Friday, September 30, 2022

Research demonstrates new electric propulsion technology for spacecraft

SEPTEMBER 29, 2022, by George Washington University

Experimental results of the μCAT-MPD thruster performance characterization.
Thrust (A), power in both stages for the short gap 
(B), total power for the long and short gaps
 (C), and ion velocity 
(D) versus the second-stage (MPD) voltage UMPD. Ti cathode, Cathode material is titanium.
Science Advances (2022). DOI: 10.1126/sciadv.adc9850

The most popular electric propulsion technologies used for miniature satellites—the Hall Thruster—has major limitations. Now, new research, led by Michael Keidar, the A. James Clark Professor of Engineering at the George Washington University, demonstrates an important breakthrough in satellite propulsion that suggests a way to use electric engines in different modalities.

Among the findings, Keider and his research team identified metal as a better and more efficient fuel source for the thrusters studied. They also found that it's possible to have an increase in thrust to power ratio in addition to an increase of exhaust velocity.

The paper, "Demonstration of electric micropropulsion multimodality," was published in Science Advances.



Explore further Image: T6 ion thruster firing



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Finland closes a main motorway so fighter jet pilots can practice landings and take-offs

Finland closes one of its main motorways so fighter jet pilots can practice landings and take-offs as it steps up war games amid tensions with Russia over Ukraine invasion

  • The Joutsa site has not been used for decades by the Air Force due to highway
  • But it took the Air Force a few days to clear roadsides and prepare it for exercise
  • They practised landing and 'hot refuelling' a fighter jet with its engines running

Finland has closed one of its main motorways so fighter jets can practice landings and take-offs as it steps up war games amid tensions with Russia over the Ukraine invasion. 

The reserve road base in Joutsa, Central Finland, has not been used for decades due to its importance as the main highway connecting the capital Helsinki to the more northern parts of the country. 

But it took the Air Force just a few days to clear the roadsides and prepare it.

The exercise at the road base in Joutsa involved some 200 staff and Finland's F/A-18 Hornet fighter jets, older Hawk Mk 51 trainer planes and other military aircraft.

Locals gathered on the roadside in Joutsa on Wednesday to follow the drill where pilots practised landing on a 2-kilometre (1.24 mile) stretch of the closed highway.

They watched ground staff rehearsing 'hot refuelling' a fighter jet with its engines running.    

Finland, which is applying for NATO membership amid the war in Ukraine, has a dozen similar reserve runways designed for wartime use around the country.

The reserve road base in Joutsa, Central Finland, has not been used for decades due to its importance as the main highway connecting the capital Helsinki to the more northern parts of the country. But it took the Air Force just a few days to clear the roadsides and prepare the Joutsa site for the exercise. Pictured: One of the jets flying

The reserve road base in Joutsa, Central Finland, has not been used for decades due to its importance as the main highway connecting the capital Helsinki to the more northern parts of the country. But it took the Air Force just a few days to clear the roadsides and prepare the Joutsa site for the exercise. Pictured: One of the jets flying 

Finland, which is applying for NATO membership amid the war in Ukraine, has a dozen similar reserve runways designed for wartime use around the country. The exercise at the road base in Joutsa involved some 200 staff and Finland's F/A-18 Hornet fighter jets, older Hawk Mk 51 trainer planes and other military aircraft. Pictured: One of the air craft

Finland, which is applying for NATO membership amid the war in Ukraine, has a dozen similar reserve runways designed for wartime use around the country. The exercise at the road base in Joutsa involved some 200 staff and Finland's F/A-18 Hornet fighter jets, older Hawk Mk 51 trainer planes and other military aircraft. Pictured: One of the air craft 

People watched ground staff rehearsing 'hot refuelling' a fighter jet with its engines running (pictured is one of the jets)

 People watched ground staff rehearsing 'hot refuelling' a fighter jet with its engines running (pictured is one of the jets)

The head of Finnish Air Force Academy, Colonel Vesa Mantyla, said: 'Mainly I believe all the road bases are in quite good condition so easily taken into the operations in a couple of days.'

In order to protect its fleet, the Finnish Air Force can rapidly disperse all its aircraft across the country and rehearses on the road bases annually. 

Colonel Mantyla said: 'The threat from Russia or the actions from Russia with the cruise missiles and ballistic missiles (in Ukraine) proves that the concept of dispersed operations is right.'

Plane spotters in the area watch the take-offs and landings as the Air Force practise (pictured)

Plane spotters in the area watch the take-offs and landings as the Air Force practise (pictured)

Locals gathered on the roadside in Joutsa on Wednesday to follow the drill where pilots practised landing on a 2-kilometre (1.24 mile) stretch of the closed highway (pictured)

Locals gathered on the roadside in Joutsa on Wednesday to follow the drill where pilots practised landing on a 2-kilometre (1.24 mile) stretch of the closed highway (pictured)

A local pensioner, Veikko Haapala, 79, who was plane spotting, said that he trusted the Finnish defence forces to be able to defend the country, particularly with the help of NATO allies.   

Mr Haapala said: 'I do feel somewhat anxious, given how the world situation has gotten, over how we defend ourselves.'

Meanwhile, another local, Seija Viinikainen, 57, welcomed the exercise amid the Ukraine war turning the situation 'dubious'.

She said: 'Finns too need to be awake and count in even these small countryside runways so that the military is prepared to use them and the conscripts can exercise on them as well.' 

One of the planes involved in the exercise on the tarmac before it takes off (pictured)

One of the planes involved in the exercise on the tarmac before it takes off (pictured)

Crowds of people gathered to see the exercise unfolding in Finland as the country steps up its war games (pictured)

Crowds of people gathered to see the exercise unfolding in Finland as the country steps up its war games (pictured)

The head of Finnish Air Force Academy, Colonel Vesa Mantyla, said: 'Mainly I believe all the road bases are in quite good condition so easily taken into the operations in a couple of days'

The head of Finnish Air Force Academy, Colonel Vesa Mantyla, said: 'Mainly I believe all the road bases are in quite good condition so easily taken into the operations in a couple of days'

It comes after Finland closed its borders to Russian tourists after a huge influx of military aged men fled the country following Putin's mobilisation order.  

Passenger traffic on the border is significantly limited, with Russian civilians on tourist visas no longer allowed to enter the Nordic country.

Thursday, September 29, 2022

Space News: NASA captures clearest view of Neptune's rings in over 30 years

 

NASA captures clearest view of Neptune's rings in over 30 years


NASA’s James Webb Space Telescope has captured the clearest view of Neptune’s rings in over 30 years, allowing the planet to be seen in a new light.


 By SARA WEINSTEIN , Jerusalem Post, SEPTEMBER 28, 2022  



NASA’s James Webb Space Telescope has captured the clearest view of Neptune’s rings in over 30 years, allowing the planet to be seen in a new light. 

The new image shows seven of Neptune’s 14 known moons and provides a very clear view of the planet's rings, some of which have not been seen since 1989 when NASA’s Voyager 2 flew by Neptune and observed it for the first time.

“It has been three decades since we last saw these faint, dusty rings, and this is the first time we’ve seen them in the infrared,” says Neptune system expert and interdisciplinary scientist for Webb Heidi Hammel.

Because of its unique qualities, Neptune has always spiked the fascination of researchers

Discovered in 1846, Neptune is located 30 times farther from the Sun than Earth, orbiting in the remote region of the outer solar system. At such a distance, the Sun is so small that midday on Neptune is similar to a dim evening on Earth.


NASA captures clearest images of Neptune's rings



What discoveries were made from the Webb image?

The chemical makeup of Neptune’s interior characterizes it as an ice giant. Compared to Saturn and Jupiter, which are gas giants, Neptune has more elements that are heavier than hydrogen and helium. This is shown in Hubble Space Telescope images, one of many observations that have recorded methane-ice clouds and their evolving features over the years, as Neptune’s blue appearance at various wavelengths is caused by small amounts of gaseous methane. 

But Neptune does not appear blue to Webb.

“In fact, the methane gas so strongly absorbs red and infrared light that the planet is quite dark at these near-infrared wavelengths, except where high-altitude clouds are present,” writes Laura Betz. “Such methane-ice clouds are prominent as bright streaks and spots, which reflect sunlight before it is absorbed by methane gas.”

Furthermore, scientists recognized a thin, bright line around the planet's equator. 

“A thin line of brightness circling the planet’s equator could be a visual signature of global atmospheric circulation that powers Neptune’s winds and storms,” she writes. “The atmosphere descends and warms at the equator, and thus glows at infrared wavelengths more than the surrounding, cooler gases.”

Webb also revealed seven of Neptune’s 14 known moons, including its largest and brightest moon Triton.

“Covered in a frozen sheen of condensed nitrogen, Triton reflects an average of 70% of the sunlight that hits it. It far outshines Neptune in this image because the planet’s atmosphere is darkened by methane absorption at these near-infrared wavelengths,” writes Betz.

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Wednesday, September 28, 2022

De Havilland Canada to Open New Aircraft Manufacturing Facility in Alberta

22.09.2022 By Canadian Defense Review.


De Havilland Aircraft of Canada Limited has announced that the site of its new aircraft manufacturing facility will be in Wheatland County, Alberta, approximately 30 minutes east of Calgary.

This new facility will be called De Havilland Field and will consist of a new, state-of-the-art aircraft assembly facility, runway, parts manufacturing and distribution centres and maintenance repair and overhaul centre.

In addition, educational space for training the workforce of the future is planned as well as general office buildings and a De Havilland Canada aircraft museum. These operations will complement our current parts manufacturing facilities in Victoria, British Columbia as well as our new engineering and customer support centre of excellence in Toronto, Ontario.

De Havilland Field will be the site of final assembly for the DHC-515 Firefighter aircraft which was launched earlier this year, the DHC-6 Twin Otter as well as the Dash 8-400 aircraft. We are currently working towards bringing the DHC-6 Twin Otter and Dash 8-400 aircraft back into production.

The location of De Havilland Field is ideal, having access to a large, young and diverse labour pool in Alberta, family-friendly cost of living, and a world-class international airport that can support efficient parts distribution to our global customer base. We anticipate that once in full operation, there will be up to 1500 jobs located at De Havilland Field.

The development of De Havilland Field is subject to an amendment to the Wheatland County Area Structure Plan as well as re-zoning by the County. De Havilland expects to submit these applications shortly and is committed to working with Wheatland County and Wheatland County residents as we move through the Area Structure Plan and re-zoning processes. In addition, there are approval processes required by Transport Canada and the Impact Assessment Agency of Canada.


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Tuesday, September 27, 2022

Diamond From 660 Kilometers Below Earth's Surface Reveals a Water-Rich Environment

NATURE: 27 September 2022, By MICHELLE STARR

Some of the major inclusions in the diamond, including enstatite, ringwoodite, coesite, and possibly perovskite.
 (Gu et al., Nat. Geosci., 2022)

Deep below the surface of our world, far beyond our feeble reach, enigmatic processes grind and roil.

Every now and then, the Earth disgorges clues to their nature: tiny chthonic diamonds encasing skerricks of rare mineral. From these tiny fragments we can glean tidbits of information about our planet's interior.

A diamond recently unearthed in a diamond mine in Botswana is just such a stone. It's riddled with flaws containing traces of ringwoodite, ferropericlase, enstatite, and other minerals that suggest the diamond formed 660 kilometers (410 miles) below Earth's surface.

Moreover, they suggest that the environment in which they formed – a divide between the upper and lower mantle called the 660-kilometer discontinuity (or, more simply, the transition zone) – is rich in water.

"The occurrence of ringwoodite together with the hydrous phases indicate a wet environment at this boundary," write a team of researchers led by mineral physicist Tingting Gu of the Gemological Institute of New York and Purdue University.

Most of Earth's surface is clad in ocean. Yet considering the thousands of kilometers between the surface and the planet's core, they're barely a puddle. Even at its deepest point the ocean is just shy of 11 kilometers (7 miles) thick, from the wave-tops to floor.

But Earth's crust is a cracked and fragmented thing, with separate tectonic plates that grind together and slip under each other's edges. At these subduction zones water seeps deeper into the planet, reaching as far as the lower mantle.

Over time it makes its way back to the surface via volcanic activity. This slurp-down, spew-out cycle is known as the deep water cycle, separate from the water cycle active at the surface. Knowing how it works, and how much water is down there, is also important for understanding the geological activity of our planet. The presence of water can influence the explosiveness of a volcanic eruption, for example, and play a role in seismic activity.

Because we can't get down there, though, we have to wait for evidence of the water to come to us, as it does in the form of diamonds that form crystal cages in the extreme heat and pressure.

Gu and her colleagues recently studied just such a gem in detail, finding 12 mineral inclusions and a milky inclusion cluster. Using micro-Raman spectroscopy and X-ray diffraction, the researchers probed these inclusions to determine their nature.

Among the inclusions they found an assemblage of ringwoodite (magnesium silicate) in contact with ferropericlase (magnesium/iron oxide) and enstatite (another magnesium silicate with a different composition).

At the high pressures at the transition zone, ringwoodite decomposes into ferropericlase, as well as another mineral called bridgmanite. At lower pressures closer to the surface, bridgmanite becomes enstatite. Their presence in the diamond tells a story of a journey, indicating the stone formed at depth before making its way back up to the crust.

That wasn't all. The ringwoodite in particular had features suggesting it is hydrous in nature – a mineral that forms in the presence of water. Meanwhile, other minerals found in the diamond, such as brucite, are also hydrous. These clues suggest that the environment in which the diamond formed was pretty danged wet.

Evidence of water at the transition zone has been found before, but this evidence hasn't been sufficient to gauge how much water is down there. Was it a chance inclusion from a small, localized pocket of water, or is it positively sloshy down there? The work of Gu and her team points more towards sloshiness.

"Although the formation of upper-mantle diamonds is often associated with the presence of fluids, super-deep diamonds with similar retrogressed mineral assemblages rarely have been observed accompanied with hydrous minerals," they write in their paper.

"Even though a local H2O enrichment was suggested for the mantle transition zone based on the previous ringwoodite finding, the ringwoodite with hydrous phases, reported here – representative of a hydrous peridotitic environment at the transition zone boundary – indicates a more broadly hydrated transition zone down to and cross the 660-kilometer discontinuity."

Previous research has found that Earth is sucking down way more water than we had thought prior. This could finally give us an answer as to where it's all going.



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Monday, September 26, 2022

Mysterious ripples in the Milky Way were caused by a passing dwarf galaxy

SEPTEMBER 23, 2022, by Lund University
https://phys.org/news/2022-09-mysterious-ripples-milky-dwarf-galaxy.html

Credit: CC0 Public Domain

Using data from the Gaia space telescope, a team led by researchers at Lund University in Sweden has shown that large parts of the Milky Way's outer disk vibrate. The ripples are caused by a dwarf galaxy, now seen in the constellation Sagittarius, that shook our galaxy as it passed by hundreds of millions of years ago.

Our cosmic home, the Milky Way, contains between 100 and 400 billion stars. Astronomers believe that the galaxy was born 13.6 billion years ago, emerging from a rotating cloud of gas composed of hydrogen and helium. Over billions of years, the gas then collected in a rotating disk where the stars, such as our sun, were formed.

In a new study published in Monthly Notices of the Royal Astronomical Society, the research team presents their findings about the stars in the outer regions of the galactic disk.

"We can see that these stars wobble and move up and down at different speeds. When the dwarf galaxy Sagittarius passed the Milky Way, it created wave motions in our galaxy, a little bit like when a stone is dropped into a pond," Paul McMillan, the astronomy researcher at Lund Observatory who led the study, explains.

By using data from the European space telescope Gaia, the research team was able to study a much larger area of the Milky Way's disk than was previously possible. By measuring how strong the ripples are in different parts of the disk, the researchers have begun to piece together a complex puzzle, providing clues about Sagittarius' history and orbit around our home galaxy.

"At the moment, Sagittarius is slowly being torn apart, but 1–2 billion years ago it was significantly larger, probably around 20% of the mass of the Milky Way's disk," says Paul McMillan.

The researchers were surprised by how much of the Milky Way they could study using the data from Gaia. To date the telescope, which has been in operation since 2013, has measured the movement across the sky of approximately two billion stars and the movement towards or away from us of 33 million.

"With this new discovery, we can study the Milky Way in the same way that geologists draw conclusions about the structure of the Earth from the seismic waves that travel through it. This type of 'galactic seismology' will teach us a lot about our home galaxy and its evolution," Paul McMillan concludes.




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Saturday, September 24, 2022

Planetary-scale 'heat wave' discovered in Jupiter's atmosphere

SEPTEMBER 23, 2022, by Europlanet Media Centre

Europlanet Media Centre A panning-view of Jupiter’s upper atmospheric temperatures, 1000 kilometers above the cloud tops. Jupiter is shown on top of a visible image for context. In this snapshot, the auroral region (near the northern pole, in yellow/white) appears to have shed a massive, planetary-scale wave of heating towards the equator. The feature is over 130,000 kilometers long, or 10-Earth diameters, and is hundreds of degrees warmer than the background.
 For video see: https://youtu.be/gWT0QwSoVls. 
Credit: Hubble / NASA / ESA / A. Simon (NASA GSFC) / J. Schmidt. 
Credit: James O’Donoghue

https://youtu.be/gWT0QwSoVls

An unexpected "heat wave" of 700 degrees Celsius, extending 130,000 kilometers (10 Earth diameters) in Jupiter's atmosphere, has been discovered. James O'Donoghue, of the Japanese Aerospace Exploration Agency (JAXA), has presented the results this week at the Europlanet Science Congress (EPSC) 2022 in Granada.

Jupiter's atmosphere, famous for its characteristic multicolored vortices, is also unexpectedly hot: in fact, it is hundreds of degrees hotter than models predict. Due to its orbital distance millions of kilometers from the sun, the giant planet receives under 4% of the amount of sunlight compared to Earth, and its upper atmosphere should theoretically be a frigid -70 degrees Celsius. Instead, its cloud tops are measured everywhere at over 400 degrees Celsius.

"Last year we produced—and presented at EPSC2021—the first maps of Jupiter's upper atmosphere capable of identifying the dominant heat sources," said Dr. O'Donoghue. "Thanks to these maps, we demonstrated that Jupiter's auroras were a possible mechanism that could explain these temperatures."

Just like the Earth, Jupiter experiences auroras around its poles as an effect of the solar wind. However, while Earth's auroras are transient and only occur when solar activity is intense, auroras at Jupiter are permanent and have a variable intensity. The powerful auroras can heat the region around the poles to over 700 degrees Celsius, and global winds can redistribute the heat globally around Jupiter.

Looking more deeply through their data, Dr. O'Donoghue and his team discovered the spectacular "heat wave" just below the northern aurora, and found that it was traveling towards the equator at a speed of thousands of kilometers per hour.

The heat wave was probably triggered by a pulse of enhanced solar wind plasma impacting Jupiter's magnetic field, which boosted auroral heating and forced hot gases to expand and spill out towards the equator.

"While the auroras continuously deliver heat to the rest of the planet, these heat wave 'events' represent an additional, significant energy source," added Dr. O'Donoghue. "These findings add to our knowledge of Jupiter's upper-atmospheric weather and climate, and are a great help in trying to solve the 'energy crisis' problem that plagues research into the giant planets."


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Defense News: Israel tests missile for defending maritime assets after Hezbollah threat

 

Israel tests missile for defending maritime assets after Hezbollah threat


IAI's Gabriel 5 surface-to-surface missile can hit mobile and stationary targets, on land or at sea.