Torus Or Dome: Which Makes the Better Martian Home
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Of 13 Human Mars Mission Design – the Ultimate Systems Challenge
Human Mars Mission Design – The Ultimate Systems Challenge John F. Connolly a, B. Kent Joostenb, Bret Drakec, Steve Hoffmanc, Tara Polsgroved, Michelle Ruckera, Alida Andrewsc, Nehemiah Williamsa a NASA Johnson Space Center, 2101 NASA Parkway, Houston, Texas 77058, john.connolly- [email protected], [email protected], [email protected] b Consultant,2383 York Harbour Ct., League City, TX 77573, [email protected] c The Aerospace Corporation, 2310 E El Segundo Blvd, El Segundo, California 90245, [email protected], [email protected], [email protected] d NASA Marshall Space Flight Center, Redstone Arsenal, Huntsville, Alabama 35812, [email protected] Abstract A human mission to Mars will occur at some time in the coming decades. When it does, it will be the end result of a complex network of interconnected design choices, systems analyses, technical optimizations, and non-technical compromises. This mission will extend the technologies, engineering design, and systems analyses to new limits, and may very well be the most complex undertaking in human history. It can be illustrated as a large menu, or as a large decision tree. Whatever the visualization tool, there are numerous design decisions required to assemble a human Mars mission, and many of these interconnect with one another. This paper examines these many decisions and further details a number of choices that are highly interwoven throughout the mission design. The large quantity of variables and their interconnectedness results in a highly complex systems challenge, and the paper illustrates how a change in one variable results in ripples (sometimes unintended) throughout many other facets of the design. -
Isolated and Confined Environments
17 Isolated and Confined Environments Carole Tafforin Ethospace, Toulouse, France Characteristics of space analogue environments with regard to human per- formance concern the crew adaptation in a socio-psychological context and in a temporal dynamics. Isolation, confinement and time are major features on Earth to reproduce an extra-terrestrial environment for manned mission simulations. In the current space missions (low Earth orbit, LEO) and in the perspective of interplanetary missions (near-Earth asteroid, Moon, Mars), men and women will have to adapt to social constraints (crew size, multinationality, mixed-gender) and spatial restrictions (volume, multi-chambers, life-support) on short-term, medium-term and long-term durations. The crewmembers also will have to perform intra-vehicular activities (IVA)and extra-vehicular activ- ities (EVA). For training, preventing and optimizing such tasks, simulations of living and working together in isolated and confined environments, and simulations of operating with a space suit on geological surfaces are the new requirements. During the two decades (1991–2011), space simulators (confinement) and analogue settings (isolation) were adequately developed on Earth with the ultimate goal of walking on Mars. Time periods extended up to 500 days. Space analogue environments are located worldwide (Canada, United States, Russia, Europe, Antarctica and Arctic). Mission durations in space analogue environments cover days, weeks and years. Isolation and confinement facilities implemented for such simulations are listed in Table 17.1. Over a 7-day duration, the Canadian Astronaut Program Space Unit Life Simulation (CAPSULS) was an Earth-based initiative that simulated a typical space shuttle or space station mission [1]. CAPSULS provided the Canadian astronaut participants with space mission training. -
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. -
Questioning the Surface of Mars As the 21St Century's Ultimate Pioneering Destination in Space
Questioning The Surface Of Mars As The 21st Century's Ultimate Pioneering Destination In Space Small Bodies Assessment Group Meeting #13 Washington D.C. 1 July 2015 Questioning Mars As The Ultimate Pioneering Destination In Space Background And Context • Foreseeable human-initiated activity in space can be divided into two categories - Exploring (e.g. Lewis & Clark ca. 1805): survey foreign territory + A major component of NASA's charter + Can be conducted by humans directly or by robots under human control + Virtual human presence is possible via tele-robotics stationed < 100,000 km away + Mars never approaches Earth closer than 56 million km - Pioneering (e.g. Pilgrims ca.1620): put down multi-generation roots in foreign territory + NOT in NASA's charter + MUST be conducted by humans in situ and ultimately return sustained profits + Any examples to date are dubious and Earth-centered (e.g. communication satellites) • Mars is widely accepted as the ultimate 21st century pioneering destination in space - Why would 202,586* adults volunteer in 2013 for a one-way trip to the surface of Mars? - What are potential obstacles to pioneering the surface of Mars? - Might there be more accessible and hospitable pioneering destinations than Mars? * The number of applications actually completed and submitted to Mars One was reported in 2015 to be 4227. Daniel R. Adamo ([email protected]) 1 1 July 2015 Questioning Mars As The Ultimate Pioneering Destination In Space History† Indicates Humans Pioneer For Compelling Reasons • Escape from war, starvation, -
Design of a Human Settlement on Mars Using In-Situ Resources
46th International Conference on Environmental Systems ICES-2016-151 10-14 July 2016, Vienna, Austria Design of a Human Settlement on Mars Using In-Situ Resources Marlies Arnhof1 Vienna University of Technology, Vienna, 1040, Austria Mars provides plenty of raw materials needed to establish a lasting, self-sufficient human colony on its surface. Due to the planet's vast distance from Earth, it is neither possible nor economically reasonable to provide permanent, interplanetary supply. In-situ resource utilization (ISRU) will be necessary to keep the Earth launch burden and mission costs as low as possible, and to provide – apart from propellant and life support – a variety of construction material. However, to include outposts on other planets into the scope of human spaceflight also opens up new psychological and sociological challenges. Crews will live in extreme environments under isolated and confined conditions for much longer periods of time than ever before. Therefore, the design of a Mars habitat requires most careful consideration of physiological as well as psychosocial conditions of living in space. In this design for a Martian settlement, the author proposes that – following preliminary automated exploration – a basic surface base brought from Earth would be set up. Bags of unprocessed Martian regolith would be used to provide additional shielding for the habitat. Once the viability of the base and its production facilities are secured, the settlement would be expanded, using planetary resources. Martian concrete – processed regolith with a polymeric binder – would be used as main in-situ construction material. To provide optimum living and working conditions, the base would respond to the environment and the residents' number and needs, thereby evolving and growing continuously. -
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 -
Human Mars Mission Architecture Plan to Settle the Red Planet with 1000 People
Human Mars Mission Architecture Plan to Settle the Red Planet with 1000 People Malaya Kumar Biswal M1, Vishnu S2, Devika S Kumar3, Sairam M4 Pondicherry University, Kalapet, Puducherry, India - 605 014 Abstract Exploration is one of the attentive endeavor to mankind and a strategy for evolution. We have been incessantly reconnoitering our planet and universe from Mesopotamian era to modern era. The progression of rocketry and planetary science in past century engendered a futuristic window to explore Mars which have been a source of inspiration to hundreds of astronomers and scientists. Globally, it invigorated space exploration agencies to make expedition for planetary exploration to Mars and Human Mars Missions. Scientists and engineers have portrayed numerous Human Mars Mission proposals and plans but currently the design reference mission 5.0 of NASA is the only mission under study. Here we propose a mission architecture for permanent Human Mars Settlement with 1000 peoples with multiple launch of sufficient cargoes and scientific instruments. Introduction: This paper focuses on design of Human Mars Mission with reference to the instructions by Mars Society. We proposed mission architecture for carrying 1000 peoples onboard spaceship (Marship). Overall mission architecture outline map and Human Mars Settlement Map is provided next to this page. We divided the whole mission architecture into three phases starting from orbital launch of launch vehicles and Mars colony establishment. We proposed novel habitat for protection during robust dust storms, various method to make the colony economically successful, minerals and their applications, administrative methods, water extraction, plantation, landing patterns, estimation of masses of food to be carried out and customizable system for re-use and recycling. -
HI-SEAS Habitat Energy Requirements and Forecasting T ∗ S.T
Acta Astronautica 162 (2019) 50–55 Contents lists available at ScienceDirect Acta Astronautica journal homepage: www.elsevier.com/locate/actaastro HI-SEAS habitat energy requirements and forecasting T ∗ S.T. Englera, , K. Binsteda, H. Leungb a Department of Information and Computer Science, University of Hawaii, POST Building, Rm 317,1680 East-West Road, Honolulu, HI 96822, United States b Department of Electrical and Computer Engineering, University of Calgary, 2500 University Drive NW, Calgary, Alberta, T2N 1N4, Canada ARTICLE INFO ABSTRACT Keywords: Travel to other planetary bodies represents a major challenge to resource management. Previous manned ex- Analog ploration missions of long duration have been resupplied with food, water, and air as required. Manned missions Simulation to other planetary bodies will have durations of years with little to no possibility of resupply. Consequently, Manned missions monitoring and forecasting resource consumption are mission-critical capabilities. The Hawaii Space Exploration Machine learning Analog and Simulation, a long-duration planetary analog simulation, has recently completed its fifth long-term Mars habitat isolation mission conducted to assess the energy, food, and water needs of a six-person long-term planetary Planetary habitat mission. This study presents a novel method for forecasting energy consumption, which incorporates the emotional state of the habitat crew. Gathered data show inhabitants in small environments can be influenced considerably by the actions of a single member. This can result in dramatic changes in consumption that could cause forecasting models to deviate to the point of total failure. Previous work found that inclusion of the daily activities and the psychological states of the crew allows for higher accuracy in long-duration forecasts. -
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. -
19660003720.Pdf
Copy No. LUNAR NAVIGATION STUDY FINAL REPORT (June 1964 to May 1965) SUMMARY VOLUME BSR 1134 June 1965 Prepared for: George C. Marshall Space Flight Center Huntsville, Alabama under Contract No. NAS8- 11292 Authors : L. J. Abbeduto W.G. Green M. E. Amdursky T. F. King D.K. Breseke R.B. Odden J. T. Broadbent P.I. Pressel R. A. Gill T.T. Trexler H. C. Graboske C. Waite BENDIX SYSTEMS DIVISION OF THE BENDIX CORPORATION Ann Arbor, Michigan CONTENTS Page 1. INTRODUCTION 1 2. STUDY APPROACH 1 3. DEFINITIONS OF TYPICAL MISSIONS 2 4. NAVIGATION SYSTEM CONCEPTS 4 5. NAVIGATION TECHNIQUE SURVEY 4 5. 1 POSITION FIX 4 5.2 DEAD RECKONING 9 5.3 PILOTING 10 6. TYPICAL NAVIGATION REQUIREMENTS 11 7. NAVIGATION COMPONENT SURVEY 14 8. LUNAR PHYSICAL AND MISSION PARAMETERS 15 9. ERROR MODELS 18 10. POSITION FIX ERROR MODEL 19 11. INITIAL AZIMUTH ERROR MODEL 22 12. DEAD-RECKONING ERROR MODEL 23 13. ERROR MODEL DIAGRAM - CONCEPT 1 29 14. ERROR MODEL DIAGRAM - CONCEPT 2 29 15. ERROR MODEL DIAGRAM - CONCEPT 3 32 16. SUMMARY OF RESULTS 38 17. CONCLUSIONS AND RECOMMENDATIONS 36 ii ILLUSTRATIONS Figure Title Page 1 Block Diagram of Study Approach 2 2 Passive, Nongyro System Block Diagram 5 3 Inertial System Block Diagram 6 4 RF Technology System Block Diagram 7 5 Vehicle Position Error Ellipsoid 19 6 Astronomical Triangle 22 7 Star Azimuth Definition 23 8 Path Density Functions 24 9 Vehicle Path, Latitude and Longitude 26 10 Altitude vs Distance Traveled 27 11 System Error vs Time 28 12 Concept 1- Passive, Nongyro System Flow Diagram 30 13 Concept 2 - Inertial System