Comprehensive Review of ‘A Brief History of the Universe (and Our Place in It)’: Discover the Cosmic Big Picture

Illustration of the tidal disruption event (TDE), showcasing a star being torn apart by a supermassive black hole's gravity, forming a fan-shaped debris pattern around it.

Space Exploration: Insights into Black Holes

Mark Garlick/Science Photo Library

A Brief History of the Universe
By Sarah Alam Malik, Published by Simon & Schuster (UK, February 12) and William Morrow (USA, May 5)

Published in 1988, Stephen Hawking’s A Brief History of Time revolutionized the field of cosmology and became a bestseller. As a curious teenager, I attempted to read it, but I never finished. Now, nearly four decades later, particle physicist Sara Alam Malik offers her own perspective on cosmology with A Brief History of the Universe (and Our Place in It).

While Hawking’s work began with Aristotle’s heliocentric theory from 340 BC, Malik traces our understanding back to Babylonian astronomical observations recorded in cuneiform around the 7th century BC. The journey then progresses through the contributions of Aristotle and Ptolemy, reaching the flourishing of astronomical sciences in the Islamic Golden Age during the 6th century AD.

This concise history propels readers through significant milestones by page 47, covering Galileo’s discovery of Jupiter’s moons, Newton’s apple, and Einstein’s general relativity, ultimately exploring the mysteries of galaxies and black holes, leading to the concept of the universe’s thermal death. Malik adeptly connects cosmic-scale truths with the intricate world of quantum mechanics, stating, “The building blocks of the universe turned out to be as amazing as the structure of the universe they created.”

Unlike Hawking’s technical depth, Malik adopts a broader perspective, bringing to life characters such as Dmitri Mendeleev, who created the periodic table, and Fritz Zwicky, the pioneer of dark matter. Her narrative highlights a diverse cast, including medieval Islamic astronomers and groundbreaking women like Vera Rubin, who overcame gender barriers to reshape our understanding of galaxies.

Written with a more contemporary tone, Malik discusses topics Hawking could not forecast in 1988, such as the Large Hadron Collider, revealing the emotional impact of scientific breakthroughs like the Higgs boson discovery through compelling anecdotes.

This book is not only a “brief history of the universe” but emphasizes “and our place in it.” It narrates humanity’s discovery of the cosmos, underscoring our journey enabled by the giants before us. It evokes awe and humility, reminding us, “It remains a wonder of human existence that we can understand worlds so far removed from our own.” Each era has crafted its narrative of the universe, often believing its own version.

At its best, Malik’s work dives deeply into cosmic and quantum mysteries, aligning with her expertise in dark matter. While chapters on the origin of life, its future, and machine intelligence may feel less thorough, her warm, clear prose covers an impressive breadth within just 223 pages. As an 18-year-old, I might have navigated this complex narrative and been inspired to follow in Hawking’s footsteps.

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Source: www.newscientist.com

Unveiling the Ultimate Dark Matter Map: Discovering Unprecedented Cosmic Structures

dark matter distribution

Dark Matter Distribution: Hubble vs. James Webb

Credit: Dr. Gavin Leroy/Professor Richard Massey/COSMOS-Webb Collaboration

In a groundbreaking study, scientists leveraged subtle distortions in the shapes of over 250,000 galaxies to construct the most detailed dark matter map to date, paving the way for insights into some of the universe’s greatest enigmas.

Dark matter, elusive by nature, does not emit any detectable light. Its existence can only be inferred through its gravitational interactions with normal matter. Researchers, including Jacqueline McCreary from Northeastern University, utilized the James Webb Space Telescope (JWST) to map a region of the sky larger than the full moon.

“This high-resolution image depicts the scaffold of a small segment of the universe,” noted McCreary. The new map boasts double the resolution of previous ones created by the Hubble Space Telescope, encompassing structures much farther away.

The researchers studied approximately 250,000 galaxies, noting that their shapes, while interesting, serve primarily as a backdrop for understanding gravitational distortions. As Liliya Williams from the University of Minnesota explained, “These galaxies merely act as the universe’s wallpaper.” The critical component is the way dark matter’s gravitational pull warps the light from these distant galaxies—a phenomenon known as gravitational lensing. The more distorted the shape of these galaxies is from a perfect circle, the greater the amount of dark matter situated between us and them.

By analyzing these optical distortions, the team was able to derive a map illustrating massive galaxy clusters and the cosmic web filaments linking them. Many of these newly identified structures deviate from prior observations of luminous matter, suggesting they are predominantly composed of dark matter. “Gravitational lensing is one of the few and most effective techniques for detecting these structures across vast regions,” Williams stated.

This research is significant, considering that dark matter constitutes about 85% of the universe’s total matter, crucial for the formation and evolution of galaxies and clusters. Understanding its distribution could shed light on its behavior and composition, according to Williams.

“This achievement is not just observational but also paves the way for various analyses, including constraints on cosmological parameters, the relationship between galaxies and their dark matter halos, and their growth and evolution over time,” McCreary highlighted. These parameters include the strength of dark energy, the enigmatic force driving the universe’s accelerating expansion.

While initial findings from the JWST map align with the Lambda CDM model of the universe, McCreary emphasizes that a thorough analysis of the data is still required to unearth new insights. “At first glance, it appears consistent with Lambda CDM, but I remain cautious. A final assessment will depend on complete results.”

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Source: www.newscientist.com

Discovering a Barred Spiral Galaxy: Unveiling Cosmic Secrets Just 2 Billion Years Post-Big Bang

Using high-resolution images, NIRCam, a near-infrared camera aboard the NASA/ESA/CSA James Webb Space Telescope, has led astronomers to discover COSMOS-74706, one of the earliest known barred spiral galaxies. This discovery is pivotal in shaping our understanding of cosmic evolution.



COSMOS-74706: Unsharp mask overlaid on F200W, F277W, and F356W filter configurations. The white lines represent logarithmic spirals along the galaxy’s arm structure while the lines indicate the north-south bar structure. Image credit: Daniel Ivanov.

The barred spiral galaxy COSMOS-74706 existed approximately 11.5 billion years ago.

“This galaxy developed its bar just two billion years after the universe’s inception,” stated Daniel Ivanov, a graduate student at the University of Pittsburgh.

“Stellar bars are linear features found at the centers of galaxies, confirming their namesakes.”

COSMOS-74706’s bar comprises a dense collection of stars and gas, appearing as a bright line bisecting the galaxy when viewed perpendicularly to its plane.

Stellar bars significantly influence a galaxy’s evolution, funneling gas from the outskirts into the center, which feeds the supermassive black hole and can inhibit star formation within the galactic disk.

While previous reports identified barred spiral galaxies, their analyses were inconclusive due to the less reliable optical redshift methods compared to the spectroscopy used for COSMOS-74706 verification.

In some instances, a galaxy’s light was distorted by a massive object, leading to a phenomenon known as gravitational lensing.

“Essentially, COSMOS-74706 is the most redshifted spectroscopically confirmed lensless barred spiral galaxy,” Ivanov noted.

“We were not surprised to find barred spiral galaxies so early in the universe’s timeline.”

“In fact, some simulations suggest the bar formed at redshift 5, or roughly 12.5 billion years ago.”

“However, I believe we shouldn’t expect to find many of these galaxies just yet.”

This discovery helps refine the timeline for bar formation, making it a significant finding.

Ivanov and colleagues presented their discoveries on January 8th during the 247th Annual Meeting of the American Astronomical Society.

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Daniel Ivanov et al. 2026 zspec>3 barred spiral without lens. AAS247

Source: www.sci.news

Revolutionary Solution for Cosmic Acceleration: Overcoming Dark Energy Challenges

Researchers from the Center for Applied Space Technology and Microgravity at the University of Bremen and the University of Transylvania in Brașov have unveiled a groundbreaking theoretical framework that challenges our understanding of the universe’s accelerating expansion, potentially rendering dark energy obsolete. They suggest that this acceleration may be an intrinsic characteristic of space-time geometry, rather than a result of unknown cosmic forces.

This artist’s impression traces the evolution of the universe from the Big Bang, through the formation of the Cosmic Microwave Background, to the emergence of galaxies. Image credit: M. Weiss / Harvard-Smithsonian Center for Astrophysics.

For over 25 years, scientists have been puzzled by the unexpected observation that the expansion of the universe is accelerating, counter to the gravitational pull.

In the 1990s, astronomers identified this acceleration through observations of distant Type Ia supernovae, leading to the prevalent theory of dark energy, an invisible force believed to drive this expansion.

Nevertheless, the actual nature of dark energy remains elusive within the Standard Model of cosmology.

Dr. Christian Pfeiffer and his team propose that we may better understand this cosmic acceleration by re-evaluating the geometric framework used to describe gravity.

Central to modern cosmology is Einstein’s theory of general relativity, which details how matter and energy shape space-time.

The universe’s evolution is modeled using the Friedman equation, which originates from Einstein’s principles.

The researchers introduce an innovative solution based on Finsler gravity, an extension of Einstein’s theory.

This approach enhances our understanding of spacetime geometry and allows for a more nuanced exploration of how matter, especially gases, interacts with gravity.

Unlike general relativity, which depends on rigid geometric forms, Finsler gravity presents a more versatile space-time geometry.

With this methodology, the authors recalibrated the equations governing cosmic expansion.

Informed by the Finsler framework, the modified Friedman equation predicts the universe’s acceleration phenomena without necessitating the introduction of dark energy.

In essence, the accelerating expansion emerges directly from the geometry of space-time itself.

“This is a promising hint that we may explain the universe’s accelerating expansion partly without dark energy, drawing from generalized space-time geometry,” Pfeiffer remarked.

This concept does not entirely dismiss dark energy or invalidate the Standard Model.

Instead, it implies that some effects attributed to dark energy might have their roots in a deeper understanding of gravity.

“This fresh geometric outlook on the dark energy dilemma provides avenues for a richer comprehension of the universe’s foundational laws,” stated Dr. Pfeiffer.

The research team’s paper is published in the Journal of Cosmology and Astroparticle Physics.

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Christian Pfeiffer et al. 2025. From a moving gas to an exponentially expanding universe, the Finsler-Friedman equation. JCAP 10:050; DOI: 10.1088/1475-7516/2025/10/050

Source: www.sci.news

Discover the Mental Health Benefits of Stargazing in 2026: A Guide to Cosmic Wellness

Explore the wonders of the universe with New Scientist's insightful articles and detailed analyses on science, technology, health, and environmental news.

This year will be a transformative journey of self-care inspired by the stars.

It has been 20 years since I first experienced profound envy witnessing someone’s ability to navigate the night sky. Back in 2006, while covering a conference in La Jolla, California, I had the chance to meet renowned astrophysicist Neil de Grasse Tyson. One evening, at dinner under the stars, he dazzled us with a laser pointer, mapping out constellations effortlessly. That moment ignited a promise to become a stargazer upon returning home.

Yet, I haven’t fully embraced my stargazing journey. Beyond the familiar Orion and the Big Dipper lies a vast universe I have yet to explore. One could attribute this to urban streetlights, but perhaps it’s also the realization that a love for the night sky is often nurtured during childhood. Those fortunate enough to be introduced to stargazing, typically by family, tend to develop a lasting connection and report better mental health.

Connecting with the universe promotes well-being. Research indicates that this connection is associated with numerous positive mental health benefits. In fact, studies suggest it even encourages generosity.

The term Noctocaelador, from Latin meaning “night,” “sky,” and “worship,” was coined by William Kelly in 2003 to describe the joy and mental health benefits of stargazing. Participants of his study expressed sentiments like, “I truly enjoyed gazing at the night sky” and “Stargazing uplifted my mood.”

In a follow-up study, Kelly discovered that noctcaelador is linked to personality traits, particularly openness to new experiences, often developed early in life.

This aligns with recent findings on Gen Z’s affinity for the night sky. Holly Brenna McNiven’s research indicates that many in this generation report a love for stargazing, attributing it to positive aspects of well-being tied to early experiences with astronomy.Her master’s project at Trinity Saint David’s, University of Wales, suggests that many young people cultivate their stargazing passion through shared experiences, particularly with familial connections.

Regrettably, I missed out on fostering a love for the stars in my early years, but it’s not too late. Nowadays, we don’t always need clear and dark nights to appreciate the universe. With the rising levels of light pollution, it’s reassuring that we can still connect through various resources. Who needs a clear sky when digital platforms like TikTok have unveiled a vibrant community of astronomers, affectionately termed “SpaceTok”?

While most users are from Gen Z, I remain grateful that even during cloudy nights, I can explore the universe through literature. Brian May’s new book, Endless Islands, offers stunning stereoscopic photographs of galaxies. For Christmas, I received Nigel Henbest’s Stargazing 2026, a comprehensive guide to this year’s celestial highlights. With a laser pointer in hand, I’ll soon be navigating the stars as effortlessly as Tyson.

Michael Brooks is a science journalist and author with a focus on physics.

Topics:

  • Mental Health/
  • Stargazing

Source: www.newscientist.com

Discovery of Three Supermassive Black Holes Merging into One: A Cosmic Event Unveiled

Supermassive black holes absorbing matter

Supermassive black holes can consume or merge with other black holes.

Mark Garlick/Science Photo Library

Recent studies reveal that three galaxies featuring supermassive black holes at their cores are merging into a colossal galaxy—a phenomenon rarely observed in astronomy.

Astronomers posit that to achieve their immense sizes, supermassive black holes often need to engulf or merge with other massive black holes during galactic collisions. Discovering these events is challenging, as they are short-lived compared to a black hole’s lifespan. These mergers are most easily detected when a black hole is actively consuming matter and emitting light, which is not frequently the case. Currently, only around 150 pairs of merging galactic black holes have been identified.

Researchers at the U.S. Naval Research Laboratory in Washington, D.C., led by Emma Schwartzman, have identified a trio of supermassive black holes actively feeding and functioning as a single system. “The more galaxies involved, the rarer this system becomes,” Schwartzman noted.

Each supermassive black hole emits low-frequency radiation as radio waves, which can penetrate dust that obscures other forms of light. This characteristic enabled Schwartzman and her team to conduct observations using the Very Long Baseline Array in Hawaii and the Very Large Array in New Mexico, effectively ruling out alternate light sources such as star-filled galaxies.

“What’s particularly intriguing is that all three of these black holes show signs of merging. There’s no guarantee we will observe emissions in the radio spectrum that we haven’t detected before,” Schwartzman commented.

According to Isabella Lamperti, a researcher at the University of Florence, there are visible indications that the galaxies are beginning to interact. Given that two of the galaxies are approximately 70,000 light-years apart, and the third is 300,000 light-years away, this interaction is still in a relatively early phase.

However, considering their life spans spanning billions of years, we are witnessing a dramatic conclusion. “It’s akin to capturing the final moments of a melodrama where the galaxies converge,” commented Emma Kuhn from Ruhr University Bochum, Germany.

Simulating the merging of three active supermassive black holes presents substantial difficulty, but observing this unique system will provide physicists with better insights into more intricate mergers, according to Kuhn. “This marks the initial step in unraveling the physics underlying the system,” she stated.

Explore the Mysteries of the Universe in Cheshire, England

Join a weekend filled with learning alongside some of science’s brightest minds as you delve into the mysteries of the universe. The program includes a fascinating tour of the iconic Lovell Telescope.

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Source: www.newscientist.com

SPHEREx: Mapping the Entire Sky in Infrared for Unprecedented Cosmic Insights

NASA’s SPHEREx (Spectrophotometer for the Exploration of the History of the Universe, Era of Reionization, and Ice) space telescope has successfully created the first comprehensive 102-color infrared map of the entire sky, utilizing observations collected from May to December 2025. While these 102 infrared wavelengths are invisible to the human eye, their widespread presence in the universe enables scientists to tackle significant questions, such as understanding monumental events on Earth. The milliseconds following the Big Bang profoundly influenced the 3D distribution of billions of galaxies. Furthermore, this invaluable data will aid in studying the evolution of galaxies over the universe’s 13.8 billion-year history and analyzing the distribution of essential life ingredients within our Milky Way galaxy.



This infrared image from SPHEREx features color emissions from stars (blue, green, and white), hot hydrogen gas (blue), and cosmic dust (red). Image credit: NASA/JPL-Caltech.

The Earth completes approximately 14.5 rotations in a single day. Spherex travels from north to south, crossing over both poles.

Each day, SPHEREx captures around 3,600 images along a defined circular path in the sky. As time progresses and the planets orbit the sun, SPHEREx’s observational field shifts accordingly.

After six months, the observatory managed to explore the cosmos, capturing a full 360 degrees of the sky.

NASA’s Jet Propulsion Laboratory in Southern California oversees this mission, which commenced sky mapping in May and achieved its inaugural all-sky mosaic in December.

Over its two-year primary mission, SPHEREx plans to conduct three additional all-sky scans, merging these maps to enhance measurement sensitivity.

Dr. Sean Domagal Goldman, director of the Astrophysics Division at NASA Headquarters, remarked, “It’s astounding that SPHEREx has gathered such a wealth of data in just six months. This information, combined with data from other missions, provides deeper insights into the universe.”

“We essentially have 102 new maps of the entire sky, each featuring distinct wavelengths and delivering unique information about celestial objects.”

“Astronomers will find valuable insights here, as NASA’s mission will facilitate answers to fundamental questions regarding the universe’s beginnings and its evolution, ultimately shedding light on our position within it.”

“SPHEREx is a medium-sized astrophysics mission delivering groundbreaking science,” stated Dave Gallagher, director of NASA’s Jet Propulsion Laboratory.

“This remarkable project exemplifies how bold ideas can transform into reality, unlocking immense potential for groundbreaking discoveries.”

Every one of the 102 colors detected by SPHEREx corresponds to a wavelength of infrared light, each of which conveys unique information about galaxies, stars, planet-forming regions, and other cosmic phenomena.

For instance, dense dust clouds in our galaxy, where stars and planets are born, shine brightly at specific wavelengths but remain completely invisible at others.

This separation of light into its component wavelengths is known as spectroscopy.

While prior missions, including NASA’s Wide-Field Infrared Surveyor, have mapped the entire sky, none have achieved the same diversity of colors as SPHEREx.

In contrast, the NASA/ESA/CSA James Webb Space Telescope can perform spectroscopy at significantly longer wavelengths than SPHEREx, but its field of view is thousands of times smaller.

The diversity of colors combined with a wide observational field is what renders SPHEREx exceptionally powerful.

“The true superpower of SPHEREx lies in its ability to capture the entire sky in 102 colors approximately every six months,” declared SPHEREx Project Manager Beth Fabinski, Ph.D., of NASA’s Jet Propulsion Laboratory.

“It’s incredible how much information we can collect in a short timeframe.”

“This makes us akin to telescopic mantis shrimps, equipped with an extraordinary polychromatic visual detection system capable of observing a vast area around us.”

Source: www.sci.news

Asteroid Collision Near a Nearby Star Unravels Cosmic Mystery

Composite image of Fomalhaut’s dust belt (center hidden). The inset displays dust cloud cs1 taken in 2012 together with dust cloud cs2 from 2023.

NASA, ESA, Paul Karas/University of California, Berkeley

Around the star Fomalhaut, asteroids are involved in collisions that generate massive dust clouds. This is the first time astronomers are witnessing these events, offering insights into the early days of our solar system.

Fomalhaut has had its share of unusual findings. In 2008, Paul Kalas, based on observations from the Hubble Space Telescope in 2004 and 2005, reported a potential giant planet orbiting the young star. Over the years, however, the nature of this peculiar object, dubbed Fomalhaut b, has sparked heated debates. It could either be a planet slightly larger than Jupiter or simply a cloud of debris.

Now, Kalas and his team have revisited Fomalhaut using Hubble. “In 2023, we utilized the same equipment as before, and Fomalhaut b was undetectable. It was effectively gone,” says Kalas, “What appeared was a new Fomalhaut b.”

This new bright feature, named Fomalhaut CS2 (short for “circumstellar light source”), cannot be a planet, as it would have been identified earlier. The leading theory is that it represents a dust cloud resulting from the collision of two large asteroids or planetesimals, each approximately 60 kilometers in diameter. The disappearance of Fomalhaut b implies that it may have been a similar dust cloud all along.

“These sources exhibit noise and instability, so we’re still far from drawing definitive conclusions,” notes David Kipping at Columbia University. “Yet, all existing evidence aligns well with a broader narrative of collisions between protoplanets in nascent systems.”

Interestingly, it’s unexpected to observe such a significant break twice. “The hypothesis suggests that we shouldn’t witness such impacts more than once every 100,000 years, if not even more infrequently. And yet, for some unexplained reason, we seem to observe it twice within 20 years,” Kalas explains. “Fomalhaut lights up like a holiday tree and it’s astounding.”

This might indicate that collisions among planetesimals are occurring more frequently than previously thought, particularly around relatively young stars like Fomalhaut. Kalas and his team plan to conduct further observations over the next three years utilizing both Hubble and the more powerful James Webb Space Telescope (JWST) to track the behavior of Fomalhaut CS2 and attempt to pick up faint signals from Fomalhaut b.

This presents a rare opportunity to witness these collisions first-hand. “To comprehend these violent phenomena, we no longer need to rely solely on theoretical models; we can observe them in real time,” Kalas states. Further observations may enlighten us not only about young planetary systems generally but also about our own early solar system’s position in the cosmic landscape.

“We have long pondered whether the collisions that formed our moon are typical of what occurs throughout the universe, and now we have strong evidence suggesting they are indeed common,” Kipping remarked. “Perhaps we are not as unique as some may assume.”

Exploring the Mysteries of the Universe: Cheshire, England

Join a weekend with some of science’s brightest minds as you delve into the mysteries of the universe, featuring a tour of the renowned Lovell Telescope.

Topics:

Source: www.newscientist.com

Stellar-Mass Black Hole Triggers Record-Breaking Cosmic Burst by Collapsing Companion Star

Astronomers have utilized data gathered from a network of space and terrestrial telescopes to identify AT 2024wpp, the most radiant blue light transient (LFBOT) ever recorded. These uncommon, ephemeral, and exceedingly luminous outbursts have perplexed scientists for a decade, but the extraordinary brightness and comprehensive multiwavelength data from AT 2024wpp indicate that they cannot be attributed to typical stellar explosions such as supernovae. Instead, recent observations reveal that AT 2024wpp was generated by an extreme tidal disruption event, where a black hole, with a mass approximately 100 times that of the Sun, dismantles a massive companion star over the course of just a few days, converting a significant portion of the star’s mass into energy.



This composite image contains X-ray and optical data for the LFBOT event at 2024wpp. Image credits: NASA / CXC / University of California, Berkeley / Nayana others. / Legacy Survey / DECaLS / BASS / MzLS / SAO / P. Edmonds / N. Walk.

LFBOTs derive their name from their intense brightness, being visible from hundreds of millions to billions of light years away, and their ephemeral nature, lasting merely a few days.

They emit high-energy light across the blue spectrum into ultraviolet and X-rays.

The inaugural observation was made in 2014, but the first LFBOT with sufficient data for analysis was recorded in 2018, termed AT 2018cow, in accordance with standard naming conventions.

Researchers nicknamed it “cow”, alongside other LFBOTs dubbed “tongue-twisted koala” (ZTF18abvkwla), “Tasmanian devil” (AT 2022tsd), and “finch” (AT 2023fhn). AT 2024wpp is likely to be known as Wasp.

Researchers determined that AT 2024wpp was not a supernova after assessing the energy output of the phenomenon.

The energy was found to be 100 times greater than that produced by typical supernovae.

The emitted energy must convert roughly 10% of the Sun’s rest mass into energy over a brief period of weeks.

Specifically, observations from Gemini South disclosed excess near-infrared radiation emitted by a luminous source.

This marks the second instance astronomers have witnessed such an occurrence, with the first being AT 2018cow, which seemingly doesn’t occur in regular stellar explosions.

These observations establish near-infrared excess as a defining characteristic of FBOT, yet no model can adequately explain it.

“The energy released by these bursts is so immense that it cannot be accounted for by a nuclear collapse or any typical stellar explosion,” stated Nathalie LeBaron, a graduate student at the University of California, Berkeley.

“The main takeaway from AT 2024wpp is that the model we initially proposed is incorrect. This is definitely not an ordinary exploding star.”

Scientists suggest that the intense high-energy light emitted during this extreme tidal disruption stems from the black hole binary system’s prolonged parasitic behavior.

As they piece together this history, it appears the black hole has been gradually siphoning material from its companion star, enveloping itself in a ring of material too distant to be consumed.

Subsequently, when the companion star ventured too near and was shredded, the new material became ensnared in a rotating accretion disk, colliding with pre-existing material and releasing X-rays, ultraviolet light, and blue radiation.

Much of the gas from the companion star ended up spiraling toward the black hole’s poles, where it was expelled as material jets.

Authors calculated that the jet was traveling at about 40% the speed of light and emitted radio waves upon interacting with surrounding gas.

Similar to most LFBOTs, AT 2024wpp is situated in a galaxy characterized by active star formation, making the presence of large stars likely.

Located 1.1 billion light years away, AT 2024wpp is 5 to 10 times more brilliant than AT 2018cow.

The companion star that was torn apart was estimated to be over 10 times the mass of the Sun.

“It may have been what is referred to as a Wolf-Rayet star, a very hot evolved star that has depleted much of its hydrogen,” remarked the astronomers.

“This would account for the weak hydrogen emission observed from AT 2024wpp.”

The findings are published in two papers: Astrophysics Journal Letter.

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Natalie LeBaron others. 2025. Brightest known fast blue light transient AT 2024wpp: unprecedented evolution and properties from ultraviolet to near-infrared. APJL in press. arXiv: 2509.00951

AJ Nayana others. 2025. Brightest known fast blue light transient AT 2024wpp: unprecedented evolution and properties in X-rays and radio. APJL in press. arXiv: 2509.00952

Source: www.sci.news

Astronomers Uncover 50-Million-Light-Year-Long Spinning Cosmic Web Filament

A recently uncovered galactic filament measures at least 50 million light-years in length and is situated 140 million light-years away. A galaxy orbits around the filament’s core, making it one of the largest rotating structures found to date.



Illustration depicting the rotation (right) of neutral hydrogen in a galaxy situated within an elongated filament (center). The galaxies demonstrate coherent bulk rotational motion that traces a large-scale cosmic web (left). Image credit: Lyla John.

Cosmic filaments stand as the largest known structures in the universe, comprising extensive thread-like formations of galaxies and dark matter that serve as the framework of the cosmos.

They also function as “highways” through which matter and momentum funnel into galaxies.

A nearby filament, home to numerous galaxies spinning in the same direction, represents an excellent opportunity to investigate how galaxies developed their current spin and gas content.

This structural arrangement could also provide a basis to test theories regarding how the universe’s rotation accumulates over vast distances.

In a recent study, astronomer Lyra Jung and colleagues from the University of Oxford discovered that 14 nearby hydrogen-rich galaxies form a slender line stretching approximately 5.5 million light-years long and 117,000 light-years wide.

This alignment exists within a considerably larger cosmic filament, about 50 million light-years long, which encompasses over 280 additional galaxies.

Notably, many of these galaxies seem to rotate in the same direction as the filament itself, a pattern that exceeds what would be expected if their rotation were random.

This observation challenges existing models and implies that the universe’s structure may have a more potent and prolonged impact on galaxy rotation than was previously assumed.

Astronomers observed that galaxies flanking the filament’s core were moving in opposite directions, suggesting that the entire formation is in motion.

The team employed a model of filament mechanics to estimate a rotational speed of 110 km/s and calculated the radius of the filament’s dense core region to be about 163,000 light-years.

“What makes this structure remarkable is not just its size, but also the interplay of spin arrangement and rotational motion,” stated Dr. Jung.

“You can liken it to a teacup ride at a theme park. Each galaxy represents a spinning teacup, but the entire platform, the cosmic filament, is also in rotation.”

“This dual motion provides valuable insights into how galaxies acquire rotation from the larger structures they inhabit.”

The filaments appear to be relatively young and undisturbed.

The significant number of gas-rich galaxies, minimal internal motion, and their so-called dynamically cool state imply that the galaxy is still in its formative stages.

Hydrogen serves as the fundamental material for star formation, meaning that galaxies rich in hydrogen gas are actively gathering and retaining the necessary fuel to create stars.

Thus, exploring these galaxies could yield insights into both the early and ongoing phases of galaxy evolution.

Hydrogen-rich galaxies also serve as excellent indicators of gas flow along cosmic filaments.

Due to atomic hydrogen’s susceptibility to motion, its presence aids in mapping how gas is directed through filaments and into galaxies, shedding light on how angular momentum travels through the cosmic web and influences galaxy shape, rotation, and star formation.

“This filament serves as a fossil record of the universe’s flow,” remarked astronomer Dr. Madalina Tudrache from the Universities of Cambridge and Oxford.

“It helps us comprehend how galaxies gain rotation and evolve over time.”

The researchers used data from the MeerKAT radio telescope in South Africa, one of the most powerful telescopes globally, comprising an array of 64 linked satellite dishes.

This rotating filament was detected via an extensive sky survey known as MIGHTEE.

By integrating this data with optical observations from the DESI and SDSS surveys, the study revealed cosmic filaments displaying both spin alignment and bulk rotation in coherent galaxies.

Professor Matt Jarvis from the University of Oxford stated: “This highlights the ability to combine data from various observatories to achieve a deeper understanding of how vast structures and galaxies form in the Universe.”

The findings are detailed in the following article: paper in Royal Astronomical Society Monthly Notices.

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Madalina N. Tudrache and others. 2025. A 15 Mpc rotating galactic filament with redshift z = 0.032 is available for purchase. MNRAS 544 (4): 4306-4316; doi: 10.1093/mnras/staf2005

Source: www.sci.news

Ancient Mayan Ruins Reveal 3,000-Year-Old Cosmic Map

A monumental ancient structure unearthed in Mexico could uncover how the early Maya civilization perceived the universe. Among them, new research indicates that the 3,000-year-old site known as Aguada Fénix served as a cosmogram, representing a geometric map of the cosmos.

Archaeologists initially discovered a large cross-shaped cavity (termed a cross hole) concealed within dense jungle in 2020. Upon closer inspection, they discovered that this was merely one of numerous interconnected holes linked by canals. The cumulative volume of these cross holes exceeds 3.8 million cubic meters, equivalent to nearly one and a half pyramids of Giza or over 1,500 Olympic-sized swimming pools.

Researchers from the University of Arizona utilized laser technology to identify Aguada Fénix from aerial views, situated in the current state of Tabasco on the Gulf Coast.

They now assert that the earliest examples of these findings in Mesoamerica—colored pigments discovered in pits—align with the four cardinal directions: north, south, east, and west. Specifically, vibrant blue azurite represents north, yellow ocher marks south, green malachite signifies east, and pearl-like shells denote west.

Mineral pigments found arranged to correspond with cardinal directions. Researchers suspect that the western deposits may originally included red pigments that have faded over time. – Photo credit: Takeshi Inomata/University of Arizona

According to Independent Maya Expert Dr. James A. Doyle, “The cross shape and color symbolism embedded in the architecture physically embody the concept of how the Earth’s planes are organized and directed.” The BBC Science Focus article also highlights that “the dams and canals underscore the significance of water both practically and symbolically, which is mirrored in the blue and green pigments, shells, and greenstone products.”

Crucially, the new study published in Scientific Progress posits that the construction was a collective effort by a non-hierarchical community, as there is no evidence linking dwellings, palaces, or a central ruling class to late Maya architecture.

Given the size of the structures (Doyle describes them as “some of the largest ever constructed in this area”), it is believed that at least 1,000 individuals would have collaborated over several years to carve the rock and create the cosmogram.

These individuals were likely not coerced by an elite class but were part of an egalitarian society that sought a communal space for stargazing and sharing astronomical knowledge. These vast areas probably also served for trade, social interactions, and religious ceremonies.

Researchers believe this jade artifact depicts a woman in the act of giving birth. – Photo credit: Takeshi Inomata/University of Arizona

Archaeologists have uncovered not only pigments but also jade carvings, primarily reflecting natural experiences rather than deities or leaders. These carvings largely depict animals, although some seem to portray women in childbirth.

Doyle emphasizes that there is still much to uncover about social equality at Aguada Fénix, particularly concerning the enigmatic jade woman.

“What if she represented a strong leader, akin to figures seen in many later societies across Mesoamerica, the Caribbean, and the central Andes?” he queried.

“As excavations progress and our understanding of Aguada Fénix’s builders deepens, we will gain a clearer insight into the disparities in wealth and influence.”

Read more:

Source: www.sciencefocus.com

A Faraway Galaxy Entangled in a Cosmic Web

Simulation of Large-Scale Galactic Structures

Illustris Collaboration/ESO

A cosmic network is disrupting a galaxy’s star-forming abilities. Galaxies require gas to generate stars, and a distant dwarf galaxy, nearly 100 million light-years away, is being deprived of this essential material by an expansive web of cosmic constituents.

While one half of the galaxy known as AGC 727130 seems relatively normal, its opposite side shows gas stretching well beyond its perimeter, being torn apart by unseen forces. Researchers from Columbia University in New York identified this collapsing galaxy utilizing the Very Large Array, a radio observatory situated in New Mexico Nicholas Luber.

Even though AGC 727130 is in proximity to two other dwarf galaxies, the researchers concluded that it isn’t close enough to engage with them in a way that would create turbulent gas. Their findings imply that the gas is expelled through a mechanism known as ram pressure stripping. This occurs when a galaxy traverses an intragalactic cloud—in this case, part of the cosmic web—leaving behind its gas. Without this gas, galaxies become “quenched” and are unable to create new stars.

The filamentous structures in the cosmic web are so slender that it would likely take more than one filament to strip gas from a galaxy, yet AGC 727130 resides at the junction of multiple filaments. “The concept that a cosmic web could extract gas from galaxies through collisional pressure is not surprising and likely happens frequently, but it’s challenging to confirm,” states Luber. “We were fortunate to observe this phenomenon.”

Identifying such galaxies poses a challenge because the gas removal is a gradual process, and galaxies that have already lost their gas tend to be exceedingly faint. “What’s intriguing about this outcome is that low-mass extinguished dwarf galaxies are exceptionally rare; only a few, less than 0.06 percent, are believed to exist without a substantial host galaxy,” comments Julia Blue Bird, a radio astronomer based in New Mexico.

Even among that limited number of extinguished dwarf galaxies, only a scant few have had their gas stripped by the cosmic web rather than through interactions with other galaxies. “This might be… the first definitive case of such an occurrence,” remarks Jacqueline Van Gorcom from Columbia University. Several large radio telescopes are poised to unveil new gas maps across extensive regions of the universe, which could provide additional insights regarding these galaxies.

This discovery is crucial in addressing a cosmological dilemma known as the missing satellite problem. Current cosmological models suggest there should be significantly more dwarf galaxies orbiting larger ones than we currently observe. “We struggle to find many quenched dwarfs; is it because they’re hard to detect, or are they simply not present? This suggests that quenching may also be occurring far from larger galaxies,” states team member Sabrina Stierwalt from Occidental College in California. Uncovering additional galaxies quenched by the cosmic web could help reconcile discrepancies between model predictions and actual observations.

Topic:

Source: www.newscientist.com

Fascinating Tale of the Supreme Cosmic Principle

Where did the speed of light come from and why is it so stubborn?

NASA, ESA, CXC, SSC

This excerpt is from the Lost in Space-Time newsletter, where we share intriguing ideas every month. You can Click here to register for Lost in Time and Space.

If you’ve taken a physics class, you likely have “memorable” instances of measuring light speed, spending hours setting mirrors, lenses, and light sources just right to achieve the result: just under 300 million meters per second. This figure is a fundamental constant in physics and vital for comprehending the universe.

When observing space, light is our primary resource. While we have other means, like gravitational waves, they currently offer limited insights, so I might be exaggerating a tad. Almost all advancements in astronomy and cosmology derive from collecting light that has traversed from the edge of reality over millions, or even billions, of years. Light from our nearest star takes over four years to reach us. The duration it takes for light to travel may be one of the most practical yet least intuitive aspects of physics.

Humans have debated light’s speed long before we truly understood light itself. For centuries, many intellectuals believed that the glowing in certain animals’ eyes at particular angles indicated they emitted light, resembling a lantern. Nonetheless, they debated whether light traveled instantaneously or required time to propagate, a question not thoroughly tested until the 17th century.

An early endeavor to quantify it involved placing a lantern at a distance and measuring the time difference between it lighting up and the observer seeing the light. This method proved ineffective (Galileo and his peers failed to attain conclusive measurements because the lantern was too close), leading scientists to explore more complex and accurate approaches. The first effective instrument was developed in 1675 by Ole Römer while measuring Jupiter’s moon Io’s orbital period. He observed that the period seemed to vary as the distance from Earth to Jupiter fluctuated, which seemed perplexing. Why would Io’s orbit correlate with Earth’s positioning? The only variation was the time it took for light to travel from Io to Earth, diminishing as the two grew closer. A colleague, Christian Huygens, calculated that light’s speed was around 220,000,000 meters per second. Although this estimate lacked precision due to unknown earthly movements, it established a foundation for later refinements. By the early 18th century, measurements were within a few percent of the current consensus of light’s speed in vacuum: 299,792,458 meters per second.

This prompts two inquiries: Why is the speed of light seemingly arbitrary, and why is there a speed limit at all? The first question is straightforward, linked to our units. Meters and seconds (or miles and hours) originated from human experiences. For instance, a mile equals 1,000 steps and has no relation to fundamental constants. The second question is more complex, entwined with special relativity.

The answer lies in perhaps the most recognizable equation: e=mc2. This equation implies that energy and mass can be interchanged. When objects move at extremely high or relativistic speeds, I like to think of them possessing momentum, blending mass and velocity. To increase an object’s speed, we must continually supply more energy. A massive object achieving light speed would require infinite momentum, equating to infinite energy or mass. This situation is unattainable. As an object nears light speed, its mass escalates, making further acceleration unfeasible. Light, having no mass, circumvents this dilemma.

Moreover, special relativity illustrates that an outside, stationary observer would perceive something quite unusual. When an object travels at relativistic speeds, time appears to slow down from an external viewpoint. If I were moving away from you at 99% of light speed, I’d observe my aging decelerating. This phenomenon is termed time dilation. Concurrently, another effect, length contraction, would have you notice that I’m shrinking increasingly as I accelerate. From my frame of reference, I wouldn’t perceive time slowing down or my stature diminishing, but from your outlook, the closer I get to light speed, the shorter and more ageless I appear.

Herein lies a paradox: if I somehow reached light speed, time would seemingly stop for an outside observer as my height approaches zero. I would cease to exist, along with time and space. Luckily, the laws of physics preclude that scenario. Only massless entities can attain that speed limit: photons, gluons, and gravitational effects. Nothing surpasses light speed through space and time.

Rather than feeling disheartened by the universe’s speed limitations, we should celebrate them. The speed of light carries a crucial consequence: it underpins the whole notion of causality. All physics, and our comprehensive understanding of everything, hinges on the principle that effects always follow causes, never the other way around.

Consider this: as I approach light speed, you observe my time slowing down. It will cease entirely when I attain light speed. Should I exceed light speed, from your perspective, I’d be reversing time. If I transmitted a signal faster than light, a hypothetical message defying physics, you’d receive it before I sent it. Absent a universal speed limit, discerning which events caused which effects would be impossible, rendering the universe largely incomprehensible.

Finally, here’s a thought-provoking notion: if all signals require time to travel, and time progresses variably in frames of reference moving at different speeds, what does simultaneous meaning? If I wink at my reflection, the reflected wink arrives slightly later than my physical action, due to light needing to bounce off my face, towards the mirror, and back into my eyes. If two events simultaneously occurred across the universe, I must ask, “By whose standard?” Depending on the distance separating two locations, event 1 might have occurred first for one observer, while event 2 happened prior to event 1 for another. There is no objective simultaneity, no definitive “same time.” This reality stems solely from light’s finite speed. Fascinating, right?

Topic:

Source: www.newscientist.com

VST Unveils “Cosmic Bat” in the Southern Sky

Astronomers using ESO’s VLT Survey Telescope have captured a stunning image of a large nebula that strikingly resembles the silhouette of a bat.



This VST image reveals a gaseous cloud formed like a space bat. The vibrant red glow is produced by hydrogen atoms energized by the powerful radiation from young stars within the cloud. Notable features include RCW 94, which makes up the right wing, and RCW 95, which forms the body, though the remaining bat elements lack official designations. Image credit: ESO / VPHAS+ Team / VVV Team.

“Located about 10,000 light-years away, this ‘space bat’ navigates between the southern constellations Circinus and Norma,” ESO astronomers stated.

“It spans an area of the sky equivalent to four full moons, seemingly foraging in the illuminated spots above.”

“This nebula acts as a stellar nursery, a vast area of gas and dust where new stars are born.”

“The young stars emit sufficient energy to excite surrounding hydrogen atoms, causing them to produce the striking red hue evident in this captivating image.”

“The dark filaments of the nebula resemble the skeletal structure of our space bat.”

“These formations accumulate cooler, denser gas compared to their surroundings, with dust particles obstructing visible light from the stars behind.”

“Named for its extensive catalog of bright star-forming regions in the southern sky, the most prominent clouds are RCW94, representing the right side of the bat, and RCW95, forming the body; however, the other parts of the bat remain unnamed.”

This remarkable image was captured by ESO’s VLT Survey Telescope (VST) at the Paranal Observatory in Chile’s Atacama Desert.

“VST is ideally suited for capturing these large, eerie entities,” astronomers remarked.

“It features OmegaCAM, a cutting-edge 268-megapixel camera, enabling VST to photograph vast sections of the sky.”

“The image is a composite made from observations through various filters that capture different colors and wavelengths of light.”

“Most bat shapes, including the vivid red glow, were recorded in visible light as part of the VST Photometric Hα Survey of the South Galactic Plane and Bulge (VPHAS+).”

“Additional infrared data enhance the coloration of the densest regions within the nebula, obtained with ESO’s Visible Infrared Survey Telescope for Astronomy (VISTA) as part of the VISTA Variable of the Vía Láctea (VVV) survey.”

“Both surveys are accessible to anyone eager to delve into this limitless expanse of astrophotography.”

Source: www.sci.news

Quantum-Inspired Algorithm May Uncover Hidden Cosmic Objects

Galaxy clusters create gravitational lenses, bending light around them

NASA, ESA, Michael Gladders (University of Chicago); Acknowledgment: Judy Schmidt

Quantum physics might hold the key to unraveling the mysteries of celestial objects that remain undetectable or poorly observed through telescopes.

In our quest to comprehend the universe, we gather and scrutinize light emitted by stars and various celestial entities. However, this light often doesn’t travel in a straight path. When passing near massive entities like planets or black holes, the light’s trajectory can curve, resulting in a distorted image, akin to having an additional lens in the process.

Considering smaller objects that lack significant mass, traditional imaging strategies often fall short when dealing with “microlensing” effects. Researchers including Liu Zhenning at the University of Maryland have demonstrated that light analysis protocols that respect the quantum aspects may yield superior results.

They aimed to utilize the quantum features of light to deduce the mass of objects responsible for microlensing. According to Liu, microlensing is detectable when light brightness increases, signaling the presence of an object obscuring our view. However, if this object doesn’t possess substantial mass, its weight remains indeterminate from the light characteristics already measured by the telescope. Such bodies could encompass solitary small black holes or wandering planets.

Given that light consists of photons—quantum particles—there’s valuable information embedded in the quantum nature of its journey to Earth. Notably, when a photon encounters multiple paths around an object, the travel time discrepancies impact its quantum properties. Due to the wave-like characteristics of quantum particles, these photons can traverse both paths simultaneously, mimicking a water wave around a rock. The team’s methodology is adept at analyzing the time differences of both routes, which can be transformed into mass estimates for the objects.

Liu mentions that while planets and black holes inducing microlensing may not be completely imperceptible by other means, these techniques could necessitate more light collection, implying the need for larger telescopes. Quantum methods, however, can function effectively even with smaller photon counts.

For instance, his team’s mathematical assessments indicate that their protocol is particularly effective for stars located in the galactic bulge, a section of the Milky Way where dark matter candidates have been previously identified using gravitational lensing techniques. Because this new approach doesn’t demand a sophisticated quantum computer and can be employed with more conventional devices combined with classical computers to capture and analyze individual photons, it’s poised for real-world testing in the near future.

Daniel Oy, a professor at the University of Strathclyde in the UK, asserts that quantum methodologies significantly enhance the extraction of time-delayed data from light, an enhancement he characterizes as a pivotal advancement in quantum technology. He posits that since quantum theory sets limits on measurement precision in physics, it aligns perfectly with the challenge of detecting faint astronomical signals like those from a limited number of photons.

reference: arXiv, DOI: 10.48550/arXiv.2510.07898

topic:

  • astrophysics/
  • quantum physics

Source: www.newscientist.com

Physicists Suggest a Cosmic ‘Knot’ Could Have Influenced the Early Universe Briefly

Knots are prevalent in various fields of mathematics and physics today. A collaborative team of Japanese and German physicists proposes the existence of a “knot-dominated epoch” in the universe’s early days, suggesting that knots were essential building blocks during this time. This intriguing hypothesis can be investigated through gravitational wave observations. Additionally, they theorize that the conclusion of this period will involve the collapse of the knot due to quantum tunneling, leading to an Asymmetry between matter and antimatter in space.



Model proposed by Eto et al.. It suggests a brief, knot-dominated epoch when these intertwined energy fields outweighed everything else, a scenario that can be investigated through gravitational wave signals. Image credit: Muneto Nitta / Hiroshima University.

Mathematically, knots are defined as closed curves embedded in three-dimensional space and can be found not just in tying neckties but across numerous scientific disciplines today, as noted by Lord Kelvin.

Although his theory postulated that atoms are knots of etheric vortices was ultimately refuted, it sparked advancements in knot theory and its application in multiple areas of physics.

“Our study tackles one of the core mysteries of physics: why the universe is predominantly composed of matter rather than antimatter,” remarked Professor Munehito Nitta, a physicist at Hiroshima University and Keio University.

“This question is crucial as it relates directly to the existence of stars, galaxies, and ourselves.”

“The Big Bang was expected to produce equal amounts of matter and antimatter, with the intent that each particle would annihilate its counterpart, leaving only radiation.”

“Yet, the universe is overwhelmingly composed of matter, with only trace amounts of antimatter.”

“Calculations indicate that to achieve the matter we see today, only one extra particle of matter is needed for every billion matter-antimatter pairs.”

“Despite its remarkable achievements, the Standard Model of particle physics fails to resolve its inconsistencies.”

“That prediction is significantly off.”

“Unraveling the origin of the slight excess of matter, a phenomenon known as baryogenesis, remains one of the greatest unresolved enigmas in physics.”

By merging the measured baryon number minus lepton number (BL) symmetry with the Peksey-Quinn (PQ) symmetry, Professor Nitta and his associates demonstrated that the knot could have spontaneously formed in the early universe, resulting in the observed surplus.

These two well-studied extensions to the standard model address some of its most confounding gaps.

PQ symmetry offers a solution to the strong CP problem, which explains the absence of the small electric dipole moments that theories predict for neutrons, simultaneously introducing axions, a leading candidate for dark matter.

BL symmetry, conversely, elucidates why neutrinos, elusive particles that can seamlessly pass through entire planets, possess mass.

Maintaining the PQ symmetry globally, rather than merely measuring it, safeguards the delicate axion physics that addresses the strong CP problem.

In physics, “measuring” a symmetry implies allowing it to operate freely at any locale and moment in time.

However, this regional freedom requires nature to introduce new mechanisms for force transmission to clarify the equations.

By acknowledging BL symmetry, the researchers not only validated the existence of heavy right-handed neutrinos (crucial for averting anomalies in the theory and central to the primary burr formation model) but also incorporated superconducting behavior, likely providing the magnetic foundation for some of the universe’s earliest knots.

As the universe cooled following the Big Bang, its symmetry may have fractured through a series of phase transitions, leaving behind string-like defects called cosmic strings, which some cosmologists theorize may still persist.

Even though thinner than a proton, a cosmic string can stretch across a mountain.

As the universe expanded, these writhing filaments would twist and intertwine, preserving traces of the primal conditions that once existed.

The breakdown of BL symmetry formed a flux tube string, while PQ symmetry resulted in a flux-free superfluid vortex.

This contrast renders them compatible.

The BL flux tube grants the Chern-Simons coupling of the PQ superfluid vortex a point of attachment.

This coupling subsequently channels the PQ superfluid vortex into the BL flux tube, counteracting the tension that might otherwise disrupt the loop.

The outcome is a metastable, topologically locked structure known as a knot soliton.

“No prior studies had simultaneously considered these two symmetries,” notes Professor Nitta.

“In a way, our good fortune lay in this. By integrating them, we uncovered a stable knot.”

While radiation diminishes energy as waves traverse through space and time, knots exhibit properties akin to matter and dissipate energy far more gradually.

They subsequently surpassed all other forms, heralding an era of knot domination, where their energy density eclipsed that of radiation in the universe.

However, this dominance was short-lived. Ultimately, the knot succumbed to quantum tunneling, an elusive process where particles slip through energy barriers as though they were nonexistent.

This decay yielded heavy dextral neutrinos, a consequence of the inherent BL symmetry within its framework.

These colossal, elusive particles eventually transformed into lighter and more stable variations that favored matter over antimatter, shaping the universe we recognize today.

“Essentially, this decay releases a cascade of particles, including right-handed neutrinos, scalar particles, and gauge particles,” explained Dr. Masaru Hamada, a physicist at the German Electron Synchrotron Institute and Keio University.

“Among them, right-handed neutrinos are particularly noteworthy since their decay can inherently generate a discrepancy between matter and antimatter.”

“These massive neutrinos decompose into lighter particles, such as electrons and photons, sparking a secondary cascade that reheats the universe.”

“In this manner, they can be regarded as the ancestors of all matter in the universe today, including our own bodies, while knots might be considered our forebears.”

Once the researchers delved into the mathematics underlying the model—analyzing how efficiently the knot produced right-handed neutrinos, the mass of those neutrinos, and the degree of heat generated post-collapse—the observed matter-antimatter imbalance naturally emerged from their equations.

Rearranging the equations, with an estimated mass of 1012 gigaelectronvolts (GeV) for heavy dextral neutrinos, and assuming that most energy retained by the knot was utilized to generate these particles, the model yielded a natural reheating temperature of 100 GeV.

This temperature fortuitously coincides with the final opportunity for the universe to produce matter.

Should the universe cool beyond this point, the electroweak reactions that convert neutrino discrepancies into matter would cease permanently.

Reheating to 100 GeV may have also reshaped the cosmic gravitational wave spectrum, shifting it toward higher frequencies.

Forthcoming observatories such as Europe’s Laser Interferometer Space Antenna (LISA), the United States’ Cosmic Explorer, and Japan’s Decihertz Interferometer Gravitational-Wave Observatory (DECIGO) may someday detect these subtle tonal variations.

Dr. Minoru Eto, a physicist at Yamagata University, Keio University, and Hiroshima University, remarked, “The cosmic string is a variant of topological soliton, an entity defined by a quantity that remains unchanged regardless of how much it is twisted or stretched.”

“This characteristic not only guarantees stability but also indicates that our results are not confined to the specifics of the model.”

“While this work is still theoretical, we believe it represents a significant advancement towards future development, as the foundational topology remains constant.”

Although Lord Kelvin initially proposed that knots were fundamental components of matter, the researchers assert that their findings present the first realistic particle physics model in which knots could significantly contribute to the origin of matter.

“The next step involves refining our theoretical models and simulations to more accurately forecast the formation and collapse of these knots, connecting their signatures with observable signals,” said Professor Nitta.

“In particular, upcoming gravitational wave experiments like LISA, Cosmic Explorer, and DECIGO will enable the testing of whether the universe indeed experienced a knot-dominated era.”

The team’s work appears in the journal Physical Review Letters.

_____

Minoru Eto et al. 2025. Tying the Knot in Particle Physics. Physics. Pastor Rhett 135, 091603; doi: 10.1103/s3vd-brsn

Source: www.sci.news

How Did Cosmic Events Influence the Evolution of Hymonin?

Did asteroid impacts shape the trajectory of human evolution?

Anna Ivanova/Alamy

This excerpt is from our “Human Stories” newsletter focusing on the archaeological revolution. Subscribe and receive it monthly in your inbox.

I remember when the concept of an asteroid impact causing the extinction of the dinosaurs was a new and thrilling idea. Luis Alvarez and his team first put forth this theory in 1980—the year before I was born. It was a bold assertion, despite the absence of concrete impact crater evidence at the time, relying instead on an unusual rock formation. It wasn’t until the 1990s, with the identification of the Chicxulub impact crater, that the theory gained substantial traction in paleontological circles. To this day, scientists debate whether the impact was the primary driver of extinction or if dinosaurs were already in decline prior to the asteroid’s strike.

Clearly, nothing comparable occurred during the period of human evolution. The Chicxulub impact was notably catastrophic.

Yet, Earth faces numerous other cosmic hazards. A theory suggests that around 42,000 years ago, anomalies in the Earth’s magnetic field may have triggered a global ecological crisis, potentially contributing to the extinction of Neanderthals. This theory was initially proposed in 2021 in Science, and my colleague Karina Shah covered it in a news article.

Moreover, various cosmic events can affect our planet. Smaller meteorite impacts can severely disrupt ecosystems in their vicinity. Additionally, radiation from exploding stars and “supernovae” subject life on Earth to ongoing existential threats, including that of humans and their extinct relatives.

So, did cosmic events play a role in shaping human evolution?

Magnetic Field Fluctuations

Earth’s magnetic field shields us from intense solar radiation and cosmic rays

Milos Kojadinovic/Alamy

Let us first examine the Earth’s magnetic field. Generated by the movement of molten metals within the Earth’s core, this magnetic field extends far into space, offering protection from harsh solar radiation and cosmic rays.

However, this magnetic field is not entirely stable. Every 100,000 years, it undergoes a flip where the north magnetic pole becomes the south pole. During these reversals, the field’s strength diminishes, allowing more radiation to penetrate the surface.

While these events aren’t catastrophic, there are also “excursions,” where the field strength wanes over extended periods, sometimes altering direction before returning to its original state without a full reversal.

The Laschamps event, occurring about 42,000 years ago, is a notable example where the magnetic field almost completely reversed. A 2021 study indicated this event lasted several hundred years, manifesting severe changes in atmospheric ozone levels. The researchers posited that these shifts likely incited “global climate change, resulting in environmental upheaval, extinction events, and alterations in archaeological records.”

Recent follow-up research has refined these ideas, suggesting that during the field’s excursion, phenomena such as auroras would have been visible farther south, affecting areas like Europe and North Africa and potentially exposing populations to harmful UV rays.

The authors further proposed that early modern humans in western Eurasia might have used a red pigment called ochre as a form of sunscreen, while also developing better clothing techniques. Such adaptations may have aided their survival against increased radiation exposure, unlike Neanderthals who lacked such adaptations.

Interestingly, the timing of the Laschamps event aligns closely with the last known presence of Neanderthals, raising questions about its possible role in their extinction.

Nevertheless, if we take a broader view of the past seven million years of human evolution, multiple magnetic field fluctuations have occurred. How did these excursions and reversals affect life during those times?

Historically, the last complete magnetic reversal occurred during the Brunhes-Matuyama transition around 795,000-773,000 years ago, long before Neanderthals but perhaps around the time of a common ancestor with us. Further explorations reveal numerous magnetic inversions throughout the past seven million years.

While smaller excursions are more frequent, securing evidence of them is challenging. A 2008 analysis identified 14 confirmed excursions over the past two million years, plus six others with weaker support.

Considering that Neanderthals experienced at least three excursions prior to the Laschamps event, why would this particular event lead to their extinction?

In fact, the Laschamps event posed significant hazards; if Neanderthals were vulnerable, it’s likely that other species suffered as well. Many megafauna species became extinct in Australia around 50,000 years ago, yet large animals in the Americas survived much longer, well into the 13,000-year mark. Notably, there was no significant spike in extinctions around 42,000 years ago.

This raises skepticism regarding the hypothesis linking the Laschamps event to Neanderthal extinction. While it may have contributed, it likely wasn’t the primary factor.

Similar issues plague claims about cosmic events impacting human evolution.

Impact Events

I’m fascinated by meteorite impacts. For an interesting afternoon rabbit hole, check out Impact Earth, an interactive map showcasing impact craters on our planet. For example, consider the Zhamanshin Hypervelocity Impact Crater in Kazakhstan, which is 13 km wide and is about 910,000 years old, or the Puntas Macrater in Nicaragua, which is 14 km wide and dates back 804,000 years. Both are notable compared to the Barringer Crater in Arizona, which measures just 1.2 km and is 61,000 years old.

Impact Earth catalogues 48 craters and sediments from the last 2.6 million years of geological history. If we expand our view back to the dawn of humanity, the number increases. Some noteworthy examples include:

Keep in mind, none of these impacts come close to the scale of the Chicxulub crater. The largest craters are merely one-tenth the size. Nevertheless, such impacts can have significant localized effects.

Moreover, the timing and location of impacts matter. For instance, a significant event in Kazakhstan 6 million years ago likely did not affect humans, as they were confined to Africa at that time. However, what remained undisclosed was any research investigating the ecological repercussions of the Aouelloul and Roller Kamm impacts in Africa.

Another notable impact occurred around 790,000 years ago, resulting in unique tektites scattered across Southeast Asia and Australia. A 2019 study linked this to possibly the impact crater in Laos, measuring approximately 15 km in diameter. While it might have influenced Neanderthals, it was simply too distant and too early for it to be critical. However, it was undoubtedly significant for Homo erectus living in that region, but not impactful enough to change their survival as a species around 117,000 to 108,000 years ago.

The Exploding Stars

Supernovae emit massive pulses of matter and radiation

NASA/DOE/Fermi LAT collaboration, CXC/SAO/JPL-Caltech/Steward/O. Krause et al., NRAO/AUI

What about the more distant events, like exploding stars? When massive stars become supernovae, they release a massive outpouring of matter and radiation that traverses the galaxy. For years, we have known that nearby supernovae leave signatures in the rock record in the form of iron isotopes.

It’s challenging to pinpoint specific instances, but it appears a few supernovae events have occurred within the last 4 million years. Some research indicates event timelines such as 2.3 million years ago. I’ve also found other studies identifying incidents at 1.5-3.2 million years and 65-8.7 million years ago. Recently, researchers discovered evidence of supernova radiation hitting Earth around 2-3 million years ago.

This leads to speculation about potential impacts. One proposal suggests extra cosmic rays from a supernova might increase cloud cover, thus lowering temperatures, which could have influenced australopithecines living in Africa at that time. Perhaps.

Physicist Adrian Mellott of the University of Kansas has spent two decades delving into what he terms “astrobiophysics.” He investigates how cosmic events such as supernovae might influence life on Earth. Much of this research pertains to periods before the advent of Homo, but not all.

Mellott highlights a significant moment around 2.6 million years ago when the Pliocene epoch transitioned into the Pleistocene. During this time, large marine extinctions may have coincided with supernova activity. He posits that supernovae could have bombarded Earth with cosmic particles, potentially leading to climate change characterized by more frequent wildfires and increased cancer rates. However, many paleontologists who identified the extinction instead link it to diminishing productive coastal habitats.

The universe presents an extensive array of threats. It’s vital to understand that numerous potentially perilous cosmic events have transpired during human evolution. Yet, limited evidence supports the notion that any of these incidents led to the extinction of human ancestors or any other species.

Thus, I tend to believe that asteroid impacts, supernovae, and shifts in the Earth’s magnetic field played a minimal role in the grand story of human evolution. While some cosmic events may have had localized impacts, they aren’t equivalent to eradicating human species or catalyzing new adaptations.

Keep this perspective in mind the next time you read sensational headlines claiming cosmic events led to the demise of Neanderthals or other species.

Neanderthals, Ancient Humans, Cave Art: France

Join New Scientist’s Kate Douglas on an enthralling journey through time as she delves into the significant Neanderthal and Upper Paleolithic sites across southern France, from Bordeaux to Montpellier.

Source: www.newscientist.com

Underground Microbial Life Could Endure on Mars, Europa, and Enceladus with the Help of Cosmic Rays

A recent study conducted by New York University Abu Dhabi suggests that radiolysis, triggered by cosmic rays in galaxies, may serve as a potential energy source for microbial metabolism within the subsurface environments of rocky celestial bodies such as Mars, Europa, and Enceladus.

NASA’s Cassini spacecraft captured this stunning mosaic of Enceladus as it flew past this geologically active moon of Saturn on October 5, 2008. Image credit: NASA/JPL/Space Science Institute.

While ionized radiation is known for its detrimental effects on biological systems, such as causing damage to DNA and generating reactive oxygen species, it can also yield biologically beneficial outcomes.

Though direct exposure to high radiation levels can be harmful to biological activity, ionizing radiation can create numerous biologically useful products.

One such process involves the generation of valuable biological products through charged particle-induced radiolysis.

“We investigated the consequences of cosmic rays striking surfaces containing water or ice,” noted Dr. Dimitra Atli, PhD, from New York University Abu Dhabi, alongside colleagues from Washington University, the University of Tennessee, Rice University, and Santander University.

“The impact of these rays breaks down water molecules and releases tiny particles known as electrons.”

“Certain bacteria on Earth are capable of utilizing these electrons for energy, akin to how plants harness sunlight.”

“This phenomenon, known as radiolysis, allows for life to persist in dark, cold environments devoid of sunlight.”

This newly reorganized color view presents a massive surface of Europa. The image scale is 1.6 km per pixel, with the northern part of Europa on the right. Image credit: NASA/JPL-Caltech/Seti Institute.

Researchers utilized computer simulations to assess the energy output of this process on the icy moons of Mars, Jupiter, and Saturn.

These icy moons are believed to harbor liquid water beneath their thick ice crusts.

Findings indicate that Enceladus is the most promising candidate for supporting life in this manner, followed closely by Mars and Europa.

“This discovery reshapes our understanding of potential habitats for life,” Dr. Atri commented.

“Rather than confining our search to warm, sunlit planets, we can now consider cold, dark regions where water lies beneath the surface and is subjected to cosmic rays.”

“Life might exist in many more locations than previously thought.”

This image captured by Mars Express’s high-resolution stereo camera reveals an overview of Mars, with patches of yellow, orange, blue, and green on a muted gray background, depicting various surface compositions. Image credits: ESA/DLR/FU BERLIN/G. MICHAEL/CC BY-SA 3.0 IGO.

In their research, the authors introduce a new concept termed the Radiolysis Habit Zone.

Unlike the traditional “Goldilocks zone”—the region around a star where planets can sustain liquid water—this new zone emphasizes the potential for subsurface water that can be energized by cosmic radiation.

Given that cosmic rays are ubiquitous throughout the universe, this suggests that numerous additional locations may harbor life.

“These findings offer fresh directions for future space exploration,” remarked Reservers.

“Scientists can target the underground environments of these icy moons and Mars instead of solely searching for life on their surfaces.

“This study paves the way for thrilling new avenues in life exploration across the cosmos, implying that even the coldest and darkest regions may have conditions suitable for life.”

The study will be published in International Journal of Astrobiology.

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Dimitra Atri et al. 2025. Estimating the potential of ionizing radiation-induced radiolysis for microbial metabolism in Earth’s planets and moons with tenuous atmospheres. International Journal of Astrobiology 24:E9; doi:10.1017/s1473550425100025

Source: www.sci.news

We May Have Finally Cracked the Mystery of Ultra-High Energy Cosmic Rays

Artistic rendering inspired by actual images of the IceCube neutrino detectors in Antarctica.

icecube/nsf

Our focus lies in understanding the true nature of the rarest and most energetic cosmic rays, which aids in deciphering their elusive origins.

The universe continuously showers us with bursts of particles. Brian Clark, from the University of Maryland, explains that the most energetic particles are termed ultra-high energy cosmic rays, possessing more energy than particles accelerated in labs. However, they are quite rare. Researchers are still investigating their sources and the constituent particles remain largely unidentified. Clark and his team are now analyzing the composition using data from the IceCube Neutrino detector situated in Antarctica.

Previous detections of ultra-high energy cosmic rays by the Pierre Auger Observatory in Argentina and a telescope array in Utah have led to disagreements. Clark posits that it remains uncertain whether these rays are mainly composed of protons or if they consist of a mix of other particles. The IceCube data sheds light on this, indicating that protons account for about 70% of these rays, with the remainder composed of heavier ions like iron.

Team member Maximilian Meyer from Chiba University in Japan notes that while IceCube data complements other measurements, it primarily detects neutrinos—by-products resulting from collisions between ultra-high-energy cosmic rays and residual photons from the Big Bang. Detecting and simulating neutrinos is inherently challenging.

The characteristics of cosmic ray particles influence how the magnetic fields generated in space affect their trajectories. Thus, comprehending their structure is crucial for the challenging endeavor of tracing their origins, according to Toshihiro Fujii from Osaka Metropolitan University in Japan.

These mysterious origins have given rise to numerous astonishing enigmas, such as the Amaterasu particle cosmic rays. Interestingly, it seems to have originated from a region in space near the Milky Way that lacks clear astronomical candidates for its source.

Clark expresses optimism about solving many of these mysteries within the next decade, as new observational tools, including an upgrade to IceCube, will soon be operational. “This domain has a clear roadmap for how we can address some of these questions,” he states.

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Source: www.newscientist.com

Mysterious Galaxy Patterns Might Have Been Formed by a Cosmic Bullet

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The lines of galaxies that emerged after the collision of the two dwarf galaxies, which tore gases from one another.

Keim et al./Decals

A curious dwarf galaxy may have originated from a bullet-like collision in the universe.

Michael Keim from Yale University and his team employed the Keck Observatory in Hawaii to examine the distinctive trails of 12 small dwarf galaxies located approximately 75 million light-years from the Milky Way.

The orientation and velocity of the galaxies indicate that they resulted from a head-on impact between two galaxies known as NGC 1052-DF2 and NGC 1052-DF4. This collision expelled gas, which eventually coalesced into a group of stars due to gravitational attraction.

“They’re exceptionally unique,” states Kayme. “This is the only known system of its kind.”

Keim and his colleagues named this system after a similar cluster of large galaxies referred to as Bullet Clusters.

It is believed that the two galaxies collided at a speed of 350 kilometers per second around 9 billion years ago. As they passed through one another, gas was stripped from each galaxy. “While it’s improbable for two stars to collide,” notes Kayme, “the same does not apply to gas clouds.”

Interestingly, the remnants of stars left after the collision appear to lack dark matter. This is quite unusual, as most galaxies contain a substantial amount of dark matter, often comprising over 90% of their total mass.

Keim and his team theorize that this anomaly may stem from dark matter’s inability to interact with regular matter during the gas stripping process or because it remained unaffected by the interaction.

This finding may challenge alternative theories regarding dark matter, which posit that discrepancies in stellar and galactic behavior stem from gravitational effects rather than the existence of dark matter particles. “This suggests that dark matter is indeed a particle that can be separated from a galaxy,” explains Kayme.

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Source: www.newscientist.com

First Image from the World’s Largest Digital Camera Unveils Galaxy Collisions and Cosmic Wonders

Images and videos from the Vera C. Rubin Observatory showcase over 10 hours of test observations before being revealed. The event was live streamed on Monday from Washington, DC.

Keith Bector, an associate professor from the University of Wisconsin-Madison physics department, has contributed to the Rubin Observatory for nearly a decade as a system verification scientist, ensuring that all components of the observation deck function properly.

He mentioned that the team was present as images streamed in real-time from the camera.

“In the control room, there was a moment when all engineers and scientists gazed at these images. We were able to observe more details about stars and galaxies,” Vector explained to NBC News. “Understanding this on an intellectual level is one thing, but on an emotional level, I realized I was part of something truly extraordinary, all happening in real-time.”

One of the newly released images enabled the Rubin Observatory to identify galaxies billions of light-years away, alongside asteroids in the solar system and stars in the Milky Way.

“In fact, most of the objects captured in these images exhibit light that was emitted before our solar system was formed,” highlighted Bechtol. “We are witnessing light that reflects billions of years of the universe’s history, and many of these galaxies have never before been observed.”

Astronomers are eagerly awaiting the first images from the new observatory, affirming that experts will aid in unraveling some of the universe’s greatest mysteries and revolutionizing our understanding.

“We are entering the golden age of American science,” stated Harriet Kang, acting director of the Energy Department of Science. She elaborated in a statement.

“We anticipate that the observation deck will provide profound insights into our past, future, and potentially the fate of the universe,” Kang remarked during a Monday event.

The Vera C. Rubin Observatory is collaboratively managed by the Energy Agency and the National Science Foundation.

Named after an American astronomer renowned for uncovering evidence of dark matter in space, the observatory is situated atop Cerro Pachon, a mountain in central Chile. It is designed to capture around 1,000 images of the southern hemisphere sky each night, covering the entire visible southern sky every three to four nights.

These early images stem from a series of test observations and mark the commencement of a bold decade-long mission to scan the sky continuously, capturing all visible details and changes.

“The entire observatory design is centered on this capability, enabling you to point, shoot, and repeat,” Bechtol noted. “Every 40 seconds, the view shifts to a new part of the sky. Imagine bringing the night sky back to life in a way we’ve never experienced before.”

By repeating this process nightly over the next decade, scientists aim to create extensive images of the visible southern sky, tracking bright stars, moving asteroids in the solar system, measuring supernova explosions, and observing other cosmic phenomena.

“Utilizing this groundbreaking scientific facility, we will delve into many mysteries of the universe, including the dark matter and dark energy that fills our cosmos,” stated Brian Stone, Chief of Staff of the National Science Foundation, in a statement.

Source: www.nbcnews.com

These Cosmic Beasts Are Sparkling the Largest Explosion Since the Big Bang

The immense void of space implies that only one star can occupy a region at a time.

This phenomenon occurs because the mass of these stars is 80 billion times lighter than Earth, with three colossal entities devouring stars ten times larger than our Sun.

A recent study from the University of Hawaii reveals that astronomers, while analyzing data from NASA and the European Space Agency, have identified three ultra-massive black holes. A gigantic one consumes stars far exceeding the sizes of those that orbit the center of our solar system.

The explosions reported by these researchers happened when the black holes tore apart and engulfed the remnants of these stars, yielding the largest events since the Big Bang that shaped our universe.

“What excites me about this research is that we are extending the boundaries of our understanding of the most energetic environments in the universe,” stated Anna Payne, a staff scientist at the Institute of Space Telescope Science and co-author, in a NASA article.

Black holes are cosmic entities that remain unseen by the naked eye, possessing a gravitational force so intense it can capture everything, including light itself. Supermassive black holes, the largest varieties, reside at the centers of galaxies, gradually consuming planets and other materials.

When a star falls under the influence of a supermassive black hole, new research published this week suggests it could end in a dramatic explosion categorized as an “extreme nuclear transient.”Journals advance in science

“These occurrences are unique as they provide the only means for us to illuminate a massive black hole that would typically remain dormant,” noted University of Hawaii graduate student Jason Hinkle in a related article from NASA.NASA article.

Hinkle serves as the lead author of a new study that documents two such events for the first time in the last decade.

Two of the three supermassive black holes were observed by ESA missions in 2016 and 2018, marking the first time they were documented. The third, cataloged as ZTF20Abrbeie, was discovered by the Caltech Observatory in California in 2020 and officially recorded in 2023.

The explosion’s magnitude rivals only that of the Big Bang, which initiated the universe.

Differing from typical stellar explosions, the variations in X-rays, optical, and ultraviolet emissions in these events indicated a “star-consuming black hole.”

NASA explains that black holes actually become brighter during these cosmic occurrences, with their luminosity lasting several months.

This brightness offers scientists a new methodology to uncover additional black holes in the far reaches of the early universe. As astronomers peer into the cosmos, the farther they look, the more ancient light they detect. For instance, light from the Sun takes eight minutes to reach Earth.

“You can use these three objects as a template for what to search for in the future,” Payne remarked.

Source: www.nbcnews.com

Cosmic ray showers are crucial in setting off lightning strikes

It is not well known how lightning starts in a thunderstorm. With the newly developed 3D mapping and polarization system, physicists at the Los Alamos National Laboratory observed that some lightning not only began with positive high-speed discharges, but also faster and wider negative discharges soon began. Surprisingly, the signal polarization is tilted from the direction of the discharge propagation, and the polarization of the two opposite discharges rotates towards each other, indicating that the initiating high-speed discharge is not driven solely by the storm electric field. The authors analyzed these observations in a cosmic ray shower and found that these seemingly strange features could be consistently explained.



Lightning starts with a positive fast discharge followed by a faster, broader negative discharge observed in 3D. The signal polarization from the direction of discharge propagation tilts and rotates between two opposite high-speed discharges. These functions are through a cosmic ray shower that pretreats the discharge path and directs the direction of the discharge current. Image credit: ELG21.

“Scientists still don’t fully understand how lightning starts in a thunderstorm,” says Dr. Xuan-Min Shao, the lead author of the study.

“We noticed an unusual pattern of how lightning started using 3D radio frequency mapping and polarization techniques. Instead of a speedy electrical discharge, the flash of lightning quickly, faster, and negative emissions followed.”

Generally, after the opposition to electrical charge (positive and negative) is separated by clouds, lightning begins, resulting in the emissions that people consider lightning.

In their study, utilizing an innovative, Los Alamos-developed mapping and polarization system called BIMAP-3D, Dr. Xiao and colleagues observed that signal polarization from these discharges had a diagonal pattern from the direction of propagation.

This indicates that something other than the electric field played a role in the initiation of lightning.

In addition to being oblique, physicists have noticed that the direction of polarization has changed between positive and negative emissions.

They attribute this behavior to cosmic ray showers, high-energy particles from spaces entering the Earth’s atmosphere.

These cosmic rays can generate secondary high-energy electrons and positrons in the atmosphere, further ionizing the air, creating paths into thunder, and travel faster after lightning.

Researchers found that high-energy electrons and positrons are pushed in different directions by the Earth’s magnetic field and the cloud’s electric field, leading to oblique discharge currents, i.e. tilted polarization from the path of the cosmic ray shower.

Positrons and electrons were deflected in different directions of the electromagnetic field, explaining why they behaved differently between fast positive and negative discharges.

“This concept can also explain the common case that involves only high-speed positive discharges, and therefore the onset of most lightning flashes,” the scientist said.

Their result It was released on March 3rd Journal of Go Physical Research: Atmosphere.

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Xuan-Min Shao et al. 2025. 3D radio frequency mapping and polarization observations show that a flash of lightning was ignited by a cosmic ray shower. JGR atmosphere 130 (5): E2024JD042549; doi: 10.1029/2024JD042549

Source: www.sci.news

Physicists suggest that ultra-high energy cosmic rays originate from neutron star mergers

Ultra-high energy cosmic rays are the highest energy particles in the universe, and their energy is more than one million times greater than what humans can achieve.

Professor Farrar proposes that the merger of binary neutron stars is the source of all or most ultra-high energy cosmic rays. This scenario can explain the unprecedented, mysterious range of ultra-high energy cosmic rays, as the jets of binary neutron star mergers are generated by gravity-driven dynamos and therefore are roughly the same due to the narrow range of binary neutron star masses. Image credit: Osaka Metropolitan University / L-Insight, Kyoto University / Riunosuke Takeshige.

The existence of ultra-high energy cosmic rays has been known for nearly 60 years, but astrophysicists have not been able to formulate a satisfactory explanation of the origins that explain all observations to date.

A new theory introduced by Glennnies Farrer at New York University provides a viable and testable explanation of how ultra-high energy cosmic rays are created.

“After 60 years of effort, it is possible that the origins of the mysterious highest energy particles in the universe have finally been identified,” Professor Farrar said.

“This insight provides a new tool to understand the most intense events in the universe. The two neutron stars fuse to form a black hole. This is the process responsible for creating many valuable or exotic elements, including gold, platinum, uranium, iodine, and Zenon.”

Professor Farrer proposes that ultra-high energy cosmic rays are accelerated by the turbulent magnetic runoff of the dual neutron star merger, which was ejected from the remnants of the merger, before the final black hole formation.

This process simultaneously generates powerful gravitational waves. Some have already been detected by scientists from the Ligo-Virgo collaboration.

“For the first time, this work explains two of the most mystical features of ultra-high energy cosmic rays: the harsh correlation between energy and charge, and the extraordinary energy of just a handful of very high energy events,” Professor Farrar said.

“The results of this study are two results that can provide experimental validation in future work.

(i) Very high energy cosmic rays occur as rare “R process” elements such as Xenon and Tellurium, motivating the search for such components of ultra-high energy cosmic ray data.

(ii) Very high-energy neutrinos derived from ultra-high-energy cosmic ray collisions are necessarily accompanied by gravitational waves generated by the merger of proneutron stars. ”

study It will be displayed in the journal Physical Review Letter.

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Glennys R. Farrar. 2025. Merger of dichotomous neutron stars as the source of the finest energy cosmic rays. Phys. Pastor Rett 134, 081003; doi:10.1103/physrevlett.134.081003

Source: www.sci.news

This week, seven planets light up the sky, but the cosmic show will soon come to an end

As we approach February, Skywatchers have a final opportunity to witness the “Planet Parade” lighting up the night sky.

The celestial event, where all seven planets in the solar system, apart from Earth, are visible most weeks, is set to provide the best viewing chances for Skywatchers worldwide on Friday. This is because mercury, which only recently appeared on the horizon, will be at its highest point above the horizon.

Starting from Friday, mercury and Saturn will become too dim and too low on the horizon for most observers.

If the conditions are right, it should be possible to spot five out of the seven planets with the naked eye with mercury and Saturn in mind. However, a telescope is necessary to view Uranus and Neptune.

Planetary parades occur when multiple planets are visible simultaneously and spread out in an arc across the sky. While not uncommon, it is rare for all seven planets to be visible at the same time. Four planets were visible before sunrise in August, but NASA states that five will not be visible again until October 2028.

To observe the planets in the sky this week, it is best to find locations on clear nights with minimal light pollution.

Saturn is visible near the horizon (it sets below the sky, making it harder to see during moonrise). Mercury has been far from the sun in recent weeks, making it easier to locate. After sunset, near Saturn, it can be seen low in the western sky.

Venus is also situated in the western part of the sky and is usually the easiest planet to spot due to its brightness.

Jupiter can be observed at dusk. NASA. Mars, meanwhile, is the last planet to set before sunrise.

Michael Shanahan, planetarium director at Liberty Science Center in New Jersey, suggests searching for mercury and Saturn with binoculars near the sunset point shortly after dusk.

As it gets darker, Jupiter, the brightest star in the sky, can be seen overhead. Towards the east, Mars on Earth remains quite bright,” he added.

Shanahan also mentioned that beyond Friday, individuals can witness what he described as “Planetal Ballet against the Starry Background.”

“Around March 10th, Venus will appear too low. Currently, Venus is a bright spot resembling an airplane,” he noted.

Planetary alignments occur due to the planets orbiting the Sun in a relatively flat, disc-like plane. They move along this metaphorical racetrack at their own pace. Mercury completes its orbit in 88 days, Venus takes 225 days, and Saturn takes over 29 years to orbit the Sun.

When multiple planets align on the same side of the metaphorical track, Jackie Faherty, an astronomer and senior research scientist at the American Museum of Natural History in New York City, explained to NBC News earlier this month.

Source: www.nbcnews.com

KM3NET continues to observe the highest energy cosmic neutrinos

The newly detected neutrino, called KM3-230213A, has an incredible energy of 220 peta-electronic (PEV), making it one of the most powerful basic particles ever detected. Its energy was about 100 million times more energy than visible photons, and about 30 times the highest neutrino energy previously detected.



Visual impressions of ultra-high energy neutrino events observed in KM3NET/ARCA. Image credit: km3net.

Cosmic neutrinos are generated near or along cosmic ray propagation pathways, leading to the generation of secondary unstable particles, which then collapse into neutrinos.

Cosmic rays interacting in the Earth's atmosphere generate atmospheric neutrinos that form the experimental background of cosmic neutrinos.

Monitor a huge amount of neutrino observatory to detect space neutrinos. Cherenkov Light It is induced by the passage of charged particles due to neutrino interactions within or near the detector.

“This high-energy neutrino is extremely rare and makes it a monumental discovery,” says Professor Miroslav Filipovich of Western Sydney University.

“This finding represents the most energetic neutrinos ever observed, providing evidence that such high energy neutrinos are being produced in the universe.”

“Detecting such extraordinary particles brings us closer to understanding the most powerful forces that shape our universe.”

Detection of KM3-230213a is KM3NET Telescopephotoelectron-filled tubes are used to capture light from charged particles generated when neutrinos interact with the detector.

“KM3NET's research infrastructure consists of two detector arrays of optical sensors deep in the Mediterranean,” the physicist said.

“The ARCA detector is located approximately 3,450 m deep off the coast of Portopalo Di Capo Passero in Sicily, Sicily, Italy, and is connected to the INFN coastal station, Nazionali Del Sud using electro-optic cables.”

“ARCA's geometry is optimized for research into high-energy cosmic neutrinos.”

“The ORCA detector is located at a depth of approximately 2,450 m in France's offshore Toulon and is optimized for studying neutrino oscillations.”

“Both detectors are under construction, but they are already working.”

The KM3-230213A event recorded light of over 28,000 photons, providing clear trajectories and compelling evidence suggesting the cosmic origin of the particles.

“KM3NET can reconstruct neutrino trajectories and energy,” says Dr. Luke Burns of Western Sydney University.

“To create neutrinos like these, like explosive stars and super-large black holes, requires extreme cosmic conditions.”

“The work of following up on the radiotelescope, like the Australia Square Kilometer Array Pathfinder, helps unlock their secrets.”

The researchers concluded that it is difficult to clearly determine its origin based on a single neutrino.

Future observations will focus on constructing clearer images of such events in order to construct clearer images of such events.

“The energy of the KM3-230213A event is much greater than the energy of neutrinos detected so far,” the scientists said.

“This suggests that neutrinos may be derived from a different cosmic accelerator than low-energy neutrinos, or this could be the first detection of cosmicogenic neutrinos. Universe.”

Team's paper Published in the February 12th issue of the journal Nature.

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KM3NET collaboration. 2025. Observation of ultra-high energy cosmic neutrinos using KM3NET. Nature 638, 376-382; doi:10.1038/s41586-024-08543-1

Source: www.sci.news

Researchers find unusually high levels of cosmic formation beryllium in the Pacific Ocean

A team of scientists from Helmholtz Senturm Dresden Rossendorf, Tad Dresden Institute of Technology, and the Australian National University have discovered an “unexpected” accumulation of Beryllium-10 from the bottom of the central and North Pacific Oceans.

Col et al. Report on the discovery of anomalies in the beryllium-10 concentration profiles of several deep-sea ferromanganese crusts (stars) from the late Miocene central and North Pacific Oceans. The main bottom (blue line) and surface (red line) ocean currents of the thermal halin circulation are shown. Image credit: Koll et al., doi: 10.1038/s41467-024-55662-4.

Radionuclides are types of nuclei (isotopes) that decay into other elements over time.

They are used to date archaeological and geological samples, and radiocarbon dating is one of the best-known methods.

“The major ocean floors on Earth show one of the most pristine geological archives documenting environmental conditions and changes over millions of years, the ferromanganese crust,” Zentrum Dresden-Rossendorf and his colleagues.

“Dating these marine archives can be achieved through fossils through changes in biostratigraphy, isotope, or elemental composition. Alternatively, we can analyze the imprinted changes in the Earth's magnetic field due to magnetic stratigraphy. Masu.”

“Another commonly employed technique is dating space-forming nuclides,” they added.

“The radionuclide Beryllium-10 is continuously produced in the upper atmosphere, primarily through cosmic ray spallation for nitrogen and oxygen.”

“The residence time of Beryllium-10 in the atmosphere is about 1-2 years for it to adhere to the aerosol and precipitate.”

“In the ocean, atmospheric beryllium-10 mixes with the stable beryllium-9 of the lithosphere, which is transported to the ocean by river runoff and river dust, primarily after erosion of terrestrial minerals.”

Dr. Koll and co-authors have discovered long-term cosmicogenic beryllium-10 anomalies in central and North Pacific samples.

Such anomalies can be attributed to changes in ocean currents or astrophysical events that occurred during the late Miocene era around 10 million years ago.

The findings have the potential to serve as a global time marker for promising advances in dating geological archives over millions of years.

“For a period of millions of years, such space-forming time markers still do not exist,” Dr. Koll said.

“However, this beryllium abnormality can act as such a marker.”

result It will be displayed in the journal Natural Communication.

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D. Koll et al. 2025. Cosmic genome 10It becomes abnormal in the late Miocene as an independent time marker for marine archives. Nut commune 16, 866; doi:10.1038/s41467-024-55662-4

Source: www.sci.news

The Strongest Material in the Universe: Ultra-Dense Cosmic “Pasta”

The concept of “strength” in materials refers to their ability to withstand deformation caused by external forces.

Typically, the strongest materials are the densest ones because atoms in close proximity offer greater resistance to compression. However, factors like structural properties can also influence strength, leading to exceptions like graphene, which is the strongest natural material despite not being the densest like osmium.

Some high-density states of matter, formed when massive stars collapse, are incredibly strong compared to ordinary matter. For instance, white dwarf stars have a structure composed of carbon and oxygen nuclei surrounded by electrons experiencing degeneracy pressure, preventing further compression.

However, in cases of extreme density like neutron stars, the degeneracy pressure of densely packed nuclei and free protons and neutrons overcomes electron degeneracy pressure, halting further collapse.

Nuclear pasta is created by the conflicting forces of protons and neutrons, resulting in various shapes. This tightly bound and incredibly strong material is believed to be the most robust substance in the universe. – Credit: Mark Garlick

The material within neutron stars is about 100 trillion times denser than anything found on Earth. While the exact structure is complex and uncertain, a theorized thin layer within the star undergoes a transition from normal to ultra-dense matter, forming different shapes known as nuclear pasta.

Scientists consider this ultra-dense material to be the strongest substance in the universe, estimated to be at least 10 billion times stronger than steel.


This article addresses the question (from Colin Davids of Bridgewater): “What is the strongest material in the universe?”

If you have any questions, please email us at: questions@sciencefocus.comor send us a messagefacebook, twitterorInstagram Page (remember to include your name and location).

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Webb finds mysterious cosmic question mark in distorted galaxy formation

Seven billion years ago, the universe’s star formation boom began to slow. What did our Milky Way galaxy look like at that time? Astronomers using the NASA/ESA/CSA James Webb Space Telescope have discovered a clue in the form of a cosmic question mark, the result of an unusual alignment in space spanning several light-years.



Galaxy cluster MACS-J0417.5-1154 is so massive that it warps the fabric of space-time and distorts the appearance of galaxies behind it. This phenomenon is known as gravitational lensing. This natural phenomenon magnifies distant galaxies, sometimes causing them to appear multiple times in the image, as Webb saw here. Two distant interacting galaxies (a spiral galaxy seen face-on and a dusty red galaxy seen edge-on) appear multiple times, tracing a familiar shape across the sky. Active star formation and the remarkably perfect spiral shape of the galaxy seen face-on indicate that these galaxies are just beginning to interact. Image credit: NASA/ESA/CSA/STScI/V. Estrada-Carpenter, Saint Mary’s University.

“There are only three or four known examples of similar gravitational lensing configurations in the observable universe, so this discovery is exciting as it demonstrates the power of Webb and suggests that we may find more like it in the future,” said Dr Guillaume Despres, from St Mary’s University.

The region has previously been observed by the NASA/ESA Hubble Space Telescope, but Webb was the first to spot the dusty red galaxy forming an intriguing question mark shape.

This is because the wavelengths of light that Hubble detects are trapped in space dust, while longer wavelengths of infrared light pass through Webb’s instruments and can be detected.

Astronomers used both telescopes to observe the galaxy cluster. MACS-J0417.5-1154The cluster is so large that it distorts the fabric of space-time, acting like a magnifying glass.

This will allow astronomers to see clearer details of the much more distant galaxies behind the cluster.

But the same gravitational effects that expand galaxies also cause distortions, which can result in galaxies appearing spread out in an arc across the sky, or appearing multiple times.

This optical illusion in space is called gravitational lensing.

The red galaxy Webb uncovered, along with the spiral galaxy it interacts with, previously detected by Hubble, is magnified and distorted in an unusual way that requires a special and rare alignment between the distant galaxy, the lens, and the observer — something astronomers call hyperbolic umbilical gravitational lensing.

This explains five images of the galaxy pair seen in the Webb image, four of which trace the top of the question mark.

The question mark points are, from our perspective, unrelated galaxies that happen to be in the right place and spacetime.

In addition to developing a case study for Webb, Niris Noting the ability of their infrared imaging device and slitless spectrometer to detect star formation locations in galaxies billions of light years away, the research team also couldn’t help but notice the shape of the question mark.

“This is really cool. I got interested in astronomy when I was younger because I saw amazing images like this,” said Dr Marcin Sawicki, also from Saint Mary’s University.

“Knowing when, where and how star formation occurs in galaxies is crucial to understanding how galaxies have evolved throughout the history of the universe,” said Dr Vicente Estrada Carpenter from Saint Mary’s University.

“The results show that star formation is widespread in both. The spectral data also confirm that the newly discovered dusty galaxy is located at the same distance as the frontal spiral galaxy, suggesting that the two are probably starting to interact.”

“Both galaxies in the question mark pair show several dense regions of active star formation, likely the result of the gas in the two galaxies colliding.”

“But neither galaxy seems particularly disturbed, so perhaps we are seeing the beginning of an interaction.”

“These galaxies, seen billions of years ago when star formation was at its peak, are similar in mass to the Milky Way at that time,” Dr Sawicki said.

“Thanks to Webb, we can now study what our galaxy was like in its teenage years.”

Team paper Published in Monthly Bulletin of the Royal Astronomical Society.

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Vicente Estrada Carpenter others2024. CANUCS JWST/NIRISS We will use grism spectroscopy to investigate when, where and how star formation occurs in a pair of galaxies at cosmic noon. MNRAS 532 (1): 577-591; doi: 10.1093/mnras/stae1368

This article is based on a press release provided by NASA.

Source: www.sci.news

Surprising discovery: AMS detector detects a higher-than-expected number of cosmic rays containing deuterons

Deuteron It is believed that atomic nuclei consisting of protons and neutrons, like those of helium-3 nuclei, are formed in collisions between helium-4 nuclei and other nuclei in the interstellar medium. If this were the case, the flux ratio of deuterons to helium-4 should be similar to that of helium-3 to helium-4. However, this is not the case. Alpha Magnetic Spectrometer Astronauts aboard the International Space Station (AMS) are watching.

Aguilar othersThe deuteron flux was measured using the Alpha Magnetic Spectrometer (AMS) on board the International Space Station.

Cosmic rays are high-energy particles with energies ranging from MeV to 10.20 Electronic V.

These properties are studied from measurements of the energy (stiffness) spectrum (number of particles per unit time, solid angle, surface area, and energy as a function of energy), which is characterized by a rapid decrease in the spectrum as the energy increases.

Cosmic rays with energies below PeV are thought to originate in our own Milky Way galaxy.

The elemental composition of these galactic cosmic rays is dominated by hydrogen nuclei, primarily protons, with helium nuclei making up about 10%, and electrons and nuclei heavier than helium making up just 1% each.

The species synthesized in stars, such as protons, electrons, and most atomic nuclei, are called primary cosmic rays.

Light nuclei, synthesized by nuclear fusion in the cores of stars, are more abundant than heavy nuclei because their production becomes energetically unfavorable as mass increases.

The synthesis of atomic nuclei heavier than iron, such as nickel, occurs through explosive phenomena such as supernova explosions that occur at the end of the life of massive stars, so atomic nuclei heavier than iron are extremely rare.

When primary nuclei are ejected from their source in space, they can collide with interstellar material and split into lighter species.

This is the primary production mechanism for atomic nuclei that are energetically unfavorable to produce by stellar nucleosynthesis, such as lithium, beryllium, boron, fluorine, scandium, titanium, and vanadium. These are called secondary cosmic rays.

Compared to primary nuclei of similar mass, secondary nuclei are less abundant and, as stiffness increases, their stiffness spectrum decreases faster than that of primary nuclei.

The energy (or rigidity) dependence of the cosmic ray spectrum arises from a combination of source-directed emission, acceleration, and propagation mechanisms that occur during a cosmic ray's passage through the galaxy.

Cosmic rays are diffusely accelerated by expanding shock waves, propagate diffusely through the interstellar medium, and are scattered by irregularities in the galactic magnetic field, both of which depend on the particle's momentum, and thus on its magnetic stiffness.

Cosmic ray propagation is described by a stiffness-dependent diffusion coefficient that incorporates the properties of turbulence in the galactic magnetic field.

“Hydrogen nuclei are the most abundant species of cosmic ray,” members of the AMS collaboration wrote in the paper.

“They are made up of two stable isotopes: protons and deuterons.”

“Big Bang nucleosynthesis predicts negligible production of deuterium, and over time the abundance of deuterons has decreased from its primordial value, with the ratio of deuterons to protons measured in the interstellar medium being 0.00002.”

“Deuterons are thought to arise primarily from the interaction of helium with interstellar matter, rather than being accelerated in supernova remnants like primary cosmic ray protons and helium-4.”

“Deuterons, along with helium-3, are called secondary cosmic rays.”

For the latest study, AMS physicists examined data from 21 million cosmic deuterons detected by AMS between May 2011 and April 2021.

When investigating how the deuteron flux varies with rigidity, a surprising feature was discovered.

The AMS data show that these ratios differ significantly above a stiffness of 4.5 GV, with the deuteron to helium-4 ratio decreasing more slowly with stiffness than the helium-3 to helium-4 ratio.

Furthermore, and again contrary to expectations, when stiffness exceeds 13 GV, the data show that the flux of deuterons is nearly the same as the flux of protons, the primary cosmic ray.

Simply put, researchers found more deuterons than expected from collisions between main helium-4 nuclei and interstellar matter.

“Measuring deuterons is very challenging due to the large cosmic proton background radiation,” said Dr Samuel Ting, spokesman for the AMS collaboration.

“Our unexpected results show how little we know about cosmic rays.”

“Future upgrades to AMS will increase the acceptance rate by 300 percent, enabling AMS to measure all charged cosmic rays with 1 percent accuracy, providing the experimental basis for the development of accurate cosmic ray theory.”

The team's paper was published in the journal Physics Review Letter.

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M. Aguilar others(AMS Collaboration). 2024. Properties of cosmic deuterons measured with the Alpha Magnetic Spectrometer. Physiotherapy Rev Lett 132(26):261001;doi:10.1103/PhysRevLett.132.261001

Source: www.sci.news

Amateur astronomers find speedy L-type subdwarf star in our cosmic neighborhood

At an estimated distance of 140 parsecs (457 light years), the L-type subdwarf star CWISE J124909+362116.0 (J1249+36 for short) has a total velocity of at least 600 km/s, exceeding the local galactic escape velocity. Remarkably, the star may have been ejected from a globular cluster in the outer reaches of the Milky Way sometime in the past 10 to 30 million years.

A simulation of the hypothetical J1249+36 white dwarf binary ends with the white dwarf star exploding in a supernova. Image courtesy of Adam Makarenko / WM Keck Observatory.

J1249+36 was first discovered by a citizen scientist. Backyard Worlds: Planet 9 Program.

The star immediately stood out as its speed across the sky was initially estimated to be around 600 km/s.

This speed is fast enough for the star to escape the gravity of the Milky Way, making it a potential hypervelocity star.

To better understand the properties of J1249+36, Professor Adam Burgasser of the University of California, San Diego, and his colleagues used the W. M. Keck Observatory to measure its infrared spectrum.

These data revealed that the object is a rare L-type subdwarf star, a class of stars with an extremely low mass and temperature.

Spectral data and imaging data from multiple ground-based telescopes allowed the team to precisely measure J1249+36's position and velocity in space, and predict its orbit within the Milky Way galaxy.

“What makes this source so interesting is that its speed and orbit suggest it is moving fast enough to escape the Milky Way,” Professor Burgasser said.

The researchers focused on two scenarios to explain J1249+36's unusual orbit.

In the first scenario, J1249+36 was originally a low-mass companion to a white dwarf.

If a companion star is in a very close orbit with a white dwarf, it can transfer mass, causing periodic explosions called novae. If the white dwarf gathers too much mass, it can collapse and explode as a supernova.

“In this type of supernova, the white dwarf is completely destroyed, so the companion star is freed to fly away at the orbital velocity it was originally moving at, plus a bit of a supernova blast,” Prof Burgasser said.

“Our calculations show that this scenario holds true. However, because the white dwarf no longer exists and the remnants of the explosion that probably occurred millions of years ago have already dissipated, we have no conclusive evidence that this is its origin.”

In the second scenario, J1249+36 was originally a member of a globular cluster, a tightly bound group of stars that is immediately recognizable by its distinctive spherical shape.

The centers of these clusters are predicted to contain black holes with a wide range of masses.

These black holes can also form binary systems, and such systems prove to be great catapults for any star that happens to get too close to them.

“When a star encounters a black hole binary, the complex dynamics of this three-body interaction can cause the star to be thrown out of the globular cluster,” said Dr Kyle Kremer, an astronomer at the University of California, San Diego.

The scientists ran a series of simulations and found that, on rare occasions, these types of interactions can cause low-mass subdwarf stars to be ejected from globular clusters and follow orbits similar to the one observed in J1249+36.

“This is a proof of concept, but we don't actually know which globular cluster this star is from,” Dr Kremer said.

“By tracking J1249+36 back in time, we find that it lies in a very crowded part of the sky that may be hiding undiscovered star clusters.”

To determine whether one of these scenarios, or some other mechanism, can explain J1249+36's orbit, the team wants to take a closer look at its elemental composition.

For example, the explosion of a white dwarf star could produce heavy elements that could pollute J1249+36's atmosphere as they escape.

Stars in the Milky Way's globular clusters and satellite galaxies also have unique presence patterns that could shed light on the origins of J1249+36.

“We're basically looking for a chemical fingerprint that will pinpoint exactly what system this star came from,” says Roman Gerasimov, also of the University of California, San Diego.

“Whether J1249+36's high-speed movement is the result of a supernova, a chance encounter with a black hole binary, or some other scenario, its discovery offers astronomers a new opportunity to learn more about the history and dynamics of the Milky Way.”

The astronomers discovery this week's 244th Meeting of the American Astronomical Society In Madison, Wisconsin.

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Adam Burgasser others2024. A superfast L-type subdwarf star passes near the solar system. 224 AustraliaAbstract #3

Source: www.sci.news

Three million years ago, a cosmic cloud left Earth exposed to interstellar space

Illustration of a protection bubble around the sun (yellow dot) and the earth (blue dot)

Harvard Radcliffe Institute

Two to three million years ago, the solar system encountered galactic-scale turbulence and collided with dense interstellar clouds, potentially altering both the Earth's climate and evolution.

Only recently have researchers been able to map the Sun's orbit through the Galaxy, particularly in relation to the relatively dense hydrogen clouds that pass through the interstellar medium, the vast expanse of space between star systems.

the current, Merab Offer A research team from Boston University in Massachusetts has found evidence that one of these clouds, a “local cold cloud ribbon” in Lynx, likely intersects with the Sun's heliosphere.

The heliosphere is a protective cocoon or bubble formed by the solar wind pushing out to the edge of the solar system. Within the heliosphere, the planet is protected from the worst gamma radiation in the galaxy.

The new study proposes that as the solar system passed through the interstellar cloud, the heliosphere retreated from it and moved inward toward the Sun. The researchers think that the heliosphere may have shrunk so much that Earth was outside the protective cocoon provided by the solar wind, perhaps for around 10,000 years.

Merab and his colleagues used the European Space Agency's Gaia satellite to map the location of the dense, cold clouds and the sun's past orbit.

Ofer says the heliosphere's encounter with the cold cloud coincides with deposits of the elements plutonium-244 and radioactive iron-60 in Antarctic ice, deep-sea cores and lunar samples. These elements, which originated from distant supernovae, would have been captured in interstellar clouds and deposited while Earth was outside the heliosphere.

“There are signs of an increase in these elements over the past two years. [million] “The solar cloud record going back 3 million years provides compelling evidence that the Sun did in fact pass through it around 2 million years ago,” Offer says. “The exposure of Earth to a cloud of cold interstellar material and the associated increase in atmospheric hydrogen and radiation almost certainly had a major impact on Earth and its climate.”

Sarah Spitzer The University of Michigan researcher says the paper provides “compelling” evidence that the heliosphere was exposed to a much denser interstellar cloud two to three million years ago. As the solar system passed through that dense, cold cloud, Earth would have been outside the heliosphere and directly exposed to the interstellar environment, she says.

“Understanding this can teach us about the impact interstellar material has had on life on Earth in the past,” Spitzer says, “but it also helps us better understand the impact the heliosphere has on life on Earth today, what would happen if Earth were exposed to interstellar material again in the future, and when that might happen.”

Evan Economo Researchers from Japan's Okinawa Institute of Science and Technology say it's intriguing to consider how encounters in “our nearby space” could have influenced the environment experienced by life on Earth.

“The heliosphere is part of the extended environment experienced by life on the Earth's surface, influencing climate and radiation from space,” he says. “If we had been outside the heliosphere for a period of time, it could have altered the evolutionary trajectory of a wide range of life, including humans. Such connections are highly speculative at this point, but they provide us with new research directions.”

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Source: www.newscientist.com

Scientists are baffled by the discovery of a mysterious cosmic sphere in the universe

Discovered by chance in 2019, Odd radio circles (ORCs) are circular regions of faint radio radiation with bright edges that are not visible to optical, infrared, ultraviolet, and X-ray wavelengths.

Some ORCs contain galaxies at their centers, while others do not, but what sets them apart is their size, which is significantly larger than normal galaxies. Some ORCs display a double ring structure, while others have a single ring. There are also some with internal arc-like structures that might be linked to galaxies surrounded by bubbles of radio emission.

While objects with high spherical symmetry are common in the universe, ORCs appear to be distinct from them all, prompting astronomers to classify them as a new type of object.


ORCs could potentially be a type of spherical shock wave generated by fast radio bursts, gamma-ray bursts, or neutron star mergers. If this is the case, they must be extremely ancient to have grown to such a large size.

Alternatively, they may be associated with material jets emanating from the central regions of radio galaxies, but explaining their size and the absence of central objects in all galaxies is challenging.

One intriguing theory suggests that ORCs are created by the fusion of two supermassive black holes in a central galaxy. The available data also support the idea that the shell is caused by a “shock termination” of high-energy particle winds from the central “starburst” galaxy.

Another hypothesis proposes that the ORC is the throat of a “wormhole,” a theoretical passage through spacetime. However, astronomers have yet to agree on the true nature of ORC.

This article addresses the question (by Bradford’s Brendan Owens): “What are strange radio circles?”

If you have any questions, please email us at: questions@sciencefocus.comor send us a message Facebook, Xor Instagram Page (remember to include your name and location).

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The Internet: A Cosmic Creation by David Bowie that Revolutionized the Music Industry

IAlthough it’s far from his best album, or even the best album of the 1990s, Hours… is David Bowie’s most important album of the decade. However, it wasn’t the music’s fault, but the way it was released. The first album by an artist on the Major His label appeared as a download before it was physically released.

Rolling Stone, writing about the album in August 1999 ahead of its September release, called The Hours a “cyber coup.” This is a continuation of Bowie’s enthusiasm for releasing music online, which began with his 1996 single ‘Telling Lies’. He was also very active. He embraced webcasting and in 1998 he founded his own internet service provider with BowieNet. “I couldn’t be happier with the opportunity to bring the music industry closer to making digital downloads the norm rather than the exception,” he says. How did Bowie explain the release of “Hours…” at the time? “We all know that broadband opportunities are still not available to the overwhelming majority of people, so we hope that the success of this experiment will be measured in hundreds of downloads, not thousands. But just as color television broadcasts and film content on home videotape were necessary first steps to expand the industry’s consumer use, I believe this small step will help my own and others’ We hope this will lead to a huge leap forward for people and ultimately give consumers more choice and easier choice, allowing them to access the music they enjoy.”




The strangeness of cyberspace… David Bowie’s artwork for The Hours…

In early 1998, Virgin Records/EMI made Massive Attack’s Mezzanine available for streaming in its entirety online, with track-by-track previews available over several weeks, in conjunction with its physical release. At the time, the British Phonographic Industry (BPI) warned against this, suggesting that streaming experiments could increase the likelihood of albums being pirated and burned onto CDs by tech-savvy individuals. This did not stop other major labels and their label acts from experimenting from time to time. Def Leppard and Red Hot Chili Peppers made their latest albums, Euphoria and Californication, respectively, available for streaming in full on June 4, 1999, four days before the records hit stores. Bob Merlis of the Chili Peppers’ label, Warner Bros., said, “Getting airplay is getting airplay. You just have to define the atmosphere.” “Since I can’t download it, I thought this was a good idea.”

But Bowie’s album release was designed to be a huge step forward. In 1999 he Interview by Jeremy Paxman He appeared on BBC Newsnight to talk about his career, art and what gives him the most energy – the internet. This 16-minute interview is still published on the BBC website, especially since Bowie’s death in January 2016, as evidence of his remarkable foresight regarding the impact of the internet on art, politics and society. Shared frequently. “I don’t think we’ve even seen the tip of the iceberg,” he told the weary and cynical Paxman. “I think the possibilities that the Internet brings to society are unimaginable, for better or worse. I think we are actually on the cusp of something both exhilarating and frightening.” Paxman says in his own words. suggested that it was just a “tool” that inspired Bowie to take action. “No, it’s not,” he said. “No, it’s an extraterrestrial!”

He went on to say that the Internet…

Source: www.theguardian.com

An undisclosed ice base uncovers ethereal cosmic particles in Antarctica

Scientists have faced a challenge for nearly a century: How do you detect the undetectable, like the elusive neutrino? But now, in a groundbreaking discovery, neutrinos from elsewhere in the Milky Way have been detected for the first time, shedding light on a new era of neutrino astronomy.

The discovery of neutrinos has opened up new possibilities, and researchers like Steve Sclafani from the University of Maryland are excited about this new frontier. Neutrinos, the second most abundant elementary particles in the universe, are notoriously difficult to detect due to their elusive nature. When Austrian physicist Wolfgang Pauli proposed their existence in the 1930s, he thought they could never be detected, but he was proven wrong in 1956.

The discovery of neutrinos from outside the Milky Way was made possible by the IceCube Neutrino Observatory, a massive telescope located near the South Pole. By detecting high-energy neutrinos from distant galaxies, scientists are uncovering the mysteries of cosmic particle accelerators. These accelerators, like supermassive black holes, can provide clues about the origins of cosmic rays and other cosmic phenomena.

Small particles, huge targets

The IceCube detector, operated by a collaboration of scientists from around the world, works by detecting Cherenkov radiation emitted when high-energy neutrinos interact with the ice. This innovative approach allowed researchers to distinguish Milky Way neutrinos from other background signals, leading to the detection of hundreds of neutrinos over a 10-year period.

By studying the distribution of these neutrinos, scientists hope to learn more about the origins of cosmic rays and other high-energy phenomena in our galaxy. With plans to expand the IceCube observatory and improve detection methods, the future of neutrino astronomy looks promising.

Birth of neutrino astronomy

The detection of high-energy neutrinos from the Milky Way marks a new era in astronomy, providing researchers with a unique tool to study cosmic phenomena. By tracking these neutrinos back to their sources, scientists hope to uncover the mechanisms behind cosmic particle accelerators and other cosmic mysteries.

Neutrino astronomy offers a new perspective on the universe, allowing researchers to peer into the heart of energetic and turbulent environments near supermassive black holes. This discovery opens up a whole new window on the universe, providing invaluable insights into the workings of the cosmos.

New perspective

Neutrino astronomy has the potential to revolutionize our understanding of the universe, offering a rare glimpse into the inner workings of cosmic particle accelerators and other energetic phenomena. By studying the origins of high-energy neutrinos, researchers can uncover the mysteries of the cosmos and explore new frontiers in astrophysics. Exciting times lie ahead for neutrino astronomy, with new discoveries and advancements on the horizon.

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About our experts

Mirko Hünefeld from Dortmund University of Technology and Steve Sclafani from the University of Maryland are leading scientists in the field of neutrino astronomy. Their contributions to the IceCube observatory have helped advance our understanding of the universe and unlock new insights into cosmic phenomena.

Source: www.sciencefocus.com

Unraveling the Enigmatic Giant Examoon: Exploring the Cosmic Mysteries of Pandora’s Box







Document


This artist’s impression shows a gas giant exoplanet orbiting a Sun-like star, represented by Kepler-1625b. Credit: NASA

The discovery of giant exomoons around the planets Kepler-1625b and Kepler-1708b raises questions. Since the planets orbit, it is not uncommon for these exoplanets to have moons around them. This makes them even more difficult to detect. So far, only two of the more than 5,300 known exoplanets have been discovered to have moons. New data analysis shows that scientific statements are rarely black and white, that behind every result there is more or less uncertainty, and that the path to a statement often resembles a thriller. Masu.

Introduction to Exomoon research

In observations of the planets Kepler-1625b and Kepler-1708b with the Kepler and Hubble Space Telescopes, researchers discovered the first traces of such moons. New research calls these previous claims into question. Scientists from the Max Planck Institute for Solar System Research and Sonnenberg Observatory in Germany report in the same journal. natural astronomy

The “planet-only” interpretation of the observations is more definitive.

For their analysis, the researchers used Pandora, a newly developed computer algorithm that facilitates and accelerates the search for the Exum Moon. They also investigated what types of exomoons could in principle be discovered with modern space-based astronomical observations. Their answers are quite shocking.

Examoon: A rare entity in observation

In our solar system, with the exception of Mercury and Mercury, the fact that a planet orbits one or more moons is more the rule than the exception. Venus, all other planets have such companions.

For gas giants Saturn Researchers have discovered 140 natural satellites to date. Therefore, scientists believe that planets in distant star systems are also likely to have moons. But so far, there is only evidence for two such examooons: Kepler-1625b and Kepler-1708b. This low yield is not surprising. After all, distant satellites are naturally much smaller than their home world, and therefore much more difficult to find. And combing through observations of thousands of exoplanets for evidence of satellites is extremely time-consuming.

Pandora: Exomoon search algorithm

To make searching easier and faster, the authors of the new study utilize a search algorithm called Pandora that they developed and optimized for exomoon searches. They announced the method last year And the algorithm is available to all researchers as open source code. When applied to observational data from Kepler-1625b and Kepler-1708b, the results were surprising.

“We wanted to confirm the discovery of exomoons around Kepler-1625b and Kepler-1708b,” said MPS scientist Dr. Rene Heller, lead author of the new study. “However, unfortunately, our analysis shows that this is not the case,” he added.


Source: scitechdaily.com

Exploring the Cosmic Landscape: Nueva Vizcaya, Philippines

This Copernicus Sentinel 2 image shows the Nueva Vizcaya province in the Philippines, highlighting its agricultural landscape and urban areas through a false color composite. The image depicts different seasons in different colors, revealing intricate details about crop growth stages, flooded rice fields, and urbanization. Credit: Contains corrected Copernicus Sentinel data (2022-23) processed by ESA. CC BY-SA 3.0 IGO

This pseudocolor satellite image from Copernicus Sentinel 2 brightens the center of Nueva Vizcaya province on Luzon, the Philippines’ largest and most populous island.

The image’s color is due to it being a multitemporal composite consisting of three Copernicus Sentinel 2 images acquired in the mission’s near-infrared channel over a 10-month period. Each acquisition is assigned a different color. Red is the acquisition in May 2022 during the hot dry season, green is the acquisition in September 2022 during the rainy season, and blue is the acquisition in March 2023 during the cool dry season.

This combination highlights different characteristics such as crop type and changes that occur between acquisitions indicating different growth stages.

A patchwork of brightly colored farmland stands out from the center of the image to the bottom left. Areas of red and green shades mean that plant growth took place in May and September, respectively. The fields visible in shades of blue, which make up most of the image, indicate that plant growth occurred mainly in March, during the cool dry season.

Perhaps due to intensive rice production, there are irrigation canals between the fields, and most fields remain flooded all year round. A bright white area, such as the one in the middle of a field, indicates a zone covered with dense vegetation.

Straight lines and gray areas represent roads and urban areas. These include Nueva Vizcaya’s largest town, Solano, visible in the lower left surrounded by blue fields, and Bayombong, the provincial capital further south.

The dark curving lines represent rivers, the largest of which is the Magat River, flowing northeast through the image. If you look closely, you can see different colors along the river’s flow. This is probably due to changes in water levels and river channels at different times of the year.

Copernicus Sentinel 2 has 13 spectral channels and is designed to provide data that can be used to map and monitor agricultural land, as the mission frequently revisits the same areas and has high spatial resolution. , changes in inland waters can be closely monitored.

In January 2023, ESA and the European Commission signed an agreement to build the first Copernicus mirror site in Southeast Asia in the Philippines. This new initiative will strengthen the Philippines’ response capacity and resilience to natural and man-made disasters through the strategic use of space data.


Source: scitechdaily.com