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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. -
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. -
IAF-01-T.1.O1 Progress on the International Space Station
https://ntrs.nasa.gov/search.jsp?R=20150020985 2019-08-31T05:38:38+00:00Z IAF-01-T.1.O1 Progress on the International Space Station - We're Part Way up the Mountain John-David F. Bartoe and Thomas Holloway NASA Johnson Space Center, Houston, Texas, USA The first phase of the International Space Station construction has been completed, and research has begun. Russian, U.S., and Canadian hardware is on orbit, ard Italian logistics modules have visited often. With the delivery of the U.S. Laboratory, Destiny, significant research capability is in place, and dozens of U.S. and Russian experiments have been conducted. Crew members have been on orbit continuously since November 2000. Several "bumps in the road" have occurred along the way, and each has been systematically overcome. Enormous amounts of hardware and software are being developed by the International Space Station partners and participants around the world and are largely on schedule for launch. Significant progress has been made in the testing of completed elements at launch sites in the United States and Kazakhstan. Over 250,000 kg of flight hardware have been delivered to the Kennedy Space Center and integrated testing of several elements wired together has progressed extremely well. Mission control centers are fully functioning in Houston, Moscow, and Canada, and operations centers Darmstadt, Tsukuba, Turino, and Huntsville will be going on line as they are required. Extensive coordination efforts continue among the space agencies of the five partners and two participants, involving 16 nations. All of them continue to face their own challenges and have achieved significant successes. -
Experiencing Hubble
PRESCOTT ASTRONOMY CLUB PRESENTS EXPERIENCING HUBBLE John Carter August 7, 2019 GET OUT LOOK UP • When Galaxies Collide https://www.youtube.com/watch?v=HP3x7TgvgR8 • How Hubble Images Get Color https://www.youtube.com/watch? time_continue=3&v=WSG0MnmUsEY Experiencing Hubble Sagittarius Star Cloud 1. 12,000 stars 2. ½ percent of full Moon area. 3. Not one star in the image can be seen by the naked eye. 4. Color of star reflects its surface temperature. Eagle Nebula. M 16 1. Messier 16 is a conspicuous region of active star formation, appearing in the constellation Serpens Cauda. This giant cloud of interstellar gas and dust is commonly known as the Eagle Nebula, and has already created a cluster of young stars. The nebula is also referred to the Star Queen Nebula and as IC 4703; the cluster is NGC 6611. With an overall visual magnitude of 6.4, and an apparent diameter of 7', the Eagle Nebula's star cluster is best seen with low power telescopes. The brightest star in the cluster has an apparent magnitude of +8.24, easily visible with good binoculars. A 4" scope reveals about 20 stars in an uneven background of fainter stars and nebulosity; three nebulous concentrations can be glimpsed under good conditions. Under very good conditions, suggestions of dark obscuring matter can be seen to the north of the cluster. In an 8" telescope at low power, M 16 is an impressive object. The nebula extends much farther out, to a diameter of over 30'. It is filled with dark regions and globules, including a peculiar dark column and a luminous rim around the cluster. -
Expedition 16 Adding International Science
EXPEDITION 16 ADDING INTERNATIONAL SCIENCE The most complex phase of assembly since the NASA Astronaut Peggy Whitson, the fi rst woman Two days after launch, International Space Station was fi rst occupied seven commander of the ISS, and Russian Cosmonaut the Soyuz docked The International Space Station is seen by the crew of STS-118 years ago began when the Expedition 16 crew arrived Yuri Malenchenko were launched aboard the Soyuz to the Space Station as Space Shuttle Endeavour moves away. at the orbiting outpost. During this ambitious six-month TMA-11 spacecraft from the Baikonur Cosmodrome joining Expedition 15 endeavor, an unprecedented three Space Shuttle in Kazakhstan on October 10. The two veterans of Commander Fyodor crews will visit the Station delivering critical new earlier missions aboard the ISS were accompanied by Yurchikhin, Oleg Kotov, components – the American-built “Harmony” node, the Dr. Sheikh Muzaphar Shukor, an orthopedic surgeon both of Russia, and European Space Agency’s “Columbus” laboratory and and the fi rst Malaysian to fl y in space. NASA Flight Engineer Japanese “Kibo” element. Clayton Anderson. Shukor spent nine days CREW PROFILE on the ISS, returning to Earth in the Soyuz Peggy Whitson (Ph. D.) TMA-10 on October Expedition 16 Commander 21 with Yurchikhin and Born: February 9, 1960, Mount Ayr, Iowa Kotov who had been Education: Graduated with a bachelors degree in biology/chemistry from Iowa aboard the station since Wesleyan College, 1981 & a doctorate in biochemistry from Rice University, 1985 April 9. Experience: Selected as an astronaut in 1996, Whitson served as a Science Offi cer during Expedition 5. -
Star Formation Relations and CO Sleds Across the J-Ladder and Redshift 3 on the ESA Herschel Space Observatory20 (Pilbratt Et Al
Draft version July 17, 2014 Preprint typeset using LATEX style emulateapj v. 5/2/11 STAR FORMATION RELATIONS AND CO SPECTRAL LINE ENERGY DISTRIBUTIONS ACROSS THE J-LADDER AND REDSHIFT T. R. Greve1, I. Leonidaki2, E. M. Xilouris2, A. Weiß3, Z.-Y. Zhang4,5, P. van der Werf6, S. Aalto7, L. Armus8, T. D´ıaz-Santos8, A.S. Evans9,10, J. Fischer11, Y. Gao12, E. Gonzalez-Alfonso´ 13, A. Harris14, C. Henkel3, R. Meijerink6,15, D. A. Naylor16 H. A. Smith17 M. Spaans15 G. J. Stacey18 S. Veilleux14 F. Walter19 Draft version July 17, 2014 ABSTRACT 0 We present FIR[50 − 300 µm]−CO luminosity relations (i.e., log LFIR = α log LCO + β) for the full CO rotational ladder from J = 1 − 0 up to J = 13 − 12 for a sample of 62 local (z ≤ 0:1) (Ultra) 11 Luminous Infrared Galaxies (LIRGs; LIR[8−1000 µm] > 10 L ) using data from Herschel SPIRE-FTS and ground-based telescopes. We extend our sample to high redshifts (z > 1) by including 35 (sub)- millimeter selected dusty star forming galaxies from the literature with robust CO observations, and sufficiently well-sampled FIR/sub-millimeter spectral energy distributions (SEDs) so that accurate FIR luminosities can be deduced. The addition of luminous starbursts at high redshifts enlarge the range of the FIR−CO luminosity relations towards the high-IR-luminosity end while also significantly increasing the small amount of mid-J/high-J CO line data (J = 5 − 4 and higher) that was available prior to Herschel. This new data-set (both in terms of IR luminosity and J-ladder) reveals linear FIR−CO luminosity relations (i.e., α ' 1) for J = 1 − 0 up to J = 5 − 4, with a nearly constant normalization (β ∼ 2). -
Sts-110 F R a M E W O R K F O R E X P a N D I N G S T a T I O N R E S E a R C H
STS-110 F R A M E W O R K F O R E X P A N D I N G S T A T I O N R E S E A R C H WWW.SHUTTLEPRESSKIT.COM Updated March 20, 2001 STS-110 Table of Contents Mission Overview ..................................................................................................... 1 Mission Objectives .................................................................................................. 7 New, Safer Engines to Propel Atlantis ................................................................... 9 Crewmembers ......................................................................................................... 11 Flight Day Summary Timeline ............................................................................... 15 Rendezvous and Docking ..................................................................................... 16 Spacewalk STS-110 Extravehicular Activity ............................................................................... 20 Payloads Payload Overview .................................................................................................... 28 Central Integrated Truss Structure ........................................................................... 30 Mobile Transporter ................................................................................................... 35 Experiments: DTOs and DSOs Science Payloads .................................................................................................... 39 Biomass Production System ................................................................................... -
Expedition 8 MISSION OVERVIEW
Expedition 8 MISSION OVERVIEW To Improve Life Here, Science Comes to the Forefront To Extend Life to There, To Find Life Beyond. Experiments from earlier expeditions will Education Payload Operations (EPO) remain aboard the International Space include three educational activities that That is NASAs vision. Station (ISS), continuing to benefit from will focus on demonstrating science, long-term exposure to microgavity, and mathematics, technology, engineering or Michael Foale, additional studies in the life and physical geography principles. Expedition 8 Commander, NASA ISS sciences and space technology development Group Activation Packs -- YEAST will Science Officer: will be added. evaluate the role of individual genes in the When we look back fifty years to this time, we Most of the research complement for response of yeast to space flight conditions. wont remember the experiments that were Expedition 8 will be carried out with The results of this research could help performed, we wont remember the assembly scientific research facilities and samples clarify how mammalian cells grow under that was done, we may barely remember any already on board the Space Station. microgravity conditions and determine if individuals. What we will know was that countries Additional experiments are being evaluated genes are altered. came together to do the first joint international and prepared to take advantage of the Synchronized Position Hold, Engage, project, and we will know that that was the seed limited cargo space on the Soyuz or Reorient, Experimental Satellites that started us off to the moon and Mars. Progress vehicles. The research agenda for (SPHERES) will allow scientists to study the expedition remains flexible. -
Spaceport News Pioneering the Future America's Gateway to the Universe
May 14, 1999 Vol. 38, No. 10 Fortieth Anniversary Spaceport News Pioneering the Future America's gateway to the universe. Leading the world in preparing and launching missions to Earth and beyond. John F. Kennedy Space Center Preparing GOES to go Packing up for a trip to the space station Packing li ght isn't an option for the seven-member crew of STS-96, scheduled to lift off to the Inter national Space Station (ISS) on May 20 from Kennedy Space Center's Launch Pad 39B. The 10-day flight will take about two tons of supplies - including laptop computers, a printer, cameras, maintenance tools, spare parts and clothing- to the orbiting space station in the SPACEHAB double module. Discovery will be the first orbiter to dock with the fledgling station since the crew of Endeavour departed the outpost in December 1998. At Astrotech in Titusville, STS-96 will also be the first Fla., the GOES-L weather logistics flight to the new station. satellite was encapsulated in Discovery will spend five days its fairing before transfer to linked to the ISS, transferring and Launch Pad 36B at Cape installing gear that could not be Canaveral Air Station. The fourth of a new (See STS-96, Page 5) advanced series of geo At left, In the payload changeout room at stationary weather satellites Launch Pad 39B, technicians moved the for the National Oceanic and SPACEHAB double module from the payload canister on April 28 and placed it Atmospheric Administration in Space Shuttle Discovery's payload bay (NOAA), GOES-Lis a three for STS-96. -
The Evolution of Cluster E and S0 Galaxies Measured from The
A Mon. Not. R. Astron. So c. 000, 000{000 (0000) Printed 12 May1999 (MN L T Xstyle le v1.4) E The evolution of cluster E and S0 galaxies measured from ? the Fundamental Plane 1;2 yzx 3;4;5 zx 6;7;8 x 3;5 x Inger Jrgensen Marijn Franx , Jens Hjorth , Pieter G. van Dokkum 1 McDonald Observatory, The University of Texas at Austin, RLM 15.308, Austin, TX 78712, USA 2 Gemini Observatory, 670 N. A`ohoku Pl., Hilo, HI 96720, USA (Postal address for IJ) 3 Kapteyn Institute, P.O.Box 800, 9700 AVGroningen, The Netherlands 4 Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 5 Leiden Observatory, P.O.Box 9513, 2300 RA Leiden, The Netherlands (Postal address for MF and PvD) 6 Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK 7 NORDITA, Blegdamsvej 17, DK-2100 Copenhagen , Denmark 8 Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen , Denmark (Postal address for JH) May 5, 1999, accepted for publication in Mon. Not. Royal Astron. Sco., Gemini Preprint #43 ABSTRACT Photometry has b een obtained for magnitude limited samples of galaxies in the two rich clusters Ab ell 665 (37 galaxies) and Ab ell 2218 (61 galaxies). Both clusters have m a redshift of 0.18. The limiting magnitude of the samples is 19 in the I-band. Sp ec- troscopy has b een obtained for seven galaxies in A665 and nine galaxies in A2218, all of whichalsohaveavailable photometry. Sp ectroscopy has b een obtained for two additional galaxies in A2218, one of whichisabackground galaxy. -
The Flight Plan
M A R C H 2 0 2 1 THE FLIGHT PLAN The Newsletter of AIAA Albuquerque Section The American Institute of Aeronautics and Astronautics AIAA ALBUQUERQUE MARCH 2021 SECTION MEETING: MAKING A DIFFERENCE A T M A C H 2 . Presenter. Lt. Col. Tucker Hamilton Organization USAF F-35 Developmental Test Director of Operations INSIDE THIS ISSUE: Abstract I humbly present my flying experiences through SECTION CALENDAR 2 pictures and videos of what it takes and what it is like to be an Experimental Fighter Test Pilot. My personal stories include NATIONAL AIAA EVENTS 2 major life-threatening aircraft accidents, close saves, combat SPACE NUCLEAR PROPULSION REPORT 3 flying revelations, serendipitous opportunities testing first of its kind technology, flying over 30 aircraft from a zeppelin to a ALBUQUERQUE DECEMBER MEETING 5 MiG-15 to an A-10, and managing the Joint Strike Fighter De- velopmental Test program for all three services. Through ALBUQUERQUE JANUARY MEETING 6 these experiences you will learn not just what a Test Pilot does, but also gain encour- ALBUQUERQUE FEBRUARY MEETING 7 agement through my lessons learned on how to make a difference in your local com- munities…did I mention cool flight test videos! CALL FOR SCIENCE FAIR JUDGES 9 Lt Col Tucker "Cinco" Hamilton started his Air Force career as an CALL FOR SCHOLARSHIP APPLICATIONS 10 operational F-15C pilot. He supported multiple Red Flag Exercises and real world Operation Noble Eagle missions where he protect- NEW AIAA HIGH SCHOOL MEMBERSHIPS 10 ed the President of the United States; at times escorting Air Force One. -
Expedition 11 Opening the Door for Return to Flight
EXPEDITION 11 OPENING THE DOOR FOR RETURN TO FLIGHT When the crew of STS-114, the mission that The Expedition 11 crew of Krikalev, the will return the Space Shuttle to fl ight, arrives expedition and Soyuz Commander, and at the International Space Station, Russian Phillips, the Flight Engineer and ISS Science Cosmonaut Sergei Krikalev and American Offi cer, began their six-month mission to the Astronaut John Phillips, will be ready to ISS with a lift-off April 15, 2005, aboard a welcome them onboard the orbiting outpost. Soyuz spacecraft launched from the Baikonur Cosmodrome in Kazakhstan. Once they arrived at the Space Station, the new team replaced the Expedition 10 crew of Leroy Chiao and Salizhan Sharipov, who had been aboard the ISS since Oct. 15, 2004. Joining the Expedition 11 crew aboard Soyuz TMA-6 was European Space Agency Astronaut Roberto Vittori, an Italian Air Force pilot. He spent eight days on the Station, conducting a variety of experiments before returning home with Chiao and Sharipov. During the Expedition 11 mission, 15 scientifi c investigations are planned, most of which United Space Alliance Training Team member Oscar focus on how the human body changes and Koehler, left, assists Cosmonaut Sergei Krikalev, adapts to the microgravity environment of Orbiting 221 miles above the Earth, the International Space Station is seen with the Port One truss and right, and astronaut John Phillips as they participate space. Starboard One truss in place. in a training session in the Johnson Space Center’s Virtual Reality Lab. This type of computer training The ISS experiments are part of a step-by-step and beyond.