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Soyuz TMA-11 / Expedition 16 Manuel De La Mission
Soyuz TMA-11 / Expedition 16 Manuel de la mission SOYUZ TMA-11 – EXPEDITION 16 Par Philippe VOLVERT SOMMAIRE I. Présentation des équipages II. Présentation de la mission III. Présentation du vaisseau Soyuz IV. Précédents équipages de l’ISS V. Chronologie de lancement VI. Procédures d’amarrage VII. Procédures de retour VIII. Horaires IX. Sources A noter que toutes les heures présentes dans ce dossier sont en heure GMT. I. PRESENTATION DES EQUIPAGES Equipage Expedition 15 Fyodor YURCHIKHIN (commandant ISS) Lieu et Lieu et date de naissance : 03/01/1959 ; Batumi (Géorgie) Statut familial : Marié et 2 enfants Etudes : Graduat d’économie à la Moscow Service State University Statut professionnel: Ingénieur et travaille depuis 1993 chez RKKE Roskosmos : Sélectionné le 28/07/1997 (RKKE-13) Précédents vols : STS-112 (07/10/2002 au 18/10/2002), totalisant 10 jours 19h58 Oleg KOTOV(ingénieur de bord) Lieu et date de naissance : 27/10/1965 ; Simferopol (Ukraine) Statut familial : Marié et 2 enfants Etudes : Doctorat en médecine obtenu à la Sergei M. Kirov Military Medicine Academy Statut professionnel: Colonel, Russian Air Force et travaille au centre d’entraînement des cosmonautes, le TsPK Roskosmos : Sélectionné le 09/02/1996 (RKKE-12) Précédents vols : - Clayton Conrad ANDERSON (Ingénieur de vol ISS) Lieu et date de naissance : 23/02/1959 ; Omaha (Nebraska) Statut familial : Marié et 2 enfants Etudes : Promu bachelier en physique à Hastings College, maîtrise en ingénierie aérospatiale à la Iowa State University Statut professionnel: Directeur du centre des opérations de secours à la Nasa Nasa : Sélectionné le 04/06/1998 (Groupe) Précédents vols : - Equipage Expedition 16 / Soyuz TM-11 Peggy A. -
Lift Off to the International Space Station with Noggin!
Lift Off to the International Space Station with Noggin! Activity Guide for Parents and Caregivers Developed in collaboration with NASA Learn About Earth Science Ask an Astronaut! Astronaut Shannon Children from across the country had a Walker unique opportunity to talk with astronauts aboard the International Space Station (ISS)! NASA (National Aeronautics and Space Administration) astronaut Shannon Astronaut Walker and JAXA (Japan Aerospace Soichi Noguchi Exploration Agency) astronaut Soichi Noguchi had all of the answers! View NASA/Noggin Downlink and then try some out-of-this- world activities with your child! Why is it important to learn about Space? ● Children are naturally curious about space and want to explore it! ● Space makes it easy and fun to learn STEM (Science, Technology, Engineering, and Math). ● Space inspires creativity, critical thinking and problem solving skills. Here is some helpful information to share with your child before you watch Ask an Astronaut! What is the International Space Station? The International Space Station (ISS) is a large spacecraft that orbits around Earth, approximately 250 miles up. Astronauts live and work there! The ISS brings together astronauts from different countries; they use it as a science lab to explore space. Learn Space Words! Astronauts Earth An astronaut is someone who is Earth is the only planet that people have trained to go into space and learn lived on. The Earth rotates - when it is day more about it. They have to wear here and our part of the Earth faces the special suits to help them breathe. Sun, it is night on the other side of the They get to space in a rocket. -
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. -
Expedition 11, Space Tourist Back on Earth 11 October 2005
Expedition 11, Space Tourist Back on Earth 11 October 2005 The Soyuz TMA spacecraft undocked from the station at 5:49 p.m. EDT. Its re-entry was flawless. It brought the three men aboard to a landing about 53 miles northeast of Arkalyk after 179 days and 23 minutes in space for the E11 crew. The recovery team reached the capsule in minutes. Krikalev and Phillips will spend several weeks in Star City, near Moscow, for debriefing and medical examinations. They launched from the Baikonur Cosmodrome in Kazakhstan last April 14. During their increment they performed a spacewalk, continued station maintenance and did scientific experiments. While aboard the station, Krikalev became the world's most experienced spacefarer. On Aug. 16 The Expedition 11 landed back on Earth Monday his cumulative time in space passed the record of at 9:09 p.m. EDT after undocking from the 747 days, 14 hours and 14 minutes set by international space station at 5:49 p.m. EDT. Cosmonaut Sergei Avdeyev. Krikalev previously Commander Sergei Krikalev, Flight Engineer John had completed two long-duration spaceflights Phillips and Spaceflight Participant US millionaire aboard the Mir space station, served as a member businessman Greg Olsen boarded a Soyuz TMA-6 of the Expedition 1 crew of the space station and Monday afternoon for re-entry in Kazakhstan. flown two space shuttle missions. The station's new crewmembers arrived at the By Monday's landing, Krikalev's cumulative time in station on Oct. 3. Expedition 12 Commander Bill space had reached 803 days and 9 hours and 39 McArthur and Flight Engineer Valery Tokarev will minutes. -
Parent Memo-26 |
Dear Parent, Hope you are well, As part of our Science and Technology Week, we are pleased to inform you that we will be hosting special events and activities for all students. One of the highlighted activities is a visit by a special guest speaker, Astronaut Nicole Stott. Nicole Stott is an American engineer and a retired NASA astronaut. She worked for NASA for 27 years in various positions and is one of very few women who conducted a spacewalk. Astronaut Stott served as a Flight Engineer on ISS Expedition 20 and Expedition 21 and was a Mission Specialist on STS-128 and STS-133. Please find attached her biography which denotes her very impressive career as an engineer, astronaut and director of missions. Nicole is the first person to tweet from space, and is an artist who has created several paintings while in space. She represents a perfect example of why we believe art must be integrated into the world of STEM to inspire creativity and innovation. This celebrated astronaut will be interacting with all of our students virtually starting May 3rd until May 6th 2020. Please find below the scheduled visits: Grade Date / Time Grades 5 and 6 Sunday, May 3rd at 1:00 p.m. Grades 7 and 8 Monday, May 4th at 1:00 p.m. Grades 9 and 10 Tuesday, May 5th at 1:00 p.m. Grades 11 and 12 Wednesday, May 6th at 1:00 p.m. Zoom Meeting IDs will be emailed to all students the night before. Each class will submit questions to the teachers beforehand and 6 of the best questions will be asked in the session to be answered by Astronaut Stott. -
XXIX Congress Report XXIX Planetary Congress • Austria • 2016 Photos: OEWF
XXIX Congress Report XXIX Planetary Congress • Austria • 2016 Photos: OEWF 1 John-David Bartoe, 2 Alexander Ivanchenkov, 3 Ulrich Walter, 4 Gerhard Thiele, 5 Georgi Iva- nov, 6 Yuri Gidzenko, 7 Bertalan Farkas, 8 Kevin Ford, 9 Pavel Vinogradov, 10 Charlie Walker, 11 Kimiya Yui, 12 Anatoli Artsebarskii, 13 Shannon Lucid, 14 Reinhold Ewald, 15 Claudie Haigneré, 16 Joe Acaba, 17 Ernst Messerschmid, 18 Jan Davis, 19 Franz Viehbock, 20 Loren Shriver, 21 Miroslaw Hermaszewski. 22 Sultan bin Salman al-Saud, 23 Yang Liwei, 24 Richard Garriott, 25 Mark Brown, 26 Carl Walz, 27 Bill McArthur, 28 Owen Garriott, 29 Anna Fisher, 30 George Zam- ka, 31 Rick Hieb, 32 Jerry Ross, 33 Alexander Volkov, 34 André Kuipers, 35 Jean-Pierre Haign- eré, 36 Toktar Aubakirov, 37 Kay Hire, 38 Michael Fincke, 39 John Fabian, 40 Pedro Duque, 41 Michael Foreman, 42 Sergei Avdeev, 43 Vladimir Kovolyonok, 44 Alexandar Aleksandrov, 45 Alexander Alexandrov, 46 Drew Feustel, 47 Dumitru Prunariu, 48 Alexei Leonov, 49 Rusty Sch- weickart, 50 Klaus-Dietrich Flade, 51 Anton Shkaplerov, 52 Alexander Samokutyaev, 53 Sergei Krikalev, 54 Viktor Savinykh, 55 Soichi Noguchi, 56 Bonnie Dunbar, 57 Vladimir Aksyonov, 58 Scott Altman, 59 Yuri Baturin, 60 Susan Helms, 61 Ulf Merbold, 62 Stephanie Wilson, 63 Chiaki Mukai, 64 Charlie Camarda, 65 Julie Payette, 66 Dick Richards, 67 Yuri Usachev, 68 Michael Lo- pez-Alegria, 69 Jim Voss, 70 Rex Walheim, 71 Oleg Atkov, 72 Bobby Satcher, 73 Valeri Tokarev, 74 Sandy Magnus, 75 Bo Bobko, 76 Helen Sharman, 77 Susan Kilrain, 78 Pam Melroy, 79 Janet Kavandi, 80 Tony Antonelli, 81 Sergei Zalyotin, 82 Frank De Winne, 83 Alexander Balandin, 84 Sheikh Muszaphar, 85 Christer Fuglesang, 86 Nikolai Budarin, 87 Salizhan Sharipov, 88 Vladimir Titov, 89 Bill Readdy, 90 Bruce McCandless II, 91 Vyacheslav Zudov, 92 Brian Duffy, 93 Randy Bresnik, 94 Oleg Artemiev XXIX Planetary Congress • Austria • 2016 One hundred and four astronauts and cosmonauts from 21 nations gathered Oc- tober 3-7, 2016 in Vienna, Austria for the XXIX Planetary Congress of the Associa- tion of Space Explorers. -
Introduction to Astronomy from Darkness to Blazing Glory
Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice: -
The Reference Mission of the NASA Mars Exploration Study Team
NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor Science Applications International Corporation Houston, Texas David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 This publication is available from the NASA Center for AeroSpace Information, 800 Elkridge Landing Road, Linthicum Heights, MD 21090-2934 (301) 621-0390. Foreword Mars has long beckoned to humankind interest in this fellow traveler of the solar from its travels high in the night sky. The system, adding impetus for exploration. ancients assumed this rust-red wanderer was Over the past several years studies the god of war and christened it with the have been conducted on various approaches name we still use today. to exploring Earth’s sister planet Mars. Much Early explorers armed with newly has been learned, and each study brings us invented telescopes discovered that this closer to realizing the goal of sending humans planet exhibited seasonal changes in color, to conduct science on the Red Planet and was subjected to dust storms that encircled explore its mysteries. The approach described the globe, and may have even had channels in this publication represents a culmination of that crisscrossed its surface. these efforts but should not be considered the final solution. It is our intent that this Recent explorers, using robotic document serve as a reference from which we surrogates to extend their reach, have can continuously compare and contrast other discovered that Mars is even more complex new innovative approaches to achieve our and fascinating—a planet peppered with long-term goal. -
Arxiv:1907.00616V1 [Astro-Ph.IM] 1 Jul 2019 282 75, Vol
Mem. S.A.It. Vol. 75, 282 c SAIt 2008 Memorie della The Transient High-Energy Sky and Early Universe Surveyor (THESEUS) L. Amati1, E. Bozzo2, P. O’Brien3, and D. G¨otz4 (on behalf of the THESEUS consortium) 1 INAF-OAS Bologna, via P. Gobetti 101, I-40129 Bologna, Italy e-mail: [email protected] 2 Department of Astronomy, University of Geneva, chemin d’Ecogia 16, 1290 Versoix, Switzerland 3 Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, United Kingdom 4 CEA, Universit Paris-Saclay, F-91191 Gif-sur-Yvette, France Abstract. The Transient High-Energy Sky and Early Universe Surveyor (THESEUS) is a mission concept developed in the last years by a large European consortium and currently under study by the European Space Agency (ESA) as one of the three candidates for next M5 mission (launch in 2032). THESEUS aims at exploiting high-redshift GRBs for getting unique clues to the early Universe and, being an unprecedentedly powerful machine for the detection, accurate location (down to ∼arcsec) and redshift determination of all types of GRBs (long, short, high-z, under-luminous, ultra-long) and many other classes of transient sources and phenomena, at providing a substantial contribution to multi-messenger time- domain astrophysics. Under these respects, THESEUS will show a strong synergy with the large observing facilities of the future, like E-ELT, TMT, SKA, CTA, ATHENA, in the electromagnetic domain, as well as with next-generation gravitational-waves and neutrino detectors, thus greatly enhancing their scientific return. Key words. THESEUS – Space mission Concept – ESA – M5 – Gamma-ray Bursts – Cosmology – Gravitational Waves – Multi-messenger Astrophysics. -
From the Heliosphere Into the Sun Programme Book Incuding All
511th WE-Heraeus-Seminar From the Heliosphere into the Sun –SailingagainsttheWind– Programme book incuding all abstracts Physikzentrum Bad Honnef, Germany January 31 – February 3, 2012 http://www.mps.mpg.de/meetings/heliocorona/ From the Heliosphere into the Sun A meeting dedicated to the progress of our understanding of the solar wind and the corona in the light of the upcoming Solar Orbiter mission This meeting is dedicated to the processes in the solar wind and corona in the light of the upcoming Solar Orbiter mission. Over the last three decades there has been astonishing progress in our understanding of the solar corona and the inner heliosphere driven by remote-sensing and in-situ observations. This period of time has seen the first high-resolution X-ray and EUV observations of the corona and the first detailed measurements of the ion and electron velocity distribution functions in the inner heliosphere. Today we know that we have to treat the corona and the wind as one single object, which calls for a mission that is fully designed to investigate the interwoven processes all the way from the solar surface to the heliosphere. The meeting will provide a forum to review the advances over the last decades, relate them to our current understanding and to discuss future directions. We will concentrate one day on in- situ observations and related models of the inner heliosphere, and spend another day on remote sensing observations and modeling of the corona – always with an eye on the symbiotic nature of the two. On the third day we will direct our view towards the future. -
Arxiv:2009.03244V1 [Astro-Ph.HE] 7 Sep 2020
Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions Peter Kretschmara, Felix Furst¨ b, Lara Sidolic, Enrico Bozzod, Julia Alfonso-Garzon´ e, Arash Bodagheef, Sylvain Chatyg,h, Masha Chernyakovai,j, Carlo Ferrignod, Antonios Manousakisk,l, Ignacio Negueruelam, Konstantin Postnovn,o, Adamantia Paizisc, Pablo Reigp,q, Jose´ Joaqu´ın Rodes-Rocar,s, Sergey Tsygankovt,u, Antony J. Birdv, Matthias Bissinger ne´ Kuhnel¨ w, Pere Blayx, Isabel Caballeroy, Malcolm J. Coev, Albert Domingoe, Victor Doroshenkoz,u, Lorenzo Duccid,z, Maurizio Falangaaa, Sergei A. Grebenevu, Victoria Grinbergz, Paul Hemphillab, Ingo Kreykenbohmac,w, Sonja Kreykenbohm nee´ Fritzad,ac, Jian Liae, Alexander A. Lutovinovu, Silvia Mart´ınez-Nu´nez˜ af, J. Miguel Mas-Hessee, Nicola Masettiag,ah, Vanessa A. McBrideai,aj,ak, Andrii Neronovh,d, Katja Pottschmidtal,am,Jer´ omeˆ Rodriguezg, Patrizia Romanoan, Richard E. Rothschildao, Andrea Santangeloz, Vito Sgueraag,Rudiger¨ Staubertz, John A. Tomsickap, Jose´ Miguel Torrejon´ r,s, Diego F. Torresaq,ar, Roland Walterd,Jorn¨ Wilmsac,w, Colleen A. Wilson-Hodgeas, Shu Zhangat Abstract High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology, they have attracted the interest of the high energy astrophysical community since the dawn of X-ray Astronomy. In more recent years, they have challenged our comprehension of physical processes in many more energy bands, ranging from the infrared to very high energies. In this review, we provide a broad but concise summary of the physical processes dominating the emission from high mass X-ray binaries across virtually the whole electromagnetic spectrum. -
SPACE SHUTTLE MISSIONS SUMMARY Page 210 - STS-127/2JA
Revision T, PCN-4 March 2010 SPACE SHUTTLE MISSIONS SUMMARY Page 210 - STS-127/2JA LANDING SITE/ SSME-TL CREW LAUNCH SITE, RUNWAY, NOM-ABORT SRB ORBIT PAYLOAD MISSION HIGHLIGHTS (6+1 UP/6+1 DN) FLT ORBITER LIFTOFF TIME, CROSSRANGE EMERG RSRM FSW WEIGHTS, (LAUNCH SCRUBS/DELAYS, NO. LANDING LANDING THROTTLE AND INC HA/HP PAYLOADS/ TAL WEATHER, ASCENT I-LOADS, (PCN4 Change Col SITES, TIMES PROFILE ET EXPERIMENTS FIRSTS, SIGNIFICANT ANOMALIES, ETC.) 3) ABORT TIMES FLT DURATION, ENG. S.N. TITLE, NAMES WINDS & EVA'S Revision T, PCN-4 March 2010 SPACE SHUTTLE MISSIONS SUMMARY Page 210 - STS-127/2JA STS- OV-105 CDR: KSC 15 (KSC 104/104/10 BI-138 CARGO: Brief Mission Summary: STS-127 ( 29th (Flight 23) Mark Polansky KSC 39A 71) 9% 51. DIRECT OI- 36253LBS mission to ISS) was a “16 day marathon 127/ 196:22:03:09Z 6 INSERTION 33 ENDEAVO (Flt 3 - STS-98,STS- 212:14:48:07Z RSRM (29) (3) construction mission”. The final pieces of ISS- UR 116) 6:03:10 PM EDT 09:48:07 AM PREDICTED: 106 PAYLOAD the Japanese Kibo Complex including an 2JA P794/R262/V185/M22 (P) CDT 100/104.5/1 POST OMS- CHARGEABLE: Experiment Exposed Facility “Porch” and 8 6:03:10 PM EDT FRIDAY (15) 04.5/ ET-131 2: 24682 LBS the unpressurized Experiment Logistics (A) 123.8x32.3 SEQ OMS PODS 07/31/09 (12 ) 72/104.5 Module were delivered along with spare Wednesday SLWT NM DEPLOYED: FLT # LPO3 -33 PLT equipment intended to keep ISS (15) 35 24266 LBS 127 RPO4 29 Doug Hurley DEORBIT ACTUAL: operational long after Shuttle is retired.