Space Times, Donald Beattie Raised a Number of Interesting Richard M
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Hip # 987-1088
Hip No. Consigned by Tate Farms Hip No. 987 Jess Sizzlin SI 92 987 1997 Sorrel Mare Streakin La Jolla SI 99 {Streakin Six SI 104 Mr Jess Perry SI 113 { Bottom’s Up SI 82 Scoopie Fein SI 99 {Sinn Fein SI 98 Jess Sizzlin SI 92 Legs La Scoop SI 95 3654393 Easy Jet SI 100 {Jet Deck SI 100 Sizzlin Kim SI 86 Lena’s Bar TB SI 95 (1987) { Sun Spots {Double Bid SI 100 Winsum Miss SI 95 By MR JESS PERRY SI 113 (1992). Champion 2-year-old, $687,184 [G1]. Sire of 799 ROM, 107 stakes winners, $39,619,142, incl. champions APOL- LITICAL JESS SI 107 (world champion, $1,399,831, Los Alamitos Derby [G1]), ONE FAMOUS EAGLE SI 101 ($1,387,453 [G1]). Sire of the dams of 46 stakes winners, incl. BODACIOUS DASH SI 101 ($756,495 [G1]), JES A GAME SI 111 ($323,978 [G2]), TERRIFIC SYNERGY SI 92 ($288,066 [RG2]). 1st dam SIZZLIN KIM SI 86, by Easy Jet. Placed to 3. Dam of 7 foals, 6 to race, 3 winners, including– Jess Sizzlin SI 92 (f. by Mr Jess Perry). Stakes placed winner, below. Streakin Kim (f. by Streakin La Jolla). Unplaced. Dam of– Kims Corona SI 97 (g. by Corona Cocktail). 3 wins to 4, $38,666. 2nd dam SUN SPOTS, by Double Bid. Unraced. Dam of 13 starters, 7 ROM, incl.– SUN KISSES SI 102 (f. by Game Plan). 7 wins to 3, $68,935, Shebester Derby, Mystery Derby. Dam of Exquisite Expense SI 99 ($42,264 [G3]). -
The Following Are Edited Excerpts from Two Interviews Conducted with Dr
Interviews with Dr. Wernher von Braun Editor's note: The following are edited excerpts from two interviews conducted with Dr. Wernher von Braun. Interview #1 was conducted on August 25, 1970, by Robert Sherrod while Dr. von Braun was deputy associate administrator for planning at NASA Headquarters. Interview #2 was conducted on November 17, 1971, by Roger Bilstein and John Beltz. These interviews are among those published in Before This Decade is Out: Personal Reflections on the Apollo Program, (SP-4223, 1999) edited by Glen E. Swanson, whick is vailable on-line at http://history.nasa.gov/SP-4223/sp4223.htm on the Web. Interview #1 In the Apollo Spacecraft Chronology, you are quoted as saying "It is true that for a long time we were not in favor of lunar orbit rendezvous. We favored Earth orbit rendezvous." Well, actually even that is not quite correct, because at the outset we just didn't know which route [for Apollo to travel to the Moon] was the most promising. We made an agreement with Houston that we at Marshall would concentrate on the study of Earth orbit rendezvous, but that did not mean we wanted to sell it as our preferred scheme. We weren't ready to vote for it yet; our study was meant to merely identify the problems involved. The agreement also said that Houston would concentrate on studying the lunar rendezvous mode. Only after both groups had done their homework would we compare notes. This agreement was based on common sense. You don't start selling your scheme until you are convinced that it is superior. -
Apollo 13 Mission Review
APOLLO 13 MISSION REVIEW HEAR& BEFORE THE COMMITTEE ON AERONAUTICAL AND SPACE SCIENCES UNITED STATES SENATE NINETY-FIRST CONGRESS SECOR’D SESSION JUR’E 30, 1970 Printed for the use of the Committee on Aeronautical and Space Sciences U.S. GOVERNMENT PRINTING OFFICE 47476 0 WASHINGTON : 1970 COMMITTEE ON AEROKAUTICAL AND SPACE SCIENCES CLINTON P. ANDERSON, New Mexico, Chairman RICHARD B. RUSSELL, Georgia MARGARET CHASE SMITH, Maine WARREN G. MAGNUSON, Washington CARL T. CURTIS, Nebraska STUART SYMINGTON, bfissouri MARK 0. HATFIELD, Oregon JOHN STENNIS, Mississippi BARRY GOLDWATER, Arizona STEPHEN M.YOUNG, Ohio WILLIAM B. SAXBE, Ohio THOJfAS J. DODD, Connecticut RALPH T. SMITH, Illinois HOWARD W. CANNON, Nevada SPESSARD L. HOLLAND, Florida J4MES J. GEHRIG,Stad Director EVERARDH. SMITH, Jr., Professional staffMember Dr. GLENP. WILSOS,Professional #tad Member CRAIGVOORHEES, Professional Staff Nember WILLIAMPARKER, Professional Staff Member SAMBOUCHARD, Assistant Chief Clerk DONALDH. BRESNAS,Research Assistant (11) CONTENTS Tuesday, June 30, 1970 : Page Opening statement by the chairman, Senator Clinton P. Anderson-__- 1 Review Board Findings, Determinations and Recommendations-----_ 2 Testimony of- Dr. Thomas 0. Paine, Administrator of NASA, accompanied by Edgar M. Cortright, Director, Langley Research Center and Chairman of the dpollo 13 Review Board ; Dr. Charles D. Har- rington, Chairman, Aerospace Safety Advisory Panel ; Dr. Dale D. Myers, Associate Administrator for Manned Space Flight, and Dr. Rocco A. Petrone, hpollo Director -___________ 21, 30 Edgar 11. Cortright, Chairman, hpollo 13 Review Board-------- 21,27 Dr. Dale D. Mvers. Associate Administrator for Manned SDace 68 69 105 109 LIST OF ILLUSTRATIOSS 1. Internal coinponents of oxygen tank So. 2 ---_____-_________________ 22 2. -
VIRVĖ SAVO KARTUVĖMS Kapitalistų Sandėriai Su Komunistais Vytautas Meškauskas
T e oc. oi' 5 □ TL i r. s t r c ba š' 7243 So» Albanv fk., ' yi Chiccęp, III, ‘ 304.29 ; I0TEKA Į -----THE LITHUANIAN NATIONAL NEVVSPAPER -------- P.O. BOX 03206 > 6116 ST. CLAIR AVENUE > CLEVELAND, OHIO 44103 Vol.LXIV Balandis - April 19, 1979 Nr.16 *< TAUTINES MINTIES LIETUVIŲ LAIKRAŠTIS VIRVĖ SAVO KARTUVĖMS Kapitalistų sandėriai su komunistais Vytautas Meškauskas Turiu pasakyti, kad Leninas išpranašavo visą proce Konkrečiai kalbant, pereitų są. Leninas, kuris didesnę savo gyvenimo dalį praleido metų prekybos su sovietais Vakaruose, bet ne Rusijoje, kuris geriau pažinojo Vaka apyvarta siekė tik 2.8 biijonus rus kaip Rusiją, visados rašė ir sakė, jog Vakarų kapi dolerių, t.y. tik trečdalį pre talistai padarys viską, kad sustiprintų SSSR ekonomiją. kybos su ... Taiwanu. Biznie Jie konkuruos savo tarpe, kad mums parduoti gerybes rius tačiau vilioja ne tiek da pigiau ir greičiau, tik tam, kad sovietai jas pirktų ne iš bartinės, kiek ateities galimy bės. Šiaip ar taip, Sovietiją vieno, bet iš kito. Jis sakė: jie taip darys negalvodami sudaro rinką su 250 milijonų apie savo pačių ateitį. Vienu sunkiu momentu partijos gyventojų. posėdyje Maskvoje jis drąsino: "Draugai, nepasiduokit Nepaisant to, kad bolševi panikai, jei mums pasidarys labai sunku, mes duosime kai konfiskavo visus užsienie virvę buržuazijai, ir buržuazija pati pasikars." čių kapitalus, buvusius caro Tada, Kari Radek,... kuris buvo labai sąmojingas, Rusijoje - vien Singerio kom paklausė: Vladimire Iličiau, bet iš kur mes paimsime tiek panija prieš karą ten turėjo daug virvės buržuazijos pasikorimui?” Leninas nerūpes 27,000 tarnautojų. Vakarų tingai atsakė: "Jie mus ja aprūpins." kapitalistai padėjo sovietų (Iš Aleksandro Solženicyno 1975 m. -
Apollo Over the Moon: a View from Orbit (Nasa Sp-362)
chl APOLLO OVER THE MOON: A VIEW FROM ORBIT (NASA SP-362) Chapter 1 - Introduction Harold Masursky, Farouk El-Baz, Frederick J. Doyle, and Leon J. Kosofsky [For a high resolution picture- click here] Objectives [1] Photography of the lunar surface was considered an important goal of the Apollo program by the National Aeronautics and Space Administration. The important objectives of Apollo photography were (1) to gather data pertaining to the topography and specific landmarks along the approach paths to the early Apollo landing sites; (2) to obtain high-resolution photographs of the landing sites and surrounding areas to plan lunar surface exploration, and to provide a basis for extrapolating the concentrated observations at the landing sites to nearby areas; and (3) to obtain photographs suitable for regional studies of the lunar geologic environment and the processes that act upon it. Through study of the photographs and all other arrays of information gathered by the Apollo and earlier lunar programs, we may develop an understanding of the evolution of the lunar crust. In this introductory chapter we describe how the Apollo photographic systems were selected and used; how the photographic mission plans were formulated and conducted; how part of the great mass of data is being analyzed and published; and, finally, we describe some of the scientific results. Historically most lunar atlases have used photointerpretive techniques to discuss the possible origins of the Moon's crust and its surface features. The ideas presented in this volume also rely on photointerpretation. However, many ideas are substantiated or expanded by information obtained from the huge arrays of supporting data gathered by Earth-based and orbital sensors, from experiments deployed on the lunar surface, and from studies made of the returned samples. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Executive Summary
c -- . b * NASAICR- AFFORDABLE IN-SPACE TRANSPORTATION PHASE II 0 ANADVANCED CONCEPTS PROJECT October 16-17,1996 Technical Interchange Meeting EXECUTIVE SUMMARY Office of Space Access and Technology, NASA Headquarters Advanced Concepts Office, NASA Marshall Space Flight Center National Aeronautics and Space Administration 0 University of Alabama in Huntsville 5-25620 AFFORDABLE IN-SPACE TRANSPORTATION TECHNICAL INTERCHANGE MEETING SECTION 1 1.0 Introduction The Affordable In-Space Transportation (AIST) program was established by the NASA Office of Space Access to improve transportation and lower the costs from Low Earth Orbit (LEO) to Geostationary Earth Orbit (GEO) and beyond (to Lunar orbit, Mars orbit, inner solar system missions, and return to LEO). A goal was established to identify and develop radically innovative concepts for new upper stages for Reusable Launch Vehicles (RLV) and Highly Reusable Space Transportation (HRST) systems. New architectures and technologies are being identified which have the potential to meet a cost goal of $1,000 to $2,000 per pound for transportation to GEO and beyond for overall mission cost (including the cost to LEO). A Technical Interchange Meeting (TIM) was held on October 16 and 17, 1996 in Huntsville, Alabama to review previous studies, present advanced concepts and review technologies that could be used to meet the stated goals. The TIM was managed by NASA-Marshall Space Flight Center (MSFC) Advanced Concepts Office with Mr. Alan Adams providing TIM coordination. Mr. John C. Mankins of NASA Headquarters provided overall sponsorship. The University of Alabama in Huntsville (UAH) Propulsion Research Center hosted the TIM at the UAH Research Center. -
Challenger Accident in a Rogers Commission Hearing at KSC
CHALLENGER By Arnold D. Aldrich Former Program Director, NSTS August 27, 2008 Recently, I was asked by John Shannon, the current Space Shuttle Program Manager, to comment on my experiences, best practices, and lessons learned as a former Space Shuttle program manager. This project is part of a broader knowledge capture and retention initiative being conducted by the NASA Johnson Space Center in an “oral history” format. One of the questions posed was to comment on some of the most memorable moments of my time as a Space Shuttle program manager. Without question, the top two of these were the launch of Challenger on STS‐51L on January 28, 1986, and the launch of Discovery on STS‐26 on September 29, 1988. Background The tragic launch and loss of Challenger occurred over 22 years ago. 73 seconds into flight the right hand Solid Rocket Booster (SRB) broke away from the External Tank (ET) as a result of a burn‐ through in its aft most case to case joint and the Space Shuttle vehicle disintegrated resulting in the total loss of the vehicle and crew. The events leading up to that launch are still vivid in my mind and deeply trouble me to this day, as I know they always will. This paper is not about what occurred during the countdown leading up to the launch – those facts and events were thoroughly investigated and documented by the Rogers Commission. Rather, what I can never come to closure with is how we, as a launch team, and I, as one of the leaders of that team, allowed the launch to occur. -
Nasa Johnson Space Center Oral History Project Oral History Transcript
NASA JOHNSON SPACE CENTER ORAL HISTORY PROJECT ORAL HISTORY TRANSCRIPT FAROUK EL-BAZ INTERVIEWED BY REBECCA WRIGHT BOSTON, MASSACHUSETTS – NOVEMBER 2, 2009 WRIGHT: Today is November 2, 2009. This oral history interview is being conducted with Dr. Farouk El-Baz in Boston, Massachusetts, for the Johnson Space Center Oral History Project. Interviewer is Rebecca Wright, assisted by Jennifer Ross-Nazzal. We certainly would like to start by telling you thank you. We know you‘re a very busy person with a very busy schedule, so thank you for finding time for us today. EL-BAZ: You‘re welcome to come here, because this is part of the history of the United States. It‘s important that we all chip in. WRIGHT: We‘re glad to hear that. We know your work with NASA began as early as 1967 when you became employed by Bellcomm [Incorporated]. Could you share with us how you learned about that opportunity and how you made that transition into becoming an employee there? EL-BAZ: Just the backdrop, I finished my PhD here in the US. First job offer was from Germany. It was in June 1964; I was teaching there [at the University of Heidelberg] until December 1965. I went to Egypt then, tried to get a job in geology. I was unable for a whole year, so I came back to the US as an immigrant in the end of 1966. For the first three months of 1967, I began to search for a job. When I arrived in the winter, most of the people that I knew 2 November 2009 1 Johnson Space Center Oral History Project Farouk El-Baz were at universities, and most universities had hired the people that would teach during the year. -
Killer Corsairs How the Navy Got Them in Line
JAY LENO’S STASH OF AIRPLANE ENGINES JULY 2021 Vought F4U Corsair KILLER CORSAIRS HOW THE NAVY GOT THEM IN LINE Asteroid Threat A Preemptive Strike p.34 AIRSPACEMAG.COM APOLLO 15 ● AT 50 FIRST CARON THE MOON CREDIT 48 AIR & SPACE airspacemag.com BEFORE APOLLO15, ASTRONAUTS COULD EXPLORE ONLY AS FAR AS THEY COULD WALK. ■ BY EARL SWIFT WHEN APOLLO 14 landed astronauts on the moon for the third time in February 1971, it was met with a week-long yawn by the press and the public. The TV networks carried live coverage of the launch and paid some mind to the long translunar coast, where misfortune had called on Apollo 13, but offered only occasional snippets of Alan Shepard and Ed Mitchell’s time on the lunar surface. News from Fra Mauro was dutifully passed along by the country’s newspapers, but with palpable lack of enthusiasm. America had grown jaded about moon missions, it seemed. But fact was, the second and third lunar landings made for lousy TV. To viewers, they looked pretty much the same as Apollo 11: The astronauts were on foot. The TV camera was stationary and positioned near the lun175 Excerpted and condensed ar module. Its low-resolution footage captured the crew from Across the Airless Wilds: The Lunar Rover and bouncing around base camp, doing nothing especially stir- the Triumph of the Final ring. In fact, Apollo 14’s single made-for-TV moment is Moon Landings, by Earl the only thing many older Americans remember about it: Swift. HarperCollins, 2021. Alan Shepard’s golf shot that went for “miles and miles” in the weak lunar gravity. -
Cambridge University Press 978-1-107-03629-1 — the Atlas of Mars Kenneth S
Cambridge University Press 978-1-107-03629-1 — The Atlas of Mars Kenneth S. Coles, Kenneth L. Tanaka, Philip R. Christensen Index More Information Index Note: page numbers in italic indicates figures or tables Acheron Fossae 76, 76–77 cuesta 167, 169 Hadriacus Cavi 183 orbit 1 Acidalia Mensa 86, 87 Curiosity 9, 32, 62, 195 Hadriacus Palus 183, 184–185 surface gravity 1, 13 aeolian, See wind; dunes Cyane Catena 82 Hecates Tholus 102, 103 Mars 3 spacecraft 6, 201–202 Aeolis Dorsa 197 Hellas 30, 30, 53 Mars Atmosphere and Volatile Evolution (MAVEN) 9 Aeolis Mons, See Mount Sharp Dao Vallis 227 Hellas Montes 225 Mars Chart 1 Alba Mons 80, 81 datum (zero elevation) 2 Hellas Planitia 220, 220, 226, 227 Mars Exploration Rovers (MER), See Spirit, Opportunity albedo 4, 5,6,10, 56, 139 deformation 220, See also contraction, extension, faults, hematite 61, 130, 173 Mars Express 9 alluvial deposits 62, 195, 197, See also fluvial deposits grabens spherules 61,61 Mars Global Surveyor (MGS) 9 Amazonian Period, history of 50–51, 59 Deimos 62, 246, 246 Henry crater 135, 135 Mars Odyssey (MO) 9 Amenthes Planum 143, 143 deltas 174, 175, 195 Herschel crater 188, 189 Mars Orbiter Mission (MOM) 9 Apollinaris Mons 195, 195 dikes, igneous 82, 105, 155 Hesperia Planum 188–189 Mars Pathfinder 9, 31, 36, 60,60 Aram Chaos 130, 131 domical mound 135, 182, 195 Hesperian Period, history of 50, 188 Mars Reconnaissance Orbiter (MRO) 9 Ares Vallis 129, 130 Dorsa Argentea 239, 240 Huygens crater 183, 185 massif 182, 224 Argyre Planitia 213 dunes 56, 57,69–70, 71, 168, 185, -
Leading Msl to Water: Paleolacustrine Landing Sites Redux
LEADING MSL TO WATER: PALEOLACUSTRINE LANDING SITES REDUX. J.W. Rice, Jr., Mars Space Flight Facility, Department of Geosciences, Arizona StateUniversity, Tempe, AZ 85287, [email protected] Introduction: The highest priority landing site tered bedrock outcrops. This is consistent with a for achieving the scientific objectives (assessment lacustrine setting. of local region for habitat potential for past or present life) of the Mars Science Laboratory will Holden Crater be a paleolacustrine basin containing accessible Location: 26.1.S,326E layered sediments. Ideally, this type of landing Diameter: 154 km site would be selected from both morphologic and Elevation: –2.200km mineralogic evidence. The MER Project had the Thermal Inertia: 320-470 SI units luxury of selecting two landing sites. One site Geology: Uzboi Vallis cuts the SW rim of based on mineralogy (Meridiani Planum) and one Holden. The southern floor of Holden contains on morphology (Gusev Crater). To date the Me- laterally continuous layered sediments, distribu- ridiani site has proven to be the wettest. The mor- tary fan (225km2), inverted channels and mean- phologic approach was unsuccessfully attempted dering channels. Medium thermal inertia repre- with the Gusev Crater site. However, it should be sents a combination of coarser loose particles, mentioned that some of us (voices in the wilder- crusted fines, a fair number of scattered rocks, ness) argued that the morphologic and geologic and/or perhaps a few scattered bedrock outcrops. evidence in Gusev Crater was much more com- This is consistent with a lacustrine setting. plicated and that the commonly accepted lacus- trine story was flawed. MSL will only get one Palos Crater chance.