Jacobs KSC Activity Book

Total Page:16

File Type:pdf, Size:1020Kb

Jacobs KSC Activity Book AMAZING SPACE Artemis Generation Activity Book SPACE LAUNCH SYSTEM (SLS) ISS International Space Station Orion Crew Capsule Will carry astronauts Mobile Launcher 380 feet tall SLS Rocket VAB Vehicle Assembly Building Crawler Transporter-2 Travels at 1 mile per hour SPACE MAZE MILKY WAY SCRAMBLE 9 UENPNET 7 EMRURCY 10 HRATE 8 VNEUS EJUTPIR 5 AUNTSR 4 ARSUUN 1 USN 11 6 MRAS 3 OUTLP 2 OMON 1 2 3 4 5 6 7 8 9 10 11 Unscramble the letters to find the names of the planets in our Solar System. Then use the code to find the hidden phrase! Answers on last page THE PLANETS 1 2 3 4 5 6 7 8 9 Across: 1. Begins with V 3. Begins with P 6. Begins with U 8. Begins with E 9. Begins with M Down: 2. Begins with N 4. Begins with J 5. Begins with M 7. Begins with S Answers on last page WORD SEARCH s s o t h s m o o n p t t m a r s c g c l d a d l t r o a s a s n r e e a m l u n u t k h u n e a n e n c l e n u t x e t o r b i t l l y v r x h t r a e u c t o t u l p s p a c e comet planet earth pluto galaxy rocket lunar space mars star moon sun orbit venus SOLAR SYSTEM CROSSWORD 6 7 1 2 8 3 4 5 9 Across: 1. The star at the center of the Solar System 2. This blue planet is officially the weirdest: it smells like rotten eggs due to hydrogen sulfide, instead of spinning like a top it lays on it’s side, and it’s the coldest. 3. The smallest planet and closest planet to the sun. 4. The only planet that has liquid water on its surface. 5. This planet was named after the Roman god of the sea. Down: 3. The red planet. 6. This planet has more than 50 moons. 7. This planet’s many rings are made up of millions of ice crystals. 8. The brightest planet in the Solar System. 9. This former planet is now a dwarf planet. Answers on last page ROCKET MAZE Outer Space Launch THE SPACE RACE 7 1 8 2 9 3 10 4 5 6 Across: 1. Our home planet, Mother __________ 2. The galaxy that contains our Solar System 3. The ringless, dwarf planet 4. The second planet from the sun and is named after the roman goddess of love 5. Space Launch System (acronym) 6. Vehicle Assembly Building (acronym) Down: 2. Jupiter has more than 50 of these 5. The sun is a _________ in the center of the Solar System 7. The ____________-transporter transports rockets to Launch Pad 39B 8. Mobile Launch Platform (acronym) 9. We are go for ___________! 10. Kennedy Space Center (acronym) Answers on next page ANSWER KEY MILKY WAY SCRAMBLE THE PLANETS 9 1 2 N E P T U N E V E N U S 7 M E R C U R Y E 3 10 P L U T O E A R T H 4 5 8 J M T V E N U S 6 7 U R A N U S S J U P I T E R P R N A 5 8 S A T U R N I S E A R T H 4 U R A N U S T U 1 9 S U N E M E R C U R Y 11 6 M A R S R N 3 P L U T O 2 M O O N 1 2 3 4 5 6 7 8 9 10 11 S O L A R S Y S T E M SOLAR SYSTEM CROSSWORD THE SPACE RACE 6 7 7 J S C 1 2 1 S U N U R A N U S E A R T H 8 P T V A 3 8 2 9 I M E R C U R Y E M M I L K Y WA Y 3 10 T A R N P L U T O A L K 4 5 9 4 E A R T H N E P T U N E P O U V E N U S R S L S N N R C U 5S L S C T T H 6 O V A B R Activity book courtesy of.
Recommended publications
  • Mission to Jupiter
    This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines.
    [Show full text]
  • JUICE Red Book
    ESA/SRE(2014)1 September 2014 JUICE JUpiter ICy moons Explorer Exploring the emergence of habitable worlds around gas giants Definition Study Report European Space Agency 1 This page left intentionally blank 2 Mission Description Jupiter Icy Moons Explorer Key science goals The emergence of habitable worlds around gas giants Characterise Ganymede, Europa and Callisto as planetary objects and potential habitats Explore the Jupiter system as an archetype for gas giants Payload Ten instruments Laser Altimeter Radio Science Experiment Ice Penetrating Radar Visible-Infrared Hyperspectral Imaging Spectrometer Ultraviolet Imaging Spectrograph Imaging System Magnetometer Particle Package Submillimetre Wave Instrument Radio and Plasma Wave Instrument Overall mission profile 06/2022 - Launch by Ariane-5 ECA + EVEE Cruise 01/2030 - Jupiter orbit insertion Jupiter tour Transfer to Callisto (11 months) Europa phase: 2 Europa and 3 Callisto flybys (1 month) Jupiter High Latitude Phase: 9 Callisto flybys (9 months) Transfer to Ganymede (11 months) 09/2032 – Ganymede orbit insertion Ganymede tour Elliptical and high altitude circular phases (5 months) Low altitude (500 km) circular orbit (4 months) 06/2033 – End of nominal mission Spacecraft 3-axis stabilised Power: solar panels: ~900 W HGA: ~3 m, body fixed X and Ka bands Downlink ≥ 1.4 Gbit/day High Δv capability (2700 m/s) Radiation tolerance: 50 krad at equipment level Dry mass: ~1800 kg Ground TM stations ESTRAC network Key mission drivers Radiation tolerance and technology Power budget and solar arrays challenges Mass budget Responsibilities ESA: manufacturing, launch, operations of the spacecraft and data archiving PI Teams: science payload provision, operations, and data analysis 3 Foreword The JUICE (JUpiter ICy moon Explorer) mission, selected by ESA in May 2012 to be the first large mission within the Cosmic Vision Program 2015–2025, will provide the most comprehensive exploration to date of the Jovian system in all its complexity, with particular emphasis on Ganymede as a planetary body and potential habitat.
    [Show full text]
  • Materials for Liquid Propulsion Systems
    https://ntrs.nasa.gov/search.jsp?R=20160008869 2019-08-29T17:47:59+00:00Z CHAPTER 12 Materials for Liquid Propulsion Systems John A. Halchak Consultant, Los Angeles, California James L. Cannon NASA Marshall Space Flight Center, Huntsville, Alabama Corey Brown Aerojet-Rocketdyne, West Palm Beach, Florida 12.1 Introduction Earth to orbit launch vehicles are propelled by rocket engines and motors, both liquid and solid. This chapter will discuss liquid engines. The heart of a launch vehicle is its engine. The remainder of the vehicle (with the notable exceptions of the payload and guidance system) is an aero structure to support the propellant tanks which provide the fuel and oxidizer to feed the engine or engines. The basic principle behind a rocket engine is straightforward. The engine is a means to convert potential thermochemical energy of one or more propellants into exhaust jet kinetic energy. Fuel and oxidizer are burned in a combustion chamber where they create hot gases under high pressure. These hot gases are allowed to expand through a nozzle. The molecules of hot gas are first constricted by the throat of the nozzle (de-Laval nozzle) which forces them to accelerate; then as the nozzle flares outwards, they expand and further accelerate. It is the mass of the combustion gases times their velocity, reacting against the walls of the combustion chamber and nozzle, which produce thrust according to Newton’s third law: for every action there is an equal and opposite reaction. [1] Solid rocket motors are cheaper to manufacture and offer good values for their cost.
    [Show full text]
  • Ulyssesulysses
    UlyssesUlysses Achievements: first in situ investigation of the inner heliosphere from the solar equator to the poles; first exploration of the dusk sector of Jupiter’s magnetosphere; fastest spacecraft at launch (15.4 km/s) Launch date: 6 October 1990 Mission end: planned September 2004 Launch vehicle/site: NASA Space Shuttle Discovery from Kennedy Space Center, USA Launch mass: 370 kg (including 55 kg scientific payload) Orbit: heliocentric, 1.34x5.4 AU, inclined 79.1° to ecliptic, 6.2 year period Principal contractors: Dornier (prime), British Aerospace (AOCS, HGA), Fokker (thermal, nutation damper), FIAR (power), Officine Galileo (Sun sensors), Laben (data handling), Thomson-CSF (telecommand), MBB (thrusters)] Ulysses is making the first-ever of the heliosphere, and slow wind study of the particles and fields in confined to the equatorial regions), the inner heliosphere at all solar the discovery that high- and low- latitudes, including the polar latitude regions of the heliosphere regions. A Jupiter flyby in February are connected in a much more 1992 deflected Ulysses out of the systematic way than previously ecliptic plane into a high-inclination thought, the first-ever direct solar orbit, bringing it over the Sun’s measurement of interstellar gas south pole for the first time in (both in neutral and ionised state) September 1994 and its north pole and dust particles, and the precise 10.5 months later. Ulysses spent a measurement of cosmic-ray isotopes. total of 234 days at latitudes >70°, These, together with numerous other reaching a maximum 80.2° in both important findings, have resulted in hemispheres. The mission was more than 700 publications to date originally to end in September 1995, in the scientific literature.
    [Show full text]
  • Apollo Rocket Propulsion Development
    REMEMBERING THE GIANTS APOLLO ROCKET PROPULSION DEVELOPMENT Editors: Steven C. Fisher Shamim A. Rahman John C. Stennis Space Center The NASA History Series National Aeronautics and Space Administration NASA History Division Office of External Relations Washington, DC December 2009 NASA SP-2009-4545 Library of Congress Cataloging-in-Publication Data Remembering the Giants: Apollo Rocket Propulsion Development / editors, Steven C. Fisher, Shamim A. Rahman. p. cm. -- (The NASA history series) Papers from a lecture series held April 25, 2006 at the John C. Stennis Space Center. Includes bibliographical references. 1. Saturn Project (U.S.)--Congresses. 2. Saturn launch vehicles--Congresses. 3. Project Apollo (U.S.)--Congresses. 4. Rocketry--Research--United States--History--20th century-- Congresses. I. Fisher, Steven C., 1949- II. Rahman, Shamim A., 1963- TL781.5.S3R46 2009 629.47’52--dc22 2009054178 Table of Contents Foreword ...............................................................................................................................7 Acknowledgments .................................................................................................................9 Welcome Remarks Richard Gilbrech ..........................................................................................................11 Steve Fisher ...................................................................................................................13 Chapter One - Robert Biggs, Rocketdyne - F-1 Saturn V First Stage Engine .......................15
    [Show full text]
  • 4.1.6 Interplanetary Travel
    Interplanetary 4.1.6 Travel In This Section You’ll Learn to... Outline ☛ Describe the basic steps involved in getting from one planet in the solar 4.1.6.1 Planning for Interplanetary system to another Travel ☛ Explain how we can use the gravitational pull of planets to get “free” Interplanetary Coordinate velocity changes, making interplanetary transfer faster and cheaper Systems 4.1.6.2 Gravity-assist Trajectories he wealth of information from interplanetary missions such as Pioneer, Voyager, and Magellan has given us insight into the history T of the solar system and a better understanding of the basic mechanisms at work in Earth’s atmosphere and geology. Our quest for knowledge throughout our solar system continues (Figure 4.1.6-1). Perhaps in the not-too-distant future, we’ll undertake human missions back to the Moon, to Mars, and beyond. How do we get from Earth to these exciting new worlds? That’s the problem of interplanetary transfer. In Chapter 4 we laid the foundation for understanding orbits. In Chapter 6 we talked about the Hohmann Transfer. Using this as a tool, we saw how to transfer between two orbits around the same body, such as Earth. Interplanetary transfer just extends the Hohmann Transfer. Only now, the central body is the Sun. Also, as you’ll see, we must be concerned with orbits around our departure and Space Mission Architecture. This chapter destination planets. deals with the Trajectories and Orbits segment We’ll begin by looking at the basic equation of motion for interplane- of the Space Mission Architecture.
    [Show full text]
  • Aas 19-829 Trajectory Design for a Solar Polar
    AAS 19-829 TRAJECTORY DESIGN FOR A SOLAR POLAR OBSERVING CONSTELLATION Thomas R. Smith,∗ Natasha Bosanac,y Thomas E. Berger,z Nicole Duncan,x and Gordon Wu{ Space-based observatories are an invaluable resource for forecasting geomagnetic storms caused by solar activity. Currently, most space weather satellites obtain measurements of the Sun’s magnetic field along the Sun-Earth line and in the eclip- tic plane. To obtain complete and regular polar coverage of the Sun’s magnetic field, the University of Colorado Boulder’s Space Weather Technology, Research, and Education Center (SWx TREC) and Ball Aerospace are currently developing a mission concept labeled the Solar Polar Observing Constellation (SPOC). This concept comprises two spacecraft in low-eccentricity and high-inclination helio- centric orbits at less than 1 astronomical unit (AU) from the Sun. The focus of this paper is the design of a trajectory for the SPOC concept that satisfies a variety of hardware and mission constraints to improve solar magnetic field models and wind forecasts via polar viewpoints of the Sun. INTRODUCTION Space weather satellites are essential in developing accurate solar magnetic field models and so- lar wind forecasts to provide advance warnings of geomagnetic storms. Measurements of the solar magnetic field are the primary inputs to forecasts of the solar wind and, thus, the arrival times of coronal mass ejections (CMEs). Space-based magnetogram and doppler velocity measurements of the Sun’s magnetic field are valuable in developing these models and forecasts.
    [Show full text]
  • Voyage to Jupiter. INSTITUTION National Aeronautics and Space Administration, Washington, DC
    DOCUMENT RESUME ED 312 131 SE 050 900 AUTHOR Morrison, David; Samz, Jane TITLE Voyage to Jupiter. INSTITUTION National Aeronautics and Space Administration, Washington, DC. Scientific and Technical Information Branch. REPORT NO NASA-SP-439 PUB DATE 80 NOTE 208p.; Colored photographs and drawings may not reproduce well. AVAILABLE FROMSuperintendent of Documents, U.S. Government Printing Office, Washington, DC 20402 ($9.00). PUB TYPE Reports - Descriptive (141) EDRS PRICE MF01/PC09 Plus Postage. DESCRIPTORS Aerospace Technology; *Astronomy; Satellites (Aerospace); Science Materials; *Science Programs; *Scientific Research; Scientists; *Space Exploration; *Space Sciences IDENTIFIERS *Jupiter; National Aeronautics and Space Administration; *Voyager Mission ABSTRACT This publication illustrates the features of Jupiter and its family of satellites pictured by the Pioneer and the Voyager missions. Chapters included are:(1) "The Jovian System" (describing the history of astronomy);(2) "Pioneers to Jupiter" (outlining the Pioneer Mission); (3) "The Voyager Mission"; (4) "Science and Scientsts" (listing 11 science investigations and the scientists in the Voyager Mission);.(5) "The Voyage to Jupiter--Cetting There" (describing the launch and encounter phase);(6) 'The First Encounter" (showing pictures of Io and Callisto); (7) "The Second Encounter: More Surprises from the 'Land' of the Giant" (including pictures of Ganymede and Europa); (8) "Jupiter--King of the Planets" (describing the weather, magnetosphere, and rings of Jupiter); (9) "Four New Worlds" (discussing the nature of the four satellites); and (10) "Return to Jupiter" (providing future plans for Jupiter exploration). Pictorial maps of the Galilean satellites, a list of Voyager science teams, and a list of the Voyager management team are appended. Eight technical and 12 non-technical references are provided as additional readings.
    [Show full text]
  • Access to the Outer Solar System
    Interstellar Probe Study Webinar Series Access to the Outer Solar System Presenters • Michael Paul • Program Manager, Interstellar Probe Study, Johns Hopkins APL • Robert Stough • Payload Utilization Manager for NASA’s SLS Rocket, NASA Marshall Space Flight Center 12:05 PM EDT Thursday, 9 July 2020 Interstellar Probe Study Website http://interstellarprobe.jhuapl.edu NOW: The Heliosphere and the Local Interstellar Medium Our Habitable Astrosphere Sol G2V Main Sequence Star 24 km/s Habitable Mira BZ Camelopardalis LL Orionis IRC+10216 Zeta Ophiuchi Interstellar Probe Study 9 July 2020 2 Voyager – The Accidental Interstellar Explorers Uncovering a New Regime of Space Physics Global Topology Cosmic Ray Shielding Unexpected Field Direction Force Balance Not Understood Required Hydrogen Wall Measured (Voyager) Interstellar Probe Study 9 July 2020 3 Opportunities Across Disciplines Modest Cross-Divisional Contributions with High Return Extra-Galactic Background Light Dwarf Planets and KBOs Early galaxy and star formation Solar system formation Today Arrokoth Big Bang Pluto 13.7 Gya First Stars & Galaxies Circum-Solar Dust Disk ~13Gya Imprint of solar system evolution Sol 4.6 Ga HL-Tau 1 Ma! Poppe+2019 Interstellar Probe Study 9 July 2020 4 Earth-Jupiter-Saturn Sequences • Point Solutions indicated per year (capped at C3 = 312.15km2/s2) C3 Speed Dest. 2037 2 2 Year Date (km /s ) CA_J (rJ) CA_S (rS) (AU/yr) (Lon, Lat) 2036 17 Sept 182.66 1.05 2.0 5.954 (247,0) 2038 2037 15 Oct 312.15 1.05 2.0 7.985 (230,0) 2038 14 Nov 312.15 1.05 2.0 7.563 (241,0.1) 2036 2039 2039 15 Nov 274.65 1.05 2.0 5.055 (256,0.3) Interstellar Probe Study 9 July 2020 5 SPACE LAUNCH SYSTEM INTERSTELLAR PROBE Robert Stough SLS Spacecraft/Payload Integration & Evolution (SPIE) July 9, 2020 0760 SLS EVOLVABILITY FOUNDATION FOR A GENERATION OF DEEP SPACE EXPLORATION 322 ft.
    [Show full text]
  • NASA Launch Services Manifest
    Launch Options - Future Options • Constellation Architecture • Commercial Alternatives – SpaceX – Orbital Sciences • EELV Options • DIRECT • Side-Mount Shuttle Derived • Space (or “Senate”) Launch System • Recent Developments © 2012 David L. Akin - All rights reserved http://spacecraft.ssl.umd.edu U N I V E R S I T Y O F U.S. Future Launch Options MARYLAND 1 ENAE 791 - Launch and Entry Vehicle Design Attribution • Slides shown are from the public record of the deliberations of the Augustine Commission (2009) • Full presentation packages available at http:// www.nasa.gov/ofces/hsf/meetings/index.html U N I V E R S I T Y O F U.S. Future Launch Options MARYLAND 2 ENAE 791 - Launch and Entry Vehicle Design Review of Human Spaceflight Plans Constellation Overview June 17, 2009 Doug Cooke www.nasa.gov Jeff Hanley Constellation Architecture Earth Departure Stage Altair Lunar Lander Orion Ares I Crew Exploration Crew Launch Vehicle Vehicle Ares V Cargo Launch Vehicle Constellation is an Integrated Architecture National Aeronautics and Space Administration 2 Key Exploration Objectives 1. Replace Space Shuttle capability, with Shuttle retirement in 2010 2. To ensure sustainability, development and operations costs must be minimized 3. Develop systems to serve as building blocks for human exploration of the solar system using the Moon as a test bed 4. Design future human spaceflight systems to be significantly safer than heritage systems 5. Provide crew transport to ISS by 2015, to the lunar surface for extended durations by 2020, and to Mars by TBD 6. Separate crew from cargo delivery to orbit 7. Maintain and grow existing national aerospace supplier base 8.
    [Show full text]
  • Launch Vehicle Family Album
    he pictures on the next several pages serve as a Launch Vehicle Tpartial "family album" of NASA launch vehicles. NASA did not develop all of the vehicles shown, but Family Album has employed each in its goal of "exploring the atmosphere and space for peaceful purposes for the benefit of all." The album contains historic rockets, those in use today, and concept designs that might be used in the future. They are arranged in three groups: rockets for launching satellites and space probes, rockets for launching humans into space, and concepts for future vehicles. The album tells the story of nearly 40 years of NASA space transportation. Rockets have probed the upper reaches of Earth's atmosphere, carried spacecraft into Earth orbit, and sent spacecraft out into the solar system and beyond. Initial rockets employed by NASA, such as the Redstone and the Atlas, began life as intercontinental ballistic missiles. NASA scientists and engineers found them ideal for carrying machine and human payloads into space. As the need for greater payload capacity increased, NASA began altering designs for its own rockets and building upper stages to use with existing rockets. Sending astronauts to the Moon required a bigger rocket than the rocket needed for carrying a small satellite to Earth orbit. Today, NASA's only vehicle for lifting astronauts into space is the Space Shuttle. Designed to be reusable, its solid rocket boosters have parachute recovery systems. The orbiter is a winged spacecraft that glides back to Earth. The external tank is the only part of the vehicle which has to be replaced for each mission.
    [Show full text]
  • Explore! Jupiter's Family Secrets
    National Aeronautics and Space Administration Explore! Jupiter’s Family Secrets Children Ages 8–13 Juno Informal Education Activity Guide Jet Propulsion Laboratory Educational Product California Institute of Technology Educators Children Ages 8–13 EG-2012-04-021-JPL National Aeronautics and Space Administration Explore! Jupiter’s Family Secrets OVERVIEW OF ACTIVITIES For Children Ages 8 to 13 The following five activities align with national standards for grades K–4 and 5–8. Jump Start: Jupiter! Activity Jump Start: Jupiter! is a 60-minute kick-off for children ages 8 to 13 that sets the stage for further explorations and activities in Explore! Jupiter’s Family Secrets. As a group, children discuss what 1 they know about the solar system and Jupiter. They work in teams to read about the Sun, eight planets, asteroid belt, and the dwarf planet Pluto. They use their knowledge to create a poster about each object, which can be displayed in the library and used to create the Jump to Jupiter outdoor course. The children revisit what they have learned and prepare to explore further. Jump to Jupiter Activity Children ages 8 to 13 help create and then navigate an outdoor course of the traditional “plan- ets” (including dwarf planet Pluto), which are represented by small common objects. By counting 2 the jumps needed to reach each object, children experience firsthand the vast scale of our solar system. The children’s posters from Jump Start: Jupiter! may be used to construct the course. Planet Party Activity In this 30-minute activity, children ages 7 and up and their families go outside on a clear evening and view the sky to see the planets for themselves.
    [Show full text]