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The geologic time scale or geological time scale ( GTS) is a representation of based on the of . It is a system of chronological dating that uses chronostratigraphy (the process of relating to time) and (a scientific branch of that aims to determine the age of rocks). It is used primarily by (including , , , , and ) 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 , properties, and . 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 is to precisely define global chronostratigraphic units of the International Chronostratigraphic Chart (ICC) that are used to define divisions of geological time. The chronostratigraphic divisions are in turn used to define geochronologic units.


Principles
The geologic time scale is a way of representing based on events that have occurred through Earth's history, a time span of about 4.54 ± 0.05 billion years. 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 System/Period and thus the boundary between the and Paleogene systems/periods. For divisions prior to the , 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.

Historically, regional geologic time scales were used 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.

(2025). 9780321745767, Prentice Hall.

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. 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. However, it is now known that not all sedimentary layers are deposited purely horizontally, 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. 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.

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.

The relationships of 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. 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. This allows for a correlation of strata even when the horizon between them is not continuous.


Divisions of geologic time
The geologic time scale is divided into chronostratigraphic units and their corresponding geochronologic units.

  • An is the largest geochronologic time unit and is equivalent to a chronostratigraphic .
    (2025). 9780191874901 .
    There are four formally defined eons: the , , and .
  • An is the second largest geochronologic time unit and is equivalent to a chronostratigraphic . There are ten defined eras: the , , , , , , , , and , with none from the Hadean eon.
  • A is equivalent to a chronostratigraphic system. There are 22 defined periods, with the current being the period. As an exception, two subperiods are used for the .
  • An is the second smallest geochronologic unit. It is equivalent to a chronostratigraphic series. There are 37 defined epochs and one informal one. The current epoch is the . There are also 11 subepochs which are all within the and Quaternary. The use of subepochs as formal units in international chronostratigraphy was ratified in 2022.
  • An is the smallest hierarchical geochronologic unit. It is equivalent to a chronostratigraphic stage. There are 96 formal and five informal ages. The current age is the .
  • A is a non-hierarchical formal geochronology unit of unspecified rank and is equivalent to a chronostratigraphic . These correlate with magnetostratigraphic, lithostratigraphic, or units as they are based on previously defined stratigraphic units or geologic features.

+Formal, hierarchical units of the geologic time scale (largest to smallest) !Chronostratigraphic unit (strata) !Geochronologic unit (time) !Time span
EonothemEonSeveral hundred million years to two billion years
ErathemEraTens to hundreds of millions of years
SystemPeriodMillions of years to tens of millions of years
SeriesEpochHundreds of thousands of years to tens of millions of years
SubseriesSubepochThousands of years to millions of years
StageAgeThousands of years to millions of years

The subdivisions and are used as the geochronologic equivalents of the chronostratigraphic and , e.g., Early 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 System the Silurian System and they were deposited 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 and 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
is the element of [[stratigraphy]] that deals with the relation between rock bodies and the relative measurement of geological time. It is the process where distinct strata between defined stratigraphic horizons are assigned to represent a relative interval of geologic time.
     

A 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.

A is a subdivision of geologic time. It is a numeric representation of an intangible property (time). These units are arranged in a hierarchy: eon, era, period, epoch, subepoch, age, and subage.

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).
is the field of geochronology that numerically quantifies geologic time.
     

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

A (GSSA) is a numeric-only, chronologic reference point used to define the base of geochronologic units prior to the Cryogenian. These points are arbitrarily defined. 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, for 'million '). For example, Ma, the lower boundary of the Period, is defined as 201,400,000 years old with an uncertainty of 200,000 years. Other units commonly used by geologists are (gigaannum, billion years), and (kiloannum, thousand years), with the latter often represented in calibrated units ().


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 becomes the Phanerozoic Eon). Names of erathems in the Phanerozoic were chosen to reflect major changes in the history of life on Earth: (old life), (middle life), and (new life). Names of systems are diverse in origin, with some indicating chronologic position (e.g., Paleogene), while others are named for (e.g., Cretaceous), (e.g., ), or are tribal (e.g., ) 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 or type locality. The name of stages should also be derived from a geographic feature in the locality of its stratotype or type locality.

Informally, the time before the Cambrian is often referred to as the or pre-Cambrian (Supereon).

+Time span and of geologic eonothem/eon names !Name !Time span !Duration (million years) !Etymology of name
From Greek φανερός ( phanerós) 'visible' or 'abundant' and ζωή ( zoē) 'life'.
From Greek πρότερος ( próteros) 'former' or 'earlier' and ζωή ( zoē) 'life'.
From Greek ἀρχή ( archē) 'beginning, origin'.
From , , 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
From Greek καινός ( kainós) 'new' and ζωή ( zōḗ) 'life'.
From Greek μέσο ( méso) 'middle' and ζωή ( zōḗ) 'life'.
From Greek παλιός ( palaiós) 'old' and ζωή ( zōḗ) 'life'.
From Greek νέος ( néos) 'new' or 'young', πρότερος ( próteros) 'former' or 'earlier', and ζωή ( zōḗ) 'life'.
From Greek μέσο ( méso) 'middle', πρότερος ( próteros) 'former' or 'earlier', and ζωή ( zōḗ) 'life'.
From Greek παλιός ( palaiós) 'old', πρότερος ( próteros) 'former' or 'earlier', and ζωή ( zōḗ) 'life'.
From Greek νέος ( néos) 'new' or 'young' and ἀρχαῖος ( arkhaîos) 'ancient'.
From Greek μέσο ( méso) 'middle' and ἀρχαῖος ( arkhaîos) 'ancient'.
From Greek παλιός ( palaiós) 'old' and ἀρχαῖος ( arkhaîos) 'ancient'.
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
First introduced by in 1829 for sediments in 's Basin that appeared to be younger than Tertiary rocks. 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.)
Derived from Greek νέος ( néos) 'new' and γενεά ( geneá) 'genesis' or 'birth'.
Derived from Greek παλιός ( palaiós) 'old' and γενεά ( geneá) 'genesis' or 'birth'.
~~Derived from Terrain Crétacé used in 1822 by Jean d'Omalius d'Halloy in reference to extensive beds of within the . From page 373: "La troisième, qui correspond à ce qu'on a déja appelé formation de la craie, sera désigné par le nom de terrain crétacé." (The third, which corresponds to what was already called the "chalk formation", will be designated by the name "chalky terrain".) Ultimately derived from crēta 'chalk'.
~Named after the . Originally used by Alexander von Humboldt as 'Jura Kalkstein' (Jura limestone) in 1799. Alexandre Brongniart was the first to publish the term Jurassic in 1829.
From the Trias of Friedrich August von Alberti in reference to a trio of formations widespread in southern .
Named after the historical region of , .
Means 'coal-bearing', from the carbō ( coal) and ferō ( to bear, carry).
Named after , England.
Named after the tribe, the .
Named after the Celtic tribe, .
Named for , a form of the Welsh name for , Cymru.
~Named for the . Ediacara is possibly a corruption of 'Yata Takarra' 'hard or stony ground'.
~From Greek κρύος ( krýos) 'cold' and γένεσις ( génesis) 'birth'.
~From Greek τόνος ( tónos) 'stretch'.
From Greek στενός ( stenós) 'narrow'.
From Greek ἔκτᾰσῐς ( éktasis) 'extension'.
From Greek κάλυμμᾰ ( kálumma) 'cover'.
From Greek σταθερός ( statherós) 'stable'.
From Greek ὀροσειρά ( oroseirá) 'mountain range'.
From Greek ῥύαξ ( rhýax) 'stream of lava'.
From Greek σίδηρος ( sídēros) ''.
+Time span and etymology of geologic series/epoch names !Name !Time span !Duration (million years) !Etymology of name
From Greek ὅλος ( hólos) 'whole' and καινός ( kainós) 'new'
Coined in the early 1830s from Greek πλεῖστος ( pleîstos) 'most' and καινός ( kainós) 'new'
Coined in the early 1830s from Greek πλείων ( pleíōn) 'more' and καινός ( kainós) 'new'
Coined in the early 1830s from Greek μείων ( meíōn) 'less' and καινός ( kainós) 'new'
Coined in the 1850s from Greek ὀλίγος ( olígos) 'few' and καινός ( kainós) 'new'
Coined in the early 1830s from Greek ἠώς ( ēōs) 'dawn' and καινός ( kainós) 'new', referring to the dawn of modern life during this epoch
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'
See

See

See

Named for , China, an anglicization of Mandarin 乐平 ( lèpíng) 'peaceful music'
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
From Latin cis- (before) + Russian Урал ( Ural), referring to the western slopes of the
Upper Pennsylvanian Named for the US state of , from + Latin silvanus (forest) + -ia by analogy to Transylvania
Middle Pennsylvanian
Lower Pennsylvanian
Upper Mississippian Named for the Mississippi River, from Ojibwe ᒥᐦᓯᓰᐱ ( misi-ziibi) 'great river'
Middle Mississippian
Lower Mississippian
See
Named for the Homolka a Přídolí nature reserve near , Czechia
Named after , England
Named for the in , England
Named after , Wales
See
Middle Ordovician
From Mandarin 芙蓉 ( fúróng) 'lotus', referring to the state symbol of
Named for the mountains of , Mandarin for 'sprouting peaks'
Cambrian Series 2 (informal) See
Named for Terre-Neuve, a French of Newfoundland


History of the geologic time scale

Early history
The most modern geological time scale was not formulated until 1911 by (1890 – 1965), who drew inspiration from (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. The broader concept of the relation between rocks and time can be traced back to (at least) the of from 1200 BC to 600 AD. (c. 570–487 ) 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. This view was shared by a few of Xenophanes's scholars and those that followed, including (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 was also recognized by Chinese naturalist
(1995). 9780860784920, Variorum. .
(1031–1095) and -philosophers, notably the Brothers of Purity, who wrote on the processes of stratification over the passage of time in their treatises. Their work likely inspired that of the 11th-century (Ibn Sînâ, 980–1037) who wrote in The Book of Healing (1027) on the concept of stratification and superposition, pre-dating by more than six centuries. Avicenna also recognized fossils as "petrifications of the bodies of plants and animals",
(2025). 048626372X, Williams & Wilkins. . 048626372X
with the 13th-century (c. 1200–1280), who drew from natural philosophy, extending this into a theory of a petrifying fluid. These works appeared to have little influence on in who looked to the to explain the origins of fossils and sea-level changes, often attributing these to the 'Deluge', including Ristoro d'Arezzo in 1282. 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':

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 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. 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." Later, in the 19th century, academics further developed theories on stratification. William Smith, often referred to as the "Father of Geology" 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”. 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. 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."


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. In De solido intra solidum naturaliter contento dissertationis prodromus Steno states:
  • 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 ). While Steno's principles were simple and attracted much attention, applying them proved challenging. 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". (1687–1784) also used primary and secondary divisions for rock units but his mechanism was volcanic. In this early version of the 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. 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 (1726–1797), in particular his Theory of the Earth, first presented before the Royal Society of Edinburgh in 1785. Hutton's theory would later become known as uniformitarianism, popularised by (1748–1819) and later (1797–1875) in his Principles of Geology. Their theories strongly contested the 6,000 year age of the Earth as suggested determined by 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, , 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
During the 19th century, the debate regarding Earth's age was renewed, with geologists estimating ages based on rates and sedimentary thicknesses or ocean chemistry, and physicists determining ages for the cooling of the Earth or the Sun using basic or orbital physics. 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 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 , , and 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. Early attempts at determining ages of uranium minerals and rocks by Ernest Rutherford, , Robert Strutt, and Arthur Holmes, would culminate in what are considered the first international geological time scales by Holmes in 1911 and 1913. The discovery of in 1913 by , 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.


Modern international geological time scale
The establishment of the IUGS in 1961 and acceptance of the Commission on Stratigraphy (applied in 1965)
(1986). 9783924500191, Herausgegeben von der Senckenbergischen Naturforschenden Gesellschaft. .
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".

Following on from Holmes, several A Geological Time Scale books were published in 1982,

(1982). 9780521247283, Cambridge University Press. .
1989,
(1990). 9780521383615, Cambridge University Press. .
2004,
(2025). 9780511082016, Cambridge University Press. .
2008, 2012,
(2025). 9780444594488, Elsevier. .
2016,
(2025). 9780444594686, Elsevier. .
and 2020.
(2025). 9780128243619 .
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. Subsequent Geologic Time Scale books (2016 and 2020) 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.


Major proposed revisions to the ICC

Proposed Anthropocene Series/Epoch
First suggested in 2000, 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. 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. Nevertheless, the definition of the Anthropocene as a geologic time period rather than a geologic event remains controversial and difficult.


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. This work assessed the geologic history of the currently defined eons and eras of the Precambrian, and the proposals in the "Geological Time Scale" books 2004, 2012, and 2020. Their recommend revisions 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)
      • 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: 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
     

ICC pre-Cambrian timeline (v2024/12, current ), shown to scale: 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
     


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. 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.
(2025). 9780444594259, Elsevier.
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)
    • Chaotian Era/Erathem ( 4567–4404 Ma) – the name alluding both to the mythological Chaos and the chaotic phase of .
    • 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, .
  • Archean Eon/Eonothem ( 4030–2420 Ma)
    • Paleoarchean Era/Erathem ( 4030–3490 Ma)
      • Acastan Period/System ( 4030–3810 Ma) – named after the , one of the oldest preserved pieces of continental crust.
      • Isuan Period/System ( 3810–3490 Ma) – named after the Isua Greenstone Belt.
    • Mesoarchean Era/Erathem ( 3490–2780 Ma)
      • Vaalbaran Period/System ( 3490–3020 Ma) – based on the names of the (Southern Africa) and (Western Australia) , to reflect the growth of stable continental nuclei or proto- kernels.
      • 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.
    • Neoarchean Era/Erathem ( 2780–2420 Ma)
      • Methanian Period/System ( 2780–2630 Ma) – named for the inferred predominance of
      • Siderian Period/System ( 2630–2420 Ma) – named for the voluminous banded iron formations formed within its duration.
  • Proterozoic Eon/Eonothem ( 2420–538.8 Ma)
    • Paleoproterozoic Era/Erathem ( 2420–1780 Ma)
      • Oxygenian Period/System ( 2420–2250 Ma) – named for displaying the first evidence for a global oxidising atmosphere.
      • 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) first fossil appearance of .
      • Columbian Period/System ( 2060–1780 Ma) – named after the Columbia.
    • Mesoproterozoic Era/Erathem ( 1780–850 Ma)
      • Rodinian Period/System ( 1780–850 Ma) – named after the supercontinent , stable environment.

Proposed pre-Cambrian timeline (GTS2012), shown to scale: 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
     

ICC pre-Cambrian timeline (v2024/12, current ), shown to scale: 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
     


Table of geologic time
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 Eon looks longer than the rest, it merely spans ~538.8 million years (~11.8% of Earth's history), whilst the previous three eons collectively span ~4,028.2 million years (~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). The use of subseries/subepochs has been ratified by the ICS.

While some regional terms are still in use, the table of geologic time conforms to the , ages, and colour codes set forth by the International Commission on Stratigraphy in the official International Chronostratigraphic Chart. 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 project as a service and at a end-point.


4.2-kiloyear event, Austronesian expansion, increasing industrial CO2.*
8.2-kiloyear event, Holocene climatic optimum. flooding of and . becomes a desert. End of Stone Age and start of . Humans finally expand into the Arctic Archipelago and .*
Climate stabilises. Current and Holocene extinction begins. Agriculture begins. Humans spread across the and , the , and the Americas (mainland and the ).*
('') , last glacial period, ending with . Toba eruption. Pleistocene megafauna (including the last terror birds) extinction. Humans expand into and the .
Mid-Pleistocene Transition occurs, high amplitude 100 ka . Rise of .*
CalabrianFurther cooling of the climate. Giant go extinct. Spread of across .*
Start of Quaternary glaciations and unstable climate. Rise of the Pleistocene megafauna and .*
Greenland ice sheet develops as the cold slowly intensifies towards the Pleistocene. Atmospheric and content reaches present-day levels while landmasses also reach their current locations (e.g. the Isthmus of Panama joins the and , while allowing a faunal interchange). The last non-marsupial metatherians go extinct. common in East Africa; begins.*
of the Mediterranean Basin. Cooling climate continues from the Miocene. First equines and . in Africa.*
with hypersaline lakes in empty Mediterranean Basin. Sahara desert formation begins. Moderate icehouse climate, punctuated by and re-establishment of East Antarctic Ice Sheet. , the last non-crocodilian and go extinct. After separating from gorilla ancestors, chimpanzee and human ancestors gradually separate; and in Africa.*
*
Middle Miocene climate optimum temporarily provides a warm climate. Extinctions in middle Miocene disruption, decreasing shark diversity. First . Ancestor of .*
*
in Northern Hemisphere. Start of forming Southern Alps in New Zealand. Widespread forests slowly massive amounts of , gradually lowering the level of atmospheric from 650 down to around 100 ppmv during the Miocene. Modern and mammal families become recognizable. The last of the primitive whales go extinct. become ubiquitous. Ancestor of , including humans. Afro-Arabia collides with Eurasia, fully forming the and closing the Tethys Ocean, while allowing a faunal interchange. At the same time, Afro-Arabia splits into and .
*
Grande Coupure extinction. Start of widespread Antarctic glaciation. Rapid and diversification of fauna, especially (e.g. first and ). Major evolution and dispersal of modern types of . , miacoids and condylarths go extinct. First (modern, fully aquatic whales) appear.*
*
Moderate, cooling climate. Archaic (e.g. , , "" etc.) flourish and continue to develop during the epoch. Appearance of several "modern" mammal families. and diversify after returning to water. continue to diversify. First , , and . The multituberculates and leptictidans go extinct by the end of the epoch. Reglaciation of Antarctica and formation of its ; End of and of the in North America. begins in Greece and .*
*
Two transient events of global warming (PETM and ETM-2) and warming climate until the Eocene Climatic Optimum. The decreased levels from 3500 ppm to 650 ppm, setting the stage for a long period of cooling. Greater India collides with Eurasia and starts Himalayan Orogeny (allowing a biotic interchange) while Eurasia completely separates from North America, creating the North Atlantic Ocean. Maritime Southeast Asia diverges from the rest of Eurasia. First , , , and true .*
Starts with and the K–Pg extinction event, wiping out all non-avian dinosaurs and pterosaurs, most marine reptiles, many other vertebrates (e.g. many Laurasian metatherians), most cephalopods (only and survived) and many other invertebrates. Climate tropical. and (avians) diversify rapidly into a number of lineages following the extinction event (while the marine revolution stops). Multituberculates and the first widespread. First large birds (e.g. and ) and mammals (up to bear or small hippo size). in Europe and Asia begins. First and (stem primates) appear. migrate to Australia.*
*
*
proliferate (after developing many features since the Carboniferous), along with new types of , while other seed plants (gymnosperms and seed ferns) decline. More modern fish begin to appear. , , , and all common. Many new types of (e.g. , , , and ) evolve on land, while appear in water and probably cause the last temnospondyls to die out; and and modern types of sharks appear in the sea. The revolution started by marine reptiles and sharks reaches its peak, though ichthyosaurs vanish a few million years after being heavily reduced at the . Toothed and coexist with pterosaurs. Modern , (including , who migrate to South America) and (including , and ) mammals appear while the last non-mammalian cynodonts die out. First . Many snails become terrestrial. Further breakup of Gondwana creates , , , , , Greater India, and the , and and the islands of the Indian (and some of the Atlantic) Ocean. Beginning of and of the . Atmospheric oxygen and carbon dioxide levels similar to present day. disappear. Climate initially warm, but later it cools.*
*
*
*
*
*
~ *
~
~ *
~ *
~ *
~
Climate becomes humid again. (especially , and ) and common. , including , , and , become the dominant land vertebrates. Mammals diversify into , , , , , and but mostly remain small. First , and . First , , , and . ichthyosaurs and diverse. Rhynchocephalians throughout the world. , and abundant. very common, along with , , , and and . Breakup of into and , with the latter also breaking into two main parts; the and form. forms. in North America. Rangitata and Cimmerian orogenies taper off. Atmospheric levels 3–4 times the present-day levels (1200–1500 ppmv, compared to today's 400 ppmv). (last pseudosuchians) seek out an aquatic lifestyle. Mesozoic marine revolution continues from late Triassic. disappear.
*
*
*
*
*
*
*
*
dominant on land as and in the air as . also arise from bipedal archosaurs. and (a group of sauropterygians) dominate large marine fauna. become smaller and nocturnal, eventually becoming the first true , while other remaining synapsids die out. (archosaur relatives) also common. called remained common in Gondwana, before being replaced by advanced gymnosperms. Many large aquatic amphibians. extremely common. and fish appear, as do many modern orders and suborders. First . 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 Ma). Carnian pluvial event occurs around 234–232 Ma, allowing the first dinosaurs and (including ) to radiate. Triassic–Jurassic extinction event occurs 201 Ma, wiping out all and the , many marine reptiles (e.g. all sauropterygians except and all ichthyosaurs except ), all except crocodylomorphs, pterosaurs, and dinosaurs, and many ammonoids (including the whole ), bivalves, brachiopods, corals and sponges. First .~
~
~ *
~ *
*
unite into , creating the , and Appalachians, among other mountain ranges (the superocean or Proto-Pacific also forms). End of Permo-Carboniferous glaciation. Hot and dry climate. A possible drop in oxygen levels. ( and ) become widespread and dominant, while and remain common, with the latter probably giving rise to in this period. In the mid-Permian, lycophytes are heavily replaced by ferns and seed plants. and evolve. The very large arthropods and non-tetrapod tetrapodomorphs go extinct. Marine life flourishes in warm shallow reefs; and brachiopods, bivalves, , ammonoids (including goniatites), and all abundant. arise from earlier diapsids, and split into the ancestors of lepidosaurs, , , , , ichthyosaurs, , and . Cynodonts evolve from larger therapsids. Olson's Extinction (273 Ma), End-Capitanian extinction (260 Ma), and Permian–Triassic extinction event (252 Ma) occur one after another: more than 80% of life on Earth becomes extinct in the lattermost, including most plankton, corals ( and die out fully), brachiopods, bryozoans, gastropods, ammonoids (the goniatites die off fully), insects, parareptiles, synapsids, amphibians, and crinoids (only articulates survived), and all , , , , , and . and Innuitian orogenies in North America. in Europe/Asia tapers off. orogeny in Asia. Hunter-Bowen Orogeny on Australian continent begins (c. 260–225 Ma), forming the New England Fold Belt.*
*
*
*
*
*
*
*

Pennsylvanian
radiate suddenly; some (esp. and Palaeodictyoptera) of them as well as some and become very large. First forests (, ferns, , , , etc.). Higher atmospheric levels. Ice Age continues to the Early Permian. , brachiopods, bryozoa, bivalves, and corals plentiful in the seas and oceans. First . Testate proliferate. collides with and Siberia-Kazakhstania, the latter of which forms and the . Variscan orogeny continues (these collisions created orogenies, and ultimately ). (e.g. temnospondyls) spread in Euramerica, with some becoming the first . Carboniferous Rainforest Collapse occurs, initiating a dry climate which favors amniotes over amphibians. Amniotes diversify rapidly into , , , and . remained common before they died out by the end of the period. First .
Moscovian
*
Mississippian
Large flourish and amphibious live amid -forming coastal , radiating significantly one last time. First . First , , , and insects and first . First five-digited (amphibians) and . In the oceans, and are dominant and diverse; (especially and ) abundant. , , , and brachiopods (, , etc.) recover and become very common again, but and decline. Glaciation in East continues from Late Devonian. Tuhua Orogeny in New Zealand tapers off. Some lobe finned fish called rhizodonts become abundant and dominant in freshwaters. Siberia collides with a different small continent, .
Viséan*
*
First , , (, from earlier ), first trees (the progymnosperm ), and first (palaeoptera and neoptera). and , and corals, and are all abundant in the oceans. First fully coiled cephalopods ( and , independently) with the former group very abundant (especially ). Trilobites and ostracoderms decline, while jawed fishes (, and , and and early ) proliferate. Some transform into digited , slowly becoming amphibious. The last non-trilobite artiopods die off. First (like ) and . Pressure from jawed fishes cause eurypterids to decline and to lose their shells while anomalocarids vanish. "Old Red Continent" of persists after forming in the Caledonian orogeny. Beginning of for of North Africa, and Appalachian Mountains of North America, also the , , and Tuhua orogenies in New Zealand. A series of extinction events, including the massive and ones, wipe out many acritarchs, corals, sponges, molluscs, trilobites, eurypterids, graptolites, brachiopods, crinozoans (e.g. all ), and fish, including all placoderms and ostracoderms.*
*
*
*
*
*
*
thickens. First and fully terrestrialised arthropods: , (including ), and . diversify rapidly, becoming widespread and dominant. Cephalopods continue to flourish. True , along with , also roam the seas. and corals, ( Pentamerida, , etc.), and all abundant. and diverse; 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 , above (thus Euramerica forms). tapers off. Icehouse period ends late in this period after starting in Late Ordovician. on Australian continent tapers off.*
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*
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*
The Great Ordovician Biodiversification Event occurs as plankton increase in number: diversify into many new types (especially brachiopods and molluscs; e.g. long cephalopods like the long lasting and diverse ). Early , articulate ( Orthida, Strophomenida, etc.), , (nautiloids), , , , many types of (, , , , , and , etc.), branched , and other taxa all common. still persist and common. Cephalopods become dominant and common, with some trending toward a coiled shell. Anomalocarids decline. Mysterious appear. First and fish appear, the latter probably giving rise to the at the end of the period. First uncontroversial terrestrial and fully terrestrialised . Ice age at the end of this period, as well as a series of mass extinction events, killing off some cephalopods and many brachiopods, bryozoans, echinoderms, graptolites, trilobites, bivalves, corals and .*
*
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Middle*
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(formerly )
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*
Stage 10Major diversification of (fossils mainly show bilaterian) life in the Cambrian Explosion as oxygen levels increase. Numerous fossils; most modern (including , , , , and ) appear. Reef-building 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 (including ), worms, inarticulate (unhinged lampshells), , , , pentaradial echinoderms (e.g. , and ), and numerous other animals. are dominant and giant predators, while many Ediacaran fauna die out. and molluscs diversify rapidly. , (e.g., ), and continue to present day. First from earlier chordates. Petermann Orogeny on the Australian continent tapers off (550–535 Ma). Ross Orogeny in Antarctica. Delamerian Orogeny (c. 514–490 Ma) on Australian continent. Some small terranes split off from Gondwana. Atmospheric content roughly 15 times present-day () levels (6000 ppm compared to today's 400 ppm) and start colonising land. 3 extinction events occur 517, 502 and 488 Ma, the first and last of which wipe out many of the anomalocarids, artiopods, hyoliths, brachiopods, molluscs, and conodonts (early jawless vertebrates).~
~ *
~ *
~ *
~ *
~
Series 2Stage 4~
Stage 3~
Stage 2~
*
Good of primitive . flourish worldwide in seas, possibly appearing after an , possibly caused by a large-scale oxidation event. First (unknown affinity among animals), and . Enigmatic vendozoans include many soft-jellied creatures shaped like bags, disks, or quilts (like ). Simple of possible worm-like Trichophycus, etc. in North America. in Indian subcontinent. Beginning of Pan-African Orogeny, leading to the formation of the short-lived Ediacaran supercontinent , which by the end of the period breaks up into , , Siberia and . Petermann Orogeny forms on Australian continent. Beardmore Orogeny in Antarctica, 633–620 Ma. forms. An increase in oceanic levels.~ *
Possible "" period. still rare. Late Ruker / Nimrod Orogeny in Antarctica tapers off. First uncontroversial fossils. First hypothetical and .~
Final assembly of supercontinent occurs in early Tonian, with breakup beginning c. 800 Ma. Sveconorwegian orogeny ends. Grenville Orogeny tapers off in North America. Lake Ruker / Nimrod Orogeny in Antarctica, 1,000 ± 150 Ma. Edmundian Orogeny (c. 920–850 Ma), , Western Australia. Deposition of Adelaide Superbasin and Centralian Superbasin begins on Australian continent. First hypothetical (from holozoans) and terrestrial algal mats. Many endosymbiotic events concerning red and green algae occur, transferring plastids to (e.g. , ), , , , and (the events may have begun in the Mesoproterozoic) while the first (e.g. ) also appear: eukaryotes diversify rapidly, including algal, eukaryovoric and biomineralised forms. of simple eukaryotes. Neoproterozoic oxygenation event (NOE), 850–540 Ma.
Narrow highly belts due to as forms, surrounded by the Pan-African Ocean. Sveconorwegian orogeny starts. Late Ruker / Nimrod Orogeny in Antarctica possibly begins. Musgrave Orogeny (c. 1,080–), , Central Australia. decline as proliferate.
continue to expand. colonies in the seas. Grenville Orogeny in North America. Columbia breaks up.
expand. Barramundi Orogeny, , Northern Australia, and Isan Orogeny, 1,600 Ma, Mount Isa Block, Queensland. First (the first eukaryotes with from cyanobacteria; e.g. and ) and (giving rise to the first and ). (remains of marine algae possibly) start appearing in the fossil record.
First uncontroversial : with nuclei and endomembrane system. Columbia forms as the second undisputed earliest supercontinent. Kimban Orogeny in Australian continent ends. Yapungku Orogeny on , in Western Australia. Mangaroon Orogeny, 1,680–1,620 Ma, on the in Western Australia. Kararan Orogeny (1,650 Ma), Gawler craton, . Oxygen levels drop again.
The atmosphere becomes much more while more cyanobacterial stromatolites appear. Vredefort and asteroid impacts. Much . and Trans-Hudsonian Orogenies in North America. Early Ruker Orogeny in Antarctica, 2,000–1,700 Ma. Glenburgh Orogeny, , Australian continent 2,005–1,920 Ma. Kimban Orogeny, in Australian continent begins.
Bushveld Igneous Complex forms. glaciation. First hypothetical . Multicellular Francevillian biota. Kenorland disassembles.
Great Oxidation Event (due to ) increases oxygen. Sleaford Orogeny on Australian continent, 2,440–2,420 Ma.
Stabilization of most modern ; possible mantle overturn event. Insell Orogeny, 2,650 ± 150 Ma. Abitibi greenstone belt in present-day and begins to form, stabilises by 2,600 Ma. First uncontroversial , , and first terrestrial .
(probably colonial phototrophic bacteria, like cyanobacteria). Oldest . Humboldt Orogeny in Antarctica. Blake River Megacaldera Complex begins to form in present-day and , ends by roughly 2,696 Ma.
Prokaryotic (e.g. ) and (e.g. ) diversify rapidly, along with early . First known . Oldest definitive . First microbial mats, stromatolites and MISS. Oldest on Earth (such as the and the ) may have formed during this period. Rayner Orogeny in Antarctica.
First uncontroversial : at first with around 4000 Ma, after which true cells () evolve along with and -based genes around 3800 Ma. The end of the Late Heavy Bombardment. Orogeny in Antarctica, 4,000 ± 200 Ma.
Formation of of the oldest known rock () c. 4,031 to 3,580 Ma. Possible first appearance of . First hypothetical . End of the Early Bombardment Phase. Oldest known (, 4,404 ± 8 Ma). Asteroids and comets bring water to Earth, forming the first oceans. Formation of (4,510 Ma), probably from a giant impact. Formation of Earth (4,543 to 4,540 Ma)


Non-Earth based geologic time scales
Some other planets and satellites in the have sufficiently rigid structures to have preserved records of their own histories, for example, Venus, Mars and the Earth's . Dominantly fluid planets, such as the , 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.


Lunar (selenological) time scale
The geologic history of Earth's Moon has been divided into a time scale based on markers, namely , , and . 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 (, , , , Copernican), with the Imbrian divided into two series/epochs (Early and Late) were defined in the latest Lunar geologic time scale. 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.


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).

A second time scale based on mineral alteration observed by the OMEGA on board the . 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). 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
     


See also
  • Age of the Earth
  • Evolutionary history of life
  • Formation and evolution of the Solar System
  • Geological history of Earth
  • Geology of Mars
  • Geon (geology)
  • History of Earth
  • History of geology
  • History of paleontology
  • List of fossil sites
  • List of geochronologic names
  • Lunar geologic timescale
  • Martian geologic timescale
  • New Zealand geologic time scale
  • Timeline of the Big Bang
  • Timeline of evolution
  • Timeline of the geologic history of the United States
  • Timeline of human evolution
  • Timeline of natural history
  • Timeline of paleontology


Notes

Further reading


External links

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