Geologic time scale
From
Wikipedia, the free encyclopedia: http://en.wikipedia.org/wiki/Geologic_time_scale
See notes at the ends of "Major events" about carbon dioxide concentrations.
The geologic
time scale is a chronologic schema (or idealized Model) relating stratigraphy
to time that is used by geologists and other earth
scientists
to describe the timing and relationships between events that have occurred
during the history of Earth. The table of geologic time spans
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 4.570 billion 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.
Graphical timelines
The second and
third timelines are each subsections of their preceding timeline as indicated
by asterisks.
Millions of Years
The Holocene (the
latest epoch) is
too small to be shown clearly on this timeline.
Units in geochronology and stratigraphy[1] |
||
Segments of
rock (strata) in chronostratigraphy |
Periods of
time in geochronology |
Notes |
Eon |
4 total, half a billion years or more |
|
Era |
12 total, several hundred million years |
|
Period |
21 major and 2 minor |
|
Epoch |
48 total, tens of millions of years |
|
Age |
Over 100, each spanning millions of years |
|
Chron |
Generic term for any identifiable time period; not
necessarily part of a hierarchy |
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 ages. The terms eonothem, erathem, system, series, and stage are used to refer to the layers of rock that correspond
to these periods of geologic time.
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.[citations needed]
See the main articles: history of geology and history of paleontology.
Earth history mapped to 24 hours
The first
geologic time scale was proposed in 1913 by the British geologist Arthur
Holmes.[2]
He greatly furthered the newly created discipline of geochronology
and published the world renowned book The Age of the Earth in 1913 in
which he estimated the Earth's age to be at least 1.6 billion years.[3]
Aristotle
realized that fossil seashells from rocks were similar to those found on the
beach, indicating the fossils were once living animals. He deduced that the
positions of land and sea had changed and these changes occurred over long
periods of time. Leonardo da Vinci concurred with Aristotle's view
that fossils were the remains of ancient life.[4]
One of the
principles underlying geologic time scales was the principle of superposition of strata, first
proposed in the 11th century by the Persian
geologist, Avicenna
(Ibn Sina). However, he rejected the explanation of fossils as organic remains.[5]
While discussing the origins of mountains in The Book of Healing in 1027, he outlined
the principle as follows:[6][7]
"It is also possible that the sea
may have happened to flow little by little over the land consisting of both
plain and mountain, and then have ebbed away from it. ... It is possible that
each time the land was exposed by the ebbing of the sea a layer was left, since
we see that some mountains appear to have been piled up layer by layer, and it
is therefore likely that the clay from which they were formed was itself at one
time arranged in layers. One layer was formed first, then at a different
period, a further was formed and piled, upon the first, and so on. Over each
layer there spread a substance of different material, which formed a partition
between it and the next layer; but when petrification took place something
occurred to the partition which caused it to break up and disintegrate from
between the layers (possibly referring to unconformity). ... As to the
beginning of the sea, its clay is either sedimentary or primeval, the latter
not being sedimentary. It is probable that the sedimentary clay was formed by
the disintegration of the strata of mountains. Such is the formation of
mountains."
His
contemporary, Abū Rayhān
Bīrūnī (973-1048), discovered the existence of shells and fossils in regions
that once housed seas and later evolved into dry land, such as the Indian subcontinent. Based on this evidence, he
realized that the Earth
is constantly evolving and proposed that the Earth had an age, but that its
origin was too distant to measure.[8]
Later in the 11th century, the Chinese naturalist, Shen Kuo
(1031-1095), also recognized the concept of 'deep time'.[9]
The principles
underlying geologic (geological) time scales were later laid down by Nicholas
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 law 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:
A comparative geological timescale
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
Paleocene-Pliocene) and "Quaternary" (now Pleistocene-Holocene)
remained in use as names of geological periods well into the 20th 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"[10]
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.[11]
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 Mountains. 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[12]
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.[13].
A UML model for how the timescale is structured, relating it to the GSSP, is
also available[14].
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. (See lunar geologic timescale for a discussion
of the geologic subdivisions of Earth's moon.) The height of each table entry
does not correspond to the duration of each subdivision of time.
Geologic
time scale[hide]
Supereon |
Eon |
Era |
Period[15] |
Major
events |
Start,
million years ago[16] |
||
The last
glacial period ends and rise of human civilization. Quaternary
Ice Age recedes, and the current interglacial begins. Younger Dryas cold spell occurs,
Sahara
Desert forms from savannah, and agriculture begins, allowing
humans to build cities. Paleolithic/Neolithic (Stone Age) cultures begin around
10,000 BC,
giving way to Copper Age
(3500 BC) and Bronze Age
(2500 BC). Cultures continue to grow in complexity and technical advancement
through the Iron Age (1200 BC), giving rise
to many pre-historic cultures
throughout the world, eventually leading into Classical Antiquity, such as Ancient Rome and even to the Middle Ages and present day. Little Ice Age (stadial) causes brief cooling in
Northern
Hemisphere from 1400 to 1850. Also refer to the List
of archaeological periods for clarification on early cultures and
ages. Mount Tambora
erupts in 1815, causing the Year
Without a Summer (1816) in Europe and North America from a volcanic winter. atmospheric
CO2
levels start creeping from 100 ppmv at the end of the last glaciation to the
current level of 385 parts per million volume (ppmv), causing,
according to some sources, global warming and climate change, possibly from anthropogenic sources, such as
the Industrial
Revolution[18] |
|||||||
Flourishing and then extinction of
many large mammals (Pleistocene
megafauna). Evolution of anatomically modern humans. Quaternary
Ice Age continues with glaciations
and interstadials
(and the accompanying fluctuations from 100 to 300 ppmv in atmospheric
Carbon
Dioxide levels[18]), further intensification of Icehouse
Earth conditions, roughly 1.6 MYA[20]. Last glacial maximum (30,000 years
ago), last
glacial period (18,000-15,000 years ago). Dawn of human stone-age
cultures, with increasing
technical complexity than previous ice age cultures, such as engravings
and clay statues (Venus of
Lespugue), particularly in the Mediterranean
and Europe. Lake Toba supervolcano erupts 75,000 years
before present, causing a volcanic winter and pushes
humanity to the brink of extinction. |
0.126 ± 0.005* |
||||||
0.500? |
|||||||
1.806 ± 0.005* |
|||||||
2.588 ± 0.005* |
|||||||
Intensification of present Icehouse
conditions, Present
(Quaternary) ice age begins roughly 2.58 MYA; cool and dry climate. Australopithecines,
many of the existing genera of mammals, and recent mollusks
appear. Homo habilis
appears. |
3.600 ± 0.005* |
||||||
5.332 ± 0.005* |
|||||||
Moderate
Icehouse climate, puncuated by ice ages; Orogeny in northern hemisphere. Modern mammal and bird families became recognizable. Horses and mastodons diverse. Grasses become ubiquitous. First apes appear (for reference see the article: "Sahelanthropus
tchadensis"). Kaikoura Orogeny forms Southern Alps in New Zealand, continues today.
Orogeny of the Alps in Europe slows, but continues to this day. Carpathean
orogeny forms Carpathian
Mountains in Central
and Eastern Europe.
Hellenic
orogeny in Greece and Aegean Sea slows, but continues to this day.
Middle Miocene Disruption occurs.
Widespread forests slowly draw in massive amounts of
atmospheric Carbon Dioxide, gradually lowering the level
atmospheric CO2 from 650 ppmv down to around 100 ppmv[18]. |
7.246 ± 0.05* |
||||||
11.608 ± 0.05* |
|||||||
13.65 ± 0.05* |
|||||||
15.97 ± 0.05* |
|||||||
20.43 ± 0.05* |
|||||||
23.03 ± 0.05* |
|||||||
Warm
but cooling climate, moving towards Icehouse; Rapid evolution and diversification of
fauna, especially mammals. Major evolution and
dispersal of modern types of flowering plants |
28.4 ± 0.1* |
||||||
33.9 ± 0.1* |
|||||||
Moderate,
cooling climate. Archaic mammals (e.g. Creodonts, Condylarths, Uintatheres, etc) flourish and
continue to develop during the epoch. Appearance of several
"modern" mammal families. Primitive whales diversify. First grasses. Reglaciation of Antarctica and formation of its ice cap; Azolla event triggers ice age, and the Icehouse
Earth climate that would follow it to this day, from the
settlement and decay of seafloor algae drawing
in massive amounts of atmospheric Carbon
Dioxide[18], lowering it from 3800 ppmv down to 650 ppmv. End of Laramide
and Sevier
Orogenies of the Rocky Mountains in North America. Orogeny of the Alps in Europe
begins. Hellenic
Orogeny begins in Greece and Aegean Sea. |
37.2 ± 0.1* |
||||||
40.4 ± 0.2* |
|||||||
48.6 ± 0.2* |
|||||||
55.8 ± 0.2* |
|||||||
Climate
tropical. Modern plants appear;
Mammals diversify into a number
of primitive lineages following the extinction of the dinosaurs. First large
mammals (up to bear or small hippo size). Alpine orogeny in Europe and Asia begins. Indian Subcontinent collides with Asia 55 MYA[20], Himalayan
Orogeny starts between 52 and 48 MYA. |
58.7 ± 0.2* |
||||||
61.7 ± 0.3* |
|||||||
65.5 ± 0.3* |
|||||||
Flowering plants proliferate,
along with new types of insects. More
modern teleost
fish begin to appear. Ammonites, belemnites, rudist bivalves, echinoids
and sponges
all common. Many new types of dinosaurs
(e.g. Tyrannosaurs,
Titanosaurs,
duck
bills, and horned dinosaurs)
evolve on land, as do Eusuchia (modern crocodilians); and mosasaurs and modern sharks appear in the sea. Primitive birds gradually replace pterosaurs.
Monotremes,
marsupials and placental mammals appear. Break
up of Gondwana. Beginning of Laramide
and Sevier Orogenies of the Rocky Mountains. Atmospheric
Carbon
Dioxide close to present-day levels. |
70.6 ± 0.6* |
||||||
83.5 ± 0.7* |
|||||||
85.8 ± 0.7* |
|||||||
89.3 ± 1.0* |
|||||||
93.5 ± 0.8* |
|||||||
99.6 ± 0.9* |
|||||||
112.0 ± 1.0* |
|||||||
125.0 ± 1.0* |
|||||||
130.0 ± 1.5* |
|||||||
136.4 ± 2.0* |
|||||||
140.2 ± 3.0* |
|||||||
145.5 ± 4.0* |
|||||||
Gymnosperms (especially conifers, Bennettitales and cycads) and ferns common.
Many types of dinosaurs, such as sauropods, carnosaurs,
and stegosaurs.
Mammals common but small. First birds and lizards. Ichthyosaurs and plesiosaurs diverse. Bivalves, Ammonites and belemnites abundant. Sea urchins very common, along
with crinoids, starfish, sponges, and terebratulid and rhynchonellid brachiopods. Breakup of Pangaea into Gondwana and Laurasia. Nevadan orogeny in North
America. Rantigata
and Cimmerian
Orogenies taper off. Atmospheric Carbon Dioxide levels 4-5 times
the present day levels (1200-1500 ppmv, compared to today's 385 ppmv[18]). |
150.8 ± 4.0* |
||||||
155.7 ± 4.0* |
|||||||
161.2 ± 4.0* |
|||||||
164.7 ± 4.0 |
|||||||
167.7 ± 3.5* |
|||||||
171.6 ± 3.0* |
|||||||
175.6 ± 2.0* |
|||||||
183.0 ± 1.5* |
|||||||
189.6 ± 1.5* |
|||||||
196.5 ± 1.0* |
|||||||
199.6 ± 0.6* |
|||||||
Archosaurs dominant on land as dinosaurs, in the oceans as Ichthyosaurs and nothosaurs, and in the air as pterosaurs. cynodonts become smaller and
more mammal-like, while first mammals and crocodilia appear. Dicrodium
flora common on land. Many large aquatic temnospondyl amphibians. Ceratitic ammonoids extremely
common. Modern corals
and teleost
fish appear, as do many modern insect
clades. 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 MYA) |
203.6 ± 1.5* |
||||||
216.5 ± 2.0* |
|||||||
228.0 ± 2.0* |
|||||||
237.0 ± 2.0* |
|||||||
245.0 ± 1.5* |
|||||||
Lower/Early
("Scythian") |
249.7 ± 1.5* |
||||||
251.0 ± 0.7* |
|||||||
Landmasses unite into supercontinent Pangaea, creating the Appalachians.
End of Permo-Carboniferous glaciation. Synapsid reptiles (pelycosaurs and therapsids)
become plentiful, while parareptiles and temnospondyl amphibians
remain common. In the mid-Permian, coal-age flora
are replaced by cone-bearing
gymnosperms (the first true seed
plants) and by the first true mosses. Beetles and flies evolve. Marine life flourishes in warm shallow
reefs; productid
and spiriferid brachiopods,
bivalves, forams,
and ammonoids
all abundant. Permian-Triassic extinction event
occurs 251 mya: 95% of life on Earth becomes extinct, including all trilobites, graptolites, and blastoids. Ouachita
and Innuitian
orogenies in North America. Uralian orogeny in Europe/Asia tapers off. Altaid
orogeny in Asia. Hunter-Bowen
Orogeny on Australian Continent begins, (c. 260-225
MYA). Forms the MacDonnell
Ranges. |
253.8 ± 0.7* |
||||||
260.4 ± 0.7* |
|||||||
265.8 ± 0.7* |
|||||||
268.4 ± 0.7* |
|||||||
270.6 ± 0.7* |
|||||||
275.6 ± 0.7* |
|||||||
284.4 ± 0.7* |
|||||||
294.6 ± 0.8* |
|||||||
299.0 ± 0.8* |
|||||||
Winged insects radiate suddenly;
some (esp. Protodonata
and Palaeodictyoptera)
are quite large. Amphibians
common and diverse. First reptiles and
coal forests (scale trees, ferns, club trees, giant horsetails, Cordaites, etc.).
Highest-ever atmospheric
oxygen levels. Goniatites, brachiopods,
bryozoa, bivalves, and corals plentiful in the seas and oceans. Testate forams proliferate.
Uralian orogeny in Europe and Asia. Variscan orogeny occurs towards
middle and late Mississippian Periods. |
303.9 ± 0.9* |
||||||
306.5 ± 1.0* |
|||||||
311.7 ± 1.1* |
|||||||
318.1 ± 1.3* |
|||||||
Large primitive trees, first land
vertebrates, and amphibious sea-scorpions live amid coal-forming coastal swamps. Lobe-finned rhizodonts
are dominant big fresh-water predators. In the oceans, early sharks are common and quite
diverse; echinoderms (especially crinoids and blastoids) abundant. Corals, bryozoa, goniatites
and brachiopods (Productida,
Spiriferida, etc.) very common.
But trilobites
and nautiloids decline. Glaciation
in East Gondwana. Tuhua
Orogeny in New Zealand tapers off. |
326.4 ± 1.6* |
||||||
345.3 ± 2.1* |
|||||||
359.2 ± 2.5* |
|||||||
First clubmosses, horsetails
and ferns appear, as do the first seed-bearing plants (progymnosperms), first trees (the progymnosperm Archaeopteris), and first
(wingless) insects.
Strophomenid and atrypid
brachiopods, rugose and tabulate
corals, and crinoids are all abundant in the
oceans. Goniatite ammonoids are plentiful, while
squid-like coleoids arise. Trilobites and
armoured agnaths decline, while jawed fishes (placoderms, lobe-finned and ray-finned fish, and early sharks) rule the seas. First amphibians still aquatic.
"Old Red Continent" of Euramerica. Beginning of Acadian
Orogeny for Anti-Atlas
Mountains of North Africa,
and Appalachian
Mountains of North America,
also the Antler, Variscan,
and Tuhua
Orogeny in New Zealand. |
374.5 ± 2.6* |
||||||
385.3 ± 2.6* |
|||||||
391.8 ± 2.7* |
|||||||
397.5 ± 2.7* |
|||||||
407.0 ± 2.8* |
|||||||
411.2 ± 2.8* |
|||||||
416.0 ± 2.8* |
|||||||
no faunal stages defined |
First Vascular plants (the rhyniophytes
and their relatives), first millipedes
and arthropleurids on land. First jawed
fishes, as well as many armoured
jawless fish, populate the seas.
Sea-scorpions reach large size. Tabulate and rugose corals, brachiopods (Pentamerida,
Rhynchonellida, etc.), and crinoids all abundant. Trilobites and mollusks
diverse; graptolites not as varied.
Beginning of Caledonian Orogeny for hills in England, Ireland, Wales, Scotland,
and the Scandinavian
Mountains. Also continued into Devonian period as the Acadian
Orogeny, above. Taconic Orogeny tapers off. Lachlan
Orogeny on Australian Continent tapers off. |
418.7 ± 2.7* |
|||||
421.3 ± 2.6* |
|||||||
422.9 ± 2.5* |
|||||||
426.2 ± 2.4* |
|||||||
428.2 ± 2.3* |
|||||||
436.0 ± 1.9* |
|||||||
439.0 ± 1.8* |
|||||||
443.7 ± 1.5* |
|||||||
Invertebrates diversify into
many new types (e.g., long straight-shelled cephalopods). Early corals, articulate brachiopods (Orthida, Strophomenida,
etc.), bivalves, nautiloids, trilobites, ostracods, bryozoa, many types of echinoderms
(crinoids, cystoids,
starfish,
etc.), branched graptolites,
and other taxa all common. Conodonts
(early planktonic vertebrates) appear. First green plants and fungi on land. Ice age at end of
period. |
445.6 ± 1.5* |
||||||
460.9 ± 1.6* |
|||||||
468.1 ± 1.6* |
|||||||
471.8 ± 1.6* |
|||||||
478.6 ± 1.7* |
|||||||
488.3 ± 1.7* |
|||||||
Major diversification of life in
the Cambrian Explosion. Many fossils; most modern animal phyla appear. First chordates
appear, along with a number of extinct, problematic phyla. Reef-building Archaeocyatha abundant; then
vanish. Trilobites, priapulid
worms, sponges,
inarticulate brachiopods
(unhinged lampshells), and many other animals numerous. Anomalocarids are giant
predators, while many Ediacaran fauna die out. Prokaryotes, protists (e.g., forams), fungi and algae continue to present day. Gondwana emerges. Petermann
Orogeny on the Australian Continent tapers off (550-535
MYA). Ross Orogeny in Antarctica. Adelaide
Geosyncline (Delamerian Orogeny), majority of orogenic activity
from 514-500 MYA. Lachlan Orogeny on Australian Continent, c. 540-440 MYA. Atmospheric
Carbon
Dioxide content roughly 20-35 times present-day (Holocene) levels (6000 ppmv
compared to today's 385 ppmv)[18] |
496.0 ± 2.0* |
||||||
501.0 ± 2.0* |
|||||||
513.0 ± 2.0 |
|||||||
other faunal stages/ |
542.0 ± 1.0* |
||||||
Good fossils of the first multi-celled
animals. Ediacaran biota flourish worldwide in seas.
Simple trace fossils
of possible worm-like Trichophycus,
etc. First sponges
and trilobitomorphs.
Enigmatic forms include many soft-jellied creatures shaped like bags, disks,
or quilts (like Dickinsonia).
Taconic
Orogeny in North America.
Aravalli Range orogeny in Indian Subcontinent. Beginning of Petermann
Orogeny on Australian Continent. Beardmore Orogeny in
Antarctica, 633-620 MYA. |
630 +5/-30* |
||||||
Possible "Snowball Earth" period. Fossils still rare. Rodinia landmass begins to break
up. Late Ruker / Nimrod Orogeny in Antarctica tapers off. |
850[24] |
||||||
Rodinia supercontinent persists.
Trace fossils of simple multi-celled
eukaryotes.
First radiation of dinoflagellate-like
acritarchs. Grenville Orogeny tapers off in North America. Pan-African
Orogeny in Africa. Lake
Ruker / Nimrod Orogeny in Antarctica,
1000 ± 150 MYA. Edmundian Orogeny (c. 920 - 850 MYA), Gascoyne Complex, Western
Australia. Adelaide
Geosyncline laid down on Australian
Continent, beginning of Adelaide
Geosyncline (Delamerian Orogeny) in that continent. |
1000[24] |
||||||
Narrow highly metamorphic belts due to orogeny as Rodinia formed. Late Ruker /
Nimrod Orogeny in Antarctica possibly begins. Musgrave Orogeny (c. 1080 MYA),
Musgrave Block, Central
Australia. |
1200[24] |
||||||
Platform covers continue to
expand. Green algae colonies in the seas. Grenville Orogeny in North America. |
1400[24] |
||||||
Platform covers expand.
Barramundi Orogeny, MacArthur
Basin, Northern
Australia, and Isan Orogeny, c. 1600 MYA, Mount Isa Block, Queensland |
1600[24] |
||||||
First complex single-celled life: protists with nuclei. Columbia
is the primordial supercontinent. Kimban Orogeny in Australian Continent
ends. Yapungku Orogeny on North
Yilgarn craton, in Western
Australia. Mangaroon Orogeny, 1680-1620 MYA, on the Gascoyne Complex in Western
Australia. Kararan Orogeny (1650- MYA), Gawler Craton, South Australia. |
1800[24] |
||||||
The atmosphere
became oxygenic. Vredefort and Sudbury Basin asteroid impacts.
Much orogeny. Penokean
and Trans-Hudsonian Orogenies in North
America. Early Ruker Orogeny in Antarctica, 2000 - 1700 MYA. Glenburgh
Orogeny, Glenburgh
Terrane, Australian Continent c. 2005 - 1920 MYA. Kimban Orogeny, Gawler craton in Australian
Continent begins. |
2050[24] |
||||||
Bushveld Formation formed. Huronian
glaciation. |
2300[24] |
||||||
Oxygen
Catastrophe: banded
iron formations formed. Sleaford Orogeny on Australian Continent, Gawler
Craton 2440-2420 MYA. |
2500[24] |
||||||
Stabilization of most modern cratons; possible mantle overturn event. Insell
Orogeny, 2650 ± 150 MYA. Abitibi
greenstone belt in present-day Ontario and Quebec begins to form, stablizes
by 2600 MYA. |
2800[24] |
||||||
First stromatolites (probably colonial cyanobacteria). Oldest macrofossils. Humboldt Orogeny
in Antarctica. Blake
River Megacaldera Complex begins to form in present-day Ontario and Quebec, ends by roughly 2696
MYA. |
3200[24] |
||||||
First known oxygen-producing bacteria. Oldest definitive microfossils.
Oldest cratons on earth (such as the Canadian Shield and the Pilbara
Craton) may have formed during this period[25]. Rayner Orogeny in Antarctica. |
3600[24] |
||||||
Simple single-celled life
(probably bacteria and perhaps archaea). Oldest probable microfossils. |
3800 |
||||||
This era overlaps the end of the Late
Heavy Bombardment of the inner solar
system. |
c.3850 |
||||||
This era gets its name from the lunar
geologic timescale when the Nectaris
Basin and other major lunar
basins were formed by large impact events. |
c.3920 |
||||||
Oldest known rock (4030 Ma)[28]. The first Lifeforms and
self-replicating
RNA molecules
may have evolved on earth around 4000 Ma during this era. Naiper Orogeny in Antarctica, 4000 ± 200 MYA. |
c.4150 |
||||||
Oldest known mineral (Zircon, 4406±8 Ma[29]). Formation of Moon (4533 Ma), probably from giant
impact. Formation of Earth (4567.17
to 4570 Ma) |
c.4570 |
|