International Space Station Overview Research and On-Orbit Facilities Non-Partner Participation
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Attachment J-4 Applicable and Reference Documents Lists
NNJ12GA46C SECTION J Attachment J-4 MISSION AND PROGRAM INTEGRATION CONTRACT Attachment J-4 Applicable and Reference Documents Lists J-A4-1 NNJ12GA46C SECTION J Attachment J-4 MISSION AND PROGRAM INTEGRATION CONTRACT This attachment contains applicable documents for the contract effort. The contractor shall comply with these requirements in performing Statement of Work (SOW) requirements. This attachment is structured as follows: Table J4-1: Applicable Documents List Table J4-2: Reference Documents List Table J4-3: Book Editor/Book Coordinated/Managed Documents List Table J4-4: Orion Documents List The documents identified within Table J4-1 or within a document listed in this table (second tier) are applicable to this contract. Requirements written in these documents have full force and effect as if their text were written in this contract to the extent that the requirements relate to context of the work to be performed within the scope of this contract. When a document is classified as “reference,” the document is provided for information about the ISS Program execution and the Mission and Program Integration Contract’s role in the ISS Program. The general approach for interpreting whether a document impacts the contractor’s performance is that if a document is “applicable,” then the contractor has solid requirements that derive from that document. Applicable documents contain additional requirements and are considered binding to the extent specified. Applicable documents cited in the text of the document in a manner that indicates applicability such as follows: • In accordance with • As stated in • As specified in • As defined in • Per • In conformance with When a document is classified as “reference,” the document is provided for general context of the ISS Program execution and for influence on the performance of the Mission and Program Integration Contract in its role of support to the ISS Program. -
AAS/AIAA Astrodynamics Specialist Conference
DRAFT version: 7/15/2011 11:04 AM http://www.alyeskaresort.com AAS/AIAA Astrodynamics Specialist Conference July 31 ‐ August 4, 2011 Girdwood, Alaska AAS General Chair AIAA General Chair Ryan P. Russell William Todd Cerven Georgia Institute of Technology The Aerospace Corporation AAS Technical Chair AIAA Technical Chair Hanspeter Schaub Brian C. Gunter University of Colorado Delft University of Technology DRAFT version: 7/15/2011 11:04 AM http://www.alyeskaresort.com Cover images: Top right: Conference Location: Aleyska Resort in Girdwood Alaska. Middle left: Cassini looking back at an eclipsed Saturn, Astronomy picture of the day 2006 Oct 16, credit CICLOPS, JPL, ESA, NASA; Middle right: Shuttle shadow in the sunset (in honor of the end of the Shuttle Era), Astronomy picture of the day 2010 February 16, credit: Expedition 22 Crew, NASA. Bottom right: Comet Hartley 2 Flyby, Astronomy picture of the day 2010 Nov 5, Credit: NASA, JPL-Caltech, UMD, EPOXI Mission DRAFT version: 7/15/2011 11:04 AM http://www.alyeskaresort.com Table of Contents Registration ............................................................................................................................................... 5 Schedule of Events ................................................................................................................................... 6 Conference Center Layout ........................................................................................................................ 7 Conference Location: The Hotel Alyeska ............................................................................................... -
Information Summaries
TIROS 8 12/21/63 Delta-22 TIROS-H (A-53) 17B S National Aeronautics and TIROS 9 1/22/65 Delta-28 TIROS-I (A-54) 17A S Space Administration TIROS Operational 2TIROS 10 7/1/65 Delta-32 OT-1 17B S John F. Kennedy Space Center 2ESSA 1 2/3/66 Delta-36 OT-3 (TOS) 17A S Information Summaries 2 2 ESSA 2 2/28/66 Delta-37 OT-2 (TOS) 17B S 2ESSA 3 10/2/66 2Delta-41 TOS-A 1SLC-2E S PMS 031 (KSC) OSO (Orbiting Solar Observatories) Lunar and Planetary 2ESSA 4 1/26/67 2Delta-45 TOS-B 1SLC-2E S June 1999 OSO 1 3/7/62 Delta-8 OSO-A (S-16) 17A S 2ESSA 5 4/20/67 2Delta-48 TOS-C 1SLC-2E S OSO 2 2/3/65 Delta-29 OSO-B2 (S-17) 17B S Mission Launch Launch Payload Launch 2ESSA 6 11/10/67 2Delta-54 TOS-D 1SLC-2E S OSO 8/25/65 Delta-33 OSO-C 17B U Name Date Vehicle Code Pad Results 2ESSA 7 8/16/68 2Delta-58 TOS-E 1SLC-2E S OSO 3 3/8/67 Delta-46 OSO-E1 17A S 2ESSA 8 12/15/68 2Delta-62 TOS-F 1SLC-2E S OSO 4 10/18/67 Delta-53 OSO-D 17B S PIONEER (Lunar) 2ESSA 9 2/26/69 2Delta-67 TOS-G 17B S OSO 5 1/22/69 Delta-64 OSO-F 17B S Pioneer 1 10/11/58 Thor-Able-1 –– 17A U Major NASA 2 1 OSO 6/PAC 8/9/69 Delta-72 OSO-G/PAC 17A S Pioneer 2 11/8/58 Thor-Able-2 –– 17A U IMPROVED TIROS OPERATIONAL 2 1 OSO 7/TETR 3 9/29/71 Delta-85 OSO-H/TETR-D 17A S Pioneer 3 12/6/58 Juno II AM-11 –– 5 U 3ITOS 1/OSCAR 5 1/23/70 2Delta-76 1TIROS-M/OSCAR 1SLC-2W S 2 OSO 8 6/21/75 Delta-112 OSO-1 17B S Pioneer 4 3/3/59 Juno II AM-14 –– 5 S 3NOAA 1 12/11/70 2Delta-81 ITOS-A 1SLC-2W S Launches Pioneer 11/26/59 Atlas-Able-1 –– 14 U 3ITOS 10/21/71 2Delta-86 ITOS-B 1SLC-2E U OGO (Orbiting Geophysical -
Jules Verne ATV Launch Approaching 11 February 2008
Jules Verne ATV launch approaching 11 February 2008 will carry up to 9 tonnes of cargo to the station as it orbits 400 km above the Earth. Equipped with its own propulsion and navigation systems, the ATV is a multi-functional spacecraft, combining the fully automatic capabilities of an unmanned vehicle with the safety requirements of a crewed vehicle . Its mission in space will resemble that, on the ground, of a truck (the ATV) delivering goods and services to a research establishment (the space station). A new-generation high-precision navigation system will guide the ATV on a rendezvous trajectory towards the station. In early April, Jules Verne will automatically dock with the station’s Russian Preview of the maiden launch and docking of ESA's Jules Verne ATV. Jules Verne will be lifted into space on Service Module, following a number of specific board an Ariane 5 launch vehicle. Credits: ESA - D. operations and manoeuvres (on 'Demonstration Ducros Days') to show that the vehicle is performing as planned in nominal and contingency situations. It will remain there as a pressurised and integral After the successful launch of ESA’s Columbus part of the station for up to six months until a laboratory aboard Space Shuttle Atlantis on controlled re-entry into the Earth’s atmosphere Thursday (7 February), it is now time to focus on takes place, during which it will burn up and, in the the next imminent milestone for ESA: the launch of process, dispose of 6.3 tonnes of waste material no Jules Verne, the first Automated Transfer Vehicle longer needed on the station. -
Level Ministerial and Scientific Event a New Era of Blue Enlightenment
Report on the High- Level Ministerial and Scientific Event A New Era of Blue Enlightenment 12-14 July 2017 Lisbon, Portugal October 2017 EUROPEAN COMMISSION Directorate-General for Research and Innovation Directorate F — Bioeconomy Unit F.4 — Marine Resources Contact: Sieglinde Gruber E-mail: [email protected] [email protected] European Commission B-1049 Brussels EUROPEAN COMMISSION Report on the High-Level Ministerial and Scientific Event A New Era of Blue Enlightenment 12-14 July 2017 Directorate-General for Research and Innovation 2017 Bioeconomy EN 3 EUROPE DIRECT is a service to help you find answers to your questions about the European Union Freephone number (*): 00 800 6 7 8 9 10 11 (*) The information given is free, as are most calls (though some operators, phone boxes or hotels may charge you) LEGAL NOTICE This document has been prepared for the European Commission however it reflects the views only of the authors, and the Commission cannot be held responsible for any use which may be made of the information contained therein. More information on the European Union is available on the internet (http://europa.eu). Luxembourg: Publications Office of the European Union, 2016. PDF ISBN 978-92-79-73529-5 doi: 10.2777/64644 KI-04-17-849-EN-N © European Union, 2017. Reproduction is authorised provided the source is acknowledged. Cover images: © Lonely, # 46246900, 2011. © ag visuell #16440826, 2011. © Sean Gladwell #6018533, 2011. © LwRedStorm, #3348265. 2011. © kras99, #43746830, 2012. Source: Fotolia.com Internal document image(s): © European Union, 2017, Source: EC - Audiovisual Service, Photo: Bruno Portela 3 "The Sea, the great unifier, is man's only hope. -
The International Space Station and the Space Shuttle
Order Code RL33568 The International Space Station and the Space Shuttle Updated November 9, 2007 Carl E. Behrens Specialist in Energy Policy Resources, Science, and Industry Division The International Space Station and the Space Shuttle Summary The International Space Station (ISS) program began in 1993, with Russia joining the United States, Europe, Japan, and Canada. Crews have occupied ISS on a 4-6 month rotating basis since November 2000. The U.S. Space Shuttle, which first flew in April 1981, has been the major vehicle taking crews and cargo back and forth to ISS, but the shuttle system has encountered difficulties since the Columbia disaster in 2003. Russian Soyuz spacecraft are also used to take crews to and from ISS, and Russian Progress spacecraft deliver cargo, but cannot return anything to Earth, since they are not designed to survive reentry into the Earth’s atmosphere. A Soyuz is always attached to the station as a lifeboat in case of an emergency. President Bush, prompted in part by the Columbia tragedy, made a major space policy address on January 14, 2004, directing NASA to focus its activities on returning humans to the Moon and someday sending them to Mars. Included in this “Vision for Space Exploration” is a plan to retire the space shuttle in 2010. The President said the United States would fulfill its commitments to its space station partners, but the details of how to accomplish that without the shuttle were not announced. The shuttle Discovery was launched on July 4, 2006, and returned safely to Earth on July 17. -
Professor Jun'ichiro Kawaguchi: Particles Brought Back From
Japan Aerospace Exploration Agency January 2011 No. 03 Special Features Professor Jun’ichiro Kawaguchi: Refl ecting on the Hayabusa mission and the future of space exploration Particles brought back from Asteroid Itokawa: What methods did researchers use to discover particles inside Hayabusa’s sample-return capsule? Contents No. 03 Japan Aerospace Exploration Agency 1−7 Interview with Professor Jun’ichiro Welcome to JAXA TODAY Kawaguchi The Japan Aerospace Exploration Agency (JAXA) works to realize its Midori Nishiura, advisor to JAXA vision of contributing to a safe and prosperous society through the on public affairs, interviewed pursuit of research and development in the aerospace fi eld to deepen Professor Jun’ichiro Kawaguchi humankind’s understanding of the universe. JAXA’s activities cover a on such topics as the development broad spectrum of the space and aeronautical fi elds, including satellite of Japan’s space probes and the development and operation, astronomical observation, planetary future of space exploration. exploration, participation in the International Space Station (ISS) project, and the development of new rockets and next-generation aeronautical technology. 8-11 With the aim of disseminating information about JAXA’s activities How many particles from Itokawa and recent news relating to Japan’s space development programs to was Hayabusa able to capture? as wide an audience as possible, we launched JAXA TODAY in January 2010. Marking the fi rst anniversary of the launch of JAXA TODAY, in What methods did research- this, the third issue, we feature an interview with Professor Jun’ichiro ers use to discover the particles Kawaguchi, who led the Hayabusa project, and also provide a close-up brought back from Asteroid look at how the particles brought back from Asteroid Itokawa were dis- Itokawa inside Hayabusa’s covered inside Hayabusa’s sample-return capsule. -
Presentation71.Pdf
The KiboCUBE Programme December 14, 2017 United Nations / South Africa Symposium on Basic Space Technology “Small satellite missions for scientific and technological advancement” Masanobu TSUJI Japan Aerospace Exploration Agency (JAXA) 1 Credit : JAXA/NASA ISS: Japan’s Capabilities and Contributions ISS Kibo (International Space Station) (Japanese Experiment Module) HTV (H-II Transfer Vehicle) ▪ ISS is a huge manned construction located about 400km above the Earth. ▪ 15 countries participate in the ISS program ▪ Japan strives to make concrete international contributions through extensive utilization of Kibo and HTV. H-IIB Credit : JAXA/NASA 2 ISS: Japan’s Capabilities and Contributions Kibo: Japanese Experiment Module Kibo has a unique Exposed Facility (EF) with an Airlock (AL) and a Remote Manipulator System (JEMRMS), and has a high capacity to exchange experimental equipment. Robotic Arm (JEM-Remote Manipulator System) Airlock Credit : JAXA/NASA 3 “Kibo” is Unique! – Exposed Facility Small Satellite Deployment platform using J-SSOD AtIn present,recent years, satellite a growing deployers numberother ofthan universities J-SSOD andthat companiesuse Kibo include around the world have beenthe NanoRacks developing CubeSat the DeployerMicro/Nano (NRCSD)-satellite and (under 100kg, mainlyCyclops CubeSat). (Space Station Integrated Kinetic Launcher for Orbital Payload Systems). Credit : JAXA/NASA J-SSOD#2 NRCSD#1 Cyclops#1 J-SSOD Microsat#1 J-SSOD#1 J-SSOD Upgrade#1 4 Ref: Prof. 2017 Nano/Microsatellite Market Forecast (SpaceWorks Enterprises -
We Need Your Colouring Skills!
We need your colouring skills! What do you think the colours of Mercury are? DID YOU KNOW? ercury • Mercury is the smallest planet in our solar system. • It is only slightly larger than the Earth’s Moon. • One day on Mercury is as long as 59 days on Earth. • A year on Mercury is as long as 88 Earth days • Temperatures on Mercury are extreme, reaching 430°C during the day, and -180°C at night. DID YOU KNOW? The Erth Depending on where you are on the globe, you could be spinning through space at just over 1,000 miles per hour. Water covers 70 percent of Earth's surface. 1 million Earths could fit in the Sun. Earth's atmosphere is composed of about 78 percent nitrogen, 21 percent oxygen, 0.9 percent argon, and 0.1 percent other gases. Earth is the only planet not named after a god. We need your colouring skills! What colours will you choose? We need your colouring skills! What do you think the colours of Jupiter are? DID YOU KNOW? Jupiter • Jupiter is the largest planet in the solar system. • Jupiter is as large as 1,300 Earths. • It's the 3rd brightest object in the night sky. • There's a big red spot on Jupiter, which is in fact a storm that has been raging for more than 350 years. DID YOU KNOW? Saturn • Saturn is the 2nd largest planet in the Solar System. • 764 Earths could fit inside Saturn. • Saturn's rings are made of ice and rock. They span 175,000 miles We need your and yet they’re only 20 metres thick. -
Highlights in Space 2010
International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren UNITED NATIONS 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France Tel: +33 1 45 67 42 60 Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 E-mail: : [email protected] E-mail: [email protected] Fax. + 33 1 44 76 74 37 URL: www.iislweb.com OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL : http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 *1180239* V.11-80239—January 2011—775 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no. -
The Need for Detailed Ionic Composition of the Near-Earth Plasma
HeliophysicsHELIO 2050 2050 White Papers (2021) R. Ilie4094.pdf THE NEED FOR DETAILED IONIC COMPOSITION OF THE NEAR-EARTH PLASMA An impressive body of work has been devoted to the escape of H+, He+ and O+ ions from Earth’s ionosphere, and their circulation and redistribution throughout the terrestrial magneto- sphere (Schunk and Raitt, 1980; Schunk and Sojka, 1997; Winglee et al., 2002; Glocer et al., 2009; Ilie et al., 2015; Ilie and Liemohn, 2016). However, the transport and energization of N+, in addi- tion to that of O+, has not been considered by most studies, even though a number of direct and indirect measurements made to describe the ionic composition of the ionosphere-magnetosphere system, have established that N+ is a significant ion species in the ionosphere and its presence in the magnetosphere is significant. A wide range in the magnitude oftheN+ to O+ density ratio has been reported, with significant variations not only with geomagnetic activity, but also with solar cycle, season, time of day, latitude, etc (Mall et al., 2002; Christon et al., 2002). These vari- ations suggest that N+ and O+, while relatively close in mass, they obey different chemical and energization processes, and possibly follow different paths of energization. In addition, observations from the WIND STICS ISIS 2 spacecraft (Hoffman et al., 1974) indicated that not only N+, but also molecular ions were ob- served in the Earth’s magnetosphere Geotail STICS AMPTE and ionosphere. Measurements from CCE Explorer 31 Akebono SMS the Arase satellite (Miyoshi et al., MMS ISIS-2 IMS DE-1 RIMSS e-POP 2018) showed the existence of molec- OGO-6 OGOGO-2-2 IMSS Sputnik3 IMS AE-C ular ions in the Earth’s ring cur- RMS IMS rent region, even under moderate ge- omagnetic storm conditions. -
Butina Keynote
Vision A human outpost in space bringing nations together for the benefit of life on Earth… and beyond. We will make revolutionary discoveries and establish a permanent international presence of humans in space, to advance the exploration of the solar system and enable commerce in space. U.S. Core complete Mission Safely build, operate, and utilize a continuously inhabited orbital research facility through a partnership of governments, industries, and academia. International partner complete dimensions: 171 ft. long, 240 ft. wide, 90 ft. high, 15,000 cubic feet of living space. weight: 197 tons (404,000 lbs.) ISS today science capabilities: laboratories from four space agencies planned, U.S. Lab “Destiny” operating since Feb. 2001. orbital inclination/path: 51.6 degrees, covering 90% of the world’s population. altitude: approximately 240 miles above the Earth. speed: 17,500 miles per hour, orbiting the Earth 16 times a day. The International Space Station is more powerful, and 4 times larger, than any human space craft ever built. Over 100 people have visited the ISS so far, 17% for the second time. United States 16 International Participants Canada Russia Europe 5 International Partners Japan ISS Technical Configuration Elements Currently on Orbit Elements Pending US Shuttle Launch Science Power Module (SPM) Elements Pending Russian Launch Docking Compartment (DC) 1 Zarya Control Module Zvezda Service Module PMA 1 S1 Truss SO Truss Port SM MMOD Shields Segment Segment Photovoltaic AMS ULC1 P1 Truss Arrays ULC2 Port MT/ CETA Research Module (RM) Mobile Segment Rails S3/4 Truss Servicing Segment System P6 Truss Multipurpose Laboratory Segment Module (MLM) Express Pallets Starboard MT/ CETA Rails P5 Truss S6 Truss Segment Segment ESP-3 P3/4 Truss S5 Truss Segment Segment ESP-4 Canadarm2 Starboard Photovoltaic Arrays Dextre (SPDM) Mobile Remote Servicer Base System (MBS), JEM ELM-PS Mobile Transporter (MT) ESP-2 Z1 Truss Segment JEM RMS & Exposed Facility Airlock PMA 3 Node 1 Cupola U.S.