mercredi 22 juillet 2015

Pulsar Punches Hole in Stellar Disk












NASA - Chandra X-ray Observatory patch.

July 22, 2015


Images above: This trio of images contains evidence from NASA’s Chandra X-ray Observatory that a clump of stellar material has been jettisoned away from a double star system at incredibly high speeds. This system, known as PSR B1259-63/LS 2883 – or B1259 for short – is comprised of two objects in orbit around one another. The first is a star about 30 times as massive as the Sun that has a disk of material swirling around it. The other is a pulsar, an ultra-dense neutron star left behind when an even more massive star underwent a supernova explosion. Images Credits: NASA/CXC/PSU/G.Pavlov et al.

A fast-moving pulsar appears to have punched a hole in a disk of gas around its companion star and launched a fragment of the disk outward at a speed of about 4 million miles per hour. NASA’s Chandra X-ray Observatory is tracking this cosmic clump, which appears to be picking up speed as it moves out.

The double star system PSR B1259-63/LS 2883 – or B1259 for short – contains a star about 30 times as massive as the Sun and a pulsar, an ultra-dense neutron star left behind when an even more massive star underwent a supernova explosion.

The pulsar emits regular pulses as it spins 20 times a second, and moves in a highly elliptical orbit around its companion star. The combination of rapid rotation and intense magnetic field of the pulsar has generated a strong wind of high-energy particles moving away from the pulsar at near the speed of light.

The massive companion star, meanwhile, is rotating close to break-up speed and is spinning off a disk of material. As the pulsar makes its closest approach to the star every 41 months, it passes through this disk

“These two objects are in an unusual cosmic arrangement and have given us a chance to witness something special,” said George Pavlov of Penn State University in State College, Pennsylvania, lead author of a paper describing these results. “As the pulsar moved through the disk, it appears that it punched a clump of material out and flung it away into space.”

Even though the clump is rather large, spanning a hundred times the size of our Solar System, it is also quite thin. The material in it has the mass equivalent to all the water in the Earth’s oceans.

“After this clump of stellar material was knocked out, the pulsar’s wind appears to have accelerated it, almost as if it had a rocket attached,” said co-author Oleg Kargaltsev of George Washington University (GWU) in Washington, DC.

Chandra X-ray Observatory. Image Credits: NASA/CXC

Astronomers observed B1259, which is located about 7,500 light years from Earth, three times with Chandra between December 2011 and February 2014. These observations show the clump moving away from B1259 at an average speed of about 7% of the speed of light. The data also indicate that the clump has been accelerated to 15% of the speed of light between the second and third observations.

“This just shows how powerful the wind blasting off a pulsar can be,” said co-author Jeremy Hare, also of GWU. “The pulsar’s wind is so strong that it could ultimately eviscerate the entire disk around its companion star over time.”

The X-ray emission observed by Chandra is likely produced by a shock wave created as the pulsar’s wind rams into the clump of material. The ram pressure generated by this interaction could also accelerate the clump.

Chandra will continue monitoring B1259 and its moving clump with observations scheduled for later this year and in 2016.

These results appeared in the June 20, 2015 issue of The Astrophysical Journal and are available online (http://arxiv.org/abs/1505.07155). NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

Read More from NASA's Chandra X-ray Observatory: http://chandra.harvard.edu/photo/2015/psrb1259/

For Chandra images, multimedia and related materials, visit: http://www.nasa.gov/chandra

Images (mentioned), Text, Credits: NASA/Marshall Space Flight Center/Janet Anderson/Chandra X-ray Center/Megan Watzke/Lee Mohon.

Greetings, Orbiter.ch

ALMA Witnesses Assembly of Galaxies in the Early Universe for the First Time












ALMA - Atacama Large Millimeter/submillimeter Array logo.

22 July 2015

ALMA witnesses assembly of galaxy in early Universe (annotated)

The Atacama Large Millimeter/submillimeter Array (ALMA) has been used to detect the most distant clouds of star-forming gas yet found in normal galaxies in the early Universe. The new observations allow astronomers to start to see how the first galaxies were built up and how they cleared the cosmic fog during the era of reionisation. This is the first time that such galaxies are seen as more than just faint blobs.

When the first galaxies started to form a few hundred million years after the Big Bang, the Universe was full of a fog of hydrogen gas. But as more and more brilliant sources — both stars and quasars powered by huge black holes — started to shine they cleared away the mist and made the Universe transparent to ultraviolet light [1]. Astronomers call this the epoch of reionisation, but little is known about these first galaxies, and up to now they have just been seen as very faint blobs. But now new observations using the power of ALMA are starting to change this.

A team of astronomers led by Roberto Maiolino (Cavendish Laboratory and Kavli Institute for Cosmology, University of Cambridge, United Kingdom) trained ALMA on galaxies that were known to be seen only about 800 million years after the Big Bang [2]. The astronomers were not looking for the light from stars, but instead for the faint glow of ionised carbon [3] coming from the clouds of gas from which the stars were forming. They wanted to study the interaction between a young generation of stars and the cold clumps that were assembling into these first galaxies.

ALMA witnesses assembly of galaxy in early Universe

They were also not looking for the extremely brilliant rare objects — such as quasars and galaxies with very high rates of star formation — that had been seen up to now. Instead they concentrated on rather less dramatic, but much more common, galaxies that reionised the Universe and went on to turn into the bulk of the galaxies that we see around us now.

From one of the galaxies — given the label BDF 3299 — ALMA could pick up a faint but clear signal from the glowing carbon. However, this glow wasn’t coming from the centre of the galaxy, but rather from one side.

Co-author Andrea Ferrara (Scuola Normale Superiore, Pisa, Italy) explains the significance of the new findings: “This is the most distant detection ever of this kind of emission from a ‘normal’ galaxy, seen less than one billion years after the Big Bang. It gives us the opportunity to watch the build-up of the first galaxies. For the first time we are seeing early galaxies not merely as tiny blobs, but as objects with internal structure!”

The astronomers think that the off-centre location of the glow is because the central clouds are being disrupted by the harsh environment created by the newly formed stars — both their intense radiation and the effects of supernova explosions — while the carbon glow is tracing fresh cold gas that is being accreted from the intergalactic medium.

By combining the new ALMA observations with computer simulations, it has been possible to understand in detail key processes occurring within the first galaxies. The effects of the radiation from stars, the survival of molecular clouds, the escape of ionising radiation and the complex structure of the interstellar medium can now be calculated and compared with observation. BDF 3299 is likely to be a typical example of the galaxies responsible for reionisation.

Atacama Large Millimeter/submillimeter Array (ALMA)

“We have been trying to understand the interstellar medium and the formation of the reionisation sources for many years. Finally to be able to test predictions and hypotheses on real data from ALMA is an exciting moment and opens up a new set of questions.This type of observation will clarify many of the thorny problems we have with the formation of the first stars and galaxies in the Universe,” adds Andrea Ferrara.

Roberto Maiolino concludes: “This study would have simply been impossible without ALMA, as no other instrument could reach the sensitivity and spatial resolution required. Although this is one of the deepest ALMA observations so far it is still far from achieving its ultimate capabilities. In future ALMA will image the fine structure of primordial galaxies and trace in detail the build-up of the very first galaxies.”

Notes:

[1] Neutral hydrogen gas very efficiently absorbs all the high-energy ultraviolet light emitted by young hot stars. Consequently, these stars are almost impossible to observe in the early Universe. At the same time, the absorbed ultraviolet light ionises the hydrogen, making it fully transparent. The hot stars are therefore carving transparent bubbles in the gas. Once all these bubbles merge to fill all of space, reionisation is complete and the Universe becomes transparent.

[2] They had redshifts ranging from 6.8 to 7.1.

[3] Astronomers are particularly interested in ionised carbon as this particular spectral line carries away most of the energy injected by stars and allows astronomers to trace the cold gas out of which stars form. Specifically, the team were looking for the emission from singly ionised carbon (known as [C II]). This radiation is emitted at a wavelength of 158 micrometres, and by the time it is stretched by the expansion of the Universe arrives at ALMA at just the right wavelength for it to be detected at a wavelength of about 1.3 millimetres.

More information:

This research was presented in a paper “The assembly of “normal” galaxies at z∼7 probed by ALMA”, by R. Maiolino et al., to appear in Monthly Notices of the Royal Astronomical Society on 22 July 2015.

The team is composed of R. Maiolino (Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom; Kavli Institute for Cosmology, University of Cambridge, Cambridge, United Kingdom) S. Carniani (Cavendish Laboratory; Kavli Institute for Cosmology; Universitá di Firenze, Florence, Italy), A. Fontana (INAF–Osservatorio Astronomico di Roma, Italy), L. Vallini (Scuola Normale Superiore, Pisa, Italy; Universitá di Bologna, Bologna, Italy), L. Pentericci (INAF–Osservatorio Astronomico di Roma, Italy), A. Ferrara (Scuola Normale Superiore, Pisa, Italy), E. Vanzella (INAF–Bologna Astronomical Observatory, Bologna, Italy), A. Grazian (INAF–Osservatorio Astronomico di Roma, Italy), S. Gallerani (Scuola Normale Superiore, Pisa, Italy), M. Castellano (INAF–Osservatorio Astronomico di Roma, Italy), S. Cristiani (INAF–Trieste Astronomical Observatory, Trieste, Italy), G. Brammer (Space Telescope Science Institute, Baltimore, Maryland, USA), P. Santini (INAF–Osservatorio Astronomico di Roma, Italy), J. Wagg (Square Kilometre Array Organization, Jodrell Bank Observatory, United Kingdom) and R. Williams (Cavendish Laboratory; Kavli Institute for Cosmology).

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of ESO, the US National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the National Science Council of Taiwan (NSC) and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).

ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.

ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It is supported by 16 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile. 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 a major partner in ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre European Extremely Large Telescope, the E-ELT, which will become “the world’s biggest eye on the sky”.

Links:

Research paper: http://www.eso.org/public/archives/releases/sciencepapers/eso1530/eso1530a.pdf

Photos of ALMA: http://www.eso.org/public/images/archive/search/?adv=&subject_name=Atacama%20Large%20Millimeter/submillimeter%20Array

For more information about Atacama Large Millimeter/submillimeter Array (ALMA), visit: https://www.eso.org/sci/facilities/alma.html

Related links:

Cavendish Laboratory: http://www.phy.cam.ac.uk/

Kavli Institute for Cosmology, University of Cambridge: http://www.kicc.cam.ac.uk/

Images, Text, Credits: ESO/R. Maiolino.

Best regards, Orbiter.ch

mardi 21 juillet 2015

New Horizons Finds Second Mountain Range in Pluto’s ‘Heart’












NASA - New Horizons Mission logo.

July 21, 2015


Image above: A newly discovered mountain range lies near the southwestern margin of Pluto’s Tombaugh Regio (Tombaugh Region), situated between bright, icy plains and dark, heavily-cratered terrain. This image was acquired by New Horizons’ Long Range Reconnaissance Imager (LORRI) on July 14, 2015 from a distance of 48,000 miles (77,000 kilometers) and sent back to Earth on July 20. Features as small as a half-mile (1 kilometer) across are visible. Image Credits: NASA/JHUAPL/SWRI.

Pluto’s icy mountains have company. NASA’s New Horizons mission has discovered a new, apparently less lofty mountain range on the lower-left edge of Pluto’s best known feature, the bright, heart-shaped region named Tombaugh Regio (Tombaugh Region).

These newly-discovered frozen peaks are estimated to be one-half mile to one mile (1-1.5 kilometers) high, about the same height as the United States’ Appalachian Mountains. The Norgay Montes (Norgay Mountains) discovered by New Horizons on July 15 more closely approximate the height of the taller Rocky Mountains.

The new range is just west of the region within Pluto’s heart called Sputnik Planum (Sputnik Plain). The peaks lie some 68 miles (110 kilometers) northwest of Norgay Montes.

This newest image further illustrates the remarkably well-defined topography along the western edge of Tombaugh Regio.

“There is a pronounced difference in texture between the younger, frozen plains to the east and the dark, heavily-cratered terrain to the west,” said Jeff Moore, leader of the New Horizons Geology, Geophysics and Imaging Team (GGI) at NASA’s Ames Research Center in Moffett Field, California. “There’s a complex interaction going on between the bright and the dark materials that we’re still trying to understand.”

While Sputnik Planum is believed to be relatively young in geological terms – perhaps less than 100 million years old - the darker region probably dates back billions of years. Moore notes that the bright, sediment-like material appears to be filling in old craters (for example, the bright circular feature to the lower left of center).

This image was acquired by the Long Range Reconnaissance Imager (LORRI) on July 14 from a distance of 48,000 miles (77,000 kilometers) and sent back to Earth on July 20. Features as small as a half-mile (1 kilometer) across are visible. The names of features on Pluto have all been given on an informal basis by the New Horizons team.

Views of Pluto Through the Years


Animation above: This animation combines various observations of Pluto over the course of several decades. The first frame is a digital zoom-in on Pluto as it appeared upon its discovery by Clyde Tombaugh in 1930 (image courtesy Lowell Observatory Archives). The other images show various views of Pluto as seen by NASA's Hubble Space Telescope beginning in the 1990s and NASA's New Horizons spacecraft in 2015. The final sequence zooms in to a close-up frame of Pluto released on July 15, 2015. Animation Credits: NASA/Hubble/JHUAPL/SWRI.

New Horizons is part of NASA’s New Frontiers Program, managed by the agency’s Marshall Space Flight Center in Huntsville, Alabama. The Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland, designed, built and operates the New Horizons spacecraft and manages the mission for NASA’s Science Mission Directorate. SwRI leads the mission, science team, payload operations and encounter science planning.

For more information about New Horizons mission, visit: http://www.nasa.gov/mission_pages/newhorizons/main/index.html and http://www.nasa.gov/subject/3143/dwarf-planets

Image (mentioned), Animation (mentioned), Text, Credits: NASA/Tricia Talbert/Rob Garner.

Greetings, Orbiter.ch

Rosetta - Contact lost with Philae












ESA - Rosetta Mission patch.

July 21, 2015

Over the last few weeks, Rosetta has been flying along the terminator plane of Comet 67P/Churyumov-Gerasimenko, at distances from 180 km down to 153 km and at latitudes between 0 and 54 degrees, in order to find the best location to communicate with Philae.

However, over the weekend of 10–11 July, the star trackers again struggled to lock on to stars at the closer distances thanks to confusion due to dust particles in the comet’s increasingly-active environment. Because safety of the spacecraft is the first priority, it is therefore being moved back to safer distances of 170–190 km.

No contact has been made with Philae since Thursday 9 July. The data acquired at that time are being investigated by the lander team to try to better understand Philae’s situation.

For example, included in the latest data set was information on the sunlight reaching the lander’s different solar panels.


Image above: 360º view around the point of Philae's final touchdown. The three feet of Philae’s landing gear can be seen in some of the frames. Superimposed on top of the image is a sketch of the Philae lander in the configuration the lander team believed it was in November 2014. Image Credits: ESA/Rosetta/Philae/CIVA.

“The profile of how strongly the Sun is falling on which panels has changed from June to July, and this does not seem to be explained by the course of the seasons on the comet alone,” explains Philae’s project manager, Stephan Ulamec at DLR.

One possible explanation being discussed at DLR’s Lander Control Center is that the position of Philae may have shifted slightly, perhaps by changing its orientation with respect to the surface in its current location. The lander is likely situated on uneven terrain, and even a slight change in its position – perhaps triggered by gas emission from the comet – could mean that its antenna position has also now changed with respect to its surroundings. This could have a knock-on effect as to the best position Rosetta needs to be in to establish a connection with the lander.

Another separate issue under analysis is that one of the two transmission units of the lander appears not to be working properly, in addition to the fact that one of the two receiving units is damaged.

Philae is programmed to switch periodically back and forth between these two transmission units, and after tests on the ground reference model, the team has sent a command to the lander to make it work with just one transmitter. As Philae is able to receive and accept commands of this kind in the “blind”, it should execute it as soon as it is supplied with solar energy during the comet’s day.


Image above: The Philae Ground Reference Model. Image Credit: DLR.

The current status of Philae remains uncertain and is a topic of on-going discussion and analysis. But in the meantime, further commands are being prepared and tested to allow Philae to re-commence operations. The lander team wants to try to activate a command block that is still stored in Philae’s computer and which was already successfully performed after the lander’s unplanned flight across to the surface to its final location. This “safe block” set of activities includes temperature measurements by the thermal probe MUPUS, measurements by ROMAP and SESAME, and analysis by PTOLEMY and COSAC in sniffing mode, and do not involve moving any mechanism on lander. No detailed commands are needed: if operated in the currently stored configuration, the “safe block” only needs to be activated.

If this commanding works, Philae could re-start its scientific measurements and, if a link is established with Rosetta, it would be able to send its data back to Earth, via the orbiter.


Image above: Philae's instruments. Image Credits: ESA/ATG media.

The team has already tried to ‘call’ ROMAP in a similar way to the commands sent to the CONSERT instrument earlier in the month, but so far no confirmation signal has been returned. The situation continues to be analysed with the available data.

“Philae is obviously still functional, because it sends us data, even if it does so at irregular intervals and at surprising times,” adds Stephan Ulamec. “Several times we were afraid that the lander would remain off – but it has repeatedly taught us otherwise”.

From the end of this week, Rosetta will begin alternating lander communication attempts with its own scientific observations of the comet, including exploration of the southern latitudes, which have only started to become illuminated in recent months.


Image above: Comet 67P/C-G on 7 July 2015. Image Credits: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0.

“Studying these regions is an important part of our long-term science goals in the lead up to and beyond perihelion next month, when the comet is at its closest to the Sun along its orbit and activity will be at a maximum,” comments Nicolas Altobelli, acting Rosetta project scientist while Matt Taylor is on holiday.

“Although the mission will now focus its scientific priority on the orbiter, Rosetta will continue attempting – up to and past perihelion – to obtain Philae science packets once a stable link has been acquired,” adds Patrick Martin, Rosetta mission manager.

About Rosetta:

Rosetta is an ESA mission with contributions from its Member States and NASA. Rosetta's Philae lander is contributed by a consortium led by DLR, MPS, CNES and ASI.

For more information about Rosetta mission, visit: http://www.esa.int/Our_Activities/Space_Science/Rosetta

Where is Rosetta?: http://sci.esa.int/where_is_rosetta/

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

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

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

Frequently asked questions: http://www.esa.int/Our_Activities/Space_Science/Rosetta/Frequently_asked_questions

Images (mentioned), Text, Credit: European Space Agency (ESA).

Best regards, Orbiter.ch

lundi 20 juillet 2015

Breakthrough Initiatives, Hawking looking aliens







Breakthrough Initiatives logo.

July 20, 2015

The famous British astrophysicist Stephen Hawking, has launched an ambitious program to observe the far reaches of space in search for extraterrestrial intelligent life.

Yuri Milner and Stephen Hawking at the press conference

"In an infinite universe, there must be traces of life," said Stephen Hawking, who is about to embark on the search for extraterrestrial life.

Supported by the Russian physicist and industry founder Yuri Milner, the 10-year project, called "Breakthrough Listen" and endowed with $ 100 million (€ 92 million), is presented as the most ambitious ever undertaken to find a sign of extraterrestrial intelligence.

Breakthrough Initiatives Introduced by Seth MacFarlane

"It is time to find an answer"

"In an infinite universe, there must be evidence of life. Somewhere in the cosmos, perhaps, intelligent life look, "said Stephen Hawking launch the program at the Royal Society Science Academy in London.

"Either way, it is no greater question. It's time to commit to finding the answer, to seek life beyond Earth. We need to know, "added the scientist.

Aliens life in the cosmos?

To carry out this research, the project will use the resources of the most powerful telescopes in an attempt to flush out the manifestation of an intelligent activity, such as a radio frequency or a laser beam.

This program will be conducted in partnership with the project "Breakthrough Message", a competition to create digital messages representing humanity.

For more information about Breakthrough Initiatives, visit: http://www.breakthroughinitiatives.org/

Images, Video, Text, Credits: ATS/Breakthrough Initiatives/Getty/NASA/Orbiter.ch Aerospace.

Cheers, Orbiter.ch

CERN - An international blog series from ATLAS












CERN - European Organization for Nuclear Research logo.

July 20, 2015

More than 3000 scientists from all over the world, including about 1000 graduate students, collaborate on the ATLAS experiment – an all-purpose detector on the Large Hadron Collider (LHC). The detector, which first started taking data in 2008, is investigating a wide range of physics, from the search for the Higgs boson to extra dimensions and particles that could make up dark matter.

ATLAS in Collision Mode : 13TeV. (Video: ATLAS/CERN)

The detector is currently taking data from collisions in the LHC at 13 teraelectronvolts (TeV). In the video above you can see how members of the collaboration fared on 3 June 2015, when beams collided at this new energy in the LHC for the first time.

The new blog series "From ATLAS around the World," showcases the diversity of people, jobs and research topics it takes to keep the ATLAS experiment up and running. Contributors come from as far afield as Turkey, Japan, Hong Kong, Australia, South Africa.

The Large Hadron Collider (LHC) - To discover the secrets of matter and the Universe

Ever wondered how many Turkish physicists it takes to blog from the Bosphorous? What it's like to be a physicist down under? Or even where you can meet a giraffe at a physics workshop?

Check out From ATLAS around the World: http://atlas.ch/blog/?cat=68

Editor's Note:

The blogger who nevertheless remains the center of the action is this blog: Orbiter.ch Space News, the publisher and author lives above (exactly 110 meters above) of a portion of the LHC tunnel and 500 meters of ATLAS detector. There is no other blogger closest to CERN. If scoop there, you will be informed in the instant! (I still have not seen a black hole). http://orbiterchspacenews.blogspot.ch/

Note:

CERN, the European Organization for Nuclear Research, is one of the world’s largest and most respected centres for scientific research. Its business is fundamental physics, finding out what the Universe is made of and how it works. At CERN, the world’s largest and most complex scientific instruments are used to study the basic constituents of matter — the fundamental particles. By studying what happens when these particles collide, physicists learn about the laws of Nature.

The instruments used at CERN are particle accelerators and detectors. Accelerators boost beams of particles to high energies before they are made to collide with each other or with stationary targets. Detectors observe and record the results of these collisions.

Founded in 1954, the CERN Laboratory sits astride the Franco–Swiss border near Geneva. It was one of Europe’s first joint ventures and now has 22 Member States.

Related articles:

LHC at 13 teraelectronvolts (TeV): http://orbiterchspacenews.blogspot.ch/2015/05/cern-first-images-of-collisions-at-13.html

Discovery of a new class of particles at the LHC: http://orbiterchspacenews.blogspot.ch/2015/07/discovery-of-new-class-of-particles-at.html

Related links:

Large Hadron Collider (LHC): http://home.web.cern.ch/topics/large-hadron-collider

ATLAS experiment: http://home.web.cern.ch/about/experiments/atlas

Higgs boson: http://home.web.cern.ch/topics/higgs-boson

Dark matter: http://home.web.cern.ch/about/physics/dark-matter

Extra dimensions: http://home.web.cern.ch/about/physics/extra-dimensions-gravitons-and-tiny-black-holes

For more information about the European Organization for Nuclear Research (CERN), visit: http://home.web.cern.ch/

Image, Video, Text, Credits: CERN/Cian O'Luanaigh/Roland Berga (Orbiter.ch).

Best regards, Orbiter.ch

Robotic Servicing Demonstrations Continue Onboard the Space Station












ISS - International Space Station patch.

July 20, 2015

It's back, it's updated, and it's making great progress – all on the International Space Station (ISS).

NASA's Robotic Refueling Mission (RRM), a groundbreaking demonstration of new satellite-servicing technologies and techniques, recently resumed operations on the space station after a two-year hiatus. Within five days, the RRM team had outfitted the RRM module with fresh hardware for a series of technology demonstrations and tested a new, multi-capability inspection tool.


Image above: High above Earth on the International Space Station, the Dextre robot (at end of robot arm, center right) prepares for operations on the RRM module (platform at top right of image, bottom left of platform). Image Credit: NASA.

“The International Space Station is the ultimate test bed for new technologies,” explains Benjamin Reed, deputy project manager of the Satellite Servicing Capabilities Office (SSCO) at NASA's Goddard Space Flight Center. “It gives us the opportunity to practice and test technologies in an environment that just cannot be replicated on the ground.”

Known by its creative team as the "little ISS experiment that could," RRM broke uncharted ground in 2011-2013 with a set of activities that debuted robotic tools and procedures to refuel the propellant tanks of existing satellites. Its second phase of operations, which took place in April and May and will resume again later in 2015, offers something entirely different and just as disruptive, says Reed.

"We’ve outfitted the RRM module with new hardware so we can shift our focus to satellite inspection, instrument life extension, and even techniques for instrument swap-out,” says Reed. Such servicing technologies could open new possibilities for owners of spacecraft in low and geosynchronous Earth orbit, he says.

Shifting the Paradigm

Limited options currently exist for satellite owners when the unexpected occurs on orbit. If a solar array fails to deploy, or a micrometeorite strike affects a spacecraft's component, there is typically no way to see the potential cause of the anomaly or the extent of the damage.

Even healthy satellites will eventually deplete the valuable commodities that keep them, and their instruments, running at top condition. The SSCO team, the creators of RRM, want to change the status quo.


Image above: RRM operations demonstrate satellite-servicing technologies using the RRM module (right) and the Dextre robot (top center). Behind them, the ISS solar array is visible. Image Credit: NASA.

“We envision a future where robots, outfitted with a caddy stocked with tools, can help satellite owners diagnose and deliver timely aid to their spacecraft – ultimately extending their service lives,” says Frank Cepollina, veteran leader of the five servicing missions to the Hubble Space Telescope, and current associate director of the Satellite Servicing Capabilities Office. “Each task that RRM demonstrates gives NASA and the fledgling satellite-servicing community the confidence that these capabilities are real, that the technologies are proven, and that they can eventually work on a subsequent mission."

Operations on the International Space Station

The new RRM hardware launched to the ISS in two shipments, on board the Japanese HTV-4 cargo vehicle in August 2013, and the European Automated Transfer Vehicle-5 in August 2014. 

The second phase of RRM activities kicked off in April with the Canadian Space Agency’s Dextre robot transferring and installing two new RRM task boards and a tool onto the existing RRM module. From there, the team dove straight into a set of operations that debuted a new, multi-capability inspection tool named VIPIR, the Visual Inspection Poseable Invertebrate Robot.


Image above: VIPIR’s three cameras – the Motorized Zoom Lens (left), a video borescope, (center) and a camera for situational awareness (right) were put to the test during RRM operations in May 2015. Image Credit: NASA.

Shiny and silver, with a shape reminiscent of an old-time movie reel projector, the team built VIPIR to test a set of cameras for spacecraft inspection and anomaly diagnosis.

"When we asked the satellite community about their needs, we repeatedly heard how valuable an inspection capability could be for insurance companies and satellite manufacturers," says Reed. "Being able to see exactly how or why a component failed on orbit could mean the difference between launching more spacecraft with the same faulty design, or making a fix on the ground assembly line." 

Robotic inspection capabilities can also be used for routine spacecraft maintenance and anomaly recovery, he explained, potentially saving astronauts from taking a trip into the harsh space environment.


Image above: Held by the Dextre robot (not shown), the VIPIR tool (right) approaches the RRM module (left) to demonstrate the tool’s video borescope. Image Credit: NASA.

To demonstrate a range of inspection capabilities, NASA equipped VIPIR with two unique inspection cameras, as well as a fixed camera that helps human operators on the ground control the tool during operations.

On its side, VIPIR holds its workhorse mid-range inspection camera with a miniature, motorized 8-24mm optical zoom lens, about the size of a roll of quarters. This motorized zoom lens (MZL) can resolve worksite details as tiny as 0.02 inch – an area thinner than a credit card – while maintaining a tool distance of a few feet.

For close-up inspection jobs, VIPIR also carries a tiny, color, 1.2 mm diameter camera, nestled at the end of a 34-inch deployable video borescope. Operators can command the borescope’s tip to articulate up to 90 degrees in four opposing directions. With its miniscule dimensions, this borescope camera is one of the world’s tiniest cameras, and is the smallest camera to ever be flown by NASA in space. Developed commercially, it is typically used by the medical industry for endoscopies and other similar procedures.

Successful Operations in Space

Held by the Dextre robot and commanded from the ground, VIPIR worked through its on-orbit checklist during its operations. First, it used its zoom lens to capture images of RRM hardware and the space station. VIPIR’s borescope camera also captured imagery as it worked its way through an obstacle course on an RRM task board, like a snake burrowing through a nest.

NASA's VIPIR Tool on Orbit

Video above: Follow along with the VIPIR video borescope as it makes its way through the RRM obstacle course. Video Credit: NASA.

In the end, VIPIR operations were declared a success. Collected data, now under analysis, will help the RRM team determine what type of camera system and operational techniques would be best suited for different tasks on potential future missions.

“Doing RRM on the ISS gives us a controlled, representative environment to evaluate new technologies, gain invaluable experience, and get the type of data that help inform future efforts,” says Reed. For example, the team detected resolvable image motion during the motorized zoom lens operations, which had not been present during ground testing.


Image above: VIPIR’s borescope camera successfully captured imagery as it worked its way through an obstacle course on an RRM task board. Image Credit: NASA.

Before VIPIR opened its eyes in space, another RRM-hosted experiment also saw the light of “day” during its transfer to the RRM module. A set of advanced solar cells, mounted to one of the new RRM task boards, was exposed to the space environment to provide data on how these energy-generating packs perform in space conditions. The RRM team hosted this experiment on behalf of the Photovoltaic and Electrochemical Systems Branch at the Glenn Research Center.

What’s Next

"We’re very happy with the RRM results to date,” says Jill McGuire, RRM Project Manager,“ and we're excited to see what RRM unlocks for NASA and the satellite community.”

With these two demonstrations complete, the RRM team is taking a breath before they plunge into the next set of operations, occurring later in 2015. Using the two new task boards, the RRM team will demonstrate technologies and procedures that could be used to prepare a spacecraft for cryogen replenishment. They will also practice making the types of electrical connections that would be needed to install plug-and-play satellite instruments.

"Step by step,” says Cepollina, “these technologies are building essential capabilities that, in turn, equip us to boldly build and maintain a robust space infrastructure. Keep on watching RRM on the International Space Station. There is more to come."

Related links:

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

Robotic Refueling Mission (RRM): http://ssco.gsfc.nasa.gov/robotic_refueling_mission.html

Satellite Servicing Capabilities Office (SSCO): http://ssco.gsfc.nasa.gov/

NASA's Goddard Space Flight Center: http://www.nasa.gov/goddard

Canadian Space Agency’s Dextre robot: http://www.asc-csa.gc.ca/eng/iss/dextre/

Images (mentioned), Video (mentioned), Text, Credits: NASA's Goddard Space Flight Center/Adrienne Alessandro/Rob Garner.

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