Evolutionary Catastrophes: the Science of Mass Extinction
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Vincent COURTILLOT - Publications
1 Vincent COURTILLOT - Publications Books (or Book Chapters) 1- La dérive des continents V. COURTILLOT et P. TAPPONNIER In La mémoire de la Terre, par A. ADOUTTE,…,V.COURTILLOT,…. , 115-125, Seuil, Paris, 1992. 2- La Vie en Catastrophes V. COURTILLOT 279 pp., Fayard, Paris, 1995. (translated in German and English, 1999) 3- Evolutionnary Catastrophes: The Science of Mass Extinction V. COURTILLOT 171 pp., Cambridge University Press, Cambridge, 1999. (translation and update) Paperback in 2002 4- La dynamique du Globe contrôle-t’elle l’évolution des espèces ? V. COURTILLOT in Qu’est ce que la vie ? Y. Michaud ed., Université de tous les savoirs, vol. 1, pp. 149-162, Editions Odile Jacob, Paris, 2000. 5- L’observation du globe V. COURTILLOT in Le renouvellement de l’observation dans les sciences, Y. Michaud ed., Université de tous les savoirs, pp. 115-118, Editions Odile Jacob, Paris, 2003. 6- Volcanisme et évolution de la vie sur terre V. COURTILLOT in Qu’est ce que la diversité de la vie ?, Y. Michaud ed., Université de tous les savoirs, pp. 133-145, Editions Odile Jacob, Paris, 2003. 7- Nouveau Voyage au Centre de la Terre (provisional title) V. COURTILLOT Editions Odile Jacob, Paris,to be published September 2009. Articles for the public at large (Scientific American type) 1- Les panaches, moteur de la dérive des continents V. COURTILLOT La Recherche, 32, 270-272 (1973) 2- Crise de l'énergie: la solution géothermique 2 V. COURTILLOT La Recherche, 35, 586-587 (1973) 3- Volcanisme et tectonique en Islande P. TAPPONNIER, V. COURTILLOT La Recherche, 37, (1973) 4- La prédiction des tremblements de terre V. -
C.V. De Vincent Courtillot, Membre De L'académie Des Sciences
Vincent Courtillot Élu Membre le 18 novembre 2003 dans la section Sciences de l'univers Vincent Courtillot, né en 1948, ancien élève de l'École des mines de Paris, docteur ès sciences, diplômé de l'université de Stanford (Californie), est professeur de géophysique à l'université Denis- Diderot à Paris. Il a enseigné à l'université de Stanford, Santa Barbara et au California Institute of Technology (Caltech). Il a été directeur de la recherche et des études doctorales au ministère de l'Éducation nationale, conseiller spécial du Ministre de l'Éducation nationale, de la recherche et de la technologie (1997-1998), puis directeur de la recherche (1998-2001). Il a fondé et présidé le premier Conseil scientifique de la Ville de Paris (2002-2009). Il est le directeur sortant de l'Institut de Physique du Globe de Paris (2004-2010). Géophysicien, Vincent Courtillot est un spécialiste du paléomagnétisme et de la géodynamique. Il a apporté de nombreux résultats sur les déformations continentales, les épanchements basaltiques ainsi que leurs conséquences et a très fortement contribué aux grandes études de reconstruction paléogéographique. Les premiers travaux de V. Courtillot portent sur la théorie des champs de potentiel et les variations temporelles du champ magnétique terrestre (découverte des sauts d’accélération séculaire). La réalisation d’un levé aéromagnétique en Afar lui permet de découvrir le premier exemple de propagation d’un rift en milieu continental. En 1980 il fonde avec J.P. Pozzi le laboratoire de paléomagnétisme de l’IPGP et il s’associe ensuite avec P.Y. Gillot pour cofonder à l’université Paris Sud – Orsay un laboratoire de géochronologie multi-techniques. -
The ``Van Zijl'' Jurassic Geomagnetic Reversal Revisited
The “van Zijl” Jurassic geomagnetic reversal revisited Maud Moulin, Vincent Courtillot, Frédéric Fluteau, Jean-Pierre Valet To cite this version: Maud Moulin, Vincent Courtillot, Frédéric Fluteau, Jean-Pierre Valet. The “van Zijl” Jurassic ge- omagnetic reversal revisited. Geochemistry, Geophysics, Geosystems, AGU and the Geochemical Society, 2012, 13 (3), 10.1029/2011GC003910. hal-02139522 HAL Id: hal-02139522 https://hal.archives-ouvertes.fr/hal-02139522 Submitted on 24 May 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Article Volume 13, Number 3 13 March 2012 Q03010, doi:10.1029/2011GC003910 ISSN: 1525-2027 The “van Zijl” Jurassic geomagnetic reversal revisited Maud Moulin Equipe de Paléomagnétisme, Institut de Physique du Globe, UMR 7154, Sorbonne Paris Cité, F-75005 Paris, France Sciences de la Terre, de l’Environnement et des Planètes, Université Paris Diderot, Sorbonne Paris Cité, F-75013 Paris, France Now at Département de Géologie, Université Jean Monnet, F-42023 Saint Etienne, France ([email protected]) Vincent Courtillot, Frédéric Fluteau, and Jean-Pierre Valet Equipe de Paléomagnétisme, Institut de Physique du Globe, UMR 7154, Sorbonne Paris Cité, F-75005 Paris, France Sciences de la Terre, de l’Environnement et des Planètes, Université Paris Diderot, Sorbonne Paris Cité, F-75013 Paris, France [1] We have collected two new detailed records of what could be the second oldest well documented reversal, the “van Zijl” Jurassic (180 Ma) reversal recorded in the thick basalt sequences of the Karoo large igneous province in Lesotho and South Africa. -
Apparent and True Polar Wander and the Geometry of the Geomagnetic
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. B11, 2300, doi:10.1029/2000JB000050, 2002 Correction published 10 October 2003 Apparent and true polar wander and the geometry of the geomagnetic field over the last 200 Myr Jean Besse and Vincent Courtillot Laboratoire de Pale´omagne´tisme, UMR 7577, Institut de Physique du Globe de Paris, Paris, France Received 8 November 2000; revised 15 January 2002; accepted 20 January 2002; published 15 November 2002. [1] We have constructed new apparent polar wander paths (APWPs) for major plates over the last 200 Myr. Updated kinematic models and selected paleomagnetic data allowed us to construct a master APWP. A persistent quadrupole moment on the order of 3% of the dipole over the last 200 Myr is suggested. Paleomagnetic and hot spot APW are compared, and a new determination of ‘‘true polar wander’’ (TPW) is derived. Under the hypothesis of fixed Atlantic and Indian hot spots, we confirm that TPW is episodic, with periods of (quasi) standstill alternating with periods of faster TPW (in the Cretaceous). The typical duration of these periods is on the order of a few tens of millions of years with wander rates during fast tracks on the order of 30 to 50 km/Myr. A total TPW of some 30° is suggested for the last 200 Myr. We find no convincing evidence for episodes of superfast TPW such as proposed recently by a number of authors. Comparison over the last 130 Myr of TPW deduced from hot spot tracks and paleomagnetic data in the Indo-Atlantic hemisphere with an independent determination for the Pacific plate supports the idea that, to first order, TPW is a truly global feature of Earth dynamics. -
Convective Patterns Under the Indo-Atlantic T Box R
Earth and Planetary Science Letters 239 (2005) 233–252 www.elsevier.com/locate/epsl Convective patterns under the Indo-Atlantic T box r Anne Davaille a,*, Ele´onore Stutzmann a, Grac¸a Silveira b,c, Jean Besse a, Vincent Courtillot a a Institut de Physique du Globe and CNRS, 4 Place Jussieu, 75252 Paris cedex 05, France b Centro de Geofı´sica da Universidade de Lisboa Edifı´cio C8, Campo Grande, 1749-016 LISBOA, Portugal c Instituto Superior de Engengaria de Lisboa Avenida Conselheiro Emı´dio Navarro, 1949-014 LISBOA, Portugal Received 4 January 2005; received in revised form 23 July 2005; accepted 27 July 2005 Available online 10 October 2005 Editor: S. King Abstract Using fluid mechanics, we reinterpret the mantle images obtained from global and regional tomography together with geochemical, geological and paleomagnetic observations, and attempt to unravel the pattern of convection in the Indo-Atlantic bboxQ and its temporal evolution over the last 260 Myr. The T box r presently contains a) a broad slow seismic anomaly at the CMB which has a shape similar to Pangea 250 Myr ago, and which divides into several branches higher in the lower mantle, b) a bsuperswellQ centered on the western edge of South Africa, c) at least 6 bprimary hotspotsQ with long tracks related to traps, and d) numerous smaller hotspots. In the last 260 Myr, this mantle box has undergone 10 trap events, 7 of them related to continental breakup. Several of these past events are spatially correlated with present-day seismic anomalies and/or upwellings. Laboratory experiments show that superswells, long-lived hotspot tracks and traps may represent three evolutionary stages of the same phenomenon, i.e. -
Post-Impact Structural Crater Modification Due to Sediment Loading: an Overlooked Process
Meteoritics & Planetary Science 42, Nr 11, 2013–2029 (2007) Abstract available online at http://meteoritics.org Post-impact structural crater modification due to sediment loading: An overlooked process Filippos TSIKALAS†* and Jan Inge FALEIDE2 Department of Geosciences, University of Oslo, P.O. Box 1047 Blindern, NO-0316 Oslo, Norway †Present address: ENI Norge AS, P.O. Box 101 Forus, NO-4064 Stavanger, Norway *Corresponding author. E-mail: [email protected]; [email protected] (Received 02 November 2006; revision accepted 16 February 2007) Abstract–Post-impact crater morphology and structure modifications due to sediment loading are analyzed in detail and exemplified in five well-preserved impact craters: Mjølnir, Chesapeake Bay, Chicxulub, Montagnais, and Bosumtwi. The analysis demonstrates that the geometry and the structural and stratigraphic relations of post-impact strata provide information about the amplitude, the spatial distribution, and the mode of post-impact deformation. Reconstruction of the original morphology and structure for the Mjølnir, Chicxulub, and Bosumtwi craters demonstrates the long-term subsidence and differential compaction that takes place between the crater and the outside platform region, and laterally within the crater structure. At Mjølnir, the central high developed as a prominent feature during post-impact burial, the height of the peak ring was enhanced, and the cumulative throw on the rim faults was increased. The original Chicxulub crater exhibited considerably less prominent peak- ring and inner-ring/crater-rim features than the present crater. The original relief of the peak ring was on the order of 420–570 m (currently 535–575 m); the relief on the inner ring/crater rim was 300– 450 m (currently ∼700 m). -
Resolving the Timing of Events Around the Cretaceous-Paleogene Boundary
Resolving the timing of events around the Cretaceous-Paleogene Boundary By Courtney Jean Sprain A dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in Earth and Planetary Science in the Graduate Division of the University of California, Berkeley Committee in charge: Professor Paul R. Renne, Chair Professor Mark A. Richards Professor William A. Clemens Spring 2017 Resolving the timing of events around the Cretaceous-Paleogene Boundary Copyright 2017 by Courtney Jean Sprain Abstract Resolving the timing of events around the Cretaceous-Paleogene Boundary by Courtney Jean Sprain Doctor of Philosophy in Earth and Planetary Science University of California, Berkeley Professor Paul R. Renne, Chair Despite decades of study, the exact cause of the Cretaceous-Paleogene boundary (KPB) mass extinction remains contentious. Hypothesized scenarios center around two main environmental perturbations: voluminous (>106 km3) volcanic eruptions from the Deccan Traps in modern-day India, and the large impact recorded by the Chicxulub crater. The impact hypothesis has gained broad support, bolstered by the discoveries of iridium anomalies, shocked quartz, and spherules at the KPB worldwide, which are contemporaneous with the Chicxulub impact structure. However, evidence for protracted extinctions, particularly in non-marine settings, and paleoenvironmental change associated with climatic swings before the KPB, challenge the notion that the impact was the sole cause of the KPB mass extinction. Despite forty years of study, the relative importance of each of these events is unclear, and one key inhibitor is insufficient resolution of existing geochronology. In this dissertation, I present work developing a high-precision global chronologic framework for the KPB that outlines the temporal sequence of biotic changes (both within the terrestrial and marine realms), climatic changes, and proposed perturbations (i.e. -
© in This Web Service Cambridge University
Cambridge University Press 978-0-521-81928-2 - Perilous Planet Earth: Catastrophes and Catastrophism Through the Ages Trevor Palmer Index More information Index Abbas, Asfar and Samar, 206 Alvarez, Walter, 214–18, 222, 223, 226, 234, 235, Abu Ruwash (Egypt), 325, 326 237, 238, 242, 250, 272, 278, 280, 282, 283, acid rain, 204, 222, 232, 233, 239, 336, 342, 365 350 American Association for the Advancement of acquired characteristics, inheritance of, 29, 33, 61, Science, 124 80, 86–8, 91, 93, 167, 173. American Museum of Natural History, 107, 138, Acraman impact structure (Australia), 257 151, 164, 300 actualism, principle of, 19, 46, 77 amino acids, 92, 235 adaptive evolution, 88–91, 97, 102, 147, 148, 151, ammonites, 215, 229, 265, 269 155–7, 169, 178, 181 ammonoids, 133, 265, 269 adaptive mutations, 175 Amor asteroids, 192 Afar region (Ethiopia), hominid fossils from, 108, 1999 AN10 (asteroid), 200 161, 162, 289 Ancient Mysteries (James and Thorpe), 319, 320, Africa–Eurasia collision, 26, 287, 302 347, 348 Agassiz, Louis, 41, 49, 53, 54, 59, 72 Anders, Mark, 233 Ager, Derek, 30 Anderson, David, 352 age of the Earth, 5, 6, 14, 18, 19, 33, 34, 82, 83, Andromedid meteors, 57 172, 173 Angkor complex (Cambodia), 328, 329 Ahrens, Thomas, 208 Annals of Fulda, 353–8 Akkad civilisation, 340 Annals of St. Bertin, 353–6 Akrotiri (Santorini), 131, 132, 335 Annals of Xanten, 353–7 Al’Amarah Crater (Iraq), 348 anoxia, 256, 257, 259–64, 267, 268, 284–6, 315, Alamo Crater (Nevada), 261 366 Alaska earthquake, 211 Antarctica–Australia separation, 269, -
Evolutionary Catastrophes: the Science of Mass Extinction Vincent Courtillot Frontmatter More Information
Cambridge University Press 0521583926 - Evolutionary Catastrophes: The Science of Mass Extinction Vincent Courtillot Frontmatter More information Evolutionary Catastrophes Why did the dinosaurs and two-thirds of all living species vanish from the face of the Earth sixty-five million years ago? Throughout the history of life, a small number of cat- astrophic events have caused mass extinction and changed the path of evolution forever. Two main theories have emerged to account for these dramatic events: asteroid impact and massive volcanic eruptions, both leading to nuclear-like winter. In recent years, the impact hypothesis has gained precedence, but Vincent Courtillot suggests that cataclysmic volcanic activity can be linked not only to the K–T mass extinction but also to most of the main mass extinction events in the history of the Earth. Courtillot’s book explodes some of the myths surrounding one of the most controversial arguments in science. It shows among other things that the impact and volcanic scenarios may not be mutually exclusive. This story will fascinate everyone interested in the history of life and death on our planet. VINCENT COURTILLOT is a graduate of the Paris School of Mines, Stanford University, and University of Paris. He is Professor of Geophysics at the University of Paris (Denis Diderot) and heads a research group at Institut de Physique du Globe. His work has focused on time variations of the Earth’s magnetic field, plate tectonics (continental rift- ing and collision), magnetic reversals, and flood basalts and their possible relation to mass extinctions. He has published papers in professional journals, and a book entitled La Vie en Catastrophes (Fayard, Paris, France, ). -
Evolutionary Catastrophes: the Science of Mass Extinction Vincent Courtillot Frontmatter More Information
Cambridge University Press 978-0-521-89118-9 - Evolutionary Catastrophes: The Science of Mass Extinction Vincent Courtillot Frontmatter More information Evolutionary Catastrophes Why did the dinosaurs and two-thirds of all living species vanish from the face of the Earth sixty-five million years ago? Throughout the history of life, a small number of cat- astrophic events have caused mass extinction and changed the path of evolution forever. Two main theories have emerged to account for these dramatic events: asteroid impact and massive volcanic eruptions, both leading to nuclear-like winter. In recent years, the impact hypothesis has gained precedence, but Vincent Courtillot suggests that cataclysmic volcanic activity can be linked not only to the K–T mass extinction but also to most of the main mass extinction events in the history of the Earth. Courtillot’s book explodes some of the myths surrounding one of the most controversial arguments in science. It shows among other things that the impact and volcanic scenarios may not be mutually exclusive. This story will fascinate everyone interested in the history of life and death on our planet. VINCENT COURTILLOT is a graduate of the Paris School of Mines, Stanford University, and University of Paris. He is Professor of Geophysics at the University of Paris (Denis Diderot) and heads a research group at Institut de Physique du Globe. His work has focused on time variations of the Earth’s magnetic field, plate tectonics (continental rift- ing and collision), magnetic reversals, and flood basalts and their possible relation to mass extinctions. He has published papers in professional journals, and a book entitled La Vie en Catastrophes (Fayard, Paris, France, ). -
African Meteorite Impact Craters: Characteristics and Geological Importance
Journal of African Earth Sciences, Vol. 18, No. 4, pp. 263-295, 1994 Pergamon Copyright © 1994 Elsevier Science Ltd Printed in Great Britain. All rights reserved 0899-5362/94 $7.00 + 0.00 0899-5362(94)00044-1 African meteorite impact craters: characteristics and geological importance CHRISTIAN KOEBERLt~ 1Institute of Geochemistry, University of Vienna, Dr.-Karl-Lueger-Ring 1, A-1010 Vienna, Austria. 2Economic Geology Research Unit, Depa~ i.ment of Geology, University of the Witwatemmnd,Johannesburg 2050, South Africa. (Received 26 October 1993 : accepted 12 May 1994) Abslzact - Geologists have realized that impact cratering is the single most important surface-forming and modifying process for the other terrestrial planets and the satellites of all planets. The recognition of impact cratering as an important geological process on earth has been rather slow. However, geologists are now realizing that giant impacts have had a determining influence on the geological and biological evolution of our planet. The study of impact craters allows important conclusions, not only about the origin mid history of our solar system and its planets, but also about a fundamentally important geological process. In addition, impact craters may have a definite economic importance as some craters have been shown to contain important mineral or oil deposits. F'dtesn meteorite impact craters have so far been identified on the African continent:. Amguid (Algeria), Aomunga (Chad), Aouelloul (Mauritania), B.P. (Libya), Bosumtwi (Ghana), Highbury (Zimbabwe), Kalkkop (South Africa), Oasis (Libya), Ouarkziz (Algeria), Roter Kamm (Namibia), Saitpan (South Africa), Talemzane (Algeria), Tenoumer (Mauritania), T'm Bider (Algeria), and V~:lefort (South Africa). -
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Index [Italic page numbers indicate major references] A arsenic, 116, 143, 168 brecciation, shock, 225, 231 Ashanti crater, Ghana. See Bosumtwi Brent crater, Ontario, 321 Abitibi Subprovince, 305 crater, Ghana bromine, 137 Acraman depression, South Australia, A thy ris Broodkop Shear Zone, 180 211, 212, 218 gurdoni transversalis, 114 Budevska crater, Venus, 24 geochemistry, 216 hunanensis, 114 Bunyeroo Formation, 209, 210, 219, geochronology, 219 aubrite, 145 220, 221, 222 melt rock, 216, 218 augite, 159 Bushveld layered intrusion, 337 paleomagnetism, 219 Australasian strewn field, 114, 133, See also Acraman impact structure 134, 137, 138, 139, 140, 143, Acraman impact structure, South C 144, 146 Australia, 209 australite, 136, 141, 145, 146 Cabin-Medicine Lodge thrust system, Adelaid Geosyncline, 210, 220, 222 Austria, moldavites, 142 227 adularía, 167 Cabin thrust plate, 173, 225, 226, Aeneas on Dione crater, Earth, 24 227, 231, 232 aerodynamically shaped tektites, 135 B calcite, 112, 166 Al Umchaimin depression, western Barbados, tektites, 134, 139, 142, 144 calcium, 115, 116, 128 Iraq, 259 barium, 116, 169, 216 calcium oxide, 186, 203, 216 albite, 209 Barrymore crater, Venus, 44 Callisto, rings, 30 Algoman granites, 293 Basal Member, Onaping Formation, Cambodia, circular structure, 140, 141 alkali, 156, 159, 167 266, 267, 268, 271, 272, 273, Cambrian, Beaverhead impact alkali feldspar, 121, 123, 127, 211 289, 290, 295, 296, 299, 304, structure, Montana, 163, 225, 232 almandine-spessartite, 200 307, 308, 310, 311, 314 Canadian Arctic,