Burckle Crater

The Burckle crater is an undersea topographic feature about 29 kilometres (18 mi; 16 nmi) in diameter[1] in the southwestern Indian Ocean. A team of Earth scientists called the Holocene Impact Working Group propose the feature to be an impact crater; these claims are disputed by other geologists.[2]

Burckle crater
Burckle crater is located in Indian Ocean
Burckle crater
Burckle crater
Location of Burckle Crater in the Indian Ocean
Impact crater/structure
ConfidenceHypothesized, contested
Diameter~29 km (18 mi; 16 nmi)
Depth3,800 m (12,500 ft)
Age~5000 years (Holocene)
ExposedNo
DrilledNo
Bolide typeUnknown, possibly remains of a comet
Location
Coordinates30.865°S 61.365°E / -30.865; 61.365

Description

The feature is located east of Madagascar and west of Western Australia in the southern Indian ocean, adjacent to the SW Indian Ocean Ridge. Its position was determined in 2006 by the Holocene Impact Working Group using prehistoric chevron dune formations in Australia and Madagascar. Based on the hypothesis these dunes were formed by a megatsunami resulting from an impact, the researchers were able to triangulate the location of Burckle crater. The hypothesis that these chevron dunes were caused by a megatsunami has been challenged by geologists Jody Bourgeois and R. Weiss in 2009. Using a computer model to simulate a tsunami, they argue that the structures are more consistent with aeolian processes.[3] The tsunami origin of these chevrons is also disputed by other Earth scientists.[2]

Other problems with the claim include:

  • The Holocene Impact Working Group has suggested that multiple significant impact events occurred in the past 10,000 years, but astrononomical models indicate that impact events large enough to cause "hazardous tsunamis" should be expected only about once per 100,000 years, making the Working Group's claims improbable enough that they call for very strong evidence.[2]
  • The evidence for their claims is mostly based on the locations of coastal sedimentary deposits that they have identified and termed "chevrons", and interpret as having been caused by run-up from impact-generated megatsunamis. Other geologists before and after the Working Group consider them to be parabolic sand dunes. The chevrons in Madagascar are precisely aligned with the normal prevailing wind direction at the site as shown by modern weather data, implying that they likely were deposited gradually by wind under present-day conditions, as sand dunes, and not in a catastrophic tsunami.[2]
  • The Working Group reported finding nickel and iron splash droplets fused to foraminiferal tests in slides taken from deep ocean cores near Burckle Crater. But this interpretation is problematic because formaminifera tests are calcium carbonate, which chemically decomposes at about 500 degrees C, while nickel and iron melt at temperatures higher than 1400 degrees C. Additionally, comparable splash droplets fused to foraminifera tests have not been reported from any of the sediment studies done near Chicxulub crater.[2]
  • Setting out to identify past impact events by looking for holes in the ground has often proven dubious as a methodology, including the time a sheep watering hole was called "Sirente Crater".[2]

Burckle crater is located at 30.865°S 61.365°E / -30.865; 61.365 in the Indian Ocean and is 3,800 metres (12,500 ft) below the surface.

See also

References

  1. Abbott et al., 2006
  2. Pinter & Ishman, 2008, p.37
  3. Bourgeois & Weiss, 2009

Bibliography

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