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Legend E D 1 M LV Y P Y B a B O
O L P V T D IN E E A B T N R UT D A P C K R T R E A S R D E D N A X R M N I CRE R S Y C T E I V P K D R I R D E I- D P E 2 D K R O EVERGREEN RD G 5 I STELLA DR E - A O E S 2 E BAPTIST RD L R W BAPTIST RD P Y L 5 A A E O D D C W CIR W T X N LL L P P O GU HOLBEIN DR BECKY DR I T R I A R R F D T SE O E O E O K FIEL N S O C 1 R D T CONE RD O I W X PINE A 5 V B E D C M P OLE P D I N 8 E O T P N AM R N CIR P D DI O RWOO D R E P O U VIEW LN ASANT D 1 C E N T D O PL R L D O R G 5 R G B T R R D R 8 R E D E A C N E B I N E M E O I R M S D N T L C S T O R D N F D P P A I S C T H P R D F N A W A I U E H A A R O D R H L R O R U O M A C R E E D A H A L E C Y DEBY PL C A L T M D R B T C D P R K A H RI E O R R R A P A L E I T D D S V L E O Q P H A R C R L S L T R ST D HOLBROOK L L P L L W E A A Y L GH B T L R I P Y K S O E I E I E R AT L C R H D A D L N R B R I R A T D G H L O R E O R M RD C D IN P R TANNENBAU D N I N R I D D N N N R C E D G O L A G U K O S R U O E S Y U O C DF E S SPRING VALLE E E O RD R R R M H F ECOACH L NB STAG W D I T C I L C B E T T E I W W U L H W O S DT CT D A E E W AN E I O R T U S L D L B V R B T C L C N A C Q N I A O W K R D L M I L R V A S A E E A R C O E C R J T I I A O R S O R N H D L T O R S L A PL M N DR TR D A D O UT C S H R E R E L RS LOOP D O P C J HAY CREEK RD D S O N R L C O T U DR D K U R E ROC R A R R P D ED S N K N D M O E I Y TS L BAR X R U N HE P B T IG H S L ES A R N Y N T D ERT INN W L E O S T B D V H R I OU TA L B C ES R N E D I R RY W E B E O T T LL K W E O R R IT P E OD S O RANGELY DR E Q L K R R S B R -
America's First Moon Landing
America’s First Moon Landing (July 21, 1969) Apollo 11, which was launched into his oval mural commemorating America’s Moon landing space from the Kennedy Space Center, embellishes the Brumidi Corridors in the Senate wing of the Florida, began its epic voyage to the Moon on July 16, 1969. On board were Capitol. The mural’s three main elements are: the rocket that Commander Neil A. Armstrong, Lunar propelled the astronauts into orbit; astronauts Neil Armstrong Module Pilot Edwin E. ”Buzz“ Aldrin, Jr., and Buzz Aldrin planting the United States flag on the Moon, and Command Module Pilot Michael with the lunar module Eagle in the background and the space capsule Collins. After 24 hours in lunar orbit, the T command/service module, Columbia, Columbia circling the Moon; and a view of Earth as seen from the Moon. separated from the lunar module, Eagle. Although the Eagle landed on the Moon in the afternoon of July 20, Armstrong and Aldrin began their descent to the lunar surface in the Eagle while Armstrong and Aldrin did not erect the flag until the next morning, which Collins stayed behind to pilot the explains why the scene is dated July 21, 1969. Columbia. The lunar module touched Muralist Allyn Cox painted the work. The son of artists Kenyon down on the Moon at Tranquility Base on July 20, 1969, at 4:17 P.M. EDT.Arm and Louise King Cox, Allyn Cox was born in New York City. He was strong reported, “The Eagle has landed.” educated at the National Academy of Design and the Art Students League At 10:56 P.M., Armstrong stepped in New York, and the American Academy in Rome. -
Surface Characteristics of Transneptunian Objects and Centaurs from Photometry and Spectroscopy
Barucci et al.: Surface Characteristics of TNOs and Centaurs 647 Surface Characteristics of Transneptunian Objects and Centaurs from Photometry and Spectroscopy M. A. Barucci and A. Doressoundiram Observatoire de Paris D. P. Cruikshank NASA Ames Research Center The external region of the solar system contains a vast population of small icy bodies, be- lieved to be remnants from the accretion of the planets. The transneptunian objects (TNOs) and Centaurs (located between Jupiter and Neptune) are probably made of the most primitive and thermally unprocessed materials of the known solar system. Although the study of these objects has rapidly evolved in the past few years, especially from dynamical and theoretical points of view, studies of the physical and chemical properties of the TNO population are still limited by the faintness of these objects. The basic properties of these objects, including infor- mation on their dimensions and rotation periods, are presented, with emphasis on their diver- sity and the possible characteristics of their surfaces. 1. INTRODUCTION cally with even the largest telescopes. The physical char- acteristics of Centaurs and TNOs are still in a rather early Transneptunian objects (TNOs), also known as Kuiper stage of investigation. Advances in instrumentation on tele- belt objects (KBOs) and Edgeworth-Kuiper belt objects scopes of 6- to 10-m aperture have enabled spectroscopic (EKBOs), are presumed to be remnants of the solar nebula studies of an increasing number of these objects, and signifi- that have survived over the age of the solar system. The cant progress is slowly being made. connection of the short-period comets (P < 200 yr) of low We describe here photometric and spectroscopic studies orbital inclination and the transneptunian population of pri- of TNOs and the emerging results. -
Observational Studies of the Galaxy Peculiar Velocity Field
OBSERVATIONAL STUDIES OF THE GALAXY PECULIAR VELOCITY FIELD by Philip Andrew James Astrophysics Group Blackett Laboratory Imperial College of Science, Technology and Medicine London SW7 2BZ A thesis submitted for the degree of Doctor of Philosophy of the University of London and for the Diploma of Imperial College November 1988 1 ABSTRACT This thesis describes two observational studies of the peculiar velocity field of galaxies over scales of 50-100 Jr1 Mpc, and the consequences of these measurements for cosmological theories. An introduction is given to observational cosmology, emphasising the crucial questions of the nature of the dark matter and the formation of structure. The principal cosmological models are discussed, and the role of observations in developing these models is stressed. Consideration is given to those observations that are likely to prove good discriminators between the competing models, particular emphasis being given to studies of the coherent velocities of samples of galaxies. The first new study presented here uses optical photometry and redshifts, from the literature, for First Ranked Cluster Galaxies (FRCG’s). These galaxies are excellent standard candles, and thus ideal for peculiar velocity studies. A simple one dimensional analysis detects no relative motion between the Local Group of galaxies and 60 FRCG’s with redshifts of up to 15000 kms-1. This is shown to imply a streaming motion of the cluster galaxies of at least 600 kms_1 relative to the CBR. The second observational study is a reanalysis of the Rubin et al. (1976a,b) sample of Sc galaxies. Near-IR photometry is used in our reanalysis to minimise the effects of extinction and to facilitate the use of luminosity indicators in reducing the effects of selection biases. -
Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur
Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur To cite this version: Alex Soumbatov-Gur. Phobos, Deimos: Formation and Evolution. [Research Report] Karpov institute of physical chemistry. 2019. hal-02147461 HAL Id: hal-02147461 https://hal.archives-ouvertes.fr/hal-02147461 Submitted on 4 Jun 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur The moons are confirmed to be ejected parts of Mars’ crust. After explosive throwing out as cone-like rocks they plastically evolved with density decays and materials transformations. Their expansion evolutions were accompanied by global ruptures and small scale rock ejections with concurrent crater formations. The scenario reconciles orbital and physical parameters of the moons. It coherently explains dozens of their properties including spectra, appearances, size differences, crater locations, fracture symmetries, orbits, evolution trends, geologic activity, Phobos’ grooves, mechanism of their origin, etc. The ejective approach is also discussed in the context of observational data on near-Earth asteroids, main belt asteroids Steins, Vesta, and Mars. The approach incorporates known fission mechanism of formation of miniature asteroids, logically accounts for its outliers, and naturally explains formations of small celestial bodies of various sizes. -
Active Source Seismology from Anthropogenic Sources During The
Active Source Seismology from Anthropogenic1 1 Sources2 During3 the4 Apollo 11 Lunar Mission A. S. Khatib , N. C. Schmerr , B. Feist , J. B. Plescia , N. E. Petro 1 [email protected], University of Maryland, College Park MD, 2 NASA Johnson Space Center, Houston TX, 3 Johns Hopkins University Applied Physics Laboratory, Baltimore MD, 4 NASA Goddard Space Flight Center, Greenbelt MD I. Introduction III. Spatial array V. Time correction The Passive Seismic Experiment Package (PSEP) deployed by The time-stamps on the seismic signal were generated upon the Apollo 11 astronauts Neil Armstrong and Buzz Aldrin during reception of the signal at base stations; seismic event times must their extravehicular activity (EVA) on July 21st, 1969 provided the take into account the radio wave travel time between generation first seismic data from another body in the Solar System [1,2]. The at Tranquility Base and the nearest receiving base station on Earth. primary sources of seismicity in the Apollo 11 seismic data were The travel times are calculated and subtracted from the event times. the movements and activities of the astronauts, ascent of the The time-stamps on the audio signal were generated upon Lunar Module (LM), and thermoelastic and volatile venting from reception of the signal at Mission Control in Houston; audio event the LM descent module. times must take into account the radio wave travel time between Here we use the anthropogenic sources of seismic signal from generation at Tranquility Base and the nearest receiving base station the movements of the astronauts on the surface to perform an on Earth, and the travel time between the base station and Houston. -
2018 Annual Convention
One Hundred Forty-First ANNUAL CONVENTION New Jersey State Firemen’s Association CONVENTION HALL Wildwood, New Jersey 2 0 September 14 & 15, 2018 1 8 NEW JERSEY STATE FIREMEN'S ASSOCIATION I FIRST SESSION Friday, September 14, 2018 – 1:00 P.M. Registration 9:30 A.M. to 12:30 P.M. ORDER OF BUSINESS 1. Call to Order by President Frank B. Gunson III 2. Invocation – Chaplain Dan Schafer 3. Presentation of Colors Wildwood City Fire Department Honor Guard - Cape May County Pledge of Allegiance to the Flag Vice President Robert F. Ordway National Anthem Firefighter Glenn D. Roemmich Note: All nouns and pronouns in the masculine gender shall be construed to include the female gender. 4. Reading of Call to Convention 5. Convention Committee Appointments Credential Committee Mr. Brian Van Hook Sergeant-at-Arms Mr. Belford Rivera Resolution Committee Mr. Frank P. Cavallo, Jr., Esquire Judge of Elections Mr. Stephen Fazekas 6. Introduction of Elected Officials: New Jersey Governor Wildwood Mayor Ernie Troiano, Jr. 7. Introduction of Wildwood Fire Department Chief Chief Daniel F. Speigel 8. Introduction of Guests and Executive Officers: John Siciliano Executive Director of Wildwood Convention Center Richard J. Mikutsky Director of Fire Safety Ronald Stokes President of New Jersey State Fire Chiefs’Association II NEW JERSEY STATE FIREMEN'S ASSOCIATION Wayne Welk, Vice President New Jersey Firemen’s Mutual Benevolent Association Elisa Fantozzi President of New Jersey State Exempt Firemen’s Association Richard J. Kosmoski President of New Jersey Volunteer Fire Chiefs Tom Campbell Director of Marketing, Deborah Heart and Lung Center 9. Report of Credential Committee Brian VanHook, Chairman 10. -
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. -
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. -
North Carolina Obituaries Courier Tribune Name Date of Paper Page # Date of Death Abbott, Blannie Allen 7-Aug-84 7A 6-Aug-84
North Carolina Obituaries Courier Tribune Name Date of Paper Page # Date of Death Abbott, Blannie Allen 7-Aug-84 7A 6-Aug-84 Abbott, Douglas L. 1-Sep-82 12A 30-Aug-82 Abbott, Helen Hartsook 3-Dec-82 9A 2-Dec-82 Abbott, Molly Jeane 3-Nov-81 8A 31-Oct-81 Abbott, Nora Johnson Mitchell 14-Oct-83 12A 13-Oct-83 Abbott, Roger 1-Aug-84 6A 31-Jul-84 Abercrombie, Dodd 5-Oct-80 6A 3-Oct-80 Abernathy, Ray Paul 29-Jun-80 8A 28-Jun-80 Abernathy, Shaun Travis 24-May-83 8A 24-May-83 Abrams, Reagan Vincent 28-Sep-80 6A 26-Sep-80 Abston, Thomas Earl 30-Dec-82 10A 29-Dec-82 Ackerman, Elsie K. 20-Apr-82 8A 19-Apr-82 Acree, Una Mae Phillips 6-Jul-81 6A 5-Jul-81 Adams, Anna Threadgill 9-Dec-85 9A 8-Dec-85 Adams, Annie Vaughn 12-Mar-85 6A 11-Mar-85 Adams, Bernice Hooper 6-Jul-82 8A 5-Jul-82 Adams, Dora Carrick 13-Jun-80 10A 12-Jun-80 Adams, Edward Vance 23-May-83 6A 23-May-83 Adams, Herman Hugh Sr. 29-Oct-81 8A 27-Oct-81 Adams, James Clifton 18-Sep-84 9A 17-Sep-84 Adams, John Edwin 1-Mar-84 10A 29-Feb-84 Adams, T.B. 15-Oct-82 10A 14-Oct-82 Adams, Velma D. 11-Aug-81 8A 10-Aug-81 Adcock, Plackard C. 6-Jul-82 8A 5-Jul-82 Aderholt, Daniel H. 17-May-85 10A 13-May-85 Adkins, Clarence Odell 1-Jan-85 7A 1-Jan-85 Adkins, E.G. -
Alexandre Amorim -.:: GEOCITIES.Ws
Alexandre Amorim (org) 2 3 PREFÁCIO O Boletim Observe! é uma iniciativa da Coordenação de Observação Astronômica do Núcleo de Estudo e Observação Astronômica “José Brazilício de Souza” (NEOA-JBS). Durante a reunião administrativa do NEOA-JBS em maio de 2010 foi apresentada a edição de Junho de 2010 para apreciação dos demais coordenadores do Núcleo onde houve aprovação unânime em usar o Boletim Observe! como veículo de informação das atividades e, principalmente, observações astronômicas. O Boletim Observe! é publicado mensalmente em formato eletrônico ou impresso separadamente, prezando pela simplicidade das informações e encorajando os leitores a observar, registrar e publicar os eventos astronômicos. Desde a sua primeira edição o Boletim Observe! conta com a colaboração espontânea de diversos astrônomos amadores e profissionais. Toda edição do Observe! do mês de dezembro é publicado um índice dos artigos do respectivo ano. Porém, desde aquela edição de Junho de 2010 foram publicados centenas de artigos e faz-se necessário consultar assuntos que foram tratados nas edições anteriores do Observe! e seus respectivos autores. Para isso publicaremos anualmente esse Índice de Assuntos, permitindo a consulta rápida dos temas abordados. Florianópolis, 1º de dezembro de 2018 Alexandre Amorim Coordenação de Observação Astronômica do NEOA-JBS 4 Ano I (2010) Nº 1 – Junho 2010 Eclipse da Lua em 26 de junho de 2010 Amorim, A. Júpiter sem a Banda Equatorial Sul Amorim, A. Conjunção entre Júpiter e Urano Amorim, A. Causos do Avelino Alves, A. A. Quem foi Eugênia de Bessa? Amorim, A. Nº 2 – Julho 2010 Aprendendo a dimensionar as distâncias angulares no céu Neves, M.