mardi 19 février 2013

Engineers Design Plant Habitat For Space Station












ISS - International Space Station patch.

February 19, 2013

 International Space Station

Some of the research on the International Space Station focuses on meeting the needs of long-term spaceflight to destinations such as asteroids or Mars. A group of engineers at NASA's Kennedy Space Center in Florida is developing a plant habitat with a large growth chamber to learn the effects of long-duration microgravity exposure to plants in space.

Through most of Kennedy's history, the space center has focused on receiving, processing and launching vehicles developed at other centers. Design projects such as the plant habitat give people at the Florida spaceport an opportunity to further use their extensive knowledge base in preparing flight hardware.

"This is the first Kennedy-led space station payload of this magnitude," said Bryan Onate, Plant Habitat Project manager in the ISS Ground Processing and Research Directorate. "We're using in-house expertise to develop the plant habitat to go on an EXPRESS rack in the station's Destiny laboratory. It will provide a large, enclosed, environmentally-controlled chamber designed to support commercial and fundamental plant research onboard the space station."

The plant habitat is configured as a payload that will be mounted on a standard Expedite the Processing of Experiments to Space Station, or EXPRESS, rack. The multipurpose payload rack system stores and supports research and science experiments across many disciplines by providing structural interfaces, power, data, cooling, water and other needs to operate science payloads in orbit.


Image above: Some of the research on the International Space Station is already focusing on meeting the needs of long-term spaceflights beyond low-Earth orbit. During Expedition 29 in 2011, Russian cosmonaut Sergei Volkov checks the progress of new growth in the Rastenia investigation aboard the space station. (NASA).

The compact facility is about 21 inches high, 36 inches wide and 24 inches deep and would use about 735 watts of power.

"NASA is conducting plant research aboard the space station because during future long-duration missions, life in space may depend on it," Onate said.

As NASA plans missions beyond low-Earth orbit, relying on plant growth aboard a spacecraft will play an important role.

"The ability of plants to provide high quality science within a tightly closed system, a source of food and recycle carbon dioxide into breathable oxygen may prove crucial for astronauts and add to the body of knowledge as they live in space for months at a time," he said.

Onate explained that most of the experiments conducted on the space station are developed by principal investigators from universities or other research institutions.

"The plant habitat is an effort to attract a broader audience of principle investigators that need a large growth area for a long duration," he said. "In order to expedite this capability on the space station, we have contracted with Orbital Technologies Corp. to help us design, fabricate and certify the plant habitat for flight."

Based in Madison, Wis., Orbital Technologies Corp., better known as ORBITEC, is a leading subsystems integrator and high-technology development company.

The plant habitat's design includes the ability to control temperature, humidity, carbon dioxide levels and lighting.

"Lighting is an important part of plant growth," Onate said. "We're using LEDs in this payload. Our experience shows that the LEDs work well in plant growth experiments in our labs here at Kennedy."


Image above: NASA is using in-house expertise to develop this plant habitat to go on an EXPRESS rack, like the one pictured above, in the International Space Station's Destiny laboratory. It will provide a large, enclosed, environmentally controlled chamber designed to support commercial and fundamental plant research aboard the space station. (NASA).

Within the plant habitat there is a tray called a science carrier that will hold various types of plants. The science carrier is a removable and reconfigurable tray that will provide the primary structural support and final water delivery to the root-zone for in-orbit plant growth experimentation.

The science carrier consists of a structural element, a water delivery mechanism, and a standard interface plate that will provide instrumentation support as part of the basic plant habitat capabilities. The carrier also will provide additional instrumentation interfaces for other experiment-specific measurement data required to allow investigators to extend the habitat's basic capabilities.

"Our design will allow principal investigators to modify the carriers depending on the type of plants they want to grow and the kind of experiments they have in mind," Onate said.

Plant habitat investigations can use the microgravity of space and can run 30, 60 or 90 days depending on the nature of the research.

"These trays will have a system of tubes allowing astronauts conducting the experiment to inject water and other plant nutrients into the media supporting plant growth," Onate said.

One of the next steps for the plant habitat is a preliminary design review in February. During the review, engineers will report on how the project is progressing to ensure the design meets system requirements within acceptable risk and falls within schedule and budget constraints.

"One of the design challenges we're dealing with now is the physical size and power requirements for the plant habitat," Onate said. "Weight, volume and maximizing valuable space station resources are always an important consideration for any payload designed for spaceflight."

"Launch of the Kennedy-designed plant habitat will likely go up on a SpaceX Dragon spacecraft," Onate said. "It is targeted for launch in December 2015."

International Space Station: http://www.nasa.gov/mission_pages/station/main/index.html

Expedite the Processing of Experiments to Space Station, or EXPRESS: http://www.nasa.gov/mission_pages/station/research/experiments/EXPRESS_Racks.html

Images (mentioned), Text, Credit: NASA's Kennedy Space Center/ Bob Granath.

Greetings, Orbiter.ch

Russia asteroid impact: ESA update and assessment‏











Asteroid Watch.

19 February 2013

The first firm details of the 15 February asteroid impact in Russia, the largest in more than a century, are becoming clear. ESA is carefully assessing the information as crucial input for developing the Agency’s asteroid-hunting effort.

At 03:20 GMT on 15 February, a natural object entered the atmosphere and disintegrated in the skies over Chelyabinsk, Russia.

Asteroid trace over Chelyabinsk, Russia, on 15 February 2013

Extensive video records indicate a northeast to southwest path at a shallow angle of 20° above the horizontal. The entry speed is estimated at around 18 km/s – more than 64 000 km/h.

According to calculations by Peter Brown at the University of Western Ontario, Canada, drawing on extremely low-frequency sound waves detected by a global network, the object is estimated to have been about 17 m across with a mass of 7000–10 000 tonnes when it hit atmosphere.

It exploded with a force of nearly 500 kilotons of TNT – some 30 times the energy released by the Hiroshima atomic bomb – around 15–20 km above the ground.

With our current understanding of near-Earth objects, events of this magnitude are expected once every several of tens to 100 years.

Questions and answers with ESA's near-Earth object team

Nicolas Bobrinsky, Head of ESA’s Space Situational Awareness (SSA) programme, and Detlef Koschny, responsible for the programme’s Near-Earth Object activity, responded to questions about the event.

Orbit around Sun

- Was this event related to the predicted flyby of asteroid 2012 DA14, which passed Earth at 19:27 GMT that same day at just 28 000 km?

DVK: The trajectory, the location of entry into the atmosphere and the large time separation between the two events indicate that the Russian object was unrelated to 2012 DA14.

- What caused the damage on the ground? Did pieces hit people or buildings?

DVK: Many media reported that an airburst caused window breakage and some structural damage in downtown Chelaybinsk. Normally, some damage begins to occur at around five times normal air pressure at sea level. Widespread window damage is expected around 10–20 times this value.

As the explosion and fireball progressed along a shallow trajectory, the cylindrical blast wave would have propagated directly to the ground and would have been intense.

The terminal part of the explosion probably likely occurred almost directly over Chelyabinsk. This was perhaps the single greatest contributor to the blast damage.

Scientists have found fragments of the meteorite Chelyabinsk (in Russian)

We are waiting for confirmation from the Russian authorities that pieces of the object – bits of meteorite – have been found in the region. We’re unaware of any media reports of anyone or any structure being hit by any debris from the object itself.

Related links:

Space Situational Awareness: http://www.esa.int/Our_Activities/Operations/Space_Situational_Awareness2

Russian asteroid strike: http://orbiterchspacenews.blogspot.ch/2013/02/russian-asteroid-strike.html

Stranger in the night: space rock to make close Earth flyby: http://www.esa.int/Our_Activities/Operations/Stranger_in_the_night_space_rock_to_make_close_Earth_flyby

Asteroid 2012 DA14 - Near-Earth Asteroid Makes View Appearance: http://orbiterchspacenews.blogspot.ch/2013/02/asteroid-2012-da14-near-earth-asteroid.html

Spotting an ancient asteroid: http://www.esa.int/Our_Activities/Operations/Spotting_an_ancient_asteroid

SSA NEO Data Centre: http://neo.ssa.esa.int/

More information:

Centre for Planetary Science and Exploration: http://planetsci.uwo.ca/

Infrasound monitoring: http://www.ctbto.org/verification-regime/monitoring-technologies-how-they-work/infrasound-monitoring/

UNCOPUOS: http://www.oosa.unvienna.org/oosa/COPUOS/copuos.html

UNCOPUOS - 2013 session - presentations: http://www.unoosa.org/oosa/en/COPUOS/stsc/2013/presentations.html

Images, Video, Text, Credits: ESA / Alex Alishevskikh CC BY-SA 2.0 via http://www.flickr.com/photos/alexeya/ NASA / ROSCOSMOS TV / Russia 24.

Greetings, Orbiter.ch

The Patrouille Suisse will continue to exist












Swiss Air Force - Patrouille Suisse patch.

February 19, 2013

The outcry caused by the announcement of the "death" of the Swiss aerobatic team, the defense minister backtracked. But the aircraft will lose the Swiss colors.

The Swiss army will continue to have an aerobatic flight training, but not in red and white, said the defense minister in an interview. It would cost 50 million francs more each year to keep the F-5 Tiger aircraft currently used by the Patrouille Suisse, he said.

Actual colors of the Patrouille Suisse with F-5E Tiger II

In its previous announcement, he called the Patrouille Suisse of "Folklore" and claimed that his grounding was motivated by economic reasons. In reaction to these remarks, many politicians and citizens have exclaimed: "It is as bad to buy a plane that Gripen is Folklore".

Reactions to a possible suppression of the Patrouille Suisse surprised, says defense minister in an interview published Tuesday by the newspaper "Nordwestschweiz." "It has been clear for months with the shelved F-5 Tiger Patrouille Suisse no longer exist in its current form."

If Tiger F-5 were retained, the Air Force possesses three fleets after the planned purchase of Swedish Gripen: F/A-18, Gripen and the Tiger. According to the minister of defense, he "would cost 30 million francs more than today."

"We can not afford it." But the army will continue to have training in aerobatics. "We have planes and pilots trained accordingly. But we can not paint the Swiss cross on the devices. "

Problem of quantity
There is a problem of quantity, says the head of the Department of Defense (DDPS). The Air Force currently has 54 Tiger yet. Eleven of them made up the Patrouille Suisse. In the future, Switzerland will have more than 55 Gripen and F/A-18. "We can not do paint ten of them."

The defense minister said last week that the aerobatic formation of the Swiss army colors should disappear aviation landscape. He made the announcement at a meeting of the Committee of the security policy of the National Council.

F/A-18 Hornet in Patrouille Suisse, the question remains open

The question whether the Patrouille Suisse fly with Gripen or F/A-18 remains open, said the defense minister. The old Tiger could still fly two or three years. "But then it would definitely be finished."

Editor Note: there is actually a bigger problem of quantity, as I wrote in a previous article (see links at the end of the article), the performance of the Gripen are so inadequate that 3 Gripen to make the work of a Rafale, so to ensure all future missions with only 22 aircraft, the choice of the Rafale should win, it's a safe bet that the file will end in popular vote and in this case, the Gripen will be refused.

The Rafale, the best choice for Swiss Air Force!

Discover or read previous articles on this issue:

Choice of a new fighter aircraft of the Swiss Air Force: Description and comparison:
http://orbiterchspacenews.blogspot.ch/2013/01/choice-of-new-fighter-aircraft-of-swiss.html

Swiss Air Force - The Gripen saga continues ...:
http://orbiterchspacenews.blogspot.ch/2013/02/swiss-air-force-gripen-saga-continues.html

Patrouille Suisse: a boss flies to the rescue:
http://orbiterchspacenews.blogspot.ch/2013/02/patrouille-suisse-boss-flies-to-rescue.html

Images, Text, Credits: ATS / Swiss Air Force / Orbiter.ch Aerospace.

Best regards, Orbiter.ch

lundi 18 février 2013

Asteroid Steins' Hidden Gems












ESA - Rosetta Mission patch.

18 February 2013

 Steins revisited

ESA’s Rosetta spacecraft snapped images of asteroid Steins as it flew by the diamond-shaped asteroid on 5 September 2008, revealing a tiny world with a big history of collisions.

The images were taken by Rosetta’s Wide Angle Camera as the spacecraft flew within 800 km of the 5 km-wide asteroid, and later processed by amateur astronomer Ted Stryk to produce the image presented here.

By emphasising the shadows, the processing reveals high-contrast features, such as bright crater rims against their dark, shadowed interiors. However, this technique can also create some artifacts, such as the illusion of boulders protruding from the surface, that are not present in the raw data.

One striking feature is the gaping hole at the south pole (top in this image) of Steins – its largest impact crater at about 2 km wide and nearly 300 m deep. This crater is named ‘Diamond’ following the gem nomenclature chosen after the asteroid’s overall shape earned it the nickname ‘diamond in the sky’.

The circular crater in the centre of the asteroid as seen in this viewing angle is called Topaz and is about 650 m wide and 80 m deep.

A chain of several craters can be seen stretching from the asteroid’s north pole (bottom in this image) right up to Diamond crater.

So far, around 40 craters have been found, but the imposing Diamond crater likely influenced the appearance of the entire asteroid because the debris thrown out from this dramatic collision would have scattered over the surface, imprinting over other, older craters.

Rosetta spacecraft

Rosetta has since passed by asteroid Lutetia in July 2010 and is now in deep-space hibernation. It will wake up on 20 January 2014 and rendezvous with comet 67P/Churyumov–Gerasimenko in May 2014. A few months later, its Philae probe will separate to make the first controlled landing on a comet.

Comets are considered to be the primitive building blocks of the Solar System, and Rosetta will help scientists to learn more about their role in the evolution of our local cosmic neighbourhood.

More about:

Rosetta: http://www.esa.int/Our_Activities/Space_Science/Rosetta

Related link:

This image on Ted Stryk’s blog: http://planetimages.blogspot.nl/2012/04/steins-closest-approach.html

New science paper on Steins’ craters: http://www.sciencedirect.com/science/article/pii/S0019103512003272

Rosetta data archive: http://www.sciops.esa.int/index.php?project=PSA&page=rosetta

Rosetta in depth: http://sci.esa.int/rosetta

Images, Text, Credits: ESA / J. Huart / MPS for OSIRIS Team / MPS / UPD / LAM / IAA / RSSD / INTA / UPM / DASP / IDA; processing by T. Stryk.

Greetings, Orbiter.ch

samedi 16 février 2013

Patrouille Suisse: a boss flies to the rescue










Breitling Jet Team logo.

Feb. 16, 2013

"It is unacceptable that fifty years are destroyed for financial reasons after all small scale of a country," unworthy Thedy Schneider, Breitling boss.

Breitling is ready to repaint its jets and lend military pilots to continue the tradition

In response to the decision of the Swiss Minister of Defence, ending the Patrouille Suisse in 2016, a watchmaker and instruments manufacturer for aviation, proposes to his own squadron of free L-39 Albatros available for military pilots, even the paint colors of Switzerland.

Patrouille Suisse logo painted on actual Northrop F-5E Tiger II

This case of replacement of the Northrop F-5E Tiger II from the Swiss Air Force, the controversy continues, with the grounding of the Patrouille Suisse, after reviewing the file, many questions remain about the funding that Gripen remains unclear (Final invoice and funding from the Swiss Government and Swedish Government).

Discover or read previous articles on this issue:

Choice of a new fighter aircraft of the Swiss Air Force: Description and comparison:
http://orbiterchspacenews.blogspot.ch/2013/01/choice-of-new-fighter-aircraft-of-swiss.html

Swiss Air Force - The Gripen saga continues ...:
http://orbiterchspacenews.blogspot.ch/2013/02/swiss-air-force-gripen-saga-continues.html

Breitling Jet Team:
http://www.breitling-jet-team.com/

Images, Text, Credits: Breitling Jet Team / Patrouille Suisse / Orbiter.ch Aerospace.

Cheers, Orbiter.ch

vendredi 15 février 2013

Asteroid 2012 DA14 - Near-Earth Asteroid Makes View Appearance











Asteroid Watch.

Feb. 15, 2013

 Asteroid 2012 DA14 as Seen from Siding Spring, Australia

This animated set of images, from the telescope known as the iTelescope.net Siding Spring Observatory, shows asteroid 2012 DA14 as the streak moving from left to right in the field of view. The images were taken around 9:40 a.m. PST (12:40 p.m. EST, or 17:40 UTC) on Feb. 15, 2013. The exposure time was 5 seconds long. Image courtesy of E. Guido/N. Howes/Remanzacco Observatory.

These are some of many images that may be taken of the asteroid during its close - but safe - encounter with Earth. It will be observed by numerous optical observatories worldwide in an attempt to determine its rough shape, spin rate and composition. NASA scientists will use NASA's Goldstone Solar System Radar, located in California's Mojave Desert, to take radar images of the asteroid to determine its precise size and shape on Feb. 16, 18, 19 and 20. The NASA Near Earth Object Observation (NEOO) Program will continue to track the asteroid and predict its future orbit.


Diagram depicting the passage of asteroid 2012 DA14 through the Earth-moon system on Feb. 15, 2013. Image credit: NASA/JPL-Caltech.

Asteroid 2012 DA14 is about 150 feet (45 meters) in diameter. It is expected to fly about 17,200 miles (27,000 kilometers) above Earth's surface at the time of closest approach, which is about 11:25 a.m. PST (2:25 p.m. EST) on Feb. 15. This distance is well away from Earth and the swarm of low Earth-orbiting satellites, including the International Space Station, but it is inside the belt of satellites in geostationary orbit (about 22,200 miles, or 35,800 kilometers, above Earth's surface.) The flyby of 2012 DA14 is the closest-ever predicted approach to Earth for an object this large.

Gingin Observatory Spots Near-Earth Asteroid at Closest Approach

Video above: Observatory in Australia around the time of its closest approach, 11:24:42 a.m. PST (2:24:42 p.m. EST, or 19:24:24 UTC), Feb. 15, 2013.

At that time, the asteroid was about 17,150 miles (27,600 kilometers) above Earth's surface. The asteroid appears streaked because the telescope was focused on the stars while the asteroid passed through the field of view. Images courtesy of Gingin Observatory/Tonello.

Outbound Near-Earth Asteroid, as Seen from Spain

Video above: This set of images from the La Sagra Sky Survey, operated by the Astronomical Observatory of Mallorca in Spain, shows the passage of asteroid 2012 DA14 shortly after its closest – and safe -- approach to Earth. The images were taken around 12:59 p.m. PST (3:59 p.m. EST, or 20:59 UTC) on Feb. 15, 2013. The images have been sped up 10 times.

In the last set of images, the fainter object that passes near the top of the field of view is a satellite or another asteroid. Images courtesy of La Sagra Sky Survey.

The NASA Near Earth Object Observation (NEOO) Program detects and tracks asteroids and comets passing close to Earth using ground- and space-based telescopes. The network of projects supported by this program, commonly called "Spaceguard," discovers these objects, characterizes a subset of them and plots their orbits to determine if any could be potentially hazardous to our planet.

The Near-Earth Object Program Office at JPL manages the technical and scientific activities for NASA's Near-Earth Object Observation Program of the Science Mission Directorate in Washington. JPL is a division of the California Institute of Technology in Pasadena. The NEOO Program Office performs more precise orbit determination on the objects, and predicts whether any will become an impact hazard to the Earth, or any other planet in the solar system.

More information is available at: http://www.nasa.gov/topics/solarsystem/features/asteroidflyby.html

Asteroid and Comet Watch site: http://www.nasa.gov/mission_pages/asteroids/main/index.html

Images (mentioned), Videos (mentioned), Text, Credit: NASA.

Best regards, Orbiter.ch

Russian Asteroid Strike











Asteroid Watch.

15 February 2013

A space rock a few metres across exploded in Earth’s atmosphere above the city of Chelyabinsk, Russia today at about 03:15 GMT. The numerous injuries and significant damage remind us that what happens in space can affect us all.

Chelyabinsk asteroid vapour trail

While precise information on the size, mass and composition of the object are yet to be confirmed, videos show a fireball and explosion consistent with an asteroid up to a few metres in size exploding in the atmosphere, possibly several to ten kilometres above the surface.

 Slow Motion Moment of  Meteorite Explosion in Russia

In this type of event, if the explosion altitude is less than 10 km or so, the resulting shockwave can cause damage on the ground, such as shattering windows. Debris from the object may be found later.

“Current information, which is not yet complete nor confirmed, points to a small asteroid,” said Detlef Koschny, Head of Near-Earth Object activity at ESA’s Space Situational Awareness (SSA) programme office.

Chelyabinsk, location of the asteroid strike

“There is no way it could have been predicted with the technical means available today. What can be said with near certainty is that this object has no connection with asteroid 2012 DA14.”

Asteroid 2012 DA14 made a close flyby of Earth at 19:27 GMT (20:27 CET) today.

Finding objects that pass close to our planet and are large enough to do damage if they enter our atmosphere is a major goal of ESA’s SSA programme.

In addition to conducting its own sky searches using ESA's Optical Ground Station in Tenerife, Spain, SSA is partnering with existing European and international asteroid survey activities. 

It also sponsors astronomer groups in Europe, supporting surveys carried out with their own equipment or allocating observation time on its Tenerife telescope. The office also provides access to orbit predictions, close flyby details and related data via its technical website at http://neo.ssa.esa.int

 Asteroid 2012 DA14 size comparative

“Today’s event is a strong reminder of why we need continuous efforts to survey and identify near-Earth objects,” said Thomas Reiter, ESA’s Director of Human Spaceflight and Operations.

“Our SSA programme is developing a system of automated optical telescopes that can detect asteroids and other objects in solar orbits.”

 In cooperation with survey efforts worldwide, ESA’s goal is to spot near-Earth objects larger than 40 m at least three weeks before closest approach to our planet.

To achieve this, ESA, European industry and partner agencies are developing a system of automated 1 m-diameter telescopes capable of imaging the complete sky in one night.

In addition to Russian media, who reported immediately, all media worldwide have published images of notable damage around Chelyabinsk, and reports also mention numerous casualties.

“Our most sincere sympathies are with those suffering injury and property loss due to this event in Russia,” added Thomas Reiter.

Related links:

Space Situational Awareness: http://www.esa.int/Our_Activities/Operations/Space_Situational_Awareness2

Stranger in the night: space rock to make close Earth flyby: http://www.esa.int/Our_Activities/Operations/Stranger_in_the_night_space_rock_to_make_close_Earth_flyby

Spotting an ancient asteroid: http://www.esa.int/Our_Activities/Operations/Spotting_an_ancient_asteroid

SSA NEO Data Centre: http://neo.ssa.esa.int/

Near Earth Objects - Dynamic Site: http://newton.dm.unipi.it/neodys/

Images, Video, Text, Credits: ESA / Eumetsat / RT / Youtube.

Greetings, Orbiter.ch