A Deep Space 6U Cubesat with Mission Enabling Ion Propulsion Technology
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New Moon Explorer Mission Concept
New Moon Explorer Mission Concept Les JOHNSONa,*, John CARRa,Jared Jared DERVANa, Alexander FEWa, Andy HEATONa, Benjamin Malphrusd, Leslie MCNUTTa, Joe NUTHb, Dana Tursec, and Aaron Zuchermand aNASA MSFC, Huntsville, AL USA bNASA GSFC, Huntsville, AL USA cRoccor, Longmont, CO USA dMorehead State University, Morehead, KY USA Abstract New Moon Explorer (NME) is a smallsat reconnaissance mission concept to explore Earth’s ‘New Moon’, the recently discovered Earth orbital companion asteroid 469219 Kamoʻoalewa (formerly 2016HO3), using solar sail propulsion. NME would determine Kamoʻoalewa’s spin rate, pole position, shape, structure, mass, density, chemical composition, temperature, thermal inertia, regolith characteristics, and spectral type using onboard instrumentation. If flown, NME would demonstrate multiple enabling technologies, including solar sail propulsion, large-area thin film power generation, and small spacecraft technology tailored for interplanetary space missions. Leveraging the solar sail technology and mission expertise developed by NASA for the Near Earth Asteroid (NEA) Scout mission, affordably learning more about our newest near neighbor is now a possibility. The mission is not yet planned for flight. Keywords: Kamoʻoalewa, solar sail, moon, Apollo asteroid 1. Introduction The emerging capabilities of extremely small spacecraft, coupled with solar sail propulsion, offers an opportunity for low-cost reconnaissance of the recently- discovered asteroid 469219 Kamoʻoalewa (formerly 2016HO3). While Kamoʻoalewa is not strictly a new moon, it is, for all practical purposes, an orbital companion of the Earth as the planet circles the sun. Kamoʻoalewa’s orbit relative to the Earth can be seen in Figure 1. Using the technologies developed for the NASA Fig. 1 The orbit of Earth’s companion, Kamoʻoalewa Near Earth Asteroid (NEA) Scout mission, a 6U as both it and the Earth orbit the Sun. -
The Cubesat Mission to Study Solar Particles (Cusp) Walt Downing IEEE Life Senior Member Aerospace and Electronic Systems Society President (2020-2021)
The CubeSat Mission to Study Solar Particles (CuSP) Walt Downing IEEE Life Senior Member Aerospace and Electronic Systems Society President (2020-2021) Acknowledgements – National Aeronautics and Space Administration (NASA) and CuSP Principal Investigator, Dr. Mihir Desai, Southwest Research Institute (SwRI) Feature Articles in SYSTEMS Magazine Three-part special series on Artemis I CubeSats - April 2019 (CuSP, IceCube, ArgoMoon, EQUULEUS/OMOTENASHI, & DSN) ▸ - September 2019 (CisLunar Explorers, OMOTENASHI & Iris Transponder) - March 2020 (BioSentinnel, Near-Earth Asteroid Scout, EQUULEUS, Lunar Flashlight, Lunar Polar Hydrogen Mapper, & Δ-Differential One-Way Range) Available in the AESS Resource Center https://resourcecenter.aess.ieee.org/ ▸Free for AESS members ▸ What are CubeSats? A class of small research spacecraft Built to standard dimensions (Units or “U”) ▸ - 1U = 10 cm x 10 cm x 11 cm (Roughly “cube-shaped”) ▸ - Modular: 1U, 2U, 3U, 6U or 12U in size - Weigh less than 1.33 kg per U NASA's CubeSats are dispensed from a deployer such as a Poly-Picosatellite Orbital Deployer (P-POD) ▸NASA’s CubeSat Launch initiative (CSLI) provides opportunities for small satellite payloads to fly on rockets ▸planned for upcoming launches. These CubeSats are flown as secondary payloads on previously planned missions. https://www.nasa.gov/directorates/heo/home/CubeSats_initiative What is CuSP? NASA Science Mission Directorate sponsored Heliospheric Science Mission selected in June 2015 to be launched on Artemis I. ▸ https://www.nasa.gov/feature/goddard/2016/heliophys ics-cubesat-to-launch-on-nasa-s-sls Support space weather research by determining proton radiation levels during solar energetic particle events and identifying suprathermal properties that could help ▸ predict geomagnetic storms. -
Solar Sail Propulsion for Deep Space Exploration
Solar Sail Propulsion for Deep Space Exploration Les Johnson NASA George C. Marshall Space Flight Center NASA Image We tend to think of space as being big and empty… NASA Image Space Is NOT Empty. We can use the environments of space to our advantage NASA Image Solar Sails Derive Propulsion By Reflecting Photons Solar sails use photon “pressure” or force on thin, lightweight, reflective sheets to produce thrust. 4 NASA Image Real Solar Sails Are Not “Ideal” Billowed Quadrant Diffuse Reflection 4 Thrust Vector Components 4 Solar Sail Trajectory Control Solar Radiation Pressure allows inward or outward Spiral Original orbit Sail Force Force Sail Shrinking orbit Expanding orbit Solar Sails Experience VERY Small Forces NASA Image 8 Solar Sail Missions Flown Image courtesy of Univ. Surrey NASA Image Image courtesy of JAXA Image courtesy of The Planetary Society NanoSail-D (2010) IKAROS (2010) LightSail-1 & 2 CanX-7 (2016) InflateSail (2017) NASA JAXA (2015/2019) Canada EU/Univ. of Surrey The Planetary Society Earth Orbit Interplanetary Earth Orbit Earth Orbit Deployment Only Full Flight Earth Orbit Deployment Only Deployment Only Deployment / Flight 3U CubeSat 315 kg Smallsat 3U CubeSat 3U CubeSat 10 m2 196 m2 3U CubeSat <10 m2 10 m2 32 m2 9 Planned Solar Sail Missions NASA Image NASA Image NASA Image Near Earth Asteroid Scout Advanced Composite Solar Solar Cruiser (2025) NASA (2021) NASA Sail System (TBD) NASA Interplanetary Interplanetary Earth Orbit Full Flight Full Flight Full Flight 100 kg spacecraft 6U CubeSat 12U CubeSat 1653 m2 86 -
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. -
Developing Technologies for Biological Experiments in Deep Space
Developing technologies for biological experiments in deep space Sergio R. Santa Maria Elizabeth Hawkins Ada Kanapskyte NASA Ames Research Center [email protected] NASA’s life science programs STS-1 (1981) STS-135 (2011) 1973 – 1974 1981 - 2011 2000 – 2006 – Space Shuttle International Skylab Bio CubeSats Program Space Station Microgravity effects - Nausea / vomit - Disorientation & sleep loss - Body fluid redistribution - Muscle & bone loss - Cardiovascular deconditioning - Increase pathogenicity in microbes Interplanetary space radiation What type of radiation are we going to encounter beyond low Earth orbit (LEO)? Galactic Cosmic Rays (GCRs): - Interplanetary, continuous, modulated by the 11-year solar cycle - High-energy protons and highly charged, energetic heavy particles (Fe-56, C-12) - Not effectively shielded; can break up into lighter, more penetrating pieces Challenges: biology effects poorly understood (but most hazardous) Interplanetary space radiation Solar Particle Events (SPEs) - Interplanetary, sporadic, transient (several min to days) - High proton fluxes (low and medium energy) - Largest doses occur during maximum solar activity Challenges: unpredictable; large doses in a short time Space radiation effects Space radiation is the # 1 risk to astronaut health on extended space exploration missions beyond the Earth’s magnetosphere • Immune system suppression, learning and memory impairment have been observed in animal models exposed to mission-relevant doses (Kennedy et al. 2011; Britten et al. 2012) • Low doses of space radiation are causative of an increased incidence and early appearance of cataracts in astronauts (Cuccinota et al. 2001) • Cardiovascular disease mortality rate among Apollo lunar astronauts is 4-5-fold higher than in non-flight and LEO astronauts (Delp et al. -
KPLO, ISECG, Et Al…
NationalNational Aeronautics Aeronautics and Space and Administration Space Administration KPLO, ISECG, et al… Ben Bussey Chief Exploration Scientist Human Exploration & Operations Mission Directorate, NASA HQ 1 Strategic Knowledge Gaps • SKGs define information that is useful/mandatory for designing human spaceflight architecture • Perception is that SKGs HAVE to be closed before we can go to a destination, i.e. they represent Requirements • In reality, there is very little information that is a MUST HAVE before we go somewhere with humans. What SKGs do is buy down risk, allowing you to design simpler/cheaper systems. • There are three flavors of SKGs 1. Have to have – Requirements 2. Buys down risk – LM foot pads 3. Mission enhancing – Resources • Four sets of SKGs – Moon, Phobos & Deimos, Mars, NEOs www.nasa.gov/exploration/library/skg.html 2 EM-1 Secondary Payloads 13 CUBESATS SELECTED TO FLY ON INTERIM EM-1 CRYOGENIC PROPULSION • Lunar Flashlight STAGE • Near Earth Asteroid Scout • Bio Sentinel • LunaH-MAP • CuSPP • Lunar IceCube • LunIR • EQUULEUS (JAXA) • OMOTENASHI (JAXA) • ArgoMoon (ESA) • STMD Centennial Challenge Winners 3 3 3 Lunar Flashlight Overview Looking for surface ice deposits and identifying favorable locations for in-situ utilization in lunar south pole cold traps Measurement Approach: • Lasers in 4 different near-IR bands illuminate the lunar surface with a 3° beam (1 km spot). Orbit: • Light reflected off the lunar • Elliptical: 20-9,000 km surface enters the spectrometer to • Orbit Period: 12 hrs distinguish water -
Payload Design for the Lunar Flashlight Mission
Lunar and Planetary Science XLVIII (2017) 1709.pdf Payload Design For The Lunar Flashlight Mission. B. A. Cohen1, P. O. Hayne2, B. T. Greenhagen3, D. A. Paige4, J. M. Camacho2, K. Crabtree5, C. Paine2, R. G. Sellar5; 1NASA Marshall Space Flight Center, Huntsville AL 35812 ([email protected]), 2Jet Propulsion Laboratory, Pasadena CA 91109, 3Applied Physics Laboratory, Johns Hopkins University, Laurel MD 20723, 4UCLA, Los Angeles, CA 90095, 5 Photon Engineering, Tucson AZ 85711. Introduction: Recent reflectance data from LRO lengths in rapid sequence, while a receiver system de- instruments suggest water ice and other volatiles may tects the reflected light. Derived reflectance and water be present on the surface in lunar permanently- ice band depths will be mapped onto the lunar surface shadowed regions, though the detection is not yet de- in order to identify locations where H2O ice is present finitive [1-3]. Understanding the composition, quanti- at or above 0.5 wt% concentration. ty, distribution, and form of water and other volatiles In the past year, we have advanced the design for associated with lunar permanently shadowed regions the Lunar Flashlight payload to meet our measurement (PSRs) is identified as a Strategic Knowledge Gap requirement within the limited mass and power availa- (SKG) for NASA’s human exploration program. These ble for the instrument system. We optimized the laser polar volatile deposits are also scientifically interest- wavelengths for maximum sensitivity to water ice ab- ing, having potential to reveal important information sorption bands. The selected wavelengths are 1.064 (- about the delivery of water to the Earth-Moon system. -
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. -
Theoretical and Experimental Investigation of Hall Thruster Miniaturization by Noah Zachary Warner
Theoretical and Experimental Investigation of Hall Thruster Miniaturization by Noah Zachary Warner S.B., Aeronautics and Astronautics, Massachusetts Institute of Technology, 2001 S.M., Aeronautics and Astronautics, Massachusetts Institute of Technology, 2003 SUBMITTED TO THE DEPARTMENT OF AERONAUTICS AND ASTRONAUTICS IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY AT THE MASSACHUSETTS INSTITUTE OF TECHNOLOGY JUNE 2007 © 2007 Massachusetts Institute of Technology. All rights reserved. Signature of Author . Department of Aeronautics and Astronautics May 25, 2007 Certified by . Manuel Martínez-Sánchez Professor of Aeronautics and Astronautics Thesis Supervisor Certified by . Jack Kerrebrock Professor Emeritus of Aeronautics and Astronautics Certified by . Oleg Batishchev Principal Research Scientist in Aeronautics and Astronautics Certified by . Vladimir Hruby President, Busek Company, Inc. Accepted by . Jaime Peraire Professor of Aeronautics and Astronautics Chair, Committee on Graduate Students 2 Theoretical and Experimental Investigation of Hall Thruster Miniaturization by Noah Zachary Warner Submitted to the Department of Aeronautics and Astronautics on May 25, 2007 in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Aeronautics and Astronautics in the field of Space Propulsion ABSTRACT Interest in small-scale space propulsion continues to grow with the increasing number of small satellite missions, particularly in the area of formation flight. Miniaturized Hall thrusters have been identified as a candidate for lightweight, high specific impulse propul- sion systems that can extend mission lifetime and payload capability. A set of scaling laws was developed that allows the dimensions and operating parameters of a miniaturized Hall thruster to be determined from an existing, technologically mature baseline design. -
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. -
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.