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Galaktika Group: Orbital City «EFIR» «Ethereal Dwelling» Space Colony Concept by Tsiolkovsky
Galaktika group: Orbital city «EFIR» «ethereal dwelling» space colony concept by tsiolkovsky BASIC PRINCIPLES OF CONSTRUCTING A SPACE COLONY UPON THE CONCEPT BY K.E. TSIOLKOVSKY: IN-SPACE ASSEMBLING MANKIND WILL NOT FOREVER REMAIN ON EARTH, BUT IN THE PURSUIT OF LIGHT AND SPACE WILL FIRST USING MATERIALS FROM PLANETS AND ASTEROIDS TIMIDLY EMERGE FROM THE BOUNDS OF THE ATMOSPHERE, AND THEN ADVANCE UNTIL HE HAS CONQUERED THE WHOLE ARTIFICIAL GRAVITY OF CIRCUMSOLAR SPACE. PLANTS CULTIVATION HE PRESENTED HIS RESEARCHES IN THE BOOKS: BEYOND THE PLANET EARTH, BIOLOGICAL LIFE IN COSMOS, ETHEREAL ISLAND, ETC. COLONY CONCEPTS [SHORT] REVIEW BERNAL'S SPHERE, STANFORD TORUS, O’NEILL’S CYLINDER BERNAL’S SPHERE STANFORD TORUS O’NEILL’S CYLINDER JOHN DESMOND BERNAL 1929 POPULATION: STUDENTS OF THE STANFORD UNIVERSITY 1975 GERARD K. O'NEILL, 1979 POPULATION: 20 MLN. 20—30 THOUSAND INHABITANTS DIAMETER POPULATION: 10 THND. AND MORE INHABITANTS INHABITANTS DIAMETER OF CYLINDERS: 6.4 KM ABOUT 16 KM DIAMETER1.8KM AND MORE LENGTH OF CYLINDERS: 32 KM ORBITAL CITY «EFIR» scheme and characteristics TOP VIEW residential torus ASSEMBLY DOCK radiators electric power station elevator 10,000 INHABITANTS DIAMETER OF TORUS – 2 KILOMETRES variable gravity module MASS OF ORBITAL CITY – 25 MLN. TONS RESIDENTIAL AREA DESCRIPTION OF THE INTERIOR AREA RESIDENTIAL AREA CHARACTERISTICS DIAMETER OF TORUS - 2 KILOMETRES ROTATION PERIOD - ONE FULL-CIRCLE TURN PER 63 SECONDS RESIDENTIAL AREA WIDTH - 300 METERS RESIDENTIAL AREA HEIGHT - 150 METERS AREA OF RESIDENTIAL ZONE - 200 HA MAXIMUM POPULATION - 10-40 THOUSAND DESIGNED POPULATION DENSITY IS 50 PEOPLE/HA TO 200 PEOPLE/HA RESIDENTIAL AREA DESCRIPTION OF THE INTERIOR AREA LOGISTICS transport plans for passengers and cargoes ORBITAL CITY AT THE LAGRANGIAN POINT INTERPLANETARY 25 MLN. -
General Issue
Journal of the British Interplanetary Society VOLUME 72 NO.5 MAY 2019 General issue A REACTION DRIVE Powered by External Dynamic Pressure Jeffrey K. Greason DOCKING WITH ROTATING SPACE SYSTEMS Mark Hempsell MARTIAN DUST: the Formation, Composition, Toxicology, Astronaut Exposure Health Risks and Measures to Mitigate Exposure John Cain THE CONCEPT OF A LOW COST SPACE MISSION to Measure “Big G” Roger Longstaff www.bis-space.com ISSN 0007-084X PUBLICATION DATE: 26 JULY 2019 Submitting papers International Advisory Board to JBIS JBIS welcomes the submission of technical Rachel Armstrong, Newcastle University, UK papers for publication dealing with technical Peter Bainum, Howard University, USA reviews, research, technology and engineering in astronautics and related fields. Stephen Baxter, Science & Science Fiction Writer, UK James Benford, Microwave Sciences, California, USA Text should be: James Biggs, The University of Strathclyde, UK ■ As concise as the content allows – typically 5,000 to 6,000 words. Shorter papers (Technical Notes) Anu Bowman, Foundation for Enterprise Development, California, USA will also be considered; longer papers will only Gerald Cleaver, Baylor University, USA be considered in exceptional circumstances – for Charles Cockell, University of Edinburgh, UK example, in the case of a major subject review. Ian A. Crawford, Birkbeck College London, UK ■ Source references should be inserted in the text in square brackets – [1] – and then listed at the Adam Crowl, Icarus Interstellar, Australia end of the paper. Eric W. Davis, Institute for Advanced Studies at Austin, USA ■ Illustration references should be cited in Kathryn Denning, York University, Toronto, Canada numerical order in the text; those not cited in the Martyn Fogg, Probability Research Group, UK text risk omission. -
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. -
California State University, Northridge Low Earth Orbit
CALIFORNIA STATE UNIVERSITY, NORTHRIDGE LOW EARTH ORBIT BUSINESS CENTER A Project submitted in partial satisfaction of the requirements for the degree of Master of Science in Engineering by Dallas Gene Bienhoff May 1985 The Proj'ectof Dallas Gene Bienhoff is approved: Dr. B. J. Bluth Professor T1mothy Wm. Fox - Chair California State University, Northridge ii iii ACKNOWLEDGEHENTS I wish to express my gratitude to those who have helped me over the years to complete this thesis by providing encouragement, prodding and understanding: my advisor, Tim Fox, Chair of Mechanical and Chemical Engineering; Dr. B. J. Bluth for her excellent comments on human factors; Dr. B. J. Campbell for improving the clarity; Richard Swaim, design engineer at Rocketdyne Division of Rockwell International for providing excellent engineering drawings of LEOBC; Mike Morrow, of the Advanced Engineering Department at Rockwell International who provided the Low Earth Orbit Business Center panel figures; Bob Bovill, a commercial artist, who did all the artistic drawings because of his interest in space commercialization; Linda Martin for her word processing skills; my wife, Yolanda, for egging me on without nagging; and finally Erik and Danielle for putting up with the excuse, "I have to v10rk on my paper," for too many years. iv 0 ' PREFACE The Low Earth Orbit Business Center (LEOBC) was initially conceived as a modular structure to be launched aboard the Space Shuttle, it evolved to its present configuration as a result of research, discussions and the desire to increase the efficiency of space utilization. Although the idea of placing space stations into Earth orbit is not new, as is discussed in the first chapter, and the configuration offers nothing new, LEOBC is unique in its application. -
Sustainable Space Colony Swarm Architecture
Sustainable Space Colony Swarm Architecture A SPACE COLONY AND ITS SUPPORTING SWARM ARCHITECTURE Basic principles & preconditions Main focus Global solution the needs and goals of people sufficient room and the natural habitat that our body and mind needs A collaborative network Safety and Security Services with a sufficiently large population, with a large variety in ages, types of people and skills of a space colony extensively supported on many levels and its supporting swarm architecture Collision Prevention Services Holistic approach With multiple habitats, with for object impact defense, multi-layer architecture support from Earth mostly autonomous, consisting of Safe & robust support from celestial bodies: multiple types of telescopes Moon, Venus, Mars and Asteroids distributed information artificial gravity, radiation protection, atmosphere, water, food and light support in space: and knowledge processing robustness by default: safety, energy, flight vector adjustment services, compartmentalization, logistics, manufacturing by autonomous unit(s) distributed implementation, cloud overblow facility multilayer redundancy with fallback, With a space armada backup facilities & resources at Lagrangian points: Remote controlled repairs fleet impact and collision prevention clouds of space stations, Environment sustainability services with settlements, Mindset for humans, flora and fauna manufacturing, either safe or not, with regular internal and external evacuation drills air and water purification energy supply artificial gravity provisioning -
Interstellar Travel and the Fermi Paradox
Interstellar Travel If aliens haven’t visited us, could we go to them? In this lecture we will have some fun speculating about future interstellar travel by humans. Please keep in mind that, as we discussed earlier, this cannot be considered a solution for the problems that we have on Earth, for the simple reason that the expense per person is utterly prohibitive and will remain so in any conceivable future scenario. Nonetheless, given enough time it could be that we have the capacity to move out into the galaxy. Incidentally, we will leave discussions of really far-out concepts such as wormholes to a future class. Interstellar distances The major barrier to interstellar travel is the staggering distance between stars. The closest one to the Sun is Proxima Centauri, which is 4.3 light years away but not a likely host to planets. There are, however, a few possibilities within roughly 10 light years, so that is a good target. How far is 10 light years? By definition it is how far light travels in 10 years, but let’s put this into a more familiar context. A moderately brisk walking pace is 5 km/hr, and since one light year is about 10 trillion kilometers, you would need about 20 trillion hours, or about 2.3 billion years, to walk that distance. The fastest cars sold commercially go about 400 km/hr, so you would need about three billion hours or a bit less than thirty million years. The speed of the Earth in its orbit, which is comparable to the speed of the fastest spacecraft we have constructed (all unmanned, of course), is about 30 km/s and even at that rate it would take about a hundred thousand years to travel ten light years. -
Ground Into Sky: the Topology of Interstellar
The Avery Review Fred scharmen – Ground into Sky: The Topology of Interstellar Christopher Nolan’s Interstellar was nominated for five Oscars. The Citation: Fred Scharmen, “Ground Into Sky: The Topology of Interstellar,” in The Avery Review, no. 6 movie won the Oscar for Best Visual Effects, many of which were created with (March 2015), http://averyreview.com/issues/6/ analog camera techniques. It has been controversial for its use of emotional ground-into-sky. themes, and its scientific accuracy. The physics in the film is either shockingly sloppy, or accurate enough to generate new peer-reviewed research, depend- ing on which review you read. [1] [2] But the best and most curious thing about [1] Phil Plait, “Interstellar Science: What the movie gets wrong and really wrong about black Interstellar is its topology. holes, relativity, plot, and dialogue,” Slate, http:// Again and again, in different ways, we see the ground lifting up to www.slate.com/articles/health_and_science/ space_20/2014/11/interstellar_science_review_ become the sky. The first appearance of this effect is early in the movie—the the_movie_s_black_holes_wormholes_relativity.html, horizon-obliterating dust storms that sweep across the American Midwest. accessed February 24, 2015. Cooper (the main character) and his family are at a baseball game when a dust [2]: Adam Rogers, “Wrinkles in Spacetime: The Warped Astrophysics of Interstellar,” Wired, http:// storm rises, looming like a growing mountain. Drought and blight have killed the www.wired.com/2014/10/astrophysics-interstellar- plant life that binds the soil, the near-future world of the movie has become a black-hole/, accessed February 24, 2015. -
Interstellar Travel Or Even 1.3 Mlbs at Launch
Terraforming Mars: By Aliens? Astronomy 330 •! Sometime movies are full of errors. •! But what can you do? Music: Rocket Man– Elton John Online ICES Question •! ICES forms are available online, so far 39/100 Are you going to fill out an ICES form before the students have completed it. deadline? •! I appreciate you filling them out! •! Please make sure to leave written comments. I a)! Yes, I did it already. find these comments the most useful, and typically b)! Yes, sometime today that’s where I make the most changes to the c)! Yes, this weekend course. d)! Yes, I promise to do it before the deadline of May6th! e)! No, I am way too lazy to spend 5 mins to help you or future students out. Final Final •! In this classroom, Fri, May 7th, 0800-1100. •! A normal-sized sheet of paper with notes on both •! Will consist of sides is allowed. –! 15 question on Exam 1 material. •! Exam 1and 2 and last year’s final are posted on –! 15 question on Exam 2 material. class website (not Compass). –! 30 questions from new material (Lect 20+). –! +4 extra credit questions •! I will post a review sheet Friday. •! A total of 105 points, i.e. 5 points of extra credit. •! Final Exam grade is based on all three sections. •! If Section 1/2 grade is higher than Exam 1/2 grade, then it will replace your Exam 1/2 grade. Final Papers Outline •! Final papers due at BEGINNING of discussion •! Rockets: how to get the most bang for the buck. -
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. -
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. -
The Shape of Space: NASA Designs for Orbital Space Settlements.Pdf
The Shape of Space: NASA Designs for Orbital Space Settlements 12/16/18, 12:37 PM YOU ARE READING AN ARTICLE PRINTED FROM PLACES, THE JOURNAL OF PUBLIC SCHOLARSHIP ON ARCHITECTURE, LANDSCAPE, AND URBANISM. READ MORE AT PLACESJOURNAL.ORG. The Shape of Space What the orbital space habitats designed for NASA in 1975 can teach us about living in new geometries. FRED SCHARMEN AUGUST 2018 Bernal Sphere, 1975. [Rick Guidice/Nasa Ames Research Center] “The sky starts at your feet. Think how brave you are to walk around.” 1 — Anne Herbert “Space is not only high, it’s low. It’s a bottomless pit.” 2 — Sun Ra Buckminster Fuller had an unusual way of talking about stairs. Instead of downstairs and upstairs, he encouraged people to say instairs and outstairs. “They all laugh about it,” he wrote, “But if they try saying in and out for a few days in fun, they find themselves beginning to realize that they are indeed going inward and outward in respect to the center of Earth, which is our Spaceship Earth. And for the first time they begin to feel real 3 reality.” Writing in 1970, at the dawn of extra-planetary space travel, Fuller identified a break in humans’ spatial perception. Standing on Earth, we see the ground plane as flat, but we know the planet is a sphere. To describe motion and existence in a vast universe, where planetary surfaces are the exception, we would need a new language. For centuries, the space away from the Earth’s surface — “outer” space — has confounded attempts to make sense of it with terrestrial geometric schemes.