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Aerospace Dimensions Leader's Guide
Leader Guide www.capmembers.com/ae Leader Guide for Aerospace Dimensions 2011 Published by National Headquarters Civil Air Patrol Aerospace Education Maxwell AFB, Alabama 3 LEADER GUIDES for AEROSPACE DIMENSIONS INTRODUCTION A Leader Guide has been provided for every lesson in each of the Aerospace Dimensions’ modules. These guides suggest possible ways of presenting the aerospace material and are for the leader’s use. Whether you are a classroom teacher or an Aerospace Education Officer leading the CAP squadron, how you use these guides is up to you. You may know of different and better methods for presenting the Aerospace Dimensions’ lessons, so please don’t hesitate to teach the lesson in a manner that works best for you. However, please consider covering the lesson outcomes since they represent important knowledge we would like the students and cadets to possess after they have finished the lesson. Aerospace Dimensions encourages hands-on participation, and we have included several hands-on activities with each of the modules. We hope you will consider allowing your students or cadets to participate in some of these educational activities. These activities will reinforce your lessons and help you accomplish your lesson out- comes. Additionally, the activities are fun and will encourage teamwork and participation among the students and cadets. Many of the hands-on activities are inexpensive to use and the materials are easy to acquire. The length of time needed to perform the activities varies from 15 minutes to 60 minutes or more. Depending on how much time you have for an activity, you should be able to find an activity that fits your schedule. -
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. -
Building Cold War Warriors: Socialization of the Final Cold War Generation
BUILDING COLD WAR WARRIORS: SOCIALIZATION OF THE FINAL COLD WAR GENERATION Steven Robert Bellavia A Dissertation Submitted to the Graduate College of Bowling Green State University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY May 2018 Committee: Andrew M. Schocket, Advisor Karen B. Guzzo Graduate Faculty Representative Benjamin P. Greene Rebecca J. Mancuso © 2018 Steven Robert Bellavia All Rights Reserved iii ABSTRACT Andrew Schocket, Advisor This dissertation examines the experiences of the final Cold War generation. I define this cohort as a subset of Generation X born between 1965 and 1971. The primary focus of this dissertation is to study the ways this cohort interacted with the three messages found embedded within the Cold War us vs. them binary. These messages included an emphasis on American exceptionalism, a manufactured and heightened fear of World War III, as well as the othering of the Soviet Union and its people. I begin the dissertation in the 1970s, - during the period of détente- where I examine the cohort’s experiences in elementary school. There they learned who was important within the American mythos and the rituals associated with being an American. This is followed by an examination of 1976’s bicentennial celebration, which focuses on not only the planning for the celebration but also specific events designed to fulfill the two prime directives of the celebration. As the 1980s came around not only did the Cold War change but also the cohort entered high school. Within this stage of this cohorts education, where I focus on the textbooks used by the cohort and the ways these textbooks reinforced notions of patriotism and being an American citizen. -
Commercial Lunar Propellant Architecture a Collaborative Study of Lunar Propellant Production
Commercial Lunar Propellant Architecture A Collaborative Study of Lunar Propellant Production 1 To the Memory of: Dr. Paul D. Spudis (1952–2018) Dr. Spudis earned his master’s degree from Brown University and his Ph.D. from Arizona State University in Geology with a focus on the Moon. His career included work at the US Geological Survey, NASA, John Hopkins University Applied Physics Laboratory, and the Lunar and Planetary Institute advocating for the exploration and the utilization of lunar resources. His work will continue to inspire and guide us all on our journey to the Moon. “By going to the Moon we can learn how to extract what we need in space from what we find in space. Fundamentally that is a skill that any spacefaring civilization has to master. If you can learn to do that, you’ve got a skill that will allow you to go to Mars and beyond.” ii Authors David Kornuta, United Launch Alliance, CisLunar Project Lead1 Angel Abbud-Madrid, Colorado School of Mines, Professor of Space Resources Jared Atkinson, Honeybee Robotics, Senior Geophysical Engineer Jonathan Barr, United Launch Alliance, Program Manager Gary Barnhard, Xtraordinary Innovative Space Partnership, CEO Dallas Bienhoff, Cislunar Space Development Company LLC, Founder Brad Blair, NewSpace Analytics, Managing Partner Vanessa Clark, Atomos Nuclear and Space, Chief Executive and Technology Officer Justin Cyrus, Lunar Outpost, CEO Blair DeWitt, Lunar Station Corporation, CEO and Co-Founder Chris Dreyer, Colorado School of Mines, Professor of Space Resources Barry Finger, Paragon -
Washington University Record, October 6, 1994
Washington University School of Medicine Digital Commons@Becker Washington University Record Washington University Publications 10-6-1994 Washington University Record, October 6, 1994 Follow this and additional works at: http://digitalcommons.wustl.edu/record Recommended Citation "Washington University Record, October 6, 1994" (1994). Washington University Record. Book 666. http://digitalcommons.wustl.edu/record/666 This Article is brought to you for free and open access by the Washington University Publications at Digital Commons@Becker. It has been accepted for inclusion in Washington University Record by an authorized administrator of Digital Commons@Becker. For more information, please contact [email protected]. ZCT8 «0N XP9 NVWdAO>l V130WVS sw WASHINGTON UNIVERSITY IN ST. LOUIS Vol. 19 No. 7 Oct. 6, 1994 Historic grant bolsters science education Washington University is one of 62 directs the Washington University Under- areas as protein biochemistry, DNA manip- Howard Hughes Medical Institute," said U.S. universities to receive a graduate Biological Sciences Education ulation, and microbial genetics, and com- Chancellor William H. Danforth. "This portion of $86 million from the Program. The University also was awarded puters for simulations and modeling. support helps bring the excitement of Howard Hughes Medical Institute (HHMI) a five-year grant of $1.7 million as part of The program is the largest of several research and discovery to students of all to improve the quality of science education the program in 1992. HHMI initiatives to improve science educa- ages, and it gives our faculty the opportu- for American students. Washington University will use the tion from elementary school through nity to work with elementary and second- The $86 million represents the largest grant to support: postgraduate training. -
Psychology of Space Exploration Psychology of About the Book Douglas A
About the Editor Contemporary Research in Historical Perspective Psychology of Space Exploration Psychology of About the Book Douglas A. Vakoch is a professor in the Department As we stand poised on the verge of a new era of of Clinical Psychology at the California Institute of spaceflight, we must rethink every element, including Integral Studies, as well as the director of Interstellar Space Exploration the human dimension. This book explores some of the Message Composition at the SETI Institute. Dr. Vakoch Contemporary Research in Historical Perspective contributions of psychology to yesterday’s great space is a licensed psychologist in the state of California, and Edited by Douglas A. Vakoch race, today’s orbiter and International Space Station mis- his psychological research, clinical, and teaching interests sions, and tomorrow’s journeys beyond Earth’s orbit. include topics in psychotherapy, ecopsychology, and meth- Early missions into space were typically brief, and crews odologies of psychological research. As a corresponding were small, often drawn from a single nation. As an member of the International Academy of Astronautics, intensely competitive space race has given way to inter- Dr. Vakoch chairs that organization’s Study Groups on national cooperation over the decades, the challenges of Interstellar Message Construction and Active SETI. communicating across cultural boundaries and dealing Through his membership in the International Institute with interpersonal conflicts have become increasingly of Space Law, he examines -
4. Lunar Architecture
4. Lunar Architecture 4.1 Summary and Recommendations As defined by the Exploration Systems Architecture Study (ESAS), the lunar architecture is a combination of the lunar “mission mode,” the assignment of functionality to flight elements, and the definition of the activities to be performed on the lunar surface. The trade space for the lunar “mission mode,” or approach to performing the crewed lunar missions, was limited to the cislunar space and Earth-orbital staging locations, the lunar surface activities duration and location, and the lunar abort/return strategies. The lunar mission mode analysis is detailed in Section 4.2, Lunar Mission Mode. Surface activities, including those performed on sortie- and outpost-duration missions, are detailed in Section 4.3, Lunar Surface Activities, along with a discussion of the deployment of the outpost itself. The mission mode analysis was built around a matrix of lunar- and Earth-staging nodes. Lunar-staging locations initially considered included the Earth-Moon L1 libration point, Low Lunar Orbit (LLO), and the lunar surface. Earth-orbital staging locations considered included due-east Low Earth Orbits (LEOs), higher-inclination International Space Station (ISS) orbits, and raised apogee High Earth Orbits (HEOs). Cases that lack staging nodes (i.e., “direct” missions) in space and at Earth were also considered. This study addressed lunar surface duration and location variables (including latitude, longi- tude, and surface stay-time) and made an effort to preserve the option for full global landing site access. Abort strategies were also considered from the lunar vicinity. “Anytime return” from the lunar surface is a desirable option that was analyzed along with options for orbital and surface loiter. -
Surveyor 1 Space- Craft on June 2, 1966 As Seen by the Narrow Angle Camera of the Lunar Re- Connaissance Orbiter Taken on July 17, 2009 (Also See Fig
i “Project Surveyor, in particular, removed any doubt that it was possible for Americans to land on the Moon and explore its surface.” — Harrison H. Schmitt, Apollo 17 Scientist-Astronaut ii Frontispiece: Landing site of the Surveyor 1 space- craft on June 2, 1966 as seen by the narrow angle camera of the Lunar Re- connaissance Orbiter taken on July 17, 2009 (also see Fig. 13). The white square in the upper photo outlines the area of the enlarged view below. The spacecraft is ca. 3.3 m tall and is casting a 15 m shadow to the East. (NASA/LROC/ ASU/GSFC photos) iii iv Surveyor I: America’s First Moon Landing by William F. Mellberg v © 2014, 2015 William F. Mellberg vi About the author: William Mellberg was a marketing and public relations representative with Fokker Aircraft. He is also an aerospace historian, having published many articles on both the development of airplanes and space vehicles in various magazines. He is the author of Famous Airliners and Moon Missions. He also serves as co-Editor of Harrison H. Schmitt’s website: http://americasuncommonsense.com Acknowledgments: The support and recollections of Frank Mellberg, Harrison Schmitt, Justin Rennilson, Alexander Gurshstein, Paul Spudis, Ronald Wells, Colin Mackellar and Dwight Steven- Boniecki is gratefully acknowledged. vii Surveyor I: America’s First Moon Landing by William F. Mellberg A Journey of 250,000 Miles . December 14, 2013. China’s Chang’e 3 spacecraft successfully touched down on the Moon at 1311 GMT (2111 Beijing Time). The landing site was in Mare Imbrium, the Sea of Rains, about 25 miles (40 km) south of the small crater, Laplace F, and roughly 100 miles (160 km) east of its original target in Sinus Iridum, the Bay of Rainbows. -
Pm AGENCY Office of Education (DREW), Washington, P
itOCUITT RESUME 2-45t 95 . - ,RC 010 425 .. UTROR' Niatuw, Duane; Rickman, Uncle TITLE The. History and Culture of the'Indiand of Wilahington State ---A curriculua'GuiAer..Revised 1975. ,INmpUTION Washington Office of the State Superintendent of .' Public Instruction, Olympia.; Washington Univ., v .1 . 'Seattle. Coll. of Edication. , ;pm AGENCY Office of Education (DREW), Washington, p. C. r 08-,DATE . 75' Lima -------,_ 248p.: - BOBS PRICE HF-$0443-7801.414.71 Plus POstage. " -DESCRIPTORS Activities; fAmericarLindians; Audioviival lids; *Bibliographies; Cat:mad-inn-Concept Formation; Conflict; *Cultural Awareness; CuTttialBackground. Cultural Differences; *CurriCulumOuideal-iducat4onal Objectives; *Elementary 'Secondary- Education;. Enrichment; Futures (of Society) * 'History; Instructional Materials: InterdiLiplOau Approach:. / Organizations (Groups); Problems; *Reionice ., Haterfals; Social Change; Students; Teachers IDENTIF*S' *Washington -,,,. 'AB4T4CT - 0 social. Designed to be utilized as a supplementtar,,, studies crr culum (any level) .in-the public schodlgirofAiasking,ton thiscurricula*,- guide on: the histOry 4AWc4tt#4 of . ..- 4t4te. ... NAshington's American Indians includes; ailindez; a 0.14-00-;#04ia . , guide;-a guide to teaching materialetsauath0-2, .., resource ._..., -_,,,......- -, ,study,itself. The content of the course of St04200#441'6 ;:thee .: 11#10 4;eisearlii life of the Indians ofilvall#00,01*4,the::,. NMshington Indians! encounter with non 4andiane;,04-0400,0 ,,, .InAians of Washington. The subject patter iso.0#4110kiii*OePt P ' A4'n'Of'Socialissuesand is developedbysielliWWCO:i01041. '. ,,,f ,4ener4imationS, and values derived from all at 00,:4140(science dirge 04Ines;specific objectives and actAvitieg:4Sik 4414- c -60d. e:)14.1liggraphy/resources section inclu400: 40040, l is: ,; mt. ipii; gases: newspapers and journ4s1 twOotdM, MOta 'Wit organizations and institutions; U.S. -
The Tsiolkovskiy Crater Landslide, the Moon: an LROC View
Icarus 337 (2020) 113464 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus The Tsiolkovskiy crater landslide, the moon: An LROC view Joseph M. Boyce a,*, Peter Mouginis-Mark a, Mark Robinson b a Hawaii Institute for Geophysics and Planetology, University of Hawaii, Honolulu 96822, USA b School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85281, USA ARTICLE INFO ABSTRACT Keywords: Evidence suggests that the lobate flow feature that extends ~72 km outward from the western rim of Tsiol Moon surface kovskiy crater is a long runout landslide. This landslide exhibits three (possibly four) morphologically different Landslides parts, likely caused by local conditions. All of these, plus the ejecta of Tsiolkovskiy crater, and its mare fill are Impact processes approximately of the same crater model age, i.e., ~3.55 � 0.1 Ga. The enormous size of this landslide is unique Geological processes on the Moon and is a result of a combination of several geometric factors (e.g., its location relative to Fermi Terrestrial planets crater), and that Tsiolkovskiy crater was an oblique impact that produced an ejecta forbidden zone on its western side (Schultz, 1976). The landslide formed in this ejecta free zone as the rim of Tsiolkovskiy collapsed and its debris flowedacross the relatively smooth, flatfloor of Fermi crater. In this location, it could be easily identified as a landslide and not ejecta. Its mobility and coefficientof friction are similar to landslides in Valles Marineris on Mars, but less than wet or even dry terrestrial natural flows.This suggests that the Mars landslides may have been emplaced dry. -
Concept of a Human-Attended Lunar Outpost
Paper ID #16714 Concept of a Human-Attended Lunar Outpost Mr. Thomas W. Arrington, Texas A&M University Thomas Arrington worked as the student Project Manager for the Human Attended Lunar Outpost senior design project for the the Department of Aerospace Engineering at Texas A&M University in College Station. He has interned with Boeing Research and Technology three times, and was an active member of the Texas A&M University Sounding Rocketry Team. Mr. Nicolas Federico Hurst, Texas A&M 2015 Capstone Design Spacecraft Nico Hurst is a student of Texas A&M University. He recently graduated from the Aerospace Engineering department with my bachelor’s of science and will be continuing his education with a master’s of science in finance. Mr. David B. Kanipe, Texas A&M University After receiving a BS in Aerospace Engineering in May 1970, followed by a MS in Aerospace Engineering in August 1971 from Texas A&M University, Mr. Kanipe accepted a position with NASA at the Manned Spacecraft Center in Houston and began his professional career in November 1972. A month after his arrival at NASA, the last Apollo mission, Apollo 17, was launched. Obviously, that was exciting, but in terms of his career, the commencement of the Space Shuttle Program in November 1972 was to have far more impact. As a result, David was able to begin his career working on what he says was the most interesting and exciting project he could possibly imagine: the Space Shuttle. Over his career, David held successively influential management positions including Deputy Branch Chief of the Aerodynamics Branch in the Aeroscience and Flight Mechanics Division, Chief of the GN&C Analysis and Design Branch, Deputy Chief of the Aeroscience and Flight Mechanics Division, and for the final 10 years of his career, Chief of the Aeroscience and Flight Mechanics Division in the Engineering Directorate at the Johnson Space Center. -
Origin of the Anomalously Rocky Appearance of Tsiolkovskiy Crater
Icarus 273 (2016) 237–247 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Origin of the anomalously rocky appearance of Tsiolkovskiy crater ∗ Benjamin T. Greenhagen a, , Catherine D. Neish b, Jean-Pierre Williams c, Joshua T.S. Cahill a, Rebecca R. Ghent d,e,PaulO. Hayne f, Samuel J. Lawrence g,NoahE. Petro h, Joshua L. Bandfield i a Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099, United States b Department of Earth Sciences, Western University Biological & Geological Sciences Building, Room 1026 1151 Richmond St. N. London, ON N6A 5B7 Canada c Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles 595 Charles Young Drive East, Box 951567 Los Angeles, CA 90095-1567, United States d Department of Earth Sciences, Earth Sciences Centre 22 Russell Street Toronto, Ontario, M5S 3B1, Canada e Planetary Science Institute, 1700 East Fort Lowell, Suite 106 Tucson, AZ 85719-2395, United States f Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive Pasadena, CA 91109 ASU, United States g School of Earth and Space Exploration, PO Box 871404 Tempe, AZ 85287-1404, United States h NASA’s Goddard Space Flight Center, 8800 Greenbelt Rd Greenbelt, MD 20771, United States i Space Science Institute, 4750 Walnut Street | Suite 205 Boulder, Colorado 80301, United States a r t i c l e i n f o a b s t r a c t Article history: Rock abundance maps derived from the Diviner Lunar Radiometer instrument on the Lunar Reconnais- Received 3 August 2015 sance Orbiter (LRO) show Tsiolkovskiy crater to have high surface rock abundance and relatively low re- Revised 6 February 2016 golith thickness.