New Release: Adrift in the Cosmos


Massive Tsunami

A significant tsunami could strike the U.S. coast unexpectedly, with experts cautioning that cities are insufficiently prepared. Here’s what we’re learning about the impending major earthquake likely to impact the Pacific Northwest.

Understanding Social Anxiety

Researchers are uncovering evidence that social anxiety is deeply embedded in our biology rather than being solely a psychological issue. As it has biological origins, there are strategies available to help you conquer it during party season.

Defend Against Winter Flu

The holiday season can significantly weaken our immune systems, making it crucial to consider the natural cycles influencing it. The cold, dark winter combined with the warmth of December presents a favorable environment for illness. However, there are methods to bolster your body’s immunity in anticipation of this challenge, leveraging the latest insights from science.

Exploring Near-Death Experiences

By examining individuals who have encountered near-death experiences, scientists are starting to unravel the brain’s activities at the end of life. Remarkably, our brains seem to have a protective mechanism that allows us to transition peacefully, devoid of fear, which is quite reassuring.

Also

  • Super Agers: Experts are eager to identify traits among ‘superagers’ that might unveil the secrets to sustaining memory. Although various genetic and lifestyle factors are in play, certain shared characteristics of superaging are emerging that we can all adopt during the festive season.
  • Holiday Gift Guide:This is an unapologetic Christmas gift guide tailored for tech enthusiasts this year.
  • Q&A: I’ve got answers to your queries. This month, we’re curious: Do any animals use others for play? Is it possible for them to swallow their tongues? Why are marine fossils found atop Mount Everest? Are board games beneficial for the brain? How can we enhance our persuasive skills? What would it entail to navigate through an asteroid belt? How improbable is our universe? If a python consumed you, what would occur? How does the moon’s gradual distancing from Earth affect us?

Issue 427 available Tuesday, December 9, 2025

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Cosmos: AI Researcher Claims to Achieve Six Months of Work in Just Hours

Can AI conduct scientific research?

Tonio Yumui/Getty

AI researchers can work autonomously for extended periods, completing studies in hours that would take humans months. While developers assert that they have made several “new contributions” to science, skepticism remains among some experts.

The platform, referred to as Kosmos, consists of multiple AI agents adept at data analysis and literature review, aiming to generate groundbreaking scientific insights.

“We have dedicated nearly two years to training AI scientists,” states Sam Rodricks, from Edison Scientific, the company behind Kosmos. “The limitation of previous AI scientists has always been the complexity of the concepts they produce.”

Kosmos endeavors to overcome this challenge. Typically, a session can last up to 12 hours; during this time, when a user inputs a scientific dataset, Kosmos examines roughly 1,500 pertinent academic papers while generating and executing 42,000 lines of code to analyze the data. At the end, the AI compiles a summary of the findings and relevant citations, along with a proposal for further analysis that can initiate the next cycle.

After a predetermined number of cycles, the system produces a report featuring scientific conclusions supported by relevant citations, akin to an academic publication. An assessment from a collective of scholars found that 20 of these cycles corresponded to about six months of their research efforts.

Rodriques remarked that the conclusions drawn by the system tend to be fairly accurate. Edison asked individuals with doctoral-level knowledge in biology to evaluate 102 claims made by Kosmos. The research team discovered that 79.4% of these claims were overall substantiated, including 85.5% concerning data analysis and 82.1% of claims referenced in existing literature. Nevertheless, Kosmos struggles to synthesize this information and generate new claims, achieving an accuracy rate of just 57.9% in this area.

Edison asserts that Kosmos has made seven verifiable scientific discoveries, all of which have been confirmed and replicated by independent specialists in the field using external datasets and diverse methodologies. According to the Kosmos team, four of these discoveries are genuinely novel, while the remaining three were previously documented, though in preprints or unpublished studies.

Among the claimed discoveries is a novel method for identifying when cellular pathways falter as Alzheimer’s disease advances. Another finding suggests that individuals with higher levels of a natural antioxidant enzyme known as superoxide dismutase 2 (SOD2) in their blood may experience less heart scarring.

However, reactions to these claims from the scientific community have varied. The “discovery” related to SOD2 is deemed unremarkable by Fergus Hamilton of the University of Bristol, UK. “That specific causal assertion probably won’t withstand scrutiny as a new finding, and there are methodological flaws inherent in the analysis,” he comments. Professor Rodriques acknowledged that the SOD2 finding had been previously established in mice, but claimed this is the first time it has been recognized at the population level in humans through genomics.

Hamilton pointed out that the data analysis code which the agent attempted to execute malfunctioned, causing Kosmos to overlook potentially essential data while arriving at the same conclusions as existing studies.

“Several critical assumptions were made that were imperative for achieving accurate analysis,” he notes. “The software package fails entirely, yet key elements were ignored.” Additionally, in this instance, the data was so processed beforehand that Kosmos “only managed to accomplish around 10 percent of the task,” he suggests.

Hamilton commends the team behind Kosmos for addressing his queries and concerns raised on social media. “While this presents a substantial step forward conceptually, specific technical critiques of this study remain: [the] work is still far from zero,” he states.

“We’re entirely open to the possibility that some of the findings we present could be incorrect or flawed. This is part and parcel of scientific inquiry,” says Rodricks. “Nevertheless, the fact that it has garnered such intricate criticism highlights the system’s potential.”

Others express admiration for Kosmos’ performance overall. “This highlights the immense potential for AI to aid scientific research, but we must remain cautious about the independent use of AI scientists,” states Ben Glocker from Imperial College London. “Even though this study showcases some remarkable achievements, we still lack understanding of the failure modes.”

“We believe embracing tools like Kosmos and developing others is essential. However, we should not lose sight of the fact that science encompasses more than just a data-centric approach,” mentions Noah Jansiracusa from Bentley University, Massachusetts. “There is profound thought and creativity involved, and it would be unwise to disregard scientific pursuits that are amenable to automation solely because they are suitable for AI.”

Rodricks himself concedes that Kosmos is best utilized as a collaborator, rather than a replacement for researchers. “It is capable of performing many impressive tasks,” he asserts. “It requires thorough review and validation, and it may not always be entirely accurate.”

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Source: www.newscientist.com

Soviet Cosmos 482 Spacecraft Collides with Unknown Locations on Earth

The Soviet spacecraft, which was launched on a failed mission to Venus in 1972, is thought to have crashed to Earth early Saturday morning.

The European Space Agency monitored the craft’s uncontrolled descent and reported that it was last tracked by German radar. By the time of the anticipated crash, radar could no longer locate Cosmos 482, concluding that “it is likely that re-entry has already occurred.”

No injuries have been reported.

Cosmos 482 was part of the Soviet Venera Program, a series of probes designed to study Venus. While ten of these missions successfully landed on the harsh planet, the rocket carrying Cosmos 482 malfunctioned, leaving its upper stage, including the descent module, trapped in Earth’s orbit.

For the next 53 years, the approximately 3-foot-wide, 1,069-pound spacecraft orbited Earth in a smaller, elliptical path until it was close enough to descend into the atmosphere.

It’s common for space debris to re-enter the Earth’s atmosphere. The ESA reports that over 2,400 human-made objects fell from space in 2022. Most burned up upon re-entry, with the majority not landing in the ocean.

However, Cosmos 482 was engineered to withstand the dense atmosphere of Venus and operate on a planet with an average temperature of 867 degrees Fahrenheit (464°C). This design means it was theoretically robust enough to endure a routine re-entry through Earth’s atmosphere.

There are no recorded instances of space debris causing human fatalities. An ESA official stated in a blog post about Cosmos-482, “The risk of a satellite re-entering and causing injury is exceedingly low. The annual chance of an individual being harmed by orbital debris is less than one in 100 billion. By comparison, a person is approximately 65,000 times more likely to be struck by lightning.”

On Friday, U.S. space forces estimated that the spacecraft would re-enter the atmosphere at 1:52 AM on Saturday over the Pacific Ocean, west of Guam.

Source: www.nbcnews.com

China and the US race to study neutrinos, the mysterious ‘ghost particles’ of the cosmos

Trillions of neutrinos pass through our bodies every second. The sun produces them through nuclear fusion. The same goes for nuclear power plants. Some come from supernova explosions in space. Neutrinos are paired with antineutrinos, which scientists believe mirror the behavior of neutrinos.

As such, JUNO is designed to capture antineutrinos, specifically the antineutrinos emitted by two nuclear power plants located approximately 53 miles from the observatory.

The 13-story JUNO sphere will be filled with a special liquid called a scintillator and submerged in a cylinder of purified water, said project leader Wang Yifang, director of the China Institute of High Energy Physics.

When the antineutrinos pass through the liquid, they trigger a chemical process that produces a brief burst of light that can be picked up by sensors inside the sphere.

“This event will cause a flash that will last only about 5 nanoseconds, and we hope to capture it with thousands of photomultiplier tubes surrounding the sphere,” he says, as a worker behind him says, Mr. Wang, wearing a helmet, spoke while installing the doubler. “We hope to catch 60 events per day.”

Thanks to its approach, JUNO should be able to measure differences in antineutrino masses about 10 times more accurately than previous instruments.

First of three new neutrino observatories

JUNO is part of China’s ambitious efforts to become a global scientific powerhouse. In a speech this year, President Xi Jinping laid out plans to transform the country into a science and technology superpower by 2035.

October 11th, workers at the bottom of JUNO.Eric Baclinao/NBC News

JUNO is expected to be the first of three next-generation neutrino observatories to open over the next decade, making it a kind of spearhead in a new era of physics. In Japan, the Hyper-Kamiokande Observatory is scheduled to open in 2027. And a U.S.-backed program called the Deep Neutrino Experiment (DUNE) calls for particle accelerators to send beams of neutrinos underground from Illinois to North Dakota starting in 2027. 2031.

The three upcoming observatories are both complementary and competitors, as they all plan to use different techniques to detect particles. Each project involves extensive international collaboration aimed at advancing the field, creating new spin-off technologies and training a new wave of scientists.

“When you start these experiments, it’s not unlikely that you’ll observe something unexpected,” said Chris Marshall, an assistant professor of physics at the University of Rochester who works on the DUNE project. “Trying to unravel these very complex effects will require multiple experiments measuring things in different ways.”

The ability of each observatory to answer important physics questions depends in part on how well researchers can collaborate between and among projects. But there is growing concern among some scientists around the world that rising geopolitical tensions between the United States and China, and the resulting deterioration in their scientific relations, could hinder progress. are.

In recent years, the United States has pursued policies to prevent Chinese scientists from bringing American-based technology to the country and to prevent China from poaching its scientific stars.

Wang said the U.S. is denying visa applications for 2022 and 2023 without explanation and limiting U.S. involvement in JUNO.

“In science, cooperation and competition are good, but it can’t be all about competition,” he said.

On October 11, Mr. Wang pointed out to journalists the underlying characteristics of JUNO’s domain.Eric Baclinao/NBC News

U.S.-based scientists also said they have found new obstacles to cooperation with Chinese scientists.

“From the U.S. side, it’s becoming increasingly difficult to obtain funding for collaborations with Chinese colleagues,” Patrick Huber, director of the Center for Neutrino Physics at Virginia Tech, said in an email. It has also become much more difficult for our Chinese colleagues to obtain U.S. visas.” .

“It’s not impossible to collaborate with Chinese scientists, but it’s becoming increasingly difficult,” said Ignacio Taboada, a physics professor at the Georgia Institute of Technology who directs an existing neutrino observatory in Antarctica. “I’m working on it,” he said.

Solving the mystery of neutrinos

The data generated by JUNO could go a long way toward solving important mysteries about how and why neutrinos change shape more than other elementary particles.

Neutrinos can oscillate, or transform, between three so-called “flavors” during their travels: muon, tau, and electron. For example, the sun sends electron neutrinos toward Earth, but they can also arrive as muon neutrinos. When neutrinos interact (which rarely happens), they settle on a particular flavor.

Additionally, scientists believe that neutrinos travel as one of three different mass states, and that state helps determine the likelihood of a neutrino interacting as a particular flavor. However, it is not yet clear which state has the largest population.

Scientists also found that neutrinos and antineutrinos may deform differently as they travel, and that those differences may account for some of the imbalance in the physics between matter and antimatter in the universe. I think there is.

Journalists take photos at the top of JUNO’s sphere on October 11th.Eric Baclinao/NBC News

If so, learning more about the masses and oscillations of neutrinos and antineutrinos will help researchers find a missing page in the Standard Model of physics (the rulebook of particles and their interactions), or something that has never been known before. This could help researchers understand whether missing particles or forces are having invisible effects. role.

“Our beautiful theory of reality, the Standard Model, is not the final theory,” said Sergio Bertolucci, an Italian particle physicist and DUNE co-spokesperson. “It turns out that we need to know more about neutrinos to answer things that the standard model can’t answer.”

Wang hopes JUNO will win the race to determine the neutrino mass hierarchy before the United States and other countries.

“We just want to be good scientists. In science, being first is most important. There’s nothing to be second,” he said. “As a scientist, I can’t always be a follower. I want to have my own thing.”

Entrance to the Jiangmen Underground Neutrino Observatory in China.Eric Baclinao/NBC News

If JUNO explains the neutrino mass story before DUNE comes online, the U.S.-led project will be able to measure that question differently and confirm JUNO’s results.

DUNE’s plan is to measure neutrinos as they leave the Illinois facility, then travel 800 miles around Earth, where they can interact and oscillate. If the neutrinos arrive in South Dakota and can be detected, scientists could compare the flavor combinations of the neutrinos at the beginning and end of their journey. However, the project experienced delays and cost overruns.

“JUNO’s uniquely rich dataset, alone or in combination with other experiments, will play a key role in determining bulk orders by 2030,” said Professor Pedro Ochoa said in physics and astronomy from the University of California, Irvine.

However, several scientists involved in neutrino observation projects acknowledged that it is impossible to predict how much benefit the research will actually bring to Earth. They suggested that in the future, new technologies could be spun off, driving innovation in data-intensive computing and advancing particle accelerator science.

“We can’t make electric light by improving candles, so we need to take a step forward. We need a break,” said John C., a particle physicist at the U.S. Department of Energy’s Brookhaven National Laboratory and co-spokesperson for the DUNE project. Mary Bishai says. “Basic research inherently creates discontinuities.”

Wang put it another way, saying his work is driven by pure curiosity: “I work in ‘useless’ science.”

Source: www.nbcnews.com

8 of the most bizarre locations in the cosmos

Embark on a journey through the most peculiar corners of the cosmos, where the laws of “normal” reality are left behind. Explore places where time can be squeezed, bubbles blown, and glass rain falls… sideways.

Diamond Planet – Planet 55 Cancer e

Artwork for exoplanet 55 Cancri e. – Image courtesy of Science Photo Library

At a distance of 41 light years lies the star 55 Cancri, or Copernicus, accompanied by a planet named 55 Cancri e, also called Jansen’s Star, completing an orbit in just over 17 hours.

With a mass eight times that of Earth, 55 Cancri e is a scorching super-Earth with temperatures soaring to 2,400 °C (4,350 °F), capable of melting almost any metal.

In 2010, a study discovered that the planet’s host star has a high carbon-to-oxygen ratio, hinting at the possibility of carbon existing mainly in diamond form on 55 Cancri e. It may be a blazing planet adorned with diamonds.

However, subsequent investigations have revealed a different carbon-to-oxygen ratio, casting doubt on the diamond hypothesis. Nonetheless, even if the ratio doesn’t align, 55 Cancri e could still hold the title of the most valuable planet in the known universe.

The deformed star Vega

Vega, the egg-shaped star – Image credit: Matúš Motlo/Wikipedia

Vega, a brilliant star in the sky, serves as a reference point for measuring the brightness of other stars. Astronomers use apparent magnitude, Vega’s magnitude being zero. A magnitude 1 star is 2.5 times dimmer, while a magnitude -1 star is 2.5 times brighter than Vega.

Vega has also taken on the role of the North Star in the past due to Earth’s axial movements. The star’s rapid rotation, complete every 12.5 hours, causes it to bulge at its equator, giving it an egg-shaped appearance unlike the Sun’s near-perfect sphere.

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Curveball Cluster – Globular Cluster NGC 6791

Open cluster NGC 6791, Hubble Space Telescope image. – Image courtesy of Science Photo Library

NGC 6791, a globular cluster, challenges traditional classifications by blending characteristics of both globular and open clusters. Its ancient, metal-rich stars with unique compositions defy typical cluster norms, hinting at a new cluster type distinct from the traditional categories.

Learn more about the universe’s mysteries and anomalies with Professor Brian Cox from the BBC: universe.

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Source: www.sciencefocus.com

Webb uncovers incredible black hole in the ancient cosmos

Using the NASA/ESA/CSA James Webb Space Telescope, astronomers observed a very red quasar-like object. A2744-QSO1 Its color suggests that A2744-QSO1's black hole lies behind a thick veil of dust obscuring much of its light. The researchers also measured the black hole's mass (40 million solar masses) and found it to be much more massive compared to its host galaxy than what has been seen in more localized examples. . This discovery suggests that it may represent the missing link between black hole seeds and the first luminescent quasars.



A composite color image of A2744-QSO1. Image credit: Furutaku other, doi: 10.1038/s41586-024-07184-8.

“We were very excited when Webb started transmitting its first data,” said Dr. Lukas Furtak, a postdoctoral researcher at Ben-Gurion University of the Negev.

“As we were scanning the data coming in for the UNCOVER program, three very compact objects with red flowers stood out to us.”

“Because of its 'red dot' appearance, we immediately suspected it to be a quasar-like object.”

“Using a numerical lensing model we built for the Abell 2744 galaxy cluster, we found that the three red dots are multiples of the same background light source seen when the universe was just 700 million years old. “We determined that it must be an image of Adi Zitlin, also from Ben-Gurion University in the Negev.

“Analysis of the object's color shows that it is not a typical star-forming galaxy,” said Professor Rachel Bezanson, an astronomer at the University of Pittsburgh.

“This further supports the supermassive black hole hypothesis.”

“Together with its compact size, it became clear that this was probably a supermassive black hole, but it was still different from other quasars discovered earlier.”

The astronomers then analyzed the JWST/NIRSpec spectrum of A2744-QSO1.

“The spectrum was just shocking,” said Professor Ivo Rabe of Swinburne University of Technology.

“The spectrum obtained by combining the signals from the three images and the lens magnification corresponds to 1,700 hours that Webb observed the object without a lens, making it the deepest spectrum Webb obtained for a single object in the early universe. Masu.”

“Using the spectrum, we were able to not only confirm that this red compact object is a supermassive black hole and measure its precise redshift, but also estimate its mass based on the width of its emission line. We were able to get a solid estimate,” Dr. Furtak said.

“The gas orbits the black hole's gravitational field, achieving extremely high velocities not seen in other parts of the galaxy.”

“Due to the Doppler shift, the light emitted from the accreting material is redshifted on one side and blueshifted on the other side, depending on its velocity.”

“This makes the emission lines in the spectrum wider.”

But this measurement brought yet another surprise. The black hole's mass appears to be disproportionately large compared to the mass of its host galaxy.

“All the light in that galaxy would have to fit within a small region about the size of a modern star cluster,” said Dr. Jenny Green, an astronomer at Princeton University.

“The source's gravitational lensing magnification provided an exquisite constraint on size.”

“Even if you pack all possible stars into such a small region, the black hole will end up being at least 1% of the total mass of the system.”

“In fact, it has now been discovered that several other supermassive black holes in the early Universe exhibit similar behavior, which provides insight into the growth of black holes and host galaxies, and the interactions between them. This provides some interesting insights, but this is not well understood.”

Astronomers do not know whether such supermassive black holes grow from the remains of stars, for example, or perhaps from material that collapsed directly into black holes in the early universe.

“In some ways, this is an astrophysical chicken-and-egg problem,” says Professor Zitlin.

“Currently we don't know whether galaxies or black holes formed first, how big the first black holes were, and how they grew.”

“Recently, many more such 'little red dots' and other active galactic nuclei have been detected in the Webb, so we hope to have a better idea soon.”

of the team result appear in the diary Nature.

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LJ Furutak other. High black hole-to-host mass ratio in the lensed AGN of the early Universe. Nature, published online on February 14, 2024. doi: 10.1038/s41586-024-07184-8

Source: www.sci.news

Largest black hole energizes the most luminous entity in the cosmos

Artist's impression of record-breaking quasar J0529-4351

ESO/M.Kornmesser

A quasar 500 trillion times brighter than the Sun has earned the title of the brightest known object in the universe. It appears to be powered by a supermassive black hole that devours a sun-sized mass every day.

Quasars are the centers of galaxies where gas and dust falling into a supermassive black hole emit energy in the form of electromagnetic radiation. christian wolff Researchers at the Australian National University in Canberra will discover a new object called J0529-4351 in 2022 by scouring data from the Gaia Space Telescope and looking for extremely bright objects outside the Milky Way that have been mistaken for stars. The brightest quasar was discovered for the first time.

Follow-up observations from the Very Large Telescope (VLT) in Chile revealed that it is the brightest object in the universe as we know it.

Wolf and his colleagues used an instrument on the VLT called a spectrometer to analyze the light coming from J0529-4351 and calculate how much was produced by the black hole's swirling disk of gas and matter, called the accretion disk. did. This revealed that J0529-4351 is the fastest growing black hole in the universe, swallowing about 413 solar masses per year, or more than one sun per day.

Using the spectra of these lights, the researchers calculated that the mass of the black hole was between 5 billion and 50 billion solar masses.

Wolf and his colleagues also discovered the brightest quasar to date in 2018, about half as bright as J0529-4351. Wolf believes this new discovery is likely to account for most of the observable sky and remain the record holder for some time. Now, thanks to extensive star catalogs like those created by Gaia, they can be studied in great detail. “This is the largest unicorn we've ever found with the longest horn on its head. I don't think this record will ever be surpassed,” Wolf says.

The quasar's accretion disk appears to be the widest ever known, measuring 7 light-years in diameter. It says this provides a rare opportunity to directly image a black hole and precisely measure its mass. Christine Dunn At Durham University, UK. “This is large enough and bright enough that it can be solved with current equipment,” he says Done. “That means we can more directly measure the mass of this monster black hole. I was very excited about that.”

VLT is currently upgrading its spectroscopic equipment as part of the Gravity+ project, which should allow it to resolve the characteristics of J0529-4351 in detail. This means different parts of a quasar's accretion disk can be distinguished and better understood, but it could take several years, Dunn said.

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Source: www.newscientist.com

Webb uncovers massive inactive galaxy with mature stars in the ancient cosmos

The formation of galaxies through the stepwise hierarchical coassembly of baryons and cold dark matter halos is a fundamental paradigm underpinning modern astrophysics and predicts a significant decline in the number of giant galaxies in the early Universe. . Very massive quiescent galaxies have been observed 1 to 2 billion years after the Big Bang. These form between 300 million and 500 million years ago and are very limiting for theoretical models, as only some models can form massive galaxies this early. The spectrum of newly discovered quiescent galaxy ZF-UDS-7329 reveals features typical of much older stellar populations. Detailed modeling shows that the stellar population formed about 1.5 billion years ago, when dark matter halos with sufficient host mass had not yet assembled in the standard scenario. This observation may indicate the existence of an undetected early population of galaxies and potentially large gaps in our understanding of the nature of early stellar populations, galaxy formation, and/or dark matter.



This web image shows ZF-UDS-7329, a rare massive galaxy that formed very early in the universe. Image credit: Glazebrook other., doi: 10.1038/s41586-024-07191-9.

Galaxy formation is a fundamental paradigm underpinning modern astrophysics, and a significant decrease in the number of massive galaxies in the early universe is predicted.

Very large quiescent galaxies have been observed 1 to 2 billion years after the Big Bang, casting doubt on previous theoretical models.

Professor Carl Glazebrook, from Swinburne University of Technology, said: “We have been tracking this galaxy for seven years, observing it for hours with two of the largest telescopes on Earth to find out its age.” Ta.

“But it was too red and too faint to be measured. In the end, we had to go outside Earth and use the web to see its properties.”

“This was truly a team effort, from the infrared sky survey that began in 2010 to identifying this galaxy as an anomaly, and the many hours spent with the Keck Telescope and the Very Large Telescope. But we couldn’t confirm it, and finally, last year, we spent a lot of effort trying to figure out how to process the web data and analyze this spectrum.”

“We are now beyond the realm of possibility to have identified the oldest giant stationary monster deep in the universe,” said Dr Temmiya Nanayakkara, an astronomer at Swinburne University of Technology.

“This pushes the limits of our current understanding of how galaxies form and evolve.”

“The key question now is how do stars form so quickly, so early in the universe, and how do they form at a time when other parts of the universe are forming stars? “What kind of mysterious mechanism could cause it to suddenly stop forming?”

“Galaxy formation is determined primarily by how dark matter is concentrated.”

“The presence of these extremely massive galaxies in the early universe poses significant challenges to our standard model of cosmology.”

“This is because dark matter structures large enough to accommodate these massive galaxies are unlikely to have formed yet.”

“More observations are needed to help us understand how common these galaxies are and how massive they really are.”

“This could open new doors in our understanding of the physics of dark matter,” Professor Glazebrook said.

“Webb continues to discover evidence that massive galaxies form early.”

“This result sets a new record for this phenomenon. It’s very impressive, but it’s just one object. But we want to discover more. If I If we were to do this, it would seriously disrupt our understanding of galaxy formation.”

This finding is reported in the following article: paper Published in this week’s magazine Nature.

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K. Glazebrook other. A huge galaxy that formed stars at z ~ 11. Nature, published online on February 14, 2024. doi: 10.1038/s41586-024-07191-9

Source: www.sci.news