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[[File:Geologic time scale - spiral - ICS colours (light) - path text.svg|upright=1.35|alt=Geologic time scale proportionally represented as a log-spiral. The image also shows some notable events in Earth's history and the general evolution of life.|thumb|The geologic time scale, proportionally represented as a [[Logarithmic spiral|log-spiral]] with some major events in Earth's history. A [[megaannus]] (Ma) represents one million (10<sup>6</sup>) years.]]
[[File:Geologic time scale - spiral - ICS colours (light) - path text.svg|upright=1.35|alt=Geologic time scale proportionally represented as a log-spiral. The image also shows some notable events in Earth's history and the general evolution of life.|thumb|The geologic time scale, proportionally represented as a [[Logarithmic spiral|log-spiral]] with some major events in Earth's history. A [[megaannus]] (Ma) represents one million (10<sup>6</sup>) years.]]


The '''geologic time scale''' or '''geological time scale''' ('''GTS''') is a representation of [[time]] based on the [[geologic record|rock record]] of [[Earth]]. It is a system of [[chronological dating]] that uses [[chronostratigraphy]] (the process of relating [[stratum|strata]] to time) and [[geochronology]] (a scientific branch of [[geology]] that aims to determine the age of rocks). It is used primarily by [[Earth science|Earth scientists]] (including [[geologist]]s, [[paleontology|paleontologists]], [[geophysics|geophysicists]], [[geochemistry|geochemists]], and [[paleoclimatology|paleoclimatologists]]) to describe the timing and relationships of events in geologic history. The time scale has been developed through the study of rock layers and the observation of their relationships and identifying features such as [[lithology|lithologies]], [[paleomagnetism|paleomagnetic]] properties, and [[fossil]]s. The definition of standardised international units of geological time is the responsibility of the [[International Commission on Stratigraphy]] (ICS), a constituent body of the [[International Union of Geological Sciences]] (IUGS), whose primary objective<ref name="ICS_statutes">{{Cite web |title=Statues & Guidelines |url=https://stratigraphy.org/statutes |access-date=2022-04-05 |website= |publisher=International Commission on Stratigraphy}}</ref> is to precisely define global chronostratigraphic units of the International Chronostratigraphic Chart (ICC)<ref name="ICC_Cohen_2013">{{Cite journal |last1=Cohen |first1=K.M. |last2=Finney |first2=S.C. |last3=Gibbard |first3=P.L. |last4=Fan |first4=J.-X. |date=2013-09-01 |title=The ICS International Chronostratigraphic Chart |journal=Episodes |language=en |edition=updated |volume=36 |issue=3 |pages=199–204 |doi=10.18814/epiiugs/2013/v36i3/002 |s2cid=51819600 |issn=0705-3797|doi-access=free }}</ref> that are used to define divisions of geological time. The chronostratigraphic divisions are in turn used to define geochronologic units.<ref name="ICC_Cohen_2013" />
The '''geologic time scale''' or '''geological time scale''' ('''GTS''') is a representation of [[time]] based on the [[geologic record|rock record]] of [[Earth]]. It is a system of [[chronological dating]] that uses [[chronostratigraphy]] (the process of relating [[stratum|strata]] to time) and [[geochronology]] (a scientific branch of [[geology]] that aims to determine the age of rocks). It is used primarily by [[Earth science|Earth scientists]] (including [[geologist]]s, [[paleontology|paleontologists]], [[geophysics|geophysicists]], [[geochemistry|geochemists]], and [[paleoclimatology|paleoclimatologists]]) to describe the timing and relationships of events in geologic history. The time scale has been developed through the study of rock layers and the observation of their relationships and identifying features such as [[lithology|lithologies]], [[paleomagnetism|paleomagnetic]] properties, and [[fossil]]s. The definition of standardised international units of geological time is the responsibility of the [[International Commission on Stratigraphy]] (ICS), a constituent body of the [[International Union of Geological Sciences]] (IUGS), whose primary objective<ref name="ICS_statutes">{{Cite web |title=Statues & Guidelines |url=https://stratigraphy.org/statutes |access-date=2022-04-05 |website= |publisher=International Commission on Stratigraphy}}</ref> is to precisely define global chronostratigraphic units of the International Chronostratigraphic Chart (ICC){{ref icc}} that are used to define divisions of geological time. The chronostratigraphic divisions are in turn used to define geochronologic units.<ref name="ICS" />


== Principles ==
== Principles ==
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The [[law of superposition]] that states that in undeformed stratigraphic sequences the oldest strata will lie at the bottom of the sequence, while newer material stacks upon the surface.<ref name="Steno_1669" /><ref name="Hutton_1795v1" /><ref name="Lyell_1832v1" /><ref name="Boggs-2011" /> In practice, this means a younger rock will lie on top of an older rock unless there is evidence to suggest otherwise.
The [[law of superposition]] that states that in undeformed stratigraphic sequences the oldest strata will lie at the bottom of the sequence, while newer material stacks upon the surface.<ref name="Steno_1669" /><ref name="Hutton_1795v1" /><ref name="Lyell_1832v1" /><ref name="Boggs-2011" /> In practice, this means a younger rock will lie on top of an older rock unless there is evidence to suggest otherwise.


The [[principle of original horizontality]] that states layers of sediments will originally be deposited horizontally under the action of gravity.<ref name="Steno_1669" /><ref name="Lyell_1832v1" /><ref name="Boggs-2011" /> However, it is now known that not all sedimentary layers are deposited purely horizontally,<ref name="Boggs-2011" /><ref name=Mehta_et_al_1994>{{Cite journal |last1=Mehta |first1=A |last2=Barker |first2=G C |date=1994-04-01 |title=The dynamics of sand |url=https://iopscience.iop.org/article/10.1088/0034-4885/57/4/002 |journal=Reports on Progress in Physics |volume=57 |issue=4 |pages=383–416 |doi=10.1088/0034-4885/57/4/002 |issn=0034-4885}}</ref> but this principle is still a useful concept.
The [[principle of original horizontality]] that states layers of sediments will originally be deposited horizontally under the action of gravity.<ref name="Steno_1669" /><ref name="Lyell_1832v1" /><ref name="Boggs-2011" /> However, it is now known that not all sedimentary layers are deposited purely horizontally,<ref name="Boggs-2011" /><ref name=Mehta_et_al_1994>{{Cite journal |last1=Mehta |first1=A |last2=Barker |first2=G C |date=1994-04-01 |title=The dynamics of sand |url=https://iopscience.iop.org/article/10.1088/0034-4885/57/4/002 |journal=Reports on Progress in Physics |volume=57 |issue=4 |pages=383–416 |doi=10.1088/0034-4885/57/4/002 |bibcode=1994RPPh...57..383M |issn=0034-4885}}</ref> but this principle is still a useful concept.


The [[principle of lateral continuity]] that states layers of sediments extend laterally in all directions until either thinning out or being cut off by a different rock layer, i.e. they are laterally continuous.<ref name="Steno_1669" /> Layers do not extend indefinitely; their limits are controlled by the amount and type of sediment in a [[sedimentary basin]], and the geometry of that basin.
The [[principle of lateral continuity]] that states layers of sediments extend laterally in all directions until either thinning out or being cut off by a different rock layer, i.e. they are laterally continuous.<ref name="Steno_1669" /> Layers do not extend indefinitely; their limits are controlled by the amount and type of sediment in a [[sedimentary basin]], and the geometry of that basin.
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The geologic time scale is divided into chronostratigraphic units and their corresponding geochronologic units.
The geologic time scale is divided into chronostratigraphic units and their corresponding geochronologic units.


* An '''{{visible anchor|eon}}''' is the largest geochronologic time unit and is equivalent to a chronostratigraphic [[eonothem]].<ref name="dictionary_of_geology_2020">{{Cite book |url=https://www.worldcat.org/oclc/1137380460 |title=A dictionary of geology and earth sciences |date=2020 |author=Michael Allaby |isbn=978-0-19-187490-1 |edition=Fifth |location=Oxford |oclc=1137380460}}</ref> There are four formally defined eons: the [[Hadean]], [[Archean]], [[Proterozoic]] and [[Phanerozoic]].<ref name="ICC_Cohen_2013" />
* An '''{{visible anchor|eon}}''' is the largest geochronologic time unit and is equivalent to a chronostratigraphic [[eonothem]].<ref name="dictionary_of_geology_2020">{{Cite book |title=A dictionary of geology and earth sciences |date=2020 |author=Michael Allaby |isbn=978-0-19-187490-1 |edition=Fifth |location=Oxford |oclc=1137380460}}</ref> There are four formally defined eons: the [[Hadean]], [[Archean]], [[Proterozoic]] and [[Phanerozoic]].<ref name="ICS" />
* An '''{{visible anchor|era}}''' is the second largest geochronologic time unit and is equivalent to a chronostratigraphic [[erathem]].<ref name="ICS_chronostrat" /><ref name="dictionary_of_geology_2020" /> There are ten defined eras: the [[Eoarchean]], [[Paleoarchean]], [[Mesoarchean]], [[Neoarchean]], [[Paleoproterozoic]], [[Mesoproterozoic]], [[Neoproterozoic]], [[Paleozoic]], [[Mesozoic]] and [[Cenozoic]], with none from the Hadean eon.<ref name="ICC_Cohen_2013" />
* An '''{{visible anchor|era}}''' is the second largest geochronologic time unit and is equivalent to a chronostratigraphic [[erathem]].<ref name="ICS_chronostrat" /><ref name="dictionary_of_geology_2020" /> There are ten defined eras: the [[Eoarchean]], [[Paleoarchean]], [[Mesoarchean]], [[Neoarchean]], [[Paleoproterozoic]], [[Mesoproterozoic]], [[Neoproterozoic]], [[Paleozoic]], [[Mesozoic]] and [[Cenozoic]], with none from the Hadean eon.<ref name="ICS" />
* A '''{{visible anchor|period}}''' is equivalent to a chronostratigraphic [[system (stratigraphy)|system]].<ref name="ICS_chronostrat" /><ref name="dictionary_of_geology_2020" /> There are 22 defined periods, with the current being the [[Quaternary]] period.<ref name="ICC_Cohen_2013" /> As an exception, two subperiods are used for the [[Carboniferous|Carboniferous Period]].<ref name="ICS_chronostrat" />
* A '''{{visible anchor|period}}''' is equivalent to a chronostratigraphic [[system (stratigraphy)|system]].<ref name="ICS_chronostrat" /><ref name="dictionary_of_geology_2020" /> There are 22 defined periods, with the current being the [[Quaternary]] period.<ref name="ICS" /> As an exception, two subperiods are used for the [[Carboniferous|Carboniferous Period]].<ref name="ICS_chronostrat" />
* An '''{{visible anchor|epoch}}''' is the second smallest geochronologic unit. It is equivalent to a chronostratigraphic [[series (stratigraphy)|series]].<ref name="ICS_chronostrat" /><ref name="dictionary_of_geology_2020" /> There are 37 defined epochs and one informal one. The current epoch is the [[Holocene]]. There are also 11 subepochs which are all within the [[Neogene]] and Quaternary.<ref name="ICC_Cohen_2013" /> The use of subepochs as formal units in international chronostratigraphy was ratified in 2022.<ref name="Aubry_2022_subseries">{{Cite journal |last1=Aubry |first1=Marie-Pierre |last2=Piller |first2=Werner E. |last3=Gibbard |first3=Philip L. |last4=Harper |first4=David A. T. |last5=Finney |first5=Stanley C. |date=2022-03-01 |title=Ratification of subseries/subepochs as formal rank/units in international chronostratigraphy |journal=Episodes |language=en |volume=45 |issue=1 |pages=97–99 |doi=10.18814/epiiugs/2021/021016 |s2cid=240772165 |issn=0705-3797|doi-access=free }}</ref>
* An '''{{visible anchor|epoch}}''' is the second smallest geochronologic unit. It is equivalent to a chronostratigraphic [[series (stratigraphy)|series]].<ref name="ICS_chronostrat" /><ref name="dictionary_of_geology_2020" /> There are 37 defined epochs and one informal one. The current epoch is the [[Holocene]]. There are also 11 subepochs which are all within the [[Neogene]] and Quaternary.<ref name="ICS" /> The use of subepochs as formal units in international chronostratigraphy was ratified in 2022.<ref name="Aubry_2022_subseries">{{Cite journal |last1=Aubry |first1=Marie-Pierre |last2=Piller |first2=Werner E. |last3=Gibbard |first3=Philip L. |last4=Harper |first4=David A. T. |last5=Finney |first5=Stanley C. |date=2022-03-01 |title=Ratification of subseries/subepochs as formal rank/units in international chronostratigraphy |journal=Episodes |language=en |volume=45 |issue=1 |pages=97–99 |doi=10.18814/epiiugs/2021/021016 |s2cid=240772165 |issn=0705-3797|doi-access=free }}</ref>
* An '''{{visible anchor|age}}''' is the smallest hierarchical geochronologic unit. It is equivalent to a chronostratigraphic [[stage (stratigraphy)|stage]].<ref name="ICS_chronostrat" /><ref name="dictionary_of_geology_2020" /> There are 96 formal and five informal ages.<ref name="ICC_Cohen_2013" /> The current age is the [[Meghalayan]].
* An '''{{visible anchor|age}}''' is the smallest hierarchical geochronologic unit. It is equivalent to a chronostratigraphic [[stage (stratigraphy)|stage]].<ref name="ICS_chronostrat" /><ref name="dictionary_of_geology_2020" /> There are 96 formal and five informal ages.<ref name="ICS" /> The current age is the [[Meghalayan]].
* A ''{{visible anchor|chron}}'' is a non-hierarchical formal geochronology unit of unspecified rank and is equivalent to a chronostratigraphic [[chronozone]].<ref name="ICS_chronostrat" /> These correlate with [[Magnetostratigraphy|magnetostratigraphic]], [[Lithostratigraphy|lithostratigraphic]], or [[Biostratigraphy|biostratigraphic]] units as they are based on previously defined stratigraphic units or geologic features.
* A ''{{visible anchor|chron}}'' is a non-hierarchical formal geochronology unit of unspecified rank and is equivalent to a chronostratigraphic [[chronozone]].<ref name="ICS_chronostrat" /> These correlate with [[Magnetostratigraphy|magnetostratigraphic]], [[Lithostratigraphy|lithostratigraphic]], or [[Biostratigraphy|biostratigraphic]] units as they are based on previously defined stratigraphic units or geologic features.


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A {{em|[[Global Standard Stratigraphic Age]]}} (GSSA)<ref name="Remane_1996_GSSP">{{Cite journal |last1=Remane |first1=Jürgen |last2=Bassett |first2=Michael G |last3=Cowie |first3=John W |last4=Gohrbandt |first4=Klaus H |last5=Lane |first5=H Richard |last6=Michelsen |first6=Olaf |last7=Naiwen |first7=Wang |last8=the cooperation of members of ICS |date=1996-09-01 |title=Revised guidelines for the establishment of global chronostratigraphic standards by the International Commission on Stratigraphy (ICS) |journal=Episodes |language=en |volume=19 |issue=3 |pages=77–81 |doi=10.18814/epiiugs/1996/v19i3/007 |issn=0705-3797|doi-access=free }}</ref> is a numeric-only, chronologic reference point used to define the base of geochronologic units prior to the Cryogenian. These points are arbitrarily defined.<ref name="ICS_chronostrat"/> They are used where GSSPs have not yet been established. Research is ongoing to define GSSPs for the base of all units that are currently defined by GSSAs.
A {{em|[[Global Standard Stratigraphic Age]]}} (GSSA)<ref name="Remane_1996_GSSP">{{Cite journal |last1=Remane |first1=Jürgen |last2=Bassett |first2=Michael G |last3=Cowie |first3=John W |last4=Gohrbandt |first4=Klaus H |last5=Lane |first5=H Richard |last6=Michelsen |first6=Olaf |last7=Naiwen |first7=Wang |last8=the cooperation of members of ICS |date=1996-09-01 |title=Revised guidelines for the establishment of global chronostratigraphic standards by the International Commission on Stratigraphy (ICS) |journal=Episodes |language=en |volume=19 |issue=3 |pages=77–81 |doi=10.18814/epiiugs/1996/v19i3/007 |issn=0705-3797|doi-access=free }}</ref> is a numeric-only, chronologic reference point used to define the base of geochronologic units prior to the Cryogenian. These points are arbitrarily defined.<ref name="ICS_chronostrat"/> They are used where GSSPs have not yet been established. Research is ongoing to define GSSPs for the base of all units that are currently defined by GSSAs.


The standard international units of the geologic time scale are published by the International Commission on Stratigraphy on the International Chronostratigraphic Chart; however, regional terms are still in use in some areas. The numeric values on the International Chronostratigrahpic Chart are represented by the unit [[Megaannum|Ma]] (megaannum, for 'million [[year]]s'). For example, {{Period start|Jurassic}} {{Period start error|Jurassic}} Ma, the lower boundary of the [[Jurassic]] Period, is defined as 201,400,000 years old with an uncertainty of 200,000 years. Other [[Si prefix|SI prefix]] units commonly used by geologists are [[Gigaannum|Ga]] (gigaannum, billion years), and [[Kiloannums|ka]] (kiloannum, thousand years), with the latter often represented in calibrated units ([[Before Present|before present]]).
The standard international units of the geologic time scale are published by the International Commission on Stratigraphy on the International Chronostratigraphic Chart. However, regional terms are still in use in some areas. The numeric values on the International Chronostratigrahpic Chart are represented by the unit [[Megaannum|Ma]] (megaannum, for 'million [[year]]s'). For example, {{Period start|Jurassic}} {{Period start error|Jurassic}} Ma, the lower boundary of the [[Jurassic]] Period, is defined as 201,400,000 years old with an uncertainty of 200,000 years. Other [[Si prefix|SI prefix]] units commonly used by geologists are [[Gigaannum|Ga]] (gigaannum, billion years), and [[Kiloannums|ka]] (kiloannum, thousand years), with the latter often represented in calibrated units ([[Before Present|before present]]).


== Naming of geologic time ==
== Naming of geologic time ==
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|{{Period span/brief|Quaternary|1}}
|{{Period span/brief|Quaternary|1}}
|{{#expr:{{Period start|Quaternary}}-{{Period end|Quaternary}}}}
|{{#expr:{{Period start|Quaternary}}-{{Period end|Quaternary}}}}
|First introduced by [[Jules Desnoyers]] in 1829 for sediments in [[France]]'s [[Seine]] Basin that appeared to be younger than [[Tertiary]]{{efn|The Tertiary is a now obsolete geologic system/period spanning from 66 Ma to 2.6 Ma. It has no exact equivalent in the modern ICC, but is approximately equivalent to the merged Palaeogene and Neogene systems/periods.<ref name="Head_etal_2008">{{Cite journal |last1=Head |first1=Martin J. |last2=Gibbard |first2=Philip |last3=Salvador |first3=Amos |date=2008-06-01 |title=The Quaternary: its character and definition |journal=Episodes |language=en |volume=31 |issue=2 |pages=234–238 |doi=10.18814/epiiugs/2008/v31i2/009 |doi-access=free |issn=0705-3797}}</ref><ref name ="Gibbard_etal_2010">{{Cite journal |last1=Gibbard |first1=Philip L. |last2=Head |first2=Martin J. |last3=Walker |first3=Michael J. C. |last4=the Subcommission on Quaternary Stratigraphy |date=2010-01-20 |title=Formal ratification of the Quaternary System/Period and the Pleistocene Series/Epoch with a base at 2.58 Ma |url=https://onlinelibrary.wiley.com/doi/10.1002/jqs.1338 |journal=Journal of Quaternary Science |language=en |volume=25 |issue=2 |pages=96–102 |doi=10.1002/jqs.1338 |bibcode=2010JQS....25...96G |issn=0267-8179}}</ref>|name=Tertiary|group=note}} rocks.<ref name="Desnoyers_1829">{{cite journal |last1=Desnoyers |first1=J. |title=Observations sur un ensemble de dépôts marins plus récents que les terrains tertiaires du bassin de la Seine, et constituant une formation géologique distincte; précédées d'un aperçu de la nonsimultanéité des bassins tertiares |journal=Annales des Sciences Naturelles |date=1829 |volume=16 |pages=171–214, 402–491 |url=https://www.biodiversitylibrary.org/item/29350#page/177/mode/1up |trans-title=Observations on a set of marine deposits [that are] more recent than the tertiary terrains of the Seine basin and [that] constitute a distinct geological formation; preceded by an outline of the non-simultaneity of tertiary basins |language=fr}} [https://www.biodiversitylibrary.org/item/29350#page/199/mode/1up From p. 193:] ''"Ce que je désirerais ... dont il faut également les distinguer."'' (What I would desire to prove above all is that the series of tertiary deposits continued – and even began in the more recent basins – for a long time, perhaps after that of the Seine had been completely filled, and that these later formations – ''Quaternary'' (1), so to say – should not retain the name of alluvial deposits any more than the true and ancient tertiary deposits, from which they must also be distinguished.)  However, on the very same page, Desnoyers abandoned the use of the term "Quaternary" because the distinction between Quaternary and Tertiary deposits wasn't clear.  From p. 193:  ''"La crainte de voir mal comprise ... que ceux du bassin de la Seine."'' (The fear of seeing my opinion in this regard be misunderstood or exaggerated, has made me abandon the word "quaternary", which at first I had wanted to apply to all deposits more recent than those of the Seine basin.)</ref>
|First introduced by [[Jules Desnoyers]] in 1829 for sediments in [[France]]'s [[Seine]] Basin that appeared to be younger than [[Tertiary (period)|Tertiary]]{{efn|The Tertiary is a now obsolete geologic system/period spanning from 66 Ma to 2.6 Ma. It has no exact equivalent in the modern ICC, but is approximately equivalent to the merged Palaeogene and Neogene systems/periods.<ref name="Head_etal_2008">{{Cite journal |last1=Head |first1=Martin J. |last2=Gibbard |first2=Philip |last3=Salvador |first3=Amos |date=2008-06-01 |title=The Quaternary: its character and definition |journal=Episodes |language=en |volume=31 |issue=2 |pages=234–238 |doi=10.18814/epiiugs/2008/v31i2/009 |doi-access=free |issn=0705-3797}}</ref><ref name ="Gibbard_etal_2010">{{Cite journal |last1=Gibbard |first1=Philip L. |last2=Head |first2=Martin J. |last3=Walker |first3=Michael J. C. |last4=the Subcommission on Quaternary Stratigraphy |date=2010-01-20 |title=Formal ratification of the Quaternary System/Period and the Pleistocene Series/Epoch with a base at 2.58 Ma |url=https://onlinelibrary.wiley.com/doi/10.1002/jqs.1338 |journal=Journal of Quaternary Science |language=en |volume=25 |issue=2 |pages=96–102 |doi=10.1002/jqs.1338 |bibcode=2010JQS....25...96G |issn=0267-8179}}</ref>|name=Tertiary|group=note}} rocks.<ref name="Desnoyers_1829">{{cite journal |last1=Desnoyers |first1=J. |title=Observations sur un ensemble de dépôts marins plus récents que les terrains tertiaires du bassin de la Seine, et constituant une formation géologique distincte; précédées d'un aperçu de la nonsimultanéité des bassins tertiares |journal=Annales des Sciences Naturelles |date=1829 |volume=16 |pages=171–214, 402–491 |url=https://www.biodiversitylibrary.org/item/29350#page/177/mode/1up |trans-title=Observations on a set of marine deposits [that are] more recent than the tertiary terrains of the Seine basin and [that] constitute a distinct geological formation; preceded by an outline of the non-simultaneity of tertiary basins |language=fr}} [https://www.biodiversitylibrary.org/item/29350#page/199/mode/1up From p. 193:] ''"Ce que je désirerais ... dont il faut également les distinguer."'' (What I would desire to prove above all is that the series of tertiary deposits continued – and even began in the more recent basins – for a long time, perhaps after that of the Seine had been completely filled, and that these later formations – ''Quaternary'' (1), so to say – should not retain the name of alluvial deposits any more than the true and ancient tertiary deposits, from which they must also be distinguished.)  However, on the very same page, Desnoyers abandoned the use of the term "Quaternary" because the distinction between Quaternary and Tertiary deposits wasn't clear.  From p. 193:  ''"La crainte de voir mal comprise ... que ceux du bassin de la Seine."'' (The fear of seeing my opinion in this regard be misunderstood or exaggerated, has made me abandon the word "quaternary", which at first I had wanted to apply to all deposits more recent than those of the Seine basin.)</ref>
|-
|-
|[[Neogene]]
|[[Neogene]]
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|{{Period span/brief|Cambrian|1}}
|{{Period span/brief|Cambrian|1}}
|{{#expr:{{Period start|Cambrian}}-{{Period end|Cambrian}}}}
|{{#expr:{{Period start|Cambrian}}-{{Period end|Cambrian}}}}
|Named for [[Cambria]], a [[latin]]ised form of the Welsh name for [[Wales]], ''Cymru''.<ref>{{cite EB1911|wstitle=Cambria}}</ref>
|Named for [[Cambria]], a [[Latin]]ised form of the Welsh name for [[Wales]], ''Cymru''.<ref>{{cite EB1911|wstitle=Cambria}}</ref>
|-
|-
|[[Ediacaran]]
|[[Ediacaran]]
|{{Period span/brief|Ediacaran|1}}
|{{Period span/brief|Ediacaran|1}}
|~{{#expr:{{Period start|Ediacaran}}-{{Period end|Ediacaran}}}}
|~{{#expr:{{Period start|Ediacaran}}-{{Period end|Ediacaran}}}}
|Named for the [[Ediacara Hills]]. Ediacara is possibly a corruption of [[Kuyani]] 'Yata Takarra' 'hard or stony ground'.<ref name="Butcher_2004">{{cite web |last=Butcher |first=Andy |date=26 May 2004 |title=Re: Ediacaran |url=http://listserv.linguistlist.org/cgi-bin/wa?A2=ind0405&L=australian-linguistics-l&D=1&P=264 |url-status=dead |archive-url=https://web.archive.org/web/20071023012434/http://listserv.linguistlist.org/cgi-bin/wa?A2=ind0405&L=australian-linguistics-l&D=1&P=264 |archive-date=23 October 2007 |access-date=19 July 2011 |work=LISTSERV 16.0 - AUSTRALIAN-LINGUISTICS-L Archives}}</ref><ref name="AHD_Ediacara_Fossil_Site">{{cite web |title=Place Details: Ediacara Fossil Site – Nilpena, Parachilna, SA, Australia |url=http://www.environment.gov.au/cgi-bin/ahdb/search.pl?mode=place_detail;place_id=105880 |url-status=live |archive-url=https://web.archive.org/web/20110603074010/http://www.environment.gov.au/cgi-bin/ahdb/search.pl?mode=place_detail;place_id=105880 |archive-date=3 June 2011 |access-date=19 July 2011 |work=Australian Heritage Database |publisher=Commonwealth of Australia |department=Department of Sustainability, Environment, Water, Population and Communities |df=dmy-all}}</ref>
|Named for the [[Ediacara Hills]]. Ediacara is possibly a corruption of [[Kuyani]] 'Yata Takarra' 'hard or stony ground'.<ref name="Butcher_2004">{{cite web |last=Butcher |first=Andy |date=26 May 2004 |title=Re: Ediacaran |url=http://listserv.linguistlist.org/cgi-bin/wa?A2=ind0405&L=australian-linguistics-l&D=1&P=264 |archive-url=https://web.archive.org/web/20071023012434/http://listserv.linguistlist.org/cgi-bin/wa?A2=ind0405&L=australian-linguistics-l&D=1&P=264 |archive-date=23 October 2007 |access-date=19 July 2011 |work=LISTSERV 16.0 - AUSTRALIAN-LINGUISTICS-L Archives}}</ref><ref name="AHD_Ediacara_Fossil_Site">{{cite web |title=Place Details: Ediacara Fossil Site – Nilpena, Parachilna, SA, Australia |url=http://www.environment.gov.au/cgi-bin/ahdb/search.pl?mode=place_detail;place_id=105880 |url-status=live |archive-url=https://web.archive.org/web/20110603074010/http://www.environment.gov.au/cgi-bin/ahdb/search.pl?mode=place_detail;place_id=105880 |archive-date=3 June 2011 |access-date=19 July 2011 |work=Australian Heritage Database |publisher=Commonwealth of Australia |department=Department of Sustainability, Environment, Water, Population and Communities }}</ref>
|-
|-
|[[Cryogenian]]
|[[Cryogenian]]
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=== Early history ===
=== Early history ===
The most modern geological time scale was not formulated until 1911<ref name="Holmes_19113">{{Cite journal |last1=Holmes |first1=Arthur |date=1911-06-09 |title=The association of lead with uranium in rock-minerals, and its application to the measurement of geological time |journal=Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character |volume=85 |issue=578 |pages=248–256 |bibcode=1911RSPSA..85..248H |doi=10.1098/rspa.1911.0036 |issn=0950-1207 |doi-access=free}}</ref> by [[Arthur Holmes]] (1890 – 1965), who drew inspiration from [[James Hutton]] (1726–1797), a Scottish Geologist who presented the idea of uniformitarianism or the theory that changes to the Earth's crust resulted from continuous and uniform processes.<ref>{{Cite web |title=James Hutton {{!}} Father of Modern Geology, Scottish Naturalist {{!}} Britannica |url=https://www.britannica.com/biography/James-Hutton |access-date=2024-12-03 |website=www.britannica.com |language=en}}</ref> The broader concept of the relation between rocks and time can be traced back to (at least) the [[philosopher]]s of [[Ancient Greece]] from 1200 BC to 600 AD. [[Xenophanes|Xenophanes of Colophon]] (c. 570–487&nbsp;[[Common era|BCE]]) observed rock beds with fossils of seashells located above the sea-level, viewed them as once living organisms, and used this to imply an unstable relationship in which the sea had at times [[Marine transgression|transgressed]] over the land and at other times had [[Marine regression|regressed]].<ref name="Fischer_20093">{{Cite journal |last1=Fischer |first1=Alfred G. |last2=Garrison |first2=Robert E. |date=2009 |title=The role of the Mediterranean region in the development of sedimentary geology: a historical overview |url=https://onlinelibrary.wiley.com/doi/10.1111/j.1365-3091.2008.01009.x |journal=Sedimentology |language=en |volume=56 |issue=1 |pages=3–41 |bibcode=2009Sedim..56....3F |doi=10.1111/j.1365-3091.2008.01009.x |s2cid=128604255}}</ref> This view was shared by a few of Xenophanes's scholars and those that followed, including [[Aristotle]] (384–322 BC) who (with additional observations) reasoned that the positions of land and sea had changed over long periods of time. The concept of [[deep time]] was also recognized by [[History of science and technology in China|Chinese naturalist]] [[Shen Kuo]]<ref name="Nathan 19953">{{Cite book |last=Sivin |first=Nathan |url=http://worldcat.org/oclc/956775994 |title=Science in ancient China: researches and reflections |date=1995 |publisher=Variorum |isbn=0-86078-492-4 |oclc=956775994}}</ref> (1031–1095) and [[Islam]]ic [[scientist]]-philosophers, notably the [[Brethren of Purity|Brothers of Purity]], who wrote on the processes of stratification over the passage of time in their [[Encyclopedia of the Brethren of Purity|treatises]].<ref name="Fischer_20093" /> Their work likely inspired that of the 11th-century [[Persians|Persian]] [[polymath]] [[Avicenna]] (Ibn Sînâ, 980–1037) who wrote in ''[[The Book of Healing]]'' (1027) on the concept of stratification and superposition, pre-dating [[Nicolas Steno]] by more than six centuries.<ref name="Fischer_20093" /> Avicenna also recognized fossils as "petrifications of the bodies of plants and animals",<ref name="Adams_19383">{{Cite book |last=Adams |first=Frank D. |url=http://worldcat.org/oclc/165626104 |title=The Birth and Development of the Geological Sciences |date=1938 |publisher=Williams & Wilkins |isbn=0-486-26372-X |oclc=165626104}}</ref> with the 13th-century [[Dominican Order|Dominican]] [[bishop]] [[Albertus Magnus]] (c. 1200–1280), who drew from [[Aristotle|Aristotle's]] natural philosophy, extending this into a theory of a petrifying fluid.<ref name="Johnson">{{Cite journal |last1=Johnson |first1=Chris |last2=Bentley |first2=Callan |last3=Panchuk |first3=Karla |last4=Affolter |first4=Matt |last5=Layou |first5=Karen |last6=Jaye |first6=Shelley |last7=Kohrs |first7=Russ |last8=Inkenbrandt |first8=Paul |last9=Mosher |first9=Cam |last10=Ricketts |first10=Brian |last11=Estrada |first11=Charlene |title=Geologic Time and Relative Dating |url=https://open.maricopa.edu/fallglg102/part/sedimentary-rocks-and-environments/ |journal=Maricopa Open Digital Press |language=en}}</ref> These works appeared to have little influence on [[scholar]]s in [[Middle Ages|Medieval Europe]] who looked to the [[Bible]] to explain the origins of fossils and sea-level changes, often attributing these to the '[[Genesis flood narrative|Deluge]]', including [[Restoro d'Arezzo|Ristoro d'Arezzo]] in 1282.<ref name="Fischer_20093" /> It was not until the [[Italian Renaissance]] when [[Leonardo da Vinci]] (1452–1519) would reinvigorate the relationships between stratification, relative sea-level change, and time, denouncing attribution of fossils to the 'Deluge':<ref name="McCurdy_19383">{{Cite book |last=McCurdy |first=Edward |url=https://www.worldcat.org/search?q=no:2233803&qt=advanced&dblist=638 |title=The notebooks of Leonardo da Vinci |date=1938 |publisher=Reynal & Hitchcock |location=New York |language=English |oclc=2233803}}</ref><ref name="Fischer_20093" />
The most modern geological time scale was not formulated until 1911<ref name="Holmes_19113">{{Cite journal |last1=Holmes |first1=Arthur |date=1911-06-09 |title=The association of lead with uranium in rock-minerals, and its application to the measurement of geological time |journal=Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character |volume=85 |issue=578 |pages=248–256 |bibcode=1911RSPSA..85..248H |doi=10.1098/rspa.1911.0036 |issn=0950-1207 |doi-access=free}}</ref> by [[Arthur Holmes]] (1890 – 1965), who drew inspiration from [[James Hutton]] (1726–1797), a Scottish Geologist who presented the idea of uniformitarianism or the theory that changes to the Earth's crust resulted from continuous and uniform processes.<ref>{{Cite web |title=James Hutton {{!}} Father of Modern Geology, Scottish Naturalist {{!}} Britannica |url=https://www.britannica.com/biography/James-Hutton |access-date=2024-12-03 |website=www.britannica.com |language=en}}</ref> The broader concept of the relation between rocks and time can be traced back to (at least) the [[philosopher]]s of [[Ancient Greece]] from 1200 BC to 600 AD. [[Xenophanes|Xenophanes of Colophon]] (c. 570–487&nbsp;[[Common era|BCE]]) observed rock beds with fossils of seashells located above the sea-level, viewed them as once living organisms, and used this to imply an unstable relationship in which the sea had at times [[Marine transgression|transgressed]] over the land and at other times had [[Marine regression|regressed]].<ref name="Fischer_20093">{{Cite journal |last1=Fischer |first1=Alfred G. |last2=Garrison |first2=Robert E. |date=2009 |title=The role of the Mediterranean region in the development of sedimentary geology: a historical overview |url=https://onlinelibrary.wiley.com/doi/10.1111/j.1365-3091.2008.01009.x |journal=Sedimentology |language=en |volume=56 |issue=1 |pages=3–41 |bibcode=2009Sedim..56....3F |doi=10.1111/j.1365-3091.2008.01009.x |s2cid=128604255}}</ref> This view was shared by a few of Xenophanes's scholars and those that followed, including [[Aristotle]] (384–322 BC) who (with additional observations) reasoned that the positions of land and sea had changed over long periods of time. The concept of [[deep time]] was also recognized by [[History of science and technology in China|Chinese naturalist]] [[Shen Kuo]]<ref name="Nathan 19953">{{Cite book |last=Sivin |first=Nathan |title=Science in ancient China: researches and reflections |date=1995 |publisher=Variorum |isbn=0-86078-492-4 |oclc=956775994}}</ref> (1031–1095) and [[Islam]]ic [[scientist]]-philosophers, notably the [[Brethren of Purity|Brothers of Purity]], who wrote on the processes of stratification over the passage of time in their [[Encyclopedia of the Brethren of Purity|treatises]].<ref name="Fischer_20093" /> Their work likely inspired that of the 11th-century [[Persians|Persian]] [[polymath]] [[Avicenna]] (Ibn Sînâ, 980–1037) who wrote in ''[[The Book of Healing]]'' (1027) on the concept of stratification and superposition, pre-dating [[Nicolas Steno]] by more than six centuries.<ref name="Fischer_20093" /> Avicenna also recognized fossils as "petrifications of the bodies of plants and animals",<ref name="Adams_19383">{{Cite book |last=Adams |first=Frank D. |title=The Birth and Development of the Geological Sciences |date=1938 |publisher=Williams & Wilkins |isbn=0-486-26372-X |oclc=165626104}}</ref> with the 13th-century [[Dominican Order|Dominican]] [[bishop]] [[Albertus Magnus]] (c. 1200–1280), who drew from [[Aristotle|Aristotle's]] natural philosophy, extending this into a theory of a petrifying fluid.<ref name="Johnson">{{Cite journal |last1=Johnson |first1=Chris |last2=Bentley |first2=Callan |last3=Panchuk |first3=Karla |last4=Affolter |first4=Matt |last5=Layou |first5=Karen |last6=Jaye |first6=Shelley |last7=Kohrs |first7=Russ |last8=Inkenbrandt |first8=Paul |last9=Mosher |first9=Cam |last10=Ricketts |first10=Brian |last11=Estrada |first11=Charlene |title=Geologic Time and Relative Dating |url=https://open.maricopa.edu/fallglg102/part/sedimentary-rocks-and-environments/ |journal=Maricopa Open Digital Press |language=en}}</ref> These works appeared to have little influence on [[scholar]]s in [[Middle Ages|Medieval Europe]] who looked to the [[Bible]] to explain the origins of fossils and sea-level changes, often attributing these to the '[[Genesis flood narrative|Deluge]]', including [[Restoro d'Arezzo|Ristoro d'Arezzo]] in 1282.<ref name="Fischer_20093" /> It was not until the [[Italian Renaissance]] when [[Leonardo da Vinci]] (1452–1519) would reinvigorate the relationships between stratification, relative sea-level change, and time, denouncing attribution of fossils to the 'Deluge':<ref name="McCurdy_19383">{{Cite book |last=McCurdy |first=Edward |url=https://www.worldcat.org/search?q=no:2233803&qt=advanced&dblist=638 |title=The notebooks of Leonardo da Vinci |date=1938 |publisher=Reynal & Hitchcock |location=New York |language=English |oclc=2233803}}</ref><ref name="Fischer_20093" />


{{blockquote|text=Of the stupidity and ignorance of those who imagine that these creatures were carried to such places distant from the sea by the Deluge...Why do we find so many fragments and whole shells between the different layers of stone unless they had been upon the shore and had been covered over by earth newly thrown up by the sea which then became petrified? And if the above-mentioned Deluge had carried them to these places from the sea, you would find the shells at the edge of one layer of rock only, not at the edge of many where may be counted the winters of the years during which the sea multiplied the layers of sand and mud brought down by the neighboring rivers and spread them over its shores. And if you wish to say that there must have been many deluges in order to produce these layers and the shells among them it would then become necessary for you to affirm that such a deluge took place every year.}}
{{blockquote|text=Of the stupidity and ignorance of those who imagine that these creatures were carried to such places distant from the sea by the Deluge...Why do we find so many fragments and whole shells between the different layers of stone unless they had been upon the shore and had been covered over by earth newly thrown up by the sea which then became petrified? And if the above-mentioned Deluge had carried them to these places from the sea, you would find the shells at the edge of one layer of rock only, not at the edge of many where may be counted the winters of the years during which the sea multiplied the layers of sand and mud brought down by the neighboring rivers and spread them over its shores. And if you wish to say that there must have been many deluges in order to produce these layers and the shells among them it would then become necessary for you to affirm that such a deluge took place every year.}}
[[File:Sketch of the Succession pf Strata and their relative Altitudes.jpg|thumb|Sketch of the Succession of Strata and their Relative Altitudes (William Smith)]]
[[File:Sketch of the Succession pf Strata and their relative Altitudes.jpg|thumb|Sketch of the Succession of Strata and their Relative Altitudes (William Smith)]]
These views of da Vinci remained unpublished, and thus lacked influence at the time; however, questions of fossils and their significance were pursued and, while views against [[Genesis creation narrative|Genesis]] were not readily accepted and dissent from [[Religion|religious]] doctrine was in some places unwise, scholars such as [[Girolamo Fracastoro]] shared da Vinci's views, and found the attribution of fossils to the 'Deluge' absurd.<ref name="Fischer_20093" /> Although many theories surrounding philosophy and concepts of rocks were developed in earlier years, "the first serious attempts to formulate a geological time scale that could be applied anywhere on Earth were made in the late 18th century."<ref name="Johnson" /> Later, in the 19th century, academics further developed theories on stratification. [[William Smith (geologist)|William Smith]], often referred to as the "Father of Geology"<ref name="earthobservatory.nasa.gov-2008" /> developed theories through observations rather than drawing from the scholars that came before him. Smith's work was primarily based on his detailed study of rock layers and fossils during his time and he created "the first map to depict so many rock formations over such a large area”.<ref name="earthobservatory.nasa.gov-2008">{{Cite web |date=2008-05-08 |title=William Smith (1769-1839) |url=https://earthobservatory.nasa.gov/features/WilliamSmith |access-date=2024-12-02 |website=earthobservatory.nasa.gov |language=en}}</ref> After studying rock layers and the fossils they contained, [[William Smith (geologist)|Smith]] concluded that each layer of rock contained distinct material that could be used to identify and correlate rock layers across different regions of the world.<ref name="Smith-1816">{{Cite book |last1=Smith |first1=William |url=https://www.biodiversitylibrary.org/bibliography/106808 |title=Strata identified by organized fossils : containing prints on colored paper of the most characteristic specimens in each stratum |last2=Smith |first2=William |date=1816 |publisher=Printed by W. Arding ..., and sold by the author ..., J. Sowerby ..., Sherwood, Neely, and Jones, and Longman, Hurst, Rees, Orme, and Brown ..., and by all booksellers |location=London |doi=10.5962/bhl.title.106808}}</ref> Smith developed the concept of faunal succession or the idea that fossils can serve as a marker for the age of the strata they are found in and published his ideas in his 1816 book, "Strata identified by organized fossils."<ref name="Smith-1816" />
These views of da Vinci remained unpublished, and thus lacked influence at the time; however, questions of fossils and their significance were pursued and, while views against [[Genesis creation narrative|Genesis]] were not readily accepted and dissent from [[Religion|religious]] doctrine was in some places unwise, scholars such as [[Girolamo Fracastoro]] shared da Vinci's views, and found the attribution of fossils to the 'Deluge' absurd.<ref name="Fischer_20093" /> Although many theories surrounding philosophy and concepts of rocks were developed in earlier years, "the first serious attempts to formulate a geological time scale that could be applied anywhere on Earth were made in the late 18th century."<ref name="Johnson" /> Later, in the 19th century, academics further developed theories on stratification. [[William Smith (geologist)|William Smith]], often referred to as the "Father of Geology"<ref name="earthobservatory.nasa.gov-2008" /> developed theories through observations rather than drawing from the scholars that came before him. Smith's work was primarily based on his detailed study of rock layers and fossils during his time and he created "the first map to depict so many rock formations over such a large area".<ref name="earthobservatory.nasa.gov-2008">{{Cite web |date=2008-05-08 |title=William Smith (1769-1839) |url=https://earthobservatory.nasa.gov/features/WilliamSmith |access-date=2024-12-02 |website=earthobservatory.nasa.gov |language=en}}</ref> After studying rock layers and the fossils they contained, [[William Smith (geologist)|Smith]] concluded that each layer of rock contained distinct material that could be used to identify and correlate rock layers across different regions of the world.<ref name="Smith-1816">{{Cite book |last1=Smith |first1=William |url=https://www.biodiversitylibrary.org/bibliography/106808 |title=Strata identified by organized fossils: containing prints on colored paper of the most characteristic specimens in each stratum |last2=Smith |first2=William |date=1816 |publisher=Printed by W. Arding ..., and sold by the author ..., J. Sowerby ..., Sherwood, Neely, and Jones, and Longman, Hurst, Rees, Orme, and Brown ..., and by all booksellers |location=London |doi=10.5962/bhl.title.106808}}</ref> Smith developed the concept of faunal succession or the idea that fossils can serve as a marker for the age of the strata they are found in and published his ideas in his 1816 book, "Strata identified by organized fossils."<ref name="Smith-1816" />


=== Establishment of primary principles ===
=== Establishment of primary principles ===
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=== The advent of geochronometry ===
=== The advent of geochronometry ===
[[File:Pierre Lecomte du Noüy - LES AGES DE LA VIE SUR LA TERRE - in L'Homme et sa destinée - 1947.jpg|thumb|One example of an obsolete geological time scale (France, mid-1940s).]]
During the 19th century, the debate regarding Earth's age was renewed, with geologists estimating ages based on [[denudation]] rates and sedimentary thicknesses or ocean chemistry, and physicists determining ages for the cooling of the Earth or the Sun using basic [[thermodynamics]] or orbital physics.<ref name="Dalrymple 2001 AoE" /> These estimations varied from 15,000 million years to 0.075 million years depending on method and author, but the estimations of [[William Thomson, 1st Baron Kelvin|Lord Kelvin]] and [[Clarence King]] were held in high regard at the time due to their pre-eminence in physics and geology. All of these early geochronometric determinations would later prove to be incorrect.
During the 19th century, the debate regarding Earth's age was renewed, with geologists estimating ages based on [[denudation]] rates and sedimentary thicknesses or ocean chemistry, and physicists determining ages for the cooling of the Earth or the Sun using basic [[thermodynamics]] or orbital physics.<ref name="Dalrymple 2001 AoE" /> These estimations varied from 15,000 million years to 0.075 million years depending on method and author, but the estimations of [[William Thomson, 1st Baron Kelvin|Lord Kelvin]] and [[Clarence King]] were held in high regard at the time due to their pre-eminence in physics and geology. All of these early geochronometric determinations would later prove to be incorrect.


Line 519: Line 520:


=== Modern international geological time scale ===
=== Modern international geological time scale ===
The establishment of the IUGS in 1961<ref name="Harrison_1978">{{Cite journal |last=Harrison |first=James M. |title=The Roots of IUGS |date=1978-03-01 |journal=Episodes |volume=1 |issue=1 |pages=20–23 |doi=10.18814/epiiugs/1978/v1i1/005 |issn=0705-3797|doi-access=free }}</ref> and acceptance of the Commission on Stratigraphy (applied in 1965)<ref name="ICS_statutes_1986">{{Cite book |author=International Union of Geological Sciences. Commission on Stratigraphy |url=https://www.worldcat.org/oclc/14352783 |title=Guidelines and statutes of the International Commission on Stratigraphy (ICS) |date=1986 |publisher=Herausgegeben von der Senckenbergischen Naturforschenden Gesellschaft |others=J. W. Cowie |isbn=3-924500-19-3 |location=Frankfurt a.M. |oclc=14352783}}</ref> to become a member commission of IUGS led to the founding of the ICS. One of the primary objectives of the ICS is "the establishment, publication and revision of the ICS International Chronostratigraphic Chart which is the standard, reference global Geological Time Scale to include the ratified Commission decisions".<ref name="ICS_statutes" />
The establishment of the IUGS in 1961<ref name="Harrison_1978">{{Cite journal |last=Harrison |first=James M. |title=The Roots of IUGS |date=1978-03-01 |journal=Episodes |volume=1 |issue=1 |pages=20–23 |doi=10.18814/epiiugs/1978/v1i1/005 |issn=0705-3797|doi-access=free }}</ref> and acceptance of the Commission on Stratigraphy (applied in 1965)<ref name="ICS_statutes_1986">{{Cite book |author=International Union of Geological Sciences. Commission on Stratigraphy |title=Guidelines and statutes of the International Commission on Stratigraphy (ICS) |date=1986 |publisher=Herausgegeben von der Senckenbergischen Naturforschenden Gesellschaft |others=J. W. Cowie |isbn=3-924500-19-3 |location=Frankfurt a.M. |oclc=14352783}}</ref> to become a member commission of IUGS led to the founding of the ICS. One of the primary objectives of the ICS is "the establishment, publication and revision of the ICS International Chronostratigraphic Chart which is the standard, reference global Geological Time Scale to include the ratified Commission decisions".<ref name="ICS_statutes" />


Following on from Holmes, several ''A Geological Time Scale'' books were published in 1982,<ref name="GTS82">{{Cite book |url=https://www.worldcat.org/oclc/8387993 |title=A geologic time scale |date=1982 |publisher=Cambridge University Press |author=W. B. Harland |isbn=0-521-24728-4 |location=Cambridge [England] |oclc=8387993}}</ref> 1989,<ref name="GTS1989">{{Cite book |url=https://www.worldcat.org/oclc/20930970 |title=A geologic time scale 1989 |date=1990 |publisher=Cambridge University Press |author=W. B. Harland |isbn=0-521-38361-7 |location=Cambridge |oclc=20930970}}</ref> 2004,<ref name="GTS2004">{{Cite book |url=https://www.worldcat.org/oclc/60770922 |title=A geologic time scale 2004 |date=2004 |publisher=Cambridge University Press |author1=F. M. Gradstein |author2=James G. Ogg |author3=A. Gilbert Smith |isbn=0-511-08201-0 |location=Cambridge, UK |oclc=60770922}}</ref> 2008,<ref name="GTS2008">{{Cite journal |last1=Gradstein |first1=Felix M. |last2=Ogg |first2=James G. |last3=van Kranendonk |first3=Martin |date=2008-07-23 |title=On the Geologic Time Scale 2008 |url=http://www.schweizerbart.de/papers/nos/detail/43/63825/On_the_Geologic_Time_Scale_2008?af=crossref |journal=Newsletters on Stratigraphy |language=en |volume=43 |issue=1 |pages=5–13 |doi=10.1127/0078-0421/2008/0043-0005 |issn=0078-0421}}</ref> 2012,<ref name="GTS2012">{{Cite book |url=https://www.worldcat.org/oclc/808340848 |title=The geologic time scale 2012. Volume 2 |date=2012 |publisher=Elsevier |author=F. M. Gradstein |isbn=978-0-444-59448-8 |edition=1st |location=Amsterdam |oclc=808340848}}</ref> 2016,<ref name="GTS2016">{{Cite book |last=Ogg |first=James G. |url=https://www.worldcat.org/oclc/949988705 |title=A concise geologic time scale 2016 |date=2016 |publisher=Elsevier |others=Gabi Ogg, F. M. Gradstein |isbn=978-0-444-59468-6 |location=Amsterdam, Netherlands |oclc=949988705}}</ref> and 2020.<ref name="GTS2020">{{Cite book |url=https://www.worldcat.org/oclc/1224105111 |title=Geologic time scale 2020 |date=2020 |author1=F. M. Gradstein |author2=James G. Ogg |author3=Mark D. Schmitz |author4=Gabi Ogg |isbn=978-0-12-824361-9 |location=Amsterdam, Netherlands |oclc=1224105111}}</ref> However, since 2013, the ICS has taken responsibility for producing and distributing the ICC citing the commercial nature, independent creation, and lack of oversight by the ICS on the prior published GTS versions (GTS books prior to 2013) although these versions were published in close association with the ICS.<ref name="ICC_Cohen_2013" /> Subsequent ''Geologic Time Scale'' books (2016<ref name="GTS2016" /> and 2020<ref name="GTS2020"/>) are commercial publications with no oversight from the ICS, and do not entirely conform to the chart produced by the ICS. The ICS produced GTS charts are versioned (year/month) beginning at v2013/01. At least one new version is published each year incorporating any changes ratified by the ICS since the prior version.
Following on from Holmes, several ''A Geological Time Scale'' books were published in 1982,<ref name="GTS82">{{Cite book |title=A geologic time scale |date=1982 |publisher=Cambridge University Press |author=W. B. Harland |isbn=0-521-24728-4 |location=Cambridge [England] |oclc=8387993}}</ref> 1989,<ref name="GTS1989">{{Cite book |title=A geologic time scale 1989 |date=1990 |publisher=Cambridge University Press |author=W. B. Harland |isbn=0-521-38361-7 |location=Cambridge |oclc=20930970}}</ref> 2004,<ref name="GTS2004">{{Cite book |title=A geologic time scale 2004 |date=2004 |publisher=Cambridge University Press |author1=F. M. Gradstein |author2=James G. Ogg |author3=A. Gilbert Smith |isbn=0-511-08201-0 |location=Cambridge, UK |oclc=60770922}}</ref> 2008,<ref name="GTS2008">{{Cite journal |last1=Gradstein |first1=Felix M. |last2=Ogg |first2=James G. |last3=van Kranendonk |first3=Martin |date=2008-07-23 |title=On the Geologic Time Scale 2008 |url=http://www.schweizerbart.de/papers/nos/detail/43/63825/On_the_Geologic_Time_Scale_2008?af=crossref |journal=Newsletters on Stratigraphy |language=en |volume=43 |issue=1 |pages=5–13 |doi=10.1127/0078-0421/2008/0043-0005 |bibcode=2008NewSt..43....5G |issn=0078-0421}}</ref> 2012,<ref name="GTS2012">{{Cite book |title=The geologic time scale 2012. Volume 2 |date=2012 |publisher=Elsevier |author=F. M. Gradstein |isbn=978-0-444-59448-8 |edition=1st |location=Amsterdam |oclc=808340848}}</ref> 2016,<ref name="GTS2016">{{Cite book |last=Ogg |first=James G. |title=A concise geologic time scale 2016 |date=2016 |publisher=Elsevier |others=Gabi Ogg, F. M. Gradstein |isbn=978-0-444-59468-6 |location=Amsterdam, Netherlands |oclc=949988705}}</ref> and 2020.<ref name="GTS2020">{{Cite book |title=Geologic time scale 2020 |date=2020 |author1=F. M. Gradstein |author2=James G. Ogg |author3=Mark D. Schmitz |author4=Gabi Ogg |isbn=978-0-12-824361-9 |location=Amsterdam, Netherlands |oclc=1224105111}}</ref> However, since 2013, the ICS has taken responsibility for producing and distributing the ICC citing the commercial nature, independent creation, and lack of oversight by the ICS on the prior published GTS versions (GTS books prior to 2013) although these versions were published in close association with the ICS.<ref name="ICS" /> Subsequent ''Geologic Time Scale'' books (2016<ref name="GTS2016" /> and 2020<ref name="GTS2020"/>) are commercial publications with no oversight from the ICS, and do not entirely conform to the chart produced by the ICS. The ICS produced GTS charts are versioned (year/month) beginning at v2013/01. At least one new version is published each year incorporating any changes ratified by the ICS since the prior version.


{{Timeline geological timescale}}
{{Timeline geological timescale}}
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=== Proposed Anthropocene Series/Epoch ===
=== Proposed Anthropocene Series/Epoch ===
{{Main|Anthropocene}}
{{Main|Anthropocene}}
First suggested in 2000,<ref name="Crutzen_2021">{{Citation |last1=Crutzen |first1=Paul J. |title=The 'Anthropocene' (2000) |date=2021 |url=https://link.springer.com/10.1007/978-3-030-82202-6_2 |work=Paul J. Crutzen and the Anthropocene: A New Epoch in Earth's History |volume=1 |pages=19–21 |editor-last=Benner |editor-first=Susanne |place=Cham |publisher=Springer International Publishing |language=en |doi=10.1007/978-3-030-82202-6_2 |isbn=978-3-030-82201-9 |access-date=2022-04-15 |last2=Stoermer |first2=Eugene F. |series=The Anthropocene: Politik—Economics—Society—Science |s2cid=245639062 |editor2-last=Lax |editor2-first=Gregor |editor3-last=Crutzen |editor3-first=Paul J. |editor4-last=Pöschl |editor4-first=Ulrich}}</ref> the ''Anthropocene'' is a proposed epoch/series for the most recent time in Earth's history. While still informal, it is a widely used term to denote the present geologic time interval, in which many conditions and processes on Earth are profoundly altered by human impact.<ref>{{Cite web |title=Working Group on the 'Anthropocene' {{!}} Subcommission on Quaternary Stratigraphy |url=https://quaternary.stratigraphy.org/working-groups/anthropocene/ |archive-url=https://web.archive.org/web/20220407193255/https://quaternary.stratigraphy.org/working-groups/anthropocene/ |archive-date=2022-04-07 |access-date=2022-04-17 |language=en-US}}</ref> {{As of|2022|April}} the Anthropocene has not been ratified by the ICS; however, in May 2019 the [[Anthropocene Working Group]] voted in favour of submitting a formal proposal to the ICS for the establishment of the Anthropocene Series/Epoch.<ref name="Subramanian_2019">{{Cite journal |last=Subramanian |first=Meera |date=2019-05-21 |title=Anthropocene now: influential panel votes to recognise Earth's new epoch |url=http://www.nature.com/articles/d41586-019-01641-5 |journal=Nature |language=en |pages=d41586–019–01641–5 |doi=10.1038/d41586-019-01641-5 |pmid=32433629 |s2cid=182238145 |issn=0028-0836}}</ref> Nevertheless, the definition of the Anthropocene as a geologic time period rather than a geologic event remains controversial and difficult.<ref name="Gibbard_2021">{{Cite journal |last1=Gibbard |first1=Philip L. |last2=Bauer |first2=Andrew M. |last3=Edgeworth |first3=Matthew |last4=Ruddiman |first4=William F. |last5=Gill |first5=Jacquelyn L. |last6=Merritts |first6=Dorothy J. |last7=Finney |first7=Stanley C. |last8=Edwards |first8=Lucy E. |last9=Walker |first9=Michael J. C. |last10=Maslin |first10=Mark |last11=Ellis |first11=Erle C. |date=2021-11-15 |title=A practical solution: the Anthropocene is a geological event, not a formal epoch |journal=Episodes |volume=45 |issue=4 |pages=349–357 |language=en |doi=10.18814/epiiugs/2021/021029 |s2cid=244165877 |issn=0705-3797|doi-access=free }}</ref><ref name="Head_2021">{{Cite journal |last1=Head |first1=Martin J. |last2=Steffen |first2=Will |last3=Fagerlind |first3=David |last4=Waters |first4=Colin N. |last5=Poirier |first5=Clement |last6=Syvitski |first6=Jaia |last7=Zalasiewicz |first7=Jan A. |last8=Barnosky |first8=Anthony D. |last9=Cearreta |first9=Alejandro |last10=Jeandel |first10=Catherine |last11=Leinfelder |first11=Reinhold |date=2021-11-15 |title=The Great Acceleration is real and provides a quantitative basis for the proposed Anthropocene Series/Epoch |journal=Episodes |volume=45 |issue=4 |pages=359–376 |language=en |doi=10.18814/epiiugs/2021/021031 |s2cid=244145710 |issn=0705-3797|doi-access=free }}</ref><ref name="Zalasiewicz_2021">{{Cite journal |last1=Zalasiewicz |first1=Jan |last2=Waters |first2=Colin N. |last3=Ellis |first3=Erle C. |last4=Head |first4=Martin J. |last5=Vidas |first5=Davor |last6=Steffen |first6=Will |last7=Thomas |first7=Julia Adeney |last8=Horn |first8=Eva |last9=Summerhayes |first9=Colin P. |last10=Leinfelder |first10=Reinhold |last11=McNeill |first11=J. R. |date=2021 |title=The Anthropocene: Comparing Its Meaning in Geology (Chronostratigraphy) with Conceptual Approaches Arising in Other Disciplines |journal=Earth's Future |language=en |volume=9 |issue=3 |doi=10.1029/2020EF001896 |bibcode=2021EaFut...901896Z |s2cid=233816527 |issn=2328-4277|doi-access=free }}</ref><ref name="Bauer_2021">{{Cite journal |last1=Bauer |first1=Andrew M. |last2=Edgeworth |first2=Matthew |last3=Edwards |first3=Lucy E. |last4=Ellis |first4=Erle C. |last5=Gibbard |first5=Philip |last6=Merritts |first6=Dorothy J. |date=2021-09-16 |title=Anthropocene: event or epoch? |url=https://www.nature.com/articles/d41586-021-02448-z |journal=Nature |language=en |volume=597 |issue=7876 |pages=332 |doi=10.1038/d41586-021-02448-z |pmid=34522014 |bibcode=2021Natur.597..332B |s2cid=237515330 |issn=0028-0836}}</ref>
First suggested in 2000,<ref name="Crutzen_2021">{{Citation |last1=Crutzen |first1=Paul J. |title=The 'Anthropocene' (2000) |date=2021 |url=https://link.springer.com/10.1007/978-3-030-82202-6_2 |work=Paul J. Crutzen and the Anthropocene: A New Epoch in Earth's History |volume=1 |pages=19–21 |editor-last=Benner |editor-first=Susanne |place=Cham |publisher=Springer International Publishing |language=en |doi=10.1007/978-3-030-82202-6_2 |isbn=978-3-030-82201-9 |access-date=2022-04-15 |last2=Stoermer |first2=Eugene F. |series=The Anthropocene: Politik—Economics—Society—Science |s2cid=245639062 |editor2-last=Lax |editor2-first=Gregor |editor3-last=Crutzen |editor3-first=Paul J. |editor4-last=Pöschl |editor4-first=Ulrich}}</ref> the ''Anthropocene'' is a proposed epoch/series for the most recent time in Earth's history. While still informal, it is a widely used term to denote the present geologic time interval, in which many conditions and processes on Earth are profoundly altered by human impact.<ref>{{Cite web |title=Working Group on the 'Anthropocene' {{!}} Subcommission on Quaternary Stratigraphy |url=https://quaternary.stratigraphy.org/working-groups/anthropocene/ |archive-url=https://web.archive.org/web/20220407193255/https://quaternary.stratigraphy.org/working-groups/anthropocene/ |archive-date=2022-04-07 |access-date=2022-04-17 |language=en-US}}</ref> The definition of the Anthropocene as a geologic time period rather than a geologic event remains controversial and difficult.<ref name="Gibbard_2021">{{Cite journal |last1=Gibbard |first1=Philip L. |last2=Bauer |first2=Andrew M. |last3=Edgeworth |first3=Matthew |last4=Ruddiman |first4=William F. |last5=Gill |first5=Jacquelyn L. |last6=Merritts |first6=Dorothy J. |last7=Finney |first7=Stanley C. |last8=Edwards |first8=Lucy E. |last9=Walker |first9=Michael J. C. |last10=Maslin |first10=Mark |last11=Ellis |first11=Erle C. |date=2021-11-15 |title=A practical solution: the Anthropocene is a geological event, not a formal epoch |journal=Episodes |volume=45 |issue=4 |pages=349–357 |language=en |doi=10.18814/epiiugs/2021/021029 |bibcode=2021Episo..45..349G |s2cid=244165877 |issn=0705-3797|doi-access=free }}</ref><ref name="Head_2021">{{Cite journal |last1=Head |first1=Martin J. |last2=Steffen |first2=Will |last3=Fagerlind |first3=David |last4=Waters |first4=Colin N. |last5=Poirier |first5=Clement |last6=Syvitski |first6=Jaia |last7=Zalasiewicz |first7=Jan A. |last8=Barnosky |first8=Anthony D. |last9=Cearreta |first9=Alejandro |last10=Jeandel |first10=Catherine |last11=Leinfelder |first11=Reinhold |date=2021-11-15 |title=The Great Acceleration is real and provides a quantitative basis for the proposed Anthropocene Series/Epoch |journal=Episodes |volume=45 |issue=4 |pages=359–376 |language=en |doi=10.18814/epiiugs/2021/021031 |s2cid=244145710 |issn=0705-3797|doi-access=free }}</ref><ref name="Zalasiewicz_2021">{{Cite journal |last1=Zalasiewicz |first1=Jan |last2=Waters |first2=Colin N. |last3=Ellis |first3=Erle C. |last4=Head |first4=Martin J. |last5=Vidas |first5=Davor |last6=Steffen |first6=Will |last7=Thomas |first7=Julia Adeney |last8=Horn |first8=Eva |last9=Summerhayes |first9=Colin P. |last10=Leinfelder |first10=Reinhold |last11=McNeill |first11=J. R. |date=2021 |title=The Anthropocene: Comparing Its Meaning in Geology (Chronostratigraphy) with Conceptual Approaches Arising in Other Disciplines |journal=Earth's Future |language=en |volume=9 |issue=3 |article-number=e2020EF001896 |doi=10.1029/2020EF001896 |bibcode=2021EaFut...901896Z |s2cid=233816527 |issn=2328-4277|doi-access=free }}</ref><ref name="Bauer_2021">{{Cite journal |last1=Bauer |first1=Andrew M. |last2=Edgeworth |first2=Matthew |last3=Edwards |first3=Lucy E. |last4=Ellis |first4=Erle C. |last5=Gibbard |first5=Philip |last6=Merritts |first6=Dorothy J. |date=2021-09-16 |title=Anthropocene: event or epoch? |url=https://www.nature.com/articles/d41586-021-02448-z |journal=Nature |language=en |volume=597 |issue=7876 |page=332 |doi=10.1038/d41586-021-02448-z |pmid=34522014 |bibcode=2021Natur.597..332B |s2cid=237515330 |issn=0028-0836}}</ref>
 
In May 2019 the [[Anthropocene Working Group]] voted in favour of submitting a formal proposal to the ICS for the establishment of the Anthropocene Series/Epoch.<ref name="Subramanian_2019">{{Cite journal |last=Subramanian |first=Meera |date=2019-05-21 |title=Anthropocene now: influential panel votes to recognise Earth's new epoch |url=http://www.nature.com/articles/d41586-019-01641-5 |journal=Nature |language=en |pages=d41586–019–01641–5 |doi=10.1038/d41586-019-01641-5 |pmid=32433629 |s2cid=182238145 |issn=0028-0836}}</ref> The formal proposal was completed and submitted to the Subcommission on Quaternary Stratigraphy in late 2023 for a section in [[Crawford Lake (Halton Region)|Crawford Lake]], [[Ontario]], with heightened Plutonium levels corresponding to 1952 CE.<ref>{{cite web |title=Working Group on the 'Anthropocene' |url=https://quaternary.stratigraphy.org/working-groups/anthropocene |website=Subcommission on Quaternary Stratigraphy |publisher=International Commission on Stratigraphy |access-date=23 October 2025}}</ref> This proposal was rejected as a formal geologic epoch in early 2024, to be left instead as an "invaluable descriptor of human impact on the Earth system"<ref>{{cite web |title=Joint statement by the IUGS and ICS on the vote by the ICS Subcommission on Quaternary Stratigraphy |url=https://stratigraphy.org/news/152 |website=International Commission on Stratigraphy |publisher=International Commission on Stratigraphy |access-date=23 October 2025}}</ref>


=== Proposals for revisions to pre-Cryogenian timeline ===
=== Proposals for revisions to pre-Cryogenian timeline ===
Line 680: Line 683:


==== Van Kranendonk et al. 2012 (GTS2012) ====
==== Van Kranendonk et al. 2012 (GTS2012) ====
The book, ''Geologic Time Scale 2012,'' was the last commercial publication of an international chronostratigraphic chart that was closely associated with the ICS and the Subcommission on Precambrian Stratigraphy.<ref name="ICC_Cohen_2013" /> It included a proposal to substantially revise the pre-Cryogenian time scale to reflect important events such as the [[Formation and evolution of the Solar System|formation of the Solar System]] and the [[Great Oxidation Event]], among others, while at the same time maintaining most of the previous chronostratigraphic nomenclature for the pertinent time span.<ref name="GTS2012b">{{cite book |last=Van Kranendonk |first=Martin J. |chapter=A Chronostratigraphic Division of the Precambrian |title=The geologic time scale 2012 |date=2012 |publisher=Elsevier |isbn=978-0-44-459425-9 |editor=Felix M. Gradstein |edition=1st |location=Amsterdam |pages=359–365 |doi=10.1016/B978-0-444-59425-9.00016-0 |editor2=James G. Ogg |editor3=Mark D. Schmitz |editor4=abi M. Ogg}}</ref> {{As of|2022|April}} these proposed changes have not been accepted by the ICS. The proposed changes (changes from the current scale [v2023/09]) are italicised:
The book, ''Geologic Time Scale 2012,'' was the last commercial publication of an international chronostratigraphic chart that was closely associated with the ICS and the Subcommission on Precambrian Stratigraphy.<ref name="ICS" /> It included a proposal to substantially revise the pre-Cryogenian time scale to reflect important events such as the [[Formation and evolution of the Solar System|formation of the Solar System]] and the [[Great Oxidation Event]], among others, while at the same time maintaining most of the previous chronostratigraphic nomenclature for the pertinent time span.<ref name="GTS2012b">{{cite book |last=Van Kranendonk |first=Martin J. |chapter=A Chronostratigraphic Division of the Precambrian |title=The geologic time scale 2012 |date=2012 |publisher=Elsevier |isbn=978-0-44-459425-9 |editor=Felix M. Gradstein |edition=1st |location=Amsterdam |pages=359–365 |doi=10.1016/B978-0-444-59425-9.00016-0 |editor2=James G. Ogg |editor3=Mark D. Schmitz |editor4=abi M. Ogg}}</ref> {{As of|2022|April}} these proposed changes have not been accepted by the ICS. The proposed changes (changes from the current scale [v2023/09]) are italicised:


* Hadean Eon (4567''–4030'' Ma)
* Hadean Eon (4567''–4030'' Ma)
** [[Chaotian (geology)|''Chaotian'']] Era/Erathem (''4567–4404'' Ma) – the name alluding both to the [[Chaos (cosmogony)|mythological Chaos]] and the [[Chaos theory|chaotic]] phase of [[planet formation]].<ref name="GTS2012" /><ref name="Goldblatt_2010">{{cite journal |last1=Goldblatt |first1=C. |last2=Zahnle |first2=K. J. |last3=Sleep |first3=N. H. |last4=Nisbet |first4=E. G. |date=2010 |title=The Eons of Chaos and Hades |journal=Solid Earth |volume=1 |issue=1 |pages=1–3 |bibcode=2010SolE....1....1G |doi=10.5194/se-1-1-2010 |doi-access=free}}</ref><ref>{{cite journal |last=Chambers |first=John E. |date=July 2004 |title=Planetary accretion in the inner Solar System |url=http://www.astro.washington.edu/courses/astro321/Chambers_EPSL_04.pdf |archive-url=https://web.archive.org/web/20120419024812/http://www.astro.washington.edu/courses/astro321/Chambers_EPSL_04.pdf |archive-date=2012-04-19 |url-status=live |journal=Earth and Planetary Science Letters |volume=223 |issue=3–4 |pages=241–252 |bibcode=2004E&PSL.223..241C |doi=10.1016/j.epsl.2004.04.031}}</ref>
** [[Chaotian (geology)|''Chaotian'']] Era/Erathem (''4567–4404'' Ma) – the name alluding both to the [[Chaos (cosmogony)|mythological Chaos]] and the chaotic phase of [[planet formation]].<ref name="GTS2012" /><ref name="Goldblatt_2010">{{cite journal |last1=Goldblatt |first1=C. |last2=Zahnle |first2=K. J. |last3=Sleep |first3=N. H. |last4=Nisbet |first4=E. G. |date=2010 |title=The Eons of Chaos and Hades |journal=Solid Earth |volume=1 |issue=1 |pages=1–3 |bibcode=2010SolE....1....1G |doi=10.5194/se-1-1-2010 |doi-access=free}}</ref><ref>{{cite journal |last=Chambers |first=John E. |date=July 2004 |title=Planetary accretion in the inner Solar System |url=http://www.astro.washington.edu/courses/astro321/Chambers_EPSL_04.pdf |archive-url=https://web.archive.org/web/20120419024812/http://www.astro.washington.edu/courses/astro321/Chambers_EPSL_04.pdf |archive-date=2012-04-19 |url-status=live |journal=Earth and Planetary Science Letters |volume=223 |issue=3–4 |pages=241–252 |bibcode=2004E&PSL.223..241C |doi=10.1016/j.epsl.2004.04.031}}</ref>
** ''Jack Hillsian'' or ''Zirconian'' Era/Erathem (''4404–4030'' Ma) – both names allude to the Jack Hills Greenstone Belt which provided the oldest mineral grains on Earth, [[zircon]]s.<ref name="GTS2012" /><ref name="Goldblatt_2010" />
** ''Jack Hillsian'' or ''Zirconian'' Era/Erathem (''4404–4030'' Ma) – both names allude to the Jack Hills Greenstone Belt which provided the oldest mineral grains on Earth, [[zircon]]s.<ref name="GTS2012" /><ref name="Goldblatt_2010" />
* Archean Eon/Eonothem (''4030–2420'' Ma)
* Archean Eon/Eonothem (''4030–2420'' Ma)
Line 698: Line 701:
** Paleoproterozoic Era/Erathem (''2420–1780'' Ma)
** Paleoproterozoic Era/Erathem (''2420–1780'' Ma)
*** ''Oxygenian'' Period/System (''2420–2250'' Ma) – named for displaying the first evidence for a global oxidising atmosphere.<ref name="GTS2012" />
*** ''Oxygenian'' Period/System (''2420–2250'' Ma) – named for displaying the first evidence for a global oxidising atmosphere.<ref name="GTS2012" />
*** ''Jatulian'' or ''Eukaryian'' Period/System (''2250–2060'' Ma) – names are respectively for the Lomagundi–Jatuli δ<sup>13</sup>C isotopic excursion event spanning its duration, and for the (proposed)<ref name="El_Albani_2014">{{cite journal |last1=El Albani |first1=Abderrazak |last2=Bengtson |first2=Stefan |last3=Canfield |first3=Donald E. |last4=Riboulleau |first4=Armelle |last5=Rollion Bard |first5=Claire |last6=Macchiarelli |first6=Roberto |display-authors=etal |year=2014 |title=The 2.1 Ga Old Francevillian Biota: Biogenicity, Taphonomy and Biodiversity |journal=PLOS ONE |volume=9 |issue=6 |pages=e99438 |bibcode=2014PLoSO...999438E |doi=10.1371/journal.pone.0099438 |pmc=4070892 |pmid=24963687 |doi-access=free}}</ref><ref name="El_Albani_2010">{{cite journal |last1=El Albani |first1=Abderrazak |last2=Bengtson |first2=Stefan |last3=Canfield |first3=Donald E. |last4=Bekker |first4=Andrey |last5=Macchiarelli |first5=Roberto |last6=Mazurier |first6=Arnaud |last7=Hammarlund |first7=Emma U. |display-authors=etal |year=2010 |title=Large colonial organisms with coordinated growth in oxygenated environments 2.1 Gyr ago |url=http://www.afrikibouge.com/publications/Article%20Albani.pdf |archive-url=https://web.archive.org/web/20240616162702/https://www.afrikibouge.com/publications/Article%20Albani.pdf |url-status=dead |archive-date=16 June 2024 |journal=Nature |volume=466 |issue=7302 |pages=100–104 |bibcode=2010Natur.466..100A |doi=10.1038/nature09166 |pmid=20596019 |s2cid=4331375}}</ref> first fossil appearance of [[eukaryote]]s.<ref name="GTS2012" />
*** ''Jatulian'' or ''Eukaryian'' Period/System (''2250–2060'' Ma) – names are respectively for the Lomagundi–Jatuli δ<sup>13</sup>C isotopic excursion event spanning its duration, and for the (proposed)<ref name="El_Albani_2014">{{cite journal |last1=El Albani |first1=Abderrazak |last2=Bengtson |first2=Stefan |last3=Canfield |first3=Donald E. |last4=Riboulleau |first4=Armelle |last5=Rollion Bard |first5=Claire |last6=Macchiarelli |first6=Roberto |display-authors=etal |year=2014 |title=The 2.1 Ga Old Francevillian Biota: Biogenicity, Taphonomy and Biodiversity |journal=PLOS ONE |volume=9 |issue=6 |article-number=e99438 |bibcode=2014PLoSO...999438E |doi=10.1371/journal.pone.0099438 |pmc=4070892 |pmid=24963687 |doi-access=free}}</ref><ref name="El_Albani_2010">{{cite journal |last1=El Albani |first1=Abderrazak |last2=Bengtson |first2=Stefan |last3=Canfield |first3=Donald E. |last4=Bekker |first4=Andrey |last5=Macchiarelli |first5=Roberto |last6=Mazurier |first6=Arnaud |last7=Hammarlund |first7=Emma U. |display-authors=etal |year=2010 |title=Large colonial organisms with coordinated growth in oxygenated environments 2.1 Gyr ago |url=http://www.afrikibouge.com/publications/Article%20Albani.pdf |archive-url=https://web.archive.org/web/20240616162702/https://www.afrikibouge.com/publications/Article%20Albani.pdf |archive-date=16 June 2024 |journal=Nature |volume=466 |issue=7302 |pages=100–104 |bibcode=2010Natur.466..100A |doi=10.1038/nature09166 |pmid=20596019 |s2cid=4331375}}</ref> first fossil appearance of [[eukaryote]]s.<ref name="GTS2012" />
*** ''Columbian Period/System'' (''2060–1780'' Ma) – named after the [[supercontinent]] [[Columbia (supercontinent)|Columbia]].<ref name="GTS2012" />
*** ''Columbian Period/System'' (''2060–1780'' Ma) – named after the [[supercontinent]] [[Columbia (supercontinent)|Columbia]].<ref name="GTS2012" />
** Mesoproterozoic Era/Erathem (''1780–850'' Ma)
** Mesoproterozoic Era/Erathem (''1780–850'' Ma)
Line 832: Line 835:
     from: start till: -2500 color:white
     from: start till: -2500 color:white
</timeline>
</timeline>


==Table of geologic time==
==Table of geologic time==
{{More citations needed section|date=November 2023}}
{{More citations needed section|date=November 2023}}
The following table summarises the major events and characteristics of the divisions making up the geologic time scale of Earth. This table is arranged with the most recent geologic periods at the top, and the oldest at the bottom. The height of each table entry does not correspond to the duration of each subdivision of time. As such, this table is not to scale and does not accurately represent the relative time-spans of each geochronologic unit. While the [[Phanerozoic]] Eon looks longer than the rest, it merely spans ~539 million years (~12% of Earth's history), whilst the previous three eons{{Efn|name=Precam|group=note}} collectively span ~3,461 million years (~76% of Earth's history). This bias toward the most recent eon is in part due to the relative lack of information about events that occurred during the first three eons compared to the current eon (the Phanerozoic).<ref name="Shields_2022_pre-Cryogenian" /><ref>{{cite web |title=Geological time scale |url=https://www.digitalatlasofancientlife.org/learn/geological-time/geological-time-scale/ |access-date=January 17, 2022 |work=Digital Atlas of Ancient Life |publisher=Paleontological Research Institution}}</ref> The use of subseries/subepochs has been ratified by the ICS.<ref name ="Aubry_2022_subseries"/>
The following table summarises the major events and characteristics of the divisions making up the geologic time scale of Earth. This table is arranged with the most recent geologic periods at the top, and the oldest at the bottom. The height of each table entry does not correspond to the duration of each subdivision of time. As such, this table is not to scale and does not accurately represent the relative time-spans of each geochronologic unit. While the [[Phanerozoic]] Eon looks longer than the rest, it merely spans ~538.8 Ma (~11.8% of Earth's history), whilst the previous three eons{{Efn|name=Precam|group=note}} collectively span ~4,028.2 Ma (~88.2% of Earth's history). This bias toward the most recent eon is in part due to the relative lack of information about events that occurred during the first three eons compared to the current eon (the Phanerozoic).<ref name="Shields_2022_pre-Cryogenian" /><ref>{{cite web |title=Geological time scale |url=https://www.digitalatlasofancientlife.org/learn/geological-time/geological-time-scale/ |access-date=January 17, 2022 |work=Digital Atlas of Ancient Life |publisher=Paleontological Research Institution}}</ref> The use of subseries/subepochs has been ratified by the ICS.<ref name ="Aubry_2022_subseries"/>


While some regional terms are still in use,<ref name="GTS2012_Precambrian" /> the table of geologic time conforms to the [[nomenclature]], ages, and colour codes set forth by the International Commission on Stratigraphy in the official International Chronostratigraphic Chart.<ref name="ICS_statutes" /><ref name="ICS_IGTS">{{cite web |title=International Commission on Stratigraphy |url=https://stratigraphy.org/ |accessdate=5 June 2022 |work=International Geological Time Scale}}</ref> The International Commission on Stratigraphy also provide an online interactive version of this chart. The interactive version is based on a service delivering a machine-readable [[Resource Description Framework]]/[[Web Ontology Language]] representation of the time scale, which is available through the [[Commission for the Management and Application of Geoscience Information]] [[GeoSciML]] project as a service<ref name="web_GTSelements">{{cite web |title=Geologic Timescale Elements in the International Chronostratigraphic Chart |url=http://resource.geosciml.org/classifier/ics/ischart/ |access-date=2014-08-03}}</ref> and at a [[SPARQL]] end-point.<ref name="web_Cox_SPARQL_GTS">{{cite web |last=Cox |first=Simon J. D. |title=SPARQL endpoint for CGI timescale service |url=http://resource.geosciml.org/sparql/isc2014 |url-status=dead |archive-url=https://archive.today/20140806164132/http://resource.geosciml.org/sparql/isc2014 |archive-date=2014-08-06 |access-date=2014-08-03}}</ref><ref name="Cox_2014">{{cite journal |last1=Cox |first1=Simon J. D. |last2=Richard |first2=Stephen M. |year=2014 |title=A geologic timescale ontology and service |journal=Earth Science Informatics |volume=8 |pages=5–19 |doi=10.1007/s12145-014-0170-6 |s2cid=42345393}}</ref>
While some regional terms are still in use,<ref name="GTS2012_Precambrian" /> the table of geologic time conforms to the [[nomenclature]], ages, and colour codes set forth by the International Commission on Stratigraphy in the official International Chronostratigraphic Chart.<ref name="ICS_statutes" /><ref name="ICS_IGTS">{{cite web |title=International Commission on Stratigraphy |url=https://stratigraphy.org/ |access-date=5 June 2022 |work=International Geological Time Scale}}</ref> The International Commission on Stratigraphy also provide an online interactive version of this chart. The interactive version is based on a service delivering a machine-readable [[Resource Description Framework]]/[[Web Ontology Language]] representation of the time scale, which is available through the [[Commission for the Management and Application of Geoscience Information]] [[GeoSciML]] project as a service<ref name="web_GTSelements">{{cite web |title=Geologic Timescale Elements in the International Chronostratigraphic Chart |url=http://resource.geosciml.org/classifier/ics/ischart/ |access-date=2014-08-03}}</ref> and at a [[SPARQL]] end-point.<ref name="web_Cox_SPARQL_GTS">{{cite web |last=Cox |first=Simon J. D. |title=SPARQL endpoint for CGI timescale service |url=http://resource.geosciml.org/sparql/isc2014 |archive-url=https://archive.today/20140806164132/http://resource.geosciml.org/sparql/isc2014 |archive-date=2014-08-06 |access-date=2014-08-03}}</ref><ref name="Cox_2014">{{cite journal |last1=Cox |first1=Simon J. D. |last2=Richard |first2=Stephen M. |year=2014 |title=A geologic timescale ontology and service |journal=Earth Science Informatics |volume=8 |pages=5–19 |doi=10.1007/s12145-014-0170-6 |s2cid=42345393}}</ref>


{{sticky header}}
{{sticky header}}
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|-
|-
| style="background:{{period color|Gelasian}}" |[[Gelasian]]
| style="background:{{period color|Gelasian}}" |[[Gelasian]]
|Start of [[Quaternary glaciation]]s and unstable climate.<ref name="Hoag_2017">{{Cite journal |last1=Hoag |first1=Colin |last2=Svenning |first2=Jens-Christian |date=2017-10-17 |title=African Environmental Change from the Pleistocene to the Anthropocene |url=https://www.annualreviews.org/doi/10.1146/annurev-environ-102016-060653 |journal=Annual Review of Environment and Resources |language=en |volume=42 |issue=1 |pages=27–54 |doi=10.1146/annurev-environ-102016-060653 |issn=1543-5938 |access-date=5 June 2022 |archive-date=1 May 2022 |archive-url=https://web.archive.org/web/20220501144059/https://www.annualreviews.org/doi/10.1146/annurev-environ-102016-060653 |url-status=dead }}</ref> Rise of the [[Pleistocene megafauna]] and [[Homo habilis]].
|Start of [[Quaternary glaciation]]s and unstable climate.<ref name="Hoag_2017">{{Cite journal |last1=Hoag |first1=Colin |last2=Svenning |first2=Jens-Christian |date=2017-10-17 |title=African Environmental Change from the Pleistocene to the Anthropocene |url=https://www.annualreviews.org/doi/10.1146/annurev-environ-102016-060653 |journal=Annual Review of Environment and Resources |language=en |volume=42 |issue=1 |pages=27–54 |doi=10.1146/annurev-environ-102016-060653 |issn=1543-5938 |access-date=5 June 2022 |archive-date=1 May 2022 |archive-url=https://web.archive.org/web/20220501144059/https://www.annualreviews.org/doi/10.1146/annurev-environ-102016-060653 }}</ref> Rise of the [[Pleistocene megafauna]] and [[Homo habilis]].
| style="background:{{period color|Gelasian}}" |{{Period start|gelasian}} {{Period start error|geliasian}}<sup>*</sup>
| style="background:{{period color|Gelasian}}" |{{Period start|gelasian}} {{Period start error|geliasian}}<sup>*</sup>
|-
|-
Line 909: Line 911:
|-
|-
| style="background:{{period color|Burdigalian}}" |[[Burdigalian]]
| style="background:{{period color|Burdigalian}}" |[[Burdigalian]]
| rowspan="2" |[[Orogeny]] in [[Northern Hemisphere]]. Start of [[Kaikoura Orogeny]] forming [[Southern Alps in New Zealand]]. Widespread forests slowly [[Photosynthesis|draw in]] massive amounts of {{CO2}}, gradually lowering the level of atmospheric {{CO2}} from 650 [[ppmv]] down to around 100 ppmv during the Miocene.<ref name="Royer_2006">{{cite journal |last1=Royer |first1=Dana L. |year=2006 |title=CO<sub>2</sub>-forced climate thresholds during the Phanerozoic |url=http://droyer.web.wesleyan.edu/PhanCO2%28GCA%29.pdf |url-status=dead |journal=Geochimica et Cosmochimica Acta |volume=70 |issue=23 |pages=5665–75 |bibcode=2006GeCoA..70.5665R |doi=10.1016/j.gca.2005.11.031 |archive-url=https://web.archive.org/web/20190927033455/http://droyer.web.wesleyan.edu/PhanCO2%28GCA%29.pdf |archive-date=27 September 2019 |access-date=6 August 2015}}</ref>{{efn|For more information on this, see [[Atmosphere of Earth#Evolution of Earth's atmosphere]], [[Carbon dioxide in the Earth's atmosphere]], and [[Climate variability and change|climate change]]. Specific graphs of reconstructed {{CO2}} levels over the past ~550, 65, and 5 million years can be seen at [[:File:Phanerozoic Carbon Dioxide.png]], [[:File:65 Myr Climate Change.png]], [[:File:Five Myr Climate Change.png]], respectively.|name="atmospheric-carbon-dioxide"|group=note}} Modern [[bird]] and mammal families become recognizable. The last of the primitive whales go extinct. [[Poaceae|Grasses]] become ubiquitous. Ancestor of [[ape]]s, including humans.<ref name="web_LS_2017">{{cite web |date=10 August 2017 |title=Here's What the Last Common Ancestor of Apes and Humans Looked Like |url=https://www.livescience.com/60093-last-common-ancestor-of-apes-humans-revealed.html |website=[[Live Science]]}}</ref><ref name="Nengo_2017">{{Cite journal |last1=Nengo |first1=Isaiah |last2=Tafforeau |first2=Paul |last3=Gilbert |first3=Christopher C. |last4=Fleagle |first4=John G. |last5=Miller |first5=Ellen R. |last6=Feibel |first6=Craig |last7=Fox |first7=David L. |last8=Feinberg |first8=Josh |last9=Pugh |first9=Kelsey D. |last10=Berruyer |first10=Camille |last11=Mana |first11=Sara |date=2017 |title=New infant cranium from the African Miocene sheds light on ape evolution |url=http://www.nature.com/articles/nature23456 |journal=Nature |language=en |volume=548 |issue=7666 |pages=169–174 |doi=10.1038/nature23456 |pmid=28796200 |bibcode=2017Natur.548..169N |s2cid=4397839 |issn=0028-0836}}</ref> Afro-Arabia collides with Eurasia, fully forming the [[Alpide Belt]] and closing the Tethys Ocean, while allowing a faunal interchange. At the same time, Afro-Arabia splits into [[Africa]] and [[Arabian Plate|West Asia]].
| rowspan="2" |[[Orogeny]] in [[Northern Hemisphere]]. Start of [[Kaikoura Orogeny]] forming [[Southern Alps in New Zealand]]. Widespread forests slowly [[Photosynthesis|draw in]] massive amounts of {{CO2}}, gradually lowering the level of atmospheric {{CO2}} from 650 [[ppmv]] down to around 100 ppmv during the Miocene.<ref name="Royer_2006">{{cite journal |last1=Royer |first1=Dana L. |year=2006 |title=CO<sub>2</sub>-forced climate thresholds during the Phanerozoic |url=http://droyer.web.wesleyan.edu/PhanCO2%28GCA%29.pdf |journal=Geochimica et Cosmochimica Acta |volume=70 |issue=23 |pages=5665–75 |bibcode=2006GeCoA..70.5665R |doi=10.1016/j.gca.2005.11.031 |archive-url=https://web.archive.org/web/20190927033455/http://droyer.web.wesleyan.edu/PhanCO2%28GCA%29.pdf |archive-date=27 September 2019 |access-date=6 August 2015}}</ref>{{efn|For more information on this, see [[Atmosphere of Earth#Evolution of Earth's atmosphere]], [[Carbon dioxide in the Earth's atmosphere]], and [[Climate variability and change|climate change]]. Specific graphs of reconstructed {{CO2}} levels over the past ~550, 65, and 5 million years can be seen at [[:File:Phanerozoic Carbon Dioxide.png]], [[:File:65 Myr Climate Change.png]], [[:File:Five Myr Climate Change.png]], respectively.|name="atmospheric-carbon-dioxide"|group=note}} Modern [[bird]] and mammal families become recognizable. The last of the primitive whales go extinct. [[Poaceae|Grasses]] become ubiquitous. Ancestor of [[ape]]s, including humans.<ref name="web_LS_2017">{{cite web |date=10 August 2017 |title=Here's What the Last Common Ancestor of Apes and Humans Looked Like |url=https://www.livescience.com/60093-last-common-ancestor-of-apes-humans-revealed.html |website=[[Live Science]]}}</ref><ref name="Nengo_2017">{{Cite journal |last1=Nengo |first1=Isaiah |last2=Tafforeau |first2=Paul |last3=Gilbert |first3=Christopher C. |last4=Fleagle |first4=John G. |last5=Miller |first5=Ellen R. |last6=Feibel |first6=Craig |last7=Fox |first7=David L. |last8=Feinberg |first8=Josh |last9=Pugh |first9=Kelsey D. |last10=Berruyer |first10=Camille |last11=Mana |first11=Sara |date=2017 |title=New infant cranium from the African Miocene sheds light on ape evolution |url=http://www.nature.com/articles/nature23456 |journal=Nature |language=en |volume=548 |issue=7666 |pages=169–174 |doi=10.1038/nature23456 |pmid=28796200 |bibcode=2017Natur.548..169N |s2cid=4397839 |issn=0028-0836}}</ref> Afro-Arabia collides with Eurasia, fully forming the [[Alpide Belt]] and closing the Tethys Ocean, while allowing a faunal interchange. At the same time, Afro-Arabia splits into [[Africa]] and [[Arabian Plate|West Asia]].
| style="background:{{period color|Burdigalian}}" |{{Period start|burdigalian}} {{Period start error|burdigalian}}
| style="background:{{period color|Burdigalian}}" |{{Period start|burdigalian}} {{Period start error|burdigalian}}
|-
|-
Line 1,032: Line 1,034:
| rowspan="3" style="background:{{period color|Late Triassic}}" |[[Late Triassic|Upper/Late]]
| rowspan="3" style="background:{{period color|Late Triassic}}" |[[Late Triassic|Upper/Late]]
| style="background:{{period color|Rhaetian}}" |[[Rhaetian]]
| style="background:{{period color|Rhaetian}}" |[[Rhaetian]]
| rowspan="7" |[[Archosaur]]s dominant on land as [[pseudosuchia]]ns and in the air as [[pterosaur]]s. [[Dinosaur]]s also arise from bipedal archosaurs. [[Ichthyosaur]]s and [[nothosaur]]s (a group of sauropterygians) dominate large marine fauna. [[Cynodont]]s become smaller and nocturnal, eventually becoming the first true [[mammals]], while other remaining synapsids die out. [[Rhynchosaur]]s (archosaur relatives) also common. [[Seed ferns]] called ''[[Dicroidium]]'' remained common in Gondwana, before being replaced by advanced gymnosperms. Many large aquatic [[Temnospondyli|temnospondyl]] amphibians. [[Ceratitida]]n [[ammonoids]] extremely common. [[Scleractinia|Modern corals]] and [[teleost]] fish appear, as do many modern [[insect]] orders and suborders. First [[starfish]]. [[Andes Mountains|Andean Orogeny]] in South America. [[Cimmerian Orogeny]] in Asia. [[Rangitata Orogeny]] begins in New Zealand. [[Hunter-Bowen Orogeny]] in [[Northern Australia]], Queensland and [[New South Wales]] ends, (c. 260–225&nbsp;Ma). [[Carnian pluvial event]] occurs around 234–232 Ma, allowing the first dinosaurs and [[lepidosaurs]] (including [[rhynchocephalia]]ns) to radiate. [[Triassic–Jurassic extinction event]] occurs 201&nbsp;Ma, wiping out all [[conodonts]] and the [[Procolophonidae|last parareptiles]], many marine reptiles (e.g. all sauropterygians except [[plesiosaurs]] and all ichthyosaurs except [[parvipelvia]]ns), all [[crocopoda]]ns except crocodylomorphs, pterosaurs, and dinosaurs, and many ammonoids (including the whole [[Ceratitida]]), bivalves, brachiopods, corals and sponges. First [[diatoms]].<ref name="Medlin_1997">{{cite journal |last1=Medlin |first1=L. K. |last2=Kooistra |first2=W. H. C. F. |last3=Gersonde |first3=R. |last4=Sims |first4=P. A. |last5=Wellbrock |first5=U. |year=1997 |title=Is the origin of the diatoms related to the end-Permian mass extinction? |journal=Nova Hedwigia |volume=65 |issue=1–4 |pages=1–11 |doi=10.1127/nova.hedwigia/65/1997/1 |hdl=10013/epic.12689}}</ref>
| rowspan="7" |[[Archosaur]]s dominant on land as [[pseudosuchia]]ns and in the air as [[pterosaur]]s. [[Dinosaur]]s also arise from bipedal archosaurs. [[Ichthyosauria|Ichthyosaur]]s and [[nothosaur]]s (a group of sauropterygians) dominate large marine fauna. [[Cynodont]]s become smaller and nocturnal, eventually becoming the first true [[mammals]], while other remaining synapsids die out. [[Rhynchosaur]]s (archosaur relatives) also common. [[Seed ferns]] called ''[[Dicroidium]]'' remained common in Gondwana, before being replaced by advanced gymnosperms. Many large aquatic [[Temnospondyli|temnospondyl]] amphibians. [[Ceratitida]]n [[ammonoids]] extremely common. [[Scleractinia|Modern corals]] and [[teleost]] fish appear, as do many modern [[insect]] orders and suborders. First [[starfish]]. [[Andes Mountains|Andean Orogeny]] in South America. [[Cimmerian Orogeny]] in Asia. [[Rangitata Orogeny]] begins in New Zealand. [[Hunter-Bowen Orogeny]] in [[Northern Australia]], Queensland and [[New South Wales]] ends, (c. 260–225&nbsp;Ma). [[Carnian pluvial event]] occurs around 234–232 Ma, allowing the first dinosaurs and [[lepidosaurs]] (including [[rhynchocephalia]]ns) to radiate. [[Triassic–Jurassic extinction event]] occurs 201&nbsp;Ma, wiping out all [[conodonts]] and the [[Procolophonidae|last parareptiles]], many marine reptiles (e.g. all sauropterygians except [[plesiosaurs]] and all ichthyosaurs except [[parvipelvia]]ns), all [[crocopoda]]ns except crocodylomorphs, pterosaurs, and dinosaurs, and many ammonoids (including the whole [[Ceratitida]]), bivalves, brachiopods, corals and sponges. First [[diatoms]].<ref name="Medlin_1997">{{cite journal |last1=Medlin |first1=L. K. |last2=Kooistra |first2=W. H. C. F. |last3=Gersonde |first3=R. |last4=Sims |first4=P. A. |last5=Wellbrock |first5=U. |year=1997 |title=Is the origin of the diatoms related to the end-Permian mass extinction? |journal=Nova Hedwigia |volume=65 |issue=1–4 |pages=1–11 |doi=10.1127/nova.hedwigia/65/1997/1 |bibcode=1997NovaH..65....1M |hdl=10013/epic.12689}}</ref>
| style="background:{{period color|Rhaetian}}" |~{{Period start|rhaetian}} {{Period start error|rhaetian}}
| style="background:{{period color|Rhaetian}}" |~{{Period start|rhaetian}} {{Period start error|rhaetian}}
|-
|-
Line 1,091: Line 1,093:
| rowspan="4" style="background:{{period color|Pennsylvanian}}" |[[Pennsylvanian (geology)|Pennsylvanian]]<br/>{{efn|group=note|name=MissiPenns|This is divided into Lower/Early, Middle, and Upper/Late series/epochs}}
| rowspan="4" style="background:{{period color|Pennsylvanian}}" |[[Pennsylvanian (geology)|Pennsylvanian]]<br/>{{efn|group=note|name=MissiPenns|This is divided into Lower/Early, Middle, and Upper/Late series/epochs}}
| style="background:{{period color|Gzhelian}}" |[[Gzhelian]]
| style="background:{{period color|Gzhelian}}" |[[Gzhelian]]
| rowspan="4" |[[Pterygota|Winged insects]] radiate suddenly; some (esp. [[Protodonata]] and [[Palaeodictyoptera]]) of them as well as some [[millipede]]s and [[scorpion]]s become very large. First [[coal]] forests ([[Lepidodendron|scale trees]], ferns, [[Sigillaria|club trees]], [[Calamites|giant horsetails]], ''[[Cordaites]]'', etc.). Higher [[atmosphere of Earth|atmospheric]] [[oxygen]] levels. [[Permo-Carboniferous|Ice Age]] continues to the Early Permian. [[Goniatite]]s, brachiopods, bryozoa, bivalves, and corals plentiful in the seas and oceans. First [[woodlice]]. Testate [[foram]]s proliferate. [[Euramerica]] collides with [[Gondwana]] and Siberia-Kazakhstania, the latter of which forms [[Laurasia]] and the [[Uralian orogeny]]. Variscan orogeny continues (these collisions created orogenies, and ultimately [[Pangaea]]). [[Amphibian]]s (e.g. temnospondyls) spread in Euramerica, with some becoming the first [[amniote]]s. [[Carboniferous Rainforest Collapse]] occurs, initiating a dry climate which favors amniotes over amphibians. Amniotes diversify rapidly into [[synapsids]], [[parareptiles]], [[Captorhinidae|cotylosaurs]], [[protorothyridids]] and [[diapsids]]. [[Rhizodont]]s remained common before they died out by the end of the period. First [[sharks]].
| rowspan="4" |Continuation of the [[Variscan orogeny]] ([[Ouachita orogeny|Ouachita]] and [[Alleghanian orogeny|Alleghanian]] orogenies) with growth of the [[Central Pangean Mountains]].<ref name=":2" /> [[Uralian orogeny|Ural orogeny]] continues with continental collision between [[Kazakhstania]] and [[Laurasia|Laurussia]].<ref>{{Cite journal |last=Puchkov |first=Victor N. |date=2009 |title=The evolution of the Uralian orogen |url=https://www.lyellcollection.org/doi/abs/10.1144/SP327.9 |journal=Geological Society, London, Special Publications |volume=327 |issue=1 |pages=161–195 |doi=10.1144/SP327.9}}</ref> Humid, [[Coal forest|coal swamps]] form in [[Foreland basin|foreland basins]] of the Central Pangean Mountains and around [[North China Craton|North]] and [[South China Craton|South China]] cratons.<ref>{{Cite journal |last=Nelsen |first=Matthew P. |last2=DiMichele |first2=William A. |last3=Peters |first3=Shanan E. |last4=Boyce |first4=C. Kevin |date=2016-03-01 |title=Delayed fungal evolution did not cause the Paleozoic peak in coal production |url=https://pmc.ncbi.nlm.nih.gov/articles/PMC4780611/ |journal=Proceedings of the National Academy of Sciences of the United States of America |volume=113 |issue=9 |pages=2442–2447 |doi=10.1073/pnas.1517943113 |issn=1091-6490 |pmc=4780611 |pmid=26787881}}</ref> As the [[Late Paleozoic icehouse|Late Paleozoic Ice Age]] (LPIA) continues, waxing and waning of ice sheets causes rapid changes in global sea level, flooding these regions and depositing [[Cyclothems|cyclothem]] sequences.<ref>{{Cite journal |last=Fielding |first=Christopher R. |date=2021-06-01 |title=Late Palaeozoic cyclothems – A review of their stratigraphy and sedimentology |url=https://www.sciencedirect.com/science/article/pii/S0012825221001124 |journal=Earth-Science Reviews |volume=217 |pages=103612 |doi=10.1016/j.earscirev.2021.103612 |issn=0012-8252}}</ref> Atmospheric oxygen levels rise to over 25% before decreasing again.<ref name=":7">{{Cite journal |last=Cannell |first=Alan |last2=Blamey |first2=Nigel |last3=Brand |first3=Uwe |last4=Escapa |first4=Ignacio |last5=Large |first5=Ross |date=2022 |title=A revised sedimentary pyrite proxy for atmospheric oxygen in the Paleozoic: Evaluation for the Silurian-Devonian-Carboniferous period and the relationship of the results to the observed biosphere record |url=https://www.sciencedirect.com/science/article/pii/S0012825222001465 |journal=Earth-Science Reviews |volume=231 |pages= |doi=10.1016/j.earscirev.2022.104062 |issn=0012-8252}}</ref> Appearance of [[aragonite]] reef builders, including [[algae]] and [[Sponge|sponges]].<ref name=":1" /> Freshwater [[Eurypterid|Eurypterid]]s (sea scorpions). On land, [[Neoptera]] appear, and [[Miomoptera]] show earliest evidence for complete [[metamorphosis]]. First true terrestrial [[Amphibian|amphibians]]. [[Amniote|Amniotes]] appear and split into two groups: [[Sauropsida|sauropsids]] (reptiles) and [[Synapsida|synapsids]] (mammals).<ref name=":8">{{Cite book |last=Parker |first=Steve |title=Evolution: the Whole Story |date=2015 |publisher=Thames & Hudson Ltd |isbn=978-0-500-29173-3 |location=London}}</ref> ''[[Lepidodendron]]'' and ''[[Sigillaria]]'' [[Lycopodiopsida|lycopod]] trees dominate coal swamps, with smaller [[Equisetidae|sphenopsids]] (horsetails) and [[Pteridospermatophyta|seed fern]]s between. [[Gymnosperm|Gymnosperms]], including [[Conifer|conifer]]s and [[Cycad|cycad]]s grow on drier ground.<ref name=":1" /> LPIA peaks at Carboniferous-Permian boundary. A drop in CO<sub>2</sub> levels and increase in arid conditions<ref name=":9">{{Cite journal |last=Montañez |first=Isabel Patricia |date=2022 |title=Current synthesis of the penultimate icehouse and its imprint on the Upper Devonian through Permian stratigraphic record |url=https://www.lyellcollection.org/doi/10.1144/SP512-2021-124 |journal=Geological Society, London, Special Publications |language=en |volume=512 |issue=1 |pages=213–245 |doi=10.1144/SP512-2021-124 |issn=0305-8719}}</ref> leads to change in woodland vegetation ([[Carboniferous rainforest collapse]]).<ref>{{Cite journal |last=Lucas |first=Spencer G. |last2=DiMichele |first2=William A. |last3=Opluštil |first3=Stanislav |last4=Wang |first4=Xiangdong |date=2023-06-14 |title=An introduction to ice ages, climate dynamics and biotic events: the Late Pennsylvanian world |url=https://www.lyellcollection.org/doi/full/10.1144/SP535-2022-334 |journal=Geological Society, London, Special Publications |volume=535 |issue=1 |pages=1–15 |doi=10.1144/SP535-2022-334}}</ref>
| style="background:{{period color|Gzhelian}}" |{{Period start|gzhelian}} {{Period start error|gzhelain}}
| style="background:{{period color|Gzhelian}}" |{{Period start|gzhelian}} {{Period start error|gzhelain}}
|-
|-
Line 1,105: Line 1,107:
| rowspan="3" style="background:{{period color|Mississippian}}" |[[Mississippian (geology)|Mississippian]]<br/>{{efn|group=note|name=MissiPenns}}
| rowspan="3" style="background:{{period color|Mississippian}}" |[[Mississippian (geology)|Mississippian]]<br/>{{efn|group=note|name=MissiPenns}}
| style="background:{{period color|Serpukhovian}}" |[[Serpukhovian]]
| style="background:{{period color|Serpukhovian}}" |[[Serpukhovian]]
| rowspan="3" |Large [[Lycopodiophyta|lycopodian primitive trees]] flourish and amphibious [[eurypterid]]s live amid [[coal]]-forming coastal [[Brackish water|swamps]], radiating significantly one last time. First [[gymnosperms]]. First [[Holometabola|holometabolous]], [[paraneoptera]]n, [[polyneoptera]]n, [[odonatoptera]]n and [[ephemeroptera]]n insects and first [[barnacles]]. First five-digited [[tetrapods]] (amphibians) and [[land snails]]. In the oceans, [[Bony fish|bony]] and [[Chondrichthyes|cartilaginous fishes]] are dominant and diverse; [[echinoderm]]s (especially [[crinoid]]s and [[blastoid]]s) abundant. [[Coral]]s, [[bryozoa]]ns, [[orthocerida]]ns, [[goniatite]]s and brachiopods ([[Productida]], [[Spiriferida]], etc.) recover and become very common again, but [[Trilobita|trilobites]] and [[nautiloid]]s decline. [[Karoo Ice Age|Glaciation]] in East [[Gondwana]] continues from Late Devonian. [[Mayor Island/Tuhua|Tuhua Orogeny]] in New Zealand tapers off. Some lobe finned fish called rhizodonts become abundant and dominant in freshwaters. [[Siberia (continent)|Siberia]] collides with a different small continent, [[Kazakhstania]].
| rowspan="3" |Continents form a near circle around the opening [[Paleo-Tethys Ocean]]. Gondwana forms the southern to southwestern margin; Laurussia the west; Siberia, Amuria and Kazakhstania the north; North and South China the northeast; and, Annamia the eastern margin.<ref name=":2" /> The [[Armorican terrane|Armorican terrane]]s collide with southeastern Laurussia during the Variscan orogeny. [[Antler orogeny]] continues, and opening of the [[Slide Mountain Ocean]] along western margin of Laurussia.<ref>{{Cite journal |last=Domeier |first=Mathew |last2=Torsvik |first2=Trond H. |date=2014-05-01 |title=Plate tectonics in the late Paleozoic |url=https://www.sciencedirect.com/science/article/pii/S1674987114000061 |journal=Geoscience Frontiers |volume=5 |issue=3 |pages=303–350 |doi=10.1016/j.gsf.2014.01.002 |issn=1674-9871}}</ref> Closure of [[Ural Ocean]] between Kazakhstania and Laurussia during the Ural orogeny. Development of [[Altai Mountains|Altai]] accretionary complexes along north and eastern margin of the Paleo-Tethys.<ref>{{Cite journal |last=Xu |first=Yan |last2=Han |first2=Bao-Fu |last3=Liao |first3=Wen |last4=Li |first4=Ang |date=2022 |title=The Serpukhovian–Bashkirian Amalgamation of Laurussia and the Siberian Continent and Implications for Assembly of Pangea |url=https://onlinelibrary.wiley.com/doi/abs/10.1029/2022TC007218 |journal=Tectonics |language=en |volume=41 |issue=3 |pages=e2022TC007218 |doi=10.1029/2022TC007218 |issn=1944-9194}}</ref> Main phase of LPIA begins. Drop in global sea levels, extensive glaciation across Gondwana.<ref name=":9" /> Increasing atmospheric oxygen levels.<ref name=":7" /> Change from [[Calcite sea|calcite]] to [[Aragonite sea|aragonite seas]].<ref name=":1" /> [[Evolutionary radiation|Evolutionary radiations]] after the Late Devonian extinctions include brachiopods, bivalves, echinoderms, ammonoids, gastropods, sharks and ray-finned bony fish. [[Placoderm|Placoderm]]s and [[Graptolite|graptolite]]s die out. Proetida only group of trilobites.<ref name=":1" /><ref name=":8" /> First freshwater mollusks and sharks.<ref name=":1" /> ''[[Arthropleura]]'' (millipede) largest ever terrestrial arthropod. First flying insects ''[[Palaeodictyoptera|Paleodictyopora]].'' Fish-like (''[[Pederpes]]'') and semi-aquatic tetrapods (''[[Eucritta]]'') appear on land.<ref name=":8" /> Seedless vascular plants and seed ferns diversify.<ref name=":1" />
| style="background:{{period color|Serpukhovian}}" |{{Period start|serpukhovian}} {{Period start error|serpukhovian}}
| style="background:{{period color|Serpukhovian}}" |{{Period start|serpukhovian}} {{Period start error|serpukhovian}}
|-
|-
Line 1,117: Line 1,119:
| rowspan="2" style="background:{{period color|Late Devonian}}" |[[Late Devonian|Upper/Late]]
| rowspan="2" style="background:{{period color|Late Devonian}}" |[[Late Devonian|Upper/Late]]
| style="background:{{period color|Famennian}}" |[[Famennian]]
| style="background:{{period color|Famennian}}" |[[Famennian]]
| rowspan="7" |First [[Lycopodiopsida|lycopods]], [[ferns]], [[seed plants]] ([[seed ferns]], from earlier [[progymnosperm]]s), first trees (the progymnosperm ''[[Archaeopteris]]''), and first [[Pterygota|winged insects]] (palaeoptera and neoptera). [[Strophomenida|Strophomenid]] and [[Atrypa|atrypid]] [[brachiopod]]s, [[Rugosa|rugose]] and [[Tabulata|tabulate]] corals, and [[crinoid]]s are all abundant in the oceans. First fully coiled cephalopods ([[Ammonoidea]] and [[Nautilida]], independently) with the former group very abundant (especially [[goniatite]]s). Trilobites and ostracoderms decline, while jawed fishes ([[Placodermi|placoderms]], [[Sarcopterygii|lobe-finned]] and [[Actinopterygii|ray-finned]] [[Osteichthyes|bony fish]], and [[acanthodians]] and early [[Chondrichthyes|cartilaginous fish]]) proliferate. Some [[Tetrapodomorpha|lobe finned fish]] transform into digited [[Stegocephalia|fishapods]], slowly becoming amphibious. The last non-trilobite artiopods die off. First [[decapods]] (like [[prawns]]) and [[isopods]]. Pressure from jawed fishes cause eurypterids to decline and [[Coleoidea|some cephalopods]] to lose their shells while anomalocarids vanish. "Old Red Continent" of [[Euramerica]] persists after forming in the Caledonian orogeny. Beginning of [[Acadian Orogeny]] for [[Atlas Mountains|Anti-Atlas Mountains]] of North Africa, and [[Appalachian Mountains]] of North America, also the [[Antler Orogeny|Antler]], [[Variscan Orogeny|Variscan]], and [[Mayor Island/Tuhua|Tuhua orogenies]] in New Zealand. A series of extinction events, including the massive [[Kellwasser event|Kellwasser]] and [[Hangenberg event|Hangenberg]] ones, wipe out many acritarchs, corals, sponges, molluscs, trilobites, eurypterids, graptolites, brachiopods, crinozoans (e.g. all [[cystoids]]), and fish, including all placoderms and ostracoderms.
| rowspan="7" |Paleo-Tethys continues to open as the Armorican Terrane Assemblage (ATA) drifts north and Annamia-South China moves away from Gondwana.<ref name=":2" /><ref>{{Cite journal |last=Golonka |first=Jan |date=2020 |title=Late Devonian paleogeography in the framework of global plate tectonics |url=https://www.sciencedirect.com/science/article/pii/S0921818120300187 |journal=Global and Planetary Change |volume=186 |article-number=103129 |doi=10.1016/j.gloplacha.2020.103129 |bibcode=2020GPC...18603129G |issn=0921-8181}}</ref> [[Rheic Ocean]] closes as ATA collides with Laurussia beginning the Variscan orogeny. Other orogenies: Antler, [[Innuitian orogeny|Ellesmerian]], and [[Acadian orogeny|Acadian]] (Laurussia); Achalian (Argentina); [[Lachlan Fold Belt|Tabberabberan/Lachlan]] (Australia); [[Ross orogeny|Ross]] (Antarctica); Kazakh ([[Kazakhstania]]).<ref name=":2" /> Period of high sea-levels, greenhouse conditions but decreasing atmospheric CO<sub>2</sub> levels and slowly cooling climate with glaciations towards end.<ref name=":6">{{Cite journal |last1=Qie |first1=Wenkun |last2=Algeo |first2=Thomas J. |last3=Luo |first3=Genming |last4=Herrmann |first4=Achim |date=2019 |title=Global events of the Late Paleozoic (Early Devonian to Middle Permian): A review |url=https://www.sciencedirect.com/science/article/pii/S003101821930625X |journal=Palaeogeography, Palaeoclimatology, Palaeoecology |series=Global events of the Late Devonian to Early Permian |volume=531 |article-number=109259 |doi=10.1016/j.palaeo.2019.109259 |bibcode=2019PPP...53109259Q |issn=0031-0182}}</ref> [[Vascular plant]]s increase in size, develop large root systems and spread to upland areas. First forests, seed plants, and modern soil orders appear ([[alfisol]]s and [[ultisol]]s).<ref name=":6" /> Growth of massive reef systems. Major radiation of [[Gnathostomata|jawed fish]] with appearance of [[Actinopterygii|ray-finned]], [[Sarcopterygii|lobe-finned]], and [[Chondrichthyes|cartilaginous]] fish. Appearance of [[tetrapod]]s (evolved from lobe-finned fish). Early amphibians move on to land. First ammonoids.<ref name=":1" /> Emplacement of the Viley and Pripyat–Dniepr–Donets [[Large igneous province|large igneous provinces]] coincide with global marine [[anoxic event]]s and the [[Late Devonian mass extinction|Kellwasser]] (c. 372 Ma) and [[Hangenberg event|Hangenberg]] (c. 359 Ma) mass extinctions.<ref name=":6" /> Kellwasser extinction: c. 20% of families and c. 50% of genera of marine invertebrates lost. [[Tabulata|Tabulate coral]] and [[Stromatoporoidea|stromatoporoid]] reef ecosystems wiped out. Loss of placoderms and many groups of [[Agnatha|jawless fish]]. Hangenberg extinction: loss of c. 16% of marine families and c. 21% of marine genera, including ammonoids, [[ostracod]]s and sharks.<ref name=":6" /><ref>{{Cite journal |last1=Ernst |first1=Richard E. |last2=Rodygin |first2=Sergei A. |last3=Grinev |first3=Oleg M. |date=2020 |title=Age correlation of Large Igneous Provinces with Devonian biotic crises |url=https://www.sciencedirect.com/science/article/pii/S092181811930582X |journal=Global and Planetary Change |volume=185 |article-number=103097 |doi=10.1016/j.gloplacha.2019.103097 |bibcode=2020GPC...18503097E |issn=0921-8181}}</ref>
 
| style="background:{{period color|Famennian}}" |{{Period start|famennian}} {{Period start error|famennian}}<sup>*</sup>
| style="background:{{period color|Famennian}}" |{{Period start|famennian}} {{Period start error|famennian}}<sup>*</sup>
|-
|-
Line 1,142: Line 1,145:
| rowspan="8" style="background:{{period color|Silurian}}" |[[Silurian]]
| rowspan="8" style="background:{{period color|Silurian}}" |[[Silurian]]
| colspan="2" style="background:{{period color|Pridoli}}" |[[Pridoli epoch|Pridoli]]
| colspan="2" style="background:{{period color|Pridoli}}" |[[Pridoli epoch|Pridoli]]
| rowspan="8" |[[Ozone layer]] thickens. First [[vascular plant]]s and fully terrestrialised arthropods: [[myriapods]], [[Hexapoda|hexapods]] (including [[insects]]), and [[arachnids]]. [[Eurypterid]]s diversify rapidly, becoming widespread and dominant. Cephalopods continue to flourish. True [[jawed fish]]es, along with [[ostracoderm]]s, also roam the seas. [[Tabulate coral|Tabulate]] and [[Rugosa|rugose]] corals, [[brachiopod]]s (''Pentamerida'', [[Rhynchonellida]], etc.), [[cystoids]] and [[crinoid]]s all abundant. [[Trilobite]]s and [[mollusc]]s diverse; [[graptolite]]s not as varied. Three minor extinction events. Some echinoderms go extinct. Beginning of [[Caledonian Orogeny]] (collision between Laurentia, Baltica and one of the formerly small Gondwanan terranes) for hills in England, Ireland, Wales, Scotland, and the [[Scandinavian Mountains]]. Also continued into Devonian period as the [[Acadian Orogeny]], above (thus Euramerica forms). [[Taconic Orogeny]] tapers off. [[Andean-Saharan glaciation|Icehouse period]] ends late in this period after starting in Late Ordovician. [[Lachlan Orogeny]] on [[Australia (continent)|Australian continent]] tapers off.
| rowspan="8" |Laurentia and Avalonia-Baltica collide as Iapetus Ocean closes, [[Caledonian orogeny|Caledonian]]-[[Scandian orogeny|Scandian]] orogeny, and formation of [[Laurasia|Laurussia]]. Other orogenies: Salinic (Appalachians); Famatinian (South America) tapers off; [[Lachlan Fold Belt|Lachlan]] (Australia).<ref name=":2" /><ref name=":5">{{Cite journal |last1=Golonka |first1=Jan |last2=Porębski |first2=Szczepan J. |last3=Waśkowska |first3=Anna |date=2023-07-15 |title=Silurian paleogeography in the framework of global plate tectonics |url=https://www.sciencedirect.com/science/article/pii/S0031018223002158 |journal=Palaeogeography, Palaeoclimatology, Palaeoecology |volume=622 |article-number=111597 |doi=10.1016/j.palaeo.2023.111597 |bibcode=2023PPP...62211597G |issn=0031-0182}}</ref> Series of microcontinents and North China separate opening Paleo-Tethys and closing Paleoasian Ocean.<ref name=":5" /> Rheic Ocean widens between Gondwana and Laurussia. Siberia drifts north of equator.<ref name=":2" /> Temperatures increase as Hirnantian glaciation ends. Sea levels rise. Deposition of black shales, North Africa and Arabia, major [[hydrocarbon]] [[source rock]]s.<ref name=":2" /> Fluctuating climate with glacial advances results in changing ocean conditions causes extinction events, followed by ecological recoveries.<ref>{{Cite journal |last1=Cooper |first1=Roger A. |last2=Sadler |first2=Peter M. |last3=Munnecke |first3=Axel |last4=Crampton |first4=James S. |date=2014 |title=Graptoloid evolutionary rates track Ordovician–Silurian global climate change |url=https://www.cambridge.org/core/journals/geological-magazine/article/abs/graptoloid-evolutionary-rates-track-ordoviciansilurian-global-climate-change/6E1711BC6768CE8FFE72BD02E19FD72B |journal=Geological Magazine |language=en |volume=151 |issue=2 |pages=349–364 |doi=10.1017/S0016756813000198 |bibcode=2014GeoM..151..349C |issn=0016-7568}}</ref> Widespread evaporite deposition and hothouse climate by late Silurian.<ref name=":1" /><ref>{{Cite journal |last1=Scotese |first1=Christopher R. |last2=Song |first2=Haijun |last3=Mills |first3=Benjamin J. W. |last4=van der Meer |first4=Douwe G. |date=2021-04-01 |title=Phanerozoic paleotemperatures: The earth's changing climate during the last 540 million years |url=https://www.sciencedirect.com/science/article/pii/S0012825221000027 |journal=Earth-Science Reviews |volume=215 |article-number=103503 |doi=10.1016/j.earscirev.2021.103503 |bibcode=2021ESRv..21503503S |issn=0012-8252}}</ref> After end-Ordovician mass extinction, major radiation of graptolites, bivalves, gastropods, nautiloids, brachiopods, and crinoids. Increase in trilobites, but never fully recover. Corals and stromatoporiods diversify to produce large reefs. Proliferation of eurypterid arthropods. Earliest jawed fish ([[Acanthodii|acanthodians]]). Appearance of [[ostracoderm]]s. Appearance of [[vascular plant]]s. First land animals including [[Myriapoda|myriapods]]. First freshwater fish.<ref name=":1" />
| style="background:{{period color|Pridoli}}" |{{Period start|pridoli}} {{Period start error|pridoli}}<sup>*</sup>
| style="background:{{period color|Pridoli}}" |{{Period start|pridoli}} {{Period start error|pridoli}}<sup>*</sup>
|-
|-
Line 1,172: Line 1,175:
| rowspan="3" style="background:{{period color|Late Ordovician}}" |[[Late Ordovician|Upper/Late]]
| rowspan="3" style="background:{{period color|Late Ordovician}}" |[[Late Ordovician|Upper/Late]]
| style="background:{{period color|Hirnantian}}" |[[Hirnantian]]
| style="background:{{period color|Hirnantian}}" |[[Hirnantian]]
| rowspan="7" |The [[Great Ordovician Biodiversification Event]] occurs as plankton increase in number: [[invertebrate]]s diversify into many new types (especially brachiopods and molluscs; e.g. long [[Orthoconic|straight-shelled]] cephalopods like the long lasting and diverse [[Orthocerida]]). Early [[coral]]s, articulate [[brachiopod]]s (''Orthida'', ''Strophomenida'', etc.), [[bivalves]], [[cephalopod]]s (nautiloids), [[trilobite]]s, [[ostracod]]s, [[bryozoa]]ns, many types of [[echinoderms]] ([[blastoids]], [[cystoids]], [[crinoids]], [[sea urchins]], [[sea cucumbers]], and [[Asterozoa|star-like forms]], etc.), branched [[graptolite]]s, and other taxa all common. [[Acritarch]]s still persist and common. Cephalopods become dominant and common, with some trending toward a coiled shell. Anomalocarids decline. Mysterious [[tentaculita]]ns appear. First [[eurypterids]] and [[ostracoderm]] fish appear, the latter probably giving rise to the [[jawed fish]] at the end of the period. First uncontroversial terrestrial [[fungi]] and fully terrestrialised [[Embryophyte|plants]]. [[Late Ordovician glaciation|Ice age]] at the end of this period, as well as a series of mass [[Late Ordovician mass extinction|extinction events]], killing off some cephalopods and many brachiopods, bryozoans, echinoderms, graptolites, trilobites, bivalves, corals and [[conodonts]].
| rowspan="7" |Most continents lay in equatorial regions. Gondwana stretched to south pole. Panthalassic Ocean covered northern hemisphere. Avalonia rifted from Gondwana closing Iapetus Ocean in front, opening Rheic Ocean behind. South China close to Gondwana; North China between Siberia and Gondwana. Orogenies: [[Famatinian orogeny|Famatinian]] (South America); Benambran (Australia); [[Taconic orogeny|Taconic]] (Laurentia). Baltica and Siberia drift north.<ref name=":2" /> Early greenhouse climate, cooling to icehouse conditions during [[Hirnantian glaciation|Hirnantian Ice Age]]. Increase in atmospheric O<sub>2</sub>.<ref name=":3">{{Cite journal |last1=Liu |first1=Mu |last2=Bao |first2=Xiujuan |last3=Harper |first3=David A. T. |last4=Algeo |first4=Thomas |last5=Zhao |first5=Mingyu |last6=Saltzman |first6=Matthew |last7=Zhang |first7=Wang |last8=Chen |first8=Daizhao |last9=Yuan |first9=Shuai |last10=Chen |first10=Yihui |last11=Wei |first11=Mengyu |last12=Zhang |first12=Junpeng |last13=Luan |first13=Xiaocong |last14=Zhang |first14=Yuandong |last15=Yang |first15=Xiangrong |date=2025-10-01 |title=Diversification to extinction: oceanic and climatic context of the Ordovician |url=https://www.sciencedirect.com/science/article/pii/S0012825225001552 |journal=Earth-Science Reviews |volume=269 |article-number=105194 |doi=10.1016/j.earscirev.2025.105194 |bibcode=2025ESRv..26905194L |issn=0012-8252}}</ref> [[Great Ordovician Biodiversification Event]], major increase in new genera e.g. brachiopods, trilobites, corals, echinoderms, bryozoans, gastropods, bivalves, nautiloids, graptolites, and conodonts. Very high sea levels expand shallow continental seas, increase range of ecological niches.<ref name=":4">{{Citation |last1=Cooper |first1=R. A. |title=Chapter 20 - The Ordovician Period |date=2012-01-01 |work=The Geologic Time Scale |pages=489–523 |editor-last=Gradstein |editor-first=Felix M. |url=https://www.sciencedirect.com/science/article/pii/B9780444594259000202 |access-date=2025-07-30 |place=Boston |publisher=Elsevier |isbn=978-0-444-59425-9 |last2=Sadler |first2=P. M. |last3=Hammer |first3=O. |last4=Gradstein |first4=F. M. |editor2-last=Ogg |editor2-first=James G. |editor3-last=Schmitz |editor3-first=Mark D. |editor4-last=Ogg |editor4-first=Gabi M.}}</ref> Modern marine ecosystems established.<ref name=":3" /> Earliest jawless fish. Tabulate corals and stromatoporoids dominant reef builders. Nautiloids main predators.<ref name=":1" /> Appearance of eurypterids and asteroids. Spread of early land plants.<ref name=":3" /> [[Late Ordovician mass extinction|Late Ordovician Mass Extinction]], loss of ~85 % of marine invertebrate species. Two pulses: first with onset of glaciation affects tropical fauna; second at end of ice age, warming climate impacts cool water species.<ref name=":1" /> Drastic reduction in trilobite, brachiopod, graptolite, echinoderm, conodont, coral, and chitinozoan genera.<ref name=":4" />
| style="background:{{period color|Hirnantian}}" |{{Period start|hirnantian}} {{Period start error|hirnantian}}<sup>*</sup>
| style="background:{{period color|Hirnantian}}" |{{Period start|hirnantian}} {{Period start error|hirnantian}}<sup>*</sup>
|-
|-
Line 1,198: Line 1,201:
| rowspan="3" style="background:{{period color|Furongian}}" |[[Furongian]]
| rowspan="3" style="background:{{period color|Furongian}}" |[[Furongian]]
| style="background:{{period color|Stage 10}}" |[[Cambrian Stage 10|Stage 10]]
| style="background:{{period color|Stage 10}}" |[[Cambrian Stage 10|Stage 10]]
| rowspan="10" |Major diversification of (fossils mainly show bilaterian) life in the [[Cambrian Explosion]] as oxygen levels increase. Numerous fossils; most modern [[animal]] [[phylum|phyla]] (including [[arthropods]], [[Mollusca|molluscs]], [[annelid]]s, [[echinoderm]]s, [[hemichordate]]s and [[chordate]]s) appear. Reef-building [[archaeocyatha]]n sponges initially abundant, then vanish. Stromatolites replace them, but quickly fall prey to the [[Agronomic revolution]], when some animals started burrowing through the microbial mats (affecting some other animals as well). First [[artiopods]] (including [[trilobite]]s), [[priapulid]] worms, inarticulate [[brachiopod]]s (unhinged lampshells), [[hyoliths]], [[bryozoa]]ns, [[graptolite]]s, pentaradial echinoderms (e.g. [[blastozoa]]ns, [[crinozoa]]ns and [[eleutherozoa]]ns), and numerous other animals. [[Anomalocarid]]s are dominant and giant predators, while [[End-Ediacaran extinction|many Ediacaran fauna die out]]. [[Crustacea]]ns and molluscs diversify rapidly. [[Prokaryote]]s, [[protist]]s (e.g., [[foram]]s), [[algae]] and [[fungi]] continue to present day. First [[vertebrate]]s from earlier chordates. [[Petermann Orogeny]] on the [[Australia (continent)|Australian continent]] tapers off (550–535&nbsp;Ma). Ross Orogeny in Antarctica. [[Delamerian Orogeny]] (c. 514–490&nbsp;Ma) on [[Australia (continent)|Australian continent]]. Some small terranes split off from Gondwana. [[Atmosphere of Earth|Atmospheric]] {{CO2}} content roughly 15 times present-day ([[Holocene]]) levels (6000&nbsp;ppm compared to today's 400&nbsp;ppm)<ref name="Royer_2006" />{{efn|name="atmospheric-carbon-dioxide"|group=note}} [[Arthropod]]s and [[Embryophyte|streptophyta]] start colonising land. 3 extinction events occur 517, 502 and 488&nbsp;Ma, the [[End-Botomian mass extinction|first]] and [[Cambrian–Ordovician extinction event|last]] of which wipe out many of the anomalocarids, artiopods, hyoliths, brachiopods, molluscs, and conodonts (early jawless vertebrates).
| rowspan="10" |Gondwana stretched from the south pole to equator, separated from Laurentia and Baltica by the Iapetus Ocean. Siberia lay close to the equator, north of Baltica; North and South China close to equatorial Gondwana. Orogenies: [[Cadomian Orogeny|Cadomian]] (N.Africa/southern Europe); [[Kuunga orogeny|Kuunga]] (central Gondwana); [[Famatinian orogeny|Famatinian]] orogeny (South America); [[Adelaide Superbasin|Delamerian]] (Australia).<ref>{{Cite book |last1=Torsvik |first1=Trond H. |title=Earth history and palaeogeography |last2=Cocks |first2=Leonard Robert Morrison |date=2017 |publisher=Cambridge university press |isbn=978-1-107-10532-4 |location=Cambridge}}</ref> Greenhouse climate. High atmospheric CO<sub>2</sub> levels. Atmospheric oxygen levels rose with increase in photosynthesising organisms.<ref name=":0">{{Cite journal |last1=Pruss |first1=Sara B. |last2=Gill |first2=Benjamin C. |date=2024-07-23 |title=Life on the Edge: The Cambrian Marine Realm and Oxygenation |url=https://www.annualreviews.org/content/journals/10.1146/annurev-earth-031621-070316 |journal=Annual Review of Earth and Planetary Sciences |language=en |volume=52 |issue=52 |pages=109–132 |doi=10.1146/annurev-earth-031621-070316 |bibcode=2024AREPS..52..109P |issn=0084-6597}}</ref> Early aragonite seas replaced by mixed aragonite-calcite seas with many animals developing CaCO<sub>3</sub> skeletons.<ref>{{Cite journal |last1=Xiong |first1=Yi |last2=Wood |first2=Rachel |last3=Pichevin |first3=Laetitia |date=2023 |title=The record of sea water chemistry evolution during the Ediacaran–Cambrian from early marine cements |url=https://onlinelibrary.wiley.com/doi/abs/10.1002/dep2.211 |journal=The Depositional Record |language=en |volume=9 |issue=3 |pages=508–525 |doi=10.1002/dep2.211 |bibcode=2023DepRe...9..508X |issn=2055-4877}}</ref> Rapid diversification of animals ([[Cambrian explosion|Cambrian Explosion]]), most modern animal phyla appear, e.g. arthropods; molluscs; annelids; echinoderms; bryozoa; priapulids; brachiopods; hemichordates; and, chordates. Radiations of [[Small shelly fauna|small shelly fossils]].<ref>{{Citation |last1=Peng |first1=S. |title=Chapter 19 - The Cambrian Period |date=2012-01-01 |work=The Geologic Time Scale |pages=437–488 |editor-last=Gradstein |editor-first=Felix M. |url=https://www.sciencedirect.com/science/article/pii/B9780444594259000196 |access-date=2025-07-30 |place=Boston |publisher=Elsevier |isbn=978-0-444-59425-9 |last2=Babcock |first2=L. E. |last3=Cooper |first3=R. A. |editor2-last=Ogg |editor2-first=James G. |editor3-last=Schmitz |editor3-first=Mark D. |editor4-last=Ogg |editor4-first=Gabi M.}}</ref> Giant [[Anomalocarididae|anomalocarids]] (arthropods) dominant predators. Increase in bioturbation and grazing led to decline in [[stromatolite]]s.<ref name=":1">{{Cite book |last1=Stanley |first1=Steven |title=Earth System Science |last2=Luczaj |first2=John |publisher=W.H.Freeman and Company |year=2015 |isbn=978-1-319-15402-8 |edition=4th |location=New York}}</ref> Varying oxygen levels in oceans led to series of extinction events followed by radiations, including: earliest Cambrian loss of the Ediacaran [[acritarch]]s; [[End-Botomian mass extinction|end-Botomian extinction]], linked to the Kalkarindji [[Large igneous province|Large Igneous Province]] eruptions (c. 514 Ma) with loss of [[Archaeocyatha|archaeocyathids]] (early Cambrian reef builders) and hyoliths; and, end-Cambrian reduction in trilobite diversity.<ref name=":0" /><ref>{{Cite journal |last1=Myrow |first1=Paul M. |last2=Goodge |first2=John W. |last3=Brock |first3=Glenn A. |last4=Betts |first4=Marissa J. |last5=Park |first5=Tae-Yoon S. |last6=Hughes |first6=Nigel C. |last7=Gaines |first7=Robert R. |date=2024-03-29 |title=Tectonic trigger to the first major extinction of the Phanerozoic: The early Cambrian Sinsk event |journal=Science Advances |volume=10 |issue=13 |article-number=eadl3452 |doi=10.1126/sciadv.adl3452 |issn=2375-2548 |pmc=10980278 |pmid=38552008 |bibcode=2024SciA...10L3452M }}</ref><ref name=":1" /> Many fossil [[lagerstätte]]n, including [[Burgess Shale]] and [[Maotianshan Shales|Chengjiang Formation]], formed by rapid burial in anoxic conditions.<ref name=":0" />
| style="background:{{period color|Stage 10}}" |~{{Period start|cambrian stage 10}}
| style="background:{{period color|Stage 10}}" |~{{Period start|cambrian stage 10}}
|-
|-
Line 1,234: Line 1,237:
| rowspan="3" style="background:{{period color|Neoproterozoic}}" |[[Neoproterozoic]]
| rowspan="3" style="background:{{period color|Neoproterozoic}}" |[[Neoproterozoic]]
| style="background:{{period color|Ediacaran}}" |[[Ediacaran]]
| style="background:{{period color|Ediacaran}}" |[[Ediacaran]]
| colspan="3" |Good [[fossil]]s of primitive [[animal]]s. [[Ediacaran biota]] flourish worldwide in seas, possibly appearing after an [[Avalon explosion|explosion]], possibly caused by a large-scale oxidation event.<ref name="Williams_2019">{{Cite journal |last1=Williams |first1=Joshua J. |last2=Mills |first2=Benjamin J. W. |last3=Lenton |first3=Timothy M. |date=2019 |title=A tectonically driven Ediacaran oxygenation event |journal=Nature Communications |language=en |volume=10 |issue=1 |pages=2690 |doi=10.1038/s41467-019-10286-x |issn=2041-1723 |pmc=6584537 |pmid=31217418|bibcode=2019NatCo..10.2690W }}</ref> First [[vendozoa]]ns (unknown affinity among animals), [[cnidaria]]ns and [[bilateria]]ns. Enigmatic vendozoans include many soft-jellied creatures shaped like bags, disks, or quilts (like ''[[Dickinsonia]]''). Simple [[trace fossil]]s of possible worm-like ''[[Trichophycus pedum|Trichophycus]]'', etc. [[Taconic Orogeny]] in North America. [[Aravalli Range]] [[orogeny]] in [[Indian subcontinent]]. Beginning of [[Pan-African Orogeny]], leading to the formation of the short-lived Ediacaran supercontinent [[Pannotia]], which by the end of the period breaks up into [[Laurentia]], [[Baltica]], [[Siberia (continent)|Siberia]] and [[Gondwana]]. [[Petermann Orogeny]] forms on [[Australia (continent)|Australian continent]]. Beardmore Orogeny in Antarctica, 633–620&nbsp;Ma. [[Ozone layer]] forms. An increase in oceanic [[mineral]] levels.
| colspan="3" |Good [[fossil]]s of primitive [[animal]]s. [[Ediacaran biota]] flourish worldwide in seas, possibly appearing after an [[Avalon explosion|explosion]], possibly caused by a large-scale oxidation event.<ref name="Williams_2019">{{Cite journal |last1=Williams |first1=Joshua J. |last2=Mills |first2=Benjamin J. W. |last3=Lenton |first3=Timothy M. |date=2019 |title=A tectonically driven Ediacaran oxygenation event |journal=Nature Communications |language=en |volume=10 |issue=1 |page=2690 |doi=10.1038/s41467-019-10286-x |issn=2041-1723 |pmc=6584537 |pmid=31217418|bibcode=2019NatCo..10.2690W }}</ref> First [[vendozoa]]ns (unknown affinity among animals), [[cnidaria]]ns and [[bilateria]]ns. Enigmatic vendozoans include many soft-jellied creatures shaped like bags, disks, or quilts (like ''[[Dickinsonia]]''). Simple [[trace fossil]]s of possible worm-like ''[[Trichophycus pedum|Trichophycus]]'', etc. [[Taconic Orogeny]] in North America. [[Aravalli Range]] [[orogeny]] in [[Indian subcontinent]]. Beginning of [[Pan-African Orogeny]], leading to the formation of the short-lived Ediacaran supercontinent [[Pannotia]], which by the end of the period breaks up into [[Laurentia]], [[Baltica]], [[Siberia (continent)|Siberia]] and [[Gondwana]]. [[Petermann Orogeny]] forms on [[Australia (continent)|Australian continent]]. Beardmore Orogeny in Antarctica, 633–620&nbsp;Ma. [[Ozone layer]] forms. An increase in oceanic [[mineral]] levels.
| style="background:{{period color|Ediacaran}}" |~{{Period start|ediacaran}} {{Period start error|ediacaran}}<sup>*</sup>
| style="background:{{period color|Ediacaran}}" |~{{Period start|ediacaran}} {{Period start error|ediacaran}}<sup>*</sup>
|-
|-
| style="background:{{period color|Cryogenian}}" |[[Cryogenian]]
| style="background:{{period color|Cryogenian}}" |[[Cryogenian]]
| colspan="3" |Possible "[[Snowball Earth]]" period. [[Fossil]]s still rare. Late Ruker / Nimrod Orogeny in Antarctica tapers off. First uncontroversial [[Sponge|animal]] fossils. First hypothetical [[Amastigomycota|terrestrial fungi]]<ref name="NaranjoOrtiz_2019">{{cite journal |last1=Naranjo-Ortiz |first1=Miguel A. |last2=Gabaldón |first2=Toni |date=2019-04-25 |title=Fungal evolution: major ecological adaptations and evolutionary transitions |journal=[[Biological Reviews of the Cambridge Philosophical Society]] |publisher=[[Cambridge Philosophical Society]] ([[Wiley Publishing|Wiley]]) |volume=94 |issue=4 |pages=1443–1476 |doi=10.1111/brv.12510 |pmid=31021528 |pmc=6850671 |s2cid=131775942 |issn=1464-7931}}</ref> and [[streptophyta]].<ref name="Zarsky_2022">{{Cite journal |last1=Žárský |first1=Jakub |last2=Žárský |first2=Vojtěch |last3=Hanáček |first3=Martin |last4=Žárský |first4=Viktor |date=2022-01-27 |title=Cryogenian Glacial Habitats as a Plant Terrestrialisation Cradle – The Origin of the Anydrophytes and Zygnematophyceae Split |journal=Frontiers in Plant Science |volume=12 |pages=735020 |doi=10.3389/fpls.2021.735020 |issn=1664-462X |pmc=8829067 |pmid=35154170|doi-access=free }}</ref>
| colspan="3" |Possible "[[Snowball Earth]]" period. [[Fossil]]s still rare. Late Ruker / Nimrod Orogeny in Antarctica tapers off. First uncontroversial [[Sponge|animal]] fossils. First hypothetical [[Amastigomycota|terrestrial fungi]]<ref name="NaranjoOrtiz_2019">{{cite journal |last1=Naranjo-Ortiz |first1=Miguel A. |last2=Gabaldón |first2=Toni |date=2019-04-25 |title=Fungal evolution: major ecological adaptations and evolutionary transitions |journal=[[Biological Reviews of the Cambridge Philosophical Society]] |publisher=[[Cambridge Philosophical Society]] ([[Wiley Publishing|Wiley]]) |volume=94 |issue=4 |pages=1443–1476 |doi=10.1111/brv.12510 |pmid=31021528 |pmc=6850671 |s2cid=131775942 |issn=1464-7931}}</ref> and [[streptophyta]].<ref name="Zarsky_2022">{{Cite journal |last1=Žárský |first1=Jakub |last2=Žárský |first2=Vojtěch |last3=Hanáček |first3=Martin |last4=Žárský |first4=Viktor |date=2022-01-27 |title=Cryogenian Glacial Habitats as a Plant Terrestrialisation Cradle – The Origin of the Anydrophytes and Zygnematophyceae Split |journal=Frontiers in Plant Science |volume=12 |article-number=735020 |doi=10.3389/fpls.2021.735020 |issn=1664-462X |pmc=8829067 |pmid=35154170|bibcode=2022FrPS...1235020Z |doi-access=free }}</ref>
| style="background:{{period color|Cryogenian}}" |~{{Period start|cryogenian}} {{Period start error|cryogenian}}
| style="background:{{period color|Cryogenian}}" |~{{Period start|cryogenian}} {{Period start error|cryogenian}}
|-
|-
| style="background:{{period color|Tonian}}" |[[Tonian]]
| style="background:{{period color|Tonian}}" |[[Tonian]]
| colspan="3" |Final assembly of [[Rodinia]] supercontinent occurs in early Tonian, with breakup beginning c. 800&nbsp;Ma. [[Sveconorwegian orogeny]] ends. [[Grenville Orogeny]] tapers off in North America. Lake Ruker / Nimrod Orogeny in Antarctica, 1,000&nbsp;±&nbsp;150&nbsp;Ma. Edmundian Orogeny (c. 920–850&nbsp;Ma), [[Gascoyne Complex]], Western Australia. Deposition of [[Adelaide Superbasin]] and [[Centralian Superbasin]] begins on [[Australia (continent)|Australian continent]]. First hypothetical [[animals]] (from holozoans) and terrestrial algal mats. Many endosymbiotic events concerning red and green algae occur, transferring plastids to [[ochrophyta]] (e.g. [[diatoms]], [[brown algae]]), [[dinoflagellate]]s, [[cryptophyta]], [[haptophyta]], and [[euglenid]]s (the events may have begun in the Mesoproterozoic)<ref name="Yoon_2004">{{Cite journal |last1=Yoon |first1=Hwan Su |last2=Hackett |first2=Jeremiah D. |last3=Ciniglia |first3=Claudia |last4=Pinto |first4=Gabriele |last5=Bhattacharya |first5=Debashish |date=2004 |title=A Molecular Timeline for the Origin of Photosynthetic Eukaryotes |url=https://academic.oup.com/mbe/article-lookup/doi/10.1093/molbev/msh075 |journal=Molecular Biology and Evolution |language=en |volume=21 |issue=5 |pages=809–818 |doi=10.1093/molbev/msh075 |pmid=14963099 |issn=1537-1719|doi-access=free }}</ref> while the first [[retaria]]ns (e.g. [[forams]]) also appear: eukaryotes diversify rapidly, including algal, eukaryovoric and [[Biomineralization|biomineralised]] forms. [[Trace fossil]]s of simple [[Multicellular|multi-celled]] eukaryotes. [[Neoproterozoic oxygenation event]] (NOE), 850–540 Ma.<ref>{{Cite journal |last1=Och |first1=Lawrence M. |last2=Shields-Zhou |first2=Graham A. |date=2012-01-01 |title=The Neoproterozoic oxygenation event: Environmental perturbations and biogeochemical cycling |url=https://linkinghub.elsevier.com/retrieve/pii/S0012825211001498 |journal=Earth-Science Reviews |language=en |volume=110 |issue=1–4 |pages=26–57 |doi=10.1016/j.earscirev.2011.09.004}}</ref>
| colspan="3" |Final assembly of [[Rodinia]] supercontinent occurs in early Tonian, with breakup beginning c. 800&nbsp;Ma. [[Sveconorwegian orogeny]] ends. [[Grenville Orogeny]] tapers off in North America. Lake Ruker / Nimrod Orogeny in Antarctica, 1,000&nbsp;±&nbsp;150&nbsp;Ma. Edmundian Orogeny (c. 920–850&nbsp;Ma), [[Gascoyne Complex]], Western Australia. Deposition of [[Adelaide Superbasin]] and [[Centralian Superbasin]] begins on [[Australia (continent)|Australian continent]]. First hypothetical [[animals]] (from holozoans) and terrestrial algal mats. Many endosymbiotic events concerning red and green algae occur, transferring plastids to [[ochrophyta]] (e.g. [[diatoms]], [[brown algae]]), [[dinoflagellate]]s, [[cryptophyta]], [[haptophyta]], and [[euglenid]]s (the events may have begun in the Mesoproterozoic)<ref name="Yoon_2004">{{Cite journal |last1=Yoon |first1=Hwan Su |last2=Hackett |first2=Jeremiah D. |last3=Ciniglia |first3=Claudia |last4=Pinto |first4=Gabriele |last5=Bhattacharya |first5=Debashish |date=2004 |title=A Molecular Timeline for the Origin of Photosynthetic Eukaryotes |url=https://academic.oup.com/mbe/article-lookup/doi/10.1093/molbev/msh075 |journal=Molecular Biology and Evolution |language=en |volume=21 |issue=5 |pages=809–818 |doi=10.1093/molbev/msh075 |pmid=14963099 |issn=1537-1719|doi-access=free }}</ref> while the first [[retaria]]ns (e.g. [[forams]]) also appear: eukaryotes diversify rapidly, including algal, eukaryovoric and [[Biomineralization|biomineralised]] forms. [[Trace fossil]]s of simple [[Multicellular|multi-celled]] eukaryotes. [[Neoproterozoic oxygenation event]] (NOE), 850–540 Ma.<ref>{{Cite journal |last1=Och |first1=Lawrence M. |last2=Shields-Zhou |first2=Graham A. |date=2012-01-01 |title=The Neoproterozoic oxygenation event: Environmental perturbations and biogeochemical cycling |url=https://linkinghub.elsevier.com/retrieve/pii/S0012825211001498 |journal=Earth-Science Reviews |language=en |volume=110 |issue=1–4 |pages=26–57 |doi=10.1016/j.earscirev.2011.09.004 |bibcode=2012ESRv..110...26O }}</ref>
| style="background:{{period color|Tonian}}" |{{Period start|tonian}} {{Period start error|tonian}}{{efn|name="absolute-age"|Defined by absolute age ([[Global Standard Stratigraphic Age]]).|group=note}}
| style="background:{{period color|Tonian}}" |{{Period start|tonian}} {{Period start error|tonian}}{{efn|name="absolute-age"|Defined by absolute age ([[Global Standard Stratigraphic Age]]).|group=note}}
|-
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Line 1,293: Line 1,296:
|-
|-
| style="background:{{period color|Hadean}}" |[[Hadean]]
| style="background:{{period color|Hadean}}" |[[Hadean]]
| colspan="5" |Formation of [[protolith]] of the oldest known rock ([[Acasta Gneiss]]) c. 4,031 to 3,580 Ma.<ref name="Bowring_1999">{{cite journal |last1=Bowring |first1=Samuel A. |last2=Williams |first2=Ian S. |year=1999 |title=Priscoan (4.00&ndash;4.03 Ga) orthogneisses from northwestern Canada |journal=Contributions to Mineralogy and Petrology |volume=134 |issue=1 |pages=3 |bibcode=1999CoMP..134....3B |doi=10.1007/s004100050465 |s2cid=128376754}}</ref><ref name="Iizuka_2007">{{Citation |last1=Iizuka |first1=Tsuyoshi |date=2007 |url=https://linkinghub.elsevier.com/retrieve/pii/S0166263507150313 |volume=15 |pages=127–147 |publisher=Elsevier |language=en |doi=10.1016/s0166-2635(07)15031-3 |isbn=978-0-444-52810-0 |access-date=2022-05-01 |last2=Komiya |first2=Tsuyoshi |last3=Maruyama |first3=Shigenori|title=Chapter 3.1 the Early Archean Acasta Gneiss Complex: Geological, Geochronological and Isotopic Studies and Implications for Early Crustal Evolution |series=Developments in Precambrian Geology }}</ref> Possible first appearance of [[plate tectonic]]s. First hypothetical [[Abiogenesis|life forms]]. End of the Early Bombardment Phase. Oldest known [[mineral]] ([[Zircon]], 4,404&nbsp;±&nbsp;8&nbsp;Ma).<ref name="Wilde_2001">{{Cite journal |last1=Wilde |first1=Simon A. |last2=Valley |first2=John W. |last3=Peck |first3=William H. |last4=Graham |first4=Colin M. |date=2001 |title=Evidence from detrital zircons for the existence of continental crust and oceans on the Earth 4.4 Gyr ago |url=http://www.nature.com/articles/35051550 |journal=Nature |language=en |volume=409 |issue=6817 |pages=175–178 |doi=10.1038/35051550 |issn=0028-0836 |pmid=11196637 |s2cid=4319774}}</ref> Asteroids and comets bring water to Earth, forming the first oceans. Formation of [[Moon]] (4,510 Ma), probably from a [[Giant impact hypothesis|giant impact]]. Formation of Earth (4,543 to 4,540 Ma)
| colspan="5" |Formation of [[protolith]] of the oldest known rock ([[Acasta Gneiss]]) c. 4,031 to 3,580 Ma.<ref name="Bowring_1999">{{cite journal |last1=Bowring |first1=Samuel A. |last2=Williams |first2=Ian S. |year=1999 |title=Priscoan (4.00&ndash;4.03 Ga) orthogneisses from northwestern Canada |journal=Contributions to Mineralogy and Petrology |volume=134 |issue=1 |page=3 |bibcode=1999CoMP..134....3B |doi=10.1007/s004100050465 |s2cid=128376754}}</ref><ref name="Iizuka_2007">{{Citation |last1=Iizuka |first1=Tsuyoshi |date=2007 |url=https://linkinghub.elsevier.com/retrieve/pii/S0166263507150313 |volume=15 |pages=127–147 |publisher=Elsevier |language=en |doi=10.1016/s0166-2635(07)15031-3 |isbn=978-0-444-52810-0 |access-date=2022-05-01 |last2=Komiya |first2=Tsuyoshi |last3=Maruyama |first3=Shigenori|title=Chapter 3.1 the Early Archean Acasta Gneiss Complex: Geological, Geochronological and Isotopic Studies and Implications for Early Crustal Evolution |series=Developments in Precambrian Geology }}</ref> Possible first appearance of [[plate tectonic]]s. First hypothetical [[Abiogenesis|life forms]]. End of the Early Bombardment Phase. Oldest known [[mineral]] ([[Zircon]], 4,404&nbsp;±&nbsp;8&nbsp;Ma).<ref name="Wilde_2001">{{Cite journal |last1=Wilde |first1=Simon A. |last2=Valley |first2=John W. |last3=Peck |first3=William H. |last4=Graham |first4=Colin M. |date=2001 |title=Evidence from detrital zircons for the existence of continental crust and oceans on the Earth 4.4 Gyr ago |url=http://www.nature.com/articles/35051550 |journal=Nature |language=en |volume=409 |issue=6817 |pages=175–178 |doi=10.1038/35051550 |issn=0028-0836 |pmid=11196637 |bibcode=2001Natur.409..175W |s2cid=4319774}}</ref> Asteroids and comets bring water to Earth, forming the first oceans. Formation of [[Moon]] (4,510 Ma), probably from a [[Giant impact hypothesis|giant impact]]. Formation of Earth (4,543 to 4,540 Ma)
| style="background:{{period color|Hadean}}" |{{Period start|hadean}} {{Period start error|hadean}}{{efn|name="absolute-age"|group=note}}
| style="background:{{period color|Hadean}}" |{{Period start|hadean}} {{Period start error|hadean}}{{efn|name="absolute-age"|group=note}}
|}
|}


== Non-Earth based geologic time scales ==
== Extraterrestrial geologic time scales ==
{{Main|Lunar geologic timescale|Martian geologic timescale|Geology of Venus}}Some other [[Planet#Solar System|planets]] and [[Natural satellite|satellites]] in the [[Solar System]] have sufficiently rigid structures to have preserved records of their own histories, for example, [[Geology of Venus|Venus]], [[Geology of Mars|Mars]] and the Earth's [[Moon]]. Dominantly fluid planets, such as the [[giant planet]]s, do not comparably preserve their history. Apart from the [[Late Heavy Bombardment]], events on other planets probably had little direct influence on the Earth, and events on Earth had correspondingly little effect on those planets. Construction of a time scale that links the planets is, therefore, of only limited relevance to the Earth's time scale, except in a Solar System context. The existence, timing, and terrestrial effects of the Late Heavy Bombardment are still a matter of debate.{{efn|Not enough is known about extra-solar planets for worthwhile speculation.|group=note}}
{{Main|Lunar geologic timescale|Martian geologic timescale|Geology of Venus}}Some other [[Planet#Solar System|planets]] and [[Natural satellite|satellites]] in the [[Solar System]] have sufficiently rigid structures to have preserved records of their own histories, for example, [[Geology of Venus|Venus]], [[Geology of Mars|Mars]] and the Earth's [[Moon]]. Dominantly fluid planets, such as the [[giant planet]]s, do not comparably preserve their history. Apart from the [[Late Heavy Bombardment]], events on other planets probably had little direct influence on the Earth, and events on Earth had correspondingly little effect on those planets. Construction of a time scale that links the planets is, therefore, of only limited relevance to the Earth's time scale, except in a Solar System context. The existence, timing, and terrestrial effects of the Late Heavy Bombardment are still a matter of debate.{{efn|Not enough is known about extra-solar planets for worthwhile speculation.|group=note}}


=== Lunar (selenological) time scale ===
=== Lunar (selenological) time scale ===
The [[Geology of the Moon|geologic history]] of Earth's Moon has been divided into a time scale based on [[Geomorphology|geomorphological]] markers, namely [[impact crater]]ing, [[volcanism]], and [[erosion]]. This process of dividing the Moon's history in this manner means that the time scale boundaries do not imply fundamental changes in geological processes, unlike Earth's geologic time scale. Five geologic systems/periods ([[Pre-Nectarian]], [[Nectarian]], [[Imbrian]], [[Eratosthenian]], [[Copernican period|Copernican]]), with the Imbrian divided into two series/epochs (Early and Late) were defined in the latest Lunar geologic time scale.<ref name="Wilhelms_1987">{{Cite book |last=Wilhelms |first=Don E. |title=The geologic history of the Moon |series=Professional Paper |publisher=United States Geological Survey |year=1987 |doi=10.3133/pp1348}}</ref> The Moon is unique in the Solar System in that it is the only other body from which humans have rock samples with a known geological context.
The [[Geology of the Moon|geologic history]] of Earth's Moon has been divided into a time scale based on [[Geomorphology|geomorphological]] markers, namely [[impact crater]]ing, [[volcanism]], and [[erosion]]. This process of dividing the Moon's history in this manner means that the time scale boundaries do not imply fundamental changes in geological processes, unlike Earth's geologic time scale. Five geologic systems/periods ([[Pre-Nectarian]], [[Nectarian]], [[Imbrian]], [[Eratosthenian]], [[Copernican period|Copernican]]), with the Imbrian divided into two series/epochs (Early and Late) were defined in the latest Lunar geologic time scale.<ref name="Wilhelms_1987">{{Cite book |last=Wilhelms |first=Don E. |title=The geologic history of the Moon |series=Professional Paper |publisher=United States Geological Survey |year=1987 |doi=10.3133/pp1348 |bibcode=1987ghm..book.....W }}</ref> The Moon is unique in the Solar System in that it is the only other body from which humans have rock samples with a known geological context.
{{Timeline Lunar Geological Timescale}}
{{Timeline Lunar Geological Timescale}}


=== Martian geologic time scale ===
=== Martian geologic time scale ===
The [[geological history of Mars]] has been divided into two alternate time scales. The first time scale for Mars was developed by studying the impact crater densities on the Martian surface. Through this method four periods have been defined, the Pre-Noachian (~4,500–4,100 Ma), Noachian (~4,100–3,700 Ma), Hesperian (~3,700–3,000 Ma), and Amazonian (~3,000 Ma to present).<ref name="Tanaka_1986">{{Cite journal |last=Tanaka |first=Kenneth L. |date=1986 |title=The stratigraphy of Mars |url=http://doi.wiley.com/10.1029/JB091iB13p0E139 |journal=Journal of Geophysical Research |language=en |volume=91 |issue=B13 |pages=E139 |doi=10.1029/JB091iB13p0E139 |bibcode=1986JGR....91E.139T |issn=0148-0227}}</ref><ref name="Carr_2010">{{Cite journal |last1=Carr |first1=Michael H. |last2=Head |first2=James W. |date=2010-06-01 |title=Geologic history of Mars |url=https://www.sciencedirect.com/science/article/pii/S0012821X09003847 |journal=Earth and Planetary Science Letters |series=Mars Express after 6 Years in Orbit: Mars Geology from Three-Dimensional Mapping by the High Resolution Stereo Camera (HRSC) Experiment |language=en |volume=294 |issue=3 |pages=185–203 |doi=10.1016/j.epsl.2009.06.042 |bibcode=2010E&PSL.294..185C |issn=0012-821X}}</ref>
The [[geological history of Mars]] has been divided into two alternate time scales. The first time scale for Mars was developed by studying the impact crater densities on the Martian surface. Through this method four periods have been defined, the Pre-Noachian (~4,500–4,100 Ma), Noachian (~4,100–3,700 Ma), Hesperian (~3,700–3,000 Ma), and Amazonian (~3,000 Ma to present).<ref name="Tanaka_1986">{{Cite journal |last=Tanaka |first=Kenneth L. |date=1986 |title=The stratigraphy of Mars |url=http://doi.wiley.com/10.1029/JB091iB13p0E139 |journal=Journal of Geophysical Research |language=en |volume=91 |issue=B13 |article-number=E139 |doi=10.1029/JB091iB13p0E139 |bibcode=1986JGR....91E.139T |issn=0148-0227}}</ref><ref name="Carr_2010">{{Cite journal |last1=Carr |first1=Michael H. |last2=Head |first2=James W. |date=2010-06-01 |title=Geologic history of Mars |url=https://www.sciencedirect.com/science/article/pii/S0012821X09003847 |journal=Earth and Planetary Science Letters |series=Mars Express after 6 Years in Orbit: Mars Geology from Three-Dimensional Mapping by the High Resolution Stereo Camera (HRSC) Experiment |language=en |volume=294 |issue=3 |pages=185–203 |doi=10.1016/j.epsl.2009.06.042 |bibcode=2010E&PSL.294..185C |issn=0012-821X}}</ref>
{{Mars timescale}}
{{Mars timescale}}
A second time scale based on mineral alteration observed by the OMEGA [[spectrometer]] on board the [[Mars Express]]. Using this method, three periods were defined, the Phyllocian (~4,500–4,000 Ma), Theiikian (~4,000–3,500 Ma), and Siderikian (~3,500 Ma to present).<ref name="Bibring_2006">{{Cite journal |last1=Bibring |first1=Jean-Pierre |last2=Langevin |first2=Yves |last3=Mustard |first3=John F. |last4=Poulet |first4=François |last5=Arvidson |first5=Raymond |last6=Gendrin |first6=Aline |last7=Gondet |first7=Brigitte |last8=Mangold |first8=Nicolas |last9=Pinet |first9=P. |last10=Forget |first10=F. |last11=Berthé |first11=Michel |date=2006-04-21 |title=Global Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express Data |url=https://www.science.org/doi/10.1126/science.1122659 |journal=Science |language=en |volume=312 |issue=5772 |pages=400–404 |doi=10.1126/science.1122659 |pmid=16627738 |bibcode=2006Sci...312..400B |s2cid=13968348 |issn=0036-8075}}</ref>
A second time scale based on mineral alteration observed by the OMEGA [[spectrometer]] on board the [[Mars Express]]. Using this method, three periods were defined, the Phyllocian (~4,500–4,000 Ma), Theiikian (~4,000–3,500 Ma), and Siderikian (~3,500 Ma to present).<ref name="Bibring_2006">{{Cite journal |last1=Bibring |first1=Jean-Pierre |last2=Langevin |first2=Yves |last3=Mustard |first3=John F. |last4=Poulet |first4=François |last5=Arvidson |first5=Raymond |last6=Gendrin |first6=Aline |last7=Gondet |first7=Brigitte |last8=Mangold |first8=Nicolas |last9=Pinet |first9=P. |last10=Forget |first10=F. |last11=Berthé |first11=Michel |date=2006-04-21 |title=Global Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express Data |url=https://www.science.org/doi/10.1126/science.1122659 |journal=Science |language=en |volume=312 |issue=5772 |pages=400–404 |doi=10.1126/science.1122659 |pmid=16627738 |bibcode=2006Sci...312..400B |s2cid=13968348 |issn=0036-8075}}</ref>
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==Further reading==
==Further reading==
* {{cite journal |date=2009 |last1=Aubry|first1=Marie-Pierre|last2=Van Couvering|first2=John A.|last3=Christie-Blick|first3=Nicholas|last4= Landing|first4=Ed|last5=Pratt|first5=Brian R.|last6=Owen|first6=Donald E.|last7=Ferrusquia-Villafranca|first7=Ismael |title=Terminology of geological time: Establishment of a community standard |journal=Stratigraphy |volume=6 |issue=2 |pages=100–105 |doi=10.7916/D8DR35JQ}}
* {{cite journal |date=2009 |last1=Aubry|first1=Marie-Pierre|last2=Van Couvering|first2=John A.|last3=Christie-Blick|first3=Nicholas|last4= Landing|first4=Ed|last5=Pratt|first5=Brian R.|last6=Owen|first6=Donald E.|last7=Ferrusquia-Villafranca|first7=Ismael |title=Terminology of geological time: Establishment of a community standard |journal=Stratigraphy |volume=6 |issue=2 |pages=100–105 |doi=10.7916/D8DR35JQ}}
* {{cite journal |date=2004 |last1=Gradstein |first1=F. M. |last2=Ogg |first2=J. G. |title=A Geologic Time scale 2004 – Why, How and Where Next! |journal=Lethaia |volume=37 |issue=2 |pages=175–181 |url=https://eesc.columbia.edu/courses/w4937/Readings/Gradstein_Ogg_2004.pdf |access-date=30 November 2018 |doi=10.1080/00241160410006483 |bibcode=2004Letha..37..175G |archive-url=https://web.archive.org/web/20180417173639/http://eesc.columbia.edu/courses/w4937/Readings/Gradstein_Ogg_2004.pdf |archive-date=17 April 2018 |url-status=dead }}
* {{cite journal |date=2004 |last1=Gradstein |first1=F. M. |last2=Ogg |first2=J. G. |title=A Geologic Time scale 2004 – Why, How and Where Next! |journal=Lethaia |volume=37 |issue=2 |pages=175–181 |url=https://eesc.columbia.edu/courses/w4937/Readings/Gradstein_Ogg_2004.pdf |access-date=30 November 2018 |doi=10.1080/00241160410006483 |bibcode=2004Letha..37..175G |archive-url=https://web.archive.org/web/20180417173639/http://eesc.columbia.edu/courses/w4937/Readings/Gradstein_Ogg_2004.pdf |archive-date=17 April 2018 }}
* {{cite book |date=2004 |last1=Gradstein|first1=Felix M.|last2=Ogg|first2=James G.|last3=Smith|first3=Alan G. |title=A Geologic Time Scale 2004 |url=https://books.google.com/books?id=rse4v1P-f9kC |location=Cambridge, UK |publisher=Cambridge University Press |isbn=978-0-521-78142-8 |access-date=18 November 2011}}
* {{cite book |date=2004 |last1=Gradstein|first1=Felix M.|last2=Ogg|first2=James G.|last3=Smith|first3=Alan G. |title=A Geologic Time Scale 2004 |url=https://books.google.com/books?id=rse4v1P-f9kC |location=Cambridge, UK |publisher=Cambridge University Press |isbn=978-0-521-78142-8 |access-date=18 November 2011}}
* {{cite journal |date=June 2004 |last1=Gradstein |first1=Felix M. |last2=Ogg |first2=James G. |last3=Smith |first3=Alan G. |last4=Bleeker |first4=Wouter |last5=Laurens |first5=Lucas, J. |title=A new Geologic Time Scale, with special reference to Precambrian and Neogene |journal=Episodes |volume=27 |issue=2 |pages=83–100 |doi=10.18814/epiiugs/2004/v27i2/002 |doi-access=free }}
* {{cite journal |date=June 2004 |last1=Gradstein |first1=Felix M. |last2=Ogg |first2=James G. |last3=Smith |first3=Alan G. |last4=Bleeker |first4=Wouter |last5=Laurens |first5=Lucas, J. |title=A new Geologic Time Scale, with special reference to Precambrian and Neogene |journal=Episodes |volume=27 |issue=2 |pages=83–100 |doi=10.18814/epiiugs/2004/v27i2/002 |doi-access=free }}

Latest revision as of 18:14, 19 November 2025

Template:Short description Template:Use dmy dates Template:Use British English

Geologic time scale proportionally represented as a log-spiral. The image also shows some notable events in Earth's history and the general evolution of life.
The geologic time scale, proportionally represented as a log-spiral with some major events in Earth's history. A megaannus (Ma) represents one million (106) years.

The geologic time scale or geological time scale (GTS) is a representation of time based on the rock record of Earth. It is a system of chronological dating that uses chronostratigraphy (the process of relating strata to time) and geochronology (a scientific branch of geology that aims to determine the age of rocks). It is used primarily by Earth scientists (including geologists, paleontologists, geophysicists, geochemists, and paleoclimatologists) to describe the timing and relationships of events in geologic history. The time scale has been developed through the study of rock layers and the observation of their relationships and identifying features such as lithologies, paleomagnetic properties, and fossils. The definition of standardised international units of geological time is the responsibility of the International Commission on Stratigraphy (ICS), a constituent body of the International Union of Geological Sciences (IUGS), whose primary objective[1] is to precisely define global chronostratigraphic units of the International Chronostratigraphic Chart (ICC)Template:Ref icc that are used to define divisions of geological time. The chronostratigraphic divisions are in turn used to define geochronologic units.[2]

Principles

Script error: No such module "Labelled list hatnote". The geologic time scale is a way of representing deep time based on events that have occurred through Earth's history, a time span of about 4.54 ± 0.05 billion years.[3] It chronologically organises strata, and subsequently time, by observing fundamental changes in stratigraphy that correspond to major geological or paleontological events. For example, the Cretaceous–Paleogene extinction event, marks the lower boundary of the Paleogene System/Period and thus the boundary between the Cretaceous and Paleogene systems/periods. For divisions prior to the Cryogenian, arbitrary numeric boundary definitions (Global Standard Stratigraphic Ages, GSSAs) are used to divide geologic time. Proposals have been made to better reconcile these divisions with the rock record.[4][5]

Historically, regional geologic time scales were used[5] due to the litho- and biostratigraphic differences around the world in time equivalent rocks. The ICS has long worked to reconcile conflicting terminology by standardising globally significant and identifiable stratigraphic horizons that can be used to define the lower boundaries of chronostratigraphic units. Defining chronostratigraphic units in such a manner allows for the use of global, standardised nomenclature. The International Chronostratigraphic Chart represents this ongoing effort.

Several key principles are used to determine the relative relationships of rocks and thus their chronostratigraphic position.[6][7]

The law of superposition that states that in undeformed stratigraphic sequences the oldest strata will lie at the bottom of the sequence, while newer material stacks upon the surface.[8][9][10][7] In practice, this means a younger rock will lie on top of an older rock unless there is evidence to suggest otherwise.

The principle of original horizontality that states layers of sediments will originally be deposited horizontally under the action of gravity.[8][10][7] However, it is now known that not all sedimentary layers are deposited purely horizontally,[7][11] but this principle is still a useful concept.

The principle of lateral continuity that states layers of sediments extend laterally in all directions until either thinning out or being cut off by a different rock layer, i.e. they are laterally continuous.[8] Layers do not extend indefinitely; their limits are controlled by the amount and type of sediment in a sedimentary basin, and the geometry of that basin.

The principle of cross-cutting relationships that states a rock that cuts across another rock must be younger than the rock it cuts across.[8][9][10][7]

The law of included fragments that states small fragments of one type of rock that are embedded in a second type of rock must have formed first, and were included when the second rock was forming.[10][7]

The relationships of unconformities which are geologic features representing a gap in the geologic record. Unconformities are formed during periods of erosion or non-deposition, indicating non-continuous sediment deposition.[7] Observing the type and relationships of unconformities in strata allows geologist to understand the relative timing of the strata.

The principle of faunal succession (where applicable) that states rock strata contain distinctive sets of fossils that succeed each other vertically in a specific and reliable order.[12][7] This allows for a correlation of strata even when the horizon between them is not continuous.

Divisions of geologic time

Script error: No such module "Labelled list hatnote". The geologic time scale is divided into chronostratigraphic units and their corresponding geochronologic units.

Formal, hierarchical units of the geologic time scale (largest to smallest)
Chronostratigraphic unit (strata) Geochronologic unit (time) Time spanTemplate:Efn
Eonothem Eon Several hundred million years to two billion years
Erathem Era Tens to hundreds of millions of years
System Period Millions of years to tens of millions of years
Series Epoch Hundreds of thousands of years to tens of millions of years
Subseries Subepoch Thousands of years to millions of years
Stage Age Thousands of years to millions of years

The subdivisions Template:Em and Template:Em are used as the geochronologic equivalents of the chronostratigraphic Template:Em and Template:Em, e.g., Early Triassic Period (geochronologic unit) is used in place of Lower Triassic System (chronostratigraphic unit).

Rocks representing a given chronostratigraphic unit are that chronostratigraphic unit, and the time they were laid down in is the geochronologic unit, e.g., the rocks that represent the Silurian System Template:Em the Silurian System and they were deposited Template:Em the Silurian Period. This definition means the numeric age of a geochronologic unit can be changed (and is more often subject to change) when refined by geochronometry while the equivalent chronostratigraphic unit (the revision of which is less frequent) remains unchanged. For example, in early 2022, the boundary between the Ediacaran and Cambrian periods (geochronologic units) was revised from 541 Ma to 538.8 Ma but the rock definition of the boundary (GSSP) at the base of the Cambrian, and thus the boundary between the Ediacaran and Cambrian systems (chronostratigraphic units) has not been changed; rather, the absolute age has merely been refined.

Terminology

Template:Em is the element of stratigraphy that deals with the relation between rock bodies and the relative measurement of geological time.[14] It is the process where distinct strata between defined stratigraphic horizons are assigned to represent a relative interval of geologic time.

A Template:EmScript error: No such module "anchor". is a body of rock, layered or unlayered, that is defined between specified stratigraphic horizons which represent specified intervals of geologic time. They include all rocks representative of a specific interval of geologic time, and only this time span. Eonothem, erathem, system, series, subseries, stage, and substage are the hierarchical chronostratigraphic units.[14]

A Template:EmScript error: No such module "anchor". is a subdivision of geologic time. It is a numeric representation of an intangible property (time).[16] These units are arranged in a hierarchy: eon, era, period, epoch, subepoch, age, and subage.[14] Template:Em is the scientific branch of geology that aims to determine the age of rocks, fossils, and sediments either through absolute (e.g., radiometric dating) or relative means (e.g., stratigraphic position, paleomagnetism, stable isotope ratios). Template:Em is the field of geochronology that numerically quantifies geologic time.[16]

A Template:Em (GSSP) is an internationally agreed-upon reference point on a stratigraphic section that defines the lower boundaries of stages on the geologic time scale.[17] (Recently this has been used to define the base of a system)[18]

A Template:Em (GSSA)[19] is a numeric-only, chronologic reference point used to define the base of geochronologic units prior to the Cryogenian. These points are arbitrarily defined.[14] They are used where GSSPs have not yet been established. Research is ongoing to define GSSPs for the base of all units that are currently defined by GSSAs.

The standard international units of the geologic time scale are published by the International Commission on Stratigraphy on the International Chronostratigraphic Chart. However, regional terms are still in use in some areas. The numeric values on the International Chronostratigrahpic Chart are represented by the unit Ma (megaannum, for 'million years'). For example, Template:Period start Template:Period start error Ma, the lower boundary of the Jurassic Period, is defined as 201,400,000 years old with an uncertainty of 200,000 years. Other SI prefix units commonly used by geologists are Ga (gigaannum, billion years), and ka (kiloannum, thousand years), with the latter often represented in calibrated units (before present).

Naming of geologic time

The names of geologic time units are defined for chronostratigraphic units with the corresponding geochronologic unit sharing the same name with a change to the suffix (e.g. Phanerozoic Eonothem becomes the Phanerozoic Eon). Names of erathems in the Phanerozoic were chosen to reflect major changes in the history of life on Earth: Paleozoic (old life), Mesozoic (middle life), and Cenozoic (new life). Names of systems are diverse in origin, with some indicating chronologic position (e.g., Paleogene), while others are named for lithology (e.g., Cretaceous), geography (e.g., Permian), or are tribal (e.g., Ordovician) in origin. Most currently recognised series and subseries are named for their position within a system/series (early/middle/late); however, the International Commission on Stratigraphy advocates for all new series and subseries to be named for a geographic feature in the vicinity of its stratotype or type locality. The name of stages should also be derived from a geographic feature in the locality of its stratotype or type locality.[14]

Informally, the time before the Cambrian is often referred to as the Precambrian or pre-Cambrian (Supereon).[4]Template:Efn

Time span and etymology of geologic eonothem/eon names
Name Time span Duration (million years) Etymology of name
Phanerozoic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek φανερός (phanerós) 'visible' or 'abundant' and ζωή (zoē) 'life'.
Proterozoic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek πρότερος (próteros) 'former' or 'earlier' and ζωή (zoē) 'life'.
Archean Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek ἀρχή (archē) 'beginning, origin'.
Hadean Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Hades, Template:Langx, the god of the underworld (hell, the inferno) in Greek mythology.
Time span and etymology of geologic erathem/era names
Name Time span Duration (million years) Etymology of name
Cenozoic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek καινός (kainós) 'new' and ζωή (zōḗ) 'life'.
Mesozoic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek μέσο (méso) 'middle' and ζωή (zōḗ) 'life'.
Paleozoic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek παλιός (palaiós) 'old' and ζωή (zōḗ) 'life'.
Neoproterozoic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek νέος (néos) 'new' or 'young', πρότερος (próteros) 'former' or 'earlier', and ζωή (zōḗ) 'life'.
Mesoproterozoic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek μέσο (méso) 'middle', πρότερος (próteros) 'former' or 'earlier', and ζωή (zōḗ) 'life'.
Paleoproterozoic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek παλιός (palaiós) 'old', πρότερος (próteros) 'former' or 'earlier', and ζωή (zōḗ) 'life'.
Neoarchean Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek νέος (néos) 'new' or 'young' and ἀρχαῖος (arkhaîos) 'ancient'.
Mesoarchean Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek μέσο (méso) 'middle' and ἀρχαῖος (arkhaîos) 'ancient'.
Paleoarchean Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek παλιός (palaiós) 'old' and ἀρχαῖος (arkhaîos) 'ancient'.
Eoarchean Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek ἠώς (ēōs) 'dawn' and ἀρχαῖος (arkhaîos) 'ancient'.
Time span and etymology of geologic system/period names
Name Time span Duration (million years) Etymology of name
Quaternary Template:Period span/brief Expression error: Unrecognized punctuation character "[". First introduced by Jules Desnoyers in 1829 for sediments in France's Seine Basin that appeared to be younger than TertiaryTemplate:Efn rocks.[20]
Neogene Template:Period span/brief Expression error: Unrecognized punctuation character "[". Derived from Greek νέος (néos) 'new' and γενεά (geneá) 'genesis' or 'birth'.
Paleogene Template:Period span/brief Expression error: Unrecognized punctuation character "[". Derived from Greek παλιός (palaiós) 'old' and γενεά (geneá) 'genesis' or 'birth'.
Cretaceous ~Template:Period span/brief ~Expression error: Unrecognized punctuation character "[". Derived from Terrain Crétacé used in 1822 by Jean d'Omalius d'Halloy in reference to extensive beds of chalk within the Paris Basin.[21] Ultimately derived from Latin crēta 'chalk'.
Jurassic Template:Period span/brief ~Expression error: Unrecognized punctuation character "[". Named after the Jura Mountains. Originally used by Alexander von Humboldt as 'Jura Kalkstein' (Jura limestone) in 1799.[22] Alexandre Brongniart was the first to publish the term Jurassic in 1829.[23][24]
Triassic Template:Period span/brief Expression error: Unrecognized punctuation character "[". From the Trias of Friedrich August von Alberti in reference to a trio of formations widespread in southern Germany.
Permian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named after the historical region of Perm, Russian Empire.[25]
Carboniferous Template:Period span/brief Expression error: Unrecognized punctuation character "[". Means 'coal-bearing', from the Latin carbō (coal) and ferō (to bear, carry).[26]
Devonian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named after Devon, England.[27]
Silurian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named after the Celtic tribe, the Silures.[28]
Ordovician Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named after the Celtic tribe, Ordovices.[29][30]
Cambrian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for Cambria, a Latinised form of the Welsh name for Wales, Cymru.[31]
Ediacaran Template:Period span/brief ~Expression error: Unrecognized punctuation character "[". Named for the Ediacara Hills. Ediacara is possibly a corruption of Kuyani 'Yata Takarra' 'hard or stony ground'.[32][33]
Cryogenian Template:Period span/brief ~Expression error: Unrecognized punctuation character "[". From Greek κρύος (krýos) 'cold' and γένεσις (génesis) 'birth'.[5]
Tonian Template:Period span/brief ~Expression error: Unrecognized punctuation character "[". From Greek τόνος (tónos) 'stretch'.[5]
Stenian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek στενός (stenós) 'narrow'.[5]
Ectasian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek ἔκτᾰσῐς (éktasis) 'extension'.[5]
Calymmian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek κάλυμμᾰ (kálumma) 'cover'.[5]
Statherian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek σταθερός (statherós) 'stable'.[5]
Orosirian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek ὀροσειρά (oroseirá) 'mountain range'.[5]
Rhyacian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek ῥύαξ (rhýax) 'stream of lava'.[5]
Siderian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek σίδηρος (sídēros) 'iron'.[5]
Time span and etymology of geologic series/epoch names
Name Time span Duration (million years) Etymology of name
Holocene Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Greek ὅλος (hólos) 'whole' and καινός (kainós) 'new'
Pleistocene Template:Period span/brief Expression error: Unrecognized punctuation character "[". Coined in the early 1830s from Greek πλεῖστος (pleîstos) 'most' and καινός (kainós) 'new'
Pliocene Template:Period span/brief Expression error: Unrecognized punctuation character "[". Coined in the early 1830s from Greek πλείων (pleíōn) 'more' and καινός (kainós) 'new'
Miocene Template:Period span/brief Expression error: Unrecognized punctuation character "[". Coined in the early 1830s from Greek μείων (meíōn) 'less' and καινός (kainós) 'new'
Oligocene Template:Period span/brief Expression error: Unrecognized punctuation character "[". Coined in the 1850s from Greek ὀλίγος (olígos) 'few' and καινός (kainós) 'new'
Eocene Template:Period span/brief Expression error: Unrecognized punctuation character "[". Coined in the early 1830s from Greek ἠώς (ēōs) 'dawn' and καινός (kainós) 'new', referring to the dawn of modern life during this epoch
Paleocene Template:Period span/brief Expression error: Unrecognized punctuation character "[". Coined by Wilhelm Philippe Schimper in 1874 as a portmanteau of paleo- + Eocene, but on the surface from Greek παλαιός (palaios) 'old' and καινός (kainós) 'new'
Upper Cretaceous Template:Period span/brief Expression error: Unrecognized punctuation character "[". See Cretaceous
Lower Cretaceous Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Upper Jurassic
Template:Period span/brief Expression error: Unrecognized punctuation character "[". See Jurassic
Middle Jurassic Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Lower Jurassic
Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Upper Triassic Template:Period span/brief Expression error: Unrecognized punctuation character "[". See Triassic
Middle Triassic
Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Lower Triassic Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Lopingian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for Loping, China, an anglicization of Mandarin 乐平 (lèpíng) 'peaceful music'
Guadalupian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for the Guadalupe Mountains of the American Southwest, ultimately from Arabic وَادِي ٱل (wādī al) 'valley of the' and Latin lupus 'wolf' via Spanish
Cisuralian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Latin cis- (before) + Russian Урал (Ural), referring to the western slopes of the Ural Mountains
Upper Pennsylvanian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for the US state of Pennsylvania, from William Penn + Latin silvanus (forest) + -ia by analogy to Transylvania
Middle Pennsylvanian Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Lower Pennsylvanian Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Upper Mississippian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for the Mississippi River, from Ojibwe ᒥᐦᓯᓰᐱ (misi-ziibi) 'great river'
Middle Mississippian Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Lower Mississippian Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Upper Devonian Template:Period span/brief Expression error: Unrecognized punctuation character "[". See Devonian
Middle Devonian Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Lower Devonian Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Pridoli Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for the Homolka a Přídolí nature reserve near Prague, Czechia
Ludlow Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named after Ludlow, England
Wenlock Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for the Wenlock Edge in Shropshire, England
Llandovery Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named after Llandovery, Wales
Upper Ordovician Template:Period span/brief Expression error: Unrecognized punctuation character "[". See Ordovician
Middle Ordovician Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Lower Ordovician Template:Period span/brief Expression error: Unrecognized punctuation character "[".
Furongian Template:Period span/brief Expression error: Unrecognized punctuation character "[". From Mandarin 芙蓉 (fúróng) 'lotus', referring to the state symbol of Hunan
Miaolingian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for the Template:Ill mountains of Guizhou, Mandarin for 'sprouting peaks'
Cambrian Series 2 (informal) Template:Period span/brief Expression error: Unrecognized punctuation character "[". See Cambrian
Terreneuvian Template:Period span/brief Expression error: Unrecognized punctuation character "[". Named for Terre-Neuve, a French calque of Newfoundland

History of the geologic time scale

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Early history

The most modern geological time scale was not formulated until 1911[34] by Arthur Holmes (1890 – 1965), who drew inspiration from James Hutton (1726–1797), a Scottish Geologist who presented the idea of uniformitarianism or the theory that changes to the Earth's crust resulted from continuous and uniform processes.[35] The broader concept of the relation between rocks and time can be traced back to (at least) the philosophers of Ancient Greece from 1200 BC to 600 AD. Xenophanes of Colophon (c. 570–487 BCE) observed rock beds with fossils of seashells located above the sea-level, viewed them as once living organisms, and used this to imply an unstable relationship in which the sea had at times transgressed over the land and at other times had regressed.[36] This view was shared by a few of Xenophanes's scholars and those that followed, including Aristotle (384–322 BC) who (with additional observations) reasoned that the positions of land and sea had changed over long periods of time. The concept of deep time was also recognized by Chinese naturalist Shen Kuo[37] (1031–1095) and Islamic scientist-philosophers, notably the Brothers of Purity, who wrote on the processes of stratification over the passage of time in their treatises.[36] Their work likely inspired that of the 11th-century Persian polymath Avicenna (Ibn Sînâ, 980–1037) who wrote in The Book of Healing (1027) on the concept of stratification and superposition, pre-dating Nicolas Steno by more than six centuries.[36] Avicenna also recognized fossils as "petrifications of the bodies of plants and animals",[38] with the 13th-century Dominican bishop Albertus Magnus (c. 1200–1280), who drew from Aristotle's natural philosophy, extending this into a theory of a petrifying fluid.[39] These works appeared to have little influence on scholars in Medieval Europe who looked to the Bible to explain the origins of fossils and sea-level changes, often attributing these to the 'Deluge', including Ristoro d'Arezzo in 1282.[36] It was not until the Italian Renaissance when Leonardo da Vinci (1452–1519) would reinvigorate the relationships between stratification, relative sea-level change, and time, denouncing attribution of fossils to the 'Deluge':[40][36]

<templatestyles src="Template:Blockquote/styles.css" />

Of the stupidity and ignorance of those who imagine that these creatures were carried to such places distant from the sea by the Deluge...Why do we find so many fragments and whole shells between the different layers of stone unless they had been upon the shore and had been covered over by earth newly thrown up by the sea which then became petrified? And if the above-mentioned Deluge had carried them to these places from the sea, you would find the shells at the edge of one layer of rock only, not at the edge of many where may be counted the winters of the years during which the sea multiplied the layers of sand and mud brought down by the neighboring rivers and spread them over its shores. And if you wish to say that there must have been many deluges in order to produce these layers and the shells among them it would then become necessary for you to affirm that such a deluge took place every year.

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File:Sketch of the Succession pf Strata and their relative Altitudes.jpg
Sketch of the Succession of Strata and their Relative Altitudes (William Smith)

These views of da Vinci remained unpublished, and thus lacked influence at the time; however, questions of fossils and their significance were pursued and, while views against Genesis were not readily accepted and dissent from religious doctrine was in some places unwise, scholars such as Girolamo Fracastoro shared da Vinci's views, and found the attribution of fossils to the 'Deluge' absurd.[36] Although many theories surrounding philosophy and concepts of rocks were developed in earlier years, "the first serious attempts to formulate a geological time scale that could be applied anywhere on Earth were made in the late 18th century."[39] Later, in the 19th century, academics further developed theories on stratification. William Smith, often referred to as the "Father of Geology"[41] developed theories through observations rather than drawing from the scholars that came before him. Smith's work was primarily based on his detailed study of rock layers and fossils during his time and he created "the first map to depict so many rock formations over such a large area".[41] After studying rock layers and the fossils they contained, Smith concluded that each layer of rock contained distinct material that could be used to identify and correlate rock layers across different regions of the world.[42] Smith developed the concept of faunal succession or the idea that fossils can serve as a marker for the age of the strata they are found in and published his ideas in his 1816 book, "Strata identified by organized fossils."[42]

Establishment of primary principles

Niels Stensen, more commonly known as Nicolas Steno (1638–1686), is credited with establishing four of the guiding principles of stratigraphy.[36] In De solido intra solidum naturaliter contento dissertationis prodromus Steno states:[8][43]

  • When any given stratum was being formed, all the matter resting on it was fluid and, therefore, when the lowest stratum was being formed, none of the upper strata existed.
  • ... strata which are either perpendicular to the horizon or inclined to it were at one time parallel to the horizon.
  • When any given stratum was being formed, it was either encompassed at its edges by another solid substance or it covered the whole globe of the earth. Hence, it follows that wherever bared edges of strata are seen, either a continuation of the same strata must be looked for or another solid substance must be found that kept the material of the strata from being dispersed.
  • If a body or discontinuity cuts across a stratum, it must have formed after that stratum.

Respectively, these are the principles of superposition, original horizontality, lateral continuity, and cross-cutting relationships. From this Steno reasoned that strata were laid down in succession and inferred relative time (in Steno's belief, time from Creation). While Steno's principles were simple and attracted much attention, applying them proved challenging.[36] These basic principles, albeit with improved and more nuanced interpretations, still form the foundational principles of determining the correlation of strata relative to geologic time.

Over the course of the 18th-century geologists realised that:

  • Sequences of strata often become eroded, distorted, tilted, or even inverted after deposition
  • Strata laid down at the same time in different areas could have entirely different appearances
  • The strata of any given area represented only part of Earth's long history

Formulation of a modern geologic time scale

The apparent, earliest formal division of the geologic record with respect to time was introduced during the era of Biblical models by Thomas Burnet who applied a two-fold terminology to mountains by identifying "montes primarii" for rock formed at the time of the 'Deluge', and younger "monticulos secundarios" formed later from the debris of the "primarii".[44][36] Anton Moro (1687–1784) also used primary and secondary divisions for rock units but his mechanism was volcanic.[45][36] In this early version of the Plutonism theory, the interior of Earth was seen as hot, and this drove the creation of primary igneous and metamorphic rocks and secondary rocks formed contorted and fossiliferous sediments. These primary and secondary divisions were expanded on by Giovanni Targioni Tozzetti (1712–1783) and Giovanni Arduino (1713–1795) to include tertiary and quaternary divisions.[36] These divisions were used to describe both the time during which the rocks were laid down, and the collection of rocks themselves (i.e., it was correct to say Tertiary rocks, and Tertiary Period). Only the Quaternary division is retained in the modern geologic time scale, while the Tertiary division was in use until the early 21st century. The Neptunism and Plutonism theories would compete into the early 19th century with a key driver for resolution of this debate being the work of James Hutton (1726–1797), in particular his Theory of the Earth, first presented before the Royal Society of Edinburgh in 1785.[46][9][47] Hutton's theory would later become known as uniformitarianism, popularised by John Playfair[48] (1748–1819) and later Charles Lyell (1797–1875) in his Principles of Geology.[10][49][50] Their theories strongly contested the 6,000 year age of the Earth as suggested determined by James Ussher via Biblical chronology that was accepted at the time by western religion. Instead, using geological evidence, they contested Earth to be much older, cementing the concept of deep time.

During the early 19th century William Smith, Georges Cuvier, Jean d'Omalius d'Halloy, and Alexandre Brongniart pioneered the systematic division of rocks by stratigraphy and fossil assemblages. These geologists began to use the local names given to rock units in a wider sense, correlating strata across national and continental boundaries based on their similarity to each other. Many of the names below erathem/era rank in use on the modern ICC/GTS were determined during the early to mid-19th century.

The advent of geochronometry

File:Pierre Lecomte du Noüy - LES AGES DE LA VIE SUR LA TERRE - in L'Homme et sa destinée - 1947.jpg
One example of an obsolete geological time scale (France, mid-1940s).

During the 19th century, the debate regarding Earth's age was renewed, with geologists estimating ages based on denudation rates and sedimentary thicknesses or ocean chemistry, and physicists determining ages for the cooling of the Earth or the Sun using basic thermodynamics or orbital physics.[3] These estimations varied from 15,000 million years to 0.075 million years depending on method and author, but the estimations of Lord Kelvin and Clarence King were held in high regard at the time due to their pre-eminence in physics and geology. All of these early geochronometric determinations would later prove to be incorrect.

The discovery of radioactive decay by Henri Becquerel, Marie Curie, and Pierre Curie laid the ground work for radiometric dating, but the knowledge and tools required for accurate determination of radiometric ages would not be in place until the mid-1950s.[3] Early attempts at determining ages of uranium minerals and rocks by Ernest Rutherford, Bertram Boltwood, Robert Strutt, and Arthur Holmes, would culminate in what are considered the first international geological time scales by Holmes in 1911 and 1913.[34][51][52] The discovery of isotopes in 1913[53] by Frederick Soddy, and the developments in mass spectrometry pioneered by Francis William Aston, Arthur Jeffrey Dempster, and Alfred O. C. Nier during the early to mid-20th century would finally allow for the accurate determination of radiometric ages, with Holmes publishing several revisions to his geological time-scale with his final version in 1960.[3][52][54][55]

Modern international geological time scale

The establishment of the IUGS in 1961[56] and acceptance of the Commission on Stratigraphy (applied in 1965)[57] to become a member commission of IUGS led to the founding of the ICS. One of the primary objectives of the ICS is "the establishment, publication and revision of the ICS International Chronostratigraphic Chart which is the standard, reference global Geological Time Scale to include the ratified Commission decisions".[1]

Following on from Holmes, several A Geological Time Scale books were published in 1982,[58] 1989,[59] 2004,[60] 2008,[61] 2012,[62] 2016,[63] and 2020.[64] However, since 2013, the ICS has taken responsibility for producing and distributing the ICC citing the commercial nature, independent creation, and lack of oversight by the ICS on the prior published GTS versions (GTS books prior to 2013) although these versions were published in close association with the ICS.[2] Subsequent Geologic Time Scale books (2016[63] and 2020[64]) are commercial publications with no oversight from the ICS, and do not entirely conform to the chart produced by the ICS. The ICS produced GTS charts are versioned (year/month) beginning at v2013/01. At least one new version is published each year incorporating any changes ratified by the ICS since the prior version.

The following five timelines show the geologic time scale to scale. The first shows the entire time from the formation of Earth to the present, but this gives little space for the most recent eon. The second timeline shows an expanded view of the most recent eon. In a similar way, the most recent era is expanded in the third timeline, the most recent period is expanded in the fourth timeline, and the most recent epoch is expanded in the fifth timeline.

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Period = from:-4567.3 till:0 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:500 start:-4500 ScaleMinor = unit:year increment:100 start:-4500

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 id:phanerozoic value:rgb(0.604,0.851,0.867)
 id:cenozoic value:rgb(0.949,0.976,0.114)
 id:quaternary value:rgb(0.976,0.976,0.498)
 id:neogene value:rgb(1,0.902,0.098)
 id:paleogene value:rgb(0.992,0.604,0.322)
 id:mesozoic value:rgb(0.403,0.773,0.792)
 id:cretaceous value:rgb(0.498,0.776,0.306)
 id:jurassic value:rgb(0.204,0.698,0.788)
 id:triassic value:rgb(0.506,0.169,0.573)
 id:paleozoic value:rgb(0.6,0.753,0.553)
 id:permian value:rgb(0.941,0.251,0.157)
 id:carboniferous value:rgb(0.403,0.647,0.6)
 id:devonian value:rgb(0.796,0.549,0.216)
 id:silurian value:rgb(0.702,0.882,0.714)
 id:ordovician value:rgb(0,0.573,0.439)
 id:cambrian value:rgb(0.498,0.627,0.337)
 id:black  value:black
 id:white  value:white
 id:darkgreen value:rgb(0,0.35,0)

Period = from:-538.8 till:0 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:100 start:-500 ScaleMinor = unit:year increment:10 start:-530

Define $markred = text:"*" textcolor:red shift:(0,3) fontsize:10 Define $markgreen = text:"*" textcolor:darkgreen shift:(0,3) fontsize:10

PlotData=

 align:center textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
 bar:eon
 at:      0   align:right  $markred 
 at:   -538.8   align:left   $markred shift:(2,3)
 from: -538.8   till:    0   text:Phanerozoic color:phanerozoic
 bar:era
 at:   0     align:right $markgreen
 at:   -66 align:left  $markgreen shift:(2,3)
 from: -66 till: 0     text:Cenozoic color:cenozoic
 from: -251.902  till: -66 text:Mesozoic color:mesozoic
 from: -538.8  till: -251.902  text:Paleozoic color:paleozoic
 bar:period fontsize:8
 from: -2.58 till: 0 text:Q color:quaternary
 from: -23.03 till: -2.58 text:Neogene color:neogene
 from: -66 till: -23.03 text:Paleogene color:paleogene
 from: -145 till: -66 text:Cretaceous color:cretaceous
 from: -201.4 till: -145 text:Jurassic color:jurassic
 from: -251.902 till: -201.4 text:Triassic color:triassic
 from: -298.9 till: -251.902 text:Permian color:permian
 from: -358.9 till: -298.9 text:Carboniferous color:carboniferous
 from: -419.2 till: -358.9 text:Devonian color:devonian
 from: -443.8 till: -419.2 text:Silurian color:silurian
 from: -485.4 till: -443.8 text:Ordovician color:ordovician
 from: -538.8 till: -485.4 text:[[Cambrian] color:cambrian

</timeline>

<timeline> ImageSize = width:1100 height:100 PlotArea = left:65 right:15 bottom:20 top:5 AlignBars = justify

Colors =

 id:cenozoic value:rgb(0.949,0.976,0.114)
 id:quaternary value:rgb(0.976,0.976,0.498)
 id:holocene value:rgb(0.996,0.922,0.824)
 id:pleistocene value:rgb(1,0.937,0.686)
 id:neogene value:rgb(1,0.902,0.098)
 id:pliocene value:rgb(1,1,0.6)
 id:miocene value:rgb(1,1,0)
 id:paleogene value:rgb(0.992,0.604,0.322)
 id:oligocene value:rgb(0.996,0.753,0.478)
 id:eocene value:rgb(0.992,0.706,0.424)
 id:paleocene value:rgb(0.992,0.655,0.373)
 id:black value:black
 id:white value:white
 id:darkgreen value:rgb(0,0.35,0)

Period = from:-66 till:0 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:10 start:-60 ScaleMinor = unit:year increment:1 start:-65

Define $markred = text:"*" textcolor:red shift:(0,3) fontsize:10 Define $markgreen = text:"*" textcolor:darkgreen shift:(0,3) fontsize:10

PlotData=

 align:center textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
 bar:era
 at:     0  align:right $markgreen 
 at: start  align:left  $markgreen shift:(2,3)
 from:start till:  0    text:Cenozoic color:cenozoic
 bar:period
 at:   0      align:right $markred 
 at:   -2.58 align:left  $markred shift:(2,3)
 from: -2.58 till: 0 text:Quaternary color:quaternary fontsize:6
 from: -23.03 till: -2.58 text:Neogene color:neogene
 from: start  till: -23.03 text:Paleogene color:paleogene
 bar:epoch
 from: -0.0117 till: 0  text:H color:holocene 
 from: -2.58 till: -0.0117 text:Pleistocene color:pleistocene fontsize:5
 from: -5.333 till: -2.58 text:Pliocene color:pliocene fontsize:7
 from: -23.03 till: -5.333 text:Miocene color:miocene
 from: -33.9 till: -23.03 text:Oligocene color:oligocene
 from: -56 till: -33.9 text:Eocene color:eocene
 from: start till: -56 text:Paleocene color:paleocene

</timeline>

<timeline> ImageSize = width:1100 height:100 PlotArea = left:65 right:15 bottom:20 top:5 AlignBars = justify

Colors =

 id:quaternary value:rgb(0.976,0.976,0.498)
 id:holocene value:rgb(0.996,0.922,0.824)
 id:meghalayan value:rgb(0.992,0.929,0.925)
 id:northgrippian value:rgb(0.992,0.925,0.894)
 id:greenlandian value:rgb(0.996,0.925,0.859)
 id:pleistocene value:rgb(1,0.937,0.686)
 id:late value:rgb(1,0.949,0.827)
 id:chibanian value:rgb(1,0.949,0.780)
 id:calabrian value:rgb(1,0.949,0.729)
 id:gelasian value:rgb(1,0.929,0.702)
 id:darkgreen value:rgb(0,0.35,0)

Period = from:-2.58 till:0 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:1 start:-2

Define $markred = text:"*" textcolor:red shift:(0,3) fontsize:10 Define $markgreen = text:"*" textcolor:darkgreen shift:(0,3) fontsize:10

PlotData=

 align:center textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
 bar:period
 at: 0        align:right $markred 
 at: -2.58   align:left $markred shift:(2,3)
 from: -2.58 till: 0 text:Quaternary color:quaternary
 bar:epoch
 at: 0       align:right $markgreen
 at: -0.0117   align:left $markgreen shift:(2,3)
 from: -0.0117 till: 0      text:Holocene color:holocene
 from: -2.58 till: -0.0117 text:Pleistocene color:pleistocene
 bar:age fontsize:8
 from: -0.0042 till: 0      color:meghalayan
 from: -0.0082 till: -0.0042 color:northgrippian
 from: -0.0117 till: -0.0082 color:greenlandian
 from: -0.126 till: -0.0117 text:Late color:late
 from: -0.781 till: -0.126 text:Chibanian color:chibanian
 from: -1.806 till: -0.781 text:Calabrian color:calabrian
 from: -2.58 till: -1.806 text:Gelasian color:gelasian

</timeline>

(Horizontal scale is millions of years for the above timelines; thousands of years for the timeline below)

<timeline> ImageSize = width:1100 height:76 PlotArea = left:65 right:15 bottom:20 top:5 AlignBars = justify

Colors =

 id:holocene value:rgb(0.996,0.922,0.824)
 id:meghalayan value:rgb(0.992,0.929,0.925)
 id:northgrippian value:rgb(0.992,0.925,0.894)
 id:greenlandian value:rgb(0.996,0.925,0.859)
 id:darkgreen value:rgb(0,0.35,0)

Period = from:-11.7 till:0 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:1 start:-11

Define $markred = text:"*" textcolor:red shift:(0,3) fontsize:10 Define $markgreen = text:"*" textcolor:darkgreen shift:(0,3) fontsize:10

PlotData =

 align:center textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
 bar:epoch
 at: 0       align:right $markgreen
 at: -11.7   align:left $markgreen shift:(2,3)
 from: -11.7 till: 0      text:Holocene color:holocene
 bar:age fontsize:8
 from: -4.2 till: 0      text:Meghalayan color:meghalayan
 from: -8.2 till: -4.2 text:Northgrippian color:northgrippian
 from: -11.7 till: -8.2 text:Greenlandian color:greenlandian

</timeline>

Major proposed revisions to the ICC

Proposed Anthropocene Series/Epoch

Script error: No such module "Labelled list hatnote". First suggested in 2000,[65] the Anthropocene is a proposed epoch/series for the most recent time in Earth's history. While still informal, it is a widely used term to denote the present geologic time interval, in which many conditions and processes on Earth are profoundly altered by human impact.[66] The definition of the Anthropocene as a geologic time period rather than a geologic event remains controversial and difficult.[67][68][69][70]

In May 2019 the Anthropocene Working Group voted in favour of submitting a formal proposal to the ICS for the establishment of the Anthropocene Series/Epoch.[71] The formal proposal was completed and submitted to the Subcommission on Quaternary Stratigraphy in late 2023 for a section in Crawford Lake, Ontario, with heightened Plutonium levels corresponding to 1952 CE.[72] This proposal was rejected as a formal geologic epoch in early 2024, to be left instead as an "invaluable descriptor of human impact on the Earth system"[73]

Proposals for revisions to pre-Cryogenian timeline

Shields et al. 2021

The ICS Subcommission for Cryogenian Stratigraphy has outlined a template to improve the pre-Cryogenian geologic time scale based on the rock record to bring it in line with the post-Tonian geologic time scale.[4] This work assessed the geologic history of the currently defined eons and eras of the Precambrian,Template:Efn and the proposals in the "Geological Time Scale" books 2004,[74] 2012,[5] and 2020.[75] Their recommend revisions[4] of the pre-Cryogenian geologic time scale were as below (changes from the current scale [v2023/09] are italicised). This suggestion was unanimously rejected by the International Subcommission for Precambrian Stratigraphy, based on scientific weaknesses.

  • Three divisions of the Archean instead of four by dropping Eoarchean, and revisions to their geochronometric definition, along with the repositioning of the Siderian into the latest Neoarchean, and a potential Kratian division in the Neoarchean.
    • Archean (4000–2450 Ma)
      • Paleoarchean (4000–3500 Ma)
      • Mesoarchean (3500–3000 Ma)
      • Neoarchean (3000–2450 Ma)
        • Kratian (no fixed time given, prior to the Siderian) – from Greek κράτος (krátos) 'strength'.
        • Siderian (?–2450 Ma) – moved from Proterozoic to end of Archean, no start time given, base of Paleoproterozoic defines the end of the Siderian
  • Refinement of geochronometric divisions of the Proterozoic, Paleoproterozoic, repositioning of the Statherian into the Mesoproterozoic, new Skourian period/system in the Paleoproterozoic, new Kleisian or Syndian period/system in the Neoproterozoic.
    • Paleoproterozoic (2450–1800 Ma)
      • Skourian (2450–2300 Ma) – from Greek σκουριά (skouriá) 'rust'.
      • Rhyacian (2300–2050 Ma)
      • Orosirian (2050–1800 Ma)
    • Mesoproterozoic (1800–1000 Ma)
      • Statherian (1800–1600 Ma)
      • Calymmian (1600–1400 Ma)
      • Ectasian (1400–1200 Ma)
      • Stenian (1200–1000 Ma)
    • Neoproterozoic (1000–538.8 Ma)Template:Efn
      • Kleisian or Syndian (1000–800 Ma) – respectively from Greek κλείσιμο (kleísimo) 'closure' and σύνδεση (sýndesi) 'connection'.
      • Tonian (800–720 Ma)
      • Cryogenian (720–635 Ma)
      • Ediacaran (635–538.8 Ma)

Proposed pre-Cambrian timeline (Shield et al. 2021, ICS working group on pre-Cryogenian chronostratigraphy), shown to scale:Template:Efn <timeline> ImageSize = width:1300 height:100 PlotArea = left:80 right:20 bottom:20 top:5 AlignBars = justify Colors =

 id:proterozoic value:rgb(0.968,0.207,0.388)
 id:neoproterozoic value:rgb(0.996,0.701,0.258)
 id:ediacaran value:rgb(0.996,0.85,0.415)
 id:cryogenian value:rgb(0.996,0.8,0.36)
 id:tonian value:rgb(0.996,0.75,0.305)
 id:kleisian value:rgb(0.996,0.773,0.431)
 id:mesoproterozoic value:rgb(0.996,0.705,0.384)
 id:stenian value:rgb(0.996,0.85,0.604)
 id:ectasian value:rgb(0.996,0.8,0.541)
 id:calymmian value:rgb(0.996,0.75,0.478)
 id:paleoproterozoic value:rgb(0.968,0.263,0.44)
 id:skourian value:rgb(0.949,0.439,0.545)
 id:statherian value:rgb(0.968,0.459,0.655)
 id:orosirian value:rgb(0.968,0.408,0.596)
 id:rhyacian value:rgb(0.968,0.357,0.537)
 id:archean value:rgb(0.996,0.157,0.498)
 id:neoarchean value:rgb(0.976,0.608,0.757)
 id:mesoarchean value:rgb(0.968,0.408,0.662)
 id:paleoarchean value:rgb(0.96,0.266,0.624)
 id:hadean value:rgb(0.717,0,0.494)
 id:black value:black
 id:white value:white

Period = from:-4600 till:-538.8 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:500 start:-4500 ScaleMinor = unit:year increment:100 start:-4500 PlotData =

align:center textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
 bar:Eonothem/Eon
   from: -2450 till: -538.8 text:Proterozoic color:proterozoic
   from: -4000 till: -2450 text:Archean color:archean
   from: start till: -4000 text:Hadean color:hadean
 bar:Erathem/Era
   from: -1000 till: -538.8 text:Neoproterozoic color:neoproterozoic
   from: -1800 till: -1000 text:Mesoproterozoic color:mesoproterozoic
   from: -2450 till: -1800 text:Paleoproterozoic color:paleoproterozoic
   from: -3000 till: -2450 text:Neoarchean color:neoarchean
   from: -3300 till: -3000 text:Mesoarchean color:mesoarchean
   from: -4000 till: -3300 text:Paleoarchean color:paleoarchean
   from: start till: -4000 color:white
 bar:System/Period fontsize:7
   from: -635 till: -538.8 text:Ed. color:ediacaran
   from: -720 till: -635 text:Cr. color:cryogenian
   from: -800 till: -720 text:Tonian color:tonian
   from: -1000 till: -800 text:?kleisian color:kleisian
   from: -1200 till: -1000 text:Stenian color:stenian
   from: -1400 till: -1200 text:Ectasian color:ectasian
   from: -1600 till: -1400 text:Calymmian color:calymmian
   from: -1800 till: -1600 text:Statherian color:statherian
   from: -2050 till: -1800 text:Orosirian color:orosirian
   from: -2300 till: -2050 text:Rhyacian color:rhyacian
   from: -2450 till: -2300 text:?Skourian color:skourian
   from: -2700 till: -2450 text:Siderian color:neoarchean
   from: -3000 till: -2700 text:?Kratian color:neoarchean
   from: start till: -3000 color:white

</timeline>

ICC pre-Cambrian timeline (v2024/12, current Template:As of), shown to scale: <timeline> ImageSize = width:1300 height:100 PlotArea = left:80 right:20 bottom:20 top:5 AlignBars = justify Colors =

 id:proterozoic value:rgb(0.968,0.207,0.388)
 id:neoproterozoic value:rgb(0.996,0.701,0.258)
 id:ediacaran value:rgb(0.996,0.85,0.415)
 id:cryogenian value:rgb(0.996,0.8,0.36)
 id:tonian value:rgb(0.996,0.75,0.305)
 id:mesoproterozoic value:rgb(0.996,0.705,0.384)
 id:stenian value:rgb(0.996,0.85,0.604)
 id:ectasian value:rgb(0.996,0.8,0.541)
 id:calymmian value:rgb(0.996,0.75,0.478)
 id:paleoproterozoic value:rgb(0.968,0.263,0.44)
 id:statherian value:rgb(0.968,0.459,0.655)
 id:orosirian value:rgb(0.968,0.408,0.596)
 id:rhyacian value:rgb(0.968,0.357,0.537)
 id:siderian value:rgb(0.968,0.306,0.478)
 id:archean value:rgb(0.996,0.157,0.498)
 id:neoarchean value:rgb(0.976,0.608,0.757)
 id:mesoarchean value:rgb(0.968,0.408,0.662)
 id:paleoarchean value:rgb(0.96,0.266,0.624)
 id:eoarchean value:rgb(0.902,0.114,0.549)
 id:hadean value:rgb(0.717,0,0.494)
 id:black value:black
 id:white value:white

Period = from:-4567 till:-538.8 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:500 start:-4500 ScaleMinor = unit:year increment:100 start:-4500 PlotData =

align:center textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
   bar:Eonothem/Eon
   from: -2500 till: -538.8 text:Proterozoic color:proterozoic
   from: -4031 till: -2500 text:Archean color:archean
   from: start till: -4031 text:Hadean color:hadean
 bar:Erathem/Era
   from: -1000 till: -538.8 text:Neoproterozoic color:neoproterozoic
   from: -1600 till: -1000 text:Mesoproterozoic color:mesoproterozoic
   from: -2500 till: -1600 text:Paleoproterozoic color:paleoproterozoic
   from: -2800 till: -2500 text:Neoarchean color:neoarchean
   from: -3200 till: -2800 text:Mesoarchean color:mesoarchean
   from: -3600 till: -3200 text:Paleoarchean color:paleoarchean
   from: -4031 till: -3600 text:Eoarchean color:eoarchean
   from: start till: -4031 color:white
 bar:Sytem/Period fontsize:7
   from: -635 till: -538.8 text:Ed. color:ediacaran
   from: -720 till: -635 text:Cr. color:cryogenian
   from: -1000 till: -720 text:Tonian color:tonian
   from: -1200 till: -1000 text:Stenian color:stenian
   from: -1400 till: -1200 text:Ectasian color:ectasian
   from: -1600 till: -1400 text:Calymmian color:calymmian
   from: -1800 till: -1600 text:Statherian color:statherian
   from: -2050 till: -1800 text:Orosirian color:orosirian
   from: -2300 till: -2050 text:Rhyacian color:rhyacian
   from: -2500 till: -2300 text:Siderian color:siderian
   from: start till: -2500 color:white

</timeline>

Van Kranendonk et al. 2012 (GTS2012)

The book, Geologic Time Scale 2012, was the last commercial publication of an international chronostratigraphic chart that was closely associated with the ICS and the Subcommission on Precambrian Stratigraphy.[2] It included a proposal to substantially revise the pre-Cryogenian time scale to reflect important events such as the formation of the Solar System and the Great Oxidation Event, among others, while at the same time maintaining most of the previous chronostratigraphic nomenclature for the pertinent time span.[76] Template:As of these proposed changes have not been accepted by the ICS. The proposed changes (changes from the current scale [v2023/09]) are italicised:

  • Hadean Eon (4567–4030 Ma)
  • Archean Eon/Eonothem (4030–2420 Ma)
    • Paleoarchean Era/Erathem (4030–3490 Ma)
    • Mesoarchean Era/Erathem (3490–2780 Ma)
      • Vaalbaran Period/System (3490–3020 Ma) – based on the names of the Kaapvaal (Southern Africa) and Pilbara (Western Australia) cratons, to reflect the growth of stable continental nuclei or proto-cratonic kernels.[62]
      • Pongolan Period/System (3020–2780 Ma) – named after the Pongola Supergroup, in reference to the well preserved evidence of terrestrial microbial communities in those rocks.[62]
    • Neoarchean Era/Erathem (2780–2420 Ma)
  • Proterozoic Eon/Eonothem (2420–538.8 Ma)Template:Efn
    • Paleoproterozoic Era/Erathem (2420–1780 Ma)
      • Oxygenian Period/System (2420–2250 Ma) – named for displaying the first evidence for a global oxidising atmosphere.[62]
      • Jatulian or Eukaryian Period/System (2250–2060 Ma) – names are respectively for the Lomagundi–Jatuli δ13C isotopic excursion event spanning its duration, and for the (proposed)[79][80] first fossil appearance of eukaryotes.[62]
      • Columbian Period/System (2060–1780 Ma) – named after the supercontinent Columbia.[62]
    • Mesoproterozoic Era/Erathem (1780–850 Ma)
      • Rodinian Period/System (1780–850 Ma) – named after the supercontinent Rodinia, stable environment.[62]

Proposed pre-Cambrian timeline (GTS2012), shown to scale: <timeline> ImageSize = width:1200 height:100 PlotArea = left:80 right:20 bottom:20 top:5 AlignBars = justify Colors =

 id:proterozoic value:rgb(0.968,0.207,0.388)
 id:neoproterozoic value:rgb(0.996,0.701,0.258)
 id:ediacaran value:rgb(0.996,0.85,0.415)
 id:cryogenian value:rgb(0.996,0.8,0.36)
 id:tonian value:rgb(0.996,0.75,0.305)
 id:mesoproterozoic value:rgb(0.996,0.705,0.384)
 id:rodinian value:rgb(0.996,0.75,0.478)
 id:paleoproterozoic value:rgb(0.968,0.263,0.44)
 id:columbian value:rgb(0.968,0.459,0.655)
 id:eukaryian value:rgb(0.968,0.408,0.596)
 id:oxygenian value:rgb(0.968,0.357,0.537)
 id:archean value:rgb(0.996,0.157,0.498)
 id:neoarchean value:rgb(0.976,0.608,0.757)
 id:siderian value:rgb(0.976,0.7,0.85)
 id:methanian value:rgb(0.976,0.65,0.8)
 id:mesoarchean value:rgb(0.968,0.408,0.662)
 id:pongolan value:rgb(0.968,0.5,0.75)
 id:vaalbaran value:rgb(0.968,0.45,0.7)
 id:paleoarchean value:rgb(0.96,0.266,0.624)
 id:isuan value:rgb(0.96,0.35,0.65)
 id:acastan value:rgb(0.96,0.3,0.6)
 id:hadean value:rgb(0.717,0,0.494)
 id:zirconian value:rgb(0.902,0.114,0.549)
 id:chaotian value:rgb(0.8,0.05,0.5)
 id:black value:black
 id:white value:white

Period = from:-4567.3 till:-538.8 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:500 start:-4500 ScaleMinor = unit:year increment:100 start:-4500 PlotData =

align:center textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
 bar:Eonothem/Eon
   from: -2420 till: -541 text:Proterozoic color:proterozoic
   from: -4030 till: -2420 text:Archean color:archean
   from: -4567 till: -4030 text:Hadean color:hadean
   from: start till: -4567 color:white
 bar:Erathem/Era
   from: -850 till: -541 text:Neoproterozoic color:neoproterozoic
   from: -1780 till: -850 text:Mesoproterozoic color:mesoproterozoic
   from: -2420 till: -1780 text:Paleoproterozoic color:paleoproterozoic
   from: -2780 till: -2420 text:Neoarchean color:neoarchean
   from: -3490 till: -2780 text:Mesoarchean color:mesoarchean
   from: -4030 till: -3490 text:Paleoarchean color:paleoarchean
   from: -4404 till: -4030 text:Zirconian color:zirconian
   from: -4567 till: -4404 text:Chaotian color:chaotian
   from: start till: -4567 color:white
 bar:System/Period fontsize:7
   from: -630  till: -541 text:Ediacaran color:ediacaran
   from: -850  till: -630 text:Cryogenian color:cryogenian
   from: -1780 till: -850  text:Rodinian color:rodinian
   from: -2060 till: -1780 text:Columbian color:columbian
   from: -2250 till: -2060 text:Eukaryian color:eukaryian
   from: -2420 till: -2250 text:Oxygenian color:oxygenian
   from: -2630 till: -2420 text:Siderian color:siderian
   from: -2780 till: -2630 text:Methanian color:methanian
   from: -3020 till: -2780 text:Pongolan color:pongolan
   from: -3490 till: -3020 text:Vaalbaran color:vaalbaran
   from: -3810 till: -3490 text:Isuan color:isuan
   from: -4030 till: -3810 text:Acastan color:acastan
   from: start till: -4030 color:white

</timeline>

ICC pre-Cambrian timeline (v2024/12, current Template:As of), shown to scale: <timeline> ImageSize = width:1200 height:100 PlotArea = left:80 right:20 bottom:20 top:5 AlignBars = justify Colors =

 id:proterozoic value:rgb(0.968,0.207,0.388)
 id:neoproterozoic value:rgb(0.996,0.701,0.258)
 id:ediacaran value:rgb(0.996,0.85,0.415)
 id:cryogenian value:rgb(0.996,0.8,0.36)
 id:tonian value:rgb(0.996,0.75,0.305)
 id:mesoproterozoic value:rgb(0.996,0.705,0.384)
 id:stenian value:rgb(0.996,0.85,0.604)
 id:ectasian value:rgb(0.996,0.8,0.541)
 id:calymmian value:rgb(0.996,0.75,0.478)
 id:paleoproterozoic value:rgb(0.968,0.263,0.44)
 id:statherian value:rgb(0.968,0.459,0.655)
 id:orosirian value:rgb(0.968,0.408,0.596)
 id:rhyacian value:rgb(0.968,0.357,0.537)
 id:siderian value:rgb(0.968,0.306,0.478)
 id:archean value:rgb(0.996,0.157,0.498)
 id:neoarchean value:rgb(0.976,0.608,0.757)
 id:mesoarchean value:rgb(0.968,0.408,0.662)
 id:paleoarchean value:rgb(0.96,0.266,0.624)
 id:eoarchean value:rgb(0.902,0.114,0.549)
 id:hadean value:rgb(0.717,0,0.494)
 id:black value:black
 id:white value:white

Period = from:-4567.3 till:-538.8 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:500 start:-4500 ScaleMinor = unit:year increment:100 start:-4500 PlotData =

align:center textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
 bar:Eonothem/Eon
   from: -2500 till: -538.8 text:Proterozoic color:proterozoic
   from: -4031 till: -2500 text:Archean color:archean
   from: start till: -4031 text:Hadean color:hadean
 bar:Erathem/Era
   from: -1000 till: -538.8 text:Neoproterozoic color:neoproterozoic
   from: -1600 till: -1000 text:Mesoproterozoic color:mesoproterozoic
   from: -2500 till: -1600 text:Paleoproterozoic color:paleoproterozoic
   from: -2800 till: -2500 text:Neoarchean color:neoarchean
   from: -3200 till: -2800 text:Mesoarchean color:mesoarchean
   from: -3600 till: -3200 text:Paleoarchean color:paleoarchean
   from: -4031 till: -3600 text:Eoarchean color:eoarchean
   from: start till: -4031 color:white
 bar:System/Period fontsize:7
   from: -635 till: -538.8 text:Ediacaran color:ediacaran
   from: -720 till: -635 text:Cryogenian color:cryogenian
   from: -1000 till: -720 text:Tonian color:tonian
   from: -1200 till: -1000 text:Stenian color:stenian
   from: -1400 till: -1200 text:Ectasian color:ectasian
   from: -1600 till: -1400 text:Calymmian color:calymmian
   from: -1800 till: -1600 text:Statherian color:statherian
   from: -2050 till: -1800 text:Orosirian color:orosirian
   from: -2300 till: -2050 text:Rhyacian color:rhyacian
   from: -2500 till: -2300 text:Siderian color:siderian
   from: start till: -2500 color:white

</timeline>

Table of geologic time

Template:More citations needed section The following table summarises the major events and characteristics of the divisions making up the geologic time scale of Earth. This table is arranged with the most recent geologic periods at the top, and the oldest at the bottom. The height of each table entry does not correspond to the duration of each subdivision of time. As such, this table is not to scale and does not accurately represent the relative time-spans of each geochronologic unit. While the Phanerozoic Eon looks longer than the rest, it merely spans ~538.8 Ma (~11.8% of Earth's history), whilst the previous three eonsTemplate:Efn collectively span ~4,028.2 Ma (~88.2% of Earth's history). This bias toward the most recent eon is in part due to the relative lack of information about events that occurred during the first three eons compared to the current eon (the Phanerozoic).[4][81] The use of subseries/subepochs has been ratified by the ICS.[15]

While some regional terms are still in use,[5] the table of geologic time conforms to the nomenclature, ages, and colour codes set forth by the International Commission on Stratigraphy in the official International Chronostratigraphic Chart.[1][82] The International Commission on Stratigraphy also provide an online interactive version of this chart. The interactive version is based on a service delivering a machine-readable Resource Description Framework/Web Ontology Language representation of the time scale, which is available through the Commission for the Management and Application of Geoscience Information GeoSciML project as a service[83] and at a SPARQL end-point.[84][85]

Template:Sticky header

Extraterrestrial geologic time scales

Script error: No such module "Labelled list hatnote".Some other planets and satellites in the Solar System have sufficiently rigid structures to have preserved records of their own histories, for example, Venus, Mars and the Earth's Moon. Dominantly fluid planets, such as the giant planets, do not comparably preserve their history. Apart from the Late Heavy Bombardment, events on other planets probably had little direct influence on the Earth, and events on Earth had correspondingly little effect on those planets. Construction of a time scale that links the planets is, therefore, of only limited relevance to the Earth's time scale, except in a Solar System context. The existence, timing, and terrestrial effects of the Late Heavy Bombardment are still a matter of debate.Template:Efn

Lunar (selenological) time scale

The geologic history of Earth's Moon has been divided into a time scale based on geomorphological markers, namely impact cratering, volcanism, and erosion. This process of dividing the Moon's history in this manner means that the time scale boundaries do not imply fundamental changes in geological processes, unlike Earth's geologic time scale. Five geologic systems/periods (Pre-Nectarian, Nectarian, Imbrian, Eratosthenian, Copernican), with the Imbrian divided into two series/epochs (Early and Late) were defined in the latest Lunar geologic time scale.[127] The Moon is unique in the Solar System in that it is the only other body from which humans have rock samples with a known geological context. Template:Timeline Lunar Geological Timescale

Martian geologic time scale

The geological history of Mars has been divided into two alternate time scales. The first time scale for Mars was developed by studying the impact crater densities on the Martian surface. Through this method four periods have been defined, the Pre-Noachian (~4,500–4,100 Ma), Noachian (~4,100–3,700 Ma), Hesperian (~3,700–3,000 Ma), and Amazonian (~3,000 Ma to present).[128][129] Template:Mars timescale A second time scale based on mineral alteration observed by the OMEGA spectrometer on board the Mars Express. Using this method, three periods were defined, the Phyllocian (~4,500–4,000 Ma), Theiikian (~4,000–3,500 Ma), and Siderikian (~3,500 Ma to present).[130] <timeline> ImageSize = width:800 height:50 PlotArea = left:15 right:15 bottom:20 top:5 AlignBars = early

Period = from:-4500 till:0 TimeAxis = orientation:horizontal ScaleMajor = unit:year increment:500 start:-4500 ScaleMinor = unit:year increment:100 start:-4500

Colors =

 id:sidericol  value:rgb(1,0.4,0.3)
 id:theiicol value:rgb(1,0.2,0.5)
 id:phyllocol  value:rgb(0.7,0.4,1)

PlotData=

align:center  textcolor:black fontsize:8 mark:(line,black) width:25 shift:(0,-5)
text:Siderikan  from:-3500  till:0 color:sidericol
text:Theiikian from:-4000 till:-3500  color:theiicol
text:Phyllocian from:start till:-4000  color:phyllocol

</timeline>

See also

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Template:Div col end

Notes

Template:Notelist

References

Template:Reflist

Further reading

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  • Montenari, Michael (2022). Integrated Quaternary Stratigraphy (1st ed.). Amsterdam: Academic Press (Elsevier). ISBN 978-0-323-98913-8.
  • Montenari, Michael (2023). Stratigraphy of Geo- and Biodynamic Processes (1st ed.). Amsterdam: Academic Press (Elsevier). ISBN 978-0-323-99242-8.
  • Nichols, Gary (2013). Sedimentology and Stratigraphy (2nd ed.). Hoboken: Wiley-Blackwell. Template:ISBN
  • Williams, Aiden (2019). Sedimentology and Stratigraphy (1st ed.). Forest Hills, NY: Callisto Reference. Template:ISBN

External links

Template:Sister project Template:Sister project

Template:Geological history Template:Navboxes Template:Authority control

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