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Nördlinger Ries

Coordinates:48°53′N10°34′E / 48.883°N 10.567°E /48.883; 10.567
From Wikipedia, the free encyclopedia
Meteorite impact crater in Bavaria, Germany
For human settlement within the Nördlinger Ries region, seeDonau-Ries.
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Nördlinger Ries
Relief map of Nördlinger Ries
Impact crater/structure
ConfidenceConfirmed
Diameter24 km (15 mi)
Age14.808 ± 0.038 Ma, MiddleMiocene
ExposedYes
DrilledYes
Bolide typeAchondrite
Location
Coordinates48°53′N10°34′E / 48.883°N 10.567°E /48.883; 10.567
CountryGermany
StateBavaria andBaden-Württemberg
DistrictDonau-Ries
MunicipalityNördlingen
Nördlinger Ries is located in Germany
Nördlinger Ries
Location of the crater in Germany

TheNördlinger Ries (German pronunciation:[ˈnœʁtlɪŋɐˈʁiːs]) is animpact crater[1] and large circular depression in westernBavaria and easternBaden-Württemberg. It is located north of theDanube in the district ofDonau-Ries. The city ofNördlingen is located within the depression, about 6 kilometres (3.7 mi) south-west of its centre.

Etymology

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Ries is derived fromRaetia, since the tribe ofRaetians lived in the area in pre-Roman times.[2][3]

Description

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View ofNördlinger Ries
Suevite fromNördlinger Ries

The depression is ameteoriteimpact crater formed 14.808 ± 0.038 million years ago in theMiocene.[4][5] The crater is most commonly referred to simply as theRies crater orthe Ries. The original crater rim had an estimated diameter of 24 km (15 mi). The present floor of the depression is about 100 to 150 m (330 to 490 ft) below the eroded remains of the rim.

It was originally assumed that the Ries was ofvolcanic,glacial ortectonic origin. Oliver Sachs introduced, in this context, the term "pioneer era" (up to 1870) and marked the beginning of early modern research on the Ries (from 1870), meaning the period when the first detailed theories about the formation of the Nördlinger Ries became known.[6][7][8] In 1960Eugene Shoemaker andEdward C. T. Chao showed that the depression was caused by meteorite impact.[9] The key evidence was the presence ofcoesite, which, inunmetamorphosed rocks, can only be formed by theshock pressures associated with meteorite impact. The coesite was found insuevite fromOtting quarry,[10][9] but even before, Shoemaker was encouraged by St. George's Church inNördlingen, which is built of locally derived suevite.[10] The suevite was formed from mesozoic sediments shocked by thebolide impact.[11][12][13]

The Ries impact crater was arampart crater, thus far a unique finding on Earth.[14] Rampart craters have almost exclusively been found onMars. Rampart craters exhibit a fluidized ejecta flow after the impact of the meteorite, most simply compared to a bullet fired into the mud, with the ejecta resembling amudflow.

Another impact crater, the much smaller (3.8 km (2.4 mi) diameter)Steinheim crater,[15] is located about 42 km (26 mi) west-southwest from the center of Ries. It had previously been thought that the two craters formed simultaneously by the impact of abinary asteroid 14.8 million years ago, but a study published in 2020 suggests that Steinheim could actually be about 500,000 years younger thanNördlinger Ries.[16]

Recent computer modeling of the impact event indicates that the impactors probably had diameters of about 1.5 km (4,900 ft) (Ries) and 150 m (490 ft) (Steinheim), had a pre-impact separation of some tens of kilometers, and impacted the target area at an angle around 30 to 50 degrees from the surface in a west-southwest to east-northeast direction.[citation needed] The impact velocity is thought to have been about 20 km/s (72,000 km/h; 45,000 mph).[citation needed] The resulting explosion had the power of 40 millionHiroshima bombs, an energy of roughly 2.4×1021joules.[citation needed]

The Ries crater impact event is believed to be the source ofmoldavitetektites found in southernBohemia andMoravia (Czech Republic).[17] The tektite melt originated from a sand-rich surface layer that was ejected to distances up to 450 km (280 mi) downrange of the crater. The shape of the strewnfield suggests that the direction of impact was from thewest-southwest.[18]

Stone buildings in Nördlingen contain millions of tinydiamonds, all less than 0.2 mm (0.008 in) across. The impact that caused the Nördlinger Ries crater created an estimated 72,000tonnes (72,000,000 kg) of them when it impacted a localgraphite deposit. Stone from this area was quarried and used to build the local buildings.[19]

History

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On one edge of the Nördlinger Ries are theOfnet Caves, where, at the beginning of the 20th century, archaeologists discovered thirty-three human skulls dating to theMesolithic period.[20]

The Ries was the site of theBattle of the Ries on 13 May 841.

The landing site forApollo 14 is a heavily craterized terrain, and one of the science goals of the mission was to sample ejecta from the impact that formedMare Imbrium.Nördlinger Ries is an easily accessible, large impact crater, making it a convenient analog for lunar craters. Because of this, it was used as a location to train Apollo 14 astronauts, so that they would be able to investigate lunar impact structures and related rocks.[21] AstronautsAlan Shepard andEdgar Mitchell, as well as Apollo 14 backup astronautsEugene Cernan andJoe Engle, trained here from August 10 to August 14, 1970.[22]

In popular culture

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References

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  1. ^J. Baier:Geohistorische Bemerkungen zur Suevit-Forschung (Ries-Impakt). Geohistorische Blätter, 31(1/2), Berlin 2020.
  2. ^"37 Ries"(PDF).Entwurf einer kulturlandschaftlichen Gliederung Bayerns als Beitrag zur Biodiversität. Bayerisches Landesamt für Umwelt. 2011. Archived fromthe original(PDF) on 2018-12-12.
  3. ^Schmidt F. G. G.[in German] (1896). "The Dialect of the Ries".Modern Language Notes.11 (5):142–144.doi:10.2307/2918785.JSTOR 2918785.
  4. ^Schmieder, Martin; Kennedy, Trudi; Jourdan, Fred; Buchner, Elmar; Reimold, Wolf Uwe (2018)."A high-precision 40Ar/39Ar age for the Nördlinger Ries impact crater, Germany, and implications for the accurate dating of terrestrial impact events".Geochimica et Cosmochimica Acta.220:146–157.Bibcode:2018GeCoA.220..146S.doi:10.1016/j.gca.2017.09.036.
  5. ^Schwarz, Winfried H.; Hanel, Michael; Trieloff, Mario (February 2020)."U–Pb dating of zircons from an impact melt of the Nördlinger Ries crater".Meteoritics & Planetary Science.55 (2):312–325.Bibcode:2020M&PS...55..312S.doi:10.1111/maps.13437.ISSN 1086-9379.S2CID 214304156.
  6. ^O. Sachs:Einige wiederentdeckte geologische Kartenwerke zum Nördlinger Ries und ihre Beziehung zu den frühesten Entstehungstheorien in der Pionierzeit der Riesforschung vor 1870. In: Jahresberichte und Mitteilungen des Oberrheinischen Geologischen Vereins. 102, 2020, pages 234–266,doi:10.1127/jmogv/102/0012.
  7. ^O. Sachs:Geologische Landeskarten des Königreichs von Württemberg und die Zeit der „Württembergischen Commission der geologischen Detailaufnahme“ am Beispiel der beiden Impaktkrater Steinheimer Becken und Nördlinger Ries. In: Jahresberichte und Mitteilungen des Oberrheinischen Geologischen Vereins. 103, 2021, S. 113–152,doi:10.1127/jmogv/103/0002.
  8. ^O. Sachs:Von der Pionierzeit zur frühen Moderne der geologischen Riesforschung: Die vergessenen Karten des Nördlinger Rieses bis 1870. In: Rieser Kulturtage. 23, 2023, S. 29–96.
  9. ^abShoemaker, EM; Chao, ECT (1961). "New Evidence for the Impact Origin of the Ries Basin, Bavaria, Germany".Journal of Geophysical Research.66 (10):3371–3378.Bibcode:1961JGR....66.3371S.doi:10.1029/JZ066i010p03371.
  10. ^abCokinos C. (2009).The Fallen Sky. Penguin.ISBN 9781101133224.
  11. ^Baier, Johannes (2007). "Die Auswurfprodukte des Ries-Impakts, Deutschland".Documenta Naturae (in German).162. München.ISBN 978-3-86544-162-1.
  12. ^Baier, Johannes (2008). "Zur Herkunft der Suevit-Grundmasse des Ries-Impakt Kraters".Documenta Naturae (in German).172. Munich.ISBN 978-3-86544-172-0.
  13. ^Baier, Johannes (2012)."Die Bedeutung von Wasser während der Suevit-Bildung (Ries-Impakt, Deutschland)".Jber. Mitt. Oberrhein. Geol. Ver. (in German).94:55–69.
  14. ^Sturm, Sebastian; Wulf, Gerwin; Jung, Dietmar; Kenkmann, Thomas (2013). "The Ries impact, a double-layer rampart crater on Earth".Geology.41 (5):531–534.Bibcode:2013Geo....41..531S.doi:10.1130/G33934.1.
  15. ^Baier, Johannes; Scherzinger, Armin (2010)."Der neue Geologische Lehrpfad im Steinheimer Impakt-Krater".Jber. Mitt. Oberrhein. Geol. Ver (in German).92:9–24.
  16. ^Buchner, E.; Sach, VJ; Schmieder, M (2020)."New discovery of two seismite horizons challenges the Ries–Steinheim double-impact theory".Scientific Reports.10 (1): 22143.Bibcode:2020NatSR..1022143B.doi:10.1038/s41598-020-79032-4.PMC 7747748.PMID 33335157.
  17. ^Graup, Günther; Horn, Peter; Köhler, Horst; Müller-Sohnius, Dieter (1981). "Source material for moldavites and bentonites".Naturwissenschaften.67 (12). Berlin: 616.Bibcode:1981NW.....68..616G.doi:10.1007/BF00398615.S2CID 11282087.
  18. ^Holm-Alwmark, Sanna; Alwmark, Carl; Ferrière, Ludovic; Meier, Matthias M. M.; Lindström, Sofie; Kenny, Gavin G.; Sheldon, Emma; Schweigert, Günter; Spötl, Christoph; Whitehouse, Martin J.; Hofmann, Beda A. (2021-04-02)."Shocked quartz in distal ejecta from the Ries impact event (Germany) found at ~180 km distance, near Bernhardzell, eastern Switzerland".Scientific Reports.11 (1): 7438.Bibcode:2021NatSR..11.7438H.doi:10.1038/s41598-021-86685-2.ISSN 2045-2322.PMC 8018947.PMID 33811229.
  19. ^Emsley, John (2001).Nature's Building Blocks.Oxford University Press. p. 99.ISBN 0-19-850341-5.
  20. ^Onians, R. B. (1988).The Origins of European Thought.Cambridge University Press. p. 541.ISBN 978-0521347945.
  21. ^Pondrelli, Monica; Baker; Hauber (2018)."Geologic Tools".Planetary Geology. Springer. pp. 15–31.doi:10.1007/978-3-319-65179-8_2.ISBN 978-3-319-65177-4.
  22. ^Phinney, William (2015).Science Training History of the Apollo Astronauts. NASA SP-2015-626. p. 237.
  23. ^May, Julian (1984).A Pliocene Companion: The essential readers' guide to theSaga of the Exiles.Pan Books. p. 101.ISBN 0330289861.

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