Directed Energy for Relativistic Propulsion and Interstellar Communications
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
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. -
Breakthrough Propulsion Study Assessing Interstellar Flight Challenges and Prospects
Breakthrough Propulsion Study Assessing Interstellar Flight Challenges and Prospects NASA Grant No. NNX17AE81G First Year Report Prepared by: Marc G. Millis, Jeff Greason, Rhonda Stevenson Tau Zero Foundation Business Office: 1053 East Third Avenue Broomfield, CO 80020 Prepared for: NASA Headquarters, Space Technology Mission Directorate (STMD) and NASA Innovative Advanced Concepts (NIAC) Washington, DC 20546 June 2018 Millis 2018 Grant NNX17AE81G_for_CR.docx pg 1 of 69 ABSTRACT Progress toward developing an evaluation process for interstellar propulsion and power options is described. The goal is to contrast the challenges, mission choices, and emerging prospects for propulsion and power, to identify which prospects might be more advantageous and under what circumstances, and to identify which technology details might have greater impacts. Unlike prior studies, the infrastructure expenses and prospects for breakthrough advances are included. This first year's focus is on determining the key questions to enable the analysis. Accordingly, a work breakdown structure to organize the information and associated list of variables is offered. A flow diagram of the basic analysis is presented, as well as more detailed methods to convert the performance measures of disparate propulsion methods into common measures of energy, mass, time, and power. Other methods for equitable comparisons include evaluating the prospects under the same assumptions of payload, mission trajectory, and available energy. Missions are divided into three eras of readiness (precursors, era of infrastructure, and era of breakthroughs) as a first step before proceeding to include comparisons of technology advancement rates. Final evaluation "figures of merit" are offered. Preliminary lists of mission architectures and propulsion prospects are provided. -
Deuterium – Tritium Pulse Propulsion with Hydrogen As Propellant and the Entire Space-Craft As a Gigavolt Capacitor for Ignition
Deuterium – Tritium pulse propulsion with hydrogen as propellant and the entire space-craft as a gigavolt capacitor for ignition. By F. Winterberg University of Nevada, Reno Abstract A deuterium-tritium (DT) nuclear pulse propulsion concept for fast interplanetary transport is proposed utilizing almost all the energy for thrust and without the need for a large radiator: 1. By letting the thermonuclear micro-explosion take place in the center of a liquid hydrogen sphere with the radius of the sphere large enough to slow down and absorb the neutrons of the DT fusion reaction, heating the hydrogen to a fully ionized plasma at a temperature of ~ 105 K. 2. By using the entire spacecraft as a magnetically insulated gigavolt capacitor, igniting the DT micro-explosion with an intense GeV ion beam discharging the gigavolt capacitor, possible if the space craft has the topology of a torus. 1. Introduction The idea to use the 80% of the neutron energy released in the DT fusion reaction for nuclear micro-bomb rocket propulsion, by surrounding the micro-explosion with a thick layer of liquid hydrogen heated up to 105 K thereby becoming part of the exhaust, was first proposed by the author in 1971 [1]. Unlike the Orion pusher plate concept, the fire ball of the fully ionized hydrogen plasma can here be reflected by a magnetic mirror. The 80% of the energy released into 14MeV neutrons cannot be reflected by a magnetic mirror for thermonuclear micro-bomb propulsion. This was the reason why for the Project Daedalus interstellar probe study of the British Interplanetary Society [2], the neutron poor deuterium-helium 3 (DHe3) reaction was chosen. -
BAEN BOOKS TEACHER's GUIDE to GOING INTERSTELLAR Contents
BAEN BOOKS TEACHER’S GUIDE TO GOING INTERSTELLAR Contents: • recommended reading levels • plot summaries • essay outlines • character sketches • guides to each short story/essay including: o prepare to read… . vocabulary* . focus question/initiating activity o quiz/reading comprehension questions—multiple choice/short answer questions o critical thinking questions—higher order open-ended questions which might be utilized for quizzes/tests, class discussion, or essay prompts o suggested activities/inquiry-based exploration—suggestions for activities and projects Recommended reading levels: Going Interstellar is appropriate for a young adult audience. Classroom use of the book is most suitable for upper middle school to high school students. * Some texts in Going Interstellar contain an abundance of high-level vocabulary. For these texts, only the words and terms that are pertinent to supporting a scientific or thematic understanding are included in the “Prepare to Read” section. It is recommended that students use a dictionary while reading Going Interstellar. Background: Published by Baen books in 2012, this anthology combines short science fiction stories with scientific essays, each addressing theories and possible scenarios concerning interstellar space travel. Biographical information on the editors: • LES JOHNSON is a NASA physicist who is an expert on space propulsion systems. He is also a science fiction writer and the author of Back to the Moon. More information about Les can be found at his home website http://www.lesjohnsonauthor.com/. • JACK MCDEVITT has been publishing science fiction since 1981, and is the winner of multiple awards within the field. McDevitt’s devotion to scientifically accurate fiction is evident in his response to a question concerning how he prepares his novels: “The research is simple,” McDevitt says, “I pick up [a] phone and call a physicist” (www.sfwa.org). -
Space Propulsion.Pdf
Deep Space Propulsion K.F. Long Deep Space Propulsion A Roadmap to Interstellar Flight K.F. Long Bsc, Msc, CPhys Vice President (Europe), Icarus Interstellar Fellow British Interplanetary Society Berkshire, UK ISBN 978-1-4614-0606-8 e-ISBN 978-1-4614-0607-5 DOI 10.1007/978-1-4614-0607-5 Springer New York Dordrecht Heidelberg London Library of Congress Control Number: 2011937235 # Springer Science+Business Media, LLC 2012 All rights reserved. This work may not be translated or copied in whole or in part without the written permission of the publisher (Springer Science+Business Media, LLC, 233 Spring Street, New York, NY 10013, USA), except for brief excerpts in connection with reviews or scholarly analysis. Use in connection with any form of information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed is forbidden. The use in this publication of trade names, trademarks, service marks, and similar terms, even if they are not identified as such, is not to be taken as an expression of opinion as to whether or not they are subject to proprietary rights. Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) This book is dedicated to three people who have had the biggest influence on my life. My wife Gemma Long for your continued love and companionship; my mentor Jonathan Brooks for your guidance and wisdom; my hero Sir Arthur C. Clarke for your inspirational vision – for Rama, 2001, and the books you leave behind. Foreword We live in a time of troubles. -
JSP Fall 2012
Journal of Space Philosophy 1, no. 1 (Fall 2012) Dedicated to the belief that Space holds solutions for the betterment of humankind. And to the memory of Astronaut Neil Armstrong, Humankind’s first Lunar visitor. 2 Journal of Space Philosophy 1, no. 1 (Fall 2012) Preface Philosophy – the search for knowledge, truth, understanding, and meaning – has occupied thought since Plato’s Thirty-Six Dialogues (424-348 BC). Every person who has gazed at the heavens has wondered what it means for themselves and for humankind. Philosophy is the oldest research subject. Every science has defined its philosophical foundations. Humans have only philosophized while personally experiencing Space since the middle of the 20th Century. Kepler Space Institute takes pride in creating its online periodical Journal of Space Philosophy. A qualified Board of Editors meets the criteria for a professional peer reviewed journal. Article submissions, to [email protected], will be accepted for publication consideration from anyone on Earth or in Space. Readers will note that Kepler Space Institute creates for the first issue of the Journal its own prescription for Space Philosophy (Article #8). Evaluation and/or expansion of that philosophy is invited. With the Journal of Space Philosophy Kepler Space Institute has created a professional online Blog-interactive journal for a major academic and science discipline. Over time, this Journal will be an increasingly valuable research source for educators, students, NASA Centers, libraries, Space organizations, and Space enthusiasts. Views contained in articles will be those of the authors; not necessarily reflecting policy of Kepler Space Institute. Reproduction and downloading of Journal content for educational purposes is permitted, but authors will hold copyrights of their material and professional accreditation is required. -
Fast Transit: Mars & Beyond
Fast Transit: mars & beyond final Report Space Studies Program 2019 Team Project Final Report Fast Transit: mars & beyond final Report Internationali l Space Universityi i Space Studies Program 2019 © International Space University. All Rights Reserved. i International Space University Fast Transit: Mars & Beyond Cover images of Mars, Earth, and Moon courtesy of NASA. Spacecraft render designed and produced using CAD. While all care has been taken in the preparation of this report, ISU does not take any responsibility for the accuracy of its content. The 2019 Space Studies Program of the International Space University was hosted by the International Space University, Strasbourg, France. Electronic copies of the Final Report and the Executive Summary can be downloaded from the ISU Library website at http://isulibrary.isunet.edu/ International Space University Strasbourg Central Campus Parc d’Innovation 1 rue Jean-Dominique Cassini 67400 Illkirch-Graffenstaden France Tel +33 (0)3 88 65 54 30 Fax +33 (0)3 88 65 54 47 e-mail: [email protected] website: www.isunet.edu ii Space Studies Program 2019 ACKNOWLEDGEMENTS Our Team Project (TP) has been an international, interdisciplinary and intercultural journey which would not have been possible without the following people: Geoff Steeves, our chair, and Jaroslaw “JJ” Jaworski, our associate chair, provided guidance and motivation throughout our TP and helped us maintain our sanity. Øystein Borgersen and Pablo Melendres Claros, our teaching associates, worked hard with us through many long days and late nights. Our staff editors: on-site editor Ryan Clement, remote editor Merryl Azriel, and graphics editor Andrée-Anne Parent, helped us better communicate our ideas. -
Hyperspace NASA BPP Program Books 8
Advanced Space Propulsion Concepts for Interstellar Travel Gregory V. Meholic [email protected] Planets HR 8799 140 LY 11/14/08 Updated 9/25/2019 1 Presentation Objectives and Caveats ▪ Provide a high-level, “evolutionary”, information-only overview of various propulsion technology concepts that, with sufficient development (i.e. $), may lead mankind to the stars. ▪ Only candidate concepts for a vehicle’s primary interstellar propulsion system will be discussed. No attitude control No earth-to-orbit launch No traditional electric systems No sail-based systems No beamed energy ▪ None of the following will be given, assumed or implied: Recommendations on specific mission designs Developmental timelines or cost estimates ▪ Not all propulsion options will be discussed – that would be impossible! 2 Chapters 1. The Ultimate Space Mission 2. The Solar System and Beyond 3. Challenges of Human Star Flight 4. “Rocket Science” Basics 5. Conventional Mass Ejection Propulsion Systems State-of-the-Art Possible Improvements 6. Alternative Mass Ejection Systems Nuclear Fission Nuclear Fusion Matter/Antimatter Other Concepts 7. Physics-Based Concepts Definitions and Things to Remember Space-Time Warp Drives Fundamental Force Coupling Alternate Dimension / Hyperspace NASA BPP Program Books 8. Closing Information 3 Chapter 1: The Ultimate Space Mission 4 The Ultimate Space Mission For humans to travel to the stars and return to Earth within a “reasonable fraction” (around 15 years) of a human lifetime. ▪ Why venture beyond our Solar System? Because we have to - humans love to explore!!! Visit the Kuiper Belt and the Oort Cloud – Theoretical home to long-period comets Investigate the nature of the interstellar medium and its influence on the solar system (and vice versa) – Magnetic fields, low-energy galactic cosmic rays, composition, etc. -
Dr. Katherine R. De Kleer
Dr. Katherine R. de Kleer Assistant Professor of Planetary Science & Astronomy, California Institute of Technology web.gps.caltech.edu/∼dekleer Mailing: 1200 E California Blvd, M/C 150-21, Pasadena, CA 91125 Office: 172 S Mudd; (626) 395-4029 [email protected] EDUCATION Ph.D. Astrophysics, University of California, Berkeley Spring 2017 Thesis: \Extreme Worlds of the Outer Solar System: Dynamic Processes on Uranus & Io" Advisor: Prof. Imke de Pater M.A. Astrophysics, University of California, Berkeley Spring 2013 B.Sc. Mathematics, Massachusetts Institute of Technology Spring 2009 B.Sc. Physics with Astronomy Minor, Massachusetts Institute of Technology Spring 2009 Thesis: \Photometry and Transit-Timing Analysis for Eleven Transiting Exoplanets" Advisor: Prof. Joshua Winn RESEARCH Broad interests in planetary astronomy, in particular the surfaces and atmospheres of planets, satellites, and INTERESTS small bodies, and their relationship to interiors and thermochemical histories. ACADEMIC Assistant Professor of Planetary Science & Astronomy, Caltech June 2019-present POSITIONS Heising-Simons Foundation 51 Pegasi b Postdoctoral Fellow, Caltech 2017-2019 Visting Scholar, Keck Observatory June 2017 NSF Graduate Research Fellow, UC Berkeley 2013-2017 Graduate Student Researcher, UC Berkeley 2010; 2012-2013; 2016-2017 Visiting Research Student, Montana State University, Bozeman, Montana Fall 2015; Summer 2016 Visiting Research Student, Max Planck Institute (MPE), Garching, Germany Summer 2012 Visiting Research Student, Tel Aviv University, Tel -
What Does It Look Like to Rebrand Space Travel?
What Does It Look Like To Rebrand Space Travel? ADVERTISING In an endeavor to make out-of-this-world travel sexy again, the Commercial Spaceflight Federation is working to design glamorous and inclusive experiences for the modern age BY IDO LECHNER 18 JULY 2016 Armstrong’s footprints on the moon is a well-documented moment in history, a part of a timeline known as the Space Age which took place nearly fifty years ago. Since then, humanity has made tremendous advancements in space exploration and technology, yet the Space Age belongs to the past – few would say we’re still in it. But if the world’s first commercial spaceline Virgin Galactic, alongside aerospace manufacturers SpaceX and Blue Origin have anything to say about the matter, it would likely be that we’re living on the cusp of major breakthroughs, such as the standardization of reusable rockets and interplanetary colonization are within reach. To help the Commercial Spaceflight Federation (CSF) – the leading voice within the industry, composed of some 70+ key players in the field – innovation firm Viceroy Creative spearheaded a strategic shift aimed to make space sexy again. David Moritz, Founder and CEO of Viceroy Creative shared his thoughts on how the rebranding came about and how it will reshape spaceflight in the eyes of the public: “When we talk about the CSF, we’re talking about many companies that are heavily involved with making commercial spaceflight a reality, and most of them are fresh faces – it’s really a niche ecosystem of startups,” Moritz points out. “It all started when I noticed that most of the astronauts working for these companies don’t look as badass as they should. -
Energy Sources for Propulsion To, and for Distributed Use On, Mars
id10495406 pdfMachine by Broadgun Software - a great PDF writer! - a great PDF creator! - http://www.pdfmachine.com http://www.broadgun.com Mehtapress 2015 Print - ISSN : 2319–9814 Journal of Online - ISSN : 2319–9822 SpFauclle pEapxerploration Full Paper WWW.MEHTAPRESS.COM Mitchell Swartz Energy sources for propulsion to, and for SPSR distributed use on, Mars Received : July 06, 2015 Accepted : August 12, 2015 Published : October 14, 2015 *Corresponding author’s Name & Add. Mitchell Swartz SPSR MORE POWER IS NEEDED Curiosity, in space, measured 1.8 millisieverts per day, with 97% from galactic cosmic rays and the rest from Mars is the future. How do we know that? Because solar particles. This is a very high level which is six times as many people signed up (202,586) for a associated with carcinogenesis and other unwanted one-way ride than did for the Affordable Care Act effects. In Mars, this exposure decreased to circa 0.7 which means that people would rather buy a ticket to millisieverts per day, similar to the exposure received the vast unknown than get healthcare as they age. on the International Space Station. What is holding back the transport of humans to Mars, Other dangers beyond the unwanted irradiation and its colonization, is energy. We need more powerful include biological changes from bone loss and muscle rockets to take people there quicker, and we need more atrophy to electrolyte changes. The goal is to decrease accessible, more portable distributed power sources the transit to Mars in less time than 3 months each for exploring, making outposts on, and terraforming way, compared to the 12 to 16 months, as it is now.