mardi 18 janvier 2022

CERN - ISOLDE data get deluxe theoretical treatment

 







CERN - European Organization for Nuclear Research logo.


Jan 18, 2022

A unique combination of high-quality experimental data and several state-of-the-art nuclear-physics models has resulted in an excellent agreement between experiment and theory

The ISOLDE facility seen from above. (Image: CERN)

The atomic nucleus is a tough nut to crack. The strong interaction between the protons and neutrons that make it up depends on many quantities, and these particles, collectively known as nucleons, are subject to not only two-body forces but also three-body ones. These and other features make the theoretical modelling of atomic nuclei a challenging endeavour.

In the past few decades, however, ab initio theoretical calculations, which attempt to describe nuclei from first principles, have started to change our understanding of nuclei. These calculations require fewer assumptions than traditional nuclear models, and they have a stronger predictive power. That said, because so far they can only be used to predict the properties of nuclei up to a certain atomic mass, they cannot always be compared with so-called DFT calculations, which are also fundamental and powerful and have been around for longer. Such a comparison is essential to build a nuclear model that is applicable across the board.

In a paper just published in Physical Review Letters, an international team at CERN’s ISOLDE facility shows how a unique combination of high-quality experimental data and several ab initio and DFT nuclear-physics calculations has resulted in an excellent agreement between the different calculations, as well as between the data and the calculations.

“Our study demonstrates that precision nuclear theory from first principles is no longer a dream,” says Stephan Malbrunot of CERN, the first author of the paper. “In our work, the calculations agree with each other, as well as with our ISOLDE data on nickel nuclei, to within a small theoretical uncertainty.”

Using a suite of experimental methods at ISOLDE, including a technique to detect the light emitted by short-lived atoms when laser light is shone on them, Malbrunot and colleagues determined the (charge) radii of a range of short-lived nickel nuclei, which have the same number of protons, 28, but a different number of neutrons. These 28 protons fill a complete shell within the nucleus, resulting in nuclei that are more strongly bound and stable than their nuclear neighbours. Such “magic” nuclei are excellent test cases for nuclear theories, and in terms of their radius, nickel nuclei are the last unexplored magic nuclei that have a mass within the mass region at which both ab initio and DFT calculations can be made.

Comparing the ISOLDE radii data with three ab initio calculations and one DFT calculation, the researchers found that the calculations agree with the data, as well as with each other, to within a theoretical uncertainty of one part in a hundred.

“An agreement at this level of precision demonstrates that it will eventually become possible to build a model that is applicable across the whole chart of nuclei,” says Malbrunot.

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 23 Member States.

Related links:

Physical Review Letters: https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.128.022502

ISOLDE: https://home.cern/science/experiments/isolde

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

Image (mentioned), Text, Credits: CERN/By Ana Lopes.

Best regards, Orbiter.ch

lundi 17 janvier 2022

Steady driving towards ExoMars launch

 





ESA - ExoMars Mission logo.


Jan 17, 2022

The first simulation of the ExoMars Rosalind Franklin rover driving off its landing platform closed out an incredible year of preparations as the mission now marches with confidence towards a September launch.

Amalia drives off

ESA’s Rosalind Franklin rover starts the year with months of successful maintenance and functional tests behind it. All its instruments are go for flight, with some minor tuning left to complete this month.

“The rover is ready, and together with the recent drop test success for the parachutes, we are positive to be in time for the September launch date,” says Pietro Baglioni, ESA’s ExoMars rover team leader.

Only once every two years and for about ten days, celestial mechanics would allow the spacecraft to reach Mars from Earth in the shortest possible time – around nine months.

Amalia the rover

Rosalind now sits in an ultra-clean room at the Thales Alenia Space premises in Turin, Italy, right by its travelling companion, the Kazachok landing platform. Following a final review in April, all the components of the spacecraft – rover, descent module, landing platform and carrier – will move to the launch site in Baikonur, Kazakhstan, to prepare for lift-off.

“Just before that last trip on Earth, we will upload the final version of the software that will allow the rover to scout Mars autonomously,” explains Pietro.

First martian moves

Following the nerve-wracking descent to the surface of Mars, a long-awaited moment in the ExoMars mission will be when Rosalind leaves the landing platform and drives onto the martian soil for the first time. The egress from Kazachok is a carefully choreographed move that engineers are rehearsing on Earth.

ExoMars – Testing locomotion

The twin of ESA’s Rosalind Franklin rover has successfully left the platform during recent tests in a Mars terrain simulator at the ALTEC premises in Turin.

While the driving during these exercises takes about 15 minutes, the whole process will last a few martian days. After landing, the rover will be busy for over a week unfolding its wheels and deploying the mast, among other checkouts.  

“The egress is a long and crucial operation. We need to be gentle and run it in a very slow motion for extra safety,” explains Andrea Merlo, ExoMars head of robotics from Thales Alenia Space.

Amalia's wheels

The landing platform has two exit ramps: one at the front and another one at the back. Rosalind is designed to negotiate steep inclines on the ramps, but it is up to ground control on Earth to decide which is the safest way to drive off.

“Once the six wheels hit the martian surface, it will be the beginning of the story for this rover on Mars. We feel ready and are really looking forward to the real mission,” says Andrea.

Amalia and Rosalind

The ExoMars twin rover, until now dryly known as the Ground Test Model, has a new name: Amalia. This test model borrows its name from Professor Amalia Ercoli Finzi, a renowned astrophysicist with broad experience in spaceflight dynamics.

Amalia was  the first woman to graduate in aeronautical engineering in Italy, and besides serving as a scientific advisor for ESA and NASA, she designed the drill on Rosetta’s lander Philae and strongly pushed for the development of the ExoMars drill already 20 years ago.

“I am flattered and honoured to have this essential element of the ExoMars mission named after me. Mars is waiting for us,” said Amalia after receiving the news.

ExoMars deep drilling success on Earth

Engineers are using the Amalia rover to recreate different scenarios and help them take decisions that will keep Rosalind safe in the challenging environment of Mars. The model is fully representative of what the rover will be able to do on the Red Planet.

“The fun has started. We will use Amalia to run risky operations, from driving around martian slopes seeking the best path for science operations to drilling and analyzing rocks,” explains Andrea.

Amalia has so far demonstrated drilling soil samples down to 1.7 metres and operate all the instruments while sending scientific data to the Rover Operations Control Centre (ROCC), the operational hub that will orchestrate the roaming of the European-built rover on Mars.

It takes a team

The effort to arrive at the starting line in time has been extraordinary, with double shifts and no time for breaks in 2021 amidst COVID -19 pandemic disruptions.

“The cooperation between European and Russian industry, the coordination between space agencies and the work of the technical teams have been remarkable,” praises Pietro.

Teams have solved critical issues working in parallel, such as the parachute system and the descent module electronics, with enough margin for a launch in September 2022. Preparations for launch have started in Baikonur, and a dedicated support team is in place at ESOC centre in Darmstadt, Germany.

The ESA-Roscosmos Trace Gas Orbiter is waiting for the arrival of ExoMars to the Red Planet. In addition to its own science mission, the orbiter relays data from NASA’s Perseverance rover. Also on the martian surface since 2021 is China’s Zhurong rover.

“It’s not long to go before the European rover can finally join the other martian drivers in 2023 with a top class scientific laboratory on board,” says Pietro.

ExoMars timeline

The ExoMars programme is a joint endeavour between ESA and Roscosmos. In Europe, Thales Alenia space is the industrial prime, Leonardo provides the drill, OHB the complex laboratory mechanisms and nine different instrument teams from ESA Member States, NASA/JPL and IKI/Roscosmos provide the payload. Astrium Ltd. (ASU) is responsible for the rover vehicle. The programme also includes the Trace Gas Orbiter, which has been orbiting Mars since 2016.

Related links:

ExoMars: https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/Exploration/ExoMars

Rover Operations Control Centre (ROCC): https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/Exploration/ExoMars/A_European_mission_control_for_the_martian_rover

NASA’s Perseverance: https://www.esa.int/Enabling_Support/Operations/ESA_Mars_orbiters_support_NASA_Perseverance_landing

Human and Robotic Exploration: https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration

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

Greetings, Orbiter.ch

CLEP - Yutu-2 has traveled over 1000 metres the far side of the Moon

 







CLEP - China Lunar Exploration Program logo.


Jan 17, 2022

The "Mystery Hut" was an "irregularly shaped rock"

The Yutu-2 rover has traveled over 1000 meters, since its landing in the Von Karman Crater, located in the Aitken Basin, in the South Pole region on the far side of the Moon, on 3 January 2019.

Yutu-2 has traveled over 1000 meters the far side of the Moon

According to mission specialists, the Chang’e-4 lander and the Yutu-2 rover are in good working condition, with the rover traveling northwest to a basalt region. Chang’e-4’s landing site was named Statio Tianhe.

The routing path of the Yutu-2 rover.

In December 2021, the rover pictured what appeared to be a particularly prominent boulder, dubbed the "Mystery Hut" (神秘小屋), or "Moon Cube", which it was intended to explore in the lunar days (earth months) ahead. On 7 January 2022, news reported that the rover reached the destination area after traveling for a month, and found that the "Mystery Hut" was an "irregularly shaped rock"; to some, the rock looks a bit like a rabbit, along with a nearby much smaller rock that looks like a carrot, which may be even more fitting overall since the rover's name Yutu means "Jade Rabbit".

Related article:

Chang’e-5 sample has high-titanium content and rare Earth elements
https://orbiterchspacenews.blogspot.com/2021/12/change-5-sample-has-high-titanium.html

Related link:

China National Space Administration (CNSA): http://www.cnsa.gov.cn/english/index.html

Images, Video, Text. Credits: China National Space Administration (CNSA)/China Media Group(CMG)/China Central Television (CCTV)/SciNews/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

CASC - Long March-2D launches Shiyan-13

 







CASC - Long March-2D / Y70 - First launch of 2022 patch.


Jan 17, 2022

Long March-2D carrying Shiyan-13 liftoff

A Long March-2D launch vehicle launched the Shiyan-13 satellite from the Taiyuan Satellite Launch Center, Shanxi Province, northern China, on 17 January 2022, at 02:35 UTC (10:35 local time).

Long March-2D launches Shiyan-13

According to official sources, the Shiyan-13(试验十三) satellite entered the planned orbit successfully and will be “mainly used for space environment exploration and related technical tests.”

For more information about China Aerospace Science and Technology Corporation (CASC): http://english.spacechina.com/n16421/index.html

Images, Video, Text, Credits: China Media Group(CMG)/China Central Television (CCTV)/China Aerospace Science and Technology Corporation (CASC)/SciNews/Günter's Space Page/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

Tonga eruption heard in New Zealand, pressure waves picked up in Europe

 







Natural Disasters logo.


Jan 17, 2022

The violent eruption of underwater volcano Hunga Tonga Hunga Ha'apai on Saturday was heard in New Zealand and picked up as far away as the UK and Italy. What did people actually hear, and just how far did the shockwaves travel? We ask the experts.

Brian Hamilton heard what sounded like the booming of distant cannons from his rural Awhitu home in southwest Auckland.

Tonga eruption. Image Credits: Japan Meteorology/AP/Picture Alliance

The weather enthusiast had been monitoring satellite imagery and saw shockwaves ripple out from Hunga Tonga Hunga Ha'apai.

A friend estimated the sound would reach them in the next half hour.

He was right. The first rumbles started just after 7pm, and louder ones still at 8.

"It was like distant cannons, a popping sound ... quite surreal because beautiful blue sky on a summer day, and you could hear like fireworks a long, long way away."

Hamilton was hard of hearing and only caught the louder ones, but his wife heard more. "You could feel it in your eardrums."

Source: USGS

He is one of many across New Zealand who heard the submarine volcano exploding more than 2000km away.

Social media was abuzz with people posting from Auckland, Tauranga, Napier, Wellington, and down south as far Invercargill.

"Am I hearing the #tonga #eruption from my house in Wellington, New Zealand? Ninety per cent sure it's that," said Daniel from Lower Hutt.

"That's so crazy. I was in the middle of a barbecue and it sounded like it was right above me! Heard two about three minutes apart," said CJ from Tauranga.

"Sonic boom in Napier just observed #Tonga," tweeted Craig Ireson, saying it went on for about 20 minutes.


Video above: Water vapour imagery shows how the #eruption causes a ripple effect across the atmosphere. Absolutely enormous energy. Video Credit: WeatherWatch.co.nz.

Hunga's eruption injected a huge amount of energy into the atmosphere, said Richard Easther, Professor of Physics at the University of Auckland. "The bigger the explosion, the more air is stirred up, so the louder it's going to be."

"It's not one continuous wall of sound, it's a pulse of sound that works its way out, spreads out effectively as a circle centred on the volcano."

People in the North Island would have heard it before people in the South Island.

Sound travels about one kilometre every three seconds, so what New Zealanders heard would have taken place about two hours earlier in Tonga, some 2400km away, estimates Dr Marcus Wilson, senior lecturer of Physics at the University of Waikato.

Animation Credits: NOAA/CIRA/RAMMB

A single blast would disperse as the sound travels, arriving as a lasting rumble that can take many seconds to pass. "It will be the really low sounds you're hearing, a really deep rumbling."

"Some people will hear it more strongly than others ... these are pressure waves, basically squashing and stretching the air."

Some social media posts called it a "sonic boom" but experts say that's a misnomer.

A sonic boom is a shock wave produced by something travelling faster than the speed of sound, like the Concorde or high-performance fighter jets.

Easther says the eruption may have produced a sonic boom at the source, but by the time the pressure wave arrived in New Zealand it would have been moving as regular sound.

On the other side of the world, the UK Met Office picked up shockwaves of the Tonga volcano on its observation sites, confirming earlier readings from weather enthusiasts.

Source: Twitter

Using readings from people's backyard weather stations, Dunedin dad David Orlovich tracked the pressure wave going around the world, to Sardinia and Sicily, Kingston, and the Florida Keys.

Historically, large volcanic eruptions have made themselves seen and heard far away, like Indonesia's Krakatoa in 1883 and in New Zealand, Tarawera in 1886.

"People heard (Tarawera) in the South Island and thought it was a shooting," said Easther.

Hunga is part of a string of volcanoes forming the Tonga Arc, formed by the Pacific tectonic plate subducting under the Indo-Australian plate.

The volcano has erupted several times over the past century, in 1912, 1937, 1988, 2009, and 2014.

Little is known of those that took place in the early 1900s but of the last three, erupted volumes appear to be increasing, says senior Lecturer Marco Brenna at the University of Otago. Saturday's eruption appears to be much larger than what the volcano has done in recent history.

The Hunga Tonga-Hunga Ha'apai volcano seen from space

Video Credits: Tonga Meteorological Services/NOAA/JAXA/CNSA/SciNews.

A magma reservoir some 5 to 6km underground has been feeding previous eruptions, and likely the current one as well, he said.

Details of the Saturday eruption are still emerging. Scientists agree it may not be the last and further eruptions of equal magnitude are possible.

Related links:

National Oceanic and Atmospheric Administration (NOAA): https://www.noaa.gov/

Japan Aerospace Exploration Agency (JAXA): https://global.jaxa.jp/

United States Geological Survey (USGS): https://www.usgs.gov/

Images (mentioned), Animation (mentioned), Videos (mentioned), Text, Credits: nzherald.co.nz/By Qiuyi Tan, Reporter.

Best regards, Orbiter.ch

Data-relay system connects astronauts direct to Europe

 







ISS - International Space Station emblem.


Jan 17, 2022

Astronauts on board the International Space Station are connecting straight to Europe at light speed, thanks to the European Data Relay System.

Shiny Columbus during spacewalk

An upgrade to the communications system is delivering broadband internet speeds similar to those enjoyed by families on Earth.

It means that experiments on board the International Space Station can be monitored from Europe in close to real time. Until now, data from investigations into the effects of radiation on seeds and biomining research had to be stored on hard drives and returned to Earth many months later.

Astronauts on board the International Space Station are connecting via a radio link to one of the two geostationary satellites that form the European Data Relay System. The satellite picks up signals from the Station as it loops around the Earth every 90 minutes and relays them straight back to its European base station.

The state-of-the-art system provides speeds of up to 50 Mbit/s for downlink and up to 2 Mbit/s for uplink. The communications device which enables it – nicknamed ‘ColKa’ for ‘Columbus laboratory Ka-band terminal’ – was installed during a spacewalk in January 2021.

The Colka communications device was installed during a spacewalk

ColKa uses the European Data Relay System, which was developed as an ESA Partnership Project with satellite manufacturer Airbus, as part of ESA’s efforts to federate industry around large-scale commercial telecommunication programmes, stimulating innovative service developments to achieve economic benefits.

ESA and Airbus signed a two-year contract on 29 November 2021 to deliver data from the Station to Europe.

Colka was designed and built by British and Italian companies, using products from Belgium, Canada, France, Germany and Norway, some of which have been qualified under ESA’s Telecommunications and Integrated Applications programme of Advanced Research in Telecommunications Systems (ARTES).

Space Station communications infographic

The knowledge gained from designing, building and running ColKa will be instrumental for ESA’s telecommunications package under the ESPRIT telecommunications and refuelling module that is being designed for the lunar Gateway – an outpost over 1000 times farther from Earth than the International Space Station that will provide vital support for a sustainable, long-term human return to the lunar surface.

Related links:

Telecommunications & Integrated Applications: https://www.esa.int/Applications/Telecommunications_Integrated_Applications

International Space Station (ISS): https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/International_Space_Station

Images, Text, Credits: ESA/L. Parmitano, CC BY-SA 3.0 IGO/NASA.

Greetings, Orbiter.ch

dimanche 16 janvier 2022

Unusual Comet Chiron

 







Moscow Planetarium logo.


Jan 16, 2022

This object was discovered in 1977 by American astronomer Charles Koval at the private Palomar Observatory (California, USA). It was named after the centaur Chiron from ancient Greek mythology. The discovery of Chiron was an event and aroused great interest among scientists, as it was the first object discovered in orbit far outside the asteroid belt.

Chiron's orbit in the solar system

Later, by decision of the IAU, all other objects of this class began to be called centaurs. This is a group of asteroids located between the orbits of Jupiter and Neptune, transitional in characteristics between the main belt asteroids and Kuiper belt objects. Therefore, some of them look like comets and have unstable, highly elongated orbits.

The dimensions of space objects are determined based on the absolute magnitude and albedo, but in the case of Chiron, it is very difficult to estimate these parameters, since the variable cometary activity does not allow this to be done accurately. Therefore, data on the size of Chiron are approximate - from 180 to 220 km.

Photo of Chiron and his coma. Hubble Space Telescope, 1996

Immediately after the discovery, Chiron was classified as an asteroid, which was designated: "2060 Chiron". Already in 1988, he had signs of cometary activity. As a result, it was assigned to the class of short-period comets with the designation: "95P / Chiron". Currently, it is one of the few objects that belong to both asteroids and comets, indicating that there is no clear boundary between these two classes of objects.

Source: Moscow Planetarium.

Related links:

ROSCOSMOS Press Release: https://www.roscosmos.ru/33833/

Moscow Planetarium: https://www.roscosmos.ru/tag/moskovskiy-planetariy/

Comet: https://www.roscosmos.ru/tag/kometa/

Images, Text, Credits: ROSCOSMOS/Moscow Planetarium/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch