Largest craters on Earth[change | edit source]
The five largest confirmed impact structures are:
- Vredefort crater, South Africa: 300 km diameter, 2023 million years ago.
- Sudbury Basin, Ontario, Canada: 250 km diameter, 1850 million years ago.
- Chicxulub crater, Mexico: 170 km diameter, 65 million years ago.
- Popigai crater, Russia: 100 km diameter, 35.7 million years ago.
- Manicouagan crater, Quebec, Canada: 100 km diameter, 214 million years ago.
There are some other suggested impact structures which are larger. It is a feature of the Earth that climate, weathering and plate tectonics removes most of the older features and events. In comparison, the Moon retains a nearly complete record of its past impact events. The implication is that the Earth once suffered a similar bombardment in its early history. This period is known as the Late Heavy Bombardment, because it occurred after the Earth and Moon formed.
Largest unconfirmed craters[change | edit source]
Any of these may or may not be meteorite craters:
- Australian impact structure, Northern Territory, Australia: multiple rings 500 km – 2000 km, 545 million years ago at the Neoproterozoic/Cambrian boundary. Highly speculative at present.
- Shiva crater, Indian Ocean, west of India: ~600 km length, 400 km width, 65 million years ago. Obviously this is of high interest, because of the date.
- Ross crater, Antarctica: 550 km, Oligocene
- Cheko, Siberia, Russia: ~500 km diameter, ~100 million years ago.
- Wilkes Land crater, Antarctica: 485 km. Date unknown, but <500 mya and >100 mya.
- Bedout, Indian Ocean near Western Australia: 200 km, 250 million years ago.
Largest named craters in the Solar System[change | edit source]
- North Polar Basin/Borealis Basin (disputed) – Mars – Diameter: 10,600 km
- South Pole–Aitken basin – Moon – Diameter: 2,500 km
- Hellas Basin – Mars – Diameter: 2,100 km
- Caloris Basin – Mercury – Diameter: 1,550 km
- Imbrium Basin – Moon – Diameter: 1,100 km
Identifying impact craters[change | edit source]
- A layer of shattered rock under the floor of the crater. This layer is called a 'breccia lens'.
- Shatter cones, which are chevron-shaped impressions in rocks. Such cones are formed most easily in fine-grained rocks.
- High-temperature rock types, including laminated and welded blocks of sand, tektites, or glassy spatters of molten rock. They may have relatively large amounts of trace elements that are associated with meteorites, such as nickel, platinum, iridium, and cobalt.
- Microscopic pressure deformations of minerals. These include fracture patterns in crystals of quartz and feldspar, and formation of high-pressure materials such as diamond, derived from graphite and other carbon compounds, or varieties of shocked quartz.
References[change | edit source]
- Earth Impact Database
- French B.M. 1998. Traces of catastrophe: a handbook of shock-metamorphic effects in terrestrial meteorite impact structures. LPI Contribution #954. Houston, Texas, USA: Lunar and Planetary Institute. 
- Breccia is a rock composed of broken fragments of minerals or rock cemented together by a fine-grained matrix,
- Shatter cones are rare geological features that are only known to form in the bedrock beneath meteorite impact craters or underground nuclear explosions. They are evidence that the rock has been subjected to a high-pressure shock.
- Sagy A.; Fineberg J.; Reches Z. (2004). "Shatter cones: branched, rapid fractures formed by shock impact". Journal of Geophysical Research 109: B10209. doi:10.1029/2004JB003016. http://web.cocc.edu/breynolds/classes/UO_Geol_353/shatter%20cones.pdf.
- French, Bevan M. (2005). "Stalking the wily shatter cone: a critical guide for impact-crater hunters" (pdf). Impacts in the Field (Impact Field Studies Group) 2 (Winter): s 3–10. http://web.eps.utk.edu/~faculty/ifsg_files/newsletter/Winter_2005.pdf