mercredi 7 septembre 2011

The number of space debris reached a "critical point"










Space Junk.

Sep. 7, 2011

A waste weightless, floating in space and encasing our beloved planet. This is the ecological disaster of decades of space exploration. In a report released this week, U.S. scientists are sounding the alarm: the number of debris floating in space has reached a "critical point", which threatens more and more on satellites and astronauts.


Video above: Space Debris Video, from AIAA's 1st Biennnial Congressional Aerospace Policy Retreat, which took place 18 March 2011.

"Space is becoming more dangerous for spacecraft and astronauts," says this report Donald Kessler, former head of NASA and the president of a commission to study the issue of orbital debris. "NASA needs to find the best way to tackle all the problems caused by meteoroids and orbital debris that pose risks on men and the missions of space robots," said he.

Prohibition of debris pick another country

NASA has recorded 22 000 debris and estimated millions of those numbers too small to be recorded. Among the debris, at least 500 000 were between 1 and 10 cm in diameter, and can cause damage. Computer projections show that the number has reached a "critical point" which they will collide and create new debris, further increasing the risk of damaging the spacecraft, according to the National Research Council, an organization independent research which oversees the committee.

Space junk a conceptual artwork representing defunct satellites, failed missions, and shrapnel orbiting Earth

In 2007, China has further increased the number of debris by testing anti-satellite missile that had sprayed a weather satellite in 150 000 pieces. Or do the cleaning is not only expensive but also extremely complicated. Because the U.S. has no right under international law, to collect objects in space from other countries. "The Cold War is over but the issue of satellite technology is sensitive," says Vice-Chairman of the Committee, George Gleghorn.

The report of the Committee, 160 pages, recommends that NASA seeks the help of the State Department to address "the economic, technological, political and legal".

Current status of the launchers:

Since the sixties (early in the Mercury Program), NASA to recover some of the elements of its launch vehicles, mainly for technical and scientific expertise, a concern for ecological recovery emerged in the early 80 with the space shuttle with all elements of the launcher's back, the main tank burns in large part during its atmospheric re-entry., it was part of the basic concept, making the launch "less expensive" and more environmentally friendly "recycling" everything.

Recovery of Gemini V Booster


Image above: The external fuel tank of the orbiter falls back to earth after detaching from the space shuttle Discovery in July 2005. Engineers are analysing these photos as part of the extensive imagery data being gathered to understand falling debris during the shuttle's launch.

Space Shuttle Solid Rocket Booster Recovery


This image above provided by NASA show unidentified possible small debris recorded by digital still camera by Shuttle crew.
 
With the future launch vehicle and Ares Orion capsule, the whole is recovering.


The Russian Space Station Mir burns up as it enters the Earth's atmosphere over Nadi, Fiji, in March 2001. After 15 years of service in outer space, Mir made its re-entry to Earth.

In Russia, Soyuz, Proton, only the boosters and the first stage are generally recovered by local scrap dealers.

KAZAKHSTAN - The fiery wreck of a rocket booster after crashing

The movie "Space Tourists" illustrates the impact of the Russian space program on the environment, if you find from your rental company movie, rent it! (See Trailer below).

Space Tourists

KAZAKHSTAN - Scrap-metal dealers wait for a rocket to crash

KAZAKHSTAN - The fiery wreck of a rocket after crashing

At the ESA, since the generation Ariane 5 boosters are recovered.

 Ariane 5 solid rocket booster recovery

Over 90% of the debris fall into the oceans. Regarding the satellite end of life and other debris, the problem is their uncontrolled fall for some models.

The Automated Transfer Vehicle (ATV) is designed as the Progress cargo, to burn at its re-entry.

 ATV re-entry

Examples of falling debris in all different parts of the world:


Australian farmer James Stirton stands next to a ball of twisted metal, purported to be fallen space junk, on his farm in southwestern Queensland in March 2008. Stirton found the giant ball, which he believes is space junk from a rocket used to launch communications satellites.


Theodore Solomons sits next to the metal ball that he saw fall from the sky on a farm close to Worcester, about 150 kilometres outside of Cape Town, south Africa in April 2000. A second metal ball dropped out of the sky the following day on a farm approximately 50 kilometres outside of Cape Town. Astronomers said the balls, which were white-hot when they landed, could be parts of a decaying satellite.


A US Customs official inspects the largest piece of wreckage from the downed Skylab at the San Francisco International Airport, California, in July 1979. The one-ton piece wreckage was found in Australia.


ALTAI, Russia - Villagers collect scrap from a crashed spacecraft, surrounded by thousands of white butterflies, 2000. Environmentalists fear for the region's future due to toxic rocket fuel.


ALTAI, Russia - Dead cows lie on a cliff, 2000. Locals say that whole herds of cattle and sheep regularly die because rocket fuel poisons the soil.


A main propellant tank of a Delta 2 launch vehicle which landed in Georgetown, Texas, on Jan. 22, 1997.

Space debris fell in Saudi Arabia

How to Track Space Junk Online: http://www.wired.com/wiredscience/2009/03/howtojunk/

AIAA's 1st Biennnial Congressional Aerospace Policy Retreat: http://www.aiaa.org/content.cfm?pageid=896

Images, Videos, Text, Credits: NASA / ESA / ROSCOSMOS PAO / AFP / Le Monde.fr / BBC / AIAA / AGI / Orbiter.ch.

Best regards, Orbiter.ch

Baikonur is mounted a measuring station for the flight control interplanetary probe "Phobos-Grunt"












Roscosmos logo.

09/07/2011

At Baikonur continues preparations for the upcoming launch of the rocket "Zenit-2M" with interplanetary station "Phobos-Grunt" in November 2011.

In order to monitor and control system in the first two weeks on the 23rd floor space center (measuring station "Saturn") specialists TsENKI and OAO "Russian Space Systems" is the deployment of telemetry complex "spectrum of the X-Men." Decided to create a new station with an antenna complex "courier", previously used to work for launch communications satellites, "Lightning." Antenna diameter is only 12 meters, but the complex equipment and powerful modern highly sensitive technique allows to control the flight of interplanetary probes at a distance of several million kilometers.


Within two weeks, experts expect to complete installation of equipment, and then begin testing the transmitters, receivers and computer equipment industry. The culmination of a complex telemetry, "Spectrum-X" will be its commissioning.


Launch of "Phobos-Grunt" capabilities of the new station will not be exhausted, it will be used for flight control of other Russian interplanetary probes.

Images, Text, Credits: Press-service of Russian Federal Space Agency (Roscosmos PAO) and KC "Southern" / Translation: Orbiter.ch.

Greetings, Orbiter.ch

The “Scinence” special edition on “HAYABUSA” research reports was published











JAXA - HAYABUSA Mission patch.

August 26, 2011 (JST)

The Japan Aerospace Exploration Agency (JAXA) has been engaged in collecting and categorizing particles in the sampler container (*1), which was brought back by the instrumental module of the asteroid exploration spacecraft "HAYABUSA" from asteroid "Itokawa."

As part of this effort, JAXA has been conducting the initial analysis (*2) of particles identified as rocky using scanning electron microscope (SEM) observations, which were collected from sample catcher compartment "A."

As a part of achievements of the initial analysis, six HAYABUSA research reports were published in the "Science Magazine" dated August 26, 2011. In addition, the cover of this magazine features these achievements.

This is also epoch-making news since the special issues that the asteroid explorer "HAYABUSA's" neighborhood observation on asteroid "Itokawa" in June 2006, the solar observation satellite "HINODE" in December 2007 and "KAGUYA" in February 2009.

The titles of the research reports in Science magazine are as follows:

1) Itokawa dust particles: A direct link between S-type asteroids and ordinary chondrites
2) Oxygen Isotopic Compositions of Asteroidal Materials Returned from Itokawa by the Hayabusa Mission
3) Neutron Activation Analysis of a Particle Returned from Asteroid Itokawa
4) Three-dimensional structure of Hayabusa sample: Origin and evolution of Itokawa regolith
5) Incipient space weathering observed on the surface of Itokawa dust
6) Irradiation history of Itokawa regolith material deduced from noble gases in the Hayabusa samples

*1 The HAYABUSA sampler container consists of 2 compartments that are called Sample Catcher A and B.

*2 "Initial analysis" means the analysis of typical particles to obtain information necessary for categorizing (identification, classification and numbering) as a part of curation activity (*3).

*3 "Curation activity" means the retrieval of particles, preservation, categorizing and allocation and their necessary analysis.

Science Magazine 26 August 2011 : Cover


A small rocky particle, 150 microns in size, brought buck from asteroid "Itokawa " by the asteroid exploration spacecraft "HAYABUSA."

Mission website:

Science: http://www.sciencemag.org/magazine.dtl
Asteroid Explorer "HAYABUSA" (MUSES-C): http://www.jaxa.jp/projects/sat/muses_c/index_e.html
Tohoku University: http://www.tohoku.ac.jp/english/
KEK / Tohoku University: http://www.kek.jp/intra-e/press/2011/082613/
Hokkaido University: http://www.hokudai.ac.jp/en/
Tokyo Metropolitan University: http://www.tmu.ac.jp/english/index.html
Osaka University: http://www.osaka-u.ac.jp/en/index.html
The University of Tokyo: http://www.u-tokyo.ac.jp/index_e.html

Appendix: Research Reports Titles with Outlines

Author: Tomoki Nakamura (Tohoku University) et al.
Title: Itokawa dust particles: A direct link between S-type asteroids and ordinary chondrites
Abstract: The Hayabusa spacecraft successfully recovered dust particles from the surface of near-Earth asteroid 25143 Itokawa. Synchrotron-radiation X-ray diffraction and transmission and scanning electron microscope analyses indicate that the mineralogy and mineral chemistry of the Itokawa dust particles are identical to those of thermally metamorphosed LL chondrites, consistent with spectroscopic observations made from Earth and by the Hayabusa Spacecraft. Our results directly demonstrate that ordinary chondrites, the most abundant meteorites found on the Earth, come from S-type asteroids. Mineral chemistry indicates that the majority of regolith surface particles suffered long-term thermal annealing and subsequent impact shock, suggesting that Itokawa is an asteroid made of reassembled pieces of the interior portions of a once larger asteroid.

Author: Hisayoshi Yurimoto (Hokkaido University) et al.
Title:Oxygen Isotopic Compositions of Asteroidal Materials Returned from Itokawa by the Hayabusa Mission
Abstract:Meteorite studies suggest that each solar system object has a unique oxygen isotopic composition. Chondrites have been believed to be derived from asteroids, but oxygen isotopic compositions of asteroids themselves have not been established. We have measured by secondary ion mass spectrometry oxygen isotopic compositions of rock particles from asteroid 25143 Itokawa returned by the Hayabusa spacecraft. Compositions of the particles are depleted in 16O relative to terrestrial materials and indicate that Itokawa, an S-type asteroid, is one of the sources of the LL or L group of equilibrated ordinary chondrites. We have the first direct oxygen-isotope link between chondrites and their parent asteroid.

Author: Mitsuru Ebihara (Tokyo Metropolitan University) et al.
Title:Neutron Activation Analysis of a Particle Returned from Asteroid Itokawa
Abstract:A single grain (~3 μg) returned by the Hayabusa spacecraft was analyzed by neutron activation analysis. This grain is mainly composed of olivine with minor amounts of plagioclase, troilite and metal. Our results establish that the Itokawa sample has similar chemical characteristics (Fe/Sc and Ni/Co ratios) to chondrite, confirming that this grain is extraterrestrial in origin and has primitive chemical compositions. Estimated Ir/Ni and Ir/Co ratios for metal in the Itokawa samples are about five times lower than CI values. A similar depletion of Ir was observed in chondrules metals of ordinary chondrites. These metals must have condensed from the nebular where refractory siderophile elements already condensed and were segregated.

Author: Akira Tsuchiyama (Osaka University) et al.
Title:Three-dimensional structures of Hayabusa sample: Origin and evolution of Itokawa regolith
Abstract:Regolith particles on the asteroid Itokawa were recovered by the Hayabusa mission. Thee-dimensional (3D) structures of these particles examined by X-ray microtomography give information for comparison with meteorites and about regolith formation. Modal abundances of minerals, bulk density (3.4 g/cm3), and the 3D textures indicate a mixture of equilibrated and less-equilibrated LL chondrite materials. No particles showing melting were observed. 3D shape features of these particles (size and shape distributions, and the presence of particles with rounded edges) are different from the lunar regolith and suggest that they were formed by meteoroid impacts on the asteroid surface, and eroded by seismic-induced grain motion in the smooth terrain. The results indicate that the returned samples are a good representation of the surface materials on Itokawa.

Author: Takaaki Noguchi (Ibaraki University) et al.
Title:Incipient space weathering observed on the surface of Itokawa dust
Abstract:The reflectance spectra of the most abundant meteorites, ordinary chondrites, are different from the abundant S-type asteroids. This discrepancy hasbeen thought to be due to space weathering, which is an alteration of surfaces of airless bodies exposed to the space environment. Here we report evidence of space weathering on particles returned from the S-type asteroid Itokawa by the Hayabusa spacecraft. Surface modification was found in 5 out of 10 particles, which varies depending on mineral species. Sulfur-bearing Fe-rich nanoparticles (npFe) exist in a thin (5-15 nm) surface layer on olivine, low-Ca pyroxene, and plagioclase, suggestive of vapor deposition. Sulfur-free npFe exist deeper inside (<60 nm) ferromagnesian silicates. Their texture suggests formation by metamictization and in-situ reduction of Fe2+.

Author: Keisuke Nagao (The University of Tokyo) et al.
Title:Irradiation history of Itokawa regolith material deduced from noble gases in the Hayabusa samples
Abstract: Noble gas isotopes were measured in three rocky grains from asteroid Itokawa to elucidate a history of irradiation from cosmic rays and solar wind on its surface. Large amounts of solar helium (He), neon (Ne), and argon (Ar) trapped in various depths in the grains were observed, which can be explained by multiple implantations of solar wind particles into the grains, combined with preferential He loss caused by frictional wear of space-weathered rims on the grains. Short residence time of less than 8 million years was implied for the grains by an estimate on cosmic-ray.produced 21Ne. Our results suggest that Itokawa is continuously losing its surface materials into space at a rate of tens of centimeters per million years. The lifetime of Itokawa should be much shorter than the age of our solar system.

Images, Text, Credit: Japan Aerospace Exploration Agency (JAXA).

Greetings, Orbiter.ch

Young Stars Take a Turn in the Spotlight












ESO - European Southern Observatory logo.

7 September 2011

 The star cluster NGC 2100 in the Large Magellanic Cloud

ESO’s New Technology Telescope (NTT) has captured a striking image of the open cluster NGC 2100. This brilliant star cluster is around 15 million years old, and located in the Large Magellanic Cloud, a nearby satellite galaxy of the Milky Way. The cluster is surrounded by glowing gas from the nearby Tarantula Nebula.

Observers often overlook NGC 2100 because of its close proximity to the impressive Tarantula Nebula (eso0650) and the super star cluster RMC 136 (eso1030). The glowing gas of the Tarantula Nebula even tries to steal the limelight in this image — the bright colours here are the nebula’s outskirts. This new picture was created from exposures through several different colour filters using the EMMI instrument [1] on the New Technology Telescope at ESO’s La Silla Observatory in Chile. The stars are shown in their natural colours, while light from glowing ionised hydrogen (shown here in red) and oxygen (shown in blue) is overlaid.

The star cluster NGC 2100 in the constellation of Dorado

The colours that appear in nebulae depend on the temperatures of the stars lighting them up. The hot young stars in the Tarantula Nebula, which lie in the super star cluster RMC 136, are above and to the right of this image, and are powerful enough to cause oxygen to glow [2] showing up as blue nebulosity in this picture. Below NGC 2100 the red glow indicates either that the outer reaches of the influence of the hot stars of RMC 136 has been reached, or that cooler, and older, stars, that are only able to excite hydrogen are the dominant influence in this region. The stars that make up NGC 2100 are older and less energetic, and hence have little or no nebulosity associated with them.

The star cluster NGC 2100 in context

Star clusters are groups of stars that formed around the same time from a single cloud of gas and dust. The stars with the most mass tend to form in the centre of the cluster, while those with less mass dominate the outer regions. This, along with the greater number of stars concentrated in the centre, makes the middle of the cluster brighter than the outer regions.

Zooming in on the star cluster NGC 2100 in the Large Magellanic Cloud

NGC 2100 is an open cluster, which means its stars are relatively loosely bound by gravity. These clusters have a lifespan measured in tens or hundreds of millions of years, as they eventually disperse through gravitational interaction with other bodies. Globular clusters, which look similar to the untrained eye, contain many more older stars and are much more tightly bound, and so have far longer lifespans: many globular clusters have been measured to be almost as old as the Universe itself. So while NGC 2100 might be older than its neighbours in the Large Magellanic Cloud, it is still a youngster by the standards of star clusters.

Data for this image of the under-appreciated young cluster were selected from the depths of ESO’s data archives by Hidden Treasures entrant David Roma as part of the astrophotography competition held by ESO in 2010 [3].

Notes:

[1] EMMI stands for ESO Multi Mode Instrument. It is both a camera for imaging and a spectrograph.

[2] Most of the glow from oxygen comes from oxygen atoms that have lost two electrons. This strong emission is very common in nebulae but was mysterious to early astronomical spectroscopists and was initially thought to be coming from a new element given the name Nebulium.

[3] 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. To find out more about Hidden Treasures, visit http://www.eso.org/public/outreach/hiddentreasures/.

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 two survey telescopes. VISTA works in the infrared and is the world’s largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 40-metre-class European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become “the world’s biggest eye on the sky”.

Links:

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

    David Roma’s Hidden Treasures image: http://www.flickr.com/photos/55944793@N02/5178599427/in/pool-1562202@N22/

Images, Text, Credit: ESO / IAU and Sky & Telescope / Video: ESO / R. Gendler / N. Risinger (skysurvey.org). Music: John Dyson (from the album Moonwind).

Cheers, Orbiter.ch

mardi 6 septembre 2011

NASA Spacecraft Images Offer Sharper Views Of Apollo Landing Sites














NASA - Lunar Reconnaissance Orbiter (LRO) patch / NASA - Apollo Program logo.

Sept. 6, 2011

NASA's Lunar Reconnaissance Orbiter (LRO) captured the sharpest images ever taken from space of the Apollo 12, 14 and 17 landing sites. Images show the twists and turns of the paths made when the astronauts explored the lunar surface.

At the Apollo 17 site, the tracks laid down by the lunar rover are clearly visible, along with the last foot trails left on the moon. The images also show where the astronauts placed some of the scientific instruments that provided the first insight into the moon's environment and interior.

"We can retrace the astronauts' steps with greater clarity to see where they took lunar samples," said Noah Petro, a lunar geologist at NASA's Goddard Space Flight Center in Greenbelt, Md., who is a member of the LRO project science team.

Apollo 17, LRO image released today (image 1)

Apollo 17, LRO image released in 2009 (image 2)

The first image was released today; the second image is a zoom-in on an LRO image released in 2009. LRO was moved into a lower orbit to capture the new image. The images do not line up perfectly because of differences in lighting conditions, angle of the LRO Camera, and other variables. Image brightness and contrast have been altered to highlight surface details. (Credit: NASA's Goddard Space Flight Center/ASU).

All three images show distinct trails left in the moon's thin soil when the astronauts exited the lunar modules and explored on foot. In the Apollo 17 image, the foot trails, including the last path made on the moon by humans, are easily distinguished from the dual tracks left by the lunar rover, which remains parked east of the lander.

Apollo 17 area by LRO

"The new low-altitude Narrow Angle Camera images sharpen our view of the moon's surface," said Arizona State University researcher Mark Robinson, principal investigator for the Lunar Reconnaissance Orbiter Camera (LROC). "A great example is the sharpness of the rover tracks at the Apollo 17 site. In previous images the rover tracks were visible, but now they are sharp parallel lines on the surface."

At each site, trails also run to the west of the landers, where the astronauts placed the Apollo Lunar Surface Experiments Package (ALSEP) to monitor the moon's environment and interior. This equipment was a key part of every Apollo mission.

It provided the first insights into the moon's internal structure, measurements of the lunar surface pressure and the composition of its atmosphere. Apollo 11 carried a simpler version of the science package.

 Apollo 12, LRO image released today (image 1)

Apollo 12, LRO image released in 2009 (image 2)

The first image was released today; the second image is a zoom-in on an LRO image released in 2009. LRO was moved into a lower orbit to capture the new image. The images do not line up perfectly because of differences in lighting conditions, angle of the LRO Camera, and other variables. Image brightness and contrast have been altered to highlight surface details. (Credit: NASA's Goddard Space Flight Center/ASU).

One of the details that shows up is a bright L-shape in the Apollo 12 image. It marks the locations of cables running from ALSEP's central station to two of its instruments. Although the cables are much too small for direct viewing, they show up because they reflect light very well.
 Apollo 12 area by LRO

The higher resolution of these images is possible because of adjustments made to LRO's orbit, which is slightly oval-shaped or elliptical. "Without changing the average altitude, we made the orbit more elliptical, so the lowest part of the orbit is on the sunlit side of the moon," said Goddard's John Keller, deputy LRO project scientist. "This put LRO in a perfect position to take these new pictures of the surface."


Image above: The paths left by astronauts Alan Shepard and Edgar Mitchell on both Apollo 14 moon walks are visible in this image. (At the end of the second moon walk, Shepard famously hit two golf balls.) The descent stage of the lunar module Antares is also visible. (Credit: NASA's Goddard Space Flight Center/ASU).

The maneuver lowered LRO from its usual altitude of approximately 31 miles (50 kilometers) to an altitude that dipped as low as nearly 13 miles (21 kilometers) as it passed over the moon's surface. The spacecraft has remained in this orbit for 28 days, long enough for the moon to completely rotate. This allows full coverage of the surface by LROC's Wide Angle Camera. The cycle ends today when the spacecraft will be returned to its 31-mile orbit.

"These images remind us of our fantastic Apollo history and beckon us to continue to move forward in exploration of our solar system," said Jim Green, director of the Planetary Science Division at NASA Headquarters in Washington.


Video above: NASA Goddard's Dr. Noah Petro discusses the significance of the new Apollo images from LRO. (Credit: Chris Smith, NASA's Goddard Space Flight Center).

LRO was built and managed by Goddard. Initial research was funded by the Exploration Systems Mission Directorate at NASA Headquarters. In September 2010, after a one-year successful exploration mission, the mission turned its attention from exploration objectives to scientific research in NASA's Science Mission Directorate.

To learn more about LRO, visit: http://www.nasa.gov/lro

Related Links:

Apollo Revisited: More images of Apollo sites from LRO: http://www.nasa.gov/mission_pages/apollo/revisited/index.html

Additional imagery related to this story from ASU's LROC website: http://lroc.sese.asu.edu/news/?archives/454-Skimming-the-Moon.html

Images, (mentioned), Video (mentioned), Text, Credit: NASA's Goddard Space Flight Center / Nancy Neal-Jones / Steve Cole.

Greetings, Orbiter.ch

Cleaning up with space tech








Aerospace Engineering - Technology Transfer.

6 September 2011

There’s just about nowhere that state-of-the-art space technologies cannot reach – from the martian atmosphere to those hard-to-clean spots under the couch. The search for space dust is giving us cleaner homes.

Just ask Heinrich Iglseder, the Austrian scientist who created a technique to study dust in space that is now being used in a super-efficient Miele household vacuum cleaner.

Space dust coming off comet 73P-Schwassmann–Wachmann

He invented a detector to measure interstellar dust’s chemical composition, speed and direction. It was sent into space three times as part of Japanese and US–German space missions. Thanks to his device, these missions identified ‘dust tails’ in space, where dust was concentrated at levels 100 to 1000 times higher than usual.

This is important to know because high-speed space dust can seriously damage satellite parts such as solar cells.

Iglseder and dust detector on Bremsat

But there are other reasons to study space dust. “Interstellar particles are the seeds for human biological life,” explained Dr Iglseder.

Dust is a health problem

Dust detector on Japanese Nozomi

Here on Earth, dust – particularly the super-fine particles generated from human activities like diesel engine combustion – can have a deeply negative effect on people’s health.

“I have friends suffering from allergies,” Dr Iglseder said. “They came to me and said, 'can’t you do something about this problem?'”

As a result, he started looking into ways to reduce dust in people’s homes, and the biggest problem he found was the carpets.

“Poisons like lead and cadmium, toxic particles and carcinogens accumulate in carpets. To get a hygienic environment, it’s absolutely necessary to clean the floors well.”

Space dust sensor for vacuum cleaning

So Dr Iglseder adapted his space sensor for a regular vacuum cleaner. Coloured lights let you know if the area you are cleaning is actually dust-free, or still needs more work.

Miele incorporated this Allergotec Hygiene Sensor into their Medicair vacuum cleaner, geared towards people with allergies.

“I think it’s really practical,” said Miele press spokeswoman Reinhild Portmann of the straight-from-space technology.

Clean with space dust sensor

“You have an objective measurement of how clean the floors are.”

Frank M. Salzgeber, Head of the ESA Technology Transfer Programme Office, adds: “To foster more of those kinds of transfers in Austria from space to non-space, we are now teaming up with the Austrian Research Promotion Association to establish the national Austrian Technology Transfer Programme initiative.”

“I expect that we will soon find more exciting projects and innovative transfers from Austrian companies.”

‘Green’ for all dust taken

Dr Igelseder admits that it’s his wife who does the lion’s share of the vacuuming around their house – but says she likes the sensor.

Green light for dust-free

Mounted in the vacuum cleaner manifold, his sensor checks the amount of dust passing. ‘Traffic lights’ on the nozzle show red for ‘still too much dust’, orange for ‘medium’, yellow for ‘slightly’ and green for ‘no more dust’.

“With the sensor, she can see that, in some areas, it’s clean after one or two strokes. In other areas, five or six strokes might be needed. She tells me she wouldn’t like to clean without the sensor now.”

More on ESA’s Technology Transfer Programme and its National Technology Transfer Initiative on ESA TTP website: http://www.esa.int/ttp

Related links:

Space technology to strengthen Austrian industry: http://www.esa.int/SPECIALS/TTP2/SEM6SMUTTRG_0.html

National Technology Transfer Initiatives: http://www.esa.int/SPECIALS/TTP2/SEMA8ESMTWE_0.html

Technology Transfer Programme Office: http://www.esa.int/SPECIALS/TTP2/

ESA Technology: http://www.esa.int/SPECIALS/Technology/index.html

Images, Text, Credits: NASA / ESA / JPL / H. Weaver (APL / JHU) / M. Mutchler and Z. Levay (STScI) / H. Iglseder.

Best regards, Orbiter.ch

lundi 5 septembre 2011

ESA - André makes a PromISSe












ESA - PromISSe mission logo.

5 September 2011

All the pieces are coming together for the next long mission by a European astronaut. Now it has a name and logo. ESA today revealed the name of André Kuipers' mission: PromISSe.

ESA called on citizens of its member states last June to propose a name for André’s mission and received more than 200 proposals in just a month. Surprisingly, they also came from Slovenia, Australia, India, Mexico and Argentina.

The judges weighed the eligible entries from a wide range of people, from a 13-year-old Italian to an 82-year-old Dutchman.

The vast majority came from the Netherlands – André’s home country – and the winner is one of those.

Logo presentation at EAC today

It was not a declared intent to embed the abbreviation of the International Space Station in the logo, but both the design and the chosen name have it.

PromISSe represents ‘Programme for Research in Orbit Maximising the Inspiration from the Space Station for Europe’, explained the winner, Wim Holwerda, a 61-year-old Dutchman.

Wim believes that the name “symbolises the promise space exploration poses to the future of our planet and humankind, as well as the role Europe can play in it.”

Three powerful messages are integrated in PromISSe: the crucial role of scientific research, a greater use of the Space Station and the inspirational value of ESA space programmes.

An inspirational mission patch

The logo for the mission features the Space Station orbiting Earth, accompanied by three icons and six stars.

André aboard ISS in 2006

The PromISSe name crowns a circular design belted with orange cords, while the International Space Station acronym is highlighted in the same colour to bring out the Dutch participation in the mission.

The core of the logo is a globe free of national borders. A silhouette of the ISS is shown circling Earth, about to fly over Europe.

The icons on the left represent the mission’s three crucial elements: science, technology and education.

The globe stands for a knowledge-based society focused on our planet. The electronic circuit denotes technology. The conical laboratory flask illustrates scientific research.

André Kuipers with Don Pettit and Oleg Kononeko at the GCTC

The six stars represent the six crewmembers, the six months that André will stay in space and, as the stars are similar to those on the EU flag, the European character.

André will work on the Station as a member of Expedition 30. His launch is expected in early December, but the specific date will be selected after the Soyuz launch vehicle is returned to service following the Progress loss in August.

Related links:

DELTA mission: http://www.esa.int/SPECIALS/Delta_Mission/index.html

DELTA: Photo gallery: http://www.esa.int/esa-mmg/mmg.pl?mission=Delta+(Astronaut+Kuipers)&type=I

Images, Text, Credits: ESA / S. Corvaja / A. Schepers.

Greetings, Orbiter.ch