Category: 7. Science

  • This interstellar comet may be a frozen relic from before the Sun

    This interstellar comet may be a frozen relic from before the Sun

    A mystery interstellar object discovered last week is likely to be the oldest comet ever seen – possibly predating our solar system by more than three billion years, researchers say.

    The “water ice-rich” visitor, named 3I/ATLAS, is only the third known object from beyond our solar system ever spotted in our cosmic neighbourhood and the first to reach us from a completely different region of our Milky Way galaxy.

    It could be more than seven billion years old, according to University of Oxford astronomer Matthew Hopkins – who is discussing his findings at the Royal Astronomical Society’s National Astronomy Meeting 2025 in Durham – and may be the most remarkable interstellar visitor yet.

    Unlike the previous two objects to enter our solar system from elsewhere in the cosmos, 3I/ATLAS appears to be travelling on a steep path through the galaxy, with a trajectory that suggests it originated from the Milky Way’s ‘thick disk’ – a population of ancient stars orbiting above and below the thin plane where the Sun and most stars reside.

    “All non-interstellar comets such as Halley’s comet formed with our solar system, so are up to 4.5 billion years old,” Hopkins said.

    “But interstellar visitors have the potential to be far older, and of those known about so far our statistical method suggests that 3I/ATLAS is very likely to be the oldest comet we have ever seen.”

    The object was first spotted on July 1, 2025, by the ATLAS survey telescope in Chile, when it was about 670 million km from the Sun.

    Hopkins’ research predicts that, because 3I/ATLAS likely formed around an old, thick-disk star, it should be rich in water ice.

    “This is an object from a part of the galaxy we’ve never seen up close before,” said Professor Chris Lintott, co-author of the study and presenter of the BBC’s The Sky at Night.

    “We think there’s a two-thirds chance this comet is older than the solar system, and that it’s been drifting through interstellar space ever since.”

    As it approaches the Sun, sunlight will heat 3I/ATLAS’s surface and trigger cometary activity, or the outgassing of vapour and dust that creates a glowing coma and tail.

    Early observations already suggest the comet is active, and possibly larger than either of its interstellar predecessors, 1I/’Oumuamua (spotted in 2017) and 2I/Borisov (2019).

    If confirmed, this could have implications for how many similar objects future telescopes, such as the new Vera C. Rubin Observatory, are likely to detect. It may also provide clues about the role that ancient interstellar comets play in seeding star and planet formation across the galaxy.

    “We’re in an exciting time: 3I is already showing signs of activity. The gases that may be seen in the future as 3I is heated by the Sun will test our model,” said co-author Dr Michele Bannister, of the University of Canterbury in New Zealand.

    “Some of the biggest telescopes in the world are already observing this new interstellar object – one of them may be able to find out!”

    The discovery of 3I caught the team by the surprise. It happened as they were gearing up for the beginning of survey operations with the Vera C. Rubin Observatory, which their model predicts will discover between 5 and 50 interstellar objects.

    “The solar system science community was already excited about the potential discoveries Rubin will make in the next 10 years, including an unprecedented number of interstellar objects,” said co-researcher Dr Rosemary Dorsey, of the University of Helsinki.

    “The discovery of 3I suggests that prospects for Rubin may now be more optimistic; we may find about 50 objects, of which some would be similar in size to 3I. This week’s news, especially just after the Rubin First Look images, makes the upcoming start of observations all the more exciting.”

    The team’s findings come from applying a model developed during Hopkins’ doctoral research, which simulates the properties of interstellar objects based on their orbits and likely stellar origins.

    Just a week before the comet’s discovery, Hopkins had defended his thesis, and when 3I/ATLAS was announced, he was set to go on holiday. Instead, he found himself comparing real-time data to his predictions.

    “Rather than the quiet Wednesday I had planned, I woke up to messages like ‘3I!!!!!!!!!!’,” said Hopkins. “It’s a fantastic opportunity to test our model on something brand new and possibly ancient.”

    The researchers’ model, dubbed the Ōtautahi-Oxford Model, marks the first real-time application of predictive modelling to an interstellar comet.

    For those keen to catch a glimpse of 3I/ATLAS, it should be visible through a reasonably-sized amateur telescope in late 2025 and early 2026.

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  • From Microbiota to Microgravity: What’s Inside The FASEB Journal’s Latest Issue

    From Microbiota to Microgravity: What’s Inside The FASEB Journal’s Latest Issue

    Newswise — ROCKVILLE, MD (July 22, 2025) — The 15 July 2025 issue (Vol. 39, Issue 13) of The FASEB Journal showcases a diverse collection of cutting-edge research and reviews spanning gut microbiota, aging in altered gravity, innovative therapeutic strategies, and the cellular mechanisms driving diseases from cardiovascular conditions to cancer. This issue’s articles highlight advances in understanding collective cell migration, macrophage regulation, and the impacts of diet and microbiota on human health, while also exploring promising interventions for conditions like osteoporosis, neuroblastoma, endometriosis, and more. Together, these studies reflect the journal’s commitment to advancing knowledge across the biological and biomedical sciences.

    REVIEW ARTICLES
    Deciphering the Effect of Ginsenoside Rk3 on Gut Microbiota and Its Applications

    Aging and Altered Gravity: A Cellular Perspective

    Honokiol Targeting SIRT3: From Molecular Mechanisms to Therapeutic Opportunities

    Dynamic Leader–Follower Hierarchies in Collective Cell Migration

    Research Progress on the Regulation of Macrophages for Cardiovascular Diseases

    Small Molecules as Regulators of Liquid–Liquid Phase Separation: Mechanisms and Strategies for New Drug Discovery

    Food Additives: Emerging Detrimental Roles on Gut Health

    RESEARCH ARTICLES
    Resistance and Aerobic Preconditioning Delays Unloading-Induced Multisystemic Physiological Changes: The NEBULA Project

    Skeletal Muscle Mitochondria Contain Nuclear-Encoded RNA Species Prior to and Following Adaptation to Exercise Training in Rats

    Exploring PU.1 as a Therapeutic Target to Mitigate Oxidative Stress and Inflammation in Peritoneal Dialysis-Induced Peritoneal Fibrosis

    Vasopressin-Sensitive Aqp2 Regulation Mediated by the TAZ-NR4A1 Axis in Renal Collecting Duct Cells

    Nutritionally Responsive PMv DAT Neurons Are Dynamically Regulated During Pubertal Transition

    Mitochondrial Calcium Uniporter-Mediated Regulation of the SIRT3/GSK3β/β-Catenin Signaling Pathway in Vascular Remodeling

    Therapeutic Potential of GeGen Decoction for the Treatment of Polycystic Ovary Syndrome

    Trained Immunity Induced by Oxidized Low-Density Lipoprotein Is Dependent on Glutaminolysis

    M2-Like Macrophages Exhibit Sialic Acid-Enhanced Efferocytosis via the Siglec CD22

    Homocysteine: Canary in the Coal Mine or Hidden Threat? A Biochemical Study on the Role of Plasma Thiols

    Microgravity-Induced Cognitive Decline: Investigating the Pathogenic Mechanisms of RyR2 Hyperphosphorylation and S107 Intervention

    Obesity Affects IVF Outcomes and Mevalonic Acid Rescues the Side Effects of Statins on Follicle Growth

    MRGPRX2 Mediates Mast Cell-Induced Endometriosis Pain Through the Sensitization of Sensory Neurons via Histamine/HRH1/TRPV1 Signaling Pathway

    SRSF5 Regulates Trophoblast Apoptosis by Inhibiting NR2F2 Transcriptional Activity Through MLX Ubiquitin Degradation Mediated by Alternative Splicing in Preeclampsia

    Akkermansia muciniphila-Derived Outer Membrane Vesicles as a Novel Therapeutic Approach for Mastitis: Insights From In Vitro and Vivo Studies

    ATF7–PINK1 Axis Governs Mitophagy and Intestinal Inflammation in Ulcerative Colitis

    TLR7/8 Agonist R848 Regulates X Sperm Energy Metabolism in Dairy Cows via Inhibiting Glycolysis and Fatty Acid β-Oxidation by LKB1/AMPK Pathway

    Genetic and Functional Dissection of the NFKB2 Gene: Implications for Milk Fatty Acid Biosynthesis in Dairy Cattle

    Cellular Landscape of Synovial Chondromatosis Synovium Revealed by Single-Cell RNA Sequencing

    Genome-Wide CRISPR-Cas9 Knockout Screening Identifies Genes Modulating Cisplatin-Induced Cytotoxicity in Renal Proximal Tubule Epithelial Cells

    MS275 Inhibits Neuroblastoma Cell Growth by Mediating H3K27ac/PROX1 Axis In Silico and In Vitro

    The Regulatory Mechanisms of Treponema pallidum Enolase on Macrophages: From Enzymatic Activity to Signal Transduction

    NTPDase8 Protects Against Liver Ischemia–Reperfusion Injury in Mice

    Exosomal Gene Biomarkers in Osteosarcoma: Mifepristone as a Targeted Therapeutic Revealed by Multi-Omics Analysis

    AlkB Homolog 5 Regulates Hexokinase 2-Mediated Glycolysis and Participates in the Progression of Endometriosis

    Single-Cell RNA Sequencing Highlights a Contribution of Human Amniotic Mesenchymal Stem Cells-Derived Exosomes to Androgenetic Alopecia

    MiR-30d-5p Regulates Bone Remodeling and Vessel Remodeling in Osteoporosis by Targeting GRP78

    Integration of Pharmacodynamics, Proteomics, and Metabolomics to Elucidate Effect and Mechanism of Rehmanniae Radix in the Treatment of T2DM

    Comparing Soy and Milk Protein Regulation of Hepatic Omega-3 Fatty Acid Biosynthesis

    Non-Invasive Ultrasound Treatment Enhances the Release of Skeletal Muscle-Derived Extracellular Vesicles in Mice

    Antiproliferative and Apoptotic Effects of Mono/Combined Treatment of Abemaciclib and Regulation of Neuroblastoma-Related miRNAs

    Cholesterol Within Phosphatidylcholine Liposomes Attenuates the Expression of Cytokines

    Wnt Activation in Mature Dermal Adipocytes Leads to Lipodystrophy and Skin Fibrosis via ATGL-Dependent Lipolysis

    Non-Surgical Periodontal Therapy and Metformin Improve Bone Loss in Obese Mice With Periodontitis by Modulating the Gut Microbiota

    Therapeutic Effects of Mesenchymal Stem Cell Secretome Derived From Adipose Tissue, Umbilical Cord, and Bone Marrow Against Extended-Spectrum Beta-Lactamase-Producing and Non-Producing Escherichia coli Strains Isolated From Urinary Tract Infections

    Lycium barbarum Polysaccharide Ameliorates Hindlimb Unloading-Induced Bone Loss by Targeting Noggin

    Multi-Omics Integration Reveals Gut Microbiota-Bile Acid Crosstalk Underlying Baizhu Shaoyao Decoction’s Therapeutic Efficacy in Weaning Stress of Piglets

    Quercetin and Kaempferol Mitigate Endotoxin-Induced Skeletal Muscle Wasting by Inhibiting KLF15 Expression and Restoring the Antioxidant System

    Comparison of Two MPTP Doses on Mouse Behaviors and Pathologies

    Dietary Manganese Modulates Microbiota and Intestinal N-Acylethanolamines in a Sex-Specific Manner in Mice With Diet-Induced Obesity

    RESEARCH LETTER
    Effect of Renal Denervation on Early and Late Stages of Diabetic Nephropathy

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    About The FASEB Journal
    The FASEB Journal, the flagship publication of the Federation of American Societies for Experimental Biology (FASEB), leads in publishing groundbreaking multidisciplinary research in biology and biomedical sciences. It spans all levels of biological organization, from molecular to population studies. The journal drives advances in basic, translational, pre-clinical, and early clinical research. Known for its rigorous peer-review process, The FASEB Journal is dedicated to advancing high-quality scientific discoveries and shaping the future of science.

    About FASEB
    FASEB is comprised of 22 scientific member societies with 110,000 members, making it the largest coalition of biomedical research associations in the United States. FASEB’s mission is to advance health and well-being by promoting research and education in biological and biomedical sciences through collaborative advocacy and service to member societies and their members. Visit faseb.org for more information.

    Find FASEB Online
    Website: www.faseb.org
    X: @FASEBorg
    LinkedIn: FASEB
    Instagram: @FASEBofficial
    Bluesky: @faseborg.bsky.social


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  • Nobel Laureate Conversation: Prof. J. Michael Kosterlitz

    Nobel Laureate Conversation: Prof. J. Michael Kosterlitz

    Newswise — CQ1: Can you share the story behind your discovery of Kosterlitz-Thouless (KT) transition? Is there any preceding research that relates to or inspires you to discover KT transition?

    A1: When I accepted the postdoc position in Birmingham, I intended to shift from high-energy physics to a different field, perhaps condensed matter physics. I spoke with several faculty members to get their advice. One day, David Thouless showed me some experimental results on thin helium films, which clearly indicated a phase transition that didn’t align with existing theories. Although I was not David’s student or postdoc, and he probably didn’t even expect me to come up with anything given his very vague ideas, I decided to make efforts. After several months, I eventually came back and showed him what I got. We decided to write and publish this, and the rest is the history you’ve all known.

    Q2: KT transition has challenged the conventional wisdom at the time, did you encounter any skepticism?

    A2: Thouless and I were exactly the right people to look at this problem. The situation was clearly awkward because there was a conflict between theory and experiment, and the theory looked extremely reasonable. At that time, I was completely ignorant of condensed matter physics. But luckily in this case, ignorance turned out to be an advantage as I wasn’t burdened by the conventional notions, so I was free to explore new ideas with nothing to influence my thinking. We managed to solve this problem because we realized that instead of thinking about the low energy excitation, the only possibility was to think higher energy excitation, essential for the vortex excitations, the only excitations that we can destroy superfluidity.

    Q3: What were the key inspirations that led you to explore topology in condensed matter physics?

    A3: I have to admit, I didn’t even know what topology was at the time. I only had a vague idea that it was a branch of mathematics concerned with characterizing various shapes, but I had no idea of its importance until I had done a lot of calculations. I then talked to Thouless and he said these vortices were topological excitations, and that’s how ‘topological physics’ came into the picture. But it doesn’t change anything, because what I really did and understood was physics. So to me it was simple and intuitive. Thouless found those vortex behaviors look like topology to him. And we can bring those fancy mathematical names to physics, but underneath is physics only.

    Q4: Following your theoretical breakthrough, many of the experimental verification were conducted in the years after, did those verification timelines match your expectations?

    A4: After we finished and published the work, we were eager about experimental verifications. At that time, a few experimental groups were studying helium films, particularly, John Reppy’s group at Cornell had been working on thin superfluid films for quite some time. So I went to Cornell for a one-year postdoc, and one day I was giving a seminar about what Thouless and I had achieved, but it seemed that almost no one really followed our reasoning. I remember that even Kenneth G. Wilson—who later won Nobel Prize in Physics 1982 – was also there and asked me a question about irrelevant variables. I had no idea what he was talking about, so I sort of hummed and hawed basically giving a non-answer to his question. But there was one single person in that room who really got it: a bright young graduate student named David R. Nelson (now professor at Harvard). From then on, we got along very well.

    So back then, what we did involve new physics and all sorts of heretical ideas, but turned out to be right. It really needed young and open minds to grasp and develop it further. Nelson and I later collaborated on calculating the normalized superfluid density at the transition point. We managed to come up with this universal jump prediction, where the ratio of the superfluid density is a universal constant in terms of various fundamental properties, e.g., mass of the helium atoms, Plank’s constant. And this is in principle a measurable quantity, because the superfluid density is basically the stiffness constant, to be measured by the flow properties.

    Then there was still a slight problem to conquer. Superfluidity says that there’s no dissipation in the flow, which implies that the flow velocity is finite. However, the theoretical prediction was at zero flow velocity and zero frequency. An extrapolation from the dynamical predictions was needed to agree perfectly with all the experimental measurements, which was later done by Nelson, Vinay Ambegaokar and B.I. Halperin. It took a few years for the physical community to accept that the weird theory (KT transition) was correct.

    Q5: The KT transition has led to applications in superconductivity, superfluidity, and 2D materials, what’s your perspective towards them?

    A5: The applications to superconductivity and related phenomena seemed natural. One could say that a superconductor is also a type of superfluid, and our theory should be applicable to it as well. The vortices are the essential excitations to consider in the superfluid and the vortex cores can be described as point particles in two dimensions, which interacts as Coulomb interactions. You can use the same vortex language for superconductivity except that the vortices in a superconducting film interact with a screened Coulomb interaction with a finite screening length.

    Thouless and I published a paper predicting that there should be no phase transition in superconducting films. But it turned out that the screening length in a thin superconducting film is often so long—even bigger than the experimental system itself. Thus it’s very nice to see that our theory of superfluid can also apply to some superconducting films. Similarly, for two-dimensional material whose penetration length is larger than its scale in one dimension, KT transition can also be applied to.

    Thouless came up with all sorts of wonderful applications based on topological ideas.

    The only frustrating part was that I had a health issue that kept me from participating for about six months. Since then, the KT transition has found applications across a wide range of systems, both quantum and classical.

    Q6: Topological concepts are now widely used in physics, leading to promising applications of topological insulators and quantum computing, what’s your vision about them?

    A6: David Thouless deserves more credit for introducing topological ideas into physics. But since I was involved in it, I suppose my name has become associated with it as well. My perspective on this is fairly simple-minded. In quantum computing, you need some sort of object to carry information, so these topological objects are especially useful because they’re not local—they spread and therefore less susceptible to local imperfections, which are inevitable in normal material. In my opinion, it was the key advantage of these topological materials.

    Q7: Could you name the three most important unsolved questions in condensed matter physics?

    A7: Prediction is not my advantage. I prefer to jump in and explore, and then you will naturally know what is important. One of the important unsolved questions to me is in driven out of equilibrium systems:

    ‘Consider a driven out of equilibrium system has a set of possible stationary states. Is any of the states unique?’

    To answer this one, I think one need to include some stochastic noise into the system and to have it started. It eventually will come to a stage of one stationary state. Is there a stationary state unique or deterministic? Or does it depend on initial conditions? Such important question—tying with the evolution of life—may not seem a question to many. However to me, it is the ultimate question, and no other problems are of equal importance.

    Q8: One of your remarkable achievements is to implement topology in physics, showcasing a paradigm of breaking the boundary of disciplines. Our journal eLight is targeting at expanding the boundary of optics and exploring cross-disciplinary research. What should be most valued, when exploring cross-disciplinary research? What kind of cross-disciplinary research could generate broad impact?

    A8: I thought about such questions—but without any answers. The truth is, many major discoveries come out of the blue. Some strange and ridiculous ideas may eventually turn out to be relevant and correct. I don’t believe anyone can predict which field or direction an important idea will come from—it could emerge from anywhere. So, don’t focus on making a broad impact while you’re doing research. When I was working on KT transition, I wasn’t aiming for Nobel Prize. I pursued it simply because it made sense to me. The idea of waking up one morning and saying, ‘Today, I’m going to do something worthy of a Nobel Prize’ would be nice, but that’s not how science works. There’s no way of telling what is going to be important. The only thing one can do is to conquer some problem that truly interests you. Have fun doing it and if you’re lucky, it will turn out to be important with applications here and there.

    Cross-discipline is of course important, and you should try to make people from other disciplines to understand your works. David R. Nelson understood me and tried to prepare an experiment, and I witnessed experiments I had never thought about. Cross-discipline can make theorists and experimentalists understand each other, and find the truth. No matter how fancy your theory is, the ultimate authority is whether the prediction of your theory can be verified or not.

    Q9: Looking back, was there a defining moment or a crucial insight that helped you persist in your research despite early skepticism?

    A9: What has mattered most to me wasn’t a particular thought or idea—it was meeting the right people and finding the right problem to work on. My personal advice for overcoming skepticism is this: find a problem that genuinely excites you. Once you’re excited, you’re motivated, and that motivation will carry you through. If your work is sound and correct, the skepticism will eventually fade away.

    Another key insight is to have fun with your research. That’s easier said than done, because if you are paid to do research, usually what you find fun is not what whoever paying you finds fun. Many people prioritize success over fun, but the unfortunate truth is, not many people actually achieve success. That’s why it’s important to let go of the pressure to be important or famous.

    Instead, find a problem which turns you on, then dive in—without worrying about what others think. If you’re lucky, it might turn out to be important. And actually, I personally believe that if you’re genuinely having fun doing your research, you will get a better chance of being successful as well.

    Q10: What advice would you give to younger generation interested in theoretical physics?

    A10: Personally, I’ve been extremely lucky. My father was a well-known academic—brilliant with full of unconventional or even heretical ideas. He was also a determined person, firmly believing that his ideas were important and worth working on. This attitude infected me and my academic career was dedicated to trying to understand things. My advice to young generation, as through the whole conversation, is to ‘have fun’. You are pursuing a pathway to scientists. Scientists may not make the greatest living; to me, I enjoy it because I am paid to have fun.

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    References

    DOI

    10.1186/s43593-025-00090-0

    Original Source URL

    https://doi.org/10.1186/s43593-025-00090-0

    About eLight

    The eLight will primarily publish the finest manuscripts, broadly covering all sub-fields of optics, photonics and electromagnetics. In particular, we focus on those emerging topics and cross-disciplinary researches related to optics.


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  • Tracking Molecules In the Interstellar Medium

    Tracking Molecules In the Interstellar Medium

    Stars don’t form out of nothing, but tracking the gas and dust that do eventually form stars is hard. They float around the galaxy at almost absolute zero, emitting essentially no light, and generally making life difficult for astronomers. But, part of how they make life difficult is actually the key to studying them – they have “absorption lines” that detail what kind of material the light is passing through on its way to Earth. A new paper from Harvey Liszt of America’s National Radio Astronomy Observatory and Maryvonne Gerin of the Sorbonne details how tracking those absorption lines via radio astronomy can trace the “dark neutral medium” of interstellar gas throughout the galaxy.

    The paper describes the findings of 88 “sight lines”, which in this context is a straight line from Earth to a very bright object, like a quasar or another galaxy. As the light from these bright objects makes it way toward Earth, some of the light is absorbed by the interstellar medium (ISM), creating a distinct dark spot in the spectra coming from the light source.

    These absorption lines are particularly strong in the radio spectrum, so the paper focused on data from two different radio antennas. The Atacama Large Millimeter/Submillimeter Array (ALMA), one of the world’s best know radio telescopes, the Institut de radioastronomie millimétrique at the Sorbonne, and the Arizona Radio Observatory, all contributed data to this paper, with some of the data gathered as long as 30 years ago.

    Dr. Christopher McKee discusses what makes up the interstellar medium. Credit – Serious Science YouTube Channel

    Six different ions were the focus of this paper, with varying levels of success. The formyl cation (HCO+) was the most commonly found molecule, being present in 72 of the 86 sight lines it had data collected for. It seemed to be the best predictor of where molecule hydrogen gas, the most abundant molecule in the universe, but one that is really hard to directly detect, might be. It forms when H2 and some other elements are hit by cosmic rays, so a large amount of HCO+ would also be indicative that a large amount of H2 would reside in the same area.

    Hydrogen Cyanide (HCN) was another key molecule in the study. Astronomers previously thought this molecule was only present in large quantities in dense clouds of gas where stars were actively forming. However, the paper shows it is present throughout the ISM, forcing some further refinement of the formational process of this molecule.

    The ethynyl radical (C2H) was another key component in the study. It is the second most abundant after HCO+, and, as a very simple hydrocarbon, can show how simple hydrocarbons can morph into more complex ones as they undergo reactions in the ISM. The study also notes that the ratio of C2H to HCO+ changes based on the location conditions in that region of space, such as the dust content, so calculating that ratio for different areas might shed (figurative) light on other processes happening there.

    Lecture on how gas and dust in the interstellar medium blocks light in absorption lines. Credit – Introduction to Astronomy – Wagner YouTube channel

    Other molecules were harder to track. The study didn’t find any carbon monosulfide (CS) at all. Carbon monoxide (CO) was only ever found on sight lights with HCO+, making it redundant, even though it was about 100x brighter than the emission from HCO+.

    Regular formyl radicals (HCO) are also ubiquitous throughout the galaxy, but, according to the paper, their absorption lines are much harder to detect, making them less useful in estimating the presence of these dark gas clouds. HCO+ has a much more clearly defined lines, making it easier to use for this purpose.

    It turns out tracing all these gases throughout the galaxy is one effective way to track down potential areas of star formation, and to watch as the ISM itself starts to clump together in the beginning of that process. As more powerful telescopes come online and we are able to increase the signal to noise ratio of some of these molecule’s signals, they will eventually present a clearer picture of this “dark” part of the universe that is teeming with the next round of star stuff.

    Learn More:

    H. Liszt & M. Gerin – CO, CS, HCO, HCO+, C2H, and HCN in the diffuse interstellar medium

    UT – How Astronomers Mapped the Interstellar Medium – And Discovered The Local Bubble

    UT – Where Does Cosmic Dust Come From? The JWST Provides an Answer

    UT – Astronomy Jargon 101: Interstellar Medium

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  • Spacecraft equipped with a solar sail could deliver earlier warnings of space weather threats to Earth’s technologies

    Spacecraft equipped with a solar sail could deliver earlier warnings of space weather threats to Earth’s technologies

    The burgeoning space industry and the technologies society increasingly relies on – electric grids, aviation and telecommunications – are all vulnerable to the same threat: space weather.

    Space weather encompasses any variations in the space environment between the Sun and Earth. One common type of space weather event is called an interplanetary coronal mass ejection.

    These ejections are bundles of magnetic fields and particles that originate from the Sun. They can travel at speeds up to 1,242 miles per second (2,000 kilometers per second) and may cause geomagnetic storms.

    They create beautiful aurora displays – like the northern lights you can sometimes see in the skies – but can also disrupt satellite operations, shut down the electric grid and expose astronauts aboard future crewed missions to the Moon and Mars to lethal doses of radiation.

    I’m a heliophysicist and space weather expert, and my team is leading the development of a next-generation satellite constellation called SWIFT, which is designed to predict potentially dangerous space weather events in advance. Our goal is to forecast extreme space weather more accurately and earlier.

    The dangers of space weather

    Commercial interests now make up a big part of space exploration, focusing on space tourism, building satellite networks, and working toward extracting resources from the Moon and nearby asteroids.

    Space is also a critical domain for military operations. Satellites provide essential capabilities for military communication, surveillance, navigation and intelligence.

    As countries such as the U.S. grow to depend on infrastructure in space, extreme space weather events pose a greater threat. Today, space weather threatens up to US$2.7 trillion in assets globally.

    In September 1859, the most powerful recorded space weather event, known as the Carrington event, caused fires in North America and Europe by supercharging telegraph lines. In August 1972, another Carrington-like event nearly struck the astronauts orbiting the Moon. The radiation dose could have been fatal. More recently, in February 2022, SpaceX lost 39 of its 49 newly launched Starlink satellites because of a moderate space weather event.

    Today’s space weather monitors

    Space weather services heavily rely on satellites that monitor the solar wind, which is made up of magnetic field lines and particles coming from the Sun, and communicate their observations back to Earth. Scientists can then compare those observations with historical records to predict space weather and explore how the Earth may respond to the observed changes in the solar wind.

    Earth’s magnetic field naturally protects living things and Earth-orbiting satellites from most adverse effects of space weather. However, extreme space weather events may compress – or in some cases, peel back – the Earth’s magnetic shield.

    This process allows solar wind particles to make it into our protected environment – the magnetosphere – exposing satellites and astronauts onboard space stations to harsh conditions.

    Most satellites that continuously monitor Earth-bound space weather orbit relatively close to the planet. Some satellites are positioned in low Earth orbit, about 100 miles (161 kilometers) above Earth’s surface, while others are in geosynchronous orbit, approximately 25,000 miles (40,000 km) away.

    At these distances, the satellites remain within Earth’s protective magnetic shield and can reliably measure the planet’s response to space weather conditions. However, to more directly study incoming solar wind, researchers use additional satellites located farther upstream – hundreds of thousands of miles from Earth.

    The U.S., the European Space Agency and India all operate space weather monitoring satellites positioned around the L1 Lagrange point – nearly 900,000 miles (1,450,000 km) from Earth – where the gravitational forces of the Sun and Earth balance. From this vantage point, space weather monitors can provide up to 40 minutes of advance warning for incoming solar events.

    A diagram showing the Earth, the Sun and the Moon, with the five Lagrange points labeled. L1 is beyond the Moon's orbital path around Earth, closer to the Sun.
    The Lagrange points are equilibrium points for smaller objects, like the Earth, that orbit around a larger object, like the Sun. The L1 point is between the Earth and the Sun, where the gravitational pulls of the two objects balance out. Since the Sun’s pull is so much stronger than the Earth’s, the point is much closer to Earth. Xander89/Wikimedia Commons, CC BY-SA

    Advance warning for space weather

    Increasing the warning time beyond 40 minutes – the current warning time – would help satellite operators, electric grid planners, flight directors, astronauts and Space Force officers better prepare for extreme space weather events.

    For instance, during geomagnetic storms, the atmosphere heats up and expands, increasing drag on satellites in low Earth orbit. With enough advance warning, operators can update their drag calculations to prevent satellites from descending and burning up during these events. With the updated drag calculations, satellite operators could use the satellites’ propulsion systems to maneuver them higher up in orbit.

    Airlines could change their routes to avoid exposing passengers and staff to high radiation doses during geomagnetic storms. And future astronauts on the way to or working on the Moon or Mars, which lack protection from these particles, could be alerted in advance to take cover.

    Aurora lovers would also appreciate having more time to get to their favorite viewing destinations.

    The Space Weather Investigation Frontier

    My team and I have been developing a new space weather satellite constellation, named the Space Weather Investigation Frontier. SWIFT will, for the first time, place a space weather monitor beyond the L1 point, at 1.3 million miles (2.1 million kilometers) from Earth. This distance would allow scientists to inform decision-makers of any Earth-bound space weather events up to nearly 60 minutes before arrival.

    Satellites with traditional chemical and electric propulsion systems cannot maintain an orbit at that location – farther from Earth and closer to the Sun – for long. This is because they would need to continuously burn fuel to counteract the Sun’s gravitational pull.

    To address this issue, our team has spent decades designing and developing a new propulsion system. Our solution is designed to affordably reach a distance that is closer to the Sun than the traditional L1 point, and to operate there reliably for more than a decade by harnessing an abundant and reliable resource – sunlight.

    SWIFT would use a fuelless propulsion system called a solar sail to reach its orbit. A solar sail is a hair-thin reflective surface – simulating a very thin mirror – that spans about a third of a football field. It balances the force of light particles coming from the Sun, which pushes it away, with the Sun’s gravity, which pulls it inward.

    While a sailboat harnesses the lift created by wind flowing over its curved sails to move across water, a solar sail uses the momentum of photons from sunlight, reflected off its large, shiny sail, to propel a spacecraft through space. Both the sailboat and solar sail exploit the transfer of energy from their respective environments to drive motion without relying on traditional propellants.

    A solar sail could enable SWIFT to enter an otherwise unstable sub-L1 orbit without the risk of running out of fuel.

    NASA successfully launched its first solar sail in 2010. This in-space demonstration, named NanoSail-D2, featured a 107-square-foot (10 m2 ) sail and was placed in low Earth orbit. That same year, the Japanese Space Agency launched a larger solar sail mission, IKAROS, which deployed a 2,110 ft2 (196 m2 ) sail in the solar wind and successfully orbited Venus.

    An illustration of a solar sail, which looks like a large, thin square of foil, flying through space.
    An illustration of the solar sail used on the IKAROS space probe. These sails use light particles as propulsion. Andrzej Mirecki, CC BY-SA

    The Planetary Society and NASA followed up by launching two sails in low Earth orbit: LightSail, with an area of 344 ft2 (32 m2 ), and the advanced composite solar sail system, with an area of 860 ft2 (80 m2 ).

    The SWIFT team’s solar sail demonstration mission, Solar Cruiser, will be equipped with a much larger sail – it will have area of 17,793 ft2 (1,653 m2 ) and launch as early as 2029. We successfully deployed a quadrant of the sail on Earth early last year.

    To transport it to space, the team will meticulously fold and tightly pack the sail inside a small canister. The biggest challenge to overcome will be deploying the sail once in space and using it to guide the satellite along its orbital path.

    If successful, Solar Cruiser will pave the way for SWIFT’s constellation of four satellites. The constellation would include one satellite equipped with sail propulsion, set to be placed in an orbit beyond L1, and three smaller satellites with chemical propulsion in orbit at the L1 Lagrange point.

    The satellites will be indefinitely parked at and beyond L1, collecting data in the solar wind without interruption. Each of the four satellites can observe the solar wind from different locations, helping scientists better predict how it may evolve before reaching Earth.

    As modern life depends more on space infrastructure, continuing to invest in space weather prediction can protect both space- and ground-based technologies.

    This article is republished from The Conversation, a nonprofit, independent news organization bringing you facts and trustworthy analysis to help you make sense of our complex world. It was written by: Mojtaba Akhavan-Tafti, University of Michigan

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    Mojtaba Akhavan-Tafti receives funding from NASA. He is the Principal Investigator of Space Weather Investigation Frontier (SWIFT).

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  • This tiny rice plant could feed the first lunar colony

    This tiny rice plant could feed the first lunar colony

    The future of sustained space habitation depends on our ability to grow fresh food away from Earth. The revolutionary new collaborative Moon-Rice project is using cutting-edge experimental biology to create an ideal future food crop that can be grown in future deep-space outposts, as well as in extreme environments back on Earth.

    Modern space exploration relies heavily on resupplies of food from Earth, but this tends to be largely pre-prepared meals that rarely contain fresh ingredients. To counteract the negative effects that the space environment can have on human health, it’s important to have a reliable source of food rich in vitamins, antioxidants, and fibres.

    The Moon-Rice project aims to develop the perfect crop for sustaining life in space for long-duration missions, such as the occupation of permanent bases on the Moon or on Mars. “Living in space is all about recycling resources and living sustainably,” says Marta Del Bianco, a plant biologist at the Italian Space Agency. “We are trying to solve the same problems that we face here on Earth.”

    Dr Del Bianco explains that one of the major challenges is the current size of crops grown on Earth. Even many dwarf varieties of rice are still too big to be grown reliably in space. “What we need is a super-dwarf, but this comes with its own challenges,” she says. “Dwarf varieties often come from the manipulation of a plant hormone called gibberellin, which can reduce the height of the plant, but this also creates problems for seed germination. They’re not an ideal crop, because in space, you just don’t have to be small, you must also be productive.”

    The Moon-Rice project is not just a solo effort by the Italian Space Agency and also involves the collaboration of three Italian Universities. “The University of Milan has a very strong background in rice genetics, the University of Rome ‘Sapienza’ specialises in the manipulation of crop physiology and the University of Naples ‘Federico II’ has an amazing heritage in space crop production,” says Dr Del Bianco. “We started this four-year project nine months ago, so it’s very much a work in progress, but the preliminary results we have now are really promising,” says Dr Del Bianco.

    “Researchers at the University of Milan are isolating mutant rice varieties that can grow to just 10 cm high, so they’re really tiny and this is a great starting point,” says Dr Del Bianco. “At the same time, Rome has identified genes that can alter the plant architecture to maximize production and growth efficiency.” Additionally, since meat production will be too inefficient for resource and space-limited space habitats, Dr Del Bianco and her team are looking into enriching the protein content of the rice by increasing the ratio of protein-rich embryo to starch.

    Dr Del Bianco’s own personal focus is on how the rice plants will cope with micro-gravity. “We simulate micro-gravity on Earth by continually rotating the plant so that the plant is pulled equally in all directions by gravity. Each side of the plant gets activated continuously and it doesn’t know where the up and down is,” says Dr Del Bianco. “It’s the best we can do on Earth because, unfortunately, doing experiments in real microgravity conditions, i.e. in space, is complex and expensive.”

    Not only can fresh food be more nutritious than pre-cooked and packaged space meals, but it has significant psychological benefits too. “Watching and guiding plants to grow is good for humans, and while pre-cooked or mushy food can be fine for a short period of time, it could become a concern for longer-duration missions,” says Dr Del Bianco.

    Space exploration is a very demanding job, which requires astronauts to be in peak physical and psychological condition. “If we can make an environment that physically and mentally nourishes the astronauts, it will reduce stress and lower the chances of people making mistakes. In space, the best case of a mistake is wasted money, and the worst case is the loss of lives,” says Dr Del Bianco.

    The Moon-Rice project is not only beneficial for space explorers but will have useful applications for growing plants in controlled environments on Earth too. “If you can develop a robust crop for space, then it could be used at the Arctic and Antarctic poles, or in deserts, or places with only a small amount of indoor space available,” says Dr Del Bianco.

    This research is being presented at the Society for Experimental Biology Annual Conference in Antwerp, Belgium on the 9th July 2025.

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  • Tracing Black Carbon’s Journey to the Ocean

    Tracing Black Carbon’s Journey to the Ocean

    Source: Global Biogeochemical Cycles

    Whether from a forest on fire or gasoline powering a car, organic matter rarely combusts completely: Remnants such as char and soot can persist in the environment for decades. Over time, as physical and biological processes break down the scorched leftovers, some of the carbon they contain leaches into groundwater, lakes, and rivers, eventually making its way to the ocean.

    This carbon, known as dissolved black carbon (DBC), represents the ocean’s largest identified reservoir of stable dissolved organic carbon. Yet the isotopic signature of DBC in the ocean does not match what rivers alone supply. This discrepancy suggests there are one or more unknown sources of DBC entering the ocean that are not accounted for in the global carbon budget.

    To address this knowledge gap, Zhao et al. conducted six field surveys along China’s eastern coast, in the Jiulong, Changjiang (Yangtze), and Pearl River estuaries. By gathering samples during all four seasons, the researchers aimed to quantify changes in DBC and shed light on how it moves through coastal ecosystems toward the sea. Prior research focused only on individual estuaries and didn’t always account for how processes may vary across seasons and tide cycles.

    The findings from the new study reveal submarine groundwater discharge (SGD) as a likely missing source of DBC. The scientists observed that as seawater pushed into estuaries during flood tides, DBC levels rose. Conversely, when water flowed out of the estuaries during ebb tides, DBC concentrations fell. They suggest that this pattern occurs because the salty ocean water that mixes into the estuaries during flood tides promotes the release of DBC from groundwater into the water column.

    The researchers estimate that globally, SGD contributes approximately 20% of the riverine discharge of DBC that enters the ocean each year. Given the role that DBC plays in carbon sequestration and biogeochemical cycling in the ocean, the findings underscore the importance of including estuarine processes in global carbon models. (Global Biogeochemical Cycles, https://doi.org/10.1029/2025GB008532, 2025)

    —Aaron Sidder, Science Writer

    Citation: Sidder, A. (2025), Tracing black carbon’s journey to the ocean, Eos, 106, https://doi.org/10.1029/2025EO250248. Published on 11 July 2025.
    Text © 2025. AGU. CC BY-NC-ND 3.0
    Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

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  • Anchoring Is Damaging the Fragile Antarctic Seabed

    Anchoring Is Damaging the Fragile Antarctic Seabed

    Marine scientist Matthew Mulrennan was piggybacking on a tourist vessel around the Antarctic Peninsula’s coasts, surveying a seabed teeming with life, when his underwater cameras came across a gray seafloor scarred with ridges.

    Anchoring had churned up the sediment, leaving lifeless patches strewn with crushed sponges. The damage had narrowly missed three giant volcano sponges, which can live for up to 15,000 years and grow larger than the divers who study them.

    “We saw a lot of life on the seafloor and not a lot of regulation around its protection,” said Mulrennan, founder of KOLOSSAL, an ocean exploration and conservation nonprofit in California.

    Anchoring churns up the seabed, destroying life and leaving regular furrows, akin to plow marks. Credit: Matt Mulrennan/KOLOSSAL

    Mulrennan’s footage, which was released alongside a recent study in Frontiers in Conservation Science, provides evidence that the seafloor impacts of anchoring now extend to remote polar waters.

    A Vulnerable Ecosystem

    Retreating sea ice is opening Antarctica’s coast to increasing amounts of ship traffic, including tourist cruises. “Most visitors want to see the penguins, seals, and whales,” Mulrennan said, but the seafloor, which is home to 95% of the continent’s biodiversity, “is where the real action is.”

    With large areas of the Southern Ocean unexplored, scientists estimate that as many as 17,000 species might live on the seabed.

    Colorful life lies on the Antarctic seabed, including the 50-armed death star starfish and the giant volcano sponge, the oldest animal on the planet. Credit: Matt Mulrennan/KOLOSSAL

    Many Antarctic species, such as the giant volcano sponge, are uniquely adapted to extreme cold and play an important ecological role, Mulrennan said. “They filter water, sequester carbon, provide food and habitat.”

    “These are probably some of the most vulnerable ecosystems to anchor in in the world.”

    “These are probably some of the most vulnerable ecosystems to anchor in in the world,” Mulrennan said. Although relatively fast-growing tropical reef communities may start to recover from anchoring in roughly a decade or so, “it could take hundreds or potentially thousands of years for Antarctic ecosystems to grow in the exact same way,” he said.

    Mulrennan surveyed 36 sites around the Antarctic Peninsula between 2022 and 2023, finding anchor damage only at Yankee Harbour on Greenwich Island.

    He showed the footage to Sally Watson, a geophysicist at Earth Sciences New Zealand and a study coauthor, who matched the characteristically uniform, curved gouges to anchor damage observed elsewhere.

    Anchors can dig through 80 centimeters of sediment, but most damage is caused by the connected chain, which sweeps sideways because of winds and currents and can excavate 50 centimeters of sediment where it lies on the seafloor. From above, the scars resemble a broomstick, explained Watson, composed of one main scour stemming from the anchor connected to a series of branching gouges dug as the chain shifts in the sediment.

    “Most of the really important life is within the uppermost 10 centimeters,” Watson said. “Anchoring blasts through that.”

    In 2022, Watson and her colleagues published the first estimate of anchoring’s global footprint, putting its damage on par with bottom trawling.

    Anchors and Icebergs

    Anchoring isn’t the only thing churning up the Antarctic seafloor. Icebergs can drift into shallow water and drag along the seabed—causing well-documented impacts around the Antarctic Peninsula’s coastline, said Lloyd Peck, a marine biologist from the British Antarctic Survey who was not involved in the study.

    Diver surveys show that iceberg scouring can destroy up to 99% of life on the shallow seabed. Regularly uprooted by icebergs, shallow-living species recover relatively quickly, in around a decade.

    Waters deeper than 30 meters are struck less often, Peck said, allowing complex, slow-growing organisms to establish themselves. The slow growth also means these deeper areas take longer to recover.

    At Yankee Harbour, Mulrennan observed the scours in waters 70 meters in depth, so he is confident they were caused by anchoring rather than by icebergs. Peck agreed, noting the large, slow-growing volcano sponges nearby. “That suggests the iceberg scouring is going to be very rare here,” he explained.

    “Activities in Antarctica are bound by strict conservation rules, yet ship anchoring goes almost completely unregulated.”

    Peck said that compared to iceberg scouring, anchoring will have a minor imprint across the Antarctic Peninsula. But the location of an anchoring impact is as important as its scope, he noted. “This is about disrupting sheltered areas that icebergs can’t reach.”

    Species-rich areas in deeper waters, such as Yankee Harbour, could be acting as refugia, Peck explained, reseeding surrounding areas with life after they are scoured by icebergs. To avoid wider ecosystem impacts, he said, “we should be making every effort to avoid anchoring in areas of undisturbed biodiversity.”

    In addition to tourist cruises, research vessels, shipping fleets, and private yachts operate in Antarctic waters. “Activities in Antarctica are bound by strict conservation rules” for all visitors, Mulrennan said, “yet ship anchoring goes almost completely unregulated.”

    Watson and Mulrennan have several suggestions to mitigate anchoring impacts, including limiting time vessels spend on anchor and the use of designated anchorages, where ecological impact can be monitored and limited.

    Above all, anchoring needs wider recognition as a conservation concern, not just in Antarctica but globally, Watson said. “I think we could do better, by changing the way we anchor, the gear we use, but at least understanding that this is not a no-consequences game.”

    Erin Martin-Jones, Science Writer

    Citation: Martin-Jones, E. (2025), Anchoring is damaging the fragile Antarctic seabed, Eos, 106, https://doi.org/10.1029/2025EO250246. Published on 11 July 2025.
    Text © 2025. The authors. CC BY-NC-ND 3.0
    Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

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  • Unmanned devices tested in South China Sea-Xinhua

    Unmanned devices tested in South China Sea-Xinhua

    An intelligent seawater sampling unmanned aerial vehicle (UAV) departs from the “Xiangyanghong 10” in the northern waters of the South China Sea, July 9, 2025. Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

    A thermal-imaging surveillance unmanned aerial vehicle (UAV) takes off from the “Xiangyanghong 10” to conduct scientific research in the northern waters of the South China Sea, July 8, 2025. Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

    An unmanned survey vessel conducts scientific research in the northern waters of the South China Sea, July 9, 2025. Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

    An aeromagnetic fixed-wing unmanned aerial vehicle (UAV) flies over the “Xiangyanghong 10” to conduct scientific research in the northern waters of the South China Sea, July 9, 2025.

    Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

    Chief scientist of the “Innovative Integrated Intelligent Systems Expedition” Lin Jian (C), also dean and chair professor of the Advanced Institute for Ocean Research at Southern University of Science and Technology, supervises operations of scientific research aboard the “Xiangyanghong 10” in the northern waters of the South China Sea, July 8, 2025. Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

    Researchers hoist an autonomous underwater vehicle into the sea in the northern waters of the South China Sea, July 8, 2025. Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

    The “Xiangyanghong 10” conducts “Unmanned Swarm” scientific research in the northern waters of the South China Sea, July 8, 2025. Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

    The “Dolphin 3” surface rescue robot conducts test in the northern waters of the South China Sea, July 9, 2025. Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

    A cross-domain robot takes off from the “Xiangyanghong 10” to conduct scientific research in the northern waters of the South China Sea, July 8, 2025. Chinese researchers successfully carried out scientific tests involving various types of drones, unmanned surface vessels, and autonomous underwater vehicles aboard the “Xiangyanghong 10” in the northern waters of the South China Sea in recent days.

    The “Innovative Integrated Intelligent Systems Expedition,” led by the Advanced Institute for Ocean Research under Southern University of Science and Technology, in collaboration with multiple research institutes, high-tech companies, and science popularization organizations, conducted real-time assessments of the innovation, integration, and intelligence of these unmanned scientific exploration devices. (Xinhua/Zhang Jiansong)

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  • Experimental Chinese satellite turns up in unexpected orbit

    Experimental Chinese satellite turns up in unexpected orbit

    HELSINKI —A Chinese Shiyan satellite appears in a low-inclination orbit never before used by the country, after a week-long detection delay and uncertainty over its mission.

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    Andrew Jones covers China’s space industry for SpaceNews. Andrew has previously lived in China and reported from major space conferences there. Based in Helsinki, Finland, he has written for National Geographic, New Scientist, Smithsonian Magazine, Sky… More by Andrew Jones


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