Human Mars Mission Architecture Plan to Settle the Red Planet with 1000 People
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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. -
Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
IMPLICATIONS for FUNCTION in MICROGRAVITY Introduction
Journal of Vestibular Research. Vol. 8. No.1. pp. 81-94.1998 Copyright I!:I 1998 Elsevier Science Inc. Printed in the USA. All rights reserved 0957-4271/98 $19.00 + .00 ELSEVIER PIT S0957-4271(97)00055-4 Review SLEEP AND VESTIBULAR ADAPTATION: IMPLICATIONS FOR FUNCTION IN MICROGRAVITY J. Allan Hobson, Robert Stickgold, Edward F. Pace-Schott, and Kenneth R. Leslie Laboratory of Neurophysiology. Massachusetts Mental Health Center, Harvard Medical School, Boston, Massachusetts : : ,. "" .. 1>.. .. I. II ~ ,... "" ,... " - r' - .... .. ,... .. ... ,. .. ~ 'f''''' .. .... p .... - - • .. _.... • - _ E-mail: [email protected] o Abstract - Optimal human performance de Introduction pends upon integrated sensorimotor and cognitive functions, both of which are known to be exquis The functions of sleep remain unknown. The itely sensitive to loss of sleep. Under the micro compelling idea that sleep subserves neuronal gravity conditions of space flight, adaptation of plasticity was first clearly articulated by Giuseppe both sensorimotor (especially vestibular) and cog nitive functions (especially orientation) must occur Moruzzi (1). This hypothesis has been tested in quickly-and be maintained-despite any concur many ways, induding the systematic perturba rent disruptions of sleep that may be caused by tion of the vestibular system. The close interre microgravity itself, or by the uncomfortable sleep lationship between the vestibular nuclei and the ing conditions of the spacecraft. It is the three-way sleep inducing structures of the pontine brain interaction between sleep quality, general work ef stem has been extensively studied by Moruzzi's ficiency, and sensorimotor integration that is the colleagues, especially Ottavio Pompeiano (2). It subject of this paper and the focus of new work in is the purpose of this paper to discuss the con our laboratory. -
Introduction to Astronomy from Darkness to Blazing Glory
Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice: -
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. -
Sleep and Daily Rhythms
Activities Guide for Teachers National Space Biomedical Research Institute Houston, Texas The National Space Biomedical Research Institute (NSBRI) is combining the basic research capabilities of some of the nation’s leading biomedical research centers with operational and applied research conducted by the National Aeronautics and Space Administration (NASA) to understand and achieve safe and effective long-term human exploration and development of space. The NSBRI’s discoveries and research products will help to counter the effects of weightlessness and space radiation and will contribute to the health and well-being of all mankind. National Space Biomedical Research Institute One Baylor Plaza, NA-425 Houston, Texas 77030-3498 http://www.nsbri.org The activities described in this book are intended for school-age children under direct supervision of adults. The authors, Baylor College of Medicine and the National Space Biomedical Research Institute cannot be responsible for any accidents or injuries that may result from conduct of the activities, from not specifically following directions, or from ignoring cautions contained in the text. The opinions, findings and conclusions expressed in this publication are solely those of the authors and do not necessarily reflect the views of Baylor College of Medicine or the National Space Biomedical Research Institute. Authors: Nancy P. Moreno, Ph.D. and Barbara Z. Tharp, M.S. Cover Illustration: T Lewis Design and Production: Martha S. Young Acknowledgments The authors gratefully acknowledge the support of Bobby R. Alford, M.D.; Laurence R. Young, Sc.D.; and Ronald J. White, Ph.D.; as well as the contributions of the following science reviewers: Mary A. -
NETS 2020 Template
بÀƵƧǘȁǞƧƊǶ §ȲȌǐȲƊǿ ƊƧDzɈȌɈǘƵwȌȌȁƊȁƮȌȁ ɈȌwƊȲȺɈǘȲȌɐǐǘƊƮɨƊȁƧǞȁǐ خȁɐƧǶƵƊȲɈƵƧǘȁȌǶȌǐǞƵȺƊȁƮ ǞȁȁȌɨƊɈǞȌȁ ǞȺ ȺȯȌȁȺȌȲƵƮ Ʀɯ ɈǘƵ ƊDz ªǞƮǐƵ yƊɈǞȌȁƊǶ ׁׂ׀ׂ y0À² ÀǘǞȺ ƧȌȁǏƵȲƵȁƧƵ خׁׂ׀ׂ ةɈǘ׀׃ƊȁƮ ɩǞǶǶƦƵ ǘƵǶƮ ǏȲȌǿȯȲǞǶ ׂ׆ɈǘٌةmƊƦȌȲƊɈȌȲɯ ɩǞǶǶ ƦƵ ǘƵǶƮ ɨǞȲɈɐƊǶǶɯ ȺȌ ɈǘƊɈ ɈǘƵ ƵȁɈǞȲƵ y0À² خƧȌǿǿɐȁǞɈɯǿƊɯȯƊȲɈǞƧǞȯƊɈƵǞȁɈǘǞȺƵɮƧǞɈǞȁǐǿƵƵɈǞȁǐ ǐȌɨخȌȲȁǶخخׁׂ׀ȁƵɈȺׂششبǘɈɈȯȺ Nuclear and Emerging Technologies for Space Sponsored by Oak Ridge National Laboratory, April 26th-30th, 2021. Available online at https://nets2021.ornl.gov Table of Contents Table of Contents .................................................................................................................................................... 1 Thanks to the NETS2021 Sponsors! ...................................................................................................................... 2 Nuclear and Emerging Technologies for Space 2021 – Schedule at a Glance ................................................. 3 Nuclear and Emerging Technologies for Space 2021 – Technical Sessions and Panels By Track ............... 6 Nuclear and Emerging Technologies for Space 2021 – Lightning Talk Final Program ................................... 8 Nuclear and Emerging Technologies for Space 2021 – Track 1 Final Program ............................................. 11 Nuclear and Emerging Technologies for Space 2021 – Track 2 Final Program ............................................. 14 Nuclear and Emerging Technologies for Space 2021 – Track 3 Final Program ............................................. 18 -
Lightweight, High-Temperature Radiator for In-Space Nuclear- Electric Power and Propulsion
University of Massachusetts Amherst ScholarWorks@UMass Amherst Doctoral Dissertations Dissertations and Theses Summer November 2014 Lightweight, High-Temperature Radiator for In-Space Nuclear- Electric Power and Propulsion Briana N. Tomboulian University of Massachusetts Amherst Follow this and additional works at: https://scholarworks.umass.edu/dissertations_2 Part of the Heat Transfer, Combustion Commons, Propulsion and Power Commons, and the Systems Engineering and Multidisciplinary Design Optimization Commons Recommended Citation Tomboulian, Briana N., "Lightweight, High-Temperature Radiator for In-Space Nuclear-Electric Power and Propulsion" (2014). Doctoral Dissertations. 247. https://doi.org/10.7275/5972048.0 https://scholarworks.umass.edu/dissertations_2/247 This Open Access Dissertation is brought to you for free and open access by the Dissertations and Theses at ScholarWorks@UMass Amherst. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of ScholarWorks@UMass Amherst. For more information, please contact [email protected]. Lightweight, High-Temperature Radiator for In-Space Nuclear-Electric Power and Propulsion A Dissertation Presented by BRIANA N. TOMBOULIAN Submitted to the Graduate School of the University of Massachusetts Amherst in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY September 2014 Mechanical and Industrial Engineering Department © Copyright by Briana N. Tomboulian 2014 All Rights Reserved Lightweight, High-Temperature Radiator -
European Astronaut Selection ESA Prepares for the Missions of the 21 St Century
European Astronaut Selection ESA prepares for the missions of the 21 st century With the selection of its first astronauts ESA’s human spaceflight activities in 1978 and the first Spacelab mission are now entering a new era, with ESA in 1983, the European Space Agency astronauts working aboard the (ESA) took its first steps into human International Space Station (ISS), spaceflight. The advent of the Columbus Columbus starting operations, and orbital laboratory project required a the new ‘ATV’ cargo ship delivering second selection of astronauts in 1992. fresh supplies to the Station. The exploration of the Solar System will be one of humanity’s most exciting adventures in the near future. All of the world’s spacefaring nations are preparing for this huge enterprise, and an astronaut corps is essential for Europe, thanks to ESA, to take part in this endeavour. Now is the time for ESA to seek new talents to reinforce its astronaut team, to prepare for missions to the ISS, the Moon and beyond. T The Selection | How? When? Where? h e S e l e c t i o n How can I apply? You can apply online via the ESA web portal (www.esa.int/ astronautselection). Registration is in two steps: • pre-registration: provide identity information and a JAR-FCL 3, Class 2 medi- cal examination certificate, from an Aviation Medical Examiner who has been certified by his/her national Aviation Medical Authority; • a password then allows you to access the application form. T The Selection | How? When? Where? h e S e l e • initial selection according to basic criteria; c t i What are the o • psychological tests for selected candidates; n • second round of psychological tests and interviews; steps in the • medical tests; selection • job interview. -
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.