C., Zahnle, K. J., Sleep, N. H., and Nisbet, E. G., 2010
Lower boundary definition
Formation of the Earth
Upper boundary definition
Collision 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.
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]
Eon
Era
Period
Age (Ga)
Chaotian
Neochaotian
Titanomachaen
> ~4.5
Hyperitian
Eochaotian
Erebrean
Nephelean
Proposed Chaotian time intervals (2012) [2]
Eon
Era
Age (Ga)
Hadean
Jack Hillsian or Zirconian
4.404 to 4.030
Chaotian
4.568 to 4.404
See also
Age of the Earth
Formation and evolution of the Solar System
Geologic time scale
References
↑ 1.01.1Goldblatt, C.; Zahnle, K.J.; Sleep, N.H.; Nisbet, E.G. (2 February 2010). "The Eons of Chaos and Hades". Solid Earth1 (1): 1–3. doi:10.5194/se-1-1-2010. Bibcode: 2010SolE....1....1G. https://www.solid-earth.net/1/1/2010/se-1-1-2010.html.
↑ 2.02.1Van Kranendonk, Martin J. (2012), Altermann, Wladyslaw; Beard, Brian L.; Hoffman, Paul F.; Johnson, Clark M.; Kasting, James F.; Melezhik, Victor A.; Nutman, Allen; Papineau, Dominic; Pirajno, Franco, "A Chronostratigraphic Division of the Precambrian" (in en), The Geologic Time Scale (Elsevier): pp. 299–392, doi:10.1016/b978-0-444-59425-9.00016-0, ISBN 978-0-444-59425-9, https://linkinghub.elsevier.com/retrieve/pii/B9780444594259000160, retrieved 2020-07-31
↑Connelly, J.N.; Bollard, J.; Bizzarro, M. (2017). "Pb–Pb chronometry and the early Solar System" (in en). Geochimica et Cosmochimica Acta201: 345–363. doi:10.1016/j.gca.2016.10.044.
↑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". Nature409 (6817): 175–178. doi:10.1038/35051550. PMID 11196637. Bibcode: 2001Natur.409..175W.
↑https://stratigraphy.org/chart
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Eras
Neoarchean (2.5–2.8 Gya)
Mesoarchean (2.8–3.2 Gya)
Paleoarchean (3.2–3.6 Gya)
Eoarchean (3.6–4 Gya)
Hadean eon (4–4.6 Gya)
kya = thousands years ago. Mya = millions years ago. Gya = billions years ago.
See also: Geologic time scale
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