Mars Aerocapture Systems Study

Total Page:16

File Type:pdf, Size:1020Kb

Mars Aerocapture Systems Study NASA/TM-2006-214522 Mars Aerocapture Systems Study Henry S. Wright Langley Research Center, Hampton, Virginia David Y. Oh Jet Propulsion Laboratory, Pasadena, California Carlos H. Westhelle Johnson Space Center, Houston, Texas Jody L. Fisher National Institute of Aerospace, Hampton, Virginia R. Eric Dyke Swales Aerospace, Hampton, Virginia Karl T. Edquist Langley Research Center, Hampton, Virginia James L. Brown Ames Research Center, Hampton, Virginia Hilary L. Justh Marshall Space Flight Center, Huntsville, Alabama Michelle M. Munk Marshall Space Flight Center, Huntsville, Alabama November 2006 The NASA STI Program Office . in Profile Since its founding, NASA has been dedicated to the • CONFERENCE PUBLICATION. Collected advancement of aeronautics and space science. The papers from scientific and technical NASA Scientific and Technical Information (STI) conferences, symposia, seminars, or other Program Office plays a key part in helping NASA meetings sponsored or co-sponsored by NASA. maintain this important role. • SPECIAL PUBLICATION. Scientific, The NASA STI Program Office is operated by technical, or historical information from NASA Langley Research Center, the lead center for NASA’s programs, projects, and missions, often scientific and technical information. The NASA STI concerned with subjects having substantial Program Office provides access to the NASA STI public interest. Database, the largest collection of aeronautical and space science STI in the world. The Program Office is • TECHNICAL TRANSLATION. English- also NASA’s institutional mechanism for language translations of foreign scientific and disseminating the results of its research and technical material pertinent to NASA’s mission. development activities. These results are published by NASA in the NASA STI Report Series, which Specialized services that complement the STI includes the following report types: Program Office’s diverse offerings include creating custom thesauri, building customized databases, • TECHNICAL PUBLICATION. Reports of organizing and publishing research results ... even completed research or a major significant phase providing videos. of research that present the results of NASA programs and include extensive data or For more information about the NASA STI Program theoretical analysis. Includes compilations of Office, see the following: significant scientific and technical data and information deemed to be of continuing • Access the NASA STI Program Home Page at reference value. NASA counterpart of peer- http://www.sti.nasa.gov reviewed formal professional papers, but having less stringent limitations on manuscript length • E-mail your question via the Internet to and extent of graphic presentations. [email protected] • TECHNICAL MEMORANDUM. Scientific • Fax your question to the NASA STI Help Desk and technical findings that are preliminary or of at (301) 621-0134 specialized interest, e.g., quick release reports, working papers, and bibliographies that contain minimal annotation. Does not contain extensive • Phone the NASA STI Help Desk at analysis. (301) 621-0390 • CONTRACTOR REPORT. Scientific and • Write to: technical findings by NASA-sponsored NASA STI Help Desk contractors and grantees. NASA Center for AeroSpace Information 7121 Standard Drive Hanover, MD 21076-1320 NASA/TM-2006-214522 Mars Aerocapture Systems Study Henry S. Wright Langley Research Center, Hampton, Virginia David Y. Oh Jet Propulsion Laboratory, Pasadena, California Carlos H. Westhelle Johnson Space Center, Houston, Texas Jody L. Fisher National Institute of Aerospace, Hampton, Virginia R. Eric Dyke Swales Aerospace, Hampton, Virginia Karl T. Edquist Langley Research Center, Hampton, Virginia James L. Brown Ames Research Center, Hampton, Virginia Hilary L. Justh Marshall Space Flight Center, Huntsville, Alabama Michelle M. Munk Marshall Space Flight Center, Huntsville, Alabama National Aeronautics and Space Administration Langley Research Center Hampton, Virginia 23681-2199 November 2006 Available from: NASA Center for AeroSpace Information (CASI) National Technical Information Service (NTIS) 7121 Standard Drive 5285 Port Royal Road Hanover, MD 21076-1320 Springfield, VA 22161-2171 (301) 621-0390 (703) 605-6000 Contents Contents............................................................................................................................................................................... i List of Tables ..................................................................................................................................................................... ii List of Figures ................................................................................................................................................................... iii Introduction........................................................................................................................................................................ 1 Symbols and Abbreviations .............................................................................................................................................. 2 Study Overview ................................................................................................................................................................. 5 MASS Problem Statement ............................................................................................................................................ 5 Aerocapture Assumptions............................................................................................................................................. 5 Study Programmatics .................................................................................................................................................... 6 Summary Results........................................................................................................................................................... 6 Comparison to Other Aeropass Missions ................................................................................................................ 6 Comparison to an All-Propulsive Option ................................................................................................................ 7 Mission Analysis ............................................................................................................................................................... 7 Mission Assessment ...................................................................................................................................................... 7 Constraints ................................................................................................................................................................. 8 Investigation of the Opportunities............................................................................................................................ 9 Baseline Mission Architecture.................................................................................................................................... 10 Arrival State (Arrival Navigation).............................................................................................................................. 11 Aerocapture Process ........................................................................................................................................................ 12 Modeling of the Atmosphere of Mars ............................................................................................................................ 12 Mars Global Reference Atmospheric Model (Mars-GRAM)................................................................................... 12 Mars-GRAM Auxiliary Profiles from Observed Data.............................................................................................. 13 Configuration and Aerodynamics................................................................................................................................... 13 Aeroshell Configuration Basis (60° vs 70° Sphere Cone) ........................................................................................ 13 Aerodynamics .............................................................................................................................................................. 14 Guidance and Integrated Trajectory Performance......................................................................................................... 15 HYPAS Guidance........................................................................................................................................................ 15 POST2 Trajectory Simulation .................................................................................................................................... 16 Simulation Results and Performance ......................................................................................................................... 16 Aeroheating Environment ............................................................................................................................................... 17 Forebody Heating Environments................................................................................................................................18 Afterbody Heating Environments............................................................................................................................... 18 Radiative
Recommended publications
  • MARS SCIENCE LABORATORY ORBIT DETERMINATION Gerhard L. Kruizinga(1)
    MARS SCIENCE LABORATORY ORBIT DETERMINATION Gerhard L. Kruizinga(1), Eric D. Gustafson(2), Paul F. Thompson(3), David C. Jefferson(4), Tomas J. Martin-Mur(5), Neil A. Mottinger(6), Frederic J. Pelletier(7), and Mark S. Ryne(8) (1-8)Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, +1-818-354-7060, fGerhard.L.Kruizinga, edg, Paul.F.Thompson, David.C.Jefferson, tmur, Neil.A.Mottinger, Fred.Pelletier, [email protected] Abstract: This paper describes the orbit determination process, results and filter strategies used by the Mars Science Laboratory Navigation Team during cruise from Earth to Mars. The new atmospheric entry guidance system resulted in an orbit determination paradigm shift during final approach when compared to previous Mars lander missions. The evolving orbit determination filter strategies during cruise are presented. Furthermore, results of calibration activities of dynamical models are presented. The atmospheric entry interface trajectory knowledge was significantly better than the original requirements, which enabled the very precise landing in Gale Crater. Keywords: Mars Science Laboratory, Curiosity, Mars, Navigation, Orbit Determination 1. Introduction On August 6, 2012, the Mars Science Laboratory (MSL) and the Curiosity rover successful performed a precision landing in Gale Crater on Mars. A crucial part of the success was orbit determination (OD) during the cruise from Earth to Mars. The OD process involves determining the spacecraft state, predicting the future trajectory and characterizing the uncertainty associated with the predicted trajectory. This paper describes the orbit determination process, results, and unique challenges during the final approach phase.
    [Show full text]
  • IMU/MCAV Integrated Navigation for the Powered Descent Phase Of
    Overview of Chinese Current Efforts for Mars Probe Design Xiuqiang Jiang1,2, Ting Tao1,2 and Shuang Li1,2 1. College of Astronautics, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, China 2. Space New Technology Laboratory, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, China Email: [email protected], [email protected] Abstract Mars exploration activities have gathered scientific data and deepened the current understanding about the Martian evolution process and living environment. As a terrestrial planet, Mars is also an excellent proving ground of some innovative special-purpose aerospace technologies. In the U.S., Soviet Union (Russia), Europe, and India, missions sending spacecraft to explore Mars currently exist, and the first three have landed their spacecrafts on the surface of Mars. China has programmed five Mars landing missions in next 20 years, and some critical technologies for Mars landing mission have been studied beforehand. In this paper, we will report Chinese Mars exploration mission scenario and the latest progress in dynamics study and guidance navigation and control (GNC) system design for Chinese first Mars probe. Some elementary design rules and index will be described according to simulation experiments, analysis and survey. Several new coping strategies will be proposed to be competent for the challenges of the Mars entry descent and landing (EDL) dynamics process. Details of the work, the supporting data and preliminary conclusions of the investigation will be presented. Based on our current efforts, one candidate system configuration architecture of Chinese first Mars probe will be shown and elaborated in the end. United States launched the “Mars Pathfinder (MPF)” 1.
    [Show full text]
  • An Assessment of Aerocapture and Applications to Future Missions
    Post-Exit Atmospheric Flight Cruise Approach An Assessment of Aerocapture and Applications to Future Missions February 13, 2016 National Aeronautics and Space Administration An Assessment of Aerocapture Jet Propulsion Laboratory California Institute of Technology Pasadena, California and Applications to Future Missions Jet Propulsion Laboratory, California Institute of Technology for Planetary Science Division Science Mission Directorate NASA Work Performed under the Planetary Science Program Support Task ©2016. All rights reserved. D-97058 February 13, 2016 Authors Thomas R. Spilker, Independent Consultant Mark Hofstadter Chester S. Borden, JPL/Caltech Jessie M. Kawata Mark Adler, JPL/Caltech Damon Landau Michelle M. Munk, LaRC Daniel T. Lyons Richard W. Powell, LaRC Kim R. Reh Robert D. Braun, GIT Randii R. Wessen Patricia M. Beauchamp, JPL/Caltech NASA Ames Research Center James A. Cutts, JPL/Caltech Parul Agrawal Paul F. Wercinski, ARC Helen H. Hwang and the A-Team Paul F. Wercinski NASA Langley Research Center F. McNeil Cheatwood A-Team Study Participants Jeffrey A. Herath Jet Propulsion Laboratory, Caltech Michelle M. Munk Mark Adler Richard W. Powell Nitin Arora Johnson Space Center Patricia M. Beauchamp Ronald R. Sostaric Chester S. Borden Independent Consultant James A. Cutts Thomas R. Spilker Gregory L. Davis Georgia Institute of Technology John O. Elliott Prof. Robert D. Braun – External Reviewer Jefferey L. Hall Engineering and Science Directorate JPL D-97058 Foreword Aerocapture has been proposed for several missions over the last couple of decades, and the technologies have matured over time. This study was initiated because the NASA Planetary Science Division (PSD) had not revisited Aerocapture technologies for about a decade and with the upcoming study to send a mission to Uranus/Neptune initiated by the PSD we needed to determine the status of the technologies and assess their readiness for such a mission.
    [Show full text]
  • Gravity-Assist Trajectories to Jupiter Using Nuclear Electric Propulsion
    AAS 05-398 Gravity-Assist Trajectories to Jupiter Using Nuclear Electric Propulsion ∗ ϒ Daniel W. Parcher ∗∗ and Jon A. Sims ϒϒ This paper examines optimal low-thrust gravity-assist trajectories to Jupiter using nuclear electric propulsion. Three different Venus-Earth Gravity Assist (VEGA) types are presented and compared to other gravity-assist trajectories using combinations of Earth, Venus, and Mars. Families of solutions for a given gravity-assist combination are differentiated by the approximate transfer resonance or number of heliocentric revolutions between flybys and by the flyby types. Trajectories that minimize initial injection energy by using low resonance transfers or additional heliocentric revolutions on the first leg of the trajectory offer the most delivered mass given sufficient flight time. Trajectory families that use only Earth gravity assists offer the most delivered mass at most flight times examined, and are available frequently with little variation in performance. However, at least one of the VEGA trajectory types is among the top performers at all of the flight times considered. INTRODUCTION The use of planetary gravity assists is a proven technique to improve the performance of interplanetary trajectories as exemplified by the Voyager, Galileo, and Cassini missions. Another proven technique for enhancing the performance of space missions is the use of highly efficient electric propulsion systems. Electric propulsion can be used to increase the mass delivered to the destination and/or reduce the trip time over typical chemical propulsion systems.1,2 This technology has been demonstrated on the Deep Space 1 mission 3 − part of NASA’s New Millennium Program to validate technologies which can lower the cost and risk and enhance the performance of future missions.
    [Show full text]
  • Space Vehicle Conceptual Design Blue Team March 20, 2021
    Hephaestus: Space Vehicle Conceptual Design Blue team March 20, 2021 Connor Cruickshank, Joel Lundahl, Birgir Steinn Hermannsson, Greta Tartaglia M.Sc. students, KTH Royal Institute of Technology, Stockholm, Sweden Abstract—A hypothetical contest has been issued to summit ms Structural mass Olympus Mons. This report details a conceptual design of a space P Power vehicle intended for that purpose. Functional requirements of the p Combustion chamber pressure vehicle were defined, and the primary subsystems identified. The 02 SpaceX Starship was chosen to serve as a design baseline and pe Exhaust gas exit pressure a comparison of suitable launch vehicles was made. Subsystems S Drag surface such as propulsion, reaction control, power generation, thermal T Thrust management and radiation shielding were considered, as well as ue Exhaust gas exit velocity interior design of the space vehicle and its protection measures W Weight for Mars entry and activities. The consequences of an engine-out scenario were studied. t Metric tonne The Starship launch system was deemed the most suitable launch vehicle candidate. Six Raptor engines were selected for the spacecraft main propulsion system, with 8 smaller thrusters I. INTRODUCTION for reaction control. A radiator mass of 890 kg was estimated In the year 2038 a challenge was issued for a team of for the thermal management system, and lithium metal hydride was determined an adequate radiation shielding material for the pioneers to be the first to reach the peak of Olympus Mons, the crew quarters. A radiation shelter was integrated into the pantry, highest mountain in the solar system. The reward for the first to and layouts of the crew quarters and cargo bay were prepared.
    [Show full text]
  • Study of a Crew Transfer Vehicle Using Aerocapture for Cycler Based Exploration of Mars by Larissa Balestrero Machado a Thesis S
    Study of a Crew Transfer Vehicle Using Aerocapture for Cycler Based Exploration of Mars by Larissa Balestrero Machado A thesis submitted to the College of Engineering and Science of Florida Institute of Technology in partial fulfillment of the requirements for the degree of Master of Science in Aerospace Engineering Melbourne, Florida May, 2019 © Copyright 2019 Larissa Balestrero Machado. All Rights Reserved The author grants permission to make single copies ____________________ We the undersigned committee hereby approve the attached thesis, “Study of a Crew Transfer Vehicle Using Aerocapture for Cycler Based Exploration of Mars,” by Larissa Balestrero Machado. _________________________________________________ Markus Wilde, PhD Assistant Professor Department of Aerospace, Physics and Space Sciences _________________________________________________ Andrew Aldrin, PhD Associate Professor School of Arts and Communication _________________________________________________ Brian Kaplinger, PhD Assistant Professor Department of Aerospace, Physics and Space Sciences _________________________________________________ Daniel Batcheldor Professor and Head Department of Aerospace, Physics and Space Sciences Abstract Title: Study of a Crew Transfer Vehicle Using Aerocapture for Cycler Based Exploration of Mars Author: Larissa Balestrero Machado Advisor: Markus Wilde, PhD This thesis presents the results of a conceptual design and aerocapture analysis for a Crew Transfer Vehicle (CTV) designed to carry humans between Earth or Mars and a spacecraft on an Earth-Mars cycler trajectory. The thesis outlines a parametric design model for the Crew Transfer Vehicle and presents concepts for the integration of aerocapture maneuvers within a sustainable cycler architecture. The parametric design study is focused on reducing propellant demand and thus the overall mass of the system and cost of the mission. This is accomplished by using a combination of propulsive and aerodynamic braking for insertion into a low Mars orbit and into a low Earth orbit.
    [Show full text]
  • Development of Supersonic Retropropulsion for Future Mars Entry, Descent, and Landing Systems
    JOURNAL OF SPACECRAFT AND ROCKETS Vol. 51, No. 3, May–June 2014 Development of Supersonic Retropropulsion for Future Mars Entry, Descent, and Landing Systems Karl T. Edquist∗ and Ashley M. Korzun† NASA Langley Research Center, Hampton, Virginia 23681 Artem A. Dyakonov‡ Blue Origin, LLC, Kent, Washington 98032 Joseph W. Studak§ NASA Johnson Space Center, Houston, Texas 77058 Devin M. Kipp¶ Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, 91109 and Ian C. Dupzyk** Lunexa, LLC, San Francisco, California 94105 DOI: 10.2514/1.A32715 Recent studies have concluded that Viking-era entry system deceleration technologies are extremely difficult to scale for progressively larger payloads (tens of metric tons) required for human Mars exploration. Supersonic retropropulsion is one of a few developing technologies that may enable future human-scale Mars entry systems. However, in order to be considered as a viable technology for future missions, supersonic retropropulsion will require significant maturation beyond its current state. This paper proposes major milestones for advancing the component technologies of supersonic retropropulsion such that it can be reliably used on Mars technology demonstration missions to land larger payloads than are currently possible using Viking-based systems. The development roadmap includes technology gates that are achieved through ground-based testing and high-fidelity analysis, culminating with subscale flight testing in Earth’s atmosphere that demonstrates stable and controlled flight. The component technologies requiring advancement include large engines (100s of kilonewtons of thrust) capable of throttling and gimbaling, entry vehicle aerodynamics and aerothermodynamics modeling, entry vehicle stability and control methods, reference vehicle systems engineering and analyses, and high-fidelity models for entry trajectory simulations.
    [Show full text]
  • Co-Optimization of Mid Lift to Drag Vehicle Concepts for Mars Atmospheric Entry
    10th AIAA/ASME Joint Thermophysics and Heat Transfer Conference AIAA 2010-5052 28 June - 1 July 2010, Chicago, Illinois Co-Optimization of Mid Lift to Drag Vehicle Concepts for Mars Atmospheric Entry Joseph A. Garcia1 , James L. Brown2 , David J. Kinney1 and Jeffrey V. Bowles1 NASA Ames Research Center, Moffett Field, CA 94035, USA and Loc C. Huynh3. Xun J. Jiang3, Eric Lau3, and Ian C. Dupzyk4 ELORET Corporation, Moffett Field, CA 94035, USA As NASA continues to make plans for future robotic precursor and eventual human missions to Mars, the need to characterize and develop designs for entry vehicles capable of delivering large masses to the surface of Mars will persist. In combination with this, NASA has recognized that the current heritage technology for Mars’ Entry Decent and Landing (EDL) does not have the capability to land the required payload masses. Both the Thermal Protection System (TPS) and the Descent/Landing systems require new design approaches. Because of these needs, NASA has performed an Entry, Descent and Landing Systems Analysis (EDL-SA) study for high mass exploration and science missions to identify key enabling technology areas for further investment. One key technology area identified includes rigid aeroshell shapes for aerodynamic performance and controllability. In this investigation, a system optimization study of alternative aeroshell shapes for Mars exploration class payloads of approximately 40 metric tons has been conducted. This system optimization is accomplished using a Multi-disciplinary Design Optimization (MDO) framework which accounts for the aeroshell shape, trajectory, thermal protection system, and vehicle subsystem closure along with a Multi Objective Genetic Algorithm (MOGA) for the initial shape exploration.
    [Show full text]
  • 1 Iac-06-C4.4.7 the Innovative Dual-Stage 4-Grid Ion
    IAC-06-C4.4.7 THE INNOVATIVE DUAL-STAGE 4-GRID ION THRUSTER CONCEPT – THEORY AND EXPERIMENTAL RESULTS Cristina Bramanti, Roger Walker, ESA-ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands [email protected], Roger. Walker @esa.int Orson Sutherland, Rod Boswell, Christine Charles Plasma Research Laboratory, Research School of Physical Sciences and Engineering, The Australian National University, Canberra, ACT 0200, Australia [email protected], [email protected], [email protected]. David Fearn EP Solutions, 23 Bowenhurst Road, Church Crookham, Fleet, Hants, GU52 6HS, United Kingdom [email protected] Jose Gonzalez Del Amo, Marika Orlandi ESA-ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands [email protected], [email protected] ABSTRACT A new concept for an advanced “Dual-Stage 4-Grid” (DS4G) ion thruster has been proposed which draws inspiration from Controlled Thermonuclear Reactor (CTR) experiments. The DS4G concept is able to operate at very high specific impulse, power and thrust density values well in excess of conventional 3-grid ion thrusters at the expense of a higher power-to-thrust ratio. A small low-power experimental laboratory model was designed and built under a preliminary research, development and test programme, and its performance was measured during an extensive test campaign, which proved the practical feasibility of the overall concept and demonstrated the performance predicted by analytical and simulation models. In the present paper, the basic concept of the DS4G ion thruster is presented, along with the design, operating parameters and measured performance obtained from the first and second phases of the experimental campaign.
    [Show full text]
  • Single-Stage Drag Modulation GNC Performance for Venus Aerocapture Demonstration
    See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/330197775 Single-Stage Drag Modulation GNC Performance for Venus Aerocapture Demonstration Conference Paper · January 2019 DOI: 10.2514/6.2019-0016 CITATIONS READS 5 32 3 authors, including: Evan Roelke University of Colorado Boulder 9 PUBLICATIONS 18 CITATIONS SEE PROFILE Some of the authors of this publication are also working on these related projects: Multi-Event Drag Modulated Aerocapture Guidance View project All content following this page was uploaded by Evan Roelke on 14 September 2020. The user has requested enhancement of the downloaded file. Single-Stage Drag Modulation GNC Performance for Venus Aerocapture Demonstration Roelke, E.∗, Braun, R.D.†, and Werner, M.S.‡ University of Colorado Boulder The future of space exploration is heavily reliant on innovative Entry, Descent, and Landing (EDL) technologies. One such innovation involves aeroassist technology, mainly aerocapture, which involves a single pass through the upper atmosphere of a planetary body from an incom- ing hyperbolic trajectory to capture into an elliptical orbit. Previous aerocapture guidance studies focused on lift modulation using reaction-control system (RCS) thrusters. This pa- per investigates the guidance law performance of drag-modulated aerocapture for a single, discrete, jettison event. Venus is selected as the target planet to observe performance in the most challenging environment. Three different guidance algorithms are studied, including a deceleration curve-fit, a pure state-predictor, and a numerical predictor-corrector utilizing both bisection and Newton-Raphson root-finding methods. The performance is assessed us- ing Monte Carlo simulation methods. The deceleration curve-fit achieves a capture rate of over 55% for a 2000km apoapsis target and 1000km tolerance.
    [Show full text]
  • Space Propulsion Technology for Small Spacecraft
    Space Propulsion Technology for Small Spacecraft The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Krejci, David, and Paulo Lozano. “Space Propulsion Technology for Small Spacecraft.” Proceedings of the IEEE, vol. 106, no. 3, Mar. 2018, pp. 362–78. As Published http://dx.doi.org/10.1109/JPROC.2017.2778747 Publisher Institute of Electrical and Electronics Engineers (IEEE) Version Author's final manuscript Citable link http://hdl.handle.net/1721.1/114401 Terms of Use Creative Commons Attribution-Noncommercial-Share Alike Detailed Terms http://creativecommons.org/licenses/by-nc-sa/4.0/ PROCC. OF THE IEEE, VOL. 106, NO. 3, MARCH 2018 362 Space Propulsion Technology for Small Spacecraft David Krejci and Paulo Lozano Abstract—As small satellites become more popular and capa- While designations for different satellite classes have been ble, strategies to provide in-space propulsion increase in impor- somehow ambiguous, a system mass based characterization tance. Applications range from orbital changes and maintenance, approach will be used in this work, in which the term ’Small attitude control and desaturation of reaction wheels to drag com- satellites’ will refer to satellites with total masses below pensation and de-orbit at spacecraft end-of-life. Space propulsion 500kg, with ’Nanosatellites’ for systems ranging from 1- can be enabled by chemical or electric means, each having 10kg, ’Picosatellites’ with masses between 0.1-1kg and ’Fem- different performance and scalability properties. The purpose tosatellites’ for spacecrafts below 0.1kg. In this category, the of this review is to describe the working principles of space popular Cubesat standard [13] will therefore be characterized propulsion technologies proposed so far for small spacecraft.
    [Show full text]
  • The Spacedrive Project – First Results on Emdrive and Mach-Effect Thrusters BARCELO RENACIMIENTO HOTEL, SEVILLE, SPAIN / 14 – 18 MAY 2018
    SP2018_016 The SpaceDrive Project – First Results on EMDrive and Mach-Effect Thrusters BARCELO RENACIMIENTO HOTEL, SEVILLE, SPAIN / 14 – 18 MAY 2018 Martin Tajmar(1), Matthias Kößling(2), Marcel Weikert(3) and Maxime Monette(4) (1-4) Institute of Aerospace Engineering, Technische Universität Dresden, Marschnerstrasse 32, 01324 Dresden, Germany, Email: [email protected] KEYWORDS: Breakthrough Propulsion, Propellant- Recent efforts therefore concentrate on using less Propulsion, EMDrive, Mach-Effect Thruster propellantless laser propulsion. For example, the proposed Breakthrough Starshot project plans to use ABSTRACT: a 100 GW laser beam to accelerate a nano- Propellantless propulsion is believed to be the spacecraft with the mass of a few grams to reach our best option for interstellar travel. However, photon closest neighbouring star Proxima Centauri in around rockets or solar sails have thrusts so low that maybe 20 years [2]. The technical challenges (laser power, only nano-scaled spacecraft may reach the next star steering, communication, etc.) are enormous but within our lifetime using very high-power laser maybe not impossible [3]. Such ideas stretch the beams. Following into the footsteps of earlier edge of our current technology. However, it is breakthrough propulsion programs, we are obvious that we need a radically new approach if we investigating different concepts based on non- ever want to achieve interstellar flight with spacecraft classical/revolutionary propulsion ideas that claim to in size similar to the ones that we use today. In the be at least an order of magnitude more efficient in 1990s, NASA started its Breakthrough Propulsion producing thrust compared to photon rockets. Our Physics Program, which organized workshops, intention is to develop an excellent research conferences and funded multiple projects to look for infrastructure to test new ideas and measure thrusts high-risk/high-payoff ideas [4].
    [Show full text]