Nobel Prize Winner Plans to Develop World’s Most Powerful Quantum Computer

Ryan Wills, New Scientist. Alamy

John Martinis is a leading expert in quantum hardware, who emphasizes hands-on physics rather than abstract theories. His pivotal role in quantum computing history makes him indispensable to my book on the subject. As a visionary, he is focused on the next groundbreaking advancements in the field.

Martinis’s journey began in the 1980s with experiments that pushed the limits of quantum effects, earning him a Nobel Prize last year. During his graduate studies at the University of California, Berkeley, he tackled the question of whether quantum mechanics could apply to larger scales, beyond elementary particles.

Collaborating with colleagues, Martinis developed circuits combining superconductors and insulators, demonstrating that multiple charged particles could behave like a single quantum entity. This discovery initiated the macroscopic quantum regime, forming the backbone of modern quantum computers developed by giants like IBM and Google. His work led to the adoption of superconducting qubits, the most common quantum bits in use today.

Martinis made headlines again when he spearheaded a team at Google that built the first quantum computer to achieve quantum supremacy. For nearly five years, this machine could independently verify the outputs of random quantum circuits, though it was eventually surpassed by classical computers in performance.

Approaching seven decades of age, Martinis still believes in the potential of superconducting qubits. In 2024, he co-founded QoLab, a quantum computing startup proposing revolutionary methodologies aimed at developing a genuinely practical quantum computer.

Carmela Padavich Callahan: Early in your career, you fundamentally impacted the field. When did you realize your experiments could lead to technological advancements?

John Martinis: I questioned whether macroscopic variables could bypass quantum mechanics, and as a novice in the field, I felt it was essential to test this assumption. A fundamental quantum mechanics experiment intrigued me, even though it initially seemed daunting.

Our first attempt was a simple and rapid experiment using contemporary technology. The outcome was a failure, but I quickly pivoted. Learning about microwave engineering, we tackled numerous technical challenges before achieving subsequent successes.

Over the next decade, our work on quantum devices laid a solid foundation for quantum computing theory, including the breakthrough Scholl algorithm for factorizing large numbers, essential for cryptography.

How has funding influenced research and the evolution of technology?

Since the 1980s, the landscape has transformed dramatically. Initially, there was uncertainty about manipulating single quantum systems, but quantum computing has since blossomed into a vast field. It’s gratifying to see so many physicists employed to unravel the complexities of superconducting quantum systems.

Your involvement during quantum computing’s infancy gives you a unique perspective on its trajectory. How does that inform your current work?

Having long experience in the field, I possess a deep understanding of the fundamentals. My team at UC Santa Barbara developed early microwave electronics, and I later contributed to foundational cooling technology at Google for superconducting quantum computers. I appreciate both the challenges and opportunities in scaling these complex systems.

Cryostat for Quantum Computers

Mattia Balsamini/Contrasto/Eyeline

What changes do you believe are necessary for quantum computers to become practical? What breakthroughs do you foresee on the horizon?

After my tenure at Google, I reevaluated the core principles behind quantum computing systems, leading to the founding of QoLab, which introduces significant changes in qubit design and assembly, particularly regarding wiring.

We recognized that making quantum technology more reliable and cost-effective requires a fresh perspective on the construction of quantum computers. Despite facing skepticism, my extensive experience in physics affirms that our approach is on the right track.

It’s often stated that achieving a truly functional, error-free quantum computer requires millions of qubits. How do you envision reaching that goal?

The most significant advancements will arise from innovations in manufacturing, particularly in quantum chip fabrication, which is currently outdated. Many leading companies still use techniques reminiscent of the mid-20th century, which is puzzling.

Our mission is to revolutionize the construction of these devices. We aim to minimize the chaotic interconnections typically associated with superconducting quantum computers, focusing on integrating everything into a single chip architecture.

Do you foresee a clear leader in the quest for practical quantum computing in the next five years?

Given the diverse approaches to building quantum computers, each with its engineering hurdles, fostering various strategies is valuable for promoting innovation. However, many projects do not fully contemplate the practical challenges of scaling and cost control.

At QoLab, we adopt a collaborative business model, leveraging partnerships with hardware companies to enhance our manufacturing capabilities.

If a large-scale, error-free quantum computer were available tomorrow, what would your first experiment be?

I am keen to apply quantum computing solutions to challenges in quantum chemistry and materials science. Recent research highlights the potential for using quantum computers to optimize nuclear magnetic resonance (NMR) experiments, as classical supercomputers struggle with such complex quantum issues.

While others may explore optimization or quantum AI applications, my focus centers on well-defined problems in materials science, where we can craft concrete solutions with quantum technologies.

Why have mathematically predicted quantum applications not materialized yet?

While theoretical explorations in qubit behavior are promising, real-life qubits face significant noise challenges, making practical implementations far more complex. Theoretical initiatives comprehensively grasp theory but often overlook the intricacies of hardware development.

Through my training with John Clark, I cultivated a strong focus on noise reduction in qubits, which has proven beneficial in experiments showcasing quantum supremacy. Addressing these challenges requires dedication to understanding qubit design intricacies.

As we pursue advancements, a dual emphasis on hardware improvements and application innovation remains crucial in the journey to unlock quantum computing’s full potential.

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Source: www.newscientist.com

Hurricane Melissa: One of the Most Powerful Atlantic Storms Ever Recorded

Satellite image capturing Hurricane Melissa on October 28th

Associated Press/Alamy Stock Photo

Jamaica is experiencing severe impacts from Hurricane Melissa, which is forecasted to be the most powerful hurricane to strike the Atlantic Ocean, bringing up to 1 meter (40 inches) of rainfall. It is virtually certain that global warming has intensified Hurricane Melissa.

According to studies, the warm waters that fueled the storm’s rapid intensification are 500 to 700 times more likely to be influenced by climate change. This was highlighted by Daniel Guilford and his team at Climate Central, a non-profit based in the US.

“The figure of ‘500 to 700 times more likely’ is substantial,” Guilford noted. “This clearly indicates that the extreme temperatures witnessed around Melissa wouldn’t be possible without human-induced climate change.”

Tropical cyclones like Melissa derive their energy from warm ocean waters. When storms pass over warmer surfaces, more water vapor is generated. As this moist, warm air rises and cools, condensation occurs, releasing latent heat. This process generates energy that fuels tropical cyclones.

In the central Caribbean, where Melissa rapidly intensified into a Category 5 hurricane, sea surface temperatures were recorded at 1.4 degrees Celsius (2.5 degrees Fahrenheit) higher than typical for October. These elevated temperatures extend to significant depths, resulting in an abundance of thermal energy within the oceans.


As Melissa stirs the ocean, sea surface temperatures remain elevated, bringing deeper, warmer water to the surface. Conversely, if only a shallow warm layer exists, colder water rises, depleting the storm’s energy.

“Hurricane Melissa is shaping up to be a perfect storm. The warm ocean has been rapidly escalating in intensity recently, while its slow movement could lead to extensive rainfall as it makes landfall,” said Lianne Archer, a researcher at the University of Bristol in the UK. “These conditions are largely intensified by the additional heat present in the oceans and atmosphere driven by climate change.”

The combination of strong winds and heavy rainfall poses a severe threat to Jamaica. Reports indicate that three individuals have already lost their lives as preparations continue for the storm, anticipated to make landfall around 11 a.m. or 12 p.m. local time.

“This presents one of the most alarming scenarios,” commented Hannah Cloke, a researcher from the University of Reading in the UK. “The nation will bear deep and lasting scars from this storm, making recovery a challenging endeavor for impacted regions.”

Historical studies of past disasters indicate that such events can stifle economic growth for years. Though some economists speculate a quick recovery could spur growth, this notion has often proven to be unfounded.

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Source: www.newscientist.com

Why Hurricane Melissa Ranks Among the Most Powerful Atlantic Storms in History

Satellite image of Hurricane Melissa captured on October 28

Associated Press/Alamy Stock Photo

Jamaica is facing severe impacts from what is possibly the strongest hurricane to hit the Atlantic Ocean. Current forecasts predict up to 1 meter (40 inches) of rainfall. There’s little doubt that global warming has intensified Hurricane Melissa.

According to the authors, the warm waters that sped up Melissa’s intensification are 500 to 700 times more likely due to climate change. Initial assessments by Daniel Guilford and his colleagues at Climate Central, a U.S. non-profit organization, reveal this.

“‘500 to 700 times more likely’ is an astonishing figure,” Guilford stated. “This clearly indicates that the extreme temperatures observed around Melissa would not be feasible without human-induced climate change.”

Tropical storms like Melissa draw their energy from warm ocean waters. The hotter the sea surface, the more water vapor is generated when a storm passes above it. As the warm, moist air rises, the vapor condenses and releases latent heat, warming the air and encouraging further condensation. This process fuels tropical cyclones.

In the central Caribbean, where Melissa rapidly intensified into a Category 5 hurricane, sea surface temperatures were 1.4 degrees Celsius (2.5 degrees Fahrenheit) above the October average. Since these extreme temperatures penetrate to significant depths, there is abundant excess thermal energy available in the ocean.

This indicates that sea surface temperatures remain elevated as Melissa churns the ocean and draws up cooler, deeper water. Conversely, if only a thin layer of warm water exists, the storm brings up cold water, cutting off its energy supply.

“A perfect storm continues to build for Hurricane Melissa. The warm ocean has been rapidly strengthening over recent days, and its slow movement may bring additional rainfall as it makes landfall,” stated Lian Archer, a researcher at the University of Bristol in the UK. “Many of these conditions are being exacerbated by heightened heat in the oceans and atmosphere attributable to climate change.”

The combination of powerful winds and extreme rainfall poses a significant risk of severe damage to Jamaica. So far, three lives have been lost as preparations for the storm continue, which is expected to make landfall around 11 a.m. or noon local time.

“This is one of the most troubling scenarios,” remarked Hannah Cloke, a researcher at the University of Reading in the UK. “The entire nation will suffer long-term and potentially permanent damage from this storm, and recovery will require significant effort for those affected.”

Research into past disasters suggests that such events can depress economic growth for decades. While economists propose that quicker recovery or even growth driven by recovery efforts is possible, these notions have generally proven to be overly optimistic.

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Source: www.newscientist.com

What Makes Quantum Computers So Powerful?

3D rendering of a quantum computer’s chandelier-like structure

Shutterstock / Phong Lamai Photography

Eleven years ago, I began my PhD in theoretical physics and honestly had never considered or written about quantum computers. Meanwhile, New Scientist was busy crafting the first “Quantum Computer Buyer’s Guide,” always ahead of its time. A glance through reveals how things have changed—John Martinis from UC Santa Barbara was recognized for developing an array of merely nine qubits and earned a Nobel Prize in Physics just last week. Curiously, there was no mention of quantum computers built using neutral atoms, which have rapidly transformed the field in recent years. This sparked my curiosity: how would a quantum computer buyer’s guide look today?

At present, around 80 companies globally are producing quantum computing hardware. My reporting on quantum computing has allowed me to witness firsthand how the industry evolves, complete with numerous sales pitches. If choosing between an iPhone and an Android is challenging, consider navigating the press lists of various quantum computing startups.

While there’s significant marketing hype, the challenge in comparing these devices stems from the lack of a clear standard for building quantum computers. For instance, potential qubit options include superconducting circuits, cryogenic ions, and light. With such diverse components, how does one assess their differences? This aspect will hone in on each quantum computer’s performance.

This marks a shift from the early days, where success was measured by the number of qubits—the foundational elements of quantum information processing. Many research teams have surpassed the 1000-qubit threshold, and the trajectory for achieving even more qubits appears to be becoming clearer. Researchers are exploring standard manufacturing methods, such as creating silicon-based qubits, and leveraging AI to enhance the size and capabilities of quantum computers.

Ideally, more qubits should always translate to greater computational power, enabling quantum computers to tackle increasingly complex challenges. However, in reality, ensuring each additional qubit doesn’t impede the performance of existing ones presents significant technical hurdles. Thus, it’s not just the number of qubits that counts, but how much information they can retain and how effectively they can communicate without losing data accuracy. A quantum computer could boast millions of qubits, but if they’re susceptible to errors that disrupt computations, they become virtually ineffective.

The extent of this “glitch” or noise can be measured by metrics like “gate fidelity,” which reflects how accurately a qubit or pair can perform operations, and “coherence time,” which gauges how long a qubit can maintain a viable quantum state. However, we must also consider the intricacies of inputting data into a quantum computer and retrieving outcomes, despite some favorable metrics. The growth of the quantum computing industry is partly attributed to the emergence of companies focused on qubit control and interfacing quantum internals with non-quantum users. A thorough buyer’s guide for quantum computers in 2025 should encompass these essential add-ons. Choosing a qubit means also selecting a qubit control system and an error correction mechanism. I recently spoke with a researcher developing an operating system for quantum computers, suggesting that such systems may become a necessity in the near future.

If I were to create a wish list for the short term, I would favor a machine capable of executing at least a million operations: a million-step quantum computing program with minimal error rates and robust error correction. John Preskill from the California Institute of Technology refers to this as the “Mega-Quop” machine. Last year, he expressed confidence that such machines would be fault-tolerant and powerful enough to yield scientifically significant discoveries. Yet, we aren’t there yet. The quantum computers at our disposal currently manage tens of thousands of operations, but error correction has only been effectively demonstrated for smaller tasks.

Quantum computers today are akin to adolescents—growing toward utility but still faced with developmental challenges. As a result, the question I frequently pose to quantum computer vendors is, “What can this machine actually accomplish?”

In this regard, it’s vital to compare not only various types of quantum computers but also contrast them with classical counterparts. Quantum hardware is costly and complex to manufacture, so when is it genuinely the sole viable solution for a given issue?

One method to tackle this inquiry is to pinpoint calculations traditional computers cannot resolve without unlimited time. This concept is termed “quantum supremacy,” and it keeps quantum engineers and mathematicians consistently preoccupied. Instances of quantum supremacy do exist, but they raise concerns. To be meaningful, such cases must be applicable, facilitating the construction of capable machines that can execute them, while also being demonstrable enough for mathematicians to assure that no conventional computer could compete.

In 1994, physicist Peter Shor devised a quantum computing algorithm for factoring large numbers, a technique that could potentially compromise the prevalent encryption methods utilized by banks worldwide. A sufficiently large quantum computer that could manage its own errors might execute this algorithm, yet mathematicians have yet to convincingly demonstrate that classical computers can’t efficiently factor large numbers. The most prominent claims of quantum supremacy often fall into this gray area, with some eventually being outperformed by classical machines. Ongoing demonstrations of quantum supremacy appear currently to serve primarily as confirmations of the quantum characteristics of the computers accomplishing them.

Conversely, in the mathematical discipline of “query complexity,” the superiority of quantum solutions is rigorously demonstrable, but practical algorithms remain elusive. Recent experiments have also introduced the notion of “quantum information superiority,” wherein quantum computers solve tasks using fewer qubits than traditional computers would require, focusing on the physical components instead of time. Though this sounds promising—indicating that quantum computers may solve problems without extensive scaling—they are not recommended for purchase simply because the tasks in question often lack pivotal real-world applications.

It’s undeniable that several real-world challenges are well-suited for quantum algorithms, like understanding molecular properties relevant to agriculture or medicine, or solving logistic issues like flight scheduling. Yet, researchers lack full clarity on these applications, often opting to state, “it seems.”

For instance, recent research on the prospective applications of quantum computing in genomics by Aurora Maurizio from the San Raffaele Scientific Institute in Italy and Guglielmo Mazzola at the University of Zurich suggests that traditional computing methods excel so significantly that “quantum computing may, in the near future, only yield speedups for a specific subset of sufficiently complex tasks.” Their findings indicate that while quantum computers could potentially enhance research in combinatorial problems within genomics, their application needs to be very precise and calculated.

In reality, for numerous issues not specifically designed to demonstrate quantum supremacy, there exists a spectrum in what constitutes “fast,” particularly when one considers that quantum computers might ultimately run algorithms quicker than classical computers, despite overcoming noise and technical challenges. However, this speed may not always offset the hardware’s significant costs. For example, the second-best-known quantum algorithm, Shor’s search algorithm, offers a non-exponential speedup, reducing computation time at a square root level instead. Ultimately, the question of how fast is “fast enough” to justify the transition to quantum computing may depend on individual buyers.

While it’s frustrating to include this in a purported buyer’s guide, my discussions with experts indicate that there remains far more uncertainty about what quantum computers can achieve than established knowledge. Quantum computing is an intricate, costly future technology; however, its genuine added value to our lives remains vague beyond serving the financial interests of a select few companies. This might not be satisfying, but it reflects the unique, uncharted territory of quantum computing.

For those of you reading this out of the desire to invest in a powerful, reliable quantum computer, I encourage you to proceed and let your local quantum algorithm enthusiast experiment with it. They may offer better insights in the years to come.

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Source: www.newscientist.com

Powerful Image Captures the Hidden Struggles of Southeast Asia’s Fishing Industry

Fishermen unload their catch in the Philippines

Nicole Tung

These striking images capture the efforts of photographer Nicole Tung, who dedicated nine months to documenting the human and environmental toll of overfishing in Southeast Asia. Since the 1950s, fishing has rapidly evolved from a traditional craft into a global industry, primarily in developed nations. The rise in overfishing and illegal catch practices is alarming, driven by the increasing demand from a growing population.

Tung emphasizes the significance of the region as a vital part of the global fisheries market. Her project received funding from the €50,000 Kaminyak Photojournalism Award for fieldwork, which shifted her perspective on seafood consumption. Rather than suggesting complete abstention, she advocates for greater awareness and informed choices from consumers.

She expressed her distress over harrowing accounts from Indonesian fishermen, who detailed the violence and dreadful conditions they encounter at sea.

The image above illustrates a fisherman delivering a catch of tuna at General Santos fishport in the Philippines after a month at sea, including Bigger Tuna and Blue Marlin.

Thai dock worker

Nicole Tung

In other scenes, dock workers from Myanmar sort fish species being offloaded in Ranong, Thailand. Below, the indigenous Ulak Roy people and Thai villagers from Koh Lipe gather wood from nearby islands during a festival celebrating the end of the fishing and tourism season. They utilize the materials to construct ceremonial boats as offerings to their ancestors.

Indigenous Urak Lawoi people and Thai villagers sail their boats in Thailand

Nicole Tung

In this concluding image, a family of Filipino fishermen prepares bait for their fishing line in Quezon, Palawan, Philippines.

Family preparing to fish in the Philippines

Nicole Tung

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Source: www.newscientist.com

Blowwinner Review: Engaging and Powerful Books Uncover the Biases That Influence Our Lives

Despite significant changes since the 1950s, women continue to shoulder more domestic responsibilities

ClassicStock/Alamy

Earn money
Melissa Hogenboom (Canongate Books, August 14th, UK)

Why do individuals without jobs feel uplifted when their partners are unemployed? How do women develop empathy as they mature? Why does a disordered room appear untidy when it belongs to Jennifer, but not John? These pressing issues are explored by Melissa Hogenboom in her book Earn money: and other power imbalances that affect your life. The book uncovers the hidden power dynamics and subconscious cognitive biases that influence our behaviors and choices.

This narrative goes beyond individual actions; it serves as a well-researched examination of how stereotypes and unseen disparities shape everything from household chores to career advancement.

Fair warning: it may provoke anger—especially regarding household responsibilities. Studies indicate that in heterosexual relationships, domestic duties are typically assumed by women unless addressed directly. Women tend to take on more odd jobs, even when they log more hours at work. Hogenboom notes that some studies imply this might be an unconscious “compensation” strategy for unconventional family dynamics.

Gender biases begin early in life. Mothers engage more extensively during pregnancy, whereas fathers share more about their feelings with daughters and their achievements with sons. Studies have found that fathers react more deeply to their daughters’ emotions.

This reinforces the notion that women are inherently nurturing or empathetic—a stereotype that influences various realms, from parenting to leadership roles. In fact, while empathy can be partially genetic, there are no innate differences between genders.

When societal pressures are lifted, a new truth may surface. As highlighted in a case study of same-sex male couples, “The assumption that if parents remain at home without societal pressures, they will naturally share childcare responsibilities is quite misguided,” says one participant. “If my partner had suggested returning to work within a fortnight, I would have been furious.”

Hogenboom also points out that mothers in same-sex relationships may encounter fewer career obstacles after maternity leave compared to those in heterosexual partnerships, indicating that maternity alone does not dictate such penalties.

The myth of mutuality deludes couples that they have achieved a good balance of labor.

The book sheds light on the intangible forces predominantly managed by men: hidden inequalities often perceived as normal. At times, Hogenboom asserts, “Women, here’s the evidence you need to justify your exhaustion.”

Notably, the persistent challenges faced by men who seek to address these power disparities are highlighted. A study referenced by Hogenboom found that men requesting part-time roles often face skepticism more than women and encounter taunts like “Where’s your mom?” They often struggle to be taken seriously and may be viewed as less committed, complicating their social dynamics within parenting communities.

Couples who believe they have achieved equality might be surprised by how Hogenboom reveals these unseen dynamics of authority. She argues that systematic inequalities represent a dominant form of power in relationships, often overlooked—even by the couples who experience them.

The perception of mutuality can lead couples to falsely believe they maintain an even distribution of responsibilities. However, they may be deceiving themselves if they don’t consider whose needs are genuinely met and who does the work. For instance, your partner might “cook all the meals,” but have you handled the meal planning, grocery shopping, cleaning, and budgeting?

Fortunately, Hogenboom offers actionable advice. If you find yourself overwhelmed, she suggests handling tasks comprehensively: “It eliminates hidden burdens when ownership of the entire task is taken.”

Her recommendations provide a much-needed relief amidst the wealth of data presented. While authoritative and insightful, Hogenboom’s writing style leaves little room for reflection.

However, moments of reflection are necessary. Earn money constructs a convincing argument to recognize the influence of concealed power dynamics and informs how to address them. This leads to fairer relationships and more successful careers, potentially saving marriages.

Helen Thomson is an author based in London.

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Source: www.newscientist.com

Don’t Miss This Review: A Powerful and Heart-Wrenching Critique of Social Media’s Harsh Realities | Movies

“The internal documents disclosed to Congress by Facebook whistleblowers suggest that “Weens are herd animals,” with references to “the stories” of the addicts that highlight a strong irony and obfuscation. Snapchat seems to have shifted its focus in its efforts to expand its user base.

Drawing from the investigative work of Bloomberg journalist Olivia Carville, this film discusses the endeavors of Minnow’s legal team in seeking justice for social media victims, confronting the predatory practices of Silicon Valley. It tells the harrowing stories of families devastated by extreme online content. This includes children or teenagers who tragically replicated dangerous self-harm or suicide methods from videos, or those who lost their lives after encountering online predators. The struggle here involves challenging Section 230, a legal shield established in the Telecommunications Act of 1996. Meanwhile, Mark Zuckerberg continues to engage in harmful practices.

The Center’s founder, Matthew Bergman, has compared social media companies to tobacco firms, alleging that these companies put profit above user well-being. While the film effectively illustrates this connection and the consequent harm, it doesn’t imply that the path to accountability is straightforward. Gaining justice for individual cases and proving that tech companies deliberately design their algorithms to provoke our darker tendencies and impulses represents a significant challenge. A crucial goal is to prevent the dismissal of the Snapchat case due to Section 230. This may appear as a minor victory, but it’s a necessary first step. This narrative is a vital piece of public journalism that articulates what many of us only sense.


“Don’t Look Away” is set to shock audiences in British cinemas starting August 8th.

In the UK, youth suicide charity Papyrus offers support at 0800 068 4141 or via email at pat@papyrus-uk.org. The Samaritans can be reached at Freephone 116 123 or by emailing jo@samaritans.org or jo@samaritans.ie. In the US, you can contact the National Suicide Prevention Lifeline at 988 or chat for support. Alternatively, text 741741 to connect with a crisis counselor. In Australia, call Lifeline at 13 1114. For other international helplines, visit befrienders.org.

Source: www.theguardian.com

Research Reveals That 14,350 Years Ago, the Most Powerful Known Solar Storm Triggered Radiocarbon Spikes

Solar particle events from the sun are infrequent but powerful, significantly influencing the creation of cosmic genic isotopes. For instance, radiocarbon (14c) in the terrestrial environment leaves a distinct mark on natural archives, such as dating artifacts. Over the last 12,000 years, eight such events have been identified, the most notable occurring in 775 AD. Recently, a candidate for a new extreme solar particle event was discovered, marked by the largest known radiocarbon peak dating back to 12350 BC. A recent study indicates this event was 18% more intense than the 775 CE event and likely transpired between January and April of that year, with early March being the most probable time frame.

Illustration of the artist of Solar Storm. Image credit: NASA.

“Solar particle storms significantly enhance the natural production of cosmic isotopes, such as radiocarbon, in the atmosphere due to cosmic rays from galaxies,” stated Kseniia Golubenko, a postdoctoral researcher at the University of Oulu, along with her colleagues.

“Such enhancements, preserved in annual tree rings, act as clear timestamps in the universe, enabling absolute dating of tree samples.”

“These dramatic spikes, referred to as Miyake Events, are named after the Japanese researcher who first identified them. They provide crucial data for scientists examining solar activity, ancient Earth systems, and space climate.”

“Miyake events help us pinpoint the exact calendar year of floating archaeological timelines,” added Professor Ilya Usoskin from Oulu University.

“The radiocarbon signals from such events have enabled researchers to accurately date Viking settlements in Newfoundland and Neolithic communities in Greece.”

For the reconstruction of solar particle storms under ancient glacial climate conditions, the authors developed and utilized a new chemical climate model called SOCOL:14C-EX.

This model was successfully validated using tree ring data from the 775 CE event and applied to ice age conditions to analyze the event from 12350 BC.

“The ancient events of 12350 BC are the only known extreme solar particle occurrences aside from the stable warm climate of the last 12,000 years,” Dr. Golubenko stated.

“Our estimates reveal that, compared to the largest events of the modern satellite era, the Particle Storm of 2005 was over 500 times weaker.”

“Other documented solar particle storms took place in 994 BC, 663 BC, 5259 BC, and 7176 BC, with several more candidates currently under investigation.”

“The 12350 BCE occurrence also establishes new worst-case scenarios,” she added.

“Understanding its magnitude is vital for assessing the risks posed by future solar storms.”

The team’s paper was published in the journal Earth and Planet Science Letters.

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Kseniia Golubenko et al. 2025. The new SOCOL:14C-EX model reveals that radiocarbon spikes from the late glacial age of 12350 BC were caused by record extreme solar storms. Earth and Planet Science Letters 661:119383; doi:10.1016/j.epsl.2025.119383

Source: www.sci.news

What Defines a Kentucky Derby Champion? A Big Heart, Powerful Lungs, and Strong Legs

Horses have honed their abilities, such as running, jumping, and pulling, as humans have bred and trained them for various purposes over thousands of years. The 151st Derby, the most-watched horse racing event, not only highlights the skills of these animals but also raises concerns about their treatment and well-being. Advocates have long voiced worries about injuries and fatalities, especially after twelve horses died at Churchill Downs two years ago.

There’s no doubt that the relationships between humans and horses have transformed warfare, agriculture, and society.

Timothy Winegard, a historian at Colorado Mesa University and author of the recent book, The Horse, remarked, “We’ve combined our intellect with the horse’s size, strength, stamina, and speed to create the most unstoppable animal coalition.”

Why Are Horses So Powerful?

The horse’s heart and lungs contribute significantly to its remarkable power.

Hearts typically weigh between 10-12 pounds (4.5-5.4 kg), roughly 1% of the horse’s body weight, compared to about 0.5% for a typical human heart. The famous horse Secretariat, who won the Triple Crown in 1973, was later found to have a heart weighing over 20 pounds (9.1 kg).

A horse’s heart is designed for exercise, with a resting heart rate around 34 beats per minute that can rise to 220 or 240 during a race—much faster than a human’s maximum during intense exertion.

Derma Sotogake training on the mornings of the 2023 Kentucky Derby.
Andy Lions/Getty Images

“One unique aspect of horses is their incredible capacity to circulate blood throughout their bodies. They can achieve high heart rates while remaining safe,” explained Sarah Reed, a researcher at the University of Connecticut.

Additionally, horses possess a lung capacity of 60 liters, ten times that of a human.

“This extensive lung capacity allows oxygen to efficiently transfer from the air to the blood, which is essential for sustaining aerobic energy,” noted Farmer.

Recent research published in the journal Science indicates that genetic mutations enable horses to mitigate the adverse effects associated with ultra-high energy production.

“Horses are exceptional athletes because they can deliver significantly more oxygen to their muscles than elite Olympic athletes. They have larger energy reserves and more efficient systems…and these mutations play a role in both aspects.”

What Contributes to a Horse’s Speed and Skills?

Various biological characteristics enhance a horse’s abilities.

Horses store excess red blood cells in their spleens, which are released to enhance oxygen transport during intense exertion.

“During exercise, adrenaline triggers the spleen to circulate these excess red blood cells,” said veterinarian Hillary Clayton. “Essentially, what a horse accomplishes is a form of ‘natural blood doping.’”

Honoring Marie at Churchill Downs in 2024.
Charlie Riedel / AP

Furthermore, a horse’s brain is adept at processing sensory information and reacting swiftly. Although their frontal lobe—the section associated with thinking and planning—is proportionally smaller than that of humans, horses are hardwired for play and independent running without fear, as explained by Dr. Scott Bailey, a veterinarian at Clayborne Farm. This focus is critical for athletic performance.

The bone structure and muscle makeup are also advantageous. The ligaments and tendons in their hind legs function like springs, and as Farmer noted, like other large prey animals, they possess “long, slender legs designed for running.”

What Are the Risks for Horses?

Adjustments that enhance a horse’s speed also increase the risk of injuries. Their slender legs endure the impact of each stride, and over time, repetitive stress during racing and training can lead to tendon and ligament damage, Reed stated.

In 2023, fatalities occurred not only at Churchill Downs but also at other major racecourses, affecting public perceptions of the sport and prompting changes. No specific cause of death was identified. However, in 2024, Churchill Downs improved the equipment used on its racing surfaces and added a veterinarian dedicated to horse safety and integrity.

Source: www.nbcnews.com

Astronomers report powerful winds of materials from central black hole in NGC 4945

Astronomers using the Muse Instrument with ESO’s extremely large telescope (VLT) detected ultra-large black hole-driven winds with the Burred Spiral Galaxy NGC 4945.

This image shows NGC 4945, a spiral galaxy that exceeds 12 million light-years in the constellation of Centaurus. The super-large black hole-driven wind of the NGC 4945 is shown in red in the inset. Image credits: ESO/Marconcini et al.

NGC 4945 It is more than 12 million light years away from Earth, the constellation of Centaurus.

Otherwise known as the Caldwell 83. That’s what this galaxy was like I discovered it by James Dunlop, the Sottsch astronomer in 1826.

NGC 4945 hosts one of the closest active, ultra-large black holes to Earth.

“At the heart of almost every galaxy, they are very large black holes,” the ESO astronomer explained in a statement.

“Some people are not particularly hungry, as they are in the heart of our own Milky Way.”

“However, the super-large black hole in NGC 4945 is greedy and consumes a huge amount of problems.”

Astronomers have studied the ultra-high Massive black holes of the NGC 4945 using the Muse Instrument, an ESO’s extremely large telescope (VLT).

“Contrary to the all-consuming reputation typical of black holes, this messy eater is blowing away the powerful winds of ingredients,” they said.

“This cone-shaped wind is shown in red in the inset and is covered in a wider image taken with La Silla’s MPG/ESO telescope.”

“In fact, this wind moves so fast that it completely escapes the galaxy, giving in to space in intergalactic space.”

“This is part of a new study measuring how the wind moves in several nearby galaxies,” they added.

“Muse’s observations show that these incredibly fast winds show strange behavior. They actually speed up far from the central black hole, and accelerate even further on their journey to the outskirts of the galaxy.”

“This process suggests that black holes control the fate of the host galaxy by ejecting potential star-forming material from the galaxy and attenuating the star’s fertility.”

“It also shows that more powerful black holes can hamper their own growth by removing the gas and dust they feed, bringing the entire system closer to a kind of galactic equilibrium.”

“Now, these new results bring us one step closer to understanding the mechanisms of wind acceleration that are responsible for galaxy evolution and the history of the universe.”

Survey results It will be displayed in the journal Natural Astronomy.

____

C. Marconcini et al. Evidence of rapid acceleration of AGN-driven winds at the Kiloparsec scale. Nut Athlonreleased on March 31, 2025. doi:10.1038/s41550-025-02518-6

Source: www.sci.news

New research suggests that the powerful Marzcake shock can travel to even more distant red planets than believed.

In new research, researchers on the planetary Used Global and high -resolution orbital images to discover fresh 21.5 m (71 feet) impact craters that appeared at the same time as one of the Marsquakes detected by NASA's Insight Lander. This means that the seismometer detected a meteor strike, not a geological activity in the planet. In the related research, they scan Through a large number of orbital image data, the 123 shock crater was formed from December 2018 to December 2022.

Calambus et al。 Textonically Active Cerberus Fossae A new 21.5-m MARS Impact Crater is associated with the Insight earthquake event S0794A. Image credit: NASA / JPL-CALTECH / Arizona University.

NASA's Insight Lander set the first seismometer on Mars and detected more than 1,300 Marsquakes. This is generated by the shaking deep of the planet (caused by a rock broken under heat and pressure) and a cosmic rock that collides with the surface.

Scientists not only glimpse the inside of Mars, as science glimpses how the waves of the earthquake change from these earthquakes when passing through the earth's crust, mantle, and core. I understand how all the rocky world, including the month, is formed.

In the past, researchers shot new shock craters images and found seismic data that matched the date and location of the crater layer.

However, two new studies indicate that the shaking and the new effects detected in Cerberus Fossae, which are particularly prone to earthquakes of 1,640 km (1,019 miles) of 1,640 km (1,019 miles) from insights, are the first correlation. Masu.

The diameter of the shock crater is 21.5 m, which is far from the insight than the scientist expected, based on earthquake energy.

Mars crusts have unique characteristics that are considered to suppress seismic waves generated by impact. The new analysis of Cerberusfossae concluded that the generated waves take more direct routes than the planet mantle.

The Insight team needs to re -evaluate the internal configuration and structural models of Mars, and explain how to make the impact -generated earthquake signals so deep.

“We thought that the energy detected from most of the earthquake events was moving through the crust of Mars,” said Dr. Constantinoscharamanbus, a researcher of Imperial College London. Masu.

“This discovery shows a deeper and faster path -it is called an earthquake highway, so that the earthquake can reach the farthest of the earth through the mantle.”

Researchers also wanted to find a crater within the location of about 3,000 km (1,864 miles) and find something that was formed while the Lander seismometer was recorded.

By comparing images before and after the context camera mounted on NASA's Mars Reconnasance Orbiter (MRO), I found 123 fresh craters to interact with INSIGHT data. Of these, 49 was a potential agreement with the earthquake detected by the Lander seismometer.

“I thought that CERBERUS FOSSAE has generated many high -frequency earthquake signals related to internal generated earthquakes, which suggests that some activities are not born there, and actually from the impact. Dr. Charalambous said.

The results of the survey also emphasize how researchers use AI to improve planetary science by using all data collected by NASA and ESA missions.

“Now, we have a lot of images from the moon and Mars, so the struggle is to process and analyze data,” said Dr. Dr., a member of the Bern University researcher. I mentioned it.

“We have finally arrived in the big data era of planetary science.”

Two new papers are posted journal Global physics research book

______

VT BICKEL et al。 2025. New impact on Mars: Related to systematic identification and insight earthquake events. Global physics research book 52 (3): E2024GL109133; DOI: 10.1029/2024GL109133

Constantinos Chara Ranboo et al。 2025. New impact on Mars: Unleash CERBERUS FOSSAE's shock detection. Global physics research book 52 (3): E2024GL110159; DOI: 10.1029/2024GL110159

Source: www.sci.news

The Factors Behind Hurricane Milton’s Powerful Tornadoes

overview

  • Hurricane Milton’s tornado outbreak in Florida was the leading cause of death and damage from the storm.
  • On Wednesday, South Florida experienced one of the strongest tornadoes on record. Overall this year, the United States has seen an unusually high number of violent tornadoes associated with hurricanes.
  • Early research shows that in a warmer world, tropical cyclones can produce more tornadoes.

Hurricane Milton wreaked havoc earlier than expected before making landfall this week, as supercell thunderstorms featuring rotating updrafts and the potential to spawn tornadoes raced across the state.

The resulting twister caused the National Weather Service to issue 126 tornado warnings, and the agency The Storm Prediction Center has filed 45 preliminary reports of tornadoes..

In St. Lucie County, a tornado destroyed a retirement community and killed five people, accounting for nearly one-third of the 17 deaths reported so far in the aftermath of the hurricane.

As Florida begins the long process of recovering and recovering from Hurricane Milton, tornado outbreaks are causing deaths and damage in a state accustomed to tropical storms but less accustomed to powerful twisters. has emerged as the main cause.

One of the strongest tornadoes in South Florida history occurred on a day that will likely go down in Florida history as one of the worst tornado outbreaks ever observed in Florida during a cyclone.

Swirling winds reached 160 miles per hour in Palm Beach Gardens, tearing apart concrete walls and tearing off large sections of roofs from new homes. Breaking news from the National Weather Service.

“This is the first EF-3 on record for the South Florida area south of Lake Okeechobee,” said Donal Harrigan, NWS meteorologist in Miami. EF-3 refers to tornadoes with estimated wind speeds of 136 to 160 miles per hour (EF stands for Enhanced Fujita Scale; Started operation at the National Weather Service in 2007).

Harrigan added that several other observed twisters may be rated EF-3 after damage assessment.

“You can probably count on one hand how many EF-3s have been in this state historically, potentially multiple times a day,” he said.

Overall this year, the United States has seen an unusually high number of powerful tornadoes associated with hurricanes.

Tornadoes are common when hurricanes make landfall, but most are on the weaker end of the spectrum. Less than 1% of tornadoes associated with tropical systems that make landfall are rated EF-3 or higher. By contrast, four out of five hurricanes that made landfall in the United States this year produced tornadoes with EF-3 strength.

From 1995 to 2023, only five tornadoes caused by tropical cyclones received such high ratings.

A home is destroyed in Lakewood Park, Florida, on Thursday, a day after a tornado struck the area.Giorgio Vieira/AFP – Getty Images

Early research suggests that tropical cyclones could produce more tornadoes in a warmer world. In a study published in June, researchers modeled hurricanes Ivan, Katrina, Rita, and Harvey in a warmer future climate. Their results show that the number of potential tornado storms caused by a tropical cyclone is 56% to 299% increase by mid-century Assuming the pace of fossil fuel pollution remains steady.

It is not yet known whether climate change played a role in the twisters associated with this year’s storms. But Bill Gallus, an author of the June study and a professor of meteorology at Iowa State University, said “it was really unusual that conditions in South Florida were this volatile” during Milton.

A situation is considered unstable if, due to differences in density and temperature, a mass of air rises or falls rapidly, which means that thunderstorms can form.

“When I looked at the instability graph, I was shocked. It was about as high as you’d see in Kansas chasing storms,” ​​Gallus said. “Hurricanes have produced more tornadoes, but Florida alone has never produced so many tornadoes.”

He added that this type of instability is “expected to become more common” in a warming world.

One reason Milton produced so many tornadoes is that hurricane thunderstorms traveled far from the center.

“With the first tornado, it looked like a certain band of showers and storms from Milton were actually erupting well in front of the hurricane,” Gallus said.

The outer storm belt eventually became isolated and ended without interference from other systems. Those were thunderstorms that produced tornadoes. This is a reminder that hurricanes can become a threat long before landfall and even far from the storm’s center, experts said.

Another important factor for Milton’s tornadoes is heat. The hurricane approached the Florida coast in the afternoon and encountered particularly warm conditions, as the thunderstorms were quite far away at the edge of the hurricane, in addition to wind shear (changes in wind direction and speed with altitude). This allowed it to grow stronger than a typical hurricane setup.

“There was plenty of time to warm up the atmosphere,” Gallus said. “Most hurricanes get very little heat from the sun. Tornadoes form under heavy rain and cover.”

In hurricanes like Milton, where winds blow counterclockwise, tornadoes tend to form on the leading edge of the storm and to its right, sometimes called the dirty side. This region is also the windiest.

How it unfolded during Milton, Gallus said, noting that the twister “started in the exact place you see most tornadoes form.”

But in Milton’s case, he noted, the tornadoes were particularly concentrated.

Because Milton crossed the Florida peninsula for a short distance, “the tornado area was small, and I think it was one of the most concentrated tornadoes ever produced by a hurricane,” Gallus said.

More research is needed into exactly how climate change will affect tornadoes produced by hurricanes. However, the impact of global warming on extreme rainfall is more certain and clear.

A report released Friday by the World Weather Attribution Project, a consortium of scientists considered an authority on analyzing extreme weather events and determining the impact of climate change on specific events, says: It turned out. Rainfall amounts for single-day events like Milton are currently about 20% to 30% higher due to climate change.. The analysis found that Milton’s wind speeds were likely 10% stronger due to climate change.

The researchers also found that Hurricane Helen was wetter and windier because of climate change. Separate preliminary reports say climate change is likely to increase Helen’s rainfall by up to 50% over three days in some of the worst-hit areas.

Source: www.nbcnews.com

Review of the Shokz OpenRun Pro 2: Enhancing Bone Conduction Headphones with Powerful Bass

SSo-called bone conduction headphones are a runner’s best friend, allowing you to stay fully aware of the outside world while listening to motivational music. But the technology doesn’t produce decent bass, a problem that open-ear headphone maker Shokz believes it has solved with its latest OpenRun Pro 2.


A successor to the popular OpenRun Pro and OpenSwim series, the OpenRun Pro 2 costs £169 (€199 / $175 / AU$299) and is similar to most of its competitors, with bone conduction pods secured in front of the ears by two loops and a band that wraps around the back of the head.

What makes these headphones unique is that the pods have open-air speakers built into them, allowing music to be streamed towards the outer ear. Bone conduction The speakers vibrate your cheekbones to send sound directly to your inner ear, while open-air speakers handle the bass and the rest of the sound is sent to the listener via bone conduction.

Open-air speakers emit sound from grilles in the pods that are located directly in front of the wearer’s ears. Photo: Samuel Gibbs/The Guardian

They don’t deliver the skull-shaking bass of larger over-ear headphones, but the OpenRun Pro 2 sounds fuller and rounder than its predecessor, and won’t send thumping noises through your cheeks even at louder volumes. Instruments, drums, and vocals have more depth, making them especially great for podcasts and dance tracks. The Shokz smartphone app offers an equalizer to fine-tune the sound of the headphones, as well as other updates and adjustments.

But the open-air speakers block out a lot more background noise than traditional bone-conduction headphones, significantly reducing awareness of cars, cyclists, and other runners. They’re still far better than earbuds or other headphones, but the difference was noticeable when listening at moderate volumes while running.

Only at 50% volume will nearby people be able to hear the music a little better than regular bone conduction earphones – they’re less noticeable than cheaper earphones and aren’t loud enough to be an issue when running.

specification

  • water resistance: IP55 (water-resistant)

  • Connectivity: Bluetooth 5.3 (SBC)

  • Battery life: 12 hr

  • size: 30.9 x 21.7 x 24.3mm

  • Weight: 30.3 g

  • driver: Air conduction and bone conduction

  • charging: USB-C

Bluetooth upgrade and comfortable fit

The USB-C charging port is hidden behind a rubber door to protect it from the elements. Photo: Samuel Gibbs/The Guardian

Another big upgrade from previous Shokz is support for Bluetooth 5.3 with multipoint, meaning you can connect two devices at the same time. This is especially useful if you want to connect to a running watch and a phone at the same time. You can even take a call while listening to music and lap guidance from the watch without stopping.

The headphones fit very well, with a nice balance between the front and back of the ears, and the back band is just the right amount of flexible, putting enough pressure on the sides of your head without being too restrictive. A mini version is also available for those who want a tighter fit.

The volume buttons are on the headphone body behind the right ear, and the multifunction button that controls playback is on the outside of the pod in front of the left ear. The microphone for calls is on the right pod and works well enough, although callers said my voice sounded a bit distant and quiet.

The battery lasts for 12 hours on a single charge and fully charges in about an hour via the USB-C port. The headphones are splash-resistant, so they’re fine for a sweaty run, but that doesn’t mean they’re safe to immerse in water.

The headphones come with a lightweight shell case for safe storage when traveling. Photo: Samuel Gibbs/The Guardian

Sustainability

Shokz claims that the batteries in the earbuds and case will retain at least 80% of their original capacity for 800 full charge cycles. Shokz does not offer trade-in, recycling or repair services, and the batteries cannot be replaced. The headphones do not contain any recycled materials, and the company has not released an environmental impact report.

price

The OpenRun Pro 2 costs £169 (€199 / $175 / AU$299).

By comparison, the Shokz OpenRun costs £130, the Suunto Wing costs £145, the Creative Outlier Free Pro+ costs £80 and the Bose Ultra Open earphones cost £250.

verdict

The OpenRun Pro 2 solves the bass-deficient issue of bone conduction headphones by adding open-air speakers that handle the bass.

They don’t deliver skull-shaking bass, but they deliver a rich sound that’s just as good as standard earphones, making them a marked improvement over previous earphones. The trade-off, however, is a slightly worse situational awareness at moderate volumes. This isn’t a deal-breaker for me, but if you like to listen to music loud while running, it might negate the point of buying bone conduction headphones.

The addition of Bluetooth multipoint, which lets you connect to two devices simultaneously, is a nice touch, as is the 12-hour battery life and the fact that charging is done via a standard USB-C cable rather than a proprietary port.

The Shokz are not cheap and are not suitable for general use as headphones, but the biggest problem is that they cannot be repaired and the battery is not replaceable, so they end up being disposable and lose a star.

Strong Points: Much rounder sound than bone conduction, open air recognition, splash proof, solid battery life, standard USB-C charging, Bluetooth multipoint, great for running.

Cons: They offer slightly less recognition than bone conduction alone, are expensive, don’t support high-quality Bluetooth audio formats, and are not repairable or have replaceable batteries.

Actual click buttons make it easy to adjust volume and control playback while working out. Photo: Samuel Gibbs/The Guardian

Source: www.theguardian.com

Completion of the world’s most powerful camera

SLAC National Accelerator Laboratory scientists and engineers have completed work on the most powerful camera ever created.

The Legacy Survey of Space and Time camera (LSST) boasts an impressive 3,200-megapixel capacity and is approximately the size of a small car, weighing around 3,000 kg. The installation of these cameras in the newly constructed Vera C. Rubin Observatory building will allow scientists to capture incredibly detailed images of the Southern Hemisphere’s skies over the next decade.

Multiple organizations were involved in the production of the camera. Brookhaven National Laboratory contributed a digital sensor array, Lawrence Livermore National Laboratory designed and built the lenses, and the Institute of Particle and Nuclear Research at the National Center for Scientific Research in France played a role as well.

With the completion of SLAC’s LSST camera and its integration with Rubin Observatory systems in Chile, the project is on track to produce comprehensive night sky maps. University of Washington professor Željko Ivezic, the Rubin Observatory construction director, emphasized the significance of this achievement.

The LSST camera team successfully attached the cryostat to the camera body on April 8, 2022 – Image courtesy of Travis Lange/SLAC National Accelerator Laboratory

The new camera’s capabilities are immense, including photographing the entire visible sky every few nights, potentially discovering billions of stars and galaxies over the next decade. It would require hundreds of ultra-high-definition TV screens to display a single image at full resolution.

The LSST camera is being installed facing the ground towards completion.Roughly the size of a small car and weighing 3 tons, the camera has a 5-foot-wide front lens, a 3,200-megapixel sensor, and is cooled to -100°C to reduce noise – Image credit : Jacqueline Ramseyer Orrell/ SLAC National Accelerator Laboratory

The camera’s detailed images of the Southern Hemisphere sky aim to fill gaps in previous space observations and provide insights into galaxy distribution, dark energy, dark matter, and other astronomical mysteries. By detecting weak gravitational lensing and studying the evolution of the universe, astronomers hope to gain valuable insights from this data.

Travis Lange, LSST camera deputy project manager, shines a flashlight on the completed LSST camera – Image credit: Jacqueline Ramseyer Orrell/SLAC National Accelerator Laboratory

Researchers believe the LSST camera could aid in the creation of more detailed maps of solar system objects and help identify near-Earth object threats. The installation of the camera at the Vera C. Rubin Observatory in Chile is expected to be completed soon.

A look inside the completed LSST camera – Image credit: Jacqueline Ramseyer Orrell/SLAC National Accelerator Laboratory
Most of the LSST camera team in a clean room with completed cameras, taken in January 2024 – Image credit: Jacqueline Ramseyer Orrell/SLAC National Accelerator Laboratory (Jacqueline Ramseyer Orrell/SLAC National Accelerator Laboratory)

Vera C. Rubin Observatory – the new home for cameras

The nearly completed Vera C Rubin Observatory is visible at sunset in January 2022 – Image credit: Vera C Rubin Observatory/NOIRLab/AURA/NSF/J Fuentes

Following the completion of the LSST camera, preparations are underway to transport it to the Vera C. Rubin Observatory atop a rugged Andean mountain pass. Its initial imaging is expected in early 2025, allowing the public to witness its capabilities by 2027.


The camera will be installed atop the Simoni Survey Telescope at the Vera C. Rubin Observatory high in the Chilean Andes – Image courtesy of Rubin Observatory/NSF/AURA

About our experts:

Željko Ivezic: With a PhD in physics from the University of Kentucky, Željko Ivezic’s expertise lies in electromagnetic radiation analysis and celestial body observation. He spearheads the Rubin Observatory/LSST project as the construction project director, bringing a wealth of experience in scientific research.

Read more:

Source: www.sciencefocus.com

Is the potential for more powerful electric bikes cause for concern over increased fire risk?

The UK Government has initiated a consultation to gather public and industry input on increasing the legal power of electric bike models from 250W to 500W in the UK. This move has sparked concerns in the fire protection community.

Electric bicycles utilize various types of batteries, with lithium-ion technology being the common choice. These batteries come in different shapes and sizes, such as cylindrical or box-shaped configurations.

Battery packs in electric bikes are composed of multiple cells connected in series and parallel to provide the necessary voltage and capacity. Incidents of fires linked to lithium-ion batteries are on the rise, posing risks to users of electric bikes and e-scooters.

Recent data disclosed in May 2023 by the Guardian newspaper revealed that defective electric bikes and e-scooters have caused injuries to 190 individuals and claimed eight lives in the UK. The London Fire Brigade noted a substantial increase in battery-related fires in 2023, with a rise of 78% compared to the previous year.

Potential causes of fires in lithium-ion batteries include mechanical or thermal shock, overcharging, and reactive materials interacting with each other, leading to heat generation and abnormal electrical behavior. Despite the benefits of higher wattage batteries in electric bikes, there are concerns about the increased risk of fires and other safety issues.

To mitigate the risk of battery fires, users are advised to avoid tampering with batteries, charge them within the recommended parameters, and store them in a safe environment away from flammable materials. Adherence to manufacturer guidelines and proper disposal of damaged batteries are crucial in preventing incidents of fires.

Source: www.sciencefocus.com

The most powerful laser ever created is “Sound Laser”

“Phonon laser” emits sound particles instead of light

Dmytro Radzinkov/Alamy

Tiny floating beads are the core of an unprecedentedly bright laser that fires particles of sound instead of light.

Just as light rays are made up of many particles called photons, sound is also made up of particle-like clumps called phonons. For decades, researchers have created “phonon lasers” that output these particles in narrow beams, similar to the way optical lasers emit photons.

Now, Hui Jin Researchers at Hunan Normal University in China have developed the brightest phonon laser ever.

The heart of their device was a silica bead about the size of a typical bacterium, roughly micrometers long. They used two beams of light to levitate a bead and surrounded it with a reflective cavity. The tiny vibrations of this bead generated phonons, which were captured and amplified within the cavity. This continued until there were enough phonons to form a laser-like beam.

Several research groups had previously tested similar designs. But Jin and his colleagues added electrodes directly beneath the beads to generate carefully selected electromagnetic signals. This modification increased the laser’s “brightness” (the amount of power delivered at each phonon frequency) by a factor of 10, making the beam tighter and longer lasting. Previous devices developed by Jin’s team and others could only operate for a few minutes, but the latest phonon lasers can operate for more than an hour.

Because phonons are less affected by traveling through liquids, they may be more effective than traditional lasers for imaging water tissue in biomedicine and some deep-sea monitoring devices, Jin said. To tell.

But Richard North Researchers from the Delft University of Technology in the Netherlands say the current experimental setup is too complex, requiring precise alignment of all components. Phonon lasers can require years of research and engineering before they can match the usefulness of comparable optical lasers.

“Given the impact optical lasers have had on modern life, there is excitement about phonon lasers, but only time will tell if they will have a comparable impact,” he says.

topic:

Source: www.newscientist.com

Powerful winter storm causes historic California palm tree to fall into ocean


Refugio State Beach, Calif. — Severe storms that hit California have caused damage in some parts of the state. the most iconic tree.

A majestic palm tree that normally flanks Refugio State Beach just north of Santa Barbara has fallen over the past few days. Images show how a huge 100-year-old tree fell into the sea and was completely uprooted.

Local officials say multiple factors caused the trees to fall. Years of coastal erosion were combined with powerful storm surges and supersaturated soil from a series of atmospheric rivers that brought heavy rain and high winds across the state.

“When the ground becomes saturated, the trees begin to fall, and both eucalyptus and palm trees fall over because the ground becomes too wet for their roots to hold in the ground.” Santa Barbara Craig Vanderswag, chief of the County Fire Battalion, told NBC News.

California State Parks Channel Coast District Superintendent Dena Bellman said officials have tagged several more trees on the coast as at high risk of falling, especially with the new heavy rains hitting California. Ta.

Due to this threat, the park is currently temporarily closed to the public.

The dramatic footage is a symbol of the power of these atmospheric rivers, which climate experts say is growing stronger as the planet's temperature rises.

Los Angeles received 75% of its annual average precipitation in the first three weeks of February alone. The city has received more rainfall than Seattle, New Orleans and Miami, and is about 2 inches away from setting a record for the wettest February.

Source: www.nbcnews.com

New Study Claims Megalodon Sharks Were Not as Powerful as Previously Believed

A recent study suggests that the megalodon’s body shape might not have been as chunky as previously thought. Contrary to popular belief, researchers now suspect that this prehistoric fish, also known as the megalodon (Otodus megalodon), may have had a more elongated form, akin to modern slim sharks.

The typical estimation of the megalodon’s length is between 15 to 20 meters (50 to 65 feet), and they inhabited the earth’s oceans from 15 million to 3.6 million years ago. However, the fossil record contains limited evidence of the megalodon, mainly consisting of teeth and vertebrae rather than intact skeletons.

While previous estimates of its body size were based on the bodies of contemporary great white sharks (Carcharodon carcharius), resulting in the assumption of a thick and round body shape, a new study published in the Old Trogia Electronica journal suggests that the megalodon was more than just a larger version of the great white shark. The study contends that the animal may have had similarities to the slimmer modern mako shark.

So what’s the controversy?

Essentially, two groups of scientists are at odds over the actual size and shape of the megalodon.

A study led by scientists from DePaul University and the University of California, Riverside (UCR) employed a CT scanner on a live great white shark to compare its vertebral skeleton to existing reconstructions of the megalodon’s spinal column. This study suggests significant enough differences between the two sharks to propose that the megalodon was not merely a larger great white shark.

However, a UK-based research team utilized advanced 3D modeling to study the body structures of various shark species, including great whites, mako sharks, and salmon sharks. With this approach, they concluded that the megalodon may have been even larger than previously anticipated, with a dorsal fin comparable in size to an adult’s height.

The earlier study’s authors critiqued the new findings, asserting that they rely on circular logic and lack statistical validation. They also mentioned the absence of raw data for future researchers to verify or reproduce the study’s results. Their study was peer-reviewed by prominent shark experts from around the world, although not by the authors of the new study.

Yeah, but…can Jason Statham still defeat Megalodon?

Regardless of the megalodon’s shape, the lifespan and dietary habits of this extinct shark remain unclear. To further advance their understanding, researchers will need to find a complete or near-complete skeleton. The potential elongated body of the megalodon, if confirmed, could prompt a reassessment of its life, diet, and extinction causes.

As for the debate over the megalodon’s size and shape, the fact that it was a large, formidable predator is indisputable. However, the question of whether Jason Statham could defeat it in battle remains up for discussion.

“Even with the interpretation of the megalodon’s shape as more slender, I don’t think the odds for that matchup will change significantly,” Cooper stated. “Regardless of which theory you favor, whether the shark was fat or skinny, the short answer is that megalodon was still a very large shark. Either way, it’s a massive challenge for Statham.”

About our experts

Jack Cooper is a postdoctoral researcher in palaeontology at Swansea University. His research covers scientific report, scientific progress and the Fish Biology Journal.

Professor Catalina Pimiento is a Senior Lecturer in Paleontology at Swansea University. Her research specializes in Frontiers of ecology and evolution, natural ecology and evolution, and scientific progress.

Professor John Hutchinson is Professor of Evolutionary Biomechanics at the Royal Veterinary College. His research spans nature communications, anatomy journal, and scientific progress.

read more:

Source: www.sciencefocus.com

The Top 10 Most Powerful Animals in the World

What is the strongest animal in the world? This is an important question, especially if you are moving and can’t afford to hire movers.

But suppose you have an animal that helps you get around. Which one should you choose? What is the strongest animal? Who can lift the most weight?

To answer this most important question, we have compiled a list of the strongest animals on Earth today. Get ready to journey through a world of brute force as you marvel at incredibly strong birds, muscular polar bears, and powerful punching cows.

10. Harpy Eagle – Can lift 18 kg (twice its own body weight)

A female harpy eagle (Harpia harpyja) carries prey such as a skinned and half-eaten coati (Nasua nasua) to her nest. Pousada Curpila Dalaras, southwestern Brazil.Photo credit: Alamy

Female harpy eagles are the strongest birds in the world. Females are stronger than males and can lift up to 18 kg, about twice their own body weight. This is useful when choosing prey and means a greater variety of animals are available for dinner.

They are apex predators at the top of the food chain. And when you see strength like this, you can see why.

9. Leopard – Can lift 125 kg (about twice its body weight).

A leopard (Panthera pardus) takes shelter in a tree at Sabi Sands Nature Reserve in Mpumalanga, South Africa.Photo credit: David Silverman/Getty Images

The average male leopard weighs between 30 kg and 70 kg, and the largest leopards can lift weights of 125 kg using strong jaw muscles and powerful legs and claws.

Leopards are not as strong as rivals like tigers and lions, so after hunting they need this strength to pull large prey up trees to protect them from rivals. This ability is also useful for storing food out of reach for later consumption.

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Source: www.sciencefocus.com

NASA captures starscape as Sun releases powerful X2.8 flare




NASA’s Solar Dynamics Observatory

NASA’s Solar Dynamics Observatory (SDO) captured this image of a solar flare on December 14 (as seen by the bright flash in the top right).

This image shows a subset of extreme ultraviolet light that highlights the very hot material within the flare, color-coded teal. Credit: NASA/SDO

NASA observed a significant X2.8 solar flare on December 14, 2023, with potential impacts on Earth’s technological systems. NOAASpace Weather Forecast Center.

The sun emitted a strong solar flare, reaching its peak at 12:02 p.m. EST, December 14, 2023. NASA’s Solar Dynamics Observatory, which constantly monitors the Sun, captured images of the event.

A solar flare is a powerful explosion of energy. Flares and solar eruptions can affect radio communications, power grids, and navigation signals, posing a danger to spacecraft and astronauts.

This flare is classified as an X2.8 flare. The X class indicates the most powerful flare, and the numbers provide more information about its strength.

Solar flares like this one, captured by NASA satellites orbiting the sun, emit large amounts of radiation. Credit: NASA

Solar flares are intense bursts of radiation emitted from the release of magnetic energy associated with sunspots. These are among the most powerful phenomena in the solar system and can have significant effects on Earth’s space environment.

These flares are classified according to their intensity. The classification is as follows.
X class flare: The most intense flare. They can cause global radio interference and long-term radiation storms that can affect satellites and astronauts. X-class flares are further classified by number, with higher numbers indicating more powerful flares. For example, an X2 flare is twice as strong as an X1 flare and four times as strong as an X0.5 flare.
M class flare: Medium intensity flare. In polar regions, it can cause short-term radio interference and small radiation storms. While not as powerful as an X-class flare, they can still have a noticeable impact on Earth’s space weather.
C class flare: These are small flares that have little noticeable impact on Earth. These are more common than M-class and X-class flares, but are usually too weak to significantly affect space weather.
B class and A class flares: These are even smaller flares and are often undetectable without specialized solar observation equipment. They have minimal, if any, impact on the planet.

This classification is based on the peak luminous flux (number of photons) in watts per square meter measured in Earth’s orbit by the GOES spacecraft. This system allows you to quickly and easily communicate the strength of solar flares and their potential impact on space weather and Earth.

Artist’s concept for the Solar Dynamics Observatory (SDO). Credit: NASA/Goddard Space Flight Center Conceptual Image Lab

NASA’s Solar Dynamics Observatory

NASA’s Solar Dynamics Observatory (SDO) is a pivotal mission in the study of the Sun, playing a key role in understanding our closest star. Launched on February 11, 2010, SDO is specifically designed to observe and understand solar activity that influences weather on Earth and in space.

The primary goal of SDO is to better understand the Sun’s influence on Earth and near-Earth space by studying the solar atmosphere simultaneously at small space and time scales and at many wavelengths. This is very important for understanding the influence of the Sun on the Earth, especially the magnetic field and the space environment.

The SDO is equipped with a range of advanced equipment. The Atmospheric Imaging Assembly (AIA) acquires high-resolution images of the solar atmosphere, the Solar Seismic and Magnetic Imager (HMI) studies the solar magnetic field and the dynamic motion of the Sun’s interior, and the Extreme Ultraviolet Fluctuations Experiment (EVE) studies the solar magnetic field. Measure. UV output.

One of SDO’s most important contributions is its ability to continuously observe the Sun in detail at multiple wavelengths. These observations provide a comprehensive view of solar activity, including flares, coronal mass ejections, and changes in the solar magnetic field. Data from SDO has helped advance our understanding of the Sun’s complex and dynamic magnetic field, its energy output, and how these factors interact to drive space weather.

In summary, NASA’s Solar Dynamics Observatory is a key asset in solar science, providing valuable data that helps scientists better understand the behavior of the Sun and its effects on space weather and Earth.


Source: scitechdaily.com