Adapted from a release written by Alison Auld for Dalhousie University
Lamont’s R/V Marcus G. Langseth. Credit: Anne Becel
A new study published in Science Advances has revealed the first detailed images of a newly developing subduction zone off the coast of British Columbia’s Haida Gwaii archipelago.
The international team of researchers collected the data for this study during a 2021 cruise by the Lamont-Doherty Earth Observatory’s research vessel, the Marcus G. Langseth. They used a 15-kilometer-long underwater cable equipped with thousands of underwater microphones, called hydrophones, in the area off northern British Columbia to map the deep structure of the Earth’s subsurface.
Their data confirmed that the Queen Charlotte fault system can generate powerful megathrust earthquakes, which are capable of producing strong shaking and tsunamis.
Map of the study area, showing the location of the Queen Charlotte Fault (QCF) in relation to the Pacific (PAC), North America (NA), Yakutat (YAK), Explorer (EXP) and Juan De Fuca (JdF) tectonic plates.
Megathrusts are found in areas where one tectonic plate dives beneath another, in this case the Pacific plate being pushed under the North American plate. This area is known for generating powerful tremors. In fact, the Queen Charlotte fault system represents the greatest seismic hazard in Canada, producing the country’s largest recorded earthquake in 1949 and a notable earthquake in 2012 that created a tsunami.
“This region is actively becoming a subduction zone, so understanding the fault structure here tells us about the early stages of subduction zone development,” says lead author Collin Brandl, a postdoctoral research scientist at the Lamont-Doherty Earth Observatory, part of the Columbia Climate School. “Our study provides the first direct observations of the Haida Gwaii thrust, the “megathrust” of this system, which can help improve hazard analysis in the region, better preparing residents for future earthquakes and tsunamis.”
Brandl’s co-authors are part of an international team, with scientists from the University of New Mexico, Western Washington University, the U.S. Naval Research Laboratory, Boise State University, Nova Scotia’s Dalhousie University, the University of British Columbia, the University of Victoria, the Geological Survey of Canada, and the Universidad de Chile.
Press interviews with Collin Brandl can be arranged by emailing press@columbia.edu.
In nature’s endless game of survival and attraction, appearances can deceive. A soft flutter of wings might signal prey, a wasp, or danger. A bright color could warn of poison or invite a mate. But in one curious case, a dancing jumping spider has taken deception to a whole new level.
Jumping spiders are not what people typically imagine when they think of showy, dramatic displays. Yet one species, the Maratus vespa, does something few creatures dare. This jumping spider imitates one of its biggest threats – a wasp.
This surprising performance raised a question that scientists at the University of Cincinnati couldn’t ignore: why would a spider mimic a predator during something as important as courtship?
That question led to an experiment unlike most in behavioral biology. And the journey from simple curiosity to machine-aided discovery unveiled a strange and brilliant piece of evolutionary theater.
Jumping spiders in a wasp disguise
With travel restrictions in place during the COVID-19 pandemic, fieldwork came to a halt. But curiosity did not. Biologists at the University of Cincinnati turned to computers, hoping to uncover the secrets behind the spider’s dramatic disguise.
Humans often see faces where none exist, on rocks, in tree bark, even in cloud formations. Scientists wondered if the spider’s “wasp face” was a real mimicry or simply a trick of human perception.
To answer this question, the researchers needed a third party without such bias. They used computer vision techniques and machine learning.
Neural networks were trained to identify and classify images of different insect and spider species based on patterns and shapes. The test included 62 species, from jumping spiders to flies and wasps.
Wasp-like spiders trick algorithm
The results surprised the researchers. The artificial intelligence made classification errors nearly 12 percent of the time across all species. Thirteen species were identified correctly every single time. But others were harder to pin down.
“The original idea was inspired by one species, a peacock jumping spider called Maratus vespa, which is Latin for wasp,” said UC student and study lead author Olivia Harris.
In the case of Maratus vespa and a few other spiders, the AI struggled more than usual. It misidentified these spiders as wasps more than 20 percent of the time. Even without human bias, the computer saw what looked like a wasp.
This revealed something important. The spider’s mimicry may be strong enough to fool not just people but machines as well. If artificial intelligence gets confused, real predators might too.
Spider’s dance looks like a wasp
Maratus vespa is no ordinary spider. During courtship, it performs an elaborate dance. It raises its abdomen to display bright, bold patterns. The colors echo those of a wasp’s body. But it doesn’t stop there.
This jumping spider also raises side flaps on its body. The added shape creates the outline of a wasp’s triangular face.
The mimicry becomes more convincing with movement, colors, and structure. And this illusion, oddly enough, is used in one of the most vulnerable moments of its life, mating.
“That got us thinking,” Harris said. “Why would a spider want to look like a wasp, which is a predator of spiders, especially as a primary element of its courtship display?” The answer lies in attention, survival, and split-second timing.
Male jumping spiders seeking attention
Jumping spiders are highly visual animals. They have multiple sets of eyes, each with different abilities. Females especially are careful observers.
When they detect movement from afar, particularly something that resembles a predator, they freeze and focus.
It turns out, this reaction might give males a critical opening. If the female thinks a wasp is nearby, she becomes alert but still. That moment of pause may allow the male spider to begin his courtship display.
The study’s authors believe the male uses this mimicry as a tactic. It isn’t to scare her, but to capture her attention and hold it long enough to start the dance.
Spiders aren’t the only tricksters
Nature is full of strange strategies when it comes to attracting mates. Some male moths, for example, imitate the ultrasonic calls of bats. This discourages females from flying away.
In Africa, topi antelope bulls pretend to spot predators to stop females from leaving their territory.
“But this is the only case we’ve found of males mimicking a predator visually,” she said.
Visual mimicry as a courtship trick remains extremely rare. That makes the Maratus vespa spider an unusual and fascinating example.
The study suggests this behavior represents a form of sensory exploitation. The male takes advantage of how the female processes visual information.
The limits of illusion
Professor Nathan Morehouse, who co-authored the study, explained that the illusion works best from a distance or from the female’s side view.
These angles rely on her peripheral vision, which sees only in green. At that range, the bright pattern and angular shape suggest danger. But when the male moves closer, the illusion wears off.
“Females will not be fooled forever. If they were, they would be robbed of the ability to make mate choices, which would put the species at a long-term disadvantage,” Morehouse said. “It’s beneficial for the males to break the illusion.”
In other words, the mimicry is a tool to get noticed, not to deceive permanently. The female must still decide if the male is worthy. And once she’s focused, she uses her color-sensitive front eyes to make that decision.
Jumping spiders posing as wasps
The team now hopes to follow up with behavioral studies. They want to test if live female spiders behave differently based on the strength of the male’s visual mimicry.
Do some jumping spiders copy wasps better than others? Do females prefer males with more convincing patterns? And can these differences affect which males succeed in passing on their genes?
These questions may reveal even more about how animals use deception not just for survival, but for love.
In the meantime, Maratus vespa continues to dance its strange, bright, and possibly risky dance in the wilds of Australia. A spider pretending to be its enemy, all in the name of romance.
The study is published in the journal Behavioral Ecology.
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In 2008, Erez Ben-Yosef unearthed a piece of Iron Age “trash” and inadvertently revealed the strongest magnetic-field anomaly ever found.
Ben-Yosef, an archaeologist at Tel Aviv University, had been working in southern Jordan with Ron Shaar, who was analyzing archaeological materials around the Levant. Shaar, a geologist at The Hebrew University of Jerusalem, was building a record of the area’s magnetic field.
The hunk of copper slag — a waste byproduct of forging metals — they found recorded an intense spike in Earth’s magnetic field around 3,000 years ago.
When Ben-Yosef’s team first described their discovery, many geophysicists were skeptical because the magnitude of the spike was unprecedented in geologic history. “There was no model that could explain such a spike,” Ben-Yosef told Live Science.
Related: Major ‘magnetic anomaly’ discovered deep below New Zealand’s Lake Rotorua
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So Shaar worked hard to give them more evidence. After they had analyzed and described samples from around the region for more than a decade, the anomaly was accepted by the research community and named the Levantine Iron Age Anomaly (LIAA). From about 1100 to 550 B.C., the magnetic field emanating from the Middle East fluctuated in intense surges.
Shaar and Ben-Yosef were using a relatively new technique called archaeomagnetism. With this method, geophysicists can peer into the magnetic particles inside archaeological materials like metal waste, pottery and building stone to recreate Earth’s magnetic past.
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This technique has some advantages over traditional methods of reconstructing Earth’s magnetic field, particularly for studying the relatively recent past.
Generally, scientists study Earth’s past magnetic field by looking at snapshots captured in rocks as they cooled into solids. But rock formation doesn’t happen often, so for the most part, it gives scientists a glimpse of Earth’s magnetic field hundreds of thousands to millions of years ago, or after relatively rare events, like volcanic eruptions. Past magnetic-field data helps us understand the “geodynamo” — the engine that generates our planet’s protective magnetic field. This field is generated by liquid iron slowly moving around the planet’s outer core, and this movement can also affect, and in turn be affected by, processes in the mantle, Earth’s middle layer. So differences in the magnetic field hint at turmoil roiling deep below the surface in Earth’s geodynamo.
Locations where researchers have found archaeological samples with evidence of the Levantine Iron Age Anomaly. (Image credit: Locations where evidence of the Levantine Iron Age Anomaly has been found.)
“We cannot directly observe what is going on in Earth’s outer core,” Shaar told Live Science. “The only way we can indirectly measure what is happening in the core is by looking at changes in the geomagnetic field.”
Knowing what the magnetic field did in the past can help us predict its future. And some studies suggest our planet’s magnetic field is weakening over time. The magnetic field shields us from deadly space radiation, so its weakening could lead to a breakdown in satellite communications, and potentially increase cancer risk. As a result, predicting the magnetic field based on its past behavior has become ever more important. But observational data of the magnetic field’s intensity only began in 1832, so it’s difficult to make predictions about the future if we only dimly understand the forces that steered the magnetic field in the past. Archaeomagnetism has started to fill these gaps.
How do we see the magnetic field from an archaeological artifact?
Archaeomagnetism takes advantage of our human ancestors’ harnessing of the earth around them — they started building firepits, making bricks and ceramics, and eventually, smelting metals.
In each of these tasks, materials are heated to intense temperatures. At high enough temperatures, thermal energy makes the particles inside a material dance around. Then, as the material is removed from the fire and cools, the magnetically sensitive particles inside naturally orient in the direction of Earth’s magnetic field, like miniature compass needles. They become “stuck” in place as the material hardens, and will retain this magnetic orientation unless the material is heated again.
The settled magnetic particles in an archaeological artifact offer a unique snapshot of the magnetic field at the time the material was last hot. This snapshot is regional, spanning a radius of about 310 miles (500 kilometers) around the sample — the scale at which the magnetic field is thought to be uniform, Shaar said. When the sample is dated with radiocarbon or other techniques, scientists can begin to build a chronological record of an area’s magnetic field.
These artifacts are so helpful for geophysicists because Earth’s magnetic field constantly drifts. For instance, in 2001, the magnetic north pole was closer to the very northern tip of Canada, but by 2007, it had moved over 200 miles (320 km) closer to the geographic north pole. That’s because two large “lobes” of strong magnetism, called flux patches, in the outer core underneath Canada and Siberia act as funnels for the magnetic field, pulling it into Earth. As these lobes shift, they move magnetic north.
And while most of the planet’s magnetic-field lines go from north to south, about 20% diverge from these paths, swirling to form eddies called magnetic anomalies.
It’s these anomalies that researchers are struggling to explain, and that artifacts could reveal.
A growing field
Although archaeomagnetism has been around since the 1950s, magnetic-field-measuring technologies, like the magnetometer, have improved dramatically since then. Refined statistical analysis techniques also now allow much more detailed interpretation of archaeomagnetic data.
To get all of the data in one place and synthesize our understanding of Earth’s magnetic field, scientists have started to build a global database called Geomagia50, hosted at the University of Minnesota’s (UM) Institute for Rock Magnetism. But even as the technique grows in popularity, there are many hurdles to widespread adoption.
“The equipment is quite expensive,” Maxwell Brown, a UM geophysicist and custodian of the Geomagia50 database, told Live Science. The most precise magnetometers can cost between $700,000 and $800,000, Brown said. “So there are only a few labs in the [United States] that have one of these.”
Yoav Vaknin, an archaeologist at Tel-Aviv University and The Hebrew University of Jerusalem, collects samples from a burnt Iron Age structure in Jerusalem. (Image credit: Yoav Vaknin)
As a result, about 90% of the data in the Geomagia50 database has come from Europe, Brown said. Africa doesn’t have a single magnetometer available to geophysicists for archaeomagnetic sampling, meaning our magnetic snapshot of the continent is largely blank. Additionally, there are no current avenues for the average archaeologist to send their artifacts to be sampled, Ben-Yosef added. Anyone without a magnetometer has to set up an official partnership with someone who does have one.
Even if the equipment is available, sampling takes time and expertise, Shaar said. Measuring the direction of the field can sometimes be relatively simple, but understanding the intensity of the field takes much more work. The sample must be heated and reheated 20 separate times, gradually replacing the original magnetization and destroying the sample.
“It sounds like it’s an easy thing: We put it in a magnetometer or instrument, and we get the results. No. For each artifact, we spend two months working in the lab, making experiments and then getting the results. It’s a complicated, experimental procedure,” Shaar explained.
This lack of global data limits our understanding of what the magnetic field has been up to in recent history. “We clearly have a very strong bias [toward Europe] in the data distribution,” Monika Korte, a geophysicist and magnetic modeler at Germany’s GFZ Helmholtz Centre for Geosciences, told Live Science. “Where we have sparse data we have just a very blurred picture, a very rough idea of what’s going on.”
Geographic diversity is important, as samples taken from one area can indicate the magnetic field only in that area.
For instance, other data similar to the Levantine Iron Age Anomaly’s intense spikes of magnetic strength have been spotted in places like China and Korea around the Iron Age as well, but there’s not enough evidence to confirm these as bona fide anomalies or to say whether they are related to the Levantine Iron Age Anomaly, Korte said.
Why should we learn more about historic anomalies?
The discovery of the Levantine Iron Age Anomaly redefined our previous understanding of the potential strength of the field, Shaar said. Understanding how much the magnetic field can change may seem like a purely abstract endeavor, but these ancient fluctuations may have implications for modern times.
Another important anomaly is the South Atlantic Anomaly (SAA), a region of weakened magnetic field that spans central South America in a strip that ends near southern Africa. It likely first emerged 11 million years ago, caused by the slight difference in location of the magnetic axis and the rotational axis at Earth’s core. As the magnetic field is slightly off-center to the rotational axis, the field dips in strength over the South Atlantic, though the field’s interaction with the churning mantle may also contribute to the anomaly.
The South Atlantic Anomaly still exists today, and has disrupted communications from satellites and the International Space Station, as the weak magnetic field in the region lets through more radiation from solar wind. Studying the SAA throughout its history has helped scientists understand how our magnetic field changes over time, and how such anomalies alter the likelihood of a magnetic field reversal, when Earth’s north and south poles flip.
But although scientists have a reasonable understanding of the South Atlantic Anomaly, its weakened magnetic field is very different from the strong spikes of the Levantine Iron Age Anomaly, which has baffled geophysicists. And though researchers haven’t pinpointed the exact extent of the anomaly, its seemingly small scale of around 1,000 miles (1,609 km) across, combined with the extremely high spikes in the magnetic field, isn’t easily explained.
Some geomagnetists had suggested that the Levantine Iron Age Anomaly developed due to a narrow flux patch that developed on the outer core under the equator before it drifted north towards the Levant, potentially contributing to other spikes of intensity recorded in China. The inverse of the large lobes that funnel the magnetic field into the planet at the North Pole, this “positive” flux patch would have pushed the field out in a powerful burst. Others believed the single flux patch didn’t travel, instead multiple grew under the Levant, erupted, and decayed in place. Still, no theories can explain why the flux patch developed in the first place.
With the most up-to-date archaeomagnetic data, geomagnetist Pablo Rivera at the Complutense University of Madrid published a paper in January that simulated both the Levantine Iron Age Anomaly and the South Atlantic Anomaly. By modeling their movement over time, his work suggested that both anomalies may have been influenced by a superplume underneath Africa — a massive blob of hot rock on the barrier between the core and the mantle that may disrupt the flow of the geodynamo below it.
However, much is still unknown.
“So far, there is not a single simulation that really describes all the [magnetic] features that we see well,” Korte told Live Science.
Many archaeomagnetic data points from around the globe suggest there may be more intensity spikes that could help resolve the mystery and create a unifying theory to explain the SAA, the LIAA and other spikes. But there currently isn’t enough data to describe them accurately, or even begin to understand their causes.
“We don’t really understand what causes these anomalies, but we hope to learn more about how the geodynamo operates and what kinds of changes we also can expect for the future magnetic field,” Korte said.
This certainty is needed now more than ever, as more of our communications take to the skies. More than 13,500 satellites currently orbit Earth — a dramatic increase from only around 3,000 in 2020. The Government Accountability Agency estimates that another 54,000 satellites will launch by 2030. These satellites monitor weather patterns, send phone and TV signals, and create GPS.
Satellites are generally protected from space radiation by Earth’s magnetic field. But in places where the field is weaker, such as above the South Atlantic Anomaly, satellites have more memory problems as radiation bombards onboard computers and corrupts data.
Filling out the picture
Despite the expense and technical challenges of archaeomagnetism, there are many initiatives to expand the amount of data. In the U.S., the Institute for Rock Magnetism is expanding its archaeomagnetism program to begin building a more thorough history of the magnetic field in the Midwest, hoping to build their own localized dating system using archaeomagnetism, similar to the record Shaar and his collaborators have built in the Levant.
Interest in archaeomagnetism is also growing around the globe. The first archaeomagnetism data from Cambodia was published in 2021, and the first regional model of the magnetic field of Africa for the recent past was published in 2022.
As the field of archaeomagnetism grows, scientists can start building a better understanding of how features like superplumes affect the magnetic field. The past 50 or so years of data has captured “only a really tiny snapshot in time,” Shaar said, and “maybe there are more [anomalies] to find.”
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Chemists at The Ohio State University have developed a new approach for generating reactive carbon-based intermediates known as metal carbenes, according to a study published in Science. These intermediates serve as essential building blocks in the synthesis of pharmaceuticals and materials.
Carbenes are short-lived, highly reactive species that contain a divalent carbon atom. While valuable in chemical transformations, they are often challenging to produce due to their instability and the hazardous conditions typically required for their formation.
The Ohio State team reports a method that uses iron as a catalyst along with chlorine-containing molecules that release radicals. Together, these components generate carbenes under milder conditions. The resulting carbenes can then undergo a reaction to form cyclopropanes – three-membered ring structures commonly found in medicines and agrochemicals.
“Our goal all along was to determine if we could come up with new methods of accessing carbenes that others hadn’t found before,” said David Nagib, co-author of the study, a distinguished professor in arts and sciences and a professor of chemistry and biochemistry at The Ohio State University. “Because if you could harness them in a milder catalytic way, you could reach new reactivity, which is essentially what we did.”
Cyclopropanes are valued for their compact size and high ring strain, which can influence the biological activity of compounds. Although many synthetic routes to these structures exist, the new method provides an alternative path by accessing carbenes that were previously difficult or impossible to create.
Enabling faster and safer transformations
The researchers also found that their new method can also be carried out effectively in water, raising the possibility that carbenes could one day be generated inside of living cells. Such an approach could be transformative in discovering new drug targets, according to the researchers.
Having access to a new way of creating carbenes that can replace the current, more wasteful approaches, could also help to bring down the cost of drugs by making their production safer and easier.
Similarly, the researchers hope that this method could help to prevent shortages of important medicines, including antibiotics, antidepressants and treatments for conditions such as heart disease, COVID and HIV.
Looking ahead, the team plans to continue refining the approach and exploring how the reaction might be extended to other catalysts and molecular targets.
“Our team at Ohio State came together in the coolest, most collaborative way to develop this tool,” Nagib said. “So we’re going to continue racing to show how many different types of catalysts it could work on and make all kinds of challenging and valuable molecules.”
Reference: Nguyen KNM, Mo X, DeMuynck BM, et al. Harnessing carbene polarity: Unified catalytic access to donor, neutral, and acceptor carbenes. Science. 2025;389(6756):183-189. doi: 10.1126/science.adw4177
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Last month, the parachutes on Hélène Huby’s small spacecraft failed to deploy, and the vehicle and its cargo crashed into the ocean on Earth.
It was both a success and a failure.
The success was that after Huby founded The Exploration Company in Europe, she managed to move nimbly with the “Mission Possible” spacecraft such that it cost less than $25 million to build and reached space in less than three years. The vehicle ticked off a number of successes in spaceflight before making a controlled descent through the atmosphere.
But at 26 km above the planet, as the spacecraft slowed to Mach one, The Exploration Company lost contact. Huby was not sure how this loss would be received in Europe, where failures in spaceflight have not been traditionally well-tolerated.
“What was interesting is the feedback I got in Europe,” Huby said in an interview this week at the company’s offices in Houston. “The German Space Agency, the French space agency, the European Space Agency said, OK, that’s a great achievement. For the time and money we spent, performing 80 percent of that mission was a good investment.”
No drop tests
After the spacecraft was lost on June 24, the company established an independent investigation team. Huby said it is “99 percent” confirmed there was a problem with the deployment of the parachutes, either the drogue chutes or the main parachutes. The fault was not with the provider of the parachutes themselves, US-based Airborne Systems, but the company’s mechanism, she said.
To save time and money, The Exploration Company did not conduct any drop tests. Such a campaign would have added millions of dollars to a program that was trying to be lean, plus a year of schedule to a mission attempting to move fast.
“We made a mistake, basically, to underestimate the risks,” she said. In retrospect, Huby added, the company could have done more testing on the ground.
Now the firm faces a big decision: How to proceed from here. One option is building another small spacecraft, similar to Mission Possible, for testing purposes. But there is limited commonality in the parachute system for this vehicle and the larger Nyx spacecraft the company is building for operational missions. So if the Mission Possible parachutes were to work, that would not guarantee success for Nyx.
The NSF–DOE Vera C. Rubin Observatory has released its first images, demonstrating its capabilities just two months after beginning trial operations. Built in Chile over nearly three decades at a cost of more than one billion dollars, the American observatory’s debut images showcase its exceptional imaging power.
The telescope features an exceptionally wide field of view — 3.5 degrees by 3.5 degrees — with each image covering a section of the sky approximately 45 times larger than the full Moon. It is designed to capture around 1,000 images per night, enabling a complete survey of the southern sky every three to four nights. This means each region of the sky will be imaged about 800 times over the course of the telescope’s planned 10 years of operation.
3 View gallery
Giant images with unprecedented detail. The Trifid Nebula and Lagoon Nebula, located several thousand light-years away, captured in a composite made from 678 exposures by the Vera C. Rubin Observatory
(Photo: RubinObs/NOIRLab/SLAC/NSF/DOE/AURA)
Unlike narrow-field telescopes, which are designed to zoom in on individual objects and examine them in detail, wide-field telescopes scan large areas of the sky. This broad view allows scientists to monitor changes and transient phenomena, discover previously unknown celestial objects, and, when needed, guide other telescopes to study them more closely.
The Rubin telescope is equipped with an 8.4-meter primary mirror — modest in comparison to upcoming next-generation ground-based telescopes like the Giant Magellan Telescope, which will feature a 25-meter mirror and is expected to begin operations in 2030. While not larger than many current operational telescopes, Vera Rubin’s great advantage lies in its extremely sophisticated camera, roughly the size of a small car and weighing about three tons. Each image it captures is 3,200 megapixels, making it the largest digital camera in the world.
The camera aboard the Rubin telescope uses six color filters, each isolating a narrow wavelength range — effectively capturing one color at a time. A sophisticated mechanical system allows the filters to be swapped within minutes, enabling near-simultaneous imaging of the same region of sky in several colors. Final images are composites of many individual exposures and contain enormous amounts of data.
Due to the size of its mirror, the telescope is not designed to focus on specific details such as a specific galaxy or solar system, unlike large ground-based telescopes or space telescopes like James Webb and Hubble. Instead, its strength lies in its wide-field, high-detail images, which are expected to allow for the identification of countless celestial objects and, as noted, enable the continuous monitoring of dynamic processes over time. In total, the telescope is expected to collect about 20 terabytes of data each night (that’s 20,000 gigabytes), and over the course of its operations, to accumulate approximately 500 petabytes (half a billion gigabytes) of information — comprising astronomical images and a detailed catalog of billions of stars, galaxies, and other celestial bodies.
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Billions of galaxies in one snap
(Photo: RubinObs/NOIRLab/SLAC/NSF/DOE/AURA/P. Horálek (Institute of Physics in Opava))
The telescope is expected to collect about 20 terabytes of data each night (20,000 gigabytes) and, over its 10-year operational lifetime, to accumulate roughly 500 petabytes (half a billion gigabytes) of astronomical images and detailed catalogs of billions of stars, galaxies, and other celestial bodies.
Researchers estimate that the Rubin telescope will identify more stars and planetary systems than any previous instrument, while also boosting planetary defense efforts through the detection of numerous asteroids — including some that may pose future threats to Earth. Even during its trial phase, the telescope identified more than 2,000 previously unknown asteroids in just ten hours of imaging. For comparison, the current global discovery rate is about 20,000 new asteroids per year.
“NSF-DOE Rubin Observatory will capture more information about our universe than all optical telescopes throughout history combined,” said Brian Stone, acting director of the U.S. National Science Foundation (NSF). “Through this remarkable scientific facility, we will explore many cosmic mysteries, including the dark matter and dark energy that permeate the universe.”
Even during its trial phase, the Vera C. Rubin Observatory identified more than 2,000 previously unknown asteroids. A video demonstration of the telescope’s detection capabilities.
The Vera C. Rubin Observatory is located at the summit Cerro Pachón in central Chile, at an elevation of nearly 2,700 meters (8,860 feet) above sea level. In recent decades, Chile has become the world’s hub for optical astronomy — thanks to a combination of geographic and human factors: high mountain peaks that allow observation above a portion of the atmosphere, dry air with minimal cloud cover, and remote locations free from light pollution.
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The NSF–DOE Vera C. Rubin Observatory in Chile
(Photo: RubinObs/NOIRLab/SLAC/NSF/DOE/AURA/P. Horálek (Institute of Physics in Opava))
Named after American astronomer Vera Rubin (1928–2016) — who made groundbreaking discoveries about the rotational speeds of galaxies and whose work laid the foundation for the dark matter theory — the idea of an invisible mass that explains galaxies’ unexpectedly rapid motion — the telescope is expected to significantly advance our understanding of the universe. Researchers also hope it will help unravel the mystery of dark energy, the force thought to drive the universe’s accelerated expansion, and shed light on other fundamental cosmic puzzles.
The telescope is jointly operated by scientists at the SLAC National Accelerator Laboratory (part of the U.S. Department of Energy) and NOIRLab, the U.S. National Science Foundation’s center for ground-based optical astronomy. It operates in collaboration with a broad network of international partners — including Israel, which will contribute through its ULTRASAT space telescope project, currently under development at the Weizmann Institute of Science and scheduled for launch in about two years. Like the Rubin telescope, ULTRASAT will feature a wide field of view and repeatedly scan the sky — but in ultraviolet rather than visible light, making the two telescopes complementary in many aspects. Under the collaboration agreement, American researchers will gain access to ULTRASAT’s data, while Israeli scientists will be able to use data from the Rubin telescope.
The immense amount of data expected to be produced by the observatory will add to a growing number of major sky-mapping initiatives in recent years, including the Milky Way maps produced by the European Space Agency’s Gaia space telescope, which recently completed its mission, and another sky survey by NOIRLab. Also joining this expanding list of sky surveys is LAST, an array of telescopes developed by the Weizmann Institute of Science, which recently began operating in southern Israel. Although LAST covers smaller areas of the sky than the Vera Rubin Telescope, it revisits each section multiple times per night to track rapidly changing phenomena — generating even more data than the new Rubin telescope is expected to produce. Each project has its own strengths and scientific goals, but together — and thanks to advances in computing and big data technologies now transforming astronomy — we are now collecting an unprecedented wealth of information about our universe.
The Rubin Telescope also supports an educational program that gives students and teachers access to its data and images for learning and research. “The Vera Rubin Telescope is an investment in our future,” said Michael Kratsios, then-Director of the White House Office of Science and Technology Policy. “It will lay down a cornerstone of knowledge today on which our children will proudly build tomorrow.”
The College of Agriculture, Biotechnology & Natural Resources mourns the passing of David A. Schooley, Ph.D., a distinguished professor emeritus of biochemistry, a renowned insect endocrinologist, and a beloved educator and mentor. He joined the University in 1988 and served with distinction until 2013, leaving a legacy of scientific innovation and student-focused education.
David earned his doctorate in organic chemistry from Stanford University in 1968 under famed chemist Carl Djerassi, whose research, along with that of other scientists, helped pave the way for the development of the birth control pill. David later held leadership roles at Zoecon Corporation, where he helped develop methoprene, a synthetic, environmentally safe insect hormone analog now used worldwide to combat mosquito-borne diseases. His early identification of the first four juvenile hormone molecules left a lasting mark in the field of insect physiology and public health.
David continued his prolific research career after joining the University of Nevada, Reno, publishing nearly 200 articles in leading journals. His work has been cited more than 11,000 times by researchers around the world. Much of his research focused on insect diuretic hormones and helped reshape how scientists understand hormone function, evolution and potential biomedical parallels.
During his tenure, David played a key role in establishing the Nevada Proteomics Center, now known as the Mick Hitchcock, Ph.D. Proteomics Center, securing funding to bring state-of-the-art mass spectrometry capabilities to the University. His efforts helped launch a wave of interdisciplinary research across departments.
A passionate educator, David mentored dozens of students in biochemistry, and launched many of them into successful scientific careers. He received the University’s Teacher of the Year and Outstanding Researcher Awards, as well as the Nevada Regents’ Researcher Award.
“David was one of the most decent people I have ever known and is largely responsible for me becoming the scientist I am today,” said Vincent Lombardi, David’s former doctoral student and now an associate professor in the Department of Microbiology and Immunology. “He was an amazing scientist and an exceptional mentor.”
David’s contributions earned national and international recognition, including the Kenneth A. Spencer Award from the American Chemical Society, the Ted Hopkins Insect Physiologist Award from Kansas State University and the Invertebrate Neuropeptide Award from the International Peptide Society. He also served on many editorial boards and was active in several scientific societies.
Colleagues remember him as a brilliant scientist and generous mentor.
“Dave Schooley was a world leader in insect peptide hormones and juvenile hormone,” said Bob Ryan, a former colleague and professor of biochemistry. “His meticulous, impactful research played a key role in building what is now a thriving arthropod research group in the Department of Biochemistry & Molecular Biology. Recruiting him was a major achievement for the department at the time.”
Those who had the privilege to work with and get to know David over his tenure at the University will certainly miss him as a dear, witty and humorous colleague.
The College joins the scientific community and the family of David in mourning his loss. We extend our heartfelt condolences to his wife, Eleanor, and their children and grandchildren.
Scientists have uncovered a genetic variant, inherited from Neanderthals, that may limit athletic performance.
The mutation is thought to affect roughly 8% of modern-day Europeans and influences the activity of a key enzyme in the production of energy in skeletal muscle.
In a study published July 10 in the journal Nature Communications, researchers analyzed more than 2,700 individuals, which revealed that those who carried the Neanderthal gene variant were half as likely to become top athletes as those without the variant.
The variant was found in up to 8% of present-day Europeans, 3% of Native Americans and 2% of South Asians, while it was absent in Africans, East Asians and African-Americans. “Since modern humans mixed with Neanderthals around 50,000 years ago, particularly in Europe and Western Asia, non-African populations today carry about 1–2% Neanderthal DNA,” Dominik Macak, the study’s first author and Doctoral Student at Max-Planck-Institute for Evolutionary Anthropology, told Live Science in an email.
While the Neanderthal variant is not linked with any major health issues, its impact on the body’s ability to produce energy during intense exercise could lead to reduced athletic performance in endurance and power sports, the researchers say.
During exercise, cells gain energy by breaking down a molecule called adenosine triphosphate (ATP), often described as our body’s “batteries”. One way that our body creates ATP, particularly during intense exercise, is by turning two molecules of adenosine diphosphate (ADP) into one molecule of ATP and one of adenosine monophosphate (AMP).
The ATP produced by this reaction is used to power energetic processes in our cells, while the AMP byproduct is removed by an enzyme called AMPD1. It’s this enzyme that is impaired in those with the Neanderthal gene variant, the researchers found.
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To test the impacts of this gene variant, scientists recreated the Neanderthal version of the AMPD1 enzyme in the lab. They found that it was 25% less active than the enzyme produced in humans with other variants of the gene. Next, they genetically engineered mice to express the altered AMPD1 and found that the enzyme was up to 80% less active than the non-Neanderthal variant.
The researchers then analyzed the prevalence of the gene among elite athletes and non-athletes. They found that 4% to 14% of athletes carried this genetic variant, while 9% to 19% of non-athletes had the variant. Carrying just one copy of the Neanderthal gene (out of the two copies inherited from parents) led to a 50% lower probability of achieving elite athletic status, the data suggested.
Those that carry the Neanderthal gene may struggle with more extreme exercise because the impaired enzyme will allow AMP to build up in their muscles, making it harder for them to produce ATP as fast as their cells need. However, having the Neanderthal gene variant is unlikely to affect most people’s daily activities, where energy is obtained by other means. It is only during endurance sports or in exercises that demand muscular power that carriers might be at a slight disadvantage, the researchers said.
But how might this variant have impacted the Neanderthals themselves? “It’s very unlikely that this single genetic variant played a role in the extinction of the Neanderthals,” Macak said. “We find it in both early and later Neanderthal individuals, suggesting it was stably present over thousands of years. Additionally, some modern humans today carry mutations that disrupt the AMPD1 protein entirely, often without any major health issues. So, while the gene affects muscle metabolism, it likely wasn’t a decisive factor in their ability to survive.”
Researchers from the University of Tokyo in collaboration with Aisin Corporation have demonstrated that universal scaling laws, which describe how the properties of a system change with size and scale, apply to deep neural networks that exhibit absorbing phase transition behavior, a phenomenon typically observed in physical systems. The discovery not only provides a framework describing deep neural networks but also helps predict their trainability or generalizability. The findings were published in the journal Physical Review Research.
In recent years, it seems no matter where we look, we come across artificial intelligence in one form or another. The current version of the technology is powered by deep neural networks: numerous layers of digital “neurons” with weighted connections between them. The network learns by modifying the weights between the “neurons” until it produces the correct output. However, a unified theory describing how the signal propagates between the layers of neurons in the system has eluded scientists so far.
“Our research was motivated by two drivers,” says Keiichi Tamai, the first author, “partially by industrial needs as brute-force tuning of these massive models takes a toll on the environment. But there was a second, deeper pursuit: the scientific understanding of the physics of intelligence itself.”
This is where Tamai’s background in statistical physics of phase transitions gave him the first hint. Absorbing phase transitions refer to a sharp shift at a tipping point from an active to an absorbing phase, from which the system cannot escape without outside help. An example of such a physical system would be a fire burning out. Crucially, these systems exhibit universal behaviors near the tipping point and can be described using universal scaling laws if certain properties are preserved. If deep neural networks exhibit absorbing phase transitions, then then universal scaling laws may apply, providing unified framework for describing how they function. Consequently, researchers would be able to predict whether a signal would “burn out” in a certain deep learning set up.
To investigate, the researchers combined theory with simulations. They derived the exponents, which are universal across systems, and scaling factors, which differ across systems, from theory when possible and used simulations to confirm the scaling laws in more complex cases.
“What a coincidence, I thought,” Tamai says, remembering when he first noticed the link between deep neural networks and absorbing phase transitions. “I never imagined I would end up doing research on deep learning, let alone finding an effective use of a concept I worked on as a doctoral student in physics.”
The finding also brings us closer to understanding the physics of intelligence itself, as it reinvigorates the brain criticality hypothesis, which states that some biological networks operate near phase transitions. Tamai is excited about the prospects of this line of research.
“Alan Turing hinted at this connection as early as 1950, but the tools weren’t ready back then. With the rapid accumulation of evidence in neuroscience and the rise of near-human-level AI, I believe we’re at a perfect moment to revisit and deepen our understanding of this fundamental relationship.”
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