mardi 3 octobre 2017

Eye Checks and Cargo Ops Ahead of Thursday Spacewalk












ISS - Expedition 53 Mission patch.

October 3, 2017

International Space Station (ISS). Animation Credit : NASA

Three Expedition 53 astronauts conducted eye exams Tuesday morning two days ahead of a spacewalk. The crew is also preparing for a pair of upcoming commercial cargo missions.

Commander Randy Bresnik, who is leading all three spacewalks this month, joined his fellow spacewalkers for a periodic eye exam. Bresnik and Flight Engineers Mark Vande Hei and Joe Acaba scanned their eyes using an ultrasound device with guidance from doctors on the ground monitoring the crew’s health.


Image above: Astronaut Joe Acaba calculates his mass inside the Columbus laboratory module using the Space Linear Acceleration Mass Measurement Device (SLAMMD). The device generates a known force against a crew member mounted on an extension arm with the resulting acceleration used to calculate the subject’s mass. Image Credit: NASA.

Paolo Nespoli, from the European Space Agency, did some rearranging inside the Japanese Kibo laboratory module today. He is preparing Kibo for new science gear arriving on a pair of private space freighters in November. Orbital ATK’s Cygnus resupply ship is due to launch mid-November and the SpaceX Dragon is planned to launch at the end of November.

Related links:

Space Linear Acceleration Mass Measurement Device (SLAMMD): https://www.nasa.gov/mission_pages/station/research/experiments/640.html

Orbital ATK’s Cygnus: https://www.nasa.gov/orbital

SpaceX Dragon: https://www.nasa.gov/spacex

Expedition 53: https://www.nasa.gov/mission_pages/station/expeditions/expedition53/index.html

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

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

Image (mentioned), Animation (mentioned), Text, Credits: NASA/Mark Garcia.

Best regards, Orbiter.ch

Seeing Double: Scientists Find Elusive Giant Black Hole Pairs












NASA - Chandra X-ray Observatory patch.

Oct. 3, 2017

Astronomers have identified a bumper crop of dual supermassive black holes in the centers of galaxies. This discovery could help astronomers better understand how giant black holes grow and how they may produce the strongest gravitational wave signals in the Universe.

Illustration of supermassive black hole pair. Image Credits: NASA/CXC/A.Hobart

The new evidence reveals five pairs of supermassive black holes, each containing millions of times the mass of the Sun. These black hole couples formed when two galaxies collided and merged with each other, forcing their supermassive black holes close together.

The black hole pairs were uncovered by combining data from a suite of different observatories including NASA’s Chandra X-ray Observatory, the Wide-Field Infrared Sky Explorer Survey (WISE), and the ground-based Large Binocular Telescope in Arizona.

“Astronomers find single supermassive black holes all over the universe,” said Shobita Satyapal, from George Mason University in Fairfax, Virginia, who led one of two papers describing these results. “But even though we’ve predicted they grow rapidly when they are interacting, growing dual supermassive black holes have been difficult to find.”

Before this study fewer than ten confirmed pairs of growing black holes were known from X-ray studies, based mostly on chance detections. To carry out a systematic search, the team had to carefully sift through data from telescopes that detect different wavelengths of light.

Starting with the Galaxy Zoo project, researchers used optical data from the Sloan Digital Sky Survey (SDSS) to identify galaxies where it appeared that a merger between two smaller galaxies was underway. From this set, they selected objects where the separation between the centers of the two galaxies in the SDSS data is less than 30,000 light years, and the infrared colors from WISE data match those predicted for a rapidly growing supermassive black hole.


Image above: This graphic shows two of five new pairs of supermassive black holes recently identified by astronomers using a combination of data from NASA’s Chandra X-ray Observatory, the Wide-Field Infrared Sky Explorer Survey (WISE), and the ground-based Large Binocular Telescope in Arizona. Image Credits: X-ray (J122104): NASA/CXC/George Mason Univ./S.Satyapal et al.; X-ray (J140737): NASA/CXC/Univ. of Victoria/S.Ellison et al.; Optical: SDSS; Illustration: NASA/CXC/A.Hobart.

Seven merging systems containing at least one supermassive black hole were found with this technique. Because strong X-ray emission is a hallmark of growing supermassive black holes, Satyapal and her colleagues then observed these systems with Chandra. Closely-separated pairs of X-ray sources were found in five systems, providing compelling evidence that they contain two growing (or feeding) supermassive black holes.

Both the X-ray data from Chandra and the infrared observations, suggest that the supermassive black holes are buried in large amounts of dust and gas.

“Our work shows that combining the infrared selection with X-ray follow-up is a very effective way to find these black hole pairs,” said Sara Ellison of the University of Victoria in Canada, who led the other paper describing these results. “X-rays and infrared radiation are able to penetrate the obscuring clouds of gas and dust surrounding these black hole pairs, and Chandra’s sharp vision is needed to separate them”.

The paper led by Ellison used additional optical data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey to pinpoint one of the new black hole pairs.  One member of this black hole pair is particularly powerful, having the highest X-ray luminosity in a black hole pair observed by Chandra to date.

This work has implications for the burgeoning field of gravitational wave astrophysics. While scientists using the Laser Interferometer Gravitational-Wave Observatory (LIGO) have detected the signals of merging black holes, these black holes have been of the smaller variety weighing between about eight and 36 times the mass of the Sun.

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

The merging black holes in the centers of galaxies are much larger. When these supermassive black holes draw even closer together, they should start producing gravitational waves. The eventual merger of the dual supermassive black holes in hundreds of millions of years would forge an even bigger black hole. This process would produce an astonishing amount of energy when some of the mass is converted into gravitational waves.

“It is important to understand how common supermassive black hole pairs are, to help in predicting the signals for gravitational wave observatories,” said Satyapal. “With experiments already in place and future ones coming online, this is an exciting time to be researching merging black holes. We are in the early stages of a new era in exploring the universe.”

LIGO is not able to detect gravitational waves from supermassive black hole pairs. Instead, pulsar timing arrays such as the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) are currently performing this search. In the future, the Laser Interferometer Space Antenna (LISA) project could also search for these gravitational waves.

Four of the dual black hole candidates were reported in a paper by Satyapal et al. that was recently accepted for publication in The Astrophysical Journal, and appears online (https://arxiv.org/abs/1707.03921). The other dual black hole candidate was reported in a paper by Ellison et al., which was published in the September 2017 issue of the Monthly Notices of the Royal Astronomical Society and appears online (https://arxiv.org/abs/1705.05465).

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.

NASA's Jet Propulsion Laboratory in Pasadena, California, managed and operated WISE for NASA's Science Mission Directorate in Washington. The Space Dynamics Laboratory in Logan, Utah, built the science instrument. Ball Aerospace & Technologies Corp. of Boulder, Colorado, built the spacecraft. Science operations and data processing take place at the Caltech/IPAC. Caltech manages JPL for NASA.

Read More from NASA's Chandra X-ray Observatory: http://chandra.harvard.edu/photo/2017/doubleagn/

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

Images (mentioned), Animation (mentioned), Text, Credits: NASA/Lee Mohon/Marshall Space Flight Center/Molly Porter.

Best regards, Orbiter.ch

Metal with Memory: Shaping the Future of Aviation











NASA logo.

Oct. 3, 2017

While aeronautics researchers across the globe continue to develop technologies that will make air travel more efficient, more sustainable and safer, there is a group of NASA researchers who are altering the long-held view that wings have to stick straight out from an aircraft and stay that way.

Through NASA’s Convergent Aeronautics Solutions (CAS) Project, a team of engineers working within its Spanwise Adaptive Wing (SAW) project is investigating the feasibility of bending or shaping portions of an aircraft’s wings in-flight, potentially increasing performance and efficiency by reducing weight and drag.


Image above: The outer wing section of an F/A-18 research plane is disassembled at NASA’s Armstrong Flight Research Center in Edwards, California for delivery to NASA Glenn Research Center in Cleveland, Ohio. Image Credit: NASA.

The ability to fold wings isn’t new. Since the dawn of ship-based aviation, U.S. Navy aircraft have been required to fold their wings for space conservation. Currently, this type of wing folding, or actuation, happens only on deck and serves no aerodynamic purpose. Other aircraft, like the XB-70, have folded their wings in flight with success. However, these fold systems required bulky, multipart structures, including hydraulics, pneumatics and electric motors, which weigh hundreds of pounds and take up valuable space.

NASA XB-70 Valkyrie. Image Credit: NASA

NASA’s engineers believe folding wings in-flight using advanced materials and technologies is a potential game-changer for future aircraft. The innovative actuation system that NASA and engineers from The Boeing Company are developing uses a revolutionary material that will accomplish this goal using less complex, lighter and more compact hardware than conventional systems.

That material is shape memory alloy (SMA), an engineered nickel-titanium alloy that can be trained to return to a desired shape after deformation by applying heat.

“By applying a temperature stimuli, you can trigger a physical change in the metal,” said Dr. Othmane Benafan, materials research engineer at NASA Glenn Research Center in Cleveland and the SAW project’s co-principle investigator. “It undergoes a reversible phase transformation much like ice melting and refreezing. The difference is it transitions from one solid state to another. The changes that happen at the atomic level are reversible, meaning the SMA is designed to bend and then return to its original shape once heat is applied.”        

Much like folding a wing, SMA isn’t a new breakthrough. It is commercially available and its unique properties make it an attractive alternative to common actuators. However, current commercial SMAs have limited capabilities and can only be operated at or near room temperature.

The material NASA is developing is similar to these alloys, but with increased capabilities, higher operational loads, higher operating temperatures and energy density. The material has more predictable properties and can be accurately controlled, making it well-suited for aeronautics applications. It is also unique in regards to memory or “training,” because the rare microstructural features produce a better, more stable material. 


Image above: Dr. Othmane Benafan, co-principle investigator for the Spanwise Adaptive Wing Project, inspects a model of the shape memory alloy actuator and the outer wing section from an F/A-18 research plane. Image Credit: NASA.

For the SAW project, NASA is using SMA materials as torque-tube actuators. In this configuration, a single or group of trained SMA tubes are heated via internal heaters or external electrical coils, triggering them to twist and perform the desired actuation to drive a folding wing. Electrically-induced temperature change is only one possible stimuli. SMA can also be activated by using bleed air from the aircraft’s engines or simply through the ambient temperature changes experienced during flight. This compact, lightweight application, which is also extremely quiet, allows the entire actuator package to be attached at the wing hinge point.  Conventional actuation approaches typically cannot fit in this area, leading to heavy and complex linkages or transmissions to drive a wing fold or similar aerodynamic surface.

But going from the test bench to replacing proven systems with SMA will require the development of a complete actuation and control system, and this is where Boeing’s expertise and previous experience comes in.  

“We’ve done a lot of work with NASA to look at how we develop the material: how we melt it, how we forge it, how we turn it into a component, how we train it and how we integrate it into an aircraft,” said Jim Mabe, technical fellow at Boeing Research and Technology. “We’re not only developing the SMA technology, we’re developing everything around it to simplify integration. So, when requests do come in, we don’t have to do any of the science or research. We can quickly engineer an actuator according to application requirements. The way I look at it, putting SMA into an aircraft is becoming more of an engineering problem than a science problem because we’ve made huge strides maturing the science and processes.”

 Boeing ecoDemonstrator Program. Image Credit: Boeing

Being involved in NASA’s SAW project is just one of Boeing’s endeavors into wing shaping and SMA applications. Boeing previously used SMA as part of a flight test program in 2012, where it integrated a compact SMA torque tube actuator into a small trailing edge flap on a 737-800, one of Boeing’s ecoDemonstrator aircraft.

“We believe SMA could be something that will change the industry,” said Mabe. “This technology will eventually open the door to several different development approaches. And it’s not just limited to wings and flaps; there are other potential aircraft applications we can apply this material to as well.”

While NASA prepares to integrate SMA into SAW’s subscale flight-test of the Prototype-Technology Evaluation and Research Aircraft (PTERA) later this fall at NASA’s Armstrong Flight Research Center in Edwards, California, the team at NASA Glenn wants to get a head start on ground testing SMA actuators on a large-scale wing.

“This testing is critical as we want to move quickly from subscale into full-size demonstration in the coming years,” said Benafan. “It will allow us to better understand how SMA will work in a real wing at different loads and operating conditions.”

To do this, NASA Armstrong removed a wing section from one of its F/A-18 scientific research aircraft for testing at NASA Glenn. The F/A-18 was selected not only because of NASA’s access to the Boeing-built aircraft, but also for the wing-fold system required by the U.S. Navy.

NASA F/A-18 Systems Research Aircraft. Image Credit: NASA

The wing section, which was delivered to NASA Glenn in July, will have all of the factory fold mechanics removed, and it will be retrofitted with a 20,000-inch-pound SMA torque-tube actuator.

“We are using the F/A-18 wing as a test article to demonstrate the actuation concept at a much larger scale compared to what we have now, which is close to a few hundred inch-pounds” said Benafan. “We need to understand if scaling up is feasible from all aspects, including material performance, work densities and control of the actuators.”       

When activated, the wing actuators will heat up and twist to move the 300-pound section over a 180-degree sweep. That can be 90 degrees from the flight-ready position to the vertical folded position, as well as moving 90 degrees down. More importantly, NASA wants to demonstrate actuation to any position desired within that 180-degree sweep.

Through the full-scale ground tests and the upcoming subscale flight test, the SAW project team is working to transform aircraft design through SMA-enhanced wing shaping. Ultimately, this shaping capability could increase aircraft performance during all phases of flight, including ground, subsonic and, possibly, supersonic.

SAW is a collaboration between NASA, The Boeing Company and Area-I, and it is part of NASA’s CAS project under the agency’s Transformative Aeronautics Concepts Program.

Related links:

Convergent Aeronautics Solutions (CAS): https://www.nasa.gov/aeroresearch/programs/tacp/cas

Spanwise Adaptive Wing (SAW): https://www.nasa.gov/feature/nasa-to-test-in-flight-folding-spanwise-adaptive-wing-to-enhance-aircraft-efficiency

Shape memory alloy (SMA): https://www.grc.nasa.gov/WWW/StructuresMaterials/AdvMet/research/shape_memory.html

Prototype-Technology Evaluation and Research Aircraft (PTERA): https://www.nasa.gov/sites/default/files/atoms/files/fs-108-afrc.pdf

Images (mentioned), Text, Credits: NASA Glenn Research Center/Jimi Russell.

Greetings, Orbiter.ch

NASA May Extend BEAM’s Time on the International Space Station











NASA - Bigelow Expandable Activity Module (BEAM) patch.

Oct. 3, 2017

NASA is exploring options with Bigelow Aerospace to extend the life of the privately owned Bigelow Expandable Activity Module. Known as BEAM, the module is attached to the International Space Station and continues to perform well during its technology demonstration mission. NASA has issued a synopsis of an intended contract action to partner with Bigelow Aerospace to extend the life of the expandable habitat and use it for long-term in-orbit storage. This step continues NASA’s commitment to expand private-public partnerships, scientific research and commercial applications aboard station to maximize the benefits from humanity’s premiere laboratory in microgravity.

Expandable Habitat on International Space Station. Image Credit: NASA

NASA’s use of BEAM as part of a human-rated system will allow Bigelow Aerospace to demonstrate its technology for future commercial applications in low-Earth Orbit. Initial studies have shown that soft materials can perform as well as rigid materials for habitation volumes in space and that BEAM has performed as designed in resistance to space debris.

BEAM launched on the eighth SpaceX Commercial Resupply Service mission in 2016. After being attached to the Tranquility Node using the station’s robotic Canadarm2, it was filled with air to expand it for a two-year test period to validate overall performance and capability of expandable habitats. Since the initial expansion, a suite of sensors installed by the crew automatically take measurements and monitor BEAM’s performance to help inform designs for future habitat systems. Learning how an expandable habitat performs in the thermal environment of space and how it reacts to radiation, micrometeoroids and orbital debris will provide information to address key concerns about living in the harsh environment of space. This extension activity will deepen NASA’s understanding of expandable space systems by making the BEAM a more operational element of the space station to be actively used in storage and crew operations.

Space station crew members have entered BEAM 13 times since its expansion in May 2016. The crew has conducted radiation shielding experiments, installed passive radiation badges called Radiation Area Monitors, and they routinely collect microbial air and surface samples. These badges and samples are returned to Earth for standard microbial and radiation analysis at the Johnson Space Center.

The original plan called for engineers to robotically jettison BEAM from the space station following the two-year test and validation period, allowing it to burn up during its descent through Earth’s atmosphere. However, after almost a year and a half into the demonstration with positive performance, NASA now intends to continue supporting BEAM for stowage use and to allow Bigelow Aerospace to use the module as a test-bed for new technology demonstrations. A new contract would likely begin later this year, overlapping the original planned test period, for a minimum of three years, with two options to extend for one additional year. At the end of the new contract, the agency may consider further life extension or could again consider jettisoning BEAM from the station.

The Bigelow Expandable Activity Module (BEAM). Image Credit: Bigelow

Using the space inside BEAM would allow NASA to hold between 109 to 130 Cargo Transfer Bags of in-orbit stowage, and long-term use of BEAM would enable NASA to gather additional performance data on the module’s structural integrity, thermal stability and resistance to space debris, radiation and microbial growth to help NASA advance and learn about expandable space habitat technology in low-Earth orbit for application toward future human exploration missions. Given that the volume of each Cargo Transfer Bag is about 1.87 cubic feet (0.53 cubic meters), use of BEAM for stowage will free an equivalent space of about 3.7 to 4.4 International Standard Payload Racks, enabling more space in the ISS for research.

With an extension of the partnership, Bigelow also would be able to continue to demonstrate its technology for future commercial applications in low-Earth orbit. The public-private partnership between NASA and Bigelow supports NASA’s objective to develop deep space habitation capabilities for human missions beyond Earth orbit while fostering commercial capabilities for non-government applications to stimulate the growth of the space economy.

Related links:

Bigelow Expandable Activity Module (BEAM): https://www.nasa.gov/mission_pages/station/research/experiments/1804.html

Commercial Space: http://www.nasa.gov/exploration/commercial/index.html

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

Images (mentioned), Text, Credits: NASA/Erin Mahoney.

Greetings, Orbiter.ch

Gaia data help prepare for a rare celestial alignment of Neptune's largest moon












ESA - Gaia Mission patch.

03 October 2017

On 5 October 2017, the largest moon of Neptune will pass in front of a distant star. This rare event will temporarily block the star's light from Earth and provide an excellent opportunity to study the moon's intriguing atmosphere. Data from ESA's Gaia mission is allowing astronomers to precisely plan their observations.

Image of Triton from Voyager 2. Image Credits: NASA/JPL

Alignments of this kind are called occultations. This particular one will be visible from Earth along a track that just skims the southern states of the USA, crosses the Atlantic and then passes through Europe. Observations are planned from Belgium, France, Germany, Greece, Italy, Spain, Switzerland and the UK, by both professional and amateur observers.

Triton is the largest moon of Neptune. In terms of size it is an almost identical twin to Pluto. Also like Pluto, Triton possesses a tenuous nitrogen atmosphere, which the astronomers are keen to study.

As the moon drifts in front of the star, some of the starlight passes through the atmosphere and is diverted through a process called refraction. This results in a dimming of the star, from which density, pressure and temperature profiles of the atmosphere can be derived.

Occultation of a star by Triton. Image Credits: ESA/ATG medialab

To get the best data from the occultation, astronomers have to be on the central track. This is where the alignment between the Earth, Triton and the star is perfect. At this point, astronomers get to see a 'central flash'. This momentary brightening occurs because the atmosphere of Triton acts like a lens that focuses the starlight to Earth. This gives access to the deepest possible atmospheric layers, just a few kilometres above the surface.

However, from the initial prediction of the occultation, the central path's track across the Earth's surface was uncertain by about 1200-1500km. This made it easy to be in the wrong place and miss the flash completely. This is where Gaia came in.


Image above: Ground trace of Triton occultation. Image Credits: Google, INEGI, ORION-ME; annotation: ERC Lucky Star project.

Data from the publicly available first Gaia release (Gaia DR1) could already give a more accurate ground track but Gaia DR1 only provides this star's position. Knowing its motion on the sky, a quantity called the proper motion, would help to improve the accuracy even more. However, despite Gaia DR1 containing 2 million proper motions, this particular star's motion would only become available in April 2018 with the Gaia second data release (Gaia DR2).

Since the forthcoming Triton occultation presents a rare opportunity to study the atmosphere, Josselin Desmars, an astronomer from the Observatoire de Paris in France, decided to approach the Gaia team and make a special request on behalf of the ERC Lucky Star project. The project, led by Bruno Sicardy from Université Pierre et Marie Curie and Observatoire de Paris, studies the poorly-known, but important, Trans-Neptunian Objects. Desmars coordinates the predictions of this Triton event using recent astrometric measurements of Neptune's moon made in Brazil.

"In April 2017, we asked the Gaia team if we could get some stars from their upcoming second data release in order to refine the prediction and gather observing stations along the central flash," says Desmars. The Gaia team agreed on the importance of the observation and released the preliminary Gaia DR2 position and proper motion to help the campaign [1].

Armed with this information, a much more accurate track has been calculated. Now the various observing stations across Europe can be placed at well-defined offsets to ensure that at least one of them sees the central flash.

Gaia spacecraft. Image Credit: ESA

The first definitive measurements of Triton's atmosphere were made in 1989 by the Voyager 2 spacecraft during its flyby. It discovered that the atmosphere was extremely tenuous (just one 70 000th of the surface pressure of Earth), extended up to 800 km from the moon's surface, and possessed a temperature of around 38 Kelvin (-235 °C).

Eight years later, an occultation took place that allowed astronomers using the Hubble Space Telescope to measure the atmosphere again. They saw something surprising. Triton's atmospheric temperature had increased by 5%, which could indicate that Triton was warming during the Neptunian summer.

The occultation on 5 October is the first favourable one since 1997 and astronomers want to see if the warming trend has continued.

"We hope to get a lot of observations from professionals and amateurs to let us really study the atmosphere," says Desmars.

This is not the first time Gaia data have been provided for such an event. Desmars also used preliminary Gaia DR2 data for occultations of Chariklo, a distant asteroid. This asteroid is known to have a ring system surrounding it, like a mini Saturn. The Gaia data helped to improve the predicted occultation paths, leading to very successful observational campaigns in the summer of this year.

[1] In May, the Gaia team released the preliminary data for the star that will be occulted by Triton. This week, the Gaia team made public preliminary astrometric data for an additional few hundred stars in the field surrounding Triton to allow astronomers to further improve the occultation predictions. The team cautions that for all of these preliminary data full validation is not yet done and therefore some caution is required when interpreting the results.

Notes for Editors:

The star that will be occulted by Triton is UCAC4 410-143659, a 12.7 V-magnitude (12.2 G-magnitude) star, situated in the constellation of Aquarius.

Observations of this occultation by Triton are coordinated by Bruno Sicardy (Université Pierre et Marie Curie and Observatoire de Paris), leader of the ERC Lucky Star project.

Related Links:

Triton stellar occultation 5/6 October 2017 - Mike Kretlow: http://astro.kretlow.de/?Solar-System---Occultations/Triton-Occultation-2017

First Gaia release (Gaia DR1): http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=58272

Gaia second data release (Gaia DR2): https://www.cosmos.esa.int/web/gaia/release

ERC Lucky Star project: http://cordis.europa.eu/project/rcn/199073_en.html

ESA's Gaia mission: http://www.esa.int/Our_Activities/Space_Science/Gaia

Related article:

Catching the Shadow of a Neptunian Moon
http://orbiterchspacenews.blogspot.ch/2017/10/catching-shadow-of-neptunian-moon.html

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

Best regards, Orbiter.ch

Africa, classified








ESA - Sentinel-2 Mission logo.

3 October 2017

From the barren Sahara to lush jungles, the first high-resolution map classifying land cover types on the entire African continent has been released. The map was created using a year’s worth of data from the Sentinel-2A satellite.

At a resolution of 20 m per pixel, you can now explore African’s diverse landscapes from grasslands to croplands, water bodies to deserts.

African land cover

Land-cover mapping breaks down the different types of material on Earth’s surface. This information is important for understanding changes in land use, modelling climate change extent and impacts, conserving biodiversity and managing natural resources.

The map released this week comprises 180 000 Sentinel-2A images representing 90 terrabytes captured between December 2015 and December 2016. Considering the size of the map – about six gigabytes – a web interface was developed to visualise the data.

The map was developed under ESA’s Climate Change Initiative (CCI) Land Cover project, and users are invited to provide their feedback on the new map through an online form.

“The prototype high-resolution land cover map at 20m over Africa is an impressive demonstration of the Sentinel-2A data availability and of the present capabilities for the processing of such huge volumes of data,” said Frédéric Achard from the Joint Research Centre.

Sentinel-2

“The community dealing with land resources in Africa will surely look forward with great interest to this prototype and to its future development.”

ESA has been coordinating global land cover maps since 2002 through its GlobCover and CCI Land Cover projects at a resolution of 300 m. While the latest map of Africa is based on observations from one of the twin Sentinel-2 satellites, the launch of Sentinel-2B in March has put the possibility of a global map at 10 m within reach.

The pair of Sentinel-2 satellites offer ‘colour vision’ for Europe’s Copernicus programme. They each carry a multispectral imager with 13 spectral bands that can be used for agricultural and forestry practices and for helping manage food security. Satellite images can be used to determine various plant indices such as leaf area chlorophyll and water content.

Related links:

User feedback form: http://2016africalandcover20m.esrin.esa.int/feedback.php

Africa land cover map at 20 m: http://2016africalandcover20m.esrin.esa.int/viewer.php

Land Cover CCI: https://www.esa-landcover-cci.org/

JRC: https://ec.europa.eu/jrc/en/science-areas

Related missions:

Sentinel-2: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-2

Images, Text, Credits: Contains modified Copernicus Sentinel data (2015-2016), processed by Land Cover CCI, ESA/ATG medialab.

Greetings, Orbiter.ch

lundi 2 octobre 2017

ATLAS and CMS celebrate their 25th anniversaries












CERN - European Organization for Nuclear Research logo.

2 Oct 2017


Image above: This special ATLAS and CMS birthday cake, baked and decorated by a member of the ATLAS collaboration, Katharine Leney, represents two event displays, one from each detector, in the icing. (Image: CERN).

ATLAS and CMS are like close sisters, the best of friends and competitors all at once. Today they are both celebrating their 25th birthdays. On 1 October 1992, the two collaborations each submitted a letter of intent for the construction of a detector to be installed at the proposed Large Hadron Collider (LHC). These two documents, each around one hundred pages long, are considered the birth certificates of the two general-purpose experiments. They each contain fairly precise technical specifications, close to that of the two detectors that were eventually built, and an already long list of institutes and scientists that had joined the collaborations. The letters of intent for ALICE and LHCb, the LHC’s two other large experiments, followed a few months later.

Several months earlier, 600 physicists and engineers from 250 institutes around the world had met in Évian-les-Bains to discuss the physics and detectors of the LHC. Design proposals for various experiments were then made public. Carlo Rubbia, the Director-General of CERN at the time, proposed a schedule for selecting which experiments would go ahead, with letters of intent to be submitted for evaluation by a peer review committee. This resulted in the creation of the LHC Committee (LHCC), which began evaluating the proposals that autumn.

In June 1993, the LHCC gave the green light to the two general-purpose experiments, which then had to develop detailed technical proposals. This marked the start of a long and difficult journey that pushed the boundaries of technology and human endeavour, but which eventually led to a major discovery, that of the Higgs boson, and many other important results, the list of which keeps on growing.

- Visit the ATLAS and CMS websites to find out more about the events of the last 25 years: https://atlas.cern/atlas25 and https://cms25.web.cern.ch/

- ATLAS has been organising a series of Facebook Live events today, with a Q&A session at 6pm CEST. Visit the ATLAS Facebook page: https://www.facebook.com/ATLASexperiment/

- You can also read the ATLAS letter of intent and the CMS letter of intent:
https://cds.cern.ch/record/291061/files/cm-p00043027.pdf
https://cds.cern.ch/record/290808/files/cern-lhcc-92-003.pdf

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 links:

ATLAS: http://home.cern/about/experiments/atlas

CMS: http://home.cern/about/experiments/cms

ALICE: http://home.cern/about/experiments/alice

LHCb: http://home.cern/about/experiments/lhcb

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

For more information about European Organization for Nuclear Research (CERN), Visit: http://home.cern/

Image (mentioned), Text, Credits: CERN/Corinne Pralavorio.

Best regards, Orbiter.ch