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A Teacher's Guide
A Teacher’s Guide for LIFE on Earth – and Beyond: An Astrobiologist’s Quest About the Book: Astrobiologists have searched Earth’s most extreme environments in their quest to understand what factors are necessary to sustain life. Dr. Chris McKay’s scientific journey has taken him from the freezing cold of Antarctica’s Dry Valleys to the rocky wasteland of the Atacama Desert in Chile to the permafrost-covered tundra of Siberia. By studying environments on Earth that resemble those on Mars and elsewhere in the solar system, Dr. McKay hopes that his experiments will help answer the ultimate question: is there life beyond Earth? About the Author: Pamela Turner has written for kids and young adults, mostly about science and nature. She also has a strong interest in multicultural literature because she’s lived in and worked in Kenya, South Africa, Japan, the Philippines, and the Marshall Islands. Hardback ISBN 978-1580891332 Honors and Awards: School Library Journal starred review, Booklist starred review, Bank Street College of Education Best Books List, AAAS/Subaru Science Writing Prize Prize finalist, Booklist Top Ten Sci-Tech Books for Youth, NSTA Outstanding Science Trade Book, Booklist Editors’ Choice, CCBC Choice. Booklist Starred Review: "Astrobiologists look outward from the Earth seeking evidence of life elsewhere in the Universe. But, as this fascinating book shows, they also travel to places on Earth where extreme conditions may be similar to those on distant worlds... Turner's absorbing account gives enough detail to create vivid impressions of McKay's explorations and enough background information to show what his amazing findings imply. -
Bibliography
Bibliography Books and reports Blandford, R.D. (Chair) New Worlds, New Horizons in Astronomy and Astrophysics Committee for a Decadal Survey of Astronomy and Astrophysics, National Research Council, 2010 Bondi, Hermann. et al Pioneering in Outer Space Heinemann Educational Books, 1971 Clarke, Arthur C. The Exploration of Space Temple Press, London, 1951 Department of Energy/NASA Satellite Power Systems Concept Development and Evaluation Program. DoE/NASA, October 1978 http://www.nss.org/settlement/ssp/library/1978DOESPS-ReferenceSystemReport.pdf Satellite Power Systems (SPS) Space Transportation Cost Analysis and Evaluation. DoE/NASA, November 1980 http://www.nss.org/settlement/ssp/library/1980DOESPS- SpaceTransportationCostAnalysis.pdf Dick, Steven J. (editor) Remembering the Space Age: Proceedings of the 50th Anniversary Conference. NASA SP-2008-4703, 2008 http://history.nasa.gov/Remembering_Space_Age_A.pdf © Springer International Publishing AG 2017 235 M. van Pelt, Dream Missions, Springer Praxis Books, DOI 10.1007/978-3-319-53941-6 236 Bibliography Dyson, George Project Orion: The True Story of the Atomic Spaceship Henry Holt & Company, Inc., USA, 2002 Ehricke, Krafft A. Solar Transportation In Space Age in Fiscal Year 2001, Proceedings of the Fourth AAS Goddard Memorial Symposium American Astronautical Society, 1966 Friedman, Louis. Human Spaceflight, from Mars to the Stars The University of Arizona Press, 2015 Gatland, Kenneth W. & Bono, Philip Frontiers of Space Blandford Press, UK, 1969 Hansen, James R. Chapter 9, Skipping “The Next Logical Step” in Spaceflight Revolution; NASA Langley Research Center from Sputnik to Apollo NASA History Series SP-4308, USA, 1994 http://history.nasa.gov/SP-4308/ch9.htm Koelle, Heinz-Hermann. Nova and Beyond, a Review of Heavy Lift Launch Vehicle Concepts in the Post-Saturn Class Technical University Berlin, Germany, 2001 Konecci, Eugene B. -
Bio-Preservation Potential of Sediment in Eberswalde Crater, Mars
Western Washington University Western CEDAR WWU Graduate School Collection WWU Graduate and Undergraduate Scholarship Fall 2020 Bio-preservation Potential of Sediment in Eberswalde crater, Mars Cory Hughes Western Washington University, [email protected] Follow this and additional works at: https://cedar.wwu.edu/wwuet Part of the Geology Commons Recommended Citation Hughes, Cory, "Bio-preservation Potential of Sediment in Eberswalde crater, Mars" (2020). WWU Graduate School Collection. 992. https://cedar.wwu.edu/wwuet/992 This Masters Thesis is brought to you for free and open access by the WWU Graduate and Undergraduate Scholarship at Western CEDAR. It has been accepted for inclusion in WWU Graduate School Collection by an authorized administrator of Western CEDAR. For more information, please contact [email protected]. Bio-preservation Potential of Sediment in Eberswalde crater, Mars By Cory M. Hughes Accepted in Partial Completion of the Requirements for the Degree Master of Science ADVISORY COMMITTEE Dr. Melissa Rice, Chair Dr. Charles Barnhart Dr. Brady Foreman Dr. Allison Pfeiffer GRADUATE SCHOOL David L. Patrick, Dean Master’s Thesis In presenting this thesis in partial fulfillment of the requirements for a master’s degree at Western Washington University, I grant to Western Washington University the non-exclusive royalty-free right to archive, reproduce, distribute, and display the thesis in any and all forms, including electronic format, via any digital library mechanisms maintained by WWU. I represent and warrant this is my original work, and does not infringe or violate any rights of others. I warrant that I have obtained written permissions from the owner of any third party copyrighted material included in these files. -
J. Judson Wynne, Ph.D. PROFESSIONAL PREPARATION
J. Judson Wynne, Ph.D. CURRICULUM VITAE The SETI Institute, Carl Sagan Center 189 Bernardo Ave., Mountain View, CA 94043 Phone: 928.863.8628 (cell), Email: [email protected], Web: http://www.jutwynne.com PROFESSIONAL PREPARATION Northern Arizona University (2014) Ph.D. Biological Sciences; emphasis ecology Title: On Sampling, Habitat and Relict Species of Cave-dwelling Arthropods of the American Southwest and Easter Island Northern Arizona University (2003) M.S. EnvironMental Science and Policy; eMphasis wildlife ecology and reMote sensing Title: Landscape-scale Modeling of Vegetation Land Cover and Songbird Habitat, Pinaleños Mountains, Arizona Vrije Universiteit Brussel, BelGium (1998) Certificate in Ecotechnie (Distinction: Magna cum laude) UNESCO-Cousteau European Postgraduate PrograMMe of Ecotechnie GeorGia Southern University (1993) B.S. Major: CoMMunications, Minor: Anthropology PUBLICATIONS Peer-Reviewed Publications (16) Harvey, M.S. and J.J. Wynne. In Press. Cave-dwelling Pseudoscorpions (Arachnida, Pseudoscorpiones) of Arizona, with descriptions of two short-range endeMic species froM North RiM Grand Canyon. Journal of Arachnology. Wynne, J.J., E.C. Bernard, F.G. Howarth, S. SoMMer, F.N. Soto-AdaMes, S. Taiti, E.L. Mockford, M. Horrocks, L. Pakarati, and V. Pakarati-Hotus. 2014. Disturbance relicts in a rapidly changing world: the Rapa Nui (Easter Island) factor. BioScience 64: 711–718. Wynne, J.J. and K.D. Voyles. 2014. Cave-dwelling arthropods and vertebrates of North RiM Grand Canyon, with notes on ecology and Management. Western North American Naturalist 74: 1–17. Wynne, J.J. 2014. Reign of the Red Queen: The future of bats hangs in the balance. The Explorers Journal 92: 40–45. -
Humanity and Space
10/17/2012!! !!!!!! Project Number: MH-1207 Humanity and Space An Interactive Qualifying Project Submitted to WORCESTER POLYTECHNIC INSTITUTE In partial fulfillment for the Degree of Bachelor of Science by: Matthew Beck Jillian Chalke Matthew Chase Julia Rugo Professor Mayer H. Humi, Project Advisor Abstract Our IQP investigates the possible functionality of another celestial body as an alternate home for mankind. This project explores the necessary technological advances for moving forward into the future of space travel and human development on the Moon and Mars. Mars is the optimal candidate for future human colonization and a stepping stone towards humanity’s expansion into outer space. Our group concluded space travel and interplanetary exploration is possible, however international political cooperation and stability is necessary for such accomplishments. 2 Executive Summary This report provides insight into extraterrestrial exploration and colonization with regards to technology and human biology. Multiple locations have been taken into consideration for potential development, with such qualifying specifications as resources, atmospheric conditions, hazards, and the environment. Methods of analysis include essential research through online media and library resources, an interview with NASA about the upcoming Curiosity mission to Mars, and the assessment of data through mathematical equations. Our findings concerning the human aspect of space exploration state that humanity is not yet ready politically and will not be able to biologically withstand the hazards of long-term space travel. Additionally, in the field of robotics, we have the necessary hardware to implement adequate operational systems yet humanity lacks the software to implement rudimentary Artificial Intelligence. Findings regarding the physics behind rocketry and space navigation have revealed that the science of spacecraft is well-established. -
Astrobio Novel 5 Firstedition Hir
National Aeronautics and Space Administration Issue #5 Produced by the NASA Astrobiology Program to commemorate 50 years of Exobiology and Astrobiology at NASA. www.nasa.gov PB 1 Astrobiology A History of Exobiology and Astrobiology at NASA This is the story of life in the Universe—or at least the story as we know it so far. As scientists, we strive to understand the environment in which we live and how life re- lates to this environment. As astrobiologists, we study an environment that includes not just the Earth, but the entire Universe in which we live. The year 2010 marked 50 years of Exobiology and Astrobiology research at the Na- tional Aeronautics and Space Administration (NASA). To celebrate, the Astrobiology Program commissioned this graphic history. It tells the story of some of the most important people and events that have shaped the science of Exobiology and Astro- biology. At just over 50 years old, this field is relatively young. However, as you will see, the questions that astrobiologists are trying to answer are as old as humankind. Concept & Story Mary Voytek Linda Billings Aaron L. Gronstal Artwork Aaron L. Gronstal Script Aaron L. Gronstal Editor Linda Billings Layout Aaron L. Gronstal Copyright 2015, NASA Astrobiology Program First edition printed in 2015 Issue #5—Astrobiology and the Earth The year 2010 marked the 50th anniversary of NASA’s Exobiology Program, estab- lished in 1960 and expanded into a broader Astrobiology Program in the 1990s. To commemorate the past half century of research, we are telling the story of how this field developed and how the search for life elsewhere became a key compo- nent of NASA’s science strategy for exploring space. -
Cambridge University Press 978-1-107-03629-1 — the Atlas of Mars Kenneth S
Cambridge University Press 978-1-107-03629-1 — The Atlas of Mars Kenneth S. Coles, Kenneth L. Tanaka, Philip R. Christensen Index More Information Index Note: page numbers in italic indicates figures or tables Acheron Fossae 76, 76–77 cuesta 167, 169 Hadriacus Cavi 183 orbit 1 Acidalia Mensa 86, 87 Curiosity 9, 32, 62, 195 Hadriacus Palus 183, 184–185 surface gravity 1, 13 aeolian, See wind; dunes Cyane Catena 82 Hecates Tholus 102, 103 Mars 3 spacecraft 6, 201–202 Aeolis Dorsa 197 Hellas 30, 30, 53 Mars Atmosphere and Volatile Evolution (MAVEN) 9 Aeolis Mons, See Mount Sharp Dao Vallis 227 Hellas Montes 225 Mars Chart 1 Alba Mons 80, 81 datum (zero elevation) 2 Hellas Planitia 220, 220, 226, 227 Mars Exploration Rovers (MER), See Spirit, Opportunity albedo 4, 5,6,10, 56, 139 deformation 220, See also contraction, extension, faults, hematite 61, 130, 173 Mars Express 9 alluvial deposits 62, 195, 197, See also fluvial deposits grabens spherules 61,61 Mars Global Surveyor (MGS) 9 Amazonian Period, history of 50–51, 59 Deimos 62, 246, 246 Henry crater 135, 135 Mars Odyssey (MO) 9 Amenthes Planum 143, 143 deltas 174, 175, 195 Herschel crater 188, 189 Mars Orbiter Mission (MOM) 9 Apollinaris Mons 195, 195 dikes, igneous 82, 105, 155 Hesperia Planum 188–189 Mars Pathfinder 9, 31, 36, 60,60 Aram Chaos 130, 131 domical mound 135, 182, 195 Hesperian Period, history of 50, 188 Mars Reconnaissance Orbiter (MRO) 9 Ares Vallis 129, 130 Dorsa Argentea 239, 240 Huygens crater 183, 185 massif 182, 224 Argyre Planitia 213 dunes 56, 57,69–70, 71, 168, 185, -
Krista Marie Soderlund the University of Texas at Austin Institute for Geophysics, John A
Krista Marie Soderlund The University of Texas at Austin Institute for Geophysics, John A. & Katherine G. Jackson School of Geosciences J.J. Pickle Research Campus, Bldg. 196 (ROC), 10100 Burnet Rd. (R2200), Austin, TX 78758-4445 [email protected], Office: 512-471-0449, Cell: 218-349-3006, FAX: 512-471-8844 Research Interests Geophysical Fluid Dynamics, Magnetohydrodynamics, Planetary Science, Cryosphere Education University of California, Los Angeles Ph.D., Geophysics and Space Physics, 2011 M.S., Geophysics and Space Physics, 2009 Florida Institute of Technology B.S., Double major in Physics & Space Science, 2005, Summa Cum Laude Employment University of Texas at Austin, Institute for Geophysics Research Associate, September 2014-Present UTIG Postdoctoral Fellow, October 2011-September 2014 University of California, Los Angeles, Department of Earth and Space Sciences Graduate Student Researcher, Advisor: Dr. Jonathan M. Aurnou, 2006-2011 California Institute of Technology, Division of Geological and Planetary Sciences Summer Undergraduate Research Fellow, Dr. Joann M. Stock, 2005 NASA Jet Propulsion Laboratory, CA Consultant, Dr. Bonnie J. Buratti, 2006 Planetary Geology & Geophysics Undergrad Research Program, Dr. B.J. Buratti, 2004 Florida Institute of Technology, Department of Physics and Space Science Undergraduate Researcher, Dr. Niescja E. Turner, 2004-2005 Naval Oceanographic Office, Hydrology Code, Stennis Space Center, MS Physical science aid, 2003 Mission Experience Saturn Probe Interior and aTmosphere Explorer (SPRITE) -
A Star's Birth Holds Early Clues to Life Potential 25 July 2016, by Elizabeth Howell, Astrobiology Magazine
A star's birth holds early clues to life potential 25 July 2016, by Elizabeth Howell, Astrobiology Magazine serpent). Their goal was to see how light scattering affects the view of the cloud at the mid-infrared wavelength of 8 microns (?m). Ultimately, the astronomers hope to use this data to get a better look inside the clouds. "One thing we have to do is evaluate the mass that is sitting in the center of the cloud, which is ready to collapse to make a star," said co-author Laurent Pagani, a researcher at the National Center for Scientific Research (CNRS) in Paris, France. His former doctoral student, Charlène Lefèvre, led the research. Their work was recently published in the journal Astronomy and Astrophysics under the title, "On the importance of scattering at 8 ?m: Brighter than you think." Funding for the research The dust cloud L183, identified as a likely region of came from CNRS and the French government. future solar systems, was imaged by the Spitzer Space Telescope for research published in 2010. Credit: NASA/JPL-Caltech/Observatoire de Paris/CNRS Our solar system began as a cloud of gas and dust. Over time, gravity slowly pulled these bits together into the Sun and planets we recognize today. While not every system is friendly to life, astronomers want to piece together how these systems are formed. A challenge to this research is the opacity of dust clouds to optical wavelengths (the ones that humans can see). So, astronomers are experimenting with different wavelengths, such as infrared light, to better see the center of dense dust clouds, where young stars typically form. -
The Dorsa Argentea Formation: Synthesis of Glacial Features and History of Late Noachian-Early Hesperian Martian Climate Change
45th Lunar and Planetary Science Conference (2014) 1477.pdf THE DORSA ARGENTEA FORMATION: SYNTHESIS OF GLACIAL FEATURES AND HISTORY OF LATE NOACHIAN-EARLY HESPERIAN MARTIAN CLIMATE CHANGE. K. E. Scanlon and J. W. Head III, Department of Geological Sciences, Brown University, Providence, RI, USA. <[email protected]> Introduction: The Noachian and Hesperian-aged ge- Cavi Angusti and Argentea Planum have been inter- omorphological units mapped [1-2] as the Dorsa Ar- preted as the remnants of a proglacial lake [3, 21]. gentea Formation (DAF) and the Hesperian-Noachian undivided unit cover a combined area of ~1.5 · 106 km2 [3] surrounding and offset from the south pole of Mars. The units are characterized by sinuous and braided ridges, including the Dorsa Argentea for which the formation is named [e.g. 4-10], several regions of pit- ted terrain, the Cavi Angusti and Sisyphi Cavi [e.g. 11- 13]; and steep-sided mountains, the Sisyphi Montes [e.g. 14]. A radar reflector closely correlated with the outline of the deposit is consistent with high concentra- tions of volatiles in and underlying the deposit [15]. In earlier work based on Mariner and Viking im- ages, researchers proposed volcanic, tectonic, inverted stream, aeolian, and clastic dike origins for the Dorsa Argentea and other sinuous ridges (e.g., [1, 5]; see re- view in [3]) and widely agreed on an aeolian origin for the cavi [e.g. 11, 12]. Howard [4] was the first to pro- Fig. 1. Features interpreted to be of glacial origin in the Dorsa Ar- pose a glacial origin for the deposit, wherein the sinu- gentea formation include cavi interpreted as melt-out terrains [e.g. -
Ames Research Center FY 2004 Implementation Plan
Table of Contents iii Letter from the Director 1 Ames Research Center in NASA Vision and Mission 5 Supporting NASA Themes and Goals 10 Space Science Enterprise 18 Earth Science Enterprise 21 Biological and Physical Research Enterprise 25 Education Enterprise 26 Space Flight Enterprise 28 Aerospace Technology Enterprise 43 Current Capabilities 46 Ames Core Capabilities 51 Ames Workforce 53 Ames Real Property 54 Ames Campus Research Facilities 59 Future Plans 62 Future Research Activities 67 Building the Future Workforce (cover) This image shows 69 Future of Ames Property an "end on" view of a simulated carbon 73 Implementing Strategies nanotube that is being compressed—the spheres represent carbon atoms, and they are colored according to their 82 Appendix: For More Information— potential energy. Carbon nanotubes are of great interest to nanotech- nologists at Ames and elsewhere, since they have very useful mechanical and electrical properties. Ames Research Center i 2004 Implementation Plan Letter From the Director Ames Research Center boasts a proud history most fundamental questions, the Astrobiology of innovation and discovery that spans more than scientists and NASA Astrobiology Institute cen- 60 years. Today, at the beginning of the 21st Cen- tered at Ames ask: How does life begin and evolve? tury, we face new challenges and new opportu- Is there life elsewhere in the Universe? What is the nities. Our responses will define us as an institu- future of life on Earth and beyond? Ames created tion. We will measure ourselves by our creativ- the interdisciplinary field of Astrobiology less ity, innovation, and dedication to The NASA than a decade ago and today leads more than Vision. -
NASA ASTROBIOLOGY STRATEGY 2015 I
NASA ASTROBIOLOGY STRATEGY 2015 i CONTRIBUTIONS Editor-in-Chief Lindsay Hays, Jet Propulsion Laboratory, California Institute of Technology Lead Authors Laurie Achenbach, Southern Illinois University Karen Lloyd, University of Tennessee Jake Bailey, University of Minnesota Tim Lyons, University of California, Riverside Rory Barnes, University of Washington Vikki Meadows, University of Washington John Baross, University of Washington Lucas Mix, Harvard University Connie Bertka, Smithsonian Institution Steve Mojzsis, University of Colorado Boulder Penny Boston, New Mexico Institute of Mining and Uli Muller, University of California, San Diego Technology Matt Pasek, University of South Florida Eric Boyd, Montana State University Matthew Powell, Juniata College Morgan Cable, Jet Propulsion Laboratory, California Institute of Technology Tyler Robinson, Ames Research Center Irene Chen, University of California, Santa Barbara Frank Rosenzweig, University of Montana Fred Ciesla, University of Chicago Britney Schmidt, Georgia Institute of Technology Dave Des Marais, Ames Research Center Burckhard Seelig, University of Minnesota Shawn Domagal-Goldman, Goddard Space Flight Center Greg Springsteen, Furman University Jamie Elsila Cook, Goddard Space Flight Center Steve Vance, Jet Propulsion Laboratory, California Institute of Technology Aaron Goldman, Oberlin College Paula Welander, Stanford University Nick Hud, Georgia Institute of Technology Loren Williams, Georgia Institute of Technology Pauli Laine, University of Jyväskylä Robin Wordsworth, Harvard