Category: 7. Science

  • Mars says hello as NASA’s Europa Clipper warms up radar • The Register

    Mars says hello as NASA’s Europa Clipper warms up radar • The Register

    NASA’s Europa Clipper probe checked out its radar as the spacecraft hurtled past Mars on the way to Jupiter’s moon Europa.

    The Mars flyby in March was primarily to use the planet’s gravitational pull to tweak the Europa Clipper’s trajectory. However, boffins were able to use the proximity of the planet to calibrate the spacecraft’s infrared camera and test its radar ahead of its arrival at Europa in 2030, NASA has confirmed.

    Engineers were unable to test the flight version of the radar instrument on Earth. Engineering models were tested outside the Jet Propulsion Laboratory (JPL) in Southern California, but the flight hardware needed to be kept sterile so could only be tested in a clean room.

    NASA has access to some enormous clean rooms, and the spacecraft was assembled and tested in the giant High Bay 1 clean room at JPL. However, there wasn’t sufficient space to test the fully assembled radar. According to NASA, a chamber about 250 feet (76 meters) long would have been needed to test the “echo” or bounceback of the instrument’s signals.

    The radar, REASON (Radar for Europa Assessment and Sounding: Ocean to Near-surface), employs two pairs of antennas that stick out from the enormous solar arrays of the Europa Clipper. Since scientists have been studying the Martian terrain for decades, and the vehicle would be whizzing past, it seemed a good place to perform a dry run of the instrument and shake out any bugs before the spacecraft arrives at Europa.

    The spacecraft bounced radio waves off Mars as it flew by the planet, starting at 3,100 miles (5,000 kilometers) down to 550 miles (884 kilometers) above the surface. Sixty gigabytes of data were collected, which started downloading to Earth in mid-May.

    When the spacecraft gets to Europa, the instrument will operate as close as 16 miles (25 kilometers) from the moon’s surface.

    According to NASA, the test was a success. JPL’s Trina Ray, Europa Clipper Deputy Science Manager, said: “The engineers were excited that their test worked so perfectly.”

    “The scientists seeing the data for the first time were ecstatic. Now, the science team is getting a head start on learning how to process the data and understand the instrument’s behavior compared to models.

    “They are exercising those muscles just like they will out at Europa.”

    Europa Clipper, the largest spacecraft NASA has ever created for a planetary mission, was launched in October 2024 atop a SpaceX Falcon Heavy rocket. As well as the March flyby of Mars, it will also take a gravity assist from Earth in 2026 before arriving in the Jupiter system in 2030.

    While the radar has been tested, engineers still have a nervous wait to see how the spacecraft’s electronics will react to the harsh radiation environment of Jupiter. There is a possibility that some of the parts might fail, although NASA believes the affected transistors will be able to “support the baseline mission.”

    Once at Europa, the spacecraft’s three main objectives are to determine the thickness of the moon’s icy shell, investigate its composition, and characterize its structure or physical properties. ®

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  • Live Science crossword puzzle #4: The building blocks of DNA — 14 across

    Live Science crossword puzzle #4: The building blocks of DNA — 14 across

    If you enjoyed this, see how quickly you can complete our most recent science crossword puzzle, updated every Monday.

    Note: Our crosswords are currently best experienced on desktop.

    Previous science crosswords

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  • Gigantic, meat-eating dinosaurs didn’t all have strong bites

    Gigantic, meat-eating dinosaurs didn’t all have strong bites

    image: 

    Dinosaur bite illustrations.


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    Credit: Rowe and Rayfield, Current Biology

    A new analysis of the bite strength of 18 species of carnivorous dinosaurs shows that while the Tyrannasaurus rex skull was optimized for quick, strong bites like a crocodile, other giant, predatory dinosaurs that walked on two legs—including spinosaurs and allosaurs—had much weaker bites and instead specialized in slashing and ripping flesh. Reported in the Cell Press journal Current Biology on August 4, these findings demonstrate that meat-eating dinosaurs followed different evolutionary paths in terms of skull design and feeding style despite their similarly gigantic sizes.  

    “Carnivorous dinosaurs took very different paths as they evolved into giants in terms of feeding biomechanics and possible behaviors,” said Andrew Rowe of the University of Bristol, UK. 

    “Tyrannosaurs evolved skulls built for strength and crushing bites, while other lineages had comparatively weaker but more specialized skulls, suggesting a diversity of feeding strategies even at massive sizes. In other words, there wasn’t one ‘best’ skull design for being a predatory giant; several designs functioned perfectly well.” 
     
    Rowe has always been fascinated by big carnivorous dinosaurs, and he considers them interesting subjects for exploring basic questions in organismal biology. In this study, he and co-author Emily Rayfield wanted to know how bipedalism—or walking on two legs—influenced skull biomechanics and feeding techniques. 

    It was previously known that despite reaching similar sizes, predatory dinosaurs evolved in very different parts of the world at different times and had very different skull shapes. For Rowe and Rayfield, those facts raised questions about whether their skulls were functionally similar under the surface or if there were notable differences in their predatory lifestyles. As there are no massive, bipedal carnivores alive today—ever since the end-Cretaceous mass extinction event—the authors note that studying these animals offers intriguing insights into a way of life which has since disappeared.  

    To examine the relationship between body size and skull biomechanics, the authors used 3D technologies including CT scans and surface scans analyze the skull mechanics, quantify the feeding performance, and measure the bite strength across 18 species of therapod, a group of carnivorous dinosaurs ranging from small to giant. While they expected some differences between species, they were surprised when their analyses showed clear biomechanical divergence.  

    “Tyrannosaurids like T. rex had skulls that were optimized for high bite forces at the cost of higher skull stress,” Rowe says. “But in some other giants, like Giganotosaurus, we calculated stress patterns suggesting a relatively lighter bite. It drove home how evolution can produce multiple ‘solutions’ to life as a large, carnivorous biped.” 
     
    Skull stress didn’t show a pattern of increase with size. Some smaller therapods experienced greater stress than some larger species due to increased muscle volume and bite forces. The findings show that being a predatory biped didn’t always equate to being a bone-crushing giant. Unlike T. rex, some dinosaurs, including the spinosaurs and allosaurs, became giants while maintaining weaker bites more suited for slashing at prey and stripping flesh.  

    “I tend to compare Allosaurus to a modern Komodo dragon in terms of feeding style,” Rowe says. “Large tyrannosaur skulls were instead optimized like modern crocodiles with high bite forces that crushed prey. This biomechanical diversity suggests that dinosaur ecosystems supported a wider range of giant carnivore ecologies than we often assume, with less competition and more specialization.” 

    ### 

    This research was supported by funding from the Biotechnology and Biological Sciences Research Council.  

    Current Biology, Rowe & Rayfield, “Carnivorous dinosaur lineages adopt different skull performances at gigantic size” https://www.cell.com/current-biology/fulltext/S0960-9822(25)00811-5

    Current Biology (@CurrentBiology), published by Cell Press, is a bimonthly journal that features papers across all areas of biology. Current Biology strives to foster communication across fields of biology, both by publishing important findings of general interest and through highly accessible front matter for non-specialists. Visit: http://www.cell.com/current-biology. To receive Cell Press media alerts, contact press@cell.com. 


    Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.


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  • SpaceX lifts 28 Starlink satellites in landmark reusable booster mission

    SpaceX lifts 28 Starlink satellites in landmark reusable booster mission

    Aug. 4 (UPI) — SpaceX launched dozens of new Starlink satellites into orbit overnight after initial delays over weather in the company’s 69th liftoff this year.

    The Starlink 10-30 mission saw liftoff at 3:57 a.m. EDT from pad 40 at Cape Canaveral Space Force Station in Florida after its original 2:01 a.m. time slot had to be changed due to persistent storms.

    The Falcon 9 and its joint Falcon Heavy rocket carried 28 Starlink satellites to its growing constellation of Internet-ready satellite devices.

    But it marked a milestones for SpaceX with the 450th launch of its flight-proven booster 1080, which flew for its 21st time.

    Initially there was an 85% chance for favorable weather in the forecast, according to the 45th Weather Squadron.

    But strong thunderstorms via a low-pressure system hung over the region and temporarily delayed the launch as Tropical Storm Dexter gains strength.

    A little over 8 minutes after liftoff the B1080 landed on SpaceX’s drone ship “Just Read the Instructions” in the Atlantic Ocean in the 131st landing on the drone ship vessel.

    So far this year SpaceX has launched over 1,650 Starlink satellites in the Elon Musk-run company’s bid to expand global Internet access.

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  • Researchers Find Culprit Behind Sea Star Disease

    Researchers Find Culprit Behind Sea Star Disease

    The underside of an adult sunflower sea star at UW Friday Harbor Laboratories.Dennis Wise/University of Washington

    Sunflower sea stars are the largest sea stars in the world: They have up to 24 arms and grow to the size of a bicycle tire.

    Starting in 2013, these creatures and other sea star species along the west coast of North America died in epidemic proportions. The stars had harrowing symptoms: Their arms contorted before falling off completely. Over the past decade, sea star wasting disease has killed billions of sea stars in up to 20 species by effectively “melting” their tissues.

    The disease has wiped out more than 90% of the once-common sunflower sea stars, most critically in the continental U.S., landing them on the International Union for Conservation of Nature’s Red List of critically endangered species. The loss of sunflower sea stars, which support kelp forests by feeding on kelp-eating sea urchins, has had widespread and lasting effects on coastal ecosystems.

    Until now, no one knew what caused sea star wasting disease. But on Aug. 4, an international research effort including scientists from the University of Washington has finally revealed the cause: a strain of the bacterium Vibrio pectenicida. Vibrio is a genus of bacteria that has devastated coral and shellfish as well as humans (for example, Vibrio cholerae is the pathogen that causes cholera).

    The researchers published this finding in Nature Ecology & Evolution.

    a person holds a sea star

    Drew Harvell holds a sunflower star at UW Friday Harbor Laboratories.David O Brown/Cornell University

    “This is the discovery of the decade for me,” said co-author Drew Harvell, a UW affiliate professor in the School of Aquatic and Fishery Sciences and Friday Harbor Laboratories. “We have studied both the cause and the impacts of this disease for the entire epidemic. What’s crazy is that the answer was just sitting right there in front of us. This Vibrio is a sneaky critter because it doesn’t show up on histology like other bacteria do.”

    “From initial studies, we thought the culprit was a virus,” Harvell continued. “So it was a surprise to find the pathogen in a more common group of bacteria.”

    The long-awaited result showing V. pectenicida strain FHCF-3 as the causative agent comes after a four-year research process. Scientists explored many possible pathogens, including viruses. At first, the researchers looked in sunflower sea star tissues before they homed in on the high levels of V. pectenicida in sick sea star “blood,” or coelomic fluid.

    “When we looked at the coelomic fluid between exposed and healthy sea stars, there was basically one thing different: Vibrio,” said senior author Alyssa Gehman, a marine disease ecologist at the Hakai Institute and the University of British Columbia. “We all had chills. We thought, ‘That’s it. We have it. That’s what causes wasting.’”

    Harvell attributes the team’s success to:

    • Having the right facilities at the U.S. Geological Service with proper quarantine and high-quality water flow
    • A talented research team that had pathology, virology and bacteriology experience
    • Having access to a source of the right test animals, including sunflower sea stars raised in captivity by co-author Jason Hodin, UW senior research scientist at Friday Harbor Laboratories.
    three sunflower sea stars in a tank. There are mussel shells beneath them.

    Adult sunflower sea stars feeding on mussels at UW Friday Harbor Laboratories. The stars suck out and ingest the soft tissues of mussels, then discard the shells, which collect at the bottom of the tank. The sea star on the bottom, “Charlotte,” is the mother of the lab’s stars grown in captivity.Dennis Wise/University of Washington

    a person in a lab holding a sea star in one hand and a syringe in the other

    Grace Crandall injects a sea star to expose it to wasting disease at the start of a new experiment.Grace Crandall/University of Washington

    “I observed and collected health data on nearly every single sea star twice a day for the majority of experiments for all four summers,” said co-author Grace Crandall, a UW doctoral student in the School of Aquatic and Fishery Sciences. “I have loved sea stars and have been fascinated by diseases since childhood. To get to participate so actively in research that combines both of these interests has been a dream come true. I’m excited about getting to work on a project with such consequential findings for the conservation of these important sea stars: to find both the cause of sea star wasting disease, and to better understand their immune response.”

    To confirm that V. pectenicida was the culprit, co-author Amy M. Chan, a research scientist at UBC, created pure cultures of V. pectenicida from the coelomic fluid of sick sea stars. The team then injected the cultured pathogen into healthy sea stars, which developed symptoms of sea star wasting disease – the final proof.

    “When we lose billions of sea stars, that really shifts the ecological dynamics,” said lead author Melanie Prentice, an evolutionary ecologist at the Hakai Institute and UBC. “In the absence of sunflower stars, sea urchin populations increase, which means the loss of kelp forests, and that has broad implications for all the other marine species and humans that rely on them. So losing a sea star goes far beyond the loss of that single species.”

    four people standing in a lab smiling. There are tanks containing sea stars in front of them.

    The team poses in the lab at the USGS Marrowstone Marine Field Station. From left to right: Alyssa Gehman, Grace Crandall, Melanie Prentice and Drew Harvell.Grace Crandall/University of Washington

    Now that scientists have identified the pathogen behind sea star wasting disease, they can look into the drivers of disease and potential hallmarks of resilience. Researchers are particularly interested in studying the link between sea star wasting disease and rising ocean temperatures. The effects of the disease seem to be stronger in warmer water, and other species of Vibrio are also known to proliferate in warm water, Gehman said.

    Researchers and project partners hope the discovery will help guide management and recovery efforts for sea stars and the ecosystems affected by their decline.

    /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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  • ‘The discovery of the decade’: Researchers have found the culprit behind sea star wasting disease

    ‘The discovery of the decade’: Researchers have found the culprit behind sea star wasting disease

    August 4, 2025

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  • Scientists achieve megabase-scale precision genome editing in eukaryotic cells

    Scientists achieve megabase-scale precision genome editing in eukaryotic cells

    image: 

    Iterative Recombinase Technologies Mediated Precision Chromosome Engineering


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    Credit: IGDB

    A team of Chinese researchers led by Prof. GAO Caixia from the Institute of Genetics and Developmental Biology of the Chinese Academy of Sciences has developed two new genome editing technologies, known collectively as Programmable Chromosome Engineering (PCE) systems.

    The study, published online in Cell on August 4, achieves multiple types of precise DNA manipulations ranging from kilobase to megabase scale in higher organisms, especially plants.

    Extensive research has demonstrated the immense potential of the site-specific recombinase Cre-Lox system for precise chromosomal manipulation. However, its broader application has been hindered by three critical limitations: (1) reversible recombination reactions—stemming from the inherent symmetry of Lox sites—can negate desired edits; (2) the tetrameric nature of Cre recombinase complicates engineering efforts, hindering activity optimization; and (3) residual Lox sites after recombination may compromise editing precision.

    The research team addressed each of these challenges and developed novel methods to advance the state of this technology. First, they built a high-throughput platform for rapid recombination site modification and proposed an asymmetric Lox site design. This led to the development of novel Lox variants that reduce reversible recombination activity by over 10-fold (approaching the background level of negative controls) while retaining high-efficiency forward recombination.

    They then leveraged their recently developed AiCE (AI-informed Constraints for protein Engineering), model—a protein-directed evolution system integrating general inverse folding models with structural and evolutionary constraints—to develop AiCErec, a recombinase engineering method. This approach enabled precise optimization of Cre’s multimerization interface, yielding an engineered variant with a recombination efficiency 3.5 times that of wild-type Cre.

    Lastly, they designed and refined a scarless editing strategy for recombinases. By harnessing the high editing efficiency of prime editors, they developed Re-pegRNA, a method that uses specifically designed pegRNAs to perform re-prime editing on residual Lox sites, precisely replacing them with the original genomic sequence, thereby ensuring seamless genome modifications.

    The integration of these three innovations led to the creation of two programmable platforms, PCE and RePCE. These platforms allow flexible programming of insertion positions and orientations for different Lox sites, enabling precise, scarless manipulation of DNA fragments ranging from kilobase to megabase scale in both plant and animal cells. Key achievements include: targeted integration of large DNA fragments up to 18.8 kb, complete replacement of 5-kb DNA sequences, chromosomal inversions spanning 12 Mb, chromosomal deletions of 4 Mb, and whole-chromosome translocations.

    As a proof of concept, the researchers used this technology to create herbicide-resistant rice germplasm with a 315-kb precise inversion, showcasing its transformative potential for genetic engineering and crop improvement.

    This pioneering work not only overcomes the historical limitations of the Cre-Lox system but also opens new avenues for precise genome engineering in a variety of organisms.


    Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.

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  • Not All Giant Carnivorous Dinosaurs Had Strong Bites

    Not All Giant Carnivorous Dinosaurs Had Strong Bites

    A new analysis of the bite strength of 18 species of carnivorous dinosaurs shows that while the Tyrannasaurus rex skull was optimized for quick, strong bites like a crocodile, other giant, predatory dinosaurs that walked on two legs—including spinosaurs and allosaurs—had much weaker bites and instead specialized in slashing and ripping flesh. Reported in the Cell Press journal Current Biology on August 4, these findings demonstrate that meat-eating dinosaurs followed different evolutionary paths in terms of skull design and feeding style despite their similarly gigantic sizes.

    “Carnivorous dinosaurs took very different paths as they evolved into giants in terms of feeding biomechanics and possible behaviors,” said Andrew Rowe of the University of Bristol, UK.

    “Tyrannosaurs evolved skulls built for strength and crushing bites, while other lineages had comparatively weaker but more specialized skulls, suggesting a diversity of feeding strategies even at massive sizes. In other words, there wasn’t one ‘best’ skull design for being a predatory giant; several designs functioned perfectly well.”

    Rowe has always been fascinated by big carnivorous dinosaurs, and he considers them interesting subjects for exploring basic questions in organismal biology. In this study, he and co-author Emily Rayfield wanted to know how bipedalism—or walking on two legs—influenced skull biomechanics and feeding techniques.

    It was previously known that despite reaching similar sizes, predatory dinosaurs evolved in very different parts of the world at different times and had very different skull shapes. For Rowe and Rayfield, those facts raised questions about whether their skulls were functionally similar under the surface or if there were notable differences in their predatory lifestyles. As there are no massive, bipedal carnivores alive today—ever since the end-Cretaceous mass extinction event—the authors note that studying these animals offers intriguing insights into a way of life which has since disappeared. 

    To examine the relationship between body size and skull biomechanics, the authors used 3D technologies including CT scans and surface scans analyze the skull mechanics, quantify the feeding performance, and measure the bite strength across 18 species of therapod, a group of carnivorous dinosaurs ranging from small to giant. While they expected some differences between species, they were surprised when their analyses showed clear biomechanical divergence.

    “Tyrannosaurids like T. rex had skulls that were optimized for high bite forces at the cost of higher skull stress,” Rowe says. “But in some other giants, like Giganotosaurus, we calculated stress patterns suggesting a relatively lighter bite. It drove home how evolution can produce multiple ‘solutions’ to life as a large, carnivorous biped.”

    Skull stress didn’t show a pattern of increase with size. Some smaller therapods experienced greater stress than some larger species due to increased muscle volume and bite forces. The findings show that being a predatory biped didn’t always equate to being a bone-crushing giant. Unlike T. rex, some dinosaurs, including the spinosaurs and allosaurs, became giants while maintaining weaker bites more suited for slashing at prey and stripping flesh.

    “I tend to compare Allosaurus to a modern Komodo dragon in terms of feeding style,” Rowe says. “Large tyrannosaur skulls were instead optimized like modern crocodiles with high bite forces that crushed prey. This biomechanical diversity suggests that dinosaur ecosystems supported a wider range of giant carnivore ecologies than we often assume, with less competition and more specialization.”

    /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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  • New Technique Reveals Chemistry of Periodic Table’s Base

    New Technique Reveals Chemistry of Periodic Table’s Base

    Key Takeaways

    • Scientists at Berkeley Lab’s 88-Inch Cyclotron developed a new technique for atom-at-a-time chemistry that opens up the next generation of heavy- and superheavy-element studies.
    • This is the first time researchers have made a direct measurement of a molecule containing an element with more than 99 protons (nobelium, element 102).
    • It’s also the first direct comparison of chemistry between molecules made with extremes of the actinide elements (actinium and nobelium).
    • Understanding elements’ chemistries helps researchers better predict their behavior and design ways to produce or use specific molecules. That knowledge could improve the radioisotopes used in medicine.

    The periodic table is one of the triumphs of science. Even before certain elements had been discovered, this chart could successfully predict their masses, densities, how they would link up with other elements, and a host of other properties.

    But at the bottom of the periodic table, where massive atoms are practically bursting at the seams with protons, its predictive power might start to break down. Experiments to study the chemistry of the heaviest elements – especially the superheavy elements, which have more than 103 protons – have long been a challenge. Despite using specialized facilities, researchers have been unable to definitively identify the molecular species they produce in experiments. This uncertainty has hindered progress in the field, since scientists have had to rely on educated guesses rather than precise knowledge of the chemistry being observed.

    Now, researchers have used the 88-Inch Cyclotron at the Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab) to develop a new technique to make and directly detect molecules containing heavy and superheavy elements. In a study published today in the journal Nature, a team of researchers from Berkeley Lab, UC Berkeley, and The University of Alabama used the method to create molecules containing nobelium, element 102. It is the first time scientists have directly measured a molecule containing an element greater than 99.

    “What is really exciting is that this opens the door to the next generation of atom-at-a-time chemistry studies – so looking at the chemistry of superheavy elements and asking whether or not they are in the correct positions on the periodic table,” said Jennifer Pore, scientist at Berkeley Lab and lead author of the paper. “I think we’re going to completely change how superheavy-element chemistry is done.”

    The team’s setup also produced molecules containing actinium, element 89. This let them simultaneously study the extremes of the actinide series, the group on the periodic table that spans elements 89 to 103. Researchers recorded how frequently actinium and nobelium bonded with one or more water or nitrogen molecules, providing new information about how the actinides interact within the same experiment.

    “This was the first time anyone’s ever done a direct comparison of an early actinide to a late actinide element,” Pore said. “We weren’t surprised by any of the chemistry results – they fit with what makes sense for the trend. But the fact that we could see the chemistry of these things we’re producing one atom at a time, and directly observe the molecular species, was really exciting.”

    What was a surprise to the researchers was how effortlessly they made the nobelium molecules in the first place.

    Unexpected molecules

    The original plan for the experiment went like this: The 88-Inch Cyclotron would accelerate a beam of calcium isotopes into a target of thulium and lead, producing a spray of particles that included the actinides of interest. The Berkeley Gas Separator would clear out the extra particles, sending only the actinium and nobelium to a cone-shaped gas catcher. Exiting that funnel at supersonic speeds, the gas would expand, interacting with another jet of reactive gas to create molecules. Electrodes would then speed those molecules into FIONA, a state-of-the-art spectrometer that could measure their masses and determine exactly what molecules had formed.

    But before the researchers had a chance to inject their reactive gas, they noticed something unexpected: They were already recording molecules containing nobelium in their detector. Stray nitrogen and water, present in only minuscule amounts within FIONA, had combined with the nobelium atoms.

    “We assumed that we would not be making molecules in the experiment before we wanted to,” said Jacklyn Gates, a nuclear scientist at Berkeley Lab and co-author of the paper. “The fact that we do is an important point, because no other atom-at-a-time chemistry setups have molecule identification availability, and they have always assumed that they don’t make molecules.”

    A series of metal boxes and pipes sit on a purple base. Two people work on different components, one adjusting wires attached to a box, the other moving cables in an overhead rack.

    Researchers previously thought that the stringent processes to clean the gas in their systems would leave an insignificant amount of water and nitrogen molecules behind, and that there wouldn’t be enough energy in their reactions to break those bonds and reform molecules unintentionally. But that wasn’t the case.

    “For the types of molecules we’re making here, you don’t have to break bonds. The metal ions find the water and they stick together to form these molecular species,” Pore said. “There are potential implications for superheavy-element studies, because we made a lot of molecules even with our clean setup. With this result, researchers will have to think more carefully about what they’re actually making in their systems.”

    Unexpected molecule formation could help explain previous conflicting experiments that studied whether flerovium, element 114, behaves like a noble gas (elements that tend not to interact with other materials because of the way their electrons are arranged). This discovery may also shed new light on the interpretation of recent studies on element 113 and 115, and inform all future gas-phase studies of superheavy elements.

    Three rows of ball-and-stick models show different bonding arrangements of nobelium.

    Fabulous FIONA

    After the unexpected discovery of nobelium molecules, the research team temporarily diverted from their original experiment. They ran their setup non-stop for 10 days, collecting nearly 2,000 molecules made of actinium or nobelium. That’s a large amount by heavy element chemistry standards, but still an incredibly small number. For comparison, a drop of water contains more than a sextillion (that’s 1 followed by 21 zeros) molecules.

    “This is very different than the traditional chemistry most people think of, where you have beakers with lots and lots of liquid,” Pore said. “We’re working with extremely small amounts of material, far beyond what the human eye can detect. The ability to extract meaningful information from these tiny samples is a big deal. FIONA is much faster than anything that’s ever been done before, and more sensitive. This is important because everything we study is radioactive and only exists for a few seconds or less before it disappears.”

    Sensitivity and speed are essential as researchers move to study the chemistry of heavier and heavier elements, which grow increasingly difficult to make and quicker to decay as they become more massive. While previous techniques were limited to molecules that lived for about 1 second, the team’s experimental setup can study ones that only survive for 0.1 seconds, and the experimenters have control of how long the particles are trapped at every stage of the process.

    Two people work on FIONA. Cables wrapped in foil connect to the instruments and a panel of electronics.Red, blue, and white ball-and-stick models of molecules are projected onto two people in a hallway.

    Previous experiments measured the secondary particles made when a molecule with a superheavy element decayed – but they couldn’t identify the exact original chemical species. Most measurements reported a range of possible molecules and were based on assumptions from better-known elements. The new approach is the first to directly identify the molecules by measuring their masses, removing the need for such assumptions.

    “FIONA is really the secret sauce for the chemistry, and FIONA wasn’t even designed to do chemistry,” Gates said. “It was designed just to do mass measurements, so this is like a fun side hustle. We can do these chemistry studies with very little modification to the system, and we have this unique capability of identifying molecular species. There’s going to be a lot of new, exciting results coming out using this technique.”

    Researchers plan to use their approach with several early superheavy elements, pairing the atoms with fluorine-containing gases and short-chain hydrocarbons to reveal fundamental chemistry at the bottom of the periodic table.

    Better models, better medicine

    A better understanding of heavy and superheavy elements has several benefits. Experiments can check the chemistries of the elements, making sure they are grouped correctly on the periodic table and improving its predictive power. At the same time, researchers are also assessing models of the atom and the fundamental forces at play.

    Odd chemical behavior in the heavier elements arises in part from “relativistic effects.” The large number of protons in the nucleus creates an intense charge that pulls on the inner electrons, speeding them up. As some of the electrons are sucked towards the center of the atom, they shield some of the outer electrons from the pull. These effects can cause an element’s chemistry to behave in unexpected ways. (The color of gold, different from the gray of so many other metals, is one such example.)

    Jennifer Pore stands holding a piece of equipment and is talking to Jacklyn Gates, seated at a computer. The lab equipment of the FIONA detector setup is prominent.

    “The electrons behave very differently in elements where you have these large relativistic effects, and the effect is expected to be even stronger in the superheavy elements,” Pore said. “This is why they might potentially not be in the right place on the periodic table.”

    There are also practical applications, particularly in improving radioactive isotopes used in medical treatment. One of great interest is an isotope of actinium (actinium-225), which has shown promising results in treating certain metastatic cancers. However, the isotope is difficult to make and only available in small quantities every year, limiting access for clinical trials and treatment. Scientists are just beginning to understand its chemistry.

    “People have been forced to skip the fundamental chemistry step to figure out how to get it into patients,” said Pore. “But if we could understand the chemistry of these radioactive elements better, we might have an easier time producing the specific molecules needed for cancer treatment.”

    This work included collaboration between Berkeley Lab’s Nuclear Science Division and Chemical Sciences Division, and was funded in part by DOE’s Nuclear Physics, Basic Energy Sciences, and Laboratory Directed Research and Development (LDRD) programs.

    /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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  • New Technique Sheds Light on Chemistry at the Bottom of the Periodic Table

    New Technique Sheds Light on Chemistry at the Bottom of the Periodic Table

    “The electrons behave very differently in elements where you have these large relativistic effects, and the effect is expected to be even stronger in the superheavy elements,” Pore said. “This is why they might potentially not be in the right place on the periodic table.”

    There are also practical applications, particularly in improving radioactive isotopes used in medical treatment. One of great interest is an isotope of actinium (actinium-225), which has shown promising results in treating certain metastatic cancers. However, the isotope is difficult to make and only available in small quantities every year, limiting access for clinical trials and treatment. Scientists are just beginning to understand its chemistry.

    “People have been forced to skip the fundamental chemistry step to figure out how to get it into patients,” said Pore. “But if we could understand the chemistry of these radioactive elements better, we might have an easier time producing the specific molecules needed for cancer treatment.”

    This work included collaboration between Berkeley Lab’s Nuclear Science Division and Chemical Sciences Division, and was funded in part by DOE’s Nuclear Physics, Basic Energy Sciences, and Laboratory Directed Research and Development (LDRD) programs.

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