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I N S I D E T H I S I S S
Publications and Products of August/août 2003 Volume/volume 97 Number/numéro 4 [701] The Royal Astronomical Society of Canada Observer’s Calendar — 2004 This calendar was created by members of the RASC. All photographs were taken by amateur astronomers using ordinary camera lenses and small telescopes and represent a wide spectrum of objects. An informative caption accompanies every photograph. It is designed with the observer in mind and contains comprehensive The Journal of the Royal Astronomical Society of Canada Le Journal de la Société royale d’astronomie du Canada astronomical data such as daily Moon rise and set times, significant lunar and planetary conjunctions, eclipses, and meteor showers. The 1998, 1999, and 2000 editions each won the Best Calendar Award from the Ontario Printing and Imaging Association (designed and produced by Rajiv Gupta). Individual Order Prices: $16.95 CDN (members); $19.95 CDN (non-members) $14.95 USD (members); $17.95 USD (non-members) (includes postage and handling; add GST for Canadian orders) The Beginner’s Observing Guide This guide is for anyone with little or no experience in observing the night sky. Large, easy to read star maps are provided to acquaint the reader with the constellations and bright stars. Basic information on observing the Moon, planets and eclipses through the year 2005 is provided. There is also a special section to help Scouts, Cubs, Guides, and Brownies achieve their respective astronomy badges. Written by Leo Enright (160 pages of information in a soft-cover book with otabinding that allows the book to lie flat). Price: $15 (includes taxes, postage and handling) Skyways: Astronomy Handbook for Teachers Teaching Astronomy? Skyways Makes it Easy! Written by a Canadian for Canadian teachers and astronomy educators, Skyways is: Canadian curriculum-specific; pre-tested by Canadian teachers; hands-on; interactive; geared for upper elementary; middle school; and junior high grades; fun and easy to use; cost-effective. -
9Th Grade Ela
9TH GRADE ELA Week of: MAY 11TH WICHITA PUBLIC SCHOOLS 9th, 10th, 11th and 12th Grades Your child should spend up to 90 minutes over the course of each day on this packet. Consider other family-friendly activities during the day such as: Learn how to do laundry. Create a cartoon image Make a bucket list of Look up riddles to Wash the laundry, of your family. things to do after the solve with someone fold and put the quarantine is over with in your family. laundry away. your family. Mindful Minute: Write Do a random act of Teach someone in your Put together a puzzle down what a typical day kindness for someone in family to play one of your with your family. was like pre-quarantine your house. video games. and during quarantine. How have things changed? *All activities are optional. Parents/Guardians please practice responsibility, safety, and supervision. For students with an Individualized Education Program (IEP) who need additional support, Parents/Guardians can refer to the Specialized Instruction and Supports webpage, contact their child’s IEP manager, and/or speak to the special education provider when you are contacted by them. Contact the IEP manager by emailing them directly or by contacting the school. The Specialized Instruction and Supports webpage can be accessed by clicking HERE or by navigating in a web browser to https://www.usd259.org/Page/17540 WICHITA PUBLIC SCHOOLS CONTINUOUS LEARNING HOTLINE AVAILABLE 316-973-4443 MARCH 30 – MAY 21, 2020 MONDAY – FRIDAY 11:00 AM – 1:00 PM ONLY For Multilingual Education Services (MES) support, please call (316) 866-8000 (Spanish and Proprio) or (316) 866-8003 (Vietnamese). -
Geomorphology, Stratigraphy, and Paleohydrology of the Aeolis Dorsa Region, Mars, with Insights from Modern and Ancient Terrestrial Analogs
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 12-2016 Geomorphology, Stratigraphy, and Paleohydrology of the Aeolis Dorsa region, Mars, with Insights from Modern and Ancient Terrestrial Analogs Robert Eric Jacobsen II University of Tennessee, Knoxville, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Part of the Geology Commons Recommended Citation Jacobsen, Robert Eric II, "Geomorphology, Stratigraphy, and Paleohydrology of the Aeolis Dorsa region, Mars, with Insights from Modern and Ancient Terrestrial Analogs. " PhD diss., University of Tennessee, 2016. https://trace.tennessee.edu/utk_graddiss/4098 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Robert Eric Jacobsen II entitled "Geomorphology, Stratigraphy, and Paleohydrology of the Aeolis Dorsa region, Mars, with Insights from Modern and Ancient Terrestrial Analogs." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Devon M. Burr, -
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. -
The Creative Process
The Creative Process THE SEARCH FOR AN AUDIO-VISUAL LANGUAGE AND STRUCTURE SECOND EDITION by John Howard Lawson Preface by Jay Leyda dol HILL AND WANG • NEW YORK www.johnhowardlawson.com Copyright © 1964, 1967 by John Howard Lawson All rights reserved Library of Congress catalog card number: 67-26852 Manufactured in the United States of America First edition September 1964 Second edition November 1967 www.johnhowardlawson.com To the Association of Film Makers of the U.S.S.R. and all its members, whose proud traditions and present achievements have been an inspiration in the preparation of this book www.johnhowardlawson.com Preface The masters of cinema moved at a leisurely pace, enjoyed giving generalized instruction, and loved to abandon themselves to reminis cence. They made it clear that they possessed certain magical secrets of their profession, but they mentioned them evasively. Now and then they made lofty artistic pronouncements, but they showed a more sincere interest in anecdotes about scenarios that were written on a cuff during a gay supper.... This might well be a description of Hollywood during any period of its cultivated silence on the matter of film-making. Actually, it is Leningrad in 1924, described by Grigori Kozintsev in his memoirs.1 It is so seldom that we are allowed to study the disclosures of a Hollywood film-maker about his medium that I cannot recall the last instance that preceded John Howard Lawson's book. There is no dearth of books about Hollywood, but when did any other book come from there that takes such articulate pride in the art that is-or was-made there? I have never understood exactly why the makers of American films felt it necessary to hide their methods and aims under blankets of coyness and anecdotes, the one as impenetrable as the other. -
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 -
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center a for Rockets and Satellites
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center A For Rockets and Satellites {NASA-TM-79399) LHNAS TRANSI]_INT PHENOMENA N78-301 _7 CATAI_CG (NASA) 109 p HC AO6/MF A01 CSCl 22_ Unc.las G3 5 29842 NSSDC/WDC-A-R&S 78-03 Lunar Transient Phenomena Catalog Winifred Sawtell Cameron July 1978 National Space Science Data Center (NSSDC)/ World Data Center A for Rockets and Satellites (WDC-A-R&S) National Aeronautics and Space Administration Goddard Space Flight Center Greenbelt) Maryland 20771 CONTENTS Page INTRODUCTION ................................................... 1 SOURCES AND REFERENCES ......................................... 7 APPENDIX REFERENCES ............................................ 9 LUNAR TRANSIENT PHENOMENA .. .................................... 21 iii INTRODUCTION This catalog, which has been in preparation for publishing for many years is being offered as a preliminary one. It was intended to be automated and printed out but this form was going to be delayed for a year or more so the catalog part has been typed instead. Lunar transient phenomena have been observed for almost 1 1/2 millenia, both by the naked eye and telescopic aid. The author has been collecting these reports from the literature and personal communications for the past 17 years. It has resulted in a listing of 1468 reports representing only slight searching of the literature and probably only a fraction of the number of anomalies actually seen. The phenomena are unusual instances of temporary changes seen by observers that they reported in journals, books, and other literature. Therefore, although it seems we may be able to suggest possible aberrations as the causes of some or many of the phenomena it is presumptuous of us to think that these observers, long time students of the moon, were not aware of most of them. -
Geologic Map of the Source Region of Shalbatana Vallis, Mars
Geologic Map of the Source Region of Shalbatana Vallis, Mars Dan Berman, Cathy Weitz, Alexis Rodriguez, and David Crown Planetary Mappers Meeting Flagstaff, AZ June 12-13, 2017 Introduction •We are currently producing a 1:500,000-scale USGS geologic map of MTM quadrangles 00042 and 00047 in the Xanthe Terra region of Mars (2.5°S - 2.5°N, 310° - 320°E). The map region has been extensively modified by outflow channels and chaotic terrains and contains cratered plains deformed by subsidence. Mapping is being conducted on a THEMIS IR daytime base mosaic, with CTX and HiRISE images as supplements where available. •The overarching goal of this project is to develop an understanding of how regionally integrated hydrologic systems have been affected by (1) impact crater formation, (2) melting of subsurface ice leading to the generation of subsurface cavity space and then subsidence, and (3) erosional and depositional flooding events of various types and ages. Chryse Planitia Kasei Vallis Simud Vallis Tiu Maja Vallis Vallis Chryse Chaos Ares Vallis Shalbatana Xanthe Vallis Terra Hydraotes Chaos Ganges Chasma Description of Map Units Plains Units •cratered plains 1 – smooth to mottled, heavily cratered plains marked by secondary chains, wrinkle ridges, and zones of incipient collapse. Ejecta of many large craters entirely or partly eroded •cratered plains 2 – similar to cratered plains 1, with dark signature in THEMIS day IR (bright in night IR) and some knobs Crater Units •crater material – crater ejecta, rim, and floor materials •crater fill material -
The Best for 2010
ＩＳＳＮ ０９１７－７３８８ COMMUNICATIONS IN 東亞天文學會『火星通信』since 1986 MARS No.366 10 January 2010 OBSERVATIONS Published by the OAA Mars Section AllAll the the Best Best for for 2010 2010 CMO Editors T ASADA, M MINAMI, M MURAKAMI T NAKAJIMA, A NISHITA Forthcoming 2009/2010 Mars (11) WhyandHowDoWeObservethePlanetMars?I Masatsugu MINAMI 南政次(Mn) We suppose no astronomer forgets a special red andusuallyrotatedaroundtheSun,thehistoryof star which shined brilliantly and largely in the sky the laws of motion must have changed. in2003.Alotofpeoplewereawareofthefactand Mars continued also as a mysterious star even after knew it was the planet Mars, the same star that the telescope was invented, even after it gradually enchanted and puzzled the people from the ancient became bigger and bigger. Ever since Huygens re‐ times. It apparently moved around among the con‐ vealed Syrtis Mj, the markings on the surface of the stellations in a complex manner in some seasons. So planet almost have been known that they could stay 熒惑 in the old China it was called “ ”whoseletters stable just like seas and lands and could be an ob‐ imply uncanny and fascinated at the same time. It ject of the attractive scientific stories. Almost all was also a strange thing since the great bright red stories surrounding Mars were turned out to be star visited every fifteen or seventeen years. It was negative (just before the 1909 revelation), but we thus so intrinsically to give rise to several stories may say any true science cannot reach straightfor‐ which looked beyond human knowledge. wardly its true goal: Rather the deep science expe‐ On the other hand this strange star also continued riences a zigzagged way and rather the great sci‐ to give us a lot of hints to our scientific minds. -
R. M. E. Williams, 2017, Shaler: a Fluvial Sedimentary Deposit on Mars, Sedimentology
Rebecca M. (Eby) Williams Planetary Science Institute (p) 608-729-7786 (e) [email protected] Education: PhD., 2000, Planetary Sciences, Washington University, St. Louis, MO B.A., 1995, Cum Laude, Physics and Geology, Franklin & Marshall College, Lancaster, PA Relevant Work History: Planetary Science Institute, Tucson, AZ 2011-Present Senior Scientist 2005-2010 Research Scientist Smithsonian Institution, Center for Earth and Planetary Science, Washington, DC 2004-2006 Research Associate, Lindbergh Fellow Malin Space Science Systems, Inc., San Diego, CA 2002-2004 Staff Scientist 2001-2002 Post-Doctoral Research Associate Awards & Service: 2006 NASA Carl Sagan Fellowship for Early Career Researchers 2011 MRO CTX Science Team NASA Group Achievement Award 2013 MSL Science Office Development and Operations Team, NASA Group Achievement Award 2013-Present ESA ExoMars Landing Site Selection Working Group (LSSWG) Member 2015 NASA Next Orbiter to Mars Science Advisory Group (NEX-SAG) Member 2015 MSL Prime Mission Science and Operations Team, NASA Group Achievement Award 2017 Friend of Education, Waunakee Teachers Association Field Experience: Deltas in Patagonia, Chile, PI, November 2018. Inverted paleochannels & alluvial fans, Pampa del Tamarugal region, Atacama Desert, Chile, PI, Nov 2010, June 2012, May 2016, Nov. 2017. Inverted paleochannels, Ebro Basin, Spain, Co-I, Feb. 2017 (PI Michael Lamb). Rover operations testing, Co-I, near Vernal, UT, Oct. 2017; Green River, UT, April 2016 (GeoHeuristic Operational Strategies Testing, GHOST, PI Aileen Yingst). Inverted paleochannels near Baker, CA, PI, Sep 2014, April 2016. Inverted paleochannels near Cadney, South Australia, PI, May 2011. Meandering channels of the Quinn River, Nevada, Co-I, July 2010, Oct. 2011. Inverted paleochannels, Cape York Peninsula, Queensland, Australia, PI, July 2009. -
Journal of the Association of Lunar & Planetary Observers
ISSN-0039-2502 Journal of the Association of Lunar & Planetary Observers The Strolling Astronomer Volume 45, Number 1, Winter 2003 Now in Portable Document Format (PDF) for MacIntosh and PC-Compatible Computers Inside...Inside...Inside... More on lunar domes While not the subject of this month’s dome study, we present here a view of lunar dome Mons Gruithuisen Delta (named for Franz von Paul Gruithuisen, a German physician-turned- astronomer) taken from an orbiting Apollo spacecraft. See page 12 for details. • Also . * An ALPO project team to study Saturn’s rings * Isophotes of the Sun * Getting ready for the upcoming Mercury/Venus transits * Getting ready for the Mars apparition * Jupiter and Saturn apparition reports Cover Graphic: John Sanford . plus reports about your ALPO section activities and much, much more. THE ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS (ALPO) P.O. Box 13456, Springfield, Illinois 62791-3456 U.S.A. Thank you for your interest in our organization. The Association of Lunar and Planetary Observers (ALPO) was founded by Walter H. Haas in 1947, and incorporated in 1990, as a medium for advancing and conducting astronomical work by both profes- sional and amateur astronomers who share an interest in Solar System observations. We welcome and provide services for all indi- viduals interested in lunar and planetary astronomy. For the novice observer, the ALPO is a place to learn and to enhance observational techniques. For the advanced amateur astronomer, it is a place where one's work will count. For the professional astronomer, it is a resource where group studies or systematic observing patrols add to the advancement of astronomy.