Postscript-The Hammer and the Pendulum
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13076197 Tanvir Tabassum Final Version of Submission.Pdf
Finding Close Encounters: Toward a consensus on the influence of the stellar flybys on the Solar System over 10 million years Supervised by: Author: Dr Fabo Feng Tabassum Shahriar Tanvir Dr James L Collett Professor Hugh Jones Centre for Astrophysics Research School of Physics, Astronomy and Mathematics University of Hertfordshire Submitted to the University of Hertfordshire in partial fulfilment of the requirements of the degree of Master of Science by Research. October 2018 Abstract This thesis is a study of possible stellar encounters of the Sun, both in the past and in the future within ±10 Myr of the current epoch. This study is based on data gleaned from the first Gaia data release (Gaia DR1). One of the components of the Gaia DR1 is the TGAS catalogue. TGAS contained five astrometric parameters for more than two million stars. Four separate catalogues were used to provide radial velocities for these stars. A linear motion approximation was used to make a cut within an initial catalogue keeping only the stars that would have perihelia within 10 pc. 1003 stars were found to have a perihelion distance less than 10 pc. Each of these stars was then cloned 1000 times from their covariance matrix from Gaia DR1. The stars’ orbits were numerically integrated through a model galactic potential. After the integration, a particularly interesting set of candidates was selected for deeper study. In particular stars with a mean perihelion distance less than 2 pc were chosen for a deeper study since they will have significant influence on the Oort cloud. 46 stars were found to have a mean perihelion distance less than 2 pc. -
A Possible Albian Impact Crater at Murshid, Southern Oman
GeoArabia, Vol. 7, No. 4, 2002 Gulf PetroLink, Bahrain A possible Albian impact crater at Murshid, southern Oman Bruce Levell1, Pascal Richard2 and Folco Hoogendijk2, Petroleum Development Oman ABSTRACT During interpretation of a 3-D seismic survey in southern Oman a solitary, 2.5-km-wide circular basin with a central peak and raised rim was identified in the subsurface 35 km west of the Marmul oil field. The feature is the only one of its kind in the area. The basinal structure is probably of Late Cretaceous (Albian) age and the regional geology strongly suggests that it is neither a volcanic crater nor related to salt-dome tectonics or salt dissolution. It possibly represents a crater formed by a terrestrial impact event and has been named the Murshid crater. This report does not constitute a detailed investigation of the possible impact crater but rather records the 3-D seismic observations and the drilling that has taken place near the structure so far. INTRODUCTION During interpretation of a newly acquired 3-D seismic survey for oil exploration in southern Oman, a solitary 2.5-km-diameter circular basinal feature was identified as a possible impact structure and was named the Murshid crater. It lies 35 km west of the Marmul oil field in the South Oman Salt Basin (Figure 1). The center of the structure is at latitude 18º10’59"N, longitude 54º55’08”E, and it is buried at a depth of approximately 380 m below mean sea level (680 m below the ground surface). The authors are petroleum geologists who felt that the Murshid basinal structure needed reporting to the wider scientific community. -
Magnetic Properties and Redox State of Impact Glasses: a Review and New Case Studies from Siberia
geosciences Review Magnetic Properties and Redox State of Impact Glasses: A Review and New Case Studies from Siberia Pierre Rochette 1,* , Natalia S. Bezaeva 2,3, Andrei Kosterov 4 ,Jérôme Gattacceca 1, Victor L. Masaitis 5, Dmitry D. Badyukov 6, Gabriele Giuli 7 , Giovani Orazio Lepore 8 and Pierre Beck 9 1 Aix Marseille Université, CNRS, IRD, Coll. France, INRA, CEREGE, 13545 Aix-en-Provence, France; [email protected] 2 Institute of Geology and Petroleum Technologies, Kazan Federal University, 4/5 Kremlyovskaya Str., 420008 Kazan, Russia; [email protected] 3 Institute of Physics and Technology, Ural Federal University, 19 Mira Str., 620002 Ekaterinburg, Russia 4 St. Petersburg State University, 199034 St. Petersburg, Russia; [email protected] 5 A.P. Karpinsky Russian Geological Research Institute (VSEGEI), Sredny prospect 74, 199106 St. Petersburg, Russia; [email protected] 6 V.I. Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, 19 Kosygin str., 119991 Moscow, Russia; [email protected] 7 School of Science and Technology-Geology division, University of Camerino, Via Gentile III da Varano, 62032 Camerino (MC), Italy; [email protected] 8 CNR-IOM-OGG c/o ESRF, 71 Avenue des Martyrs CS 40220, F-38043 Grenoble, France; [email protected] 9 Université Grenoble Alpes, CNRS, IPAG, UMR5274, 38041 Grenoble, France; [email protected] * Correspondence: [email protected]; Tel.: +33-442971562 Received: 26 February 2019; Accepted: 11 May 2019; Published: 15 May 2019 Abstract: High velocity impacts produce melts that solidify as ejected or in-situ glasses. We provide a review of their peculiar magnetic properties, as well as a new detailed study of four glasses from Siberia: El’gygytgyn, Popigai, urengoites, and South-Ural glass (on a total of 24 different craters or strewn-fields). -
October 2003 SOCIETY
ISSN 0739-4934 NEWSLETTER HISTORY OF SCIENCE VOLUME 32 NUMBER 4 October 2003 SOCIETY those with no interest in botany, the simple beauty of the glass is enough. Natural History Delights in Cambridge From modern-life in glass to long-ago life, it’s only a short walk. The museum houses ant to discuss dinosaurs, explore microfossils of some of the Earth’s earliest life Wancient civilizations, learn wild- forms, as well as fossil fish and dinosaurs – flower gardening, or study endangered such as the second ever described Triceratops, species? If variety is the spice of life, then and the world’s only mounted Kronosaurus, a the twenty-one million specimens at the 42-foot-long prehistoric marine reptile. Harvard Museum of Natural History show a Among its 90,000 zoological specimens the museum bursting with life, much of it unnat- museum also has the pheasants once owned urally natural. by George Washington. And many of the The museum will be the site of the opening mammal collections were put together in the reception for the 2003 HSS annual meeting. 19th century by “lions” in the history of sci- The reception begins at 7 p.m. Thursday, 20 ence, like Louis Agassiz. November, and tickets will be available at the Much of the museum’s collection of rocks and meeting registration desk. Buses will run from ores is the result of field work, but the museum the host hotel to the museum. houses not only that which has been dug up, but The Harvard MNH is an ideal spot for his- also that which has fallen out of the sky. -
Searching for Extraterrestrial Intelligence
THE FRONTIERS COLLEctION THE FRONTIERS COLLEctION Series Editors: A.C. Elitzur L. Mersini-Houghton M. Schlosshauer M.P. Silverman J. Tuszynski R. Vaas H.D. Zeh The books in this collection are devoted to challenging and open problems at the forefront of modern science, including related philosophical debates. In contrast to typical research monographs, however, they strive to present their topics in a manner accessible also to scientifically literate non-specialists wishing to gain insight into the deeper implications and fascinating questions involved. Taken as a whole, the series reflects the need for a fundamental and interdisciplinary approach to modern science. Furthermore, it is intended to encourage active scientists in all areas to ponder over important and perhaps controversial issues beyond their own speciality. Extending from quantum physics and relativity to entropy, consciousness and complex systems – the Frontiers Collection will inspire readers to push back the frontiers of their own knowledge. Other Recent Titles Weak Links Stabilizers of Complex Systems from Proteins to Social Networks By P. Csermely The Biological Evolution of Religious Mind and Behaviour Edited by E. Voland and W. Schiefenhövel Particle Metaphysics A Critical Account of Subatomic Reality By B. Falkenburg The Physical Basis of the Direction of Time By H.D. Zeh Mindful Universe Quantum Mechanics and the Participating Observer By H. Stapp Decoherence and the Quantum-To-Classical Transition By M. Schlosshauer The Nonlinear Universe Chaos, Emergence, Life By A. Scott Symmetry Rules How Science and Nature are Founded on Symmetry By J. Rosen Quantum Superposition Counterintuitive Consequences of Coherence, Entanglement, and Interference By M.P. -
In-Depth Study of Photometric Variability and Radiative Timescales for Atmospheric Evolution in Four L Dwarfs
Weather on Other Worlds IV: In-Depth Study of Photometric Variability and Radiative Timescales for Atmospheric Evolution in Four L Dwarfs Item Type text; Electronic Thesis Authors Flateau, Davin C. Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 30/09/2021 07:25:39 Link to Item http://hdl.handle.net/10150/594630 WEATHER ON OTHER WORLDS IV: IN-DEPTH STUDY OF PHOTOMETRIC VARIABILITY AND RADIATIVE TIMESCALES FOR ATMOSPHERIC EVOLUTION IN FOUR L DWARFS by Davin C. Flateau A Thesis Submitted to the Faculty of the DEPARTMENT OF PLANETARY SCIENCES In Partial Fulfillment of the Requirements For the Degree of MASTER OF SCIENCE In the Graduate College THE UNIVERSITY OF ARIZONA 2015 2 STATEMENT BY AUTHOR This thesis has been submitted in partial fulfillment of requirements for an advanced degree at the University of Arizona and is deposited in the University Library to be made available to borrowers under rules of the Library. Brief quotations from this thesis are allowable without special permission, provided that accurate acknowledgment of the source is made. Requests for permission for extended quotation from or reproduction of this manuscript in whole or in part may be granted by the head of the major department or the Dean of the Graduate College when in his or her judgment the proposed use of the material is in the interests of scholarship. -
Impact Glasses from Zhamanshin Crater (USSR)
80 Earth awl Plauelaty Science Leuers, 78 (1986) 80-88 Elsevier Science Publishers B.V., Amsterdam - Printed in The Netherlands IS1 Impact glassesfrom Zhamanshin crater (U.S.S.R.) : chemical composition and discussion of origin Christian Koeberl ’ and Kurt Fredriksson 2 ’ Insritrrre of Geochemisny, Uniuersiry oj Vienna, P.O. Box 73. A-1094 Viema (Arcsrriu) ’ Deparanettr of Mineral Scierrces, Snlithsotriatl Jrlstirurion, Washingron. DC 20560 (U.S.A.) Received October 12, 1985; revised version received February 17, 1986 Three silica-rich zhamanshinites and one irghizite from the Zhamanshin impact crater (northern Aral area, U.S.S.R.) have been analyzed for up to 40 major, minor, and trace elements. All data point to a clear distinction between these impact glasses and other tektites or impact glasses. e.g. from the Australasian strewn field. Halogens are generally enriched in the irghizites and zhamanshinites when compared to normal splash for tektites. with zhamanshinites enriched more than irghizites. The same holds also for the alkali metals and a number of other volatile elements like Sb and As. Nickel and cobalt are enriched in the irghizite sample IO a considerable degree, suggesting meteoritic contamination. This view is also supported by gold and selenium data, but for quantifications.other siderophile elements need to be considered. Chromium is not a valid indicator of meteoritic contamination. because small amounts of ultra-basic igneous material may completely alter the picture. The rare earth elements do show a sedimentary pattern, consistent with two or three different source materials and a variation which is probably mostly due to dilution with silica-rich materials. -
Exoplanet Meteorology: Characterizing the Atmospheres Of
Exoplanet Meteorology: Characterizing the Atmospheres of Directly Imaged Sub-Stellar Objects by Abhijith Rajan A Dissertation Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy Approved April 2017 by the Graduate Supervisory Committee: Jennifer Patience, Co-Chair Patrick Young, Co-Chair Paul Scowen Nathaniel Butler Evgenya Shkolnik ARIZONA STATE UNIVERSITY May 2017 ©2017 Abhijith Rajan All Rights Reserved ABSTRACT The field of exoplanet science has matured over the past two decades with over 3500 confirmed exoplanets. However, many fundamental questions regarding the composition, and formation mechanism remain unanswered. Atmospheres are a window into the properties of a planet, and spectroscopic studies can help resolve many of these questions. For the first part of my dissertation, I participated in two studies of the atmospheres of brown dwarfs to search for weather variations. To understand the evolution of weather on brown dwarfs we conducted a multi- epoch study monitoring four cool brown dwarfs to search for photometric variability. These cool brown dwarfs are predicted to have salt and sulfide clouds condensing in their upper atmosphere and we detected one high amplitude variable. Combining observations for all T5 and later brown dwarfs we note a possible correlation between variability and cloud opacity. For the second half of my thesis, I focused on characterizing the atmospheres of directly imaged exoplanets. In the first study Hubble Space Telescope data on HR8799, in wavelengths unobservable from the ground, provide constraints on the presence of clouds in the outer planets. Next, I present research done in collaboration with the Gemini Planet Imager Exoplanet Survey (GPIES) team including an exploration of the instrument contrast against environmental parameters, and an examination of the environment of the planet in the HD 106906 system. -
The 3D.Y Knom Example Is /1"<
t Sixth International Congress on Glass - Washington, D. C., 1962. Fossil Glasses Produced by Inpact of Meteorites, Asteroids 2nd Possibly Comets with the Planet Xarth* A. J. Zzhen :&uon Insticute, Pittsburgh, ?ennsylvania (U. S. A. ) Sunnary / (to be trmslzted izto Frerzh and German) - i in recent thes one of the nost intriging aysteries of geGlogy has ceen the occurrence of aerodgnasicdly-shaped glasses on five continents of the earth. Tnese glasses mder discussion are obviously not of f-d- guritic origin. 3ecent research indicates that these glasses laom as tektites are the result of meteorite, esteroid, or sossibly comet hpact. Lqact glass?s, io generzl, differ Tram volcanic glasses in that they are lo;;.tr in ?,iater zontent, have laver gallium and germiun ccntents, and are rot necessarily ia mgnaticalljr unstable continental areas. These hpac- tites may be divided as follovs: (1)Glasses found in or near terrestrial neteorite craters. These glasses usually contain numerous s-,'nerules 02 nickel-iron, coesite, chunlks of partially melted meteoritic inatter and even stishovite. Shattered or fractured melted mi-nerals such as quarts are comxonly gresent. Aerodpaaic-shaping nay or nay not be present in this t-ne. &m?les are Canyon Diablo and Wabar Crster glasses. (2) Impzct- glasses zssociated with craters uitn no evidence of meteoritic mterial i? the @.ass or surrounding the explosisn site. The 3d.y knom example is /1"< Tnis vork vas supported by Xatiocal A-eroEautizs and Space P.dministretioq,$ 3esezrch Grant NsG-37-6O Supplement 1-62. Page 2 glass associated with AoueUoul Crater in the Western Sahara Desert. -
13. Late Pliocene-Pleistocene Glaciation
13. LATE PLIOCENE - PLEISTOCENE GLACIATION W. A. Berggren, Woods Hole Oceanographic Institution, Woods Hole, Massachusetts The discussion in this chapter is broken down into two increase in the former exceeding that of the latter; or parts: the first deals with glaciation in the North Atlantic as (v) less detritals, clay and carbonate deposited per unit time revealed in the data obtained on Leg 12; in the second part (that is, decreased sedimentation rate) with the decrease in an attempt is made to provide a chronologic framework of the latter exceeding the former. In view of the demon- Late Pliocene-Pleistocene glaciation and to correlate gla- strable increase in sedimentation rate above the preglacial/ cial/interglacial sequences as recorded in land and deep-sea glacial boundary at Sites 111, 112 and 116 due to increased sediments. amounts of detrital minerals and the fact that glacial periods in high latitudes are characterized by a carbonate GLACIATION IN THE NORTH ATLANTIC minimum (Mclntyre et al., in press) it can be seen that the One of the most significant aspects of Leg 12 was the correct explanation for the increase in natural gamma activ- various results which were obtained regarding glaciation in ity in the glacial part of the section is rather complex. Thin the North Atlantic. Glacial sediments were encountered at bands of carbonate were found at various levels intercalated all sites in the North Atlantic with the exception of Site with detrital-rich clays which indicates interglacial intervals, 117 (for the purpose of this discussion the North Atlantic so that the correct explanation probably lies with (iii) encompasses Sites 111 through 117; Sites 118 and 119 are above. -
Shock Papers 2016
Shock Physics Papers 2016 Abbas, S.H., Jang, J.-K., Lee, J.-R. and Kim, Z. 2016 "Development of an FPGA-based multipoint laser pyroshock measurement system for explosive bolts" Rev. Sci. Instrum. 87 073302 Adushkin, V.V. and Oparin, V.N. 2016 "From the alternating-sign explosion response of rocks to the pendulum waves in stressed geomedia. 4" J. Mining Sci. 52 1-35 Agarwal, G. and Dongare, A.M. 2016 "Shock wave propagation and spall failure in single crystal magnesium at atomic scales" J. Appl. Phys. 119 145901 Ageev, E.I., Kudryashov, S.I., Nikonorov, N.V., Nuryev, R.K., Petrov, A.A., Samokhvalov, A.A. and Veiko, V.P. 2016 "Non-contact ultrasonic acquisition of femtosecond laser-driven ablative Mbar-level shock waves on titanium alloy surface" Appl. Phys. Letts 108 084106 Ageev, E.I., Bychenkov, V.Y., Ionin, A.A., Kudryashov, S.I., Petrov, A.A., Samokhvalov, A.A. and Veiko, V.P. 2016 "Double-pulse femtosecond laser peening of aluminum alloy AA5038: Effect of inter-pulse delay on transient optical plume emission and final surface micro-hardness" Appl. Phys. Letts 109 211902 Agrawal, V., Peralta, P., Li, Y. and Oswald, J. 2016 "A pressure-transferable coarse- grained potential for modeling the shock Hugoniot of polyethylene" J. Chem. Phys. 145 104903 Ahn, D.H., Kim, W., Kang, M., Park, L.J., Lee, S. and Kim, H.S. 2016 "Corrigendum to ‘Plastic deformation and microstructural evolution during the shock consolidation of ultrafine copper powders’" Mater. Sci. Engng A 654 379-380 Akin, M.C., Fratanduono, D.E. -
A Tomography Approach to Investigate Impactite Structure
3rd International Conference on Tomography of Materials and Structures Lund, Sweden, 26-30 June 2017, ICTMS2017-110 A TOMOGRAPHY APPROACH TO INVESTIGATE IMPACTITE STRUCTURE A. Fedrigo*1,2, K. Marstal1,3, A. Bjorholm Dahl1, M. Lyksborg1, C. Gundlach1, M. Strobl2 & C. Bender Koch4 1Danish Technical University, Denmark 2European Spallation Source ESS ERIC, Sweden 3ERASMUS MC, Netherland 4Copenhagen University, Denmark Keywords: Neutron imaging, image registration, bimodal imaging, computed tomography. Summary: We investigate the structure of impactites from the Wabar iron meteorite impact site in Saudi Arabia. In order to understand the physical and chemical processes involved in the formation of the impactite, we applied a non-destructive investigation approach, which combines X-ray and neutron tomography. This bi-modal imaging method allowed for a better understanding of the impactite’s chemical composition. 1. INTRODUCTION Meteorite impacts have recently been recognised among the most important processes able to modify planetary surfaces. It also happens to be one of the least understood in details. In particular it is a challenge to understand both the extent of impacts and the physical and chemical changes that occur during and following the impact, where materials (e.g., rocks, sand, meteorite fragments, etc.) are subjected to temperatures of several thousands degrees and pressures of several GPa. In addition, most accessible Earth impact areas are highly affected by weathering, which causes extensive secondary chemical alterations. Iron meteorites impact on planetary surfaces cause shock-induced rock deformations that happens both at macroscopic and at microscopic level, e.g. shatter cones (macroscopic) and planar deformation features in quartz (microscopic). Another indicator often correlated to meteoritic impacts is the presence of iridium concentration anomalies [1, 2].