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Friday, November 22, 2024

SPACE/COSMOS

The first ‘zoomed-in’ image of a star outside our galaxy


By AFP
November 21, 2024

The image of the massive star, which is encircled by a mysterious "egg-shaped cocoon" - Copyright AFP Andrej ISAKOVIC

Scientists said Thursday they have taken the first ever close-up image of a star outside of the Milky Way, capturing a blurry shot of a dying behemoth 2,000 times bigger than the Sun.

Roughly 160,000 light years from Earth, the star WOH G64 sits in the Large Magellanic Cloud, a satellite galaxy of our home Milky Way.

It is a red supergiant, which is the largest type of star in the universe because they expand into space as they near their explosive deaths.

The image was captured by a team of researchers using a new instrument of the European Southern Observatory’s Very Large Telescope in Chile.

Keiichi Ohnaka, an astrophysicist at Chile’s Andres Bello National University, said that “for the first time, we have succeeded in taking a zoomed-in image of a dying star”.

The image shows the bright if blurry yellow star enclosed inside an oval outline.

“We discovered an egg-shaped cocoon closely surrounding the star,” Ohnaka said in a statement.

“We are excited because this may be related to the drastic ejection of material from the dying star before a supernova explosion,” added the lead author of a study published in the journal Astronomy & Astrophysics.

– ‘Witness a star’s life in real time’ –

Ohnaka’s team has been watching the star for some time.

In 2005 and 2007 they used the Very Large Telescope’s interferometer, which combined the light from two telescopes, to learn more about the star.

But capturing an image remained out of reach until a new instrument called GRAVITY — which combines the light of four telescopes — recently came online.

When they compared all their observations, the astronomers were surprised to find that the star had dimmed over the last decade.

“The star has been experiencing a significant change in the last 10 years, providing us with a rare opportunity to witness a star’s life in real time,” said study co-author Gerd Weigelt of Germany’s Max Planck Institute for Radio Astronomy.

Red supergiants — such as Betelgeuse in the Orion constellation — are “one of the most extreme of its kind, and any drastic change may bring it closer to an explosive end,” added study co-author Jacco van Loon of Keele University in the UK.

In their final stages of life, before they go supernova, red supergiants shed their outer layers of gas and dust in a process that can last thousands of years.

It could be this expelled material that is making the star appear dimmer, the scientists said.

This could also explain the strange shape of the dust cocoon that surrounds the star.

Another explanation for the egg-shaped cocoon could be that there is another star hidden somewhere inside that has not yet been discovered.

Gaza boy dreamed of ride to Moon but Israeli missile 'tore him into pieces'

"He said to me 'I hope a rocket comes and I can go to the Moon'. He didn't realise that the rocket would come and tear him up into pieces," says mother of Abdul Aziz, 7, who was killed by Israel along with his brother Hamza, 5 and sister Laila, 3.



AA

Relatives of the Palestinians who were killed in an attack on Al Mawasi area of Khan Younis mourn as dead bodies were taken from the Nasser Hospital for burial in Khan Yunis, Gaza on November 21, 2024. / Photo: AA


As Areej al-Qadi tearfully kissed the bodies of her three young children killed by Israel in an air strike in Gaza, another mourner lashed out at the United States and Arab leaders for not ending the genocide.

Palestinians in Gaza attending one funeral after another after more than a year of Israeli genocide feel abandoned and angry that their pleas for help have gone largely unanswered.

Qadi said her son Abdul Aziz, 7, killed by Israel along with his brother Hamza, 5 and sister Laila, 3, while they played outside in the southern Gaza city of Khan Younis, had wanted to be an astronaut.

"He said to me 'I hope a rocket comes and I can go to the Moon'. He didn't realise that the rocket would come and tear him up into pieces," she said.

"What right does America have, talking about democracy, justice and equality? said displaced mourner Ra'fat al-Shaer. "Also a message to the Arab world, to the heads of the Arab nations. How long will this continue?"

Arab countries have not backed their own calls for an end to the suffering of fellow-Muslims with any threats to end diplomatic agreements with Israel despite the killings of tens of thousands of civilians.


Reuters
Mourners gather next to the bodies of Palestinian children killed by Israel in a strike, during a funeral in Khan Younis in southern Gaza, on November 21, 2024.




'They were all martyred'

Israel has killed more than 44,000 people, wounded more than 104,000 and turned Gaza, one of the world's most densely populated places, into a wasteland of crushed cement and twisted metal.


Most of Gaza's population of 2.4 million people has been displaced and the enclave is at risk of famine, more than a year into Israel's genocide.


Many analysts say the reported death toll is a conservative estimate.


A letter to US President Joe Biden from a group of almost 100 American doctors who served in Gaza estimated a death toll of more than 118,000 in October 2024. And according to the UK medical journal The Lancet, the death toll could be more than 180,000.


People like Mahmoud Bin Hassan al-Thalatha, the father of the three children he said were killed along with other innocent people by Israel on a bustling street, say their only recourse is prayer.


"My children were martyred, the people walking were martyred, and the stall vendor was martyred while he was sitting down, they were all martyred. May God have mercy on them."

SOURCE: Reuters TRT World

Fly my encrypted data to the moon — or to the Canadian Space Agency’s first quantum communication satellite anyways


By Abigail Gamble
November 21, 2024
DIGITAL JOURNAL

Katanya Kuntz is a a quantum physicist and CEO and Co-founder of Qubo Consulting Corp. — Photo by Jennifer Friesen, Digital Journal

“Imagine a rat’s maze,” says Katanya Kuntz, a quantum physicist, CEO and co-founder of Qubo Consulting Corp.

She’s explaining how quantum technology works, during an interview with Digital Journal at Calgary Innovation Week.

You’ve got a rat at one end of the maze, and cheese at the other end. A classic computer is going to test out one path at a time, to figure out which path will get them to the cheese.

“But a quantum computer can try all possibilities simultaneously at once, and then find the path,” she said.

Which means, it figures out the best path much more quickly. And that’s thanks to quantum physics.

Here’s how quantum physics and technology work:

“We’ve had quantum physics for more than 100 years,” Kuntz explains. It’s the study of the microscopic building blocks of pretty much everything in the universe — like atoms. And they have different, rather wacky rules that we’re not used to experiencing in everyday life.

Some of what we understand about these building blocks or particles (their principles or rules) has been applied to what were called Quantum 1.0 technologies for a while, says Kuntz.

Essentially, everyday tools like lasers, LED lights, electronics, MRI and x-ray machines are created by applying the foundational principles of quantum physics to a technological process.

To return to the rat maze analogy…

In quantum physics, one of the “basic” rules is that a particle can exist in multiple places, simultaneously.

A particle doesn’t have a fixed location until we look at it. This happens because particles behave like waves of probability rather than fixed objects. Until we observe or measure a particle, it’s in a state of uncertainty, where all possible outcomes coexist.

So a quantum computer can explore every different maze path that’s possible, all at the same time.

Cool, huh?

It gets cooler though, because these days, scientists are working on technologies that use the more complicated quantum principle of entanglement to create “quantum networks” or a “quantum Internet” that will enable next-level data encryption. It’s Quantum 2.0.
Photo by Jennifer Friesen, Digital Journal


How Quantum 2.0 is going to protect our data so it’s unhackable

An exciting example of Quantum 2.0 technology is Canada’s first quantum communication satellite that’s set to launch in 2025 or 2026, which will help secure our data in a whole new way, says Kuntz.

In addition to her role at Qubo, Kuntz is the science team coordinator for this mission, which is called the Quantum EncrYption and Science Satellite (QEYSSat), and is owned by the Canadian Space Agency.

What’s the satellite going to do exactly?

The QEYSSat science team is going to beam a laser up from the Earth to communicate with it.

“So there’s a ground station in Waterloo, Ontario,” Kuntz explains, “It’s literally a telescope … we’re going to shoot a laser up.” And this will be a “quantum uplink” sending particles of light — called photons — up from the ground to space.

Quantum communication systems are sent to space because satellites allow secure communication over long distances, something that’s hard to achieve on Earth due to interference and the limited range of ground-based fibre systems.

These photon signals can be used to encode and encrypt everything from online banking to sensitive transaction records to private government data, and are much, much more secure than any of the other encryption technologies we use today.

“With quantum, you can actually encrypt the information securely. So it’s theoretically 100% secure,” explains Kuntz.

And this level of encryption is increasingly necessary as hacking and ransomware threats become a bigger concern, she says.

“Calgary’s Public Library system got hacked about a month ago and was held hostage, and they still don’t have internet, computers, printers, anything electronic. There’s literally a sign when you walk into the public libraries here that says, ‘no technology.’ And you can take out books, but you can’t return books because they can’t check anything.”

How and why we need quantum satellite encryption:

When you encode information on the individual photons, if a hacker is trying to access your data, it will affect the light stream, and you’ll know because you’re monitoring that channel, says Kuntz.

“This is to everyone’s benefit,” she says and is part of the Canadian government’s quantum strategy, prepping for the day when the first quantum computers come online. This could happen in the next five to 15 years, says Kuntz.

“There’s around 20 countries already that have quantum satellite missions, so we’re not the first,” she says. But the value of having our own in Canada is to establish our own secure quantum network.

“So it’s our national sovereignty to have our own quantum Internet. It protects our own public information.”

Katanya Kuntz spoke with Abigail Gamble for Digital Journal during Calgary Innovation Week. Photo by Jennifer Friesen, Digital Journal


Everyone else needs to prepare for our quantum future too

It’s not just governments who need to prepare for the quantum future, says Kuntz. Businesses and organizations can (and probably should) start looking now for quantum solutions to their problems.

And by problems, she means almost any challenge that includes a lot of complex variables.

For instance: “There are cities that are using quantum optimization algorithms, like Tokyo, to improve their transportation and waste management,” Kuntz says.

Some of the complex challenges quantum can help navigate include:

“If there’s events in the city, how is that going to affect the waste management? If there’s [extra] traffic flow, if there’s [unexpected] weather events, if there’s suddenly a snow dump, that’s going to really affect your routes, and maybe your garbage trucks won’t get to all their stops.”

Quantum tools can help provide solutions in situations like these, that are faster (like our rat to cheese scenario) and ensure the data involved is more secure (with next-level encryptions).

The speed and security of quantum can be used to improve the efficiency of every sector from finance, to aviation to agriculture and manufacturing, Kuntz says. “It’s not just one industry. This is touching every single industry in the world.”

She also notes that companies and organizations alike need to be prepared for when quantum computers come online, because they’ll be able to hack anything that isn’t quantum encrypted.

“Elect somebody in your company to be your technology evangelist, and have a small budget for their training.” Once they understand quantum a little better, Kuntz recommends sending them off to find people and tools who can help do a “cryptographic inventory” of your assets.

“Engage with a quantum company and start exploring,” she says.



Written By Abigail Gamble
Abigail is a writer, editor, journalist and content strategist based in Toronto and El Salvador.

Tuesday, November 19, 2024

SPACE / COSMOS

Egg-shaped galaxies may be aligned to the black holes at their hearts, astronomers find


The Conversation
November 18, 2024

The active galaxy Centaurus A, with jets emanating from the central black hole. ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimetre); NASA/CXC/CfA/R.Kraft et al. (X-ray), CC BY

Black holes don’t have many identifying features. They come in one color (black) and one shape (spherical).

The main difference between black holes is mass: some weigh about as much as a star like our Sun, while others weigh around a million times more. Stellar-mass black holes can be found anywhere in a galaxy, but the really big ones (known as supermassive black holes) are found in the cores of galaxies.

These supermassive behemoths are still quite tiny when seen in cosmic perspective, typically containing only around 1% of their host galaxy’s mass and extending only to a millionth of its width

However, as we have just discovered, there is a surprising link between what goes on near the black hole and the shape of the entire galaxy that surrounds it. Our results are published in Nature Astronomy.

When black holes light up

Supermassive black holes are fairly rare. Our Milky Way galaxy has one at its centre (named Sagittarius A*), and many other galaxies also seem to host a single supermassive black hole at their core.


Under the right circumstances, dust and gas falling into these galactic cores can form a disk of hot material around the black hole. This “accretion disk” in turn generates a super-heated jet of charged particles that are ejected from the black hole at mind-boggling velocities, close to the speed of light.

When a supermassive black hole lights up like this, we call it a quasar.

How to watch a quasar

To get a good look at quasar jets, astronomers often use radio telescopes. In fact, we sometimes combine observations from multiple radio telescopes located in different parts of the world.

Using a technique called very long baseline interferometry, we can in effect make a single telescope the size of the entire Earth. This massive eye is much better at resolving fine detail than any individual telescope.

As a result, we can not only see objects and structures much smaller than we can with the naked eye, we can do better than the James Webb Space Telescope.



Black holes are millions of times smaller than galaxies, yet make jets that are pointed in the same direction as the entire galaxy. Optical image: NASA, ESA, R.M. Crockett (University of Oxford, U.K.), S. Kaviraj (Imperial College London and University of Oxford, U.K.), J. Silk (University of Oxford), M. Mutchler (Space Telescope Science Institute, Baltimore, USA), R. O'Connell (University of Virginia, Charlottesville, USA), and the WFC3 Scientific Oversight Committee. Top right: MOJAVE Collaboration, NRAO/NSF. Bottom right: Event Horizon Telescope / ESO (same as before) CC BY-SA

This is the technique that was used to make the first “black hole image” in 2019, showing the halo of light generated around the supermassive black hole hosted by the galaxy M87.


Quasar jets that can be detected using very long baseline interferometry can be millions of light years long and are almost always found in elliptical galaxies. Using very long baseline interferometry, we can observe them all the way down to a few light years or so from their black hole of origin.

The direction of the jet near its source tells us about the orientation of the accretion disk, and so potentially the properties of the black hole itself.


Connection to the host galaxy


What about the host galaxies? A galaxy is a three-dimensional object, formed of hundreds of billions of stars.

But it appears to us (observed in optical or infrared) in projection, either as an ellipse or a spiral. We can measure the shape of these galaxies, tracing the profile of starlight, and measure the long axis and short axis of the two-dimensional shape.

In our paper, we compared the direction of quasar jets with the direction of this shorter axis of the galaxy ellipse, and found that they tend to be pointing in the same direction. This alignment is more statistically significant than you would expect if they were both randomly oriented.

This is surprising, as the black hole is so small (the jets we measure are only a few light years in length) compared to the host galaxy (which can be hundreds of thousands or even millions of light years across).

It is surprising that such a relatively small object can affect, or be affected by, the environment on such large scales. We might expect to see a correlation between the jet and the local environment, but not with the whole galaxy.
How galaxies form

Does this have something to say about the way galaxies form?


Spiral galaxies are perhaps the most famous kind of galaxy, but sometimes they collide with other spirals and form elliptical galaxies. We see these three-dimensional egg-shaped blobs as two-dimensional ellipses on the sky.

The merger process triggers quasar activity in ways we don’t fully understand. As a result, almost all quasar jets that can be detected using very long baseline interferometry are hosted in elliptical galaxies.

The exact interpretation of our results remains mysterious, but is important in the context of the recent James Webb Space Telescope discovery of highly massive quasars (with massive black holes), which have formed much earlier in the universe than expected. Clearly, our understanding of how galaxies form and how black holes influence that needs to be updated.


David Parkinson, Research Scientist in Astrophysics, The University of Queensland and Jeffrey Hodgson, Assistant Professor in Astrophysics, Sejong University

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


AnalySwift receives NASA STTR contract to transform spacecraft infrastructure for secondary uses during long-duration missions



Company and Purdue will develop composite heater layer and better engineering tools for composites



Purdue University

Kawai Kwok, Purdue University and AnalySwift, NASA STTR contract, reassembly 

image: 

Kawai Kwok, an associate professor in Purdue University’s School of Aeronautics and Astronautics, will be the primary investigator on a project with commercial software provider AnalySwift LLC. NASA has awarded AnalySwift a $156,424 Phase I Small Business Technology Transfer contract for the research.

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Credit: (Purdue University photo/Alan Cesar)




WEST LAFAYETTE, Ind. — AnalySwift LLC, a Purdue University-affiliated company, has received a Phase I STTR (Small Business Technology Transfer) contract from NASA worth $156,424.

Allan Wood, AnalySwift president and CEO, said the contract will fund two advancements: processes and hardware to disassemble spacecraft components and reassemble them for a secondary use, and software for multiphysics simulation and analysis of the involved thermoplastics.

Kawai Kwok, associate professor in Purdue’s School of Aeronautics and Astronautics, is the principal investigator.

Wood said long-duration crewed missions to the moon, Mars and beyond require infrastructure, such as trusses, to be constructed sustainably on these surfaces. But there are immense logistical challenges in transporting heavy and large payloads to space.

“The AnalySwift project proposes a novel method of disassembling and reassembling thermoplastic composite joints in space,” he said. “Our proposed method enables reconfiguration of truss structures in space, transitioning away from the current one-time use model to a scalable and sustainable approach.”

Kwok said spacecraft components could be quickly and easily repurposed into vastly different geometries.

“For example, a lunar lander support truss could become a vertical solar array support truss,” he said. “There are other applications, depending on mission needs using the same set of structural elements and innovative multiphysics modeling.”

Contract deliverables

Kwok said AnalySwift will develop a composite heater layer for the trusses and other infrastructure; it will be embedded with nanostructured carbon fillers. The layer will be made from the same thermoplastic matrix as the adhered composite parts. The layer will bring the matrix to the processing temperature for interface debonding by mechanical forces.

“Lightweight conductive nanocarbon thin films will be encapsulated inside semicrystalline thermoplastics such as PEEK (polyether ether ketone),” he said. “The disassembled struts and joints will be reassembled to the repurposed configuration via resistance welding using the same or additional heaters. The proposed in situ heating and reassembly method enables spacecraft components to be reutilized, which greatly reduces the logistical footprint to deliver technologies to space.”

Liang Zhang, senior research scientist at AnalySwift, said the company also will develop better engineering tools for composites, enabling reliable multiphysics simulation of their technique to repurpose lightweight structures made from thermoplastics.

“Theoretical and computational developments will include a new software tool or module, Thermoplastic Composites Multiphysics,” he said. “This multiphysics modeling framework will simulate the debonding and bonding processes of thermoplastic composite joint-strut interfaces using embedded carbon nanoheaters.”

Kwok said the framework has broader applications for thermoplastics.

“Advancements include developing multiphysics models and data for electrical heating and welding, including establishing relations between bonding strength and the process conditions of temperature, pressure and time,” he said. “More specifically, the disassembly and assembly processes of a nanocomposite is simulated using a third-party commercial finite element code with user subroutines defining the governing behavior of the material system.”

Zhang said AnalySwift’s multiphysics simulation tool will determine force, pressure and temperature histories during assembly and disassembly processes.

“More specifically, it will incrementally solve the constitutive relations as an initial value problem, extract temperature distributions at specific time points, and calculate the time and power required for completion,” he said.

Non-space applications

Wood said the processes and hardware advancements for disassembly and reassembly are more applicable to space applications, but the software has other potential uses.

“It can be particularly useful where simulation tools can improve utilization possibilities for high-performance thermoplastics,” he said. “Additional applications can be likely for aerospace, defense, automotive, marine, energy, electronics, sporting goods and medical devices. Applications also extend beyond simulation and into repair for thermoplastics.”

About AnalySwift

AnalySwift LLC is a provider of composite simulation software, which enables an unprecedented combination of efficiency and accuracy, including multiphysics structural and micromechanics modeling. Drawing on cutting-edge university technology, AnalySwift’s powerful solutions save orders of magnitude in computing time without a loss of accuracy so users can consider more design options and arrive at the best solution more quickly. The technologies deliver the accuracy of detailed 3D finite element analysis at the efficiency of simple engineering models. SwiftComp was developed at Purdue University and licensed from the Purdue Research Foundation. Contact AnalySwift at info@analyswift.com.

About Purdue Innovates Office of Technology Commercialization

The Purdue Innovates Office of Technology Commercialization operates one of the most comprehensive technology transfer programs among leading research universities in the U.S. Services provided by this office support the economic development initiatives of Purdue University and benefit the university’s academic activities through commercializing, licensing and protecting Purdue intellectual property. In fiscal year 2024, the office reported 145 deals finalized with 224 technologies signed, 466 invention disclosures received, and 290 U.S. and international patents received. The office is managed by the Purdue Research Foundation, a private, nonprofit foundation created to advance the mission of Purdue University. Contact otcip@prf.org for more information.

About Purdue University

Purdue University is a public research institution demonstrating excellence at scale. Ranked among top 10 public universities and with two colleges in the top four in the United States, Purdue discovers and disseminates knowledge with a quality and at a scale second to none. More than 105,000 students study at Purdue across modalities and locations, including nearly 50,000 in person on the West Lafayette campus. Committed to affordability and accessibility, Purdue’s main campus has frozen tuition 13 years in a row. See how Purdue never stops in the persistent pursuit of the next giant leap — including its first comprehensive urban campus in Indianapolis, the Mitch Daniels School of Business, Purdue Computes and the One Health initiative — at https://www.purdue.edu/president/strategic-initiatives.

Media contact: Steve Martin, sgmartin@prf.org


New idea may crack enigma of the Crab Nebula’s ‘zebra’ pattern



University of Kansas
Zebra-pattern pulsar 

image: 

Medvedev modeled wave diffraction off a circular reflecting region with radially varying index of refraction outside of it to better understand the Crab Nebula’s zebra pattern.

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Credit: Mikhail Medvedev




LAWRENCE — A theoretical astrophysicist from the University of Kansas may have solved a nearly two-decade-old mystery over the origins of an unusual "zebra" pattern seen in high-frequency radio pulses from the Crab Nebula.

His findings have just been published in Physical Review Letters (PRL), among the most prestigious physics journals.

The Crab Nebula features a neutron star at its center that has formed into a 12-mile-wide pulsar pinwheeling electromagnetic radiation across the cosmos.

“The emission, which resembles a lighthouse beam, repeatedly sweeps past Earth as the star rotates,” said lead author Mikhail Medvedev, professor of physics & astronomy at KU. “We observe this as a pulsed emission, usually with one or two pulses per rotation. The specific pulsar I’m discussing is known as the Crab Pulsar, located in the center of the Crab Nebula 6,000 light years away from us.”

The Crab Nebula is the remnant of a supernova that appeared in 1054.

“Historical records, including Chinese accounts, describe an unusually bright star appearing in the sky,” said the KU researcher.

But unlike any other known pulsar, Medvedev said the Crab Pulsar features a zebra pattern — unusual band spacing in the electromagnetic spectrum proportional to band frequencies, and other weird features like high polarization and stability.

“It’s very bright, across practically all wave bands,” he said. “This is the only object we know of that produces the zebra pattern, and it only appears in a single emission component from the Crab Pulsar. The main pulse is a broadband pulse, typical of most pulsars, with other broadband components common to neutron stars. However, the high-frequency interpulse is unique, ranging between 5 and 30 gigahertz — frequencies similar to those in a microwave oven.”

Since this pattern was discovered in a 2007 paper, the KU researcher said the pattern had proved “baffling” for investigators.

“Researchers proposed various emission mechanisms, but none have convincingly explained the observed patterns,” he said.

Using data from the Crab Pulsar, Medvedev established a method using wave optics to gauge the density of the pulsar’s plasma – the “gas” of charged particles (electrons and positrons) — using a fringe pattern found in the electromagnetic pulses.

“If you have a screen and an electromagnetic wave passes by, the wave doesn’t propagate straight through,” Medvedev said. “In geometrical optics, shadows cast by obstacles would extend indefinitely — if you’re in the shadow, there’s no light; outside of it, you see light. But wave optics introduces a different behavior — waves bend around obstacles and interfere with each other, creating a sequence of bright and dim fringes due to constructive and destructive interference.”

This well-known fringe pattern phenomenon is caused by consistent constructive interference but has different characteristics when radio waves propagate around a neutron star.

“A typical diffraction pattern would produce evenly spaced fringes if we just had a neutron star as a shield,” the KU researcher said. “But here, the neutron star’s magnetic field generates charged particles constituting a dense plasma, which varies with distance from the star. As a radio wave propagates through the plasma, it passes through dilute areas but is reflected by dense plasma. This reflection varies by frequency: Low frequencies reflect at large radii, casting a bigger shadow, while high frequencies create smaller shadows, resulting in different fringe spacing.”

In this way, Medvedev determined the Crab Pulsar’s plasma matter causes diffraction in the electromagnetic pulses responsible for the neutron star’s singular zebra pattern.

“This model is the first one capable of measuring those parameters,” Medvedev said. “By analyzing the fringes, we can deduce the density and distribution of plasma in the magnetosphere. It's incredible because these observations allow us to convert fringe measurements into a density distribution of the plasma, essentially creating an image or performing tomography of the neutron star's magnetosphere.”

Next, Medvedev said his theory can be tested with collection of more data from the Crab Pulsar and fine-tuned by factoring in its powerful and strange gravitational and polarization effects. The new understanding of how a plasma matter alters a pulsar’s signal will change how astrophysicists understand other pulsars.

“The Crab Pulsar is somewhat unique — it’s relatively young by astronomical standards, only about a thousand years old, and highly energetic,” he said. “But it’s not alone; we know of hundreds of pulsars, with over a dozen that are also young. Known binary pulsars, which were used to test Einstein’s general relativity theory, can also be explored with the proposed method. This research can indeed broaden our understanding and observation techniques for pulsars, particularly young, energetic ones.”