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  • Space Ice Differs More from Water Than Expected

    Space Ice Differs More from Water Than Expected

    “Space ice” contains tiny crystals and is not, as previously assumed, a completely disordered material like liquid water, according to a new study by scientists at UCL (University College London) and the University of Cambridge.

    Ice in space is different to the crystalline (highly ordered) form of ice on Earth. For decades, scientists have assumed it is amorphous (without a structure), with colder temperatures meaning it does not have enough energy to form crystals when it freezes.

    In the new study, published in Physical Review B, researchers investigated the most common form of ice in the Universe, low-density amorphous ice, which exists as the bulk material in comets, on icy moons and in clouds of dust where stars and planets form.

    They found that computer simulations of this ice best matched measurements from previous experiments if the ice was not fully amorphous but contained tiny crystals (about three nanometres wide, slightly wider than a single strand of DNA) embedded within its disordered structures.

    In experimental work, they also re-crystallised (i.e. warmed up) real samples of amorphous ice that had formed in different ways. They found that the final crystal structure varied depending on how the amorphous ice had originated. If the ice had been fully amorphous (fully disordered), the researchers concluded, it would not retain any imprint of its earlier form.

    Lead author Dr Michael B. Davies, who did the work as part of his PhD at UCL Physics & Astronomy and the University of Cambridge, said: “We now have a good idea of what the most common form of ice in the Universe looks like at an atomic level.

    “This is important as ice is involved in many cosmological processes, for instance in how planets form, how galaxies evolve, and how matter moves around the Universe.”

    The findings also have implications for one speculative theory about how life on Earth began. According to this theory, known as Panspermia, the building blocks of life were carried here on an ice comet, with low-density amorphous ice the space shuttle material in which ingredients such as simple amino acids were transported.

    Dr Davies said: “Our findings suggest this ice would be a less good transport material for these origin of life molecules. That is because a partly crystalline structure has less space in which these ingredients could become embedded.

    “The theory could still hold true, though, as there are amorphous regions in the ice where life’s building blocks could be trapped and stored.”

    Co-author Professor Christoph Salzmann, of UCL Chemistry, said: “Ice on Earth is a cosmological curiosity due to our warm temperatures. You can see its ordered nature in the symmetry of a snowflake.

    “Ice in the rest of the Universe has long been considered a snapshot of liquid water – that is, a disordered arrangement fixed in place. Our findings show this is not entirely true.

    “Our results also raise questions about amorphous materials in general. These materials have important uses in much advanced technology. For instance, glass fibers that transport data long distances need to be amorphous, or disordered, for their function. If they do contain tiny crystals and we can remove them, this will improve their performance.”

    For the study, the researchers used two computer models of water. They froze these virtual “boxes” of water molecules by cooling to -120 degrees Centigrade at different rates. The different rates of cooling led to varying proportions of crystalline and amorphous ice.

    They found that ice that was up to 20% crystalline (and 80% amorphous) appeared to closely match the structure of low-density amorphous ice as found in X-ray diffraction studies (that is, where researchers fire X-rays at the ice and analyse how these rays are deflected).

    Using another approach, they created large “boxes” with many small ice crystals closely squeezed together. The simulation then disordered the regions between the ice crystals reaching very similar structures compared to the first approach with 25% crystalline ice.

    In additional experimental work, the research team created real samples of low-density amorphous ice in a range of ways, from depositing water vapour on to an extremely cold surface (how ice forms on dust grains in interstellar clouds) to warming up what is known as high-density amorphous ice (ice that has been crushed at extremely cold temperatures).

    The team then gently heated these amorphous ices so they had the energy to form crystals. They noticed differences in the ices’ structure depending on their origin – specifically, there was variation in the proportion of molecules stacked in a six-fold (hexagonal) arrangement.

    This was indirect evidence, they said, that low-density amorphous ice contained crystals. If it was fully disordered, they concluded, the ice would not retain any memory of its earlier forms.

    The research team said their findings raised many additional questions about the nature of amorphous ices – for instance, whether the size of crystals varied depending on how the amorphous ice formed, and whether a truly amorphous ice was possible.

    Amorphous ice was first discovered in its low-density form in the 1930s when scientists condensed water vapour on a metal surface cooled to -110 degrees Centigrade. Its high-density state was discovered in the 1980s when ordinary ice was compressed at nearly -200 degrees Centigrade.

    The research team behind the latest paper, based both at UCL and the University of Cambridge, discovered medium-density amorphous ice in 2023. This ice was found to have the same density as liquid water (and would therefore neither sink nor float in water).

    Co-author Professor Angelos Michaelides, from the University of Cambridge, said: “Water is the foundation of life but we still do not fully understand it. Amorphous ices may hold the key to explaining some of water’s many anomalies.”

    Dr Davies said: “Ice is potentially a high-performance material in space. It could shield spacecraft from radiation or provide fuel in the form of hydrogen and oxygen. So we need to know about its various forms and properties.”

    /Public Release. This material from the originating organization/author(s) might be of the point-in-time nature, and edited for clarity, style and length. Mirage.News does not take institutional positions or sides, and all views, positions, and conclusions expressed herein are solely those of the author(s).View in full here.

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  • Scientists behind threatened NASA missions…

    Scientists behind threatened NASA missions…

    In one sentence, what does the mission you’re working on aim to do? 

    Initially focusing on Jupiter’s interior, atmosphere and aurora, [Juno] has expanded during its extended mission to be a full system explorer capable of investigating the Galilean satellites, rings, inner moons, radiation belts, and boundaries of Jupiter’s magnetosphere.

    What potential discoveries are at stake if Juno is defunded or cancelled?

    Juno provides a unique opportunity to investigate previously unexplored regions of the Jovian system. Its next phase includes close flybys of the moons Thebe, Amalthea, Adrastea, and Metis. In addition to scientific exploration, Juno is providing critical new information directly relevant to national security by teaching us how space systems can survive and even reverse degradation from exposure to intense radiation.

    How does Juno fit into NASA’s overall mission?

    In addition to helping to lay a foundation for NASA’s Europa Clipper and ESA’s Jupiter Icy Moons Explorer (JUICE) missions enroute to Jupiter, Juno is providing the basis of understanding to compare the characteristics of Jupiter with the other giant planets in the Solar System: Saturn, Uranus and Neptune. This is vital for our understanding of Solar System formation and evolution, and for understanding planetary systems throughout the galaxy.

    Why should this mission matter to people?

    Continuing NASA’s Juno mission is a strategic investment in planetary science, offering continued insights into the Jupiter system and informing future exploration missions. The mission’s unique capabilities, cost-effectiveness, and alignment with strategic priorities make it an invaluable asset to the scientific community and the nation’s space exploration goals.

    How many people are on your team?

    There are about 200 people working on Juno, mostly part time.

    How many states are represented by the Juno team?

    10 states.


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  • AI-Powered Universal Strategy for Protein Engineering Unveiled

    AI-Powered Universal Strategy for Protein Engineering Unveiled

    A team of Chinese researchers led by Prof. GAO Caixia from the Institute of Genetics and Developmental Biology (IGDB) of the Chinese Academy of Sciences has developed a groundbreaking method that could transform the field of protein engineering. The new approach, called AI-informed Constraints for protein Engineering (AiCE), enables rapid and efficient protein evolution by integrating structural and evolutionary constraints into a generic inverse folding model—without the need to train specialized artificial intelligence (AI) models.

    The study, published in Cell on July 7, addresses many of the challenges associated with traditional protein engineering techniques.

    The ideal protein engineering strategy would achieve optimal performance with minimal effort. However, existing approaches are often limited in terms of cost, efficiency, and scalability. Current AI-based protein engineering methods are often computationally intensive, underscoring the need for more accessible and user-friendly alternatives that preserve predictive accuracy and enable broader adoption across the research community.

    In this study, the researchers first developed AiCEsingle, a module designed to predict high-fitness (HF) single amino acid substitutions. It enhances prediction accuracy by extensively sampling inverse folding models—AI models that generate compatible amino acid sequences based on protein 3D structures—while incorporating structural constraints.

    Benchmarking against 60 deep mutational scanning (DMS) datasets demonstrated that AiCEsingle outperforms other AI-based methods by 36–90%. Its effectiveness for complex proteins and protein–nucleic acid complexes was also validated. Notably, incorporating structural constraints alone yielded a 37% improvement in accuracy.

    To address the challenge of negative epistatic interactions in combinatorial mutations, the researchers developed the AiCEmulti module, which integrates evolutionary coupling constraints. This allows for accurate prediction of multiple high-fitness mutations at minimal computational cost, expanding the tool’s versatility and practical utility.

    Using the AiCE framework, the researchers successfully evolved eight proteins with diverse structures and functions, including deaminases, nuclear localization sequences, nucleases, and reverse transcriptases. These engineered proteins have enabled the creation of several next-generation base editors for applications in precision medicine and molecular breeding. These include: enABE8e, a cytosine base editor with a ~50% narrower editing window; enSdd6-CBE, an adenine base editor with 1.3× higher fidelity; and enDdd1-DdCBE, a mitochondrial base editor showing a 13× increase in activity.

    AiCE represents a simple, efficient and broadly applicable strategy for protein engineering. By unlocking the potential of existing AI models, it offers a promising new direction for the field and enhances the interpretability of AI-driven protein redesign.

    /Public Release. This material from the originating organization/author(s) might be of the point-in-time nature, and edited for clarity, style and length. Mirage.News does not take institutional positions or sides, and all views, positions, and conclusions expressed herein are solely those of the author(s).View in full here.

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  • Common bacteria found in the stomach has no symptoms but could cause 12 million cancers, study warns

    Common bacteria found in the stomach has no symptoms but could cause 12 million cancers, study warns

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    A common bacteria found in the stomach could cause nearly 12 million cancers among people born over a single decade, a new study suggests.

    Over the course of their lives, 15.6 million people born between 2008 and 2017 are expected to develop stomach cancer – and 76 per cent may be caused by the Helicobacter pylori bacteria, according to the study published in the journal Nature Medicine.

    Stomach cancer is largely preventable, but the prognosis is poor once a patient is diagnosed. It is the fifth most common form of cancer worldwide, killing an estimated 770,000 people per year.

    Chronic infection with H. pylori is a major cause, and it helps explain the rise in stomach cancers among young people in recent years, the study found.

    Most people are infected with H. pylori as children, and they may be infected for years without knowing it because the infection doesn’t cause symptoms. But it can also cause ulcers or inflammation in the stomach lining.

    The bacteria can spread by mouth, for example kissing, or through contact with vomit or stool.

    Where stomach cancer cases will rise

    Researchers from the World Health Organization’s (WHO) cancer research agency analysed stomach cancer data from 185 countries in 2022.

    They projected that under current trends, 11.9 million people could be diagnosed with stomach cancer attributable to H. pylori infection by 2101, which is the year someone born in 2017 would turn 84.

    The vast majority of bacteria-linked stomach cancer cases – 8 million – are expected in Asia. Another nearly 471,000 cases are projected in the European Union, the United Kingdom, Switzerland, Norway and Iceland.

    The burden of stomach cancer is also shifting globally. While sub-Saharan Africa currently has relatively few cases, the researchers expect stomach cancer cases tied to H. pylori to rise to 1.4 million by 2101 – six times higher than the rate in 2022 – due to ageing and population changes.

    “With demographic changes set to increase the gastric cancer burden in many parts of the world, there is an urgent need for coordinated prevention strategies and for regional health systems to be prepared to manage the growing burden,” said Dr Jin Young Park, one of the study’s co-authors and head of the gastric cancer prevention team at the WHO’s International Agency for Research on Cancer (IARC).

    The study has some limitations, notably poor data quality in lower-income countries that can make it harder to make confident predictions.

    But the researchers said the data is clear enough for health authorities around the world to take action.

    They called for countries to invest in initiatives to screen and quickly treat people for H. pylori infection. Their analysis shows that such programmes could reduce the number of expected stomach cancer cases by up to 75 per cent.

    “It is essential that health authorities make gastric cancer prevention a priority and accelerate efforts to control it,” Park said.

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  • See a rare dinosaur or a chunk of Mars during Sotheby’s ‘Geek Week’

    See a rare dinosaur or a chunk of Mars during Sotheby’s ‘Geek Week’

    New Yorkers may not think of Sotheby’s, the tony auction house on the Upper East Side, as a place to casually pop in to, let alone a place to see dinosaurs or Martian meteorites.

    But during “Geek Week,” that’s exactly what’s on free public view. From July 8 to 15, Sotheby’s is displaying some remarkable objects of natural history, science and space exploration before they hit the auction block.

    This year’s standout is a six-foot-tall, 10-foot-long juvenile Ceratosaurus, one of only four known specimens of this extremely rare Jurassic dinosaur.

    The roughly 150 million-year-old fossil, which has been reconstructed with a few ceramic elements to replace missing pieces, was discovered in Wyoming in 1996, according to Cassandra Hatton, Sotheby’s vice chairman of science and natural history.

    It’s expected to sell for between 4 and 6 million dollars.

    The sale includes more than 100 ancient items, sourced from various collectors, including dinosaur skulls and claws, chunks of meteorites, a 4,000-year-old stone axe and astonishing, iridescent slices of mineral and crystal, all on view.

    Another showstopper is a 54-pound Martian meteorite – the largest known piece of Mars on Earth. This chunk of the Red Planet is believed to have been chipped off by one of only 16 known asteroid strikes powerful enough to launch debris into space, before landing in the Sahara desert.

    “That chunk had to be loose enough to break off, and then it had to get on the right trajectory to travel 140 million miles to Earth, and then it had to land in a spot where someone could find it,” Hatton said. “And then we were lucky enough that someone came by who knew enough about meteorites to recognize that it wasn’t just a big rock.”

    Hatton said scientists were able to confirm the meteorite’s extraterrestrial origin by extracting gas trapped in bubbles inside the rock and comparing it to Martian atmospheric data transmitted from NASA’s Viking lander in 1976.

    The sale also includes objects that went to space with astronaut Buzz Aldrin, from his collection.

    Another highlight includes what Hatton describes as the finest operational Apple-1 computer in existence: one of 50 machines hand-built by Steve Wozniak and Steve Jobs in 1976.

    The Apple founders had built a few prototypes and were shopping them around town, Hatton said, when a local shopkeeper happened to see their presentation at the Home Brew Computer Club, an early computer hobbyist group in Menlo Park, California. He asked for 50, which sent the techies scrambling for parts to fulfill a bigger order than they’d anticipated.

    The sale also includes one of Jobs’ earliest business cards, expected to sell for $5,000 to 8,000.

    For those who associate Sotheby’s with high-stakes blue-chip art sales and exclusivity, Geek Week is a reminder that the auction house doubles as a pop-up museum.

    Hatton said she’s the only science specialist on staff.

    “I go from scientific books and manuscripts to tech, dinosaurs, minerals, meteorites, space exploration,” Hatton said. “I do hip-hop sales sometimes too. It all connects together somehow, in my mind.”

    Sotheby’s Geek Week is at 1334 York Ave. from July 8 through 15, open from 10 a.m. to 5 p.m. every day except Sunday, when it opens at 1 p.m. No RSVP is required.

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  • NASA’s Hubble and Webb Telescopes Reveal Two Faces of a Star Cluster Duo

    NASA’s Hubble and Webb Telescopes Reveal Two Faces of a Star Cluster Duo

    A riotous expanse of gas, dust, and stars stake out the dazzling territory of a duo of star clusters in this combined image from NASA’s Hubble and Webb space telescopes.

    Open clusters NGC 460 and NGC 456 reside in the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. Open clusters consist of anywhere from a few dozen to a few thousand young stars loosely bound together by gravity. These particular clusters are part of an extensive complex of star clusters and nebulae that are likely linked to one another. As clouds of gas collapse, stars are born. These young, hot stars expel intense stellar winds that shape the nebulae around them, carving out the clouds and triggering other collapses, which in turn give rise to more stars.

    In these images, Hubble’s view captures the glowing, ionized gas as stellar radiation blows “bubbles” in the clouds of gas and dust (blue), while Webb’s infrared vision highlights the clumps and delicate filamentary structures of dust (red). In Hubble images, dust is often seen silhouetted against and blocking light, but in Webb’s view, the dust – warmed by starlight – shines with its own infrared glow. This mixture of gas and dust between the universe’s stars is known as the interstellar medium.

    The nodules visible in these images are scenes of active star formation, with stars ranging from just one to 10 million years old. In contrast, our Sun is 4.5 billion years old. The region that holds these clusters, known as the N83-84-85 complex, is home to multiple, rare O-type stars, hot and extremely massive stars that burn hydrogen like our Sun. Astronomers estimate there are only around 20,000 O-type stars among the approximately 400 billion stars in the Milky Way.

    The Small Magellanic Cloud is of great interest to researchers because it is less enriched in metals than the Milky Way. Astronomers call all elements heavier than hydrogen and helium – that is, with more than two protons in the atom’s nucleus – “metals.”  This state mimics conditions in the early universe, so the Small Magellanic Cloud provides a relatively nearby laboratory to explore theories about star formation and the interstellar medium at early stages of cosmic history. With these observations of NGC 460 and NGC 456, researchers intend to study how gas flows in the region converge or divide; refine the collision history between the Small Magellanic Cloud and its fellow dwarf galaxy, the Large Magellanic Cloud; examine how bursts of star formation occur in such gravitational interactions between galaxies; and better understand the interstellar medium.

    Explore More

    Media Contact:

    Claire Andreoli
    NASA’s Goddard Space Flight CenterGreenbelt, MD
    claire.andreoli@nasa.gov

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  • India U19 Vs England U19 LIVE Score: India Eye Wickets As 1-Down England Gain Momentum In Chase – NDTV Sports

    India U19 Vs England U19 LIVE Score: India Eye Wickets As 1-Down England Gain Momentum In Chase – NDTV Sports

    1. India U19 Vs England U19 LIVE Score: India Eye Wickets As 1-Down England Gain Momentum In Chase  NDTV Sports
    2. ENG vs IND 2nd Test Day 3 session timings, England vs India live streaming  Business Standard
    3. ENG vs IND: Watch Vaibhav Suryavanshi In Action — Time, Venue & Live Streaming Details  ABP Live English
    4. IND U19 vs ENG U19 LIVE Cricket Score, 5th ODI: England win by 7 wickets as India seal series 3-2  The Indian Express
    5. ENG U-19 vs IND U-19 Live Streaming Info, 5th ODI: When and where to watch India U-19 tour of England 2025; match details, squads  Sportstar

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  • How solar power helped European grids pass ‘the stress test’ during the recent heatwave

    How solar power helped European grids pass ‘the stress test’ during the recent heatwave

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    Europe’s latest heatwave dialled up daily power demand by up to 14 per cent, as Europeans turned up their air conditioning to stay cool.

    But the sunshine also increased the availability of solar energy, the same analysis from energy think tank Ember shows, helping Europe’s power grids pass “the stress test” of extreme heat. 

    Between 28 June and 2 July, peak daily temperatures averaged out at 35°C in Germany and Spain – where some local temperatures crossed 40°C – and 34°C in France. 

    As a result of soaring air con use, daily power demand soared by up to 14 per cent in Spain, 9 per cent in France, and 6 per cent in Germany, compared to the previous week.

    “Despite the huge pressure, European grids passed the stress test, and solar electricity played a major role in keeping them running,” says Pawel Czyzak, Europe Programme Director at Ember.

    How did solar energy help get Europe through the heatwave?

    June 2025 saw the highest EU solar generation on record at 45 terrawatt hours (TWh), a 22 per cent increase from the year before. This flooded grids with cheap, clean electricity during daytime hours.

    In the peak days of the heatwave, solar delivered up to 50 gigawatts (GW) of power in Germany, generating 33-39 per cent of the country’s electricity.

    By contrast, thermal power plants struggled in the heat. In France, 17 out of 18 nuclear power plants faced capacity reductions during the heatwave, with some shut down completely due to high river temperatures which meant their waters couldn’t be used as usual to cool the reactors. 

    The Beznau nuclear power plant in Switzerland also had its capacity halved as the River Aare crept up to 25°C – a decision taken to protect the ecosystem. 

    In Poland – where there are long-running concerns about the cooling of coal power plants – the government and grid operator PSE proposed an ‘anti-blackout package’ at the peak of the heatwave on 2 July.

    Other parts of power systems also struggle during the heatwaves. The overheating of cables is the likely cause of power outages in Italy on 1 July, Ember notes.

    The heatwave triggered a spike in electricity prices

    “The surplus of solar energy during the day helped prevent blackouts,” says Czyzak. “However, the use of energy storage is still insufficient, leading to reduced energy supply after sunset. This translated into a sharp increase in electricity prices.”

    According to Ember’s analysis, this supply-demand imbalance caused average daily power prices to double or even triple in some countries. 

    Between 24 June 24 and 1 July, average daily electricity prices rocketed by 175 per cent in Germany, 108 per cent in France, 106 per cent in Poland, and 15 per cent in Spain. During the evening peak on 1 July, prices spiked above €470/MWh in Poland and €400/MWh in Germany. 

    Interconnectors – cables used to connect the electricity systems of neighbouring countries – ensured these price spikes dissipated quickly, Ember explains. 

    As the heatwave swept across Europe, peaking in Madrid on Sunday 29 June, Paris on Tuesday 1 July, and Berlin and Warsaw on Wednesday 3 July, interconnectors helped deliver electricity to where it was needed most.

    Solar electricity storage and renewable ‘energy islands’

    But the continent’s power infrastructure still needs a serious upgrade to cope with increasingly severe heatwaves due to climate change

    Greater battery storage is needed to spread out the variable energy that solar and wind produce, Ember says. And better demand flexibility – i.e. shifting non-critical demand to periods of abundant supply – will help ease peak stress on the grid.

    “Perhaps the biggest opportunity is to store solar electricity, to help power air conditioning well into the evening,” says Czyzak.

    The experts are also calling for more investment in distributed energy sources capable of starting the network on their own, such as solar farms with grid-forming inverters. Unlike traditional grid-following inverters that only sync with the existing grid, these inverters can start without an external voltage supply. 

    A recent project by the UK National Energy System Operator (NESO) showed the potential of this solution, exploring how wind and solar could be used to restart the grid after a blackout. It recommended building renewables-powered energy islands that are later joined to the whole grid. 

    Belgium’s transmission system operator is testing grid-forming assets too. It’s all part of the global goal to triple renewable energy capacity by 2030, a measure to mitigate the climate crisis – and the increasing heatwaves it is bringing.

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  • New Intel Core Ultra gaming CPUs rumored to boost clock speeds, arrive this year

    New Intel Core Ultra gaming CPUs rumored to boost clock speeds, arrive this year

    Intel will launch a refreshed lineup of its Intel Core Ultra 200 CPUs later this year, with the chips based on a refreshed variant of the Intel Arrow Lake architecture that powers its current flagship gaming CPUs, according to a new report. These so-called Intel Arrow Lake refresh chips are expected to come with increases in clock speed as well as AI number crunching, for modest all-around gains in performance.

    The new Intel CPU lineup could help bolster the company’s efforts to attract gaming PC users to once again buy its chips, after several years of AMD’s X3D CPUs proving dominant in gaming performance and topping our best gaming CPU charts. However, the new report also suggests the performance gains will be modest, so this is far from a nailed-on certainty.

    The Intel Arrow Lake refresh data comes from ZDNet Korea, which according to a machine translated version of the page, states that “Intel is set to release ‘Arrow Lake Refresh’, a desktop PC processor that slightly improves the performance of its Core Ultra 200S processor, in the second half of this year.”

    The site doesn’t cite any source for this, so this is all just rumor for the time being. However, crucially, it goes on to say that “the prevailing opinion is that the performance improvement is not that great compared to the previous generation (14th generation, Raptor Lake Refresh).”

    In other words, while Intel may be bringing a little more general performance to the table with its Intel Arrow Lake refresh chips – expected to arrive with model names based on the Intel Core Ultra 200 schema – they won’t be expected to take either the general performance crown from the Intel Core i9-14900K or the gaming performance crown from the AMD Ryzen 7 9800X3D.

    Instead, the biggest boost is expected to be in AI. Intel’s current Core Ultra 200 desktop chips aren’t Microsoft CoPilot+ certified thanks to their AI-processing NPU not being quite powerful enough, so a slight increase would allow them to tick that box.

    For most gaming PC builders, though, it’s looking much more like future AMD Zen 6 CPUs will be the next big leap in gaming CPU performance. Though those aren’t expected to arrive until 2026.

    Meanwhile, despite its gaming performance not being chart-topping, our Intel Core Ultra 7 265K review shows Intel’s latest is still a very capable CPU. What’s more, recent price drops mean it’s currently far cheaper than the 9800X3D, at well under $300.

    Whatever model of CPU you’re rocking, if you’re looking to get the most from your system, a RAM upgrade could be ideal. If you’re stuck on 8GB or even 16GB, a move to 32GB could allow your system to spread its wings. Check out our best gaming RAM guide to find the best upgrade for your needs.

    You can also follow us on Google News for daily PC games news, reviews, and guides. We also have a vibrant community Discord server, where you can chat about this story with members of the team and fellow readers.

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  • Scientists Discover Giant Sand Bodies Beneath The North

    Scientists Discover Giant Sand Bodies Beneath The North

    Scientists have discovered hundreds of giant sand bodies beneath the North Sea that appear to defy fundamental geological principles and could have important implications for energy and carbon storage.

    Using high-resolution 3D seismic (sound wave) imaging, combined with data and rock samples from hundreds of wells, researchers from The University of Manchester in collaboration with industry, identified vast mounds of sand—some several kilometers wide—that appear to have sunk downward, displacing older, lighter and softer materials from beneath them.

    The result is stratigraphic inversion—a reversal of the usual geological order in which younger rocks are typically deposited on top of older ones—on a previously unseen scale.

    While stratigraphic inversion has previously been observed at small scales, the structures discovered by the Manchester team, now named “sinkites,” are the largest example of the phenomenon documented so far.

    The finding, published in the journal Communications Earth & Environment, challenges scientists understanding of the subsurface and could have implications for carbon storage.

    “This discovery reveals a geological process we haven’t seen before on this scale,” said lead author Professor Mads Huuse from The University of Manchester. “What we’ve found are structures where dense sand has sunk into lighter sediments that floated to the top of the sand, effectively flipping the conventional layers we’d expect to see and creating huge mounds beneath the sea.”

    It is believed the sinkites formed millions of years ago during the Late Miocene to Pliocene periods, when earthquakes or sudden shifts in underground pressure may have caused the sand to liquefy and sink downward through natural fractures in the seabed. This displaced the underlying, more porous but rigid, ooze rafts—composed largely of microscopic marine fossils—bound by shrinkage cracks, sending them floating upwards. The researchers have dubbed these lighter, uplifted features “floatites.”

    The finding could help scientists better predict where oil and gas might be trapped and where it’s safe to store carbon dioxide underground.

    “This research shows how fluids and sediments can move around in the Earth’s crust in unexpected ways. Understanding how these sinkites formed could significantly change how we assess underground reservoirs, sealing, and fluid migration—all of which are vital for carbon capture and storage,” said Huuse. 

    Now the team are busy documenting other examples of this process and assessing how exactly it impacts our understanding of subsurface reservoirs and sealing intervals.

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