Glasford crater

Last updated
Glasford crater
Glasford crater 20231022 0061.jpg
Site of crater from south, at intersection of Cowser and Kingston Mines Rds.
Impact crater/structure
ConfidenceConfirmed
Diameter4 kilometres (2.5 mi)
Depth350 metres (1,150 ft)
Age < 430 Ma
ExposedNo
DrilledYes
Location
Coordinates 40°36′N89°47′W / 40.600°N 89.783°W / 40.600; -89.783
CountryUSA
StateIllinois
Municipality Glasford, Illinois

The Glasford crater, also known as the Glasford Disturbance, Glasford Structure, [1] and Glasford Cryptoexplosion Structure [2] , is a buried impact crater in southern Peoria County, Illinois, in the United States. [3] It is one of two known meteor craters in Illinois. [4]

It is 4 kilometers (2.5 mi) in diameter and the age is estimated to be less than 430 million years (Silurian or younger). [5] [6] It was formed in a marine environment in the Late Ordovician period. [7] [8] The meteorite is estimated between 50 and 90 million tons and likely originated in the asteroid belt between Mars and Jupiter. [9]

The Glasford crater was discovered by the Central Illinois Light Company (formerly CILCO, now Ameren) while drilling wells for underground natural gas storage. [10] [11] It is not visible from the surface, as it is covered by agricultural farmland. [12] [11] The present day location is near the intersection of Cowser and Kingston Mines roads. [9] It was identified in 1963 as a probable impact structure. [5] [13] In the 1980s, scientists identified shatter cones. [5] Geologists estimate the meteor released a large amount of energy, roughly equivalent to 20,000 nuclear bombs, 460 million tons of TNT, or two to three times the energy of the Mount St. Helens eruption. [11] [9]

According to research by geologist Charles Monson, the Glasford crater may be connected to the Great Ordovician Meteor Shower. [14] Dr. Birger Schmitz's study suggests that the dust from the meteor impact may have impacted Earth's climate and contributed to the mid-Ordovician Ice Age. [4] [14]

Related Research Articles

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An impact crater is a circular depression in the surface of a solid astronomical object formed by the hypervelocity impact of a smaller object. In contrast to volcanic craters, which result from explosion or internal collapse, impact craters typically have raised rims and floors that are lower in elevation than the surrounding terrain. Lunar impact craters range from microscopic craters on lunar rocks returned by the Apollo program and small, simple, bowl-shaped depressions in the lunar regolith to large, complex, multi-ringed impact basins. Meteor Crater is a well-known example of a small impact crater on Earth.

<span class="mw-page-title-main">Meteorite</span> Solid debris from outer space that hits a planetary surface

A meteorite is a solid piece of debris from an object, such as a comet, asteroid, or meteoroid, that originates in outer space and survives its passage through the atmosphere to reach the surface of a planet or moon. When the original object enters the atmosphere, various factors such as friction, pressure, and chemical interactions with the atmospheric gases cause it to heat up and radiate energy. It then becomes a meteor and forms a fireball, also known as a shooting star; astronomers call the brightest examples "bolides". Once it settles on the larger body's surface, the meteor becomes a meteorite. Meteorites vary greatly in size. For geologists, a bolide is a meteorite large enough to create an impact crater.

<span class="mw-page-title-main">Meteor Crater</span> Meteorite impact crater in northern Arizona

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<span class="mw-page-title-main">Impact event</span> Collision of two astronomical objects

An impact event is a collision between astronomical objects causing measurable effects. Impact events have physical consequences and have been found to regularly occur in planetary systems, though the most frequent involve asteroids, comets or meteoroids and have minimal effect. When large objects impact terrestrial planets such as the Earth, there can be significant physical and biospheric consequences, though atmospheres mitigate many surface impacts through atmospheric entry. Impact craters and structures are dominant landforms on many of the Solar System's solid objects and present the strongest empirical evidence for their frequency and scale.

<span class="mw-page-title-main">Glasford, Illinois</span> Village in Illinois, United States

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<span class="mw-page-title-main">Kaali crater</span> Group of nine impact craters in Estonia

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<span class="mw-page-title-main">Neugrund crater</span> Meteorite crater in Estonia

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<span class="mw-page-title-main">Rock Elm Disturbance</span>

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<span class="mw-page-title-main">Sierra Madera crater</span>

Sierra Madera crater is a meteorite crater (astrobleme) in southwestern Pecos County, Texas, United States. The central peak of the rebound structure of the impact crater rises 793 ft (242 m) above the surrounding land. The peak is visible from U.S. Highway 385 between Fort Stockton, Texas and Marathon, Texas. The Sierra Madera crater is located on private property on the La Escalera Ranch.

<span class="mw-page-title-main">Grove Karl Gilbert</span> American geologist (1843–1918)

Grove Karl Gilbert, known by the abbreviated name G. K. Gilbert in academic literature, was an American geologist.

In geology, a cryptoexplosion structure is an explosion of unknown cause. The term is now largely obsolete. It was once commonly used to describe sites where there was geological evidence of a large-scale explosion within the Earth's crust, but no definitive evidence for the cause such as normal volcanic rocks. These sites are usually circular with signs of anomalous rock deformation contrasting with the surrounding region, and often showing evidence that crustal material had been uplifted and/or blown outwards. The assumption was that some unusual form of volcanism, or a gas explosion originating within the crust, was the cause. The use of the term went away with the rise of the science of impact crater recognition in the late 20th century. Most structures described as cryptoexplosions turned out to be eroded impact craters, caused by the impact of meteorites. Today geologists discount former cryptoexplosion theories.

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The Santa Fe impact structure is an eroded remnant of a bolide impact crater in the Sangre de Cristo Mountains northeast of Santa Fe, New Mexico. The discovery was made in 2005 by a geologist who noticed shatter cones in the rocks in a decades-old road cut on New Mexico State Road 475 between Santa Fe and Hyde Memorial State Park. Shatter cones are a definitive indicator that the rocks had been exposed to a shock of pressures only possible in a meteor impact or a nuclear explosion.

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The Ordovician meteor event was a dramatic increase in the rate at which L chondrite meteorites fell to Earth during the Middle Ordovician period, about 467.5±0.28 million years ago. This is indicated by abundant fossil L chondrite meteorites in a quarry in Sweden and enhanced concentrations of ordinary chondritic chromite grains in sedimentary rocks from this time. This temporary increase in the impact rate was most likely caused by the destruction of the L chondrite parent body 468 ± 0.3 million years ago having scattered fragments into Earth-crossing orbits, a chronology which is also supported by shock ages in numerous L chondrite meteorites that fall to Earth today. It has been speculated that this influx contributed to, or possibly even instigated, the Great Ordovician Biodiversification Event, although this has been questioned.

References

  1. Freeberg, Jacquelyn H. (1966). Terrestrial impact structures: a bibliography. Washington: U.S. Govt. Print. Off. p. 42.
  2. Ryan, Robert; Buschbach, T. C. (1963). "Tectonic History of the Glasford Cryptoexplosion Structure: ABSTRACT". AAPG Bulletin. 47 (2): 368–369. ISSN   0149-1423.
  3. "Glasford". Earth Impact Database . Planetary and Space Science Centre University of New Brunswick Fredericton . Retrieved 2009-08-13.
  4. 1 2 Jolley, Tiffany (2019-11-12). "Prairie Research Institute News". blogs.illinois.edu. Retrieved 2023-10-02.
  5. 1 2 3 Monson, Charles C.; Sweet, Dustin; Segvic, Branimir; Zanoni, Giovanni; Balling, Kyle; Wittmer, Jacalyn M.; Ganis, G. Robert; Cheng, Guo (2019). "The Late Ordovician (Sandbian) Glasford structure: A marine‐target impact crater with a possible connection to the Ordovician meteorite event". Meteoritics & Planetary Science. 54 (12): 2927–2950. doi:10.1111/maps.13401. ISSN   1086-9379. OSTI   1767765. S2CID   210296191 via Wiley.
  6. "Glasford". www.passc.net. Retrieved 2023-10-02.
  7. Alwmark, C; Monson, C.C. (2021). "The Late Ordovician (Sandbian) Glasford structure: A marine‐target impact crater with a possible connection to the Ordovician meteorite event". 52nd Lunar and Planetary Science Conference 2021. 54 (12): 2927–2950. doi:10.1111/maps.13401. OSTI   1767765. S2CID   210296191.
  8. Buschbach, Robert Ryan T. C. (1963). "Ordovician Explosion Structure at Glasford, Illinois". AAPG Bulletin. 47 via ResearchGate.
  9. 1 2 3 "Meteor cratered central Illinois". Burlington Hawk Eye. 1999-09-20. p. 4.
  10. Meteorite Research - Progress Report Archived 2006-05-24 at the Wayback Machine , Research Subcommittee, Associate Committee on Meteorites, National Research Council of Canada, 1967
  11. 1 2 3 Vlahos, Nick (2017-02-20). "Nick in the AM: When a meteor landed near Glasford". Peoria Journal Star. Retrieved 2023-10-02.
  12. "GLASFORD IMPACT STRUCTURE – Crater Explorer" . Retrieved 2023-10-02.
  13. "Where Meteor Crashed Near Glasford". Peoria Journal Star. 1963-04-09.
  14. 1 2 Shelley, Tim (2019-11-19). "Glasford Meteor May Have Played A Role in Ancient Ice Age". WCBU Peoria. Retrieved 2023-10-02.