mardi 20 décembre 2022

NASA InSight – Update

 






NASA - InSight Mars Lander patch.


Dec 20, 2022

NASA InSight’s Power Level as of Dec. 12, 2022

InSight Mars Lander: Probing the Martian Interior. Image Credits: NASA/JPL-Caltech

As of Dec. 12, 2022, InSight is generating an average of ~285 watt-hours of energy per Martian day, or sol. The tau, or level of dust cover in the atmosphere, was estimated at .96 (typical tau levels outside of dust season range from 0.6-0.7).

NASA InSight – Dec. 19, 2022

On Dec. 18, 2022, NASA’s InSight did not respond to communications from Earth. The lander’s power has been declining for months, as expected, and it’s assumed InSight may have reached its end of operations. It’s unknown what prompted the change in its energy; the last time the mission contacted the spacecraft was on Dec. 15, 2022.

The mission will continue to try and contact InSight.

Related articles:

NASA Prepares to Say ‘Farewell’ to InSight Spacecraft
https://orbiterchspacenews.blogspot.com/2022/11/nasa-prepares-to-say-farewell-to.html

NASA’s InSight Gets a Few Extra Weeks of Mars Science
https://orbiterchspacenews.blogspot.com/2022/06/nasas-insight-gets-few-extra-weeks-of.html

InSight's Final Selfie
https://orbiterchspacenews.blogspot.com/2022/05/insights-final-selfie.html

Related link:

InSight Mars Lander: https://www.nasa.gov/mission_pages/insight/main/index.html

Image (mentioned), Text, Credits: NASA/Naomi Hartono.

Best regards, Orbiter.ch

lundi 19 décembre 2022

Week Begins with Bone Research, Cargo Operations Ahead of Spacewalk

 







ISS - Expedition 68 Mission patch.


Dec 19, 2022

Life science and cargo operations kicked off the week for the Expedition 68 crew aboard the International Space Station. Two astronauts are also planning to exit the orbiting lab on Wednesday for a seven-hour spacewalk.

NASA Flight Engineers Josh Cassada and Nicole Mann took turns with Japan Aerospace Exploration Agency (JAXA) Flight Engineer Koichi Wakata on Monday servicing research samples for an experiment exploring how bones heal in space. The investigation may provide insights into debilitating bone conditions helping advance bone healing therapies for patients on and off the Earth.

International Space Station (ISS). Animation Credit: ESA

All three astronauts also partnered with NASA Flight Engineer Frank Rubio and worked throughout Monday inside the Northrop Grumman Cygnus space freighter attached to the Earth-facing port of the Unity module. The quartet rotated in and out of the vehicle unpacking cargo including crew supplies, new science experiments, and station hardware, as well as stowing trash and old gear inside the space freighter for disposal.

Rubio then spent the afternoon installing multi-layer insulation inside the Harmony module’s space-facing international docking adapter to which the SpaceX Dragon resupply ship is docked. Wakata started his day preparing samples for an experiment run inside the Materials Science Laboratory, a space physics research device sponsored by ESA (European Space Agency). Mann photographed a student-designed study that is exploring new methods to degrade plastic waste in space.

Cassada and Rubio are planning to go on their third spacewalk together at 7:45 a.m. EST on Wednesday. The pair will install another roll-out solar array, also known as an International Space Station Roll-Out Solar Array (iROSA), on the space station’s truss structure. This time the duo will maneuver to the opposite side of the truss structure and install the station’s fourth iROSA on the Port-4 truss structure. The pair will spend about seven hours on the installation job live on NASA TV on the agency’s app and its website.

Image above: NASA astronaut and Expedition 68 Flight Engineer Josh Cassada is photographed on Dec. 3, holding a roll-out solar array as he rides the Canadarm2 robotic arm toward the Starboard-4 truss segment installation site. Image Credit: NASA.

NASA and Roscosmos continue to evaluate an external cooling loop leak from the Soyuz MS-22 spacecraft docked to the Rassvet module of the International Space Station. Temperatures and humidity within the Soyuz spacecraft remain within acceptable limits. Roscosmos has identified the source of the leak as the external cooling loop of the Soyuz.

As part of the ongoing evaluation and investigation, a robotic inspection of the suspected leak area was completed Dec. 18, using cameras on the Canadarm2 robotic arm. A small hole was observed, and the surface of the radiator around the hole showed discoloration. Roscosmos is evaluating the imagery to determine if this hole could have resulted from micrometeoroid debris or if it is one of the pre-manufactured radiator vent holes.

Space station operations and research continue while station managers and international partners collect and analyze data, and work to develop a forward course of action for the Soyuz and its crew.

With help from the cosmonauts aboard the station, Roscosmos conducted tests on additional Soyuz systems on Dec. 16, including a short demonstration of the spacecraft’s propulsion system. So far, testing has shown no additional issues.

The Soyuz MS-22 spacecraft carried NASA astronaut Frank Rubio and Roscosmos cosmonauts Sergey Prokopyev and Dmitri Petelin into space after launching from the Baikonur Cosmodrome in Kazakhstan on Sept. 21.

Image above: The Soyuz MS-22 crew ship is pictured docked to the Rassvet module. In the background, the Prichal docking module is attached to the Nauka multipurpose laboratory module. Image Credit: NASA.

The leak was first detected around 7:45 p.m. EST Dec. 14, when pressure sensors in the cooling loop showed low readings. Data analysis indicates the majority of the cooling fluid had leaked out by 1:30 p.m. Dec. 15.

At the time of the leak, Prokopyev and Petelin were preparing to conduct a spacewalk. The spacewalk was postponed, so the cosmonauts did not exit the space station or become exposed to the leaking coolant.

Back inside station, Prokopyev and Petelin configured the Poisk module and its airlock to its normal status. Prokopyev later collected obsolete hardware for disposal aboard Cygnus and also tested a 3D printer. Petelin inspected cable connections and inventoried spare parts aboard the station. Flight Engineer Anna Kikina spent the morning exploring futuristic spacecraft and robotic piloting techniques then worked in the afternoon servicing an oxygen generator.

Related article:

NASA to Air Live Coverage of US Spacewalk for Solar Array Installation
https://www.nasa.gov/press-release/nasa-to-air-live-coverage-of-us-spacewalk-for-solar-array-installation

Related links:

Expedition 68: https://www.nasa.gov/mission_pages/station/expeditions/expedition68/index.html

How bones heal in space: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8846

Unity module: https://www.nasa.gov/mission_pages/station/structure/elements/unity

Harmony module: https://www.nasa.gov/mission_pages/station/structure/elements/harmony

Materials Science Laboratory: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=1854

Port-4 truss structure: https://www.nasa.gov/mission_pages/station/structure/elements/truss-structure

Rassvet module: https://www.nasa.gov/mission_pages/station/structure/elements/rassvet

Canadarm2 robotic arm: https://www.nasa.gov/mission_pages/station/structure/elements/mobile-servicing-system.html

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

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

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

Best regards, Orbiter.ch

NASA Enables Future of Science Observation through Tri-band Antennas

 






NASA - Space Communications and Navigation (SCaN) patch.


Dec 19, 2022

NASA’s Near Space Network enables spacecraft exploring the solar system and Earth to send back essential science data for researchers and scientists to investigate and make profound discoveries.

Near Space Network antennas. Image credit: NASA

Now, the network has integrated four new global antennas to further support science and exploration missions. In December 2022, antennas in Fairbanks, Alaska; Wallops Island, Virginia; Punta Arenas, Chile; and Svalbard, Norway went online to provide present and future missions with S-, X-, and Ka-band communications capabilities.

These new antennas were created to support missions capturing immense amounts of data. Just as scientists increase their instrument capabilities, NASA also advances its communications systems to enable missions near-Earth and in deep space.

This upgrade is bringing unprecedented flexibility to the Near Space Network and will enhance direct-to-Earth communications – the process by which a satellite takes a picture and then sends the image over radio waves to an antenna on Earth. This data is then processed and sent to scientists. The Near Space Network is managed by NASA’s Space Communications and Navigation (SCaN) program office, which oversees development and enhancement of NASA’s two primary communications networks: the Near Space and Deep Space networks.

Image above: KSAT antenna in Svalbard, Norway, with radome fully installed. Image Credit: KSAT.

The Near Space Network provides missions with communications services through a blend of government-owned and commercial assets. To develop these new antennas, the team worked with commercial partner Kongsberg Satellite Services (KSAT), who created the Chile and Norway antennas, while NASA developed the other two in Virginia and Alaska.

Now operational, the four antennas are integrated into the network’s service catalog, advancing its capabilities to support science and exploration missions that use enhanced instrumentation. Now, missions using the network will be able to send back terabytes of data for processing and discovery.

An example is the upcoming Plankton, Aerosol, Clouds, ocean Ecosystem (PACE) mission, which will help researchers better understand ocean ecosystems and carbon cycling and reveal how aerosols might fuel phytoplankton growth on the ocean’s surface.

Image above: NASA's new tri-band antenna in Fairbanks, Alaska. Image Credit: NASA.

“Missions like the PACE satellite incorporate high-resolution science instruments,” said Damaris Guevara, project lead for the networking upgrade. “These instruments require advanced space communications capabilities, like Ka-band, to get the entirety of their data back to Earth.”

The new antennas also will have new networking capabilities.

All four ground stations are incorporating Delay/Disruption Tolerant Networking (DTN). DTN will empower missions with unparalleled connectivity by storing and forwarding data at points along the network to ensure critical information reaches its destination. DTN is an advanced communications capability being developed and tested by NASA’s SCaN and Space Technology Mission Directorate.

Additionally, to enhance mission teams’ access to data, the network incorporates cloud-based data storage services. Satellites like PACE will downlink their data to an antenna, and that data will go through the ground station’s high-rate data processors to a cloud-based storage and data access service that will allow mission teams to acquire their data faster and from almost anywhere. This reduces hardware needs and lowers overall storage costs.

Image above: Rendering of NASA's Plankton, Aerosol, Clouds, ocean Ecosystem (PACE) satellite on orbit. Image Credit: NASA.

Multiple missions will benefit from this new infrastructure and advanced capabilities, including the NASA-Indian Space Research Organization Synthetic Aperture Radar (NISAR) satellite. Launching in 2024, NISAR will measure Earth’s changing ecosystems, dynamic surfaces, ice masses, and more.

With four new antennas around the globe, the Near Space Network is advancing its capabilities to support science and exploration missions that use enhanced instrumentation. Now, missions using the network will be able to send back terabytes of data for processing and discovery.

Related links:

Near Space Network (NSN): https://esc.gsfc.nasa.gov/projects/NSN

Space Communications and Navigation (SCaN): https://www.nasa.gov/directorates/heo/scan/index.html

Deep Space Networks (DSN): https://www.nasa.gov/directorates/heo/scan/services/networks/deep_space_network

Kongsberg Satellite Services (KSAT): https://www.ksat.no/

Delay/Disruption Tolerant Networking (DTN): https://www.nasa.gov/directorates/heo/scan/engineering/technology/delay_disruption_tolerant_networking

NASA-Indian Space Research Organization Synthetic Aperture Radar (NISAR): https://nisar.jpl.nasa.gov/

Plankton, Aerosol, Clouds, ocean Ecosystem (PACE): https://pace.gsfc.nasa.gov/

Images (mentioned), Text, Credits: NASA/GSFC/By Katherine Schauer.

Greetings, Orbiter.ch

Teams Train for Starliner’s First Crewed Flight

 











Boeing / NASA - Crew Flight Test (CFT) Mission patch.


Dec 19, 2022

NASA and Boeing teams continue to conduct training and testing ahead of the Boeing Crew Flight Test (CFT), scheduled to launch in April 2023 to the International Space Station for the agency’s Commercial Crew Program.

For the crewed flight test, Boeing’s CST-100 Starliner spacecraft will launch aboard a United Launch Alliance Atlas V rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station in Florida, returning approximately eight days later in White Sands, New Mexico.

Image above: The NASA astronauts for Boeing’s Crew Flight Test (CFT) arrive in the high bay of Boeing’s Commercial Crew and Cargo Processing Facility at NASA’s Kennedy Space Center in Florida on Oct. 18, 2022. From left are Suni Williams, pilot; Barry “Butch” Wilmore, commander; and Mike Fincke, CFT backup spacecraft test pilot. Photo credit: Boeing.

Most recently, the CFT Super Suited Week took place at NASA’s Johnson Space Center in Houston in late October through early November. During the training, NASA astronauts Barry “Butch” Wilmore and Suni Williams, CFT commander and pilot, respectively, and Mike Fincke, CFT backup spacecraft test pilot, donned their spacesuits while participating in various simulations, good day and bad day scenarios, and spacecraft ingress and egress. The event also gave the crew extended time to get comfortable wearing their suits.

Prior to that, the astronauts participated in a crew validation test in October to evaluate and fine tune operations. These tests provide astronauts with hands-on training while giving the launch pad crew further experience with crucial tasks. In addition, teams can address issues encountered during previous checks and identify items that still need to be resolved prior to launch.

During the exercise, the astronauts suited up and tested the pressurized crew module to assess seat fit, suit functionality, cabin temperature, audio, and day of launch operations. The teams cycled through different environmental control configurations and flow rates, including oxygen and emergency gas, so the crew will be accustomed to a variety of scenarios on orbit. The astronauts also familiarized themselves with camera, tablet, and wireless application set-up. Communication checks went well between the Mission Control Center and the crew in the spacecraft.

Boeing CST-100 Starliner. Animation Credit: Boeing

Overall, the training activities gave the astronauts and support teams confidence in operations and built their knowledge base for subsequent flight preparation activities.

“Preparing for this flight doesn’t feel like traditional training that Suni and I went through for missions on the space shuttle or Soyuz,” Wilmore said. “We’re thoroughly embedded in all aspects of developing a brand-new spacecraft, making this more akin to an experimental process. The entire team is learning how to plan, train, and fly Starliner into space.”

Following a successful CFT mission, NASA will begin the final process of certifying the Starliner spacecraft and systems for crew missions to the space station. Regular, long-duration commercial crew rotation missions enable NASA to continue the research and technology investigations taking place aboard the orbiting laboratory. Such research benefits people on Earth and lays the groundwork for future exploration of the Moon and Mars, starting with the agency’s Artemis missions, which include landing the first woman and first person of color on the lunar surface.

Related links:

NASA’s Commercial Crew Program: https://www.nasa.gov/exploration/commercial/crew/index.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

Image (mentioned), Animation (mentioned), Text, Credits: NASA/Linda Herridge.

Greetings, Orbiter.ch

40-Year Study Finds Mysterious Patterns in Temperatures at Jupiter

 






Jupiter animated. 


Dec 19, 2022

Based partly on data from generations of NASA missions, including NASA’s Voyager and Cassini, the work could help scientists determine how to predict weather on Jupiter.

Image above: These infrared images of Jupiter with color added were obtained by the European Southern Observatory’s Very Large Telescope in 2016 and contributed to the new study. The colors represent temperatures and cloudiness: The bluer areas are cold and cloudy, and the orange areas are warmer and cloud-free. Image Credits: ESO/L.N. Fletcher.

Scientists have completed the longest-ever study tracking temperatures in Jupiter’s upper troposphere, the layer of the atmosphere where the giant planet’s weather occurs and where its signature colorful striped clouds form. The work, conducted over four decades by stitching together data from NASA spacecraft and ground-based telescope observations, found unexpected patterns in how temperatures of Jupiter’s belts and zones change over time. The study is a major step toward a better understanding of what drives weather at our solar system’s largest planet and eventually being able to forecast it.

Jupiter’s troposphere has a lot in common with Earth’s: It’s where clouds form and storms churn. To understand this weather activity, scientists need to study certain properties, including wind, pressure, humidity, and temperature. They have known since NASA’s Pioneer 10 and 11 missions in the 1970s that, in general, colder temperatures are associated with Jupiter’s lighter and whiter bands (known as zones), while the darker brown-red bands (known as belts) are locations of warmer temperatures.

But there weren’t enough data sets to understand how temperatures vary over the long-term. The new research, published Dec. 19 in Nature Astronomy, breaks ground by studying images of the bright infrared glow (invisible to the human eye) that rises from warmer regions of the atmosphere, directly measuring Jupiter’s temperatures above the colorful clouds. The scientists collected these images at regular intervals over three of Jupiter’s orbits around the Sun, each of which lasts 12 Earth years.

In the process, they found that Jupiter’s temperatures rise and fall following definite periods that aren’t tied to the seasons or any other cycles scientists know about. Because Jupiter has weak seasons – the planet is tilted on its axis only 3 degrees, compared to Earth’s jaunty 23.5 degrees – scientists didn’t expect to find temperatures on Jupiter varying in such regular cycles.

The study also revealed a mysterious connection between temperature shifts in regions thousands of miles apart: As temperatures went up at specific latitudes in the northern hemisphere, they went down at the same latitudes in the southern hemisphere – like a mirror image across the equator.

“That was the most surprising of all,” said Glenn Orton, senior research scientist at NASA’s Jet Propulsion Laboratory and lead author of the study. “We found a connection between how the temperatures varied at very distant latitudes. It’s similar to a phenomenon we see on Earth, where weather and climate patterns in one region can have a noticeable influence on weather elsewhere, with the patterns of variability seemingly ‘teleconnected’ across vast distances through the atmosphere.”

The next challenge is to find out what causes these cyclical and seemingly synchronized changes.

“We’ve solved one part of the puzzle now, which is that the atmosphere shows these natural cycles,” said co-author Leigh Fletcher of the University of Leicester in England. “To understand what’s driving these patterns and why they occur on these particular timescales, we need to explore both above and below the cloudy layers.”

One possible explanation became apparent at the equator: The study authors found that temperature variations higher up, in the stratosphere, seemed to rise and fall in a pattern that is the opposite of how temperatures behave in the troposphere, suggesting changes in the stratosphere influence changes in the troposphere and vice versa.

Decades of Observations

Orton and his colleagues began the study in 1978. For the duration of their research, they would write proposals several times a year to win observation time on three large telescopes around the world: the Very Large Telescope in Chile as well as NASA’s Infrared Telescope Facility and the Subaru Telescope at the Maunakea Observatories in Hawaii.

During the first two decades of the study, Orton and his teammates took turns traveling to those observatories, gathering the information on temperatures that would eventually allow them to connect the dots. (By the early 2000s, some of the telescope work could be done remotely.)

Then came the hard part – combining multiple years’ worth of observations from several telescopes and science instruments to search for patterns. Joining these veteran scientists on their long-duration study were several undergraduate interns, none of whom had been born when the study began. They are students at Caltech in Pasadena, California; Cal Poly Pomona in Pomona, California; Ohio State University in Columbus, Ohio; and Wellesley College in Wellesley, Massachusetts.

Scientists hope the study will help them eventually be able to predict weather on Jupiter, now that they have a more detailed understanding of it. The research could contribute to climate modeling, with computer simulations of the temperature cycles and how they affect weather – not just for Jupiter, but for all giant planets across our solar system and beyond.

“Measuring these temperature changes and periods over time is a step toward ultimately having a full-on Jupiter weather forecast, if we can connect cause and effect in Jupiter’s atmosphere,” Fletcher said. “And the even bigger-picture question is if we can someday extend this to other giant planets to see if similar patterns show up.”

Related links:

Nature Astronomy: https://www.nature.com/articles/s41550-022-01839-0

Jupiter: https://www.nasa.gov/jupiter

Image (mentioned), Text, Credits: NASA/Tony Greicius/Karen Fox/Alana Johnson/JPL/Gretchen McCartney.

Greetings, Orbiter.ch

One year ago, a perfect launch for the James Webb Space Telescope

 











Arianespace / NASA / ESA / CSA - Flight VA256 Mission poster.


Dec 19, 2022

Webb liftoff on Ariane 5

The voice counted backwards in French from ten to one, then announced, “Décollage” – lift-off. The 15-year-long collaboration between NASA, ESA and the Canadian Space Agency had just entered its most critical phase: the launch itself. What happened next would determine whether the James Webb Space Telescope made it into space or not.

Webb launch campaign highlights

“On the day of launch, the pressure was extremely high. We were very confident of our success because we had had basically 15 years of preparation, but still the pressure was high after a long launch campaign with a number of technical issues to solve,” says Daniel de Chambure, Head of the ESA Kourou Office, French Guiana, and previously Ariane 5’s Webb Project Manager.

It is no exaggeration to say that the world was watching. Years of development and promises had turned Webb into a highly anticipated successor to the NASA/ESA Hubble Space Telescope. Webb was nothing less than an ‘Apollo moment’ for astronomy, an extraordinarily complex and ambitious mission. Humankind was waiting for our next ‘big eye in the sky’, a giant leap in technological ability that would extend our vision back to the very origins of galaxies and stars.

The hopes of a new generation of astronomers were riding in the nosecone of the ESA-provided Ariane 5 rocket that had just disappeared into the clouds above Europe’s Spaceport in Kourou, French Guiana.

The ascent itself was scheduled to last about 30 minutes. Kourou’s job would be over when they received confirmation that Webb had automatically deployed its solar panel, was generating its own power, and talking to the team at the Space Telescope Science Institute (STScI) in Baltimore, Maryland, USA.

Rehearsals and simulations

Massimo Stiavelli, who leads the Webb mission office in Baltimore, knew the stakes were high: no solar panel – no mission. In the years leading up to this moment, Massimo and the flight operations team at STScI would perform rehearsals over and over again for what to do with Webb once it was in space. These rehearsals were fully simulated on computers, so they felt very real. At first everything would be ‘nominal’. This means that the spacecraft would behave as expected. Then, the small team of engineers who programmed the simulations would begin to inject anonymous problems into the mix that the flight team would have to diagnose and correct.

“The scariest of these was in the rehearsal when the solar panel didn't deploy. So we were running on batteries and you know that you will run out of energy at some point,” says Massimo.

Impression of Webb’s journey to space

In the simulation, Massimo’s team tried everything. They sent manual commands to order the deployment. When that didn’t work, they started ‘a number of dance moves’ in which they shook the spacecraft, hoping to dislodge the panel. Finally, as time was running out, and the team had tried every trick in the book, the simulation cooperated, and the panel deployed.

“That was very tense, and something that we didn't want to try in real life,” says Massimo.

But before the flight operators took over, Daniel and his team had to make good on their promise of getting Webb safely into orbit.

The extreme accuracy of the launch

The day started early. Daniel woke at 04:00 that Christmas morning and made his way to work, where he confirmed that everything was still nominal with the launcher on the pad. An hour and a half before launch, he entered the main launch control room and oversaw the completion of the last tasks before launch. As a standard procedure, all of these final preparations must be completed forty minutes before launch. Then, the team waits.

“You become a bit stressed because you have to wait,” he says. To take his mind off those stresses he met with the media to answer their questions. Then seven minutes before the launch, he returned to control room as the final countdown began.

Everything was automatic at this stage. The flight operations team devoted their entire attention to monitoring the status of the launcher – ready to abort if something were to go wrong. In the final seconds, ignition took place: first the main engine, then seven seconds later the boosters.         

The rocket left the pad. The operators continued to monitor the telemetry information being sent back by the launcher, looking for even the smallest deviation from what they predicted.

The team followed the ascent and its various steps. First, the boosters were separated, then the fairing opened up into two halves to reveal Webb at an altitude of 110 km, then the first stage separated, the second stage ignited and later shut down. Finally, Ariane let go of Webb at an altitude of 1400 km. The camera on the rocket watched as the space telescope drifted away, making an adjustment to its trajectory as it went. A few minutes later, when it was precisely on its course, Webb automatically deployed its solar panel, and began communicating with Massimo’s team in Baltimore. Daniel and his team had done their job.

But it didn’t quite happen like that.

Webb separation from Ariane 5

In the several minutes it would take for Webb to calculate and execute its trajectory manoeuvre, it was assumed that the spacecraft would drift out of sight of the rocket’s camera, and the solar panel deployment would take place unseen. But 70 seconds after the separation, the solar panel deployed.

In Kourou, the reason was obvious. Ariane’s launch has been so precise that the attitude correction manoeuvre was superfluous. Webb’s onboard software realised this and so it skipped to the next task on the list, which was to deploy the solar panel and make contact with Baltimore. It was a stunning confirmation of the accuracy of the launch.

“I still remember seeing the reactions of the various ESA and NASA colleagues around me when it happened. Everyone was so delighted,” says Daniel.

Special modifications

The extreme accuracy of the launch injection at separation was the result of some additional things that the Kourou team had done. First was the decision to calibrate the launcher’s Inertial Management Units (IMUs) as late as possible before the launch itself. These units return information about how the rocket is moving, and feed back into the onboard computations that control the guidance systems. Being so carefully calibrated, the Ariane 5 knew exactly where it was and where it was going.

Webb and Ariane 5: a fit made perfect

Secondly, the team were very careful to match the pairing and alignment of the acceleration rockets of the upper stage, so that after the upper stage was ignited there was no jitter and the trajectory remained undisturbed.

Beyond the trajectory, the team also made another special modification, this time to protect Webb itself. NASA was extremely concerned that any residual atmosphere in the nosecone could cause that air bubbles trapped into the folded sunshield could inflate and tear-off the telescope’s delicate sunshield layers. So, ESA developed a system that would force the final molecules of air out of the nosecone before the fairing split and exposed Webb to the vacuum of space. “This was also a great achievement for us to see that the residual pressure was well below requirements after several demonstrations carried out on previous Ariane 5 flights,” says Daniel.

While the confirmation that this system had worked did not come until later when the sunshield was unfurled and seen to be undamaged, the early deployment of the solar panel was immediately obvious to the team. Even so, the real value of the launcher’s extreme injection accuracy only became known that evening when the Baltimore team commanded the spacecraft to make another manoeuvre.

Massimo was on duty as they prepared for Mid-Course Correction 1a. This was the essential extra push to make sure Webb was going to successfully reach its designated position 1.5 million km away from Earth. To calculate the rocket burn necessary, Webb was tracked for almost 12 hours and then the flight dynamics team at NASA’s Goddard Space Flight Center crunched the numbers. That’s when the scale of Ariane’s achievement started to become truly obvious.

The orbital injection had been so accurate, the burn would not be anything like as long as was anticipated. “Already there, we knew that we were going to have extra fuel,” says Massimo.

After the manoeuvre, they started tracking and calculating again. It turned out that the fuel they saved could now be used to help Webb stay in its operational orbit, and so extend the mission’s life.

Double the science, double the discoveries

Cosmic Cliffs in Carina – NIRCam

When the calculations were completed, NASA announced that thanks to ESA and its contributing partners Arianespace, ArianeGroup and CNES, the lifetime of Webb was now double. Instead of a 10-year mission, Webb was carrying enough fuel to keep it operational for 20. Double the observations, double the science, double the discoveries.

Webb's portrait of the Pillars of Creation (MIRI)

By turning one routine launch into Ariane 5’s finest hour, the European team had doubled humankind’s next big leap towards understanding its origins.

Webb’s first deep field

“This was a very nice moment and reward for all of us, especially after the many thanks received from the NASA Webb Project team,” says Daniel.

Neptune close-up (NIRCam Image)

At the time, however, the celebration was rather muted. Taking place on Christmas Day 2021, most of the people involved were keen to return home to their families. But the memories of what they achieved that day are still strong.

Protostar L1527

“You see on the base that people are very proud to have launched Webb. You still see them wearing their Webb polo shirts,” says Daniel. And in the understated world of spacecraft operations, there can be no bigger statement of pride than that.

More information

Webb is the largest, most powerful telescope ever launched into space. Under an international collaboration agreement, ESA provided the telescope’s launch service, using the Ariane 5 launch vehicle. Working with partners, ESA was responsible for the development and qualification of Ariane 5 adaptations for the Webb mission and for the procurement of the launch service by Arianespace. ESA also provided the workhorse spectrograph NIRSpec and 50% of the mid-infrared instrument MIRI, which was designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona. Webb is an international partnership between NASA, ESA and the Canadian Space Agency.

Related links:

ESA - James Webb Space Telescope (JWST):

https://www.esa.int/Science_Exploration/Space_Science/Webb

https://esawebb.org/

NASA - James Webb Space Telescope (JWST):

https://www.nasa.gov/mission_pages/webb/main/index.html

https://webb.nasa.gov/

CSA-ASC - James Webb Space Telescope (JWST):

https://www.asc-csa.gc.ca/eng/satellites/jwst/

https://www.asc-csa.gc.ca/eng/satellites/jwst/news.asp

Images, Videos, Text, Credits: ESA/CNES/Arianespace/NASA, ESA, CSA, and STScI, J. DePasquale (STScI), A. Pagan (STScI), CC BY-SA 3.0 IGO.

Best regards, Orbiter.ch

dimanche 18 décembre 2022

CERN - ATLAS moves into top gear for Run 3

 







CERN - ATLAS Experiment logo.


Dec 18, 2022

In their first Run 3 results, the ATLAS collaboration measured two Standard Model processes: the production of Z bosons and top-quark pairs

Image above: Event display of a pair of top quarks decaying, recorded in the ATLAS detector on 18 July 2022. (Image: CERN).

After over three years of upgrade and maintenance work, the Large Hadron Collider began its third period of operation (Run 3) in July 2022. Since then, the world’s most powerful particle accelerator has been colliding protons at a record-breaking energy of 13.6 TeV. The ATLAS collaboration has just released its first measurements of these record collisions, studying data collected in the first half of August 2022.

The researchers measured the rates of two well-known processes: the production of top-quark pairs and the production of a Z boson, which proceed through strong and electroweak interactions, respectively. The ratio of their cross sections is sensitive to the inner structure of the proton, and their measurement sets constraints on the relative probabilities that reactions are initiated by quarks and gluons.

These early measurements also validate the functionality of the ATLAS detector and its reconstruction software, which underwent many improvements in preparation for Run 3.

Physicists focused on Z-boson decays to electron and muon pairs, and on top-quark decays to a W boson and a jet – collimated sprays of particles – originating from a bottom quark. The W boson subsequently decays into one electron or muon and an invisible neutrino. As the analysis uses very early Run 3 data, physicists relied on preliminary calibrations of the leptons, jets and luminosity. These were derived promptly after the first data became available.

ATLAS measured a top-quark pair to Z boson production ratio that is consistent with the Standard Model prediction within the current experimental uncertainty of 4.7%.

The calibration and corresponding uncertainties will be improved as more data is processed. Future updates of the calibration will allow researchers to measure the cross sections with greater precision.

To validate their results, physicists performed a series of cross-checks. These included measuring the ratio of the cross section each time the LHC was injected with a new fill of protons for a data-taking run.

More analyses using the Run 3 data will follow, exploiting the unprecedented energies and the increased LHC data set.

Read more on the ATLAS website: https://atlas.cern/Updates/Briefing/First-Run3-Measurements

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:

Large Hadron Collider (LHC): https://home.cern/about/accelerators/large-hadron-collider

ATLAS experiment: https://home.cern/science/experiments/atlas

Z boson: https://home.cern/science/physics/z-boson

W boson: https://home.cern/science/physics/w-boson-sunshine-and-stardust

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

Image (mentioned), Text, Credits: CERN/By ATLAS collaboration.

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