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STS-103 Table of Contents Mission Overview
Refining the Hubble Space Telescope's View of the Universe SPACESPACESPACE SHUTTLESHUTTLESHUTTLE PRESSKITPRESSKITPRESSKIT WWW.SHUTTLEPRESSKIT.COM Updated November 24, 1999 STS-103 Table of Contents Mission Overview ......................................................................................................... 1 Mission Profile .............................................................................................................. 8 Crew.............................................................................................................................. 10 Flight Day Summary Timeline ...................................................................................................14 Rendezvous Rendezvous, Retrieval and Deploy ......................................................................................................18 EVA Hubble Space Telescope Extravehicular Activity ..................................................................................21 EVA Timeline ........................................................................................................................................24 Payloads Fine Guidance Sensor .........................................................................................................................27 Gyroscopes .........................................................................................................................................28 New Advanced Computer .....................................................................................................................30 -
Call for M5 Missions
ESA UNCLASSIFIED - For Official Use M5 Call - Technical Annex Prepared by SCI-F Reference ESA-SCI-F-ESTEC-TN-2016-002 Issue 1 Revision 0 Date of Issue 25/04/2016 Status Issued Document Type Distribution ESA UNCLASSIFIED - For Official Use Table of contents: 1 Introduction .......................................................................................................................... 3 1.1 Scope of document ................................................................................................................................................................ 3 1.2 Reference documents .......................................................................................................................................................... 3 1.3 List of acronyms ..................................................................................................................................................................... 3 2 General Guidelines ................................................................................................................ 6 3 Analysis of some potential mission profiles ........................................................................... 7 3.1 Introduction ............................................................................................................................................................................. 7 3.2 Current European launchers ........................................................................................................................................... -
Wubbo Ockels Happy Energy, Traveling Space & Treasuring Life on Our Planet
WUBBO OCKELS Happy EnErgy, travEling SpacE & trEaSuring lifE on our planEt 6th issue 2011 TRAVEL&EARTH BEYOND EcoplacES: Brazil, gili iSlandS,Scotland & morE miss univErSE doutzEn KroES - tHE maya WiSdom 2012 w fotografie: aLique ways possible. last year he even spoke at the “aruba goes green” conference together with former uSa vice president & nobel prize Winner al gore on state-of-the- art technology in green Energy. photographer alique and i arranged a photo shoot with this inspirational man for the cover and story. i made a healthy lunch, and we had a long (over 2 hours) interview in the sun on a canal in amsterdam, so i could learn more about this young-at- heart “OYL Eco Hero”. i think we all had a great day, and it shows! When i thought of flights to Space, i immediately thought of doutzen Kroes, who will be the first model to go to Space in 2014. i’m excited to bring you her story in this magazine. Space is a captivating place. galileo, the maya, the Egyptians - they all looked at the stars and used them as guides. the maya were also very interested in time. Birgitte rasine (who was introduced to me by top model and regular OYL contributor, anne-marie van dijk) is an expert on the maya people and their calendar. She offers some insight into this subject, especially WELCOME! regarding the “doomsday” 2012 prophecy. Should we find shelter? his is issue #6 and we are all that we should protect these go travel somewhere and hide? set to talk about one of my amazing spots. -
HD 97658 and Its Super-Earth Spitzer & MOST Transit Analysis and Seismic Modeling of the Host Star
The space photometry revolution CoRoT3-KASC7 joint meeting HD 97658 and its super-Earth Spitzer & MOST transit analysis and seismic modeling of the host star Valerie Van Grootel (University of Liege, Belgium) M. Gillon (U. Liege), D. Valencia (U. Toronto), N. Madhusudhan (U. Cambridge), D. Dragomir (UC Santa Barbara), and the Spitzer team 1. Introducing HD 97658 and its super-Earth The second brightest star harboring a transiting super-Earth HD 97658 (V=7.7, K=5.7) HD 97658 b, a transiting super-Earth • • Teff = 5170 ± 50 K (Howard et al. 2011) Discovery by Howard et al. (2011) from Keck- Hires RVs: • [Fe/H] = -0.23 ± 0.03 ~ Z - M sin i = 8.2 ± 1.2 M • d = 21.11 ± 0.33 pc ; from Hipparcos P earth - P = 9.494 ± 0.005 d (Van Leeuwen 2007) orb • Transits discovered by Dragomir et al. (2013) with MOST: RP = 2.34 ± 0.18 Rearth From Howard et al. (2011) From Dragomir et al. (2013) Valerie Van Grootel – CoRoT/Kepler July 2014, Toulouse 2 2. Modeling the host star HD 97658 Rp α R* 2/3 Mp α M* Radial velocities Transits + the age of the star is the best proxy for the age of its planets (Sun: 4.57 Gyr, Earth: 4.54 Gyr) • With Asteroseismology: T. Campante, V. Van Eylen’s talks • Without Asteroseismology: stellar evolution modeling Valerie Van Grootel – CoRoT/Kepler July 2014, Toulouse 3 2. Modeling the host star HD 97658 • d = 21.11 ± 0.33 pc, V = 7.7 L* = 0.355 ± 0.018 Lsun • +Teff from spectroscopy: R* = 0.74 ± 0.03 Rsun • Stellar evolution code CLES (Scuflaire et al. -
Space Reporter's Handbook Mission Supplement
CBS News Space Reporter's Handbook - Mission Supplement Page 1 The CBS News Space Reporter's Handbook Mission Supplement Shuttle Mission STS-125: Hubble Space Telescope Servicing Mission 4 Written and Produced By William G. Harwood CBS News Space Analyst [email protected] CBS News 5/10/09 Page 2 CBS News Space Reporter's Handbook - Mission Supplement Revision History Editor's Note Mission-specific sections of the Space Reporter's Handbook are posted as flight data becomes available. Readers should check the CBS News "Space Place" web site in the weeks before a launch to download the latest edition: http://www.cbsnews.com/network/news/space/current.html DATE RELEASE NOTES 08/03/08 Initial STS-125 release 04/11/09 Updating to reflect may 12 launch; revised flight plan 04/15/09 Adding EVA breakdown; walkthrough 04/23/09 Updating for 5/11 launch target date 04/30/09 Adding STS-400 details from FRR briefing 05/04/09 Adding trajectory data; abort boundaries; STS-400 launch windows Introduction This document is an outgrowth of my original UPI Space Reporter's Handbook, prepared prior to STS-26 for United Press International and updated for several flights thereafter due to popular demand. The current version is prepared for CBS News. As with the original, the goal here is to provide useful information on U.S. and Russian space flights so reporters and producers will not be forced to rely on government or industry public affairs officers at times when it might be difficult to get timely responses. All of these data are available elsewhere, of course, but not necessarily in one place. -
Asteroseismology with Corot, Kepler, K2 and TESS: Impact on Galactic Archaeology Talk Miglio’S
Asteroseismology with CoRoT, Kepler, K2 and TESS: impact on Galactic Archaeology talk Miglio’s CRISTINA CHIAPPINI Leibniz-Institut fuer Astrophysik Potsdam PLATO PIC, Padova 09/2019 AsteroseismologyPlato as it is : a Legacy with CoRoT Mission, Kepler for Galactic, K2 and TESS: impactArchaeology on Galactic Archaeology talk Miglio’s CRISTINA CHIAPPINI Leibniz-Institut fuer Astrophysik Potsdam PLATO PIC, Padova 09/2019 Galactic Archaeology strives to reconstruct the past history of the Milky Way from the present day kinematical and chemical information. Why is it Challenging ? • Complex mix of populations with large overlaps in parameter space (such as Velocities, Metallicities, and Ages) & small volume sampled by current data • Stars move away from their birth places (migrate radially, or even vertically via mergers/interactions of the MW with other Galaxies). • Many are the sources of migration! • Most of information was confined to a small volume Miglio, Chiappini et al. 2017 Key: VOLUME COVERAGE & AGES Chiappini et al. 2018 IAU 334 Quantifying the impact of radial migration The Rbirth mix ! Stars that today (R_now) are in the green bins, came from different R0=birth Radial Migration Sources = bar/spirals + mergers + Inside-out formation (gas accretion) GalacJc Center Z Sun R Outer Disk R = distance from GC Minchev, Chiappini, MarJg 2013, 2014 - MCM I + II A&A A&A 558 id A09, A&A 572, id A92 Two ways to expand volume for GA • Gaia + complementary photometric information (but no ages for far away stars) – also useful for PIC! • Asteroseismology of RGs (with ages!) - also useful for core science PLATO (miglio’s talk) The properties at different places in the disk: AMR CoRoT, Gaia+, K2 + APOGEE Kepler, TESS, K2, Gaia CoRoT, Gaia+, K2 + APOGEE PLATO + 4MOST? Predicon: AMR Scatter increases towards outer regions Age scatter increasestowars outer regions ExtracGng the best froM GaiaDR2 - Anders et al. -
Gaianir Combining Optical and Near-Infra-Red (NIR) Capabilities with Time-Delay-Integration (TDI) Sensors for a Future Gaia-Like Mission
Proposal title: GaiaNIR Combining optical and Near-Infra-Red (NIR) capabilities with Time-Delay-Integration (TDI) sensors for a future Gaia-like mission. PI: Dr. David Hobbs, Lund Observatory, Box 43, SE-221 00 Lund, Sweden. Email: [email protected]. Tel.: +46-46-22 21573 Core team members: The following minimum team is needed to initiate the project. D. Hobbs Lund Observatory, Sweden. A. Brown Leiden Observatory, Holland. A. Mora Aurora Technology B.V., Spain. C. Crowley HE Space Operations B.V., Spain. N. Hambly University of Edinburgh, UK. J. Portell Institut de Ciències del Cosmos, ICCUB-IEEC, Spain. C. Fabricius Institut de Ciències del Cosmos, ICCUB-IEEC, Spain. M. Davidson University of Edinburgh, UK. Proposal writers: See Appendix A. Other supporting scientists: See Appendix B and Appendix C. Senior science advisors: E. Høg Copenhagen University (Retired), Denmark. L. Lindegren Lund Observatory, Sweden. C. Jordi Institut de Ciències del Cosmos, ICCUB-IEEC, Spain. S. Klioner Lohrmann Observatory, Germany. F. Mignard Observatoire de la Côte d’Azur, France. arXiv:1609.07325v2 [astro-ph.IM] 22 May 2020 Fig. 1: Left is an IR image from the Two Micron All-Sky Survey (image G. Kopan, R. Hurt) while on the right an artist’s concept of the Gaia mission superimposed on an optical image, (Image ESA). Images not to scale. 1 1. Executive summary ESA recently called for new “Science Ideas” to be investigated in terms of feasibility and technological developments – for tech- nologies not yet sufficiently mature. These ideas may in the future become candidates for M or L class missions within the ESA Science Program. -
Astronomy & Astrophysics a Hipparcos Study of the Hyades
A&A 367, 111–147 (2001) Astronomy DOI: 10.1051/0004-6361:20000410 & c ESO 2001 Astrophysics A Hipparcos study of the Hyades open cluster Improved colour-absolute magnitude and Hertzsprung{Russell diagrams J. H. J. de Bruijne, R. Hoogerwerf, and P. T. de Zeeuw Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, The Netherlands Received 13 June 2000 / Accepted 24 November 2000 Abstract. Hipparcos parallaxes fix distances to individual stars in the Hyades cluster with an accuracy of ∼6per- cent. We use the Hipparcos proper motions, which have a larger relative precision than the trigonometric paral- laxes, to derive ∼3 times more precise distance estimates, by assuming that all members share the same space motion. An investigation of the available kinematic data confirms that the Hyades velocity field does not contain significant structure in the form of rotation and/or shear, but is fully consistent with a common space motion plus a (one-dimensional) internal velocity dispersion of ∼0.30 km s−1. The improved parallaxes as a set are statistically consistent with the Hipparcos parallaxes. The maximum expected systematic error in the proper motion-based parallaxes for stars in the outer regions of the cluster (i.e., beyond ∼2 tidal radii ∼20 pc) is ∼<0.30 mas. The new parallaxes confirm that the Hipparcos measurements are correlated on small angular scales, consistent with the limits specified in the Hipparcos Catalogue, though with significantly smaller “amplitudes” than claimed by Narayanan & Gould. We use the Tycho–2 long time-baseline astrometric catalogue to derive a set of independent proper motion-based parallaxes for the Hipparcos members. -
Echostar Annual Report Year Ended December 31, 2012 March 20, 2013
NASDAQ: SATS 100 Inverness Terrace East Englewood, CO 80112 303.706.4000 | echostar.com EchoStar Annual Report Year Ended December 31, 2012 March 20, 2013 Dear EchoStar Corporation Shareholders; 2012 was a very busy year for EchoStar. One of the most exciting accomplishments for 2012 was the addition of two new satellites to our growing fleet through the successful launches of EchoStar XVI and EchoStar XVII, bringing our total number of owned, leased and managed spacecraft to twenty-two. EchoStar operates the world’s fourth largest commercial geostationary satellite fleet and we continue to solidify our position as a premier global leader in satellite communications and operations. EchoStar ended 2012 with revenue of $3.1 billion, a growth of 13% over 2011. EBITDA in 2012 was $794 million, a growth of 64% over 2011. We generated a healthy $508 million of cash from operating activities in 2012 as a result primarily of the strong net income in 2012 and ended the year with a strong balance sheet with $1.5 billion of cash and marketable securities. EchoStar reached two very important long-term North America goals in 2012 with the market implementation of the HughesNet Gen4 service and the roll-out of the Hopper Whole Home DVR solution for DISH. Both solutions are garnering high praise and rapid adoption by consumers, a glowing testament to the capabilities and ingenuity of the EchoStar team. Additional notable accomplishments for 2012 include the very successful introduction of two new Slingbox retail products, several large enterprise contract renewals and new customers for Hughes data network services around the globe, and above-forecast sales of set-top-box products and video services to our established operator customers. -
82: a Context for International Cooperation and Competition (Part
Appendix B NASA's Approach to International Cooperation* Since the space program of United States began, the launched beyond man’s ability to repair easily.2 A National Aeronautics and Space Administration great deal of senior management attention, time and (NASA) has pursued a vigorous and successful’ pro- money is spent making sure that the last 3 to 5 per- gram of international cooperation, grounded in the cent of a project is done correctly. The importance of National Aeronautics and Space Act of 1958.** One this for international projects is that NASA managers possible reason for NASA’s success derives from a key want as much insight into them as they have into a feature of its cooperative efforts: while NASA has in- NASA-only project. This dictates a principle of “keep ternational programs, it does not fund an international it simple” in management and technical interfaces. This program. There is no “international” line item in the means that NASA prefers bilateral relations over proj- NASA budget and no money set aside especially for ects that might involve three or more countries or orga- international programs. Funding for international proj- nizations. ects must come out of the budgets of the NASA pro- The concern with technical and scientific excellence gram offices (essentially science, applications, space also contributes to NASA’s international programs in flight, and aeronautics), The Associate Administrators another fundamental way. From the very beginning of the Program Offices and their managers are rated the principal area of international space cooperation not on how many international projects they have, has been in the sciences. -
Franklin Chang-Díaz, Chairman and CEO, Ad Astra Rocket Company
Franklin Chang-Díaz, Chairman and CEO, Ad Astra Rocket Company: “The production of hydrogen through the electrolysis of water is a way of storing energy for use when needed” gerencia de riesgos y seguros Franklin Chang-Díaz, Chairman and CEO, Ad Astra Rocket Company: “The production of hydrogen through the electrolysis of water is a way of storing energy for use when needed” After earning a degree in Mechanical Engineering and a PhD in Plasma Physics, Franklin Chang-Díaz joined NASA in the early ‘80s as the first Latin American astronaut ever. Over 25 years of active service, he completed seven space missions and spent over 1,600 hours in space. After retiring, he founded Ad Astra Rocket, an aerospace engineering company that is researching electric propulsion engines and applying these advances to public transportation in his native Costa Rica The start of your space career dates back to the 1980s. What was the situation back then and what prospects were available? It was the start of the space shuttle era. Flights began in 1981, but they were very infrequent, as the technology was still under development. In 1980, there were only American astronauts at NASA, except for two Europeans (Claude Nicollier from Switzerland and Wubbo Ockels from the Netherlands) who entered the program in my group, marking the start of collaboration with the European Space Agency, which had just been established. My first space flight was in January 1986. During my 25 years at NASA, I participated as an astronaut on seven missions, sharing the world record for space flights with my colleague Jerry Ross. -
STS-103 Eng Hires
STS-103 European Space Agency’s role in space telescope servicing mission Astronauts set for Hubble challenge European Space Agency astronauts Claude Nicollier and Jean-François Clervoy are key members of the crew of the Space Shuttle Discovery that will carry out a new round of repairs and maintenance on the Hubble Space Telescope. The mission’s main objective is to replace Hubble’s failing pointing system, which allows astronomers to aim precisely at stars, planets and other celestial targets. ubble, a joint NASA-ESA computer and insulation material Claude Nicollier (left) and Jean-François project, is one of the most during two spacewalks. He will also Shuttle mission will keep Hubble Clervoy of ESA (inset picture) discuss the Hsuccessful orbiting obser- become the first European to walk in Hubble servicing mission vatories ever, having provided a space from the Space Shuttle. wealth of new scientific data about on target for astronomers Jean-François Clervoy will operate hundreds of astronomical objects. the Shuttle’s robotic arm during operation of the robotic arm. fourth gyroscope fails. Mission facts It continues to conduct scientific demanding phases of the mission, observations but its pointing system Hubble was launched in 1990 with With less than three working Flight STS-103 including initial capture of the has begun to fail so the Space an expected orbital lifetime of 20 gyroscopes Hubble would remain satellite and during the spacewalks. Orbiter Discovery Shuttle is being launched on an years. ESA contributed a 15 safely in orbit but could not continue earlier than planned mission to Nicollier is on his fourth flight into percent share to its development with science observations.