mercredi 19 janvier 2011

Astronaut Steve Bowen Named To STS-133 Space Shuttle Crew; Media Teleconference scheduled for 3:30 p.m. CST












NASA - STS-133 Mission patch.

Jan. 19, 2011

NASA selected astronaut Steve Bowen as a mission specialist on STS-133, the next space shuttle mission planned for launch on Feb. 24. Bowen replaces astronaut Tim Kopra, who was injured in a bicycle accident over the weekend. The agency will hold a media teleconference at 3:30 p.m. CST on Wednesday, Jan. 19, to discuss the change in crew personnel.

The teleconference panelists are:
-- Bill Gerstenmaier, NASA associate administrator for Space Operations
-- Peggy Whitson, chief of the Astronaut Office

"Tim is doing fine and expects a full recovery, however, he will not be able to support the launch window next month," said Peggy Whitson, chief of the Astronaut Office at NASA's Johnson Space Center in Houston. "If for some unanticipated reason STS-133 slips significantly, it is possible that Tim could rejoin the crew."

The crew change should not affect the mission's target launch date.

Space Shuttle Discovery on launch pad

"Steve is an ideal candidate, and we have complete confidence he'll contribute to a fully successful STS-133 mission," Whitson said. "He has performed five prior spacewalks. That extensive experience, coupled with some adjustments to the spread of duties among the crew, will allow for all mission objectives to be accomplished as originally planned in the current launch window."

Bowen will begin training this week with the STS-133 crew, which includes Commander Steve Lindsey, Pilot Eric Boe, and Mission Specialists Alvin Drew, Michael Barratt and Nicole Stott. Bowen also will train to perform the two planned spacewalks of the mission. He will join Alvin Drew to move a failed ammonia pump and perform other external configurations to the station.

The STS-133 mission to the International Space Station will deliver the Permanent Multipurpose Module, an external platform that holds large equipment and critical spare components for the station. The mission also will deliver Robonaut 2, or R2, the first human-like robot in space.

Audio of the teleconference will be streamed live at: http://www.nasa.gov/newsaudio

For Bowen's complete astronaut biographical information, visit: http://www.jsc.nasa.gov/Bios/htmlbios/bowen-sg.html

For Kopra's complete astronaut biographical information, visit: http://www.jsc.nasa.gov/Bios/htmlbios/kopra-tl.html

For information on the STS-133 mission, visit: http://www.nasa.gov/shuttle

Images, Text, Credit: NASA.

Best regards, Orbiter.ch

NASA Television To Air Space Station Spacewalk












ISS - Expedition 26 Mission patch.

Jan. 19, 2011

Two Russian cosmonauts on the International Space Station will conduct a spacewalk Friday, Jan. 21, to prepare the complex for future assembly and experiment work. The spacewalk will air live on NASA Television beginning at 8 a.m. CST.

Expedition 26 Flight Engineers Dmitry Kondratyev and Oleg Skripochka will perform the six-hour spacewalk.They will install an experimental Russian radio transmission system, retrieve existing experiments and install a TV camera on the Rassvet mini-research module that will assist in future dockings of vehicles to that port.


The Russian cosmonauts will exit the Pirs docking compartment airlock around 8:20 a.m. in their Russian Orlan spacesuits. The spacewalk will be the first for Kondratyev, who will wear the spacesuit marked with red stripes, and the second for Skripochka, who will wear the suit with blue stripes. Skripochka's first spacewalk was Nov. 15, 2010, and lasted six hours and 27 minutes.

For more information about the International Space Station visit: http://www.nasa.gov/station

For NASA TV downlink, schedule and streaming video information, visit: http://www.nasa.gov/ntv

Images, Text, Credits: NASA / ROSCOSMOS / RuSpace.

Cheers, Orbiter.ch

The Orion Nebula: Still Full of Surprises












ESO - European Southern Observatory logo.

19 January 2011


 This ethereal-looking image of the Orion Nebula was captured using the Wide Field Imager on the MPG/ESO 2.2-metre telescope at the La Silla Observatory, Chile. This nebula is much more than just a pretty face, offering astronomers a close-up view of a massive star-forming region to help advance our understanding of stellar birth and evolution. The data used for this image were selected by Igor Chekalin (Russia), who participated in ESO’s Hidden Treasures 2010 astrophotography competition. Igor’s composition of the Orion Nebula was the seventh highest ranked entry in the competition, although another of Igor’s images was the eventual overall winner.

The Orion Nebula, also known as Messier 42, is one of the most easily recognisable and best-studied celestial objects. It is a huge complex of gas and dust where massive stars are forming and is the closest such region to the Earth. The glowing gas is so bright that it can be seen with the unaided eye and is a fascinating sight through a telescope. Despite its familiarity and closeness there is still much to learn about this stellar nursery. It was only in 2007, for instance, that the nebula was shown to be closer to us than previously thought: 1350 light-years, rather than about 1500 light-years.

The jewel in Orion’s sword

Astronomers have used the Wide Field Imager on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile to observe the stars within Messier 42. They found that the faint red dwarfs in the star cluster associated with the glowing gas radiate much more light than had previously been thought, giving us further insights into this famous object and the stars that it hosts. The data collected for this science project, with no original intention to make a colour image, have now been reused to create the richly detailed picture of Messier 42 shown here.

Zooming in on the Orion Nebula

The image is a composite of several exposures taken through a total of five different filters. Light that passed through a red filter as well as light from a filter that shows the glowing hydrogen gas, were coloured red. Light in the yellow–green part of the spectrum is coloured green, blue light is coloured blue and light that passed through an ultraviolet filter has been coloured purple. The exposure times were about 52 minutes through each filter.

Panning across the Orion Nebula

This image was processed by ESO using the observational data found by Igor Chekalin (Russia) [1], who participated in ESO’s Hidden Treasures 2010 astrophotography competition [2], organised by ESO in October–November 2010, for everyone who enjoys making beautiful images of the night sky using real astronomical data.

Notes:

[1] Igor searched through ESO’s archive and identified datasets that he used to compose his image of Messier 42, which was the seventh highest ranked entry in the competition, out of almost 100 entries. His original work can be seen here.  Igor Chekalin was awarded the first prize of the competition for his composition of Messier 78, and he also submitted an image of NGC3169, NGC3166 and SN 2003cg, which was ranked second highest.

[2] ESO’s Hidden Treasures 2010 competition gave amateur astronomers the opportunity to search through ESO’s vast archives of astronomical data, hoping to find a well-hidden gem that needed polishing by the entrants. Participants submitted nearly 100 entries and ten skilled people were awarded some extremely attractive prizes, including an all expenses paid trip for the overall winner to ESO's Very Large Telescope (VLT) on Cerro Paranal, in Chile, the world’s most advanced optical telescope. The ten winners submitted a total of 20 images that were ranked as the highest entries in the competition out of the near 100 images.
More information

ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world’s most advanced visible-light astronomical observatory and VISTA, the world’s largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become “the world’s biggest eye on the sky”.

Links:

    * ESO’s Hidden Treasures 2010 competition: http://www.eso.org/public/outreach/hiddentreasures/index.html

    * Research papers:
          o http://adsabs.harvard.edu/abs/2009ApJS..183..261D
          o http://iopscience.iop.org/0004-637X/722/2/1092

    * Photos of La Silla Observatory: http://www.eso.org/public/images/archive/category/lasilla/

Images, Text, Credits: ESO and Igor Chekalin / IAU and Sky & Telescope / Video: Credit: ESO, Fujii, A., Gendler, R. and Chekalin, I. / Music: John Dyson (from the album "Moonwind").

Greetings, Orbiter.ch

mardi 18 janvier 2011

ESA’s Mercury mapper feels the heat












ESA - BepiColombo Mission patch.

18 January 2011

 BepiColombo's Mercury Magnetospheric Orbiter in the Large Space Simulator

Key components of the ESA-led Mercury mapper BepiColombo have been tested in a specially upgraded European space simulator. ESA’s Large Space Simulator is now the most powerful in the world and the only facility capable of reproducing Mercury’s hellish environment for a full-scale spacecraft.

The Mercury Magnetospheric Orbiter (MMO) has survived a simulated voyage to the innermost planet. The octagonal spacecraft, which is Japan’s contribution to BepiColombo, and its ESA sunshield withstood temperatures higher than 350°C.

This is a taste of things to come for the spacecraft. BepiColombo will encounter fully ten times the radiation power received by a satellite in orbit around Earth and, to simulate this, the Large Space Simulator (LSS) at ESA’s ESTEC centre in the Netherlands had to be specially adapted.

BepiColombo's Component spacecraft in orbit around Mercury

Engineers talk about the power of the Sun in units called the solar constant. This is how much energy is received every second through a square metre of space at the distance of Earth’s orbit.

“Previously, the LSS was capable of simulating a solar constant or two. Now it has been upgraded to produce ten solar constants,” says Jan van Casteren, ESA BepiColombo project manager.

The improvements have been achieved in two ways: the lamps from the simulators are being used at their maximum power and the mirrors that focus the beam have been adjusted.

Instead of producing a parallel beam of light 6 m across, they now concentrate the light into a cone just 2.7 m in diameter when it reaches the spacecraft. This creates a beam so fierce that a new shroud with a larger cooling capacity had to be installed to ‘catch’ the light that missed the spacecraft and prevent the chamber walls from heating up.

BepiColombo feels the heat

BepiColombo consists of separate modules. The MMO will investigate the magnetic environment of Mercury. It is kept cool during its six-year cruise to Mercury by the sunshield. These are the two modules that have now completed their thermal tests.

“The sunshield test was successful. Its function to protect the MMO spacecraft during the cruise phase was demonstrated,” says Jan.

“ESA’s Large Space Simulator is now the most powerful in the world and the only facility capable of reproducing Mercury’s hellish environment for a full-scale spacecraft.”

Once at Mercury, most of the Sun’s fearsome heat will be prevented from entering BepiColombo by special thermal blankets. They consist of multiple layers including a white ceramic outer layer and several metallic layers to reflect as much heat as possible back into space.

“The tests allowed us to measure the thermal blanket’s performance. The results allow us to prepare some adjustments for the tests of the Mercury Planetary Orbiter next year,” says Jan.

BepiColombo's scientists and engineers discuss the mission

In addition to enduring temperatures of 350°C, ESA’s Mercury Planetary Orbiter (MPO) will go where no spacecraft has gone before: down into a low elliptical orbit around Mercury, of between just 400 km and 1500 km above the planet’s scorching surface.

At that proximity, Mercury is worse than a hot plate on a cooker, releasing floods of infrared radiation into space. So, the MPO will have to deal with this as well as the solar heat. The MPO begins its tests in the LSS in the summer.

Related links:

BepiColombo industrial contract signed: http://www.esa.int/esaSC/SEM7UR3MDAF_index_0.html

BepiColombo mission to be presented to the media: http://www.esa.int/esaSC/SEM7C83MDAF_index_0.html

ESA gives go-ahead to build BepiColombo: http://www.esa.int/esaSC/SEMC8XBE8YE_index_0.html

Spot the targets of Europe's space explorers: http://www.esa.int/esaSC/ESA6B1G18ZC_exploring_0.html

Mercury shows its dark side: http://www.esa.int/esaSC/SEM6ABS1VED_index_0.html

Images, Animations, Video, Text, Credits: ESA / C. Carreau / JAXA.

Best regards, Orbiter.ch

lundi 17 janvier 2011

First Human Space Flight by Yuri A. Gagarin 50th Anniversary (1961-2011)

















ROSCOSMOS - Vostok-1 Mission logo / ROSCOSMOS - Vostok-1 Mission patch.

18.01.2011

Vostok 1 was the first human spaceflight. The Vostok 3KA spacecraft was launched on April 12, 1961, taking into space Yuri Gagarin, a cosmonaut from the Soviet Union (ex-USSR or CCCP).

Yuri A. Gagarin First Human Space Flight  12 April 1961

The Vostok 1 mission was the first time anyone had journeyed into outer space and the first time anyone had entered into orbit. The Vostok 1 was launched by the Soviet space program and designed by the Soviet rocket scientists Sergey Korolyov and Kerim Kerimov.

Vostok-1 launch, 12 April 1961

Kedr to Make Space Mission

Launch campaign of the Progress M-09M cargo vehicle continues at Baikonur.

Last week a small spacecraft was loaded into the vehicle together with other standard cargo items.
The satellite name was adopted by Yu.A. Gagarin call sign in his historical flight, namely Kedr.

Vostok-1 spacecraft

The satellite’s signal will be transmitted at radio amateur frequency of 145.95 MHz. Kedr has radio amateur call sign RS1S.  Kedr is to be launched by Russian Cosmonauts during the future EVA.

Vostok-1 landed
 
The satellite is to be delivered to the ISS by Progress M-09М to begin its mission on Jan. 28.

Related Link:

Simulate the first human flight with Orbiter SFS 2006 or 2006P1 (not compatible with Orbiter 2010):
http://www.orbithangar.com/search_quick.php?text=vostok+1&submit.x=0&submit.y=0

Images, Text, Credits: ROSCOSMOS PAO / Orbithangar.com.

Greetings, Orbiter.ch

ISS Crew Successfully Extinguished Virtual Fire














ISS - International Space Station patch / ISS - Expedition 26 Mission patch.

18.01.2011 (Moscow time)

Last week the crew of the International Space Station successfully extinguished virtual fire in their orbital outpost, Russian cosmonauts Dmitry Kondratiev told in his blog in Roscosmos web.


«We had a fire onboard training last week. The crew had to extinguish the fire in Japanese module of the ISS. The crew splits in three groups. The first one, together with the commander, talks to the Mission control teams and manages the actions. The second group extinguishes the fire, and the third group helps the second one”, Dmitry explains.


According to him, similar OBTs are run regularly in order to master the skills of the crew on different accidents in the station.


Dmitry notes that the crew this time was successful with extinguishing the fire, and the ground experts were satisfied with the training results.

Images, Text, Credits: ROSCOSMOS PAO.

Cheers, Orbiter.ch

dimanche 16 janvier 2011

JAXA - KOUNOTORI 2 / H-IIB F2 live launch broadcast














JAXA - KOUNOTORI 2 (HTV-2) Mission patch.

Jan. 16, 2011

KOUNOTORI-2 / H-IIB F2 live launch broadcast starts at 2:30 p.m. on Jan. 20!


JAXA will broadcast a live launch report of the KOUNOTORI2/H-IIB Launch Vehicle No.2 from 2:30 p.m. on January 20 (Thur.) You can watch the live report at public viewing sites including JAXA offices and science museums as well as through cable TV and some websites. Why don’t you watch the live launch with us?

Broadcast Schedule:

   1. KOUNOTORI2(HTV2)/H-IIB No.2 Launch:
      from 2:30 p.m. on January 20 (Thu, JST) (for one and a half hours)

   2. Final Approach to the ISS, Capture by the SSRMS:
      from 7:50 p.m. on January 27 (Thu, JST) (for one hour)

   3. HTV docking with the ISS:
      from 10:30 p.m. on January 27 (Thu, JST) (for one hour)

KOUNOTORI-2 (HTV-2) cutaway description

 The H-IIB Launch Vehicle is Japan’s large-scale rocket whose launch capability is at the highest level in the world. It was successfully developed in a short period by making the best use of technologies acquired through the experience of the H-IIA Launch Vehicle to realize a low-cost and low-risk launch vehicle. The H-IIB Launch Vehicle No. 2 (H-IIB F2) is scheduled to be launched on January 20 (Thu.,) 2011 to inject its payload, the second H-II Transfer Vehicle (HTV2) into its orbit.

H-IIB Launcher with HTV-2

The H-IIB Test Flight was launched exactly at the scheduled launch time and date on September 11, 2009, and that was the first punctual launch of the first flight of Japan’s major launch vehicles. The H-IIB TF then successfully injected the HTV1 (technological demonstration flight) in its planned orbit. The H-IIB/HTV launch won praise throughout the world including from NASA, and was highly evaluated for its international contribution. As the H-IIB/HTV launch will be the only means for large-size cargo transportation to the International Space Station after the scheduled retirement of the Space Shuttle, the H-IIB F2 will be launched with the high expectations of the world.

 H-II Transfer Vehicle  KOUNOTORI  (HTV) Key Space Transfer

KOUNOTORI2/H-IIB Launch Vehicle No.2 Special Site: http://www.jaxa.jp/countdown/h2bf2/index_e.html

Images, Text, Credits: Japan Aerospace Exploration Agency (JAXA) / Mitsubishi Heavy Industries.

Greetings, Orbiter.ch