Unclaimedproperty2021.Pdf

Total Page:16

File Type:pdf, Size:1020Kb

Unclaimedproperty2021.Pdf LAST_NAME FIRST_NAME MIDDLE_NAME Combined Name ACOSTA DONNA ACOSTA,DONNA ADAMS THE ESTATE OF EOLA G ADAMS,THE ESTATE OF EOLA G ALEXANDER ANTON ALEXANDER,ANTON ALEXANDRIA CHANCERY OFFICE OF DIOCES OF ALEXANDRIA,CHANCERY OFFICE OF DIOCES OF ANDERSON EUNICE ANDERSON,EUNICE ANDERSON JOE ANDERSON,JOE ARMSTRONG JOAN ARMSTRONG,JOAN ARMSTRONG JUANITA ARMSTRONG,JUANITA ARMSTRONG RAQUEL ARMSTRONG,RAQUEL ARMSTRONG TONY ARMSTRONG,TONY ARNOLD MYRTLE ARNOLD,MYRTLE ATKINSON DARIAN ATKINSON,DARIAN AUBIN THE ESTATE OF PEGGY ANN AUBIN,THE ESTATE OF PEGGY ANN BADON JOSEPH BADON,JOSEPH BAGGETT THE ESTATE OF CATHERINE BAGGETT,THE ESTATE OF CATHERINE BAILEY BRANDI BAILEY,BRANDI BAILEY JOE BAILEY,JOE BAILEY JULIA BAILEY,JULIA BAILEY MICAHEL BAILEY,MICAHEL BALTAZAR CHRISTOPHER BALTAZAR,CHRISTOPHER BALTAZAR DARREN BALTAZAR,DARREN BALTAZAR JR JERRY BALTAZAR JR,JERRY BAUM MAE BAUM,MAE BAYLES MELODY BAYLES ,MELODY BAYLOR RONNIE BAYLOR,RONNIE BEAL ROGER BEAL,ROGER BEAUVAIS THE ESTATE OF GRACIE BEAUVAIS,THE ESTATE OF GRACIE BELL CRAWFORD BELL,CRAWFORD BELL TIA SIERRA BELL,TIA SIERRA BELLEAU THE ESTATE OF JOSEPH BELLEAU,THE ESTATE OF JOSEPH BERRY C F BERRY,C F BETZ PAKIMA ARNEL BETZ,PAKIMA ARNEL BICE ESTATE OF ARTHUR BICE,ESTATE OF ARTHUR BLACKMON THE ESTATE OF KEITH BLACKMON,THE ESTATE OF KEITH BLAIR LECIA BLAIR,LECIA BLOUNT KIMBERLY BLOUNT,KIMBERLY BON JASON BON,JASON BOUDREAUX THE ESTATE OF VIRGINIA BOUDREAUX,THE ESTATE OF VIRGINIA BOWMAN TYMEL BOWMAN,TYMEL BOYD SHIRLEY BOYD,SHIRLEY BREVELLE LAURA BREVELLE,LAURA BROWN ADAM J BROWN,ADAM J BROWN ADAM P BROWN,ADAM P BROWN BRIANA BROWN,BRIANA BROWN CALVIN BROWN,CALVIN BROWN CHERYL BROWN,CHERYL BROWN GLYNDA BROWN,GLYNDA BROWN THE ESTAET OF LINDA BROWN,THE ESTAET OF LINDA BROWN THE ESTATE OF BRIMMER BROWN,THE ESTATE OF BRIMMER BRUMFIELD JEFFERY BRUMFIELD,JEFFERY BRYANT RHONDA BRYANT,RHONDA BURCHELL ESTATE OF THEA BURCHELL,ESTATE OF THEA BURCHELL THE ESTATE OF THEA BURCHELL,THE ESTATE OF THEA BURNS JAVON BURNS,JAVON BURNS TYRONE BURNS,TYRONE BURRELL BRENDA BURRELL,BRENDA BURTON ASHLEY BURTON,ASHLEY BURTON JR NELSON BURTON JR,NELSON BUTLER SR THE ESTATE OF EUGENE BUTLER SR,THE ESTATE OF EUGENE CAHILL AUGUSTINE CAHILL,AUGUSTINE CAPPO SARAH CAPPO,SARAH CARR LINDA CARR,LINDA CARRIER DEBORAH CARRIER,DEBORAH CARRUTH ROBERT CARRUTH,ROBERT CARTER TIMOTHY CARTER,TIMOTHY CASAWAY DELORES CASAWAY,DELORES CAWTHRAN ORLANDO CAWTHRAN,ORLANDO CHAISSON MARJORIE CHAISSON,MARJORIE CHAMPAGNE LOUIS CHAMPAGNE,LOUIS CHAMPAGNE THERESA CHAMPAGNE,THERESA CHAPMAN RONNIE CHAPMAN,RONNIE CHRETIEN THE ESTATE OF HELEN CHRETIEN,THE ESTATE OF HELEN CHURCH ST. FRANCIS XAVIER CATHOLIC CHURCH,ST.
Recommended publications
  • On Celestial Wings / Edgar D
    Library of Congress Cataloging-in-Publication Data Whitcomb. Edgar D. On Celestial Wings / Edgar D. Whitcomb. p. cm. Includes bibliographical references. 1. United States. Army Air Forces-History-World War, 1939-1945. 2. Flight navigators- United States-Biography. 3. World War, 1939-1945-Campaigns-Pacific Area. 4. World War, 1939-1945-Personal narratives, American. I. Title. D790.W415 1996 940.54’4973-dc20 95-43048 CIP ISBN 1-58566-003-5 First Printing November 1995 Second Printing June 1998 Third Printing December 1999 Fourth Printing May 2000 Fifth Printing August 2001 Disclaimer This publication was produced in the Department of Defense school environment in the interest of academic freedom and the advancement of national defense-related concepts. The views expressed in this publication are those of the author and do not reflect the official policy or position of the Department of Defense or the United States government. This publication has been reviewed by security and policy review authorities and is cleared for public release. Digitize February 2003 from August 2001 Fifth Printing NOTE: Pagination changed. ii This book is dedicated to Charlie Contents Page Disclaimer........................................................................................................................... ii Foreword............................................................................................................................ vi About the author ..............................................................................................................
    [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]
  • GSA TODAY a Publication of the Geological Society of America
    Vol. 5, No. 6 June 1995 GSA TODAY A Publication of the Geological Society of America 1995 ANNUAL MEETING New Orleans, Louisiana • November 6–9 ABSTRACTS DUE JULY 12 For abstract forms (303) 447-2020, ext. 161; E-mail: [email protected] SOFTWARE FAIR PROPOSALS DUE SEPTEMBER 1 For information: (504) 286-6791; fax 504-286-7396; E-mail: [email protected] PREREGISTRATION DUE SEPTEMBER 29 Registration and housing forms enclosed INFORMATION (303) 447-2020, ext. 184 or 1-800-472-1988; fax 303-447-0648; E-mail: [email protected] he theme for the 1995 Annual Meeting is Bridging the Gulf. This theme has several meanings. In particular, we will draw attention to the Gulf of Mexico–Caribbean, and the surrounding T American continents, bridging the knowledge gap that exists across a region divided by polit- ical boundaries and language but sharing a common geologic framework. Bridging the Gulf also addresses the need to develop a closer link between technology and the science of geology and to educate the public on issues critical to the development of intelligent policies on the environment and geologic hazards. We also hope to bridge the gulf between the past and the future with both a retrospection on the past 25 years of plate tectonics and a look at the future as geology responds to society’s needs. Finally, we view the city of New Orleans, the Mississippi River and its delta, and the Gulf Coast as a laboratory where the long- term effects of humans on the environment can be examined. NEW ORLEANS: The Crescent City–New Orleans is nestled on the inside of a south-looping meander of the Mississippi River.
    [Show full text]
  • Arxiv:2012.15102V2 [Hep-Ph] 13 May 2021 T > Tc
    Confinement of Fermions in Tachyon Matter at Finite Temperature Adamu Issifu,1, ∗ Julio C.M. Rocha,1, y and Francisco A. Brito1, 2, z 1Departamento de F´ısica, Universidade Federal da Para´ıba, Caixa Postal 5008, 58051-970 Jo~aoPessoa, Para´ıba, Brazil 2Departamento de F´ısica, Universidade Federal de Campina Grande Caixa Postal 10071, 58429-900 Campina Grande, Para´ıba, Brazil We study a phenomenological model that mimics the characteristics of QCD theory at finite temperature. The model involves fermions coupled with a modified Abelian gauge field in a tachyon matter. It reproduces some important QCD features such as, confinement, deconfinement, chiral symmetry and quark-gluon-plasma (QGP) phase transitions. The study may shed light on both light and heavy quark potentials and their string tensions. Flux-tube and Cornell potentials are developed depending on the regime under consideration. Other confining properties such as scalar glueball mass, gluon mass, glueball-meson mixing states, gluon and chiral condensates are exploited as well. The study is focused on two possible regimes, the ultraviolet (UV) and the infrared (IR) regimes. I. INTRODUCTION Confinement of heavy quark states QQ¯ is an important subject in both theoretical and experimental study of high temperature QCD matter and quark-gluon-plasma phase (QGP) [1]. The production of heavy quarkonia such as the fundamental state ofcc ¯ in the Relativistic Heavy Iron Collider (RHIC) [2] and the Large Hadron Collider (LHC) [3] provides basics for the study of QGP. Lattice QCD simulations of quarkonium at finite temperature indicates that J= may persists even at T = 1:5Tc [4] i.e.
    [Show full text]
  • Imagining Outer Space Also by Alexander C
    Imagining Outer Space Also by Alexander C. T. Geppert FLEETING CITIES Imperial Expositions in Fin-de-Siècle Europe Co-Edited EUROPEAN EGO-HISTORIES Historiography and the Self, 1970–2000 ORTE DES OKKULTEN ESPOSIZIONI IN EUROPA TRA OTTO E NOVECENTO Spazi, organizzazione, rappresentazioni ORTSGESPRÄCHE Raum und Kommunikation im 19. und 20. Jahrhundert NEW DANGEROUS LIAISONS Discourses on Europe and Love in the Twentieth Century WUNDER Poetik und Politik des Staunens im 20. Jahrhundert Imagining Outer Space European Astroculture in the Twentieth Century Edited by Alexander C. T. Geppert Emmy Noether Research Group Director Freie Universität Berlin Editorial matter, selection and introduction © Alexander C. T. Geppert 2012 Chapter 6 (by Michael J. Neufeld) © the Smithsonian Institution 2012 All remaining chapters © their respective authors 2012 All rights reserved. No reproduction, copy or transmission of this publication may be made without written permission. No portion of this publication may be reproduced, copied or transmitted save with written permission or in accordance with the provisions of the Copyright, Designs and Patents Act 1988, or under the terms of any licence permitting limited copying issued by the Copyright Licensing Agency, Saffron House, 6–10 Kirby Street, London EC1N 8TS. Any person who does any unauthorized act in relation to this publication may be liable to criminal prosecution and civil claims for damages. The authors have asserted their rights to be identified as the authors of this work in accordance with the Copyright, Designs and Patents Act 1988. First published 2012 by PALGRAVE MACMILLAN Palgrave Macmillan in the UK is an imprint of Macmillan Publishers Limited, registered in England, company number 785998, of Houndmills, Basingstoke, Hampshire RG21 6XS.
    [Show full text]
  • Martian Crater Morphology
    ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter.
    [Show full text]
  • A La Torre Aaker Aalbers Aaldert Aarmour Aaron
    A LA TORRE ABDIE ABLEMAN ABRAMOWITCH AAKER ABE ABLES ABRAMOWITZ AALBERS ABEE ABLETSON ABRAMOWSKY AALDERT ABEEL ABLETT ABRAMS AARMOUR ABEELS ABLEY ABRAMSEN AARON ABEKE ABLI ABRAMSKI AARONS ABEKEN ABLITT ABRAMSON AARONSON ABEKING ABLOTT ABRAMZON AASEN ABEL ABNER ABRASHKIN ABAD ABELA ABNETT ABRELL ABADAM ABELE ABNEY ABREU ABADIE ABELER ABORDEAN ABREY ABALOS ABELES ABORDENE ABRIANI ABARCA ABELI ABOT ABRIL ABATE ABELIN ABOTS ABRLI ABB ABELL ABOTSON ABRUZZO ABBA ABELLA ABOTT ABSALOM ABBARCROMBIE ABELLE ABOTTS ABSALON ABBAS ABELLS ABOTTSON ABSHALON ABBAT ABELMAN ABRAHAM ABSHER ABBATE ABELS ABRAHAMER ABSHIRE ABBATIELLO ABELSON ABRAHAMI ABSOLEM ABBATT ABEMA ABRAHAMIAN ABSOLOM ABBAY ABEN ABRAHAMOF ABSOLON ABBAYE ABENDROTH ABRAHAMOFF ABSON ABBAYS ABER ABRAHAMOV ABSTON ABBDIE ABERCROMBIE ABRAHAMOVITZ ABT ABBE ABERCROMBY ABRAHAMOWICZ ABTS ABBEKE ABERCRUMBIE ABRAHAMS ABURN ABBEL ABERCRUMBY ABRAHAMS ABY ABBELD ABERCRUMMY ABRAHAMSEN ABYRCRUMBIE ABBELL ABERDEAN ABRAHAMSOHN ABYRCRUMBY ABBELLS ABERDEEN ABRAHAMSON AC ABBELS ABERDEIN ABRAHAMSSON ACASTER ABBEMA ABERDENE ABRAHAMY ACCA ABBEN ABERG ABRAHM ACCARDI ABBERCROMBIE ABERLE ABRAHMOV ACCARDO ABBERCROMMIE ABERLI ABRAHMOVICI ACE ABBERCRUMBIE ABERLIN ABRAHMS ACERO ABBERDENE ABERNATHY ABRAHMSON ACESTER ABBERDINE ABERNETHY ABRAM ACETO ABBERLEY ABERT ABRAMCHIK ACEVEDO ABBETT ABEYTA ABRAMCIK ACEVES ABBEY ABHERCROMBIE ABRAMI ACHARD ABBIE ABHIRCROMBIE ABRAMIN ACHENBACH ABBING ABIRCOMBIE ABRAMINO ACHENSON ABBIRCROMBIE ABIRCROMBIE ABRAMO ACHERSON ABBIRCROMBY ABIRCROMBY ABRAMOF ACHESON ABBIRCRUMMY ABIRCROMMBIE ABRAMOFF
    [Show full text]
  • Talking Book Topics November-December 2016
    Talking Book Topics November–December 2016 Volume 82, Number 6 About Talking Book Topics Talking Book Topics is published bimonthly in audio, large-print, and online formats and distributed at no cost to participants in the Library of Congress reading program for people who are blind or have a physical disability. An abridged version is distributed in braille. This periodical lists digital talking books and magazines available through a network of cooperating libraries and carries news of developments and activities in services to people who are blind, visually impaired, or cannot read standard print material because of an organic physical disability. The annotated list in this issue is limited to titles recently added to the national collection, which contains thousands of fiction and nonfiction titles, including bestsellers, classics, biographies, romance novels, mysteries, and how-to guides. Some books in Spanish are also available. To explore the wide range of books in the national collection, visit the NLS Union Catalog online at www.loc.gov/nls or contact your local cooperating library. Talking Book Topics is also available in large print from your local cooperating library and in downloadable audio files on the NLS Braille and Audio Reading Download (BARD) site at https://nlsbard.loc.gov. An abridged version is available to subscribers of Braille Book Review. Library of Congress, Washington 2016 Catalog Card Number 60-46157 ISSN 0039-9183 About BARD Most books and magazines listed in Talking Book Topics are available to eligible readers for download. To use BARD, contact your cooperating library or visit https://nlsbard.loc.gov for more information.
    [Show full text]
  • POLYGONAL IMPACT CRATERS on CHARON. C.B. Beddingfield1,2, R
    51st Lunar and Planetary Science Conference (2020) 1241.pdf POLYGONAL IMPACT CRATERS ON CHARON. C.B. Beddingfield1,2, R. Beyer1,2, R.J. Cartwright1,2, K. Singer3, S. Robbins3, S.A. Stern3, V. Bray4, J.M. Moore2, K. Ennico2, C.B. Olkin3, J.R. Spencer3, H.A. Weaver5, L.A. Young3, A.Verbiscer6, J. Parker3, and the New Horizons Geology, Geophysics, and Imaging (GGI) Team; 1SETI In- stitute, Mountain View, CA, 2NASA Ames Research Center, Mountain View, CA ([email protected]), 3Southwest Research Institute, Boulder, CO, 4University of Arizona, Tucson, AZ, 5John Hopkins University Applied Physics Laboratory, Laurel, MD, 6University of Virginia, Charlottesville, VA. Introduction: Polygonal impact craters (PICs) re- flect pre-existing extensional and strike-slip faults and fractures in the target material [e.g. 1-9]. PIC straight rim segments therefore can provide important infor- mation for deciphering the tectonic histories of plane- tary bodies [e.g. 8]. The only known PIC formation mechanism is the presence of pre-existing sub-vertical structures within the target material [e.g. 5, 7, 11-13]. In contrast, circular impact craters (CICs) are in- ferred to result from impact events in non-tectonized target material. CICs can also form in pre-fractured tar- get material if the fractures are widely or closely spaced, if the fracture system is highly complex, or if the target material is covered by a thick layer of non-cohesive sed- iment that limits interactions between the impactor and the underlying bedrock/ice [e.g. 14]. Consequently, PICs and CICs are useful tools to distinguish between Fig.
    [Show full text]
  • At NALC's Doorstep
    Volume 134/Number 2 February 2021 In this issue President’s Message 1 Branch Election Notices 81 Special issue LETTER CARRIER POLITICAL FUND The monthly journal of the NATIONAL ASSOCIATION OF LETTER CARRIERS ANARCHY at NALC’s doorstep— PAGE 1 { InstallInstall thethe freefree NALCNALC MemberMember AppApp forfor youryour iPhoneiPhone oror AndroidAndroid smartphonesmartphone As technology increases our ability to communicate, NALC must stay ahead of the curve. We’ve now taken the next step with the NALC Member App for iPhone and Android smartphones. The app was de- veloped with the needs of letter carriers in mind. The app’s features include: • Workplace resources, including the National • Instantaneous NALC news with Agreement, JCAM, MRS and CCA resources personalized push notifications • Interactive Non-Scheduled Days calendar and social media access • Legislative tools, including bill tracker, • Much more individualized congressional representatives and PAC information GoGo to to the the App App Store Store oror GoogleGoogle Play Play and and search search forfor “NALC “NALC Member Member App”App” toto install install for for free free President’s Message Anarchy on NALC’s doorstep have always taken great These developments have left our nation shaken. Our polit- pride in the NALC’s head- ical divisions are raw, and there now is great uncertainty about quarters, the Vincent R. the future. This will certainly complicate our efforts to advance Sombrotto Building. It sits our legislative agenda in the now-restored U.S. Capitol. But kitty-corner to the United there is reason for hope. IStates Capitol, a magnificent First, we should take solace in the fact that the attack on our and inspiring structure that has democracy utterly failed.
    [Show full text]
  • Executive Summary
    The Boston University Astronomy Department Annual Report 2010 Chair: James Jackson Administrator: Laura Wipf 1 2 TABLE OF CONTENTS Executive Summary 5 Faculty and Staff 5 Teaching 6 Undergraduate Programs 6 Observatory and Facilities 8 Graduate Program 9 Colloquium Series 10 Alumni Affairs/Public Outreach 10 Research 11 Funding 12 Future Plans/Departmental Needs 13 APPENDIX A: Faculty, Staff, and Graduate Students 16 APPENDIX B: 2009/2010 Astronomy Graduates 18 APPENDIX C: Seminar Series 19 APPENDIX D: Sponsored Project Funding 21 APPENDIX E: Accounts Income Expenditures 25 APPENDIX F: Publications 27 Cover photo: An ultraviolet image of Saturn taken by Prof. John Clarke and his group using the Hubble Space Telescope. The oval ribbons toward the top and bottom of the image shows the location of auroral activity near Saturn’s poles. This activity is analogous to Earth’s aurora borealis and aurora australis, the so-called “northern” and “southern lights,” and is caused by energetic particles from the sun trapped in Saturn’s magnetic field. 3 4 EXECUTIVE SUMMARY associates authored or co-authored a total of 204 refereed, scholarly papers in the disciplines’ most The Department of Astronomy teaches science to prestigious journals. hundreds of non-science majors from throughout the university, and runs one of the largest astronomy degree The funding of the Astronomy Department, the Center programs in the country. Research within the for Space Physics, and the Institute for Astrophysical Astronomy Department is thriving, and we retain our Research was changed this past year. In previous years, strong commitment to teaching and service. only the research centers received research funding, but last year the Department received a portion of this The Department graduated a class of twelve research funding based on grant activity by its faculty.
    [Show full text]
  • Secondary Craters on Europa and Implications for Cratered Surfaces
    Vol 437|20 October 2005|doi:10.1038/nature04069 LETTERS Secondary craters on Europa and implications for cratered surfaces Edward B. Bierhaus1, Clark R. Chapman2 & William J. Merline2 For several decades, most planetary researchers have regarded the craters were typically not spatially random, but instead appeared in impact crater populations on solid-surfaced planets and smaller clumps and clusters16 even at distances far (several hundred kilo- bodies as predominantly reflecting the direct (‘primary’) impacts metres) from the nearest large primary crater. This clustered spatial of asteroids and comets1. Estimates of the relative and absolute distribution contrasts with primary impacts, which are spatially ages of geological units on these objects have been based on this random. The low spatial density and unusual non-random spatial assumption2. Here we present an analysis of the comparatively distribution of Europa’s small craters enabled us to achieve what has sparse crater population on Jupiter’s icy moon Europa and suggest been previously difficult, namely unambiguous identification and that this assumption is incorrect for small craters. We find that quantification of the contribution of distant secondary craters to the ‘secondaries’ (craters formed by material ejected from large total crater SFD. This, in turn, allows us to re-examine the overall primary impact craters) comprise about 95 per cent of the small crater age-dating methodology. We discuss the specifics of the craters (diameters less than 1 km) on Europa. We therefore con- Europa data first. clude that large primary impacts into a solid surface (for example, We measured more than 17,000 craters in 87 low-compression, ice or rock) produce far more secondaries than previously low-sun, high-resolution Europa images (scales ,60 m pixel21), believed, implying that the small crater populations on the which cover nine regions totalling 0.2% of Europa’s surface (a much Moon, Mars and other large bodies must be dominated by larger percentage of Europa has been imaged at lower resolutions), secondaries.
    [Show full text]