Category: 7. Science

  • The Colorful Bioengineered Succulents That Actually Glow In The Dark

    The Colorful Bioengineered Succulents That Actually Glow In The Dark





    You’ve spent a ton of time in the garden this season, perfecting everything your eyes can see and your hands can touch. By daylight, your sprawling outdoor paradise is a gorgeous sight to behold, but come nightfall, all your hard work literally fades to black. So, what does one do with this night-clad, soil-and-roots situation, save for a few solar lights here or there? After all, it’s not like plants can just glow in the dark — or can they?

    Horticultural science is a wonderful thing, especially when talented minds come up with a way to make plants gleam majestically in the midnight hour. In a recent study, a research team led by Shuting Liu — a bioengineer at South China Agricultural University — dove into the nitty-gritty of turning common succulents into illumination-enhanced garden fixtures, and we’re champing at the bit to land this flora in our own botanical bastions. Let’s unpack this rather enchanting discovery.

    Phosphors have arrived to give bioluminescence a break

    Up to this point, whenever plants glowed, it was thanks to bioluminescence, a naturally occurring process where chemicals like luciferin, luciferase, and oxygen run the show. Stir this molecular melting pot enough, and you get bioluminescent lighting. Organisms like foxfire fungi and Jack-o-Lantern mushrooms are renowned for their luminescent abilities, as are some species of jellyfish, squid, and fireflies. Scientists have even found three types of glow-in-the dark sharks! 

    Contextually, genetic modification can be a hot-button topic, even as it relates to plant life. Over the years, scientists have harvested bioluminescent materials from various fungi, injecting these chemicals into non-glowing plants, and the results are pretty astonishing. But after a successful batch of succulent experiments — in which phosphors were used to make plants glow, instead of bioluminescent elements — Liu and her team achieved a breakthrough.

    Injecting plant leaves with microscopic afterglow particles has proved to be cheaper than genetic modification and less risky for overall plant health. Liu and her crew hypothesized that the phosphors would allow the succulents to deliver a powerful glow experience (sans photosynthesis), and they were right.

    It took a minute to find the right balance between variables, including soil porosity, injection volume and pressure, and phosphor size, but once Liu’s team settled on the mesophyll cell wall of the succulent’s plant leaves, they struck gold (semi-literally). This is a part of the plant involved in photosynthesis, making it a natural choice for hanging onto Liu’s phosphors. Charge the plants with all-day sunlight or LED bulbs, and you’ve got yourself an armada of glowing succulents.

    What does this mean for our gardens and greenhouses?

    While Liu still plans to conduct long-form testing to ensure the phosphors are not negatively impacting the succulent leaves, the future of bioengineering looks very bright (we couldn’t wait to write that line).

    Not too long from now, we could be walking around in full bioengineered gardens, with several plant types hosting the phosphors that reacted so well to succulent leaves. For now, the plants only hold their glow for about two hours after being exposed to LED light or sunshine, and experimentation is still underway, but depending on how bright and colorful these hypothetical gardens could be, we may not need to worry about wiring up a greenhouse with expensive lighting fixtures. The same goes for on-property walking paths usually lit by light posts staked into the ground.

    Who knew that phosphor-packed plants might one day be responsible for cutting down on our utility bills? Liu’s study is very much still in its infancy, but we’re eager to see how this exciting biotechnology improves and evolves through the coming years. Should the long-term effects prove inconsequential, we could be looking at entire city blocks lit by plant light.



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  • Archaeologists Find Traces of Indigo Dye on 34,000-Year-Old Grinding Tools from Georgia

    Archaeologists Find Traces of Indigo Dye on 34,000-Year-Old Grinding Tools from Georgia

    Archaeologists from the Ca’ Foscari University of Venice and elsewhere have found traces of indigotin — a blue secondary compound, also known as indigo — on unknapped ground stone tools recovered from Dzudzuana Cave, located in the foothills of the Caucasus in Georgia. Indigotin forms through a reaction between atmospheric oxygen and the natural glycoside precursors in the leaves of Isatis tinctoria. This proves that the plant, despite not being edible, was intentionally processed as early as 34,000 years ago.

    Five pebbles from Dzudzuana Cave, Georgia. Image credit: Longo et al., doi: 10.1371/journal.pone.0321262.

    Modern humans first appear in the archaeological record around 300,000 years ago, in Africa.

    Most of the evidence for their cognitive and technological abilities is based on recovered assemblages of chipped stone artifacts and animal bones since these endure far longer in the archaeological record than plants.

    Accordingly, the Paleolithic narrative centers primarily on animal hunting and stone tool manufacture.

    Perishable materials, the so-called ‘missing majority,’ notably plants for which there is growing evidence for their use as food, string and cordage, weaving and medicine, are largely missing, creating a partial narrative.

    There is therefore, a need to identify and demonstrate the use of plants and the roles they played in a wide range of activities, many of which may still be unknown.

    “Rather than viewing plants solely as food resources, as is often the case, we highlight their role in complex operations, likely involving the transformation of perishable materials for use in different phases of daily life among Homo sapiens 34,000 years ago,” said Dr. Laura Longo, an archaeologist at the Ca’ Foscari University of Venice.

    “While research continues to improve the identification of elusive plant-derived residues, typically absent from conventional studies, our multi-analytical approach opens new perspectives on the technological and cultural sophistication of Upper Paleolithic populations, who skilfully exploited the inexhaustible resource of plants, fully aware of the power of plants.”

    In their study, the researchers examined 34,000-year-old stone tools recovered from Dzudzuana Cave in Georgia.

    They found traces of mechanical processing of soft and moist materials, compatible with plant materials such as leaves.

    Using various microscopy techniques (optical and confocal), they unexpectedly revealed blue residues — sometimes fibrous — alongside starch grains.

    These residues were mainly concentrated in the areas of the tools showing visible wear.

    To determine the nature of the blue-colored residues, the scientists employed advanced microspectroscopic techniques, notably Raman and FTIR spectroscopy.

    These analyses confirmed the presence of the indigotin chromophore in several samples.

    “Once the molecule responsible for the blue colour was identified, a new challenge emerged: how and why did these residues become associated with the working surfaces of the tools?” the authors said.

    They then investigated the porosity of the stones — a key factor in their ability to trap and preserve biogenic residues.

    Both microscopic fragments of the archaeological tools and larger samples from experimental replicas were analyzed using micro-CT tomography.

    The analysis confirmed the presence of pores with volumes suitable for retaining micrometric remains.

    As a result, the team designed a series of replicative experiments.

    First, raw lithic materials similar to those used by the prehistoric inhabitants of Dzudzuana were sourced.

    Pebbles were collected by Nino Jakeli from the Nikrisi River, which runs just below the cave.

    Controlled experiments followed, mechanically processing various plants, including those used for fiber production (e.g. bast fibers) and those potentially capable of generating indigotin.

    “We used a stringent approach to contamination control and biomolecular analysis to provide evidence for a new perspective on human behavior, and the applied technical and ecological knowledge that is likely to have prevailed in the Upper Paleolithic,” the reserchers said.

    “Whether this plant was used as a colourant, as medicine, or indeed for both remains unknown, but offers a new perspective on the fascinating possibilities of non-edible plant use.”

    The findings were published online in the journal PLoS ONE.

    _____

    L. Longo et al. 2025. Direct evidence for processing Isatis tinctoria L., a non-nutritional plant, 32-34,000 years ago. PLoS One 20 (5): e0321262; doi: 10.1371/journal.pone.0321262

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  • Antarctic algae that once cooled Earth are now disappearing

    Antarctic algae that once cooled Earth are now disappearing

    For something you can’t see with the naked eye, algae sure know how to shake things up. Around 14,000 years ago, microscopic Antarctic algae helped slow down global warming by pulling huge amounts of carbon dioxide out of the atmosphere.

    Scientists just figured out how they did it – and why the same process that once helped cool the planet could play a critical role in shaping the future of our climate.

    Antarctic Algae changed the climate


    Back then, Earth was gradually warming after the last ice age. However, something unusual occurred in the Southern Hemisphere: the warming paused.

    This period, referred to as the Antarctic Cold Reversal, was a time when sea ice expanded quickly in winter and melted quickly in spring. That spring melt converted the Southern Ocean into a super buffet for a particular type of algae, Phaeocystis.

    These tiny ocean plants went wild. They multiplied, and in doing so, they pulled vast quantities of carbon dioxide – one of the primary drivers of global warming – out of the atmosphere and stored it away in the sea.

    Here’s the twist: until now, we had no idea Phaeocystis even played a role. Scientists couldn’t find any trace of them in the usual fossil records.

    Now, thanks to a new method that recovers ancient DNA from the ocean floor, researchers from the Alfred Wegener Institute in Germany have filled in this crucial missing piece of the climate puzzle.

    Unlocking Antarctica’s hidden record

    The team studied a sediment core taken from nearly 2,000 feet deep in the Bransfield Strait, just off the Antarctic Peninsula. Layer by layer, this core preserves snapshots of ocean history going back 14,000 years.

    By analyzing the ancient DNA trapped in that sediment, the scientists found genetic fingerprints of Phaeocystis during the cold reversal period. No one had ever identified these algae in the past using standard geochemical methods.

    “Our study shows that these algal blooms contributed to a significant reduction in global atmospheric CO2 levels during a climatically important transition phase characterized by high sea ice extent,” said Josefine Friederike Weiß from the Alfred Wegener Institute, lead author of the study.

    They also measured something else: a high ratio of barium to iron in the sediment. That ratio is tied to how much organic material – like dead algae – sinks to the seafloor. In this case, the data pointed to intense algal growth during times of heavy spring melt.

    “The further the sea ice expands in winter, the larger the area in spring where nutrient-rich meltwater enters the surface sea – and therefore the zone where Phaeocystis algae find ideal growth conditions. As a result, greater sea ice extent leads directly to a larger region with high algal productivity.”

    Why today’s melting ice is a warning

    The same Phaeocystis algae that once helped cool the world are now struggling to survive. With Antarctic sea ice declining at a record rate, the conditions that previously drove these algae blooms are vanishing.

    That’s not just bad news for the algae. These blooms power entire food webs. They feed tiny animals, which feed fish, which in turn feed everything from squid to seals. If Phaeocystis disappears, the whole system could unravel.

    Even worse, these algae are really good at one specific job: getting carbon to sink deep into the ocean. Losing them could mean more carbon sticks around in the atmosphere, heating the planet faster.

    And there’s another concern. Phaeocystis releases a gas called dimethyl sulfide (DMS), which helps form clouds. More clouds mean more sunlight bounces back into space. Fewer algae mean fewer clouds. That’s one more way climate change could end up feeding on itself.

    Antarctic algae holds future lessons

    The study shows why scientists must look beyond conventional methods. By combining geological tools with DNA analysis, researchers are creating a more accurate picture of how the ocean shapes our climate – and how it might respond in the future.

    The research also highlights a larger trend in climate science. For years, scientists focused mainly on ice cores and chemical markers.

    Now, by analyzing the genetic material of ancient microbes, we can see what species were doing during pivotal climate events – and what those behaviors could mean for us today.

    This is important because forecasting future climate change isn’t only about tracking temperature or carbon levels. It’s about understanding the living systems that help regulate them – such as the algae and the seas they inhabit.

    The full study was published in the journal Nature Geoscience.

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  • Fairy circles may point to clean energy natural hydrogen reserves

    Fairy circles may point to clean energy natural hydrogen reserves

    The race to replace fossil fuels has inspired researchers to explore many unconventional potential sources. Among these, natural hydrogen, which is found deep underground, is gaining attention.

    It is seen as a possible building block for a cleaner energy future. Yet, it remains difficult to predict where this hidden hydrogen lies.


    A recent study from the University of Vienna suggests that mysterious features on Earth’s surface, called fairy circles, could reveal the presence of these underground reserves.

    The round patches, where vegetation is damaged or absent, may point the way to a sustainable energy source.

    What are fairy circles?

    Across many parts of the world, unusual circular patterns appear on the landscape, drawing attention from scientists and local communities alike.

    These formations, known as fairy circles, can be found in regions as distant and varied as Russia, Namibia, Brazil, and Australia.

    They often stand out sharply from the surrounding environment due to the presence of vast rings or depressions with sparse or no vegetation.

    Despite their size – sometimes hundreds of meters across – the depressions themselves are relatively shallow, sinking only a few meters into the ground.

    For decades, these circles remained a geological and ecological mystery. Researchers speculated about many possible explanations, ranging from termite activity to natural gas seepage.

    Questions still remain

    However, no single theory could fully account for their global presence. It wasn’t until roughly ten years ago that a significant breakthrough emerged.

    Scientists discovered that these fairy circles were not just barren patches of land but active sites where natural hydrogen escapes from reservoirs deep underground.

    This finding revealed a surprising connection to one of the cleanest potential energy sources known.

    Still, even with this discovery, questions persisted.

    The mechanisms that shaped these depressions, and the reasons their size might vary depending on the depth and pressure of hydrogen, remained largely unknown. This left both geologists and the energy sector eager for clearer answers.

    Linking hydrogen and fairy circles

    This information is critical for the energy industry. Natural hydrogen carries a negligible carbon footprint, making it an attractive sustainable option.

    “But before expensive drilling can be carried out, we need to understand how fairy circles form, how large the deposits might be and how deep we need to drill,” explained Martin Schöpfer from the University of Vienna and NiMBUC Geoscience.

    A study supported by OMV and led by Schöpfer used geomechanical computer simulations to show why hydrogen-emitting fairy circles sink.

    The simulations revealed that interactions between gas, water flow, and soil create a two-step process that leads to surface collapse.

    Soufflé effect explained

    The team compared the phenomenon to a soufflé. Loose sediments, like sand or clay, sit above solid rock.

    When hydrogen enters the sediment, it pushes water upward, uplifting the surface. Plants suffer from the altered gas mixture and die, leaving bare patches.

    “You could say that the sediment rises like a soufflé, but here geomechanical processes are at work, whereas with a soufflé it is chemical processes,” explained Schöpfer. When the hydrogen flow stops, pressure drops and the sediment compacts.

    “The soil compresses and subsides, similar to a collapsing soufflé,” he added.

    Matching nature and models

    Simulations aligned closely with real fairy circles found in Russia, Brazil, and Australia. The research showed a clear pattern: larger circles indicate deeper and higher-pressure hydrogen sources underground.

    “These findings are a real breakthrough,” emphasizes Bernhard Grasemann, deputy head of the Department of Geology.

    “Fairy circles could thus serve as natural signposts in the future for finding underground hydrogen sources – a potentially inexhaustible and environmentally friendly energy source.”

    Hydrogen from fairy circles matters

    The energy sector is closely watching these developments.

    “The energy sector’s interest in natural hydrogen as a potential new energy source with a negligible carbon footprint is growing, especially in comparison to all other types of artificially produced hydrogen,” noted Gabor Tari, chief geologist at OMV.

    He pointed out that natural, or white and golden hydrogen, along with orange hydrogen, may become cheaper and more profitable than traditional forms, such as black, gray, blue, pink, or green hydrogen.

    This is why OMV supports basic research that explores hydrogen’s future role in energy transitions.

    Next steps in research

    Although promising, many questions remain. Schöpfer stresses the need for additional studies.

    These may include testing different soil types, simulating pulsing gas emissions, and conducting field research to examine chemical reactions that could further influence subsidence.

    If fairy circles do serve as natural guides to underground hydrogen, they could reshape global energy strategies. Unlocking this hidden source may bring the world one step closer to a truly sustainable energy system.

    This could drive innovation across industries, reduce global reliance on carbon-heavy fuels, and open opportunities for affordable, clean energy.

    The study is published in the journal Geology.

    Featured image: A new study by the University of Vienna explains why “fairy circles” – circular areas where vegetation is damaged, as seen here in the São Francisco Basin in Brazil – subside and how their diameter is related to the depth of the hydrogen source. Credit: Alain Prinzhofer/University of Vienna

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  • NSF NRAO Hosts SpectrumX Field Experiment at the Very Large Array

    NSF NRAO Hosts SpectrumX Field Experiment at the Very Large Array

    The U. S. National Science Foundation’s National Radio Astronomy Observatory (NSF NRAO) recently collaborated with NSF SpectrumX, the Spectrum Innovation Center, to host a large-scale spectrum research experiment at the U.S. National Science Foundation Very Large Array (NSF VLA) in New Mexico.

    This week-long effort, conducted in July 2025, brought together researchers, students, and experts from across academia, government, and industry to study spectrum usage in the 7.125 to 7.4 GHz band—frequencies of increasing importance to both science and emerging sixth-generation (6G) communications. Because of the unique sensitivity of the NSF VLA, the experiment provided a vital opportunity to explore how future spectrum allocations may affect radio astronomy and other passive scientific applications. Read the full release HERE. 

    About NRAO
    The National Radio Astronomy Observatory is a facility of the U.S. National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.

    Contact:

    Corrina C. Jaramillo Feldman, Senior Public Information Officer
    National Radio Astronomy Observatory
    cfeldman@nrao.edu
    (505) 366-7267
    public.nrao.edu

    About SpectrumX

    SpectrumX is funded by the NSF as part of its Spectrum Innovation Initiative, under grant number AST 21-32700. SpectrumX is the world’s largest academic hub where all radio spectrum stakeholders can innovate, collaborate, and contribute to maximizing social welfare of this precious resource.

    To learn more about SpectrumX, please visit spectrumx.org.

    Contact:

    Stephanie Loney, Research Communications Specialist
    NSF SpectrumX / Notre Dame Research / University of Notre Dame
    sloney@nd.edu / 574.631.7804
    spectrumx.org

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  • Stressed Ice Generates Electricity, Researchers Find

    Stressed Ice Generates Electricity, Researchers Find

    Don’t mess with ice. When it’s stressed, ice can get seriously sparky.

    Scientists have discovered that ordinary ice—the same substance found in iced coffee or the frosty sprinkle on mountaintops—is imbued with remarkable electromechanical properties. Ice is flexoelectric, so when it’s bent, stretched, or twisted, it can generate electricity, according to a Nature Physics paper published August 27. What’s more, ice’s peculiar electric properties appear to change with temperature, leading researchers to wonder what else it’s hiding.

    The paper changes “how we view ice: from a passive material to an active material that may be at play for both fundamentals and applications,”
    Xin Wen, study lead author and a nanophysicist at Institut Catala de Nanociencia i Nanotecnologia in Spain, told Gizmodo in an email.

    A cold case in molecular chemistry

    An unsolved mystery in molecular chemistry is why the structure of ice prevents it from being piezoelectric. By piezoelectricity, scientists refer to the generation of an electric charge when mechanical stress changes a solid’s overall polarity, or electric dipole moment.

    The water molecules that make up an ice crystal are polarized. But when these individual molecules organize into a hexagonal crystal, the geometric arrangement randomly orients the dipoles of these water molecules. As a result, the final system can’t generate any piezoelectricity.

    However, it’s well known that ice can naturally generate electricity, an example being how lightning strikes emerge from the collisions between charged ice particles. Because ice doesn’t appear to be piezoelectric, scientists were confused as to how the ice particles became charged in the first place.

    “Despite the ongoing interest and large body of knowledge on ice, new phases and anomalous properties continue to be discovered,” the researchers noted in the paper, adding that this unsatisfactory knowledge gap suggests “our understanding of this ubiquitous material is incomplete.”

    A shockingly simple solution

    Fortunately, science likes to compartmentalize seemingly fundamental concepts. Electricity is no exception, so the researchers decided to investigate different “types” of electricity.

    Geometry posed the biggest obstacle to understanding ice’s observed electric behavior, so the team opted for flexoelectricity, which can “exist in materials of any symmetry,” they explained.

    For the experiment, they placed a slab of ice between two electrodes while simultaneously confirming that any electricity produced wasn’t piezoelectric. To their excitement, bending the ice slab created an electric charge, and at all temperatures, too. What they didn’t expect, however, was a thin ferroelectric layer that formed at the ice slab surface below -171.4 degrees Fahrenheit (-113 degrees Celsius).

    “This means that the ice surface can develop a natural electric polarization, which can be reversed when an external electric field is applied—similar to how the poles of a magnet can be flipped,” Wen explained in a statement.

    Surprisingly, “ice may have not just one way to generate electricity but two: ferroelectricity at very low temperatures and flexoelectricity at higher temperatures all the way to 0 [degrees C],” Wen added.

    The utility of stressed-out ice

    The finding is both useful and informative, the researchers said. First, the “flip” between flexoelectricity and ferroelectricity puts ice “on par with electroceramic materials such as titanium dioxide, which are currently used in advanced technologies like sensors and capacitors,” they noted.

    Perhaps more apparent is the finding’s connection to natural phenomena, namely thunderstorms. According to the paper, the electric potential generated from flexoelectricity in the experiment closely matched that of the energy produced by colliding ice particles. At the very least, it would make sense for flexoelectricity to be partly involved in how ice particles interact inside thunderclouds.

    “With this new knowledge of ice, we will revisit ice-related processes in nature to find if there is any other profound consequence of ice flexoelectricity that has been overlooked all the way,” Wen told Gizmodo.

    Both conclusions will need further scrutiny, the researchers admitted. Nevertheless, the findings offer illuminating new insight into something as common as ice—and demonstrate how much there’s still to be learned about our world.

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  • Ice melt is the main driver of Earth’s sea-level surge happening now

    Ice melt is the main driver of Earth’s sea-level surge happening now

    The water level of the Earth’s oceans does not increase by chance. Every millimeter has a cause. When sea levels rise, the reasons are buried in melting ice, warming seas, and the transfer of water from land to ocean.

    Scientists now treat global mean sea level as one of the clearest signals of climate change. And that signal has become louder in the past 30 years.

    Building 30-year record


    Researchers at Hong Kong Polytechnic University (PolyU) have built the first 30-year record of global ocean mass change.

    The study, led by Professor Jianli Chen and Dr. Yufeng Nie, used satellite laser ranging, or SLR, to track water added to the seas between 1993 and 2022.

    Before now, reliable mass records began only in 2002, with the GRACE mission.

    The results of the latest study, published in the Proceedings of the National Academy of Sciences, close that gap and strengthen confidence in how scientists monitor rising sea levels.

    Ice melt and sea-level rise

    Sea level rises for two main reasons. Warm water expands, and melting ice adds mass to the ocean. The PolyU record shows how much mass matters.

    Between 1993 and 2022, global sea level rose by about 90 millimeters (3.5 inches).

    Around 60 percent of that came from added ocean mass, not expansion. In the past two decades, the contribution from ice loss has accelerated, pushing the rate of rise from 3.2 to 3.6 millimeters (0.13 to 0.14 inches) per year.

    Satellites track sea-level rise

    SLR is not a new technology. It has been used for decades to measure satellite distances. But its data were once too coarse to track ocean mass.

    The PolyU team solved that by applying forward modeling, a method that corrects distortions along land-ocean boundaries and accounts for geocenter motion.

    The result is a continuous and reliable record that lines up with the GRACE observations, despite the older method’s limitations.

    The weight of melting ice

    Breaking down the numbers shows where the rise comes from. Greenland added about 0.60 millimeters (0,24 inches) of sea-level rise each year between 1993 and 2022. Glaciers contributed a similar amount. Antarctica added 0.40 millimeters (0.16 inches).

    Changes in land water storage, such as reservoirs and groundwater use, added about 0.32 millimeters (0.012 inches).

    Since the 2000s, Greenland has become the single largest source, while melting ice sheets and glaciers combined now account for about 85 percent of all ocean mass increase.

    The study also picked up short-term swings. Sea levels dipped during the 2010–2011 La Niña and rose sharply during the 2015–2016 El Niño event.

    GRACE captured these shifts with high precision, while SLR detected them more roughly. Even with noise, the agreement between the two systems builds trust in the results. The long-term signal remains unmistakable: ice melt drives today’s rising seas.

    The budget closes

    For years, scientists struggled to match observed sea-level rise with the sum of its causes. That gap created doubts.

    The PolyU study shows the budget now closes. The combined effects of warming water and ocean mass increase line up with altimetry observations almost perfectly.

    From 1993 to 2022, the numbers differ by less than 0.1 millimeters per year (0.0004 of an inch). That closure means researchers can now account for nearly every drop.

    Climate and sea-level rise

    “In recent decades, climate warming has led to accelerated land ice loss, which has played an increasingly dominant role in driving global sea-level rise,” said Professor Jianli Chen.

    “Our research enables the direct quantification of global ocean mass increase and provides a comprehensive assessment of its long-term impact on sea-level budget. This offers crucial data for validating coupled climate models used to project future sea-level rise scenarios,” added Prof. Chen.

    This point highlights the urgency of connecting observational science with climate models. Accurate data on ocean mass strengthens the ability to project how coastlines may change in decades to come.

    “The research showed that the ocean-mass changes derived from SLR analysis align well with the total sea-level changes observed by satellite altimeters, after accounting for the effect of ocean thermal expansion. This demonstrates that the traditional SLR technique can now serve as a novel and powerful tool for long-term climate change studies,” noted Dr. Yufeng Nie.

    What comes next

    The work proves SLR still has value. It cannot match the fine detail of GRACE, but it extends the record back another decade and cross-checks existing data.

    Improvements are possible. Adding other satellite systems and refining models could sharpen results even further. What matters most is the message: the oceans are rising faster, and melting ice is the main reason.

    Sea-level rise no longer hides behind uncertainty. The numbers tell the same story across methods. Thermal expansion is steady, but ice loss is climbing.

    The seas are rising, and they are rising faster than before. The message is clear, and it is one that humanity cannot afford to ignore.

    The study is published in the journal Proceedings of the National Academy of Sciences.

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  • NASA Spaceline Current Awareness List #1,164 29 August 2025 (Space Life Science Research Results)

    NASA Spaceline Current Awareness List #1,164 29 August 2025 (Space Life Science Research Results)

    The abstract in PubMed or at the publisher’s site is linked when available and will open in a new window.

  • McGregor HR, Hupfeld KE, Pasternak O, Beltran NE, De Dios YE, Bloomberg JJ, Wood SJ, Riascos RF, Reuter-Lorenz PA, Seidler RD.Crewmember demographic factors and their association with brain and ocular changes following spaceflight.npj Microgravity. 2025 Aug 28;11:59.PI: R.D. SeidlerNote: ISS results. This article may be obtained online without charge.

    Journal Impact Factor: 5.1

    Funding: “This study was supported by NASA grant #NNX11AR02G awarded to RDS, SJW, PARL, and JJB. HRM was supported by an NSERC postdoctoral fellowship, a Translational Research Institute for Space Health Postdoctoral Fellowship, and a NASA Human Research Program augmentation grant. KEH was supported by National Institute on Aging fellowships F99AG068440 and K00AG068440.”

  • Friedman MA, Zeineddine Y, Tuyambaze O, Elhawabri W, Al Shammary A, Stodieck L, Ferguson VL, Donahue H.Simulated microgravity accurately models long-duration spaceflight effects on bone and skeletal muscle in skeletally immature mice.Bone Rep. 2025 Sep;26:101871.PI: M.A. FriedmanNote: Hindlimb unloading study.

    Journal Impact Factor: 2.6

    Funding: “This work is supported by the Translational Research Institute for Space Health Postdoctoral Fellowship (NASA Cooperative Agreement NNX16AO69A), Center for the Advancement of Science in Space User Agreement UA-2019-888, and National Institutes of Health 3UM1TR004360-02S2.”

  • Lonner TL, Austin CR, Blake JS, Gupta P, Katz JM, Gopinath AR, Clark TK.Impact of sickness induced by centrifugation on tilt perception.Front Neurol. 2025 Aug 12;16:1628938.PI: T.K. ClarkNote: This article is part of Research Topic “Impact of Vestibular Dysfunction Studies on Space Flight Health Challenges” (https://genelab.nasa.gov). The Research Topic also includes articles from previous Current Awareness Lists #1,075 https://doi.org/10.3389/fneur.2023.1284029 and #1,139 https://doi.org/10.3389/fneur.2025.1556553. This article may be obtained online without charge.

    Journal Impact Factor: 2.8

    Funding: “This work was supported by the National Aeronautics and Space Administration Human Research Program under Grant No. 80NSSC23K0449.”

  • Hughes AM, Jenkins BE, Bauer LV, Kiss JZ.Performance and accuracy of the automated measurement software: Simple Online Automated Plant Phenomics (SOAPP).Gravit Space Res. 2025 Aug 7;13(1):51-64.PI: J.Z. KissNote: This article may be obtained online without charge.

    Journal Impact Factor: 2.0

    Funding: PI reports past NASA funding.

  • Johns S, Wiegman E, Bakshi A, Gilroy S.The cyclic nucleotide-gated channels CNGC2 and CNGC4 support systemic wound responses in Arabidopsis thaliana.Front Plant Sci. 2025 Aug 21;16:1545065.PI: S. GilroyNote: This article may be obtained online without charge.

    Journal Impact Factor: 4.8

    Funding: “The authors are grateful for funding for this work from NSF MCB2016177, NASA 80NSSC21K0577 and 80NSSC19K0126, and the Wisconsin Space Grant Consortium.”

  • Evans MA, Walsh K.Clonal hematopoiesis in cancer and cardiovascular disease: JACC: CardioOncology state-of-the-art review.JACC: CardioOncology. 2025 Aug;7(5):470-95.PI: K. WalshNote: This article may be obtained online without charge.

    Journal Impact Factor: 12.8

    Funding: “These studies were supported by National Institutes of Health grants AG073249 and AG086508, Department of Defense grant CA210887, and National Aeronautics and Space Administration grant 80NSSC21K0549 to Dr Walsh.”

  • Walsh RFL, Smith LT, Bisgay A, Stephenson AR, Goel N, Alloy LB.Sleep duration as a mediator of the association between caffeine intake and mood symptoms: An intensive longitudinal study of young adults with and without bipolar spectrum disorders.Chronobiology International. 2025 Aug 18;1-11. Online ahead of print.PI: N. GoelJournal Impact Factor: 1.7

    Funding: “This study was supported in part by the National Science Foundation’s Graduate Research Fellowship to Rachel Walsh and by National Institute of Mental Health R01 grants [MH077908, MH102310, and MH126911] to Lauren B. Alloy. Namni Goel was supported in part by National Aeronautics and Space Administration (NASA) grants [NNX14AN49G] and [80NSSC20K0243] and National Institutes of Health grant [R01DK117488].”

  • Bouvet P, Bevilacqua C, Ambekar Y, Antonacci G, Au J, Caponi S, Chagnon-Lessard S, Czarske J, Dehoux T, Fioretto D, Fu Y, Guck J, Hamann T, Heinemann D, Jähnke T, Jean-Ruel H, Kabakova I, Koski K, Koukourakis N, Krause D, La Cavera S, Landes T, Li J, Mahmodi H, Margueritat J, Mattarelli M, Monaghan M, Overby DR, Perez-Cota F, Pontecorvo E, Prevedel R, Ruocco G, Sandercock J, Scarcelli G, Scarponi F, Testi C, Török P, Vovard L, Weninger WJ, Yakovlev V, Yun S-H, Zhang J, Palombo F, Bilenca A, Elsayad K.Consensus statement on Brillouin light scattering microscopy of biological materials.Nat Photon. 2025 Jul 3;19(7):681-91.Note: This article may be obtained online without charge.

    Journal Impact Factor: 32.9

    Funding: “…support from NASA, BARDA, the NIH and USFDA under contract/agreement no. 80ARC023CA002.”

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  • Marsquakes reveal exactly how the Red Planet was formed

    Marsquakes reveal exactly how the Red Planet was formed

    Scientists have been curious for years about what is hidden beneath the surface of Mars. With its freezing temperatures, red dust, and dry valleys, the surface of the planet has received most of the attention. But something big is buried deep inside Mars’ mantle.

    Thanks to NASA’s Insight lander, we’re finally getting a clearer look below the surface. And what’s there is surprising: leftover chunks from ancient cosmic crashes are buried deep in the planet’s mantle.


    These rocky fragments aren’t small. Some are as wide as 2.5 miles (4 kilometers). They’re scattered across Mars’ interior like forgotten debris from the solar system’s wild early days.

    Mars got slammed – hard

    Giant space rocks – possibly even protoplanets – crashed into Mars some 4.5 billion years ago. They impacted hard enough to melt enormous chunks of the planet’s crust and mantle, and form vast oceans of molten rock.

    When those impacts occurred, they shattered the surface. They blasted rocky debris, including parts of the impactors, deep into the interior of the Red Planet.

    Unlike Earth, which constantly reshuffles its crust through plate tectonics, Mars’ crust is made of a single plate that has stayed mostly stable.

    That’s why those ancient impact scars haven’t been erased. The fragments are still down there, frozen in place like time capsules.

    “We’ve never seen the inside of a planet in such fine detail and clarity before,” said Constantinos Charalambous of Imperial College London, the paper’s lead author.

    “What we’re seeing is a mantle studded with ancient fragments. Their survival to this day tells us Mars’ mantle has evolved sluggishly over billions of years. On Earth, features like these may well have been largely erased.”

    Scientists believe giant impacts — like the one depicted in this artist’s concept — occurred on Mars 4.5 billion years ago, injecting debris from the impact deep into the planet’s mantle. NASA’s InSight lander detected this debris before the mission’s end in 2022. Credit: NASA/JPL-Caltech
    Scientists believe giant impacts – like the one depicted in this artist’s concept – occurred on Mars 4.5 billion years ago, injecting debris from the impact deep into the planet’s mantle. NASA’s InSight lander detected this debris before the mission’s end in 2022. Click image to enlarge. Credit: NASA/JPL-Caltech

    InSight sees into Mars’ mantle

    All of this comes from a mission called InSight, short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport. It was run by NASA’s Jet Propulsion Laboratory in Southern California and the lander arrived on Mars in 2018.

    InSight was the first lander to place a seismometer on Mars’ surface. That device was incredibly sensitive and recorded 1,319 marsquakes before the mission ended in 2022.

    Quakes send out waves that travel through the planet. As those waves move through different materials, they change speed and direction.

    Scientists can study how those waves behave to figure out what’s inside the planet, kind of like how doctors use ultrasound to see inside the human body.

    “We knew Mars was a time capsule bearing records of its early formation, but we didn’t anticipate just how clearly we’d be able to see with InSight,” said Tom Pike of Imperial College London, coauthor of the paper.

    What causes marsquakes?

    Marsquakes still happen, usually for two reasons. Some are caused when rocks crack under pressure and heat. Others are caused by meteoroids slamming into the surface.

    A study published earlier this year in Geophysical Research Letters showed that meteoroid impacts can create high-frequency seismic waves.

    These waves travel deep into the mantle, which is a thick layer of rock beneath the crust. The mantle can be nearly 960 miles (1,545 kilometers) thick, and reach temperatures as high as 2,732 °F (1,500 °C).

    Eight of the marsquakes recorded by InSight had strong, high-frequency signals that got noticeably scrambled and delayed.

    “When we first saw this in our quake data, we thought the slowdowns were happening in the Martian crust,” Pike said.

    “But then we noticed that the farther seismic waves travel through the mantle, the more these high-frequency signals were being delayed.”

    Buried lumps in Mars’ mantle

    Computer simulations helped scientists figure it out. Those delays only happened when the quake waves passed through small regions of the mantle that had a different composition from everything around them. These were the buried impact fragments.

    Some were massive. Others were smaller. All were mixed into the mantle, which Charalambous compared to “shattered glass – a few large shards with many smaller fragments.”

    That fits with what we already know: In the early solar system, planets like Mars got hit often and hard.

    Charalambous said the fact that these features are still visible “tells us Mars hasn’t undergone the vigorous churning that would have smoothed out these lumps.”

    A cutaway view of Mars in this artist’s concept (not to scale) reveals debris from ancient impacts scattered through the planet’s mantle. On the surface at left, a meteoroid impact sends seismic signals through the interior; at right is NASA’s InSight lander. Credit: NASA/JPL-Caltech
    A cutaway view of Mars in this artist’s concept (not to scale) reveals debris from ancient impacts scattered through the planet’s mantle. On the surface at left, a meteoroid impact sends seismic signals through the interior; at right is NASA’s InSight lander. Click image to enlarge. Credit: NASA/JPL-Caltech

    What other planets might be hiding

    This discovery doesn’t just help us understand Mars. It also gives clues about other rocky planets – especially ones that don’t have tectonic activity, like Venus and Mercury.

    If Mars is holding onto traces of ancient impacts deep in its mantle, maybe those planets are, too.

    Mars has always been a quiet planet on the surface. But now we know that, deep inside, it’s holding the scars of an ancient and violent past – and it hasn’t let them go.

    The study was published in the journal Science.

    Image credit: NASA/JPL-Caltech

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  • Platelets found to mop up DNA fragments and improve early cancer detection

    Platelets found to mop up DNA fragments and improve early cancer detection

    Platelets are probably best known for their role in blood clotting, making scabs and related, if less salubrious, contributions to heart attacks and strokes. But these tiny, saucer-shaped blood cells have other physiological duties as well, including surveillance for viral or bacterial infections, the recruitment of immune cells to the site of a suspected incursion and even the direct destruction of pathogens. Now, thanks to the findings of a Ludwig Cancer Research study, we can add to this rich portfolio an additional and critically important function.

    Researchers led by Ludwig Oxford’s Bethan Psaila and postdoc Lauren Murphy report in the current issue of Science that platelets may also help suppress systemic inflammation. Better yet, the way they do so can be readily harnessed to significantly improve the early and minimally invasive detection of cancer and the sensitivity of prenatal screening.

    While platelets do not have their own nuclei, we discovered that they act like sponges, mopping up the fragments of DNA that are released by dead and dying cells. Our bodies employ multiple mechanisms to clear these bits of DNA from the bloodstream, as they can provoke inflammatory and autoimmune disorders if they accumulate. Our findings suggest platelets play an important role in limiting the abundance of DNA fragments in plasma. Fascinatingly, we also discovered that they then release these pieces of DNA when they are activated, suggesting that platelets can deploy their DNA cargo in a manner that prevents nonspecific inflammation yet elicits targeted inflammatory responses where they’re needed, such as, say, at a site of injury.”


    Bethan Psaila, Ludwig Oxford

    Cell-free (cf) DNA can also include traces of circulating tumor cell-derived DNA (ctDNA). An increasingly sophisticated suite of technologies now exists to isolate and analyze ctDNA for the noninvasive detection of cancers and monitoring of responses to therapy. But ctDNA levels are very low, especially in the earliest stages of disease, when cancers are best detected. Its rarity reduces the sensitivity of cancer screening by such “liquid biopsies”.

    As it happens, the cfDNA collected for these diagnostics is currently isolated from blood plasma after all the blood cells, including platelets, have been discarded. The findings of this study suggest that a substantial proportion of cfDNA, including that derived from tumor cells, is contained within platelets, and this important source of information is therefore being missed.

    “We’ve demonstrated that platelets take up DNA fragments that bear the mutational signatures of cancer cells,” said Murphy. “This is true not only in patients with advanced cancer but, remarkably, also in people who have pre-cancerous polyps in their colon, suggesting that platelets may offer an additional and so far untapped reservoir of cfDNA that could significantly improve the sensitivity of liquid biopsies.”

    The finding that circulating platelets bear the genetic signatures of cancer has significant implications for cancer prevention.

    What prompted the researchers to look for DNA in cells that lack a nucleus?

    Platelets have a notable morphological quirk: they’re shot through, like sponges, with a network of membrane-lined channels called the open canalicular system. These channels allow them to release certain biomolecules essential to clotting and tissue repair upon activation and to pick up others, like viral RNA and DNA, as they circulate. Given the latter capability, Psaila hypothesized several years ago at a multi-institutional, cross-disciplinary brainstorming session organized by the philanthropy Cancer Research UK that platelets might also be picking up genomic cfDNA.

    In partnership with senior author Chris Gregory at the University of Edinburgh, Psaila prepared a pitch, winning a small award that allowed her to hire a research assistant, Murphy, to validate this hypothesis. A year later, the researchers had exciting data that helped Murphy secure a position in a PhD program and a major early detection project grant from Cancer Research UK.

    They and their colleagues, including Ludwig Oxford’s Benjamin Schuster-Böckler, whose lab conducted computational analysis for this study, showed that platelets indeed mop up human cfDNA in lab cultures and clinical samples. To prove that they weren’t just seeing residual DNA from megakaryocytes-nucleated cells from which platelets are derived-the researchers examined DNA from the platelets of pregnant women known to be carrying males. They report that they could predict the sex of the baby in every blood sample they analyzed by detecting fragments of the Y chromosome in the platelets, which could only have come from fetal cfDNA they’d mopped up in their travels.

    “Given their abundance, ease of isolation and tissue-wide perfusion, platelets are ideally positioned to serve as biosensors for genetic perturbations across tissues,” said Psaila.

    Future work in the lab will seek to clarify the role of platelets in the physiological management of cfDNA and the fate and consequences of DNA fragments released upon platelet activation.

    This study was funded by Ludwig Cancer Research, Cancer Research UK, the UK Medical Research Council, Rosetrees Trust, Kidani Memorial Trust and Yosemite.

    Bethan Psaila is an associate member of the Oxford Branch of the Ludwig Institute for Cancer Research and an associate professor in hematology at the University of Oxford.

    Source:

    Journal reference:

    Murphy, L., et al. (2025). Platelets sequester extracellular DNA, capturing tumor-derived and free fetal DNA. Science. doi.org/10.1126/science.adp3971

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