Revolutionary Fully 3D Printed Microscope Set to Make Waves in 2025

3D Printed Microscope

Dr. Liam M. Rooney/University of Strathclyde

In early 2025, excitement surged within the research community with the release of a groundbreaking preprint paper detailing the world’s first fully 3D printed microscope. This innovative device was constructed in just hours and costs a fraction of traditional models.

Dr. Liam Rooney, a professor at the University of Glasgow, explained to New Scientist that the response to their revolutionary microscope has been overwhelming, attracting interest from biomedical researchers, community organizations, and even filmmakers. He stated, “The community response has been remarkable.” This significant research has been published in the Microscope Journal.

For the microscope’s body, the team employed designs from the Open Flexure project, a public resource for 3D printing scientific instruments. Utilizing a commercial camera and light source, they controlled the entire system using a Raspberry Pi computer.

The true innovation lies in the 3D-printed microscope lenses made from clear plastic, drastically reducing costs and enhancing accessibility. Traditional microscopes can cost thousands; in contrast, this new model can be assembled for less than £50.

“Since January, we have printed approximately 1,000 lenses in various shapes,” remarked team member Gail McConnell, from the University of Strathclyde.

Several companies producing commercial products that require optics have reached out to discuss potential collaborations, as affordable, lightweight 3D-printed lenses are still uncommon in large-scale production. The team has successfully used the microscope to analyze blood samples and tissue sections from mouse kidneys, validating its utility for medical and biological research.

The researchers aim to democratize access to microscopy, and they are making strides toward that goal. Collaboration with a lab at the Kwame Nkrumah University of Science and Technology in Ghana is underway to enhance microscope accessibility for researchers and students across West Africa. Additionally, they’ve secured funding from the UK Institute for Technology Strategy, and are involved in programs designed to upskill and empower students facing educational barriers.

Furthermore, the team has developed a new microscope course through the Strathclyde Light Microscopy Course, aimed at researchers of all experience levels and providing a unique educational opportunity in the UK. Rooney noted, “This is revolutionizing our teaching methods.”

Looking towards the future, there is substantial potential for further enhancements in 3D printed microscopes. The research team is working to improve resolution without raising costs and have found methods to enhance image contrast by 67%.

McConnell emphasized that the microscope’s design leverages consumer electronics and accessible 3D printing technologies, stating that the future advancements and capabilities are limited only by current 3D printing technology. “As these printers advance, so will our capabilities. The only bottleneck is technology, not creativity,” she explained. “We’re frequently contacted by individuals eager to see new designs.”

Source: www.newscientist.com

Gravitational Waves Confirm Stephen Hawking’s Black Hole Theory

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Illustration of two black holes merging and emitting gravitational waves throughout the universe

Maggie Chiang from the Simons Foundation

Stephen Hawking’s theorem, established over 50 years ago, has aided astronomers in detecting waves produced by extraordinarily powerful collisions as they traverse Earth at light speed, shedding light on the merging of black holes thanks to significant advancements in gravitational wave astronomy.

In 1971, Hawking introduced the Black Hole Area theorem, which posits that when two black holes combine, the resultant event horizon cannot be smaller than the combined size of the original black holes. This theorem aligns with the second law of thermodynamics, which asserts that the entropy of a system cannot decrease.

The merging of black holes warps the structure of the universe, generating tiny ripples in space-time known as gravitational waves that move through the cosmos at the speed of light. Five gravitational wave observatories on Earth search for waves that are 10,000 times smaller than an atom. These include two detectors in the US—LIGO, a laser interferometer, alongside Italy’s Virgo, Japan’s Kagura, and Germany’s GEO600.

The recent event, named GW250114, mirrors the event that first detected gravitational waves in 2015.

Now, the upgraded LIGO detector is three times more sensitive than it was in 2015, enabling the capture of waves from collisions with remarkable detail. This has allowed scientists to confirm Hawking’s theorem, proving that the size of the event horizon actually increases following a merger.

When black holes collide, they generate gravitational waves with overtones akin to the sound of a ringing bell, as noted by Laura Nuttall, a member of the LVK team at the University of Portsmouth, UK. Previously, these overtones were too rapid to be detected clearly enough to assess the area of the event horizon before and after a merger, a crucial requirement to test Hawking’s theory. The initial 2021 study supporting the theory confirmed it at a 95% confidence level, but the latest findings suggest an impressive 99.999% confidence.

Over the past ten years, scientists have witnessed approximately 300 black hole collisions while observing gravitational waves. However, none have been as strong as GW250114, which was twice as powerful as any previously detected gravitational wave.

“What we are discovering in our data has tremendous implications for understanding basic physics,” remarked a researcher. “We’re eager for nature to provide us with further astonishing revelations.”

Only LIGO was operational when GW250114’s waves reached Earth; other detectors in the LVK collaboration were not active. This did not affect the validation of Hawking’s theory but limited researchers’ ability to pinpoint the waves’ origins more precisely.

Future upgrades to LIGO and upcoming observatories are anticipated to enhance sensitivity, offering deeper insights into black hole physics, according to Ian Harry, also from the University of Portsmouth and part of the LVK team. “We may miss some events, but we will certainly capture similar phenomena again,” Harry expressed. “Perhaps with our next set of upgrades in 2028, we might witness something of this magnitude and gain deeper insights.”

These findings pave the way for future research into quantum gravity, a field where physicists aim to reconcile general relativity with quantum mechanics. Nuttall stated that the latest results indicate that both theories remain compatible, although inconsistencies are expected in future observations.

“At some point, discrepancies are likely to emerge, especially when close signals appear noisy as the detector’s sensitivity improves,” Nuttall explained.

Moreover, the recent data from LVK enabled scientists to confirm equations proposed by mathematician Leakir in the 1960s, which suggested that black holes could be described by two key metrics: mass and spin. Essentially, two black holes with identical mass and spin are mathematically indistinguishable. Observations from GW250114 have verified this assertion.

Physical Review Letters
doi: 10.1103/kw5g-d732

The Mystery of the Universe: Cheshire, England

Join a weekend with leading scientific minds. Unravel the mysteries of the universe in an engaging program that features a visit to the iconic Lovell telescope.

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Source: www.newscientist.com

Heat Waves May Accelerate Aging Process

Air conditioners may help prevent heatwaves from accelerating aging

Sajjad Hussain/AFP via Getty Images

The intensity of heat waves can lead to significant long-term health impacts. Prolonged exposure to high temperatures seems to speed up biological aging in individuals.

“Currently, there are two major studies that highlight the effects of heatwave exposure on aging, focusing on different populations in various countries,” says Paul Beggs from Macquarie University in Australia. “It’s crucial to take heat waves seriously, as we are not only safeguarding our health but also the well-being of those around us.”

Recent findings from Siyi Chen at the University of Hong Kong and her research team reveal important insights. They analyzed medical screening data from around 25,000 adults in Taiwan to determine biological age based on several health indicators, including inflammation, blood pressure, and organ function. This data was then compared with time series data to assess aging rates.

“Physiological changes associated with aging can appear earlier and progress more rapidly in certain individuals,” notes Beggs, who wasn’t part of this research.

The researchers calculated each participant’s cumulative heat wave exposure over two years preceding the medical screening, assessing not just the frequency of heat waves but also the intensity of temperatures experienced. It turned out that the number of heatwave days was a critical factor in the accelerated aging observed in Taiwan’s population. These findings align with another recent study investigating outdoor temperature effects on aging in older adults in the US.

In the Taiwanese population studied, greater aging effects correlated with increased cumulative exposure to heat waves. Specifically, a four-day rise in total heatwave duration linked to an increase in biological age by as much as nine days.

The impact was particularly severe for specific demographics. For instance, manual laborers experienced aging effects that were threefold greater from equivalent heat exposure compared to the broader group. Additionally, residents in rural areas showed more pronounced aging effects, suggesting that access to air conditioning could mitigate the aging repercussions of heat exposure.

Nonetheless, to effectively combat climate change and the escalating frequency of heatwaves, the advantages of air conditioning must be balanced with more sustainable cooling alternatives, warns Beggs. “Air conditioners release heat into the environment, further worsening conditions for individuals lacking such systems,” he states.

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Source: www.newscientist.com

Junho Observes Unusual Plasma Waves in Jupiter’s Aurora

Planetary researchers, utilizing data from NASA’s Juno spacecraft, have identified a novel type of plasma wave in the Aurora Zone above Jupiter’s North Pole.

This image merges observations from the NASA/ESA Hubble Space Telescope with optical images and ultraviolet observations of Jovian Aurora. Image credit: NASA/ESA.

“While the NASA/ESA/CSA James Webb Space Telescope has supplied some infrared images of the Aurora, Juno is unique as the first spacecraft to take a polar orbit around Jupiter,” stated Dr. Ali Suleiman from the University of Minnesota.

“The regions surrounding a magnetized planet like Jupiter are filled with plasma, a superheated state where atoms dissociate into electrons and ions.”

“These particles are propelled towards the planet’s atmosphere, causing the gas to illuminate as auroras.”

“On Earth, this phenomenon manifests as the recognizable green and blue lights.”

“However, Jupiter’s auroras are generally not visible to the naked eye and require UV and infrared instruments for observation.”

The research team discovered that the polar plasma density on Jupiter is so low, in combination with its strong magnetic field, that the plasma waves exhibit very low frequencies, unlike those observed around Earth.

“Plasma behaves like a liquid but is influenced by both its own magnetic field and external fields,” remarked Professor Robert Rysack from the University of Minnesota.

“Our study also sheds light on how particles inundate the polar regions, in contrast to Earth, where Jupiter’s intricate magnetic fields give rise to auroras arranged in a donut-like pattern around the poles.”

“As Juno advances its mission to further investigate this new phenomenon, we aim to collect additional data.”

The team’s findings were published in the journal on July 16th, 2025, in Physical Review Letters.

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R. Lysak et al. 2025. A new plasma regime in Jupiter’s Aurora Zone. Phys. Rev. Lett. 135, 035201; doi:10.1103/fn63-qmb7

Source: www.sci.news

When Radio Waves Illuminate Our Minds, We Experience Smell.

Preserving a keen sense of smell has multiple benefits, notably for our ability to taste.

DeanDrobot/Getty Images

Directly applying strong radio waves to an individual’s head appears to enhance the sense of smell, at least for a limited time.

Aging, trauma, and certain neurological disorders can impact the olfactory nerves, potentially diminishing the ability to smell. Many individuals have reported a reduced sense of smell following Covid-19, which can adversely affect personal preferences and may pose safety risks, such as an inability to detect gas leaks.

“Current medical practices may include surgical interventions for severe olfactory dysfunction, but more typical cases rely on chemical treatments, such as repeated exposure to scents at home,” explains Yong Woo-chan from Gang Line University in Seoul. “While treatments in other medical fields have advanced significantly, olfactory treatment has remained relatively traditional. To address this gap, we proposed the idea of electrical testing through bioelectronic stimulation as a therapeutic option.”

Chang and his team aimed to stimulate the olfactory system directly; however, due to its location deep within the head, they opted for radio wave stimulation instead.

The researchers initially engaged 28 participants without any odor issues. The participants were exposed to 15 watts of power for 5 minutes, emitted from a 5 cm square antenna positioned 10 cm from their heads. “The stimulus itself is not consciously felt by the patient,” states Chan. “However, with prolonged exposure, some might notice a slight warming sensation at the stimulation site.”

The olfactory sensitivity was assessed using standard tests like the Sniffin’ Sticks odor threshold test. This involved participants working to identify the presence of alcohol N-butanol produced from fermented sugar at varying dilutions.

Following the radiofrequency treatment, researchers observed that participants demonstrated significantly improved olfactory function, with these enhancements lasting approximately a week. Individuals with olfactory challenges may require additional treatments, according to Chan.

The research team is currently preparing studies involving individuals with smell disorders. The device has been refined to deliver more intense stimulation, which could potentially lead to even greater improvements, according to Jang.

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Source: www.newscientist.com

Ibogaine: A Psychedelic Drug That May Alleviate PTSD by Slowing Brain Waves

Ibogain, a psychedelic substance, is derived from the roots of the Iboga plant

Farmer Dods / Alamy

The psychedelic substance ibogaine has been shown to slow brain wave activity in individuals with traumatic brain injuries, potentially accounting for its effectiveness in treating symptoms of post-traumatic stress disorder (PTSD).

A study conducted last year revealed that ibogaine, sourced from the African Iboga plant, significantly enhanced the overall mental and physical well-being of military veterans suffering from traumatic brain injuries. Yet, the precise mechanisms behind these effects were previously unknown.

To investigate further, Jennifer Lismore from Stanford University and her team examined brain imaging of 30 individuals involved in the initial study. During a 5-day treatment session at a facility in Mexico, participants received a dosage of 12 milligrams of ibogaine per kilogram of body weight and participated in supportive activities like yoga, meditation, and therapy.

As part of the study, the researchers collected EEG data that recorded participants’ brain electrical activity. These scans were taken 2-3 days prior to and 3.5 days following the ibogaine treatment.

By comparing the EEG findings, Lismore and her team observed an overall deceleration in brain wave activity post-treatment, particularly in the gamma waves—the fastest brain waves—which exhibited nearly a 16% reduction in strength in the occipital region after ibogaine therapy. While gamma wave intensity saw a slight rebound after one month, levels remained significantly below those recorded prior to treatment.

Additionally, the intensity of slow theta waves rose by approximately 17% in the back of the brain and 13% at the front 3.5 days post-treatment. However, this increase lost its significance after one month.

Lismore suggests that the observed reduction in brain wave activity may clarify why ibogaine is effective for alleviating PTSD symptoms in many patients. “The deceleration of brain function has allowed patients, particularly those experiencing hyperawareness and sensitivity associated with PTSD, to find relief,” she noted. “One way to understand this slowing process is as a mitigation of the heightened distress often seen in PTSD cases.”

The temporary spike in slow theta waves could also indicate that ibogaine promotes neuroplasticity—the brain’s ability to adapt and rewire itself. Previous studies in animals have associated theta wave activity with brain adaptability, Lismore explains. By inducing a short-term increase in theta wave presence, ibogaine may create conditions conducive to improving mental health.

“Ibogaine essentially addresses the chaotic, restless nature of the brain, facilitating a sort of normalization,” remarked Conor Murray from the University of California, Los Angeles. “Ultimately, it instills a sense of security for participants, reassuring the brain.”

However, he cautions that these findings don’t fully reveal the mechanisms through which ibogaine effects these brain changes.

Another challenge is the absence of control measures, complicating the assessment of the influence from other treatment components, points out Lismore. Nonetheless, she asserts that these insights represent “a significant first step toward understanding why this treatment is so impactful.”

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Source: www.newscientist.com

Unprecedented Ocean Heat Waves Could Signal Lasting Changes in Our Seas

Warming oceans might elevate storm intensity, exemplified by Hurricane Milton in 2024

NOAA

Scientists have cautioned that the extreme ocean temperatures observed since 2023 could indicate the onset of drastic changes in global marine conditions, posing a severe risk to life on our planet.

Historic ocean heat waves unfolded in the North Atlantic and Pacific in 2023, marked by their unprecedented severity, duration, and geographical spread, many persisting for over a year.

These heat waves have led to record-high sea surface temperatures globally in 2023 and 2024, contributing to severe weather patterns on land and resulting in back-to-back years being declared the hottest on record.

“While there’s been a gradual increase in ocean temperatures over the past 40-50 years, 2023 stands out as a pivotal year, with significant ocean heat waves impacting numerous regions,” stated Matthew England from the University of New South Wales, Australia.

Sea surface temperatures worldwide remain at alarming heights, with the Mediterranean currently experiencing marine heat waves, as water temperatures exceed 5°C (9°F) during this time.


Researchers are concerned that the oceans may be shifting to new, hotter states, endangering their predictions for both short-term weather phenomena like hurricanes and long-term climate change trends.

To understand the situation, Zhenzhong Zeng from China’s Southern University of Science and Technology is collaborating with colleagues to pinpoint the causes of the 2023 global ocean heat wave by analyzing heat movement within the ocean, wind patterns, and ocean currents. They found that reduced cloud cover significantly increases solar radiation reaching the water, compounded by weak winds and the influence of the warming El Niño pattern in the Pacific Ocean.

Considering the heat wave that began in earnest in 2023 and continues in various regions, Zeng suggests this could be the start of a “new normal” for the world’s oceans. He notes that new data reveals an exponential rise in ocean heat, contradicting previous climate model forecasts.

Persistently elevated water temperatures severely impact marine ecosystems, heightening the risk of coral reef collapse, causing mass die-offs, and leading to shifts in marine species distributions. This also exacerbates heating on land, resulting in intensified droughts, heatwaves, wildfires, and storms.

Zeng expressed that he is “very alarmed” by this potential sea regime change, adding, “I believe nearly all predictions made by Earth System models are incorrect.”

Conversely, some experts argue that it may be premature to declare fundamental shifts in ocean dynamics. Neil Holbrook from the University of Tasmania in Australia points out that there is currently no “clear evidence” to indicate we have reached a critical turning point, given the limited years of data to assess. “I cannot predict what will happen next year; [ocean temperatures] could return to more typical patterns,” he remarked.

However, Holbrook stressed that without substantial reductions in greenhouse gas emissions, “marine heat waves will likely continue to gain intensity and duration, potentially escalating faster than various marine species can adapt.”

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Source: www.newscientist.com

Improved Air Quality Linked to Rise in Urban Heat Waves

Heatwaves are increasing in frequency as global smog diminishes

Claudio Reyes/AFP via Getty Images

As the world works to eliminate harmful aerosol pollution, heatwaves are becoming more common, exposing the intensifying effects of greenhouse gases in the atmosphere. This warming trend is particularly pronounced in densely populated areas where air pollution typically rises.

“Mitigating aerosol pollution is imperative for public health,” states Geeta Persad from the University of Texas at Austin. “However, we must acknowledge that this reveals specific risks that become magnified in populated regions.”

Aerosol pollution, primarily stemming from fossil fuel combustion, has effects that generally counteract those of greenhouse gases. While gases like carbon dioxide trap heat, aerosols tend to cool the atmosphere by reflecting sunlight either directly or by altering cloud behavior. Some estimates suggest that aerosol pollution masks half of the global warming effect of greenhouse gases.

This interplay means that cleaning up air pollution can inadvertently amplify climate warming effects. However, the specific ways in which aerosol variations impact heat in populous regions have remained unclear until now.

To analyze this more precisely, Persad and her team utilized climate models to evaluate how aerosol levels influence the occurrence of land heatwaves, examining both historical data and future projections. They defined a heatwave as three consecutive days where temperatures would rank among the hottest 10% for that time of year in a pre-industrial context.

Throughout most of the 20th century, the team discovered that aerosols mitigated the rise in heat wave occurrence driven by increasing greenhouse gases. However, since 2005, this trend has shifted as aerosol reductions have accelerated the growth of global heatwaves by nearly two days each decade.

The researchers also found that aerosols exert a more significant influence on heatwave frequency in densely populated regions compared to less populated areas. In certain regions, the reduction of aerosol levels has proven to be more than twice as impactful as the increase in greenhouse gas concentrations. “If you examine the spatial distribution of aerosol concentrations, they correlate strongly with areas of high population,” remarks Persad.

In a scenario where greenhouse gas emissions rise significantly while aerosol levels gradually decrease, the team predicts a notable escalation in the frequency of heatwaves. By 2080, the number of heatwave days in densely populated regions could surge from about 40 to over 110 days annually.

“What sets this study apart is its focus on daily timescale data. You can genuinely perceive the decrease in aerosol levels across different areas of the globe,” says Shiv Priyam Raghuraman at the University of Illinois, Urbana-Champaign, who was not involved in the study. He highlights that these results arise from a single model under the most severe greenhouse gas emission scenario.

“These findings are compelling and enhance existing literature on the significant role aerosols play in climate extremes,” states Daniel Westerbert from Columbia University in New York. “It will be fascinating to see how other models might differ in their findings, and whether past observations support these results.”

Another significant uncertainty lies in the future trajectory of aerosol concentrations in the coming years, adds Persad. “Current emissions scenarios could determine aerosol trends over the next three decades,” she remarks.

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Source: www.newscientist.com

Astrophysicists Identify Gravitational Waves from the Largest Black Hole Mergers Recorded to Date

The twin detectors of the NSF’s Laser Interferometer Gravitational-Wave Observatory (LIGO) have made a groundbreaking discovery by detecting the highest composite mass recorded to date and the merger of two black holes. This event, identified as GW231123 and discovered on November 23, 2023, produced a final black hole with a mass over 225 times that of the Sun.



GW231123 An infographic detailing the merger of black holes. Image credits: Simona J. Miller/Caltech.

LIGO made history in 2015 with the first direct detection of gravitational waves, the ripples in spacetime.

In that instance, the waves were generated by the merger of black holes, culminating in a black hole with a mass 62 times that of our Sun.

The signal was simultaneously detected by LIGO’s twin detectors located in Livingston, Louisiana, and Hanford, Washington.

Since then, the LIGO team has collaborated with partners from Italy’s Virgo detectors and Japan’s KAGRA to create the LVK collaboration.

These detectors have collectively observed over 200 black hole mergers during their fourth observational run since starting in 2015.

Previously, the largest black hole merger recorded was in 2021 during the event GW190521, which had a total mass of 140 times that of the Sun.

During the GW231123 event, a black hole with a mass of 225 was formed by merging two black holes, one approximately 100 times and the other 140 times the mass of the Sun.

This discovery places it in a rare category known as intermediate mass black holes, which are heavier than those resulting from star collapses but significantly lighter than the supermassive black holes found at the centers of galaxies.

In addition to their substantial mass, these merged black holes exhibited rapid rotation.

“This is the largest black hole binary we’ve observed in gravitational waves and poses a significant challenge to our understanding of black hole formation,” stated Dr. Mark Hannam, an astrophysicist at Cardiff University and a member of the LVK collaboration.

“The existence of such a large black hole defies standard stellar evolution models.”

“One potential explanation is that the two black holes in this binary could have formed from the merger of smaller black holes.”

“This observation highlights how gravitational waves uniquely uncover the fundamental and exotic properties of black holes throughout the universe,” remarked Dr. Dave Reitze, executive director of LIGO at Caltech.

Researchers announced this week the discovery of GW231123, which will be discussed at the 24th International Conference on General Relativity and Gravity (GR24) and the 16th Edoardo Amaldi Meeting on Gravitational Waves, held jointly at the Gr-Amaldi Meeting in Glasgow, Scotland.

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LIGO-Virgo-KAGRA Collaboration. GW231123: The largest black hole binary detected by gravitational waves. Gr-Amaldi 2025

Source: www.sci.news

Can Humans Thrive Beneath the Waves? Exploring a Live Underwater Experiment

In recent years, the desire to establish human colonies beyond Earth, whether to escape environmental issues or explore uncharted territories, has gained significant traction.

While much attention is given to proposed bases on the Moon and Mars, there’s a more challenging and lesser-known frontier much closer to home: the ocean’s depths.

This concept isn’t new. Since the 1960s, with pioneers like French oceanographer Jacques Cousteau, individuals have created and spent extended periods in aquatic habitats.

NASA has been sending teams to the Aquarius Reef Base since 2001. This research facility, located 20 meters (around 65 feet) underwater off the Florida coast, has allowed scientists, engineers, and future astronauts to live in the module for 7 to 14 days.

With advancements in technology, prolonged underwater stays may become feasible. The UK company, Deep, is leveraging this technology to design habitats for extended underwater living. But, is the technology the only challenge we face?

Above the Atmosphere, Under the Sea

Humans are quite vulnerable. We struggle without oxygen or sunlight and are not fond of extreme pressure changes. Thus, we might not be the best candidates for life at the ocean floor.

This doesn’t imply that we can’t thrive in inhospitable environments.

Since 2000, astronauts have spent significant periods aboard the International Space Station (ISS).

Several astronauts have been documented living in the ISS for over 300 consecutive days, but Valeri Polyakov holds the record, having spent 437 days aboard the Mir Space Station in Russia between 1994 and 1995.

Moreover, astronauts returning from lengthy missions often face health issues, such as reduced bone density and muscle atrophy. What does this mean for those who aim to live underwater?

The most extensive study is that of Rudiger Koch, a German aerospace engineer who lived in a capsule submerged 11 meters (36 feet) under the Caribbean Sea for 120 days between 2024 and 2025.

Rudiger Koch on the balcony of the capsule where he lived between 2024 and 2025.

Koch reported no health issues upon celebrating with champagne and cigars.

In second place is Professor Joseph Dituri, who spent 100 days studying the physical and psychological effects of living underwater in a lodge situated at the bottom of a 9-meter deep (30-foot) lagoon in Florida.

Dituri conducted daily tests during his time submerged and following his return to the surface. Notably, aside from minor setbacks, he felt quite well.

He noted improvements in sleep quality, cholesterol levels, and inflammation. His stem cell count, testosterone levels, and cognitive performance also improved.

Interestingly, Dituri appeared to have lowered his biological age (an indicator of the aging process of the body), although he was recorded as having shrunk by over 1 cm (approximately 0.5 inches) due to the pressurized environment inside the lodge.

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A Step Towards Living Underwater

With limited data, we still have a tenuous understanding of life in aquatic environments. This is where Deep comes in.

The ocean technology and exploration company aims to develop two habitats by 2027, with the goal of establishing a permanent underwater presence. They are using a submerged quarry in Gloucestershire as a testing ground for their underwater habitats.

Deep is developing two habitat models: Vanguard, designed for three-person short stays, and Sentinel, a 16-meter (52-foot) capsule intended as a long-term habitat complete with living quarters, bedrooms, and research facilities, capable of accommodating researchers at depths of up to 200 meters (656 feet) for 28 days.

The aim is to enable researchers to remain submerged for extended periods, allowing for comprehensive studies of underwater living impacts and marine life. However, achieving these depths poses significant challenges.

“The most hazardous aspects of diving occur during descent,” explains Dr. Dawn Kernagis, Deep’s scientific research director. “Divers breathe compressed gas, with fluctuating pressure increasing the risk of decompression sickness (DCS), where gas bubbles form in the bloodstream.”

While most DCS cases are mild, severe instances can impact the brain, spinal cord, respiratory system, and circulatory systems.

To mitigate these risks, Deep aims to keep researchers “saturated” in the Sentinel habitats. This means achieving a new equilibrium with the underwater environment.

“Saturated tanks, like ours, facilitate diving into greater depths and adjusting to the pressure, enabling much longer stays, ranging from hours to about a month,” states Kernagis.

Deep plans for close monitoring of researchers during their stays to better understand the long-term physical and psychological effects of deep-sea living.

The foundation laid now may support future inhabitants underwater for weeks, months, or even years. In the not-so-distant future, some of us may find ourselves living in a modern-day Atlantis.

About Our Experts

Dr. Dawn Kernagis is the director of scientific research at Deep, a UK-based ocean technology and exploration firm. She has published in numerous scientific journals, including Journal of Clinical Oncology, Proceedings of the National Academy of Sciences, and Circulation.

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Source: www.sciencefocus.com

AI Decodes Brain Waves of Paralyzed Individuals into Real-Time Audio

A man with paralysis is connected to a brain-computer interface system

Lisa E. Howard/Mitely Wairagkar et al. 2025

Men who have lost their ability to speak can engage in real-time conversations and even sing using brain-controlled synthetic voices.

The brain-computer interface captures neural activity through electrodes implanted in the brain, instantly creating audio sounds that match intended pitch, intonation, and emphasis.

“This represents a breakthrough in instantaneous speech synthesis, achieving this within 25 ms,” says Sergei Stavisky from the University of California, Davis.

While advancements are needed to improve speech clarity, Maitreyee Wairagkar, also at UC Davis, notes that the individual who lost his speech due to amyotrophic lateral sclerosis expresses happiness and feels that he has found his true voice.

Existing speech neurospheres that utilize brain-computer interfaces typically require a few seconds to convert brain activity into sound. Stavisky mentions that this delays natural conversation and if the connection falters, it can feel like speaking on a poor-quality phone call.

To create a more seamless speech experience, Wairagkar, Stavisky, and their team implanted 256 electrodes in the areas of the male brain responsible for facial muscle control necessary for speech. In subsequent sessions, they introduced thousands of sentences on a screen, recorded brain activity, and prompted the subject to vocalize with specific intonations.

“For instance, phrases like ‘How are you today?’ or variations such as ‘How are you? today?’ can significantly alter the meaning of sentences,” explains Stavisky. “This approach allows for a richer, more natural dialog, marking a significant advancement over previous technologies.”

The researchers utilized an AI model trained to link particular patterns of neural activity with corresponding words and tonal variations, resulting in synthetic speech that mirrors both the content and emotional delivery intended by the user.

The AI was trained with audio recordings from before the male’s condition deteriorated, employing voice-cloning technology to ensure the synthetic speech bore a resemblance to his original voice.

In another phase of the study, researchers attempted to teach him to sing a simple melody with varying pitches, with their models accurately interpreting the intended pitch in real time and adjusting the produced singing voice accordingly.

He also utilizes the system to communicate spontaneously, making sounds such as “hmmm,” “eww,” and forming words, as noted by Wairagkar.

“He’s a remarkably articulate and intelligent individual,” says David Brandman from UC Davis. “Despite his paralysis, he has continued to participate actively in work and engage in meaningful conversations.”

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Source: www.newscientist.com

Will Life Beneath the Waves Shape Our Future as Sea Levels Rise?

Is this the future in a world where the oceans are rising?

Deep R&D Ltd

The Bajau are indigenous marine people of Southeast Asia, often referred to as sea nomads. For millennia, they have thrived along coastlines, relying on foraging underwater without the aid of diving gear, holding their breath for astonishing durations. Yet, the early 21st century introduced multiple crises that jeopardized their way of life—industrial overfishing, pollution, coral bleaching diminished food sources, and rising sea levels consumed coastal dwellings.

In 2035, a Bajau community near Saba, North Borneo, initiated fundraising for a contemporary floating and underwater settlement. They collaborated with deep, a manufacturer of submarine habitats, to create interconnected rafts and underwater homes, developing business models that could be emulated by other maritime communities facing similar threats from rising seas. Revenue streams included extreme adventure tourism, scientific research facilities, and longevity clinics.

The first habitat comprised a network of platforms and rafts, with tunnels leading to underwater levels. While residents occupied surface structures, they increasingly utilized submerged areas for storage, sustenance, and sleep. This habitat was constructed using a 3D printing technique known as Wire arc additive manufacturing, which allowed the most effective pressure distribution in areas experiencing strain.

The deeper sections were maintained at both ambient water pressure and the corresponding atmospheric pressure from the surface. In modules situated less than 20 meters deep, occupants, referred to as Aquanauts, inhaled a unique gas mixture to prevent nitrogen narcosis. Those exiting deep modules required decompression when returning to normal atmospheric conditions. An advantage of these surrounding modules was the incorporation of a moon door, enabling Aquanauts to swim directly into the deep sea for leisure, research, and farming activities.

Undersea hotels catering to extreme tourism have surged in popularity. In the Galapagos, tourists reside in submerged hydroelectric hotels, exploring hot springs and observing some of the planet’s rarest life forms. Simultaneously, scientists harness these modules to investigate deep-sea ecosystems. Undersea mapping technologies have evolved, enabling researchers to explore vast ocean territories that were previously unreachable, fostering understanding and interactions with whales and other deep-sea creatures, leading to significant advancements in marine biology.

Aquanauts can swim directly into the deep sea for recreational, research, and agricultural activities

The Bajau have long been adapted to marine environments. With thousands of years at sea, they possess enlarged spleens that provide a higher quantity of oxygen-retaining red blood cells compared to typical humans. Some Bajau divers can spend five hours underwater, diving freely to depths of 70 meters without oxygen tanks, holding their breath for up to 15 minutes. After transitioning to seabed habitats, many Bajau began to leave behind surface living, opting instead to spend more time submerged, even resorting to gene editing to enhance their aquatic capabilities, including intentional eardrum puncturing to facilitate deeper dives, and utilizing surfactants in their lungs to aid their decompression, akin to adaptations found in diving marine mammals.

Bajau’s Diver

Marco Rayman/Alamie

Numerous communities have established depth clinical treatments. Previous research has demonstrated that exposure to intermittent daily sessions of pressurized oxygen therapy can alleviate various medical conditions and age-related diseases. Hyperbaric oxygen therapy, for instance, has proven beneficial, leading individuals who underwent consistent high-pressure sessions to possess longer telomeres and enhanced clearance of senescent cells, both of which are linked to increased longevity. The deep habitat has attracted affluent seniors looking to extend their lives, simultaneously providing a lucrative income source.

The majority of marine communities have become self-sufficient, cultivating their own food through aquaculture of fish, mollusks, and seaweed, while also growing other crops on the surface. Energy sources include a combination of solar, wind, wave, and geothermal energy, tailored to local conditions. Some communities focus on tourism, whereas others specialize in carbon capture within medical facilities. A significant amount of seaweed is harvested, sunk into the ocean depths, and sold as carbon credits.

Living beneath the waves isn’t for everyone. Nonetheless, these habitats empower those most vulnerable to climate change, giving them the tools to redefine their livelihoods and lifestyles, even in the face of rising sea levels that threaten their homes.

Rowan Hooper is the podcast editor for New Scientist and author of *How to Spend $1 Trillion: These are 10 Global Issues That Can Be Actually Fixed*. Follow him on Bluesky @rowhoop.bsky.social

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Source: www.newscientist.com

Radio Waves and X-ray Emitting Stars: A New Perspective from Our Galaxy

Askap J1832-0911 – Likely a magnetar or a highly magnetized white dwarf star – emits radio signals and X-ray pulses for 2 minutes every 44 minutes. Paper published in Nature.

A combination of radio, X-ray, and infrared radiation in the field of ASKAP J1832-0911. Image credit: Wang et al., doi: 10.1038/S41586-025-09077-W.

Askap J1832-0911 is situated roughly 15,000 light-years away from Earth in Scutum.

This star was identified by astronomers utilizing the Australian ASKAP Radio telescope.

It belongs to a category known as long-term radio transients, first detected in 2022, characterized by variations in radio wave intensity over several minutes.

This duration is thousands of times greater than the regular fluctuations observed in pulsars. It’s a neutron star that spins rapidly, emitting signals multiple times per second.

“Askap J1832-0911 follows a 44-minute cycle of radio wave intensity, placing it in the realm of long-term radio transients,” stated Dr. Ziteng Wang, an astronomer at Curtin University’s node at the International Centre for Radio Astronomical Research (ICRAR).

Using NASA’s Chandra X-Ray Observatory, researchers noted that ASKAP J1832 also exhibited regular variations in X-ray emissions every 44 minutes.

This marks the first discovery of an X-ray signal in long-term radio transients.

“Astronomers have observed countless celestial bodies through various telescopes and have never encountered anything behaving like this,” Dr. Wang remarked.

“It’s exhilarating to witness such new stellar phenomena.”

Through Chandra and the SKA Pathfinder, scientists found that Askap J1832-0911 experienced a significant reduction in both X-ray and radio wave signals over a six-month period.

Besides the long-term changes, the combination of 44-minute cycles in X-rays and radio waves differs from observations made in the Milky Way galaxy.

The authors are currently competing to determine whether Askap J1832-0911 truly represents long-term radio transients and if its unusual behavior can shed light on the origins of such objects.

Dr. Nanda Lea, an astronomer at the Institute of Space Sciences in Barcelona, Spain, commented:

“No exact match has been found so far, but some models fit better than others.”

It’s improbable that ASKAP J1832-0911 is simply a pulsar or neutron star drawn from a companion star, as its properties do not align with the typical signal strengths of these celestial objects.

Some characteristics might be attributed to neutron stars with exceptionally strong magnetic fields, known as magnetars, which are over 500,000 years old.

However, other aspects, such as its bright and variable radio emissions, make it challenging to categorize this as an aged magnetar.

In the sky, ASKAP J1832-0911 appears to be situated among debris from a supernova, which commonly contains neutron stars formed during such events.

Nevertheless, the team concluded that this proximity is likely coincidental and that the two entities are not associated with one another, suggesting that neither may host neutron stars.

They deduced that while isolated white dwarfs don’t account for the data, white dwarfs with companion stars might.

But such a scenario would necessitate the strongest known magnetic fields in white dwarfs within our galaxy.

“We continue to seek clues about this object and look for similar entities,” said Dr. Tong Bao, an astronomer at the Osservatorio Astronomico in Italy’s National Institute of Astronomy (INAF).

“Discovering mysteries like this is not frustrating; rather, it’s what makes science thrilling!”

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Z. Wang et al. Detection of X-ray radiation from bright long-term radio transients. Nature Published online on May 28, 2025. doi:10.1038/s41586-025-09077-W

Source: www.sci.news

The Massive Boulder at Clifftop, Tonga, Was Pulled by 50-Meter High Waves

Martin Köhler in front of the Maka Rahi Boulder in Tonga

Martin Köhler/University of Queensland

The massive 1,200 tonne boulders of Tonga were carried inland as towering waves of 50 meters crashed against a 30-meter-high cliff.

“This is not just an ordinary boulder. It holds the title of the largest corrugated boulder found on a cliff and ranks as the third largest boulder globally, signifying that an immense force was needed to propel it from such a height,” said Martin Köhler from the University of Queensland, Brisbane, Australia.

Locally known as Maka Rahi, which translates to a large rock, this boulder had yet to be studied by scientists.

During fieldwork in Tonga in July 2024, the villagers pointed the researchers towards some intriguing rocks they might want to examine.

“We never anticipated discovering such a substantial rock at the finale of our field studies. It dawned on us quickly that we had stumbled upon a significant find,” Kohler explained.

Measuring 14 meters in length, 12 meters in width, and approximately 7 meters in height, it was described as a “remarkable” boulder, composed of limestone coral reef horn rec rocks. Previous satellite images missed this potential Monami Boulder, as vegetation had grown atop it, with surrounding forests extending into the woodland.

Upon observing the boulder, researchers identified a massive gouge believed to have been created at the cliff’s top, approximately 200 meters from the ocean.

The team utilized computer models to ascertain how this colossal boulder ended up above sea level.

Shifting it necessitated a wave with a minimum height of 50 meters and a duration of 90 seconds, implying it moved at a velocity exceeding 22 meters per second over a minute and a half, Kohler stated. Such a colossal tsunami is relatively localized and is thought to stem from nearby underwater landslides.

Dating indicated the boulder’s age to be 6,891 years, well before the settlement of humans on the island.

“It’s hard for me to fathom a 50-meter wave since I’ve never witnessed or heard of such massive waves before,” Kohler remarked. “However, the logic follows easily when one considers this enormous boulder positioned 200 meters inland on a 39-meter-high cliff.”

Only two rocks deposited by the tsunami have been found on land: one weighing 3,400 tons and another weighing 1,500 tons.

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Source: www.newscientist.com

Early Season Heat Waves Record High Temperatures in the Southwest and Texas

This week, the country is bracing for early seasonal heat waves, with record or near-record high temperatures anticipated across the Northern and Southern Plains, Southwest, and vast regions of central and southern Texas.

On Monday, temperatures climbed into the 90s in North Dakota, South Dakota, and Minnesota, with some areas likely reaching triple-digit highs.

Beginning Tuesday, Texas will experience its hottest conditions, with temperatures exceeding 100 degrees Fahrenheit becoming commonplace throughout the state, according to the agency.

“We are expecting record-breaking heat by mid-week across much of central and southern Texas,” the Weather Service noted. I mentioned this in a short-distance forecast on Monday.

In a series of posts on X, the San Antonio Weather Service office cautioned that many people may struggle to adapt to such extreme temperatures, heightening the risk of heat-related illnesses and fatalities.

“Temperatures are slated to soar above 100 on Tuesday, with some locations potentially hitting 110 mid-week. Ensure you have access to cooling and ample hydration before the heat arrives,” the office advised. I shared this on X.

As the week continues, the heat will intensify in the central and southern plains, eventually spreading to the southeastern U.S. and Florida.

Cities likely to set new daily temperature records this week include Austin, Dallas, San Antonio, and Houston in Texas, as well as Oklahoma City; Shreveport, Louisiana; Charleston, South Carolina; and Tallahassee, Jacksonville, and Orlando in Florida.

The unseasonably high temperatures are attributed to strong high-pressure ridges situated over much of the country, particularly in Texas. These “thermal domes” effectively trap heat in the region, leading to elevated temperatures for several days.

Southern California recorded historic highs over the weekend, peaking at 103 in downtown Los Angeles, surpassing the previous record of 99 set in 1988. According to reports, this significant increase has raised concerns.

During the Los Angeles heat wave, individuals took a moment to hydrate on Sunday.
Carlin Steele/Los Angeles Times Getty Images

Research indicates that climate change is intensifying the frequency, duration, and intensity of heat waves globally. Scientists predict yet another hot summer following two consecutive years of record-breaking global temperatures (2023 and 2024).

These ongoing record temperatures are part of alarming warming trends long anticipated by climate change models. The hottest years on record since 1850 have all occurred within the last decade. According to the National Oceanic and Atmospheric Administration.

Source: www.nbcnews.com

Severe Heat Waves and Droughts Hit Eurasia Back-to-Back

Drought conditions can have severe repercussions in regions like Karapinar in Türkiye

Yasin Akgul/AFP via Getty Images

Over the past two decades, from the grain stores of Ukraine to towns in northern China, Eurasia has experienced a notable increase in droughts following extreme heat events. Tree ring analysis extending back nearly three centuries indicates that human-induced climate change is a significant factor in the acceleration of these combined catastrophes.

This phenomenon presents a severe threat due to the way heat and drought reinforce each other. Elevated temperatures deplete soil moisture, and droughts further reduce the humidity needed to mitigate the impact of subsequent heat waves. This harmful cycle contributes to decreased agricultural productivity and a heightened risk of wildfires.

Certain regions in Eurasia have encountered similar heat and drought patterns in the past, but researchers assert, “current developments exceed natural fluctuations,” according to Hans Linderholm, a researcher at the University of Gothenburg, Sweden.

The complete landscape became apparent only after Linderholm and his team compiled tree ring data covering Eurasia from 1741, which reflects temperature and precipitation variations. This allowed them to recreate a comprehensive distribution of high- and low-pressure systems that influence wet and dry conditions across the continent.

Researchers identified specific phenomena affecting the area, termed the “heatwave motion train of iolarism,” which has intensified since 2000, amplifying anomalies beyond historical measurements. This alteration is associated with atmospheric pressure changes prompted by warming in the North Atlantic and increased precipitation in some regions of North Africa, both linked to anthropogenic climate change.

Rising local temperatures can directly worsen extreme heat and drought situations. However, new research indicates that climate change is modifying the dynamics between distant atmospheric regions (referred to as teleconnections), further complicating the situation, Linderholm explains.

Climate model forecasts predict worsening conditions under all scenarios except for those with the lowest emissions. “We observe a distinct, robust trend in this new teleconnection pattern, suggesting that impacts will escalate in both speed and severity,” states Linderholm.

“It is difficult to envision how [the most affected regions will] recover,” he concludes.

Source: www.newscientist.com

New research suggests that gravitational waves are responsible for the mid-ambient atmosphere on Mars

According to a new study by planetary researchers at Tokyo Planet University, atmospheric gravity waves play an important role in driving airflows, particularly at altitudes, at latitudes.



This image from the Emirates Mars Mission shows Mars and its thin atmosphere. Image credit: UAESA/MBRSC/HOPE MARS MISSION/EXI/ANDREALUCK.

“On Earth, the large atmospheric waves caused by the rotation of a planet known as the Rossby waves are the main effect on the way stratospheric air circulates, or the lower part of the medium atmosphere.”

“However, our research shows that on Mars, gravitational waves have the dominant effect in the mid-atmosphere and at high latitudes.”

“Rossby's waves are large atmospheric or resolved waves, while gravitational waves are unresolved waves, meaning that they must be estimated using finer, more indirect means to be measured or modeled.”

“Don't confuse it with gravitational waves from the body of a large star. Gravitational waves are atmospheric phenomena when packets of air rise and fall due to buoyancy fluctuations. Their oscillating movements cause gravitational waves.”

Due to their small-scale nature and limitations of observational data, planetary researchers previously discovered that it is difficult to quantify their importance in the Martian atmosphere.

Therefore, Professor Sato and her colleagues turned to the Ensemble Mars Atmosphere Reanalysis System (EMARS) dataset generated by various space-based observations over the years to analyze seasonal variation.

“We found something interesting. Gravitational waves promote the rapid vertical movement of angular momentum, which has a major impact on the meridian or north-north in the mid-atmospheric circulation on Mars,” said Anzu Asumi, a graduate student at Tokyo University.

“It's interesting because it's more like the behavior seen in the Earth's mesosphere, not in our stratosphere.”

“This suggests that the effects of these waves may need to be better incorporated to improve existing Mars atmospheric circulation models, and could improve future climate and weather simulations.”

The team is currently planning to investigate the effects of Mars sandstorms on atmospheric circulation.

“So far, our analysis has focused on a year without large sandstorms,” ​​Professor Sato said.

“However, I think these storms could dramatically change the state of the atmosphere and strengthen the role of gravitational waves in circulation.”

“In our research, there is a basis for predicting Mars weather, which is essential to guarantee the success of future Mars missions.”

study It will be displayed in Journal of Journal Geophysics: Planets.

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Anzu Asumi et al. Climatology of the residual average circulation of the Martian atmosphere and the contribution of solutions and unresolved waves based on reanalysis datasets. Journal of Journal Geophysics: PlanetsPublished online on March 6th, 2025. doi:10.1029/2023je008137

Source: www.sci.news

Radcliffe’s Waves: The solar system’s past encounter with a massive cloud of gas and dust

Radcliffe’s wave visualization, a series of dust and gas clouds (marked here) throughout the Milky Way. Approximately 400 light years from the sun, marked yellow

Alyssa A. Goodman/Harvard University

Our solar system passed through vast waves of gas and dust about 14 million years ago, darkening the views of the Earth’s night sky. The waves may have left a trace on our planet’s geological records.

Astronomers previously discovered large ocean-like waves of milky stars, gas and dust that ripple up and down for millions of years. One of these closest and most studied is the Radcliffe waves, about 9,000 light years wide and only 400 light years from the solar system.

Now, Efrem Maconi The University of Vienna and his colleagues discovered that the waves of Radcliffe once were far closer to us, surpassing the solar system 11 to 18 million years ago.

Maconi and his team used data from Gaia Space Telescope, which tracked billions of stars in the Milky Way, to identify recently formed groups of stars within the Radcliffe Wave, and identify the dust and gas clouds that formed from them.

Using these stars, they tracked the cloud orbits in time to reveal historic locations to show how the entire wave was moving. They also calculated the past paths of the solar system, rewind the clock for 30 million years, and discovered that the waves and our sun were approaching intimately about 15-12 million years ago. It is difficult to accurately estimate when the intersection began and ended, but the team believes the solar system is within the wave range around 14 million years ago.

This would have made Earth’s galactic environment as dark as it is today, as we currently live in a relatively empty space realm. “If we are in a dense region of interstellar media, that means that the light coming from the stars will dim,” says Macconi. “It’s like being on a foggy day.”

The encounter may have left evidence in Earth’s geological records and deposited radioactive isotopes on the crust, but considering how long ago it happened, this would be difficult to measure, he says. It says it is useful to find such a galactic encounter, as explaining the geological record of the Earth is a continuous problem. Ralph Schoenrich University College London.

More speculatively, the crossing appears to have occurred during a period of cooling, known as the mid-Miocene. Maconi said the two could be linked, but this would be difficult to prove. Schoenrich thinks that is unlikely. “The rule of thumb is that geology outweighs the influence of the universe,” he says. “When you move around the continent or disrupt ocean currents, you need more because climate change is occurring.”

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Source: www.newscientist.com

Astronomers Report Our Solar System Surpassed the “Radcliffe Waves” in the Miocene Era

As our solar system orbits the Milky Way, we encounter a variety of environments, including dense regions of interstellar media. These encounters can increase the flow of interstellar dust into the solar system and the Earth's atmosphere, exposing parts of the solar system to interstellar mediums. The discovery of new galactic structures, such as the Radcliffe waves over the 9,000 Wright years, raises the question of whether the Sun encountered any of them. New research shows that the solar system trajectories intersected with the waves of Radcliffe in the Orion star-forming region 15 to 12 million years ago (Miocene era). In particular, this period coincides with the mid-Miocene climate transition on Earth, providing an interdisciplinary connection with paleoclimatology.

Radcliffe wave visualization. Image credit: Alyssa Goodman/Harvard University.

When the solar system brings the Milky Way into orbit, we encounter a variety of galactic environments with different interstellar densities, including hot voids, fronts of supernova blasts, and cold gas clouds.

The passage of the sun through dense regions of interstellar media can affect the solar system in several ways.

For example, pressure enhancement compresses the heliosphere and exposes parts of the solar system to cold, dense interstellar media.

Furthermore, the amount of interstellar dust mounted on the Earth's atmosphere can increase, potentially enhancing the delivery of radioactive isotopes such as iron-60 through dust grains.

Radcliffe's waves are narrow sinusoidal gas structures and consist of many known star-forming cloud complexes, including CMA, Orion, Taurus, Perseus, Cephaus, North American Nebula, and Cygnus.

With an estimated mass of 3 million people, this gas structure appears to vibrate consistently like a moving wave and is thought to be part of the Milky Way spiral structure.

Dr. Efrem Macconi, a doctoral student at the University of Vienna, said:

“Our Sun encountered a higher gas density region as it passed through the waves of Radcliffe in the Orion constellation.”

Using data from ESA's Gaia mission and spectroscopic observations, Dr. Maconi and his colleagues identified the passage of the solar system through the Radcliffe Wave in the Orion area.

“The findings are based on previous works identifying Radcliffe's waves,” said Professor Joanne Albes of the University of Vienna.

“We passed the Orion area as well as famous star clusters like NGC 1977, NGC 1980 and NGC 1981.”

“The area is easily visible in the winter sky in the Northern Hemisphere and in the summer in the Southern Hemisphere.”

“Look for Orion Constellation and Orion Nebula (Messier 42) – our solar system has come from that direction!”

“The increased dust from this galaxy encounter may have had some effects.”

“It could potentially leave traces of radioactive elements from supernovas in the geological record that permeate the Earth's atmosphere.”

“Current technologies may not be sensitive enough to detect these traces, but future detectors may make it possible.”

This study shows that the solar system passing through the Orion region occurred around 18.2 to 11.5 million years ago, with the most likely time between 148 and 12.4 million years ago.

This time frame is in good agreement with the mid-Miocene climate transition, and is a major shift from warm variable climate to cool climates, leading to the establishment of a continental-scale prototype Antarctic ice sheet composition.

This study raises the possibility of a link between past crossings of the solar system through galaxy neighbours and Earth's climate through interstellar dust, but the authors need further investigation of the causal relationship. It emphasizes that there is.

“The basic processes responsible for the mid-Miocene climate transition have not been fully identified, but available reconstructions are most likely to be long-term reductions in atmospheric greenhouse gas carbon dioxide concentrations. It suggests that it is a high explanation.

“However, our research highlights that interstellar dust associated with the crossing of Radcliffe's waves has affected the Earth's climate and may have played a potential role during this climate change. Masu.”

“To change the Earth's climate, the amount of extraterrestrial dust on Earth needs to be much larger than what previous data suggests.”

“Future research explores the importance of this contribution. This past climate change and current climate change is comparable as this past climate change is unfolding over a timescale of hundreds of thousands of years. It is important to note that we do not do that.”

“In contrast, the evolution of global warming today has been happening at an unprecedented rate for decades to centuries due to human activity.”

study Published in the journal Astronomy and Astrophysics.

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E. Machoni et al. 2025. Passing through the solar system through the waves of Radcliffe in the mid-Miocene. A&A 694, A167; doi: 10.1051/0004-6361/202452061

Source: www.sci.news

LIGO hunts for gravitational waves produced by mountains on neutron stars

While the solar system’s moons such as Europa and Enceladus have thin crusts over deep oceans, Mercury has a thin crust over a large metallic core. Thin sheets are generally likely to wrinkle. Europa has linear features, Enceladus has “tiger stripes” and Mercury has foliated cliffs. Neutron stars may have similar characteristics. These neutron star mountains can generate detectable oscillations in space and time known as gravitational waves, according to a new study.

Artist’s impression of a neutron star. Image credit: Sci.News.

Neutron stars are a trillion times denser than lead, and their surface features are largely unknown.

Nuclear theorists investigated the mountain-building mechanisms active on the moons and planets of the solar system.

Some of these mechanisms suggest that neutron stars likely have mountains.

A mountain in a neutron star would be much more massive than any mountain on Earth. They are so huge that the gravitational pull from these mountains alone can generate gravitational waves.

of Laser interferometer Gravitational wave observatory (LIGO) is currently looking for these signals.

“These waves are so weak that they require highly detailed and sensitive techniques carefully tuned to the expected frequencies and other signal characteristics,” said nuclear astrophysicist Jorge Morales and professor Charles Horowitz at Indiana University. It can only be discovered through search.”

“The first detection of continuous gravitational waves opens a new window on the universe and will provide unique information about neutron stars, the densest objects after black holes.”

“These signals may also provide sensitive tests of fundamental laws of nature.”

The authors investigated the similarities between neutron star mountains and surface features of solar system objects.

“While both neutron stars and certain moons, such as Jupiter’s moon Europa and Saturn’s moon Enceladus, have a thin crust over a deep ocean, Mercury has a thin crust over a large metallic core. The thin sheet Wrinkles are universally possible,” they said.

“Europa has linear features, Enceladus has tiger-like stripes, and Mercury has curved, step-like structures.”

“Mountained neutron stars may have similar types of surface features that can be discovered by observing continuous gravitational wave signals.”

“Earth’s innermost core is anisotropic, and its shear modulus is direction-dependent.”

“If the material in the neutron star’s crust is also anisotropic, a mountain-like deformation will occur, and its height will increase as the star rotates faster.”

“Such surface features could explain the maximum spin observed in neutron stars and the minimum possible deformation of radio-emitting neutron stars known as millisecond pulsars.”

team’s paper Published in a magazine Physical Review D.

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JA Morales and CJ Horowitz. 2024. The anisotropic neutron star crust, the mountains of the solar system, and gravitational waves. Physics. Rev.D 110, 044016; doi: 10.1103/PhysRevD.110.044016

Source: www.sci.news

Nanostructured filaments produce luminous waves that twist as they move

Scientists at the University of Michigan say the twisted shape of the nanostructured filaments allows them to generate bright, twisted light.



Planck's law ignores, but does not prohibit, circular polarization of blackbody radiation (BBR). BBRs consisting of nanostructured filaments with twisted shapes made of nanocarbon or metal have strong ellipticity between 500 and 3000 nanometers. The submicrometer-scale chirality of these filaments meets the dimensional requirements imposed by the fluctuation dissipation theorem, which requires symmetry breaking between absorption and emissivity according to Kirchhoff's law. The resulting BBRs exhibit emission anisotropy and brightness that are 10–100 times superior to conventional chiral photon emitters. Image credit: Lu others., doi: 10.1126/science.adq4068.

“When producing twisted light using traditional methods such as electroluminescence or photon emission, it is difficult to generate sufficient brightness,” said Dr. Jun Lu, a researcher at the University of Michigan.

“We gradually realized that there is actually a very old way of producing these photons, which does not rely on the excitation of photons and electrons, but is similar to the light bulb that Edison developed. .”

“Every object that has some heat, including yourself, constantly emits photons in the spectrum associated with its temperature.”

“If an object is the same temperature as its surroundings, it will also absorb the same amount of photons. Since black absorbs all photon frequencies, this is idealized as blackbody radiation.”

Although the filament of a tungsten bulb is much warmer than its surroundings, the law that defines blackbody radiation (Planck's law) provides a good approximation of the spectrum of photons that a tungsten bulb transmits.

The photons we see as a whole look like white light, but when we pass light through a prism, we see a rainbow of different photons inside.

This radiation is also why it appears bright in thermal images, but even room-temperature objects can appear dark because they are constantly emitting and receiving blackbody photons.

Usually, the shape of the object that emits radiation is not much considered. In most cases, objects can be imagined as spheres.

However, while the shape does not affect the spectrum of different photon wavelengths, it can affect another property: polarization.

Photons from a blackbody source are typically randomly polarized, and their waves can oscillate along any axis.

New research reveals that blackbody radiation can also be twisted if the emitter is twisted on the micro or nanoscale, with the length of each twist similar to the wavelength of the emitted light.

The strength of the twist of light, or its elliptical polarization, is determined by two main factors. One is how close the wavelength of the photon is to the length of each twist, and the other is the electronic properties of the material (in this case, nanocarbon or metal).

Twisted light is also called “chiral” because the clockwise and counterclockwise rotations are mirror images of each other.

The study was done to demonstrate the premise of a more applied project that the Michigan team wants to pursue: using chiral blackbody radiation to identify objects.

They envision robots and self-driving cars that can see like a mantis shrimp, distinguishing light waves in different directions of rotation and degrees of twist.

“Advancing the physics of blackbody radiation through chiral nanostructures is at the heart of this research. Such emitters are all around us,” said Professor Nicholas Kotov of the University of Michigan.

“For example, these findings could be important in helping autonomous vehicles tell the difference between a deer and a human. Deer fur curls differently than our fabric, so even though the wavelengths are similar, Helicity emits a different light.”

The main advantage of this method of producing twisted light is its brightness, which is up to 100 times brighter than other approaches, but the light contains a wide spectrum of both wavelengths and twists.

The authors have ideas on how to address this, including exploring the possibility of building lasers that rely on twisted light-emitting structures.

They want to further explore the infrared spectrum. The peak wavelength of blackbody radiation at room temperature is approximately 10,000 nanometers or 0.01 millimeter.

“This is a noisy spectral region, but elliptical polarization could potentially enhance the contrast,” Professor Kotov says.

of the team work Published in a magazine science.

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Jun Lu others. 2024. Bright circularly polarized blackbody radiation from twisted nanocarbon filaments. science 386 (6728): 1400-1404;doi: 10.1126/science.adq406

Source: www.sci.news

Meme coin boom following President Trump’s election waves the flag of pure gambling in cryptocurrency markets

The attention economy can be likened to a phenomenon involving a social media-created celebrity named “hawk tua girl” Hayley Welch. She played a pivotal role in the launch of a cryptocurrency asset named Hawk Memecoin, which quickly gained enormous traction before facing backlash.

Initially valued at $490 million (£385 million) on December 4, the Hawk Memecoin has now exceeded its market capitalization and is valued at $17 million. Welch, a Tennessee native, rose to fame after responding to provocative interview questions but faced criticism for allegedly deceiving her social media followers.

Critics like cryptocurrency commentator Steven Findeisen, also known as Coffeezilla, labeled Hawk’s launch as a “rug pull,” which involves hyping a crypto project for short-term gains and then abandoning it. Despite the controversy, Hawk Memecoin is still being traded, with Welch stating that her team has not sold any tokens.

The rise of meme coins like Hawk reflects the growing trend within the cryptocurrency market, with meme coins collectively valued at $118 billion compared to $20 billion at the start of the year. These coins flood the market, with platforms issuing thousands of tokens daily.

Experts argue that meme coins lack fundamental value and are merely tied to digital trends. Memecoins blend the essence of memes and cryptocurrencies, leveraging social media attention to drive speculation and investment.

Meme coin trading often revolves around internet trends and influencer endorsements, creating a speculative environment with unpredictable outcomes. Participants acknowledge the speculative nature of memecoins, likening their trading to gambling but with the potential for significant returns.




Bitcoin’s value surpassed $100,000 for the first time a month after President Trump’s victory. Photo: Kevin Wurm/Reuters

Source: www.theguardian.com

Greenland landslide triggers unprecedented waves that reverberated across the globe for over a week

Part of a mountain and glacier along Greenland’s Dikson Fjord in August 2023 (left), and the same location after a landslide in September 2023

Soren Lisgaard/Danish Army

On September 16, 2023, earthquake monitoring stations around the world picked up a strange signal that weakened over time but remained detectable for nine days.

“We thought, ‘Oh, this signal is still coming. This is definitely not an earthquake.'” Stephen Hicks Researchers at University College London have dubbed the object an “Unidentified Seismic Object,” or USO.

Hicks and his colleagues found that the signal was caused by water moving across the 1.7-mile-wide Dikson Fjord in eastern Greenland. The wave was triggered by a massive landslide, which produced a 360-foot-high tsunami.

Earthquake signals typically last only a few minutes and are a mix of different frequencies, Hicks said. USO’s frequency is about 11 millihertz and repeats every 90 seconds. When it became clear that the signal started at the same time as the Greenland landslide, Hicks and his colleagues thought there was probably a connection.

Many objects, such as bells, vibrate at a particular resonant frequency when struck. The same is true for bodies of water, from swimming pools to oceans. Disturbances such as earthquakes or wind can cause a body of water to shake, setting off a kind of standing wave called a seiche.

Based on its width and depth, the researchers calculated that Dikson Fjord has a resonant frequency of 11 millihertz, which matches the signal. What took them longer to figure out was why the fjord continued to oscillate for so long.

Immediately after the tsunami, the seiche rose seven metres on both sides of the fjord. Within a few days it receded to a few centimetres, but this was so small that it went unnoticed by a Danish navy ship sailing up the fjord three days after the landslide.

But the seiche didn’t stop, likely continuing long after the nine days had passed and becoming undetectable by distant seismic stations, Hicks said. “No seiche has ever been reported before that lasted that long or that the energy dissipated that slowly.”

The team’s computer modelling suggests that the shape of the fjord was a crucial factor: The landslide occurred 200 kilometres inland, and the fjord is blocked by a glacier at one end and curves sharply at the other. The fjord’s rounded bottom acts like a rocking chair, allowing the water to flow through with little resistance.

All these factors caused the wave to have a high degree of energy trapped inside, rather than dissipating quickly as it normally would, Hicks said.

The slide itself was a direct result of climate change. A steep glacier supported the mountainside. As the glacier thinned, it collapsed, sending an estimated 25 million cubic meters of rock and ice into the fjord. It was the first landslide ever recorded in eastern Greenland.

No one was in the area at the time, but cruise ships were traveling up the fjord. The tsunami destroyed equipment used to monitor the area and two abandoned hunting lodges.

As the planet continues to warm, we’ll likely see more of these kinds of landslides, Hicks said, noting that the findings show that climate change is affecting not just the atmosphere and oceans, but also the ground beneath our feet. “For the first time, we’re looking down at our feet and seeing some of the devastating effects of climate change,” he said.

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Source: www.newscientist.com

Lightning can generate energy waves that travel vast distances into space.

Lightning can create special energy waves

Room the Agency/Alamy

This overlooked mechanism could allow lightning energy to reach the top of the atmosphere, threatening the safety of satellites and astronauts.

When lightning strikes, the energy it carries can create special electromagnetic waves called whistlers, so named because they can be converted into sound signals. For decades, researchers thought that the whistlers produced by lightning remained confined to altitudes relatively close to the Earth's surface, below about 1,000 kilometers.

now Vikas Sonwalkar and Amani Lady Researchers at the University of Alaska Fairbanks discovered that some whistlers bounce off a layer of the atmosphere filled with charged particles called the ionosphere, which allows whistler waves and the energy they carry to travel up to 20,000 kilometers above Earth's surface—all the way into the magnetosphere, the region of space governed by Earth's magnetic field.

Researchers found evidence of these reflective whistlers in data from the Van Allen Probes, twin robotic spacecraft that measured the magnetosphere between 2012 and 2019. They also found hints of the phenomenon in studies published in the 1960s. Both the old and new data indicate that the phenomenon is very frequent and happens all the time, Reddy said.

In fact, the lightning may be depositing twice as much energy into this region as previously estimated, the researchers say, and this energy charges and accelerates nearby particles, creating electromagnetic radiation that can damage satellites and endanger the health of astronauts.

“Lightning has always been considered a bit of a smaller player. Until 10 years ago, this data wasn't available and we'd never looked at it at this level of detail.” Jacob Bortnick researcher at the University of California, Los Angeles. He says the new study is a call for others to develop a more accurate picture of the magnetosphere.

Establishing the connection between lightning and the magnetosphere is also important because changes in Earth's climate could make lightning storms more frequent, Sonwalker said.

The research team now hopes to analyze data from more satellites to learn more about how lightning-based whistlers are distributed in the magnetosphere and how they are affected by space weather.

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Source: www.newscientist.com

Theoretical astrophysicists debate the generation of gravitational waves during warp drive collapse

The basic idea of ​​a warp drive is that rather than directly exceeding the speed of light in a local frame of reference, a “warp bubble” contracts space-time in front of it and expands it behind it, allowing travel over distances faster than the speed of light as measured by a distant observer.

Craft othersWe propose a formalism for the dynamical study of warp drive spacetime and generate the first fully consistent numerical relativistic waveforms for the collapse of a warp drive bubble.

Although warp drive has its origins in science fiction novels, according to Miguel Alcubierre, an astrophysicist at the University of Wales, warp drive is explained in detail in the general theory of relativity. Be the first to propose A space-time metric that supports faster-than-light travel.

Real-world implementation has many practical barriers, such as the need for a special type of material that has negative energy, but computationally, given an equation of state describing the material, it is possible to simulate changes over time.

In a new study, theoretical astrophysicists investigated the signatures that could result from a “containment failure” of a warp drive.

“Warp drives are purely theoretical, but they are clearly described in Einstein's general theory of relativity, and numerical simulations allow us to explore the effects of warp drives on space-time in the form of gravitational waves,” said Dr Katie Clough, researcher at Queen Mary, University of London.

“The results are fascinating: the warp drive collapse produces a unique gravitational wave burst — a ripple in space-time that can be detected by gravitational wave detectors that typically target merging black holes and neutron stars.”

“Unlike chirp signals from merging objects, this signal is a short, high-frequency burst that would be undetectable by current detectors.”

“But there may be higher frequency devices in the future, and although the money hasn't been put into those devices yet, the technology exists to build them.”

“This raises the possibility that we could use these signals to look for evidence of warp drive technology, even if we can't build it ourselves.”

“In our study, the initial shape of spacetime is the warp bubble described by Alcubierre,” said Dr Sebastian Kahn, a researcher at Cardiff University.

“Although we demonstrate that an observable signal could, in principle, be found by future detectors, the speculative nature of this work is not sufficient to drive instrument development.”

The authors also take a detailed look at the energy dynamics of a collapsing warp drive.

In this process, waves of negative energy matter are released, followed by alternating waves of positive and negative energy.

This complex dance results in a net increase in energy throughout the system and, in principle, could provide another signature of collapse if the emission waves interacted with ordinary matter.

“This is a reminder that theoretical ideas can inspire us to explore the universe in new ways,” Dr Clough said.

“I'm skeptical that we'll see anything, but I think it'll be interesting enough to be worth a look.”

“For me, the most important aspect of this work is the novelty of accurately modelling the dynamics of negative energy space-time and the possibility that the technique can be extended to physical situations that could help us better understand the evolution and origin of the universe or processes at the centre of black holes,” said Professor Tim Dietrich of the University of Potsdam.

“While warp speed may still be a long way away, this research is already pushing the boundaries of our understanding of extra-dimensional space-time and gravitational waves.”

“We're going to try different models of warp drive to see how that changes the signal.”

Team paper Published online Open Astrophysics Journal.

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Katie Clough othersThe year is 2024. A phenomenon no one has seen before: gravitational waves caused by warp drive collapse. Open Astrophysics Journal 7;doi:10.33232/001c.121868

Source: www.sci.news

The impact of historical discrimination on heat waves in minority and low-income communities

Today, the South Bronx has the least amount of green space per capita in the city and is crisscrossed by power plants, waste dumps and freeways, causing significant noise and air pollution. Residents face high rates of infant mortality, cognitive impairment, heart disease, and asthma, and Mott Haven is known as ‘ Asthma Alley.’ These conditions increase vulnerability to heat.

“Environmental racism in the South Bronx is clear,” said Arif Ullah, executive director of the environmental justice group South Bronx Unite.

Similar inequities have been identified across the country. Analysis of 115 metropolitan areas from San Jose, California, to Louisville, Kentucky, to Hartford, Connecticut, neighborhoods with larger numbers of residents who identify as black, African American, Hispanic, or Latino were found to be less likely to have air conditioning.

To combat rising temperatures, New York City Mayor Eric Adams has implemented heatstroke measures. For one week, starting June 18, hundreds of locations were designated as air-conditioned facilities where residents could stay cool during the day.

New York City Emergency Management Director Zach Iscol said the city is distributing “cool kits” and indoor thermometers. He said: There is a program to help low-income residents who need heating and cooling. This year, 21,000 applications have already been received.

Installing air conditioning for people with mobility impairments is actually essential as outdoor temperatures rise — or these individuals may never be able to reach a cooling center. In areas like Brownsville, the South Bronx, and East Harlem, residents also report being exposed to crime and drug dealing when they go outside to cool off.

Celine Olivarius, who has lived in the South Bronx for nine years, brought her two grandsons, ages 9 and 4, to cool off in the fountains at Willis Playground. She expresses concern about the opioid epidemic, as drug users are injecting in the bathroom, and she worries that children might pick up needles.

Environmentalists say one solution to beat the heat in sprawling cities is to plant more trees, create green spaces like parks and meadows, and cover rooftops with vegetation.

“We need to focus on low-income communities, people of color, and immigrant communities,” Uhlfelder said. Areas with a 33 percent reduction in tree canopy area are likely to experience a 13-degree increase (7 degrees Celsius) in temperature compared to predominantly white areas just two miles away.

The New York City Council passed laws last fall to add trees to the City Charter Sustainability Plan and mandate the development of urban forest plans to increase tree cover from 22 percent to 30 percent by 2035.

“I’ve never felt anything like it,” said Howard Shillingford, a 58-year-old janitor who grew up in the South Bronx, on a recent sweltering day. It’s especially bad when he’s cleaning school staircases, where the windows often don’t open.

“Oh my goodness, those stairs look like an oven,” Shillingford said as he read the news on a computer at Mott Haven Public Library, another cooling center.

Residents in heat-stricken areas are getting resourceful. Berrios holds a wet towel to the back of her neck. Olivarria squirts her grandchildren with a toy water gun. Jorge Morales, a 54-year-old graffiti artist from the South Bronx, showers twice a day and washes his Chihuahua, Bugsy, in the sink. Residents sometimes unscrew fire hydrants, allowing water to spill off the sidewalk and onto the street.

“I don’t like wasting water, but people here do it. It’s a way of survival,” Morales, who is half Puerto Rican and half Cuban, said as he charged his phone in the same library.

Experts say extreme heat will likely become the new normal and should not be underestimated. Heat waves have become more frequent since 1936.

“If we continue on this path, the heat wave in 2044 will be much worse than the one we’re experiencing now,” said Jones, the science historian. “This is not an unusual heat wave. It is a sign of things to come.”

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Source: www.nbcnews.com

Climate change is causing extreme heat waves in the Southwest to become hotter and occur 35 times more frequently

Anthropogenic causes Climate Change I turned up the thermostat, bolstering the possibility of a heatwave this month. Grilling the Southwestern United States, Mexico, and Central AmericaThis is revealed in a new breaking research study.

Parts of the US experienced heatwaves during the day that could cause heatstroke, with temperatures rising by 2.5C (1.4C) due to global warming caused by the burning of coal, oil and natural gas. World Weather Attribution, The calculations were made Thursday by a group of scientists conducting a rapid, non-peer-reviewed study of climate factors.

“It’s like an oven out here, there’s no way I could be here,” said Magarita Salazar Pérez, 82, who lives in Veracruz, Mexico, in her home without air conditioning. Temperatures in the Sonoran Desert reached 125 degrees Fahrenheit (51.9 Celsius) last week, making it the hottest day in Mexico’s history, said Shel Winkley, a meteorologist at Climate Central and co-author of the study.

And it was even worse at night, which is what made the heatwave so deadly, said Friederike Otto, a climate scientist at Imperial College London who is leading the team investigating its causes. Climate change has caused nighttime temperatures to rise by 2.9 degrees Celsius (1.6 degrees Fahrenheit), making extreme nighttime heat 200 times more likely, Otto said.

Salazar-Perez said there isn’t the cool nighttime air that people are used to, and doctors say lower nighttime temperatures are key to surviving the heatwave.

A man holds his head in the heat at the Cogra nursing home in Veracruz, Mexico, on June 16, 2024.Felix Marquez/AP

At least 125 people have been killed so far, according to the Global Weather Attribution Team.

“This is clearly related to climate change, the level of intensity that we’re seeing, these risks,” said Karina Izquierdo, urban adviser at the Mexico City-based Red Cross Red Crescent Climate Center and co-author of the study.

Otto said what’s worrying about this heat wave, which is still heating up North America, is that it’s no longer unusual. Previous research from the group has shown that extremely extreme heat waves Not possible without climate changebut not this heat wave.

“So in that sense it’s not unusual from a meteorological standpoint, but the impacts were really bad,” Otto told The Associated Press in an interview.

“The changes over the last 20 years, which feel like yesterday, have been so dramatic,” Otto said. Her research shows that heat waves are four times more likely now than they were in 2000, when temperatures were nearly 1 degree Celsius (half a degree Celsius) cooler. “It seems so long ago, like another world.”

While other international groups of scientists, as well as global carbon emission reduction targets adopted by countries in the 2015 Paris Climate Agreement, have noted that warming has been increasing since the pre-industrial era in the mid-1800s, Otto said comparing what is happening now to the year 2000 is even more shocking.

“We’re seeing the baseline shift, and what was once extreme but rare is becoming more and more common,” said Carly Kenkel, dean of marine studies at the University of Southern California, who was not involved in the team’s investigation. She called the analysis a “logical conclusion based on the data.”

Jorge Moreno drinks flavored water while working at a construction site in Veracruz, Mexico on June 17, 2024. Felix Marquez/AP

The study looked at the five hottest days and nights across a wide swath of the continent, including Southern California, Arizona, New Mexico, Texas, Oklahoma, Mexico, Guatemala, El Salvador, Belize and Honduras. In most areas, the five days were from June 3 to 7, and the five nights were from June 5 to 9, but in some places, the peak heat began as early as May 26, Otto said.

For example, San Angelo, Texas, recorded a record 111 degrees (43.8 degrees Celsius) on June 4. Between June 2 and June 6, Corpus Christi Airport's nighttime temperatures never dropped below 80 degrees (26.7 degrees Celsius), setting a new nighttime temperature record, with two days where the temperature never dropped below 85 degrees (29.4 degrees Celsius), according to the National Weather Service.

Between June 1st and June 15th, more than 1,200 Highest daytime temperature record The United States saw a flurry of records being broken and tied, with nearly 1,800 overnight high temperature records set, according to the National Centers for Environmental Information.

The team used both current and historical temperature measurements to contrast what’s happening now with past heatwave conditions, then used a scientifically-accepted method of comparing a hypothetical simulation of a world without human-made climate change with current reality to calculate how much global warming contributed to the 2024 heatwave.

Winkley said the immediate meteorological cause is high pressure that was parked over central Mexico, blocking storms and clouds that brought cold air, then moved into the southwestern U.S. and is now bringing hot air to the eastern U.S. Tropical Storm Alberto The storm formed on Wednesday and is heading toward northern Mexico and southern Texas, where it is likely to bring rain and cause flooding.

Mexico and other places have been in the spotlight for months. Drought, Water shortage and Extreme heatMonkeys Falling from a tree in Mexico From the warmth.

The heatwave is “exacerbating existing inequalities.” Rich and poor Izquierdo said the inequality is stark in the Americas, and Kenkel agreed: Nighttime heat is accentuated because the ability to stay cool with central air conditioning depends on how affordable you are, Kenkel said.

So, Salazar-Perez was feeling very uncomfortable during this heatwave.

Source: www.nbcnews.com

Astronomers find record-breaking slowest rotating neutron star emitting radio waves

Neutron stars typically spin quickly, taking just a few seconds or even a fraction of a second to complete one revolution around their axis, but one neutron star labeled ASKAP J1935+2148 bucks this rule, emitting radio signals at a relatively slow interval of 53.8 minutes.

Artist's impression of a neutron star. Image courtesy of Sci.News.

“We're used to extreme examples when studying radio-emitting neutron stars, so the discovery of such a compact star that is still emitting radio waves despite rotating slowly was unexpected,” said Professor Ben Stappers, from the University of Manchester.

“This new generation of radio telescopes demonstrates that pushing the boundaries of our search space will reveal surprises that will shake up our understanding.”

At the end of their lives, massive stars use up all their fuel and undergo a spectacular explosion called a supernova.

What remains is a stellar remnant called a neutron star, which consists of trillions of neutrons packed into an extremely dense sphere with a mass 1.4 times that of the Sun, packed into a radius of just 10 km.

Astronomers detected an unexpected radio signal from ASKAP J1935+2148 that traveled about 16,000 light-years to Earth.

The nature of its radio emission and the rate of change of its rotation period suggest that it is a neutron star, but further study is needed to confirm what this object is.

“This discovery relied on the complementary capabilities of the ASKAP and MeerKAT telescopes, combined with our ability to probe these objects on timescales of minutes, and examine how their radiation changes from second to second,” said Dr Kaustubh Rajwade, an astronomer at the University of Oxford.

“Such synergies can shed new light on how these compact objects evolve.”

ASKAP J1935+2148 was detected by CSIRO's ASKAP radio telescope in the Wadjari Yamatji region of Western Australia.

“What's interesting is that this object exhibits three different radiation states, each with completely different properties to the others,” said Dr Manisha Caleb, an astronomer at the University of Sydney.

“The MeerKAT radio telescope in South Africa played a key role in distinguishing between these states.”

“If the signals had not come from the same point in the sky, it would be hard to believe that it was the same object producing these different signals.”

“Until the arrival of these new telescopes, the dynamic radio sky was relatively unexplored,” said Professor Tara Murphy, from the University of Sydney.

“Now we can look deeply and frequently see a variety of unusual phenomena.”

“These events give us insight into how physics works in extreme environments.”

This discovery paper In the journal Natural Astronomy.

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M. Caleb othersA radio transient phenomenon in which the radiation state switches with a period of 54 minutes. Nat AstronPublished online June 5, 2024; doi: 10.1038/s41550-024-02277-w

Source: www.sci.news

As heat waves loom, cities innovate to protect residents and prevent casualties.

In North Carolina, for instance, Ward and colleagues have assisted counties in formulating heat preparedness plans to identify their most vulnerable residents.

He emphasized that government officials should approach the rise in heat and humidity in a similar manner to how they handle hurricanes, tornadoes, and other emergencies.

“Emergency management and public health officials are already well-prepared for various extreme weather events, but they are not as well-prepared for heat-related incidents,” Ward explained.

The events of last summer raised concerns, she noted.

“It was a Category 5 heat event,” Ward explained. “The severity of what we experienced last summer was enough to bring attention to this issue.”

Research indicates that climate change is leading to an increase in the frequency, duration, and intensity of heatwaves worldwide. Last year marked the hottest year on record, and the warming trend continues. According to the European Union’s Copernicus Climate Change Agency, April saw World temperature records being set for 11 consecutive months.

Forecasts suggest that temperatures will be higher than usual across much of the United States in the next three months, as per the National Oceanic and Atmospheric Administration’s predictions. According to the National Oceanic and Atmospheric Administration.

Ward expressed optimism that cities were taking the threat of heatwaves seriously, although significant challenges lie ahead. Securing funding for preparing for extreme heatwaves, particularly in rural regions, is a major challenge.

Addressing the root social issues that exacerbate during heatwaves, such as homelessness, soaring energy costs, and economic disparities, is an even greater challenge.

However, Ward remains hopeful that the experiences of last summer have motivated some local governments to take action.

“Moving forward, I would like to see a stronger emphasis on preventive measures to reduce these exposures in the first place, so we are not constantly in response mode,” she stated.

Source: www.nbcnews.com

Strong winds have the power to generate massive waves, scientists reveal

A rogue wave is a single swell that is much higher than nearby waves and can cause damage to ships and coastal infrastructure. Ocean waves are one of the most powerful natural forces on Earth, and they could become even more powerful as global trends suggest ocean winds will blow even stronger with climate change. there is. Scientists at the University of Melbourne have discovered in a new study that rogue waves are generated by strong winds and unpredictable wave patterns, confirming an idea previously only proven in the lab.



Toffoli other.We report direct observations of surface waves from a stereo camera system and simultaneous measurements of wind speed during an expedition across the Southern Ocean during the Antarctic winter aboard a South African icebreaker. SA Agulhas II. Image credit: Alessandro Toffoli.

“Rogue waves are huge, twice as tall as nearby waves, and appear out of nowhere,” said University of Melbourne’s Professor Alessandro Toffoli, lead author of the study.

Using cutting-edge technology and embarking on an expedition to one of the most unstable ocean regions on Earth, Professor Toffoli and colleagues have introduced a new technique for 3D imaging of ocean waves.

Operating a stereo camera on a South African icebreaker SA Agulhas II During their 2017 Antarctic expedition, they captured valuable insights into the behavior of waves in this remote region.

Their method, which mimics human vision through continuous imaging, allowed researchers to reconstruct the wavy ocean surface in three dimensions, providing unprecedented clarity into ocean wave dynamics. Ta.

The first scientific measurement of a rogue wave was the 25.6 m Draupner wave recorded in the North Sea in 1995. Since the beginning of the 21st century, 16 cases of suspected rogue waves have been reported to him.

“Scientists have long theorized that Antarctica’s rough seas and fierce winds can cause large waves to ‘self-amplify’, resulting in rogue wave frequencies. “However, this has not yet been tested underwater,” Professor Toffoli said.

The team’s observations, using numerical and laboratory studies that suggested the role of wind in the formation of rogue waves, provided validation of these theories in a real marine environment.

“Our observations show that unique sea conditions with rough waves occur during the ‘young’ stage of the waves, when they are most susceptible to wind effects. This suggests that wind parameters are the missing link,” Professor Toffoli said.

“Wind creates a chaotic situation where waves of different dimensions and directions coexist.”

“The wind causes young waves to grow higher, longer and faster.”

“During this self-amplification, waves grow disproportionately at the expense of neighboring waves.”

“We show that young waves are showing signs of self-amplification and are likely to be wind-driven.”

“Once every six hours, we recorded waves that were twice as high as nearby waves.”

“This reflects laboratory models. The theory is that sea conditions are more likely to self-amplify, creating more rogue waves.”

“In contrast, no rough waves were detected in mature oceans that are not influenced by winds.”

The authors highlight the critical importance of integrating wind dynamics into predictive models for rough sea prediction.

“This shows that scientists need to take wind into account thoroughly when developing tools to predict rogue waves,” Professor Toffoli said.

of findings It was published in the magazine physical review letter.

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A. Toffoli other. 2024. Observation of the bad waters of the Southern Ocean. Physics.pastor rhett 132 (15): 154101; doi: 10.1103/PhysRevLett.132.154101

Source: www.sci.news

Heat waves today are lasting significantly longer than in the 1980s

People cooling off in Amsterdam’s heat wave

Cohen van Weel/AFP via Getty Images

An analysis of all heatwaves around the world between 1979 and 2020 found that they now last an average of 12 days, compared to eight days at the start of the study.

As the Earth continues to heat, they will last even longer, says Zhang Wei at Utah State University. “Based on trends, by around 2060 it could double to 16 days,” he says.

Zhang’s team found that heat waves not only last much longer, but also become more frequent and progress more slowly. This means that certain locations have to endure heat wave conditions more frequently and for longer.

Although heat waves are typically thought of as phenomena that affect one region, the areas affected by heat waves change over time as the weather systems responsible for the hot conditions move.

According to the research team, the speed of heat waves has slowed from around 340 kilometers per day in the 1980s to around 280 kilometers per day today. Moreover, the rate of deceleration is accelerating.

Because heat waves last longer, they reach farther, albeit at lower average speeds, increasing the total distance from about 2,500 kilometers to about 3,000 kilometers. This means that a wider area is affected.

The study did not consider the causes of this trend. However, with global warming, heat waves will become more frequent, slower moving, and last longer, meaning they will be more devastating to society and nature than ever before, unless action is taken to prevent further warming. The research team warns that this could have a negative impact.

Most previous studies on heat waves focused on specific locations or regions. Zhang’s team is one of the few that can observe how heat waves move over time.

To do this, the team divided the world into grids. A heat wave is defined as one or more grid rectangles that significantly exceed the average temperature from 1981 to 2010, specifically, temperatures exceeding 95 percent of the temperatures for that period for three or more days. it was done.

The research team found that heat waves tend to move in certain directions depending on prevailing conditions. For example, heat waves in Australia tend to move more south-east, while in Africa they tend to move west.

“I think it’s really interesting to be able to see all the properties of heat waves that you can’t capture if you consider them statically,” he says. andrea beenish He was involved in one of the few other studies at the Ludwig-Maximilians University in Munich, Germany. Seeing heat waves as moving systems.

But when thinking about what we need to do to adapt to a hotter world, regional assessments can be more helpful than global ones, Beinisch says.

She also points out that, for example, heatwave persistence numbers depend largely on how the team defines a heatwave. Even with different definitions, the overall trend remains the same, but the numbers can change significantly. “This needs to be taken into account when looking at the exact numbers,” she says.

Other studies also show that hurricanes move more slowly, he says. david keelings at the University of Florida.

“In short, this means that these incredibly dangerous events last longer in one place and the impact is felt more strongly. In general, the longer a population is exposed to heatwave conditions, the more likely they are to be hospitalized. higher rates and higher mortality rates,” he says.

topic:

  • climate change/
  • Abnormal weather

Source: www.newscientist.com

Learn about five pioneering women making waves in the tech industry

Gender gaps within science, technology, engineering, and mathematics (STEM) still persist despite significant advancements. Women continue to be underrepresented, with only 29.2% of STEM employees being women compared to nearly 50% in non-STEM occupations, as reported in the Global Gender Gap Report (2023).

However, the urgent need to address goes beyond just getting women into STEM. A recent study at UCL revealed that female she-STEM students are twice as likely to have experienced sex discrimination compared to non-STEM students.

With advancements in hackers and digital technologies, the demand for cybersecurity professionals is on the rise to combat digital threats. The global cybersecurity market is projected to reach $424.97 billion by 2030, highlighting the importance of closing the gender gap to address this deficit.

Throughout history, women in STEM fields have overcome barriers, but there is still a long way to go. Here are five remarkable women who have significantly contributed to STEM:

5 women who advanced STEM

  • Ada Lovelace (1815-1852)
  • Katherine Johnson (1918-2020)
  • Dame Stephanie Shirley “Steve” (1933-present)
  • Michelle Zatlin (1979-present)
  • Elizabeth Coulon (1994-present)

Ada Loveless

Augusta Ada, Countess of Lovelace (1815-1852) British mathematician and writer. – (Photo courtesy of Universal History Archive/Getty Images)

Ada Lovelace, a prominent figure in computer engineering, was ahead of her time. She envisioned a steam-powered flying machine at 12 and played a significant role in Charles Babbage’s analytical engine, laying the foundation for modern computing.

Katherine Johnson

Portrait of NASA/NACA female physicist and scientist Katherine Johnson, 1955. – Image courtesy of NASA. (Photo via Smith Collection/Gado/Getty Images)

Katherine Johnson, an African-American mathematician, played a crucial role in NASA’s early missions, including Glenn’s orbit in 1962 and the Apollo 13 mission. Her calculations contributed to landing humans on the moon and creating a flight plan for crew safety.

Mrs. Stephanie Shirley

Entrepreneur and philanthropist Dame Stephanie Shirley has been appointed a Member of the Order of the Brotherhood by the Duke of Cambridge. – Photo credit: John Stillwell – WPA Pool / Getty Images

Stephanie Shirley, a work-from-home pioneer, founded Freelance Programmers and overcame industry obstacles through her innovative approach, paving the way for equal labor rights. She also founded Autistica, a charity dedicated to autism research.

Michelle Zatlin

CloudFlare’s Michelle Zatlin will be on stage judging Startup Battlefield. – Photo by Steve Jennings/Getty Images for TechCrunch

Michelle Zatlin, a technology pioneer, co-founded Cloudflare, a cybersecurity company that prevents cyberattacks and safeguards internet traffic. Cloudflare’s projects, such as “Athenian” and “Project Cyber Safe Schools,” focus on election integrity and cybersecurity in schools.

Elizabeth Coulombe

Elizabeth Coulombe, co-founder of Tero. – Photo credit: Tero

Elizabeth Coulombe, the CEO of Tero, developed a device that recycles food waste into organic fertilizer in hours, addressing global food waste issues. Her innovation has prevented significant waste from reaching landfills, contributing to environmental sustainability.

Women have played pivotal roles in shaping a better world, from cybersecurity to environmental sustainability, demonstrating their impact and contributions to solving pressing global issues.

Source: www.sciencefocus.com

Neuroscientists find that brain waves aid in clearing waste from the brain during sleep

According to a new study from Washington University in St. Louis, individual neurons work together to generate rhythmic waves that propel fluid through dense brain tissue, cleaning it in the process.

Accumulation of metabolic waste products is a major cause of many neurological diseases, but there is still limited knowledge about how the brain performs self-cleaning.Jean Xie other. They demonstrate that neural networks synchronize individual action potentials to generate large-amplitude, rhythmic, self-perpetuating ion waves within the brain's interstitial fluid. Image credit: Jiang-Xie other., doi: 10.1038/s41586-024-07108-6.

“These neurons are miniature pumps,” said Dr. Li-Feng Jiang-Xie, lead author of the study.

“Synchronized neural activity facilitates fluid flow and removal of debris from the brain.”

“If we can develop this process, we could slow or prevent neurological diseases such as Alzheimer's disease and Parkinson's disease, where excess waste products such as metabolic waste and junk proteins accumulate in the brain and cause neurodegeneration. It may be possible.”

Brain cells form a dynamic network that coordinates thoughts, emotions, and body movements and is essential for memory formation and problem solving.

But to perform these energy-intensive tasks, your brain cells need fuel. When you take in nutrients from your diet, metabolic waste products are produced in the process.

“It is important that the brain processes metabolic waste products that can accumulate and contribute to neurodegenerative diseases,” said Professor Jonathan Kipnis, senior author of the study.

“We knew that sleep is a time when the brain begins a cleansing process to flush out waste and toxins that have accumulated during wakefulness. But how does that happen? I didn't understand.”

“These findings may point us to strategies and potential treatments to accelerate the removal of hazardous waste and remove it before it leads to dire consequences.”

However, cleaning the dense brain is not an easy task. The cerebrospinal fluid that surrounds the brain enters a complex network of cells, collecting toxic waste as it passes through it.

On leaving the brain, contaminated fluids must pass through a barrier in the dura mater (the outer layer of tissue that surrounds the brain under the skull) before flooding into the lymph vessels.

But what powers the flow of fluid into, into, and out of the brain?

“Researchers studied the brains of sleeping mice and discovered that neurons work together to fire electrical signals that generate rhythmic waves in the brain, prompting cleaning efforts,” says Jean. Dr. Shi said.

The study authors determined that such waves drive fluid movement.

They silenced certain brain areas so that neurons in those areas no longer produced rhythmic waves.

Without these waves, fresh cerebrospinal fluid cannot flow through the silenced brain areas and trapped waste products cannot exit the brain tissue.

“One of the reasons we sleep is to cleanse the brain,” Professor Kipnis says.

“And if we can enhance this cleansing process, perhaps we can sleep less and stay healthy.”

“Not everyone can benefit from eight hours of sleep each night, and lack of sleep can affect your health.”

“Other studies have shown that mice genetically short-sleeping have healthier brains.”

“Is it to remove waste products from the brain more efficiently?”

“Is it possible to strengthen the brain purification ability of people suffering from insomnia so that they can live with less sleep?”

of study Published in the Journal on February 28, 2024 Nature.

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LF.Jean Xie other. Neurodynamics directs cerebrospinal fluid perfusion and brain clearance. Nature, published online on February 28, 2024. doi: 10.1038/s41586-024-07108-6

Source: www.sci.news

Record-breaking heat waves will be caused by El Nino worldwide this year

A map showing the expected surface temperature anomalies in 2024 if a strong El Niño event occurs.Blue dots indicate areas where record heat is expected

Ning Jiang et al., Scientific Reports

Climate models predict this year will be the hottest 12 months on record as El Niño conditions persist in the Caribbean, Bay of Bengal, South China Sea, Alaska and parts of the Amazon.

“These are places where the risk of extreme events is increased, and these extreme events are really harmful,” team members say. michael mcfaden NOAA Pacific Marine Environmental Laboratory, Seattle, Washington.

“They negatively impact human health and increase the risk of wildfires. And in the ocean, they increase the risk of marine heatwaves, damaging marine ecosystems, fisheries and corals,” he said. Masu.

Earth’s surface temperatures are currently at record highs in many parts of the world. The main reason is global warming caused by carbon emissions from burning fossil fuels. However, in addition to this, the strong El Niño phenomenon that started in mid-2023 is causing temperatures to rise further.

When an El Niño event occurs, warm water spreads across the surface of the Pacific Ocean toward South America. This vast area of warm water transfers large amounts of ocean heat to the atmosphere, causing an increase in surface temperature.

The reverse phase, known as La Niña, reverses this process. Cold water spreads over the surface of the Pacific Ocean away from South America, absorbing heat from the atmosphere and lowering the surface temperature.

This means that the Earth’s average surface temperature typically reaches record levels during El Niño periods and then drops during La Niña periods.

McFadden and his colleagues used a computer model that took into account aerosol pollution and volcanic eruptions in addition to El Niño to try to predict where in the world record heat would occur. Their regional forecast is the average surface temperature for the period from July 2023 to June 2024.

“Even if it’s not exactly timed to a specific season, there’s real value in having this kind of warning,” McFayden says. “It gives us a grace period to prepare how best to protect life, property, marine resources and economic development.”

The research team considered two scenarios: a strong El Niño and a milder El Niño. It’s now clear that a strong El Niño is occurring, and in fact, it’s likely to be in the top five strongest El Niños since 1950, McFadden said.

In this strong El Niño scenario, the research team predicts that the global average surface temperature from July 2023 to June 2024 would be 1.1°C to 1.2°C warmer than the 1951-1980 average. Masu.

this is Equivalent to a temperature above 1.4-1.5 °C average from 1850 to 1900, new scientist This is considered a pre-industrial benchmark. This suggests that the model is underestimating the temperature since it is already above this level. From January 2023 to January 2024, the Earth’s average surface temperature was more than 1.5 °C above the 1850-1900 average, and in January 2024 it was 1.7 °C above this level.

Temperature records have already been broken during El Niño, especially in the tropics, he said. maximiliano herrera, an independent climatologist who tracks extreme temperatures. “This is amazing,” he says. “We are experiencing record heat and it is inevitable.”

topic:

Source: www.newscientist.com

Radcliffe waves found to exhibit oscillations by astronomers

Our Sun is within 300 parsecs (about 1,000 light-years) of a 2,700-parsec (about 9,000 light-years) long sinusoidal dense gas cloud known as the Radcliffe wave. The wavy shape of this structure was discovered using 3D dust mapping, but initial kinematic investigations of its oscillatory motion were inconclusive. Radcliffe waves oscillate in the plane of the Milky Way galaxy, radiating away from the galaxy's center, according to a new study.

Radcliffe waves next to the sun (yellow dot) in a cartoon model of the Milky Way. The blue dots are a group of baby stars.The white line is the theoretical model by Konietzka other. It describes the current shape and movement of the wave. The magenta and green lines show how the waves will move in the future. Image credit: Ralf Konietzka / Alyssa Goodman / Worldwide Telescope.

“By using the movement of baby stars born in gas clouds along Radcliffe waves, we can track the movement of the natal gas and show that the Radcliffe waves are actually rippling,” says Ralph.・Dr. Konietzka said. He is a student at Harvard University and the Smithsonian Center for Astrophysics.

In 2018, astronomers mapped the 3D location of a stellar nursery in the sun's galactic neighborhood.

By combining new data, ESA's Gaia Mission Using a data-intensive “3D dust mapping” technique, they noticed an emerging pattern, leading to the discovery of the 2020 Radcliffe wave.

“This is the largest coherent structure that we know of, and it's in our immediate vicinity,” said Dr. Katherine Zucker, an astronomer at the Harvard University & Smithsonian Center for Astrophysics.

“It's been there all along. We just didn't know it because we weren't able to build high-resolution models in 3D to show the distribution of gas clouds near the Sun.”

Although the 3D dust map clearly showed that Radcliffe waves were present, sufficient measurements were not available at the time to confirm whether the waves were moving.

But in 2022, astronomers used a new release of Gaia data to assign 3D motion to young star clusters in Radcliffe waves.

By understanding the location and movement of the clusters, they were able to confirm that the entire Radcliffe wave was indeed undulating, moving like what physicists call a “traveling wave.”

“Traveling waves are the same phenomenon you see in sports stadiums, where people take turns standing and sitting to do waves,” Konietzka said.

“Similarly, star clusters along Radcliffe waves move up and down, creating patterns that travel through the galaxy's backyard.”

“In the same way that fans in a stadium are pulled back into their seats by Earth's gravity, Radcliffe waves are oscillated by the Milky Way's gravity.”

No one yet knows what causes Radcliffe waves or why they behave the way they do.

“Now we can test all the different theories about why the waves formed in the first place,” Dr. Zucker said.

“Those theories range from the explosion of a giant star called a supernova to disturbances outside the galaxy, such as a dwarf satellite galaxy colliding with the Milky Way,” Konietzka added.

“It turns out we don't need significant dark matter to explain the motion we observe.”

“The gravity of ordinary matter is enough to move waves.”

Furthermore, the discovery of this oscillation has raised new questions about the predominance of these waves in both the Milky Way and other galaxies.

Radcliffe waves appear to form the backbone of the Milky Way's closest spiral arms, so the ripples in these waves may be due to the oscillations of galactic spiral arms in general, making galaxies even more dynamic than previously thought. It may suggest that you are doing something.

“The question is: What causes the displacement that causes the ripples that we see?” said Professor Alyssa Goodman, an astronomer at Harvard University and the Smithsonian Center for Astrophysics.

“And does it happen throughout the galaxy? In every galaxy? Does it happen sometimes? Does it happen all the time?

of result appear in the diary Nature.

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R. Konietzka other. Radcliffe waves are oscillating. Nature, published online on February 20, 2024. doi: 10.1038/s41586-024-07127-3

Source: www.sci.news

Scientists puzzled by mysterious burst of intergalactic radio waves hitting Earth.

It may be hard to miss, but unimaginably strong bursts of cosmic radiation happen possibly a thousand times every day. They are bright enough to overwhelm our radio telescopes from billions of light-years away.

However, fast radio bursts (FRBs) were not detected until 2007. Despite over a decade of investigation, they remain one of the most intriguing mysteries in astrophysics. Recent research offers new and promising clues about their origins, while also revealing why these space phenomena are so perplexing in the first place.

When FRBs were first discussed in seminars, the big question wasn’t “What astrophysical cause is causing this?” Instead, it was, “Isn’t this just a mechanical failure?”

FRBs last about 1 millisecond and spread out in frequency in a manner very similar to a blip from a pulsar. But the problem is, they don’t come from any known pulsars, they don’t repeat like pulsars, and they’re clearly much more powerful than any pulsar pulses we’ve seen before.



To make matters worse, for many years the only telescope that observed FRBs was the Parkes Observatory in Australia. The debate became even more heated when it turned out that some of the FRB-like bursts observed by Parkes did not come from astronomical sources.

These bursts, called “peritons,” were always suspected to be of terrestrial origin. But clever detective work by astronomers solved the case. Dr. Emily Petrov and her colleagues showed that Periton had a strong correlation with local lunchtime. In reality, radiation leaked from the observatory’s microwave when the door opened too early.

It was eventually revealed that the FRBs were indeed from far away in space. More radio telescopes were configured to record very short bursts of radio waves, and detection rates began to skyrocket.

Those bursts came from all over the sky, suggesting they didn’t originate in our galaxy. In the first decade after the discovery, theorists produced a huge number of papers explaining the possible origins of the bursts.

In 2012, repeated FRBs were discovered, ruling out origins requiring complete destruction, such as supernovae. It was soon discovered that there were many more repeated bursts, mostly occurring at irregular intervals.

As more outbursts are discovered, there is growing evidence that FRBs may be associated with extraordinarily powerful magnetars: neutron stars that rotate in extremely strong magnetic fields.

Recent evidence suggests that at least some FRBs originate from nearby spiral galaxies rather than elliptical galaxies.

Astronomers will need to continue collecting clues, looking for suggestive patterns in the data, and eagerly awaiting observational upgrades that will allow them to pinpoint the FRBs’ local environment.

Whatever the outcome, the fast radio burst is a great example of the fact that in science, when we look at the universe in new and different ways, we almost always discover something surprising that no one had ever thought to look for.

Source: www.sciencefocus.com

Thermal secrets uncovered in neutron star mergers through gravitational waves

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Scientists used supercomputer simulations to study gravitational waves produced by neutron star mergers and found a correlation between residual temperature and gravitational wave frequency. These findings are important for future gravitational wave detectors that distinguish models of hot nuclear material. Credit: SciTechDaily.com

Binary simulation neutron star This merger suggests that future detectors will distinguish between different models of hot nuclear material.

Researchers used supercomputer simulations to investigate the effects of neutron star mergers gravitational waves, found a significant relationship with debris temperature. This research will aid future advances in the detection and understanding of hot nuclear materials.

Exploring neutron star mergers and gravitational waves

When two neutron stars orbit each other, they emit ripples into spacetime called gravitational waves. These ripples drain energy from the orbit until the two stars eventually collide and combine into one object. Scientists used supercomputer simulations to investigate how the behavior of different models of nuclear material affects the gravitational waves released after these mergers. They found a strong correlation between the temperature of the debris and the frequency of these gravitational waves. Next generation detectors will be able to distinguish these models from each other.

Plot comparing density (right) and temperature (left) for two different simulations (top and bottom) of a neutron star merger, viewed from above, approximately 5 ms after the merger.Credit: Jacob Fields, Pennsylvania State University

Neutron Star: Institute for Nuclear Materials

Scientists use neutron stars as laboratories for nuclear materials under conditions that would be impossible to explore on Earth. They will use current gravitational wave detectors to observe neutron star mergers and learn how cold, ultra-dense matter behaves. However, these detectors cannot measure the signal after the stars have merged. This signal contains information about hot nuclear material. Future detectors will be even more sensitive to these signals. Because different models can also be distinguished from each other, the findings suggest that future detectors could help scientists create better models of hot nuclear material.

Detailed analysis of neutron star mergers

The study investigated neutron star mergers using THC_M1, a computer code that simulates neutron star mergers and accounts for the bending of spacetime due to the star’s strong gravitational field and neutrino processes in dense matter. . The researchers tested the effect of heat on mergers by varying the specific heat capacity of the equation of state, which measures the amount of energy required to raise the temperature of neutron star material by one degree Celsius. To ensure the robustness of their results, the researchers ran their simulations at two resolutions. They repeated the high-resolution run using a more approximate neutrino processing.

References:

“Thermal effects in binary neutron star mergers” by Jacob Fields, Aviral Prakash, Matteo Breschi, David Radice, Sebastiano Bernuzzi, and Andre da Silva Schneider, July 31, 2023. of Astrophysics Journal Letter.
DOI: 10.3847/2041-8213/ace5b2

“Identification of nuclear effects in neutrino-carbon interactions in low 3 momentum transfer” until February 17, 2016 physical review letter.
DOI: 10.1103/PhysRevLett.116.071802

Funding: This research was primarily funded by the Department of Energy, Office of Science, Nuclear Physics Program. Additional funding was provided by the National Science Foundation and the European Union.

This research used computational resources available through the National Energy Research Scientific Computing Center, the Pittsburgh Supercomputing Center, and the Pennsylvania State University Computing and Data Science Institute.

Source: scitechdaily.com

AI technology capable of translating brain waves into text

AI can decode brainwave recordings and predict words someone is reading

Vertigo3d/Getty Images

A team of scientists has announced that a sensor-equipped helmet, combined with artificial intelligence, can translate a person’s thoughts into text.

In this study, participants read passages of text while wearing hats, and their brain electrical activity was recorded through the scalp. These electroencephalogram (EEG) recordings were converted to text using an AI model called DeWave.

Lin Ching Tian Researchers from Australia’s University of Technology Sydney (UTS) say the technology is non-invasive, relatively cheap and portable.

The system is far from perfect, with an accuracy of about 40%, but recent data currently under peer review shows an improvement in accuracy of more than 60%, Lin said.

In a study published in NeurIPS conference In New Orleans, Louisiana, the DeWave program does not use spoken language, but instead has participants read sentences aloud. However, in the researchers’ latest study, participants read the text silently.

Last year, the team he led was jerry tan Researchers at the University of Texas at Austin reported similar accuracy in converting thoughts into text, but used MRI scans to interpret brain activity. Using EEG is more practical because the subject does not have to remain still in the scanner.

UTS team member Charles Zhou said the DeWave model was trained by looking at many examples where brain signals matched a particular sentence.

“For example, when you think of saying ‘hello,’ your brain sends a specific signal,” Zhou says. “DeWave learns how these signals relate to the word ‘hello’ by looking at many examples of these signals for different words and sentences.”

Once DeWave had a good understanding of the brain signals, the team connected it to an open-source large-scale language model (LLM) similar to the AI ​​that powers ChatGPT.

“This LLM is like a smart writer who can craft sentences. We tell these writers to pay attention to the signals from DeWave and use that as a guide to craft their sentences. ” says Zhou.

Finally, the team trained both DeWave and a language model together to further improve their ability to write sentences based on EEG data.

Researchers predict that further improvements to the system could revolutionize communication for people who have lost language due to stroke or other conditions, and could also have applications in robotics.

craig gin from the University of Sydney said he was impressed by Lin’s team’s work. “It’s great progress,” he says.

“People have long wanted to convert brainwaves to text, and the team’s model shows amazing accuracy. A few years ago, EEG-to-text conversion was complete and utter nonsense. .”

topic:

Source: www.newscientist.com

“Unconscious Brain Activity and Epileptic Seizures: The Role of Sleep Brain Waves”

A new study has found that the slow brain waves typical of sleep occur in epilepsy patients when they are awake, helping to prevent the brain from becoming more excited. These waves reduce epileptic activity while negatively impacting memory, suggesting a potential new therapeutic approach for epilepsy.

UCL researchers have found that slow brain waves commonly seen during sleep occur in epilepsy patients while they are awake, preventing seizures but affecting memory, suggesting a new potential treatment for epilepsy. are doing.
A new study led by researchers at University College London (UCL) has found that slow waves, which normally occur only in the brain during sleep, also occur when epilepsy patients are awake, and show that slow waves, which are associated with epilepsy symptoms, can also occur in the brain during sleep. It was found that there is a possibility of preventing increased excitement.

Methodology and findings

The study was published today (November 30) in the journal nature communications The National Institute for Health Research (NIHR) UCLH Biomedical Research Center also took part in conducting electroencephalogram (EEG) scans from electrodes in the brains of 25 patients with focal epilepsy (a type of epilepsy characterized by seizures originating from specific parts of the brain). was inspected. brain), they performed an associative memory task.
Electrodes were placed in the patient’s brain to localize abnormal activity and inform surgical treatment.
During the task, participants were presented with 27 pairs of images that remained on the screen for 6 seconds. The images are divided into nine groups of three, and each group contains photos of people, places, and objects. In each case, participants had to remember which images were grouped together. EEG data were recorded continuously throughout the task.
After reviewing EEG data, the researchers found that the brains of people with epilepsy produce slow waves lasting less than a second while they are awake and participating in tasks.
The occurrence of these “awakening” slow waves increased in response to increased brain excitability, reducing the influence of epileptic spikes on brain activity.
In particular, it reduces the “firing” of nerve cells, which the researchers say can prevent epileptic activity.

Implications and future research

Lead author Professor Matthew Walker (UCL Queen Square Institute of Neurology) said: “Sleep is crucial for repairing, maintaining, and resetting brain activity. When we are awake, our brains gradually become more excitable, which recovers during sleep.
“Recent research has shown that a specific form of brain activity, namely slow waves during sleep, plays an important role in these restorative functions. We believe that these ‘sleep’ slow waves , we wanted to consider whether this could occur during wakefulness in response to the abnormal increase in brain activity associated with epilepsy.
“This study reveals for the first time ‘arousal’ slow waves, a potential protective mechanism used by the brain to counter epileptic activity. This mechanism takes advantage of brain defense activity that normally occurs during sleep, but can also occur during wakefulness in epileptic patients. ”
As part of the study, the team also wanted to test whether the occurrence of “awake” slow waves had a negative impact on cognitive function.
Researchers found that during memory tasks, “awake” slow waves reduced neuronal activity, thus affecting cognitive performance and increasing the time patients needed to complete the task.
The researchers reported that for every additional slow wave per second, reaction time increased by 0.56 seconds.
Professor Walker said: “This observation suggests that the cognitive impairments experienced by epilepsy patients, particularly memory impairments, may be due in part to short-term impairments caused by these slow waves. “
The research team hopes that future studies will increase such activity as a potential new treatment for epilepsy patients.
Lead author Dr Laurent Sheibany (UCL Queen Square Institute of Neurology) said:
“Our study suggests that naturally occurring activity is utilized by the brain to offset pathological activity. However, slow waves of ‘wake’ may have no effect on memory performance. This comes at a cost because we know we give.
“From a purely neurobiological perspective, this study also supports the idea that sleep activity does not occur uniformly throughout the brain, but may occur in specific regions of the brain.”
Reference: “Awakening slow waves in focal human epilepsy affect network activity and cognition” November 29, 2023 nature communications.
DOI: 10.1038/s41467-023-42971-3
This research was funded by the Medical Research Council, Wellcome, UCLH Biomedical Research Center and the Swiss National Science Foundation.

Source: scitechdaily.com