|Diameter||60–160 km (37–99 mi)|
|Age||364 ± 8 Ma|
Late Devonian to Early Carboniferous
Woodleigh is a large meteorite impact crater (astrobleme) in Western Australia, centred on Woodleigh Station east of Shark Bay, Gascoyne region. A team of four scientists at the Geological Survey of Western Australia and the Australian National University, led by Arthur J. Mory, announced the discovery in the 15 April 2000 issue of Earth and Planetary Science Letters.
The crater is not exposed at the surface and therefore its size is uncertain. The original discovery team stated in 2000 that it may be up to 120 km (75 mi) in diameter, but others argue it may be much smaller, with one 2003 study suggesting a diameter closer to 60 km (37 mi). The larger estimate of 120 km, if correct, would make this crater tied for the fourth largest confirmed impact structure in the world, and imply a bolide (asteroid or comet) about 5 to 6 km (3.1 to 3.7 mi) in diameter. A more recent study in 2010 suggests the crater could be between 60 and 160 kilometres (37 and 99 mi) or more, and was produced by a comet or asteroid 6 to 12 kilometres (3.7 to 7.5 mi) wide.
The central uplift, interpreted to be 20 km (12 mi) in diameter, was first intersected by drilling activities in the late 1970s; however its significance as an impact structure was only realised in 1997 during a gravity survey. In 1999, a new core sample was taken. The thin veins of melted glass, breccia, and shocked quartz found would have formed under pressures 100,000 times greater than atmospheric pressure at sea level, or between 10 and 100 times greater than those generated by volcanic or earthquake activity. Only a large impact could have generated such conditions. The reported discovery in 2018 of the extremely rare mineral reidite in a drillcore sample from the central uplift zone, supports the interpretation of the crater as being over 100 km in diameter, and possibly the largest in Australia.
The Woodleigh impact event, originally thought to have occurred between the Late Triassic and Late Permian, is now thought to date from 364 ± 8 million years (Late Devonian). This time corresponds approximately to the Late Devonian extinction. There is evidence for other large impact events at around the same time, such as the East Warburton Basin, so if the extinction is related to impact, perhaps more than one crater was involved.
Of the two dozen or more impact craters known in Australia, the three largest are Woodleigh, Acraman, and Tookoonooka. The Gnargoo structure, which has remarkable similarities to Woodleigh, is a nearby proposed impact crater on the Gascoyne platform.
- Mory AJ, Iasky RP, Glikson AY, Pirajno F (2000). "Woodleigh, Carnarvon Basin, Western Australia: a new 120 km diameter impact structure". Earth and Planetary Science Letters. 117 (1–2): 119–128. Bibcode:2000E&PSL.177..119M. doi:10.1016/S0012-821X(00)00031-5. Abstract
- Reimold WU, Koeberl C, Hough RM, Mcdonald I, Bevan A, Amare K, French BM (2003). "Woodleigh impact structure, Australia: Shock petrography and geochemical studies". Meteoritics & Planetary Science. 38 (7): 1109–1130. Bibcode:2003M&PS...38.1109R. doi:10.1111/j.1945-5100.2003.tb00301.x. Abstract and full PDF
- Mory A, Iasky R (2000). Woodleigh — Australia's largest impact structure?. Fieldnotes, Geological Survey of Western Australia. 16. pp. 1–2. ISBN 978-0-7307-5642-2. PDF Archived 23 August 2006 at the Wayback Machine
- Gareth Barton (27 October 2010). "Giant crater may have been extinction trigger". Cosmos. Archived from the original on 12 October 2016. Retrieved 15 August 2012.
- Discovery of reidite, one of the rarest minerals on Earth, may reveal Australia's biggest crater ABC News, 16 October 2018. Retrieved 17 October 2018.
- "Woodleigh". Earth Impact Database. Planetary and Space Science Centre University of New Brunswick Fredericton. Retrieved 9 October 2017.
- R. Iaskty and A. Glikson (2005). "Gnargoo: a possible 75 km-diameter post-Early Permian – pre-Cretaceous buried impact structure, Carnarvon Basin, Western Australia", Australian Journal of Earth Sciences, Vol 52, 2005