The Future of Construction As It Applies to the Colonization of the Moon and Mars
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Climate Change and Human Health: Risks and Responses
Climate change and human health RISKS AND RESPONSES Editors A.J. McMichael The Australian National University, Canberra, Australia D.H. Campbell-Lendrum London School of Hygiene and Tropical Medicine, London, United Kingdom C.F. Corvalán World Health Organization, Geneva, Switzerland K.L. Ebi World Health Organization Regional Office for Europe, European Centre for Environment and Health, Rome, Italy A.K. Githeko Kenya Medical Research Institute, Kisumu, Kenya J.D. Scheraga US Environmental Protection Agency, Washington, DC, USA A. Woodward University of Otago, Wellington, New Zealand WORLD HEALTH ORGANIZATION GENEVA 2003 WHO Library Cataloguing-in-Publication Data Climate change and human health : risks and responses / editors : A. J. McMichael . [et al.] 1.Climate 2.Greenhouse effect 3.Natural disasters 4.Disease transmission 5.Ultraviolet rays—adverse effects 6.Risk assessment I.McMichael, Anthony J. ISBN 92 4 156248 X (NLM classification: WA 30) ©World Health Organization 2003 All rights reserved. Publications of the World Health Organization can be obtained from Marketing and Dis- semination, World Health Organization, 20 Avenue Appia, 1211 Geneva 27, Switzerland (tel: +41 22 791 2476; fax: +41 22 791 4857; email: [email protected]). Requests for permission to reproduce or translate WHO publications—whether for sale or for noncommercial distribution—should be addressed to Publications, at the above address (fax: +41 22 791 4806; email: [email protected]). The designations employed and the presentation of the material in this publication do not imply the expression of any opinion whatsoever on the part of the World Health Organization concerning the legal status of any country, territory, city or area or of its authorities, or concerning the delimitation of its frontiers or boundaries. -
Potential European Contributions to Europa Lander Mission
The Europa Initiative for ESA’s M5 mission Report to OPAG Michel Blanc, Geraint Jones, Olga Prieto-Ballesteros, Veerle Sterken, Javier Gomez-Elvira, David Mimoun, Adam Masters, Sascha Kempf, Luciano Iess, John Cooper, Zita Martins, Ralph Lorenz, Jérémie lasue, Nicolas André, Bruce Bills, Gael Choblet, Geoff Collins, Philippe Garnier, Kevin Hand, Paul Hartogh, Krishan Khurana, Andrea Longobardo, Katrin Stephan, Federico Tosi, Steve Vance, Tim van Hoolst, Roland Wagner, Frances Westall, Martin Wolverk, William Desprats, Ryan Russell, Georges Balmino, Julien Laurent-Varin and the Europa Initiative team August 11th, 2016 1 EI WORKING SCHEME Europa M5 for an ESA contribution to the Europa Lander mission Initiative Penetrator Contribution to Cubesat? Orbiter or… NASA lander A – GLOBAL GEOPHYSICSMagnetospheric interactions CHARACTERIZE EUROPA AS A COMPLEX DYNAMICAL SYSTEM B – ExosphereOF COUPLED LAYERS(neutrals, dust, plumes) FROM CORE TO PLASMA ENVELOPE THROUGH OCEAN AND CRYOSPHERE dimension RESPONDING TO E – Geophysics (internalJUPITER SYSTEM FORCING: TIDAL, MAGNETOSPHERICstructure, incl. Characterization of the ocean) themes ASTROBIOLOGY CONTRIBUTE TO NASA’s LANDER SCIENCE Science AND PROVIDE AN ADDITIONAL ELEMENT (AWL) As resources permit « Spacecraft » dimension EI contribution to EUROPA LanDer : SubmitteD LOI’s Joint Europa Mission (Blanc/Prieto-Ballesteros) • Baseline: Carrier-Orbiter + lander joint NASA/ESA mission: – P1a: Carrier-Orbiter provided by ESA, operated by NASA; – P1b: Alternative option: Carrier-Orbiter provided and operated by NASA; science platform (+ sub-systems?) provided by ESA – Science platform open to both ESA member states and NASA • Option 1: Augmented surface science: Astrobiology Wet Laboratory (AWL) provided by ESA + Member States to enhance landing site exploration. • Option 2: Augmented orbital science - cubesat released from carrier. -
NASA Develops Wireless Tile Scanner for Space Shuttle Inspection
August 2007 NASA, Microsoft launch collaboration with immersive photography NASA and Microsoft Corporation a more global view of the launch facil- provided us with some outstanding of Redmond, Wash., have released an ity. The software uses photographs images, and the result is an experience interactive, 3-D photographic collec- from standard digital cameras to that will wow anyone wanting to get a tion of the space shuttle Endeavour construct a 3-D view that can be navi- closer look at NASA’s missions.” preparing for its upcoming mission to gated and explored online. The NASA The NASA collections were created the International Space Station. Endea- images can be viewed at Microsoft’s in collaboration between Microsoft’s vour launched from NASA Kennedy Live Labs at: http://labs.live.com Live Lab, Kennedy and NASA Ames. Space Center in Florida on Aug. 8. “This collaboration with Microsoft “We see potential to use Photo- For the first time, people around gives the public a new way to explore synth for a variety of future mission the world can view hundreds of high and participate in America’s space activities, from inspecting the Interna- resolution photographs of Endeav- program,” said William Gerstenmaier, tional Space Station and the Hubble our, Launch Pad 39A and the Vehicle NASA’s associate administrator for Space Telescope to viewing landing Assembly Building at Kennedy in Space Operations, Washington. “We’re sites on the moon and Mars,” said a unique 3-D viewer. NASA and also looking into using this new tech- Chris C. Kemp, director of Strategic Microsoft’s Live Labs team developed nology to support future missions.” Business Development at Ames. -
Project Selene: AIAA Lunar Base Camp
Project Selene: AIAA Lunar Base Camp AIAA Space Mission System 2019-2020 Virginia Tech Aerospace Engineering Faculty Advisor : Dr. Kevin Shinpaugh Team Members : Olivia Arthur, Bobby Aselford, Michel Becker, Patrick Crandall, Heidi Engebreth, Maedini Jayaprakash, Logan Lark, Nico Ortiz, Matthew Pieczynski, Brendan Ventura Member AIAA Number Member AIAA Number And Signature And Signature Faculty Advisor 25807 Dr. Kevin Shinpaugh Brendan Ventura 1109196 Matthew Pieczynski 936900 Team Lead/Operations Logan Lark 902106 Heidi Engebreth 1109232 Structures & Environment Patrick Crandall 1109193 Olivia Arthur 999589 Power & Thermal Maedini Jayaprakash 1085663 Robert Aselford 1109195 CCDH/Operations Michel Becker 1109194 Nico Ortiz 1109533 Attitude, Trajectory, Orbits and Launch Vehicles Contents 1 Symbols and Acronyms 8 2 Executive Summary 9 3 Preface and Introduction 13 3.1 Project Management . 13 3.2 Problem Definition . 14 3.2.1 Background and Motivation . 14 3.2.2 RFP and Description . 14 3.2.3 Project Scope . 15 3.2.4 Disciplines . 15 3.2.5 Societal Sectors . 15 3.2.6 Assumptions . 16 3.2.7 Relevant Capital and Resources . 16 4 Value System Design 17 4.1 Introduction . 17 4.2 Analytical Hierarchical Process . 17 4.2.1 Longevity . 18 4.2.2 Expandability . 19 4.2.3 Scientific Return . 19 4.2.4 Risk . 20 4.2.5 Cost . 21 5 Initial Concept of Operations 21 5.1 Orbital Analysis . 22 5.2 Launch Vehicles . 22 6 Habitat Location 25 6.1 Introduction . 25 6.2 Region Selection . 25 6.3 Locations of Interest . 26 6.4 Eliminated Locations . 26 6.5 Remaining Locations . 27 6.6 Chosen Location . -
Warren and Taylor-2014-In Tog-The Moon-'Author's Personal Copy'.Pdf
This article was originally published in Treatise on Geochemistry, Second Edition published by Elsevier, and the attached copy is provided by Elsevier for the author's benefit and for the benefit of the author's institution, for non- commercial research and educational use including without limitation use in instruction at your institution, sending it to specific colleagues who you know, and providing a copy to your institution’s administrator. All other uses, reproduction and distribution, including without limitation commercial reprints, selling or licensing copies or access, or posting on open internet sites, your personal or institution’s website or repository, are prohibited. For exceptions, permission may be sought for such use through Elsevier's permissions site at: http://www.elsevier.com/locate/permissionusematerial Warren P.H., and Taylor G.J. (2014) The Moon. In: Holland H.D. and Turekian K.K. (eds.) Treatise on Geochemistry, Second Edition, vol. 2, pp. 213-250. Oxford: Elsevier. © 2014 Elsevier Ltd. All rights reserved. Author's personal copy 2.9 The Moon PH Warren, University of California, Los Angeles, CA, USA GJ Taylor, University of Hawai‘i, Honolulu, HI, USA ã 2014 Elsevier Ltd. All rights reserved. This article is a revision of the previous edition article by P. H. Warren, volume 1, pp. 559–599, © 2003, Elsevier Ltd. 2.9.1 Introduction: The Lunar Context 213 2.9.2 The Lunar Geochemical Database 214 2.9.2.1 Artificially Acquired Samples 214 2.9.2.2 Lunar Meteorites 214 2.9.2.3 Remote-Sensing Data 215 2.9.3 Mare Volcanism -
Fudge Space Opera
Fudge Space Opera Version 0.3.0 2006-August-11 by Omar http://www.pobox.com/~rknop/Omar/fudge/spop Coprights, Trademarks, and Licences Fudge Space Opera is licenced under the Open Gaming Licence, version 1.0a; see Appendex A. Open Game License v 1.0 Copyright 2000, Wizards of the Coast, Inc. Fudge System Reference Document Copyright 2005, Grey Ghost Press, Inc.; Authors Steffan O’Sullivan, Ann Dupuis, with additional material by other authors as indicated within the text. Available for use under the Open Game License (see Appendix I) Fudge Space Opera Copyright 2005, Robert A. Knop Jr. Open Gaming Content Designation of Product Identity: Nothing herein is designated as Product Identity as outlined in section 1(e) of the Open Gaming License. Designation of Open Gaming Content: Everything herein is designated as Open Game Content as outlined in seciton 1(d) of the Open Gaming License. Fudge Space Opera -ii- Fudge Space Opera CONTENTS Contents 1 Introduction 1 1.1 Why “Space Opera”? . ......... 1 1.2 WhatisHere ........................................ .......... 2 1.3 TheMostImportantThing .............................. ............ 2 2 Character Creation 3 2.1 GeneralNotes........................................ .......... 3 2.2 5-PointFudge....................................... ........... 3 3 Combat 7 3.1 Default Combat Options . .......... 7 3.2 Basic Armor and Weapon Mechanics . ........... 7 3.3 Cross-WeaponScaleAttacks. .............. 8 3.4 Suggested Weapon Scales . ........ 9 3.5 DamagetoPassengers ................................. ............ 9 3.6 GiantSpaceBeasts.................................... ........... 9 3.7 When To Use Fudge Scale .......................................... 10 3.8 RangedWeapons....................................... ......... 11 3.9 Explosions........................................ ............ 12 3.10 Missiles and Point Defense . .............. 12 -iii- Fudge Space Opera CONTENTS 3.11 Doing Too Many Things at Once . -
Satellite Network Providing Continuous Communications to Support
SATELLITE NETWORK PROVIDING CONTINUOUS COMMUNICATIONS TO SUPPORT MANNED AND UNMANNED EXPLORATION OF THE INNER- PLANETS A Master Thesis Submitted to the Faculty of American Public University by Ralph Leroy Spangler, Jr. In Partial Fulfillment of the Requirements for the Degree of Master of Science July 26, 2016 American Public University Charles Town, WV The author hereby grants the American Public University System the right to display these contents for educational purposes. The author assumes total responsibility for meeting the requirements set by United States copyright law for the inclusion of any materials that are not the author’s creation or in the public domain. © Copyright 2016 by Ralph Leroy Spangler, Jr. All rights reserved. 2 DEDICATION I dedicate this thesis to my wife and sons. Without their encouragement, patience, understanding, support, and most of all, love, the completion of this work would not have been possible. I cannot leave out my faithful furry companion, Veritas, who patiently laid at my feet while I worked. 3 ACKNOWLEDGMENTS I wish to thank the instructors, administration, and fellow students of American Military University for their support, insight, differing viewpoints, openness, and sometimes humor. Their commitment and involvement in my time of studies has been most appreciated. From the beginning, they reinforced the confidence I have in my abilities not only to complete a Master’s degree, but to complete it with excellence. I have found my course work throughout the Space Studies program to be stimulating and thoughtful, providing me with the tools and knowledge with which to explore past, present and future ideas and issues. -
Finding Life Beyond Earth
FINDING LIFE BEYOND EARTH Education Collection NOVA Education pbs.org/nova/education, [email protected] ! NOVA’s “Finding Life Beyond Earth” script visualized. NOVA Education pbs.org/nova/education, [email protected] ! Table of Contents Credits and Acknowledgements! 2 Overview! 4 1 — Meet the Planets! 13 2 — What Is Life?! 16 3 — Basic Ingredients for Life! 19 4 — Extreme Living! 22 5 — Home Sweet Home! 25 6 — Where to Look for Life! 29 7 — How to Search! 33 Common Misconceptions! 38 Related Resources! 39 Appendices! 40 © 2012 WGBH Educational Foundation!!1 Credits and Acknowledgements Produced by NOVA’s Department of Education, WGBH Rachel Connolly, Director of Education | NOVA Chris Randall, Senior Editorial Project Director | WGBH Education Department Maiken Lilley, Education Coordinator | NOVA Graham Veth, Education Outreach Coordinator | NOVA Rachel Gesserman, Production Assistant | NOVA Advisors Chris Dietlin, WGBH Kristen Erickson, NASA Irena Fayngold, WGBH Kay Ferrari, NASA/JPL Rebecca Jaramillo, National Institute of Aerospace Daniella Scalice, NASA Astrobiology Institute Harla Sherwood, National Institute of Aerospace Stephanie Shipp, Lunar and Planetary Institute Anita Sohus, NASA/JPL “Finding Life Beyond Earth” is produced in cooperation with NASA and the National Institute of Aerospace. Additional funding is provided by Millicent Bell through the Millicent and Eugene Bell Foundation. This material is based on work supported by the National Aeronautics and Space Administration, Langley Research Center, under the Research Cooperative Agreement No. NNL09AA00A awarded to the National Institute of Aerospace. Any opinions, findings, and conclusions or recommendations expressed in this publication are those of WGBH and do not necessarily reflect the views of the National Institute of Aerospace. -
TRANSIENT LUNAR PHENOMENA: REGULARITY and REALITY Arlin P
The Astrophysical Journal, 697:1–15, 2009 May 20 doi:10.1088/0004-637X/697/1/1 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. TRANSIENT LUNAR PHENOMENA: REGULARITY AND REALITY Arlin P. S. Crotts Department of Astronomy, Columbia University, Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027, USA Received 2007 June 27; accepted 2009 February 20; published 2009 April 30 ABSTRACT Transient lunar phenomena (TLPs) have been reported for centuries, but their nature is largely unsettled, and even their existence as a coherent phenomenon is controversial. Nonetheless, TLP data show regularities in the observations; a key question is whether this structure is imposed by processes tied to the lunar surface, or by terrestrial atmospheric or human observer effects. I interrogate an extensive catalog of TLPs to gauge how human factors determine the distribution of TLP reports. The sample is grouped according to variables which should produce differing results if determining factors involve humans, and not reflecting phenomena tied to the lunar surface. Features dependent on human factors can then be excluded. Regardless of how the sample is split, the results are similar: ∼50% of reports originate from near Aristarchus, ∼16% from Plato, ∼6% from recent, major impacts (Copernicus, Kepler, Tycho, and Aristarchus), plus several at Grimaldi. Mare Crisium produces a robust signal in some cases (however, Crisium is too large for a “feature” as defined). TLP count consistency for these features indicates that ∼80% of these may be real. Some commonly reported sites disappear from the robust averages, including Alphonsus, Ross D, and Gassendi. -
Assessment of Spectral Properties of Apollo 12 Landing Site Yann Chemin1, Ian Crawford2, Peter Grindrod2, and Louise Alexander2
Assessment of spectral properties of Apollo 12 landing site Yann Chemin1, Ian Crawford2, Peter Grindrod2, and Louise Alexander2 1Student, Birkbeck Colllege, University of London 2Birkbeck Colllege, University of London Corresponding author: Yann Chemin1 Email address: [email protected] ABSTRACT The geology and mineralogy of the Apollo 12 landing site has been the subject of recent studies that this research attempts to complement from a remote sensing point of view using the Moon Mineralogy Mapper (M3) sensor data, onboard the Chandrayaan-1 lunar orbiter. It is a higher spatial-spectral resolution sensor than the Clementine UVVis sensor and gives the opportunity to study the lunar surface with a comparatively more detailed spectral resolution. We used ISIS and GRASS GIS to study the M3 data. The M3 signatures are showing a monotonic featureless increment, with very low reflectance, suggesting a mature regolith. The regolith maturity is splitting the landing site in a younger Northwest and older Southeast. The mineral identification using the lunar sample spectra from within the Relab database found some similarity to a basaltic rock/glass mix. The spectrum features of clinopyroxene have been found in the Copernican rays and at the landing site. Lateral mixing increases FeO content away from the central part of the ray. The presence of clinopyroxene in the pigeonite basalt in the stratigraphy of the landing site brings forth some complexity in differentiating the Copernican ray’s clinopyroxene from the local source, as the spectra are twins but for their vertical shift in reflectance, reducing away from the central part of the ray. Spatial variations in mineralogy were not found mostly because of the pixel size compared to the landing site area. -
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. -
Concept for a Crewed Lunar Lander Operating from the Lunar Orbiting Platform-Gateway
69th International Astronautical Congress (IAC), Bremen, Germany, 1-5 October 2018. Copyright © 2018 by Lockheed Martin Corporation. Published by the IAF, with permission and released to the IAF to publish in all forms. IAC-18.A5.1.4x46653 Concept for a Crewed Lunar Lander Operating from the Lunar Orbiting Platform-Gateway Timothy Cichana*, Stephen A. Baileyb, Adam Burchc, Nickolas W. Kirbyd aSpace Exploration Architect, P.O. Box 179, MS H3005, Lockheed Martin Space, Denver, Colorado, U.S.A. 80201, [email protected] bPresident, 8100 Shaffer Parkway, Unit 130, Deep Space Systems, Inc., Littleton, Colorado, 80127-4124, [email protected] cDesign Engineer / Graphic Artist, 8341 Sangre de Christo Rd, Deep Space Systems, Inc., Littleton, Colorado, 80127, [email protected] dSystems Engineer, Advanced Programs, P.O. Box 179, MS H3005, Lockheed Martin Space, Denver, Colorado, U.S.A. 80201, [email protected] * Corresponding Author Abstract Lockheed Martin is working with NASA on the development of the Lunar Orbiting Platform – Gateway, or Gateway. Positioned in the vicinity of the Moon, the Gateway allows astronauts to demonstrate operations beyond Low Earth Orbit for months at a time. The Gateway is evolvable, flexible, modular, and is a precursor and mission demonstrator directly on the path to Mars. Mars Base Camp is Lockheed Martin's vision for sending humans to Mars. Operations from an orbital base camp will build on a strong foundation of today's technologies and emphasize scientific exploration as mission cornerstones. Key aspects of Mars Base Camp include utilizing liquid oxygen and hydrogen as the basis for a nascent water-based economy and the development of a reusable lander/ascent vehicle.