NSIAD-88-129FS Space Exploration: Cost, Schedule, and Performance
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AE Newsletter 2020
Colonel Shorty Powers Composite Squadron July 25, 2020 AEROSPACE Aircraft | Spacecraft | Biography | Squadron Gen. Ira C. Eaker A New Eagle Boeing to build new F-15EXs for USAF The Department of the Air Force and Boeing recently signed a deal worth 1.2 billion dollars for the first lot of eight F-15EX jets that will be delivered to Eglin Air Force Base, Florida. The aircraft will replace the oldest F-15Cs and F-15Ds in the U.S. Air Force fleet. The first two already built F-15EX aircraft will be delivered during the second quarter of 2021, while the remaining aircraft will be delivered in 2023. The Air Force plans to buy 76 F-15EX aircraft. The new F-15EX was developed to meet needs identified by the National Defense Strategy review which directed the U.S. armed services to adapt to the new threats from China and Russia. The most burdensome requirement is the need for the Air Force to add 74 new squadrons to the existing 312 squadrons by 2030. The General Ira C. Eaker was one of the forefathers of an independent Air Force. With General (then major) Spaatz, in 1929 Eaker remained aloft aboard The Question Mark, a modified Atlantic-Fokker C-2A, for nearly a week, to demonstrate a newfound capability of aerial refueling. During WWII, Eaker rose to the grade of lieutenant general and commanded the Eighth Air Force, "The Mighty Eighth" force of strategic The first F-15EX being assembled at Boeing facilities. (Photo: Boeing) Aerospace Newsletter 1 Colonel Shorty Powers Composite Squadron July 25, 2020 Eaker (continued) Air Force also seeks to lower the average aircraft age of 28 years down to 15 years without losing any capacity. -
Ulysses Awardees
Ulysses Awardees Irish Higher Project Leader - Project Leader - French Higher Funding Education Disciplinary Area Project Title Ireland France Education Institution Institution Comparing Laws with Help from Humanities including Peter Arnds IRC / Embassy TCD Renaud Colson ENSCM, Montpellier the Humanities: Translation Theory languages, Law to the Rescue of Legal Studies Novel biomarkers of interplay between neuroglobin and George Barreto HRB / Embassy UL Karim Belarbi Université de Nantes Life Sciences neuroinflammation in Parkinson’s disease Geometric Constructions of Codes Eimear Byrne IRC / Embassy UCD Martino Borello University of Lille Mathematics for Secret Sharing Schemes BOUHÉREAU: EXILE, TOLERATION Didier Poton de Humanities including Derval Conroy IRC / Embassy UCD University Paris 8 - LAGA AND CARE IN THE EARLY MODERN Xaintrailles languages PERIOD Knotting peptides for DNA Fabian Cougnon IRC / Embassy NUIG Sebastian Ulrich La Rochelle University Chemistry recognition and gene delivery Automating Segmentation and Computer Science & Kathleen Curran HRB / Embassy UCD David Bendahan Muscle Architecture Analysis from Telecommunications Aix Marseille University Diffusion Tensor Imaging The Impact of Student Exchanges Social science and Ronald Davies IRC / Embassy UCD Farid Toubal on International Trade: The Role of University of Paris- economics Cultural Similarity Dauphine -- PSL Computer Science & Three dimensional audio and Gordon Delap IRC / Embassy MU Thibaud Keller Telecommunications musical experimentation CNRS – LaBRI Multi-scale, -
Let's Go to a Comet!
Mission Rosetta Let’s go to a comet! Elsa Montagnon European Space Agency 1 What is left to explore today? 15th century Credits: ESA/AOES Medialab 21st century 2 Back to the origins… 3 What has happened since the big bang? Big bang 13 billion years ago ejects hydrogen and helium From elements to dust From water to heavy elements From dust to gas From solar cloud to the solar system: planets, asteroids, comets 4 How do we see the solar system today? Galactic Tides Nearby Stars Large Clouds LPidCtLong Period Comets Short Period Comets Galactic Tides Inner Outer Oort Oort Pluto Cloud Cloud ? Stable Stable Kuiper Belt 10 Gy 1 Gy ? 10 50 100 Alpha I, e 1000 Centauri 10^4 Ejected AU 10^5 3.10^5 5 Where are we going? Comet 67P / Churyumow-Gerasimenko 3-D reconstruction of nucleus based on 12 March, 2003 Hubble Space Telescope observations Nucleus diameter: 4km Discovered in 1969 Orbital period: 6.6 years Pole End Side Nasa, Esa and Philippe Lamy (Laboratoire d’Astrobomie Spatiale) - STScl-PRC03-26 6 A picture of the comet… Credits: ESA and European Southern Observatory 7 The Mission Rendezvous with the comet shortly after aphelion Follow the comet up to perihelion and beyond Deploy a lander on the comet surface QuickTime™ and a YUV420 codec decompressor are needed to see this picture. 8 The Journey Launch: March 2004 Launcher: Ariane 5 Rendezvous with comet: August 2014 Distance: 6.5 billions km Cruise duration: 10 years Mission duration: 2 years 9 The Cruise The comet is very far away. -
Space Shuttle Program
Space Shuttle program The Space Shuttle Columbia seconds after engine ignition, 1981 (NASA). For the first two missions only, the external fuel tank spray-on foam insulation (SOFI) was painted white. Subsequent missions have featured an unpainted tank thus exposing the orange/rust colored foam insulation. This resulted in a weight saving of over 1,000 lb (450 kg), a savings that translated directly to added payload capacity to orbit. NASA's Space Shuttle, officially called Space Transportation System (STS), is the United States government's sole manned launch vehicle currently in service. The winged shuttle orbiter is launched vertically, carrying usually five to seven astronauts and up to about 22,700 kg (50,000 lbs) of payload into low earth orbit. When its mission is complete, it reenters the earth's atmosphere and makes an unpowered gliding horizontal landing, usually on a runway at Kennedy Space Center. The Space Shuttle orbiter was manufactured by North American Rockwell, now part of the Boeing Company. Martin Marietta (now part of Lockheed Martin) designed the external fuel tank and Morton Thiokol (now part of Alliant Techsystems (ATK)) designed the solid rocket boosters. The Shuttle is the first orbital spacecraft designed for partial reusability. It carries large payloads to various orbits, provides crew rotation for the International Space Station (ISS), and performs servicing missions. While the vehicle was designed with the capacity to recover satellites and other payloads from orbit and return them to Earth, this capacity has not been used often; it is, however, an important use of the Space Shuttle in the context of the ISS program, as only very small amounts of experimental material, hardware needing to be repaired, and trash can be returned by Soyuz. -
List of Missions Using SPICE (PDF)
1/7/20 Data Restorations Selected Past Users Current/Pending Users Examples of Possible Future Users Apollo 15, 16 [L] Magellan [L] Cassini Orbiter NASA Discovery Program Mariner 2 [L] Clementine (NRL) Mars Odyssey NASA New Frontiers Program Mariner 9 [L] Mars 96 (RSA) Mars Exploration Rover Lunar IceCube (Moorehead State) Mariner 10 [L] Mars Pathfinder Mars Reconnaissance Orbiter LunaH-Map (Arizona State) Viking Orbiters [L] NEAR Mars Science Laboratory Luna-Glob (RSA) Viking Landers [L] Deep Space 1 Juno Aditya-L1 (ISRO) Pioneer 10/11/12 [L] Galileo MAVEN Examples of Users not Requesting NAIF Help Haley armada [L] Genesis SMAP (Earth Science) GOLD (LASP, UCF) (Earth Science) [L] Phobos 2 [L] (RSA) Deep Impact OSIRIS REx Hera (ESA) Ulysses [L] Huygens Probe (ESA) [L] InSight ExoMars RSP (ESA, RSA) Voyagers [L] Stardust/NExT Mars 2020 Emmirates Mars Mission (UAE via LASP) Lunar Orbiter [L] Mars Global Surveyor Europa Clipper Hayabusa-2 (JAXA) Helios 1,2 [L] Phoenix NISAR (NASA and ISRO) Proba-3 (ESA) EPOXI Psyche Parker Solar Probe GRAIL Lucy EUMETSAT GEO satellites [L] DAWN Lunar Reconnaissance Orbiter MOM (ISRO) Messenger Mars Express (ESA) Chandrayan-2 (ISRO) Phobos Sample Return (RSA) ExoMars 2016 (ESA, RSA) Solar Orbiter (ESA) Venus Express (ESA) Akatsuki (JAXA) STEREO [L] Rosetta (ESA) Korean Pathfinder Lunar Orbiter (KARI) Spitzer Space Telescope [L] [L] = limited use Chandrayaan-1 (ISRO) New Horizons Kepler [L] [S] = special services Hayabusa (JAXA) JUICE (ESA) Hubble Space Telescope [S][L] Kaguya (JAXA) Bepicolombo (ESA, JAXA) James Webb Space Telescope [S][L] LADEE Altius (Belgian earth science satellite) ISO [S] (ESA) Armadillo (CubeSat, by UT at Austin) Last updated: 1/7/20 Smart-1 (ESA) Deep Space Network Spectrum-RG (RSA) NAIF has or had project-supplied funding to support mission operations, consultation for flight team members, and SPICE data archive preparation. -
Solar Orbiter Assessment Study and Model Payload
Solar Orbiter assessment study and model payload N.Rando(1), L.Gerlach(2), G.Janin(4), B.Johlander(1), A.Jeanes(1), A.Lyngvi(1), R.Marsden(3), A.Owens(1), U.Telljohann(1), D.Lumb(1) and T.Peacock(1). (1) Science Payload & Advanced Concepts Office, (2) Electrical Engineering Department, (3) Research and Scientific Support Department, European Space Agency, ESTEC, Postbus 299, NL-2200AG, Noordwijk, The Netherlands (4) Mission Analysis Office, European Space Agency, ESOC, Darmstadt, Germany ABSTRACT The Solar Orbiter mission is presently in assessment phase by the Science Payload and Advanced Concepts Office of the European Space Agency. The mission is confirmed in the Cosmic Vision programme, with the objective of a launch in October 2013 and no later than May 2015. The Solar Orbiter mission incorporates both a near-Sun (~0.22 AU) and a high-latitude (~ 35 deg) phase, posing new challenges in terms of protection from the intense solar radiation and related spacecraft thermal control, to remain compatible with the programmatic constraints of a medium class mission. This paper provides an overview of the assessment study activities, with specific emphasis on the definition of the model payload and its accommodation in the spacecraft. The main results of the industrial activities conducted with Alcatel Space and EADS-Astrium are summarized. Keywords: Solar physics, space weather, instrumentation, mission assessment, Solar Orbiter 1. INTRODUCTION The Solar Orbiter mission was first discussed at the Tenerife “Crossroads” workshop in 1998, in the framework of the ESA Solar Physics Planning Group. The mission was submitted to ESA in 2000 and then selected by ESA’s Science Programme Committee in October 2000 to be implemented as a flexi-mission, with a launch envisaged in the 2008- 2013 timeframe (after the BepiColombo mission to Mercury) [1]. -
ESA & ESOC Overview
NASA PM Challenge 2010 Developing the International Program/Project Management Community 9/10 February 2010 Dr. Bettina Böhm Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 1 Used with Permission PURPOSE OF ESA / ACTIVITIES “To provide for and promote, for exclusively Space science peaceful purposes, cooperation among Human spaceflight European states in space research and Exploration technology and their space applications.” Earth observation Launchers [Article 2 of ESA Convention] Navigation ESA is one of the few space agencies Telecommunications in the world to combine responsibility Technology in all areas of space activity. Operations Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 2 ESA FACTS AND FIGURES Over 30 years of experience 18 Member States 2080 staff, thereof 880 in Program Directorates, 790 in Operations and Technical Support and 410 in other Support Directorates 3 500 million Euros budget Over 60 satellites designed and tested Over 60 satellites operated in-flight and 8 missions rescued 16 scientific satellites in operation Five types of launcher developed More than 180 launches made Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 3 ESA Locations EAC (Cologne) Salmijaervi ESTEC Astronaut training (Noordwijk) Satellite technology development and testing Harwell ESOC ESA HQ (Darmstadt) (Paris) Brussels Satellite operations and ground system technology development ESAC (Villanueva de la Cañada Oberpfaffenhofen -
Commercial Orbital Transportation Services
National Aeronautics and Space Administration Commercial Orbital Transportation Services A New Era in Spaceflight NASA/SP-2014-617 Commercial Orbital Transportation Services A New Era in Spaceflight On the cover: Background photo: The terminator—the line separating the sunlit side of Earth from the side in darkness—marks the changeover between day and night on the ground. By establishing government-industry partnerships, the Commercial Orbital Transportation Services (COTS) program marked a change from the traditional way NASA had worked. Inset photos, right: The COTS program supported two U.S. companies in their efforts to design and build transportation systems to carry cargo to low-Earth orbit. (Top photo—Credit: SpaceX) SpaceX launched its Falcon 9 rocket on May 22, 2012, from Cape Canaveral, Florida. (Second photo) Three days later, the company successfully completed the mission that sent its Dragon spacecraft to the Station. (Third photo—Credit: NASA/Bill Ingalls) Orbital Sciences Corp. sent its Antares rocket on its test flight on April 21, 2013, from a new launchpad on Virginia’s eastern shore. Later that year, the second Antares lifted off with Orbital’s cargo capsule, (Fourth photo) the Cygnus, that berthed with the ISS on September 29, 2013. Both companies successfully proved the capability to deliver cargo to the International Space Station by U.S. commercial companies and began a new era of spaceflight. ISS photo, center left: Benefiting from the success of the partnerships is the International Space Station, pictured as seen by the last Space Shuttle crew that visited the orbiting laboratory (July 19, 2011). More photos of the ISS are featured on the first pages of each chapter. -
The Delta Launch Vehicle- Past, Present, and Future
The Space Congress® Proceedings 1981 (18th) The Year of the Shuttle Apr 1st, 8:00 AM The Delta Launch Vehicle- Past, Present, and Future J. K. Ganoung Manager Spacecraft Integration, McDonnell Douglas Astronautics Co. H. Eaton Delta Launch Program, McDonnell Douglas Astronautics Co. Follow this and additional works at: https://commons.erau.edu/space-congress-proceedings Scholarly Commons Citation Ganoung, J. K. and Eaton, H., "The Delta Launch Vehicle- Past, Present, and Future" (1981). The Space Congress® Proceedings. 7. https://commons.erau.edu/space-congress-proceedings/proceedings-1981-18th/session-6/7 This Event is brought to you for free and open access by the Conferences at Scholarly Commons. It has been accepted for inclusion in The Space Congress® Proceedings by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. THE DELTA LAUNCH VEHICLE - PAST, PRESENT AND FUTURE J. K. Ganoung, Manager H. Eaton, Jr., Director Spacecraft Integration Delta Launch Program McDonnell Douglas Astronautics Co. McDonnell Douglas Astronautics Co. INTRODUCTION an "interim space launch vehicle." The THOR was to be modified for use as the first stage, the The Delta launch vehicle is a medium class Vanguard second stage propulsion system, was used expendable booster managed by the NASA Goddard as the Delta second stage and the Vanguard solid Space Flight Center and used by the U.S. rocket motor became Delta's third stage. Government, private industry and foreign coun Following the eighteen month development program tries to launch scientific, meteorological, and failure to launch its first payload into or applications and communications satellites. -
(IES) Measurement of the Development of Pickup Ions from Comet 67P/Churyumov-Gerasimenko
PUBLICATIONS Geophysical Research Letters RESEARCH LETTER The Rosetta Ion and Electron Sensor (IES) measurement 10.1002/2015GL063939 of the development of pickup ions from comet Key Point: 67P/Churyumov-Gerasimenko • IES observed low-energy ions in August 2014, at an 80 km distance R. Goldstein1, J. L. Burch1, P. Mokashi1, T. Broiles1, K. Mandt1, J. Hanley1, T. Cravens2, A. Rahmati2, from the comet M. Samara3, G. Clark3, M. Hässig1,4, and J. M. Webster1 1Southwest Research Institute, San Antonio, Texas, USA, 2Physics and Astronomy, University of Kansas, Lawrence, Kansas, USA, 3 4 Correspondence to: NASA Goddard Space Flight Center, Greenbelt, Maryland, USA, Physikalisches Institut, University of Bern, Bern, Switzerland R. Goldstein, [email protected] Abstract The Rosetta Ion and Electron Sensor (IES) has been measuring solar wind ions intermittently since exiting from hibernation in May 2014. On 19 August, when Rosetta was ~80 km from the comet Citation: Goldstein, R., et al. (2015), The Rosetta Ion 67P/Churyumov-Gerasimenko, which was ~3.5 AU from the Sun, IES began to see ions at its lowest energy and Electron Sensor (IES) measurement range, ~4–10 eV. We identify these as ions created from neutral species emitted by the comet nucleus, of the development of pickup ions from photoionized by solar UV radiation in the neighborhood of the Rosetta spacecraft (S/C), and attracted by the comet 67P/Churyumov-Gerasimenko, Geophys. Res. Lett., 42,3093–3099, small negative potential of the S/C resulting from the population of thermal electrons. Later, IES began to doi:10.1002/2015GL063939. see higher-energy ions that we identify as having been picked up and accelerated by the solar wind. -
Exploring the Solar Poles and the Heliosphere from High Helio-Latitude
A white paper submitted to ESA for the Voyage 2050 long- term plan ? A journey to the polar regions of a star: Exploring the solar poles and the heliosphere from high helio-latitude Louise Harra ([email protected]) and the solar polar team PMOC/WRC, Dorfstrasse 33, CH-7260 Davos Dorf & ETH-Zürich, Switzerland [Image: Polar regions of major Solar System bodies. Top left, clockwise - Near-surface zonal flows around the solar north pole Bogart et al. (2015); Earth’s changing magnetic field from ESA’s Swarm constellation; Southern polar cap of Mars from ESA’s ExoMars; Jupiter’s poles from the NASA Juno mission; Saturn’s poles from the NASA Cassini mission.] Overview We aim to embark on one of humankind’s great journeys – to travel over the poles of our star, with a spacecraft unprecedented in its technology and instrumentation – to explore the polar regions of the Sun and their effect on the inner heliosphere in which we live. The polar vantage point provides a unique opportunity for major scientific advances in the field of heliophysics, and thus also provides the scientific underpinning for space weather applications. It has long been a scientific goal to study the poles of the Sun, illustrated by the NASA/ESA International Solar Polar Mission that was proposed over four decades ago, which led to the flight of ESA’s Ulysses spacecraft (1990 to 2009). Indeed, with regard to the Earth, we took the first tentative steps to explore the Earth’s polar regions only in the 1800s. Today, with the aid of space missions, key measurements relating to the nature and evolution of Earth’s polar regions are being made, providing vital input to climate-change models. -
Alejandro Cardesín Moinelo ESA Science Operations Center Mars Express & Exomars 2016 (Slides Courtesy of Christian Erd & Peter Falkner, ESA-ESTEC)
Alejandro Cardesín Moinelo ESA Science Operations Center Mars Express & ExoMars 2016 (slides courtesy of Christian Erd & Peter Falkner, ESA-ESTEC) ESAC, 7th February 2017 Mission Flow Diagram Slide 2 Space Mission Timeline: Phases Slide 3 Science Mission Design Process Slide 4 Science Objectives – Requirements - Solutions Science Objective is the high level motivation • Which scientific question/application purpose shall the WHY? project address and what answer is sought Requirement is the translation of this objective into verifiable statements of what is needed to achieve the objective With detailed quantities (unambiguous) • WHAT? • Several levels of detail • Traceable, all the way back to the top level • Careful with conflicting requirements Solution is the response to the all requirements • There can be several solutions meeting requirements HOW? • Non-compliance needs to be negotiated Slide 5 Conflicting Requirements Farm “Optimal” Animal : Eierlegende Wollmilchsau (famous Austrian animal) Slide 6 Trade-off Trade-off allows exploring alternative solutions to a baseline Most common criteria: mass, cost budget; several System Performance system properties can be translated into them Power consumption generation of more power solar array size mass Higher telemetry volume larger HGA, more power for TM&C mass High performance complex solutions Cost more effort for verification Mass longer integration time cost Slide 7 Mission Segments, Systems & Subsystems Slide 8 Mission Analysis Launch Transfer trajectory Insertion into