Nasa Johnson Space Center Oral History Project
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
Modeling and Adjustment of THEMIS IR Line Scanner Camera Image Measurements
Modeling and Adjustment of THEMIS IR Line Scanner Camera Image Measurements by Brent Archinal USGS Astrogeology Team 2255 N. Gemini Drive Flagstaff, AZ 86001 [email protected] As of 2004 December 9 Version 1.0 Table of Contents 1. Introduction 1.1. General 1.2. Conventions 2. Observations Equations and Their Partials 2.1. Line Scanner Camera Specific Modeling 2.2. Partials for New Parameters 2.2.1. Orientation Partials 2.2.2. Spatial Partials 2.2.3. Partials of the observations with respect to the parameters 2.2.4. Parameter Weighting 3. Adjustment Model 4. Implementation 4.1. Input/Output Changes 4.1.1. Image Measurements 4.1.2. SPICE Data 4.1.3. Program Control (Parameters) Information 4.2. Computational Changes 4.2.1. Generation of A priori Information 4.2.2. Partial derivatives 4.2.3. Solution Output 5. Testing and Near Term Work 6. Future Work Acknowledgements References Useful web sites Appendix I - Partial Transcription of Colvin (1992) Documentation Appendix II - HiRISE Sensor Model Information 1. Introduction 1.1 General The overall problem we’re solving is that we want to be able to set up the relationships between the coordinates of arbitrary physical points in space (e.g. ground points) and their coordinates on line scanner (or “pushbroom”) camera images. We then want to do a least squares solution in order to come up with consistent camera orientation and position information that represents these relationships accurately. For now, supported by funding from the NASA Critical Data Products initiative (for 2003 September to 2005 August), we will concentrate on handling the THEMIS IR camera system (Christensen et al., 2003). -
NITROGEN on MARS: INSIGHTS from CURIOSITY. J. C. Stern1 , B. Sutter2, W. A. Jackson3, Rafael Na- Varro-González4, Christopher P
Lunar and Planetary Science XLVIII (2017) 2726.pdf 1 2 3 NITROGEN ON MARS: INSIGHTS FROM CURIOSITY. J. C. Stern , B. Sutter , W. A. Jackson , Rafael Na- varro-González4, Christopher P. McKay5, Douglas W. Ming6, P. Douglas Archer2, D. P. Glavin1, A. G. Fairen7,8 and Paul R. Mahaffy1. 1NASA GSFC, Code 699, Greenbelt, MD 20771, [email protected], 2Jacobs, NASA Johnson Space Center, Houston, TX 77058, 3Texas Tech University, Lubbock, TX 79409, 4Universidad Nacional Autónoma de México, México, D.F. 04510, Mexico, 5NASA Ames Research Center, Moffett Field, CA 94035, 6NASA Johnson Space Center, Houston TX 77058, 7Centro de Astrobiologia, Madrid, Spain, 8Cornell University, Ithaca, NY 14853 Introduction: Recent detection of nitrate on Mars [1] indicates that nitrogen fixation processes occurred in early martian history. Data collected by the Sample Analysis at Mars (SAM) instrument on the Curiosity Rover can be integrated with Mars analog work in order to better understand the fixation and mobility of nitrogen on Mars, and thus its availability to putative biology. In particular, the relationship between nitrate and other soluble salts may help reveal the timing of nitrogen fixation and post-depositional behavior of nitrate on Mars. In addition, in situ measurements of nitrogen abundance and isotopic composition may be used to model atmospheric conditions on early Mars. Methods: The data presented are from analyses of solid Martian drilled and scooped samples by the Sam- ple Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) Curiosity Rover. SAM performs evolved gas analysis (EGA), in which a 3 Figure 1. -
The Economic Impact of Physics Research in the UK: Satellite Navigation Case Study
The economic impact of physics research in the UK: Satellite Navigation Case Study A report for STFC November 2012 Contents Executive Summary................................................................................... 3 1 The science behind satellite navigation......................................... 4 1.1 Introduction ................................................................................................ 4 1.2 The science................................................................................................ 4 1.3 STFC’s role in satellite navigation.............................................................. 6 1.4 Conclusions................................................................................................ 8 2 Economic impact of satellite navigation ........................................ 9 2.1 Introduction ................................................................................................ 9 2.2 Summary impact of GPS ........................................................................... 9 2.3 The need for Galileo................................................................................. 10 2.4 Definition of the satellite navigation industry............................................ 10 2.5 Methodological approach......................................................................... 11 2.6 Upstream direct impacts .......................................................................... 12 2.7 Downstream direct impacts..................................................................... -
Exploration of the Moon
Exploration of the Moon The physical exploration of the Moon began when Luna 2, a space probe launched by the Soviet Union, made an impact on the surface of the Moon on September 14, 1959. Prior to that the only available means of exploration had been observation from Earth. The invention of the optical telescope brought about the first leap in the quality of lunar observations. Galileo Galilei is generally credited as the first person to use a telescope for astronomical purposes; having made his own telescope in 1609, the mountains and craters on the lunar surface were among his first observations using it. NASA's Apollo program was the first, and to date only, mission to successfully land humans on the Moon, which it did six times. The first landing took place in 1969, when astronauts placed scientific instruments and returnedlunar samples to Earth. Apollo 12 Lunar Module Intrepid prepares to descend towards the surface of the Moon. NASA photo. Contents Early history Space race Recent exploration Plans Past and future lunar missions See also References External links Early history The ancient Greek philosopher Anaxagoras (d. 428 BC) reasoned that the Sun and Moon were both giant spherical rocks, and that the latter reflected the light of the former. His non-religious view of the heavens was one cause for his imprisonment and eventual exile.[1] In his little book On the Face in the Moon's Orb, Plutarch suggested that the Moon had deep recesses in which the light of the Sun did not reach and that the spots are nothing but the shadows of rivers or deep chasms. -
Non-Collider Searches for Stable Massive Particles
Non-collider searches for stable massive particles S. Burdina, M. Fairbairnb, P. Mermodc,, D. Milsteadd, J. Pinfolde, T. Sloanf, W. Taylorg aDepartment of Physics, University of Liverpool, Liverpool L69 7ZE, UK bDepartment of Physics, King's College London, London WC2R 2LS, UK cParticle Physics department, University of Geneva, 1211 Geneva 4, Switzerland dDepartment of Physics, Stockholm University, 106 91 Stockholm, Sweden ePhysics Department, University of Alberta, Edmonton, Alberta, Canada T6G 0V1 fDepartment of Physics, Lancaster University, Lancaster LA1 4YB, UK gDepartment of Physics and Astronomy, York University, Toronto, ON, Canada M3J 1P3 Abstract The theoretical motivation for exotic stable massive particles (SMPs) and the results of SMP searches at non-collider facilities are reviewed. SMPs are defined such that they would be suffi- ciently long-lived so as to still exist in the cosmos either as Big Bang relics or secondary collision products, and sufficiently massive such that they are typically beyond the reach of any conceiv- able accelerator-based experiment. The discovery of SMPs would address a number of important questions in modern physics, such as the origin and composition of dark matter and the unifi- cation of the fundamental forces. This review outlines the scenarios predicting SMPs and the techniques used at non-collider experiments to look for SMPs in cosmic rays and bound in mat- ter. The limits so far obtained on the fluxes and matter densities of SMPs which possess various detection-relevant properties such as electric and magnetic charge are given. Contents 1 Introduction 4 2 Theory and cosmology of various kinds of SMPs 4 2.1 New particle states (elementary or composite) . -
Perchlorate and Chlorate Biogeochemistry in Ice-Covered Lakes of the Mcmurdo Dry Valleys, Antarctica
Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 98 (2012) 19–30 www.elsevier.com/locate/gca Perchlorate and chlorate biogeochemistry in ice-covered lakes of the McMurdo Dry Valleys, Antarctica W. Andrew Jackson a,⇑, Alfonso F. Davila b,c, Nubia Estrada a, W. Berry Lyons d, John D. Coates e, John C. Priscu f a Department of Civil and Environmental Engineering, Texas Tech University, Lubbock, TX 79409, USA b NASA Ames Research Center, Moffett Field, CA 95136, USA c SETI Institute, 189 Bernardo Ave., Suite 100, Mountain View, CA 94043-5203, USA d Byrd Polar Research Center, The Ohio State University, Columbus, OH 43210, USA e Department of Plant and Microbial Biology, University of California, Berkeley, CA 94720, USA f Department of Land Resources & Environmental Sciences, Montana State University, Bozeman, MT 59717, USA Received 15 February 2012; accepted in revised form 5 September 2012; available online 19 September 2012 Abstract À À We measured chlorate (ClO3 ) and perchlorate (ClO4 ) concentrations in ice covered lakes of the McMurdo Dry Valleys À À (MDVs) of Antarctica, to evaluate their role in the ecology and geochemical evolution of the lakes. ClO3 and ClO4 are À À present throughout the MDV Lakes, streams, and other surface water bodies. ClO3 and ClO4 originate in the atmosphere and are transported to the lakes by surface inflow of glacier melt that has been differentially impacted by interaction with soils À À and aeolian matter. Concentrations of ClO3 and ClO4 in the lakes and between lakes vary based on both total evaporative concentration, as well as biological activity within each lake. -
Highlights in Space 2010
International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren UNITED NATIONS 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France Tel: +33 1 45 67 42 60 Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 E-mail: : [email protected] E-mail: [email protected] Fax. + 33 1 44 76 74 37 URL: www.iislweb.com OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL : http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 *1180239* V.11-80239—January 2011—775 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no. -
NO ONE KNOWS ABOUT US by Bridget Canning. a Creative Writing
NO ONE KNOWS ABOUT US By Bridget Canning. A Creative Writing Thesis submitted to the School of Graduate Studies in partial fulfillment of the requirements for the degree of Masters of Arts in English (Creative Writing) Department of English, Memorial University of Newfoundland Abstract: No One Knows about Us is a collection of twelve contemporary short stories. As the title suggests, the characters in each story deal with secrets: relationships, longings, grudges, addictions, and trickery. For them, these secrets are simultaneously overwhelming and futile; their importance within their small worlds reflect a deeper feeling of insignificance in the greater scheme of life in a small city in a northern province hemmed on to the side of a continent. Here are a range of characters and situations set in St. John’s, Newfoundland and Labrador. The stories are mapped out in different areas of the city and move chronologically over a year, starting in fall and ending in late summer. They work together to create a small sample of life in modern-day St. John’s – one that is informed by the influences of history, economy, and weather. i Acknowledgements: This thesis would not have been accomplished without the help of the English department faculty at Memorial such as Robert Finley, Robert Chafe, and especially my thesis advisor, Lisa Moore. Thanks to the Graduate Society for their financial support. Thanks to Jonathan Weir, Deirdre Snook, and the members of the Naked Parade Writing Collective for their guidance and encouragement. ii Contents: 1. Seen, p. 1 2. With Glowing Hearts, p. 19 3. -
ALBERT VAN HELDEN + HUYGENS’S RING CASSINI’S DIVISION O & O SATURN’S CHILDREN
_ ALBERT VAN HELDEN + HUYGENS’S RING CASSINI’S DIVISION o & o SATURN’S CHILDREN )0g-_ DIBNER LIBRARY LECTURE , HUYGENS’S RING, CASSINI’S DIVISION & SATURN’S CHILDREN c !@ _+++++++++ l ++++++++++ _) _) _) _) _)HUYGENS’S RING, _)CASSINI’S DIVISION _) _)& _)SATURN’S CHILDREN _) _) _)DDDDD _) _) _)Albert van Helden _) _) _) , _) _) _)_ _) _) _) _) _) · _) _) _) ; {(((((((((QW(((((((((} , 20013–7012 Text Copyright ©2006 Albert van Helden. All rights reserved. A H is Professor Emeritus at Rice University and the Univer- HUYGENS’S RING, CASSINI’S DIVISION sity of Utrecht, Netherlands, where he resides and teaches on a regular basis. He received his B.S and M.S. from Stevens Institute of Technology, M.A. from the AND SATURN’S CHILDREN University of Michigan and Ph.D. from Imperial College, University of London. Van Helden is a renowned author who has published respected books and arti- cles about the history of science, including the translation of Galileo’s “Sidereus Nuncius” into English. He has numerous periodical contributions to his credit and has served on the editorial boards of Air and Space, 1990-present; Journal for the History of Astronomy, 1988-present; Isis, 1989–1994; and Tractrix, 1989–1995. During his tenure at Rice University (1970–2001), van Helden was instrumental in establishing the “Galileo Project,”a Web-based source of information on the life and work of Galileo Galilei and the science of his time. A native of the Netherlands, Professor van Helden returned to his homeland in 2001 to join the faculty of Utrecht University. -
In Pdf Format
lós 1877 Mik 88 ge N 18 e N i h 80° 80° 80° ll T 80° re ly a o ndae ma p k Pl m os U has ia n anum Boreu bal e C h o A al m re u c K e o re S O a B Bo l y m p i a U n d Planum Es co e ria a l H y n d s p e U 60° e 60° 60° r b o r e a e 60° l l o C MARS · Korolev a i PHOTOMAP d n a c S Lomono a sov i T a t n M 1:320 000 000 i t V s a Per V s n a s l i l epe a s l i t i t a s B o r e a R u 1 cm = 320 km lkin t i t a s B o r e a a A a A l v s l i F e c b a P u o ss i North a s North s Fo d V s a a F s i e i c a a t ssa l vi o l eo Fo i p l ko R e e r e a o an u s a p t il b s em Stokes M ic s T M T P l Kunowski U 40° on a a 40° 40° a n T 40° e n i O Va a t i a LY VI 19 ll ic KI 76 es a As N M curi N G– ra ras- s Planum Acidalia Colles ier 2 + te . -
Glossary Nov 08
NAVIGATION ACRONYMS, ABBREVIATIONS AND DEFINITIONS Collected by David Broughton These may be reproduced freely, but please inform the Royal Institute of Navigation of any amendments or additions via e-mail ([email protected]) or fax (+44 20 7591 3131). ‘ minute (= 1º/60) 112 European emergency phone number (= 911 in US, 999 in UK) 1st4sport Awarding body of the NCF Qualifications 2-AFC two-alternative forced-choice (procedure used in animal studies) 2dRMS twice distance root-mean-square Twice the root-mean-square of the radial distances from the true position to the observed positions obtained from a number of trials. Should contain 95% of observed positions. 2SOPS 2nd Space Operations Sqn (of 50th Space Wing)(USAF) Exercise command and control of GPS satellite constellation. 3DNC Three-dimensional digital navigational chart 3G third generation (of mobile phone technology or telematics) There is also 2G, 2.5G and 4G for phones. 3GPP 3G Partnership Project 3GT 3rd Generation Telematics (ERTICO and OSGi project) 802.11 a wireless interconnection standard with a range of 50 metres Also known as WiFi. An IEEE standard. 911 US emergency phone number (= 112 in Europe, 999 in UK) a atto (SI unit multiplier of 10-18) a semi-major axis of ellipse (for WGS-84 = 6,378,137 m) A-band NATO radar band 0-250 MHz = > 1.2 m A-GNSS (AGNSS) Assisted GNSS A-GPS (AGPS) Assisted GPS A-NPA Advance Notice of Proposed Amendment (EU JAA) A-NPRM Advance Notice of Proposed Rulemaking (FAA, FCC etc) A-S anti-spoofing In GPS the use of encryption to prevent a P-Code receiver locking to a bogus P-Code transmission.