IMPACT Programme Aims at Understanding the Effects of Asteroid And/Or Comet Impacts on the Development and Evolution of the Earth

The ESF IMPACT programme aims at understanding the effects of asteroid and/or comet impacts on the development and evolution of the Earth. The programme is broadly interdisciplinary, gathering scientists from fields covering the whole realm of the Earth, Life, and Environmen- tal Sciences. Impact is a key and common process in the solar system. In July 1994, the crash of comet Shoemaker-Levy 9 on planet Jupiter provided a “live” demonstration that the universe is indeed a violent place. Astronomers and planetary scientists are Impact of comet Shoemaker-Levy 9 on Jupiter in July 1994. familiar with such catastrophic events. Response of the Earth System to Impact Processes (IMPACT) They have documented the major role impacts play in shaping the surface of solid An ESF scientific programme planets; the latest formation theory for the Moon indicates that it is the result of the collision of a Mars-size object with Early Earth. However, perhaps because of its catastrophic nature, geoscientists have in their majority been slower to accept that the impact of extraterrestrial objects influences the biological, and geological evolution of the Earth. In 1980, a team of scientists from the University of California at Berkeley hypothesised that the impact of a ± 10 km diameter asteroid or comet on Earth was

Earth rise viewed from the densely cratered surface of the moon. responsible for the extinction of the dino- saurs and almost 50% of all species of fauna and flora at the end of the Cretaceous period, some 65 million years ago. Abun- dant evidence corroborating this hypothesis was gathered by US and European teams during the 1980s and culminated in 1990 with the discovery of the 200 km diameter Chicxulub impact structure buried under the tip of the Yucatan Peninsula in Mexico. This impact/extinction hypothesis triggered major research on impact processes and the biological, climatic and geological response of planet Earth. The ESF IMPACT The European Science Foundation acts programme builds on this momentum to as a catalyst foster European contributions to this exciting for the development and important research topic. of science by bringing together leading scientists and funding agencies to debate, plan and implement pan-European initiatives. 1 the impacted lithologies, coupled with highly sophisticated mathematical modelling. In this latter field – perhaps because it did not have an intense programme of military nuclear testing Scientific goals – Europe is behind the US and Russia. The ESF programme wants to develop The ESF programme is concerned such expertise in Europe. with understanding the linkage The history of life and climate on between impact processes and the Earth is recorded in sediment. Precise Earth System. It aims at document- determination of the age of impact ing consequences of impact events craters is important to establish on the Earth environment, including potential links with the changes atmospheric, climatic, biological, and observed in the fossil record. As of geological effects. A particularly today, many craters are still poorly important aspect of the programme’s dated. Thus, another priority of the research focuses on the effects on the programme is the systematic use of biodiversity of ecosystems. The ESF state-of-the-art methods to date IMPACT programme covers three impact craters and to correlate them main areas of research. with the sedimentary record.

1. The impact event Knowledge of the physical and chemical constraints of the impact process itself is still limited. First, a better understanding of the astro- nomical background, especially concerning the population of Earth orbit crossing asteroids and comets, is needed. Telescope searches discover new Earth orbit crossing asteroids 2. Energy transfer to the environ- and comets on a regular basis. The ment record of craters on Earth must be An asteroid or comet strikes Earth better assessed; today only about with a velocity ranging between Top: Impact lithology 150 impact structures are known and about 11 and 72 km/sec. A large (breccia and melt-rock) from inside the Popigai only two marine craters have been bolide will bury itself deep in the crater in Siberia found. Differences between impacts Earth crust, generating a huge crater. in a continental versus a marine The mechanism of how the enor- Right: Satellite view of environment need to be documented. mous energy released during an twin Clearwater craters (East and West) in Understanding the cratering process impact event is actually transferred Canada itself requires the detailed study of to the atmo-, hydro-, bio-, and

2 geosphere is probably the least 3. Effects on the environment understood part in the chain that The response of the environment may link impact events with envi- covers various topics, from the ronmental changes. formation of economically important mineral deposits, as in the case An impact leads to the instantaneous of the Ni-rich Sudbury crater in generation of shock waves that pen- Canada, to crater-fill sediments etrate the target area and attenuate in yielding exploitable hydrocarbon its environs. These shock waves af- reserves, to major climatic and fect the target lithologies by biological changes. Once the impact vaporising, melting, and shattering energy is imparted onto the Earth the target rock. The effect of this System, all the potential conse- shock wave is visible in some miner- quences and response of the environ- als which show evidence of shock ment need to be evaluated. Disrup- metamorphism. tions would include massive tsuna- mis, huge forest fires, as well as the introduction of large amounts of dust, water vapour, and various gaseous species into the atmosphere, and the deposition of hot and cold ejecta at great distance from the crater. Ejecta layers are highly unusual formations and contain large quantities of rare siderophile elements, shocked minerals, nanometer-sized diamonds and glass. These markers are of prime importance to trace accretionary events in the sedimentary record, to identify their origin, and to evaluate their potential global effects. A major effort of the ESF programme is the meticulous search for impact layers in sediments throughout geological times. Shocked quartz from the Manson crater in Iowa. Effects of impacts on the Earth’s Recent studies, mainly triggered by biodiversity need to be more precisely the Cretaceous-Tertiary boundary evaluated. Interpretations vary from impact/extinction scenario, seem to complete scepticism to hypotheses indicate that the injection of huge that link all important evolutionary events to impact events. To reach a quantities of gases (CO2, SO2, H2O) and dust in the atmosphere is the more balanced view, which is sup- link between impact events and ported by sound facts, the obvious first changes in the Earth System. Inte- step is to assess, as precisely as gration of the type of material and possible, which mass extinctions and/ energy released by a large impact or global changes are clearly linked to within present circulation and atmo- impact events. Studies of taxonomic spheric models can illustrate how the ranges or even relative abundance of perturbation is transmitted to, and species do not always produce signifi- influenced by the Earth System. cant patterns of biotic change, such as those observed at the Cretaceous- Tertiary boundary. The selectivity of

3 impact-induced extinctions and/or on Earth is small, but not zero. Once biotic changes is not known. What every 100 years or so, the Earth is organism succumbs to which after- struck by an NEO around 10 to 100 m effect of impact events needs to be in size that would be large enough to documented. This involves close cause tens of thousands of deaths cooperation between palaeontologists were it to strike an urban area. On a and experts on the physical and time scale of many thousand years, chemical markers of impacts, as well the Earth is impacted by objects in as high- precision dating. Such close the range 100 m to 1 km, large interaction is being developed in the enough to cause damage comparable framework of the ESF IMPACT to, or worse than, the greatest known programme. natural disasters. Finally, the hazards of impact events to humankind must be evaluated. This has been the topic of intense debates in the US and Russia, but received limited or no attention in Europe. The solar system contains a long-lived population of asteroids and comets that may strike the Earth. Around 90% of potential Earth impactors, collectively called NEOs (Near Earth Objects), are asteroids or short period comets. The other 10% are intermediate or long- period comets. The risk of an impact

Computer-enhanced image of the 4.5 km Earth orbit crossing asteroid 4179 Toutatis. Programme activities

Research and field workshops Students and young scientists are Workshops are held twice a year in highly encouraged to present their various European locations, either results, and receive financial help to close to an impact site, a key strati- attend these workshops. Each Roter Kamm crater in graphic sequence, a drill core store- workshop focuses on one key topic Namibia. house, or at an experimental facility. and tries to attract impact researchers and experts in closely related disci- plines. A volume of peer-reviewed proceedings is issued for each workshop by a major Earth Science publisher.

Short course and educational activities With a few exceptions, the curricula of Earth Science departments at European universities do not cover impact geology. The interdisciplinary nature of impact research makes it a difficult subject to teach within traditional discipline boundaries.

4 The ESF IMPACT programme has, thus, established a short course, designed especially for junior researchers, which takes place once a year and covers various aspects of impact research. The course aims at encouraging the teaching of impact processes in European universities by training the professors and researchers of tomorrow in this discipline.

Exchange grants The ESF IMPACT programme offers a limited number of exchange grants to develop collaborative projects among European scientists. Grants are meant to provide a contribution towards travel and living expenses of programme web page. An internet Model in 3 D of the Chicxulub young scientists, graduate students, discussion list and news group has crater in Mexico or postdoctoral researchers when also been set up to facilitate contacts working in another European country. and exchange of information among impact researchers world-wide. The A list of workshops and application topics range from discussion of new forms for grants and the short course results, to younger scientists seeking are available on the ESF IMPACT advice on techniques or methodol- programme web site at ogy. http://psri.open.ac.uk/esf/ Database of European impact Newsletter and web site researchers With its newsletter, the ESF Steering A list of more than 300 researchers in Committee alerts the scientific Europe who have impact as a topic of community in Europe and elsewhere interest has been established. The list about the activities of the IMPACT is updated regularly and can be programme. The Newsletter is obtained by contacting the ESF published twice a year and distrib- IMPACT programme chair or secre- uted to more than 300 scientists. tary. Information and background can be found on the ESF IMPACT

Funding

ESF scientific programmes are l'Energie Atomique, France; principally financed by the Deutsche Forschungsgemeinschaft, Foundation’s Member Organisations Germany; Magyar Tudományos on an à la carte basis. IMPACT is Akadémia, Hungary; Norges supported by: Forskningsråd, Norway; Instituto de Fonds zur Förderung der Cooperaçao Ciêntifica e Tecnológica wissenschaftlichen Forschung, Internacional, Portugal; Natur- Austria; Fonds National de la Recher- vetenskapliga Forskningsrådet, che Scientifique, Belgium; Suomen Sweden; Fonds National Suisse de la Akatemia/Finlands Akademi, Fin- Recherche Scientifique, Switzerland; land; Centre National de la Recher- Natural Environment Research che Scientifique, Commissariat à Council, United Kingdom.

5 IMPACT Steering Committee

Dr. Christian Koeberl (Chairman) Dr. Iain Gilmour Dr. Annette Moth-Wiklund Institute of Geochemistry Planetary Sciences Research Institute ESF Senior Scientific Secretary University of Vienna The Open University Mrs. Catherine Lobstein Althanstraße 14 Walton Hall ESF Administrative Assistant 1090 Vienna MK7 6AA Milton Keynes Austria United Kingdom European Science Foundation Tel: +43 1 31336 1714 Tel: +44 908 655 140 1 quai Lezay-Marnésia Fax: +43 1 31336 781 Fax: +44 908 655 910 67080 Strasbourg Cedex E-mail: [email protected] E-mail: [email protected] France WWW Home Page: Dr. Philippe Claeys (Secretary) Dr. Alan Green http://www.esf.org Institut für Mineralogie Institute of Geophysics Tel: +33 (0)3 88 76 71 30 Museum für Naturkunde Swiss Federal Institute of Technology Fax: +33 (0)3 88 37 05 32 Invalidenstr. 43 ETH-Hönggerberg Email: [email protected] 10115 Berlin 8093 Zürich Germany Switzerland Tel: +49 30 20938857 Tel: +41 1 6332657 Fax: +49 30 20938565 Fax: +41 1 6331065 For the latest information on E-mail: [email protected] E-mail: [email protected] this programme consult the IMPACT home pages Dr. Karoly Brezsnyanszky Dr. Herbert Henkel (http://www.esf.org/lp/ Geological Institute of Hungary Department of Geodesy and IMPACTa.htm) and Photogrammetry PO Box 106 (http://psri.open.ac.uk/esf/) 1142 Budapest Royal Institute of Technology Hungary 10044 Stockholm Tel: +36 1 251 4680 Sweden Pictures courtesy of Philippe Claeys, Fax: +36 1 251 0703 Tel: +46 8 790 8604 Christian Koeberl and NASA. E-mail: [email protected] Fax: +46 8 790 7343 E-mail: [email protected] Dr. Eric Buffetaut Centre National de la Recherche Dr. Jean-François Müller Scientifique Belgian Institute for Space Aeronomy 16 cour de Liégat 3 avenue Circulaire 75013 Paris 1180 Bruxelles France Belgium Tel: +33 1 45 84 81 45 Tel: +32 2 373 0486 Fax: +33 1 45 84 81 45 Fax: +32 2 374 8423 E-mail: [email protected] E-mail: jean-franç[email protected]

Dr. Alexander Deutsch Dr. Jose Munha Institut für Planetologie Departamento de Geologia Universität Münster Facultade de Ciencias Wilhelm-Klemm Strasse 10 Edificio C2, 5 Piso 48149 Münster Campo Grande Germany 1700 Lisboa Tel: +49 251 83 33 484 Portugal Fax: +49 251 83 39 083 Fax: +351 1 7500064 E-mail: [email protected] E-mail: [email protected] d’ordre 991006 Dr. Henning Dypvik Dr. Lauri J. Pesonen ° Institute of Geology Laboratory for Paleomagnetism University of Oslo Geological Survey of Finland PO Box 1047 Geophysics Section 0316 Blindern P.O. Box 96 Norway 02151 Espoo Tel: +47 22 856659 Finland Fax: +47 22 854215 Tel: +358 205 50 2269 E-mail: [email protected] Fax: +358 205 5012 March 1999

E-mail: [email protected]  European Science Foundation Ireg Strasbourg - Dépôt légal: mars 1999 N