Unusual Elements in Supernova Explosions May Influence Extraterrestrial Life

Supernova remnant Cassiopeia A

NASA/JPL-California Institute of Technology/O. Krauss (Steward Observatory)

Within Cassiopeia A, the youngest known supernova in our galaxy, scientists have uncovered unexpectedly high concentrations of chlorine and potassium. These elements, which possess an odd number of protons, are believed to be relatively rare in the universe but are crucial for the emergence of planets and life. Consequently, the findings regarding Cassiopeia A may influence our understanding of the potential locations for extraterrestrial life within the Milky Way.

Supernova remnants, or exploded stars, typically contain elevated levels of elements like oxygen and magnesium, with their cores being comprised of even-numbered protons. Elements with odd-numbered protons (often referred to as “odd Z” elements) are inherently less stable, leading to a reduced likelihood of being created via stellar nuclear fusion. This observation aligns with models of galactic chemical evolution that generally estimate meager quantities of odd Z elements.

“[As it stands] The source of these odd Z elements has been elusive.” Matsunagaumi from Kyoto University in Japan.

Matsunaga and his team recognized that high-resolution X-ray spectroscopy might shed light on the enigma. At the high temperatures prevalent in a supernova remnant, atoms lose electrons and emit unique X-ray signatures that sensitive instruments can detect. The X-ray Imaging Spectroscopy Mission (XRISM), launched in September 2023, is equipped to capture such data and conducted two observations of Cassiopeia A in December 2023.

To determine the abundance of each element, the researchers compared the faint signals from the odd Z elements against the stronger signals from even Z elements, like sulfur and argon, using them as stable reference points for more accurate measurements of the odd Z elements.

The findings revealed that the Cassiopeia A supernova generated significantly more chlorine and potassium than traditional models had anticipated. This indicates that theorists might need to reassess how large stars synthesize these uncommon elements, as certain widely accepted models fail to accommodate the specific conditions of Cassiopeia A.

“While the authors note that their observations diverge from previous models, the reality is more intricate,” says Stan Woosley of the University of California, Santa Cruz, who did not participate in the study. “Not all of our models are incorrect; some perform better than others, and certain ones correlate quite well. Importantly, these observations present astronomers with new, definitive data to refine their models and enhance our comprehension of massive stellar explosions.”

The recent measurements also empower Matsunaga and his colleagues to start evaluating various longstanding theories regarding the formation of odd Z elements in massive stars, including stellar rotation, interactions between binary star pairs, and the merging of diverse combustion layers deep inside stars. Up until now, there was no method to validate these theories against actual data.

“We still lack a complete understanding of which star types contributed to this,” states Katarina Rodders from Washington University in St. Louis, Missouri, who was not involved in the study. “Specifically, we lack clarity regarding the source of chlorine, an element abundant in our oceans.”

If these discoveries hold true for other supernova remnants, they could reshape our perceptions of how life-essential elements are distributed throughout the Milky Way. Depending on the star that seeded a planet, some areas may have a more favorable supply of life’s foundational materials than others. This raises the possibility of uneven distribution of extraterrestrial life across the galaxy.

“That is certainly a possibility,” Matsunaga remarked. “However, we cannot definitively assert this based on the current data.” It remains uncertain whether Cassiopeia A is singular in its production of such substantial quantities of odd Z elements or if it is indicative of supernova remnants in general. “Future observations of additional supernova remnants with XRISM and other upcoming instruments will be pivotal in addressing this issue.”

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Source: www.newscientist.com

New Experiment Reveals Moss Can Endure Long-Term Exposure to Space Elements

A group of Japanese scientists conducted experiments on the model moss species protenema (larval mosses), brood cells (specialized stem cells activated under stress), and sporophytes (protected spores). They investigated Physcomitrium patent to identify the most resilient spores under simulated space conditions, which were then sent to the external environment of the International Space Station (ISS). After nine months in space, over 80% of the spores survived and maintained their capacity to germinate. These findings highlight the potential of land plants like Physcomitrium patent to endure extreme environments when studied in space.



Physcomitrium patent spores demonstrate remarkable resilience to simulated space conditions. Image credit: Meng et al., doi: 10.1016/j.isci.2025.113827.

With the recent rapid changes in the global environment, exploring new avenues for the survival of life beyond Earth has become essential.

Understanding how Earth-origin organisms adapt to extreme and unfamiliar conditions, such as those found in space, is crucial for expanding human habitats on the Moon and Mars.

Researching the survival limits of organisms in both terrestrial and extraterrestrial conditions enhances our comprehension of their adaptability and prepares us for the challenges of ecosystem maintenance.

“Most living organisms, including humans, cannot endure even a brief exposure to the vacuum of space,” explains Dr. Tomomichi Fujita, a researcher at Hokkaido University.

“Yet, the moss spores maintained their vitality even after nine months of direct exposure.”

“This offers astonishing evidence that life forms evolved on Earth possess unique cellular mechanisms to withstand the challenges of space.”

In this study, Dr. Fujita and colleagues examined Physcomitrium patent, a well-studied moss commonly referred to as spread earth moss, under simulated space conditions, which included high levels of ultraviolet radiation, extreme temperature fluctuations, and vacuum settings.

They assessed three structures: Physcomitrium patent — protenema, brood cell, and sporophyte — to determine which is best suited for survival in space.

“We anticipated that the combination of space-related stressors, like vacuum, cosmic radiation, extreme temperature changes, and microgravity, would result in greater damage than any isolated stressor,” remarked Dr. Fujita.

The research revealed that UV light posed the greatest threat to survival, with sporophytes exhibiting the highest resilience among the three moss structures.

Young moss could not tolerate elevated UV levels or extreme temperatures.

Although brood cell viability was significant, the encased spores demonstrated a resistance to UV light that was 1,000 times greater.

These spores survived and germinated after enduring temperatures as low as -196 degrees Celsius for over a week and withstanding heat up to 55 degrees Celsius for a month.

The scientists proposed that the protective structures surrounding the spores may absorb UV light while physically and chemically shielding the spores inside from damage.

This resilience is likely the result of evolutionary adaptations. Moss plants, which evolved from aquatic to terrestrial species approximately 500 million years ago, have survived multiple mass extinctions.

In March 2022, the researchers sent hundreds of sporophytes aboard the Cygnus NG-17 spacecraft to the ISS.

Upon arrival, astronauts affixed the sporophyte samples to the ISS’s exterior, exposing them to space for a total of 283 days.

The spores made their return trip to Earth aboard SpaceX CRS-16, which was returned to the laboratory for analysis in January 2023.

“We had anticipated the survival rate to be nearly zero, but the results were the opposite: the majority of spores survived,” said Dr. Fujita.

“We were truly astounded by the remarkable durability of these tiny plant cells.”

Over 80% of the spores successfully completed the intergalactic journey, with nearly all of them—except for 11%—able to germinate upon returning to the lab.

The research team measured chlorophyll levels in the spores, discovering that all types exhibited normal levels, apart from a 20% reduction in chlorophyll a. Though chlorophyll a is sensitive to changes in light, this decrease did not appear to hinder the spores’ health.

“This study exemplifies the incredible resilience of life that has developed on Earth,” said Dr. Fujita.

Curious about the duration spores could survive in space, the researchers utilized pre- and post-expedition data to formulate a mathematical model.

They projected that the encased spores could endure up to 5,600 days, or around 15 years, under space conditions.

However, they emphasize that this estimate requires further validation through larger datasets to more accurately assess how long moss can thrive in space.

“Ultimately, we hope that this research paves the way for developing ecosystems in extraterrestrial environments like the Moon and Mars,” Dr. Fujita concluded.

“We desire that our moss research can serve as a foundation.”

For further details, refer to the published paper in iscience.

_____

Meng Chang Hyun et al. The extreme environmental resistance and space survivability of moss, Physcomitrium patent. iscience, published online on November 20, 2025. doi: 10.1016/j.isci.2025.113827

Source: www.sci.news

Exploring the Political Significance of Rare Earth Elements

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The U.S. depends on imports for nearly 80% of the rare earth elements necessary for critical electronics, making the securing of mining rights and import agreements a pivotal political issue. NBC News’ Zinhle Essamuah clarifies what rare earth elements are and their significance.

Source: www.nbcnews.com

Study Reveals Asteroid Sample Composition Mirrors Early Solar System Elements

The initial bodies that formed in the solar system gathered materials from stars, presolar molecular clouds, and protozoan debris. Asteroids that have not experienced planetary differentiation retain evidence of these significant materials. Nevertheless, geological processes such as hydrothermal changes can significantly modify their composition and chemistry. In a recent study, researchers scrutinized the elemental and isotopic composition of samples from the asteroid Bennu, uncovering the origin and nature of the materials associated with its parent body.

This mosaic image of the asteroid Bennu consists of 12 images collected on December 2, 2018 by a 15-mile (24 km) Polycam instrument at Osiris-Rex. Image credit: NASA/NASA’s Goddard Space Flight Center/University of Arizona.

“Our analysis shows that Bennu’s elemental composition closely resembles that of the sun,” stated LLNL scientist Greg Brennecka.

“This indicates that the materials obtained from Bennu provide a valuable reference to the initial arrangement of the entire solar system.”

“Notably, Bennu has remained largely untouched by intense heat, which would alter some of its original ingredients.”

Researchers continue to investigate how planets form, and determining the initial composition of the solar system is akin to gathering a recipe for a cake.

“With that recipe, we gain insight into how all these elements interacted to create the solar system and, ultimately, the Earth and its living beings,” Dr. Brennecca remarked.

“If we aim to understand our origins, the composition of our solar system serves as a fundamental starting point.”

Outer view of the Osiris-Rex sample collector. Sample material for the asteroid can be seen in the center right. Image credits: NASA/Erika Blumenfeld/Joseph Aebersold.

The Osiris-Rex mission by NASA has introduced new possibilities by returning pristine samples to Earth while avoiding contamination from our planet.

LLNL scientist Quinn Shollenberger commented:

“We cannot tackle the significant question of ‘origins’ without a sample on Earth.”

“One of our objectives is to ascertain which elements of the periodic table and their percentages contributed to the solar system’s inception. Bennu can help us uncover this,” noted LLNL scientist Jan Render.

To achieve these findings, researchers ground the asteroid material into fine powders and dissolved them in acid.

This mixture was then analyzed with a series of mass spectrometers to determine the concentrations of most elements within the periodic table.

From these results, scientists have sorted the samples by elements and successfully analyzed the isotopic ratios of several.

“I work at a National Laboratory that boasts remarkable analytical capabilities with state-of-the-art equipment,” shared LLNL scientist Josh Winpenny.

“It is quite rare to have all these functions consolidated in one place, allowing us to make optimal use of these valuable materials.”

“NASA’s Johnson Space Center researcher Dr. Anne Nuguen stated:

“We discovered stardust grains with compositions predating our solar system, organic materials likely formed in interstellar space, and high-temperature minerals that originated close to the sun.”

“All these components were transported over to the region that formed Bennu’s precursor asteroids.”

Survey results published in the journal Natural Astronomy.

____

JJ Burns et al. Diversity and origin of materials accumulated by Bennu’s pro-asteroids. Nat Astron Published online on August 22, 2025. doi:10.1038/s41550-025-02631-6

Source: www.sci.news

Toxic Pits: Hidden Treasure Troves for Rare Earth Elements

A tale is shared about miners who discovered copper cans in early mining-era dumps. According to them, wastewater from copper mining flowed across his land, transforming steel cans into copper.

The tale may not be entirely true, but the process is factual and is known as cementation. Montana Resource, which succeeded the Anaconda Copper Company, still employs this alchemical method in the operations at the Continental Pitmine in Butte, Montana.

Adjacent to the mine lies the Berkeley Pit, filled with 50 billion gallons of highly acidic and toxic liquid. Montana Resource channels this liquid from the pits to cascade down iron piles, converting iron into copper for production.

While there have long been methods for extracting metals from water, recent years have ushered in a global rush for metals—vital for manufacturing and technological advancements—leading to a new wave of extraction methods and processes.

Researchers are currently focusing on mineral-rich sources like wastewater, including saline water from desalination plants, oil and gas fracking water, and mining wastewater. Researchers at Oregon State University estimate that the saline water from desalination plants alone contains approximately $2.2 trillion worth of metals.

“Water is a mineral reservoir of the 21st century,” stated Peter S. Fisuke, director of the National Water Innovation Alliance in California at the Department of Energy’s Lawrence Berkeley National Laboratory. “Today’s technology allows us to gather wastewater and extract valuable resources.”

There is extensive research dedicated to recovering rare earth elements—metallic elements sought after due to their increasing demand—from waste. For instance, researchers at Indiana Geological Water Survey at Indiana University are Mining rare earths in coal waste which includes fly ash and coal tails. Additionally, researchers at the University of Texas Austin have created membranes that imitate nature for Separating rare earths from waste.

Utilizing mining wastewater is not only quicker and more economical than establishing a new mine, but it also generates lesser environmental impact.

The vast, contaminated reservoirs in the pit near Butte contain two light rare earth elements (REEs): neodymium and praseodymium. These are crucial for creating small yet powerful magnets, medical technologies, and enhancing defense applications like precision-guided missiles and electric vehicles. Notably, an F-35 Fighter Jet uses around 900 pounds of rare earth metals.

“We’re transforming significant liabilities into assets that contribute to national defense,” remarked Mark Thompson, vice president of environmental affairs at Montana Resources. “There’s a lot of complex metallurgy at play here—the real cutting-edge science.”

This is a crucial moment for exploring domestic rare earth production. The U.S. currently lags behind China, and President Trump’s trade tensions have raised concerns that China may tighten its rare earth mineral exports in response to U.S. tariffs. Experts in mineral security at the Center for Strategic and International Research warn that this gap could enable China to accelerate its defense advancements more swiftly than the U.S.

The Trump administration is particularly fixated on Greenland and Ukraine due to their valuable rare earth deposits.

Trump has recently authorized the government to commence mining on much of the seabed, including areas in international waters, to tap into mineral wealth.

There are 17 distinct types of rare earth metals identified in the Berkeley Pit. While not rare in abundance, they are often deemed scarce due to their dispersion in small quantities.

Rare earths are divided into two categories: heavy and light. Heavy rare earths, including dysprosium, terbium, and yttrium, tend to have larger atomic masses, making them more scarce and thus typically traded in smaller quantities, leading to shortages. In contrast, light rare earths are characterized by a lower atomic mass.

Acid mine drainage is a hazardous pollutant created when sulfur-containing pyrite within rocks interacts with oxygen and water during mining. This process results in the formation of sulfuric acid, which poisons waterways. This environmental issue affects thousands of abandoned mines, contaminating 12,000 miles of streams across the nation.

However, acids facilitate the dissolution of zinc, copper, rare earths, and other minerals from rock formations, presenting an opportunity for extraction techniques that were not previously available.

Paul Ziemkievich, director of the Water Institute at West Virginia University, has been researching Butte’s pit water for 25 years. Alongside a team from Virginia Tech and the chemical engineering firm L3 process development, they developed a method to extract crucial metals from acid mine drainage originating from West Virginia coal mines, the same approach utilized in Butte. Large, densely woven plastic bags filled with sludge from the water treatment plant are employed, allowing water to seep through slowly and yielding about 1-2% rare earth preconcentrate, which requires further refining through chemical processes. The final patented step involves a solvent extraction method that results in pure rare earth elements.

“One of the remarkable aspects of acid mine drainage is that our concentrations are particularly rich in heavy rare earths,” explained Dr. Ziemkiewicz. “Light rare earths carry a lesser value.”

The Butte project is awaiting news on a $75 million grant from the Department of Defense, which is critical for enhancing rare earth enrichment and commencing full-scale production.

Zinc is also abundant in the acid mine drainage mixture and serves as an essential financial asset for the process as it commands a higher market price. Nickel and cobalt are also extracted.

Demand for rare earth elements is high; however, China dominates production, manipulating prices to maintain low costs and stifle competition. This is why the Department of Defense funds various projects focused on rare earth elements and other metals. The U.S. operates only a single rare earth mine in Mountain Pass, California, which produces roughly 15% of the global supply of rare earths.

The Berkeley Pit has posed a chronic problem since 1982, when Anaconda copper companies ceased their open-pit mining operations and halted water pumping, causing it to become filled with water. The acidity levels from the mine’s drainage have proven dangerous; in 2016, thousands of snow geese that landed in the pit quickly succumbed to poisoning, with around 3,000 birds reported dead.

The Atlantic Richfield Company and Montana Resources play crucial roles in permanently treating pit water to avert pollutioning the surrounding groundwater (Montana Resources operates the continental pit adjacent to the Berkeley Pit). The Clean Water Act mandates that companies manage acid mine drainage, and enhancing treatment capabilities at the local horseshoe bend plant is more cost-effective than developing a new facility, which may also offset treatment costs while boosting profits.

Numerous research initiatives have been launched to extract suspended metals from the water. Thompson displayed a map illustrating where radiation was emitted from Butte and where water samples have been dispatched to research facilities nationwide. However, the ongoing metal production process stands as the first to demonstrate profitability.

The mineral wealth present in this region has been recognized for many years; however, extracting it has proven challenging until Dr. Ziemkiewicz’s team innovated new methods. They generate rare earths from two coal mines in West Virginia, where acid mine drainage presents ongoing issues. Each of these mines yields about 4 tons of rare earths annually.

On the other hand, the Berkeley Pit is projected to produce 40 tons annually, bolstered by significantly higher concentrations of rare earths in solution and substantial water content. Dr. Ziemkiewicz believes that this method, when applied to other mines, could potentially satisfy nearly all domestic rare earth requirements for defense-related uses.

However, certain forecasts project that demand for rare earths may surge by as much as 600% in the next few decades.

Lawrence Berkeley laboratories are investigating technologies related to water filtration, particularly experimental approaches to improve membranes, as part of their overarching efforts to purify water, recover significant minerals, and produce necessary minerals. They operate a particle accelerator known as an advanced light source, which generates bright X-ray light that enables scientists to examine various materials at an atomic scale.

The lab has collaborated with external researchers to develop a new generation of filters referred to as nanosponges, designed to capture specific target molecules like lithium.

“It’s akin to an atom catcher’s mitt,” explained Adam Uliana, CEO of Chemfinity, a Brooklyn company exploring the use of nanosponges to purify a variety of waste. “It only captures one type of metal.”

In addition to rare earths, lithium, cobalt, and magnesium have gained significant attention from researchers.

Ion exchange, a well-established technology for extracting metals from water and purifying contaminants, is also gaining interest. Lilac Solutions, a startup based in Oakland, California, has developed specialized resin beads to extract lithium from brine via ion exchange, with plans for their first production facility in Great Salt Lake, Utah.

The company’s technology involves pumping brine through an ion exchange filter to extract minerals, returning water to its source with minimal environmental disruption. If this approach proves viable on a larger scale, it could revolutionize lithium extraction, significantly decreasing the necessity for underground mines and open-pit operations.

Maglathea Metal is an Auckland-based startup that produces magnesium ingots from the saline effluent generated by desalinating seawater. The company processes the brine, which consists of magnesium chloride salts, using a current powered by renewable energy to heat the solution, resulting in the separation of salt from molten magnesium.

CEO Alex Grant noted that the process is exceptionally clean, although it has yet to be applied to magnesium production. Much of the company’s work is funded by the Department of Defense.

With China accounting for 90% of global magnesium production, the current smelting process, known as the Pidgeon process, is highly polluting and carbon-intensive, involving heating to around 2,000 degrees using coal-fired kilns. Dr. Fisuke anticipates further innovations on the horizon.

“Three converging factors are at play,” he stated. “The value of these critical materials is climbing, the expenses associated with traditional mining and extraction are escalating, and reliance on international suppliers, particularly from Russia and China, is diminishing.”

Source: www.nytimes.com

Chimpanzees Share “Fundamental Elements of Musical Rhythms” with Humans

Young Chimpanzee Drumming in Guinea

Cyril Ruoso/Naturepl.com

Musicality may have originated from a shared ancestor of chimpanzees and humans, given the similarities in their drumming techniques.

Katherine Hoheiter at The University of St Andrews and her research team analyzed 371 instances of drumming from two of the four subspecies of chimpanzees in Africa: Western chimpanzees (Pantroglogistics Vers) and Eastern chimpanzees (Pan troglodytes schweinfurthi).

They utilize their hands and feet, often on buttress roots, creating rapid rhythms mainly during rest, travel, or during displays of threat.

Hoheiter mentions that while capturing chimpanzee drumming is common, the rainforest poses significant research challenges, and gathering data for some populations took decades.

Ultimately, researchers found that chimpanzees drum significantly faster than most humans. “The longest drumming event we recorded exceeded five seconds, while the shortest was less than 0.1 seconds,” notes Hoheiter. “Chimpanzees also tend to repeat these beats, especially while traveling.”

Despite the contrasts between chimpanzee and human drumming, chimpanzees exhibit some “core components of human musical rhythms,” according to team member Vesta Eleuteri from the University of Vienna.

“They employ recognizable rhythms present in various musical cultures, which contrasts with randomly played beats. These consist of hits that are evenly spaced, akin to clock ticks,” she elaborates. “Moreover, we discovered that the Eastern and Western chimpanzee subspecies, residing on different sides of Africa, exhibit distinct rhythmic patterns.”

Eleuteri explains that Eastern chimpanzees alternate between short and long intervals between beats, while Western chimpanzees maintain equally spaced hits. Additionally, these chimpanzees initiate drumming more quickly and use more hits to commence drumming early during a unique pant-hoot call.

Miguel Rulente from the University of Girona finds the notion that different subspecies display unique drumming styles compelling. “These patterns suggest the potential for not just individual idiosyncrasies but also cultural distinctions in how groups utilize drumming as communication tools.”

It is well understood that rhythm plays a crucial role in human social interaction, whether through music, dance, or even conversational rhythms, explains Hoheiter. “I’m not implying that chimpanzee drumming reflects the sophistication of modern human rhythms. However, this research is the first to show that we share fundamental rhythmic elements, suggesting that rhythms are intrinsic to our social environment even before we evolved into humans.”

“Previously, it was claimed that rhythmicity was exclusive to humans,” states Gisela Kaplan from the University of New England. “However, a growing body of evidence suggests this is not the case.”

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Source: www.newscientist.com

Magnetic Flares Could Be Key to the Formation and Distribution of Gold and Other Heavy Elements

Since the Big Bang, the early universe has contained hydrogen, helium, and a minimal amount of lithium. Heavier elements, such as iron, were formed within stars. Yet, one of astrophysics’ greatest enigmas is how the first elements heavier than iron, like gold, were created and dispersed throughout the cosmos. A recent study by astronomers at Columbia University and other institutions suggests that a single flare from a magnetar could generate 27 equivalent masses of these elements simultaneously.

Impressions of Magnetar artists. Image credit: NASA’s Goddard Space Flight Center/S. Wesinger.

For decades, astronomers have theorized about the origins of some of nature’s heaviest elements, like gold, uranium, and platinum.

However, a fresh examination of older archival data indicates that up to 10% of these heavy elements in the Milky Way may originate from the emissions of highly magnetized neutron stars, known as magnetars.

“Until recently, astronomers largely overlooked the role that magnetars, the remnants of supernovae, might play in the formation of early galaxies,” remarked Todd Thompson, a professor at Ohio State University.

“Neutron stars are incredibly unique, dense objects known for their large size and strong magnetic fields. They are similar to black holes but not quite the same.”

The origin of heavy elements has long been a mystery, but scientists have understood that these elements can only form under specific conditions through a process known as the R process (or rapid neutron capture process).

This process was observed in 2017 when astronomers detected a collision between two super-dense neutron stars.

This event was captured using NASA telescopes and the LIGO gravitational wave observatory, providing the first direct evidence that heavy metals can be produced by celestial phenomena.

However, subsequent evidence suggests that neutron star collisions may not form heavy elements swiftly in the early universe, indicating that additional mechanisms might be necessary to account for all these elements.

Based on these insights, Professor Thompson and his colleagues realized that powerful magnetar flares could act as significant ejectors of heavy elements. This conclusion was validated by the observation of the SGR 1806-20 magnetar flare that occurred 20 years ago.

By analyzing this flare event, the researchers found that the radioactive decay of the newly formed elements aligns with theoretical predictions concerning the timing and energy released by magnetar flares after ejecting heavy R-process elements.

“This is the second time we’ve observed direct evidence of where these elements are produced, first linked to neutron star mergers,” stated Professor Brian Metzger from Columbia University.

“This marks a significant advancement in our understanding of heavy element production.”

“We are based at Columbia University,” mentioned Anildo Patel, a doctoral candidate at the institution.

The researchers also theorized that magnetar flares generate heavy cosmic rays and very fast particles, the origins of which remain unclear.

“I am always excited by new ideas about how systems and discoveries in space operate,” said Professor Thompson.

“That’s why seeing results like this is so thrilling.”

The team’s paper was published in The Astrophysical Journal Letters.

____

Anirudh Patel et al. 2025. Direct evidence for R-process nuclear synthesis in delayed MeV radiation from SGR 1806-20 magnetar giant flares. ApJL 984, L29; doi: 10.3847/2041-8213/ADC9B0

Source: www.sci.news

Key Elements of Dark Chocolate Might Promote Healthy Aging

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                    <p class="ArticleImageCaption__Title">Dark chocolate is a notable source of theobromine, a beneficial chemical</p>
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        </figure>
    </p>
    <p>While chocolate may be associated with anti-aging benefits, it’s wise to be cautious before indulging. The beneficial compounds are predominantly found in dark chocolate, and the overall health impact of chocolate consumption remains uncertain.</p>
    <p>"There are numerous aspects of dark chocolate, each with its pros and cons," says <a href="https://profiles.ucl.ac.uk/90100-ramy-saad/publications">Rumy Sars</a> from University College London.</p>

    <p>The substance in question, theobromine, is famously known to be toxic to dogs. However, that's just one aspect...</p>
</div>

Feel free to modify any specific terms or phrases further!

Source: www.newscientist.com

Studies suggest that stars break down into neutrons and combine to create heavy elements

High-energy photons produced deep within gamma-ray burst jets emerge from decayed stars can dissolve the outer stellar layer into free neutrons, causing a series of physical processes that lead to the formation of heavy elements. paper It is published on Astrophysical Journal.

The high-energy photonic jet (white and blue) passes through a collapse with a black hole at its center. The red space around the jet represents a coco where free neutrons can be captured and caused the R process. Image credit: Los Alamos National Laboratory.

The formation of the heaviest elements relies on astrophysical environments with large amounts of neutrons.

Neutrons are found in the medium under extreme pressure, either bound to the nucleus.

Free neutrons are rare because they have a half-life of less than 15 minutes.

“The creation of heavy elements such as uranium and plutonium requires extreme conditions,” says Dr. Matthew Mumpoir, a physicist at the Los Alamos National Laboratory.

“There are several viable yet rare scenarios in the universe where these elements can form, and all such locations require a large number of neutrons. We propose a new phenomenon where these neutrons are not present and dynamically generated by stars.”

The key to generating the heaviest elements in the periodic table is known as the rapid neutron capture process or R process, and is believed to be responsible for the production of all thorium, uranium and plutonium that occur naturally in the universe.

The team’s framework takes on the challenging physics of the R process and solves them by proposing reactions and processes around the collapse of the stars.

In addition to understanding the formation of heavy elements, the proposed framework will help address key issues regarding neutron transport, multi-objective simulations, and observation of rare events. All of these are interesting for national security applications, which can gather insights from research.

In the scenario proposed by researchers, when nuclear fuel is exhausted, a large star begins to die.

It is no longer able to push its own gravity up, and a black hole forms in the center of the star.

If the black hole is spinning fast enough, the framedrazing effect from the very powerful gravity near the black hole will wind up the magnetic field and fire a powerful jet.

Subsequent reactions create a wide range of photons, some of which are high-energy.

“The jet blows stars before it, creating a hot coco of material around the jet, like a freight train plowing through the snow,” said Dr. Mumpower.

At the interface of jets with star materials, high-energy photons (i.e. light) can interact with the nucleus and convert protons into neutrons.

Existing nuclei can also be dissolved in individual nuclei, creating more free neutrons to power the R process.

Team calculations suggest that interactions with light can create neutrons very quickly in nanosecond order.

For charging, a strong magnetic field traps the protons in the jet.

The merciless neutrons are ploughed from the jet to the coco.

After experiencing relativistic shock, neutrons are very dense compared to the surrounding star material, which can lead to the R process, forging heavy elements and isotopes, and banished into space when the stars are torn apart.

The process of protons converted into neutrons and the free neutrons that escape to the surrounding coco to form heavy elements, encompasses all four basic forces of nature, accompanied by a wide range of physics principles. It combines the real multiword problems, the fields of nuclear and nuclear physics, with fluid mechanics and general relationships.

Despite the team’s efforts, more challenges remain as the heavy isotopes created during the R process have never been done on Earth.

Researchers know little about their properties, including atomic weights, half-life, and more.

The high energy jet framework proposed by the team may help explain the origin of kilonovas (the glow of optical and infrared electromagnetic radiation) associated with long gamma-ray bursts.

“Star melting via high-energy photon jets provides an alternative origin for gravity and the production of kilonova that can be produced. This may not have previously been thought to be related to star collapse,” the scientist said.

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Matthew R. Mumpoir et al. 2025. Make sure there are neutrons! Hadronic optical production from large fluxes of high energy photons. APJ 982, 81; doi:10.3847/1538-4357/ADB1E3

Source: www.sci.news

Earth and Mars’ foundational materials were initially abundant in moderately volatile elements.

A new analysis of the metstones of magmatic iron challenges traditional theories about why Earth and Mars are depleted with moderately volatile elements.



Bendego met stone. Image credit: Jorge Andrade / CC by 2.0.

Medium volatile elements (MVEs) such as copper and zinc play an important role in planetary chemistry with essential elements of life, such as water, carbon, and nitrogen.

Understanding its origins provides important clues as to why the Earth has become a habitable world.

Earth and Mars contain significantly fewer MVEs than primitive metstones (chondrites), raising basic questions about the planetary layer.

This new study employs a new approach by analyzing iron meteorites (the metal core remnants of the earliest planetary building blocks) to reveal new insights.

“We’ve seen a lot of experience in the world,” said Dr. Damanveer Grewal, a researcher at Arizona State University.

“This discovery reconstructs our understanding of how the planet acquired its components.”

Until now, scientists believed that MVE was lost because they were not completely condensed in the early solar system or escaped during planetary differentiation.

However, new research reveals a different story. It is held by many MVEs on the first planet, suggesting that the building blocks of Earth and Mars later lost theirs.

Surprisingly, the authors discovered that many inner solar system planets retain abundance of MVEs like chondrites, and accretion continues despite being differentiated. It indicates that it has been saved.

This was not because Earth and Mars ancestors began to deplete with these elements, but instead occurred in the long history of collision growth, rather than incomplete condensation of solar nebulae or planet differentiation. Suggests that.

“Our work redefines how we understand the chemical evolution of planets,” Dr. Grewal said.

“It shows that the components of Earth and Mars were originally rich in these vital elements, but the intense collisions during the planet’s growth caused depletion.”

study Published in the journal Advances in Science.

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Damanveer S. Grewal et al. 2025. Enrichment of moderate volatile elements in first-generation planets of the inner solar system. Advances in Science 11 (6); doi:10.1126/sciadv.adq7848

Source: www.sci.news

Adam Buxton’s Podcast: A True Crime Story Combining Elements of ‘Serial’ and ‘Twin Peaks’

This week’s picks

in the smoke
Wide range of weekly episodes available

Adam Buxton’s new podcast is being billed as Serial meets Twin Peaks, bridging the gap between fiction and true crime. May Mac is Kay McAllister, a former tabloid journalist who launches her own pod to find out what happened to a missing man. Buxton plays a modest role as DCI Roy Burgess, who worked on the case. Although told in a true-crime style, there is no doubt that this is glossy, high-quality fiction, and is an engaging, slow-burning tale. Hannah Verdier

The Burden: Avenger
Wide range of weekly episodes available
When Miriam Lewin was 19 years old, she was kidnapped from the streets of Buenos Aires and tortured for her political beliefs. However, she survived, became a journalist, and continued to bring her perpetrators to justice. The Handmaid’s Tale’s Alexis Bledel tells Lewin’s powerful story based on in-depth interviews. HV

Julia Louis-Dreyfus in “You Hurt My Feelings.” Photo: Jung Park/AP

The Madman’s Hotel
Audible, all episodes now available
Niall Breslin grew up in the shadow of an Irish “mental hospital” and has been haunted by it ever since. But when he meets Julie Clark, whose great-grandmother was imprisoned at St. Roman’s Hospital until her death, he uncovers a story of abuse even more horrifying than he could have imagined. HV

my so-called middle age
Wide range of weekly episodes available
“You’ve read All For, right?” Reshma Saujani asks as she introduces the podcast. “Where’s my hotel room?” Even if that didn’t convince her target audience, her first guest wisdom would agree. Julia Louis-Dreyfus (above) is as stunning as ever, opening up about the ups and downs of midlife, including the joy of posing naked for Rolling Stone. HV

super sensual
Apple Podcasts, full episodes available to Apple TV+ subscribers on Mondays
If you were glued to last year’s Ghost Story, here’s a winding investigation into a creepy old family secret. This time I have a question about reincarnation. Will Sharp spoke to a woman who was involved with two girls who were hit and killed by a car on their way to church in the 1950s. However, the father says he will be reborn, and his wife gives birth to twin girls… Holly Richardson

There’s a podcast for that

Kirat Assi in the Netflix documentary series Sweet Bobby. Photo: Provided by Netflix

this week, Ammar Kalia We choose the 5 best podcasts shocking developmentfrom unsolved murders to traumatic stories of catfishing.

Source: www.theguardian.com

Webb discovers unseen elements of Messier 106

NASA has released a stunning new image of the active center of nearby spiral galaxy Messier 106, taken with the NASA/ESA/CSA James Webb Space Telescope.



This Webb image shows Messier 106, a spiral galaxy 20 million light-years away in the constellation Canes Venatici. Image courtesy of NASA / ESA / CSA / Webb / J. Glenn.

Located more than 20 million light years from Earth in the small northern constellation Canes Venatici, Messier 106 is one of the brightest spiral galaxies and closest to our Milky Way Galaxy.

Also known as M106 or NGC 4258, the galaxy was discovered in 1781 by Charles Messier's observational assistant, Pierre Méchain.

“Despite its name, Messier 106 was neither discovered nor catalogued by the famous 18th century astronomer Charles Messier,” astronomers Webb said in a statement.

“This galaxy was discovered by his assistant Pierre Méchain, but was not catalogued during his lifetime.”

“Messier 106, along with six other objects they discovered but did not record, Messier Catalogue In the 20th century.”

Messier 106 is similar in size and brightness to our galactic neighbor, the Andromeda Galaxy.

Messier 106 measures more than 130,000 light-years from end to end, but because of its great distance from the Milky Way galaxy, it appears very small from Earth's perspective.

At the center of Messier 106 lies an extremely active supermassive black hole with a mass about 40 million times that of the Sun.

Unlike the black hole at the center of our Milky Way galaxy, which only occasionally sucks in gas particles, Messier 106's black hole is actively consuming material.

“As the gas spirals toward Messier 106's black hole, it heats up and emits powerful radiation,” the astronomers said.

New images of Messier 106 Webb's near infrared camera (NIRCam).

“The observations were made as part of a dedicated program to study active galactic nuclei – luminous central regions of galaxies dominated by light emitted by dust and gas falling into a black hole,” the researchers said.

“The blue areas in this image reflect the distribution of stars throughout the central region of the galaxy.”

“Orange areas indicate warmer dust, while more intense reds represent cooler dust.”

“The blue-green, green and yellow tones near the center of the image represent the various gas distributions across the region.”

Messier 106 also has a notable feature: it has two “unusual” extra arms that are visible in radio and x-ray wavelengths, rather than visible light.

“Unlike normal arms, these are made up of hot gas rather than stars,” the scientists said.

“Astronomers think these extra arms are the result of black hole activity, a feedback effect that has been seen in other galaxies.”

“These could be caused by outflows of material produced by the violent churning of gas around the black hole, creating a phenomenon similar to waves rushing out of the ocean when they hit rocks near the shore.”

Source: www.sci.news

Neutron stars merging form heavy elements, scientists find

Since the 1920s, Edwin Hubble Ever since it was discovered that the universe is expanding, astrophysicists have been asking themselves the question, “Where does matter come from?” In the Big Bang theory, a possible explanation, not a TV show, astrophysicists propose that the universe began with an explosion, a single hot, dense point expanding, then cooling down to transform from pure energy into solid matter. But that origin story ends with the two smallest elements: hydrogen and helium. Not everything in the universe is made of these two elements, leaving scientists with a new question: “Where does other matter come from?”

The emergence of nuclear physics in the early 20th century gave astronomers their first big clue. Researchers studying stars noted that stars are very bright and require a large source of energy to produce that much light. Nuclear physicists, including Albert Einstein and his famous E = mc2 The equations showed that one of the most powerful sources of energy in the universe is the smashing of smaller atoms together to create larger ones – nuclear fusion. And that's exactly what stars do in the hot, dense regions at their centers, called “nuclear fusion.” coreBut there's a limit to this process in stars — specifically, iron, which is the 26th of the 92 naturally occurring elements. Stars create energy by colliding elements with each other, but elements bigger than iron need to generate more energy than they can give off, which is why elements heavier than iron, like gold and uranium, remain unexplained.

Researchers have discovered the next clue in a massive, bright stellar explosion in the night sky. SupernovaIt turns out that massive stars, more than 10 times the size of the Sun, burn up their accumulated elements to fuse rapidly. These stars not only shine, but also run out of energy to hold themselves together, exploding and scattering their outer layers of elements in all directions. This is a supernova explosion. For decades, astrophysicists thought that heavy elements were created from a chaotic mixture of light elements and free energy. However, careful observation of supernovae has shown that the amount of heavy elements produced in the explosion is less than what is needed to explain the abundance of heavy elements in the universe.

Astrophysicists got the final clue in 2017 when the Laser Interferometer Gravitational-Wave Observatory detected the first binary neutron star (BNS) merger. RaigoThe final stage in the life cycle of a massive star, between 10 and 25 times the mass of the Sun, is Neutron StarDuring this stage, the star's core collapses, and the electrons and protons in atoms get so close together that they fuse into neutrons. Two neutron stars orbiting each other collide, scattering debris into the surrounding galaxy. Researchers propose that this phenomenon could provide the energy and matter needed to fuse heavy elements into the heaviest naturally occurring elements.

Researchers from Peking University and Guangxi University wanted to test whether BNS mergers could produce elements heavier than iron. Because the event is extremely rare, occurring only a few dozen times per year across our galaxy, they couldn't just point their telescopes into space and hope for luck. Instead, they used advanced nuclear physics software to simulate a BNS merger.

The researchers gave their simulations specific initial conditions, such as what atoms were present in the stars when the collision began, the rates of nuclear reactions and decay, the number of electrons mixing, and the sizes of the colliding neutron stars. They then mathematically described how temperature, volume, and pressure relate to matter. Equation of stateIt simulates the effects of the collision and calculates what elements would be formed and released into space.

The team found that these BNS mergers could produce huge amounts of very heavy elements, between 300 and 30,000 times the mass of the Sun, which is 10 to 1,000 times the amount produced by supernovae. The team believes that this result could explain the abundance of heavy elements observed in the Galaxy in relation to other cosmic effects, e.g. Galactic WindHowever, the researchers acknowledged that their findings cannot explain the abundance of all heavy elements, especially those at the lower end of the atomic mass range they studied. They explained that these elements are probably still being created in the cores of collapsing stars, but suggested that future researchers should further test this hypothesis.


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Source: sciworthy.com

The process of how ancient stars produced elements unattainable by Earth

Researchers have discovered that ancient stars can produce elements with atomic masses of more than 260, heavier than those found naturally on Earth. This discovery improves our understanding of element formation in stars, particularly through the rapid neutron capture processes (r-processes) that occur in neutron stars. . Credit: SciTechDaily.com

A new study reveals that ancient stars can produce elements heavier than Earth, with atomic masses of more than 260, advancing our understanding of cosmic element formation.

How much do elements weigh? An international team of researchers has found that ancient stars had the ability to produce elements with an atomic mass of more than 260, heavier than any element on the periodic table that occurs naturally on Earth. I discovered that. This discovery deepens our understanding of element formation in stars.

space element factory

We are literally made of star stuff. Stars are elemental factories, where elements are constantly merging or breaking down to create other lighter or heavier elements. When we refer to light or heavy elements, we are talking about their atomic mass. Roughly speaking, atomic mass is based on the number of protons and neutrons in the nucleus. atom of its elements.

The heaviest elements are only known to be produced in neutron stars by rapid neutron capture processes, or r processes. Imagine a single atomic nucleus floating in a soup of neutrons. Suddenly, a bunch of these neutrons attach themselves to the nucleus in a very short time (usually less than a second), causing a change from neutrons to protons inside, and voila! Heavy elements such as gold, platinum, and uranium are formed.

Instability of heavy elements

The heaviest elements are unstable or radioactive and decay over time. One way to do this is through a split called fission.

“If you want to make heavier elements, such as lead or bismuth, you need the R process,” says Ian Roederer, associate professor of physics. north carolina state university and lead author of the study. Mr. Roederer previously attended the University of Michigan.

“We need to add a lot of neutrons very quickly, and the problem is that we need a lot of energy and a lot of neutrons to do that,” Roederer says. “And the best place to find both is at the moment of a person’s birth or death. neutron staror when neutron stars collide and the raw materials for the process are produced.

“We have a general understanding of how the r process works, but the conditions of the process are very extreme,” Roederer says. “We don’t really know how many different sites in the universe generate r-processes, and we don’t know how r-processes end. We also don’t know how many neutrons there are Can you add more? Or how heavy can the elements be? So we looked at the elements produced by nuclear fission in well-studied old stars to find out how heavy these elements are. We decided to see if we could answer some of the questions.”

Identify previously unrecognized patterns

The research team newly investigated the abundance of heavy elements in 42 well-studied stars. milky way. These stars were known to contain heavy elements formed by the r process in earlier generations of stars. By looking more broadly at the amounts of each heavy element found in these stars, rather than individually, as is more common, they identified previously unrecognized patterns.

These patterns indicated that some elements listed near the middle of the periodic table, such as silver and rhodium, were likely remnants of nuclear fission of heavy elements. The research team was able to confirm that the r process can produce atoms with an atomic mass of at least 260 before fission.

“That 260 is interesting because, even in nuclear weapons tests, nothing that heavy has ever been detected in space or in nature on Earth,” Roederer said. “But observing them in space gives us guidance on how to think about models and fission. It also gives us insight into how the rich diversity of elements came about.” may be given.”

For more information on this research, see ‘Incredibly profound’ evidence for nuclear fission throughout the universe.’

Reference: “Elemental abundance patterns in stars show splitting of nuclei heavier than uranium” Ian U. Roederer, Nicole Vassh, Erika M. Holmbeck, Matthew R. Mumpower, Rebecca Surman, John J. Cowan, Timothy C. Beers, Rana Ezzeddine, Anna Froebel, Therese T. Hansen, Vinicius M. Placko, Charlie M. Sakari, December 7, 2023. science.
DOI: 10.1126/science.adf1341

The research was published in the journal Science and was supported in part by the National Science Foundation and the National Aeronautics and Space Administration.

Source: scitechdaily.com