Chiemgau impact (hypothesis) is a term that denotes a meanwhile manifoldly proved meteorite impact that happened as an extraordinary event in prehistoric times (Bronze Age, Celtic era) in southeast Bavaria (Germany). A large cosmic body (a comet or an asteroid) hit the ground and left a big crater strewn field with all relevant impact evidence. This website focuses on all aspects of the related scientific research including reports and publications on geosciences, astronomy, archeology and science of history, but also on discussions of this spectacular research area. In the Wikipedia four-line article "Chiemgau impact hypothesis" this event is characterized as "an obsolete scientific theory" that has been raised "by a team of hobby-archaeologists". This is grossly deceptive and typifies the standpoint of a few obstinate opponents of the Chiemgau impact, hence taking their side and thwarting Wikipedia requirements.
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Barbara Rappenglück, Michael Hiltl, Kord Ernstson
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Jens Poßekel, Kord Ernstson
Collision in prehistory. – The Chiemgau Impact: research in a Bavarian meteorite crater strewn field
Keywords astrobiology diamond carbyne coalification carbonization meteorite impact chiemite
Abstract
Unusual carbonaceous matter, termed here chiemite, composed of more than 90% C from the Alpine Foreland at Lake Chiemsee in Bavaria, southeastern Germany has been investigated using optical and atomic force microscopy, X‐ray fluorescence spectroscopy, scanning and transmission electron microscopy, high‐resolution Raman spectroscopy, X‐ray diffraction and differential thermal analysis, as well as by δ13C and 14C radiocarbon isotopic data analysis. In the pumice‐like fragments, poorly ordered carbon matter co‐exists with high‐ordering monocrystalline α‐carbyne, and contains submicrometer‐sized inclusions of complex composition. Diamond and carbyne add to the peculiar mix of matter. The required very high temperatures and pressures for carbyne formation point to a shock event probably from the recently proposed Holocene Chiemgau meteorite impact. The carbon material is suggested to have largely formed from heavily shocked coal, vegetation like wood, and peat from the impact target area. The carbonization/coalification high PT process may be attributed to a strong shock that instantaneously caused the complete evaporation and loss of volatile matter and water, which nevertheless preserved the original cellular structure seen fossilized in many fragments. Relatively fresh wood encapsulated in the purported strongly shocked matter point to quenched carbon melt components possibly important for the discussion of survival of organic matter in meteorite impacts, implying an astrobiological relationship.
The Wikipedia page “Chiemgau impact hypothesis” is still manipulating science and defaming scientific research for the worst, when the visitor reads in a few sentences that the impact hypothesis is obsolete.
For some years now we have been trying to protest against this misleading of Wikipedia readers and the scientific community – in vain. Corrections we made with a host of documented quotations were deleted at once – apparently with the tolerance or even the forcing of the administrator. The initiators of this manipulation, partly close to an insult, are largely known to us as totally unrelated to the scientific research subject, which does not change the situation.
For Wikipedia, this is not a glorious fact; the claim to encyclopedic honesty and correctness is not fulfilled in this case.
The visitor and reader of this website is requested to use honest, scientifically correct and according to strict scientific rules oriented information of this website about the Chiemgau impact.. A compilation of the scientific findings, published internationally at renowned congresses and in peer-review journals, proves the existence of what is probably the largest terrestrial meteorite crater strewn field, which is also widely accepted internationally.
Rappenglück, M.A., Rappenglück, B., Ernstson, K. (2018):Cosmic collision in prehistory. The Chiemgau Impact: research in a Bavarian meteorite crater strewn field.- Zeitschrift für Anomalistik, 17 (2017), S. 235–260 (in German). Abstract
Ernstson, K. & Poßekel, J. (2017): Meteorite Impact “Earthquake” Features (Rock Liquefaction, Surface Wave Deformations, Seismites) from Ground Penetrating Radar (GPR) and Geoelectric Complex Resistivity/Induced Polarization (IP) Measurements, Chiemgau (Alpine Foreland, Southeast Germany). AGU Fall Meeting, 11-15 Dec. 2017 New Orleans. Abstract Poster
Procházka V. Trojek T. (2017): XRF- and EMP- Investigation of Glass Coatings and Melted Domains of Pebbles from Craters in Chiemgau, Germany. Lunar an Planetary Science Conference XLVIII. Abstract #2401.pdf.
Ernstson, K. (2016): EVIDENCE OF A METEORITE IMPACT-INDUCED TSUNAMI IN LAKE CHIEMSEE (SOUTHEAST GERMANY) STRENGTHENED.EVIDENCE OF A METEORITE IMPACT-INDUCED TSUNAMI IN LAKE CHIEMSEE (SOUTHEAST GERMANY) STRENGTHENED.. 47th Lunar and Planetary Science Conference, 1263.pdf.
V. Procházka, G. Kletetschka (2016): Evidence for superaparamagnetic nanoparticles in limestones from Chiemgau crater field, SE Germany. 47th Lunar and Planetary Science Conference, 2763.pdf
M. A. Rappenglück, F. Bauer, K. Ernstson, M. Hiltl (2014): Meteorite impact on a micrometer scale: iron silicide, carbide and CAI minerals from the Chiemgau impact event (Germany). – Problems and perspectives of modern mineralogy (Yushkin Memorial Seminar–2014) Proceedings of mineralogical seminar, Syktyvkar, Komi Republic, Russia 19–22 May 2014. Abstract POSTER
Ernstson, K., Hilt, M., Neumair, A. (2014): Microtektite-Like Glasses from the Northern Calcareous Alps (Southeast Germany): Evidence of a Proximal Impact Ejecta . – 45th Lunar and Planetary Science Conference,. LPI Contribution No. 1777, #1200.pdf.
Rappenglück, M.A., Bauer, F. Hiltl, M., Neumair, A., K. Ernstson, K. (2013): Calcium-Aluminium-rich Inclusions (CAIs) in iron silicide matter (Xifengite, Gupeiite, Hapkeite): evidence of a cosmic origin – 76th Annual Meteoritical Society Meeting, Meteoritics & Planetary Science, Volume 48, Issue s1, Abstract #5055. POSTER
Bauer, F. Hiltl, M., Rappenglück, M.A., Neumair, A., K. Ernstson, K. (2013): Fe2Si (Hapkeite) from the subsoil in the alpine foreland (Southeast Germany): is it associated with an impact? – 76th Annual Meteoritical Society Meeting, Meteoritics & Planetary Science, Volume 48, Issue s1, Abstract #5056. POSTER
Neumair, A., Ernstson, K. (2013): Peculiar Holocene soil layers: evidence of possible distal ejecta deposits in the Chiemgau region, Southeast Germany – 76th Annual Meteoritical Society Meeting, Meteoritics & Planetary Science, Volume 48, Issue s1, Abstract #5057. POSTER
Ernstson, K., Müller, W., Neumair, A. (2013): The proposed Nalbach (Saarland, Germany) impact site: is it a companion to the Chiemgau (Southeast Bavaria, Germany) impact strewn field? – 76th Annual Meteoritical Society Meeting, Meteoritics & Planetary Science, Volume 48, Issue s1, POSTER Abstract #5058.
K. Ernstson, T. G. Shumilova, S. I. Isaenko, A. Neumair, M. A. Rappenglück (2013): From biomass to glassy carbon and carbynes: evidence of possible meteorite impact shock coalification and carbonization. – Modern problems of theoretical, experimental and applied mineralogy (Yushkin Memorial Seminar–2013): Proceedings of mineralogical seminar, Syktyvkar: IG Komi SC UB RAS, 2013. 546 p POSTER
S. Isaenko, T. Shumilova, K. Ernstson, S. Shevchuk, A. Neumair, and M. Rappenglück (2012): Carbynes and DLC in naturally occurring carbon matter from the Alpine Foreland, South-East Germany: Evidence of a probable new impactite. – European Mineralogical Conference, Vol. 1, EMC2012-217, 2012., POSTER
B. RAPPENGLÜCK, K. ERNSTSON, I. LIRITZIS, W. MAYER, A. NEUMAIR, M. RAPPENGLÜCK and D. SUDHAUS (2012): A prehistoric meteorite impact in Southeast Bavaria (Germany): tracing its cultural implications. – 34th International Geological Congress, 5-10 August 2012 – Brisbane, Australien. Abstract
Shumilova, T. G., Isaenko S. I., Makeev B. A., Ernstson K., Neumair A., Rappenglück M. A. (2012): Enigmatic Poorly Structured Carbon Substances from the Alpine Foreland, Southeast Germany: Evidence of a Cosmic Relation. 43nd Lunar and Planetary Science Conference, 1430.pdf. Abstract.
Ernstson, K. & Neumair, A. (2011), Geoelectric Complex Resistivity Measurements of Soil Liquefaction Features in Quaternary Sediments of the Alpine Foreland, Germany, Abstract NS23A-1555 presented at 2011 Fall Meeting, AGU, San Francisco, Calif., 5-9 Dec. POSTER Abstract
Neumair, A. & Ernstson, K. (2011), Geomagnetic and morphological signature of small crateriform structures in the Alpine Foreland, Southeast Germany, Abstract GP11A-1023 presented at 2011 Fall Meeting, AGU, San Francisco, Calif., 5-9 Dec. POSTER Abstract
M. Hiltl, F. Bauer, K. Ernstson, W. Mayer, A. Neumair, and M.A. Rappenglück (2011): SEM and TEM analyses of minerals xifengite, gupeiite, Fe2Si (hapkeite?), titanium carbide (TiC) and cubic moissanite (SiC) from the subsoil in the Alpine Foreland: Are they cosmochemical? – 42nd Lunar and Planetary Science Conference (2011), 1391.pdf Abstract
K. Ernstson, C. Sideris, I. Liritzis, A. Neumair (2012): THE CHIEMGAU METEORITE IMPACT SIGNATURE OF THE STÖTTHAM ARCHAEOLOGICAL SITE (SOUTHEAST GERMANY). – Mediterranean Archaeology ans Archäometry, 12, 249-259.
Ernstson, K., Mayer W., Neumair, A., and Sudhaus, D. (2011): The sinkhole enigma in the alpine foreland, Southeast Germany: Evidence of impact-induced rock liquefaction processes. – Cent. Eur. J. Geosci., 3(4), 385-397. DOI: 10.2478/s13533-011-0038-y
Liritzis, N. Zacharias, G.S. Polymeris, G. Kitis, K. Ernstson, D. Sudhaus, A. Neumair, W. Mayer, M.A. Rappenglück, B. Rappenglück (2010): THE CHIEMGAU METEORITE IMPACT AND TSUNAMI EVENT (SOUTHEAST GERMANY): FIRST OSL DATING. – Mediterranean Archaeology and Archaeometry, Vol. 10, No. 4, pp. 17‐33.
Barbara Rappenglück, Michael A. Rappenglück, Kord Ernstson, Werner Mayer, Andreas Neumair, Dirk Sudhaus & Ioannis Liritzis (2010): The fall of Phaethon: a Greco-Roman geomyth preserves the memory of a meteorite impact in Bavaria (south-east Germany). – Antiquity, 84, 428-439.
Ernstson, K., Mayer, W., Neumair, A., Rappenglück, B., Rappenglück, M.A., Sudhaus, D. and Zeller, K.W. (2010): The Chiemgau crater strewn field: evidence of a Holocene large impact in southeast Bavaria, Germany. – Journal of Siberian Federal University, Engineering & Technology, 1 (2010 3) 72-103.
Rappenglück, B., Ernstson, K., Mayer, W., Neumair, A. Rappenglück, M.A., Sudhaus, D., and Zeller, K.W. (2009):: The Chiemgau impact: An extraordinary case study for the question of Holocene meteorite impacts and their cultural implications. – In: Belmonte, J. A. (ed.), Proceedings of the International Conference on Archaeoastronomy, SEAC 16th 2008 “Cosmology across Cultures. Impact of the Study of the Universe in Human Thinking”, Granada September 8-12, 2008, A.S.P. Conf. Ser., 2009.
Barbara and Michael Rappenglück (2006): Does the myth of Phaethon reflect an impact? – Revising the fall of Phaethon and considering a possible relation to the Chiemgau Impact. – Mediterranean Archaeology and Archaeometry, Proceedings of the International Conference on Archaeoastronomy, SEAC 14th 2006, „Ancient watching of cosmic space and observation of astronomical phenomena“, Vol. 6, No. 3 (2006), 101-109.
Kord Ernstson* (2018)
Pink quartz, not to be confused with rose quartz, is an extremely rare color variety, which is completely transparent and is only known from a few occurrences worldwide. It is believed that the pink color is due to small amounts of aluminum and phosphorus that substitute silicon, and exposure of the quartz to natural gamma radiation. Sands with a dominating proportion of pink quartz excavated from the soil and extracted from a breccia layer in the crater strewn field of the Chiemgau meteorite impact suggest that normally colorless quartz sand was irradiated during the impact event and may possibly be found at other impact sites.
Key words: Pink and rose quartz, Chiemgau meteorite impact, neutron-gamma radiation
*Faculty of Philosophy I, University of Würzburg, Germany, kernstson@ernstson.de
Direct DOWNLOAD of the POSTER. Note that for better legibility the poster PDF can considerably be enlarged on the monitor.
Already in the early days of the exploration of the Chiemgau impact crater strewn field at the beginning of the new millennium, a perfectly semicircular structure was discovered during a flight, which seemed to be punctured into the bank of the Inn river near Marktl. Geological research on the ground and sampling quickly proved the impact nature of this well 50 m measuring crater, which was introduced as No. 24 into the crater list of the Chiemgau impact, which had been meticulously conducted by local history researchers. The semicircular structure was easily explained by the erosion of floods in the valley of the Inn river
Not recorded in the topographical maps and soon blocked with a large stable it fell into oblivion and was only recently opened to the eye in full splendor by the Digital Terrain Model DGM 1 (Fig. 1).
Fig. 1. Aiching semi crater in the Inn river bank vis-à-vis the town of Marktl (UTM coordinates 338863, 5346952). Digital Terrain Model. Continue reading
At the this year’s prestigious meeting of the Lunar and Planetary Institute in The Woodlands, Texas, the following abstract articles that relate to the Chiemgau meteorite impact have been published:
Molnár M. Ventura K. Švanda P. Štaffen Z. Rappenglück M. A., Ernstson, K.:
Chrudim – Pardubice: Evidence for a Young Meteorite Impact Strewn Field in the Czech Republic – Widespread finds of rocks and glasses with shock metamorphism and typical of meteorite impact suggest a Holocene impact event in the Czech Republic.
The article reports on a newfound very young meteorite impact event in the Czech Republic amazingly similar to the Chiemgau and Saarland (Nalbach) impact events in Germany. A possibly simultaneous impact having affected Central Europe over a distance of more than 650 km is discussed. Click the abstract article!
Procházka V. Trojek T.
XRF- and EMP- Investigation of Glass Coatings and Melted Domains of Pebbles from Craters in Chiemgau, Germany
Shock-induced melting mainly of biotite (?) produced typically porous veinlets. External glass coatings are rich in K and Cu (from plant biomass?), rarely in Ni.
The Czech authors report on investigations of shocked cobbles excavated from the Kaltenbach and #004 impact craters belonging to the Chiemgau meteorite impact strewn field. Click the abstract article!
The Digital Terrain Model (DTM) and the evaluation of known and the search for new craters in the Chiemgau meteorite impact strewn field [PDF DOWNLOAD]
Kord Ernstson* (2017)
Abstract. – For several known and a few newly proposed meteorite craters in the Chiemgau meteorite impact strewn field the LiDAR data of the Digital Terrain Model DTM have been processed to reveal various maps and cross sections based on a high-resolution mesh down to 1 m and contour interval down to 0.2 m. The data processing highlights particular crater features that remain hidden in fieldwork and on conventional topographic maps and even may debunk mistaken structures.
********************************************************************************************************* *Faculty of Philosophy I, University of Würzburg, Germany, kernstson@ernstson.de
Content 1 Introduction – 2 The Chiemgau meteorite impact event 3 Data processing 3.1 Terrain imagery 3.2 Horizontal gradient 3.3 Data filtering 3.4 Cross sections 4 Examples 4.1 Small craters in the DTM 4.2 Peripheral depressions around small craters 4.3 Medium-sized craters in the DTM 4.4 Mistaken structures 5 A possible large-sized crater in the DTM 6 Discussion and conclusions 7 References Appendix
