Design of a Human Settlement on Mars Using In-Situ Resources
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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. -
A Future Mars Environment for Science and Exploration
Planetary Science Vision 2050 Workshop 2017 (LPI Contrib. No. 1989) 8250.pdf A FUTURE MARS ENVIRONMENT FOR SCIENCE AND EXPLORATION. J. L. Green1, J. Hol- lingsworth2, D. Brain3, V. Airapetian4, A. Glocer4, A. Pulkkinen4, C. Dong5 and R. Bamford6 (1NASA HQ, 2ARC, 3U of Colorado, 4GSFC, 5Princeton University, 6Rutherford Appleton Laboratory) Introduction: Today, Mars is an arid and cold world of existing simulation tools that reproduce the physics with a very thin atmosphere that has significant frozen of the processes that model today’s Martian climate. A and underground water resources. The thin atmosphere series of simulations can be used to assess how best to both prevents liquid water from residing permanently largely stop the solar wind stripping of the Martian on its surface and makes it difficult to land missions atmosphere and allow the atmosphere to come to a new since it is not thick enough to completely facilitate a equilibrium. soft landing. In its past, under the influence of a signif- Models hosted at the Coordinated Community icant greenhouse effect, Mars may have had a signifi- Modeling Center (CCMC) are used to simulate a mag- cant water ocean covering perhaps 30% of the northern netic shield, and an artificial magnetosphere, for Mars hemisphere. When Mars lost its protective magneto- by generating a magnetic dipole field at the Mars L1 sphere, three or more billion years ago, the solar wind Lagrange point within an average solar wind environ- was allowed to directly ravish its atmosphere.[1] The ment. The magnetic field will be increased until the lack of a magnetic field, its relatively small mass, and resulting magnetotail of the artificial magnetosphere its atmospheric photochemistry, all would have con- encompasses the entire planet as shown in Figure 1. -
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, -
An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger Depauw University
DePauw University Scholarly and Creative Work from DePauw University Student research Student Work 2015 An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger DePauw University Follow this and additional works at: http://scholarship.depauw.edu/studentresearch Part of the Economics Commons, and the The unS and the Solar System Commons Recommended Citation Knappenberger, Clayton, "An Economic Analysis of Mars Exploration and Colonization" (2015). Student research. Paper 28. This Thesis is brought to you for free and open access by the Student Work at Scholarly and Creative Work from DePauw University. It has been accepted for inclusion in Student research by an authorized administrator of Scholarly and Creative Work from DePauw University. For more information, please contact [email protected]. An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger 2015 Sponsored by: Dr. Villinski Committee: Dr. Barreto and Dr. Brown Contents I. Why colonize Mars? ............................................................................................................................ 2 II. Can We Colonize Mars? .................................................................................................................... 11 III. What would it look like? ............................................................................................................... 16 A. National Program ......................................................................................................................... -
2. Going to Mars
aMARTE A MARS ROADMAP FOR TRAVEL AND EXPLORATION Final Report International Space University Space Studies Program 2016 © International Space University. All Rights Reserved. The 2016 Space Studies Program of the International Space University (ISU) was hosted by the Technion – Israel Institute of Technology in Haifa, Israel. aMARTE has been selected as the name representing the Mars Team Project. This choice was motivated by the dual meaning the term conveys. aMARTE first stands for A Mars Roadmap for Travel and Exploration, the official label the team has adopted for the project. Alternatively, aMARTE can be interpreted from its Spanish roots "amarte," meaning "to love," or can also be viewed as "a Marte," meaning "going to Mars." This play on words represents the mission and spirit of the team, which is to put together a roadmap including various disciplines for a human mission to Mars and demonstrate a profound commitment to Mars exploration. The aMARTE title logo was developed based on sections of the astrological symbols for Earth and Mars. The blue symbol under the team's name represents Earth, and the orange arrow symbol is reminiscent of the characteristic color of Mars. The arrow also serves as an invitation to go beyond the Earth and explore our neighboring planet. 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 I. -
18Th EANA Conference European Astrobiology Network Association
18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures. -
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. -
Unsaturated Soils on Mars and Their Impact on Human Missions and Settlement on Mars
Unsaturated soils on Mars and their impact on human missions and settlement on Mars 1 1 Morteza Sheshpari *, Sai Vanapalli 1Department of Civil Engineering, University of Ottawa, Ottawa, ON, Canada, K1N6N5, *Corresponding author: email: [email protected] ABSTRACT Significant recent attention has been garnered by research related to the mechanics of unsaturated soils in the geoscience, geotechnical engineering, and agricultural science. Unsaturated soils are widely distributed in semi-arid and arid regions of the world. The planet Mars, like Earth, is covered with soil originating from erosion and weathering of igneous rocks. The presence of unsaturated soils from recordings of Mars orbiters and landers are discussed in this paper. The importance of these soils and the possible geohazards that they may pose for future human exploration or colonization of Mars are presented too. In conclusion, unsaturated soils appear to exist on a large scale on Mars and can contribute to geotechnical problems similar to those on Earth. We will discover valuable information about the potential problems, and hence possible solutions, for planning human activities on Mars in future. KEYWORDS: Mars, unsaturated soils, suction, duricrust, debris flow, collapsible soils, geotechnical hazards, human settlement INTRODUCTION There are plans by different authorities to have humans on Mars for exploration purposes and also for possible settlement. Main ongoing projects with regards to these plans are the Mars One project and a new proposal from NASA (1, 2).There are however several geotechnical engineering challenges that have to be addressed for success of the proposed future human projects on Mars. Geotechnical problems associated with soils on Earth located above the ground water table, (i.e. -
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. -
Martian Ice How One Neutrino Changed Astrophysics Remembering Two Former League Presidents
Published by the Astronomical League Vol. 71, No. 3 June 2019 MARTIAN ICE HOW ONE NEUTRINO 7.20.69 CHANGED ASTROPHYSICS 5YEARS REMEMBERING TWO APOLLO 11 FORMER LEAGUE PRESIDENTS ONOMY T STR O T A H G E N P I E G O Contents N P I L R E B 4 . President’s Corner ASTRONOMY DAY Join a Tour This Year! 4 . All Things Astronomical 6 . Full Steam Ahead OCTOBER 5, From 37,000 feet above the Pacific Total Eclipse Flight: Chile 7 . Night Sky Network 2019 Ocean, you’ll be high above any clouds, July 2, 2019 For a FREE 76-page Astronomy seeing up to 3¼ minutes of totality in a PAGE 4 9 . Wanderers in the Neighborhood dark sky that makes the Sun’s corona look Day Handbook full of ideas and incredibly dramatic. Our flight will de- 10 . Deep Sky Objects suggestions, go to: part from and return to Santiago, Chile. skyandtelescope.com/2019eclipseflight www.astroleague.org Click 12 . International Dark-Sky Association on "Astronomy Day” Scroll 14 . Fire & Ice: How One Neutrino down to "Free Astronomy Day African Stargazing Safari Join astronomer Stephen James ̃̃̃Changed a Field Handbook" O’Meara in wildlife-rich Botswana July 29–August 4, 2019 for evening stargazing and daytime PAGE 14 18 . Remembering Two Former For more information, contact: safari drives at three luxury field ̃̃̃Astronomical League Presidents Gary Tomlinson camps. Only 16 spaces available! Astronomy Day Coordinator Optional extension to Victoria Falls. 21 . Coming Events [email protected] skyandtelescope.com/botswana2019 22 . Gallery—Moon Shots 25 . Observing Awards Iceland Aurorae September 26–October 2, 2019 26 . -
Human Exploration of Mars Design Reference Architecture 5.0
July 2009 “We are all . children of this universe. Not just Earth, or Mars, or this System, but the whole grand fireworks. And if we are interested in Mars at all, it is only because we wonder over our past and worry terribly about our possible future.” — Ray Bradbury, 'Mars and the Mind of Man,' 1973 Cover Art: An artist’s concept depicting one of many potential Mars exploration strategies. In this approach, the strengths of combining a central habitat with small pressurized rovers that could extend the exploration range of the crew from the outpost are assessed. Rawlings 2007. NASA/SP–2009–566 Human Exploration of Mars Design Reference Architecture 5.0 Mars Architecture Steering Group NASA Headquarters Bret G. Drake, editor NASA Johnson Space Center, Houston, Texas July 2009 ACKNOWLEDGEMENTS The individuals listed in the appendix assisted in the generation of the concepts as well as the descriptions, images, and data described in this report. Specific contributions to this document were provided by Dave Beaty, Stan Borowski, Bob Cataldo, John Charles, Cassie Conley, Doug Craig, Bret Drake, John Elliot, Chad Edwards, Walt Engelund, Dean Eppler, Stewart Feldman, Jim Garvin, Steve Hoffman, Jeff Jones, Frank Jordan, Sheri Klug, Joel Levine, Jack Mulqueen, Gary Noreen, Hoppy Price, Shawn Quinn, Jerry Sanders, Jim Schier, Lisa Simonsen, George Tahu, and Abhi Tripathi. Available from: NASA Center for AeroSpace Information National Technical Information Service 7115 Standard Drive 5285 Port Royal Road Hanover, MD 21076-1320 Springfield, VA 22161 Phone: 301-621-0390 or 703-605-6000 Fax: 301-621-0134 This report is also available in electronic form at http://ston.jsc.nasa.gov/collections/TRS/ CONTENTS 1 Introduction ......................................................................................................................