David J. Moliterno, MD May 2019

Total Page:16

File Type:pdf, Size:1020Kb

David J. Moliterno, MD May 2019 David J. Moliterno, M.D. General Office Address Department of Internal Medicine University of Kentucky Medical Center 900 South Limestone Street 329 Charles T. Wethington Building Lexington, KY 40536-0200 (859) 323-5843 voice (859) 257-3537 fax e-mail: [email protected] Home Address 2204 Terranova Court Lexington, KY 40513-1839 (859) 296-1970 voice (859) 296-1971 fax (859) 230-2265 mobile Personal Data Spouse: Judith Ann Moliterno, R.N., B.S.N. Children: Nathaniel (24) and Benjamin (22) Education Undergraduate College of Arts and Sciences University of Michigan, Flint, Michigan B.S. Honors, Biology, 8/1978-5/1982 Medical School Medical College of Virginia Virginia Commonwealth University, Richmond, Virginia Doctor of Medicine, 8/1983-5/1987 Post Doctoral Training Internship Vanderbilt University Hospitals Vanderbilt University Medical Center, Nashville, Tennessee Intern in Internal Medicine, 7/1987-6/1988 Residency Vanderbilt University Hospitals & Nashville Veterans Affairs Medical Center Vanderbilt University Medical Center, Nashville, Tennessee Junior and Senior Resident in Internal Medicine, 7/1988-6/1990 David J. Moliterno, MD May 2019 Fellowships Parkland Memorial Hospital & Dallas Veterans Affairs Medical Center University of Texas, Southwestern Medical Center, Dallas, Texas Fellow in Cardiovascular Medicine, 7/1990-6/1993 Department of Cardiovascular Medicine Section of Interventional Cardiology The Cleveland Clinic Foundation, Cleveland, Ohio Fellow in Interventional Cardiology, 7/1993-6/1994 Professional Activities Faculty Appointments Vice Dean/Vice President for Clinical Affairs UK College of Medicine/UK HealthCare University of Kentucky, 4/2014-7/2016 Senior Associate Dean for Clinical Affairs College of Medicine University of Kentucky, 6/2012-3/2014 Chairman, Department of Internal Medicine Jack M. Gill Chair of Medicine University of Kentucky, 9/2011-present Physician-In-Chief, Cardiovascular Service Line University of Kentucky, 10/2009-9/2011 Professor of Medicine, Department of Internal Medicine University of Kentucky, 12/2003-present Vice-Chairman of Internal Medicine University of Kentucky, 1/2004-8/2011 Jefferson Morris Gill Professor of Cardiology University of Kentucky, 12/2003-8/2011 Chief, Division of Cardiovascular Medicine University of Kentucky, 12/2003-8/2011 Medical Director, Gill Heart Institute University of Kentucky, 12/2003-8/2011 Staff Physician Section of Interventional Cardiology Department of Cardiovascular Medicine The Cleveland Clinic Foundation Cleveland, Ohio, 7/1994-11/2003 Page 2 David J. Moliterno, MD May 2019 Faculty Appointments (continued) Medical Director, Angiographic Core Laboratory Section of Cardiac Catheterization Department of Cardiovascular Medicine The Cleveland Clinic Foundation, 7/1994-6/2001 Associate Professor of Medicine Department of Cardiovascular Medicine Cleveland Clinic Health Sciences Center of Ohio State University Cleveland, Ohio, 1/2000-11/2003 Medical Director, CIA Cleveland Clinic Cardiology Investigators’ Association The Cleveland Clinic Foundation, 7/1999-11/2003 Staff Physician Department of Cardiology MetroHealth Medical Center Cleveland, Ohio, 8/1995-11/2003 Assistant Professor of Medicine Department of Cardiology Cleveland Clinic Health Science Center of The Ohio State University Cleveland, Ohio, 7/1994-12/1999 Page 3 David J. Moliterno, MD May 2019 Accomplishments Honors Psi Chi - National Honor Society, 1982 Merck Scholastic Achievement Award, 1985 Bristol Cardiology Fellow Award, 1991 Syntex Cardiology Fellow Award, 1992 Life Member, National Registry of Who’s Who Listed in Who’s Who in Medicine and Healthcare Listed in Who’s Who in Science and Engineering Listed in Who’s Who in Medical Sciences Education Listed in Best Physicians in America Cleveland Clinic International Physician-of-the-Year Award, 1999 Listed in Guide to America’s Top Physicians, 2003 Included in Best Doctors, 2001-2016 Simon Dack Award Journal of American College of Cardiology, 2011 ACC-Kentucky Chapter, Lifetime Achievement Award, 2016 Certificates & Licensure Advanced Cardiac Life Support Board Certification in Internal Medicine (ABIM), 1991 Board Certification in Cardiovascular Medicine (ABIM), 1993 Board Certified in Interventional Cardiology (ABIM), 1999 Recertification in Cardiovascular Medicine (ABIM), 2003, 2013 Recertification in Interventional Cardiology (ABIM), 2009 State of Tennessee, medical license, 1988 (inactive) State of Texas, medical license, 1990 (inactive) State of Ohio, medical license, 1993 (inactive) State of Kentucky, medical license, 2004-present Page 4 David J. Moliterno, MD May 2019 Academic Activities Memberships American College of Cardiology, Fellow (FACC) American College of Physicians, Fellow (FACP) European Society of Cardiology, Fellow (FESC) Society for CV Angiography and Interventions, Fellow (FSCAI) American Heart Association, Fellow (FAHA) Atherosclerosis, Thrombosis, and Vascular Biology Council American Medical Association Association of Professors in Cardiology Association of University Cardiologists Frequent Journal Reviewer American Heart Journal American Journal of Cardiology Annals of Internal Medicine Circulation Journal of the American College of Cardiology Journal of the American Medical Association Journal of the American Medical Association Cardiology Journal of Thrombosis and Hemostasis Journal of Thrombosis and Thrombolysis Lancet New England Journal of Medicine Editorial Boards Editor-in-Chief, CathSAP-3 (Cardiac Catheterization and Interventional Cardiology Self-Assessment Program), 2006-2010 Chief, SAP Editorial Board, 2007-2008 Editor-in-Chief, CathSAP-4 (Cardiac Catheterization and Interventional Cardiology Self-Assessment Program), 2010-2014 Associate Editor, JACC-Cardiovascular Interventions, 2006-2016 Editor-in-Chief, JACC-Cardiovascular Interventions, 2017-present Guest Editor, Circulation, 2008-2016 Section Editor: Journal of Thrombosis and Thrombolysis, 2003-2017 ACCSAP VI (Thrombosis), 2004 Page 5 David J. Moliterno, MD May 2019 Editorial Boards (continued) Board Member, Cardiology Today’s Intervention, 2011-present Medical Editor, Cardiac Consult (Cleveland Clinic), 2001-2003 Editorial Consultant: American Heart Journal, 2005-present Cardiosource Clinical Trials, 2004-2006 Cardiovascular Revascularization Medicine, 2009-2010 Catheterization and Cardiovascular Interventions, 2006-present Current Controlled Trials in Cardiovascular Medicine, 2002-2005 Journal of Interventional Cardiology, 2004-2017 Journal of the American College of Cardiology, 2001-2005 Journal of the American College of Cardiology, 2014-present Leadership American Board of Internal Medicine Interventional Cardiology Examination Relevance Reviewer, 2005 American College of Cardiology Foundation Strategic Education Directions Committee, 2004-2006 Political Action Committee Board, 2004-2007 Publications Committee, 2006-2009 Kentucky Chapter Governor-elect, 2006-2007 Kentucky Chapter Governor Board of Governors, 2007-2010 i2 Management Advisory Committee, 2008-2009 Task Force on Clinical Expert Consensus Documents, 2007-2013 Co-Chair, i2 Annual Scientific Session, 2009-2010 Chair, i2 Annual Scientific Session, 2010-2011 Interventional Scientific Council, 2012-2014 Clinical Policy Approval Committee (CPAC), 2016-present Editorial Board Member: American College of Cardiology of Extended Learning (ACCEL), 2017-present American Heart Association Central Kentucky Chapter Board of Directors, 2004-2012 Arteriosclerosis and Thrombosis Council Clinical Cardiology Council European Society of Cardiology Thrombosis Working Group, 2002-present Page 6 David J. Moliterno, MD May 2019 Leadership University of Kentucky Medical Center Advisory Board, 2004-present Clinical Directors Council, 2006-present University Faculty Senator, 2006-2010 Medical Center Clinical Sciences Area Committee, 2007-2010 Academic Organization & Structure Committee, 2007-2009 Search Committee, Dean for the College of Medicine, 2010-2011 Clinical Faculty Compensation Committee Leader, 2011-2016 Kentucky Medical Services Finance Committee, 2011-present Kentucky Medical Services Executive Committee, 2011-present UK HealthCare Finance and Capital Committee, 2011-2016 UK HealthCare Facilities Allocation Executive Committee, 2014-2017 Search Committee, Executive Vice President for Health Affairs, 2017 Beyond Blue Corporation, Board of Directors, 2016-present Executive Management Committee, 2017-present Ambulatory Oversight Committee, 2017-present Executive Quality Committee, 2017-present Page 7 David J. Moliterno, MD May 2019 Past Principal Investigatorships and Committees 1. Clinical Events Committee: Global Use of Strategies to Open Occluded Arteries in Acute Coronary Syndromes (GUSTO II). CIBA-Geigy, Boehringer-Mannheim, Advanced Cardiovascular Systems. 2. Clinical Events Committee: A Randomized, Double-Blind, Comparative Safety and Efficacy Evaluation of Integrelin in Patients Receiving Thrombolytic Therapy for Acute Myocardial Infarction (IMPACT-AMI). COR Therapeutics. 3. Angiographic Core Laboratory Director: Evaluation of PTCA to Improve Long-term Outcomes by c7E3 Glycoprotein Receptor Blockade (EPILOG). Centocor, Eli Lilly. 4. Study Co-Principal Investigator: Prevention of Reocclusion and Inhibition of Thrombus and Myocardial Events (PRIME) Trial; A Randomized Trial of Efegatran Sulfate versus Heparin in Acute Myocardial Infarction. Eli Lilly. 5. Angiographic Core Laboratory Director: Reteplase versus Alteplase Investigation During Myocardial Infarction Trial (RAPID 2); Randomized,
Recommended publications
  • Charles Darwin: a Companion
    CHARLES DARWIN: A COMPANION Charles Darwin aged 59. Reproduction of a photograph by Julia Margaret Cameron, original 13 x 10 inches, taken at Dumbola Lodge, Freshwater, Isle of Wight in July 1869. The original print is signed and authenticated by Mrs Cameron and also signed by Darwin. It bears Colnaghi's blind embossed registration. [page 3] CHARLES DARWIN A Companion by R. B. FREEMAN Department of Zoology University College London DAWSON [page 4] First published in 1978 © R. B. Freeman 1978 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording or otherwise without the permission of the publisher: Wm Dawson & Sons Ltd, Cannon House Folkestone, Kent, England Archon Books, The Shoe String Press, Inc 995 Sherman Avenue, Hamden, Connecticut 06514 USA British Library Cataloguing in Publication Data Freeman, Richard Broke. Charles Darwin. 1. Darwin, Charles – Dictionaries, indexes, etc. 575′. 0092′4 QH31. D2 ISBN 0–7129–0901–X Archon ISBN 0–208–01739–9 LC 78–40928 Filmset in 11/12 pt Bembo Printed and bound in Great Britain by W & J Mackay Limited, Chatham [page 5] CONTENTS List of Illustrations 6 Introduction 7 Acknowledgements 10 Abbreviations 11 Text 17–309 [page 6] LIST OF ILLUSTRATIONS Charles Darwin aged 59 Frontispiece From a photograph by Julia Margaret Cameron Skeleton Pedigree of Charles Robert Darwin 66 Pedigree to show Charles Robert Darwin's Relationship to his Wife Emma 67 Wedgwood Pedigree of Robert Darwin's Children and Grandchildren 68 Arms and Crest of Robert Waring Darwin 69 Research Notes on Insectivorous Plants 1860 90 Charles Darwin's Full Signature 91 [page 7] INTRODUCTION THIS Companion is about Charles Darwin the man: it is not about evolution by natural selection, nor is it about any other of his theoretical or experimental work.
    [Show full text]
  • Glossary Glossary
    Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts.
    [Show full text]
  • Feature of the Month - August 2006
    RECENT BACK ISSUES: http://www.zone-vx.com/tlo_back.html A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: William M. Dembowski, F.R.A.S. - [email protected] Elton Moonshine Observatory - http://www.zone-vx.com 219 Old Bedford Pike (Elton) - Windber, PA 15963 FEATURE OF THE MONTH - AUGUST 2006 RHEITA E Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA March 5, 200 - 01:15 to 01:45 UT 15cm Newtonian - 170x - Seeing 7-8/10 I sketched this crater and vicinity on the evening of March 4, 2006 after observing two occultations. This feature is located amid a jumble of craters south of Mare Fecunditatis. This is an elongated crater that appears to be the result of at least three impacts. The north and south lobes are about the same size, but the southern lobe is definitely deeper. The central portion is about the size of the north and south lobes combined. There are some bits of shadow on the floor, but I saw no obvious hills or craters there. I have drawn the shadowing within and around Rheita E as I saw it. There is an obvious ridge extending westward from the south lobe. The crater Rheita F is adjacent to the south lobe of Rheita E, and has a strip of shadow parallel to the ridge from Rheita E. Rheita M is the large, shallow crater east of Rheita E's south end, and Rheita N is the small, shallow pit between them. Stevinus D is the slightly smaller, but deeper crater north of Rheita M.
    [Show full text]
  • Water on the Moon, III. Volatiles & Activity
    Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere).
    [Show full text]
  • Appendix I Lunar and Martian Nomenclature
    APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei
    [Show full text]
  • Glorious Diffraction Spikes in the Cave Astrophotographers Take Note! This Space Is Reserved for Your B&W Or Greyscale Images
    The Journal of The Royal Astronomical Society of Canada PROMOTING ASTRONOMY IN CANADA February/février 2013 Volume/volume 107 Le Journal de la Société royale d’astronomie du Canada Number/numéro 1 [758] Inside this issue: Milky Way Globular Clusters Orionid Meteor Shower by FM Radio LEDs in Astronomy The Venus Aureole Effect London Centre’s Observatory My Fast-Light Mirror Glorious diffraction spikes in The Cave Astrophotographers take note! This space is reserved for your B&W or greyscale images. Give us your best shots! Gerry Smerchanski of the Winnipeg Centre adopted the hard way to record the crater Vieta on September 27 last year. Gerry combined paper and pencil at the end of a Celestron Ultima 8 with a binoviewer at 200× to capture the crater with its small central hill and off-centre craterlet. Gerry notes that “Crater Vieta usually gets overlooked by me as it is near Gassendi, which is a favourite of mine. But the lighting was perfect to go from Gassendi down along an arc of dramatically lit craters—including Cavendish—to Vieta where the terminator was found.” Vieta is 80 km in diameter with 4500-m walls on the west side and 3000-m walls to the east. To the southeast lies the crater Fourier. Michael Gatto caught the elusive “Werner X” during its few hours of visibility on November 20 from 9 to 9:45 p.m. Michael used an 8-inch f/7.5 Newtonian on a Dob mounting from Dartmouth, N.S., in average-to-poor seeing. The sketch was done at the eyepiece with various pencils and a blending stump on paper, then scanned and darkened in Photoshop.
    [Show full text]
  • Review of Experimental Studies on the Non-Negligible Effect of the Third Invariant – a Call That Has Largely Been Ignored (See Hooke & Mellor and 11 Others (1980))
    Journal of Earth and Environmental Sciences Review Article Hutter K and Gross D. J Earth Environ Sci 7: 174. DOI: 10.29011/2577-0640.100174 Brief Historical Tour of Glacier Ice on Earth and its Role in Climate Dynamics1 Kolumban Hutter1*, Dietmar Gross1 Department of Mechanics, Darmstadt University of Technology, Darmstadt, Germany *Corresponding author: Kolumban Hutter, Department of Mechanics, Darmstadt University of Technology, Darmstadt, Germany. Email: [email protected] Citation: Hutter K and Gross D (2019) Brief Historical Tour of Glacier Ice on Earth and its Role in Climate Dynamics. J Earth Environ Sci 7: 174. DOI: 10.29011/2577-0640.100174 Received Date: 18 June, 2019; Accepted Date: 17 July, 2019; Published Date: 25 July, 2019 Abstract The science of the physics of ice crystals started almost 500 years ago with Cardano, followed by Kepler, Hooke, Dalton, the two Braggs (father and son) and Pauling. Here, we are concerned with naturally formed ice of glaciers, ice sheets and ice shelves. We do not discuss lake, river, sea and atmospheric ices, even though they equally play a role in today’s General Circulation Models (GCMs) for the Earth. The study of glacier ice started with the observation of the behavior of the dynamics of Alpine glaciers, specifically that they are not rigid, but moving bodies that deform. A ladder, left in 1788 at the icefall of the Col de Géant by de Saussure was 44 years later found at the three-glacier merge of the Mer de Glace, corresponding to a mean velocity of 375 feet/year. Hugi and Agassiz measured the motion of rocks on the middle moraine of the Unteraar-gletscher and found similar values.
    [Show full text]
  • Morphometric Characterization and Reconstruction Effect Among Lunar Impact Craters
    Earth Moon Planets (2014) 111:139–155 DOI 10.1007/s11038-014-9431-0 Morphometric Characterization and Reconstruction Effect Among Lunar Impact Craters Weiming Cheng • Jiao Wang • Cong Wan Received: 2 January 2014 / Accepted: 11 March 2014 / Published online: 19 March 2014 Ó Springer Science+Business Media Dordrecht 2014 Abstract Impact craters on the lunar surface have a variety of morphometric charac- teristics that are very useful in understanding the evolutionary history of lunar landscape morphologies. Based on digital elevation model data and photographs from China’s Chang’E-1 lunar orbiter, we develop morphologic parameters and quantitative methods for presenting the morphometric characteristics of impact craters, analyzing their relational distribution, and estimating the relative order of their formation. We also analyze features in profile where craters show signs of having formed on the edge of previously existing craters to show that superimposed impacts affect morphologic reconstructions. As a result, impact craters have significant effects on the reconstruction of ancient topography and the estimation of relative formation ages. Keywords Morphometric characterization Á Position relationship Á Relative construction age Á Chang’E-1 1 Introduction The Earth’s Moon, it’s only natural satellite, has a potentially complete record of the 4.5- billion year evolutionary history of the solar system (Ronca 1966; Ouyang 2005). Impact craters are the most obvious and typical geomorphologic units (Ronca 1969; Neukum and Ivanov 1994; Neukum et al. 1975); they form when a planetary body (meteoro, comet, etc.) impact against the surface (King 1976). The diameters of impact craters on the lunar W. Cheng (&) Á J.
    [Show full text]
  • Rimae Sirsalis
    RIMAE SIRSALIS Nieves del Río, José Castillo, Eduardo Adarve, Jorge Arranz y Alberto Martos del Grupo de Estudios Lunares “Enrique Silva”. [Página dejada intencionadamente en blanco] - 2 - INTRODUCCIÓN Rimae Sirsalis es un sistema de grietas que comprende dos estructuras de esta clase, Rima Sirsalis y Rima Sirsalis I, siendo la primera mucho más larga y mucho más perceptible que la segunda. Pertenecen a la clase de grietas rectas, cuyo aspecto es diferente del aspecto de las grietas circulares que bordean las cuencas de las grandes estructuras de impacto. Lo que tiene de particular este sistema, para que haya merecido figurar como objetivo 1 en el apartado “Call for Observations 2”, del boletín TLO 3 de ALPO 4, son sus dos características principales: siendo Rima Sirsalis la grieta más larga existente en la cara cislunar (la visible), está situada en una región cuyo suelo es geológicamente distinto de la naturaleza de suelos por los que discurren en general las grietas lunares. En efecto, las grietas lunares (llamadas en latín rimae ) son siempre estructuras volcánicas, generalmente túneles de lava cuyo techo se ha desplomado, o surcos por los cuales fluyó la lava en su día, en favor de la pendiente del suelo. Por esta razón, se las encuentra siempre sobre terrenos magmáticos, como los maria (plural de mare ), los sini (plural de sinus ), los laci (plural de lacus ), o los paludes (plural de palus ), o sea sobre los “mares”, las “bahías”, los “lagos” o las “marismas” lunares. Como ejemplos de esta condición se puede citar a Rimae Hypatia, situada en el Mare Tranquillitatis, a Rima Oppolzer, en Sinus Medii, a Rimae Bürg y Rimae Daniell, en Lacus Mortis y Lacus Somniorum, respectivamente y Rima Hesiodus en Palus Epidemiarum.
    [Show full text]
  • Meteorites and the Smithsonian Institution Russian)
    M.A. IVANOV A & M.A. NAZAROV 236 V M 1811. A report on air stones Of ai~o- 55 Principles of Meteoritics. SEVERGIN, .' . the Museum of the lmpenal KRINov, E.L. 19 . ( d) State publishers ?f lithes preserved l~ 'Technological journal, Fesenkov, V.G. e... Moscow (lll Academy of s clences., Technical/Theoretical LIterature, VIII 129-132 (in Russian). N rth Meteorites and the Smithsonian Institution Russian). R ' Moscow Nauka, ' 1809 On a New Map of the 0 em KRINOV , E.L. 1981. Iro.n am. STEHLIN; jA. d ecimen of native iron. Philoso- 2 Archipelago, an .sp .J' the Royal Society of ROY S. CLARKE, JR!, HOWARD PLOTKIN & TIMOTHY J. McCOY! Moscow, 192 (in Ru~:a~'F Chladny _ a founder phical TransactIOns OJ MASSALSKAYA, K.P. 19 . ' 'M' 'tika 11 33-46 1 Department of Mineral Sciences, National Museum of Natural History, of scientific meteontlcS. eteon , , London LXIY, l774, 46l. Th 'r • A 1807 On Aerial Stones and el STOlKQVICH,.. .' f Kharkov Kharkov, 271 Smithsonian Institution, Washington, DC 20560-0119, USA (in Russian). M' I us Showers 01" Stones Origin. Umverslty 0 , 1M 1819 On tracu 0 'J 2Department of Philosophy, University of Western Ontario, London, Canada N6A 3K7 MUKHI~,.. h~ Air (Aeroli!hes). Imperial Foun~- (in Russian). h in ~alling F~°alm 'Publisher St Petersburg, 207 (m o 1915. AstronomIc P enomena (e-mail: [email protected]) hng-HospJt ' SVI~TSK.Y, ~;st~rical Chronicles Considered from a Russian). A 2000 The meteorite collection of the usswn . "V' Bulletin of the Department NAZAROV, M.. f Sciences In: ALEKSEEVA, Scientific.
    [Show full text]
  • Atmospheric Nuclear Weapons Testing
    Battlefi eld of the Cold War The Nevada Test Site Volume I Atmospheric Nuclear Weapons Testing 1951 - 1963 United States Department of Energy Of related interest: Origins of the Nevada Test Site by Terrence R. Fehner and F. G. Gosling The Manhattan Project: Making the Atomic Bomb * by F. G. Gosling The United States Department of Energy: A Summary History, 1977 – 1994 * by Terrence R. Fehner and Jack M. Holl * Copies available from the U.S. Department of Energy 1000 Independence Ave. S.W., Washington, DC 20585 Attention: Offi ce of History and Heritage Resources Telephone: 301-903-5431 DOE/MA-0003 Terrence R. Fehner & F. G. Gosling Offi ce of History and Heritage Resources Executive Secretariat Offi ce of Management Department of Energy September 2006 Battlefi eld of the Cold War The Nevada Test Site Volume I Atmospheric Nuclear Weapons Testing 1951-1963 Volume II Underground Nuclear Weapons Testing 1957-1992 (projected) These volumes are a joint project of the Offi ce of History and Heritage Resources and the National Nuclear Security Administration. Acknowledgements Atmospheric Nuclear Weapons Testing, Volume I of Battlefi eld of the Cold War: The Nevada Test Site, was written in conjunction with the opening of the Atomic Testing Museum in Las Vegas, Nevada. The museum with its state-of-the-art facility is the culmination of a unique cooperative effort among cross-governmental, community, and private sector partners. The initial impetus was provided by the Nevada Test Site Historical Foundation, a group primarily consisting of former U.S. Department of Energy and Nevada Test Site federal and contractor employees.
    [Show full text]
  • Lunar Topographical Studies Section Banded Craters Program
    Lunar Topographical Studies Section Banded Craters Program These highly stylized drawings are intended only to give a general impression of each Group In the March 1955 Journal of the British Astronomical Association, K. W. Abineri and A. P. Lenham published a paper in which they suggested that banded craters could be grouped into the following five categories: Group 1 - (Aristarchus type) Craters are very bright, quite small, and have fairly small dark floors leaving broad bright walls. The bands, on the whole, apparently radiate from near the centre of the craters. These craters are often the centres of simple bright ray systems. Group 2 - (Conon type) Rather dull craters with large dark floors and narrow walls. Very short bands show on the walls but cannot be traced on the floors. The bands, despite their shortness, appear radial to the crater centre. Group 3 - (Messier type) A broad east-west band is the main feature of the floors. Group 4 - (Birt type) Long, usually curved, bands radiate from a non-central dull area. The brightness and size are similar to the Group 1 craters. Group 5 - (Agatharchides A type) One half of the floor is dull and the bands radiate from near the wall inside this dull section and are visible on the dull and bright parts of the floor. 1 BANDED CRATERS BY NAMED FEATURE NAMED FEATURE LUNAR LONG. LUNAR LAT. GROUP (Unnamed Feature) E0.9 S18.0 1 (Unnamed Feature) E4.8 N23.4 4 (Unnamed Feature) W45.4 S23.6 3 (Unnamed Feature) E56.6 N38.3 1 Abbot (Apollonius K) E54.8 N5.6 1 Abenezra A (Mayfair A) E10.5 22.8S 2
    [Show full text]