75Th Birthday for RMI IAC in Mexico Eye Damage in Space
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How Doc Draper Became the Father of Inertial Guidance
(Preprint) AAS 18-121 HOW DOC DRAPER BECAME THE FATHER OF INERTIAL GUIDANCE Philip D. Hattis* With Missouri roots, a Stanford Psychology degree, and a variety of MIT de- grees, Charles Stark “Doc” Draper formulated the basis for reliable and accurate gyro-based sensing technology that enabled the first and many subsequent iner- tial navigation systems. Working with colleagues and students, he created an Instrumentation Laboratory that developed bombsights that changed the balance of World War II in the Pacific. His engineering teams then went on to develop ever smaller and more accurate inertial navigation for aircraft, submarines, stra- tegic missiles, and spaceflight. The resulting inertial navigation systems enable national security, took humans to the Moon, and continue to find new applica- tions. This paper discusses the history of Draper’s path to becoming known as the “Father of Inertial Guidance.” FROM DRAPER’S MISSOURI ROOTS TO MIT ENGINEERING Charles Stark Draper was born in 1901 in Windsor Missouri. His father was a dentist and his mother (nee Stark) was a school teacher. The Stark family developed the Stark apple that was popular in the Midwest and raised the family to prominence1 including a cousin, Lloyd Stark, who became governor of Missouri in 1937. Draper was known to his family and friends as Stark (Figure 1), and later in life was known by colleagues as Doc. During his teenage years, Draper enjoyed tinkering with automobiles. He also worked as an electric linesman (Figure 2), and at age 15 began a liberal arts education at the University of Mis- souri in Rolla. -
ISS Potable Water Sampling and Chemical Analysis Results for 2016
47th International Conference on Environmental Systems ICES-2017-337 16-20 July 2017, Charleston, South Carolina ISS Potable Water Sampling and Chemical Analysis Results for 2016 John E. Straub II1, Debrah K. Plumlee2, William T. Wallace2, James T. Alverson2, Mickie J. Benoit2, Robert L. Gillispie2, David Hunter2, Mike Kuo2, and Jeffrey A. Rutz2 KBRwyle, Houston, Texas, 77058 Edgar K. Hudson3 and Leslie J. Loh4 JES Tech, Houston, Texas, 77058 and Daniel B. Gazda5 NASA Johnson Space Center, Houston, Texas, 77058 This paper continues the annual tradition, at this conference, of summarizing the results of chemical analyses performed on archival potable water samples returned from the International Space Station (ISS). 2016 represented a banner year for life aboard the ISS, including the successful conclusion for 2 crewmembers of a record 1-year mission. Water reclaimed from urine and/or humidity condensate remained the primary source of potable water for the crewmembers of ISS Expeditions 46-50. The year was also marked by the end of a long-standing tradition of U.S. sampling and monitoring of Russian Segment potable water sources. Two water samples, taken during Expedition 46 and returned on Soyuz 44 in March 2016, represented the final Russian Segment samples to be collected and analyzed by the U.S. side. Although anticipated for 2016, a rise in the total organic carbon (TOC) concentration of the product water from the U.S. water processor assembly due to breakthrough of organic contaminants from the system did not materialize, as evidenced -
Stanley G. Weinbaum's Planetary Stories
FFOORRGGOOTTTTEENN FFUUTTUURREESS BBYY SSTTAANNLLEEYY GG.. WWEEIINNBBAAUUMM FORGOTTEN FUTURES XI: THE PLANETARY SERIES BY STANLEY G. WEINBAUM COVER ILLUSTRATIONS COPYRIGHT © MARCUS L. ROWLAND 2010 This collection of stories is edited to this form to accompany Forgotten Futures XI: Planets of Peril, a role playing game based on the stories. Several other stories by Weinbaum can be downloaded in HTML form from the Forgotten Futures sites. The last story of this sequence, Tidal Moon, could not be included since it was completed posthumously by Helen Weinbaum and remains in European copyright. It can be downloaded from Project Gutenberg Australia. To the best of my knowledge and belief all European copyright in these works of Stanley Weinbaum has now expired. No copyright in these works is claimed by the current editor. While every effort has been made to remove OCR and other errors it is likely that some remain. Some obvious proofreading and editorial errors found in the original books have been corrected. I have not tried to convert American English to British English! Special thanks to Malcolm Farmer for his help with scanning, OCR, proofreading etc. Print formatting: If you print double-sided, for best results print the cover and this page single sided, and all remaining pages double sided. This is a FREE download; please inform me if you are charged any fee to obtain it in any form. Marcus L. Rowland – July 2010 A Martian Odyssey 1 July 1934 Valley of Dreams 16 November 1934 Flight on Titan 30 January 1935 Parasite Planet 43 February 1935 The Lotus Eaters 60 April 1935 The Planet of Doubt 77 October 1935 The Red Peri 94 November 1935 The Mad Moon 123 December 1935 Redemption Cairn 136 March 1936 Tidal Moon December 1938 (not included for copyright reasons) Stanley G. -
World Space Observatory %Uf02d Ultraviolet Remains Very Relevant
WORLD SPACE OBSERVATORY-ULTRAVIOLET Boris Shustov, Ana Inés Gómez de Castro, Mikhail Sachkov UV observatories aperture pointing mode , Å OAO-2 1968.12 - 1973.01 20 sp is 1000-4250 TD-1A 1972.03 - 1974.05 28 s is 1350-2800+ OAO-3 1972.08 - 1981.02 80 p s 900-3150 ANS 1974.08 - 1977.06 22 p s 1500-3300+ IUE 1978.01 - 1996.09 45 p s 1150-3200 ASTRON 1983.03 - 1989.06 80 p s 1100-3500+ EXOSAT 1983.05 - 1986. 2x30 p is 250+ ROSAT 1990.06 - 1999.02 84 sp i 60- 200+ HST 1990.04 - 240 p isp 1150-10000 EUVE 1992.06 - 2001.01 12 sp is 70- 760 ALEXIS 1993.04 - 2005.04 35 s i 130- 186 MSX 1996.04 - 2003 50 s i 1100-9000+ FUSE 1999.06 - 2007.07 39х35 (4) p s 905-1195 XMM 1999.12 - 30 p is 1700-5500 GALEX 2003.04 - 2013.06 50 sp is 1350-2800 SWIFT 2004.11 - 30 p i 1700-6500 2 ASTROSAT/UVIT UVIT - UltraViolet Imaging Telescopes (on the ISRO Astrosat observatory, launch 2015); Two 40cm telescopes: FUV and NUV, FOV 0.5 degrees, resolution ~1” Next talk by John Hutchings! 3 4 ASTRON (1983 – 1989) ASTRON is an UV space observatory with 80 cm aperture telescope equipped with a scanning spectrometer:(λλ 110-350 nm, λ ~ 2 nm) onboard. Some significant results: detection of OH (H2O) in Halley comet, UV spectroscopy of SN1987a, Pb lines in stellar spectra etc. (Photo of flight model at Lavochkin Museum).5 “Spektr” (Спектр) missions Federal Space Program (2016-2025) includes as major astrophysical projects: Spektr-R (Radioastron) – launched in 2011. -
By September 1976 the Charles Stark Draper Laboratory, Inc. Cambridge
P-357 THE HISTORY OF APOLLO ON-BOARD GUIDANCE, NAVIGATION, AND CONTROL by David G. Hoag September 1976 The Charles Stark Draper Laboratory, Inc. Cambridge, Massachusetts 02139 @ The Charles Stark Draper Laboratory, Inc. , 1976. the solar pressure force on adjustable sun vanes to drive the average speed of these wheels toward zero. Overall autonomous operation was managed on-board by a small general purpose digital computer configured by its designer, Dr. Raymond Alonso, for very low power drain except at the occasional times needing fast computation speed. A special feature of this computer was the pre-wired, read-only memory called a core rope, a configuration of particularly high storage density requiring only one magnetic core per word of memory. A four volume report of this work was published in July, 1959, and presented to the Air Force Sponsors. However, since the Air Force was disengaging from civilian space development, endeavors to interest NASA were undertaken. Dr. H. Guyford Stever, then an MIT professor, arranged a presentation with Dr. Hugh Dryden, NASA Deputy Administrator, which took place on September 15.* On November 10, NASA sent a letter of in- tent to contract the Instrumentation Laboratory for a $50,000 study to start immediately. The stated purpose was that this study would con- c tribute to the efforts of NASA's Jet Propulsion Laboratory in conducting unmanned space missions to Mars, Venus, and the Earth's moon scheduled in Vega and Centaur missions in the next few years. A relationship be- tween MIT and JPL did not evolve. JPL's approach to these deep space missions involved close ground base control with their large antenna tracking and telemetry systems, considerably different from the on- board self sufficiency method which the MIT group advocated and could best support. -
NASA's Wallops Flight Facility in Virginia
National Aeronautics and Space Administration NASA’s “Big Bang” Service Delivery Transformation: Shared Services in the Cloud Paul Rydeen NASA Shared Services Center (NSSC) Enterprise Service Center (ESC) Program Manager Agenda • National Aeronautics and Space Administration (NASA) Overview • NASA Shared Services Center (NSSC) Overview • Where We Are Today • The Migration To The Cloud • Top Takeaways NASA Vision • We reach for new heights and reveal the unknown for the benefit of humankind NASA Mission Statement • Drive advances in science, technology, aeronautics and space exploration to enhance knowledge, education, innovation, economic vitality and stewardship of Earth NASA Centers The National Aeronautics and Space Administration (NASA) • 17,605 Civil Service employees and 28,693 contractors at or near 10 Field Centers and NASA Headquarters • Four Mission Directorates: – Aeronautics Research Mission Directorate – Human Exploration & Operations Mission Directorate – Science Mission Directorate – Space Technology Mission Directorate • NASA’s FY17 budget is $19.0 billion What is the NASA Shared Services Center (NSSC)? • A business model for delivering support services • Provides high-quality service and achieves cost savings for NASA • Opened for service in March 2006 Why Shared Services for NASA? • Reduces resources expended for support • Provides better quality, more timely services at lower cost • Improves data integrity, consistency, and accountability • Standardizes core business processes • Facilitates process re-engineering and -
Britain Back in Space
Spaceflight A British Interplanetary Society Publication Britain back in Space Vol 58 No 1 January 2016 £4.50 www.bis-space.com 1.indd 1 11/26/2015 8:30:59 AM 2.indd 2 11/26/2015 8:31:14 AM CONTENTS Editor: Published by the British Interplanetary Society David Baker, PhD, BSc, FBIS, FRHS Sub-editor: Volume 58 No. 1 January 2016 Ann Page 4-5 Peake on countdown – to the ISS and beyond Production Assistant: As British astronaut Tim Peake gets ready for his ride into space, Ben Jones Spaceflight reviews the build-up to this mission and examines the Spaceflight Promotion: possibilities that may unfold as a result of European contributions to Suszann Parry NASA’s Orion programme. Spaceflight Arthur C. Clarke House, 6-9 Ready to go! 27/29 South Lambeth Road, London, SW8 1SZ, England. What happens when Tim Peake arrives at the International Space Tel: +44 (0)20 7735 3160 Station, where can I watch it, listen to it, follow it, and what are the Fax: +44 (0)20 7582 7167 broadcasters doing about special programming? We provide the Email: [email protected] directory to a media frenzy! www.bis-space.com 16-17 BIS Technical Projects ADVERTISING Tel: +44 (0)1424 883401 Robin Brand has been busy gathering the latest information about Email: [email protected] studies, research projects and practical experiments now underway at DISTRIBUTION the BIS, the first in a periodic series of roundups. Spaceflight may be received worldwide by mail through membership of the British 18 Icarus Progress Report Interplanetary Society. -
Supplementary Figure 1: Interconnected Multiplex with Six Nodes in Two Layers (A and D) and Corresponding Aggregated Networks (B and E)
Supplementary Figure 1: Interconnected multiplex with six nodes in two layers (A and D) and corresponding aggregated networks (B and E). The nodes are ranked by their eigenvector centrality in each layer separately, in the aggregated and in the whole interconnected structure (C and F). Case A, B and C. Nodes 1 and 3 have a key role in the multilayer, being bridges between the two layers. In a collaboration network they would represent scientists working on two different research areas who allow information to flow from one subject to the other. While nodes 1 and 3 gain centrality from their connections to \hubs" on different layers, they also gain centrality from their own counterparts in other layers, making them important in the multilayer network. In the aggregated network their versatility disappears, because the information is washed out by projecting on a single layer, where nodes 2 and 6 are still \hubs" but it is not possible to capture the importance of nodes 1 and 3 in bridging different areas. Case D, E and F. This example shows how aggregating the full information on a single network introduces a spurious symmetry between nodes 2, 3, 4 and 6 that is not present in the multilayer, except for 2 and 4. The resulting score in the aggregate is not able to capture the difference between these nodes (corresponding to a degeneration in the eigenspace) while it is evident that, for instance, node 6 is more central than node 3 because of its direct connection to node 1 { the \hub" { in layer 1. -
Oxford University Press Free Sample Chapter Multiplex-Multi-Level
FREE SAMPLE CHAPTER Networks and Complex Systems publications from Oxford University Press 30% online discount Networks Multilayer Networks Introduction to the Second Edition Structure and Function Theory of £49.99 £34.99 £55.00 £38.50 Complex Systems Mark Newman Ginestra Bianconi £49.99 £34.99 Stefan Thurner, Peter Klimek, Rudolf Hanel Generating Random Scale-Free Networks Agent-Based Modeling Networks and Graphs Complex Webs in and Network Dynamics £55.00 £38.50 Nature and Technology £57.50 £40.25 Ton Coolen, Alessia Annibale, £34.49 £24.14 Akira Namatame, Ekaterina Roberts Guido Caldarelli Shu-Heng Chen Order online at www.oup.com and enter the code EXCCS-18 to get a 30% discount Visit us at stand #1 to receive your free hard copy of this chapter and join our mailing list. OUP UNCORRECTED PROOF – FIRST PROOF, 3/8/2018, SPi Preface As the field of complex networks entered its maturity phase, most scientists working in this field thought that the established methodology could deal with all casesof networked systems. However, as is usually the case in the scientific enterprise, some novel observations showed that what we already know is only a limited case, and network theory has still long way to go until we can make any definitive claim. The ever-increasing availability of data in fields ranging from computer science to urban systems, medicine, economics, and finance showed that networks that were usually perceived as distinct and isolated are, in reality, interacting with other networks. While this sounds like a trivial observation, it was shown that interactions of different networks can lead to unexpected behaviors and allow systemic vulnerabilities to emerge. -
Urantia, 606 of Satania by Israel Dix © 2010
1 Urantia, 606 of Satania By Israel Dix © 2010 Numbering the Stars Said Machiventa to Abraham: "Look now up to the heavens and number the stars if you are able; so numerous shall your seed be.”(1020.6) In attempting to do just that, to number the stars, you and I will most certainly be taking a journey over some steep, rocky terrain, number-crunching math, and, out of necessity I’m afraid, plenty of interesting quotes. Lots of them. Because of this I have attempted to keep reference numbers small and out of the way on the trail, so to avoid distraction from the easy flow of this adventure in star searching. Additionally is the added energy boost in knowing that, staying the course, there is at the end of our trek a beautiful picture, a surprisingly organized structure – the Satania System of worlds. So bear with me up this hill we are about to climb. We begin with the problem that set me out on this exploration in the first place: Why does Urantia, a decimal world, end on the peculiar number of six, rather than zero which is a multiple of ten? There must be some explanation for this, and it was a minute hunch that there was an answer that led me first to explore this seemingly unimportant information. The small but nagging question kept returning to mind on occasion, “Ought Urantia to end instead on a zero?” One might get the faint sense that there is an answer to this riddle. But do we have an indication of this, or is it simply a wild chase that dead ends in an attempt to number the stars. -
Science Worksheet
Today’s activity includes a fantastic look inside our book: Get to Work with Science and Technology ASTRONAUT Life as a Scientist and Engineer in Space You will also get the chance to try packing your own luggage for a mission to space! (You will need a set of kitchen scales for this activity.) To find out more about life as an astronaut go to: https://www.rubytuesdaybooks.com/product/astronaut-life-as-a-scientist-and- engineer-in-space/ © Ruby Tuesday Books 2021 Just Another Day at Work The countdown is over. A deafening roar bursts from the base of the Soyuz-FG rocket. As people around the world hold their breath, the rocket soars into the sky on a column of flame. Blasting away from Earth are Timothy Kopra, Yuri Malenchenko and Tim Peake. Just three scientists and engineers on their way to work! In a few hours, the men will reach their destination – the International Space Station (ISS). Their training has been long and hard. But it will all be worth it to have the chance to live and work high above Earth in the most extreme laboratory ever built! ISS Expedition 46 crew members Tim Peake (left), Yuri Malenchenko (centre) and Timothy Kopra (right) preflight, 15 December, 2015. 6 Astronauts are highly skilled men and women. They may be scientists, engineers, pilots – or all three. Astronauts work for space agencies such as NASA (National Aeronautics and Space Administration) and ESA (European Space Agency). The Soyuz-FG blasts off from the Baikonur Cosmodrome in Kazakhstan. 7 The International Space Station The ISS travels through space at almost 8 kilometres per second. -
Connecting @Ll Space People Welcome Message 2
Connecting @ll Space People Welcome Message 2 IAF 2018 Events Overview 3 IAF General Assembly 4 ISF 2017 6 IAF Spring Meetings 2018 8 GLAC 2018 9 IAC 2018 10 Overview 11 Plenaries 13 Highlight Lectures 20 Late Breaking News 23 IAF Global Networking Forum (GNF) 24 IAC Special Sessions 37 IAF IDEA “3G” Diversity Events 44 IAC Hosts Summit 46 9th IAF International Meeting for Members 48 of Parliaments YPP Networking Reception 50 Emerging Space Leaders 51 Grant Programme (ESL Grants) Press Conference: Upcoming Global Conference 52 on Space for Emerging Countries, GLEC 2019 ISF 2018 54 IAF Committees’ Reports 56 Technical Committees 57 Administrative Committees 78 Published by the International Astronautical Federation (IAF) 3rd Issue - February 2019 IAF 2018 Activities 80 Copyright © International Astronautical Federation. Other 2018 Events 80 All rights reserved. No part of this magazine may be reproduced or transmitted by any form or by any The International Astronautical Federation 83 means, electronical or mechanical, including photocopying or recording by any information storage or retrieval system without prior written permission from the publishers. CONTENTS IAF 2018 Events Overview Welcome Message Spring has already event in Uruguay. For three days, than 10,000 attendees came to Meetings begun, but experts gathered in Montevideo witness this exceptional event. 2018 2019 we can look to discuss space applications back at 2018 as a very impressive with a specific focus on emerging The majority of IAF publications and successful year. This publica- space nations and Latin America. and for the first time, the IAC tion, the IAF Highlights, is sum- Final Programmes, have been marizing the main IAF events The 69th International Astro- printed in recycled paper this and activities that took place.