jeudi 9 avril 2020

New Crew Reaches Orbit, Heads Toward Station













ROSCOSMOS - Soyuz MS-16 Mission patch.

April 9, 2020


Image above: The Soyuz MS-16 rocket ascends toward space with three Expedition 63 crewmembers heading to the space station today. Image Credit: NASA TV.

After a successful launch at 4:05 a.m. EDT of the Soyuz MS-16 spacecraft, NASA astronaut Chris Cassidy and two Russian cosmonauts safely reached orbit, beginning a four-orbit, six-hour flight to reach the International Space Station and join the Expedition 62 crew. At the time of launch, the station was flying about 259 miles over northeast Kazakhstan, south of the Kazakh capital of Nur-Sultan and 587 statute miles ahead of the Soyuz as it left the launch pad.

Soyuz-2.1a launches Soyuz MS-16

Cassidy, along with Anatoly Ivanishin and Ivan Vagner of the Russian space agency Roscosmos, will dock the Soyuz to the station’s Poisk service module at 10:15 a.m. Coverage of the docking will begin on NASA TV and the agency’s website at 9:30 a.m.

About two hours after docking, hatches between the Soyuz and the station will open, and they will join Expedition 62 Commander Oleg Skripochka of Roscosmos and NASA Flight Engineers Andrew Morgan and Jessica Meir.


Image above: Expedition 63 crewmembers (from left) Chris Cassidy, Anatoly Ivanishin and Ivan Vagner pose for pictures the day before launch. Image Credit: Roscosmos.

Skripochka, Morgan, and Meir will complete their station mission and return to Earth April 17 on the Soyuz MS-15 spacecraft, which will land in Kazakhstan. Morgan launched July 20, 2019, for an extended duration mission. Meir and Skripochka launched to the space station aboard a Soyuz spacecraft on Sept. 25, 2019.

Related links:

Expedition 62: https://www.nasa.gov/mission_pages/station/expeditions/expedition62/index.html

Expedition 63: https://www.nasa.gov/mission_pages/station/expeditions/expedition63/index.html

NASA TV: http://www.nasa.gov/live

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

Images (mentioned), Video, Text, Credits: NASA/Mark Garcia/NASA TV/SciNews.

Best regards, Orbiter.ch

mercredi 8 avril 2020

NASA Finds Very Heavy Rainfall in Major Tropical Cyclone Harold













NASA & JAXA - Global Precipitation Measurement (GPM) patch.

Apr. 08, 2020

Harold – Southern Pacific Ocean

On April 8, Tropical Cyclone Harold is a major hurricane, a Category 4 on the Saffir-Simpson Hurricane Wind Scale, as it exits Fiji and heads toward the island of Tonga. NASA used satellite data to calculate the rainfall generated by this powerful and destructive storm in the Southern Pacific Ocean.

IMERG Video of Harold on Apr. 8, 2020

This animation shows the heavy precipitation associated with Tropical Cyclone Harold as it progresses from the Solomon Islands (upper left) on April 2, 2020, explosively intensifies on April 3, reaches Vanuatu (center) as a Category 4 storm on April 5 before briefly attaining Category 5 status on April 6 and passing just south of Fiji (center right) on April 7 as a Category 4 storm. Periodically, Harold’s core region produced precipitation rates in excess of 30 millimeters per hour, which is equivalent to a 7-inch-deep rain accumulation if the core region were to remain over a given location for 6 hours. The precipitation estimates in this animation come from the IMERG multi-satellite algorithm developed by NASA and run in near real-time. Credit: NASA/JAXA, B. Jason West and Owen Kelley

Harold brought flooding rains and strong hurricane-force winds to the South Pacific island nation of Fiji on Wednesday, April 8. The Fiji Meteorological Service noted that Harold’s strength ranked in the highest category of five, when passed over Fiji’s south at about midday (local time). Earlier in the week, Harold caused damages and communications outages when it passed over Vanuatu on April 7, and killed dozens of people in the Solomon Islands.

Visualizing Harold’s Heavy Rainfall

At NASA’s Goddard Space Flight Center in Greenbelt, Maryland, the heavy rain generated from Harold from April 2 to 8 was calculated and mapped in an animation.

“This animation shows the heavy precipitation associated with Tropical Cyclone Harold as it progresses from the Solomon Islands on April 2, 2020, explosively intensifies on April 3, reaches Vanuatu as a Category 4 storm on April 5 before briefly attaining Category 5 status on April 6 and passing just south of Fiji on April 7 as a Category 4 storm,” said B. Jason West, Science Data Analyst for the Precipitation Processing System (PPS) at NASA Goddard.

Global Precipitation Measurement (GPM). Image Credits: NASA/JAXA

The data showed that periodically, Harold’s core region produced precipitation rates were in excess of 30 millimeters per hour (mm/h), which is equivalent to a 7-inch-deep rain accumulation if the core region were to remain over a given location for 6 hours. The precipitation estimates in this animation come from the IMERG multi-satellite algorithm developed by NASA and run in near real-time.

What is NASA’s IMERG?

NASA’s Integrated Multi-satellitE Retrievals for GPM or IMERG, is a NASA satellite rainfall product. The near-real time rain estimates come from the NASA’s IMERG, which combines observations from a fleet of satellites, in near-real time, to provide near-global estimates of precipitation every 30 minutes. By combining NASA precipitation estimates with other data sources, we can gain a greater understanding of major storms that affect our planet.

Instead, what the IMERG does is “morph” high-quality satellite observations along the direction of the steering winds to deliver information about rain at times and places where such satellite overflights did not occur. Information morphing is particularly important over the majority of the world’s surface that lacks ground-radar coverage. Basically, IMERG fills in the blanks between weather observation stations.

Harold’s Status on April 8, 2020


Image above: This IMERG image estimates rainfall from March 30 to April 7 just west of Vanuatu in the South Pacific. The deeper red areas indicated rainfall totals up to almost 750 mm (30 inches) west and east of Vanuatu. Image Credits: NASA/JAXA, Steve Lang.

The Joint Typhoon Warning Center or JTWC noted that Harold had maximum sustained winds near 120 knots (138 mph/222 kph) on April 8 at 10 a.m. EDT (1500 UTC). That makes it a Category 4 hurricane and a major storm. Harold was located near latitude 21.2 degrees south and longitude 176.9 degrees west, approximately 248 nautical miles southeast of Suva, Fiji, and has tracked east-southeastward at 23 knots (26 mph/43 kph).

What is Ahead for Harold

JTWC forecasters said what lies ahead for Harold is a hostile environment as vertical wind shear (winds that blow at different levels of the atmosphere that can tear a storm apart) will increase, and Harold will track through cooler waters (that will not help maintain thunderstorm development which a tropical cyclone needs to maintain structure and strength). On April 9, Harold is expected to begin interacting with the mid-latitude westerlies (winds) and start extratropical transition.

Tropical cyclones/hurricanes are the most powerful weather events on Earth. NASA’s expertise in space and scientific exploration using a fleet of satellites contributes to essential services provided to the American people by other federal agencies, such as hurricane weather forecasting.

For more information about NASA’s IMERG, visit: https://pmm.nasa.gov/gpm/imerg-global-image

Category 4 hurricane and a major storm: https://www.nhc.noaa.gov/aboutsshws.php

For more information about GPM, visit: http://www.nasa.gov/gpm and http://www.jaxa.jp/projects/sat/gpm/index_e.html

Video, Images (mentioned), Text, Credits: NASA’s Goddard Space Flight Center, by Rob Gutro.

Greetings, Orbiter.ch

Space Station 20th: Six Months Until Expedition 1











ISS - International Space Station 20th Anniversary patch.

April 8, 2020

With their anticipated ground-breaking launch to the International Space Station (ISS) just six months away, the Expedition 1 crew of Commander William M. Shepard, Flight Engineer Sergei K. Krikalev, and Soyuz Commander Yuri P. Gidzenko as well as their backups Kenneth D. Bowersox, Mikhail V. Tyurin and Vladimir N. Dezhurov divided their time between Russia and the United States. In April 2000 they took a side trip to Germany to familiarize themselves with one of the collaborative science experiments for their mission. In both the United States and Russia, engineers prepared the next modules and elements to be added to the still embryonic space station.

Two views of Expedition 1 commander Shepherd during an EVA training
session in the Hydrolab facility at Star City in February 2000. Images Credit: NASA.

The Expedition 1 prime and backup crews began the year 2000 with the astronauts training in the U.S. and the cosmonauts in Russia. They spent February training together in Russia, mainly at the Gagarin Cosmonaut Training Center in Star City outside Moscow, among other things practicing for Extra-Vehicular Activities (EVAs) or spacewalks using the Russian Orlan spacesuits in the Hydrolab facility. In March, they trained at the Johnson Space Center (JSC) in Houston, conducting EVA training in the Neutral Buoyancy Laboratory and joint simulations with Shuttle crews. In April they returned to Star City for additional training on Russian segment and Soyuz spacecraft systems.

Above: Expedition 1 crewmembers (left to right) Shepherd, Krikalev, Gidzenko, Dezhurov and Tyurin pose in front of the Plasma Kristall experiment hardware. Middle: The Plasma Kristall experiment hardware. Bellow: Expedition 1 crewmembers pose with the international Plasma Kristall experiment team. Images Credit: Max Planck Institute.

Unlike subsequent expeditions, the Expedition 1 crew had a somewhat modest amount of science experiments to conduct due to the priority placed on station assembly. The Plasma Kristall-3 (PK-3) experiment, later renamed PKE-Nefedov to honor Anatoli P. Nefedov, the Russian co-principal investigator who passed away in 2001, was one of the first natural science experiments conducted on the space station. The Max Planck Institute for Extraterrestrial Physics in Garching near Munich, Germany, and the Institute for High Energy Densities in Moscow, part of the Russian Academy of Sciences, collaborated on the experiment to study the formation and behavior of plasma and dust crystals in microgravity. Earth-bound benefits from research in plasma crystals include improved means of disinfecting surfaces including wounds, aiding in the healing process. In April 2000, five of the six Expedition 1 crewmembers (Bowersox was not available) traveled from Moscow to Germany to train on the PK-3 experiment.

Above: ISS as it appeared in May 1999, with the Zarya module at left and the
Unity Node 1 at right. Bellow: The Zvezda Service Module at RKK Energia being prepared for shipment to Baikonur in April 1999. Images Credit: NASA.

On-orbit assembly of the still crew-tended ISS, begun in November 1998, was ready to continue in mid-2000 with the launch of the Russian-built Zvezda Service Module (SM), providing living accommodations for long-duration crews, including environmental control and life support equipment. The Khrunichev State Research and Production Space Center in Moscow built Zvezda and delivered it to RKK Energia’s Test and Checkout Facility in 1998 so engineers there could begin extensive testing. In May 1999, workers transported the module to the Baikonur Cosmodrome’s Area 254 for additional testing and to begin prelaunch preparations. On Feb. 10 and 11, 2000, senior managers from the U.S., Russia and the European Space Agency met in Moscow to review the status of the ISS program, in particular Zvezda’s readiness for launch. At the conclusion of the meetings, the managers established July 8 to 14 as the launch window for the module, with July 12 as the optimal date, pending recertification of the Proton rocket after a launch failure in October 1999. The recertification mandated two successful launches before Zvezda’s.

Above: STS-101 crew posing outside the Spacehab module. Bellow: Members of the STS-101 crew inspect equipment inside the Spacehab module. Images Credit: NASA.

With Zvezda’s launch date firmly set, on Feb. 18 NASA managers decided to split the next Shuttle resupply mission, STS-101 and designated as 2A.2 in the overall ISS assembly sequence, into two separate flights. The first kept the STS-101 number but was redesignated as 2A.2a and initially scheduled for April, three months prior to the arrival of Zvezda. Several delays caused the mission to slip to May. The second became a new flight, STS-106 and 2A.2b, with a planned launch date in August (ultimately flew in September) to begin outfitting Zvezda before the Expedition 1 crew arrived in early November. Both missions made use of a Spacehab pressurized module to transport supplies to ISS.

Above: MEIT underway in the SSPF – US Lab Destiny is in the framework at right, the Z1 truss is at left. Middle: Controllers monitor the MEIT. Bellow: Astronauts inside the Destiny module during the MEIT – ISS Expedition 2 crewmember James S. Voss (upper left) and STS 98 crewmembers Kenneth D. Cockrell (lower left) and Mark L. Polansky (upper right). Images Credit: NASA.

In the United States, several ISS elements had already arrived at Kennedy Space Center’s Space Station Processing Facility (SSPF) for preflight testing. These elements included the Destiny U.S. Laboratory module, the third Pressurized Mating Adaptor (PMA-3), several segments of the Integrated Truss Assembly, and the Canadian-built Canadarm2 Space Station Remote Manipulator System. Engineers in the SSPF conducted a months-long Multi-Element Integrated Test (MEIT) to ensure that the various components worked well together before they reached orbit. They connected electrical and fluid lines among the Destiny module, the Z1 and P6 truss segments and the PMA-3 and used an emulator as a stand-in for the Unity Node 1 already on orbit. In February 2000, engineers completed an End-to-End Test and a Mission Sequence Test with the Destiny module, essentially duplicating the activation of the Lab once in orbit. Shepherd and several crewmembers of STS-98, the mission that delivered the Lab to orbit, took part in the tests, as did engineers at the Johnson Space Center and the Marshall Space Flight Center. The tests identified several issues that engineers fixed on the ground, preventing major problems that would have occurred only after the elements reached orbit.

To be continued…

Related articles & link:

Space Station 20th – Women and the Space Station
https://orbiterchspacenews.blogspot.com/2020/03/space-station-20th-women-and-space.html

Space Station 20th: Long-duration Missions
https://orbiterchspacenews.blogspot.com/2020/03/space-station-20th-long-duration.html

NASA Counts Down to Twenty Years of Continuous Human Presence on International Space Station
https://orbiterchspacenews.blogspot.com/2019/11/nasa-counts-down-to-twenty-years-of.html

20 memorable moments from the International Space Station
https://orbiterchspacenews.blogspot.com/2018/11/20-memorable-moments-from-international.html

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

Images (mentioned), Text, Credits: NASA/Kelli Mars/JSC/John Uri.

Greetings, Orbiter.ch

NASA Awards Contract to Deliver Science, Tech to Moon Ahead of Human Missions












NASA - Artemis Program logo.

April 8, 2020

NASA has selected Masten Space Systems of Mojave, California, to deliver and operate eight payloads – with nine science and technology instruments – to the Moon’s South Pole in 2022, to help lay the foundation for human expeditions to the lunar surface beginning in 2024.


Image above: Masten’s XL-1 lunar lander will deliver science and technology payloads to the Moon’s South Pole in 2022. Image Credit: Masten Space Systems.

The payloads, which include instruments to assess the composition of the lunar surface, test precision landing technologies, and evaluate the radiation on the Moon, are being delivered under NASA’s Commercial Lunar Payload Services (CLPS) initiative as part of the agency’s Artemis program.

As the country and the world face the challenges of the COVID-19 pandemic, NASA is leveraging virtual presence and communications tools to safely make progress on these important lunar exploration activities, and to award this lunar surface delivery as it was scheduled prior to the pandemic.

“Under our Artemis program, we are going to the Moon with all of America,” said NASA Administrator Jim Bridenstine. “Commercial industry is critical to making our vision for lunar exploration a reality. The science and technology we are sending to the lunar surface ahead of our crewed missions will help us understand the lunar environment better than we ever have before. These CLPS deliveries are on the cutting edge of our work to do great science and support human exploration of the Moon. I’m happy to welcome another of our innovative companies to the group that is ready to start taking our payloads to the Moon as soon as possible.”

The $75.9 million award includes end-to-end services for delivery of the instruments, including payload integration, launch from Earth, landing on the Moon’s surface, and operation for at least 12 days. Masten Space Systems will land these payloads on the Moon with its XL-1 lander.

“The Moon provides great scientific value, and these payloads will advance what we know and help define and improve the science astronauts can do,” said Thomas Zurbuchen, associate administrator of NASA’s Science Mission Directorate (SMD). “Our commercial Moon delivery efforts are seeking to demonstrate how frequent and affordable access to the lunar surface benefits both science and exploration.”

The payloads that will be delivered have been developed predominantly from the two recent NASA Provided Lunar Payloads (NPLP) and Lunar Surface Instrument and Technology Payloads (LSITP) solicitations.

The nine instruments to be delivered are:

- Lunar Compact Infrared Imaging System (L-CIRiS) will deploy a radiometer – a device that measures infrared wavelengths of light – to explore the Moon's surface composition, map its surface temperature distribution, and demonstrate the instrument's feasibility for future lunar resource utilization activities.

- Linear Energy Transfer Spectrometer (LETS) is a sensor that will measure the radiation environment on the Moon’s surface. The payload also is being flown on a CLPS flight to the Moon in 2021.

- Heimdall is a flexible camera system for conducting lunar science on commercial vehicles. This innovation includes a single digital video recorder and four cameras: a wide-angle descent imager, a narrow-angle regolith imager, and two wide-angle panoramic imagers. This camera system is intended to model the properties of the Moon's regolith – the soil and other material that make up the top layer of the lunar surface – and characterize and map geologic features. Other goals for this instrument include characterizing potential landing or trafficability hazards.

- MoonRanger is a small robotic rover that weighs less than 30 pounds and will demonstrate communications and mapping technologies. It will demonstrate the ability to move quickly across long distances on the lunar surface with autonomous navigation and without the ability to communicate with Earth in real time. It is a technology that could enable exploration of destinations that are far from lunar landing sites. The MoonRanger will carry the Neutron Spectrometer System, which will measure the concentration of hydrogen in the Moon’s regolith – a possible indication of the existence of buried water.

- Mass Spectrometer Observing Lunar Operations (MSolo) is a device to measure potentially accessible resources on the Moon’s surface. It will identify gases coming off a lander during touchdown on the lunar surface to help scientists understand what elements are coming from the lunar surface and which ones are introduced by a lander itself.

- Near-Infrared Volatile Spectrometer System (NIRVSS) is a tool to measure surface composition and temperature. The instrument will characterize the variability of the lunar soils and detect volatiles such as methane, carbon dioxide, ammonia and water.

- Laser Retroreflector Array (LRA) is a series of eight small mirrors to measure distance and support landing accuracy. It requires no power or communications from the lander and can be detected by future spacecraft orbiting or landing on the Moon.

- Sample Acquisition, Morphology Filtering, and Probing of Lunar Regolith (SAMPLR) is a robotic arm that will collect samples of lunar regolith and demonstrate the use of a robotic scoop that can filter and isolate particles of different sizes. The sampling technology makes use of a flight spare from the Mars Exploration Rover project.

NASA’s MSolo: A tool for measuring lunar resources

NASA has contracted with 14 American companies to deliver science and technology to the lunar surface through competed task orders. The agency plans to issue at least two such task orders per year through which the companies can propose to take payloads to the Moon. Under the Artemis program, early commercial deliveries of payloads to the lunar surface missions enable NASA to perform science experiments, test technologies and demonstrate capabilities to further explore the Moon and prepare for human missions.

“I am very pleased to award our next delivery service task order to Masten Space Systems,” said Steven Clarke, deputy associate administrator for exploration in SMD. “With the first delivery in 2022, we are continuing to execute our strategy of providing two delivery opportunities per year of science investigations and technology demonstration payloads to the lunar surface.”

In May 2019, NASA selected two CLPS providers, Astrobotic and Intuitive Machines, who are each making progress toward sending payloads to the Moon next year. In February, NASA asked the 14 companies to provide proposals to fly the Volatiles Investigating Polar Exploration Rover (VIPER), which will be the first rover on the Moon that will look for and map the distribution of water and other important volatiles at one of the lunar poles. In addition to these deliveries and the delivery to be made by Masten Space Systems, payloads for a fifth lunar delivery are in development, and NASA will soon be initiating a new series of payload acquisitions for targeted science investigations for years to come.

Related links:

Mass Spectrometer Observing Lunar Operations (MSolo): https://www.youtube.com/watch?v=59_vhOYoWWs

Moon to Mars: https://www.nasa.gov/topics/moon-to-mars/

Find more information about the agency’s Commercial Lunar Payload Services project at: http://www.nasa.gov/clps

Read more about NASA’s Artemis program at: http://www.nasa.gov/artemis

Image (mentioned), Video, Text, Credits: NASA/Sean Potter/Grey Hautaluoma/JSC/Rachel Kraft/ Jenny Knotts.

Greetings, Orbiter.ch

Gel, respirators ... CERN come into battle against coronavirus













CERN - European Organization for Nuclear Research logo.

April 8, 2020

With a large community of researchers, the scientific organization has set up an action group dedicated to the fight against the pandemic.

Fabiola Gianotti

"We want to deploy our resources and skills to help fight the Covid-19 pandemic," said Fabiola Gianotti.

Production of hydro-alcoholic gel, design and construction of sophisticated medical equipment ... CERN, which hosts the largest particle accelerator in the world, is also launching into the battle against the coronavirus.

This organization, which is also the place where the British Tim Berners-Lee conceptualized the World Wide Web more than 30 years ago, has tremendous scientific, physical and computer resources allowing him to contribute to the global fight against the coronavirus, against which there is no treatment, no vaccine.

In a press release, CERN said on Wednesday that it had set up an action group responsible for identifying and supporting the possible contributions of the 18,000 people making up its community of scientists around the world.

"Deploy our resources"

If CERN (European Organization for Nuclear Research) was originally a European organization, today it counts Israel among its members and the United States and Russia among its observer members.

CERN announce on Twitter

“CERN is a leading laboratory for particle physics and related technologies. It therefore has certain resources, such as very advanced facilities for the design and production of prototypes, and, of course, advanced technologies and considerable expertise both in the fields of science and engineering and in that of industrialization ”, underlined its general manager, Fabiola Gianotti.

"Now we want to deploy our resources and skills to help fight the Covid-19 pandemic," she said in the statement.

Gels, respirators and masks

Projects already launched include the production of one tonne of hydro-alcoholic gel for distribution to local rescue teams. CERN's capabilities in 3D printing and workshop work have been deployed to complement the production of protective equipment such as masks and Plexiglas barriers for law enforcement in the region.

Studies are underway to deploy the formidable computing capacity of the particle physics community to assist in the search for a vaccine, while the pandemic has killed more than 82,000 since its appearance in December in China.

CERN establishes task force to contribute to global fight against COVID-19

Video above: In particular, a novel streamlined ventilator, called HEV, is being prototyped at CERN. Led by a team of physicists and engineers from the LHCbExperiment collaboration at CERN, HEV is supported by several CERN services.

A prototype of a new respirator was developed at the end of March, scientists having had the idea of ​​using the systems used to regulate the gas flows for the particle detectors. This respirator could be used for patients with mild forms, or in the healing phase, which would free up the most efficient machines for the most serious cases, according to CERN.

The organization intends to publish all of its innovations so that they are "freely reproduced as necessary".

CERN Courrier: https://cerncourier.com/a/particle-physicists-propose-stripped-down-ventilator-to-help-combat-covid-19/

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

Images, Video, Text, Credits: ATS/CERN/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

Event Horizon Telescope: Black hole produces twisting jet





Event Horizon Telescope logo.

8 April 2020

One year on from publishing the first ever image of a black hole, the team behind that historic breakthrough is back with a new picture.

This time we're being shown the base of a colossal jet of excited gas, or plasma, screaming away from another black hole at near light-speed.


Image above: The right-hand image was captured with a less powerful telescope. It shows the jet streaming away to the lower-right. In the new EHT image on the left, scientists can now see detail where the jet connects to the accretion disc. The supermassive black hole will be somewhere at the disc's centre. Image Credits: Event Horizon Telescope Collaboration .

The scene was actually in the "background" of the original target.

The scientists who operate the Event Horizon Telescope describe the jet in the journal Astronomy & Astrophysics.

3C 279 is what astronomers term a quasar - the extremely bright core of a very distant galaxy. This one is about 5.5 billion light-years from Earth.

It is well known, and was used as the calibration target to align the performance of the EHT's eight individual radio telescopes when they simultaneously made their astonishing map of the supermassive black hole at the centre of Galaxy M87.

The remarkable resolution achieved by the EHT - put to such great effect with M87 - pays dividends again with 3C 279, because we see previously unrecognised features.


Image above: M87's black hole is surrounded by a halo of bright gas pulled inwards by gravity. Image Credits: ESO/EHT Collaboration.

3C 279 also has a supermassive black hole at its heart. It's about one billion times the mass of our Sun and its gravity is pulling in and shredding any stars or gas that get too close. This material is likely being accreted on to a disc that winds around the hole, but some of it is being shot back out into space along two jets moving in opposite directions.

In previous images of 3C 279, we've been able to detect the outline of the jet coming that moves towards us (the one moving in the opposite direction is not detected). But in the new EHT picture, we can resolve detail close to the point where this jet leaves the black hole. What's more, this base area seems twisted and somewhat offset from the main axis of the jet.

"It's curious," said EHT Collaboration member Dr Ziri Younsi. "We're seeing a region that's actually pretty close to the black hole. It could be an interaction layer where the jet couples to the accretion disc and extracts all of its energy from the black hole.

"We don't really understand how jets are powered by black holes. Black holes, when they rotate rapidly, are the most efficient liberators of energy in the Universe, but the mechanism by which the jet can extract that energy is unknown. There are a few ideas, but we're not sure yet which one is the right one," the University College London, UK, researcher told BBC News.


Image above: Artwork: Quasars like 3C 279 that point one of their jets in our direction are also called blazars. Image Credits: M.Weiss/CfA.

The data in the images of M87 and 3C 279 was collected by the ENT's widely dispersed array of radio telescopes in 2017. The project has gone on to collect data on the supermassive black hole that exists at the centre of our own galaxy, the Milky Way.

"We have that data - of a region we call Sagittarius A*," said Dr Younsi. "We are working on it right now and although we have some preliminary results, these can't be shared just yet. We hope to have something perhaps before the end of this year." The team finds itself in a position to concentrate on this analysis because the observational time it had booked on the EHT array for this year got cancelled in the coronavirus outbreak.

A PDF of the A&A paper describing 3C 279 is available link bellow. Its lead author is Dr Jae-Young Kim from the Max Planck Institute for Radio Astronomy in Bonn, Germany.


Image above: Early observations used eight radio telescopes but the EHT aims to get to a network of 12. Image Credit: BBC.

The Event Horizon Telescope is a "virtual telescope" that links a large array of radio receivers - from the South Pole, to Hawaii, to the Americas and Europe. It uses a technique called very long baseline array interferometry (VLBI). This combines the observations from the dispersed network to mimic a telescope aperture that can produce the resolution necessary to perceive a pinprick on the sky. For the EHT, this pinprick is measured in microarcseconds.

To convey such performance to the general public, EHT team-members talk about the sharpness of vision as being the equivalent of seeing from Earth something the size of a grapefruit on the surface of the Moon.

Related links:

The journal Astronomy & Astrophysics:
https://www.aanda.org/component/article?access=doi&doi=10.1051/0004-6361/202037493

The Event Horizon Telescope: https://eventhorizontelescope.org/

Images (mentioned), Text, Credits: Event Horizon Telescope Collaboration/BBC/Jonathan Amos.

Greetings, Orbiter.ch

CryoSat still cool at 10








ESA - CRYOSAT 2 Mission logo.

April 8, 2020

ESA's ice mission (CRYOSAT)

Today marks 10 years since a Dnepr rocket blasted off from an underground silo in the remote desert steppe of Kazakhstan, launching one of ESA’s most remarkable Earth-observing satellites into orbit. Tucked safely within the rocket fairing, CryoSat had a tough job ahead: to measure variations in the height of Earth’s ice and reveal how climate change is affecting the polar regions. Carrying novel technology, this extraordinary mission has led to a wealth of scientific discoveries that go far beyond its primary objectives to measure polar ice. And, even at 10 years old, this incredible mission continues to surpass expectations.

The launch of a satellite is always a time to hold your breath, but CryoSat’s liftoff on 8 April 2010 was arguably more tense than most as it came less than five years after the original satellite was lost owing to a rocket malfunction.

Successful launch for ESA’s CryoSat-2 ice mission

So important was the need to understand what was happening to Earth’s ice, the decision to rebuild was taken quickly – and thankfully, this day 10 years ago heralded the beginning of a mission that was set to advance polar science like no other.

While other satellite missions can measure changes in the extent of Earth’s ice, CryoSat completes the picture by recording changes in ice height, which are used to work out changes in thickness and volume – key to understanding the total amount of ice loss.

CryoSat was designed to observe two types of ice: the vast ice sheets of Antarctica and Greenland that rest on land, and the sea ice floating in the polar oceans.

Not only do these two forms of ice have different consequences for our planet and climate, but they also pose different challenges when trying to measure their thickness.

To do this, CryoSat carries the first spaceborne synthetic aperture interferometric radar altimeter, a sensor optimised to detect sea-ice floes as they drift in the ocean and to study the rugged glaciers that drain the polar ice sheets.

In addition, CryoSat’s orbit reaches latitudes of 88° North and South, which takes it closer to the poles than all previous polar-orbiting altimetry satellites.

ESA’s Director of Earth Observation Programmes, Josef Aschbacher, said, “CryoSat is the epitome of an ESA Earth Explorer. It uses completely new technology to fill gaps in our scientific knowledge. The issue of diminishing ice linked to climate change is a real concern, and over the last 10 years this mission has been a game changer.

Antarctica and Greenland’s contribution to sea level change

“For example, CryoSat has contributed to the recent worrying findings that Greenland and Antarctica are losing ice six times faster than in the 1990s, which has clear implications for future sea-level rise. Information such as this is vital for international policy making in responding to climate change.”

Andrew Shepherd from the University of Leeds, UK, added, “CryoSat’s contribution to polar science is truly astonishing. Not only do we now have a clear picture of how much ice Earth is losing, but its measurements have helped to improve the models we use to predict future climate change – information that is critical for society to adapt.”

CryoSat has also revealed how the world’s 200 000 mountain glaciers have succumbed to climate change, thanks to advanced swath processing of its radar measurements, which allows small regions to be mapped in fine detail. This new technique takes the mission beyond its brief to study polar ice alone.

2011–16 November Arctic sea-ice thickness

Although changes in sea ice do not affect sea level directly because it is afloat, it plays a central role in the global climate system as it reflects solar radiation back into space, and because it moderates ocean heat transport around the planet by insulating the relatively warm water from the cold polar air. CryoSat has been instrumental in mapping changes in the thickness and volume of Arctic sea ice.

Prof. Shepherd added, “Despite the long-term decline in the extent of Arctic sea ice, there have been significant year-to-year fluctuations in its thickness, and its volume has fallen in only seven of the past 10 years. But even with a decade of CryoSat measurements, the seasonal cycle of sea-ice growth and decay is still too large to confidently detect a long-term trend in volume, and so continued observation is essential.

As well as fulfilling its primary role as a polar ice mission, CryoSat’s measurements have been put to good use in a wide range of alternative and innovative applications. During the winter, CryoSat has been able to record changes in the thickness of ice on lakes, and in the summer it has been used to monitor lake and river water levels across the globe – information that is important for travel and fishing, for example.

CryoSat’s measurements are now an important reference of global sea level in the polar regions and beyond, thanks to its high-inclination orbit and long-repeat cycle, allowing scientists to refine the long-term trend and to detect short-term fluctuations associated with ocean dynamics.

Gravity reveals seafloor

And, it has even revealed what lies beneath the ocean surface thanks to its ability to detect tiny changes in marine gravity, which reflect the shape of the sea bed. CryoSat’s bathymetric charts are now an important tool for studying ocean dynamics, currents and tides, as well as for ship safety.

ESA’s CryoSat Mission Manager, Tommaso Parrinello, said, “These are just some of CryoSat’s outstanding results and the mission is still going strong, but we will focus more on this at the CryoSat anniversary conference, which we’ve had to postpone until October because of the COVID-19 pandemic. In the meantime, however, I cannot praise the mission and all the people who have worked on it enough.”

ESA’s Mark Drinkwater added, “Indeed, CryoSat is still giving us incredible data to advance science, and with its new synthetic aperture radar and interferometric capabilities it has also laid the foundation for the Copernicus Polar Ice and Snow Topography Altimeter (CRISTAL) operational mission, which we are now developing on behalf of the ESA Member States and the European Commission.”

CRISTAL will fill the recognised gap in sustained long-term monitoring of polar ice variability for the Copernicus Climate Change Service and Copernicus Marine Environment Monitoring Service, maritime security and international ice charting, and in support of the EU Integrated Arctic Policy and commitments to the Paris Agreement and Green New Deal.

Related links:

CryoSat: http://www.esa.int/Applications/Observing_the_Earth/CryoSat

Observing the Earth: http://www.esa.int/Applications/Observing_the_Earth

Images, Animation, Video, Text, Credits: ESA/S. Corvaja/AOES Medialab/CPOM/Scripps Institution of Oceanography.

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