Chimera- a Low Cost Solution to Small Satellite Space Access

Total Page:16

File Type:pdf, Size:1020Kb

Chimera- a Low Cost Solution to Small Satellite Space Access Chimera- A Low Cost Solution to Small Satellite Space Access John Crowley, Virgil Hutchinson, Alex Keisner, Dave Young Mike Curry, Jonathan Jackson, John Maatsch, Pavel Piletsky Faculty Advisor: Dr. John Olds Georgia Institute of Technology Atlanta, GA 30332 Abstract Introduction The Chimera rocket was designed to enter the The small satellite market has been growing in small satellite market by offering an affordable and recent years. Interest ranges from the DoD to flexible alternative to the Pegasus launch vehicle. A universities wishing to launch scientific payloads. number of design concepts were evaluated, and one Current launch vehicles can provide services for was selected to undergo detailed analysis. This these organizations, but at a high cost. The Pegasus included disciplinary analyses in aerodynamics, launch vehicle, made by Orbital Sciences, can cost propulsion, trajectory, aeroheating, structures, $12M or higher1. weights, operations, and cost. The baseline vehicle, In many cases, universities cannot afford to pay consisting of a Minuteman 2-2 first stage, a PAM-S for a launch if it costs more than twice the cost of the second stage, and a new third stage carries a 100 and satellite that they built. Therefore they have sent out 50 kg payload to a 700 km altitude, at inclinations of an RFP to build a new low cost launcher that is 60° and 110° respectively. At this point a Monte particularly suited for their tastes. Launch altitudes Carlo Simulation was performed to determine how and inclinations are based on a survey of all the well the system met its price goals. The baseline previous launches made by universities. vehicle fails to meet the desired launch price of $5 The RFP details a business case. The item of million to a reasonable confidence level. However, interest is the price per launch paid for by the either the implementation of a cost reduction in the universities. The RFP calls for the launch costs to be cost of the first stage, or the infusion of appropriate $5M. Additionally, the notional start up company structural and propellant technologies in the design of must be able to show an internal rate of return of the third stage, help to make the desired launch price 10%. The company is also granted a loan from the viable. DoD of $500M to cover non-recurring costs. The company may use any US launch facility for a Nomenclature nominal fee of $50,000 per launch. Two design reference missions were detailed APAS Aerodynamic Preliminary Analysis within the RFP. The first was to send a 100 kg System payload to a 700 km, 60° orbit. The second mission DoD Department of Defense was to send a 50 kg payload to a 700 km, 110° orbit. DDT&E Design, Development, The constraints for the payloads were a 6 g axial load Testing & Evaluation and 2 g lateral load, and the payload could not be HABP Hypersonic Arbitrary Body exposed to a dynamic pressure of greater than 30 Pa. Program As a final note, the RFP said that US or foreign NPV Net Present Value parts could be utilized in the construction of the POST Program to Optimize launch vehicle. It was decided early in the project to Simulated Trajectories purchase most parts in order to reduce costs. RCS Reaction Control System RFP Request for Proposal Design Methodology ROSETTA Reduced Order Simulation for Evaluating Technologies The design team chose a methodology to explore and Transportation as many concepts as possible while maintaining Architectures creativity and technical feasibility. A brainstorming TFU Theoretical First Unit technique, known as a morphological matrix, was UDP Unified Distributed Panel used to look at all the possible characteristics of the vehicle. The first matrix was created to look at the 1 subsystem components and all the possible parts that Monte Carlo simulation. This is detailed in the final could fulfill them. The second matrix then combined, section of the report. through a structured selection process, these sub Config systems into eleven different concepts. Table 1 shows Virgil Aerodynamics the different types of concepts that were created John Propulsion through the morphological matrix. Dav Trajectory Mike Weights Table 1- System Concepts. & Sizing Pavel Aero- Type Number heating Balloon Assist 2 Alex Operations Alex Air Assist 3 Reliability John Cannon Assist 1 Economics MagLev Assist 1 Figure 1. Design Structure Matrix. Ground Launch 4 Disciplinary Analyses The design team then evaluated each of these qualitatively using TOPSIS. TOPSIS is an evaluation Aerodynamics method used to show how close a design is to the The stability and modicum of lift required during ideal solution. The higher the closeness value of a the atmospheric flight of the vehicle was provided by design, the better it is. The team evaluated these 11 four fins attached to the first stage of the vehicle. concepts using 19 criteria, each with a weight. These Due to the rocket’s release from the air-assist vehicle criteria and weights were developed through the use at a high flight path angle, it was assumed that the of a QFD. use of a wing to provide lift for pull-up was not The QFD maps the customer requirements and required. Each of the four fins is 1.38 meters in engineering characteristics through a relationship length, has an area of 0.679 m2, and is arranged at 35 matrix. In this matrix each of the requirements and degrees from the center neutral axis. This characteristics are rated as to how each affects the asymmetric arrangement of the fins allowed for a other based on a 1-3-9 scale. If they have a strong small increment of lift to be provided to the rocket affect on each other (i.e. cost and weight), they are along with providing stability through the first stage given a 9. The QFD then multiplies these numbers of flight. with the customer requirement importance values and The Aerodynamic Preliminary Analysis System determines a relative importance value. This (APAS), a combination of three individual programs, importance value was used as the weighting, and the was utilized in performing the aerodynamic analysis engineering characteristics were used as the criterion. of the vehicle. APAS was used to define the vehicle The TOPSIS analysis determined the ranking of geometry at each stage of flight and initialize the each of these concepts. The top two designs were a 4- analysis runs, which were based on altitude, velocity, stage ground launch vehicle and a 3-stage air assist and angle of attack. After defining the geometry and launch. analyses, the Unified Distributed Panel (UDP) These vehicles were then designed and sized program performed the subsonic and supersonic using the appropriate disciplines as seen in Figure 1. aerodynamic analysis and the Hypersonic Arbitrary The data obtained from this analysis was then fed Body Program (HABP) was used to conduct the back into TOPSIS so the final two designs could be hypersonic analysis. UDP’s analysis is based on evaluated quantitatively. The initial cost estimate of slender body theory and source and vortex panel the air assist launch was found to be approximately methods while HABP’s analysis is based on impact $9.5M and the ground launch cost estimate was theory. Aerodynamic analysis was only performed approximately $10.9M. TOPSIS ranked the air assist on the vehicle configuration from launch to payload launch as the best vehicle to use. This was confirmed fairing separation because all aerodynamic by the launch price and an evaluation by the team of coefficients were constant above an altitude of 100 the designs. The air assist launch was chosen to be km3. designed at a higher level of fidelity. The following The resulting data from the aerodynamic sections outline the results of the disciplinary analyses showed that during subsonic and sonic analyses. These analyses were performed as the flight, the fins have a lift coefficient of 0.175, which following Design Structure Matrix indicates. indicates their provision of a small increment of lift A probabilistic study was then performed on the to aid in the pull-up of the rocket. The variation of design with the help of a ROSETTA model and a zero-lift drag coefficient with Mach number for the 2 aerodynamic performance of the vehicle provided by above, both the first two stages as well as the air APAS is shown in Figure 2. launch aircraft will be existing flight hardware to 1.8 limit costs. 1.6 Table 2 – Specification of Third Stage Motor. 1.4 Stage 1 Thrust 2669 N 1.2 Isp 295 sec 1 Stage 2 d,0 C 0.8 Burn Time 33.4 sec 0.6 Exit Area 0.152 m2 0.4 Expansion Ratio 50 0.2 Propellant Mass 30.8 kg 0 Motor Mass 6.63 kg 0 1 2 3 4 5 6 7 8 9 10 Mach Number Motor Volume 0.0195 m3 Figure 2. Variation of zero-lift drag coefficient with Mach number. A list of nine possible aircraft was compiled with the flight envelope of each aircraft. From this list Propulsion three separate aircraft were chosen that seemed to Even so, buying pre-existing stages and cover the entire flight regime that is to be developing as little as possible is the surest way to investigated. These aircraft are compiled in Table 3. reduce costs and uncertainty, and thus increase the From these three and an initial investigation of chances of reaching the price goals set forth in the trajectories in POST it was determined that the B-52 RFP. Therefore, the first two stages were set as resulted in an appropriately sized rocket (to fit existing solid rocket motor stages, and only the third beneath the aircraft).
Recommended publications
  • Gnc 2021 Abstract Book
    GNC 2021 ABSTRACT BOOK Contents GNC Posters ................................................................................................................................................... 7 Poster 01: A Software Defined Radio Galileo and GPS SW receiver for real-time on-board Navigation for space missions ................................................................................................................................................. 7 Poster 02: JUICE Navigation camera design .................................................................................................... 9 Poster 03: PRESENTATION AND PERFORMANCES OF MULTI-CONSTELLATION GNSS ORBITAL NAVIGATION LIBRARY BOLERO ........................................................................................................................................... 10 Poster 05: EROSS Project - GNC architecture design for autonomous robotic On-Orbit Servicing .............. 12 Poster 06: Performance assessment of a multispectral sensor for relative navigation ............................... 14 Poster 07: Validation of Astrix 1090A IMU for interplanetary and landing missions ................................... 16 Poster 08: High Performance Control System Architecture with an Output Regulation Theory-based Controller and Two-Stage Optimal Observer for the Fine Pointing of Large Scientific Satellites ................. 18 Poster 09: Development of High-Precision GPSR Applicable to GEO and GTO-to-GEO Transfer ................. 20 Poster 10: P4COM: ESA Pointing Error Engineering
    [Show full text]
  • Digital Tracking Observations Can Discover Asteroids Ten Times
    Digital Tracking Observations Can Discover Asteroids Ten Times Fainter than Conventional Searches Aren N. Heinze1,2, Stanimir Metchev3,4,1, and Joseph Trollo3 ABSTRACT We describe digital tracking, a method for asteroid searches that greatly increases the sensitivity of a telescope to faint unknown asteroids. It has been previously used to detect faint Kuiper Belt objects using the Hubble Space Telescope and large ground- based instruments, and to find a small, fast-moving asteroid during a close approach to Earth. We complement this earlier work by developing digital tracking methodology for detecting asteroids using large-format CCD imagers. We demonstrate that the tech- nique enables the ground-based detection of large numbers of new faint asteroids. Our methodology resolves or circumvents all major obstacles to the large-scale application of digital tracking for finding main belt and near-Earth asteroids. We find that for both asteroid populations, digital tracking can deliver a factor of ten improvement over conventional searches. Digital tracking has long been standard practice for deep Kuiper Belt surveys, but even there our methodology enables deeper integrations than have yet been attempted. Our search for main belt asteroids using a one-degree imager on the 0.9m WIYN telescope on Kitt Peak validates our methodology, delivers sensitivity to asteroids in a regime previously probed only with 4-meter and larger instruments, and leads to the detection of 156 previously unknown asteroids and 59 known objects in a single field. Digital tracking has the potential to revolutionize searches for faint moving objects ranging from the Kuiper Belt through main belt and near-Earth asteroids, and perhaps even anthropogenic space debris in low Earth orbit.
    [Show full text]
  • Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA
    University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 8-2012 Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA Merek Austin Chertkow University of Tennessee, Knoxville, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Part of the Other Astrophysics and Astronomy Commons Recommended Citation Chertkow, Merek Austin, "Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA. " PhD diss., University of Tennessee, 2012. https://trace.tennessee.edu/utk_graddiss/1463 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Merek Austin Chertkow entitled "Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Physics. William Hix, Major Professor We have read this dissertation and recommend its acceptance: Kate Jones, Mike Guidry, Robert, Hinde Accepted for the Council: Carolyn R. Hodges Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Merek Austin Chertkow August 2012 c by Merek Austin Chertkow, 2012 All Rights Reserved.
    [Show full text]
  • FINAL PROGRAM #Aiaascitech
    4–8 JANUARY 2016 SAN DIEGO, CA The Largest Event for Aerospace Research, Development, and Technology FINAL PROGRAM www.aiaa-SciTech.org #aiaaSciTech 16-928 WHAT’S IMPOSSIBLE TODAY WON’T BE TOMORROW. AT LOCKHEED MARTIN, WE’RE ENGINEERING A BETTER TOMORROW. We are partnering with our customers to accelerate manufacturing innovation from the laboratory to production. We push the limits in additive manufacturing, advanced materials, digital manufacturing and next generation electronics. Whether it is solving a global crisis like the need for clean drinking water or travelling even deeper into space, advanced manufacturing is opening the doors to the next great human revolution. Learn more at lockheedmartin.com © 2014 LOCKHEED MARTIN CORPORATION VC377_164 Executive Steering Committee AIAA SciTech 2016 2O16 Welcome Welcome to the AIAA Science and Technology Forum and Exposition 2016 (AIAA SciTech 2016) – the world’s largest event for aerospace research, development, and technology. We are confident that you will come away from San Diego inspired and with the tools necessary to continue shaping the future of aerospace in new and exciting ways. From hearing preeminent industry thought leaders, to attending sessions where cutting- edge research will be unveiled, to interacting with peers – this will be a most fulfilling week! Our organizing committee has worked hard over the past year to ensure that our plenary sessions examine the most critical issues facing aerospace today, such as aerospace science and Richard George Lesieutre technology policy, lessons learned from a half century of aerospace innovation, resilient design, Christiansen The Pennsylvania and unmanned aerial systems. We will also focus on how AIAA and other stakeholders in State University Sierra Lobo, Inc.
    [Show full text]
  • Destination Dwarf Planets: a Panel Discussion
    Destination Dwarf Planets: A Panel Discussion OPAG, August 2019 Convened: Orkan Umurhan (SETI/NASA-ARC) Co-Panelists: Walt Harris (LPL, UA) Kathleen Mandt (JHUAPL) Alan Stern (SWRI) Dwarf Planets/KBO: a rogues gallery Triton Unifying Story for these bodies awaits Perihelio n/ Diamet Aphelion DocumentGoals 09.2018) from OPAG (Taken Name Surface characteristics Other observations/ hypotheses Moons er (km) /Current Distance (AU) Eris ~2326 P=38 Appears almost white, albedo of 0.96, higher Largest KBO by mass second Dysnomia A=98 than any other large Solar System body except by size. Models of internal C=96 Enceledus. Methane ice appears to be quite radioactive decay indicate evenly spread over the surface that a subsurface water ocean may be stable Haumea ~1600 P=35 Displays a white surface with an albedo of 0.6- Is a triaxial ellipsoid, with its Hi’iaka and A=51 0.8 , and a large, dark red area . Surface shows major axis twice as long as Namaka C=51 the presence of crystalline water ice (66%-80%) , the minor. Rapid rotation (~4 but no methane, and may have undergone hrs), high density, and high resurfacing in the last 10 Myr. Hydrogen cyanide, albedo may be the result of a phyllosilicate clays, and inorganic cyanide salts giant collision. Has the only may be present , but organics are no more than ring system known for a TNO. 8% 2007 OR10 ~1535 P=33 Amongst the reddest objects known, perhaps due May retain a thin methane S/(225088) A=101 to the abundant presence of methane frosts atmosphere 1 C=87 (tholins?) across the surface.Surface also show the presence of water ice.
    [Show full text]
  • By S. Alan Stern Mission to the Centaurs
    MISSION TO THE OUTER SOLAR SYSTEM p. 24 MARCH 2021 The world’s best-selling astronomy magazine GHowIA to growN aT BLACK HOLE p. 16 www.Astronomy.com $6.99 03 Vol. p. 46 49 COMPLETE GUIDE TO MOON FILTERS • + Issue 3 Unistellar’s unique scope tested p. 58 0 742 8 001096 9 Grab-and-go astroimaging p. 52 MISSION TO THE CENTAURS Planetary scientists are planning a blockbuster mission to an exotic world that’s escaped from the Kuiper Belt. BY S. ALAN STERN 22 October 2038: Centaurus crossed that billion miles from Earth to Chiron to make the first reconnais- After a journey of over a billion miles to the sance of this amazing outer solar system outer solar system, the Centaurus spacecraft world. Once all the precious images and spec- is on final approach. Dead ahead lies Chiron, tra are collected to turn Chiron from a point a mini-planet orbiting between Uranus and of light into a real place, Centaurus will Saturn. transmit them back to its international sci- A native of the Kuiper Belt formed over ence team, the most diverse ever assembled 4 billion years ago, Chiron was recently (at for any solar system mission. least in astronomical terms) What lies ahead for gravitationally dislodged from Centaurus on final there and tossed into its cur- approach to Chiron? Raw rent closer climes. Exploring exploration, fundamental it is now much easier than if discoveries, and the honor it were still in the Kuiper Belt, of being the first to visit over three times farther away.
    [Show full text]
  • The Origins of the Discovery Program, 1989-1993
    Space Policy 30 (2014) 5e12 Contents lists available at ScienceDirect Space Policy journal homepage: www.elsevier.com/locate/spacepol Transforming solar system exploration: The origins of the Discovery Program, 1989e1993 Michael J. Neufeld National Air and Space Museum, Smithsonian Institution, United States article info abstract Article history: The Discovery Program is a rarity in the history of NASA solar system exploration: a reform program that Received 18 October 2013 has survived and continued to be influential. This article examines its emergence between 1989 and Accepted 18 October 2013 1993, largely as the result of the intervention of two people: Stamatios “Tom” Krimigis of the Johns Available online 19 April 2014 Hopkins University Applied Physics Laboratory (APL), and Wesley Huntress of NASA, who was Division Director of Solar System Exploration 1990e92 and the Associate Administrator for Space Science 1992 Keywords: e98. Krimigis drew on his leadership experience in the space physics community and his knowledge of Space history its Explorer program to propose that it was possible to create new missions to the inner solar system for a NASA Space programme organization fraction of the existing costs. He continued to push that idea for the next two years, but it took the influence of Huntress at NASA Headquarters to push it on to the agenda. Huntress explicitly decided to use APL to force change on the Jet Propulsion Laboratory and the planetary science community. He succeeded in moving the JPL Mars Pathfinder and APL Near Earth Asteroid Rendezvous (NEAR) mission proposals forward as the opening missions for Discovery. But it took Krimigis’s political skill and access to Sen.
    [Show full text]
  • Book of Abstracts to Dowload
    ABSTRACT BOOK 1 TABLE OF CONTENTS Summary ........................................................................................................................................... 5 Committees ......................................................................................................................................19 Agenda ............................................................................................................................................22 List of participants ............................................................................................................................ 25 Abstracts - Day 1 - Sessions 1-2 ...............................................................................................27 Solar system-exoplanet synergies - general approach and programmatic land-scape, Rauer Heike........................................................................................................................................................................28 Horizon 2061, from overarching science goal to specific science objectives, Michel Blanc...........................................................................................................................................................................29 Formation and Orbital Evolution of Young Planetary Systems, Baruteau Clément.....31 Composition and Interior structure of solar and extrasolar giant planets, Nettelmenn Nadine [et al.].......................................................................................................................................32
    [Show full text]
  • Global Challenges
    6–10 JANUARY 2020 | ORLANDO, FL DRIVING AEROSPACE SOLUTIONS FOR GLOBAL CHALLENGES What’s going on in Page 25 aiaa.org/scitech #aiaaSciTech From the forefront of innovation to the frontlines of the mission. No matter the mission, Lockheed Martin uses a proven approach: engineer with purpose, innovate with passion and define the future. We take time to understand our customer’s challenges and provide solutions that help them keep the world secure. Their mission defines our purpose. Learn more at lockheedmartin.com. © 2019 Lockheed Martin Corporation FG19-23960_002 AIAA sponsorship.indd 1 12/10/19 3:20 PM Live: n/a Trim: H: 8.5in W: 11in Job Number: FG18-23208_002 Bleed: .25 all around Designer: Kevin Gray Publication: AIAA Sponsorship Gutter: None Communicator: Ryan Alford Visual: Male and female in front of screens. Resolution: 300 DPI Due Date: 12/10/19 Country: USA Density: 300 Color Space: CMYK NETWORK NAME: SciTech ON-SITE Wi-Fi From the forefront of innovation › PASSWORD: 2020scitech to the frontlines of the mission. CONTENTS Technical Program Committee .................................................................4 Welcome ........................................................................................................5 Sponsors and Supporters ..........................................................................7 Forum Overview ...........................................................................................8 Pre-Forum Activities .................................................................................
    [Show full text]
  • Poster Session 2 17:30 - 18:00 Tuesday, 6Th July, 2021 Sessions Poster Session
    Poster Session 2 17:30 - 18:00 Tuesday, 6th July, 2021 Sessions Poster Session 17:30 - 17:31 9 Skin Image Analysis in Contact Capacitive Imaging and High Resolution Ultrasound Imaging Mr Christos Bontozoglou1, Dr Xu Zhang2, Mrs Elena Chirikhina1, Dr Perry Xiao1 1London South Bank University, London, United Kingdom. 2Tongjing Zhejiang College, Jiaxing, China Abstract Text We present our latest research on skin image analysis in Contact Capacitive Imaging and High Resolution Ultrasound Imaging. Contact Capacitive Imaging is a novel imaging technique that can be used for in-vivo skin measurements [1-3]. With Contact Capacitive Imaging, we can analyze the skin water content, skin solvent penetrations, skin texture, and skin micro-relief analysis by mathematical algorithms and machine learning. High Resolution Ultrasound Imaging is the state of the art technology, and can produces high resolution images of the skin and superficial soft tissue to a vertical resolution of about 40 microns [4]. With High Resolution Ultrasound Imaging, we have studies the differences of different layers, such as stratum corneum, epidermis and dermis, around the different locations on the face and around different body parts. In this paper, we will first present the Contact Capacitive Imaging technology and High Resolution Ultrasound Imaging technique, then present the analyzed experimental results and discussions. Keywords Skin image analysis, capacitive imaging, high resolution ultrasound, machine learning, skin water content, skin solvent penetration, skin texture, skin thickness. References 1. Ou, X., Pan, W., Xiao, P., In vivo skin capacitive imaging analysis by using grey level co-occurrence matrix (GLCM), International journal of pharmaceutics 460 (1-2), 28-32, 2014.
    [Show full text]
  • OSIRIS-Rex Contamination Control Strategy and Implementation
    Space Sci Rev (2018) 214:19 DOI 10.1007/s11214-017-0439-4 OSIRIS-REx Contamination Control Strategy and Implementation J.P. Dworkin1 L.A. Adelman1,2 T. Ajluni1,2 A.V. Andronikov3 J.C. Aponte1,4 A.E. Bartels1 ·E. Beshore5 E.B.· Bierhaus6 J.R.· Brucato7 B.H.· Bryan6 · A.S. Burton8 ·M.P. Callahan· 9 S.L. Castro-Wallace· 8 B.C.· Clark10 S.J. Clemett· 8,11 H.C. Connolly· Jr.12 W.E. Cutlip· 1 S.M. Daly13 V. E .· E l l i o t t 1 J.E. Elsila· 1 · H.L. Enos5 D.F. Everett· 1 I.A. Franchi· 14 D.P.· Glavin1 H.V.· Graham1,15 · J.E. Hendershot· 1,16 J.W. Harris· 6 S.L. Hill· 11,13 A.R. Hildebrand· 17 G.O.· Jayne1,2 R.W. Jenkens Jr.1 K.S.· Johnson6 · J.S. Kirsch11,13· D.S. Lauretta5 A.S.· Lewis1 · J.J. Loiacono1 C.C.· Lorentson1 J.R.· Marshall18 ·M.G. Martin1,4 · · L.L. Matthias13,19· H.L. McLain1,4· S.R. Messenger· 8 R.G. Mink1 ·J.L. Moore6 K. Nakamura-Messenger· 8 J.A. Nuth· III1 C.V. Owens· 13 C.L. Parish· 6 · B.D. Perkins13 M.S. Pryzby· 1,20 C.A. Reigle· 6 K. Righter·8 B. Rizk5 J.F.· Russell6 S.A. Sandford21· J.P. Schepis1 J.· Songer6 M.F.· Sovinski1 ·S.E. Stahl·8,22 · K. Thomas-Keprta· 8,11 J.M. Vellinga· 6 M.S.· Walker1 · · · · Received: 6 April 2017 / Accepted: 27 October 2017 ©SpringerScience+BusinessMediaB.V.,partofSpringerNature2017(outsidetheUSA)2017 Abstract OSIRIS-REx will return pristine samples of carbonaceous asteroid Bennu.
    [Show full text]
  • Consumer Goods
    National Aeronautics and Space Administration National Aeronautics and Space Administration spinoff Office of the Chief Technologist NASA Headquarters Washington, DC 20546 www.nasa.gov NP-2018-08-2611-HQ 2019 Technology Transfer Program NASA Headquarters Daniel Lockney, Technology Transfer Program Executive Spinoff Program Office Goddard Space Flight Center Daniel Coleman, Editor-in-Chief Mike DiCicco, Senior Science Writer Naomi Seck, Senior Science Writer John Jones, Senior Graphics Designer This 2018 NASA photograph captured the International Rebecca Carroll, Contributing Writer Space Station in silhouette as it transited the Moon. TABLE OF CONTENTS 5 Foreword 7 Introduction 8 Executive Summary 20 NASA Technologies Benefiting Society 156 Spinoffs of Tomorrow 178 Technology Transfer Program 66 DEPARTMENTS 37 HEALTH AND MEDICINE TRANSPORTATION PUBLIC SAFETY CONSUMER GOODS 24 Unique Polymer Finds Widespread 40 Battery Innovations Power 58 NASA Brings Accuracy to World’s 84 Bowflex System Spurs Revolution in Use in Heart Devices All-Electric Aircraft Global Positioning Systems Home Fitness 27 Material for Mars Makes Life- 43 Shuttle Tire Sensors Warn Drivers of 63 Gas Regulators Keep Pilots Breathing 87 Spacesuit Air Filters Eliminate Household Saving Sutures Flat Tires Pet Odors 66 RoboMantis Offers to Take Over 30 Fluorescent Paints Spot DNA 46 Space-Age Insulator Evolves to Dangerous Missions 89 NASA Research Sends Video Game Players Damage from Radiation, Gene Editing Replace Plastic and Save Weight on a Journey to Mars SPINOFFS 70
    [Show full text]