Disintegrated Comet Trail in Southern Tibet
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Terrestrial Impact Structures Provide the Only Ground Truth Against Which Computational and Experimental Results Can Be Com Pared
Ann. Rev. Earth Planet. Sci. 1987. 15:245-70 Copyright([;; /987 by Annual Reviews Inc. All rights reserved TERRESTRIAL IMI!ACT STRUCTURES ··- Richard A. F. Grieve Geophysics Division, Geological Survey of Canada, Ottawa, Ontario KIA OY3, Canada INTRODUCTION Impact structures are the dominant landform on planets that have retained portions of their earliest crust. The present surface of the Earth, however, has comparatively few recognized impact structures. This is due to its relative youthfulness and the dynamic nature of the terrestrial geosphere, both of which serve to obscure and remove the impact record. Although not generally viewed as an important terrestrial (as opposed to planetary) geologic process, the role of impact in Earth evolution is now receiving mounting consideration. For example, large-scale impact events may hav~~ been responsible for such phenomena as the formation of the Earth's moon and certain mass extinctions in the biologic record. The importance of the terrestrial impact record is greater than the relatively small number of known structures would indicate. Impact is a highly transient, high-energy event. It is inherently difficult to study through experimentation because of the problem of scale. In addition, sophisticated finite-element code calculations of impact cratering are gen erally limited to relatively early-time phenomena as a result of high com putational costs. Terrestrial impact structures provide the only ground truth against which computational and experimental results can be com pared. These structures provide information on aspects of the third dimen sion, the pre- and postimpact distribution of target lithologies, and the nature of the lithologic and mineralogic changes produced by the passage of a shock wave. -
Stishovite and Seifertite in Lunar Meteorite Northwest Africa 4734
71st Annual Meteoritical Society Meeting (2008) 5058.pdf FIRST EVIDENCE OF HIGH PRESSURE SILICA: STISHOVITE AND SEIFERTITE IN LUNAR METEORITE NORTHWEST AFRICA 4734. H. Chennaoui Aoudjehane1-2, A. Jambon2 1Université Hassan II Aïn Chock, Laboratoire Géosciences, BP 5366 Maârif Casa- blanca Morocco (e-mail: [email protected]), 2Université Pierre et Marie Curie-Paris6 and IPGP Laboratoire MAGIE, Case 110, 4 place Jussieu, 75252 Paris France. Introduction: Silica is a rare phase in lunar rocks; it has been described as either quartz, cristobalite and/or tridymite [1]. Northwest Africa 4734, is an uncommon type of lunar rock, which may be launched paired with the LaPaz Icefield Lunar Mare basalts found in 2002-03 in Antarctica [2-6], it is a coarse grained rock of basaltic composition, exhibits a number of sig- nificant shock features, such as PDFs, extensive fracturation of pyroxene, impact melt pockets and transformation of plagioclase to maskelynite; silica is present as a minor phase. Analytical procedures: We studied the speciation of silica polymorphs to characterize the shock, using SEM imaging, Ra- man spectroscopy, CL imaging and spectroscopy. Further details can be found in [7]. Results: According to the CL spectra [7-9], cristobalite, tridymite, high-pressure silica glass, stishovite and seifertite, are all present. Special emphasis is made on stishovite and seifertite, which, like in shergottites, exhibit specific textural features [7]. Cathodoluminescence spectra characteristic of high-pressure sil- ica phases: glass, stishovite and seifertite have been recorded in addition to the original low-pressure phases. The remanence of cristobalite and tridymite underscores a significant heterogeneity of the shock supported by the rock. -
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. -
EPSC2018-833, 2018 European Planetary Science Congress 2018 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2018
EPSC Abstracts Vol. 12, EPSC2018-833, 2018 European Planetary Science Congress 2018 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2018 Impact melt boulder from northern Sweden from an unknown source Timmu Kreitsmann (1), Satu Hietala (2), Tapio Soukka (3), Jüri Plado (1), Jari Nenonen (2) and Lauri J. Pesonen (4) (1) Department of Geology, University of Tartu, Estonia ([email protected], [email protected]), (2) Geological Survey of Finland, Finland ([email protected], [email protected]), (3) Oulu Mining School, University of Oulu, Finland ([email protected]) (4) Solid Earth Geophysics Laboratory, Physics Department, University of Helsinki, Finland ([email protected]) Abstract We report an impact melt rock finding from northern Sweden, near the village of Kitkiöjärvi. There is no confirmed meteorite impact structure nearby, thus, the source is currently undiscovered. The impact origin of the finding was confirmed by the presence of planar deformation features (PDFs) in quartz. 1. Introduction Impact cratering is a common and frequent process that affects the planetary surfaces across the solar system throughout geologic time. On Earth, there are 191 confirmed impact structures which are distributed unevenly around the globe. The Fennoscandian Shield houses around 10% of them. Here, we report an impact melt rock finding that originates from an unknown structure in northern Sweden. The semi-rounded impactite boulder, sized 10 × 7 cm, was found by Tapio Soukka in 2017 from a gravel pit at the western side of village Kitkiöjärvi (67°46'16"N 23°03'06"E; Fig. 1). Figure 1: Proven impact structures in Fennoscandia. -
"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. -
A New Way to Confirm Meteorite Impact Produced Planar Features in Quartz: Combining Universal Stage and Electron Backscatter Diffraction Techniques
A new way to confirm meteorite impact produced planar features in quartz: combining Universal Stage and Electron Backscatter Diffraction techniques M.H. Voorn MSc Thesis August 2010 Utrecht University - Earth Sciences department Structural Geology and Tectonic research group Abstract As recognised from the geological record, meteorite impact events can have a severe influence on (local) geology, climate and life. Solid evidence for these events is therefore important to obtain. The most convincing evidence comes from microstructures in quartz. Upon impact, Planar Fractures (PFs) and Planar Deformation Features (PDFs) form parallel to specific crystallographic planes in quartz. Non-impact formed (tectonic) Deformation Lamellae (DL) may be hard to distinguish qualitatively from PFs or PDFs with the optical microscope, but do not form parallel to crystallographic planes. Quantitative methods using the Universal Stage (U-Stage) on the optical microscope have therefore been applied widely to (dis)confirm this parallelism. With the method, the quartz c-axis and poles to planar features are measured and plotted. An improved technique requires so-called indexing of the measured orientations using a stereographic projection template. Even when these techniques are applied, some proposed impact structures remain debated. An important reason for this is the U-stage can not provide the full crystal orientation of quartz. The goal of this thesis was to check the classical U-stage techniques for quantitatively confirming impact planar features in quartz, and to see whether the addition of Electron Backscatter Diffraction (EBSD, on the Scanning Electron Microscope: SEM) and Cathodoluminescence (CL, on the SEM) can provide more solid evidence. Six previously confirmed impact and three non-impact samples were studied. -
ANIC IMPACTS: MS and IRONMENTAL P ONS Abstracts Edited by Rainer Gersonde and Alexander Deutsch
ANIC IMPACTS: MS AND IRONMENTAL P ONS APRIL 15 - APRIL 17, 1999 Alfred Wegener Institute for Polar and Marine Research Bremerhaven, Germany Abstracts Edited by Rainer Gersonde and Alexander Deutsch Ber. Polarforsch. 343 (1999) ISSN 01 76 - 5027 Preface .......3 Acknowledgements .......6 Program ....... 7 Abstracts P. Agrinier, A. Deutsch, U. Schäre and I. Martinez: On the kinetics of reaction of CO, with hot Ca0 during impact events: An experimental study. .11 L. Ainsaar and M. Semidor: Long-term effect of the Kärdl impact crater (Hiiumaa, Estonia) On the middle Ordovician carbonate sedimentation. ......13 N. Artemieva and V.Shuvalov: Shock zones on the ocean floor - Numerical simulations. ......16 H. Bahlburg and P. Claeys: Tsunami deposit or not: The problem of interpreting the siliciclastic K/T sections in northeastern Mexico. ......19 R. Coccioni, D. Basso, H. Brinkhuis, S. Galeotti, S. Gardin, S. Monechi, E. Morettini, M. Renard, S. Spezzaferri, and M. van der Hoeven: Environmental perturbation following a late Eocene impact event: Evidence from the Massignano Section, Italy. ......21 I von Dalwigk and J. Ormö Formation of resurge gullies at impacts at sea: the Lockne crater, Sweden. ......24 J. Ebbing, P. Janle, J, Koulouris and B. Milkereit: Palaeotopography of the Chicxulub impact crater and implications for oceanic craters. .25 V. Feldman and S.Kotelnikov: The methods of shock pressure estimation in impacted rocks. ......28 J.-A. Flores, F. J. Sierro and R. Gersonde: Calcareous plankton stratigraphies from the "Eltanin" asteroid impact area: Strategies for geological and paleoceanographic reconstruction. ......29 M.V.Gerasimov, Y. P. Dikov, 0 . I. Yakovlev and F.Wlotzka: Experimental investigation of the role of water in the impact vaporization chemistry. -
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. -
Twinning, Reidite, and Zro in Shocked Zircon from Meteor Crater
Transformations to granular zircon revealed: Twinning, reidite, and ZrO2 in shocked zircon from Meteor Crater (Arizona, USA) Aaron J. Cavosie1,2,3, Nicholas E. Timms1, Timmons M. Erickson1, Justin J. Hagerty4, and Friedrich Hörz5 1TIGeR (The Institute for Geoscience Research), Department of Applied Geology, Curtin University, Perth, WA 6102, Australia 2NASA Astrobiology Institute, Department of Geoscience, University of Wisconsin–Madison, Madison, Wisconsin 53706, USA 3Department of Geology, University of Puerto Rico–Mayagüez, Mayagüez, Puerto Rico 00681, USA 4U.S. Geological Survey (USGS) Astrogeology Science Center, Flagstaff, Arizona 86001, USA 5NASA Johnson Space Center, Science Department/Jets/HX5/ARES, Houston, Texas 77058, USA ABSTRACT Granular zircon in impact environments has long been recognized but remains poorly A N35° 2.0’ W111° 0.9’ understood due to lack of experimental data to identify mechanisms involved in its genesis. Meteor Crater in Arizona (USA) contains abundant evidence of shock metamorphism, includ- N ing shocked quartz, the high-pressure polymorphs coesite and stishovite, diaplectic SiO2 glass, and lechatelierite (fused SiO2). Here we report the presence of granular zircon, a new shocked-mineral discovery at Meteor Crater, that preserve critical orientation evidence of specific transformations that occurred during formation at extreme impact conditions. The zircon grains occur as aggregates of sub-micrometer neoblasts in highly shocked Coconino Sandstone (CS) comprised of lechatelierite. Electron backscatter diffraction shows that each MCC2 site grain consists of multiple domains, some with boundaries disoriented by 65° around <110>, (main shaft) a known {112} shock-twin orientation. Other domains have {001} in alignment with {110} of neighboring domains, consistent with the former presence of the high-pressure ZrSiO4 polymorph reidite. -
Evaluating the Influence of Meteorite Impact Events on Global Potassium Feldspar Availability to the Atmosphere Since 600 Ma
Research article Journal of the Geological Society Published online November 27, 2018 https://doi.org/10.1144/jgs2018-084 | Vol. 176 | 2019 | pp. 209–224 Evaluating the influence of meteorite impact events on global potassium feldspar availability to the atmosphere since 600 Ma B. C. Coldwell1,2 & M. J. Pankhurst1,2,3,4,5* 1 Instituto Tecnológico y de Energías Renovables (ITER), 38600 Granadilla de Abona, Santa Cruz de Tenerife, Spain 2 Instituto Volcanológico de Canarias (INVOLCAN), Calle Álvaro Martín Díaz 1, 38320 San Cristóbal de La Laguna, Santa Cruz de Tenerife, Spain 3 School of Materials, University of Manchester, Manchester M13 9PJ, UK 4 Research Complex at Harwell, Harwell Campus, Didcot OX11 0FA, UK 5 School of Earth and Environment, University of Leeds, Leeds LS2 9JT, UK B.C.C., 0000-0001-9240-6240; M.J.P., 0000-0001-6844-9822 * Correspondence: [email protected] Abstract: Potassium feldspar present in global mineral aerosol (<5%) plays a disproportionate role in modulating the microphysics of mixed-phase cloud. Via exceptional ice nucleation properties, it is capable of changing cloud properties and behaviour. Here we identify times of substantial and abrupt change in the global availability of potassium feldspar since 600 Ma. Normally, weathering and vegetation cover contribute to low availability, with clay dominating mineral aerosol. Periods of maximum availability are reasoned to follow the emplacement and remobilization of ejecta blankets from major meteorite impact events, before returning to background after some hundreds to thousands of years. We review the 44 largest confirmed craters and evaluate the potassium feldspar content of their target rocks, which range from c. -
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. -
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).