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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 -
Hubble Space Telescope
HUBBLE SPACE TELESCOPE Pioneering optics made by Ball Aerospace are ® GO BEYOND WITH BALL. responsible for the Hubble Space Telescope’s iconic images and revolutionary discoveries. In total, Ball has built seven instruments for Hubble, including the five currently aboard the telescope. Beginning with the first servicing mission in 1993 through the fourth in 2009, Ball’s advanced optical technologies have extended Hubble’s operational life and enabled the telescope to help us understand our universe as never before. OUR ROLE QUICK FACTS Since scientists began formulating the idea for Hubble, • Ball-built seven science instruments for the first major optical telescope in space, Ball played a Hubble, two star trackers, five major leave- part, providing a total of seven science instruments flown behind equipment subsystems. on Hubble. Today, Ball supports COS, WFC3, ACS, STIS and NICMOS and provides on-orbit mission operations • Each of the five science instruments now support. After the last servicing mission in 2009, Hubble’s operating on the telescope were Ball-designed unprecedented science capabilities made it the premier and built. space-based telescope for ultraviolet, optical and near- • Ball-built COSTAR was installed during infrared astronomy. Servicing Mission 1 in 1993 along with JPL’s Cosmic Origins Spectrograph (COS) WFPC-2 to correct Hubble’s hazy vision. COS is the most sensitive ultraviolet spectrograph ever • Ball developed more than eight custom tools built for space and replaced the Ball-built COSTAR in 2009. to support astronauts during COS improved Hubble’s ultraviolet sensitivity at least 10 servicing missions. times and up to 70 times when observing very faint objects, like distant quasars, massive celestial objects, too faint for previous spectrographs. -
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. -
Wide Field Camera 3 Instrument Mini-Handbook for Cycle 16
Version 3.0 October 2006 Wide Field Camera 3 Instrument Mini-Handbook for Cycle 16 For long-term planning only Do not propose for WFC3 in Cycle 16 Space Telescope Science Institute 3700 San Martin Drive Baltimore, Maryland 21218 [email protected] Operated by the Association of Universities for Research in Astronomy, Inc., for the National Aeronautics and Space Administration User Support For prompt answers to any question, please contact the STScI Help Desk. • E-mail: [email protected] • Phone: (410) 338-1082 (800) 544-8125 (U.S., toll free) World Wide Web Information and other resources are available on the WFC3 World Wide Web sites at STScI and GSFC: • URL: http://www.stsci.edu/hst/wfc3 • URL: http://wfc3.gsfc.nasa.gov WFC3 Mini-Handbook Revision History Version Date Editor 3.0 October 2006 Howard E. Bond 2.0 October 2003 Massimo Stiavelli 1.0 October 2002 Mauro Giavalisco Contributors: Sylvia Baggett, Tom Brown, Howard Bushouse, Mauro Giavalisco, George Hartig, Bryan Hilbert, Randy Kimble, Matt Lallo, Olivia Lupie, John MacKenty, Larry Petro, Neill Reid, Massimo Robberto, Massimo Stiavelli. Citation: In publications, refer to this document as: Bond, H. E., et al. 2006, “Wide Field Camera 3 Instrument Mini-Handbook, Version 3.0” (Baltimore: STScI) Send comments or corrections to: Space Telescope Science Institute 3700 San Martin Drive Baltimore, Maryland 21218 E-mail:[email protected] Acknowledgments The WFC3 Science Integrated Product Team (2006) Sylvia Baggett Howard Bond Tom Brown Howard Bushouse George Hartig Bryan Hilbert Robert Hill (GSFC) -
Solar Orbiter Assessment Study and Model Payload
Solar Orbiter assessment study and model payload N.Rando(1), L.Gerlach(2), G.Janin(4), B.Johlander(1), A.Jeanes(1), A.Lyngvi(1), R.Marsden(3), A.Owens(1), U.Telljohann(1), D.Lumb(1) and T.Peacock(1). (1) Science Payload & Advanced Concepts Office, (2) Electrical Engineering Department, (3) Research and Scientific Support Department, European Space Agency, ESTEC, Postbus 299, NL-2200AG, Noordwijk, The Netherlands (4) Mission Analysis Office, European Space Agency, ESOC, Darmstadt, Germany ABSTRACT The Solar Orbiter mission is presently in assessment phase by the Science Payload and Advanced Concepts Office of the European Space Agency. The mission is confirmed in the Cosmic Vision programme, with the objective of a launch in October 2013 and no later than May 2015. The Solar Orbiter mission incorporates both a near-Sun (~0.22 AU) and a high-latitude (~ 35 deg) phase, posing new challenges in terms of protection from the intense solar radiation and related spacecraft thermal control, to remain compatible with the programmatic constraints of a medium class mission. This paper provides an overview of the assessment study activities, with specific emphasis on the definition of the model payload and its accommodation in the spacecraft. The main results of the industrial activities conducted with Alcatel Space and EADS-Astrium are summarized. Keywords: Solar physics, space weather, instrumentation, mission assessment, Solar Orbiter 1. INTRODUCTION The Solar Orbiter mission was first discussed at the Tenerife “Crossroads” workshop in 1998, in the framework of the ESA Solar Physics Planning Group. The mission was submitted to ESA in 2000 and then selected by ESA’s Science Programme Committee in October 2000 to be implemented as a flexi-mission, with a launch envisaged in the 2008- 2013 timeframe (after the BepiColombo mission to Mercury) [1]. -
A Free Spacecraft Simulation Tool
Orbiter: AFreeSpacecraftSimulationTool MartinSchweiger DepartmentofComputerScience UniversityCollegeLondon www.orbitersim.com 2nd ESAWorkshoponAstrodynamics ToolsandTechniques ESTEC,Noordwijk 13-15September2004 Contents • Overview • Scope • Limitations • SomeOrbiterfeatures: • Timepropagation • Gravitycalculation • Rigid-bodymodelandsuperstructures • OrbiterApplicationProgrammingInterface: • Concept • Orbiterinstrumentation • TheVESSELinterfaceclass • Newfeatures: • Air-breatingengines:scramjetdesign • Virtualcockpits • Newvisualeffects • Orbiterasateachingtool • Summaryandfutureplans • Demonstration Overview · Orbiterisareal-timespaceflightsimulationforWindowsPC platforms. · Modellingofatmosphericflight(launchandreentry), suborbital,orbitalandinterplanetarymissions(rendezvous, docking,transfer,swing-byetc.) · Newtonianmechanics,rigidbodymodelofrotation,basic atmosphericflightmodel. · Planetpositionsfrompublicperturbationsolutions.Time integrationofstatevectorsorosculatingelements. · Developedsince2000asaneducationalandrecreational applicationfororbitalmechanicssimulation. · WritteninC++,usingDirectXfor3-Drendering.Public programminginterfacefordevelopmentofexternalmodule plugins. · WithanincreasinglyversatileAPI,developmentfocusis beginningtoshiftfromtheOrbitercoreto3rd partyaddons. Scope · Launchsequencefromsurfacetoorbitalinsertion(including atmosphericeffects:drag,pressure-dependentengineISP...) · Orbitalmanoeuvres(alignmentoforbitalplane,orbit-to-orbit transfers,rendezvous) · Vessel-to-vesselapproachanddocking.Buildingof superstructuresfromvesselmodules(includingsimplerules -
Stsci Newsletter: 2011 Volume 028 Issue 02
National Aeronautics and Space Administration Interacting Galaxies UGC 1810 and UGC 1813 Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) 2011 VOL 28 ISSUE 02 NEWSLETTER Space Telescope Science Institute We received a total of 1,007 proposals, after accounting for duplications Hubble Cycle 19 and withdrawals. Review process Proposal Selection Members of the international astronomical community review Hubble propos- als. Grouped in panels organized by science category, each panel has one or more “mirror” panels to enable transfer of proposals in order to avoid conflicts. In Cycle 19, the panels were divided into the categories of Planets, Stars, Stellar Rachel Somerville, [email protected], Claus Leitherer, [email protected], & Brett Populations and Interstellar Medium (ISM), Galaxies, Active Galactic Nuclei and Blacker, [email protected] the Inter-Galactic Medium (AGN/IGM), and Cosmology, for a total of 14 panels. One of these panels reviewed Regular Guest Observer, Archival, Theory, and Chronology SNAP proposals. The panel chairs also serve as members of the Time Allocation Committee hen the Cycle 19 Call for Proposals was released in December 2010, (TAC), which reviews Large and Archival Legacy proposals. In addition, there Hubble had already seen a full cycle of operation with the newly are three at-large TAC members, whose broad expertise allows them to review installed and repaired instruments calibrated and characterized. W proposals as needed, and to advise panels if the panelists feel they do not have The Advanced Camera for Surveys (ACS), Cosmic Origins Spectrograph (COS), the expertise to review a certain proposal. Fine Guidance Sensor (FGS), Space Telescope Imaging Spectrograph (STIS), and The process of selecting the panelists begins with the selection of the TAC Chair, Wide Field Camera 3 (WFC3) were all close to nominal operation and were avail- about six months prior to the proposal deadline. -
Building and Maintaining the International Space Station (ISS)
/ Building and maintaining the International Space Station (ISS) is a very complex task. An international fleet of space vehicles launches ISS components; rotates crews; provides logistical support; and replenishes propellant, items for science experi- ments, and other necessary supplies and equipment. The Space Shuttle must be used to deliver most ISS modules and major components. All of these important deliveries sustain a constant supply line that is crucial to the development and maintenance of the International Space Station. The fleet is also responsible for returning experiment results to Earth and for removing trash and waste from the ISS. Currently, transport vehicles are launched from two sites on transportation logistics Earth. In the future, the number of launch sites will increase to four or more. Future plans also include new commercial trans- ports that will take over the role of U.S. ISS logistical support. INTERNATIONAL SPACE STATION GUIDE TRANSPORTATION/LOGISTICS 39 LAUNCH VEHICLES Soyuz Proton H-II Ariane Shuttle Roscosmos JAXA ESA NASA Russia Japan Europe United States Russia Japan EuRopE u.s. soyuz sL-4 proton sL-12 H-ii ariane 5 space shuttle First launch 1957 1965 1996 1996 1981 1963 (Soyuz variant) Launch site(s) Baikonur Baikonur Tanegashima Guiana Kennedy Space Center Cosmodrome Cosmodrome Space Center Space Center Launch performance 7,150 kg 20,000 kg 16,500 kg 18,000 kg 18,600 kg payload capacity (15,750 lb) (44,000 lb) (36,400 lb) (39,700 lb) (41,000 lb) 105,000 kg (230,000 lb), orbiter only Return performance -
Orbiter Processing Facility
National Aeronautics and Space Administration Space Shuttle: Orbiter Processing From Landing To Launch he work of preparing a space shuttle for the same facilities. Inside is a description of an flight takes place primarily at the Launch orbiter processing flow; in this case, Discovery. Complex 39 Area. TThe process actually begins at the end of each acts Shuttle Landing Facility flight, with a landing at the center or, after landing At the end of its mission, the Space Shuttle f at an alternate site, the return of the orbiter atop a Discovery lands at the Shuttle Landing Facility on shuttle carrier aircraft. Kennedy’s Shuttle Landing one of two runway headings – Runway 15 extends Facility is the primary landing site. from the northwest to the southeast, and Runway There are now three orbiters in the shuttle 33 extends from the southeast to the northwest fleet: Discovery, Atlantis and Endeavour. Chal- – based on wind currents. lenger was destroyed in an accident in January After touchdown and wheelstop, the orbiter 1986. Columbia was lost during approach to land- convoy is deployed to the runway. The convoy ing in February 2003. consists of about 25 specially designed vehicles or Each orbiter is processed independently using units and a team of about 150 trained personnel, NASA some of whom assist the crew in disembarking from the orbiter. the orbiter and a “white room” is mated to the orbiter hatch. The The others quickly begin the processes necessary to “safe” the hatch is opened and a physician performs a brief preliminary orbiter and prepare it for towing to the Orbiter Processing Fa- medical examination of the crew members before they leave the cility. -
Advance Level Module 2
Ministry of Education - Guyana In collaboration with the OAS and ProFuturo FOUNDATION 2020. CARICOM. ICT Route: Advanced Level MODULE 2 – DESIGNING NETWORKED INFORMATION EXPERIENCES Training Manual for Teachers of Riverine and Hinterland Regions MINISTRY OF EDUCATION ELIMINATING LITERACY, MODERNIZING EDUCATION, STRENGTHENING TOLERANCE Message form the Minister of Education Dear Teachers Across the world, the COVID 19 pandemic (Corona Virus) continues to cause undesirable disruption to the global education systems. Guyana, as you know, was not spared. As such, we implore you to keep engaging our nation’s learners and we applaud those of you who have tried and continue to try. We heard your concerns when you told us you were uncertain about how to teach using different means, that you lacked confidence, and that you felt you were not equipped. This is our first response in partnership with the OAS and ProFuturo Foundation. This training will give you the much- needed knowledge and expose you to the tools you need to deliver education differently by being innovative and by using easily available technology. We are aware that the cost of data is of great concern to you and we have remedied that by partnering with GTT and Digicel to zero rate the ProFuturo platform domain. This means that when anyone accesses the training platform, data will not be consumed. If teachers have neither devices nor connectivity, we will arrange a suitable location and if teachers, as those in the hinterland and riverine areas, cannot access either, even with our help, we have arranged for part of the program to be done through these printed modules because we know that it is only a matter of time before you are able to access connectivity and devices. -
Nasa Game Catalog
NASA GAME CATALOG Daniel Laughlin, Ph.D. Digital Medial Learning Fellow NASA Office of Education GESTAR/MSU Last Revised June 2014 0 Executive Summary NASA has been using games for education and communication since at least 1998, yet there has never been a thorough effort to gather information about all the games together, to analyze what kind of games NASA has, what lessons have been learned, or what assets might be shared and reused. As a co- chair for the National Science and Technology Council’s Digital Game Technologies Interagency Working Group, NASA found it unable to answer questions like “how many games have you built?” or “have you created any mobile games?” None of the other twenty-four working group members could answer those questions definitively either. This catalog details the extent of NASA’s game portfolio, so that others developing new games are able to build upon the lessons learned from the past. Enclosed herein are details on fourteen individual games that have been created by or for NASA as well as two collections of hosted Flash games. Each entry has information about the game, including a screen shot, point of contact (if available), and a link to the game’s site. The games are identified by genre, NASA content or contribution, and intended audience or Entertainment Software Review Board (ESRB) rating. This catalog is a living document and will be updated over time as more games are developed or discovered. It is likely that some games have been missed. NASA is the first federal entity attempting to definitively catalog its games. -
The Hubble Legacy Fields (HLF-GOODS-S) V1.5 Data Products: Combining 2442 Orbits of GOODS-S/CDF-S Region ACS and WFC3/IR Images
!1 The Hubble Legacy Fields (HLF-GOODS-S) v1.5 Data Products: Combining 2442 Orbits of GOODS-S/CDF-S Region ACS and WFC3/IR Images. Garth Illingworth1, Daniel Magee1, Rychard Bouwens2, Pascal Oesch3, Ivo Labbe2, Pieter van Dokkum3, Katherine Whitaker4, Bradford Holden1, Marijn Franx2, and Valentino Gonzalez5 Abstract We have submitted to MAST the 1.5 version data release of the Hubble Legacy Fields (HLF) project covering a 25 x 25 arcmin area over the GOODS-S (ECDF-S) region from the HST archival program AR-13252. The release combines exposures from Hubble's two main cameras, the Advanced Camera for Surveys (ACS/WFC) and the Wide Field Camera 3 (WFC3/IR), taken over more than a decade between mid-2002 to the end of 2016. The HLF includes essentially all optical (ACS/WFC F435W, F606W, F775W, F814W and F850LP filters) and infrared (WFC3/ IR F098M, F105W, F125W, F140W and F160W filters) data taken by Hubble over the original CDF-S region including the GOODS-S, ERS, CANDELS and many other programs (31 in total). The data has been released at https://archive.stsci.edu/prepds/hlf/ as images with a common astrometric reference frame, with corresponding inverse variance weight maps. We provide one image per filter of WFC3/IR images at 60 mas per pixel resolution and two ACS/WFC images per filter, at both 30 and 60 mas per pixel. Since this comprehensive dataset combines data from 31 programs on the GOODS-S/CDF-S, the AR proposal identified the MAST products by the global name "Hubble Legacy Field”, with this region being identified by “HLF-GOODS-S”.