ODQN 18-3, July 2014
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Exploration of the Moon
Exploration of the Moon The physical exploration of the Moon began when Luna 2, a space probe launched by the Soviet Union, made an impact on the surface of the Moon on September 14, 1959. Prior to that the only available means of exploration had been observation from Earth. The invention of the optical telescope brought about the first leap in the quality of lunar observations. Galileo Galilei is generally credited as the first person to use a telescope for astronomical purposes; having made his own telescope in 1609, the mountains and craters on the lunar surface were among his first observations using it. NASA's Apollo program was the first, and to date only, mission to successfully land humans on the Moon, which it did six times. The first landing took place in 1969, when astronauts placed scientific instruments and returnedlunar samples to Earth. Apollo 12 Lunar Module Intrepid prepares to descend towards the surface of the Moon. NASA photo. Contents Early history Space race Recent exploration Plans Past and future lunar missions See also References External links Early history The ancient Greek philosopher Anaxagoras (d. 428 BC) reasoned that the Sun and Moon were both giant spherical rocks, and that the latter reflected the light of the former. His non-religious view of the heavens was one cause for his imprisonment and eventual exile.[1] In his little book On the Face in the Moon's Orb, Plutarch suggested that the Moon had deep recesses in which the light of the Sun did not reach and that the spots are nothing but the shadows of rivers or deep chasms. -
Spacex CRS-4 National Aeronautics and Fourth Commercial Resupply Services Flight Space Administration
SpaceX CRS-4 National Aeronautics and Fourth Commercial Resupply Services Flight Space Administration to the International Space Station September 2014 OVERVIEW The Dragon spacecraft will be filled with more than 5,000 pounds of supplies and payloads, including critical materials to support 255 science and research investigations that will occur during Expeditions 41 and 42. Dragon will carry three powered cargo payloads in its pressurized section and two in its unpressurized trunk. Science payloads will enable model organism research using rodents, fruit flies and plants. A special science payload is the ISS-Rapid Scatterometer to monitor ocean surface wind speed and direction. Several new technology demonstrations aboard will enable bone density studies, test how a small satellite moves and positions itself in space using new thruster technology, and use the first 3-D printer in space for additive manufacturing. The mission also delivers IMAX cameras for filming during four increments and replacement batteries for the spacesuits. After four weeks at the space station, the spacecraft will return with about 3,800 pounds of cargo, including crew supplies, hardware and computer resources, science experiments, space station hardware, and four powered payloads. DRAGON CARGO LAUNCH ITEMS RETURN ITEMS TOTAL CARGO: 4885 lbs / 2216 kg 3276 lbs / 1486 kg · Crew Supplies 1380 lbs / 626 kg 132 lbs / 60 kg Crew care packages Crew provisions Food · Vehicle Hardware 403 lbs / 183 kg 937 lbs / 425 kg Crew Health Care System hardware Environment Control & Life Support equipment Electrical Power System hardware Extravehicular Robotics equipment Flight Crew Equipment Japan Aerospace Exploration Agency equipment · Science Investigations 1644 lbs / 746 kg 2075 lbs / 941 kg U.S. -
25 Years of Indian Remote Sensing Satellite (IRS)
2525 YearsYears ofof IndianIndian RemoteRemote SensingSensing SatelliteSatellite (IRS)(IRS) SeriesSeries Vinay K Dadhwal Director National Remote Sensing Centre (NRSC), ISRO Hyderabad, INDIA 50 th Session of Scientific & Technical Subcommittee of COPUOS, 11-22 Feb., 2013, Vienna The Beginning • 1962 : Indian National Committee on Space Research (INCOSPAR), at PRL, Ahmedabad • 1963 : First Sounding Rocket launch from Thumba (Nov 21, 1963) • 1967 : Experimental Satellite Communication Earth Station (ESCES) established at Ahmedabad • 1969 : Indian Space Research Organisation (ISRO) established (15 August) PrePre IRSIRS --1A1A SatellitesSatellites • ARYABHATTA, first Indian satellite launched in April 1975 • Ten satellites before IRS-1A (7 for EO; 2 Met) • 5 Procured & 5 SLV / ASLV launch SAMIR : 3 band MW Radiometer SROSS : Stretched Rohini Series Satellite IndianIndian RemoteRemote SensingSensing SatelliteSatellite (IRS)(IRS) –– 1A1A • First Operational EO Application satellite, built in India, launch USSR • Carried 4-band multispectral camera (3 nos), 72m & 36m resolution Satellite Launch: March 17, 1988 Baikanur Cosmodrome Kazakhstan SinceSince IRSIRS --1A1A • Established of operational EO activities for – EO data acquisition, processing & archival – Applications & institutionalization – Public services in resource & disaster management – PSLV Launch Program to support EO missions – International partnership, cooperation & global data sets EarlyEarly IRSIRS MultispectralMultispectral SensorsSensors • 1st Generation : IRS-1A, IRS-1B • -
NUCLEAR SAFETY LAUNCH APPROVAL: MULTI-MISSION LESSONS LEARNED Yale Chang the Johns Hopkins University Applied Physics Laboratory
ANS NETS 2018 – Nuclear and Emerging Technologies for Space Las Vegas, NV, February 26 – March 1, 2018, on CD-ROM, American Nuclear Society, LaGrange Park, IL (2018) NUCLEAR SAFETY LAUNCH APPROVAL: MULTI-MISSION LESSONS LEARNED Yale Chang The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Rd, Laurel, MD 20723 240-228-5724; [email protected] Launching a NASA radioisotope power system (RPS) trajectory to Saturn used a Venus-Venus-Earth-Jupiter mission requires compliance with two Federal mandates: Gravity Assist (VVEJGA) maneuver, where the Earth the National Environmental Policy Act of 1969 (NEPA) Gravity Assist (EGA) flyby was the primary nuclear safety and launch approval (LA), as directed by Presidential focus of NASA, the U.S. Department of Energy (DOE), the Directive/National Security Council Memorandum 25. Cassini Interagency Nuclear Safety Review Panel Nuclear safety launch approval lessons learned from (INSRP), and the public alike. A solid propellant fire test multiple NASA RPS missions, one Russian RPS mission, campaign addressed the MPF finding and led in part to two non-RPS launch accidents, and several solid the retrofit solid propellant breakup systems (BUSs) propellant fire test campaigns since 1996 are shown to designed and carried by MER-A and MER-B spacecraft have contributed to an ever-growing body of knowledge. and the deployment of plutonium detectors in the launch The launch accidents can be viewed as “unplanned area for PNH. The PNH mission decreased the calendar experiments” that provided real-world data. Lessons length of the NEPA/LA processes to less than 4 years by learned from the nuclear safety launch approval effort of incorporating lessons learned from previous missions and each mission or launch accident, and how they were tests in its spacecraft and mission designs and their applied to improve the NEPA/LA processes and nuclear NEPA/LA processes. -
The Space-Based Global Observing System in 2010 (GOS-2010)
WMO Space Programme SP-7 The Space-based Global Observing For more information, please contact: System in 2010 (GOS-2010) World Meteorological Organization 7 bis, avenue de la Paix – P.O. Box 2300 – CH 1211 Geneva 2 – Switzerland www.wmo.int WMO Space Programme Office Tel.: +41 (0) 22 730 85 19 – Fax: +41 (0) 22 730 84 74 E-mail: [email protected] Website: www.wmo.int/pages/prog/sat/ WMO-TD No. 1513 WMO Space Programme SP-7 The Space-based Global Observing System in 2010 (GOS-2010) WMO/TD-No. 1513 2010 © World Meteorological Organization, 2010 The right of publication in print, electronic and any other form and in any language is reserved by WMO. Short extracts from WMO publications may be reproduced without authorization, provided that the complete source is clearly indicated. Editorial correspondence and requests to publish, reproduce or translate these publication in part or in whole should be addressed to: Chairperson, Publications Board World Meteorological Organization (WMO) 7 bis, avenue de la Paix Tel.: +41 (0)22 730 84 03 P.O. Box No. 2300 Fax: +41 (0)22 730 80 40 CH-1211 Geneva 2, Switzerland E-mail: [email protected] FOREWORD The launching of the world's first artificial satellite on 4 October 1957 ushered a new era of unprecedented scientific and technological achievements. And it was indeed a fortunate coincidence that the ninth session of the WMO Executive Committee – known today as the WMO Executive Council (EC) – was in progress precisely at this moment, for the EC members were very quick to realize that satellite technology held the promise to expand the volume of meteorological data and to fill the notable gaps where land-based observations were not readily available. -
Design of the Wavefront Sensor Unit of ARGOS, the LBT Laser Guide Star System
UNIVERSITA` DEGLI STUDI DI FIRENZE Dipartimento di Fisica e Astronomia Scuola di Dottorato in Astronomia Ciclo XXIV - FIS05 Design of the wavefront sensor unit of ARGOS, the LBT laser guide star system Candidato: Marco Bonaglia arXiv:1203.5081v1 [astro-ph.IM] 22 Mar 2012 Tutore: Prof. Alberto Righini Cotutore: Dott. Simone Esposito A common use for a glass plate is as a beam splitter, tilted at an angle of 45◦ [:::] Since this can severely degrade the image, such plate beam splitters are not recommended in convergent or divergent beams. W. J. Smith, Modern Optical Engineering. Contents 1 Introduction 1 1.1 The Large Binocular Telescope . 2 1.2 LUCI . 4 1.3 First Light AO system . 5 1.3.1 Angular anisoplanatism . 8 1.4 Wide field AO correction . 9 1.5 Laser guide star AO . 10 1.5.1 Limits of LGS AO . 11 1.5.2 Rayleigh LGS . 13 1.6 LGS-GLAO facilities . 14 1.6.1 GLAS . 15 1.6.2 The MMT GLAO system . 15 1.6.3 SAM . 18 2 ARGOS: a laser guide star AO system for the LBT 21 2.1 System design . 22 2.2 Study of ARGOS performance . 29 2.2.1 The simulation code . 30 2.2.2 Results of ARGOS end-to-end simulations . 36 3 The wavefront sensor dichroic 43 3.1 Effects of a window in a convergent beam . 43 3.2 Aberration compensation with window shape . 47 3.2.1 Effects of a wedge between surfaces . 48 3.2.2 Effects of a cylindrical surface . -
Educator's Guide: Orion
Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations. -
Sentinel-1A Launch
SENTINEL-1A LAUNCH Arianespace’s seventh Soyuz launch from the Guiana Space Center will orbit Sentinel-1A, the first satellite in Europe’s Earth observation program, Copernicus. The European Space Agency (ESA) chose Thales Alenia Space to design, develop and build the satellite, as well as perform related tests. Copernicus is the new name for the European program previously known as GMES (Global Monitoring for Environment and Security), and is the European Commission’s second major space program, following Galileo. Copernicus is designed to give Europe continuous, independent and reliable access to Earth observation data. With the Soyuz, Ariane 5 and Vega launchers at the Guiana Space Center (CSG), Arianespace is the only launch services provider in the world capable of launching all types of payloads into all orbits, from the smallest to the largest geostationary satellites, from satellite clusters for constellations to cargo missions for the International Space Station (ISS). Arianespace sets the launch services standard for all operators, whether commercial or governmental, and guarantees access to space for scientific missions. Sentinel-1A is the 50th satellite with an Earth observation payload to be launched by Arianespace. Arianespace has seven more Earth observation missions in its order book, including four commercial missions (signed in 2013 and 2014). The Copernicus program is designed to give Europe complete independence in the acquisition and management of environmental data concerning our planet. ESA’s Sentinel programs comprise five satellite families: Sentinel-1, to provide continuity for radar data from ERS and Envisat. Sentinel-2 and Sentinel-3, dedicated to the observation of the Earth and its oceans. -
+ Return to Flight Implementation Plan -- 12Th Edition (8.4 Mb PDF)
NASA’s Implementation Plan for Space Shuttle Return to Flight and Beyond A periodically updated document demonstrating our progress toward safe return to flight and implementation of the Columbia Accident Investigation Board recommendations June 20, 2006 Volume 1, Twelfth Edition An electronic version of this implementation plan is available at www.nasa.gov NASA’s Implementation Plan for Space Shuttle Return to Flight and Beyond June 20, 2006 Twelfth Edition Change June 20, 2006 This 12th revision to NASA’s Implementation Plan for Space Shuttle Return to Flight and Beyond provides updates to three Columbia Accident Investigation Board Recommendations that were not fully closed by the Return to Flight Task Group, R3.2-1 External Tank (ET), R6.4-1 Thermal Protection System (TPS) On-Orbit Inspection and Repair, and R3.3-2 Orbiter Hardening and TPS Impact Tolerance. These updates reflect the latest status of work being done in preparation for the STS-121 mission. Following is a list of sections updated by this revision: Message from Dr. Michael Griffin Message from Mr. William Gerstenmaier Part 1 – NASA’s Response to the Columbia Accident Investigation Board’s Recommendations 3.2-1 External Tank Thermal Protection System Modifications (RTF) 3.3-2 Orbiter Hardening (RTF) 6.4-1 Thermal Protection System On-Orbit Inspect and Repair (RTF) Remove Pages Replace with Pages Cover (Feb 17, 2006) Cover (Jun. 20, 2006 ) Title page (Feb 17, 2006) Title page (Jun. 20, 2006) Message From Michael D. Griffin Message From Michael D. Griffin (Feb 17, 2006) -
Optical Satellite Communication Toward the Future of Ultra High
No.466 OCT 2017 Optical Satellite Communication toward the Future of Ultra High-speed Wireless Communications No.466 OCT 2017 National Institute of Information and Communications Technology CONTENTS FEATURE Optical Satellite Communication toward the Future of Ultra High-speed Wireless Communications 1 INTERVIEW New Possibilities Demonstrated by Micro-satellites Morio TOYOSHIMA 4 A Deep-space Optical Communication and Ranging Application Single photon detector and receiver for observation of space debris Hiroo KUNIMORI 6 Environmental-data Collection System for Satellite-to-Ground Optical Communications Verification of the site diversity effect Kenji SUZUKI 8 Optical Observation System for Satellites Using Optical Telescopes Supporting safe satellite operation and satellite communication experiment Tetsuharu FUSE 10 Development of "HICALI" Ultra-high-speed optical satellite communication between a geosynchronous satellite and the ground Toshihiro KUBO-OKA TOPICS 12 NICT Intellectual Property -Series 6- Live Electrooptic Imaging (LEI) Camera —Real-time visual comprehension of invisible electromagnetic waves— 13 Awards 13 Development of the “STARDUST” Cyber-attack Enticement Platform Cover photo Optical telescope with 1 m primary mirror. It receives data by collecting light from sat- ellites. This was the main telescope used in experiments with the Small Optical TrAn- sponder (SOTA). This optical telescope has three focal planes, a Cassegrain, a Nasmyth, and a coudé. The photo in the upper left of this page shows SOTA mounted in a 50 kg-class micro- satellite. In a world-leading effort, this was developed to conduct basic research on technology for 1.5-micron band optical communication between low-earth-orbit sat- ellite and the ground and to test satellite-mounted equipment in a space environment. -
COMPACT) Joe Mrozinski JPL, Michael Saing JPL, Mary Covert Aerospace Corp., Tim Anderson Aerospace Corp
CubeSat Or Microsat Probabilistic + Analogies Cost Tool (COMPACT) Joe Mrozinski JPL, Michael Saing JPL, Mary Covert Aerospace Corp., Tim Anderson Aerospace Corp. Copyright 2016 California Institute of Technology. Government sponsorship acknowledged. What is a CubeSat? CubeSat = Extremely small (i.e. Nanosat scale 1- 10kg) spacecraft of standard dimensions that hitchhikes to space with a traditional spacecraft. • Standard Form Factors: how many “U’s” is your Cubesat? 1 to 6 U’s: A “1U” A “2U” Cubesat is Cubesat is 3U: roughly twice as big 10x10x10 cm 6U! 11/16/16 COMPACT 2 jpl.nasa.gov What is a Microsat? A Microsat is simply a satellite with mass between 10 kg and 100 kg. Most 1-3U CubeSats are 1 - 10 kg, and fall into the “Nanosat” range. But a 6U Cubesat likely has a mass >10 kg and thus would be a microsat. CubeSat Or Microsat Probabilistic + Analogies Cost Tool (COMPACT) COMPACT is exploring CubeSats first. 11/16/16 COMPACT 3 jpl.nasa.gov NASA does not have a CubeSat Cost Estimating …But NASA Capability… clearly needs one -- ASAP! Graphic from: “CubeSat Most of Technology and Systems,” these Janson, S., Presentation to “Nanosats” USGIF Small Satellite are Working Group, 27 Cubesats May 2015 11/16/16 COMPACT 4 jpl.nasa.gov COMPACT just completed Phase 1 to begin addressing this cost estimating capability gap Phase 1 Requirement: Collect & Normalize Key Cost Driver Data for 10 CubeSats 11/16/16 COMPACT 5 jpl.nasa.gov Phase 1 Delivery: Normalized Data for 18 CubeSats 11/16/16 COMPACT 6 jpl.nasa.gov O_OREOS CINEMA EDSN GRIFEX LMRST KickSat Phase 1 Delivery: Normalized Data for: IPEX Firefly 18 CubeSats M-Cubed 2 PSSC-2 SkyCube SporeSat-1 MarCO NanoSail-D RACE RAX 1 11/16/16 M-Cubed COMPACT PharmaSat 7 jpl.nasa.gov Key Data i.e. -
Classification of Geosynchronous Objects
esoc European Space Operations Centre Robert-Bosch-Strasse 5 D-64293 Darmstadt Germany T +49 (0)6151 900 www.esa.int CLASSIFICATION OF GEOSYNCHRONOUS OBJECTS Produced with the DISCOS Database Prepared by ESA’s Space Debris Office Reference GEN-DB-LOG-00211-OPS-GR Issue 20 Revision 0 Date of Issue 28 May 2018 Status Issued Document Type Technical Note Distribution ESA UNCLASSIFIED - Limited Distribution European Space Agency Agence spatiale europeenne´ Abstract This is a status report on geosynchronous objects as of 1 January 2018. Based on orbital data in ESA’s DISCOS database and on orbital data provided by KIAM the situation near the geostationary ring is analysed. From 1523 objects for which orbital data are available (of which 0 are outdated, i.e. the last available state dates back to 180 or more days before the reference date), 519 are actively controlled, 795 are drifting above, below or through GEO, 189 are in a libration orbit and 19 are in a highly inclined orbit. For 1 object the status could not be determined. Furthermore, there are 59 uncontrolled objects without orbital data (of which 54 have not been cata- logued). Thus the total number of known objects in the geostationary region is 1582. If you detect any error or if you have any comment or question please contact: Stijn Lemmens European Space Agency European Space Operations Center Space Debris Office (OPS-GR) Robert-Bosch-Str. 5 64293 Darmstadt, Germany Tel.: +49-6151-902634 E-mail: [email protected] Page 1 / 187 European Space Agency CLASSIFICATION OF GEOSYNCHRONOUS OBJECTS Agence spatiale europeenne´ Date 28 May 2018 Issue 20 Rev 0 Table of contents 1 Introduction 3 2 Sources 4 2.1 USSTRATCOM Two-Line Elements (TLEs) .