Sunday, October 29, 2023

Sci-fi inspired tractor beams are real, and could solve a major space junk problem

By Harry Baker 
Live Science

Researchers are developing a real-life tractor beam, with the goal of pulling defunct satellites out of geostationary orbit to alleviate the space junk problem.


An artist's illustration shows how an electrostatic tractor beam could be used to pull defunct satellites out of geostationary orbit around Earth. In reality, the beam would be invisible. (Image credit: Tobias Roetsch - gtgraphics.de)

In science fiction films, nothing raises tension quite like the good guys' spaceship getting caught in an invisible tractor beam that allows the baddies to slowly reel them in. But what was once only a sci-fi staple could soon become a reality.

Scientists are developing a real-life tractor beam, dubbed an electrostatic tractor. This tractor beam wouldn't suck in helpless starship pilots, however. Instead, it would use electrostatic attraction to nudge hazardous space junk safely out of Earth orbit.

The stakes are high: With the commercial space industry booming, the number of satellites in Earth's orbit is forecast to rise sharply. This bonanza of new satellites will eventually wear out and turn the space around Earth into a giant junkyard of debris that could smash into working spacecraft, plummet to Earth, pollute our atmosphere with metals and obscure our view of the cosmos. And, if left unchecked, the growing space junk problem could hobble the booming space exploration industry, experts warn.

The science is pretty much there, but the funding is not.


The electrostatic tractor beam could potentially alleviate that problem by safely moving dead satellites far out of Earth orbit, where they would drift harmlessly for eternity.

While the tractor beam wouldn't completely solve the space junk problem, the concept has several advantages over other proposed space debris removal methods, which could make it a valuable tool for tackling the issue, experts told Live Science.

Related: 11 sci-fi concepts that are possible (in theory)

A prototype could cost millions, and an operational, full-scale version even more. But if the financial hurdles can be overcome, the tractor beam could be operational within a decade, its builders say.

"The science is pretty much there, but the funding is not," project researcher Kaylee Champion, a doctoral student in the Department of Aerospace Engineering Sciences at the University of Colorado Boulder (CU Boulder), told Live Science.

Avoiding Disaster


Tractor beams are a staple of sci-fi films and TV shows, such as Star Trek.
 
(Image credit: Star Trek)

The tractor beams depicted in "Star Wars" and "Star Trek" suck up spacecraft via artificial gravity or an ambiguous "energy field." Such technology is likely beyond anything humans will ever achieve. But the concept inspired Hanspeter Schaub, an aerospace engineering professor at CU Boulder, to conceptualize a more realistic version.

Schaub first got the idea after the first major satellite collision in 2009, when an active communications satellite, Iridium 33, smashed into a defunct Russian military spacecraft, Kosmos 2251, scattering more than 1,800 pieces of debris into Earth's orbit.

Related: How many satellites orbit Earth?

In the wake of this disaster, Schaub wanted to be able to prevent this from happening again. To do this, he realized you could pull spacecraft out of harm's way by using the attraction between positively and negatively charged objects to make them "stick" together.

Over the next decade, Schaub and colleagues refined the concept. Now, they hope it can someday be used to move dead satellites out of geostationary orbit (GEO) — an orbit around Earth's equator where an object's speed matches the planet's rotation, making it seem like the object is fixed in place above a certain point on Earth. This would then free up space for other objects in GEO, which is considered "prime real estate" for satellites, Schaub said.

How does it work?


The researchers have been testing the electron gun on pieces of metal in the lab.
 (Image credit: Nico Goda/CU Boulder)

The electrostatic tractor would use a servicer spacecraft equipped with an electron gun that would fire negatively charged electrons at a dead target satellite, Champion told Live Science. The electrons would give the target a negative charge while leaving the servicer with a positive charge. The electrostatic attraction between the two would keep them locked together despite being separated by 65 to 100 feet (20 to 30 meters) of empty space, she said.

Once the servicer and target are "stuck together," the servicer would be able to pull the target out of orbit without touching it. Ideally, the defunct satellite would be pulled into a "graveyard orbit" more distant from Earth, where it could safely drift forever, Champion said.

Related: 15 of the weirdest things we have launched into space

The electrostatic attraction between the two spacecraft would be extremely weak, due to limitations in electron gun technology and the distance by which the two would need to be separated to prevent collisions, project researcher Julian Hammerl, a doctoral student at CU Boulder, told Live Science. So the servicer would have to move very slowly, and it could take more than a month to fully move a single satellite out of GEO, he added.

That's a far cry from movie tractor beams, which are inescapable and rapidly reel in their prey. This is the "main difference between sci-fi and reality," Hammerl said.

Advantages and limitations



The amount of space junk surrounding Earth has greatly increased in recent years. Here is a comparison of space junk in 1965 (left) and 2010 (right). (Image credit: NASA)

The electrostatic tractor would have one big advantage over other proposed space junk removal methods, such as harpoons, giant nets and physical docking systems: It would be completely touchless.

"You have these large, dead spacecraft about the size of a school bus rotating really fast," Hammerl said. "If you shoot a harpoon, use a big net or try to dock with them, then the physical contact can damage the spacecraft and then you are only making the [space junk] problem worse."

Scientists have proposed other touchless methods, such as using powerful magnets, but enormous magnets are both expensive to produce and would likely interfere with a servicer's controls, Champion said.

Related: How do tiny pieces of space junk cause incredible damage?

The main limitation of the electrostatic tractor is how slowly it would work. More than 550 satellites currently orbit Earth in GEO, but that number is expected to rise sharply in the coming decades.

If satellites were moved one at a time, then a single electrostatic tractor wouldn't keep pace with the number of satellites winking out of operation. Another limitation of the electrostatic tractor is that it would work too slowly to be practical for clearing smaller pieces of space junk, so it wouldn't be able to keep GEO completely free of debris.

Cost is the other big obstacle. The team has not yet done a full cost analysis for the electrostatic tractor, Schaub said, but it would likely cost tens of millions of dollars. However, once the servicer were in space, it would be relatively cost-effective to operate it, he added.

Next steps


Researcher Julian Hammerl photographed next to the ECLIPS machine at CU Boulder. (Image credit: Nico Goda/CU Boulder)

The researchers are currently working on a series of experiments in their Electrostatic Charging Laboratory for Interactions between Plasma and Spacecraft (ECLIPS) machine at CU Boulder. The bathtub-sized, metallic vacuum chamber, which is equipped with an electron gun, allows the team to "do unique experiments that almost no one else can currently do" in order to simulate the effects of an electrostatic tractor on a smaller scale, Hammerl said.

Once the team is ready, the final and most challenging hurdle will be to secure funding for the first mission, which is a process they have not yet started.

Most of the mission cost would come from building and launching the servicer. However, the researchers would ideally like to launch two satellites for the first tests, a servicer and a target that they can maneuver, which would give them more control over their experiments but also double the cost.

Related: 10 stunning shots of Earth from space in 2022

If they can somehow wrangle that funding, a prototype tractor beam could be operational in around 10 years, the team previously estimated.

Is it viable?


Space junk is becoming a major problem for the space exploration industry. 
(Image credit: CU Boulder)

While tractor beams may sound like a pipe dream, experts are optimistic about the technology.

"Their technology is still in the infancy stage," John Crassidis, an aerospace scientist at the University at Buffalo in New York, who is not involved in the research, told Live Science in an email. "But I am fairly confident it will work."

If you shoot a harpoon, use a big net or try to dock with them, then the physical contact can damage the spacecraft and then you are only making the [space junk] problem worse.

Removing space junk without touching it would also be much safer than any current alternative method, Crassidis added.

The electrostatic tractor "should be able to produce the forces necessary to move a defunct satellite" and "certainly has a high potential to work in practice," Carolin Frueh, an associate professor of aeronautics and astronautics at Purdue University in Indiana, told Live Science in an email. "But there are still several engineering challenges to be solved along the way to make it real-world-ready."

Scientists should continue to research other possible solutions, Crassidis said. Even if the CU Boulder team doesn't create a "final product" to remove nonfunctional satellites, their research will provide a stepping stone for other scientists, he added.

If they are successful, it wouldn't be the first time scientists turned fiction into fact.

"What is today's science fiction could be tomorrow's reality," Crassidis said.

Starlink satellites ‘leaking’ signals that interfere with radio telescopes

Satellites over the Earth's surface, shown in green. 
Credit: LeoLabs, https://leolabs.space

October 29, 2023
The Conversation

Steven TingayCurtin University

When I was a child in the 1970s, seeing a satellite pass overhead in the night sky was a rare event. Now it is commonplace: sit outside for a few minutes after dark, and you can’t miss them.

Thousands of satellites have been launched into Earth orbit over the past decade or so, with tens of thousands more planned in coming years. Many of these will be in “mega-constellations” such as Starlink, which aim to cover the entire globe.

These bright, shiny satellites are putting at risk our connection to the cosmos, which has been important to humans for countless millennia and has already been greatly diminished by the growth of cities and artificial lighting. They are also posing a problem for astronomers – and hence for our understanding of the universe.

In new research accepted for publication in Astronomy and Astrophysics Letters, we discovered Starlink satellites are also “leaking” radio signals that interfere with radio astronomy. Even in a “radio quiet zone” in outback Western Australia, we found the satellite emissions were far brighter than any natural source in the sky.

An animation showing the increase in the number of satellites in Earth orbit, over the course of the space age, so far.


A problem for our understanding of the universe


Our team at Curtin University used radio telescopes in Western Australia to examine the radio signals coming from satellites.

We found expected radio transmissions at designated and licensed radio frequencies, used for communication with Earth.

However, we also found signals at unexpected and unintended frequencies.

We found these signals coming from many Starlink satellites. It appears the signals may originate from electronics on board the spacecraft.

Why is this an issue? Radio telescopes are incredibly sensitive, to pick up faint signals from countless light-years away.

Even an extremely weak radio transmitter hundreds or thousands of kilometres away from the telescope appears as bright as the most powerful cosmic radio sources we see in the sky. So these signals represent a serious source of interference.

And specifically, the signals are an issue at the location where we tested them: the site in WA where construction has already begun for part of the biggest radio observatory ever conceived, the Square Kilometre Array (SKA). This project involves 16 countries, has been in progress for 30 years, and will cost billions of dollars over the next decade.

Huge effort and expense has been invested in locating the SKA and other astronomy facilities a long way away from humans. But satellites present a new threat in space, which can’t be dodged.

What can we do about this?

It’s important to note satellite operators do not appear to be breaking any rules. The regulations around use of the radio spectrum are governed by the International Telecommunications Union, and they are complex. At this point there is no evidence Starlink operators are doing anything wrong.

The radio spectrum is crucial for big business and modern life. Think mobile phones, wifi, GPS and aircraft navigation, and communications between Earth and space.

However, the undoubted benefits of space-based communications – such as for globally accessible fast internet connections – are coming into conflict with our ability to see and explore the universe. (There is some irony here, as wifi in part owes its origins to radio astronomy.)

Regulations evolve slowly, while the technologies driving satellite constellations like Starlink are developing at lightning speed. So regulations are not likely to protect astronomy in the near term.

But in the course of our research, we have had a very positive engagement with SpaceX engineers who work on the Starlink satellites. It is likely that the goodwill of satellite operators, and their willingness to mitigate the generation of these signals, is the key to solving the issue.

In response to earlier criticisms, SpaceX has made improvements to the amount of sunlight Starlink satellites reflect, making them one-twelfth as bright in visible light as they used to be.

We estimate emissions in radio wavelengths will need to be reduced by a factor of a thousand or more to avoid significant interference with radio astronomy. We hope these improvements can be made, in order to preserve humanity’s future view of the universe, the fundamental discoveries we will make, and the future society-changing technologies (like wifi) that will emerge from those discoveries.

Steven Tingay, John Curtin Distinguished Professor (Radio Astronomy), Curtin University

This article is republished from The Conversation under a Creative Commons license. Read the original article.

James Webb telescope spots ultra-rare cosmic explosion that could reveal the origin of the universe’s heaviest elements

A kilonova explosion from a neutron-star merger and the original host galaxy of those dead stars, as seen by JWST.
A kilonova explosion from a neutron-star merger and the original host galaxy of those dead stars, as seen by JWST. (Image credit: NASA, ESA, CSA, STScI, A. Levan (IMAPP, Warw), A. Pagan (STScI))

Using an incredibly bright gamma-ray as a guide, the James Webb Space Telescope (JWST) has detected the heavy element tellurium around the site of a stellar-corpse collision. The discovery brings scientists a step closer to understanding where the universe's heaviest elements come from.

While scientists know that elements lighter than iron are forged in the hearts of massive stars, even the most massive stellar bodies aren't capable of generating hot and dense enough conditions at their cores to forge heavier elements such as gold, platinum or tellurium.

Neutron stars are created when stars can no longer perform nuclear fusion and collapse under their own gravity, creating matter so dense that a teaspoon of it would weigh 10 million tons (9 million metric tons). When neutron stars collide, this incredibly dense matter is sprayed into their immediate environment. This matter is rich in free neutrons, which can be captured by atoms, creating unstable atoms that eventually decay into elements with high numbers of protons and neutrons — the heavier elements in the periodic table. The decay of these elements also releases an explosion of electromagnetic radiation that astronomers see as a bright blast known as a kilonova.

"In the hunt for the heaviest elements, kilonovas are the main suspect," Darach Watson, an associate professor at the Niels Bohr Institute's Cosmic Dawn Center in Denmark, told Live Science.

Related: 'Remarkable' explosions from colliding, dead stars could reveal the true expansion rate of the universe

However, the "smoking gun" evidence of this process has yet to be seen, partially because kilonovas are extremely rare. This discovery made with JWST brings researchers a tantalizing step closer to that evidence.

"In the one previous good set of data we have for a kilonova, we have discovered strontium and evidence for yttrium," Watson said. "But these are relatively light, with around 85 to 90 protons and neutrons."

Watson, who co-authored a paper detailing the findings published Oct. 25 in the journal Nature, explained that tellurium,  with 128 protons and neutrons, gets scientists much closer to really heavy elements and pinpointing neutron-star mergers as the sites of heavy-element production.

"We would like to find elements closer to the heaviest elements, such as uranium, which has about 235 protons and neutrons," Watson said. "There is a very long way from around 90 to around 240.


Kilonova hunting


The kilonova and its likely host galaxy labeled in the new JWST observations. (Image credit: NASA, ESA, CSA, STScI, A. Levan (IMAPP, Warw), A. Pagan (STScI))

To take this important step and to make its first detection of a single element around a neutron star merger, JWST used the gamma-ray burst GRB 230307A, which was first detected by the Fermi Gamma-ray Space Telescope in March 2023. The emission was around 1,000 times brighter than the gamma-ray bursts that Fermi usually spots, lasted 200 seconds and seemed to be coming from a neutron-star collision, which was unusual because these events usually create much shorter-duration gamma-ray bursts.

Using an array of ground- and space-based telescopes, scientists detected the rough source of GRB 230307A in the sky. Observing the source in gamma-ray, X-ray, optical, infrared, and radio wave frequencies of light showed that the source was  characteristic of a kilonova explosion.

During the later period of the explosion, as the kilonova light moved into the infrared, it became unobservable from Earth but an excellent target for JWST's  highly-sensitive infrared detectors.

In addition to spotting the telltale emissions of tellurium, JWST pinpointed a spiral galaxy 120,000 light-years from the kilonova where the dead stars likely originated. The team suspects the neutron stars involved in the merger that created the kilonova were ejected from this galaxy as a binary pair and traveled a distance equal to the width of the Milky Way together, before finally spiraling together and merging. 

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Watson believes the detection of this heavy element around the neutron star merger wouldn't have been possible without JWST, the most powerful telescope humanity has ever put into space.

"Nothing else even gets close to the JWST!" he said. "The sensitivity of JWST is just amazing, and at these wavelengths, it is completely unparalleled. I mean, we knew in principle what it could do, but I think everybody was unprepared for this."

 

Historic space photo: A monstrous 'Halloween storm' explodes from the sun

The sun viewed through a green filter with a massive flash of light erupting from its surface
NASA's Solar and Heliospheric Observatory (SOHO) spacecraft captured this image of an enormous X-class solar flare as it erupted from the sun on October 28, 2003. The monstrous solar storm is one of the largest in recorded history. (Image credit: NASA/SOHO)

What it is: solar flare exploding on the sun's surface

When it was taken: Oct. 28, 2003

Where it is: The sun, around 93 million miles (150 million kilometers) from Earth

Why it's so special: During the spooky season of 2003, the sun spit out an unusually powerful series of solar flares, known as the "Halloween solar storms." The most powerful of these flares (pictured above) exploded from the sun's surface on Oct. 28 and launched a high-speed burst of electrically charged particles, called a coronal mass ejection (CME), that smashed into Earth the next day.

The monstrous eruption was an X-class flare — the most powerful class the sun is capable of producing — with an estimated magnitude of 45, which remains the most powerful in modern databases, according to NASA. (The flare was too powerful to be accurately detected by scientific equipment at the time, so its magnitude was calculated afterward.)

The plume of plasma erupted from a sunspot wider than 13 Earths, according to the National Oceanic and Atmospheric Administration (NOAA). The resulting CME temporarily knocked out half of the satellites orbiting Earth at the time and forced astronauts on the International Space Station to take cover from the radiation.

On Earth, the resulting geomagnetic storm raged for three days, creating temporary radio blackouts across large parts of the globe and even causing permanent damage to electrical infrastructure in some places. Auroras were also clearly visible as far south as California, Texas and Florida, according to NOAA.

Experts say the superpowered storm could have been the largest since the Carrington Event in 1859, which, excluding inexplicably powerful ancient Miyake events, is the most powerful known solar storm in human history.


If a solar storm as large as the 2003 behemoth hit Earth today, the repercussions could be much more terrifying because there are thousands more satellites in orbit and we are much more reliant on them than we were back then.

All indications suggest that the sun's upcoming period of peak activity, the solar maximum, will be the strongest in decades.