Chaotian (geology)

Last updated
Chaotian
4568 – 4404 Ma
Chronology
Subdivisions See text
Usage information
Celestial body Earth
Regional usageProposed subdivision of the Hadean eon
Definition
Chronological unit Era
Stratigraphic unit Erathem
First proposed byC., Zahnle, K. J., Sleep, N. H., and Nisbet, E. G., 2010
Lower boundary definitionFormation of the Earth
Upper boundary definitionCollision between Proto-Earth and the Protoplanet Theia

The Chaotian is a proposed time division of the geologic time scale. First proposed in 2010 [1] as an eon, it is named after Chaos, the primeval void in Greek mythology. This proposal defines the Chaotian eon as a Solar System-wide time between the initiation of planetary formation and the hypothesised collision of the trojan dwarf planet Theia with the proto-Earth.

Contents

A revised proposal in 2012 [2] suggested the Chaotian as the first era of the Hadean representing the time between the formation of the Solar System c. 4.567  Ga [3] and the oldest preserved crustal material on Earth, a detrital zircon c. 4.404 Ga [4] from the Jack Hills of the Narryer Terrane in Western Australia.

As of September 2023, neither proposal had been adopted or officially ratified by the International Union of Geological Sciences. [5]

Subdivisions

The original proposal in 2010 divided the Chaotian into two eras and four periods. No numerical upper age limits were provided, only the younger age limit of ~4.5 Ga for the boundary between the proposed Chaotian and Hadean boundary.

The revised proposal in 2012 did not subdivide the proposed Chaotian era (of the Hadean eon) into periods.

Proposed Chaotian time intervals (2010) [1]
EonEraPeriodAge (Ga)
ChaotianNeochaotianTitanomachaen> ~4.5
Hyperitian
EochaotianErebrean
Nephelean
Proposed Chaotian time intervals (2012) [2]
EonEraAge (Ga)
Hadean Jack Hillsian or Zirconian 4.404 to 4.030
Chaotian4.568 to 4.404

See also

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References

  1. 1 2 Goldblatt, C.; Zahnle, K.J.; Sleep, N.H.; Nisbet, E.G. (2 February 2010). "The Eons of Chaos and Hades". Solid Earth. 1 (1): 1–3. Bibcode:2010SolE....1....1G. doi: 10.5194/se-1-1-2010 .
  2. 1 2 Van Kranendonk, Martin J. (2012), "A Chronostratigraphic Division of the Precambrian", The Geologic Time Scale, Altermann, Wladyslaw; Beard, Brian L.; Hoffman, Paul F.; Johnson, Clark M.; Kasting, James F.; Melezhik, Victor A.; Nutman, Allen; Papineau, Dominic; Pirajno, Franco, Elsevier, pp. 299–392, doi:10.1016/b978-0-444-59425-9.00016-0, ISBN   978-0-444-59425-9 , retrieved 2020-07-31
  3. Connelly, J.N.; Bollard, J.; Bizzarro, M. (2017). "Pb–Pb chronometry and the early Solar System". Geochimica et Cosmochimica Acta. 201: 345–363. Bibcode:2017GeCoA.201..345C. doi: 10.1016/j.gca.2016.10.044 .
  4. Wilde, Simon A.; Valley, John W.; Peck, William H.; Graham, Colin M. (11 January 2001). "Evidence from detrital zircons for the existence of continental crust and oceans on the Earth 4.4 Gyr ago". Nature. 409 (6817): 175–178. Bibcode:2001Natur.409..175W. doi:10.1038/35051550. PMID   11196637. S2CID   4319774.
  5. "International Commission on Stratigraphy".