For the album by German band The Ocean, see Precambrian (album).
"Cryptozoic" redirects here. For the games publisher, see Cryptozoic Entertainment.
Precambrian Eon
4600–541 million years ago
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Millions of years

The Precambrian (or Pre-Cambrian, sometimes abbreviated ) is the earliest 4.06 billion years of Earth's history and before the current Phanerozoic Eon. The Precambrian (colored green on the right) is a supereon that is subdivided into three eons (Hadean, Archean, Proterozoic) of the geologic time scale. It spans from the formation of Earth about 4.6 billion years ago (Ga) to the beginning of the Cambrian Period, about 541 million years ago (Ma), when hard-shelled creatures first appeared in abundance. The Precambrian is so named because it preceded the Cambrian, the first period of the Phanerozoic eon, which is named after Cambria, the Latinised name for Wales, where rocks from this age were first studied. The Precambrian accounts for 89% of geologic time.


Relatively little is known about the Precambrian, despite it making up roughly seven-eighths of the Earth's history, and what is known has largely been discovered from the 1960s onwards. The Precambrian fossil record is poorer than that of the succeeding Phanerozoic, and those fossils present (e.g. stromatolites) are of limited biostratigraphic use.[1] This is because many Precambrian rocks have been heavily metamorphosed, obscuring their origins, while others have been destroyed by erosion, or remain deeply buried beneath Phanerozoic strata.[1][2]

It is thought that the Earth coalesced from material in orbit around the Sun at roughly 4,500 Ma, and may have been struck by a very large (Mars-sized) planetesimal shortly after it formed, splitting off material that formed the Moon (see Giant impact hypothesis). A stable crust was apparently in place by 4,400 Ma, since zircon crystals from Western Australia have been dated at 4,404 Ma.[3]

The term Precambrian is recognized by the International Commission on Stratigraphy as a general term including the Archean and Proterozoic eons.[4] It is still used by geologists and paleontologists for general discussions not requiring the more specific eon names. It was briefly called the Cryptozoic eon.

Life forms

For more details on this topic, see Origin of life.
Landmass positions near the end of the Precambrian

A specific date for the origin of life has not been determined. Carbon found in 3.8 billion year old rocks (Archean eon) from islands off western Greenland may be of organic origin. Well-preserved microscopic fossils of bacteria older than 3.46 billion years have been found in Western Australia.[5] Probable fossils 100 million years older have been found in the same area. There is a fairly solid record of bacterial life throughout the remainder (Proterozoic eon) of the Precambrian.

Excluding a few contested reports of much older forms from North America and India, the first complex multicellular life forms seem to have appeared at roughly 600 Ma, in the Neoproterozoic era of the Proterozoic eon. The oldest fossil evidence from that era of such complex life comes from the Lantian formation of the Ediacarian period, at least 580 million years ago. A very diverse collection of soft-bodied forms is found in a variety of locations worldwide and date to between 600 and 542 Ma. These are referred to as Ediacaran or Vendian biota. Hard-shelled creatures appeared toward the end of that time span, marking the beginning of the Phanerozoic era. By the middle of the following Cambrian period, a very diverse fauna is recorded in the Burgess Shale, including some which may represent stem groups of modern taxa. The explosion in diversity of lifeforms during the early Cambrian is called the Cambrian explosion of life.[6][7]

While land seems to have been devoid of plants and animals, cyanobacteria and other microbes formed prokaryotic mats that covered terrestrial areas.[8]

Planetary environment and the oxygen catastrophe

Weathered Precambrian pillow lava in the Temagami Greenstone Belt of the Canadian Shield

Evidence of the details of plate motions and other tectonic activity in the Precambrian has been poorly preserved. It is generally believed that small proto-continents existed prior to 3000 Ma, and that most of the Earth's landmasses collected into a single supercontinent around 1000 Ma. The supercontinent, known as Rodinia, broke up around 600 Ma. A number of glacial periods have been identified going as far back as the Huronian epoch, roughly 2200 Ma. One of the best studied is the Sturtian-Varangian glaciation, around 600 Ma, which may have brought glacial conditions all the way to the equator, resulting in a "Snowball Earth".

The atmosphere of the early Earth is not well understood. Most geologists believe it was composed primarily of nitrogen, carbon dioxide, and other relatively inert gases, and was lacking in free oxygen. There is, however, evidence that an oxygen-rich atmosphere existed since the early Archean.[9]

At present, it is still believed that molecular oxygen was not a significant fraction of Earth's atmosphere until after photosynthetic life forms evolved and began to produce it in large quantities as a byproduct of their metabolism. This radical shift from a chemically inert to an oxidizing atmosphere caused an ecological crisis, sometimes called the oxygen catastrophe. At first, oxygen would have quickly combined with other elements in Earth's crust, primarily iron, removing it from the atmosphere. After the supply of oxidizable surfaces ran out, oxygen would have begun to accumulate in the atmosphere, and the modern high-oxygen atmosphere would have developed. Evidence for this lies in older rocks that contain massive banded iron formations, that were laid down as iron oxides.


A terminology has evolved covering the early years of the Earth's existence, as radiometric dating has allowed real dates to be assigned to specific formations and features.[10] The Precambrian Supereon is divided into three eons: the Hadean (4500–3950 Ma), Archean (4000-2500 Ma) and Proterozoic (2500-541 Ma). See Timetable of the Precambrian.

It has been proposed that the Precambrian should be divided into eons and eras that reflect stages of planetary evolution, rather than the current scheme based upon numerical ages. Such a system could rely on events in the stratigraphic record and be demarcated by GSSPs. The Precambrian could be divided into five "natural" eons, characterized as follows:[12]

  1. Accretion and differentiation: a period of planetary formation until giant Moon-forming impact event.
  2. Hadean: dominated by heavy bombardment from about 4.51 Ga (possibly including a Cool Early Earth period) to the end of the Late Heavy Bombardment period.
  3. Archean: a period defined by the first crustal formations (the Isua greenstone belt) until the deposition of banded iron formations due to increasing atmospheric oxygen content.
  4. Transition: a period of continued iron banded formation until the first continental red beds.
  5. Proterozoic: a period of modern plate tectonics until the first animals.

Precambrian super-continents

The movement of Earth's plates has caused the formation and break-up of continents over time, including occasional formation of a super-continent containing most or all of the landmass. The earliest known super-continent was Vaalbara. It formed from proto-continents and was a super-continent 3.1 billion years ago. Vaalbara broke up c. 2.8 Ga ago. The super-continent Kenorland was formed c. 2.7 Ga ago and then broke sometime after 2.5 Ga into the proto-continent cratons called Laurentia, Baltica, Australia, and Kalahari. The super-continent Columbia or Nuna formed 2.0–1.8 billion years ago and broke up about 1.5–1.3 billion years ago.[13][14] The super-continent Rodinia is thought to have formed about 1 billion years ago, to have embodied most or all of Earth's continents and to have broken up into eight continents around 600 million years ago.

See also


  1. 1 2 James Monroe and Reed Wicander, The Changing Earth, 2nd ed, (Belmont: Wadsworth Publishing Company, 1997), p. 492.
  2. "Pamela J.W. Gore, "The Precambrian". Retrieved on 10/05/11".
  3. "Zircons are Forever". Retrieved 2007-04-28.
  4. Ch. 9 "Chronostratigraphic Units," note C7 and Table 4
  5. Brun, Yves and Lawrence J. Shimkets, Prokaryotic development, ASM Press, Jan. 2000, p. 114 ISBN 978-1-55581-158-7
  6. Fedonkin, Mikhail A.; James G. Gehling; Kathleen Grey; Guy M. Narbonne; Patricia Vickers-Rich (2008). The Rise of Animals: Evolution and Diversification of the Kingdom Animalia. JHU Press. ISBN 9780801886799.
  7. Dawkins, Richard; Yan Wong (2005). The Ancestor's Tale: A Pilgrimage to the Dawn of Evolution. Houghton Mifflin Harcourt. ISBN 9780618619160.
  8. Terrestrialization (Precambrian–Devonian)
  9. Clemmey, Harry; Badham, Nick (1982). "Oxygen in the Precambrian Atmosphere". Geology. 10 (3): 141–146. Bibcode:1982Geo....10..141C. doi:10.1130/0091-7613(1982)10<141:OITPAA>2.0.CO;2.
  10. Geological Society of America's "2009 GSA Geologic Time Scale."
  12. Bleeker, W. (2004) [2004]. "Toward a "natural" Precambrian time scale". In Felix M. Gradstein; James G. Ogg; Alan G. Smith. A Geologic Time Scale 2004. Cambridge University Press. ISBN 0-521-78673-8. also available at Precambrian subcommission
  13. Zhao, Guochun; Cawood, Peter A.; Wilde, Simon A.; Sun, M. (2002). "Review of global 2.1–1.8 Ga orogens: implications for a pre-Rodinia super-continent". Earth-Science Reviews. 59: 125–162. Bibcode:2002ESRv...59..125Z. doi:10.1016/S0012-8252(02)00073-9.
  14. Zhao, Guochun; Sun, M.; Wilde, Simon A.; Li, S.Z. (2004). "A Paleo-Mesoproterozoic super-continent: assembly, growth and breakup". Earth-Science Reviews. 67: 91–123. Bibcode:2004ESRv...67...91Z. doi:10.1016/j.earscirev.2004.02.003.

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