lundi 7 février 2022

Space Psychology and Ultrasonic Exploration Begin Week on Station

 







ISS - Expedition 66 Mission patch.


Feb 7, 2022

The Expedition 66 crew kicked off the week today exploring how living in space affects psychology and ways to manipulate objects with sound. The residents aboard the International Space Station also serviced U.S. spacesuits and worked on an artificial gravity-generating incubator.

NASA Flight Engineers Kayla Barron and Raja Chari took turns participating in a robotics test for the Behavioral Core Measures experiment on Monday. The monthly sessions investigate how living in a confined space in microgravity affects crew stress, performance, and behavior.


Image above: NASA astronaut Kayla Barron shows off food packets and prepares for lunch aboard the space station’s Unity module. Image Credit: NASA.

Barron then joined ESA (European Space Agency) astronaut Matthias Maurer and practiced measuring fluid pressure in the eye. She also photographed cotton cell samples growing for the Plant Habitat-05 space agriculture study. Maurer and Chari partnered together on Monday afternoon resizing a pair of U.S. spacesuits.

Maurer started his day on the Ultrasonic Tweezers study using acoustics to manipulate objects remotely and without physical contact. Vande Hei assisted the German astronaut during the experiment that explores using ultrasonics to trap and isolate objects to study samples and avoid contamination on planetary surfaces.

International Space Station (ISS). Animation Credit: ESA

NASA astronaut Thomas Marshburn worked throughout Monday on science hardware ensuring critical research operations run smoothly in weightlessness. The three-time station visitor installed and serviced components inside the Cell Biology Experiment Facility, an incubator with an artificial gravity generator. He finally swapped drying agents, or desiccants, inside science freezers that preserve research samples.

Vande Hei joined Roscosmos Flight Engineer Pyotr Dubrov in the station’s Russian segment for more wireless gear maintenance. Commander Anton Shkaplerov set up hardware that will monitor how natural and man-made events on Earth affect the upper atmosphere.

Related links:

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

Behavioral Core Measures: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7537

Plant Habitat-05: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8341

Ultrasonic Tweezers: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8443

Cell Biology Experiment Facility: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=333

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

Best regards, Orbiter.ch

ROSCOSMOS - Soyuz-2.1a launches Kosmos-2553

 







ROSCOSMOS logo.


Feb 7, 2022

Soyuz-2.1a carrying Kosmos-2553 liftoff

A Soyuz-2.1a rocket launched the Kosmos-2553 satellite from the Plesetsk Cosmodrome, Russia, on 5 February 2022, at 07:00 UTC (10:00 local time).

Soyuz-2.1a launches Kosmos-2553

According to official sources, the satellite was placed into the desired orbit and its onboard systems operate normally. The technological spacecraft Kosmos-2553 (Космос-2553) is equipped with newly developed onboard instruments and systems, designed to be tested under conditions of exposure to radiation and heavy charged particles.

ROSCOSMOS: https://www.roscosmos.ru/

Image, Video, Text, Credits: Roscosmos/Ministry of Defence of the Russian Federation/SciNews/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

Major African radio telescope will help to image black holes

 



SKAO - Square Kilometre Array Observatory logo.


Feb 7, 2022

US $25-million facility in Namibia will be Africa’s first millimetre-range radio telescope.


Image above: The Africa Millimetre Telescope in Namibia will be a repurposed version of the Swedish–ESO Submillimetre Telescope, which is currently located in La Silla, Chile. Image Credits: Y. Beletsky (LCO)/ESO.

Astronomers across Africa and Europe have reacted with delight to news that Africa’s first millimetre-range radio telescope is to be built.

The Africa Millimetre Telescope will fill a gap in the coverage of the Event Horizon Telescope (EHT), a global network of telescopes that can receive and analyse radio waves of around 1 millimetre in length — in 2019 they published the first-ever image of a black hole’s edge, known as its event horizon

The telescope will be located on or near Table Mountain in the Gamsberg Nature Reserve in Namibia. It will be a repurposed 15-metre telescope, currently located at La Silla in Chile, which is being donated by the Onsala Space Observatory in Sweden and the European Southern Observatory, headquartered near Munich, Germany.

The project, confirmed at the end of last year, is “another step toward solidifying Africa’s position as a globally competitive and capable player in the field of astronomy”, says Charles Takalana, head of the secretariat at the African Astronomical Society in Cape Town, South Africa. The telescope will “fill a missing observing window on the continent” and will be crucial for Africa’s astrophysics communities, adds Roger Deane, who directs the Wits Centre for Astrophysics at the University of Witwatersrand in Johannesburg, South Africa.

The Africa Millimetre Telescope is a collaboration between Radboud University Nijmegen in the Netherlands and the University of Namibia in Windhoek. It will be about five years before the telescope gets to see first light. The project will cost around US$25 million, including construction, operations and outreach projects in the southern African country. Half of its funding has come from Radboud University. Other funders include the University of Namibia, the European Southern Observatory and the Netherlands Research School for Astronomy in Leiden.

The telescope team is working to complete what is called a critical design review, which will help to determine the observatory’s exact location on the mountain, whether it needs to be adjacent to the mountain, or located at another site; and whether extra funding will be needed.

Telescopes in the millimetre-wavelength range can image the event horizon of a black hole, says project manager Marc Klein Wolt, who is also managing director of the Radboud Radio Lab at Radboud University. At longer wavelengths, “you only saw a blob, but at the millimetre wavelengths, you start to see the edge”.

In 2019, the EHT team published a celebrated image of the supermassive black hole at the centre of the galaxy M87. It was the first picture to show the contour of a black hole’s event horizon. “That image was the start of a new science, like the first observation of gravitational waves was the start of a new science,” Klein Wolt says. Radboud University astrophysicist Heino Falcke, who announced the first black hole image, will be the Africa Millimetre Telescope’s scientific leader.

“You have to have a telescope in the Southern Hemisphere, in southern Africa, to make all those connections [to other telescopes in the network],” Klein Wolt says. “That would allow you to observe [the sky] as the Earth rotates,” he adds.


Image above: The Africa Millimetre Telescope will be built on or close to the 2,347-metre plateau of Mount Gamsberg (pictured), in the Gamsberg Nature Reserve of Namibia. Image Credits: Manfred Gottschalk/Alamy.

However, the EHT will only require about one-fifth of the Africa Millimetre Telescope’s total observation time, says astronomer Michael Backes, co-principal investigator of the project, who is based at the University of Namibia. “The lion’s share of the time will be available for Namibian astronomers to develop their programmes,” he says.

Possible projects in Namibia include monitoring the variations in the brightness of small and large black holes in collaboration with optical telescopes and γ-ray telescopes such as the High Energy Stereoscopic System (HESS), which is also located in Namibia, and the planned Cherenkov Telescope Array in Chile, says Backes.

In the past two decades, telescopes have been set up across southern Africa. Countries with relatively clear skies and low population densities are ideal for astronomy. Telescopes there cover a wide range of wavelengths — from the optical Southern African Large Telescope and radio telescope MeerKAT in South Africa to the HESS telescope in Namibia. Late last year, the Square Kilometre Array (SKA) Observatory began awarding contracts to build its giant radio telescope, which will have thousands of dishes in South Africa and one million antennas in Australia, when the project is complete.

SKAO - a new observatory to explore the Universe

However, finding trained scientists and engineers in the continent has historically been a challenge, says Carla Sharpe, head of the Africa programme at the Cape Town-based South African Radio Astronomy Observatory, which is not yet involved in the Africa Millimetre Telescope. Since 2005, when it threw its hat in the ring to host the SKA, South Africa has awarded more than 1,000 scholarships in astronomy and engineering to fill this talent chasm locally and in SKA Africa partner countries, including Namibia.

Backes says he hopes that the Africa Millimetre Telescope will help to expand Namibia’s astronomy community. Klein Wolt adds that the team is still looking for more funding so that it can finalize the telescope location and continue to train astronomers in Namibia.

Projects such as the Africa Millimetre Telescope will help to achieve a larger programme in Africa in astronomy, radio astronomy and engineering, which are needed to help develop the continent, says Sharpe.

doi: https://doi.org/10.1038/d41586-022-00205-4

Related link:

Nature articles: https://www.nature.com/articles/543478a

https://www.nature.com/articles/d41586-020-00089-2

Event Horizon Telescope (EHT): https://eventhorizontelescope.org/

Square Kilometre Array (SKA) Observatory: https://www.skatelescope.org/

Images, Video, Text, Credits: SKAO/Nature/Sarah Wild.

Best regards, Orbiter.ch

dimanche 6 février 2022

ISS orbital altitude correction postponed to February 8

 






ROSCOSMOS - Russian Vehicles patch.


Feb 6, 2022

The correction of the height of the International Space Station orbit, previously scheduled for February 6, 2022, has been postponed to February 8 due to ballistic conditions.

To ensure the correction, the engines of the Progress MS-18 cargo ship will be involved. According to updated data from the TsNIIMash Mission Control Center (part of the Roscosmos State Corporation), they will be turned on at 10:56 Moscow time and will work for 142.3 seconds.

International Space Station (ISS)

The purpose of the correction is to form ballistic conditions before the launch of the Soyuz MS-21 transport manned spacecraft into orbit (March 18) and the landing of the Soyuz MS-19 (March 30).

Roscosmos cosmonauts Anton Shkaplerov and Pyotr Dubrov, NASA astronauts Mark Vande Hei, Raja Chari, Tom Marshburn and Kayla Barron, as well as European Space Agency astronaut Matthias Maurer are currently on the ISS.

Related article:

ISS orbital altitude correction scheduled for February 6
https://orbiterchspacenews.blogspot.com/2022/02/iss-orbital-altitude-correction.html

Related links:

ROSCOSMOS Press Release: https://www.roscosmos.ru/34051/

TsNIIMash: https://www.roscosmos.ru/tag/cniimash/

MCC: https://www.roscosmos.ru/tag/cup/

Soyuz MS-19: https://www.roscosmos.ru/tag/sojuz-ms-19/

Soyuz MS-21: https://www.roscosmos.ru/tag/sojuz-ms-21/

International Space Station (ISS): https://www.roscosmos.ru/tag/mks/

Image, Text, Credits: ROSCOSMOS/MCC/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

Volcanism on Venus

 







Moscow Planetarium logo.


Feb 6, 2022

Volcanism is characteristic of all planetary bodies of the terrestrial group - Mercury, Venus, Mars, Earth and the Moon. Currently, active volcanic activity has not been detected on any of these objects, except for the Earth.

There are a lot of volcanoes on the surface of Venus, but almost all of them are extinct. According to various sources, the total number of volcanic structures is more than 1600. Its surface consists of basalts of various types, similar to those that form at the bottom of the oceans on Earth.


The composition of the surface of Venus was determined during the landings of Soviet automatic stations. On March 1, 1982, the descent vehicle of the Venera-13 station made a soft landing on the surface of the second planet. Using an X-ray spectrometer, the composition of the rocks at the landing site was studied. As it turned out, the rocks in this place are leucite alkaline basalts, which are very numerous in the earth's crust.

Volcanic lava flows on Venus are much larger than their terrestrial counterparts and reach hundreds of kilometers in length and tens of kilometers in width. The spread of igneous material over such long distances is explained by the high temperature of the atmosphere, which slowed down the process of lava solidification.


Approximately 80% of the planet's surface is occupied by plains formed by lava flows, among which there are more than a hundred large stratovolcanoes (from Latin stratum - layer). It is a type of cone-shaped volcano, consisting of many hardened layers of lava and volcanic ash.

Other volcanic structures include volcanoes called "pancake domes". They are colloquially referred to simply as "pancakes". They form round domes with a diameter of up to 25 km and a height of no more than 700 m. Such volcanoes were formed as a result of eruptions of viscous lava rich in silica, unable to flow far from the source of the eruption.


A special place is occupied by structures that are called "arachnoids" (from the Greek - arachnid). These are large structures of volcanic origin found only on the surface of Venus. They look like concentric ovals connected by a network of faults, having some resemblance to a web, hence the name.

Exact confirmation of the presence of modern volcanic activity on Venus has not been found. But, according to some reports, there is reason to believe that Mount Maat - the second highest hill on Venus - erupted relatively recently. Its slopes are covered with fresh lava flows with no impact craters. Some researchers believe that the eruption of Mount Maat caused the strong fluctuations in the concentration of sulfur dioxide and methane in the atmosphere of Venus, discovered in the 1980s.

Source: Moscow Planetarium.

Related article:

Volcanism on Io
https://orbiterchspacenews.blogspot.com/2022/01/volcanism-on-io.html

Related links:

ROSCOSMOS Press Release: https://www.roscosmos.ru/34039/

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

Astronomy: https://www.roscosmos.ru/tag/astronomija/

Venus: https://www.roscosmos.ru/tag/venera/

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

Greetings, Orbiter.ch

Roscosmos at the request of NASA will lower the orbit of the ISS

 







ROSCOSMOS logo.


Feb 6, 2022

Rocket and Space Corporation Energia named after S.P. Koroleva (part of the Roscosmos State Corporation), at the request of colleagues from NASA, will reduce the average orbital altitude of the International Space Station by several kilometers and will constantly maintain the station’s flight at this altitude in the coming years.

“At the request of the Americans, to ensure the conditions for their experiments, we will move to another orbit. Now we will fly not in an orbit of 419 km, but 3 km less - 416 km, ”said Rafail Murtazin, head of the ballistics department of RSC Energia.

International Space Station (ISS)

According to him, such an average altitude of the ISS orbit can be maintained by the Russian side until a decision is made to flood the station.

The ISS orbit altitude corrections are carried out using the engines of the Zvezda service module of the Russian segment of the station or Progress MS cargo ships docked to it. To date, 314 ISS orbit corrections have been performed, including 165 by Progress spacecraft.

Related links:

ROSCOSMOS Press Release: https://www.roscosmos.ru/34046/

RKK Energia: https://www.roscosmos.ru/tag/rkk-ehnergija/

International Space Station (ISS): https://www.roscosmos.ru/tag/mks/

Image, Text, Credits: ROSCOSMOS/NASA/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

Tonga Eruption Sent Ripples Through Earth’s Ionosphere

 







Natural Disasters logo.


Feb. 6, 2022

NASA detected the shockwave from the underwater eruption high up in the atmosphere.


Animation above: This looping video shows a series of GOES-17 satellite images that caught an umbrella cloud generated by the underwater eruption of the Hunga Tonga-Hunga Ha’apai volcano on Jan. 15, 2022. Crescent-shaped bow shock waves and numerous lighting strikes are also visible. Animation Credits: NASA Earth Observatory image by Joshua Stevens using GOES imagery courtesy of NOAA and NESDIS.

The powerful underwater volcanic eruption that blanketed the island nation of Tonga with ash and sent tsunami waves across the world also caused ripples in Earth’s ionosphere, according to measurements from the Global Differential Global Positioning System (GDGPS) managed by NASA’s Jet Propulsion Laboratory in Southern California.

When the Hunga Tonga-Hunga Ha’apai volcano erupted on Jan. 15, 2022, it unleashed a violent explosion with the equivalent force of 4 to 18 megatons of TNT, according to estimates from NASA geologist Jim Garvin. This explosion produced an acoustic shockwave that was strong enough to perturb the ionosphere, the outer layer of the atmosphere that starts about 50 to 56 miles (80 to 90 kilometers) above Earth’s surface and contains electrons ionized by the Sun’s energy.


Graphic above: In the above image, the vertical red line in the data plot indicates the time of the eruption. The horizontal squiggles show electron density profiles over time, as recorded in the signals of four GNSS constellations, or groups of satellites: GPS, GLONASS, Galileo, and BeiDou. The slanted dashed and dotted lines indicate the velocity of the waves. Graphic Credits: NASA/JPL-Caltech/GDGPS.

The eruption also caused a tsunami, which was enhanced by the atmospheric pressure waves of the explosion – a phenomenon known as a meteotsunami. The deformation of the ocean’s surface from these large waves further disturbed the ionosphere. The GDGPS observed ionospheric disturbances caused by the explosion and subsequent meteotsunami in real time. The system monitors the density of electrons in the ionosphere (measured as total electron content units, or TECU) by tracking the delay of global navigation satellite systems (GNSS) signals as they travel through the atmosphere.

GNSS data can serve an important role in contributing to tsunami early warning systems, shaving precious time off tsunami warnings when every second of advanced notice can save lives. The NASA Research Opportunities in Space and Earth Science (ROSES) A.37 project Local Tsunami Early Warning With GNSS Earthquake Source Products, funded by the Applied Sciences Disasters program area, is using this GNSS data to detect ground movement and model earthquake activity that could lead to tsunamis. The team is integrating this data into tsunami early warning systems operated by the National Oceanic and Atmospheric Administration’s Center for Tsunami Research (CTR).

NASA’s Space Geodesy Project also supports tsunami risk reduction through collaborations with the International GNSS Service, which manages the GNSS-enhanced Tsunami Early Warning Systems (GTEWS), the International Association of Geodesy’s Global Geodetic Observing System (GGOS), and the Group on Earth Observations (GEO) Geodesy for the Sendai Framework Community Activity.

In the future, the ionospheric disturbance recorded by the GDGPS could also be integrated into these tsunami warning systems, increasing their effectiveness to warn communities and get people out of harm’s way before tsunami waves strike.

Related articles:

Dramatic Changes at Hunga Tonga-Hunga Ha‘apai
https://orbiterchspacenews.blogspot.com/2022/01/dramatic-changes-at-hunga-tonga-hunga.html

How the Tonga eruption is helping space scientists understand Mars
https://orbiterchspacenews.blogspot.com/2022/01/how-tonga-eruption-is-helping-space.html

Hunga Tonga-Hunga Ha‘apai Erupts
https://orbiterchspacenews.blogspot.com/2022/01/hunga-tonga-hunga-haapai-erupts.html

Tonga eruption heard in New Zealand, pressure waves picked up in Europe
https://orbiterchspacenews.blogspot.com/2022/01/tonga-eruption-heard-in-new-zealand.html

Related links:

Local Tsunami Early Warning With GNSS Earthquake Source Products: https://appliedsciences.nasa.gov/what-we-do/projects/local-tsunami-early-warning-gnss-earthquake-source-products

Disasters program area: https://appliedsciences.nasa.gov/what-we-do/disasters

NASA’s Space Geodesy Project: https://space-geodesy.nasa.gov/

National Oceanic and Atmospheric Administration’s Center for Tsunami Research (CTR): https://nctr.pmel.noaa.gov/

International GNSS Service: https://igs.org/

GNSS-enhanced Tsunami Early Warning Systems (GTEWS): https://www.undrr.org/publication/global-navigation-satellite-system-enhancement-tsunami-early-warning-systems

Group on Earth Observations (GEO): https://www.earthobservations.org/documents/gwp20_22/GEODESY4SENDAI.pdf

Animation (mentioned), Graphic (mentioned), Text Credits: NASA/JPL/Jane J. Lee/Andrew Wang.

Greetings, Orbiter.ch