Theoretical and Experimental Investigation of Hall Thruster Miniaturization by Noah Zachary Warner
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Analysis of Atmosphere-Breathing Electric Propulsion
Analysis of Atmosphere-Breathing Electric Propulsion IEPC-2013-421 Presented at the 33rd International Electric Propulsion Conference, The George Washington University, Washington, D.C., USA October 6{10, 2013 Tony Sch¨onherr,∗ and Kimiya Komurasakiy The University of Tokyo, Bunkyo, Tokyo, 113-8656, Japan and Georg Herdrichz University of Stuttgart, Stuttgart, Baden-W¨urttemberg, 70569, Germany To extend lifetime of commercial and scientific satellites in LEO and below (100-250 km of altitude) the recent years showed an increased activity in the field of air-breathing electric propulsion as well as beamed-energy propulsion systems. However, preliminary studies showed that the propellant flow necessary for electrostatic propulsion exceeds the mass intake possible within reasonable limits, and that electrode erosion due to oxygen flow might limit the lifetime of eventual thruster systems. Pulsed plasma thruster can be successfully operated with smaller mass intake, and operate at relatively small power demands which makes them an interesting candidate for air-breathing application in LEO, and their feasibility is investigated within this study. Further, to avoid electrode erosion, inductive plasma generator technology is discussed to derive a possible propulsion system that can handle gaseous propellant with no harmful effects. Nomenclature E = discharge energy per pulse FD = drag force imposed on satellite f = discharge frequency h = orbital altitude mbit = mass shot per pulse n = number density t = orbital lifetime I. Introduction Carrying propellant for attitude and orbit control on satellites in an Earth orbit results in an increased satellite mass, and, therefore, yields higher costs for manufacturing and launch of the spacecraft. Electric space propulsion helped in the past to reduce the mass requirements compared to standard chemical propul- sion as a result of the superior specific impulse, but limitations remain with regards to lifetime and lower ∗Assistant Professor, Department of Aeronautics and Astronautics, [email protected]. -
Herman IEPC-2019-651 PPE IPS Final
The Application of Advanced Electric Propulsion on the NASA Power and Propulsion Element (PPE) IEPC-2019-651 Presented at the 36th International Electric Propulsion Conference University of Vienna • Vienna • Austria September 15 – 20, 2019 Daniel A. Herman,1 Timothy Gray,2 NASA Glenn Research Center, Cleveland, OH, 44135, United States and Ian Johnson,3 Taylor Kerl,4 Ty Lee,5 and Tina Silva6 Maxar, Palo Alto, CA, 94303, United States Abstract: NASA is charGed with landinG the first American woman and next American man on the South Pole of the Moon by 2024. To meet this challenGe, NASA’s Gateway will develop and deploy critical infrastructure required for operations on the lunar surface and that enables a sustained presence on and around the moon. NASA’s Power and Propulsion Element (PPE), the first planned element of NASA’s cis-lunar Gateway, leveraGes prior and ongoing NASA and U.S. industry investments in high-power, long-life solar electric propulsion technoloGy investments. NASA awarded a PPE contract to Maxar TechnoloGies to demonstrate a 2,500 kg xenon capacity, 50 kW-class SEP spacecraft that meets Gateway’s needs, aligns with industry’s heritage spacecraft buses, and allows extensibility for NASA’s Mars exploration Goals. Maxar’s PPE concept desiGn, is based on their hiGh heritaGe, modular, and highly reliable 1300-series bus architecture. The electric propulsion system features two 13 kW Advanced Electric Propulsion (AEPS) strings from Aerojet Rocketdyne and a Maxar- developed system comprised of four Busek 6 kW Hall-effect thrusters mounted in pairs on larGe ranGe of motion mechanisms pointing arms with four 6 kW-class, Maxar-built PPUs derived from Geostationary Earth Orbit (GEO) heritage. -
Analysis of Planetary and Solar-Induced Perturbations on Trans-Martian Trajectory of Mars Missions Before and After Mars Orbit Insertion
Analysis of planetary and solar-induced perturbations on trans-Martian trajectory of Mars missions before and after Mars orbit insertion V U J Nwankwo1 and S K Chakrabarti1,2* 1S N Bose National Centre for Basic Sciences, Kolkata 700 098, West Bengal, India 2Indian Center for Space Physics, Kolkata 700 084, West Bengal, India Abstract: Interplanetary missions are susceptible to gravitational and nongravitational perturbing forces at every tra- jectory phase, assuming, of course, that the man made rockets and thrusters work as expected. These forces are mainly due to planetary and solar-forcing-induced perturbations during geocentric, heliocentric and Martian trajectories, and before orbit insertion. In this study, we review and/or analyze Mars orbiters mission associated perturbing forces and their possible impacts before Mars Orbit Insertion viz Earth’s oblateness, Third body (solar and lunar), solar radiation pressure, solar energetic radiation environment and atmospheric drag forces. We also model the significance of atmospheric drag force on Mangalyaan Mars orbiter mission, as a function of appropriate space environmental parameters during its 28 days in Earth’s orbit (around and during perigee passage), 300 days of heliocentric and 100 days of Martian trajectory. We have found that for a total perigee height boost of about 250 km, the cumulative orbit decay can be approximately 720 m. The approximate altitude variation could be up to 158 m with respect to the sun during 300 days of interplanetary journey toward Mars. After Mars orbit insertion, the total decay experienced by the spacecraft could be up to 701 m with decay rate of up to 9 m/day during 100 days of Martian trajectory, based on Mars–Earth atmosphere density ratio. -
A Breath of Fresh Air: Air-Scooping Electric Propulsion in Very Low Earth Orbit
A BREATH OF FRESH AIR: AIR-SCOOPING ELECTRIC PROPULSION IN VERY LOW EARTH ORBIT Rostislav Spektor and Karen L. Jones Air-scooping electric propulsion (ASEP) is a game-changing concept that extends the lifetime of very low Earth orbit (VLEO) satellites by providing periodic reboosting to maintain orbital altitudes. The ASEP concept consists of a solar array-powered space vehicle augmented with electric propulsion (EP) while utilizing ambient air as a propellant. First proposed in the 1960s, ASEP has attracted increased interest and research funding during the past decade. ASEP technology is designed to maintain lower orbital altitudes, which could reduce latency for a communication satellite or increase resolution for a remote sensing satellite. Furthermore, an ASEP space vehicle that stores excess gas in its fuel tank can serve as a reusable space tug, reducing the need for high-power chemical boosters that directly insert satellites into their final orbit. Air-breathing propulsion can only work within a narrow range of operational altitudes, where air molecules exist in sufficient abundance to provide propellant for the thruster but where the density of these molecules does not cause excessive drag on the vehicle. Technical hurdles remain, such as how to optimize the air-scoop design and electric propulsion system. Also, the corrosive VLEO atmosphere poses unique challenges for material durability. Despite these difficulties, both commercial and government researchers are making progress. Although ASEP technology is still immature, it is on the cusp of transitioning between research and development and demonstration phases. This paper describes the technical challenges, innovation leaders, and potential market evolution as satellite operators seek ways to improve performance and endurance. -
BUSEK CO. INC. Modern Spacecraft Performing Interplanetary Missions May Change Velocity by More Than 20,000 Miles Per Hour (32,000 Km/Hr)
SBIR/STTR SUCCESS An iodine plasma plume from Busek’s 600W Hall Effect Thruster during testing at NASA’s Glenn Research Center BUSEK CO. INC. modern spacecraft performing interplanetary missions may change velocity by more than 20,000 miles per hour (32,000 km/hr). To achieve these speeds, Hall Effect A Thrusters and other forms of ion propulsion may be used. For decades, xenon has been the gas of choice for most of NASA’s solar electric propulsion (SEP) systems. However, alternate propellants are needed for future missions. The high-pressure storage requirements of xenon gas coupled with fluctuating costs due to limited availability have prompted scientists to seek out alternative propellants and compatible propulsion systems. Busek Co. Inc., which has been developing state of the art Hall thrusters and solar electric PHASE III SUCCESS propulsion systems for over two decades, had a vision that iodine would provide all of the Over $3 million in Phase III and known benefits of xenon without the inherent challenges. follow-on contracts with NASA and the USAF “Iodine was a complete change in approach for Hall thrusters,” says Dr. James Szabo, Chief AGENCIES Scientist for Hall Thrusters at Busek. “Because you can launch at a much lower cost with NASA, DOD fewer volume restrictions, this isn’t just mission enhancement – it’s mission enabling.” SNAPSHOT Iodine offers NASA immense benefits when compared to xenon including mass and cost Busek has revolutionized solar savings. Iodine may be stored as a solid in low volume, low mass, low cost propellant tanks electric propulsion technology – an attractive feature when volume capacity on a spacecraft is extremely limited. -
Earth to Mars Areostationary Mission Optimization Analysis
Earth to Mars areostationary mission optimization analysis M. M. Sánchez-García, G. Barderas and P. Romero Instituto de Matemática Interdisciplinar. U. D. Astronomía y Geodesia, Facultad de Ciencias Matemáticas, Universidad Complutense de Madrid, Madrid, Spain ([email protected], [email protected], [email protected]) Abstract Mars has become one of the priorities in the planetary exploration programs. The analysis of space mission costs has become a key factor in mission planning. The determination of optimal trajectories aiming to lower costs in terms of impulses allows for more massive payloads to be transported at a minimum energy cost. Areostationary satellites are considered the most efficient and robust candidates to satisfy the control needs of the missions to Mars. Mars Areostationary Relay Satellites providing continuous coverage of a specific region of Mars are being considered for a near future. In this work, we analyze the optimization of an areostationary mission. We first determine the launch and arrival dates for an optimal minimum energy Earth-Mars transfer trajectory. Then, the minimum thrust maneuvers to capture the spacecraft from the hyperbolic arrival trajectory to Mars and place it in the areostationary orbit are analyzed. XIV.0 Reunión Científica 13-15 julio 2020 Context of the research: Previous studies The number of missions to Mars has increased over the last years, particularly robotic missions which need to be tele- commanded from the Earth. The need to control the different missions in Mars in almost real time with a relay system that provides continuous coverage of a specific region has been proposed by several authors such as Edwards et al. -
Program Management for Concurrent University Satellite Programs, Including Propellant Feed System Design Elements
Scholars' Mine Masters Theses Student Theses and Dissertations Spring 2019 Program management for concurrent university satellite programs, including propellant feed system design elements Shannah Withrow-Maser Follow this and additional works at: https://scholarsmine.mst.edu/masters_theses Part of the Aerospace Engineering Commons Department: Recommended Citation Withrow-Maser, Shannah, "Program management for concurrent university satellite programs, including propellant feed system design elements" (2019). Masters Theses. 7894. https://scholarsmine.mst.edu/masters_theses/7894 This thesis is brought to you by Scholars' Mine, a service of the Missouri S&T Library and Learning Resources. This work is protected by U. S. Copyright Law. Unauthorized use including reproduction for redistribution requires the permission of the copyright holder. For more information, please contact [email protected]. i PROGRAM MANAGEMENT FOR CONCURRENT UNIVERSITY SATELLITE PROGRAMS, INCLUDING PROPELLANT FEED SYSTEM DESIGN ELEMENTS by SHANNAH NICHOLE WITHROW A THESIS Presented to the Faculty of the Graduate School of the MISSOURI UNIVERSITY OF SCIENCE AND TECHNOLOGY In Partial Fulfillment of the Requirements for the Degree MASTER OF SCIENCE IN AEROSPACE ENGINEERING 2019 Approved by: Dr. Henry Pernicka, Advisor Dr. Suzanna Long Dr. Warner Meeks ii 2019 Shannah Nichole Withrow All Rights Reserved iii ABSTRACT Propulsion options for CubeSats are limited but are necessary for the CubeSat industry to continue future growth. Challenges to CubeSat propulsion include volume/mass constraints, availability of sufficiently small and certified hardware, secondary payload status, and power requirements. A multi-mode (chemical and electric) thruster was developed by at the Missouri University of Science and Technology to enable CubeSat propulsion missions. Two satellite buses, a 3U and 6U, are under development to demonstrate the multi-mode thruster’s capabilities. -
Busek Propulsion Systems
Busek SmallSat Technologies Planetary CubeSats Symposium Aug 17th 2018 NASA Goddard Space Flight Center Dan Courtney Michael Tsay Nathaniel Demmons Approved for public release; distribution is unlimited. Copyright 2018. busek.com © 2018 Busek Co. Inc. All Rights Reserved. Cubesat & SmallSat Propulsion (6kg-220kg) Approved for public release; distribution is unlimited. Copyright 2018. 2 BET-300-P Electrospray Thruster Busek CMNT on LISA Pathfinder : Successful Demonstration of Electrospray Thrusters for Precision Control <0.1μN resolution, <0.1μN/Hz1/2 noise BET-300-P / RCS Seeks to Provide Precision Control Electrospray Features to Small Spacecraft Approved for public release; distribution is unlimited. Copyright 2018. 3 BET-300-P Performance and Applicable Missions Performance: High T/P, Precision Actuator Customized integration T/P > 55mN/kW Wide range ~few to 150μN Deep space missions: Precision pointing: High impulse density Arcsecond precision Control <0.4μN Single RCS (vs. Vibration free reaction wheels+CG) Astronomy Laser communication • Low noise (calculated) <0.1μN/Hz1/2 [10mHz – 10Hz] Non-Keplerian orbits: Nm scale control • High impulse density ~1000Ns/U (1000s Isp) Inspection / service • Low impulse bits ~2μNs Occultation sources Distributed apertures Approved for public release; distribution is unlimited. Copyright 2018. 4 BET-300-P Example Mission Scenario 6U CubeSat observatory tasked with taking long exposure inertial-stare images • Precision ACS via electrospray holds target centroid to sub-arcsec over 10’s of seconds • Same ACS used to slew to next image position Images 100/day Impulse /image 1.7mNs/img Impulse /year 125Ns/yr Margin 100% Total impulse 250Ns/yr Mprop @ 65s Isp 400g/yr Mprop @ 1000s Isp 26g/yr Approved for public release; distribution is unlimited. -
'.';King Navigation
1980012912 -' JPL PUBLICATION 78-38 '.';king Navigation W. J. O'Neil, R. P. Rudd, D. L. Farless, C. E. Hildebrand, R. T. Mitchell, K. H. Rourke, et al. Jet Propulsion Laboratory E. A. Euler Martin Marietta Aerospace (N,%SA-C[_-l_,2517) VIklt_G ._AVIGA'IION (Jet t, u0-213_-_ : Pcopulsio[, L,_c.) 322 p _lC Alq/MF A01 _:d[,U CSCL Z2.t; hd0-_|4dj •_ [J_;c ]. a_ GJ/15 l,t7 5 'JJ ± November 15, 1979 _',r:.'> ;Y/l&_',,/I_cC7.'/',_/, : < X* ",t ,'" t National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California # 1980012912-002 JPL PUBLICATION 78-38 Viking Navigation W. J. O'Neil, R. P. Rudd, D. L. Farless, C. E. Hildebrand, R. T. Mitchell, K. H. Rourke, et al. Jet Propulsion Laboratory E. A. Euler Martin Marietta Aerospace November 15, 1979 National Aeronautics and Space Administration Jet Propulsion Laboratory : California Institute of Technology Pasadena, California 1980012912-003 The research descnbed bnth_s pubhcat_onwas camed out by the Jet Propulsion Laboratory, Cahforn_aInstitute of Technology, under NASA Contract No NAS7-100 i 1980012912-004 Abstract NASA soft-landed two Viking spacecraft on Mars in the summer t,f 1976. These were the free world's first landings on another planet. This report provides a final, comprehensive description of the navigation of the Viking spacecraft throughout their flight from Earth launch to Mars landing. The flight path design, actual int]lght control, and postflight reconstruction ale discussed in detail. The report Is comprised of an introductory chapter followed by five Olapters which essenually correspond to the organization of the Viking navigation operations, namely, Trajectory Descriptton, Interplanetary Orbit Determination, Satellite Orbit Determination, ._haneuver Analysis, and Lander Flight Path Analysis. -
Propulsion BHT-200-I Thruster
SmallSats, Iodine Propulsion Technology, Applications to Low-Cost Lunar Missions, and the iodine Satellite (iSAT) Project. Presented to Lunar Exploration Analysis Group (LEAG) October 23, 2014 The SmallSat Market SmallSat Applications – USASMDC / ARSTRAT Low Cost • Per-Unit Cost Very Low • Enables Affordable Satellite Constellations • Minimal Personnel and Logistics Tail • Frequent Technology Refresh Survivability • Fly Above Threats and Crowded Airspace • Rapid Augmentation and Reconstitution • Very Small Target Responsiveness • Short-Notice Deployment • Tasked from Theater • Persistent and Globally Available • Can Adapt to the Threat DISTRIBUTION A. Approved for public release; 24 July 2013 Release Number 3105 Why Iodine? • Today’s SmallSats have limited propulsion capability and most spacecraft have none • The State of the Art is cold gas propulsion providing 10s of m/s ∆V • No solutions exist for significant altitude or plane change, or de-orbit from high altitude • SmallSat secondary payloads have significant constraints • No hazardous propellants allowed • Limited stored energy allowed • Limited volume available • Indefinite quiescent waiting for launch integration • Iodine is uniquely suited for SmallSat applications • Iodine electric propulsion provides the high ISP * Density (i.e. ∆V per unit volume) • 1U of iodine on a 12U vehicle can provide more than 5 km/s ∆V • Enables transfer to high value operations orbits • Enables constellation deployment from a single launch • Enables de-orbit from high altitude deployment (ODAR Compliance) • Iodine enables > 10km/s for ESPA Class Spacecraft • GTO deployment to GEO, Lunar Orbits, Near Earth Asteroids, Mars and Venus • Reduces launch access by 90% • Reduces mission life cycle cost by 30 – 80% • Iodine is a solid at ambient conditions, can launch unpressurized and sit quiescent indefinitely • The technology leverages high heritage xenon Hall systems • All systems currently at TRL 5 with maturation funded to achieve TRL 6 in FY16 • The iSAT System is planned for launch readiness in early 2017 Iodine vs. -
Bi-Sat Observations of the Lunar Atmosphere Above Swirls (Bolas): Tethered Smallsat Investigation of Hydration and Space Weathering Processes at the Moon
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 2394.pdf BI-SAT OBSERVATIONS OF THE LUNAR ATMOSPHERE ABOVE SWIRLS (BOLAS): TETHERED SMALLSAT INVESTIGATION OF HYDRATION AND SPACE WEATHERING PROCESSES AT THE MOON. T. J. Stubbs1, B. K. Malphrus2, R. Hoyt3, M. A. Mesarch1, M. Tsay4, D. J. Chai1, M. K. Choi1, M. R. Collier1, J. W. Keller1, W. M. Farrell1, J. R. Espley1, J. S. Halekas5, A. P. Zucherman2, R. R. Vondrak1, P. E. Clark6, D. C. Folta1, T. E. Johnson7, G. Y. Kramer8, S. Fatemi9, J. Deca10, J. R. Gruesbeck11, J. L. McLain11, M. E. Purucker1, 1NASA Goddard Space Flight Center, Greenbelt, MD, USA, 2Morehead State University, Morehead, KY, USA, 3Teth- ers Unlimited, Inc., Bothell, WA, USA, 4Busek Co. Inc., Natick, MA, USA, 5University of Iowa, Iowa City, IA, USA, 6NASA Jet Propulsion Laboratory, Pasadena, CA, USA, 7NASA Wallops Flight Facility, Wallops, VA, USA, 8Lunar and Planetary Institute, Houston, TX, USA, 9Swedish Institute of Space Physics, Kiruna, Sweden, 10University of Colorado, Boulder, CO, USA, 11University of Maryland, College Park, MD, USA. [email protected] Introduction: Space weathering and hydration/hy- ii. how this relates to the formation of lunar swirls, droxylation of the lunar surface are fundamental pro- space weathering and the evolution of airless bodies. cesses for the Moon and other inner Solar System airless bodies [1, 2]. A thorough characterization of these pro- cesses is vital to our understanding of the evolution and origins of airless bodies, especially the production and transport of volatiles [3, 4]. At the Moon, space weath- ering of the surface regolith appears to be driven by the implantation of solar wind protons and meteoroid im- pacts, causing surfaces to darken, redden, and lose spec- tral features that could be used to constrain their mineral composition [1]. -
Characterization and Anomalous Diffusion Analysis of a 100W Low Power Annular Hall Effect Thruster Megan N
Air Force Institute of Technology AFIT Scholar Theses and Dissertations Student Graduate Works 3-21-2019 Characterization and Anomalous Diffusion Analysis of a 100w Low Power Annular Hall Effect Thruster Megan N. Maikell Follow this and additional works at: https://scholar.afit.edu/etd Part of the Propulsion and Power Commons Recommended Citation Maikell, Megan N., "Characterization and Anomalous Diffusion Analysis of a 100w Low Power Annular Hall Effect Thruster" (2019). Theses and Dissertations. 2226. https://scholar.afit.edu/etd/2226 This Thesis is brought to you for free and open access by the Student Graduate Works at AFIT Scholar. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of AFIT Scholar. For more information, please contact [email protected]. CHARACTERIZATION AND ANOMALOUS DIFFUSION ANALYSIS OF A 100W LOW POWER ANNULAR HALL EFFECT THRUSTER THESIS Megan N. Maikell, 2d Lieutenant, USAF AFIT-ENY-MS-19-M-231 DEPARTMENT OF THE AIR FORCE AIR UNIVERSITY AIR FORCE INSTITUTE OF TECHNOLOGY Wright-Patterson Air Force Base, Ohio DISTRIBUTION STATEMENT A. APPROVED FOR PUBLIC RELEASE; DISTRIBUTION UNLIMITED. The views expressed in this thesis are those of the author and do not reflect the official policy or position of the United States Air Force, Department of Defense, or the United States Government. This material is declared a work of the U.S. Government and is not subject to copyright protection in the United States. AFIT-ENY-MS-19-M-231 CHARACTERIZATION AND ANOMALOUS DIFFUSION ANALYSIS OF A 100W LOW POWER ANNULAR HALL EFFECT THRUSTER THESIS Presented to the Faculty Department of Aeronautics and Astronautics Graduate School of Engineering and Management Air Force Institute of Technology Air University Air Education and Training Command In Partial Fulfillment of the Requirements for the Degree of Master of Science in Astronautical Engineering Megan N.