Genesat (Launched Dec 2006), – Pre-Sat/Nanosail-D (Aug 2008) – Pharmasat (Launched May 2009), – O/OREOS (Planned May

Total Page:16

File Type:pdf, Size:1020Kb

Genesat (Launched Dec 2006), – Pre-Sat/Nanosail-D (Aug 2008) – Pharmasat (Launched May 2009), – O/OREOS (Planned May National Aeronautics and Space Administration Free Flyer Utilization for Biology Research John W. Hines Chief Technologist, Engineering Directorate Technical Director, Nanosatellite Missions NASA-Ames Research Center NASA Applications of BioScience/BioTechnology HumanHuman ExplorationExploration EmphasisEmphasis FundamentalFundamental ExploratiExploratioonn Subsystems BiologyBiology Subsystems EmphasisEmphasis HumansHumans SmallSmall OrganismsOrganisms (Mice,(Mice, Rats) Rats) TiTissussue,e, O Orrgansgans MammalianMammalian CellsCells Human Health Emphasis ModelModel Organisms, BioMolecules Organisms, BioMolecules MicrobesMicrobes 2 4 Free-Flyer Utilization Free Flyer Features • Advantage: Relatively inexpensive means to increase number of flight opportunities • Capabilities: – Returnable capsule to small secondary non-recoverable satellites, and/or – In-situ measurement and control with autonomous sample management • Command and Control: Fully automated or uplinked command driven investigations. • Research data: Downlink and/or receipt of the samples • Collaborations: Interagency, academic, commercial and international Russian Free Flyers Early Free Flyers NASA Biosatellite I, II, 1966-67 NASA Biosatellite III, 1969 Nominal 3d flights Nominal 20d flight • Response to microgravity & • Spaceflight responses of non-human radiation: various biological species primates • Onboard radiation source Timeline of Russian-NASA Biology Spaceflights Collaborations Bion* Characteristics Bion Rationale • Increases access to space • Proven Platforms – Relatively low cost & risk -- >98% success with modified Vostok launcher and Cosmos/Bion & Foton spacecraft – Capitalizes on existing Russian capability - NASA had a productive collaboration in 9 joint missions (starting in 1975) –Full ECLSS – Nominal Duration is 20 - 30 Days, 45+ Days planned • Complements existing flight program (STS/ISS) – Supports animal research in space – Provides long duration microgravity exposure with onboard radiation source – Potential platform for artificial gravity research – Enables use of virulent organisms and hazardous chemicals -- response to disease and toxics – Technology testbed, advanced analytical devices, telescience & robotics • Rapid science return • Science drives mission design including launch and reentry timing, orbit, and flight duration Bion: Russian Mission Scenarios Mission, Date Bion-M1, 2012 (tbd) Bion-M2, 2014 (tbd) Bion-M3, 2016 (tbd) Duration: Up to 30 days 30-40 days 45+ days Long Duration rodent study Microgravity effects on w/ or w/o on-board radiation Artificial gravity, radiation Mission adult rodents and source for microgravity- or longer duration rodent Focus: smaller specimens radiation synergy microgravity study Systems biology Russian (bone, muscle, Focus: neuroscience, …) Radiation Health Artificial Gravity No. PIs: 10-15 10-20 10-20 Domestic Free Flyers Roles of Very Small Spacecraft • Science and Exploration Missions – Biological Sciences – Astrobiology – Astrophysics – Space Sciences – Space Physics – Lunar Sciences Payload packages on larger spacecraft • Technology Demonstrations – Propulsion • Flight heritage from – Communications Cubesat missions – Mass reduction - MEMS/NEMS NASA/ARC •Use Cubesat derived – Autonomous operations technologies to support – Formation flying/constellations other spacecraft – Novel space architectures - tethers – Evolvable, reconfigurable satellites missions • Lunar Orbiters • Lunar Landers CalTech LANL Aerospace Corp MicroSatellite - Free Flyers • Microsatellites are small, rapidly deployable, highly flexible science and technology spaceflight platforms generally considered to be of mass less than 100 kg. • For the Microsatellite Free Flyer Project, the spacecraft range in mass from 5-50 kg, with initial missions utilizing platforms in the 5-10kg range • These spacecraft are capable of accommodating fully autonomous payloads and conducting in-situ measurement, monitoring and control biological experiments, with real-time analysis and data downlink. µSat-FF capabilities validated by multiple spaceflights: – GeneBox (launched Jul 2006), – GeneSat (launched Dec 2006), – Pre-Sat/Nanosail-D (Aug 2008) – PharmaSat (launched May 2009), – O/OREOS (planned May. 2010); – SALMON (planned May. 2011+) 12 MicroSatellite Free Flyer (µSat-FF) Project ScienceScience TargetsTargets && ApplicationsApplications • Goal: Provide the capability to support biological/biotechnology payloads for model organisms, mammalian cells, and other relevant specimens • Measurement Targets (subset): – Gene expression; protein expression; metabolites, signalers, excretates; growth, kill curves; behavior • Possible Applications (subset): – Combined radiation/reduced gravity consequences: mammalian cells, human gene carriers (e.g. yeast), model organisms. • DNA damage: wound healing, cancer • Cell membrane damage: central nervous system • Oxidation: compromised defense to hazards & pathogens • Protein damage: impaired bone & muscle function – Space effects on microbes/pathogens • Virulence increase/decrease • Changes in pharmacological efficacy => PharmaSat-1 • Push the envelope of miniaturization, automation: also benefits human- tended payloads, related terrestrial applications– e.g. “canary-on-a-chip” Capabilities • Fully autonomous, self-contained free-flyers. • Multiple configurations to address a multitude of research scenarios. • Mass: 4 – 50 kg total spacecraft payload in µSat-FF configuration (3 – 75 L total volume) • Accommodated on most any launch vehicle due to small size, volume • Many orbital trajectories: LEO, HEO, GEO, Lunar, etc. • Low power consumption: 4 – 50 W • Temperature control: 15 – 40 °C (4 °C with 30-50 kg version), <0.5 °C stability • Humidity control: 30 – 100%, active or passive control • Media support: liquid culture or solid/gel-supported growth; fluid exchange; bio/chemical challenges • Atmosphere: 1 atm ± 10%; active O2, CO2 control; gas exchange • In-situ, real-time analysis; autonomous data management & telemetry • Interactive with “timeout autonomy” or fully autonomous experimental control. • Sample return possible (future) Microsatellite Technologies Goal: develop modular, broadly-applicable Sample Management, Culturing technology platform that … • elucidates molecular biological effects of µ‐fluidics microgravity + radiation space-flight µ‐wellplates environment: gene & protein expression, Detection and Analysis metabolites Diffuse fluorescence, • is applicable to many micro- and small luminescence organisms: single/multicellular; adherent, Spatial Imaging non-adherent, motile cytometry • is designed for fully autonomous life support, sample processing, analysis Single-wavelength • is reconfigurable, modular in design; Multi-wavelength i.e. “replicate friendly” multiwell approach PCR • supports multiple measurement strategies and tools DNA, Spectroscopy protein • has minimum practical size, weight, power µarrays consumption: low-cost 2° payloads Applicability: Free-Flyers, ISS, Gnd R&D, Xfer Microsat Free Flyer Multi-Year Schedule Status FY09 FY10 FY11 FY12 FY13 FY14 FY15 FY16 1 4 4 4 1 1 2 2 3 1 2 3 4 1 2 3 1 2 3 4 1 2 3 2 3 4 1 2 3 4 3 4 PharmaSat (Msat FF1) MoO* MSat FF/MoO 1 MSat FF/MoO 2 Msat FF 2 MoO 3 Msat FF 3 MoO 4 Msat FF 4 MoO5 Planning Phase B Solicitation & Selection Phase C Data Analysis & Report Pre‐Phase A Phase D Launch Phase A Phase E/F 16 Note: Schedule beyond FY 2014 is notional E/PO EXAMPLE: GeneSat-1 Student Involvement Preparing the next generation of engineers with hands-on experience, solving real world problems Pre-Launch/Mission Operations 6 Universities: Arizona State University; Cal Poly, San Luis Obispo; Northeastern University; San Francisco State University; Santa Clara University; Stanford University 2 High Schools: Leland High School; Georgianna Bruce Kirby Prep School 40 Students: 19 Grad Students; 19 Undergrad Students; 2 High School Students 13 Student Projects: 3 Co-op projects; 4 Capstone projects; 2 Undergraduate Thesis Topics; 3 Graduate Thesis Topics; 1(very near term) Doctoral Thesis Topic Post-Launch Engagement University Level: Montana State University and Cal Poly: participants in the Amateur Radio Contest, Having access to your conversion factors, also permitted our students to engage in data reduction and analysis techniques. Dave Klumpar, MSU; Old Dominion University space system engineering course: homework assignment using GeneSat 1 to predict the decay rate of a satellite in a circular orbit High School Level: Manheim Central High School, Lancaster, PA 9th grade Earth Science students using GeneSat Telemetry data while studying astronomy, analyze solar cell currents, and the temperatures of the satellite as it orbits the earth using Excel to create graphs of the data. Elementary School Level: St Catherine of Sienna School in Burlingame, GeneSat Telemetry Science Fair Entry by ‘JAK’ Kitts, Age 9 Free Flyer Solicitations Bion M1 NRA (Immunology and BSP) Theme areas: Immune Function Biospeciman Sharing Program: rodent investigations Exploration Relevance: Understanding long term space environment effects on immune function can provide insight to space exploration crew health risk. Schedule: 43 Step-1 proposals received 39 invited to submit Step-2 proposals 33 Step-2 proposals received Science Definition Selections: 5 Immune and 9 BSP proposals SALMON AO (Small Complete Missions of Opportunity in FSB) Theme areas: Fundamental Space Biology investigations on microbes, cells or small animals. Schedule: Up to 2 Missions will be selected AO Release:
Recommended publications
  • Russia's Posture in Space
    Russia’s Posture in Space: Prospects for Europe Executive Summary Prepared by the European Space Policy Institute Marco ALIBERTI Ksenia LISITSYNA May 2018 Table of Contents Background and Research Objectives ........................................................................................ 1 Domestic Developments in Russia’s Space Programme ............................................................ 2 Russia’s International Space Posture ......................................................................................... 4 Prospects for Europe .................................................................................................................. 5 Background and Research Objectives For the 50th anniversary of the launch of Sputnik-1, in 2007, the rebirth of Russian space activities appeared well on its way. After the decade-long crisis of the 1990s, the country’s political leadership guided by President Putin gave new impetus to the development of national space activities and put the sector back among the top priorities of Moscow’s domestic and foreign policy agenda. Supported by the progressive recovery of Russia’s economy, renewed political stability, and an improving external environment, Russia re-asserted strong ambitions and the resolve to regain its original position on the international scene. Towards this, several major space programmes were adopted, including the Federal Space Programme 2006-2015, the Federal Target Programme on the development of Russian cosmodromes, and the Federal Target Programme on the redeployment of GLONASS. This renewed commitment to the development of space activities was duly reflected in a sharp increase in the country’s launch rate and space budget throughout the decade. Thanks to the funds made available by flourishing energy exports, Russia’s space expenditure continued to grow even in the midst of the global financial crisis. Besides new programmes and increased funding, the spectrum of activities was also widened to encompass a new focus on space applications and commercial products.
    [Show full text]
  • Venona Special Studies
    - 1 - Venona Project Special Studies Transcribed by Students of the Mercyhurst College Institute for Intelligence Studies Arranged by John Earl Haynes, Library of Congress, 2010 COVER NAMES IN NEW YORK TRAFFIC p. 2 UNIDENTIFIED COVER NAMES IN NEW YORK TRAFFIC p. 86 COVER NAMES IN SAN FRANCISCO TRAFFIC p. 92 COVER NAMES IN WASHINGTON TRAFFIC p. 123 ADDITIONAL COVERNAMES AND RELATED INFORMATION IN DIPLOMATIC TRAFFIC p. 127 REVISED TRANSLATION OF MESSAGE ON ANTENNA-LIBERAL'S WIFE ETHEL p. 135 THE COVERNAMES "ANTENNA" AND "LIBERAL" IN . MESSAGES p. 139 ESSAGES IN . INVOLVING THE COVERNAME"ENORMOZ" AND THE NAMES OF NUCLEAR PHYSICISTS, ETC. p. 147 UNDATED REPORT OF MEREDITH GARDNER p. 155 DEVELOPMENT OF THE “G--“HOMER” [“GOMER”] CASE p. 158 THE KOMAR (KRAVCHENKO) AFFAIR IN . MESSAGES p. 161 REVISED TRANSLATION OF TWO . MESSAGES ON CHANGES IN COVERNAMES p. 170 THE COVERNAME "KARAS" IN. TRAFFIC p. 178 THE COVERNAMES "TÉNOR", "BAS", AND "CHETÁ" (? IN . TRAFFIC p. 181 - 2 - Special Study Cover Names in New York Traffic - 3 - cover-name Message number Date Publication reference S/ or 3/NBF/ 19 N.Y. to M. 812 29053 JKI 06 T1022 1B-1910 0027A ABRAM N.Y. to M. 992 24063 JKR 14 T872√ 1B-7518 0005A JACK SOBLE 1086 06073 JKV 48 T873√ 2A-0011 1957 29113 NNNNNN T939√ 625 04054 JHD 48 T916√ 851 15064 JIJ 40 T10.1√ 1146 10084 JHM 41 T123√ 1251 02094 JHN 12 T301√ (to ChEKh) 0005B 1353 23094 JHO 42 T289√ 1449 12104 JIL 37 T106√ 1754 14124 JHZ 49 T6√ 48 11015 JHV 37 (NSA)T1941 AVGUR 2A-0013 1638 (AUGUR) N.Y.
    [Show full text]
  • Lunar Life Sciences Payload Assessment
    Lunar Surface Science Workshop 2020 (LPI Contrib. No. 2241) 5077.pdf LUNAR LIFE SCIENCES PAYLOAD ASSESSMENT. S. C. Sun1, F. Karouia2, M. P. Lera3, M. P. Parra1, H. E. Ray4, A. J. Ricco1, S. M. Spremo1. 1NASA Ames Research Center, 2Blue Marble Space Institute of Science, 3KBR, 4ASRC Federal Space and Defense, Inc. Introduction: The Moon provides a unique site to ISS, including systems that integrate into EXPRESS study living organisms. The fractional gravity and (EXpedite the PRocessing of ExperimentS for Space) unique radiation environment have similarities to Mars Racks or are external space exposure research facilities. and will help us understand how life will respond to These same systems can be the basis for future payload conditions on the red planet. Martian and lunar envi- systems for experiments to be performed beyond Low ronments can be simulated on the ground but not to high Earth Orbit. Such facilities would need to be adapted to fidelity. Altered gravity and increased radiation are dif- be compatible with the new research platforms and ficult to replicate simultaneously, which makes study- function in the harsher radiation environment found out- ing their combined effect difficult. The International side the magnetosphere. If Gateway and a lunar based- Space Station, and previously, the Space Shuttle, pro- lab could provide EXPRESS-compatible interfaces, lev- vided a microgravity environment, and could simulate eraging hardware developed for ISS would be more fea- fractional-g only via an onboard centrifuge. Because sible. the ISS and Space Shuttle orbits were within the Earth’s Gaps in Capabilities: Many of the payload systems magnetosphere, experiments on those platforms have that have been developed require human tending.
    [Show full text]
  • Of Mice and Materials: Payoffs of UNSGC Research Infrastructure Awards
    Utah State University DigitalCommons@USU Presentations Materials Physics 5-8-2017 Of Mice and Materials: Payoffs of UNSGC Research Infrastructure Awards JR Dennison Utah State Univesity Follow this and additional works at: https://digitalcommons.usu.edu/mp_presentations Part of the Condensed Matter Physics Commons Recommended Citation Dennison, JR, "Of Mice and Materials: Payoffs of UNSGC Research Infrastructure Awards" (2017). Utah NASA Space Grant Consortium Annual Meeting. Presentations. Paper 168. https://digitalcommons.usu.edu/mp_presentations/168 This Presentation is brought to you for free and open access by the Materials Physics at DigitalCommons@USU. It has been accepted for inclusion in Presentations by an authorized administrator of DigitalCommons@USU. For more information, please contact [email protected]. Of Mice and Materials: Payoffs of UNSGC Research Infrastructure Awards J.R. Dennison Materials Physics Group Physics Department, Utah State University Utah NASA Space Grant Consortium Annual Meeting Weber State University May 8, 2017 To paraphrase Douglas Adams, “Space is [harsh]. You just won’t believe how vastly, hugely, mind-bogglingly [harsh] it is.” Interactions with this harsh space environment can modify materials and cause unforeseen and detrimental effects to spacecraft. The Poster Child for Space Environment Effects Ag coated Mylar with micrometeoroid impact USU MISSIE SUSpECS Logan, UT II Sample Tray Before After Complex dynamic interplay between space environment, satellite motion, and materials properties Facilities & Capabilities • Four ultrahigh vacuum chambers for electron emission tests equipped with electron, ion, and photon sources, detectors, and surface analysis capabilities. Sample Characterization & Preparation • Two high vacuum chambers for resistivity tests. • Bulk composition (AA, IPC). • High vacuum chamber for electrostatic breakdown tests.
    [Show full text]
  • 18Th EANA Conference European Astrobiology Network Association
    18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures.
    [Show full text]
  • Space Biology Research and Biosensor Technologies: Past, Present, and Future †
    biosensors Perspective Space Biology Research and Biosensor Technologies: Past, Present, and Future † Ada Kanapskyte 1,2, Elizabeth M. Hawkins 1,3,4, Lauren C. Liddell 5,6, Shilpa R. Bhardwaj 5,7, Diana Gentry 5 and Sergio R. Santa Maria 5,8,* 1 Space Life Sciences Training Program, NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] (A.K.); [email protected] (E.M.H.) 2 Biomedical Engineering Department, The Ohio State University, Columbus, OH 43210, USA 3 KBR Wyle, Moffett Field, CA 94035, USA 4 Mammoth Biosciences, Inc., South San Francisco, CA 94080, USA 5 NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] (L.C.L.); [email protected] (S.R.B.); [email protected] (D.G.) 6 Logyx, LLC, Mountain View, CA 94043, USA 7 The Bionetics Corporation, Yorktown, VA 23693, USA 8 COSMIAC Research Institute, University of New Mexico, Albuquerque, NM 87131, USA * Correspondence: [email protected]; Tel.: +1-650-604-1411 † Presented at the 1st International Electronic Conference on Biosensors, 2–17 November 2020; Available online: https://iecb2020.sciforum.net/. Abstract: In light of future missions beyond low Earth orbit (LEO) and the potential establishment of bases on the Moon and Mars, the effects of the deep space environment on biology need to be examined in order to develop protective countermeasures. Although many biological experiments have been performed in space since the 1960s, most have occurred in LEO and for only short periods of time. These LEO missions have studied many biological phenomena in a variety of model organisms, and have utilized a broad range of technologies.
    [Show full text]
  • NASA Ames to Establish Nationwide Lunar Science Institute
    November 2007 Worden gives upbeat message about future work for Ames BY JOHN BLUCK "We have switched material to In an upbeat talk to a crowd that phenolic impregnated carbon abla- filled the Ames main auditorium, tor (PICA), a (heat shield) material Ames Center Director S. Pete Worden developed here," Worden noted. His outlined an exciting future at Ames projected slide also listed Ames as that includes new work in exploration, leading PICA development and test- science and aeronautics -- each about a ing both for the Crew Exploration Ve- third of the center's efforts, he said. "I hicle, now called Orion, and the Mars have a gazillion charts to go through," Science Laboratory (MSL), which has photo by Eric James NASA he said. a planned launch date in fall 2009. His wide-ranging presentation Worden said that Ames' arc jets about Ames touched on moon explo- facility "a unique facility in the world." ration, a lunar institute, moon dust re- He added, "We want to upgrade search, heat shield work for spacecraft them." destined for the moon and Mars, a Mars sample "cache box" assignment, Life Sciences rising supercomputer capability, small "We are getting additional life Ames Center Director S. Pete Worden responds satellite work with a potential for support tasks assigned by Johnson to a question during the recent upbeat talk he many missions, increased astrobiology (and Marshall)," Worden said. "This is gave to the center about the future of Ames. work, growing cooperation among significant." continued on page 5 academia, and commercial partners and Ames and much more.
    [Show full text]
  • 6 FOTON RETRIEVABLE CAPSULES This Section Is Aimed at Providing New and Experienced Users with Basic Utilisation Information Regarding Foton Retrievable Capsules
    6 FOTON RETRIEVABLE CAPSULES This section is aimed at providing new and experienced users with basic utilisation information regarding Foton retrievable capsules. It begins with an introduction to the Foton capsule. 6.1 Introduction to Foton Capsules 6.1.1 What Are Foton Capsules? Foton capsules (Figure 6-1 and Figure 6-2) are unmanned, retrievable capsules, derived from the design of the 1960’s Soviet Vostok manned spacecraft and the Zenit military reconnaissance satellite. These capsules are very similar to the Bion and Resurs-F satellites introduced by the Soviets in the 1970’s, for biological research and Earth natural resources investigation, respectively. The first Foton capsule was launched in 1985 as Cosmos 1645 and only with the fourth launch in 1988 was the spacecraft officially designated Foton (Foton-4). These capsules are launched into near-circular, low-earth orbits by a Soyuz-U rocket, providing researchers with gravity levels less than 10 -5 g, for missions lasting approximately 2 weeks. The earlier Foton missions were conceived primarily for materials science research, but later missions also began to include experiments in the fields of fluid physics, biology and radiation dosimetry. ESA’s participation in the Foton programme began in 1991 with a protein crystallisation experiment on-board Foton-7, followed by a further 35 experiments up to and including the Foton- 12 mission in 1999. In 2002, ESA provided a large number of experiments for the Foton-M1 mission (the first flight of an upgraded version of the Foton spacecraft). This mission ended in disaster when the Soyuz launcher rocket exploded shortly after lift-off due to a malfunction in one of its engines.
    [Show full text]
  • Ssc09-Xii-03
    SSC09-XII-03 The Promise of Innovation from University Space Systems: Are We Meeting It? Michael Swartwout St. Louis University 3450 Lindell Boulevard St. Louis, Missouri 63103; (314) 977-8240 [email protected] ABSTRACT A popular notion among universities is that we are innovation-drivers in the staid, risk-adverse spacecraft industry – we are to professional small satellites what small satellites are to the “battlestars”. By contrast, professional industry takes a much different perspective on university-class spacecraft; these programs are good for attracting students to space and providing valuable pre-career training, but the actual flight missions are ancillary, even unimportant. Which opinion is correct? Both are correct. The vast majority of the 111 student-built spacecraft that have flown have made no innovative contributions. That is not to say that they have been without contribution. In addition to the inarguable benefits to education, many have served as radio Amateur communications, science experiments and even technological demonstrations. But “innovative”? Not so much. However, there have been two innovative contributors, whose contributions are large enough to settle the question: the University of Surrey begat SSTL, which helped create the COTS-based small satellite industry. Stanford and Cal Poly begat CubeSats, whose contributions are still being created today. This paper provides an update to our earlier submissions on the history of student-built spacecraft. Major trends identified in previous years will be re-examined with new data -- especially the bifurcation between larger-scale, larger-scope "flagship" programs and small-scale, reduced-mission "independents". In particular, we will demonstrate that the general history of student-built spacecraft has not been one of innovation, nor of development of new space systems -- with those few, extremely noteworthy, exceptions.
    [Show full text]
  • 0418 Space Cluster Brochure FINAL
    HARWELL SPACE MultidisciplinaryCLUSTER Innovation CONTENTS HARWELL FOREWORD CAMPUS 2 Harwell Campus 4 Success of the Harwell Space Cluster 6 Multidisciplinary Innovation 5,500people 8 Building the Harwell Space Cluster 9 Vision for the Future Harwell Campus is an exciting place to be, with cutting edge 10 UK Space Industry science facilities, major organisations and a great mix of companies from start-ups to multinationals. The Campus was quick to realise 12 Stakeholder Organisations £2+bnfacilities that it needed a mechanism to encourage collaboration, knowledge 20 Companies Driving Innovation at Harwell sharing and drive innovation, which led to the development of 40 Life at Harwell thematic Clusters. It started with the Harwell Space Cluster and now includes the HealthTec and EnergyTec Clusters. 42 Harwell Tomorrow 45 Contact I have watched Harwell Campus flourish over the last seven years, including the Harwell Space Cluster, which has grown to 80 organisations employing 800 people. I don’t expect there to be any let up in this growth and I look forward to the Campus changing, literally before my very eyes. SPACE I am really excited about the opportunities at the intersections between these Clusters, such as between the Space and HealthTec Clusters. Harwell CLUSTER Campus is able to demonstrate multidisciplinary innovation every day. There is no better way to really understand what is happening than to visit. I hope that you will do just that and that you will become part of the exciting future of the Harwell Space Cluster and help the UK reach organisations80 its goal of taking 10% of the global space market by 2030.
    [Show full text]
  • 22 WRMISS 2017 Conference Program
    22nd WRMISS 2017 Conference Program 5 – 7 September 2017 Thales Alenia Space, Torino, Italy 1 22st WRMISS Conference Program: Tuesday 5th September 2017 09.00 – 09.15 Welcome 09.15 – 10.00 Invited Talk 10:00 – 10:30 Scientific Session 1 10.30 – 11.15 Coffee/Tea Break 11.15 – 12.45 Scientific Session 2 12.45 – 14.00 Lunch 14.00 – 15.30 Scientific Session 3 15.30 – 16.15 Coffee/Tea Break 16.15 – 18.00 Scientific Session 4 Guenther Reitz Welcome Walter Cugno, Cesare Lobascio and Martina Giraudo Welcome and Organisational Issues Invited Talk Roberto Battiston SPACE RADIATION SUPERCONDUCTING SHIELDS - A NEW APPROACH Scientific Session 1 Matteo Palermo Solar modulation, Forbush decreases and Solar Energetic Particles with AMS Scientific Session 2 Francis F. Badavi Evaluation of galactic cosmic rays (GCR) models using AMS2 data Results and lessons learned from calibration measurements of the TRITEL Atila Hirn 3D silicon detector telescope at the HIMAC accelerator facility Microdosimetric modeling of the relative efficiency of thermoluminescent Alessio Parisi detectors exposed to charged particles relevant for space applications Scientific Session 3 Time of Flight measurements on-board the ISS: development of LIDAL (Light A. Rizzo Ion Detector for ALTEA) apparatus ” George P. Stuart Particle Type and Energy Identification in Single Pixellated Silicon Detectors Martin Kakona AIRDOS - an open source dosimeter for measurement on board of aircraft Marianthi The sensitivity of p-MOSFET dosemeter to heavy ions Fragopoulou Scientific Session 4 Contribution of Different Particles onboard Bion-M1 Estimated by Means of Iva Ambrožová Plastic Nuclear Track Detectors The "PHOENIX" radiobiological experiment on-board the Russian segment of Andrea Stradi the ISS supported by passive dosimetry - First results Neutron Spectrometry and Dosimetry on spacecraft with passive detector Alba Zanini system Bubble-Detector Measurements for Matroshka-R and Radi-N2: ISS-47/48 Martin B.
    [Show full text]
  • Lingua Franca Nova English Dictionary
    Lingua Franca Nova English Dictionary 16 October 2012 http://lfn.wikia.com/ http://webspace.ship.edu/cgboer/lfn/ http://purl.org/net/lfn/disionario/ 1 Lingua Franca Nova (LFN) is an auxiliary constructed language created by Dr C George Boeree of Shippensburg University, Pennsylvania. This is a printable copy of the master dictionary held online at http://purl.org/net/lfn/disionario/. A printable English–LFN dictionary can be downloaded from the same location. Abbreviations ABBR = abbreviation ADJ = adjective ADV = adverb BR = British English COMP = compound word (verb + noun) CONJ = conjunction DET = determiner INTERJ = interjection N = noun NUM = numeral PL = plural PREF = prefix PRENOM = prenominal (used before a noun) PREP = preposition PREVERB = preverbal (used before a verb) PRON = pronoun SUF = suffix US = American English V = verb VI = intransitive verb VT = transitive verb Indicators such as (o-i) and (e-u) mark words in which two vowels do not form a diphthong in normal pronunciation. 2 termination; aborta natural V miscarry; N miscarriage; A abortada ADJ abortive; ADV abortively; abortiste N abortionist; antiabortiste ADJ N antiabortionist A N A (letter, musical note) abracadabra! INTERJ abracadabra! hocus-pocus! a PREP at, in, on (point in space or time); to (movement); abrasa VT embrace, hug; clamp; N embrace, hug; abrasa toward, towards, in the direction of (direction); to ursin N bear hug; abrasable ADJ embraceable, (recipient) huggable; abrasador N clamp; abrasador fisada N vise a INTERJ ah, aha (surprise, sudden realization,
    [Show full text]