Shiva Structure: a Possible KT Boundary Impact Crater on the Western Shelf of India
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Exceptionally Well-Preserved Fossils in a Middle Ordovician Impact Crater
Downloaded from http://jgs.lyellcollection.org/ by guest on September 29, 2021 Review focus Journal of the Geological Society Published Online First https://doi.org/10.1144/jgs2018-101 The Winneshiek biota: exceptionally well-preserved fossils in a Middle Ordovician impact crater Derek E.G. Briggs1,2*, Huaibao P. Liu3, Robert M. McKay3 & Brian J. Witzke4 1 Department of Geology and Geophysics, Yale University, New Haven, CT 06520, USA 2 Yale Peabody Museum of Natural History, Yale University, New Haven, CT 06520, USA 3 Iowa Geological Survey, IIHR – Hydroscience & Engineering, University of Iowa, 340 Trowbridge Hall, Iowa City, IA 52242, USA 4 Department of Earth and Environmental Sciences, University of Iowa, 115 Trowbridge Hall, Iowa City, IA 52242, USA D.E.G.B., 0000-0003-0649-6417 * Correspondence: [email protected] Abstract: The Winneshiek Shale (Middle Ordovician, Darriwilian) was deposited in a meteorite crater, the Decorah impact structure, in NE Iowa. This crater is 5.6 km in diameter and penetrates Cambrian and Ordovician cratonic strata. It was probably situated close to land in an embayment connected to the epicontinental sea; typical shelly marine taxa are absent. The Konservat-Lagerstätte within the Winneshiek Shale is important because it represents an interval when exceptional preservation is rare. The biota includes the earliest eurypterid, a giant form, as well as a new basal chelicerate and the earliest ceratiocarid phyllocarid. Conodonts, some of giant size, occur as bedding plane assemblages. Bromalites and rarer elements, including a linguloid brachiopod and a probable jawless fish, are also present. Similar fossils occur in the coeval Ames impact structure in Oklahoma, demonstrating that meteorite craters represent a novel and under-recognized setting for Konservat- Lagerstätten. -
Magyar Királyi Földtani Intézet (2006.)
' Copyright Magyar `llami Fldtani IntØzet (Geological Institute of Hungary), 2005 Minden jog fenntartva! All rights reserved! Lektorok Reviewers: BALLA ZOLTÁN, CSÁSZÁRGZA, HAAS JÁNOS, HORVÁTH ISTVÁN, JÁMBOR Á RON, KOVÁCS SÁNDOR, KUBOVICS IMRE, LESS GYRGY, LIEBE PÁL,VICZIÁN ISTVÁN Sorozatszerkesztı Serial editor: BALLA ZOLTÁN Szakszerkesztı Scientific editor: PIROS OLGA Mßszaki szerkesztı Technical editor: SIMONYI DEZS SzÆmtgØpes nyomdai elıkØsztØs DTP: PIROS OLGA, SIMONYI DEZS Bortterv Cover design: SIMONYI DEZS Kiadja a Magyar `llami Fldtani IntØzet Published by the Geological Institute of Hungary Felelıs kiad Responsible editor: KORDOS L`SZL Igazgat Director HU ISSN 03689751 3 Tartalom — Contents Működési jelentés — Activity Report HÁMOR GÉZA (1934–2007) . 7 JÁMBOR ÁRON (összeállító): Dr. Hámor Géza szakirodalmi munkássága . 8 KORDOS LÁSZLÓ: A múlt a jövő kulcsa . 17 BREZSNYÁNSZKY KÁROLY: Igazgatói beszámoló a Magyar Állami Földtani Intézet 2006. évi tevékenységéről . 19 Szakcikkek — Scientific publications RIPSZNÉ JUDIK KATALIN: A Medvednica hegység (Horvátország) és Észak-Magyarország paleozoos és mezozoos kishőmérsékletű metamorf képződményeinek összevetése. — Comparison of Palaeozoic and Mesozoic very low- grade metamorphic formations in the Medvednica Mts (Croatia) and in North Hungary. 47 PELIKÁN PÁL, IVAN FILIPOVIĆ, DIVNA JOVANOVIĆ, MILAN SUDAR, †LJUBINKO PROTIĆ, HIPS KINGA, KOVÁCS SÁNDOR, LESS GYÖRGY: A Bükki-terrénum (É-Magyarország), a Jadari-terrénum (ÉNy-Szerbia) és a Sana-Unai-terrénum (ÉNy-Bosznia) karbon, perm és triász rétegsorainak összehasonlítása. — Correlation of the Carboniferous, Permian and Triassic sequences of the Bükk, Jadar, Sana-Una terrains. 59 BUDAI TAMÁS: Platformok és medencék kialakulása és fejlődése a Bakony középső-triász története során. — Middle Triassic platform and basin evolution of the Bakony Mts, Hungary. 77 HAAS JÁNOS: A bükki és a darnói jura képződmények ősföldrajzi helyzete és kapcsolatai. -
Cretaceous - Tertiary Mass Extinction Meteoritic Versus Volcanic Causes
GENERAL I ARTICLE Cretaceous - Tertiary Mass Extinction Meteoritic Versus Volcanic Causes P V Sukumaran The bolide impact theory for mass extinctions at the Cretaceous-tertiary (K-T) boundary was a revolutionary concept. This theory was contested by short duration global volcanism as a possible alternative cause for the K-T extinction. Though there is a converging evidence for an extra-terrestrial impact coinciding with the P V Sukumaran took his terminal Cretaceous, the causative link between the M Tech degree in impact and the K-T mass extinction is debatable. Thus, Applied Geology from the while the impact theory is re-emerging, available evidence University of Saugar and has been with the is still insufficient to rule out either of the two hypotheses. Geological Survey of India since 1974. His interests Introduction include geochemistry, petrology and palae oceanography. He is It is now widely believed that life on earth began very early in presently posted to the its geological history, probably about 4000 My (million years) Marine Wing of the ago (Mojzsis and others, 1996). Since then it underwent Department and has participated in many several evolutionary branchings to the complex diversity as scientific cruises both as we see today. Nevertheless, it was not a smooth voyage for life Chief Scientist and as a all along, the evolution was punctuated by geologically participating scientist. ins tan taneous events of mass mortality. New species emerged at the expense of their predecessors following each extinction event and life went on evolving ever more vibrantly. In the geologic record of rock strata, such mass extinction events are identifiable based on sudden absence and reduction in diversity of fossil assemblage across stratigraphic boundaries. -
"Ringing" from an Asteroid Collision Event Which Triggered the Flood?
The Proceedings of the International Conference on Creationism Volume 6 Print Reference: Pages 255-261 Article 23 2008 Is the Moon's Orbit "Ringing" from an Asteroid Collision Event which Triggered the Flood? Ronald G. Samec Bob Jones University Follow this and additional works at: https://digitalcommons.cedarville.edu/icc_proceedings DigitalCommons@Cedarville provides a publication platform for fully open access journals, which means that all articles are available on the Internet to all users immediately upon publication. However, the opinions and sentiments expressed by the authors of articles published in our journals do not necessarily indicate the endorsement or reflect the views of DigitalCommons@Cedarville, the Centennial Library, or Cedarville University and its employees. The authors are solely responsible for the content of their work. Please address questions to [email protected]. Browse the contents of this volume of The Proceedings of the International Conference on Creationism. Recommended Citation Samec, Ronald G. (2008) "Is the Moon's Orbit "Ringing" from an Asteroid Collision Event which Triggered the Flood?," The Proceedings of the International Conference on Creationism: Vol. 6 , Article 23. Available at: https://digitalcommons.cedarville.edu/icc_proceedings/vol6/iss1/23 In A. A. Snelling (Ed.) (2008). Proceedings of the Sixth International Conference on Creationism (pp. 255–261). Pittsburgh, PA: Creation Science Fellowship and Dallas, TX: Institute for Creation Research. Is the Moon’s Orbit “Ringing” from an Asteroid Collision Event which Triggered the Flood? Ronald G. Samec, Ph. D., M. A., B. A., Physics Department, Bob Jones University, Greenville, SC 29614 Abstract We use ordinary Newtonian orbital mechanics to explore the possibility that near side lunar maria are giant impact basins left over from a catastrophic impact event that caused the present orbital configuration of the moon. -
Stratigraphy of Barmer Basin, Rajasthan: Implications on Cretaceous-Tertiary Boundary*
828 NOTES STRATIGRAPHY OF BARMER BASIN, RAJASTHAN: IMPLICATIONS ON CRETACEOUS-TERTIARY BOUNDARY* M.S. SISODIA Department of Geology, J.N.Vyas University, Jodhpur - 342 005 Email: [email protected] EXTENDED ABSTRACT Earth scientistshave been in pursuit for 'longto frnd the anoma\iesmd as bi-stoPtion in the morphology ofthe EaTth. tn~tliabout: (1) What killed dinosaurs at the end-Cretaceous? If we imagine a scenario of the post 65 Ma era, it is possible and (2) Had the mass extinction during the geological history that the intelligent being of the future era may find these been abrupt or is a gradual process? The objective of this changes incorporated in a thin sedimentary layer with no paper is an attempt on the basis of data collected fiom lateral continuity, and may fall into the trap of interprcting the Barmer Basin, Rajasthan, to find a plausible answer to tens of thousand years as a very very small time period. It is these two questions. to be noted that the enormity of dinosaurs must have caused The palaeontological analysis done by Sepkoski (I 992) extinction of many of the species of the Cretaceous Period. reveals that the Earth has suffered five major mass Though, final blow responsible for complete deterioration extinctions during its history: during Late Ordovician, the in the environment could be an impact that led to the death Devonian, the Pertnian, the Triassic and the Cretaceous. It of dinosaurs. is generally believed that the species become extinct when The Banner Basin is a narrow N-S trending graben. Its their rate of adaptation is not able to compete with the western margin is defined by a NNW-SSE trending fault environrnei~talstress. -
Scientific Drilling of the Boltysh Impact Crater, Ukraine
40th Lunar and Planetary Science Conference (2009) 1719.pdf SCIENTIFIC DRILLING OF THE BOLTYSH IMPACT CRATER, UKRAINE. J.S. Watson12, I. Gilmour1, S.P. Kelley2 and D.W. Jolley3. 1Planetary and Space Sciences Research Institute, The Open University, Milton Keynes, MK7 6AA, UK, 2Department of Earth and Environmental Sciences, The Open University, Milton Keynes, MK7 6AA, UK, 3Department of Geology and Petroleum Geology, University of Aberdeen, AB24 3UE, UK. Introduction: The Boltysh crater has been known span a period of up to 10Ma and contain occasional for several decades and was first drilled in the 1960s as macrofossils, including ostracods, fish and plant fos- part of a study of economic oil shale deposits. Unfor- sils. Preliminary palynological studies suggest that tunately, the cores were not curated and have been lost. initial sedimentation rates in the crater following the We have re-drilled the impact crater and have recov- impact may have been low followed by more rapid ered a near continuous record of ~400 m of organic- sedimentation through the Late Paleocene. rich sediments together with 15 m of suevite. The Boltysh crater: The Boltysh impact crater, cen- tred at 48°54’N and 32°15’E, is a complex impact structure formed on the crystalline basement rocks of the Ukrainian shield, which comprise porphyroblastic granites (age ca. 1.55 Ga) and biotite gneissses (age ca. 1.85 – 2.22 Ga) [1]. The structure is covered by Qua- ternary sediments and has been dated at 65.17±0.64 Ma [1]. At 24km diameter, the impact is unlikely to have contributed substantially to the worldwide deva- station at the end of the Cretaceous. -
Magyar Királyi Földtani Intézet (2006.)
A Magyar Állami Földtani Intézet Évi Jelentése, 2006 Meteoritkráter-tanulmányok Impact crater studies DON GYÖRGY, SOLT PÉTER Magyar Állami Földtani Intézet, H–1143 Budapest, Stefánia út 14. Tárgyszavak: meteoritkráter, szferula-szintek, Magyarmecske-anomália Összefoglalás Korábbi kutatásainkban különböző korú (perm–triász, késő-eocén, pleisztocén stb.) földtani képződményekben mutattunk ki kozmikus mikroszferula-dúsulásokat és meteorithullás-rekonstrukciót végeztünk a szórási mező szferula-eloszlása alapján. Jelen tanulmányban röviden tár- gyaljuk a meteoritkráterek geomorfológiai, kőzettani, ásványtani és geofizikai jellemzőit. A hazai impakt kráterek kutatásának története a kezde- tektől napjainkig. Eddig a feltételezett meteoritkráterek közül csak a magyarmecskei, geofizikai anomáliával kimutatott földtani szerkezet kozmikus eredete valószínű. A földtörténet során képződött nagyobb kráterek kiszórt anyaga a magyarországi földtani képződményekben is meg- található. Végül bemutatunk néhány észtországi, németországi és ukrajnai meteoritkrátert, melyeknél terepbejárás során összehasonlitó kőzetmintákat gyűjtöttünk. Keywords: impact crater, spherule-horizons, Magyarmecske-anomaly Abstract Former studies of the authors focused on cosmic spherule occurrences in the geological record, and meteorite fall reconstructions. We introduce the characteristic features (geomorphology, petrography, mineralogy, geophysics) and short description of impact cratering events. History of impact crater research in Hungary, buried crater in Magyarmecske detected -
Challenges in Indian Palaeobiology
Challenges in Indian Palaeobiology Current Status, Recent Developments and Future Directions © BIRBAL SAHNI INSTITUTE OF PALAEOBOTANY, LUCKNOW 226 007, (U.P.), INDIA Published by The Director Birbal Sahni Institute of Palaeobotany Lucknow 226 007 INDIA Phone : +91-522-2740008/2740011/ 2740399/2740413 Fax : +91-522-2740098/2740485 E-mail : [email protected] [email protected] Website : http://www.bsip.res.in ISBN No : 81-86382-03-8 Proof Reader : R.L. Mehra Typeset : Syed Rashid Ali & Madhavendra Singh Produced by : Publication Unit Printed at : Dream Sketch, 29 Brahma Nagar, Sitapur Road, Lucknow November 2005 Patrons Prof. V. S. Ramamurthy Secretary, Department of Science & Technology, Govt. of India Dr. Harsh K. Gupta Formerly Secretary, Department of Ocean Development, Govt. of India Prof. J. S. Singh Chairman, Governing Body, BSIP Prof. G. K. Srivastava Chairman, Research Advisory Committee, BSIP National Steering Committee Dr. N. C. Mehrotra, Director, BSIP - Chairman Prof. R.P. Singh, Vice Chancellor, Lucknow University - Member Prof. Ashok Sahni, Geology Department, Panjab University - Member Prof. M.P. Singh, Geology Department, Lucknow University - Member Dr. M. Sanjappa, Director, Botanical Survey of India - Member Dr. D. K. Pandey, Director (Exlporation), ONGC, New Delhi - Member Dr. P. Pushpangadan, Director, NBRI - Member Prof. S.K. Tandon, Geology Department, Delhi University - Member Dr. Arun Nigvekar, Former Chairman, UGC - Member Dr. K.P.N. Pandiyan, Joint Secretary & Financial Adv., DST - Member Local Organizing Committee Dr. N. C. Mehrotra, Director - Chairman Dr. Jayasri Banerji, Scientist ‘F’ - Convener Dr. A. K. Srivastava, Scientist ‘F’ - Member Dr. Ramesh K. Saxena, Scientist ‘F’ - Member Dr. Archana Tripathi, Scientist ‘F’ - Member Dr. -
Yaxcopoil-1 and the Chicxulub Impact
Int J Earth Sci (Geol Rundsch) (2004) 93: 1042–1065 First published in: DOI 10.1007/s00531-004-0431-6 ORIGINAL PAPER Wolfgang Stinnesbeck Æ Gerta Keller Æ Thierry Adatte Markus Harting Æ Doris Stu¨ben Æ Georg Istrate Utz Kramar Yaxcopoil-1 and the Chicxulub impact Received: 28 August 2003 / Accepted: 11 July 2004 / Published online: 29 October 2004 Ó Springer-Verlag 2004 Abstract CSDP core Yaxcopoil-1 was drilled to a depth Cenomanian organic-rich marly limestone. There is no of 1,511 m within the Chicxulub crater. An organic-rich evidence that these sediments represent crater infill due marly limestone near the base of the hole (1,495 to to megablocks sliding into the crater, such as major 1,452 m) was deposited in an open marine shelf envi- disruption of sediments, chaotic changes in lithology, ronment during the latest Cenomanian (uppermost overturned or deep dipping megablocks, major Rotalipora cushmani zone). The overlying sequence of mechanical fragmentation, shock or thermal alteration, limestones, dolomites and anhydrites (1,495 to 894 m) or ductile deformation. Breccia units that are interca- indicates deposition in various carbonate platform lated in the carbonate platform sequence are intrafor- environments (e.g., sabkhas, lagoons). A 100-m-thick mational in origin (e.g., dissolution of evaporites) and suevite breccia (894–794 m) identifies the Chicxulub dykes are rare. Major disturbances of strata by the im- impact event. Above the suevite breccia is a dolomitic pact therefore appear to have been confined to within limestone with planktic foraminiferal assemblages less than 60 km from the proposed impact center. -
6 Supplementary References
6 6 SUPPLEMENTARY REFERENCES 6 SUPPLEMENTARY REFERENCES 1203 6.1 GENERAL ENCYCLOPEDIAS Cosmology glossary. Western Washington Univ. Planetarium, Bellingham, WA; http://www.wwu.edu/depts/skywise/a101_cosmologyglossary.html. Bilder-Konversationslexikon. 4 vols., Brockhaus, Leipzig (1834). CXC Glossary of astrophysical terms. Chandra X-ray Center (CXC), operated Brockhaus Enzyklopädie. 20 vols., Brockhaus, Wiesbaden (1966–1974). for NASA by Harvard-Smithsonian Center for Astrophysics, Cambridge, Brockhaus-Konversationslexikon. 16 vols., Brockhaus, Leipzig (1892–1897). MA; http://chandra.harvard.edu/resources/glossaryA.html. Chambers’s encyclopaedia (ed. by M.D. LAW). 15 vols., International Learn- Dictionnaire des sciences naturelles (ed. by F.G. CUVIER). Levrault, Stras- ing Systems Corporation Ltd., London (1963). bourg (1816–1826). Columbia encyclopedia. Columbia University Press, New York (6th edn., Dictionary of medieval Latin from British sources (ed. by R.E. LATHAM and 2001–2005); http://www.bartleby.com/65/. D.R. HOWLETT). Oxford University Press, London; vol. 1 (1975) to vol. 6 Collier’s encyclopedia. 24 vols., Macmillan Education Co, New York (1987). (2003). Der Große Herder. 13 vols., Herder, Freiburg (1932–1935). Dictionary of mining, mineral, and related terms [compiled and edited by the Encyclopaedia Britannica. 29 vols. (11th edn., 1911). LoveToKnow™ free U.S. Bureau of Mines, U.S. Dept. of the Interior]. Am. Geol. Inst., Alex- online Encyclopedia; http://www.1911encyclopedia.org/. andria, VA (1997); http://www.maden.hacettepe.edu.tr/dmmrt/index.html. Encyclopaedia Britannica. 24 vols. (1875–1889), 24 vols. (1929), 24 vols. Dictionary of SDI (ed. by H. WALDMAN). Scholarly Resources Imprint, Wil- (1959); 30 vols. (1974–1984); 32 vols. (1985–2002) mington, DE (1988). -
'Heavenly Bounty' Some Thoughts on Impact Metallogeny
HEAVENLY BOUNTY 705 ‘Heavenly Bounty’ Some thoughts on Impact Metallogeny Impact cratering must be one of the most spectacular displays ever witnessed in the solar system. Although the ancient Indian astronomers, the ancient Vedic texts and the poets who have chronicled the history of India in the great Ra¯ma¯yana and Maha¯bha¯rata, described heavenly events in the past in lines of great poetic beauty, the subject has not evoked much interest in the modern generation of geoscientists. India has a hoary tradition of study of astronomical bodies, but these studies have come to be neglected, considered more as myths deserving no serious attention. Impact Metallogeny “Impact Metallogeny” may be defined as the study of major metallic and diamond deposits from the perspective of extra-terrestrial impacts that have been directly or indirectly responsible for metallogeny. An increasingly large body of evidence – geochemical (trace and rare element data, stable isotope systematics, field and structural data, geographical distribution patterns) is pointing to a causal link between impact processes and metallogeny either directly or indirectly. My plea is to re-examine our known large metallic and diamond areas from this fresh perspective so that we identify and characterise major impact structures and related metallogeny in the Indian sub-continent. The Mystery of Abnormal Concentration of Metals at Selected ‘Hot Spots’ in the Earth Spectacular concentrations of gold and uranium are to be found in the Witwatersrand Basin in South Africa, from where over 50,000 tonnes of gold have already been extracted and another 50,000 tonnes indicated in reserve; at Homestake Mines, (South Dakota); Colorado Mineral belt with its several large deposits; at Porcupine district of Ontario, (Canada); at Cadea (New South Wales), Kalgoorlie, Bendigo and Ballarat of Victoria, (Australia); nickel and platinum group elements at Sudbury (Canada); chromite, nickel and platinum at Bushveld (South Africa); nickel in Zimbabwe (Africa). -
Evaporite Interactions with Magma Part 3 of 3
www.saltworkconsultants.com Salty MattersJohn Warren - Saturday April 13, 2019 Evaporite interactions with magma Part 3 of 3: On-site evaporite and major extinction events? Introduction 60 The previous two articles in this series Siberian Traps dealt with heating evaporites, vola- tiles expelled into the atmosphere, 50 and major biotal extinction events. Emeishan Traps I argued that short-term heating of 40 Deccan Traps a megaevaporite mass during em- Cental Atlantic (+ Yucatan bolide) placement of a Large Igneous Prov- 30 Magmatic Province ince (LIP) or heating of evaporities at atmosphere into volatiles the site of a large bolide impact, will 20 of evaporitic volumes Large Carribean-Columbian move vast volumes of sulphurous Generic extinctions (%) Columbia Karoo Traps and halocarbon volatiles, as well as 10 Paraná Traps River Brito-Arctic Ontong-Java solids, CO2 and CH4 into the earth's No on-site upper atmosphere (Figure 1a). The Ethiopian Traps evaporites resulting catastrophic climatic effects 0 1 2 3 4 19 20 link in time and probable causes to A. Volume of ood basalts (x 106 km3) earth-scale major extinction hori- Emeishan Traps Siberian Traps zons. (Figure 1b). In this article shall (269-265Ma) (253-250Ma) examine how three of the five major Deccan Traps CAMP, Brazil Phanerozoic extinction events have 50 3. End-Permian (67-65Ma) an evaporite association, starting with (201.5Ma) the most intense extinction event of 40 1. Late Ordovican Capitanian 5. End-Cretaceous the Phanerozoic; the end-Permian 4.Late Triassic and its link to LIP emplacement into 30 two separate sequences of massive 2.