The first teaser trailer of Luca Guadagnino’s Artificial has been released.
After being dropped by Amazon MGM Studios in June, the biopic of the OpenAI tech executive Sam Altman will be released in the US on 25 December by Neon after it premieres at the New York film festival this October.
A breathtaking new view of the cosmos featuring more than half a million galaxies has been released by the NSF–DOE Vera C. Rubin Observatory, revealing its first LSST Camera image for scientific use.
Unveiling one of the most studied regions of space, the millions of galaxies featured in the new image were captured with Rubin’s 3.2-gigapixel LSST Camera, the largest digital camera currently in existence.
Mounted on the observatory’s 8.4-meter Simonyi Survey Telescope, the stunning new imagery captured with the LSST focuses on the COSMOS field, a region located within the Sextans constellation. Long a cornerstone of astronomical research, this region of the sky has remained an extensively studied area for more than two decades.
A Crowded View of the Cosmos
By stacking hundreds of individual observations into a single composite view, the Rubin imagery contains more than 500,000 galaxies and over 50,000 foreground stars, all packed into an unprecedented view of the Milky Way.
However, since the COSMOS field comprises regions of space much further from the crowded plane of our galaxy, it offers an unusually unobstructed view into more distant parts of the universe, allowing astronomers to look not only farther out into space, but also to peer billions of years back into the past by observing the light from ancient galaxies that is only now making its way to Earth.
Above: A portion of the highly detailed astronomical imagery obtained by the Rubin Observatory in its newly released imagery. The view above reprsents approximately 1/100th of Rubin’s field of view (Image Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA).
The result is a somewhat crowded view of our universe, showcasing the immensity of the cosmos in some of the most stunning astronomical imagery in recent memory.
The COSMOS Field
Since 2003, astronomers have focused their studies on the COSMOS field with the world’s most powerful observatories, including the Hubble Space Telescope, the James Webb Space Telescope, the Chandra X-ray Observatory, and the Spitzer Space Telescope.
By observing spectral ranges from radio waves to X-rays, astronomers have successfully made the region one of the premier reference fields in modern astronomy for everything from galaxy formation to the birth of stars and the evolution of the cosmos.
Now, the detailed cosmic vistas being captured by the Rubin Observatory are adding a new dimension to those earlier observations. Unlike past observations, though, Rubin will repeatedly capture imagery from the same region over the course of the decade-long Legacy Survey of Space and Time (LSST). By doing so, astronomers will not only be able to study distant galaxies in greater detail than ever before, but also will be treated to a view of gradual changes over time.
Through ongoing observations, detections of supernovae, variable stars, and other transient phenomena occurring deep in space will be revealed, along with the presence of fainter celestial objects such as galaxies that could not otherwise be seen without the age of composite imagery.
Rubin’s Work is Only Beginning
The newly released images are part of Rubin’s initial Early Data Preview 2 (EDP2), which comprises the observatory’s first science data release. Based on observations made with the LSST camera, the recent images offer a preview of things to come as the full 10-year LSST survey moves forward.
“The COSMOS deep image is just the beginning for Rubin in this region,” said Bob Blum, director of Rubin Observatory at NSF NOIRLab, in a statement. The observatory’s current efforts will be followed by a second phase, which is expected later this year, from which individual observations and specialized “difference images” will be produced, highlighting objects that exhibit changes across successive observations.
Image Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA
Altogether, the datasets will provide an emerging picture of the remarkable work astronomers are anticipating from Rubin, which will culminate in the most comprehensive cinematic record of the universe astronomers have ever assembled.
“Repeated visits to the field over the next few years will demonstrate the power of our survey design for discovery by providing our science community with a huge number of transient and variable objects like supernovae and other explosive transients for follow-up and detailed study,” Blum added.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached atmicah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
Our modern society depends heavily on communications and power networks that are highly susceptible to interference from solar storms, making these volatile space weather events a paramount concern for scientists.
Now, it turns out there may be more to fear than previously realized. Scientists are discovering that there may be no ceiling to the devastating effects solar storms may have on Earth, overturning what little sense of security may exist as a mere mathematical anomaly.
In a recent paper published in Nature, a NASA-led team discovered that the potential impact of solar storms on our technological infrastructure could be substantially more severe than currently recognized.
Solar Storms Reconsidered
According to new research, any past limitations perceived regarding the impact of solar storms on our planet are purely an illusion, which arises from imprecise data collection.
Previous observations of electric currents in the Earth’s upper atmosphere during solar storm events suggested a ceiling to how far they could increase. Yet the new paper claims that uncertainties in solar wind data are falsely giving rise to this idea.
The researchers say that the distance of the spacecraft taking solar wind measurements is the issue. Those spacecraft are millions of miles closer to the Sun than the Earth is, meaning that by the time those winds reach Earth, they have weakened considerably. Additionally, instrument error and the effects of the local plasma and field conditions all come into play.
All this, the researchers say, creates a mismatch between the measured strength of the wind and its effects on our planet’s electrical currents.
Correcting For Distance
The new findings contain one significant difference from existing research: they relied on observation platforms much closer to Earth to collect data, which included spacecraft such as NASA’s MMS and THEMIS.
Launched in 2007, THEMIS consists of five satellites that target the Earth, rather than the Sun, to study our planet’s magnetosphere and auroras. MMS consists of four spacecraft that also study the Earth’s magnetosphere.
Existing charts show the impact of solar winds on Earth leveling off at a certain threshold, which scientists had believed was the maximum saturation possible. However, in new solar wind strength data collected much closer to Earth, more accurately reflecting power at the time of impact, this saturation point disappeared. Instead, this data revealed that there is no ceiling on how heavily solar storms can charge the Earth’s electrical currents.
Solar Storm Impacts
Another crucial element in the NASA-led research is the statistical concept of regression to the mean, which holds that extreme measurements often change as more data come in. In this case, as more data on solar storm impacts on Earth recorded from various distances were collected, the plating effect disappeared. The authors note that similar effects occur in other areas of research, such as climate studies and chronic medical pain.
These new findings present a major challenge to our understanding of space weather. Scientists will now need to conduct many further observations to determine if any such ceiling exists. The threat to our infrastructure may be severe, as satellite communication underpins our modern society, not to mention the power grid, which keeps our world running.
For now, NASA continues to monitor solar storms to prepare for their potentially dangerous effects on our infrastructure, and in light of the new research, the potential for future challenges ahead may be greater than previously realized.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
For centuries, ancient seafarers have told tales of fabled lost lands. They have been known by many names—Ultima Thule, Hy-Brasil, the Fortunate Isles, and of course, the legendary lost city of Atlantis.
Now, scientists say Earth’s hidden plumbing system may be feeding one of its strangest ecosystems—an area on the Atlantic seafloor that conjures images of such legendary landscapes lost to time and memory.
Known as the Lost City hydrothermal field, this ancient Atlantic oddity is doing more than just broadening our view on how extremophiles thrive in some of our planet’s least hospitable environments: it offers a potential model for how extraterrestrial life may thrive elsewhere in our solar system.
In a recent paper published in Geophysics, Geochemistry, and Geosystems, an international team of researchers finally discovered the system behind these hydrogen- and methane-rich alkaline hot springs that feed the Lost City ecosystem.
The white carbonate chimneys that emit these gases provide an alternative to sunlight as the Lost City’s primary energy source, allowing life to thrive in a challenging deep ocean environment.
A view of the Lost City hydrothermal vent, located adjacent to the Mid-Atlantic Ridge (Image Credit: Susan Lang, University of South Carolina/National Science Foundation/ROV Jason 2018 WHOI)
Searching Near The Lost City
Those precious nutrients coming from these vents were created by underground reactions. It turns out that the water feeding the Lost City is likely part of a larger underground system, where extreme processes imbue the liquid with essential nutrients.
The discovery came from nearly a mile below the Atlantis Massif, a large block of Earth’s crust that forms an underwater mountain range. This dome-shaped region stretches for 10 miles and rises 14,000 feet above the ocean floor.
Above, a map shows the location of the Lost City on the Atlantis Massif (Image Credit: NOAA)
Geologists believe this formation originated between 1.5 and 2 million years ago, as tectonic plate movement pulled it out from beneath the Mid-Atlantic Ridge, forming a new feature on the ocean floor.
From aboard the Joint Oceanographic Institutions for Deep Earth Sampling (JOIDES) ship Resolution, scientists drilled their 4,160-foot-deep hole about 2,600 feet north of the Lost City. They were intrigued to find that the water recovered from the hole had a chemical composition extremely similar to that of water emerging from the Lost City vents.
Beneath The Ocean Floor
From their drill site, they pumped water from varying depths up to the surface for examination.
Roughly the first 1,500 feet consisted primarily of seawater and freshwater from the drilling process, yet at lower depths, they found water that had risen from beneath the rock. At the deepest depths, up to 80% of the sample came from these subterranean regions.
Their detailed analyses revealed that the water had reacted with the surrounding minerals to gain calcium while losing magnesium, a reaction that would require prolonged exposure to rocks at a temperature of at least 572°F. Despite this finding, the hole was much cooler when the team took their samples.
Typically, a water-rock reaction with gabbroic and ultramafic rock would produce such results that are high in calcium, yet with no magnesium. Other components, such as lithium, rubidium, cesium, and strontium, were found in the water at both the bore site and Lost City.
One of the Lost City’s many carbonate spires is shown in this image from the 2005 Lost City Expedition (Image Credit: IFE, URI-IAO, UW, Lost City Science Party; NOAA/OAR/OER; The Lost City 2005 Expedition)
The findings are consequential for providing the first direct evidence of this extremely hot water circulating beneath the Atlantis Massif through gabbroic and ultramafic rock. In this hidden plumbing system, seawater reaches deep within oceanic plates, providing energy to these deep-sea environments and potentially supporting their microbial life.
Feeding The Lost City
As researchers have now demonstrated that hydrogen-enriched water can naturally form deep within the Earth through rock reactions, researchers say there are major implications for our understanding of the Earth and beyond.
For one, it adds a new element to Earth’s energy cycles, explaining how life persists under such difficult, dark conditions. Secondly, it offers intriguing new ideas about how life might persist in extraterrestrial environments, as humans continue to search for it elsewhere in the cosmos. The strange conditions of the Lost City ecosystem are thought to be a potential model for how life could persist in the global oceans of ice-covered worlds such as Jupiter’s moon Europa or Saturn’s moon Enceladus.
However, some uncertainty about the samples does remain. Seawater, freshwater, and drilling contaminants were present in the samples, and the exact proportions attributable to gabbro or ultramafic rock are unknown. Also, while this is evidence for an underground connection between the borehole and the Lost City chimneys, it is not conclusive proof that they are connected.
Plans are already underway to return once the borehole has stabilized to collect pristine samples that will allow researchers to answer questions about where and how these reactions occur, as well as the amount of energy they add to the water. From the most inhospitable regions on Earth to the quest for organisms among the stars, the research underway deep within our oceans is providing new answers to how such life persists.
Micah Hanks, Editor in Chief of The Debrief, also contributed to this reporting.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
Using NSF’s Very Large Array (VLA), astronomers made the first radio detection of polarized light and Faraday rotation from a gamma-ray burst afterglow, offering an unprecedented glimpse of the magnetic fields surrounding one of the Universe’s most powerful explosions.
The molten iron core deep within our planet could be much more dynamic and complicated than previously known, as revealed in new studies that point to a current of liquid metal under the Pacific Ocean that reversed directions unexpectedly more than a decade ago.
The new findings provide additional insights into a sort of hidden “engine” driving the planet’s protective magnetic field, as detailed in new reporting featured in the Journal of Studies of Earth’s Deep Interior.
According to the research, long-held assumptions about large-scale flows occurring in Earth’s outer core are now being challenged, pushing back on previous notions that they evolve only gradually over time. Now, researchers say a broad region of molten iron beneath the equatorial Pacific abruptly shifted from a weak westward flow to a strong eastward current sometime around 2010.
Earth’s Magnetic Field
Since our planet’s magnetic field is produced by the movement of superheated, electrically conductive liquid iron that is close to 2,200 kilometers (1,370 miles) below the surface, sometimes even the most nuanced changes within these deep currents can fundamentally alter the magnetic field that shields the planet from harmful charged particles emitted by the Sun.
Discovering this unexpected reversal required scientists to combine close to three decades of ground-based magnetic observations with satellite data collected from 1997 until 2025. The European Space Agency’s (ESA) Swarm Mission provided measurements, which, combined with previous observations made possible through German CHAMP and Danish Ørsted satellites, helped researchers behind the new work to construct a precise model of the changing flow patterns occurring at the boundary between Earth’s core and mantle.
“The large-scale flow reversal beneath the Pacific raises new questions about the behavior of Earth’s deep interior,” said lead author Frederik Dahl Madsen of the University of Edinburgh’s School of Geosciences.
“Scientists now want to understand whether the reversal represents a short-lived fluctuation, part of a repeating oscillation, or a new stable equilibrium for core circulation,” Madsen said.
A Weakening Current
Among their findings, the team also said they uncovered evidence that the strong eastward current appears to have weakened since 2020, raising the possibility that the reversal could represent part of a longer natural cycle.
According to Madsen, the shift coincided with changes inferred within Earth’s solid inner core, which suggests previously unrecognized links between the planet’s deepest layers.
“The rise of the strong eastward flow in the Pacific is contemporary with a change in behaviour in the inner core, as inferred from geodesy and seismology, and we hypothesize that these changes in the deep interior are associated with the changes in flow beneath the Pacific,” Madsen said.
While such processes occur thousands of kilometers beneath our planet’s surface and pose no direct dangers, they nonetheless have a vital part in sustaining Earth’s magnetic field.
Although invisible, the magnetic shielding capability it provides protects our atmosphere from solar radiation, while supporting the technologies many of us rely on daily for navigation, space weather monitoring and forecasting, and a range of other things.
ESA scientists say that in the long term, satellite missions like its Swarm mission provide a detailed picture of what’s happening in Earth’s hidden interior. That data is also revealing how the planet’s molten core may be considerably more variable and complex than once thought.
Going forward, Madsen says he and his colleagues will continue to look at how the molten flow deep within the earth is changing over time.
“Continued monitoring will be essential to determine how the flow evolves over the coming years,” Madsen said of the team’s ongoing work.
The team’s recent study, “Principal component analysis of the 2010 reversal of core-surface flow beneath the Pacific Ocean,” was published in the Journal of Studies of Earth’s Deep Interior.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached atmicah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
An exoplanet is exerting a magnetic influence on its host star in a manner opposite to what astronomers normally observe, according to researchers at the Institute of Astrophysics of Andalusia (IAA-CSIC).
In a recent paper published in Science, IAA-CSIC researchers revealed how the exoplanet GJ 436 b is affecting its host star’s behavior in a never-before-seen way. In their work, the team developed a novel method to estimate an exoplanet‘s magnetic field strength, an important factor in determining habitability.
“Until recently it was thought that it was mainly the star that influenced the planet,” said Rafael Luque, an IAA-CSIC researcher and one of the new study’s co-authors.
Luque adds that his team’s results now offer “the clearest evidence to date of something that had already been suspected: that the opposite can also happen and that a nearby planet can alter the environment of its star.”
Life and Magnetic Fields
While the most obvious ingredients for a habitable planet are water and a breathable atmosphere, other elements are less apparent to us based on our human experience. Our planet’s invisible magnetic field protects us from the solar wind and holds the atmosphere together.
While Earth’s magnetic field guided the evolution of its atmosphere, Mars provides an example of what the loss of a magnetic field can do to an otherwise potentially habitable planet. When the Martian magnetic field disappeared four billion years ago as the planet’s core rapidly cooled, the atmosphere dissipated, followed by the loss of surface water.
As shown by the fates of two cosmic neighbors like Earth and Mars, a stable magnetic field is a key element of habitability.
With its proximity and its host star’s low mass, GJ 436 b exhibits considerable influence in the inverse of the normal planet-star relationship. Credits: IAA-CSIC/LampScience
Observing Exoplanet Magnetic Fields
Detecting magnetic fields on distant exoplanets has proven more challenging for astronomers than other observations, such as atmospheric composition. In their new paper, the IAA-CSIC team provides the first conclusive evidence of an exoplanet’s magnetic field, observed through its impact on the host star.
“In particular, we have observed that GJ 436 b, an exoplanet similar to Neptune that orbits very close to its star, causes regular changes in the brightness and energy emitted by the star at certain wavelengths,” explained lead author Daniel Revilla, an IAA-CSIC researcher who led the study as part of his doctoral thesis.
GJ 436 b provided the team with measurable signals that allowed them to infer that the exoplanet had a magnetic field and estimate its strength. The IAA-CSIC team analyzed sixteen years of spectroscopic observations of the GJ-436 system for their research, collected by the CARMENES instrument at the Calar Alto Observatory.
“Despite its smaller size, GJ 436 b would have a magnetic field between 2.33 and 27 times more intense than that of Jupiter,” said co-author Pedro J. Beloved, a researcher at the IAA-CSIC.
A Strange Interaction
In the paper, the researchers demonstrate how, in a very close orbit, a planet can flip the normal planet-star relationship, with the planet controlling the influence of gravity, radiation, and magnetic fields between the two. As the exoplanet interacts with its host star, it injects energy into the star’s chromosphere to produce a phenomenon like a stellar aurora.
This strange interaction has only been measured periodically, occurring in eight-year cycles, with observations in 2008, 2016, and 2024. Intriguingly, these years correlate to phases of the host star’s magnetic cycle, which the researchers believe affects the intensity.
“Until now, measuring the magnetic field of an exoplanet was extremely difficult,” Devilla concluded. “This property is key to knowing if a planet can protect its atmosphere and, ultimately, if it could harbor life.”
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
The experiment centered on the Aharonov–Bohm effect, a strangequantum phenomenon where electrons respond to a magnetic field even when they never actually pass through it. First predicted back in 1959, this effect has been notoriously difficult to confirm because the changes it causes in electronwaves are incredibly subtle.
In 1980, physicist Michael Berry showed that classical systems could model the Aharonov–Bohm effect. In this analogy, a vortex at the center of a water tank replaces the solenoid that creates a magnetic field in the quantum experiment. Water waves take the place of electrons. When these waves travel around the vortex, rather than through it, they acquire a measurable distortion. This appears as a pitchfork-shaped pattern in the wave fronts, showing that the vortex changes the phase of the waves without direct contact. The OIST team extended the approach by testing a new scenario.
“With waves traveling the opposite direction, you see a mirror image pattern,” says Jonas Rønning, co- author and former postdoc in the OIST unit. “The question for us was, what happens if you send waves from both directions at the same time? We thought that the patterns might cancel each other out, or both pitchfork-like patterns would be visible, but our intuition was completely wrong.”
Two Waves Walk Into a Vortex
The researchers constructed a custom tank, created a vortex at its center, and sent waves from opposite sides to meet in the middle. They used a high-speed camera to observe how the waves interacted on the water’s surface.
Without a vortex, the peaks and troughs remain in place. When the vortex is there, the standing wave breaks down. The vortex shifts the phase of the waves as they travel around it, altering the standing-wave interference pattern and creating rotating nodal lines. These are lines of momentarily flat water that spiral outward and turn in the opposite direction of the vortex.
“This was something new and unexpected,” says Aditya Singh, a PhD student in the Nonlinear and Non-equilibrium Physics Unit and co-first author of the study. “That’s what makes this fluid analogue system so valuable. It reveals topological effects — wave behaviors that occur across the whole system — that can’t be seen in quantum experiments.”
At first, the team suspected their equipment was causing the rotating lines. However, the same pattern also appeared in their computer simulations.
“When we first saw these lines, we thought they were an experimental artifact,” Singh says. “But when we also saw them in our simulations, we dropped everything and quickly worked out the mathematics underlying how they arise.”
More Speed, More Lines
As the strength of the vortex increased, more rotating nodal lines appeared, always moving in the direction opposite to the vortex. The study showed that the number of lines is quantized, meaning it is fixed to whole-number values determined by the vortex’s circulation. In other words, the topology of the vortex determines how many rotating nodal lines appear. This effect was observed across the entire wave field, not just near the vortex core as earlier models suggested.
This finding differs from Berry’s original experiment, which observed changes only near the vortex. In this case, the researchers discovered a non-local effect, a pattern that covers the entire system and depends on the overall setup. Instead of being limited to the area near the vortex, the rotating nodal lines appeared throughout the whole standing-wave pattern.
Although the practical uses of these newly discovered nodal patterns are not yet clear, the study shows that simple classical systems can reveal behaviors that are challenging to observe in quantum experiments. By making these effects visible, the researchers plan to explore more complex wave systems that could offer new insights into superconductivity and other quantum phenomena.
“One direction is to make the system more complex by introducing multiple vortices and arranging them into a lattice,” senior author Mahesh Bandi says. “That setup would mirror conditions in some superconducting materials, with the water waves behaving like a supercurrent. We don’t yet know what we’ll see — and that’s exactly what makes it worth doing.”
Austin Burgess is a writer and researcher with a background in sales, marketing, and data analytics. He holds an MBA, a Bachelor of Science in Business Administration, and a data analytics certification. His work focuses on breaking scientific developments, with an emphasis on emerging biology, cognitive neuroscience, and archaeological discoveries.
Allies of Sir Keir Starmer believe he is preparing to step down as he realises the "game is up" after facing an evaporation of support over the weekend.
Keir Starmer has been given 72 hours to quit with "dignity" or face a full-blown coup following Andy Burnham's by-election landslide as the challenger plots a Left-wing "path for Britain".
Sir Keir Starmer is braced for Ed Miliband to resign next week as part of a co-ordinated coup to force him out should he refuse to make way for an Andy Burnham coronation.
“I think if you have a creative voice in writing or design, you put yourself out there and you take a risk — this is a good time to do that,” said the Figma chief executive Dylan Field.
Can anyone or anything stop Andy Burnham becoming PM now, asks Mark Littlewood in his latest Political Betting column as he contemplates breaking his usual rule and taking the 2/5 odds-on bet.
My book, "The Physics of Creation: The Creator’s Ultimate Design for Earth," is now available for download at CreationToday.org for under $5. The book offers a unique perspective on the universe, linking physical laws to an intelligent Creator, and explores how scientific principles align with the biblical creation narrative.
By tracking fierce winds racing through the atmospheres of seven ultra-hot Jupiters, astronomers have uncovered the strongest evidence yet that magnetic fields shape weather on worlds beyond our Solar System.
This book by Matthew Littlefield seeks to explore a broad understanding of how evil works in this world, and even delves deeply into issues that the modern church has either forgotten, downplayed or even been deceived on. I strongly recommend you buy the book.
The Scofield Reference Bible, published in 1909, aimed to garner support from American Evangelicals for the Zionist state of Israel, emphasizing a dispensationalist view that separates Jewish and Christian covenants. This interpretive system has significantly influenced modern Christian thought, often at the expense of the core message of the gospel of Jesus Christ.
In this presentation I discuss the drastic reduction in human lifespans after the global flood, from 910-970 years to about 70 years. I link these changes to factors such as biological decay, genetic entropy, Earth’s altered magnetic field and loss of physiological resilience. Eternal lifespans can only be restored through Jesus Christ.
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