dimanche 23 novembre 2014

Expedition 42 Trio Launches on Time to Station












ROSCOSMOS - Soyuz TMA-15M Mission patch.

November 23, 2014

Expedition 42/43 Launches to the ISS

The Soyuz TMA-15M launched from the Baikonur Cosmodrome in Kazakhstan to the International Space Station at 4:01 p.m. EST (3:01 a.m. on Nov. 24 Baikonur time). Terry Virts of NASA, Anton Shkaplerov of the Russian Federal Space Agency (Roscosmos) and Samantha Cristoforetti of the European Space Agency now are safely in orbit.


Image above: The Soyuz TMA-15M launches on time from the Baikonur Cosmodrome at 4:01 p.m. EST. Credit: NASA TV/Screen capture: Orbiter.ch Aerospace.

Virts, Shkaplerov and Cristoforetti will dock with the station’s Rassvet module at 9:53 p.m. Welcoming them aboard will be the current station residents, Expedition 42 Commander Barry “Butch” Wilmore of NASA and Alexander Samoukutyaev and Elena Serova of Roscosmos. Wilmore, Samoukutyaev and Serova arrived at the space station in September aboard their Soyuz TMA-14M spacecraft and will remain aboard until March 2015.

Soyuz TMA-15M crew on way to ISS. Credit: NASA TV/Screen capture: Orbiter.ch Aerospace

Some of the cargo flown aboard this Soyuz will be used in research investigations that are either ongoing or planned aboard the International Space Station. Items such as questionnaires will be delivered to obtain in-flight data about crew member characteristics, such as day-to-day changes in health or incidence of pain or pressure in microgravity. One such investigation is Space Headaches which uses questionnaires to collect information about the prevalence and characteristics of crew members’ headaches in microgravity. This information is used to develop future countermeasures for headaches often caused by intracranial pressure change.

Soyuz TMA spacecraft

Read more about Space Headaches: http://www.nasa.gov/mission_pages/station/research/experiments/181.html

Read more about intracranial pressure change: http://www.nasa.gov/content/it-s-all-in-your-head-nasa-investigates-techniques-for-measuring-intracranial-pressure/

Researchers will also use biological sample kits delivered by the Soyuz spacecraft to obtain samples of blood, saliva or urine. The ongoing collection of biological samples from crew members help scientists determine if immune system impairment caused by spaceflight increases the possibility for infection or poses a significant health risk during life aboard the space station.

For more information about the International Space Station (ISS), visit: http://www.nasa.gov/mission_pages/station/main/index.html

Images, Video, Text, Credits: NASA/NASA TV.

Best regards, Orbiter.ch

vendredi 21 novembre 2014

Freon leak occurs at Russian segment of ISS, crew not in danger












ISS - International Space Station patch.

November 21, 2014

NASA’s office at Russian Mission Control near Moscow said it had no details of the situation at the moment.

International Space Station (ISS)

According to NASA’s official blog a leak of the khladon gas (Freon-218), used in the air conditioning system has occurred at the Zvezda service module of the Russian segment of the International Space Station (ISS).

“Cosmonauts Samokutyaev and Serova performed steps to release pressure in the Russian segment’s air conditioner system by venting khladon gas (Freon 218) overboard. However, several of the quick disconnects that were actuated during the procedure exhibited leaks. As a result, the Khladon was vented into the cabin instead.

Russian segment of ISS

The quantity released was approximately 100 g, which results in a density of 117 mg/m3 over the volume of ISS, which was below the stated ISS zero risk flight rule limit of 150 mg/m3. As part of nominal air scrubbing process, the Russian Air Purification System and the USOS Trace Contaminant Control System (TCCS) will remove residual Khladon from the atmosphere,” the NASA blog said.

NASA’s office at Russian Mission Control near Moscow said it had no details of the situation at the moment. Russian specialists were holding a conference to discuss the incident. Mission Control has offered no comment so far.

For more information about the International Space Station (ISS), visit: http://www.nasa.gov/mission_pages/station/main/index.html

Images, Text, Credits: ENERGIA/NASA/TASS.

Greetings, Orbiter.ch

Magnetospheric Multiscale to Launch Four Spacecraft












NASA - Magnetospheric Multiscale (MMS) patch.

November 21, 2014

In March of 2015, an unprecedented NASA mission will launch to study a process so mysterious that no one has ever directly measured in space. To create the first-ever 3-dimensional maps of this process, a process called magnetic reconnection, which occurs all over the universe, the Magnetospheric Multiscale, or MMS, mission uses four separate spacecraft equipped with ultra high speed instruments.

Launching four satellites into space simultaneously is a complicated process. In addition, each spacecraft has several booms that will unfold and extend in space once on orbit. A launch and deployment with so many moving parts is meticulously planned.

NASA Releases Narrated Animation of MMS Launch and Deploy 

How Will the 4 MMS Spacecraft Launch and Deploy?

Video above: A narrated animation of how NASA's Magnetospheric Multiscale, or MMS, mission – which consists of four separate spacecraft -- will launch into space. Video Credit: NASA/Goddard.

Watch the video to get a sneak preview of how MMS will make this journey: The four spacecraft are housed in a single rocket on their trip into space. One by one, each ejects out, before moving into a giant pyramid-shaped configuration. Next each spacecraft deploys its booms.

Once in orbit, MMS will fly through regions near Earth where this little-understood process of magnetic reconnection occurs. Magnetic reconnection happens in thin layers just miles thick, but can tap into enough power at times to create gigantic explosions many times the size of Earth.

Artist's view of NASA's Magnetospheric Multiscale spacecraft constellation

Reconnection happens when magnetic field lines explosively realign and release massive bursts of energy, while hurling particles out at nearly the speed of light in all directions. Magnetic reconnection powers eruptions on the sun and – closer to home – it triggers the flow of material and energy from interplanetary space into near-Earth space. The MMS orbit will carry the four spacecraft through reconnection regions near Earth, using this nearby natural laboratory to better understand how reconnection occurs everywhere in space.

For more information about MMS, visit: http://www.nasa.gov/mms

Image, Video (mentioned), Text, Credits: NASA's Goddard Space Flight Center/Karen C. Fox.

Greetings, Orbiter.ch

Hubble Sees a Spiral in a Furnace











NASA - Hubble Space Telescope patch.

November 21, 2014


This Hubble image is a snapshot of NGC 986 — a barred spiral galaxy discovered in 1828 by James Dunlop. This close-up view of the galaxy was captured by Hubble’s Wide Field and Planetary Camera 2 (WFPC2).

NGC 986 is found in the constellation of Fornax (The Furnace), located in the southern sky. NGC 986 is a bright, 11th-magnitude galaxy sitting around 56 million light-years away, and its golden center and barred swirling arms are clearly visible in this image.

Barred spiral galaxies are spiral galaxies with a central bar-shaped structure composed of stars. NGC 986 has the characteristic S-shaped structure of this type of galactic morphology. Young blue stars can be seen dotted amongst the galaxy’s arms and the core of the galaxy is also aglow with star formation.

Hubble orbiting Earth

To the top right of this image the stars appear a little fuzzy. This is because a gap in the Hubble data was filled in with data from ground-based telescopes. Although the view we see in this filled in patch is accurate, the resolution of the stars is no match for Hubble’s clear depiction of the spiral galaxy.

For images and more information about Hubble, visit: http://www.nasa.gov/hubble and http://hubblesite.org/ and http://www.spacetelescope.org/

Image, Video, Text, Credits: NASA/ESA.

Cheers, Orbiter.ch

Researchers Advance 'Quantum Teleportation'












NASA patch.

November 21, 2014

The world at the quantum level, at the scale of particles too small for the eye to see, is very strange. It's possible, for instance, to have two particles that are "entangled" -- that is, they function as if they were connected, even if they are many miles away from each other.

New research co-authored by Francesco Marsili, microdevices engineer at NASA's Jet Propulsion Laboratory, Pasadena, California, makes use of this phenomenon in a technological advancement published in the journal Nature Photonics. Researchers succeeded in teleporting information about the quantum state of a photon, a particle of light, over 15.5 miles (25 kilometers) of optical fiber to a crystal "memory bank," setting a new record of distance traveled in this manner. The previous record in optical fiber was 3.7 miles (6 kilometers). This complex phenomenon is called "quantum teleportation."


Cartoon above: Quantum mechanics can be confusing. This cartoon helps explain recent research by NASA Jet Propulsion Laboratory, University of Geneva and NIST. Credits: NASA/JPL.

The research could have implications for cryptography, which involves transmitting information securely, including communications between Earth and spacecraft.

"We can imprint the state of a system on another system, even when the two are far apart," Marsili said. "Using this effect in communications could help in building an intrinsically secure space communication network -- i.e., communication channels that cannot be hacked."

Marsili and colleagues at the National Institute of Standards and Technology (NIST), Boulder, Colorado, developed devices that can detect single particles of light, called photons.

"It's hard to detect a single photon, so you need to make a sensitive detector," he said. "Here at JPL, in collaboration with NIST, we developed the most sensitive detector in the world."

How quantum teleportation works is complicated, but an analogy for the principle behind it may help: Let's say there are two people, Alice and Bob. Alice wants Bob to have a photon that's in the same "state" as her photon, which we'll call photon P. For the sake of this analogy, we'll pretend that the "state" is a color, and photon P is yellow. A third person named Charlie sends out two entangled photons, photon A to Alice and photon B to Bob, which behave as if they are part of the same whole. Both of these photons start out as blue.

"In an entangled system, each part is connected to one another in a fundamental way, such that any action performed on a part of the entangled system has an effect on the whole entangled system," Marsili said.

Alice's two photons, P, which is yellow, and A, which is blue, "collide." Alice measures the photons as they annihilate one another. Although P and A are destroyed in the crash, P's yellow color is preserved. Because photon A and photon B are entangled, the yellow color is "teleported" to B. But in order to get photon B to become yellow, as photon P originally was, Alice needs to send Bob two bits of information to B the "classical" way -- for example, by sending pulses of light over an optical fiber.


Image above: This image shows crystals used for storing entangled photons, which behave as though they are part of the same whole. Scientists used these crystals in their process of teleporting the state of a photon across more than 15 miles (25 kilometers) of optical fiber. Credit: Félix Bussières/University of Geneva.

"When Alice measures the state of her photon, Bob's photon changes state as well, as if flipping a switch," Marsili said. "But Bob cannot know how the switch flipped unless Alice sends him the bits of information classically." Bob does not know that his photon has changed to yellow without that additional information.

Quantum teleportation doesn't mean someone can pop from New York to San Francisco instantaneously, but it seems like science fiction in the sense that the state of a particle (photon P) is destroyed at one location but imprinted on another remote system (photon B) without the two particles ever interacting.

Another crucial piece of this story is that Bob has a specific crystal, which serves as a memory bank, for storing his entangled photon and serving as the recipient of the quantum state.

The researchers reached the record distance of 15.5 miles (25 kilometers) between "Alice" and "Bob" thanks to the ultrasensitive detectors developed at JPL-NIST.

"Reaching this distance could not have been possible without the JPL NIST detectors," said Félix Bussières at the University of Geneva, Switzerland, who is the lead author of the study.

Quantum teleportation can be used to make systems, such as bank accounts, more secure over longer distances. This is also important to preventing attacks on communication channels in space.

"If you're communicating with your astronauts on Mars, you don't want to have hackers break the encrypted channel and give them false information," Marsili said.

The California Institute of Technology manages JPL for NASA.

FAQs About Quantum Teleportation:

You might have some questions regarding the sci-fi aspect of the recent quantum teleportation research. Francesco Marsili of NASA's Jet Propulsion Laboratory's responds:

Q: Has NASA developed Star Trek's 'transporter?'

A: "Unfortunately not. Our experiment is fundamentally different than Star Trek's transporter. The transporter teleports matter by converting matter into a signal for transport, and then converting the signal back to matter at some other location.

We teleported properties of light, so our experiment cannot lead to the transporter in the future. It is not inconceivable that one might teleport the quantum state of macroscopic material objects, but this would require that a clump of matter in the right shape would be waiting to receive the quantum state. Also, the experiment was carried out at the University of Geneva. NASA, in collaboration with the National Institute of Standards and Technology in Colorado, developed an essential part of the experiment: the detectors."

Q: Can NASA transport people through space and time?

A: "Space, but unfortunately not time. Our experiment has no implications for travel through spacetime, which would require creating Einstein-Rosen bridges (aka wormholes)."

Q: What's next?

A: "There are a number of technologies that still need to be developed to implement world-wide quantum networks. For example, next is the implementation of a quantum repeater. Quantum repeaters use entanglement, teleportation and quantum memories to transmit information over long distances. In the future, quantum cryptography may become a widespread technology. Quantum mechanics can make the communication between two users intrinsically secure."

For more information about JPL NIST detectors, visit: http://www.nist.gov/pml/div686/photons-021114.cfm

For more information about NASA's Jet Propulsion Laboratory, visit: http://www.jpl.nasa.gov/

For more information about the University of Geneva (Switzerland), visit: http://www.unige.ch/international/index_en.html

Images (mentioned), Text, Credits: NASA/JPL/Elizabeth Landau.

Greetings, Orbiter.ch

jeudi 20 novembre 2014

Stratospheric flight with a solar plane












Mission SolarStratos - To the Edge of Space logo.

November 20, 2014

Mission SolarStratos - To the Edge of Space

Neuchâtel (Switzerland), who was the first to sail around the world with a solar-powered boat, got funding for a flight over 24'000m altitude with a small solar plane.

Mission SolarStratos - To the Edge of Space - Launch 2014

Video above: Mission SolarStratos - to the Edge of Space. SolarStratos, Raphael Domjan - Go Further With Solar Energy. 3D / X-Plane modeling: Alexis Domjan/Cameraman and editor: Yannick Barthe.

Raphaël Domjan is the initiator of the SolarStratos mission, which is to bring in 2017 to more than 80,000 feet (over 24,000 meters) on a tandem solar plane. He announced in a statement that raised funds for the construction of its solar plane with several partners.

Raphael Domjan and SolarStratos plane model

At the Mission SolarStratos, Raphael Domjan hopes to reach altitudes above 24 km, where temperatures of about -70 ° C prevail. His plane, unpressurized be 7.9 m long, with a wingspan of 24.4 meters and weighs 400 kg. 22 m2 of photovoltaic cells will provide autonomy to tandem over 24 hours, which should achieve this "eco-adventure".

He will take about 5 hours to achieve the feat of climbing to the target altitude and contemplate the stars before returning to earth.

SolarStratos simulation model

Beyond this adventure, Raphaël Domjan and his team say they plan to open a door on a solar electric and near the commercial aviation space in order to create unique travel with private passengers or scientific .

After PlanetSolar

In 2012, he was teammates with curly to Monaco in the first round of the world only by solar energy. Its giant catamaran PlanetSolar, he had imagined and built, had joined its starting point in 584 days, 23 hours and 31 minutes of navigation.

PlanetSolar around the World

Swiss research and industry are at the forefront in the field of solar energy and photocells. Two other Swiss Bertrand Piccard and André Borschberg will launch next year from Abu Dhabi into a world tour with a plane with only four electric motors powered by solar energy, Solar Impulse 2. Their first prototype Solar Impulse 1 allowed them to make several long flights in Europe, Morocco, and across the United States with more stops, making them the first to accomplish such a feat.

For more information about SolarStratos, visit: http://www.solarstratos.com/

Images, Video (Mentioned), Text, Credits: SolarStratos / AFP / Translation: Orbiter.ch Aerospace.

Cheers, Orbiter.ch

Swift Gamma-Ray Burst Mission Marks Ten Years of Discovery












NASA - SWIFT Mission patch.

November 20, 2014


On Nov. 20, 2004, NASA's Swift spacecraft lifted off aboard a Boeing Delta II rocket from Cape Canaveral Air Force Station, Fla., beginning its mission to study gamma-ray bursts and identify their origins. Gamma-ray bursts are the most luminous explosions in the cosmos. Most are thought to be triggered when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole. The black hole then drives jets of particles that drill all the way through the collapsing star and erupt into space at nearly the speed of light.

Astronomers at NASA and Pennsylvania State University used Swift to create the most detailed ultraviolet light surveys ever of the Large and Small Magellanic Clouds, the two closest major galaxies. Nearly a million ultraviolet sources appear in this mosaic of the Large Magellanic Cloud, which was assembled from 2,200 images taken by Swift's Ultraviolet/Optical Telescope (UVOT) and released on June 3, 2013. The 160-megapixel image required a cumulative exposure of 5.4 days. The image includes light from 1,600 to 3,300 angstroms -- UV wavelengths largely blocked by Earth's atmosphere -- and has an angular resolution of 2.5 arcseconds at full size. The Large Magellanic Cloud is about 14,000 light-years across.

Swift Gamma-Ray Burst spacecraft. Image Credit: NASA

Viewing in the ultraviolet allows astronomers to suppress the light of normal stars like the sun, which are not very bright at such higher energies, and provides a clearer picture of the hottest stars and star-formation regions. No telescope other than UVOT can produce such high-resolution wide-field multicolor surveys in the ultraviolet.

Pennsylvania State University manages the Swift Mission Operations Center, which controls Swift's science and flight operations. Goddard manages Swift, which was launched in November 2004. The satellite is operated in collaboration with Penn State, the Los Alamos National Laboratory in New Mexico and Orbital Sciences Corp. in Dulles, Va. International collaborators are in the United Kingdom and Italy, and the mission includes contributions from Germany and Japan.

For more information about SWIFT mission, visit: http://swift.gsfc.nasa.gov/ and http://www.nasa.gov/mission_pages/swift/main/

Images, Text, Credits: NASA/Swift/S. Immler (Goddard) and M. Siegel (Penn State).

Greetings, Orbiter.ch