Map of the crater
|Diameter||23 km (14 mi)|
The Rochechouart crater is an impact crater. The initial crater morphology has been lost by erosion and there is no crater visible on site. The proper term to designate what remains of the Rochechouart impact crater is Rochechouart impact structure. The term “astrobleme” (wound of star in greek) introduced by R. Dietz since 1947 together with shatter cones as a symptomatic finger print for identifying an eroded impact crater on Earth, is also used to designate the Rochechouart impact structure. In 2008 the French State acknowledged the heritage value of the Rochechouart impact creating the “Réserve Naturelle Nationale de l’astroblème de Rochechouart-Chassenon” on 12 sites representative of characteristics geological features of the impact structure.
The Rochechouart impact is named after the name of the largest city (about 3500 inhabitants) in the area. The latter is located on the western margin of the French Massif Central near the city of Limoges, approximately 350 km south of Paris. Surprisingly, Rochechouart means rock fall in French, quite a unique premonition for naming a city some 1000 years before realizing it is built with impactites and it stands where an asteroid had fallen some 200 million years before. Chassenon, 3 times smaller than Rochechouart, is also a significant locality built in impactites. It was used 2000 years ago for building the monumental Roman baths of Cassinomagus. The name of Chassenon was added to Rochechouart for naming the Natural Reserve for political reasons aiming at pleasing and getting a larger support from the local territories. Since Napoleon, what is nowadays known as the Rochechouart impact structure is traversed by an administrative frontier separating the Charente department (capitol city being Angouleme) from Haute-Vienne (capitol city being Limoges).
The impact origin of the structure has been recognized by F. Kraut in 1969. The occurrence an unusual set of rock types referred as breccias on the crystalline rocks of the Massif Central was reported in the Rochechouart area since the start of geology, in the early 1800s. However, their interpretation either as sedimentary, volcanic, tectonic, or a mix of these, was a major subject of debate until impact became progressively recognized as a geological process in the 1960s.
The impact origin of Rochechouart was definitely confirmed in the mid 1970s with the recognition by P. Lambert of the projectile signal in the various rocks bearing up to 500 times the nickel content of the target rocks. Rochechouart was then the first impact structure to be confirmed by the presence of projectile contamination, in the absence of meteorite debris and in the absence of crater morphology. This is significant because after shock metamorphism has been recognized and used by early impact geologists as the criteria for identifying impact structures in the absence of projectile, the opponent to impact craters on Earth postulated an endogenic process so called cryptovolcanism, capable of creating the extreme shock waves responsible for craters and shock metamorphism. Rochechouart was thus on the list of cryptovolcanic structures. The recognition of a projectile signal at Rochechouart and progressively at other impact structures and especially at the K-T boundary a few years later, definitely terminated the era of cryptovolcanism and skepticism toward impact cratering.
The age of the Rochechouart impact has been and still is a matter of debate. All the techniques available have been used for dating the Rochechouart event and ages have changed with time and evolution of methods techniques. The ages (within the error bars) spans from less than 150 million years to over 240 million years. Since late 1990s the spreading has reduced and the last four determinations (since 2010) are converging toward an age between 203 and 207 million years. in the Rhaetian, two to five million years older than the Triassic-Jurassic boundary.
More age determinations will be realized in the near future at Rochechouart. Essentially all the specialists of the discipline worldwide (including those mentioned above and those involved with the 214 million years catena hypothesis (see below) are gathered as part of the CIRIR group and CIRIR program for taking advantage of the top quality material just recovered from the first ever drilling campaign at Rochechouart. The extraordinary short duration and extreme conditions of impact illustrate one of the causes of uncertainty in dating a geological process, namely the duration of the resetting event. Beyond better understanding what may cause discrepancies between measures and techniques, it is the premise for constraining the cooling kinetics of large impact, relying on precise dating, that is motivating this gathering within the scope of constraining the models and theories related to the possible role of impact craters in the emergence of life on planetary surfaces, including in the first billion years of the Earth.
Hypothetical multiple impact event
Geophysicist David Rowley, working with John Spray and Simon Kelley, suggested that Rochechouart may have been part of a hypothetical multiple impact event which also formed the Manicouagan crater in northern Quebec, Saint Martin crater in Manitoba, Obolon' crater in Ukraine, and Red Wing crater in North Dakota. All of the craters had previously been known and studied, but their paleoalignment had never before been demonstrated. Rowley has said that the chance that these craters could be aligned like this due to chance are nearly zero.
The Rochechouart impact structure is located on the margin of the French Massif Central. The target rocks exposed both in the center of the structure below the deposit, and radially outward are largely dominated by gneisses (blue and green on the map) and granites (pink on the map). These metamorphic and intrusive rocks were emplaced some 350-300 million years ago during the Variscan orogeny. The latter also referred as to Hercynian orogeny is a geologic mountain-building event caused by Late Paleozoic continental collision between the tectonic plates of Euramerica (Laurussia) and Gondwana to form the supercontinent of Pangaea. This caused the raise of Himalaya like mountain ridges of the Massif Central, among others. The mountains were already eroded and transformed into a peneplain at the time of the impact.
The center of the structure is only 15–20 km from the closest sediments. The later were deposited after the impact. Yet the impact has most probably taken place on the margin of the Massif Central forming and island at that time, close enough to the nearby sea to have triggered a prominent tsunami.
The Rochechouart impact structure is composed of central sub circular zone approximately 12 km in diameter exposing breccias and impact melt rocks (represented in grey on the map), and an annular diffuse zone approximately 25 km in diameter where breccia dykes, intense fracturing, para-authochonous breccias are locally encountered in the crystalline rocks forming the basement of the crater. The central deposits fill and landmark the initial crater low. From a stratigraphical point of view, the impact deposits form a flat quasi horizontal (slight tilt of less than 1°) continuous blanket. Yet the deposit is entailed by river valleys providing unique series of cross sections within the crater fill down to the crater floor and below.
Owing to the texture and the composition of the impact breccias, there is no significant contribution from sediments implying there was no sedimentary cover on top of the crystalline basement at the time of impact or it was shallow. The same applies for the sediments deposited in the nearby sea.
Despite of the erosion, the sequence of impactite lithologies is exceptionally complete at Rochechouart. All typologies of impactites and the whole sequence of shock metamorphic features are represented both in the deposits and in target. This includes dislocation breccia, breccia dikes, melt veins, pseudotachylites, cataclasites, shatter cones, megablocks, in the target rocks beneath and around the breccia deposits, and all types of melt free, melt poor and melt rich impactites in the deposits. Even the very fine materials (impactoclastites) depositing last and transported worldwide by the winds, is preserved forming a very fine layered horizontal deposits on top of the melt rich suevite (breccia with a debris matrix and both rock debris and melt fragments as clasts) near Chassenon (see map). This material is emplaced in a quiet environment, after all the chaos produced by the excavation, by the collapse of the cavity, and by the possible back flooding related to the tsunami induced by the impact in the nearby sea. Such a landmark of the final stage of impact deposit is exceptional at impact sites (quasi unique case among the # 200 terrestrial meteoritic impacts officially registered on Earth as of today).
Shape and size
The geometrical center of the structure is located 4 km (2.5 mi) west of Rochechouart, near the little village of la Judie (see map). The center of the structure according to the nature and distribution of the shock damage in the deposits and according to the negative gravity anomaly in the target stands about 1 km further South near Valette.
The size of the Rochechouart impact crater reported in the official impact database (23 km) has no phenomenological significance. As previously mentioned, the initial morphology of the crater is lost and there is no direct access to the initial size and shape of the crater. The 23 km correspond to the size of the area where damages attributed to impact were reported by authors in the 1970s. From the morphology of the crater floor and the impact deposit it is clear the initial crater is much larger than the 12 km zone where outcrops the remnants of the crater fill deposit. In the # 4–25 km diameter range, terrestrial impact craters are developing a central high, such as Boltysh crater, a 24 km impact crater in Ukraine. Like Rochechouart, Boltysh formed exclusively in crystalline basement. The crater is buried yet the deeper structure is known through numerous drill cores and geophysical investigation undertaken during the Soviet period in the search of hydrocarbons. The central high at Boltysh raises about 1 km above the level of crater floor in the low around the central high. There is no central high at Rochechouart, but a flat central low suggesting the central uplift has collapsed, a characteristic feature of larger impact craters. The current estimates for the Rochechouart initial crater fall in the range 40 +/-10 km.
Owing to the prominence of the siderophile contamination, a cometary projectile seems unlikely. The impactor was an asteroid. The earliest identification works involved the same heavy techniques and the same diagnostic elements (Ir, Os and other siderophiles elements) as those that became famous in the early 1980s with the identification of the extraterrestrial signal at the KT boundary worldwide. Since then the two extreme projectile types, iron meteorite and chondrite, have been argued by the successive workers. The most recent studies seems to agree with a special type of achondrite, a mix by impact of iron meteorite and silicates formerly designated as non magmatic iron meteorites.
Within the population of terrestrial impact crater Rochechouart provides a quite unique direct access for investigating major questions related to the impact cratering as geological and as a biological process. This includes the understanding of the crater fill mechanics, chronology, satellite effects such as resurge, pyroclastic explosions, landslide, and more. This covers the mechanics of large impact crater readjustments and the puzzling challenge of “fluidization”, namely making coherent rocks behave like a liquid without melting. This eventually encompass characterizing and understanding the impact induced hydrothermal cell responsible for the prominent hydrothermal overprint at Rochechouart, the possible nutriments, habitats and conditions of potential emergence of life at impact craters and the testing of the recent theories and models involving impacts as prominent actors of the habitability of planets.
Despite this exceptional potential Rochechouart was until very recently, one of the least, if not the least, investigated large impact crater on Earth. This has to do in part with the heavy vegetal cover masking the geology. But the situation is changing rapidly with the installation of the CIRIR (Center for International Research on Impact and on Rochechouart) on site and with the launch of CIRIR programs starting with the first series of drillings of the Rochechouart history. The later realized in eight sites of the National Reserve have just been completed. The scientific exploitation of the cores, with currently 60 projects and 60 teams from 12 nations scattered on 4 continents as part of the CIRIR program is just starting. The curatorial facility on site for hosting the drill cores and the surface samples as part of the impact on shelve is under construction. The sister facility for hosting scientists and students coming worldwide for studying impact cratering and or training in planetary geology, is under construction too. All this is possible because of the support of the local territories investing in the CIRIR, because of the State and the local territories both supporting the National Natural Reserve, because of the interest of the scientific community impact, and because of the value and the interest of the Rochechouart impact structure.
- "Rochechouart". Earth Impact Database. University of New Brunswick. Retrieved 2017-10-09.
- Dietz, R.S. (1963). Astroblemes: Ancient Meteorite-Impact Structures on the Earth, in, The Moon Meteorites and Comets, Edited by Gerard P. Kuiper, and Barbarra Middlehurts. University of Chicago Press. p. 285.
- Cécile Doulan et al., eds, Dossier: Cassinomagus: l'agglomération et ses thermes. Résultats des recherches récentes (2003-2010) à Chassenon (Charente) (Bordeaux: Fédération Aquitania, 2012. ISBN 2-910763-32-3. Offprint from Aquitania vol. 28, 2012)
- Kraut F. (1969). "Über ein neues Impaktit-Vorkommen im Gebiete von Rochechouart-Chassenon (Départements Haute Vienne und Charente, Frankreich)". Geologica Bavarica. 61: 428–450.
- Lambert P. (1977). . Les effets des ondes de choc naturelles et artificielles, et le cratère d’impact de Rochechouart (Limousin, France), Thèse d'État. Université de Paris-Sud, Orsay, France. pp. 515 p.
- Chao E.C., Shoemaker E.M., Madsen B.M. "First Natural Occurrence of Coesite". Science. 132-3421: 220–222.
- Lambert P. (1975). "Nickel enrichment of impact melt rocks from Rochechouart. Preliminary results and possibility of meteoritic contamination". Meteoritics. 10: 433–436. Bibcode:1975Metic..10..433L.
- Lambert P. (1976). "The meteoritic contamination in the Rochechouart crater: Statistical geochemical investigations". Symposium on Planetary Cratering Mechanics. Flagstaff, Arizona: 69–71.
- Alvarez L.W., Alvarez W., Asaro F., Michel H.V., (1980). "Extraterrestrial cause for the Cretaceous–Tertiary extinction". Science. 208: 1095–1108. Bibcode:1980Sci...208.1095A. doi:10.1126/science.208.4448.1095.
- Schmieder, M.; Buchner, E.; Schwarz, W. H.; Trieloff, M.; Lambert, P. (2010-10-05). "A Rhaetian 40Ar/39Ar age for the Rochechouart impact structure (France) and implications for the latest Triassic sedimentary record". Meteoritics & Planetary Science. 45 (8): 1225–1242. Bibcode:2010M&PS...45.1225S. doi:10.1111/j.1945-5100.2010.01070.x. Retrieved 2011-11-18.
- Horne A; (2016). (U-Th)/He, U/Pb, and Radiation Damage Dating of the Rochechouart-Chassenon Impact Structure, France-Master thesis. Arizona State University. pp. 63 pp.
- Cohen, Benjamin E.; Mark, Darren F.; Lee, Martin R.; Simpson, Sarah L. (2017-08-01). "A new high-precision 40Ar/39Ar age for the Rochechouart impact structure: At least 5 Ma older than the Triassic–Jurassic boundary". Meteoritics & Planetary Science. 52 (8): 1600–1611. Bibcode:2017M&PS...52.1600C. doi:10.1111/maps.12880. ISSN 1945-5100.
- Schmieder M., Shaulis B.J., Lapen T.J., Buchner E., Lambert P. and Kring D.A (2018). "Short report: Age of the Rochechouart (France) impact structure through LA-ICP-MS U/Pb analysis of zircon". In press.
- Smith, Roff (2011-11-16). "Dark days of the Triassic: Lost world". Nature. 479 (7373): 287–289. Bibcode:2011Natur.479..287S. doi:10.1038/479287a. PMID 22094671. Retrieved 2011-11-18.
- Lambert; et al. (2017). "CIRIR Programs: Drilling and Research Opportunities at the Rochechouart Impact Structure". Lunar and Planetary Science Conference 48th: # 1936.
- Spray, J.G., Kelley, S.P. and Rowley, D.B. (1998). "Evidence for a late Triassic multiple impact event on Earth". Nature, v. 392, pp. 171-173. Abstract
- Steele, Diana (19 March 1998). "Crater chain points to impact of fragmented comet". University of Chicago Chronicle.
- Lambert P. (2010). "Target and impact deposits at Rochechouart impact structure, France". Geological Society of America Special Paper, Special Paper 465: 509–541.
- Chèvremont, P., Floc’h, J.P., Ménillet, F., Stussi, J.M., Delbos, R., Sauret, B., Blès, J.L., Courbe, C., Vuaillat, D., and Gravelat, C. (1996). Notice Explicative, Carte Géologique de la France (1/50000), Feuille Rochechouart, (687): Orléans, France. BRGM. pp. 172pp.
- Sapers H.M., Osinski G.R., Banerjee N.R., Ferrière L., Lambert P., and Izawa R.M. (2014). "Izawa R.M., 2014, Revisiting the Rochechouart impact structure, France". Meteoritics & Planetary Science. 49-12: 2152–2168. Bibcode:2014M&PS...49.2152S. doi:10.1111/maps.12381.
- Simpson S.L., Boyce A.J., Lambert P., Lindgren P and Lee M.R. (2017). "Evidence for an impact-induced biosphere from the δ34S signature of sulphides in the Rochechouart impact structure, France". Earth and Planetary Science Letters. 460: 192–200. Bibcode:2017E&PSL.460..192S. doi:10.1016/j.epsl.2016.12.023.
- Reimold W.U., Oskierski W., and Huth J. (1987). "The pseudotachylite from Champagnac in the Rochechouart meteorite crater, France". Journal of Geophysical Research. 92 (B4):: E737–E748. Bibcode:1987JGR....92..737R. doi:10.1029/JB092iB04p0E737.
- Lambert P. "The Rochechouart crater: Shock zoning study". Earth and Planetary Science Letters. 35: 258–268.
- Pohl J., Ernstson K., and Lambert P. (1978). "Gravity measurements in the Rochechouart impact structure (France)". Meteoritics. 13: 601–604. Bibcode:1978Metic..13..601P.
- Gurov E. Kellley S.P. Koeberl C. and Dykan N.I. (2006). "Sediments and impact rock fillings in the Boltysh impact crater". in Charles Cockell, Christian Koeberl, Iain Gilmour- eds, Biological Processes Associated with Impact Events, Springer Science & Business Media: 335–358.
- Janssens M.-J., Hertogen J., Takahashi H., Anders E., and Lambert P. (1977). "Rochechouart meteorite crater: Identification of projectile". Journal of Geophysical Research. 82–5: 750–758. Bibcode:1977JGR....82..750J. doi:10.1029/JB082i005p00750.
- Horn W., and El Goresy A. (1980). "The Rochechouart crater in France: stony and not Iron meteorite?". Lunar Planetary Science XI, Lunar and Planetary Institute, Houston: 468–470.
- Koeberl C., Shukolyukov A., and Lugmair G. W. (2007). "Chromium isotopic studies of terrestrial impact craters: Identification of meteoritic components at Bosumtwi, Clearwater East, Lappajärvi, and Rochechouart". Earth and Planetary Science Letters. 256: 534546.
- Tagle, R., Schmitt, R.T., and Erzinger, J. (2009). "Identification of the projectile component in the impact structures Rochechouart, France, and Sääksjärvi, Finland: Implications for the impactor population for earth". Cosmochemica Acta. 73: 4891–4906.
|Wikimedia Commons has media related to Rochechouart crater.|