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The Historical geology is used by geologists and other scientists to describe the timing and relationships between events that have occurred during the history of Earth. The table of geological periods presented here agrees with the dates and nomenclature proposed by the International Commission on Stratigraphy, and uses the standard color codes of the United States Geological Survey.
Evidence from radiometric dating indicates that the Earth is about 4.567 billion (4,567 million) years old. The geological or deep time of Earth's past has been organized into various units according to events which took place in each period. Different spans of time on the time scale are usually delimited by major geological or palaeontological events, such as mass extinctions. For example, the boundary between the Cretaceous period and the Palaeogene period is defined by the Cretaceous–Tertiary extinction event, which marked the demise of the dinosaurs and of many marine species. Older periods which predate the reliable fossil record are defined by absolute age.
The largest defined unit of time is the supereon composed of Eons. Eons are divided into Eras, which are in turn divided into Periods, Epochs and Stages. At the same time paleontologists define a system of faunal stages, of varying lengths, based on changes in the observed fossil assemblages. In many cases, such faunal stages have been adopted in building the geological nomenclature, though in general there are far more recognized faunal stages than defined geological time units.
Geologists tend to talk in terms of Upper/Late, Lower/Early and Middle parts of periods and other units, such as "Upper Jurassic", and "Middle Cambrian". Upper, Middle, and Lower are terms applied to the rocks themselves, as in "Upper Jurassic sandstone," while Late, Middle, and Early are applied to time, as in "Early Jurassic deposition" or "fossils of Early Jurassic age." The adjectives are capitalized when the subdivision is formally recognized, and lower case when not; thus "early Miocene" but "Early Jurassic." Because geologic units occurring at the same time but from different parts of the world can often look different and contain different fossils, there are many examples where the same period was historically given different names in different locales. For example, in North America the Lower Cambrian is referred to as the Waucoban series that is then subdivided into zones based on trilobites. The same timespan is split into Tommotian, Atdabanian and Botomian stages in East Asia and Siberia. A key aspect of the work of the International Commission on Stratigraphy is to reconcile this conflicting terminology and define universal horizons that can be used around the world.
History of the time scale [change]
The principles underlying geologic (geological) time scales were laid down by Nicolaus Steno in the late 17th century. Steno argued that rock layers (or strata) are laid down in succession, and that each represents a "slice" of time. He also formulated the principle of superposition, which states that any given stratum is probably older than those above it and younger than those below it. While Steno's principles were simple, applying them to real rocks proved complex. Over the course of the 18th century geologists realized that:
- Sequences of strata were often 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 the Earth's long history.
The first serious attempts to formulate a geological time scale that could be applied anywhere on Earth took place in the late 18th century. The most influential of those early attempts (championed by Abraham Werner, among others) divided the rocks of the Earth's crust into four types: Primary, Secondary, Tertiary, and Quaternary. Each type of rock, according to the theory, formed during a specific period in Earth history. It was thus possible to speak of a "Tertiary Period" as well as of "Tertiary Rocks." Indeed, "Tertiary" (now Palaeocene-Pliocene) and "Quaternary" (now Pleistocene-Holocene) remained in use as names of geological periods well into the 21th century.
In opposition to the then-popular Neptunist theories expounded by Werner (that all rocks had precipitated out of a single enormous flood), a major shift in thinking came with the reading by James Hutton of his Theory of the Earth; or, an Investigation of the Laws Observable in the Composition, Dissolution, and Restoration of Land Upon the Globe before the Royal Society of Edinburgh in March and April 1785, events which "as things appear from the perspective of the twentieth century, James Hutton in those reading became the founder of modern geology" What Hutton proposed was that the interior of the Earth was hot, and that this heat was the engine which drove the creation of new rock: land was eroded by air and water and deposited as layers in the sea; heat then consolidated the sediment into stone, and uplifted it into new lands. This theory was dubbed "Plutonist" in contrast to the flood-oriented theory.
The identification of strata by the fossils they contained, pioneered by William Smith, Georges Cuvier, Jean d'Omalius d'Halloy and Alexandre Brogniart in the early 19th century, enabled geologists to divide Earth history more precisely. It also enabled them to correlate strata across national (or even continental) boundaries. If two strata (however distant in space or different in composition) contained the same fossils, chances were good that they had been laid down at the same time. Detailed studies between 1820 and 1850 of the strata and fossils of Europe produced the sequence of geological periods still used today.
The process was dominated by British geologists, and the names of the periods reflect that dominance. The "Cambrian," (the Roman name for Wales) and the "Ordovician," and "Silurian", named after ancient Welsh tribes, were periods defined using stratigraphic sequences from Wales. The "Devonian" was named for the English county of Devon, and the name "Carboniferous" was simply an adaptation of "the Coal Measures," the old British geologists' term for the same set of strata. The "Permian" was named after Perm, Russia, because it was defined using strata in that region by a Scottish geologist Roderick Murchison. However, some periods were defined by geologists from other countries. The "Triassic" was named in 1834 by a German geologist Friedrich Von Alberti from the three distinct layers (Latin trias meaning triad) —red beds, capped by chalk, followed by black shales— that are found throughout Germany and Northwest Europe, called the 'Trias'. The "Jurassic" was named by a French geologist Alexandre Brogniart for the extensive marine limestone exposures of the Jura Hills. The "Cretaceous" (from Latin creta meaning 'chalk') as a separate period was first defined by a Belgian geologist Jean d'Omalius d'Halloy in 1822, using strata in the Paris basin and named for the extensive beds of chalk (calcium carbonate deposited by the shells of marine invertebrates).
British geologists were also responsible for the grouping of periods into Eras and the subdivision of the Tertiary and Quaternary periods into epochs.
When William Smith and Sir Charles Lyell first recognized that rock strata represented successive time periods, time scales could be estimated only very imprecisely since various kinds of rates of change used in estimation were highly variable. While creationists had been proposing dates of around six or seven thousand years for the age of the Earth based on the Bible, early geologists were suggesting millions of years for geologic periods with some even suggesting a virtually infinite age for the Earth. Geologists and paleontologists constructed the geologic table based on the relative positions of different strata and fossils, and estimated the time scales based on studying rates of various kinds of weathering, erosion, sedimentation, and lithification. Until the discovery of radioactivity in 1896 and the development of its geological applications through radiometric dating during the first half of the 20th century (pioneered by such geologists as Arthur Holmes) which allowed for more precise absolute dating of rocks, the ages of various rock strata and the age of the Earth were the subject of considerable debate.
In 1977, the Global Commission on Stratigraphy (now the International Commission on Stratigraphy) started an effort to define global references (Global Boundary Stratotype Sections and Points) for geologic periods and faunal stages. The commission's most recent work is described in the 2004 geologic time scale of Gradstein et al.. A UML model for how the timescale is structured, relating it to the GSSP, is also available.
Geologic history shown to scale [change]
Below is the geologic history shown to scale.
From the formation of the Earth to today.
Cryo = Cryogenian
Ed. = Ediacaran
Meso = Mesozoic
C = Cainozoic
Neo = Neogene
Q = Quaternary
P = Pleistocene
H = Holocene
Table of geologic time [change]
The following table summarizes the major events and characteristics of the periods of time making up the geologic time scale. As above, this time scale is based on the International Commission on Stratigraphy. To see the table click "show" the the far right on the gray bar with the black line. The height of each table entry does not correspond to the duration of each subdivision of time. (not shown to scale)
|Supereon||Eon||Era||Period/Age4,5||Epoch||Major Events||Years Ago3,6|
|Phanerozoic||Cainozoic||Quaternary||Holocene||Rise of Human population. Last Ice age ends.||11,700|
|Pleistocene||Extinction of many large mammals. Evolution of fully modern humans||2.588 million|
|Tertiary||Neogene||Pliocene||The continents drift into their current place. Temperatures cool into Ice age late in the Neogene||5.333 million|
|Mesozoic||Cretaceous||Upper Cretaceous||Dinosaurs reach peak, become extinct in K/T extinction event; marsupial and placental mammals appear; first flowering plants||100.5 million|
|Lower Cretaceous||145 million|
|Jurassic||Upper Jurassic||first birds, early mammals; conifers, cycads and other seed plants. Supercontinent Pangaea breaks up.||163.5 million|
|Middle Jurassic||174.1 million|
|Lower Jurassic||201.3 million|
|Triassic||Upper Triassic||First dinosaurs; pterosaurs; ichthyosaurs; plesiosaurs; Egg-laying mammals.||237 million|
|Middle Triassic||247.2 million|
|Lower Triassic||252.17 million|
|Palaeozoic||Permian||P/Tr extinction event – 95% of species become extinct. Supercontinent Pangaea forms.||298.9 million|
|Carboniferous||Pennsylvanian||Abundant insects, first reptiles, coal forests||323.2 million|
|Mississippian||Large primitive trees||358.9 million|
|Devonian||First amphibians, clubmosses and horsetails appear, progymnosperms (first seed bearing plants) appear||419.2 million|
|Silurian||First land plant fossils||443.4 million|
|Ordovician||Invertebrates dominant||485.4 million|
|Cambrian||Major diversification of life in the Cambrian adaptive radiation||541 million|
|Precambrian||Proterozoic||Neoproterozoic2||Ediacaran||First multi-celled animals||635 million|
|Cryogenian||Possible Snowball Earth Period.||850 million|
|Tonian||Supercontinent Rodinia breaks up.||1,000 million|
|Mesoproterozoic||First sexually reproducing organism. The supercontinent Rodinia forms.||1,600 million|
|Palaeoproterozoic||First complex single-celled life||2,500 million|
|Archaean||Bacteria build stromatolites. 1st supercontinet Vaalbara forms and breaks up.||4,000 million|
|Hadean||Formation of Earth 4.6 Gya; formation of Moon 4.5 Gya||4,567 million|
Proposed Precambrian Timeline [change]
The Geologic Time Scale 2012 book from which the ICS approved the new time scale also included a proposal to revise the Precambrian Timeline.
- Hadean Eon - 4567-4030 MYA
- Archaean Eon - 4030-2420 MYA
- Proterozoic Eon - 2420-541 MYA
Related pages [change]
References and footnotes [change]
- John McPhee, Basin and Range, New York:Farrar, Straus and Giroux, 1981, pp.95-100.
- John McPhee, Basin and Range, pp.113-114.
- (in Russian) Great Soviet Encyclopedia (3rd ed. ed.). Moscow: Sovetskaya Enciklopediya. 1974. pp. vol. 16, p. 50.
- Felix M. Gradstein, James G. Ogg, Alan G. Smith (eds) 2005. A Geologic Time Scale 2004, Cambridge University Press. ISBN 0-521-78673-8
- Cox & Richard, A formal model for the geologic time scale and global stratotype section and point, compatible with geospatial information transfer standards, Geosphere, volume 1, pp 119-137, Geological Society of America, 2005
Other websites [change]
- GSA: Geologic Time Scale
- National Museum of Natural History - Geologic Time
- Geological Time Systems - Information model for the geologic time scale
- Exploring Time from Planck Time to the lifespan of the universe
|Precambrian (4.567 gya – 541 mya)|
|In the left column are Eons, bold are Eras, not bold are Periods. gya = billion years ago, mya = million years ago|
|Hadean (4.567 gya – 4 gya)|
|Archaean (4 gya – 2.5 gya)|
|Proterozoic (4 gya – 2.5 gya)||Palaeoproterozoic (2.5 gya – 1.6 gya)|
|Phanerozoic (541 mya – today)|
|In the left column are Eras, bold are Periods, not bold or italics are Epochs, Italics are stages. kya = thousand years ago, mya = million years ago|
|Palaeozoic (541 mya – 252.17 mya)||Cambrian (541 mya – 485.4 mya)|
|Mesozoic (252.17 mya – 66.0 mya)||Triassic (252.17 mya – 201.3 mya) Lower Triassic (252.17 mya – 247.2 mya) Middle Triassic (247.2 mya – 237 mya) Upper Triassic (237 mya – 201.3 mya)|
|Cainozoic (66.0 mya – today)||Palaeogene (66.0 mya – 23.03 mya) Palaeocene (66.0 mya – 56 mya) Eocene (56 mya - 33.9 mya) Oligocene (33.9 mya – 23.03 mya)|
|Source||International Chronostratigraphic Chart 2013. International Commission on Stratigraphy, retrieved 8 April 2013. Divisions of geologic time – major chronostratigraphic and geochronologic units USGS, retrieved 8 April 2013.|