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The Reference Mission of the NASA Mars Exploration Study Team
NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor Science Applications International Corporation Houston, Texas David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 This publication is available from the NASA Center for AeroSpace Information, 800 Elkridge Landing Road, Linthicum Heights, MD 21090-2934 (301) 621-0390. Foreword Mars has long beckoned to humankind interest in this fellow traveler of the solar from its travels high in the night sky. The system, adding impetus for exploration. ancients assumed this rust-red wanderer was Over the past several years studies the god of war and christened it with the have been conducted on various approaches name we still use today. to exploring Earth’s sister planet Mars. Much Early explorers armed with newly has been learned, and each study brings us invented telescopes discovered that this closer to realizing the goal of sending humans planet exhibited seasonal changes in color, to conduct science on the Red Planet and was subjected to dust storms that encircled explore its mysteries. The approach described the globe, and may have even had channels in this publication represents a culmination of that crisscrossed its surface. these efforts but should not be considered the final solution. It is our intent that this Recent explorers, using robotic document serve as a reference from which we surrogates to extend their reach, have can continuously compare and contrast other discovered that Mars is even more complex new innovative approaches to achieve our and fascinating—a planet peppered with long-term goal. -
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 ......................................................................................................................... -
Volcanism on Mars
Author's personal copy Chapter 41 Volcanism on Mars James R. Zimbelman Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA William Brent Garry and Jacob Elvin Bleacher Sciences and Exploration Directorate, Code 600, NASA Goddard Space Flight Center, Greenbelt, MD, USA David A. Crown Planetary Science Institute, Tucson, AZ, USA Chapter Outline 1. Introduction 717 7. Volcanic Plains 724 2. Background 718 8. Medusae Fossae Formation 725 3. Large Central Volcanoes 720 9. Compositional Constraints 726 4. Paterae and Tholi 721 10. Volcanic History of Mars 727 5. Hellas Highland Volcanoes 722 11. Future Studies 728 6. Small Constructs 723 Further Reading 728 GLOSSARY shield volcano A broad volcanic construct consisting of a multitude of individual lava flows. Flank slopes are typically w5, or less AMAZONIAN The youngest geologic time period on Mars identi- than half as steep as the flanks on a typical composite volcano. fied through geologic mapping of superposition relations and the SNC meteorites A group of igneous meteorites that originated on areal density of impact craters. Mars, as indicated by a relatively young age for most of these caldera An irregular collapse feature formed over the evacuated meteorites, but most importantly because gases trapped within magma chamber within a volcano, which includes the potential glassy parts of the meteorite are identical to the atmosphere of for a significant role for explosive volcanism. Mars. The abbreviation is derived from the names of the three central volcano Edifice created by the emplacement of volcanic meteorites that define major subdivisions identified within the materials from a centralized source vent rather than from along a group: S, Shergotty; N, Nakhla; C, Chassigny. -
Outer Planets: the Ice Giants
Outer Planets: The Ice Giants A. P. Ingersoll, H. B. Hammel, T. R. Spilker, R. E. Young Exploring Uranus and Neptune satisfies NASA’s objectives, “investigation of the Earth, Moon, Mars and beyond with emphasis on understanding the history of the solar system” and “conduct robotic exploration across the solar system for scientific purposes.” The giant planet story is the story of the solar system (*). Earth and the other small objects are leftovers from the feast of giant planet formation. As they formed, the giant planets may have migrated inward or outward, ejecting some objects from the solar system and swallowing others. The giant planets most likely delivered water and other volatiles, in the form of icy planetesimals, to the inner solar system from the region around Neptune. The “gas giants” Jupiter and Saturn are mostly hydrogen and helium. These planets must have swallowed a portion of the solar nebula intact. The “ice giants” Uranus and Neptune are made primarily of heavier stuff, probably the next most abundant elements in the Sun – oxygen, carbon, nitrogen, and sulfur. For each giant planet the core is the “seed” around which it accreted nebular gas. The ice giants may be more seed than gas. Giant planets are laboratories in which to test our theories about geophysics, plasma physics, meteorology, and even oceanography in a larger context. Their bottomless atmospheres, with 1000 mph winds and 100 year-old storms, teach us about weather on Earth. The giant planets’ enormous magnetic fields and intense radiation belts test our theories of terrestrial and solar electromagnetic phenomena. -
Mars Field Geology, Biology, and Paleontology Workshop, Summary
MARS FIELD GEOLOGY, BIOLOGY, AND PALEONTOLOGY WORKSHOP: SUMMARY AND RECOMMENDATIONS November 18–19, 1998 Space Center Houston, Houston, Texas LPI Contribution No. 968 MARS FIELD GEOLOGY, BIOLOGY, AND PALEONTOLOGY WORKSHOP: SUMMARY AND RECOMMENDATIONS November 18–19, 1998 Space Center Houston Edited by Nancy Ann Budden Lunar and Planetary Institute Sponsored by Lunar and Planetary Institute National Aeronautics and Space Administration Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Contribution No. 968 Compiled in 1999 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with the National Aeronautcis and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This volume may be cited as Budden N. A., ed. (1999) Mars Field Geology, Biology, and Paleontology Workshop: Summary and Recommendations. LPI Contribution No. 968, Lunar and Planetary Institute, Houston. 80 pp. This volume is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Phone: 281-486-2172 Fax: 281-486-2186 E-mail: [email protected] Mail order requestors will be invoiced for the cost of shipping and handling. _________________ Cover: Mars test suit subject and field geologist Dean Eppler overlooking Meteor Crater, Arizona, in Mark III Mars EVA suit. PREFACE In November 1998 the Lunar and Planetary Institute, under the sponsorship of the NASA/HEDS (Human Exploration and Development of Space) Enterprise, held a workshop to explore the objectives, desired capabilities, and operational requirements for the first human exploration of Mars. -
Alien Moons Could Bake Dry from Young Gas Giants' Hot Glow 10 March 2014, by Adam Hadhazy
Alien moons could bake dry from young gas giants' hot glow 10 March 2014, by Adam Hadhazy scenarios because they orbit another body besides their star. A new paper by Heller and his colleague Rory Barnes of the University of Washington and the NASA Virtual Planetary Laboratory examines how heat emanating from a freshly formed exoplanet, coupled with irradiation from the solar system's star, can roast the planet's moons. Before the planet cools off sufficiently, its close-orbiting moons could lose all their water, leaving them bone-dry and barren. "An exomoon's habitability is of course constrained by its location in the stellar habitable zone, but it also has a second heat source—its host planet—that has to be accounted for," said Heller, whose paper An Earthlike moon orbiting a gas giant host planet. has been accepted for publication in The Credit: NASA International Journal of Astrobiology. "With regard to this second source, our study shows that at close range, the illumination from young and hot giant planets can render their moons uninhabitable." When we think of where else life might exist in the universe, we tend to focus on planets. But on a Researchers believe moons could serve as suitable grander cosmic scale, moons could prove the more abodes for life just as well as planets. Even moons common life-friendly abode. far beyond the habitable zone, such as Jupiter's Europa and Saturn's Titan, offer tantalizing hints of A single gas giant planet in the not-too-warm, not- potential habitability thanks to the subsurface too-cold habitable zone around its star—where ocean in the former and the intriguing organic Earth and Mars correspondingly reside—could host chemistry of the latter. -
Seasonal and Interannual Variability of Solar Radiation at Spirit, Opportunity and Curiosity Landing Sites
Seasonal and interannual variability of solar radiation at Spirit, Opportunity and Curiosity landing sites Álvaro VICENTE-RETORTILLO1, Mark T. LEMMON2, Germán M. MARTÍNEZ3, Francisco VALERO4, Luis VÁZQUEZ5, Mª Luisa MARTÍN6 1Departamento de Física de la Tierra, Astronomía y Astrofísica II, Universidad Complutense de Madrid, Madrid, Spain, [email protected]. 2Department of Atmospheric Sciences, Texas A&M University, College Station, TX, USA, [email protected]. 3Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA, [email protected]. 4Departamento de Física de la Tierra, Astronomía y Astrofísica II, Universidad Complutense de Madrid, Madrid, Spain, [email protected]. 5Departamento de Matemática Aplicada, Universidad Complutense de Madrid, Madrid, Spain, [email protected]. 6Departamento de Matemática Aplicada, Universidad de Valladolid, Segovia, Spain, [email protected]. Received: 14/04/2016 Accepted: 22/09/2016 Abstract In this article we characterize the radiative environment at the landing sites of NASA's Mars Exploration Rover (MER) and Mars Science Laboratory (MSL) missions. We use opacity values obtained at the surface from direct imaging of the Sun and our radiative transfer model COMIMART to analyze the seasonal and interannual variability of the daily irradiation at the MER and MSL landing sites. In addition, we analyze the behavior of the direct and diffuse components of the solar radiation at these landing sites. Key words: Solar radiation; Mars Exploration Rovers; Mars Science Laboratory; opacity, dust; radiative transfer model; Mars exploration. Variabilidad estacional e interanual de la radiación solar en las coordenadas de aterrizaje de Spirit, Opportunity y Curiosity Resumen El presente artículo está dedicado a la caracterización del entorno radiativo en los lugares de aterrizaje de las misiones de la NASA de Mars Exploration Rover (MER) y de Mars Science Laboratory (MSL). -
Constructing the Solar System: a Smashing Success
Constructing the Solar System: A Smashing Success A Star is Born Thomas M. Davison Department of the Geophysical Sciences Compton Lecture Series October 6, 2012 T. M. Davison Constructing the Solar System Compton Lectures { Autumn 2012 1 Today's lecture 1 An overview of the Compton Lecture Series 2 A tour of the Solar System 3 Physical properties of the Solar System What can they tell us about the Solar System's formation? 4 How was our star born? The nebula hypothesis of star formation Images courtesy of NASA T. M. Davison Constructing the Solar System Compton Lectures { Autumn 2012 2 Part 1: Introduction to the lecture series Image courtesy of NASA T. M. Davison Constructing the Solar System Compton Lectures { Autumn 2012 3 Constructing the Solar System ... How did the Sun, the planets and the asteroids form? What were their histories like? One process dominates throughout Solar System history: Collisions Growth of asteroids and planets Formation of the Moon Extinction of the dinosaurs After such a violent history, we now have a habitable planet Which you could call: ... A Smashing Success! Images Courtesy of NASA T. M. Davison Constructing the Solar System Compton Lectures { Autumn 2012 4 My day job: Making an impact Computer simulations of collisions between planetesimals Simulations by T. Davison T. M. Davison Constructing the Solar System Compton Lectures { Autumn 2012 5 Compton Lecture Series Schedule 1 10/06/12 A Star is Born 2 10/13/12* Making Planetesimals: the building blocks of planets 3 10/20/12* Guest Lecturer: Mac Cathles 4 10/27/12 Asteroids, Comets and Meteorites: 10/27/12 our eyes in the early Solar System 5 11/03/12 Building the Planets 6 11/10/12 When Asteroids Collide 7 11/17/12 Making Things Hot: The thermal effects of collisions 11/24/12 No lecture: Thanksgiving weekend 8 12/01/12 Constructing the Moon 12/08/12 No lecture: Physics with a Bang! 9 12/15/12 Impact Earth: Chicxulub and other terrestrial impacts T. -
Mixing of the Asteroid Belt Due to the Formation of the Giant Planets
Accretion: Building New Worlds (2017) 2027.pdf MIXING OF THE ASTEROID BELT DUE TO THE FORMATION OF THE GIANT PLANETS. K. A. Kretke1, W. F. Bottke2,3, H. F. Levison2,3, and D. A. Kring4,5, 1SSERVI NPP Fellow ([email protected]), 2Southwest Research Institute, 1050 Walnut St, Suite 300, Boulder, CO 80302, USA, 3ISET, NASA-SSERVI, 4LPI, 3600 Bay Area Blvd, Houston, TX 77058, USA 5CLSE, NASA-SSERVI. Introduction: The asteroid belt is observed to be a evolution of a solar system forming under these condi- mixture of objects with different compositions, with tions. LIPAD is based upon the N-Body integrator volatile-poor asteroids (mostly S-complex) dominant in SWIFT [10] but uses novel algorithms to statistically the inner asteroid belt while volatile-rich (mostly C- follow bodies that are too small and numerous to be han- complex) asteroids dominate the outer asteroid belt. dled in a traditional N-body integrator. This allows us to While this general compositional stratification was orig- model how our system may have evolved starting from inally thought to be an indicator of the primordial tem- pebbles and planetesimals all the way to a mature plan- perature gradient in the protoplanetary disk, there is etary system. growing evidence that that meteorites believed to origi- To test the effect of giant planet formation in the as- nate from those different types of asteroids appear to teroid belt we placed a population planetesimals in outer come from very distinct reservoirs, with distinct iso- Solar System and allow them to accrete pebbles. To topic and elemental signatures [1,2,3]. -
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 ...................................................................................................................... -
NASA Technical Memorandum 0000
NASA/TM–2016-219182 Frontier In-Situ Resource Utilization for Enabling Sustained Human Presence on Mars Robert W. Moses and Dennis M. Bushnell Langley Research Center, Hampton, Virginia April 2016 NASA STI Program . in Profile Since its founding, NASA has been dedicated to the CONFERENCE PUBLICATION. advancement of aeronautics and space science. The Collected papers from scientific and technical NASA scientific and technical information (STI) conferences, symposia, seminars, or other program plays a key part in helping NASA maintain meetings sponsored or this important role. co-sponsored by NASA. The NASA STI program operates under the auspices SPECIAL PUBLICATION. Scientific, of the Agency Chief Information Officer. It collects, technical, or historical information from NASA organizes, provides for archiving, and disseminates programs, projects, and missions, often NASA’s STI. The NASA STI program provides access concerned with subjects having substantial to the NTRS Registered and its public interface, the public interest. NASA Technical Reports Server, thus providing one of the largest collections of aeronautical and space TECHNICAL TRANSLATION. science STI in the world. Results are published in both English-language translations of foreign non-NASA channels and by NASA in the NASA STI scientific and technical material pertinent to Report Series, which includes the following report NASA’s mission. types: Specialized services also include organizing TECHNICAL PUBLICATION. Reports of and publishing research results, distributing completed research or a major significant phase of specialized research announcements and feeds, research that present the results of NASA providing information desk and personal search Programs and include extensive data or theoretical support, and enabling data exchange services. -
GOAL Students Debate Whether Future Mars Exploration Should Be Continued with Robotic Missions And/Or Human Missions
GOAL Students debate whether future Mars exploration should be continued with robotic missions and/or human missions. OBJECTIVE Students are assigned societal roles and use information provided on role cards to argue opinions in a class debate. Students must then research their roles to provide evidence to argue their case. The teacher will decide if and how the debate is judged. NATIONAL SCIENCE STANDARDS Grade Content Standard Developing Student Underlying Fundamental Concepts and Level Understanding Area Principals 5 - 8 Science in Personal Risks and Benefits Important personal and social decisions and Social are made based on perceptions of benefits Perspectives and risks. 5 - 8 Science in Personal Science and Technology in Science influences society through its and Social Society knowledge and world view. Perspectives 5 - 8 History and Nature Science as a Human Endeavor Science is very much a human endeavor, of Science and the work of science relies on basic human qualities, such as reasoning, insight, energy, skill, and creativity 5 - 8 History and Nature Nature of Science Although scientists may disagree about of Science explanations of phenomena, about interpretations of data, or about the value of rival theories, they do agree that questioning, response to criticism, and open communication are integral to the process of science. TIME FRAME • 2 class periods (100 minutes) MATERIALS • Role Cards (1 per student group) Page 1 of 12 Mars Exploration Debate ______________________________________________________________________________ TEACHER PREPARATION • Cut out Role Cards. • Decide if and how the debate will be judged. Options include: - Have students debate, but leave open, what the future of Mars exploration should be.