Exotic Power and Propulsion Concepts
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Nasa Tm X-1864 *
NASA TECHNICAL. • £HP2fKit NASA TM X-1864 * ... MEMORANDUM oo fe *' > ;ff f- •* '• . ;.*• f PROPULSION • FOR *MANN1D E30PLORATION-k '* *Of THE SOEAE " • » £ Moedkel • - " *' ' ' y Lem$ Research Center Cleveland, Qbt® NATIONAL AERONAUTICS AND SFACE ADMINISTRATION • WASHINGTON, D. €, * AUCUST 1969 NASA TM X-1864 PROPULSION SYSTEMS FOR MANNED EXPLORATION OF THE SOLAR SYSTEM By W. E. Moeckel Lewis Research Center Cleveland, Ohio NATIONAL AERONAUTICS AND SPACE ADMINISTRATION For sale by the Clearinghouse for Federal Scientific and. Technical Information Springfield, Virginia 22151 - CFSTI price $3.00 ABSTRACT What propulsion systems are in sight for fast interplanetary travel? Only a few show promise of reducing trip times to values comparable to those of 16th century terrestrial expeditions. The first portion of this report relates planetary round-trip times to the performance parameters of two types of propulsion systems: type I is specific-impulse limited (with high thrust), and type n is specific-mass limited (with low thrust). The second part of the report discusses advanced propulsion concepts of both types and evaluates their limitations. The discussion includes nuclear-fission . rockets (solid, liquid, and gaseous core), nuclear-pulse propulsion, nuclear-electric rockets, and thermonuclear-fusion rockets. Particular attention is given to the last of these, because it is less familiar than the others. A general conclusion is that the more advanced systems, if they prove feasible, will reduce trip time to the near planets by factors of 3 to 5, and will make several outer planets accessible to manned exploration. PROPULSION SYSTEMS FOR MANNED EXPLORATION OF THE SOLAR SYSTEM* byW. E. Moeckel Lewis Research Center SUMMARY What propulsion systems are in sight for fast interplanetary travel? Only a few show promise of reducing trip times to values comparable to those of 16th century terrestrial expeditions. -
The Solar Cruiser Mission: Demonstrating Large Solar Sails for Deep Space Missions
The Solar Cruiser Mission: Demonstrating Large Solar Sails for Deep Space Missions Les Johnson*, Frank M. Curran**, Richard W. Dissly***, and Andrew F. Heaton* * NASA Marshall Space Flight Center ** MZBlue Aerospace NASA Image *** Ball Aerospace Solar Sails Derive Propulsion By Reflecting Photons Solar sails use photon “pressure” or force on thin, lightweight, reflective sheets to produce thrust. NASA Image 2 Solar Sail Missions Flown (as of October 2019) NanoSail-D (2010) IKAROS (2010) LightSail-1 (2015) CanX-7 (2016) InflateSail (2017) NASA JAXA The Planetary Society Canada EU/Univ. of Surrey Earth Orbit Interplanetary Earth Orbit Earth Orbit Earth Orbit Deployment Only Full Flight Deployment Only Deployment Only Deployment Only 3U CubeSat 315 kg Smallsat 3U CubeSat 3U CubeSat 3U CubeSat 10 m2 196 m2 32 m2 <10 m2 10 m2 3 Current and Planned Solar Sail Missions CU Aerospace (2018) LightSail-2 (2019) Near Earth Asteroid Solar Cruiser (2024) Univ. Illinois / NASA The Planetary Society Scout (2020) NASA NASA Earth Orbit Earth Orbit Interplanetary L-1 Full Flight Full Flight Full Flight Full Flight In Orbit; Not yet In Orbit; Successful deployed 6U CubeSat 90 Kg Spacecraft 3U CubeSat 86 m2 >1200 m2 3U CubeSat 32 m2 20 m2 4 Near Earth Asteroid Scout The Near Earth Asteroid Scout Will • Image/characterize a NEA during a slow flyby • Demonstrate a low cost asteroid reconnaissance capability Key Spacecraft & Mission Parameters • 6U cubesat (20cm X 10cm X 30 cm) • ~86 m2 solar sail propulsion system • Manifested for launch on the Space Launch System (Artemis 1 / 2020) • 1 AU maximum distance from Earth Leverages: combined experiences of MSFC and JPL Close Proximity Imaging Local scale morphology, with support from GSFC, JSC, & LaRC terrain properties, landing site survey Target Reconnaissance with medium field imaging Shape, spin, and local environment NEA Scout Full Scale EDU Sail Deployment 6 Solar Cruiser Mission Concept Mission Profile Solar Cruiser may launch as a secondary payload on the NASA IMAP mission in October, 2024. -
Pulsed Fusion Space Propulsion: Computational Ideal Magneto-Hydro Dynamics of a Magnetic Flux Compression Reaction Chamber
Pulsed Fusion Space Propulsion: Computational Ideal Magneto-Hydro Dynamics of a Magnetic Flux Compression Reaction Chamber G. Romanelli Master of Science Thesis Space Systems Engineering PULSED FUSION SPACE PROPULSION: COMPUTATIONAL IDEAL MAGNETO-HYDRO DYNAMICS OFA MAGNETIC FLUX COMPRESSION REACTION CHAMBER by Gherardo ROMANELLI to obtain the degree of Master of Science at the Delft University of Technology, to be defended publicly on Friday February 26, 2016 at 10:00 AM. Student number: 4299876 Thesis committee: Dr. A. Cervone, TU Delft, supervisor Prof. Dr. E. K. A. Gill, TU Delft Dr. Ir. E. Mooij, TU Delft Prof. A. Mignone, Politecnico di Torino An electronic version of this thesis is available at http://repository.tudelft.nl/. To boldly go where no one has gone before. James T. Kirk ACKNOWLEDGEMENTS First of all I would like to thank my supervisor Dr. A. Cervone who has always sup- ported me despite my “quite exotic” interests. He left me completely autonomous in shaping my thesis project, and still, was always there every time I needed help. Then, I would of course like to thank Prof. A. Mignone who decided to give his contribute to this seemingly crazy project of mine. His advice arrived just in time to give an happy ending to this story. Il ringraziamento più grande, però, va di certo alla mia famiglia. Alla mia mamma e a mio babbo, perché hanno sempre avuto fiducia in me e non hanno mai chiesto ragioni o spiegazioni alle mie scelte. Ai miei nonni, perché se di punto in bianco, un giorno di novembre ho deciso di intraprendere questa lunga strada verso l’Olanda, l’ho potuto fare anche per merito loro. -
9.0 BACKGROUND “What Do I Do First?” You Need to Research a Card (Thruster Or 9.1 DESIGNER’S NOTES Robonaut) with a Low Fuel Consumption
9.2 TIPS FOR INEXPERIENCED ROCKET CADETS 9.0 BACKGROUND “What do I do first?” You need to research a card (thruster or 9.1 DESIGNER’S NOTES robonaut) with a low fuel consumption. A “1” is great, a “4” The original concept for this game was a “Lords of the Sierra Madre” in is marginal. The PRC player*** can consider an dash to space. With mines, ranches, smelters, and rail lines all purchased and claim Hellas Basin on Mars, using just his crew card. He controlled by different players, who have to negotiate between them- needs 19 fuel steps (6 WT) along the red route to do this. selves to expand. But space does not work this way. “What does my rocket need?” Your rocket needs 4 things: Suppose you have a smelter on one main-belt asteroid, powered by a • A card with a thruster triangle (2.4D) to act as a thruster. • A card with an ISRU rating, if its mission is to prospect. beam-station on another asteroid, and you discover platinum on a third • A refinery, if its mission is to build a factory. nearby asteroid. Unfortunately for long-term operations, next year these • Enough fuel to get to the destination. asteroids will be separated by 2 to 6 AUs.* Furthermore, main belt Decide between a small rocket able to make multiple claims, Hohmann transfers are about 2 years long, with optimal transfer opportu- or a big rocket including a refinery and robonaut able to nities about 7 years apart. Jerry Pournelle in his book “A Step Farther industrialize the first successful claim. -
Humanity and Space
10/17/2012!! !!!!!! Project Number: MH-1207 Humanity and Space An Interactive Qualifying Project Submitted to WORCESTER POLYTECHNIC INSTITUTE In partial fulfillment for the Degree of Bachelor of Science by: Matthew Beck Jillian Chalke Matthew Chase Julia Rugo Professor Mayer H. Humi, Project Advisor Abstract Our IQP investigates the possible functionality of another celestial body as an alternate home for mankind. This project explores the necessary technological advances for moving forward into the future of space travel and human development on the Moon and Mars. Mars is the optimal candidate for future human colonization and a stepping stone towards humanity’s expansion into outer space. Our group concluded space travel and interplanetary exploration is possible, however international political cooperation and stability is necessary for such accomplishments. 2 Executive Summary This report provides insight into extraterrestrial exploration and colonization with regards to technology and human biology. Multiple locations have been taken into consideration for potential development, with such qualifying specifications as resources, atmospheric conditions, hazards, and the environment. Methods of analysis include essential research through online media and library resources, an interview with NASA about the upcoming Curiosity mission to Mars, and the assessment of data through mathematical equations. Our findings concerning the human aspect of space exploration state that humanity is not yet ready politically and will not be able to biologically withstand the hazards of long-term space travel. Additionally, in the field of robotics, we have the necessary hardware to implement adequate operational systems yet humanity lacks the software to implement rudimentary Artificial Intelligence. Findings regarding the physics behind rocketry and space navigation have revealed that the science of spacecraft is well-established. -
A New Vision for Fusion Energy Research: Fusion Rocket Engines for Planetary Defense Abstract We Argue That It Is Essential Fo
LA-UR-15-23198 A New Vision for Fusion Energy Research: Fusion Rocket Engines for Planetary Defense G. A. Wurden1, T. E. Weber1, P. J. Turchi2, P. B. Parks3, T. E. Evans3, S. A. Cohen4, J. T. Cassibry5, E. M. Campbell6 1Los Alamos National Laboratory 2Santa Fe, NM 3General Atomics 4Princeton Plasma Physics Laboratory 5University of Alabama, Huntsville 6Sandia National Laboratory Abstract We argue that it is essential for the fusion energy program to identify an imagination- capturing critical mission by developing a unique product which could command the marketplace. We lay out the logic that this product is a fusion rocket engine, to enable a rapid response capable of deflecting an incoming comet, to prevent its impact on the planet Earth, in defense of our population, infrastructure, and civilization. As a side benefit, deep space solar system exploration, with greater speed and orders-of-magnitude greater payload mass would also be possible. The US Department of Energy’s magnetic fusion research program, based in its Office of Science, focuses on plasma and fusion science1 to support the long term goal of environmentally friendly, socially acceptable, and economically viable electricity production from fusion reactors.2 For several decades the US magnetic fusion program has had to deal with a lack of urgency towards and inconsistent funding for this ambitious goal. In many American circles, fusion isn’t even at the table3 when it comes to discussing future energy production. Is there another, more urgent, unique, and even more important application for fusion? Fusion’s unique application As an on-board power source and thruster for fast propulsion in space,4 a fusion reactor would provide unparalleled performance (high specific impulse and high specific power) for a spacecraft. -
Advanced Ion Propulsion Using Krypton Isotope for Rocket Engine
Special Issue - 2019 International Journal of Engineering Research & Technology (IJERT) ISSN: 2278-0181 CONFCALL - 2019 Conference Proceedings Advanced Ion Propulsion using Krypton Isotope for Rocket Engine R. Saro C. Madeshwaran Dept of AERO-PITS Dept of AERO-PITS Mr. V. Keerthivasan Mr. T. Anbarasan Assistant Professor Head of the Department Dept of AERO-PITS Dept of AERO-PITS Abstract:- A Rocket engine is a storage device of rocket propellant which forms a high speed propulsive jet of fluid with a high temperature gas. Krypton isotope are used for producing hot positrons. Isotopes are obtained using neutron that produce reactors. The positrons were generated and directed towards action which on further obtain fusion propulsion. Positron dynamics reduce the speed of positron that are generated. It consists of moderator device with several layers of silicon carbide film which provide individual positrons. An electric field makes the particle to move towards each layers where the particles are cooled. The catalysed fusion reaction of positron is in a block of deuterium. When the particle triggers with deuterium, it produces thrust. FIG .1.1-ROCKET ENGINE Keywords – Positrons, Silicon carbide layer, Deuterium, Neutron capture. ADVANCED PROPULSION INTRODUCTION Spacecraft has been slow down due to chemical The word propulsion refers push forward or to move an rocket speed over years. Only speed over 1 million object forward. A propulsion system has a mechanical miles per hour is possible over the year 2050. New power which converts power to propulsive force. ion drives as being developed to provide ten times Normally, this system consists of two classifications – air better than ISP. -
Gravitational Propulsion by Help of Vacuum Holes
American Journal of Modern Physics 2015; 4(5): 254-260 Published online September 12, 2015 (http://www.sciencepublishinggroup.com/j/ajmp) doi: 10.11648/j.ajmp.20150405.15 ISSN: 2326-8867 (Print); ISSN: 2326-8891 (Online) Gravitational Propulsion by Help of Vacuum Holes Constantin Leshan Department of Nuclear Physics, T. Shevchenko National University of Kyiv, Octeabriscoe, Moldova Email address: [email protected] To cite this article: Constantin Leshan. Gravitational Propulsion by Help of Vacuum Holes. American Journal of Modern Physics . Vol. 4, No. 5, 2015, pp. 254-260. doi: 10.11648/j.ajmp.20150405.15 Abstract: A new concept, the gravitational propulsion, or "Hole Levitation", is proposed which propels vehicle by using the artificial gravity (vacuum holes). Such gravitational propulsion is similar to gravitational slingshot but without the need for large masses like planets and complicate maneuvers. The source of artificial gravitation accelerates the vehicle in one direction and the surrounding medium in the opposite direction. Therefore, it is not a reactionless drive: momentum is taken from the surrounding stars and planets and conferred on the vehicle and thus is conserved overall. The artificial gravity generator can damp or neutralize inertial forces due to the levitating vehicle is able to move with large acceleration, which is not acceptable for other means of transport. Keywords: Artificial Gravity, Vacuum Holes, Gravity Control, Levitation, Inertia Gravity assist maneuver can change the speed of a 1. Introduction spacecraft without expending propellant, but this method has Gravitational field propulsion is the concept of vehicle limits [2]. The main limit to the use of gravity assist propulsion where no propellant is necessary but instead maneuver is that large masses like planets and moons are momentum of the vehicle is changed by an interaction of the seldom in the right place to enable trip to destination. -
Orbit Transfer Problems and the Results You Obtained
MS&E 315 and CME 304 Solar sailing between Earth and Mars 1 Overview In this project, you will use your knowledge of nonlinear optimization to help a space agency design a cargo mission. The mission consists of making a cargo spacecraft perform interplanetary orbit transfers between Earth and Mars, and the agency is considering using a solar sail to propel the spacecraft. They need you to determine how the spacecraft should be operated to perform these orbit transfers in the shortest possible time for different solar sail technologies. 2 Mission information 2.1 Simplifications The agency has determined that the following simplifications are acceptable for your analysis: 1. Orbits are heliocentric, circular and co-planar. 2. Gravitational effects due to celestial bodies other than the Sun are ignored. 3. The Sun and spacecraft are modeled as point masses. 4. The Sun has spherically symmetric gravitational and radiation fields. 2.2 Problem description The problem you have to solve consists of determining how the solar sail of the spacecraft should be oriented to make the spacecraft perform each of the interplanetary orbit transfers Earth-Mars and Mars-Earth in the shortest possible time. You have to perform this analysis for some, say three, of the available solar sail technologies so that the agency can choose the most appropriate one in terms of cost and performance. Each solar sail technology is identified by a characteristic acceleration, as described in the next subsection. Figure1 shows a diagram of the orbits of interest, where rE and !E denote the radius and angular velocity, respectively, of Earth's orbit around the Sun, and rM and !M denote the radius and angular velocity, respectively, of Mars's orbit around the Sun. -
Hybrid Solar Sails for Active Debris Removal Final Report
HybridSail Hybrid Solar Sails for Active Debris Removal Final Report Authors: Lourens Visagie(1), Theodoros Theodorou(1) Affiliation: 1. Surrey Space Centre - University of Surrey ACT Researchers: Leopold Summerer Date: 27 June 2011 Contacts: Vaios Lappas Tel: +44 (0) 1483 873412 Fax: +44 (0) 1483 689503 e-mail: [email protected] Leopold Summerer (Technical Officer) Tel: +31 (0)71 565 4192 Fax: +31 (0)71 565 8018 e-mail: [email protected] Ariadna ID: 10-6411b Ariadna study type: Standard Contract Number: 4000101448/10/NL/CBi Available on the ACT website http://www.esa.int/act Abstract The historical practice of abandoning spacecraft and upper stages at the end of mission life has resulted in a polluted environment in some earth orbits. The amount of objects orbiting the Earth poses a threat to safe operations in space. Studies have shown that in order to have a sustainable environment in low Earth orbit, commonly adopted mitigation guidelines should be followed (the Inter-Agency Space Debris Coordination Committee has proposed a set of debris mitigation guidelines and these have since been endorsed by the United Nations) as well as Active Debris Removal (ADR). HybridSail is a proposed concept for a scalable de-orbiting spacecraft that makes use of a deployable drag sail membrane and deployable electrostatic tethers to accelerate orbital decay. The HybridSail concept consists of deployable sail and tethers, stowed into a nano-satellite package. The nano- satellite, deployed from a mothership or from a launch vehicle will home in towards the selected piece of space debris using a small thruster-propulsion firing and magnetic attitude control system to dock on the debris. -
Solar Sails and Lunar South Pole Coverage
Solar Sails and Lunar South Pole Coverage M. T. Ozimek,∗ D. J. Grebow,∗ K. C. Howelly Purdue University, West Lafayette, IN, 47907-2045, USA Potential orbits for continuous surveillance of the lunar south pole with just one space- craft and a solar sail are investigated. Periodic orbits are first computed in the Earth- Moon Restricted Three-Body Problem, using Hermite-Simpson and seventh-degree Gauss- Lobatto collocation schemes. The schemes are easily adapted to include path constraints fa- vorable for lunar south pole coverage. The methods are robust, generating a control history and a nearby solution with little information required for an initial guess. Five solutions of interest are identified and, using collocation, transitioned to the full ephemeris model (including the actual Sun-to-spacecraft line and lunar librations). Of the options investi- gated, orbits near the Earth-Moon L2 point yield the best coverage results. Propellant-free transfers from a geosynchronous transfer orbit to the coverage orbits are also computed. A steering law is discussed and refined by the collocation methods. The study indicates that solar sails remain a feasible option for constant lunar south pole coverage. Nomenclature x State Variable Vector t Time u Control Variable Vector r; v Position and Velocity Vectors, Earth-Moon Rotating Frame U Potential Function a Sail Acceleration Vector R; V Position and Velocity Vectors, EMEJ2000 Frame κ Characteristic Acceleration l Sun-to-Spacecraft Unit-Vector !s Angular Rate of Sun, Earth-Moon Rotating Frame n Number of Nodes ∆i Defect Vector Ti Segment Time i Control Magnitude Constraint gi Path Constraint Vector hk General Node States and/or Control Constraint X Total Design Variable Vector F Full Constraint Vector DF Jacobian Matrix φ Elevation Angle from the Lunar South Pole a Altitude from the Lunar South Pole δ Sail Clock Angle α Sail Pitch Angle E Two-Body Energy with Respect to Earth H Two-Body Angular Momentum with Respect to Earth ∗Ph.D. -
Propulsion Systems for Interstellar Exploration
The Future of Electric Propulsion: A Young Visionary Paper Competition 35th International Electric Propulsion Conference October 8-12, 2017 Atlanta, Georgia Propulsion Systems for Interstellar Exploration Steven L. Magnusen Embry-Riddle Aeronautical University, Daytona Beach, FL, USA Alfredo D. Tuesta∗ National Research Council Postdoctoral Associate, Washington, DC, USA [email protected] August 4, 2017 Abstract The idea of manned spaceships exploring nearby star systems, although difficult and unlikely in this generation or the next, is becoming less a tale of science fiction and more a concept of rigorous scientific interest. In 2003, NASA sent two rovers to Mars and returned images and data that would change our view of the planet forever. Already, scientists and engineers are proposing concepts for manned missions to the Red Planet. As we prepare to visit the planets in our solar system, we dare to explore the possibilities and venues to travel beyond. With NASA’s count of known exoplanets now over 3,000 and growing, interest in interstellar science is being renewed as well. In this work, the authors discuss the benefits and deficiencies of current and emerging technologies in electric propulsion for outer planet and extrasolar exploration and propose innovative and daring concepts to further the limits of present engineering. The topics covered include solar and electric sails and beamed energy as propulsion systems. I. Introduction Te Puke is the name for the voyaging canoe that the Polynesians developed to sail across vast distances in the Pacific Ocean at the turn of the first millennium. This primitive yet sophisticated canoe, made of two hollowed out tree trunks and crab claw sails woven together from leaves, allowed Polynesian sailors to navigate the open ocean by studying the stars.