50 Years of the UK in Space
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Giotto Steals a Ride
NEWS COM8ARYPROBE------------------------------------- JAPANESE UNIVERSITIES---- Giotto steals a ride MurmUrS of complaint Washington Munich this is a bargain", says GEM project scien JAPAN's national university professors are THE Earth lost a minute fraction of its tist Gerhard Schwehm. Schwehm said that all employees of the government, which orbital velocity earlier this week as the the second flyby would be a unique oppor puts them in an odd position when they European Space Agency (ESA) Giotto tunity to expand knowledge of comets. It want to protest to the government about space probe stole a little of the Earth's will be especially interesting, he said, to university conditions. But last month, the energy to help it on its way to a rendezvous study the interaction of the coma of the Association of National Universities finally with the comet Grigg Skjellerup. It was comet and the solar wind, as well as to succeeded, after years of trying, in winning the first time the manoeuvre, the same compare the distribution and optical funds from the Ministry of Education, "gravity assist" that helped the NASA properties of dust around Comet Grigg Culture and Science to set up a committee Voyager probe on its journey from Jupiter Skjellerup with that around Comet to study their own financial difficulties. out to Saturn and Neptune, had been exe Halley, which had at least 100 times more The association represents all the 93 cuted using the gravitation field of Earth. of it. national universities directly supported by According to ESA researcher Trevor Giotto was one of five spacecraft to the government and has responsibility for Morley, Giotto will gain 3.1 km/sec in approach Comet Halley in 1986, but it setting up the general entrance examination. -
Rosetta Craft Makes Historic Comet Rendezvous European Space Agency's Comet-Chasing Mission Arrives After 10-Year Journey
NATURE | NEWS Rosetta craft makes historic comet rendezvous European Space Agency's comet-chasing mission arrives after 10-year journey. Elizabeth Gibney 06 August 2014 ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA Comet 67P/Churyumov–Gerasimenko, as seen by Rosetta from a distance of 285 kilometres. No one can deny that it was an epic trip. The European Space Agency's comet-chasing Rosetta spacecraft has arrived at its quarry, after launching more than a decade ago and travelling 6.4 billion kilometres through the Solar System. That makes it the first spacecraft to rendezvous with a comet, and takes the mission a step closer to its next, more ambitious goal of making the first ever soft landing on a comet. Speaking from mission control in Darmstadt, Germany, Matt Taylor, Rosetta project scientist for the European Space Agency (ESA), called the space mission “the sexiest there’s ever been”. Rosetta is now within 100 kilometres of its target, comet 67P/Churyumov–Gerasimenko (or 67P for short), which in July was discovered to be shaped like a rubber duck. After a six-minute thruster burn, at 11:29 a.m. local time on 6 August, ESA scientists confirmed that Rosetta had moved into the same orbit around the Sun as the comet. Rosetta is now moving at a walking pace relative to the motion of 67P — though both are hurtling through space at 15 kilometres per second. Unlike NASA’s Deep Impact and Stardust craft, and ESA’s Giotto mission, which flew by their target comets at high speed, Rosetta will now stay with the comet, taking a ring-side seat as 67P approaches the Sun, and eventually swings around it in August 2015. -
May 14, 2010 Vol
May 14, 2010 Vol. 50, No. 10 Spaceport News John F. Kennedy Space Center - America’s gateway to the universe www.nasa.gov/centers/kennedy/news/snews/spnews_toc.html INSIDE . STS-132 payload has international flair Explorer School By Linda Herridge Symposium Spaceport News oeing’s STS-132 payload flow man- Bager, Eve Stavros, and NASA Mission Man- ager Robert Ashley, will be stationed on console in Fir- ing Room 2 of Kennedy’s Launch Control Center, Page 2 watching with anticipation as space shuttle Atlantis STS-130 crew soars into the sky from returns Launch Pad 39A. Stavros and Boeing’s Checkout Assembly and NASA/Gianni Woods Payload Processing Ser- Technicians prepare to lift the Russian-built Mini Research Module-1, or MRM-1, out of its transportation container in Kennedy’s vices, or CAPPS, team were Space Station Processing Facility for its move to the payload canister and transportation to Launch Pad 39A. instrumental in helping to prepare the Russian-built Processing Facility, about environmental testing at Stavros drew on previ- Mini Research Module-1, or five weeks before the sched- the launch pad. Boeing also ous international experi- MRM-1, and an Integrated uled launch, for transfer coordinated delivery and ence from her work on life Cargo Carrier for delivery to the launch pad and final setup of ground support sciences payloads for the orbiter integration activi- equipment at the launch pad European Space Agency in Page 3 to the International Space Station. ties,” Ashley said. “The for testing operations and the Netherlands. NASA alums According to Stavros, processing team met or beat served as the main inter- “Working with RSC lay foundation planning and coordination every schedule milestone face with the shuttle team Energia was an exercise in to process the two major despite the relatively small to ensure payload schedule payloads began more than a size of the NASA and Boe- compatibility. -
Will the Real Monster Black Hole Please Stand Up? 8 January 2015
Will the real monster black hole please stand up? 8 January 2015 how the merging of galaxies can trigger black holes to start feeding, an important step in the evolution of galaxies. "When galaxies collide, gas is sloshed around and driven into their respective nuclei, fueling the growth of black holes and the formation of stars," said Andrew Ptak of NASA's Goddard Space Flight Center in Greenbelt, Maryland, lead author of a The real monster black hole is revealed in this new new study accepted for publication in the image from NASA's Nuclear Spectroscopic Telescope Astrophysical Journal. "We want to understand the Array of colliding galaxies Arp 299. In the center panel, mechanisms that trigger the black holes to turn on the NuSTAR high-energy X-ray data appear in various and start consuming the gas." colors overlaid on a visible-light image from NASA's Hubble Space Telescope. The panel on the left shows NuSTAR is the first telescope capable of the NuSTAR data alone, while the visible-light image is pinpointing where high-energy X-rays are coming on the far right. Before NuSTAR, astronomers knew that the each of the two galaxies in Arp 299 held a from in the tangled galaxies of Arp 299. Previous supermassive black hole at its heart, but they weren't observations from other telescopes, including sure if one or both were actively chomping on gas in a NASA's Chandra X-ray Observatory and the process called accretion. The new high-energy X-ray European Space Agency's XMM-Newton, which data reveal that the supermassive black hole in the detect lower-energy X-rays, had indicated the galaxy on the right is indeed the hungry one, releasing presence of active supermassive black holes in Arp energetic X-rays as it consumes gas. -
On the Spectra of Gamma-Ray Bursts at High Energies
University of New Hampshire University of New Hampshire Scholars' Repository Doctoral Dissertations Student Scholarship Spring 1986 ON THE SPECTRA OF GAMMA-RAY BURSTS AT HIGH ENERGIES STEVEN MICHAEL MATZ University of New Hampshire, Durham Follow this and additional works at: https://scholars.unh.edu/dissertation Recommended Citation MATZ, STEVEN MICHAEL, "ON THE SPECTRA OF GAMMA-RAY BURSTS AT HIGH ENERGIES" (1986). Doctoral Dissertations. 1483. https://scholars.unh.edu/dissertation/1483 This Dissertation is brought to you for free and open access by the Student Scholarship at University of New Hampshire Scholars' Repository. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of University of New Hampshire Scholars' Repository. For more information, please contact [email protected]. INFORMATION TO USERS This reproduction was made from a copy of a manuscript sent to us for publication and microfilming. While the most advanced technology has been used to pho tograph and reproduce this manuscript, the quality of the reproduction is heavily dependent upon the quality of the material submitted. Pages in any manuscript may have indistinct print. In all cases the best available copy has been filmed. The following explanation of techniques is provided to help clarify notations which may appear on this reproduction. 1. Manuscripts may not always be complete. When it is not possible to obtain missing pages, a note appears to indicate this. 2. When copyrighted materials are removed from the manuscript, a note ap pears to indicate this. 3. Oversize materials (maps, drawings, and charts) are photographed by sec tioning the original, beginning at the upper left hand comer and continu ing from left to right in equal sections with small overlaps. -
The Most Dangerous Ieos in STEREO
EPSC Abstracts Vol. 6, EPSC-DPS2011-682, 2011 EPSC-DPS Joint Meeting 2011 c Author(s) 2011 The most dangerous IEOs in STEREO C. Fuentes (1), D. Trilling (1) and M. Knight (2) (1) Northern Arizona University, Arizona, USA, (2) Lowell Observatory, Arizona, USA ([email protected]) Abstract (STEREO-B) which view the Sun-Earth line using a suite of telescopes. Each spacecraft moves away 1 from the Earth at a rate of 22.5◦ year− (Figure 1). IEOs (inner Earth objects or interior Earth objects) are ∼ potentially the most dangerous near Earth small body Our search for IEOs utilizes the Heliospheric Imager population. Their study is complicated by the fact the 1 instruments on each spacecraft (HI1A and HI1B). population spends all of its time inside the orbit of The HI1s are centered 13.98◦ from the Sun along the the Earth, giving ground-based telescopes a small win- Earth-Sun line with a square field of view 20 ◦ wide, 1 dow to observe them. We introduce STEREO (Solar a resolution of 70 arcsec pixel− , and a bandpass of TErrestrial RElations Observatory) and its 5 years of 630—730 nm [3]. Images are taken every 40 minutes, archival data as our best chance of studying the IEO providing a nearly continuous view of the inner solar population and discovering possible impactor threats system since early 2007. The nominal visual limit- ing magnitude of HI1 is 13, although the sensitivity to Earth. ∼ We show that in our current search for IEOs in varies somewhat with solar elongation, and asteroids STEREO data we are capable of detecting and char- fainter than 13 can be seen near the outer edges. -
ARIEL – 13Th Appleton Space Conference PLANETS ARE UBIQUITOUS
Background image credit NASA ARIEL – 13th Appleton Space Conference PLANETS ARE UBIQUITOUS OUR GALAXY IS MADE OF GAS, STARS & PLANETS There are at least as many planets as stars Cassan et al, 2012; Batalha et al., 2015; ARIEL – 13th Appleton Space Conference 2 EXOPLANETS TODAY: HUGE DIVERSITY 3700+ PLANETS, 2700 PLANETARY SYSTEMS KNOWN IN OUR GALAXY ARIEL – 13th Appleton Space Conference 3 HUGE DIVERSITY: WHY? FORMATION & EVOLUTION PROCESSES? MIGRATION? INTERACTION WITH STAR? Accretion Gaseous planets form here Interaction with star Planet migration Ices, dust, gas ARIEL – 13th Appleton Space Conference 4 STAR & PLANET FORMATION/EVOLUTION WHAT WE KNOW: CONSTRAINTS FROM OBSERVATIONS – HERSCHEL, ALMA, SOLAR SYSTEM Measured elements in Solar system ? Image credit ESA-Herschel, ALMA (ESO/NAOJ/NRAO), Marty et al, 2016; André, 2012; ARIEL – 13th Appleton Space Conference 5 THE SUN’S PLANETS ARE COLD SOME KEY O, C, N, S MOLECULES ARE NOT IN GAS FORM T ~ 150 K Image credit NASA Juno mission, NASA Galileo ARIEL – 13th Appleton Space Conference 6 WARM/HOT EXOPLANETS O, C, N, S (TI, VO, SI) MOLECULES ARE IN GAS FORM Atmospheric pressure 0.01Bar H2O gas CO2 gas CO gas CH4 gas HCN gas TiO gas T ~ 500-2500 K Condensates VO gas H2S gas 1 Bar Gases from interior ARIEL – 13th Appleton Space Conference 7 CHEMICAL MEASUREMENTS TODAY SPECTROSCOPIC OBSERVATIONS WITH CURRENT INSTRUMENTS (HUBBLE, SPITZER,SPHERE,GPI) • Precision of 20 ppm can be reached today by Hubble-WFC3 • Current data are sparse, instruments not absolutely calibrated • ~ 40 planets analysed -
1 HOLD for RELEASE UNTIL PRESENTED by WITNESS March
HOLD FOR RELEASE UNTIL PRESENTED BY WITNESS March 13, 2019 Statement of James F. Bridenstine Administrator National Aeronautics and Space Administration before the Committee on Commerce, Science, and Transportation United States Senate Mr. Chairman and Members of the Committee, I am very pleased to appear before you today. NASA is proud to be at the forefront of a global effort to advance humanity’s future in space, leading the world while expanding on our Nation’s great capacity for exploration and innovation. This is a role the Agency has played for over 60 years, leveraging the talent and hard work of America’s skilled Government and aerospace industry workforce to push the boundaries of science, exploration, and technology development to achieve bold goals in the aviation and space arenas. Now, pursuant to Space Policy Directive-1 (and consistent with the NASA Transition Authorization Act of 2017), NASA is pursuing “an innovative and sustainable program of exploration with commercial and international partners to enable human expansion across the solar system and to bring back to Earth new knowledge and opportunities.” We are working on a sustainable campaign of exploration, transitioning the International Space Station (ISS), returning humans to the surface of the Moon and lunar orbit, where we will build the systems, deep space infrastructure, and operational capabilities to expand human presence beyond the Earth-Moon system, eventually embarking on human missions to Mars and other destinations. Since its inception, NASA’s historic and enduring purpose has been aligned to four major strategic thrusts – Discover, Explore, Develop, and Enable. These correspond to our missions of scientific discovery of the natural phenomena of the Earth, of other worlds, and of the cosmos as a whole. -
Four New Faculty Join AE Ormsbee Professorship Endowed Online MS
Newsletter of the Department of Aerospace Engineering University of Illinois at Urbana-Champaign Vol. 17 • 2015 Upholding AE’s Tradition of Teaching Excellence PAGE 18 Four New Faculty Join AE PAGE 4 Ormsbee Professorship Endowed PAGE 14 Online MS Program Debuts PAGE 15 Inside Welcome to the 2015 Edition of the Alumni Newsletter of Faculty News Aerospace Engineering at AE Gains Four New Faculty ....................................4 Selig and Chung Earn Promotions ...............................7 Illinois Bodony Named Willett Faculty Scholar ...........................7 In last year’s newsletter, I started my introductory Bringing Aerodynamics Research to Life, Elliott Builds on Illinois’ Tradition . 8 words by reporting with great excitement that four Friend, Colleague Recalls Professor Sivier .........................9 Mission Possible: This Device Will Self-Destruct When Heated .........10 new faculty members were going to join the Depart- Chung Co-leading $1.5 Million Development of Robot Bats for ment during the 2014-15 academic year. This was Construction Site Monitoring ...............................10 the culmination of a remarkable recruitment effort Ansell Wins Young Investigator Award for Work on Dynamic Stall that our Department had never experienced in the Unsteady Flow ..........................................11 twenty or so years that I have been in AE@Illinois. AE Scientists Examine Deflecting, Exploring Asteroids ...............12 Well, I am absolutely delighted to report once again Panesi earns NASA Early Career Faculty Award for Modeling of that four more faculty members will join AE during Mars Entry .............................................13 the 2015-16 academic year to help the Department Chasiotis, Ansell and Gerhold Recognized for Advising ..............13 with its teaching and research missions in the areas of Department News space exploration and technology, aeroelasticity, big data, topology optimization and additive manufactur- Liebeck Endows Ormsbee Professorship .........................14 ing. -
FINESSE and ARIEL + CASE: Dedicated Transit Spectroscopy Missions for the Post-TESS Era
FINESSE and ARIEL + CASE: Dedicated Transit Spectroscopy Missions for the Post-TESS Era Fast Infrared Exoplanet FINESSE Spectroscopy Survey Explorer Exploring the Diversity of New Worlds Around Other Stars Origins | Climate | Discovery Jacob Bean (University of Chicago) Presented on behalf of the FINESSE/CASE science team: Mark Swain (PI), Nicholas Cowan, Jonathan Fortney, Caitlin Griffith, Tiffany Kataria, Eliza Kempton, Laura Kreidberg, David Latham, Michael Line, Suvrath Mahadevan, Jorge Melendez, Julianne Moses, Vivien Parmentier, Gael Roudier, Evgenya Shkolnik, Adam Showman, Kevin Stevenson, Yuk Yung, & Robert Zellem Fast Infrared Exoplanet FINESSE Spectroscopy Survey Explorer Exploring the Diversity of New Worlds Around Other Stars **Candidate NASA MIDEX mission for launch in 2023** Objectives FINESSE will test theories of planetary origins and climate, transform comparative planetology, and open up exoplanet discovery space by performing a comprehensive, statistical, and uniform survey of transiting exoplanet atmospheres. Strategy • Transmission spectroscopy of 500 planets: Mp = few – 1,000 MEarth • Phase-resolved emission spectroscopy of a subset of 100 planets: Teq > 700 K • Focus on synergistic science with JWST: homogeneous survey, broader context, population properties, and bright stars Hardware • 75 cm aluminum Cassegrain telescope at L2 • 0.5 – 5.0 μm high-throughput prism spectrometer with R > 80 • Single HgCdTe detector with JWST heritage for science and guiding Origins | Climate | Discovery Advantages of Fast Infrared -
Finding Aid to the Jerry L. Ross Papers, 1889-2013
http://www.jsc.nasa.gov/Bios/portraits/ross.jpg FINDING AID TO THE JERRY L. ROSS PAPERS, 1889-2013 Purdue University Libraries Virginia Kelly Karnes Archives and Special Collections Research Center 504 West State Street West Lafayette, Indiana 47907-2058 (765) 494-2839 http://www.lib.purdue.edu/spcol © 2013 Purdue University Libraries. All rights reserved. Processed by: Mary A. Sego, August 20, 2013 Additions Added: July 25, 2015 Descriptive Summary Creator Information Ross, Jerry L., 1948- Title Jerry L. Ross papers Collection Identifier MSA 283 Date Span 1940-2013, predominant 1970-2000 Abstract This collection includes materials that document Ross' student life at Purdue, his test flight engineer work, and NASA career as an engineer and astronaut. The collection includes Purdue coursework, textbooks, and memorabilia; papers from Ross' work at Edwards Air Force Base, Wright Patterson Air Force Base, and Test Pilot School; NASA Space Shuttle training, mission documents and scrapbooks, artifacts, and flight crew films and interviews. Examples of the types of materials in the collection include aircraft flight test manuals, flight reports, mission plans, and checklists for the B-1 aircraft, Test Pilot School materials, NASA course materials, publications, and Space Shuttle Mission checklists, manuals, handbooks, an oral history interview, and 16mm and VHS films. In particular, this collection provides an insider’s view of space exploration, and a window through which we may begin to understand and take measure of the era of the United States Space Shuttle Program. Extent 46.10 cubic feet (13 c.f. boxes, 53 full width letter size mss boxes, 4 half width letter size mss box, 13 full width legal size mss, 5 half width legal size mss boxes, 1 large flight suit box, 4 large flat boxes, 1 small flat box, 2 small artifact boxes and 428 MB) Finding Aid Author Mary A. -
Sts-51G Press Kit June 1985
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION SPACE SHUTTLE MISSION STS-51G PRESS KIT JUNE 1985 ARABSAT A; MORELOS A; TELSTAR 3-D; SPARTAN 1 Edited by Richard W. Orloff, 01/2001/Page 1 STS-5IG INSIGNIA S85-31266 -- The STS-51G insignia illustrates the advances in aviation technology in the United States within a relatively short span of the twentieth century. The flags of the French (Baudry) and Saudi Arabian (Al-Saud) payload specialists appear next to their name at the bottom of the insignia. The NASA insignia design for space shuttle flights is reserved for use by the astronauts and for other official use as the NASA Administrator may authorize. Public availability has been approved only in the form of illustrations by the various news media. When and if there is any change in this policy, which we do not anticipate, it will be publicly announced. PHOTO CREDIT: NASA or National Aeronautics and Space Administration. Edited by Richard W. Orloff, 01/2001/Page 2 RELEASE NO: 85-8 June 1985 CONTACTS Charles Redmond/Sarah Keegan Headquarters, Washington, DC (Phone: 202/453-8590) James Elliott Goddard Space Flight Center, Greenbelt, MD (Phone: 301/344-6256) David Alter Johnson Space Center, Houston, TX (Phone: 713/483-5111) Jim Ball Kennedy Space Center, FL (Phone: 305/867-2468) Ralph Jackson Dryden Flight Research Facility, Edwards, CA (Phone: 805/258-8381) Edited by Richard W. Orloff, 01/2001/Page 3 RELEASE NO: 85-83 June 1985 CONTENTS GENERAL RELEASE 5 51-G BRIEFING SCHEDULE 7 GENERAL INFORMATION 8 SHUTTLE MISSION 51-G -- QUICK LOOK FACTS