2. Going to Mars
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EMC18 Abstracts
EUROPEAN MARS CONVENTION 2018 – 26-28 OCT. 2018, LA CHAUX-DE-FONDS, SWITZERLAND EMC18 Abstracts In alphabetical order Name title of presentation Page n° Théodore Besson: Scorpius Prototype 3 Tomaso Bontognali Morphological biosignatures on Mars: what to expect and how to prepare not to miss them 4 Pierre Brisson: Humans on Mars will have to live according to both Martian & Earth Time 5 Michel Cabane: Curiosity on Mars : What is new about organic molecules? 6 Antonio Del Mastro Industrie 4.0 technology for the building of a future Mars City: possibilities and limits of the application of a terrestrial technology for the human exploration of space 7 Angelo Genovese Advanced Electric Propulsion for Fast Manned Missions to Mars and Beyond 8 Olivia Haider: The AMADEE-18 Mars Simulation OMAN 9 Pierre-André Haldi: The Interplanetary Transport System of SpaceX revisited 10 Richard Heidman: Beyond human, technical and financial feasibility, “mass-production” constraints of a Colony project surge. 11 Jürgen Herholz: European Manned Space Projects 12 Jean-Luc Josset Search for life on Mars, the ExoMars rover mission and the CLUPI instrument 13 Philippe Lognonné and the InSight/SEIS Team: SEIS/INSIGHT: Towards the Seismic Discovering of Mars 14 Roland Loos: From the Earth’s stratosphere to flying on Mars 15 EUROPEAN MARS CONVENTION 2018 – 26-28 OCT. 2018, LA CHAUX-DE-FONDS, SWITZERLAND Gaetano Mileti Current research in Time & Frequency and next generation atomic clocks 16 Claude Nicollier Tethers and possible applications for artificial gravity -
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. -
Mars, the Nearest Habitable World – a Comprehensive Program for Future Mars Exploration
Mars, the Nearest Habitable World – A Comprehensive Program for Future Mars Exploration Report by the NASA Mars Architecture Strategy Working Group (MASWG) November 2020 Front Cover: Artist Concepts Top (Artist concepts, left to right): Early Mars1; Molecules in Space2; Astronaut and Rover on Mars1; Exo-Planet System1. Bottom: Pillinger Point, Endeavour Crater, as imaged by the Opportunity rover1. Credits: 1NASA; 2Discovery Magazine Citation: Mars Architecture Strategy Working Group (MASWG), Jakosky, B. M., et al. (2020). Mars, the Nearest Habitable World—A Comprehensive Program for Future Mars Exploration. MASWG Members • Bruce Jakosky, University of Colorado (chair) • Richard Zurek, Mars Program Office, JPL (co-chair) • Shane Byrne, University of Arizona • Wendy Calvin, University of Nevada, Reno • Shannon Curry, University of California, Berkeley • Bethany Ehlmann, California Institute of Technology • Jennifer Eigenbrode, NASA/Goddard Space Flight Center • Tori Hoehler, NASA/Ames Research Center • Briony Horgan, Purdue University • Scott Hubbard, Stanford University • Tom McCollom, University of Colorado • John Mustard, Brown University • Nathaniel Putzig, Planetary Science Institute • Michelle Rucker, NASA/JSC • Michael Wolff, Space Science Institute • Robin Wordsworth, Harvard University Ex Officio • Michael Meyer, NASA Headquarters ii Mars, the Nearest Habitable World October 2020 MASWG Table of Contents Mars, the Nearest Habitable World – A Comprehensive Program for Future Mars Exploration Table of Contents EXECUTIVE SUMMARY .......................................................................................................................... -
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. -
Why NASA Consistently Fails at Congress
W&M ScholarWorks Undergraduate Honors Theses Theses, Dissertations, & Master Projects 6-2013 The Wrong Right Stuff: Why NASA Consistently Fails at Congress Andrew Follett College of William and Mary Follow this and additional works at: https://scholarworks.wm.edu/honorstheses Part of the Political Science Commons Recommended Citation Follett, Andrew, "The Wrong Right Stuff: Why NASA Consistently Fails at Congress" (2013). Undergraduate Honors Theses. Paper 584. https://scholarworks.wm.edu/honorstheses/584 This Honors Thesis is brought to you for free and open access by the Theses, Dissertations, & Master Projects at W&M ScholarWorks. It has been accepted for inclusion in Undergraduate Honors Theses by an authorized administrator of W&M ScholarWorks. For more information, please contact [email protected]. The Wrong Right Stuff: Why NASA Consistently Fails at Congress A thesis submitted in partial fulfillment of the requirement for the degree of Bachelors of Arts in Government from The College of William and Mary by Andrew Follett Accepted for . John Gilmour, Director . Sophia Hart . Rowan Lockwood Williamsburg, VA May 3, 2013 1 Table of Contents: Acknowledgements 3 Part 1: Introduction and Background 4 Pre Soviet Collapse: Early American Failures in Space 13 Pre Soviet Collapse: The Successful Mercury, Gemini, and Apollo Programs 17 Pre Soviet Collapse: The Quasi-Successful Shuttle Program 22 Part 2: The Thin Years, Repeated Failure in NASA in the Post-Soviet Era 27 The Failure of the Space Exploration Initiative 28 The Failed Vision for Space Exploration 30 The Success of Unmanned Space Flight 32 Part 3: Why NASA Fails 37 Part 4: Putting this to the Test 87 Part 5: Changing the Method. -
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 ......................................................................................................................... -
SPACE EXPLORERS NEED to BE SPACE FARMERS What We Know and What We Need to Know About Plant Growth in Space
MONOGRAPH Mètode Science Studies Journal, 11 (2021). University of Valencia. DOI: 10.7203/metode.11.14606 Submitted: 10/04/2019. Approved: 04/09/2019. SPACE EXPLORERS NEED TO BE SPACE FARMERS What we know and what we need to know about plant growth in space FF.. JJavieravier MMedinaedina Space exploration will require life support systems, in which plants can provide nutrients, oxygen, moisture, and psychological well-being and eliminate wastes. In alien environments, plants must adapt to a diff erent gravity force, even the zero gravity of spacefl ight. Under these conditions, essential cellular and molecular features related to plant development are altered and changes in gene expression occur. In lunar gravity, the eff ects are comparable to microgravity, while the gravity of Mars produces milder alterations. Nevertheless, it has been possible to develop and reproduce plants in space. Current research seeks to identify signals replacing gravity for driving plant growth, such as light. Counteracting gravitational stress will help in enabling agriculture in extraterrestrial habitats. Keywords: plant biology, International Space Station (ISS), microgravity, root meristem, gene ex- pression. ■ INTRODUCTION lighting and nutrient delivery, but utilizes the cabin environment for temperature control and gas On 10 August 2015, the image of three crewmembers exchange (Figure 1b). of the International Space Station (ISS) eating «The farther and longer humans go away from a lettuce, grown and harvested onboard, impacted Earth, the greater the need to be able to grow plants mass media all over the world. «It was one small bite for food, atmosphere recycling and psychological or man, one giant leap for #NASAVEGGIE and our benefi ts», said Gioia Massa (NASA, 2015), Veggie’s #JourneytoMars. -
Growing Knowledge in Space 1 December 2011, by Stephanie Covey
Growing knowledge in space 1 December 2011, By Stephanie Covey The use of plants to provide a reliable oxygen, food and water source could save the time and money it takes to resupply the International Space Station (ISS), and provide sustainable sources necessary to make long-duration missions a reality. However, before plants can be effectively utilized for space exploration missions, a better understanding of their biology under microgravity is essential. Kennedy partnered with the three groups for four months to provide a rapid turnaround experiment opportunity using the BRIC-16 in Discovery's middeck on STS-131. And while research takes time, the process was accelerated as the end of the Space Shuttle Program neared. Arabidopsis seedlings. Credit: NASA Plants are critical in supporting life on Earth, and with help from an experiment that flew onboard space shuttle Discovery's STS-131 mission, they also could transform living in space. NASA's Kennedy Space Center partnered with the University of Florida, Miami University in Ohio and Samuel Roberts Noble Foundation to perform three different experiments in microgravity. The studies concentrated on the effects microgravity has on plant cell walls, root growth patterns and gene regulation within the plant Undifferentiated Arabidopsis cells. Credit: NASA Arabidopsis thaliana. Each of the studies has future applications on Earth and in space exploration. Howard Levine, a program scientist for the ISS "Any research in plant biology helps NASA for Ground Processing and Research Project Office future long-range space travel in that plants will be and the science lead for BRIC-16, said he sees it part of bioregenerative life support systems," said as a new paradigm in how NASA works spaceflight John Kiss, one of the researchers who participated experiments. -
Mrs. Funmilola Adebisi Oluwafemi National Space Research and Development Agency (NASRDA), Abuja, Nigeria, [email protected]
70th International Astronautical Congress 2019 Paper ID: 48743 oral IAF/IAA SPACE LIFE SCIENCES SYMPOSIUM (A1) Biology in Space (8) Author: Mrs. Funmilola Adebisi Oluwafemi National Space Research and Development Agency (NASRDA), Abuja, Nigeria, [email protected] Mr. Adhithiyan Neduncheran Sapienza University of Rome, Italy, [email protected] Mr. Shaun Andrews University of Bristol, United Kingdom, [email protected] Mr. Di Wu University of Arizona, United States, [email protected] METHODS OF SEEDS PLANTING IN SPACE: SOIL-LESS OR NOT Abstract Botanists, gardeners, and farmers alike have worked for thousands of years to perfect growth in any environment. Plants and humans are ideal companions for space travel. Amongst many other things for space travel, humans consume oxygen and release carbonIVoxide, plants return the favor by consuming carbonIVoxide and releasing oxygen. Therefore, space farming's need has being greatly recognized in space travel starting from plants need as human companion to its need for feeding the astronauts. As on Earth, the method of planting seeds for short-term and the proposed long-term space missions require the same basic ingredients for the plants to grow. It takes nutrients, water, oxygen and a good amount of light to get it grown. Astrobotany as the study of plants in space therefore needs to know how to grow them. Space environment is characterized by microgravity or reduced gravity and radiation; and cannot fully support germination, growth and development of plants. Therefore, the most efficient processes for the development of crops in space can be done through closed, controlled or soil-less cultivation systems. -
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. -
Orbital Debris: a Chronology
NASA/TP-1999-208856 January 1999 Orbital Debris: A Chronology David S. F. Portree Houston, Texas Joseph P. Loftus, Jr Lwldon B. Johnson Space Center Houston, Texas David S. F. Portree is a freelance writer working in Houston_ Texas Contents List of Figures ................................................................................................................ iv Preface ........................................................................................................................... v Acknowledgments ......................................................................................................... vii Acronyms and Abbreviations ........................................................................................ ix The Chronology ............................................................................................................. 1 1961 ......................................................................................................................... 4 1962 ......................................................................................................................... 5 963 ......................................................................................................................... 5 964 ......................................................................................................................... 6 965 ......................................................................................................................... 6 966 ........................................................................................................................ -
Mars Sample Return Using Commercial Capabilities: Mission Architecture Overview
IEEE Aerospace Conference Yellowstone Conference Center in Big Sky Montana Session: 2.06 Future Missions & Enabling Technologies for In Situ Exploration, Sample Returns Sat 3/1/2014 Sat 3/8/2014 http://www.aeroconf.org/ Authors: Andrew A. Gonzales, NASA Ames Research Center Lawrence G. Lemke, NASA Ames Research Center Carol R. Stoker , NASA Ames Research Center Nicolas T. Faber, Stinger Ghaffarian Technologies Margaret S. Race, SETI Institute Mars Sample Return Using Commercial Capabilities: Mission Architecture Overview Mars Sample Return (MSR) is the highest priority science mission for the next decade as recommended by the recent Decadal Survey of Planetary Science. This paper presents an overview of a feasibility study for an MSR mission. The objective of the study was to determine whether emerging commercial capabilities can be used to reduce the number of mission systems and launches required to return the samples, with the goal of reducing mission cost. We report the feasibility of a complete and closed MSR mission design using the following scenario that covers three synodic launch opportunities, beginning with the 2022 opportunity: A Falcon Heavy injects a SpaceX Red Dragon capsule and trunk onto a Trans Mars Injection (TMI) trajectory. The capsule is modified to carry all the hardware needed to return samples collected on Mars including a Mars Ascent Vehicle (MAV), an Earth Return Vehicle (ERV), and hardware to transfer a sample collected in a previously landed rover mission to the ERV. The Red Dragon descends to land on the surface of Mars using Super Sonic Retro Propulsion (SSRP). After previously collected samples are transferred to the ERV, the single-stage MAV launches the ERV from the surface of Mars.