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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. -
An Overview of Mars Vicinity Transportation Concepts for a Human Mars Mission
An Overview of Mars Vicinity Transportation Concepts for a Human Mars Mission Carol E. Dexter NASA/MSFC Exploration Transportation Office Larry Kos NASA/MSFC Preliminary Design Office/Mission Analysis Team Abstract To send a piloted mission to Mars, transportation systems must be developed for the Earth to Orbit, trans Mars injection (TMI), capture into Mars orbit, Mars descent, surface stay, Mars ascent, trans Earth injection (TEI), and Earth return phases. This paper presents a brief overview of the transportation systems for the Human Mars Mission (HMM) only in the vicinity of Mars. This includes: capture into Mars orbit, Mars descent, surface stay, and Mars ascent. Development of feasible mission scenarios now is important for identification of critical technology areas that must be developed to support future human missions. Although there is no funded human Mars mission today, architecture studies are focusing on missions traveling to Mars between 2011 and the early 2020's. Introduction For several years engineers and scientists at NASA have been developing mission scenarios for sending humans to Mars and returning them safely to Earth. The HMM has evolved as analyses have been completed and updated. The design reference mission (DRM) :'2 describes the baseline mission architecture at a given time, it is not intended to be a final or recommended mission scenario. As development of the HMM continues, the DRM and various mission architecture options or design reference points (DRPs) are refined and updated. Several locations are included in the DRPs: Mars, the Moon, and asteroids. At this time, only the Mars DRP has been evaluated in any detail. -
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. -
A Perspective on the Design and Development of the Spacex Dragon Spacecraft Heatshield
A Perspective on the Design and Development of the SpaceX Dragon Spacecraft Heatshield by Daniel J. Rasky, PhD Senior Scientist, NASA Ames Research Center Director, Space Portal, NASA Research Park Moffett Field, CA 94035 (650) 604-1098 / [email protected] February 28, 2012 2 How Did SpaceX Do This? Recovered Dragon Spacecraft! After a “picture perfect” first flight, December 8, 2010 ! 3 Beginning Here? SpaceX Thermal Protection Systems Laboratory, Hawthorne, CA! “Empty Floor Space” December, 2007! 4 Some Necessary Background: Re-entry Physics • Entry Physics Elements – Ballistic Coefficient – Blunt vs sharp nose tip – Entry angle/heating profile – Precision landing reqr. – Ablation effects – Entry G’loads » Blunt vs Lifting shapes – Lifting Shapes » Volumetric Constraints » Structure » Roll Control » Landing Precision – Vehicle flight and turn-around requirements Re-entry requires specialized design and expertise for the Thermal Protection Systems (TPS), and is critical for a successful space vehicle 5 Reusable vs. Ablative Materials 6 Historical Perspective on TPS: The Beginnings • Discipline of TPS began during World War II (1940’s) – German scientists discovered V2 rocket was detonating early due to re-entry heating – Plywood heatshields improvised on the vehicle to EDL solve the heating problem • X-15 Era (1950’s, 60’s) – Vehicle Inconel and Titanium metallic structure protected from hypersonic heating AVCOAT » Spray-on silicone based ablator for acreage » Asbestos/silicone moldable TPS for leading edges – Spray-on silicone ablator -
Constellation Program Overview
Constellation Program Overview October 2008 hris Culbert anager, Lunar Surface Systems Project Office ASA/Johnson Space Center Constellation Program EarthEarth DepartureDeparture OrionOrion -- StageStage CrewCrew ExplorationExploration VehicleVehicle AresAres VV -- HeavyHeavy LiftLift LaunchLaunch VehicleVehicle AltairAltair LunarLunar LanderLander AresAres II -- CrewCrew LaunchLaunch VehicleVehicle Lunar Capabilities Concept Review EstablishedEstablished Lunar Lunar Transportation Transportation EstablishEstablish Lunar Lunar Surface SurfaceArchitecturesArchitectures ArchitectureArchitecture Point Point of of Departure: Departure: StrategiesStrategies which: which: Satisfy NASA NGO’s to acceptable degree ProvidesProvides crew crew & & cargo cargo delivery delivery to to & & from from the the Satisfy NASA NGO’s to acceptable degree within acceptable schedule moonmoon within acceptable schedule Are consistent with capacity and capabilities ProvidesProvides capacity capacity and and ca capabilitiespabilities consistent consistent Are consistent with capacity and capabilities withwith candidate candidate surface surface architectures architectures ofof the the transportation transportation systems systems ProvidesProvides sufficient sufficient performance performance margins margins IncludeInclude set set of of options options fo for rvarious various prioritizations prioritizations of cost, schedule & risk RemainsRemains within within programmatic programmatic constraints constraints of cost, schedule & risk ResultsResults in in acceptable -
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. -
Silencing Nasa's Space Shuttle Crawler
SILENCING NASA’S SPACE SHUTTLE CRAWLER TRANSPORTER R. MacDonalda, C. Faszerb, and R. Margasahayamc aNoise Solutions Inc., #310 605 – 1st Street SW, Calgary, Alberta, Canada T2P 3S9 bFaszer Farquharson & Associates, #304 605 – 1st Street SW, Calgary, Alberta, Canada T2P 3S9 cNASA, John F. Kennedy Space Center, Florida, United States of America 32899 [email protected]; [email protected]; [email protected] Abstract. The crawler transporter (CT) is the world’s second largest known tracked vehicle, weighing 6 million pounds with a length of 131 feet and a width of 113 feet. The Kennedy Space Center (KSC) has two CTs that were designed and built for the Apollo program in the 1960’s, maintained and retrofitted for use in the Space Shuttle program. As a key element of the Space Shuttle ground systems, the crawler transports the entire 12-million-pound stack comprising the orbiter, the mobile launch platform (MLP), the external tank (ET), and the solid rocket boosters (SRB) from the Vehicle Assembly Building (VAB) to the launch pad. This rollout, constituting a 3.5 to 5.0 mile journey at a top speed of 0.9 miles-per-hour, requires over 8 hours to reach either Launch Complex 39A or B. This activity is only a prelude to the spectacle of sound and fury of the Space Shuttle launch to orbit in less than 10 minutes and traveling at orbital velocities of Mach 24. This paper summarizes preliminary results from the Crawler Transporter Sound Attenuation Study, encompassing test and engineering analysis of significant sound sources to measure and record full frequency spectrum and intensity of the various noise sources and to analyze the potential for noise mitigation. -
Space Shuttle Chronology Spacecalc
CBS News/Spaceflight Now STS Flight History by Launch Date 7/20/06 Space Shuttle Chronology SpaceCalc Space Shuttle DD HH MM SS Flights Notes Challenger 062 07 56 22 10 MET based on main gear Columbia 300 17 40 22 28 touchdown. Compiled from Discovery 268 15 29 30 32 news reports, NASA files. Atlantis 219 21 27 17 26 Endeavour 206 14 12 17 19 Compiled by William Harwood Program Total 1058 04 45 48 115 CBS News/Spaceflight Now OV # STS DD HH MM SS Launch Mission Description 102 N/A 01 00 00 00 00 02/28/81 Flight readiness firing 102 01 01 02 06 20 53 04/12/81 First shuttle flight 102 02 02 02 06 13 11 11/12/81 Fuel cell failure; MDM flight 102 03 03 08 00 04 46 03/22/82 White Sands, N.M., landing 102 04 04 07 01 09 31 06/27/82 Final shuttle test flight 102 05 05 05 02 14 26 11/11/82 1st STS satellites launched 99 N/A 06 00 00 00 00 12/18/82 Flight Readiness Firing 99 N/A 06 00 00 00 00 01/25/83 FRF-2 99 06 06 05 00 23 42 04/04/83 TDRS-1; 1st STS spacewalk 99 07 07 06 02 23 59 06/18/83 Three comsats 99 08 08 06 01 08 43 08/30/83 Insat, CFES 102 09 09 10 07 47 24 11/28/83 First Spacelab flight 99 10 41B 07 23 15 55 02/02/84 2 comsats lost; MMU EVA 99 11 41C 06 23 40 07 04/06/84 Solar Max repair; MMU EVA 103 N/A 41D 00 00 00 00 06/02/84 Flight readiness firing 103 N/A 41D 00 00 00 00 06/26/84 RSLS abort 103 12 41D 06 00 56 04 08/30/84 SBS, Syncom, Telstar 99 13 41G 08 05 23 38 10/05/84 ERBS; 1st female EVA 103 14 51A 07 23 44 56 11/07/84 Westar, Palapa retrieval 103 15 51C 03 01 33 23 01/24/85 DOD (Magnum?) 103 16 51D 06 23 55 23 04/12/85 -
Spacex Sends Its Latest Rocket to Space with Something Unusual Inside by Associated Press, Adapted by Newsela Staff on 02.16.18 Word Count 652 Level 820L
SpaceX sends its latest rocket to space with something unusual inside By Associated Press, adapted by Newsela staff on 02.16.18 Word Count 652 Level 820L This image from video provided by SpaceX shows owner Elon Musk's red Tesla sports car which was launched into space during the first test flight of the Falcon Heavy rocket on February 6, 2018. Photo by: SpaceX via AP CAPE CANAVERAL, Florida — The world's first space sports car is heading well beyond Mars. The red electric Tesla Roadster is aboard the brand new Falcon Heavy rocket. The company SpaceX launched the Heavy for its first test flight on February 6. Elon Musk runs the company SpaceX and the car company Tesla. Musk owns the sports car now flying through space. Musk, astronauts and many others cheered the successful launch from Florida. The Heavy is now the most powerful rocket flying these days. The space Roadster is now the fastest car ever. It is on a journey that will take it all the way to the asteroid belt between Mars and Jupiter. The asteroid belt is where unusually shaped space rocks and small planets orbit. This article is available at 5 reading levels at https://newsela.com. 1 Roadster Has Many Miles To Go Musk said the firing of the rocket's final booster engine put his car on a more distant flight than expected. It should go beyond Mars. It might almost reach the dwarf planet Ceres in the asteroid belt. Inside the car is a mannequin wearing a SpaceX spacesuit. -
Japan's Technical Prowess International Cooperation
Japan Aerospace Exploration Agency April 2016 No. 10 Special Features Japan’s Technical Prowess Technical excellence and team spirit are manifested in such activities as the space station capture of the HTV5 spacecraft, development of the H3 Launch Vehicle, and reduction of sonic boom in supersonic transport International Cooperation JAXA plays a central role in international society and contributes through diverse joint programs, including planetary exploration, and the utilization of Earth observation satellites in the environmental and disaster management fields Japan’s Technical Prowess Contents No. 10 Japan Aerospace Exploration Agency Special Feature 1: Japan’s Technical Prowess 1−3 Welcome to JAXA TODAY Activities of “Team Japan” Connecting the Earth and Space The Japan Aerospace Exploration Agency (JAXA) is positioned as We review some of the activities of “Team the pivotal organization supporting the Japanese government’s Japan,” including the successful capture of H-II Transfer Vehicle 5 (HTV5), which brought overall space development and utilization program with world- together JAXA, NASA and the International Space Station (ISS). leading technology. JAXA undertakes a full spectrum of activities, from basic research through development and utilization. 4–7 In 2013, to coincide with the 10th anniversary of its estab- 2020: The H3 Launch Vehicle Vision JAXA is currently pursuing the development lishment, JAXA defined its management philosophy as “utilizing of the H3 Launch Vehicle, which is expected space and the sky to achieve a safe and affluent society” and to become the backbone of Japan’s space development program and build strong adopted the new corporate slogan “Explore to Realize.” Under- international competitiveness. -
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. -
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