JAKE KILRAIN IS HALE at 75 Husband Will WHERE YOU Man Who Slugged with Great John L
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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. -
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. -
Widespread Crater-Related Pitted Materials on Mars: Further Evidence for the Role of Target Volatiles During the Impact Process ⇑ Livio L
Icarus 220 (2012) 348–368 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process ⇑ Livio L. Tornabene a, , Gordon R. Osinski a, Alfred S. McEwen b, Joseph M. Boyce c, Veronica J. Bray b, Christy M. Caudill b, John A. Grant d, Christopher W. Hamilton e, Sarah Mattson b, Peter J. Mouginis-Mark c a University of Western Ontario, Centre for Planetary Science and Exploration, Earth Sciences, London, ON, Canada N6A 5B7 b University of Arizona, Lunar and Planetary Lab, Tucson, AZ 85721-0092, USA c University of Hawai’i, Hawai’i Institute of Geophysics and Planetology, Ma¯noa, HI 96822, USA d Smithsonian Institution, Center for Earth and Planetary Studies, Washington, DC 20013-7012, USA e NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA article info abstract Article history: Recently acquired high-resolution images of martian impact craters provide further evidence for the Received 28 August 2011 interaction between subsurface volatiles and the impact cratering process. A densely pitted crater-related Revised 29 April 2012 unit has been identified in images of 204 craters from the Mars Reconnaissance Orbiter. This sample of Accepted 9 May 2012 craters are nearly equally distributed between the two hemispheres, spanning from 53°Sto62°N latitude. Available online 24 May 2012 They range in diameter from 1 to 150 km, and are found at elevations between À5.5 to +5.2 km relative to the martian datum. The pits are polygonal to quasi-circular depressions that often occur in dense clus- Keywords: ters and range in size from 10 m to as large as 3 km. -
Recent Channel Systems Emanating from Hale Crater Ejecta: Implications for the Noachian Landscape Evolution of Mars
Lunar and Planetary Science XXXIX (2008) 2180.pdf RECENT CHANNEL SYSTEMS EMANATING FROM HALE CRATER EJECTA: IMPLICATIONS FOR THE NOACHIAN LANDSCAPE EVOLUTION OF MARS. L. L. Tornabene1, 2, A. S. McEwen1, and the HiRISE Team1, 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, [email protected] Introduction: Impact cratering is a fundamental into linear elements that do not appear to be typical crater geologic process that dominated the distant geologic past rays, but like rays lie radial to Hale (e.g., 315°E, 32°S; of the terrestrial planets. Thereby, impacts played a 323.6°E, 35.7°S). Further, Hale has pristine morphologic significant role in the formation and evolution of planetary features at the decameter scale such as a sharp but crusts in the form of impact effects and byproducts (e.g., complexly terraced rim, a prominent central peak and only ejecta, breccias, impact melts, etc.). On Mars, impacts may small (<1 km) and few superimposed craters. The ejecta have liberated subsurface volatiles that, in the form of and secondaries from Hale are superimposed over liquid water, modified both surface morphology and surrounding terrains covering a large expanse of Mars, composition (e.g., phyllosilicates [e.g., 1]), and possibly with one swath of secondaries spanning >500 km wide. influenced early habitable environments. Although such an Hale also possesses ponded materials and channelized interaction has been inferred by studies of crater flows, which is an indication of the presence of impact- morphology [e.g., 2] and impact models [e.g., 3], direct melt bearing materials, as well as a testament to the evidence for the release of liquid water or other volatiles youthfulness and excellent state of preservation of the by Martian impacts was lacking [4]. -
Crater Geometry and Ejecta Thickness of the Martian Impact Crater Tooting
Meteoritics & Planetary Science 42, Nr 9, 1615–1625 (2007) Abstract available online at http://meteoritics.org Crater geometry and ejecta thickness of the Martian impact crater Tooting Peter J. MOUGINIS-MARK and Harold GARBEIL Hawai‘i Institute of Geophysics and Planetology, University of Hawai‘i, Honolulu, Hawai‘i 96822, USA (Received 25 October 2006; revision accepted 04 March 2007) Abstract–We use Mars Orbiter Laser Altimeter (MOLA) topographic data and Thermal Emission Imaging System (THEMIS) visible (VIS) images to study the cavity and the ejecta blanket of a very fresh Martian impact crater ~29 km in diameter, with the provisional International Astronomical Union (IAU) name Tooting crater. This crater is very young, as demonstrated by the large depth/ diameter ratio (0.065), impact melt preserved on the walls and floor, an extensive secondary crater field, and only 13 superposed impact craters (all 54 to 234 meters in diameter) on the ~8120 km2 ejecta blanket. Because the pre-impact terrain was essentially flat, we can measure the volume of the crater cavity and ejecta deposits. Tooting crater has a rim height that has >500 m variation around the rim crest and a very large central peak (1052 m high and >9 km wide). Crater cavity volume (i.e., volume below the pre-impact terrain) is ~380 km3 and the volume of materials above the pre-impact terrain is ~425 km3. The ejecta thickness is often very thin (<20 m) throughout much of the ejecta blanket. There is a pronounced asymmetry in the ejecta blanket, suggestive of an oblique impact, which has resulted in up to ~100 m of additional ejecta thickness being deposited down-range compared to the up-range value at the same radial distance from the rim crest. -
Bare-Knuckle Prize Fighting
Loyola University Chicago Loyola eCommons Faculty Publications and Other Works by History: Faculty Publications and Other Works Department 3-2019 Bare-Knuckle Prize Fighting Elliot Gorn Loyola University Chicago, [email protected] Follow this and additional works at: https://ecommons.luc.edu/history_facpubs Part of the History Commons Recommended Citation Gorn, Elliot. Bare-Knuckle Prize Fighting. The Cambridge Encyclopedia of Boxing, , : 34-51, 2019. Retrieved from Loyola eCommons, History: Faculty Publications and Other Works, This Book Chapter is brought to you for free and open access by the Faculty Publications and Other Works by Department at Loyola eCommons. It has been accepted for inclusion in History: Faculty Publications and Other Works by an authorized administrator of Loyola eCommons. For more information, please contact [email protected]. This work is licensed under a Creative Commons Attribution-Noncommercial-No Derivative Works 3.0 License. © Cambridge University Press, 2019. 34 2 ELLIOTT J. GORN The Bare- Knuckle Era Origins of the Ring Fistic combat goes back at least as far as ancient Greece and Rome. Pindar , in 474 BC , celebrated Diagoras ’ victory in the Greek Olympiad: “But do thou, O father Zeus, that rulest over the height of Atabyrium, grant honour to the hymn ordained in praise of an Olympian victor, and to the hero who hath found fame for his prowess as a boxer; and do though give him grace and reverence in the eyes of citizens and of strangers too. For he goeth in a straight course along a path that hateth insolence.” Worthy of Zeus’ blessing, the successful boxer was a man of moral as well as physical excel- lence. -
Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ 2014
Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ 2014 Edited by: James A. Skinner, Jr. U. S. Geological Survey, Flagstaff, AZ David Williams Arizona State University, Tempe, AZ NOTE: Abstracts in this volume can be cited using the following format: Graupner, M. and Hansen, V.L., 2014, Structural and Geologic Mapping of Tellus Region, Venus, in Skinner, J. A., Jr. and Williams, D. A., eds., Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ, June 23-25, 2014. SCHEDULE OF EVENTS Monday, June 23– Planetary Geologic Mappers Meeting Time Planet/Body Topic 8:30 am Arrive/Set-up – 2255 N. Gemini Drive (USGS) 9:00 Welcome/Logistics 9:10 NASA HQ and Program Remarks (M. Kelley) 9:30 USGS Map Coordinator Remarks (J. Skinner) 9:45 GIS and Web Updates (C. Fortezzo) 10:00 RPIF Updates (J. Hagerty) 10:15 BREAK / POSTERS 10:40 Venus Irnini Mons (D. Buczkowski) 11:00 Moon Lunar South Pole (S. Mest) 11:20 Moon Copernicus Quad (J. Hagerty) 11:40 Vesta Iterative Geologic Mapping (A. Yingst) 12:00 pm LUNCH / POSTERS 1:30 Vesta Proposed Time-Stratigraphy (D. Williams) 1:50 Mars Global Geology (J. Skinner) 2:10 Mars Terra Sirenum (R. Anderson) 2:30 Mars Arsia/Pavonis Montes (B. Garry) 2:50 Mars Valles Marineris (C. Fortezzo) 3:10 BREAK / POSTERS 3:30 Mars Candor Chasma (C. Okubo) 3:50 Mars Hrad Vallis (P. Mouginis-Mark) 4:10 Mars S. Margaritifer Terra (J. Grant) 4:30 Mars Ladon basin (C. Weitz) 4:50 DISCUSSION / POSTERS ~5:15 ADJOURN Tuesday, June 24 - Planetary Geologic Mappers Meeting Time Planet/Body Topic 8:30 am Arrive/Set-up/Logistics 9:00 Mars Upper Dao and Niger Valles (S. -
December 16, 2011 Vol. 115 No. 50
VOL. 115 - NO. 50 BOSTON, MASSACHUSETTS, DECEMBER 16, 2011 $.30 A COPY First Night Boston 2012 NORTH END ATHLETIC ASSOCIATION 41ST ANNUAL NORTH END CHRISTMAS PARADE Here Comes Santa Claus! by Sal Giarratani FedEx Family Festival. (Photo by Paul Marotta) This year, First Night Boston celebrates the 36th edition of the country’s oldest and largest New Year’s Eve arts festival by announcing a line-up of world class events that offer some- thing for everyone. On Saturday, December 31, 2011 from noon to midnight, First Night presents its annual day-long festival of art, music, dance, ice sculpture and more. First Night will showcase 1,000 artists in 200 exhibitions and per- formances in locations all over downtown Boston, from the Waterfront to the Fenway. First Night welcomes children, families and revelers of all ages to celebrate community While driving up from the rival of Santa by helicopter jolly ole Santa. This year First Night organizers strongly suggest through the arts. south on Route 95, I heard at Puopolo Park. marked St. Agrippina’s 17lh visiting the interactive planner at www.firstnight.org to Bruce Springsteen singing The Christmas parade was Annual Christmas Program plan attendance . The schedule is subject to change and “Santa Claus is Coming to sponsored by the North End for the kids. updates can be found on the website. Town.” This Christmas clas- Athletic Association in asso- I’m sure many other chil- All First Night outdoor events are free, though supported sic was playing on the radio as ciation with The Nazzaro dren were thinking the by sales of the First Night button, which is the ticket for I was headed to town to see Center, North End Against same thing. -
Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America
Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America There are approximately 101,135sexual abuse claims filed. Of those claims, the Tort Claimants’ Committee estimates that there are approximately 83,807 unique claims if the amended and superseded and multiple claims filed on account of the same survivor are removed. The summary of sexual abuse claims below uses the set of 83,807 of claim for purposes of claims summary below.1 The Tort Claimants’ Committee has broken down the sexual abuse claims in various categories for the purpose of disclosing where and when the sexual abuse claims arose and the identity of certain of the parties that are implicated in the alleged sexual abuse. Attached hereto as Exhibit 1 is a chart that shows the sexual abuse claims broken down by the year in which they first arose. Please note that there approximately 10,500 claims did not provide a date for when the sexual abuse occurred. As a result, those claims have not been assigned a year in which the abuse first arose. Attached hereto as Exhibit 2 is a chart that shows the claims broken down by the state or jurisdiction in which they arose. Please note there are approximately 7,186 claims that did not provide a location of abuse. Those claims are reflected by YY or ZZ in the codes used to identify the applicable state or jurisdiction. Those claims have not been assigned a state or other jurisdiction. Attached hereto as Exhibit 3 is a chart that shows the claims broken down by the Local Council implicated in the sexual abuse. -
Par Meliaceae
SMITHSONIAN COKTRIBUTIONS TO BOTANY NUMBER 4 Mason E. Hale, Jr. Morden-Smithsonian.. Expedition to Dominica: The Lichens (Parmeliaceae) SMITHSOXIAN INSTITUTION PRESS CITY OF WASHINGTON '971 ABSTRACT Hale, Mason E., Jr. Morden-Smithsonian Expedition to Dominica : The Lichens (Parmeliaceae) . Smitlzsonian Contributions to Botany, number 4, 25 pages, 1971.- A revision is made of the lichen family Parmeliaceae in Dominica, based on previous published records by Elliott and on collections by the author. Twenty-two species are now known for Parmelia, the only genus in this family on the island. A new species, Parmelia mordenii, is described from rock habitats in the dry scrub woodland. Official publication date is handstamped in a limited number of initial copies and is recorded in the Institution’s annual report, Smithsonian Year. UNITED STATES GOVERNMENT PRINTING OFFICE WASHINGTON : 1911 For sale by the Superintendent of Documents, US. Government Printing OWce Washington, D.C. 20402 - Price 45 cents (paper cover) Mason E. Hale, 3r. Morden-Smithsonian *. Expedition to Dominica: The Lichens (Parmeliaceae) Introduction Roseau Botanical Garden during a 1926 cruise, and his specimens are now preserved in the Smithsonian Dominica lies in the Windward Lesser Antilles, ap- Institution (US). The only other lichenologist to visit proximately midway between Trinidad to the south the island, as far as I can determine, is Henry Ims- and Antigua to the north. It is the most mountainous haug, who spent about a month there in 1963. His island in this chain and has been subject to the least specimens, which I have seen, are preserved at Michi- disturbance by man. There are extensive areas of gan State University (MSC) and will form part of virgin forest, and although commercial logging has the materials for his proposed lichen flora of the begun in earnest in the past five years, it will hope- West Indies. -
NEW ORLEANS NOSTALGIA Remembering New Orleans History, Culture and Traditions by Ned Hémard
NEW ORLEANS NOSTALGIA Remembering New Orleans History, Culture and Traditions By Ned Hémard Last of the Bare-Knuckles Dow Jones & Company’s issuance of hand-delivered short news briefs (called “flimsies”) to stock traders culminated in the publication of THE WALL STREET JOURNAL, July 8, 1889 (Price Two Cents), and New Orleans made the first page of the very first issue, 125 years ago. It all had to do with a highly anticipated prize fight. THE JOURNAL bulletins attempted to provide any updates on the Jake Kilrain vs. John L. Sullivan fight. Bare-knuckle fighting was illegal in all of the existing thirty-eight states, and (although New Orleans was at the vortex of this pugilistic whirlwind) Governor Francis T. Nicholls had forbidden the fight in Louisiana and had activated the state militia to prevent it. Governor Robert Lowry of Mississippi had taken similar measures. Where the bout was to be fought was shrouded in secrecy, unrevealed until the train leaving New Orleans deposited a multitude of enthusiastic fightgoers at the clandestinely arranged location. An earlier announcement (January 12, 1889) in the New Orleans Weekly Pelican heralded the upcoming contest. The confrontation between Kilrain and Sullivan is considered to be a turning point in boxing history, being the last world title bout fought under the London Prize Ring Rules and therefore the last bare-knuckle heavyweight title bout. No gloves were worn and some wrestling moves were permitted. A round concluded when one fighter was knocked down, and the fight lasted until one contestant was unable to get up off the ring floor. -
Orthodox Political Theologies: Clergy, Intelligentsia and Social Christianity in Revolutionary Russia
DOI: 10.14754/CEU.2020.08 ORTHODOX POLITICAL THEOLOGIES: CLERGY, INTELLIGENTSIA AND SOCIAL CHRISTIANITY IN REVOLUTIONARY RUSSIA Alexandra Medzibrodszky A DISSERTATION in History Presented to the Faculties of the Central European University In Partial Fulfilment of the Requirements for the Degree of Doctor of Philosophy CEU eTD Collection Budapest, Hungary 2020 Dissertation Supervisor: Matthias Riedl DOI: 10.14754/CEU.2020.08 Copyright Notice and Statement of Responsibility Copyright in the text of this dissertation rests with the Author. Copies by any process, either in full or part, may be made only in accordance with the instructions given by the Author and lodged in the Central European Library. Details may be obtained from the librarian. This page must form a part of any such copies made. Further copies made in accordance with such instructions may not be made without the written permission of the Author. I hereby declare that this dissertation contains no materials accepted for any other degrees in any other institutions and no materials previously written and/or published by another person unless otherwise noted. CEU eTD Collection ii DOI: 10.14754/CEU.2020.08 Technical Notes Transliteration of Russian Cyrillic in the dissertation is according to the simplified Library of Congress transliteration system. Well-known names, however, are transliterated in their more familiar form, for instance, ‘Tolstoy’ instead of ‘Tolstoii’. All translations are mine unless otherwise indicated. Dates before February 1918 are according to the Julian style calendar which is twelve days behind the Gregorian calendar in the nineteenth century and thirteen days behind in the twentieth century.