5938.LCCN 93641701.OCLC 29573835.S2CID 140562071. RetrievedDecember 7, 2025.
  55. ^Teitler et al. 2014, p. 78.
  56. ^Tang & Chen 2013, pp. 589–591.
  57. ^Holland 2002, pp. 3819–3820.
  58. ^Karhu, Juha A.;Holland, Heinrich D. (October 1996)."Carbon isotopes and the rise of atmospheric oxygen".Geology.24 (10).Geological Society of America:867–870.Bibcode:1996Geo....24..867K.doi:10.1130/0091-7613(1996)024<0867:CIATRO>2.3.CO;2.eISSN 1943-2682.ISSN 0091-7613.LCCN 73645581.OCLC 1788177.S2CID 129655228. RetrievedDecember 2, 2025.
  59. ^Barley, Bekker & Krapež 2005, p. 157.
  60. ^Barley, Bekker & Krapež 2005, pp. 159,167–169.
  61. ^Papineau 2010, pp. 168–170.
  62. ^Teitler et al. 2014, §§ 4.2–5, pp. 76–78.
  63. ^Kopp et al. 2005, p. 11133.
  64. ^Teitler et al. 2014, pp. 73, 76.
  65. ^Kopp et al. 2005, p. 11134.
  66. ^Teitler et al. 2014, p. 71.
  67. ^abcdePehrsson et al. 2014, p. 807.
  68. ^Hoffman 2013, p. 150.
  69. ^Hoffman 2013, p. 145.
  70. ^Brasier, A. T.; Martin, A. P.; Melezhik, V. A.; Prave, A. R.; Condon, D. J.; Fallick, A. E.; FAR-DEEP Scientists (September 2013)."Earth's earliest global glaciation? Carbonate geochemistry and geochronology of the Polisarka Sedimentary Formation, Kola Peninsula, Russia".Precambrian Research.235.Elsevier:278–294.Bibcode:2013PreR..235..278B.doi:10.1016/j.precamres.2013.06.007.eISSN 1872-7433.ISSN 0301-9268.LCCN 74642650.OCLC 1792859.S2CID 53008028. RetrievedDecember 9, 2025.
  71. ^Hoffman 2013, pp. 151–152.
  72. ^Hoffman 2013, p. 151.
  73. ^Hoffman 2013, pp. 145, 150, 152.
  74. ^Boden, Joanne S.; Nieves-Morión, Mercedes; Nürnberg, Dennis J.; Arévalo, Sergio; Flores, Enrique; Sánchez-Baracaldo, Patricia (November 27, 2025)."Evolution of multicellularity genes in Cyanobacteria in the lead up to the great oxidation event".Communications Biology.8 (1) 1721.Springer Nature.doi:10.1038/s42003-025-09247-6.eISSN 2399-3642.PMC 12669612.PMID 41309968.S2CID 283350357.Open access icon
  75. ^Hedges, S. Blair; Blair, Jaime E.; Venturi, Maria L.; Shoe, Jason L. (January 28, 2004)."A molecular timescale of eukaryote evolution and the rise of complex multicellular life".BMC Evolutionary Biology.4 2.BioMed Central.doi:10.1186/1471-2148-4-2.eISSN 2730-7182.PMC 341452.PMID 15005799.Open access icon
  76. ^Knoll & Holland 1995, p. 27.
  77. ^abIvarsson et al. 2020, pp. 5–6.
  78. ^Barlow & Kranendonk 2018, p. 450.
  79. ^Klein, Cornelis; Beukes, N. J.; Schopf, J. W. (May 1987)."Filamentous microfossils in the early proterozoic transvaal supergroup: their morphology, significance, and paleoenvironmental setting".Precambrian Research.36 (1).Elsevier:81–94.Bibcode:1987PreR...36...81K.doi:10.1016/0301-9268(87)90018-0.eISSN 1872-7433.ISSN 0301-9268.LCCN 74642650.OCLC 1792859.S2CID 129477033. RetrievedDecember 26, 2025.
  80. ^Shixing & Huineng 1992, p. 138.
  81. ^Melezhik et al. 1997, pp. 311, 327, 332.
  82. ^Bengston et al. 2017, p. 1.
  83. ^Bengston et al. 2017, pp. 1, 3.
  84. ^Bengston et al. 2017, pp. 4–5.
  85. ^abPlanavsky et al. 2012, p. 159.
  86. ^Rouxel, Bekker & Edwards 2005, pp. 1089–1090.
  87. ^Planavsky et al. 2012, pp. 161,164.
  88. ^abCanfield 2004, p. 846.
  89. ^Kah, Lyons & Frank 2004, p. 837.
  90. ^Canfield 2004, p. 844.
  91. ^Fakhraee, Mojtaba; Crowe, Sean A.; Katsev, Sergei (January 24, 2018)."Sedimentary sulfur isotopes and Neoarchean ocean oxygenation".Science Advances.4 (1) e1701835.American Association for the Advancement of Science.Bibcode:2018SciA....4.1835F.doi:10.1126/sciadv.1701835.eISSN 2375-2548.PMC 5783677.PMID 29376118.S2CID 13680145.Open access icon
  92. ^Fakhraee et al. 2019, p. 375.
  93. ^Habicht et al. 2002, p. 2374.
  94. ^Harada et al. 2025, p. 4.
  95. ^Canfield 2004, pp. 840, 842, 845.
  96. ^Canfield & Farquhar 2009, p. 8123.
  97. ^Cameron 1983, p. 54.
  98. ^Kipp et al. 2018, pp. 119–120, 123.
  99. ^Luo et al. 2018, pp. 2–4.
  100. ^abKipp et al. 2018, pp. 122–123.
  101. ^Kipp et al. 2018, p. 119.
  102. ^Wang et al. 2025, pp. 8–9.
  103. ^abPapineau 2010, p. 172.
  104. ^abBrasier et al. 2013, p. 291.
  105. ^Daly et al. 2006, p. 584.
  106. ^Ojakangas, Marmo & Heiskanen 2001, § 8, p. 278.
  107. ^Melezhik et al. 1997, p. 314.
  108. ^Tang & Chen 2013, p. 586.
  109. ^Beukes 1983, p. 140.
  110. ^Dazhong & Songnian 1985, p. 143.

Sources

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External links

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Siderian at Wikipedia'ssister projects
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).
See also:Geologic time scale  • iconGeology portal  • World portal
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