mardi 15 février 2022

Deep down temperature shifts give rise to eruptions

 





ESA - GOCE Mission logo.


Feb 15, 2022

The astonishing force of the Tonga volcanic eruption shocked the world, but the fact that this underwater volcano actually erupted came as less of a surprise to geoscientists using satellite data to study changes in the temperature deep below Earth’s surface.

The cataclysmic explosion of the Hunga Tonga-Hunga Ha‘apai volcano in January is reported to have been the biggest eruption recorded anywhere on the planet in 30 years. It sent a plume of ash soaring into the sky, left the island nation of Tonga smothered in ash, sonic booms were heard as far away as Alaska and tsunami waves raced across the Pacific Ocean.

While the Tonga eruption was powerful but short, last year’s eruption of the Cumbre Vieja volcano on the Spanish Canary Island of La Palma was less explosive but lasted for almost three months.

Although different, both of these recent eruptions remind us all of how devastating nature can be. A better understanding of the natural processes that are occurring deep below our feet might bring the possibility of predicting eruptions a little closer.

Hot and cold beneath Tonga volcano

This is one of the aims of ESA’s Science for Society 3D Earth project where an international group of geoscientists joined forces to develop a state-of-the art global model of the lithosphere, which is a term to describe Earth’s brittle crust, the top part of the upper mantle and the sub-lithospheric upper mantle down to 400 km depth. The model combines different satellite data, such as gravity data from ESA’s GOCE, with in-situ observations, primarily seismic tomography.

In their model that shows differences in temperature, or the thermal structure, of Earth’s upper mantle, the researchers could see that these volcanoes would erupt at some point. Predicting exactly when this would happen is, however, more difficult.

Javier Fullea, from Complutense University of Madrid, said, “Our WINTERC-G model, which uses in-situ tomographic and GOCE satellite gravity data, shows a branch of the Azores plume. It is visible from the surface down to a depth of 400 km, at the base of the upper mantle. The plume flows southeast towards Madeira and the Canary Islands surrounding the cold mantle beneath the north Atlantic’s African margin.

“Across the globe, we see that the Hunga Tonga volcano is located in a back arc basin, created by the subduction of the Tonga slab. Back arc volcanoes are associated with the cold slab being melted by the mantle as the slab slides down into the mantle.”

Rising heat below La Palma volcano

Sergei Lebedev, from the University of Cambridge in the UK, adds, “From such models and seismic tomography, we see structures rising from great depth beneath the Canary Islands. These anomalies reflect hot material rising to the surface of Earth and are referred to as hotspots or plumes and are a constant source for the volcanos at the surface.

“The origin of the Hunga Tonga-Hunga Ha‘apai volcano is different. It is a part of the Tonga–Kermadec arc, where the edge of the Pacific tectonic plate dives beneath the Australian Plate. Here, our imaging shows the layer of hydrated, partially molten rock above the plunging Pacific Plate, which feeds the volcanoes of the arc.”

But where do these thermal anomalies come from?

The answer lies even deeper, at a depth of around 2800 km, and is associated with structures at the core–mantle boundary: the Large-Low Seismic Velocity Provinces (LLSVPs). These prominent continent-sized structures appear to have a big impact on how the surface behaves.

Clint Conrad, from Norway’s Centre for Earth Evolution Dynamics, said, “There is a link between the flow in the mantle, where convection cells drive plate tectonics, and major plume locations. The flow along the core–mantle boundary pushes plume material against the LLSVPs, forming the plumes. In models, this flow is driven by downwelling slabs that surround the two LLSVPs. The Canary Islands, for example, site above the edge of the African LLSVP.”

However, the exact origin and build-up of the LLSVPs remains elusive. At the recent 4D Earth Science meeting alternative concepts and ideas were discussed using satellite data and seismological models, which will hopefully lead to more detailed studies of Earth interior in the near future.

Bart Root from TU Delft, one of the organisers, summarises, “Clearly a multidisciplinary approach is needed, where different types of satellite data are combined with seismological data in a common way to address the exact structure of Earth’s deep interior.”

GOCE

ESA’s Diego Fernandez noted, “I’m happy to see that this ESA Science for Society project is yielding results that will further improve our understanding of the deep-lying sources of the events such as we’ve just seen in La Palma and Tonga.

“It is worth noting that data from the GOCE satellite has been key to this research. GOCE, which mapped variations in Earth’s gravity field with extreme detail and precision, completed its mission in orbit back in 2013 – and scientists still rely on the data. This is another example of the benefits our satellite missions bring well beyond their life in orbit. ”

Related links:

GOCE: https://www.esa.int/Applications/Observing_the_Earth/FutureEO/GOCE

FutureEO: https://www.esa.int/Applications/Observing_the_Earth/FutureEO

ESA’s Science for Society 3D Earth project: https://eo4society.esa.int/projects/stse-3d-earth/

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

Images, Text, Credits: ESA/Planetary Visions/AOES-Medialab.

Best regards, Orbiter.ch

Innovation by the dozen: ESA funds 12 new OPS-SAT experiments

 





ESA - OPS-SAT patch & ESA logo.


Feb 15, 2022

ESA's OPS-SAT is a Swiss army knife in orbit. The 30-cm CubeSat packs a powerful onboard computer and an array of instruments that make it the ideal laboratory for testing innovative new technologies in space.

Thanks to the ESA Discovery programme, 12 new experiments will be doing just that, as they develop software, concepts and protocols that push the robust CubeSat to its limits and that could one day be essential parts of future spacecraft missions.

OPS-SAT – the flying laboratory

The OPS-SAT Space Lab is ESA's only spacecraft open to innovation for anyone in Europe and enables new and exciting ideas to be tested live in space without the risk of damaging a multi-million-Euro satellite. Last summer, ESA's Discovery programme issued a call for ideas for European industry and academia to apply to win funding and fly their experiments on a flight computer more powerful than any ESA has launched before.

"We were overwhelmed by the quality of the proposals we received," says OPS-SAT spacecraft manager David Evans. "Our first task was to assess them on their innovativeness, with many more than we expected passing with flying colours. That made it really tricky to narrow them down."

OPS-SAT replica

55 proposals in total were submitted through ESA's Open Space Innovation Platform (OSIP). 12 have now been awarded funding. The experiment ideas covered a wide range of ESA's activities: telecommunications, spacecraft operations, Earth observation, technology development and more, to the excitement of many across ESA.

"I am really impressed by the diversity of ideas people came up with for experiments that could be flown on OPS-SAT," adds David. "Particularly those using artificial intelligence. AI is a broad term for an effectively infinite toolbox, and it was great to see concrete applications using a variety of tools from across the field. It's clear to me that when we give academia and industry access to such a powerful processor on a satellite, there is no end to the creative things they’ll think to do with it."

More than the sum of their parts

With its call for ideas for OPS-SAT experiments, ESA was looking for innovative proposals that would benefit from the opportunity to demonstrate their concept in orbit on an active spacecraft. Proven experience in space and the investment of ESA funding are important steps for a concept's development and can help further legitimise it in the view of other potential stakeholders.

"The return on investment for all parties is improved when ESA shows its willingness to invest in these ideas," says David. "It's impressive what European industry produced with some initial seed funding. It has helped unlock further resources for industrial innovation by instilling confidence in the ideas."

OPS-SAT captures our home in space

For many experimenters seeking to build confidence in the potential commercial applications of their work, OPS-SAT is a unique opportunity. As there are multiple different teams carrying out many different experiments on board the CubeSat at once, some experimenters can offer their experiments as services to others to the benefit of all.

OPS-SAT experimenters designing flexible artificial intelligence algorithms for handling image data or designing generic ways to compress telemetry data, for example, can offer their own experiments as services to other teams that need to analyse images or send lots of data down to Earth. In doing so, the users don't have to reinvent existing applications and can focus on their experiments, while the service providers gain initial experience with feedback from end users representative of their potential future customers.

Innovation today, essential tomorrow

One of the areas ESA was particularly interested in receiving ideas was on the potential uses of OPS-SAT's Field Programmable Gate Arrays (FPGAs).

Not long ago, updating the software on a spacecraft after launch was a nail-biting affair. What if something went wrong while the spacecraft was rebooting? What if something didn't reboot correctly? While a spacecraft operator might still let out an audible sigh of relief after a software update today, they are a powerful and necessary tool for getting the most out of a satellite throughout its lifetime and for recovering a spacecraft experiencing issues.

Now, reconfiguring hardware in flight is the new frontier. Spacecraft hardware is directly controlled by a layer of simple software known as firmware – more similar to the software in the integrated chip in your refrigerator than that running your web browser right now.

Altering this firmware after launch is still risky business. But technologies like OPS-SAT's FPGAs open up new possibilities for reconfiguring satellite hardware in flight in a safe and controlled manner. This is one of the next big areas of opportunity for innovation in spacecraft operations and OPS-SAT offers a unique test-bed for the experimental approaches today that may become important routine tools tomorrow.

The Open Space Innovation Platform

OSIP provides a flexible platform that helps ESA discover novel ideas and invest in unconventional activities to support the advancement of the European space industry. The platform brings together exciting ideas from companies and institutions in Europe with ESA experts like David Evans to take them to the next level.

The Open Space Innovation Platform

"I was really impressed with how OSIP helped us reach new audiences and increase the awareness of OPS-SAT in academic and industrial communities in Europe," says David. "As a result, we have a good number of new faces who are running their first experiments on OPS-SAT under this campaign. We are very excited to see how they'll approach it."

Related article:

Interplanetary internet & cameras in space: ESA’s OPS-SAT first results
https://orbiterchspacenews.blogspot.com/2020/12/interplanetary-internet-cameras-in.html

Related links:

OPS-SAT: https://www.esa.int/Enabling_Support/Operations/OPS-SAT

Discovery and Preparation: https://www.esa.int/Enabling_Support/Preparing_for_the_Future/Discovery_and_Preparation

ESA's Open Space Innovation Platform (OSIP): https://ideas.esa.int/

Animation, Images, Text, Credits: ESA/Stijn Laagland.

Greetings, Orbiter.ch

lundi 14 février 2022

Russian Cargo Craft Blasts off to Resupply Station

 






ROSCOSMOS - Russian Vehicles patch.


Feb 15, 2022

The uncrewed Russian Progress 80 is safely in orbit headed for the International Space Station following launch at 11:25 p.m. EST (9:25 a.m. on Feb. 15 Baikonur time) from the Baikonur Cosmodrome in Kazakhstan.


Image above: Russia’s Progress 80 resupply ship blasted off on Feb. 14 at 11:25 p.m. EST from the Baikonur Cosmodrome in Kazakhstan. Image Credit: NASA TV.

The resupply ship reached preliminary orbit and deployed its solar arrays and navigational antennas as planned on its way to meet up with the orbiting laboratory and its Expedition 66 crew members.

After making 34 orbits of Earth on its journey, Progress will dock to the station’s Poisk module on the space-facing side of the Russian segment at 2:06 a.m. Thursday, Feb. 17. Live coverage on NASA TV of rendezvous and docking will begin at 1:30 a.m.

Progress MS-19 launch (on-board camera view)

Progress will deliver almost three tons of food, fuel and supplies to the International Space Station. The Russian space agency Roscosmos will determine a departure date for Progress 80.

Related link:

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

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

Best regards, Orbiter.ch

Crew Gets Ready for Pair of Cargo Missions Launching this Week

 







ISS - Expedition 66 Mission patch.


Feb 14, 2022

A Russian cargo craft is at its launch pad counting down to a lift off tonight to resupply the International Space Station. Meanwhile, the seven-member Expedition 66 crew stayed focused on a variety of research activities while getting ready for another cargo mission due to arrive early next week.

Russia’s ISS Progress 80 resupply ship stands at its launch pad at the Baikonur Cosmodrome in Kazakhstan loaded with nearly three tons of food, fuel, and supplies. The 80th cargo mission from Roscosmos is due to launch tonight at 11:25 p.m. EST and automatically dock to the Poisk module on Thursday at 2:06 a.m. live on NASA TV and the agency’s website and the NASA app.


Image above: The Nauka multipurpose laboratory module and the Prichal docking module are pictured as the space station orbited above Australia. Image Credit: NASA.

A U.S. cargo mission is also on tap to launch on Saturday at 12:40 p.m. from Wallops Flight Facility in Virginia. The Northrop Grumman Cygnus space freighter will arrive at a point about 10 meters from the space station when the Canadarm2 robotic arm, commanded by NASA Flight Engineer Raja Chari, will capture the vehicle at 4:35 a.m. next Monday. Robotics controllers on the ground will take over shortly afterward and remotely install Cygnus to the Unity module a couple of hours later. Chari and his back up NASA Flight Engineer Kayla Barron are training today on a computer for the upcoming robotics activities.

While two rockets are getting ready to blast off to the orbiting lab this week, the space lab residents stayed busy today with space science and station maintenance activities.

Progress MS-19 ready for launch

NASA Flight Engineer Mark Vande Hei continued setting up the Combustion Integrated Rack for the upcoming SoFIE, or Solid Fuel Ignition and Extinction, series of fire safety studies. Astronaut Matthias Maurer of ESA (European Space Agency) participated in a vision test then wore a specialized body suit that stimulates muscles for the EasyMotion exercise study. NASA astronaut Thomas Marshburn started the day on computer maintenance before spending the afternoon in the Tranquility module working on the U.S. treadmill.

Commander Anton Shkaplerov of Roscosmos activated the EarthKAM experiment in the Harmony module for a weeklong session of Earth photography remotely-controlled by students on the ground. Flight Engineer Pyotr Dubrov continued setting up the Nauka multipurpose laboratory module for operations.

Related links:

NASA TV: https://www.nasa.gov/nasalive

Expedition 66: https://www.nasa.gov/mission_pages/station/expeditions/expedition66/index.html

Poisk module: https://www.nasa.gov/mission_pages/station/structure/elements/poisk-mini-research-module-2

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

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

Combustion Integrated Rack: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=317

Solid Fuel Ignition and Extinction: https://go.nasa.gov/3oxUJ54

EasyMotion: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8526

Tranquility module: https://www.nasa.gov/mission_pages/station/structure/elements/tranquility/

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

Nauka multipurpose laboratory module:  https://www.roscosmos.ru/tag/nauka/

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

Image (mentioned), Video, Text, Credits: NASA/Mark Garcia/Roscosmos/SciWews.

Greetings, Orbiter.ch

NASA’s IXPE Sends First Science Image

 








 

 NASA & ASI - Imaging X-Ray Polarimetry Explorer (IXPE) patch.

Feb 14, 2022

In time for Valentine’s Day, NASA’s Imaging X-Ray Polarimetry Explorer which launched Dec. 9, 2021, has delivered its first imaging data since completing its month-long commissioning phase.

All instruments are functioning well aboard the observatory, which is on a quest to study some of the most mysterious and extreme objects in the universe.  

IXPE first focused its X-ray eyes on Cassiopeia A, an object consisting of the remains of a star that exploded in the 17th century. The shock waves from the explosion have swept up surrounding gas, heating it to high temperatures and accelerating cosmic ray particles to make a cloud that glows in X-ray light. Other telescopes have studied Cassiopeia A before, but IXPE will allow researchers to examine it in a new way.


Image above: This image of the supernova Cassiopeia A combines some of the first X-ray data collected by NASA’s Imaging X-ray Polarimetry Explorer, shown in magenta, with high-energy X-ray data from NASA’s Chandra X-Ray Observatory, in blue. Image Credits: NASA/CXC/SAO/IXPE.

In the image above, the saturation of the magenta color corresponds to the intensity of X-ray light observed by IXPE. It overlays high energy X-ray data, shown in blue, from NASA’s Chandra X-Ray Observatory. Chandra and IXPE, with different kinds of detectors, capture different levels of angular resolution, or sharpness. An additional version of this image is available showing only IXPE data. These images contain IXPE data collected from Jan. 11 to 18.

After Chandra launched in 1999, its first image was also of Cassiopeia A. Chandra’s X-ray imagery revealed, for the first time, that there is a compact object in the center of the supernova remnant, which may be a black hole or neutron star.

“The IXPE image of Cassiopeia A is as historic as the Chandra image of the same supernova remnant,” said Martin C. Weisskopf, the IXPE principal investigator based at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “It demonstrates IXPE’s potential to gain new, never-before-seen information about Cassiopeia A, which is under analysis right now.”

NASA’s Imaging X-Ray Polarimetry Explorer or IXPE. Image Credit: NASA

A key measurement that scientists will make with IXPE is called polarization, a way of looking at how X-ray light is oriented as it travels through space. The polarization of light contains clues to the environment where the light originated. IXPE’s instruments also measure the energy, the time of arrival, and the position in the sky of the X-rays from cosmic sources.

“The IXPE image of Cassiopeia A is bellissima, and we look forward to analyzing the polarimetry data to learn even more about this supernova remnant,” said Paolo Soffitta, the Italian principal investigator for IXPE at the National Institute of Astrophysics (INAF) in Rome.


Image above: This image from NASA’s Imaging X-ray Polarimetry Explorer maps the intensity of X-rays coming from the observatory’s first target, the supernova Cassiopeia A. Colors ranging from cool purple and blue to red and hot white correspond with the increasing brightness of the X-rays. The image was created using X-ray data collected by IXPE between Jan. 11-18. Image Credit: NASA.

With polarization data from Cassiopeia A, IXPE will allow scientists to see, for the first time, how the amount of polarization varies across the supernova remnant, which is about 10 light-years in diameter. Researchers are currently working with the data to create the first-ever X-ray polarization map of the object. This will reveal new clues about how X-rays are produced at Cassiopeia A.

“IXPE's future polarization images should unveil the mechanisms at the heart of this famous cosmic accelerator,” said Roger Romani, an IXPE co-investigator at Stanford University. “To fill in some of those details, we’ve developed a way to make IXPE’s measurements even more precise using machine learning techniques. We’re looking forward to what we’ll find as we analyze all the data.”

IXPE launched on a Falcon 9 rocket from Cape Canaveral, and now orbits 370 miles (600 kilometers) above Earth’s equator. The mission is a collaboration between NASA and the Italian Space Agency with partners and science collaborators in 12 countries. Ball Aerospace, headquartered in Broomfield, Colorado, manages spacecraft operations.

Imaging X-Ray Polarimetry Explorer (IXPE): https://www.nasa.gov/mission_pages/ixpe/index.html

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

Best regards, Orbiter.ch

ISRO - PSLV-XL launches EOS-04, INS-2TD and INSPIREsat-1

 







ISRO - Indian Space Research Organisation logo.


Feb 14, 2022

PSLV-C52 carrying EOS-04, INS-2TD and INSPIREsat-1 liftoff

For ISRO’s PSLV-C52 mission, a Polar Satellite Launch Vehicle (PSLV) in “XL” configuration launched three satellites, EOS-04, INS-2TD and INSPIREsat-1, from the First Launch Pad (FLP) of Satish Dhawan Space Centre (SDSC) SHAR, Sriharikota, on 14 February 2022, at 00:29 UTC (05:59 IST).

PSLV-XL launches EOS-04, INS-2TD and INSPIREsat-1

EOS-04 (1710 kg) is a Radar Imaging Satellite designed to provide high quality images under all weather conditions from a Sun-synchronous orbit (SSO) of 529 km. INS-2TD (17.5 kg) is a technology demonstrator satellite from ISRO, having a thermal imaging camera as its payload.

PSLV-C52/EOS-04, INS-2TD and INSPIREsat-1 Mission poster

INSPIREsat-1 (8.1 kg) is a student satellite developed by Indian Institute of Space Science & Technology (11ST), in association with University of Colorado, USA, to improve the understanding of ionosphere dynamics and Sun’s coronal heating processes.

Indian Space Research Organisation (ISRO): https://www.isro.gov.in/

Images, Video, Text, Credits: Indian Space Research Organisation (ISRO)/SciNews/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

Elektra - the first quadruple asteroid

 







ESO - European Southern Observatory logo.


Feb 14, 2022

First observation of a quadruple asteroid

Using the Spectro-Polarimetric High-contrast Exoplanet REsearch facility (SPHERE), installed on European Southern Observatory’s Very Large Telescope at Paranal, Chile, astronomers have imaged a third moon orbiting the asteroid 130 Elektra, making it the first quadruple asteroid ever found.

Elektra - the first quadruple asteroid

Credits:
European Southern Observatory (ESO)
First observation of a quadruple asteroid
Detection of a third moon around (130) Elektra with SPHERE/IFS
Anthony Berdeu, Maud Langlois and Frédéric Vachier
Astronomy & Astrophysics, DOI: 10.1051/0004-6361/202142623

European Southern Observatory (ESO): https://www.eso.org/public/

Image, Video, Text, Credits: SciNews/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch