Eltanin impact

The Eltanin impact is thought to be an asteroid impact in the eastern part of the South Pacific Ocean that occurred around the Pliocene-Pleistocene boundary approximately 2.51 ± 0.07  million years ago.[1] The location was at the edge of the Bellingshausen Sea 1,500 km (950 mi) southwest of Chile, with a seafloor depth of approximately 4–5 kilometres (2.5–3.1 mi).[2] The asteroid was estimated to be about one to four km (0.6 to 2.5 mi) in diameter. No crater associated with the impact has been discovered.[3] The impact likely evaporated 150 km3 (36 cu mi) of water, generating large tsunami waves hundreds of metres high.[4]

Eltanin impact
Eltanin impact is located in Atlantic Ocean
Eltanin impact
Eltanin impact
Eltanin site in the southeast Pacific Ocean
Impact crater/structure
ConfidenceHypothetical
Diameter35 km (22 mi)
Impactor diameter1–4 km (0.62–2.49 mi)
Age2.51 ± 0.07 Ma, earliest Pleistocene
Location
Coordinates57°47′S 90°47′W
The possible impact site is located at the edge of the Bellingshausen Sea (part of the Southern Ocean)

Description

The possible impact site was first discovered in 1981 as an iridium anomaly in sediment cores collected by the research vessel Eltanin, after which the site and impactor are named.[5] Later studies were done by the vessel Polarstern.[6] Sediment at the bottom of the five km (3 mi) deep ocean in the area had an iridium enrichment, a strong sign of extraterrestrial contamination. Possible debris from the asteroid is spread over an area of 500 km2 (190 sq mi). Sediments from the Eocene and Paleocene were jumbled and deposited again chaotically. Also mixed in were melted and fragmented meteorite matter. The area near the Freeden Seamounts over 20,000 km2 (7,700 sq mi) has a meteorite material surface density of 10–60 kg/m2 (2.0–12.3 lb/sq ft). Of this, 87% is melted and 13% only fragmented. This area is the region of the Earth's surface with the highest known density of meteorite material coverage.[2]

The disturbed sediment had three layers. The lowermost layer SU IV is a chaotic mixture of crumbled sediments in the form of a breccia. Above this is layer SU III consisting of layered sand, consistent with having been deposited from turbulently flowing water. Above this is SU II layer with meteorite fragments and graded silt and clay that plausibly settled out of still but dirty water.[7]

Asteroid

The supposed impacting body, the Eltanin asteroid, is estimated to have been between one and four km (0.6 and 2.5 mi) in diameter and traveling with a speed of 20 km/s (45,000 mph). The possible size of the asteroid was calculated by the amount of iridium found in the disturbed sediments. Assuming that there were 187 parts per billion of iridium in the asteroid, the known distribution of the metal leads to estimates that the body was over one km (0.6 mi) in size.[8] Based on a diameter of one km, it is estimated it would have left a crater about 35 km (22 mi) across.[3]

The composition of suspected asteroid remnants has been classified as low metal mesosiderites.[7] The bolide explosion would also have produced microspherules under half a millimeter in diameter.[9] Some of these are glass, and others have spinel and pyroxene. Elements enriched include calcium, aluminium and titanium.[2]

Tsunami

On the shorelines of the Pacific Ocean there are erosional features that are indicative of a very large tsunami. These include an erosional surface and chaotic deposits of mixed terrestrial and ocean-derived sediment. Boulders as big as buses are mixed with marine fossils and mud. The most well-characterised tsunami deposits are near the coast of Chile. Off the coast of Antarctica there are mudslides into the deep ocean from this age.[10]

The size of a possible tsunami has been calculated. An asteroid that was four km (two mi) in diameter falling onto the five km (three mi) deep ocean would have blasted the water off the ocean floor for at least 60 km (37 mi), and made a wave over 200 m (660 ft) high on the southern end of Chile and the Antarctic Peninsula. After ten hours, waves around 35 m (115 ft) would reach Tasmania, Fiji and Central America, and the New Zealand east coast would have been washed with 60 m (200 ft) high waves. If the impact object was one km (0.6 mi) in diameter, the wave heights would have been one-fifth as great.[3]

Ice age trigger

At the time of the impact in the Late Pliocene, the Earth was cooling. The impact and disruption to the weather might have helped trigger the start of ice cap formation in the Northern Hemisphere.[11] The impact would have put a large amount of water and salt into the atmosphere, disrupted ice shelves, depleted the ozone layer, caused surface acidification, and increased the Earth's albedo.[12]

See also

References
  1. Goff, James; Catherine Chagué-Goff; Michael Archer; Dale Dominey-Howes; Chris Turney (3 September 2012). "The Eltanin asteroid impact: possible South Pacific palaeomegatsunami footprint and potential implications for the Pliocene-Pleistocene transition". Journal of Quaternary Science. Wiley. 27 (7): 660. Bibcode:2012JQS....27..660G. doi:10.1002/jqs.2571. ISSN 0267-8179. S2CID 131415717.
  2. Gersonde, R.; F. T. Kyte; T. Frederichs; U. Bleil; H. W. Schenke; G. Kuhn (2005). "The late Pliocene impact of the Eltanin asteroid into the Southern Ocean – Documentation and environmental consequences" (PDF). Geophysical Research Abstracts. European Geosciences Union. Retrieved 8 October 2012.
  3. Ward, Steven N.; Erik Asphaug (2002). "Impact tsunami–Eltanin" (PDF). Deep-Sea Research Part II. Elsevier. 49 (6): 1073–1079. Bibcode:2002DSRII..49.1073W. doi:10.1016/s0967-0645(01)00147-3. Archived from the original (PDF) on 5 May 2014. Retrieved 8 October 2012.
  4. Shuvalov, Valery; Gersonde, Rainer (2014). "Constraints on interpretation of the Eltanin impact from numerical simulations". Meteoritics & Planetary Science. 49 (7): 1171–1185. Bibcode:2014M&PS...49.1171S. doi:10.1111/maps.12326. ISSN 1945-5100. S2CID 140649899.
  5. Kyte, Frank T.; Zhiming Zhou; John T. Wasson (1981). "High noble metal concentrations in a late Pliocene sediment". Nature. 292 (5822): 417–420. Bibcode:1981Natur.292..417K. doi:10.1038/292417a0. ISSN 0028-0836. S2CID 4362591.
  6. Gersonde, R.; F. T. Kyte; U. Bleil; B. Diekmann; J. A. Flores; K. Gohl; G. Grahl; R. Hagen; et al. (1997). "Geological record and reconstruction of the late Pliocene impact of the Eltanin asteroid in the Southern Ocean" (PDF). Nature. 390 (6658): 357–363. Bibcode:1997Natur.390..357G. doi:10.1038/37044. ISSN 0028-0836. PMID 11536816. S2CID 4332536.
  7. Kyte, Frank T.; Rainer Gersonde; Gerhard Kuhn (2005). "SEDIMENTATION PATTERNS OF METEORITIC EJECTA IN ELTANIN IMPACT DEPOSITS AT SITE PS58/281" (PDF). Lunar Science and Planetary Conference XXXVII. Houston Texas. Retrieved 8 October 2012.
  8. Gersonde, Rainer; Frank T. Kyte; T. Frederichs; U. Bleil; Gerhard Kuhn (2003). "New Data on the Late Pliocene Eltanin Impact into the Deep Southern Ocean" (PDF). Large Meteorite Impacts. Retrieved 8 October 2012.
  9. Kyte, Frank T.; Chikako Omura; Christopher Snead; Kevin D. McKeegan; Rainer Gersonde (2010). "Trace Elements in Refactory Eltanin Impact Spherules" (PDF). 41st Lunar and Planetary Science Conference. Retrieved 8 October 2012.
  10. Gary, Stuart; James Goff (26 September 2012). "Earth's ice age asteroid". Starstuff. ABC radio. Retrieved 8 October 2012.
  11. University of New South Wales (19 September 2012). "Did a Pacific Ocean meteor trigger the Ice Age?". Retrieved 8 October 2012.
  12. Gersonde, Reiner (2 March 2000). "Oceanic Impacts and Related Environmental Perturbations" (PDF). Catastrophic Events Conference. Retrieved 8 October 2012.
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