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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. -
Design of Low-Altitude Martian Orbits Using Frequency Analysis A
Design of Low-Altitude Martian Orbits using Frequency Analysis A. Noullez, K. Tsiganis To cite this version: A. Noullez, K. Tsiganis. Design of Low-Altitude Martian Orbits using Frequency Analysis. Advances in Space Research, Elsevier, 2021, 67, pp.477-495. 10.1016/j.asr.2020.10.032. hal-03007909 HAL Id: hal-03007909 https://hal.archives-ouvertes.fr/hal-03007909 Submitted on 16 Nov 2020 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. Design of Low-Altitude Martian Orbits using Frequency Analysis A. Noulleza,∗, K. Tsiganisb aUniversit´eC^oted'Azur, Observatoire de la C^oted'Azur, CNRS, Laboratoire Lagrange, bd. de l'Observatoire, C.S. 34229, 06304 Nice Cedex 4, France bSection of Astrophysics Astronomy & Mechanics, Department of Physics, Aristotle University of Thessaloniki, GR 541 24 Thessaloniki, Greece Abstract Nearly-circular Frozen Orbits (FOs) around axisymmetric bodies | or, quasi-circular Periodic Orbits (POs) around non-axisymmetric bodies | are of primary concern in the design of low-altitude survey missions. Here, we study very low-altitude orbits (down to 50 km) in a high-degree and order model of the Martian gravity field. We apply Prony's Frequency Analysis (FA) to characterize the time variation of their orbital elements by computing accurate quasi-periodic decompositions of the eccentricity and inclination vectors. -
First Stop on the Interstellar Journey: the Solar Gravity Lens Focus
1 DRAFT 16 May 2017 First Stop on the Interstellar Journey: The Solar Gravity Lens Focus Louis Friedman *1, Slava G. Turyshev2 1 Executive Director Emeritus, The Planetary Society 2 Jet Propulsion Laboratory, California Institute of Technology Abstract Whether or not Starshoti proves practical, it has focused attention on the technologies required for practical interstellar flight. They are: external energy (not in-space propulsion), sails (to be propelled by the external energy) and ultra-light spacecraft (so that the propulsion energy provides the largest possible increase in velocity). Much development is required in all three of these areas. The spacecraft technologies, nano- spacecraft and sails, can be developed through increasingly capable spacecraft that will be able of going further and faster through the interstellar medium. The external energy source (laser power in the Starshot concept) necessary for any flight beyond the solar system (>~100,000 AU) will be developed independently of the spacecraft. The solar gravity lens focus is a line beginning at approximately 547 AU from the Sun along the line defined by the identified exo-planet and the Sunii. An image of the exo-planet requires a coronagraph and telescope on the spacecraft, and an ability for the spacecraft to move around the focal line as it flies along it. The image is created in the “Einstein Ring” and extends several kilometers around the focal line – the spacecraft will have to collect pixels by maneuvering in the imageiii. This can be done over many years as the spacecraft flies along the focal line. The magnification by the solar gravity lens is a factor of 100 billion, permitting kilometer scale resolution of an exo-planet that might be even tens of light-years distant. -
Space Sector Brochure
SPACE SPACE REVOLUTIONIZING THE WAY TO SPACE SPACECRAFT TECHNOLOGIES PROPULSION Moog provides components and subsystems for cold gas, chemical, and electric Moog is a proven leader in components, subsystems, and systems propulsion and designs, develops, and manufactures complete chemical propulsion for spacecraft of all sizes, from smallsats to GEO spacecraft. systems, including tanks, to accelerate the spacecraft for orbit-insertion, station Moog has been successfully providing spacecraft controls, in- keeping, or attitude control. Moog makes thrusters from <1N to 500N to support the space propulsion, and major subsystems for science, military, propulsion requirements for small to large spacecraft. and commercial operations for more than 60 years. AVIONICS Moog is a proven provider of high performance and reliable space-rated avionics hardware and software for command and data handling, power distribution, payload processing, memory, GPS receivers, motor controllers, and onboard computing. POWER SYSTEMS Moog leverages its proven spacecraft avionics and high-power control systems to supply hardware for telemetry, as well as solar array and battery power management and switching. Applications include bus line power to valves, motors, torque rods, and other end effectors. Moog has developed products for Power Management and Distribution (PMAD) Systems, such as high power DC converters, switching, and power stabilization. MECHANISMS Moog has produced spacecraft motion control products for more than 50 years, dating back to the historic Apollo and Pioneer programs. Today, we offer rotary, linear, and specialized mechanisms for spacecraft motion control needs. Moog is a world-class manufacturer of solar array drives, propulsion positioning gimbals, electric propulsion gimbals, antenna positioner mechanisms, docking and release mechanisms, and specialty payload positioners. -
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets RESEARCH ARTICLE A Geophysical Perspective on the Bulk Composition of Mars 10.1002/2017JE005371 A. Khan1 , C. Liebske2,A.Rozel1, A. Rivoldini3, F. Nimmo4 , J. A. D. Connolly2 , A.-C. Plesa5 , Key Points: 1 • We constrain the bulk composition and D. Giardini of Mars using geophysical data to 1 2 an Fe/Si (wt) of 1.61 =−1.67 and a Institute of Geophysics, ETH Zürich, Zurich, Switzerland, Institute of Geochemistry and Petrology, ETH Zürich, Zurich, molar Mg# of 0.745–0.751 Switzerland, 3Royal Observatory of Belgium, Brussels, Belgium, 4Department of Earth and Planetary Sciences, University • The results indicate a large liquid core of California, Santa Cruz, CA, USA, 5German Aerospace Center (DLR), Berlin, Germany (1,640–1,740 km in radius) containing 13.5–16 wt% S and excludes a transition to a lower mantle • We use the inversion results in Abstract We invert the Martian tidal response and mean mass and moment of inertia for chemical tandem with geodynamic simulations composition, thermal state, and interior structure. The inversion combines phase equilibrium computations to identify plausible geodynamic with a laboratory-based viscoelastic dissipation model. The rheological model, which is based on scenarios and parameters measurements of anhydrous and melt-free olivine, is both temperature and grain size sensitive and imposes strong constraints on interior structure. The bottom of the lithosphere, defined as the location Supporting Information: where the conductive geotherm meets the mantle adiabat, occurs deep within the upper mantle • Supporting Information S1 (∼200–400 km depth) resulting in apparent upper mantle low-velocity zones. -
Apollo Over the Moon: a View from Orbit (Nasa Sp-362)
chl APOLLO OVER THE MOON: A VIEW FROM ORBIT (NASA SP-362) Chapter 1 - Introduction Harold Masursky, Farouk El-Baz, Frederick J. Doyle, and Leon J. Kosofsky [For a high resolution picture- click here] Objectives [1] Photography of the lunar surface was considered an important goal of the Apollo program by the National Aeronautics and Space Administration. The important objectives of Apollo photography were (1) to gather data pertaining to the topography and specific landmarks along the approach paths to the early Apollo landing sites; (2) to obtain high-resolution photographs of the landing sites and surrounding areas to plan lunar surface exploration, and to provide a basis for extrapolating the concentrated observations at the landing sites to nearby areas; and (3) to obtain photographs suitable for regional studies of the lunar geologic environment and the processes that act upon it. Through study of the photographs and all other arrays of information gathered by the Apollo and earlier lunar programs, we may develop an understanding of the evolution of the lunar crust. In this introductory chapter we describe how the Apollo photographic systems were selected and used; how the photographic mission plans were formulated and conducted; how part of the great mass of data is being analyzed and published; and, finally, we describe some of the scientific results. Historically most lunar atlases have used photointerpretive techniques to discuss the possible origins of the Moon's crust and its surface features. The ideas presented in this volume also rely on photointerpretation. However, many ideas are substantiated or expanded by information obtained from the huge arrays of supporting data gathered by Earth-based and orbital sensors, from experiments deployed on the lunar surface, and from studies made of the returned samples. -
Pioneer Anomaly: What Can We Learn from Future Planetary Exploration Missions?
56th International Astronautical Congress, Paper IAC-05-A3.4.02 PIONEER ANOMALY: WHAT CAN WE LEARN FROM FUTURE PLANETARY EXPLORATION MISSIONS? Andreas Rathke EADS Astrium GmbH, Dept. AED41, 88039 Friedrichshafen, Germany. Email: [email protected] Dario Izzo ESA Advanced Concepts Team, ESTEC, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands. Email: [email protected] The Doppler-tracking data of the Pioneer 10 and 11 spacecraft show an unmodelled constant acceleration in the direction of the inner Solar System. Serious efforts have been undertaken to find a conventional explanation for this effect, all without success at the time of writing. Hence the effect, commonly dubbed the Pioneer anomaly, is attracting considerable attention. Unfortunately, no other space mission has reached the long-term navigation accuracy to yield an independent test of the effect. To fill this gap we discuss strategies for an experimental verification of the anomaly via an upcoming space mission. Emphasis is put on two plausible scenarios: non-dedicated concepts employing either a planetary exploration mission to the outer Solar System or a piggybacked micro- spacecraft to be launched from an exploration spacecraft travelling to Saturn or Jupiter. The study analyses the impact of a Pioneer anomaly test on the system and trajectory design for these two paradigms. Both paradigms are capable of verifying the Pioneer anomaly and determine its magnitude at 10% level. Moreover they can discriminate between the most plausible classes of models of the anomaly. The necessary adaptions of the system and mission design do not impair the planetary exploration goals of the missions. I. -
Deep Space Chronicle Deep Space Chronicle: a Chronology of Deep Space and Planetary Probes, 1958–2000 | Asifa
dsc_cover (Converted)-1 8/6/02 10:33 AM Page 1 Deep Space Chronicle Deep Space Chronicle: A Chronology ofDeep Space and Planetary Probes, 1958–2000 |Asif A.Siddiqi National Aeronautics and Space Administration NASA SP-2002-4524 A Chronology of Deep Space and Planetary Probes 1958–2000 Asif A. Siddiqi NASA SP-2002-4524 Monographs in Aerospace History Number 24 dsc_cover (Converted)-1 8/6/02 10:33 AM Page 2 Cover photo: A montage of planetary images taken by Mariner 10, the Mars Global Surveyor Orbiter, Voyager 1, and Voyager 2, all managed by the Jet Propulsion Laboratory in Pasadena, California. Included (from top to bottom) are images of Mercury, Venus, Earth (and Moon), Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets (Mercury, Venus, Earth and its Moon, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and Neptune) are roughly to scale to each other. NASA SP-2002-4524 Deep Space Chronicle A Chronology of Deep Space and Planetary Probes 1958–2000 ASIF A. SIDDIQI Monographs in Aerospace History Number 24 June 2002 National Aeronautics and Space Administration Office of External Relations NASA History Office Washington, DC 20546-0001 Library of Congress Cataloging-in-Publication Data Siddiqi, Asif A., 1966 Deep space chronicle: a chronology of deep space and planetary probes, 1958-2000 / by Asif A. Siddiqi. p.cm. – (Monographs in aerospace history; no. 24) (NASA SP; 2002-4524) Includes bibliographical references and index. 1. Space flight—History—20th century. I. Title. II. Series. III. NASA SP; 4524 TL 790.S53 2002 629.4’1’0904—dc21 2001044012 Table of Contents Foreword by Roger D. -
NASA and Planetary Exploration
**EU5 Chap 2(263-300) 2/20/03 1:16 PM Page 263 Chapter Two NASA and Planetary Exploration by Amy Paige Snyder Prelude to NASA’s Planetary Exploration Program Four and a half billion years ago, a rotating cloud of gaseous and dusty material on the fringes of the Milky Way galaxy flattened into a disk, forming a star from the inner- most matter. Collisions among dust particles orbiting the newly-formed star, which humans call the Sun, formed kilometer-sized bodies called planetesimals which in turn aggregated to form the present-day planets.1 On the third planet from the Sun, several billions of years of evolution gave rise to a species of living beings equipped with the intel- lectual capacity to speculate about the nature of the heavens above them. Long before the era of interplanetary travel using robotic spacecraft, Greeks observing the night skies with their eyes alone noticed that five objects above failed to move with the other pinpoints of light, and thus named them planets, for “wan- derers.”2 For the next six thousand years, humans living in regions of the Mediterranean and Europe strove to make sense of the physical characteristics of the enigmatic planets.3 Building on the work of the Babylonians, Chaldeans, and Hellenistic Greeks who had developed mathematical methods to predict planetary motion, Claudius Ptolemy of Alexandria put forth a theory in the second century A.D. that the planets moved in small circles, or epicycles, around a larger circle centered on Earth.4 Only partially explaining the planets’ motions, this theory dominated until Nicolaus Copernicus of present-day Poland became dissatisfied with the inadequacies of epicycle theory in the mid-sixteenth century; a more logical explanation of the observed motions, he found, was to consider the Sun the pivot of planetary orbits.5 1. -
NASA Ames Research Center Intelligent Systems and High End Computing
NASA Ames Research Center Intelligent Systems and High End Computing Dr. Eugene Tu, Director NASA Ames Research Center Moffett Field, CA 94035-1000 A 80-year Journey 1960 Soviet Union United States Russia Japan ESA India 2020 Illustration by: Bryan Christie Design Updated: 2015 Protecting our Planet, Exploring the Universe Earth Heliophysics Planetary Astrophysics Launch missions such as JWST to Advance knowledge unravel the of Earth as a Determine the mysteries of the system to meet the content, origin, and universe, explore challenges of Understand the sun evolution of the how it began and environmental and its interactions solar system and evolved, and search change and to with Earth and the the potential for life for life on planets improve life on solar system. elsewhere around other stars earth “NASA Is With You When You Fly” Safe, Transition Efficient to Low- Growth in Carbon Global Propulsion Operations Innovation in Real-Time Commercial System- Supersonic Wide Aircraft Safety Assurance Assured Ultra-Efficient Autonomy for Commercial Aviation Vehicles Transformation NASA Centers and Installations Goddard Institute for Space Studies Plum Brook Glenn Research Station Independent Center Verification and Ames Validation Facility Research Center Goddard Space Flight Center Headquarters Jet Propulsion Wallops Laboratory Flight Facility Armstrong Flight Research Center Langley Research White Sands Center Test Facility Stennis Marshall Space Kennedy Johnson Space Space Michoud Flight Center Space Center Center Assembly Center Facility -
NASA History Fact Sheet
NASA History Fact Sheet National Aeronautics and Space Administration Office of Policy and Plans NASA History Office NASA History Fact Sheet A BRIEF HISTORY OF THE NATIONAL AERONAUTICS AND SPACE ADMINISTRATION by Stephen J. Garber and Roger D. Launius Launching NASA "An Act to provide for research into the problems of flight within and outside the Earth's atmosphere, and for other purposes." With this simple preamble, the Congress and the President of the United States created the national Aeronautics and Space Administration (NASA) on October 1, 1958. NASA's birth was directly related to the pressures of national defense. After World War II, the United States and the Soviet Union were engaged in the Cold War, a broad contest over the ideologies and allegiances of the nonaligned nations. During this period, space exploration emerged as a major area of contest and became known as the space race. During the late 1940s, the Department of Defense pursued research and rocketry and upper atmospheric sciences as a means of assuring American leadership in technology. A major step forward came when President Dwight D. Eisenhower approved a plan to orbit a scientific satellite as part of the International Geophysical Year (IGY) for the period, July 1, 1957 to December 31, 1958, a cooperative effort to gather scientific data about the Earth. The Soviet Union quickly followed suit, announcing plans to orbit its own satellite. The Naval Research Laboratory's Project Vanguard was chosen on 9 September 1955 to support the IGY effort, largely because it did not interfere with high-priority ballistic missile development programs. -
Nuclear Power to Advance Space Exploration Gary L
Poster Paper P. 7.7 First Flights: Nuclear Power to Advance Space Exploration Gary L. Bennett E. W. Johnson Metaspace Enterprises EWJ Enterprises Emmett, Idaho Centerville, Ohio International Air & Space Symposium and Exposition Dayton Convention Center 14-17 July 2003 Dayton, Ohio USA r ... penni.. l .. 10 p~bli . h ..... ..,."b ll .~, ... ~ t .d til. <Op)'rigbt 0 ........ aomod oa tho fin' po_" ...... A1M.IIdd ..., yri ,hl, ... rit< .. AIM hrmi.. lou Dop a_I, 18(11 AI . ..od ... B<l1 Ori .... S.11e SIlO , R.stu. VA. 20191""-i44 FIRST FLIGHTS: NUCLEAR POWER TO ADVANCE SPACE EXPLORATION Gary L. Bennett E. W. Johnson Metaspace Enterprises EWJ Enterprises 5000 Butte Road 1017 Glen Arbor Court Emmett, Idaho 83617-9500 Centerville, Ohio 45459-5421 Tel/Fax: 1+208.365.1210 Telephone: 1+937.435.2971 E-mail: [email protected] E-mail: [email protected] Abstract One of the 20th century's breakthroughs that enabled and/or enhanced challenging space flights was the development of nuclear power sources for space applications. Nuclear power sources have allowed spacecraft to fly into regions where sunlight is dim or virtually nonexistent. Nuclear power sources have enabled spacecraft to perform extended missions that would have been impossible with more conventional power sources (e.g., photovoltaics and batteries). It is fitting in the year of the 100th anniversary of the first powered flight to consider the advancements made in space nuclear power as a natural extension of those first flights at Kitty Hawk to extending human presence into the Solar System and beyond. Programs were initiated in the mid 1950s to develop both radioisotope and nuclear reactor power sources for space applications.