10. Spacecraft Configurations MAE 342 2016
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In-Depth Review of Satellite Imagery / Earth Observation Technology in Official Statistics Prepared by Canada and Mexico
In-depth review of satellite imagery / earth observation technology in official statistics Prepared by Canada and Mexico Julio A. Santaella Conference of European Statisticians 67th plenary session Paris, France June 28, 2019 Earth observation (EO) EO is the gathering of information about planet Earth’s physical, chemical and biological systems. It involves monitoring and assessing the status of, and changes in, the natural and man-made environment Measurements taken by a thermometer, wind gauge, ocean buoy, altimeter or seismograph Photographs and satellite imagery Radar and sonar images Analyses of water or soil samples EO examples EO Processed information such as maps or forecasts Source: Group on Earth Observations (GEO) In-depth review of satellite imagery / earth observation technology in official statistics 2 Introduction Satellite imagery uses have expanded over time Satellite imagery provide generalized data for large areas at relatively low cost: Aligned with NSOs needs to produce more information at lower costs NSOs are starting to consider EO technology as a data collection instrument for purposes beyond agricultural statistics In-depth review of satellite imagery / earth observation technology in official statistics 3 Scope and definition of the review To survey how various types of satellite data and the techniques used to process or analyze them support the GSBPM To improve coordination of statistical activities in the UNECE region, identify gaps or duplication of work, and address emerging issues In-depth review of satellite imagery / earth observation technology in official statistics 4 Overview of recent activities • EO technology has developed progressively, encouraging the identification of new applications of this infrastructure data. -
Quality and Reliability: APL's Key to Mission Success
W. L. EBERT AND E. J. HOFFMAN Quality and Reliability: APL’s Key to Mission Success Ward L. Ebert and Eric J. Hoffman APL’s Space Department has a long history of producing reliable spaceflight systems. Key to the success of these systems are the methods employed to ensure robust, failure-tolerant designs, to ensure a final product that faithfully embodies those designs, and to physically verify that launch and environmental stresses will indeed be well tolerated. These basic methods and practices have served well throughout the constantly changing scientific, engineering, and budgetary challenges of the first 40 years of the space age. The Space Department has demonstrated particular competence in addressing the country’s need for small exploratory missions that extend the envelope of technology. (Keywords: Quality assurance, Reliability, Spacecraft, Spaceflight.) INTRODUCTION The APL Space Department attempts to be at the and development is fundamentally an innovative en- high end of the quality and reliability scale for un- deavor, and any plan to carry out such work necessarily manned space missions. A track record of nearly 60 has steps with unknown outcomes. On the other hand, spacecraft and well over 100 instruments bears this out conventional management wisdom says that some de- as a success. Essentially, all of APL’s space missions are gree of risk and unpredictability exists in any major one-of-a-kind, so the challenge is to get it right the first undertaking, and the only element that differs in re- time, every time, by developing the necessary technol- search and development is the larger degree of risks. -
Dod Space Technology Guide
Foreword Space-based capabilities are integral to the U.S.’s national security operational doctrines and processes. Such capa- bilities as reliable, real-time high-bandwidth communica- tions can provide an invaluable combat advantage in terms of clarity of command intentions and flexibility in the face of operational changes. Satellite-generated knowledge of enemy dispositions and movements can be and has been exploited by U.S. and allied commanders to achieve deci- sive victories. Precision navigation and weather data from space permit optimal force disposition, maneuver, decision- making, and responsiveness. At the same time, space systems focused on strategic nuclear assets have enabled the National Command Authorities to act with confidence during times of crisis, secure in their understanding of the strategic force postures. Access to space and the advantages deriving from operat- ing in space are being affected by technological progress If our Armed Forces are to be throughout the world. As in other areas of technology, the faster, more lethal, and more precise in 2020 advantages our military derives from its uses of space are than they are today, we must continue to dynamic. Current space capabilities derive from prior invest in and develop new military capabilities. decades of technology development and application. Joint Vision 2020 Future capabilities will depend on space technology programs of today. Thus, continuing investment in space technologies is needed to maintain the “full spectrum dominance” called for by Joint Vision 2010 and 2020, and to protect freedom of access to space by all law-abiding nations. Trends in the availability and directions of technology clearly suggest that the U.S. -
Orion First Flight Test
National Aeronautics and Space Administration orion First Flight Test NASAfacts Orion, NASA’s new spacecraft Exploration Flight Test-1 built to send humans farther During Orion’s flight test, the spacecraft will launch atop a Delta IV Heavy, a rocket built than ever before, is launching and operated by United Launch Alliance. While into space for the first time in this launch vehicle will allow Orion to reach an altitude high enough to meet the objectives for December 2014. this test, a much larger, human-rated rocket An uncrewed test flight called Exploration will be needed for the vast distances of future Flight Test-1 will test Orion systems critical to exploration missions. To meet that need, NASA crew safety, such as heat shield performance, is developing the Space Launch System, which separation events, avionics and software will give Orion the capability to carry astronauts performance, attitude control and guidance, farther into the solar system than ever before. parachute deployment and recovery operations. During the uncrewed flight, Orion will orbit The data gathered during the flight will influence the Earth twice, reaching an altitude of design decisions and validate existing computer approximately 3,600 miles – about 15 times models and innovative new approaches to space farther into space than the International Space systems development, as well as reduce overall Station orbits. Sending Orion to such a high mission risks and costs. altitude will allow the spacecraft to return to Earth at speeds near 20,000 mph. Returning -
Detecting, Tracking and Imaging Space Debris
r bulletin 109 — february 2002 Detecting, Tracking and Imaging Space Debris D. Mehrholz, L. Leushacke FGAN Research Institute for High-Frequency Physics and Radar Techniques, Wachtberg, Germany W. Flury, R. Jehn, H. Klinkrad, M. Landgraf European Space Operations Centre (ESOC), Darmstadt, Germany Earth’s space-debris environment tracked, with estimates for the number of Today’s man-made space-debris environment objects larger than 1 cm ranging from 100 000 has been created by the space activities to 200 000. that have taken place since Sputnik’s launch in 1957. There have been more than 4000 The sources of this debris are normal launch rocket launches since then, as well as many operations (Fig. 2), certain operations in space, other related debris-generating occurrences fragmentations as a result of explosions and such as more than 150 in-orbit fragmentation collisions in space, firings of satellite solid- events. rocket motors, material ageing effects, and leaking thermal-control systems. Solid-rocket Among the more than 8700 objects larger than 10 cm in Earth orbits, motors use aluminium as a catalyst (about 15% only about 6% are operational satellites and the remainder is space by mass) and when burning they emit debris. Europe currently has no operational space surveillance aluminium-oxide particles typically 1 to 10 system, but a powerful radar facility for the detection and tracking of microns in size. In addition, centimetre-sized space debris and the imaging of space objects is available in the form objects are formed by metallic aluminium melts, of the 34 m dish radar at the Research Establishment for Applied called ‘slag’. -
GEO and GEOSS……
GEO - GEOSS Support of the CBD 2010 Targets CBD - SBSTTA Paris, 4 July 2007 Douglas Muchoney, GEO Secretariat © GEO Secretariat The Earth is a complex system of systems © GEO Secretariat Any Single Problem Requires Many Data Sets A Single Data Set Will Serve Many Communities © GEO Secretariat Solar Energy © GEO Secretariat GEOSS Implementation is a Non- binding, Voluntary Process • Relies on the Goodwill of Members and Participating Organizations • Efficient for Contribution of Components • Not a Funding Mechanism • GEO implements GEOSS © GEO Secretariat GEO Goal Improve and Coordinate Observation Systems Provide Easier & More Open Data Access Foster Use (Science, Applications, Capacity Bldg) … to answer Society’s need for informed decision making © GEO Secretariat GEOSS: A Global, Coordinated, Comprehensive and Sustained System of Observing Systems © GEO Secretariat GEOSS will Address Nine Societal Benefit Areas 1. Reduction and Prevention of Disasters 2. Human Health and Epidemiology 3. Energy Management 4. Climate Variability & Change 5. Water Management 6. Weather Forecasting 7. Ecosystems 8. Agriculture 9. Biodiversity © GEO Secretariat GEOSS achievement through 5 Transverse Areas 1. Architecture 2. Data Management 3. User Engagement 4. Capacity Building 5. Outreach © GEO Secretariat Envisat SORCE Aura/Aqua/Terra Sage QuikScat IKONOS CBERS SeaWiFS SPOT 4, 5 SPIN-2 SeaWinds Orbview 2, 3 TRMM DMC ACRIMSAT EROS A1 ERBS Radarsat ALOS Toms-EP QuickBird Grace Landsat 7 Jason UARS Space Observation© GEO Secretariat Systems In Situ Observation Systems © GEO Secretariat GEO Societal Benefit Areas 1. Reduction and Prevention of Disasters 2. Human Health 3. Energy Management 4. Climate Change 5. Water Management 6. Weather Forecasting 7. Ecosystems 8. Agriculture 9. -
Exploration of the Moon
Exploration of the Moon The physical exploration of the Moon began when Luna 2, a space probe launched by the Soviet Union, made an impact on the surface of the Moon on September 14, 1959. Prior to that the only available means of exploration had been observation from Earth. The invention of the optical telescope brought about the first leap in the quality of lunar observations. Galileo Galilei is generally credited as the first person to use a telescope for astronomical purposes; having made his own telescope in 1609, the mountains and craters on the lunar surface were among his first observations using it. NASA's Apollo program was the first, and to date only, mission to successfully land humans on the Moon, which it did six times. The first landing took place in 1969, when astronauts placed scientific instruments and returnedlunar samples to Earth. Apollo 12 Lunar Module Intrepid prepares to descend towards the surface of the Moon. NASA photo. Contents Early history Space race Recent exploration Plans Past and future lunar missions See also References External links Early history The ancient Greek philosopher Anaxagoras (d. 428 BC) reasoned that the Sun and Moon were both giant spherical rocks, and that the latter reflected the light of the former. His non-religious view of the heavens was one cause for his imprisonment and eventual exile.[1] In his little book On the Face in the Moon's Orb, Plutarch suggested that the Moon had deep recesses in which the light of the Sun did not reach and that the spots are nothing but the shadows of rivers or deep chasms. -
Thesis Submitted to Florida Institute of Technology in Partial Fulfllment of the Requirements for the Degree Of
Dynamics of Spacecraft Orbital Refueling by Casey Clark Bachelor of Aerospace Engineering Mechanical & Aerospace Engineering College of Engineering 2016 A thesis submitted to Florida Institute of Technology in partial fulfllment of the requirements for the degree of Master of Science in Aerospace Engineering Melbourne, Florida July, 2018 ⃝c Copyright 2018 Casey Clark All Rights Reserved The author grants permission to make single copies. We the undersigned committee hereby approve the attached thesis Dynamics of Spacecraft Orbital Refueling by Casey Clark Dr. Tiauw Go, Sc.D. Associate Professor. Mechanical & Aerospace Engineering Committee Chair Dr. Jay Kovats, Ph.D. Associate Professor Mathematics Outside Committee Member Dr. Markus Wilde, Ph.D. Assistant Professor Mechanical & Aerospace Engineering Committee Member Dr. Hamid Hefazi, Ph.D. Professor and Department Head Mechanical & Aerospace Engineering ABSTRACT Title: Dynamics of Spacecraft Orbital Refueling Author: Casey Clark Major Advisor: Dr. Tiauw Go, Sc.D. A quantitative collation of relevant parameters for successfully completed exper- imental on-orbit fuid transfers and anticipated orbital refueling future missions is performed. The dynamics of connected satellites sustaining fuel transfer are derived by treating the connected spacecraft as a rigid body and including an in- ternal mass fow rate. An orbital refueling results in a time-varying local center of mass related to the connected spacecraft. This is accounted for by incorporating a constant mass fow rate in the inertia tensor. Simulations of the equations of motion are performed using the values of the parameters of authentic missions in an endeavor to provide conclusions regarding the efect of an internal mass transfer on the attitude of refueling spacecraft. -
Lunar Trajectories
Transportation for Exploration: New Thoughts About Orbital Dynamics Ed Belbruno Innovative Orbital Design, Inc & Courant Insitiute(NYU) January 4, 2012 NASA FISO 1 Evolution of Astrodynamics Conic; Stable (Hohmann, 20s) (Hohmann transfers, Gravity assist(Voyager, Galileo)) Nonlinear; Stable (Apollo, 60s) Nonlinear; Unstable (ISEE-3, 70s) (Transfer to and from halo orbits, no utilization of fuel savings via dynamics – Farquhar …) Nonlinear; Unstable; Low Energy/Fuel (Hiten, 91) (First use of utilization of chaotic dynamics/manifolds to achieve new approach to space travel for ballistic capture(EB, 86, 91) and for the study of halo orbit dynamics (Llibre-Simo, 85 – Genesis, 2001) Weak Stability Boundary Theory (EB 86) 2 Hohmann Transfer Conic, Stable – 2-body 3 Figure Eight(Apollo) Nonlinear, Stable – 3-body 4 ISEEC-3 Nonlinear-Unstable – 4 body 5 Ballistic Capture Transfers Weak Stability Boundary Theory(EB 86) • Way to transfer to the Moon, and other bodies, where no DeltaV is needed for capture • New methodology to trajectory design • Thought in 1985 to be impossible 6 Background • Capture Problem Earth -> Moon (LEO -> LLO) • Hohmann Transfer: Fast (3days), Fuel Hog (Need to slow down! 1 km/s to be captured – large maneuver ) Risky Used in Apollo 7 Idea of Achieving Ballistic Capture • Sneak up on Moon - very carefully (next figure A-B-C-D) • Like a surfer catching a wave • Want to ride the „gravity transition(weak stability) boundary‟ between the Earth-Moon-Sun 8 Top – Lagrange points Bottom – Sneaking up on Moon 9 Ballistic capture is chaotic (chaos – leaf blowing in wind) 10 • WSB – generalization of Lagrange points • Forces(GM, GE, CF) balance while spacecraft moving wrt Earth-Moon (L-points – forces balance for spacecraft fixed wrt Earth-Moon) • Get a multi-dimensional region about Moon. -
Highlights in Space 2010
International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren UNITED NATIONS 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France Tel: +33 1 45 67 42 60 Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 E-mail: : [email protected] E-mail: [email protected] Fax. + 33 1 44 76 74 37 URL: www.iislweb.com OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL : http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 *1180239* V.11-80239—January 2011—775 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no. -
Type Here Your Title
Envisat SORCE Aura/Aqua/Terra Sage QuikScat IKONOS CBERS SeaWiFS SPOT 4, 5 GEO-GLAM SPIN-2 SeaWinds GLOBAL AGRICULTURALOrbview 2, 3 MONITORINGTRMM DMC ACRIMSAT EROS A1 ERBS Radarsat Jai Singh PariharALOS for the GEOGLAM group and GEO Agriculture CommunityToms-EP of Practice QuickBird Grace Landsat 7 Jason UARS © GEO Secretariat Cereal grain production per hectare (Source: SAGE, Univ. of Wisconsin, Madison, Wisc., USA) 5th GEOSS-Asia Pacific Symposium, Tokyo, April 2-4, 2012 1. The GEO-GLAM Initiative : Objectives To reinforce the international community’s capacity to produce and disseminate relevant, timely and accurate forecasts of agricultural production at national, regional and global scales. Envisat SORCE Aura/Aqua/Terra Sage QuikScat IKONOS CBERS SeaWiFS SPOT 4, 5 SPIN-2 SeaWinds Orbview 2, 3 TRMM DMC ACRIMSAT EROS A1 ERBS Radarsat ALOS Toms-EP QuickBird Grace Landsat 7 Jason UARS © GEO Secretariat Agronomy Earth Observation Agro-economy Cultivated area / crop type area Meteorology Cereal grain production per hectare (Source: SAGE, Univ. of Wisconsin, Madison, Wisc., USA) Crop yield forecast 2 1. The GEO-GLAM Initiative : Background (G20 2011) 3 1. The GEO-GLAM Initiative : Background (G20 2011) G20 Final Declaration (Nov. 2011) 44. We commit to improve market information and transparency in order to make international markets for agricultural commodities more effective. To that end, we launched: • The "Agricultural Market Information System" (AMIS) in Rome on September 15, 2011, to improve information on markets ...; • The "Global Agricultural Geo-monitoring Initiative" (GEOGLAM) in Geneva on September 22-23, 2011, to coordinate satellite monitoring observation systems … to enhance crop production projections ... 4 2. -
The Moon Is a Harsh Chromatogram: the Most Strategic Knowledge Gap (Skg) at the Lunar Surface E
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 2766.pdf THE MOON IS A HARSH CHROMATOGRAM: THE MOST STRATEGIC KNOWLEDGE GAP (SKG) AT THE LUNAR SURFACE E. Patrick, R. Blase, M. Libardoni, Southwest Research Institute®, 6220 Culebra Rd., San Antonio, TX 78238 ([email protected]) Introduction: Data from analytical instruments de- a gas chromatograph mass spectrometer (GCMS) and ployed during multiple lunar missions, combined with revealed 97% of the composition in that mass channel laboratory results[1], suggest the regolith surface of the to be N2. Henderson et al.[5] also identified amino ac- Moon traps more volatiles in gas-surface interactions ids which were attributed to contamination, but results than is currently understood. We assert that the lunar from recent more sensitive LCMS and GCMS experi- surface behaves as a giant 3-D surface chromatogram, ments by Elsila et al.[1] found some amino acid and separating gas molecules by species as each wafts other organic signatures to be extraterrestrial in origin. across the regolith according to its mobility and ad- While these and other investigations suggest contami- sorption characteristics before eventually becoming nation from the Apollo spacecraft as a likely source for trapped. Herein we present supporting evicence for this a number of observed signatures[1,2,4,5], what is not claim. explained is the nature of the trapping mechanism for In gas chromatography (GC), components of a the N2 feature in 10086, and demonstrates gas retention sample are separated within a column according to from a gas that, under most circumstances, exhibits no their individual partitioning coefficients and by such retention at temperatures around 300 K[3].