Category: 7. Science

  • WIde Separation Planets In Time (WISPIT): Two Directly Imaged Exoplanets Around The Sun-like Stellar Binary WISPIT 1

    WIde Separation Planets In Time (WISPIT): Two Directly Imaged Exoplanets Around The Sun-like Stellar Binary WISPIT 1

    [LEFT] A.1: WISPIT 1b, 1c, and background sources highlighted in the H-band median-combined image of epoch 2022-11-19. [RIGHT] WISPIT 1b, 1c, and background sources highlighted in the Ks-band median-combined image of epoch 2024-11-30. — astro-ph.EP

    Wide separation gas giant planets present a challenge to current planet formation theories, and the detection and characterisation of these systems enables us to constrain their formation pathways.

    The WIde Separation Planets In Time (WISPIT) survey aims to detect and characterise wide separation planetary-mass companions over a range of ages from <5 to 20 Myr around solar-type host stars at distances of 75-500 (median: 140) parsecs.

    The WISPIT survey carries out two 5 minute H-band exposures with the VLT/SPHERE instrument and IRDIS camera, separated by at least six months to identify co-moving companions via proper motion analysis. These two H-band observations in combination with a follow-up Ks-band observation were used to determine the colour-magnitude of the co-moving companions and to derive their masses by comparing to AMES-COND and AMES-DUSTY evolutionary tracks.

    We report the discovery of WISPIT 1b and WISPIT 1c, two gas giant exoplanets that are co-moving with the stellar binary WISPIT 1, which itself consists of a K4 star and M5.5 star in a multi-decadal orbit. The planets are at projected separations of 338 au and 840 au and have masses of 10 Mj and 4 Mj respectively.

    We identified two common proper motion planetary companions to a (previously unknown) stellar binary with a Sun-like primary. These targets are ideal for follow up characterisation with both ground and space-based telescopes.

    Monitoring of the orbit with the GRAVITY interferometer will place constraints on their eccentricity, and spectroscopic characterisation will identify the composition and metallicity, providing information on their formation pathways.

    Detail of the WISPIT 1 system. The top panel shows the SPHERE/IRDIS H-band image taken on 2022 November 19, processed with unsharp masking to suppress the stellar halo. The stellar binary WISPIT 1 (behind the coronagraph) is located in the upper left, with its companions highlighted with coloured boxes. Zoomed-in images of the unmasked observation centred on companions WISPIT 1b and WISPIT 1c, are shown in the lower left and lower right panels, respectively. — astro-ph.EP

    Richelle F. van Capelleveen, Matthew A. Kenworthy, Christian Ginski, Eric E. Mamajek, Alexander J. Bohn, Rico Landman, Tomas Stolker, Yapeng Zhang, Nienke van der Marel, Ignas Snellen

    Comments: Accepted for publication in Astronomy & Astrophysics section “10. Planets, planetary systems, and small bodies” on August 25, 2025
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2508.18456 [astro-ph.EP](or arXiv:2508.18456v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2508.18456
    Focus to learn more
    Submission history
    From: Richelle Van Capelleveen
    [v1] Mon, 25 Aug 2025 20:04:02 UTC (3,867 KB)
    https://arxiv.org/abs/2508.18456

    Astrobiology, exoplanet,

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  • Tropical Fruit Molecule Could Revolutionize Liver Cancer Treatment

    Tropical Fruit Molecule Could Revolutionize Liver Cancer Treatment

    A new chemistry breakthrough makes it possible to cheaply recreate cancer-fighting molecules found in guava. The discovery could lead to more accessible treatments for deadly liver cancers and beyond. Credit: Stock

    A new synthesis method makes guava compounds widely available. It holds promise against deadly liver cancer.

    Many modern medicines owe their origins to natural sources.

    One well-known example is willow tree bark, often referred to as “nature’s aspirin.” It contains a compound called salicin, which the human body converts into salicylic acid, a substance that reduces pain and lowers fever.

    A team led by William Chain, an associate professor in the University of Delaware’s Department of Chemistry and Biochemistry, has uncovered a promising approach to battling liver-related cancers, one of the leading causes of cancer deaths worldwide. Their research focuses on a molecule derived from a tropical fruit that may play a key role in developing new treatments.

    Creating guava-based cancer fighters

    Through a technique known as natural product total synthesis, Chain and his research group have established a laboratory pathway that uses readily available chemicals to produce molecules naturally found in guava plants. These molecules have been shown to combat aggressive liver cancers. The team’s results were published in Angewandte Chemie, a major international chemistry journal.

    Guava Fruit and Illustration of the Human Liver
    University of Delaware chemistry professor William Chain and his lab have invented a method for creating a liver cancer-fighting molecule found in guava plants using widely available chemicals. The discovery offers hope for low cost treatments against one of the world’s most deadly cancers. Credit: Jeffrey C. Chase

    This breakthrough gives scientists an efficient and inexpensive method for generating large quantities of these natural compounds. By making them more accessible, the approach could pave the way for cancer treatments that are both more effective and more affordable.

    William Chain
    William Chain. Credit: University of Delaware

    “The majority of clinically approved medicines are either made from a natural product or are based on one,” Chain said. “But there aren’t enough natural resources to make enough treatments. Now chemists will be able to take our manuscripts and basically follow our ‘recipe’ and they can make it themselves.”

    Collaboration and new pathways

    The discovery invites collaboration with scientists around the world.

    “We are the first ones to pave that road, and other people can repave it any which way. Find the shortcuts if they have to. But since we entered into that unknown territory, I think we helped shed light on this unknown pathway that can get us there. And I think that’s the cool part,” said Liam O’Grady, doctoral student in Chain’s lab and the article’s first author.

    The potential impact is enormous. The number of liver and bile duct cancer cases has grown dramatically in recent years, with one in 125 men and women globally projected to be diagnosed with hepatocellular cancer over the course of their lives.

    In the United States, chemotherapies for liver cancers are a multi-billion-dollar health burden and the current five-year survival rates for late-stage liver cancers are under 15%. In 2025, in the US alone, more than 42,000 people will be diagnosed and over 30,000 will lose their battle.

    The team is working with the National Cancer Institute on the next steps for the process and whether the guava molecule may be effective in fighting other types of cancers.

    Reference: “Enantioselective Total Synthesis of (–)-Psiguadial A” by Liam P. O’Grady, Marcel Achtenhagen, Michael F. Wisthoff, Robert S. Lewis, Katarina Pfeifer, Weifeng Zheng, Maxwell I. Martin, Glenn P. A. Yap and William J. Chain, 20 May 2025, Angewandte Chemie.
    DOI: 10.1002/ange.202506537

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  • Butterfly Nebula may rewrite what we know about Earth’s origins

    Butterfly Nebula may rewrite what we know about Earth’s origins

    When you think about Earth’s building blocks, your mind probably doesn’t jump to a giant space butterfly 3,400 light-years away. But scientists studying one of the galaxy’s most dramatic nebulae – the Butterfly Nebula – say it might offer real answers about how rocky planets like ours came to be.

    Thanks to the James Webb Space Telescope (JWST), researchers got the clearest look yet inside this strange, fiery structure. What they found were signs of dust – the kind that helped form Earth itself.

    Webb spots building blocks of planets


    Cosmic dust consists of minute mineral and organic debris suspended in space. It contains ingredients that probably took part in the beginning of life. Scientists weren’t entirely certain how it develops until now.

    The Webb Telescope directed its keen eyes toward the dense center of the Butterfly Nebula, an incredible wing-like cloud of gas and dust in the constellation Scorpius, far beyond Earth. Instead of seeing just one type of dust, scientists found two.

    “We were able to see both cool gemstones formed in calm, long-lasting zones and fiery grime created in violent, fast-moving parts of space, all within a single object,” said lead researcher Dr. Mikako Matsuura of Cardiff University.

    Most dust in space is messy and disorganized, like soot. But some forms perfect crystals – much more structured, like tiny gems. The nebula contains both, all in one place. This suggests that different kinds of cosmic environments can create very different types of dust, even right next to each other.

    “This discovery is a big step forward in understanding how the basic materials of planets, come together,” said Dr. Matsuura.

    A star hiding in plain sight

    The Butterfly Nebula’s bright, complex glow comes from a white-hot central star – one of the hottest of its kind, blazing at around 220,000 Kelvin (over 395,000°F).

    But the star itself has been hard to spot. It’s buried inside a thick, dusty ring of gas shaped like a doughnut, called a torus. That doughnut blocks visible light, making it impossible to see with regular telescopes.

    Webb’s Mid-Infrared Instrument (MIRI) employs a camera and a spectrograph that are capable of seeing through the dust. Using this technology, the researchers discovered the obscured star by identifying a glowing cloud of dust surrounding it, radiating in infrared wavelengths.

    This dusty torus is made of crystalline silicates like quartz, plus irregular grains about a millionth of a meter across – surprisingly large for cosmic dust. Their size and shape suggest they’ve been growing steadily for a long time.

    Fiery jets carve a cosmic butterfly

    Past the torus, things get more chaotic. The nebula’s shape is bipolar, meaning it has two giant lobes stretching in opposite directions like wings. A pair of high-speed jets shoot out from the center, traced by elements like iron and nickel.

    The new observations also uncovered layered shells of different atoms. Elements that need more energy to form cluster closer to the hot star, while others settle farther out. This paints a picture of a very organized – yet wild – environment.

    Another surprise came in the form of polycyclic aromatic hydrocarbons (PAHs). These carbon-based molecules are built like tiny rings and are found on Earth in things like car exhaust, smoke from campfires, and even burnt toast.

    The PAHs showed up in a place no one expected – inside an oxygen-rich planetary nebula. Usually, these kinds of molecules form in carbon-rich environments. Their presence here hints at a unique type of chemical reaction happening as fast winds from the central star slam into surrounding gas.

    The team suspects this may be the first evidence of PAHs forming under these conditions.

    Nebula chemistry reshapes rocky worlds

    Planetary nebulae – despite the name – are the final stages of medium-sized stars like our Sun. They form when those stars puff off their outer layers before cooling down into white dwarfs.

    That’s where many of the raw materials for future stars and planets are made. These nebulae might last only around 20,000 years – a blink in cosmic time – but during that period, they shape the chemistry of the galaxy.

    The Butterfly Nebula is one of the best-studied examples, previously imaged by the Hubble Space Telescope. But the James Webb Space Telescope goes deeper, letting scientists explore not just the shape of the nebula, but its internal chemistry.

    Using Webb’s detailed imaging along with radio data from the Atacama Large Millimeter/submillimeter Array, researchers found nearly 200 spectral lines – signals from different atoms and molecules. These signals showed how different chemicals are arranged in layers – revealing complex, nested structures.

    Butterfly Nebula reveals planet recipes

    The Butterfly Nebula’s beauty is just the surface. Underneath its glow lies a complicated process that turns dying stars into factories for dust and molecules – the very kind that can help form planets.

    “For years, scientists have debated how cosmic dust forms in space. But now, with the help of the powerful James Webb Space Telescope, we may finally have a clearer picture,” said Dr. Matsuura.

    With each new discovery, the question of how rocky worlds like Earth form becomes a little less mysterious – and a lot more exciting.

    The full study was published in the journal Monthly Notices of the Royal Astronomical Society.

    Image Credit: ESA/Webb, NASA & CSA, M. Matsuura, ALMA (ESO/NAOJ/NRAO), N. Hirano, M. Zamani (ESA/Webb)

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  • Scientists uncover ‘missing link’ in life’s origin chemistry

    Scientists uncover ‘missing link’ in life’s origin chemistry

    For decades, scientists have chased a mystery about how proteins’ building blocks first hooked up with RNA, the molecule carrying life’s code.

    Now, a team of chemists at University College London (UCL) has recreated this elusive step, showing how amino acids could have spontaneously attached to RNA under conditions thought to resemble those on the early Earth.

    Amino acids power the machinery of life by forming proteins, while RNA carries the instructions to build them.

    Yet how these two vital molecules first found each other has remained unsolved since researchers began probing the origins of life in the 1970s.

    Understanding origins of life

    “Life relies on the ability to synthesize proteins – they are life’s key functional molecules. Understanding the origin of protein synthesis is fundamental to understanding where life came from.

    Our study is a big step towards this goal, showing how RNA might have first come to control protein synthesis,” said Matthew Powner, senior author at UCL.

    In modern life, protein synthesis depends on an immensely complex molecular machine called the ribosome.

    It reads instructions carried in messenger RNA, which delivers a gene’s sequence from DNA to the ribosome.

    Acting like a factory assembly line, the ribosome then links amino acids together, one by one, to build a protein.

    “We have achieved the first part of that complex process, using very simple chemistry in water at neutral pH to link amino acids to RNA. The chemistry is spontaneous, selective and could have occurred on the early Earth,” Powner added.

    Thioesters and early chemistry

    Earlier efforts to attach amino acids to RNA had relied on highly reactive compounds that quickly degraded in water and caused amino acids to clump together rather than bind to RNA.

    The UCL team instead turned to a gentler activation method inspired by biology. They converted amino acids into a reactive form using thioesters, high-energy compounds vital in many of today’s biochemical processes and long hypothesized to have powered life’s first reactions.

    Powner noted that the findings unite two leading origin-of-life ideas: the “RNA world,” where RNA was the key self-replicator, and the “thioester world,” in which thioesters provided the energy for primitive metabolism.

    To make thioesters, amino acids were reacted with pantetheine, a sulfur-bearing molecule that the same group previously showed could form under early Earth-like conditions.

    That work suggested pantetheine may have been available in primordial ponds or lakes, providing the raw chemistry needed to kickstart life.

    The researchers say the next challenge is understanding how RNA could begin binding specific amino acids consistently, laying the foundation for the genetic code.

    “There are numerous problems to overcome before we can fully elucidate the origin of life, but the most challenging and exciting remains the origins of protein synthesis,” said Powner.

    Building life’s LEGO pieces

    Lead author Dr. Jyoti Singh likened the work to building with molecular LEGO bricks.

    “Imagine the day that chemists might take simple, small molecules, consisting of carbon, nitrogen, hydrogen, oxygen, and sulphur atoms, and from these LEGO pieces form molecules capable of self-replication. This would be a monumental step towards solving the question of life’s origin,” she said.

    The study showed that once amino acids were loaded onto RNA, they could link together to form peptides, the short chains of amino acids essential to life. Crucially, the activated amino acid used was a thioester derived from Coenzyme A, a molecule found in all living cells today. This discovery, the researchers suggest, could help connect early metabolism with the emergence of the genetic code and protein building.

    While the study focused on chemistry alone, the team believes such reactions were most likely to occur in shallow pools or lakes, where molecules could concentrate enough to interact.

    They tracked the microscopic reactions using advanced tools such as magnetic resonance imaging, which reveals atomic structures, and mass spectrometry, which identifies molecular sizes.

    The research was supported by the Engineering and Physical Sciences Research Council (EPSRC), the Simons Foundation, and the Royal Society.

    The findings have been published in the journal Nature.

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  • Deficiency of KMT2D causes autistic-like behavior in mice and zebrafish

    Deficiency of KMT2D causes autistic-like behavior in mice and zebrafish

    Disruption of KMT2D is associated with autism and other neurodevelopmental delay (NDD) phenotypes

    We assemble genotype and phenotype data for 9 affected individuals from 9 unrelated families with predicted deleterious variants in KMT2D through literature and two web-based databases (DECIPHER and ClinVar) (Table S1). This includes 5 individuals with de novo (n = 4) and transmitted (n = 1) truncating variants, 1 individual with missense variant, and three with unknown variants (Fig. 1A).

    Fig. 1: Deleterious variants in KMT2D and the phenotype frequencies.

    A Deleterious variants in ASD cohorts are depicted against a protein diagram for KMT2D. B The phenotype frequencies were calculated only among the patients with phenotypic information available.

    The probands were diagnosed with autism (100%, 9/9). Intelligence disability (100%, 8/8), dysmorphic facial features (100%, 7/7), cardiac anomaly (57.14%, 4/7), Speech delay (50%, 3/6), and hypotonia (50%, 3/6) were commonly co-occurred. In addition, clinodactyly of the fifth finger (42.86%, 3/7), motor delay (33.3%, 2/6), anxiety (33.3%, 2/6), joint laxity (33.3%, 2/6), hearing loss (28.57%, 2/7), feeding difficulties (28.57%, 2/7), hyperactivity (16.67%, 1/6), coordination difficulty (16.67%, 1/6), and sleep problems (16.67%, 1/6) are also observed in subsets of the patients (Fig. 1B and Table S2). In summary, a wide range of ASD or NDD phenotypes are present in probands with KMT2D mutation.

    Knockout of zebrafish kmt2d leads to developmental delay and autism-like behaviors

    To examine whether KMT2D plays an evolutionarily conserved role, we utilized zebrafish models. We targeted the gene using the CRISPR/Cas9 system and generated a -92 + 6 bp deletion allele for kmt2d, which introduces frame shifts and early truncations in the corresponding proteins (Fig. 2A). Additionally, we conducted sanger sequencing, agarose gel electrophoresis and RT-qPCR to confirm the knockout effect of kmt2d mutant (Fig. 2B, C; Figs. S1, S4). Specifically, we conducted heterozygous-by-heterozygous crosses for the −92 + 6 bp deletion alleles and screened for phenotypes, with particular emphasis on the organs and systems affected in patients with KS. The kmt2d−/− embryos exhibiting morphological abnormalities, including tail bending, yolk malformation, pericardial edema (Fig. 2D), and reduced body length at different developmental stages (Fig. 2F). RT-qPCR analysis confirmed that kmt2d mRNA expression was significantly reduced at three points in embryos with KS phenotypes (Fig. 2E). Our results indicated that the zebrafish kmt2d knockout line has been successfully established and can be utilized for further experiments.

    Fig. 2: kmt2d knockout zebrafish showed defects in social behaviors.
    figure 2

    AC Diagram of zebrafish kmt2d gene and mutation induced by CRISPR/Cas9, gray boxes indicate exons. A target site was on Exon 28 resulting in a 92-base deletion and 6-base insertion. B Sanger sequence. C results of agarose gel electrophoresis. D kmt2d−/− embryos exhibiting morphological abnormalities at the age of 24 h, 36 h and 72 h. E The expression levels of the Kmt2d gene decreased at three developmental point for embryos exhibiting KS phenotypes (Fifteen embryos per biological replicate were collected for zebrafish RT-qPCR, n = 3). F Body length was reduced in the kmt2d knockout zebrafish (n = 9). G Schematic diagram of the social preference behaviours experiment and motion trajectory chart for zebrafish. H Sniffing time exploring social region (n = 6 for wt, n = 7 for kmt2d-/+). I The distance traveled in the mating tank, which suggested that the kmt2d-/+ zebrafish had normal motor skill (n = 6 for wt, n = 7 for kmt2d−/+). Error bars represent as mean ± SD. *P  <  0.05, **P  <  0.01, ***P  <  0.001, ns: P > 0.05, Mann-Whitney U test.

    To investigate whether kmt2d haploinsufficiency leads to autistic-like behaviors in zebrafish as it does in human, we monitored the social behavior of kmt2d+/− male adult zebrafish (12 weeks of age), in which a single kmt2d allele is inactivated. Zebrafish are gregarious animals with a strong inclination toward social activity. Their social preference behavior served as indicators of their social tendencies. In our research, we examined how kmt2d+/− zebrafish interacted socially. In the social preference test, the kmt2d+/+ zebrafish consistently moved through the designated social zone throughout the trial, while the kmt2d+/− zebrafish exhibited aimless swimming patterns. The kmt2d+/− zebrafish exhibited notable differences in behavior compared to their kmt2d+/+ counterparts. Specifically, they spent significantly less time in the social zone (Fig. 2G, H). Despite maintaining typical motor skills (Fig. 2I), these kmt2d+/− zebrafish displayed a propensity for large circular movements, a repetitive behavior commonly observed in zebrafish and similar to behaviors seen in individuals with autism (Fig. 2G).

    Kmt2d deficiency mice showed defects in social behaviors and had repetitive behavior

    Using published single-cell RNA sequencing datasets16 (CNP0003837), we found that Kmt2d is widely expressed in different subregions of the hippocampus and in various types of neurons (Fig. S2A, B), and further confirmed the expression of KMT2D in the hippocampus via immunofluorescence experiments (Fig. S2C). To elucidate the relationship between the function of KMT2D in the hippocampus and autism-like behaviors, we selectively knocked down the Kmt2d gene in the hippocampal region of mice and examined its impact on their social behavior. We firstly screened for effective RNA interference (RNAi) fragments targeting Kmt2d in mouse HT22 cells (Figs. S3A–C; S5B, C). Then, adeno-associated virus (AAV) vectors carrying Kmt2d-shRNA (AAV-RNAi) or control-shRNA (AAV-nc) were injected into the hippocampus, respectively. After a four-week post-injection period, we analyzed sections of mouse brain tissue under a fluorescence microscope and observed positive GFP expression specifically in the hippocampal region (Fig. 3A). The results of RT-qPCR demonstrated that the expression level of the kmt2d gene was significantly reduced in the AAV-RNAi group compared to the AAV-nc control group (Fig. 3B). Given that KMT2D functions as a histone methyltransferase responsible for catalyzing the formation of H3K4me3, it is not surprising that the H3K4me3 levels were also decreased in the hippocampus of mice with kmt2d knockdown (Figs. 3C, D; S5A). These results indicate that we have successfully established a mouse model with hippocampal-specific knockdown of kmt2d.

    Fig. 3: Kmt2d deficiency mice showed defects in social behaviors and had repetitive behavior.
    figure 3

    A The adeno-associated virus (AAV) vectors carrying Kmt2d-shRNA (AAV-RNAi) or control-shRNA was delivered to the hippocampal. B The results of RT-qPCR showed a significantly reduced of kmt2d in the AAV-RNAi group compared to that of AAV-nc group (n = 3). C, D The level of the H3K4me3 protein. The band density was quantified and expressed as the relative gray value (compared with the control) by arbitrarily setting the control value as 1 (n = 3). E Schematic diagram of the three-box social experiment. F The distance traveled in different areas within the open field for the mice (n = 6). G Motion trajectory chart for the control (AAV-nc) and knockdown (AAV-RNAi) mice in an Open Field Assay. H Number of marbles buried (n = 6). I, J During a social interaction session, Kmt2d deficiency mice didn’t have social preferences. I sniffing time exploring S1 and E (n = 6). J motion trajectory chart for the control (AAV-nc) and knockdown (AAV-RNAi) mice. K, L The same as (I, J) but for social novelty test. K sniffing time exploring S1 and S2. (n = 6). L motion trajectory chart. Error bars represent as mean ± SD. *P  <  0.05, **P  <  0.01, ***P  <  0.001, ns: P > 0.05, Mann-Whitney U test. A Created with BioRender.com, released under a Creative Commons Attribution-NonCommercial-NoDerivs 4.0 International license.

    We assessed social behaviors in adult mice using the three-chamber sociability and social novelty tests (Fig. 3E). Control mice (AAV-nc) typically preferred social stimuli and spent more time with novel mice. In contrast, Kmt2d deficiency mice (AAV-RNAi) showed no preference for social stimuli or novel mice (Fig. 3I–L). Motor skills were normal in Kmt2d deficiency mice (Fig. 3F, G). Additionally, Kmt2d deficiency mice exhibited increased repetitive behaviors, burying more marbles than controls in the Marble Burying Test (Fig. 3H). Thus, Kmt2d deficiency mice displayed abnormal social behaviors and increased repetitive behaviors.

    Knockdown of Kmt2d decreased excitatory and increased inhibitory synaptic transmission

    To elucidate the neural mechanisms underlying the observed phenotypes, we further examined how the Kmt2d gene in the rat hippocampus influences the excitatory-inhibitory (E/I) balance—a key pathophysiological mechanism implicated in autism17. Rat hippocampal slice cultures are widely used in neurophysiological studies due to their larger hippocampal structure compared to mice, which facilitates higher success rates for slice culture and easier acquisition of stable synaptic activity signals. This allows for more accurate assessment of the impact of Kmt2d knockdown on synaptic function. For these experiments we used slice cultures from 8-to 10-day-old rats. We had screened for effective RNA interference fragments targeting Kmt2d in rat B104 cells (Fig. S3D, E) first. Then, Kmt2d knockdown was performed by an AAV vector containing Kmt2d-shRNA-eGFP infusion.

    Based on published single-cell data, we found that the expression level of kmt2d do not significantly differ among different subregions of the hippocampus (Fig. S2A). Therefore, we hypothesize that knockdown of Kmt2d may alter synaptic function in both the CA1 and DG regions. We performed paired recordings from a transfected cells and a neighboring control cell in CA1 and DG, with synaptic responses evoked by electrical stimulation of the Schaffer collateral pathway (Fig. 4A). Our results revealed the following: First, analysis of IPSCs in kmt2d knockdown neurons from the CA1 region revealed a significant increase in amplitude compared to control neurons (Fig. 4C). Second, knockdown of kmt2d decreased the amplitude of AMPAR -mediated EPSCs in CA1 neurons but did not significantly affect NMDAR-mediated EPSCs (Fig. 4E). Finally, we observed similar changes in IPSCs and EPSCs in the DG region, consistent with the findings in the CA1 region (Fig. 4D, F). These data indicate that knockdown of KMT2D leads to functional defects in synaptic transmission, resulting in an imbalance between excitation and inhibition.

    Fig. 4: Knockdown of Kmt2d decreased excitatory and increased inhibitory synaptic transmission.
    figure 4

    A Schematic diagram of hippocamcal cultured slice and dual whole-cell patch clamp. B Paired recordings from Kmt2d-shRNA-eGFP infection (bright cell) and control cell. C, D The amplitude of IPSCs in infected cells is increased compared to control cells in CA1 and DG regions, respectively (n = 10 for CA1 region; n = 9 for DG region). E, G The amplitude of AMPA receptor-mediated EPSCs in infected cells is decreased compared to control cells in CA1 and DG regions, respectively (n = 10 for CA1 region; n = 11 for DG region). F, H The amplitude of NMDA receptor-mediated EPSCs in infected cells remained unchanged compared to control cells in CA1 and DG regions, respectively (n = 9 for CA1 region; n = 11 for DG region). Error bars represent as mean ± SD. *P  <  0.05, **P  <  0.01, Mann-Whitney U test. A Created with BioRender.com, released under a Creative Commons Attribution-NonCommercial-NoDerivs 4.0 International license.

    KMT2D regulates downstream target genes related to synaptic response

    To further explore the molecular mechanisms by which KMT2D regulates autistic-like behaviors, we used RNA-seq to compare the gene expression profiles from whole 3-dpf zebrafish exhibiting KS phenotypes (Fig. 5A). A volcano plot graphically illustrates the distribution of differentially expressed genes (DEGs), revealing that 892 genes were downregulated and 617 genes were upregulated transcriptionally in the mutant zebrafish model (Fig. 5B; Supplementary Data 2). Analyses of Gene Ontology (GO) analysis showed that the DEGs were significantly enriched in glutamatergic and GABAergic pathways (Fig. 5C; Supplementary Data 2). To delve deeper into the regulatory mechanisms of KMT2D on synaptic function, we observed that multiple genes (shank2, cnksr1, csmd2 and srgap3) in the glutamatergic signaling pathway were downregulated, whereas genes (camk4, gabarabp, gabarapl2 and npas4a) in the GABAergic signaling pathway were upregulated (Fig. 5D). These findings were further corroborated by subsequent qPCR validation (Fig. 5E, F).

    Fig. 5: KMT2D regulates downstream target genes related to synaptic response.
    figure 5

    A RNA-seq analysis of zebrafish and mice samples. B Volcano plot showing differentially expressed genes (DEGs) in the km2d+/+ and kmt2d−/− zebrafish. C GO analysis of DEGs in the km2d+/+ and kmt2d−/− zebrafish. DF Differentially expressed genes associated with glutamatergic and GABAergic synapse in the km2d+/+ and kmt2d−/− zebrafish. D Heatmap of 4 upregulated genes associated with GABAergic synapse, and 6 downregulated genes associated glutamatergic synapse. C RT-qPCR of shank2b (n = 3); D RT-qPCR of gabarapb (n = 3). G Volcano plot showing DEGs in the Km2d-KD and control mice hippocampus. H GO analysis of DEGs in the Km2d-KD and control mice hippocampus. IK Differentially expressed genes associated with glutamatergic and GABAergic synapse in the Km2d-KD and control mice. I Heatmap of 6 upregulated genes associated with GABAergic synapse, and 6 downregulated genes associated glutamatergic synapse. C RT-qPCR of Cnksr1 (n = 3); D RT-qPCR of Fgf7 (n = 3). Error bars represent as mean ± SD. *P  <  0.05, **P  <  0.01, Mann-Whitney U test. Mice of Fig. 5, created with BioRender.com, released under a Creative Commons Attribution-NonCommercial-NoDerivs 4.0 International license.

    When we compared the gene expression profiles of kmt2d+/+ and kmt2d−/− zebrafish, we made consistent observations of those made in hippocampus of Kmt2d-KD mice. A total of 996 DEGs were identified, including 469 downregulated genes and 527 upregulated genes (Fig. 5G; Supplementary Data 4). DEGs are significantly enriched in pathways related to glutamatergic and GABAergic function (Fig. 5H; Supplementary Data 5). In Kmt2d-KD mice, multiple genes associated with the glutamatergic signaling pathway, such as shank2, cnksr1, csmd2 and srgap3 are significantly downregulated, while several genes related to the GABAergic signaling pathway, including fgf7, gata3, syt1 and plcl1 are significantly upregulated (Fig. 5I–K). Interestingly, several genes in the glutamatergic signaling pathway, such as shank2, cnksr1, csmd2, srgap3, rap1gab and sipal1l, showed consistent changes in both Kmt2d-KD mice and kmt2d-KO zebrafish models (Fig. 5D, I). This finding suggests that the change of glutamatergic synapse is conserved across these two distinct species models. Totally, RNA-seq analysis revealed that under conditions of low kmt2d expression, differentially expressed genes were associated with glutamatergic and GABAergic synapses, supporting the dysregulation of E-I balance in the hippocampus.

    The KMT2D network links the glutamatergic and GABAergic synaptic responses in ASD

    A better understanding of the connections between KMT2D downstream genes and ASD-associated genes will help to more effectively link KMT2D to autism-like behaviors. By surveying 996 genes that were differentially expressed in the hypothalamus of Kmt2d-KD and control mice, we found that 61 genes were associated with ASD, 223 were related to glutamatergic synaptic responses, and 47 were related to GABAergic synaptic responses (Fig. 6A, B; Supplementary Data 6). As shown in Fig. 6C, the disrupted glutamatergic synaptic responses was one of the major causes of Kmt2d-deficiency-associated ASD (Fig. 6C; Supplementary Data 6).

    Fig. 6: KMT2D connects glutamatergic and GABAergic synaptic signaling pathways with ASD.
    figure 6

    A Venn-diagram showing the overlap genes between four different gene sets: DEGs: the differentially expressed genes detected in Kmt2d-KD mice RNA-seq. Glutamatergic genes: the DEGs associated with glutamatergic synaptic response. GABAergic genes: the DEGs associated with GABAergic synaptic response. ASD genes: the genes related with ASD based on SFARI. B The ratio of DEGs associated with ASD, glutamatergic and GABAergic synaptic signaling pathway. C Conduct visualization of DEGs related to the glutamatergic and GABAergic signaling pathways using the cluGO software. D The network representing protein interaction relationship between DEGs in ASD, glutamatergic and GABAergic signaling pathways based on Kmt2d-KD mice RNA-seq.

    To further illustrate the connection among KMT2D-regulated genes, we studied a network of 118 DEGs that were involved in ASD, glutamatergic and GABAergic synaptic response, using the STRING database (Fig. 6D; Supplementary Data 7). The resulting network suggested that KMT2D regulated GABAergic synaptic response via ZFPM1, whose abnormal expressions and/or mutations have been associated with ASD and other neurological disorders18,19. We found that 16 genes, including Shank2, Syt1, Ar, Tek, P2rx7, Styk1, and Rheb were ASD genes that were involved in the glutamatergic synaptic response. The network also illustrated 4 ASD genes that were associated with the GABAergic synaptic response, including Mink1, Cacna1i, Adora2a and Hivep3. Specifically, Mink1, Cacna1i, Adora2a was found to be a common gene shared by the glutamatergic synaptic response. Overall, our network further illustrates that Kmt2d deficiency increases the risk of ASD by disrupting the glutamatergic and GABAergic synaptic responses.

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  • Proteomic study reveals new drug targets in gastric signet ring cell carcinoma

    Proteomic study reveals new drug targets in gastric signet ring cell carcinoma

    Gastric signet ring cell carcinoma (GSRCC) is a distinct subtype of gastric cancer (GC) with unique epidemiological and pathogenic characteristics. Despite its clinical significance, large-scale proteomic studies on GSRCC remain scarce, limiting our molecular understanding of the disease. Advanced mass spectrometry (MS)-based proteomics is crucial for identifying key biomarkers and drug targets, thereby enabling more effective therapeutic strategies.

    In a recent study published in Genes & Diseases, researchers from several institutions, including Tianjin University, Chinese Academy of Sciences, Zhejiang Cancer Hospital, Fudan University, Diagnosis and Therapy of Upper Gastrointestinal Cancer of Zhejiang Province, Chinese Academy of Medical Sciences and Peking Union Medical College, and University of Houston, characterizes the proteomic features and molecular mechanisms of GSRCC to date.

    Initially, the research team analyzed clinical data from over 10,000 patients with GC between January 2010 and December 2019. An in-depth proteomic analysis was conducted on tumor tissues from 112 GSRCC patients, each with over 70% signet ring cell content. Using advanced MS, the team identified 7322 proteins, establishing the largest tissue-specific peptide spectral library for GSRCC. Additionally, through unsupervised clustering, the team identified four novel proteomic subtypes of GSRCC: Metabolism (S-Mb), Microenvironment Dysregulation (S-Me), Migration (S-M) and Proliferation (S-PF).

    Two key prognostic biomarkers were identified and validated in an independent cohort of 75 patients: PRDX2, a protein associated with favorable prognosis; and DDX27, linked to poor survival outcomes. Furthermore, proteomic profiling of 79 biomarker-negative GSRCC cases revealed marked tumor heterogeneity. Notably, unsupervised clustering identified three distinct proteomic clusters, with cluster 2 linked to the poorest prognosis.

    Focusing on HER2-negative, EBV-negative, and pMMR GSRCC cases (LMT [Lack of Medical Treatment]-GSRCC), the study identified four potential drug targets: eukaryotic translation initiation factor 2 subunit gamma (EIF2S3), eukaryotic translation initiation factor 6 (EIF6), and nuclear factor kappa B subunit 2 (NFKB2). Remarkably, high expression of these proteins was associated with poor prognosis, underscoring their relevance as promising therapeutic candidates.

    Interestingly, molecular docking and cytotoxicity testing singled out neratinib-a drug approved for breast cancer treatment-as the most promising candidate. Furthermore, in vitro and in vivo studies demonstrated neratinib’s potent ability to inhibit tumor growth, cell migration, and invasion, while promoting cancer cell apoptosis, all with minimal side effects.

    In conclusion, this is the first study to focus specifically on the LMT-GSRCC population, uncovering potential biomarkers and drug targets through proteomic analysis. The findings from this study not only provide a foundation for developing novel targeted therapies but also personalized treatment strategies for GSRCC.

    Source:

    Journal reference:

    Jin, Z., et al. (2025). A comprehensive proteomic analysis uncovers novel molecular subtypes of gastric signet ring cell carcinoma: Identification of potential prognostic biomarkers and therapeutic targets. Genes & Diseases. doi.org/10.1016/j.gendis.2025.101717

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  • KMT-2018-BLG-0029Lb and OGLE-2019-BLG-0960Lb: Mass Measurements for Two Super-Earth Microlensing Planets

    KMT-2018-BLG-0029Lb and OGLE-2019-BLG-0960Lb: Mass Measurements for Two Super-Earth Microlensing Planets

    Keck NIRC2-LGS images of the two events. North is up and East is to the left. The green and red boxes indicate the target and comparison stars, respectively. Insets show zoomed-in views of each star, including the original image and the residuals following PSF subtraction, which are shown on the identical flux scale to facilitate comparison. The gray dotted circles in the residual images show the predicted lens-source separation. — astro-ph.EP

    KMT-2018-BLG-0029Lb and OGLE-2019-BLG-0960Lb were the lowest mass-ratio microlensing planets at the time of discovery. For both events, microlensing parallax measurements from the Spitzer Space Telescope implied lens systems that were more distant and massive than those inferred from the ground-based parallax.

    Here, we report on the detection of excess flux aligned to the event locations using Keck Adaptive Optics imaging, which is consistent with the expected brightness of main-sequence hosts under the ground-based parallax, but inconsistent with that predicted by Spitzer.

    Based on the excess flux, ground-based parallax, and angular Einstein radius, we determine KMT-2018-BLG-0029Lb to be a 4.2±0.5M planet orbiting a 0.70±0.07M host at a projected separation of 3.1±0.3 au, and OGLE-2019-BLG-0960Lb to be a 2.0±0.2M planet orbiting a 0.40±0.03M host at a projected separation of 1.7±0.1 au. We report on additional light-curve models for KMT-2018-BLG-0029 under the generalized inner-outer (offset) degeneracy, which were not reported in the original analysis.

    We point out inconsistencies in the inner/outer labeling of the degenerate models in the lens and source planes, and advocate for the lens-plane convention, which refers to the planet being closer or further to the host star compared to the image it perturbs. Lastly, we discuss the possibility of breaking this degeneracy via ground concurrent observations with the Roman Space Telescope.

    Keming Zhang, Sean K. Terry, Joshua S. Bloom, B. Scott Gaudi, Jessica R. Lu

    Comments: 11 pages, 5 figures, 2 tables. Accepted to the Astronomical Journal
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Astrophysics of Galaxies (astro-ph.GA)
    Cite as: arXiv:2508.18343 [astro-ph.EP] (or arXiv:2508.18343v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2508.18343
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    Submission history
    From: Keming Zhang
    [v1] Mon, 25 Aug 2025 18:00:00 UTC (4,984 KB)
    https://arxiv.org/abs/2508.18343

    Astrobiology

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • VLT/MUSE Detection Of The AB Aurigae b Protoplanet With Ha Spectroscopy

    VLT/MUSE Detection Of The AB Aurigae b Protoplanet With Ha Spectroscopy

    TOP: Other MUSE reductions showing the detection of AB Aur b from OB4. (left, middle) 6558.88 Aand 6560.13 Afrom the reduction shown in Figure 1. Average of the 6558.88 Aand 6560.13 Aslices from a classical SDI reduction (right). In each panel, we mask the field out to a separation affected by horizontal striping and saturation BOTTWO: Detection of AB Aur b from OB2 (left, middle panels) and weaker detection from OB1 in blue-shifted Hα (right). — astro-ph.EP

    We analyze high-contrast, medium-spectral-resolution Hα observations of the star AB Aurigae using the Very Large Telescope’s Multi Unit Spectroscopic Explorer (MUSE).

    In multiple epochs, MUSE detects the AB Aur b protoplanet discovered from Subaru/SCExAO data in emission at wavelengths slightly blue-shifted from the Hα line center (i.e. at 6558.88–6560.13 Å; ∼ -100 km s−1) and in absorption at redshifted wavelengths (6562.8–6565.1 Å; ∼ 75 km s−1).

    AB Aur b’s Hα spectrum is inconsistent with that of the host star or the average residual disk spectrum and is dissimilar to that of PDS 70 b and c. Instead, the spectrum’s shape resembles that of an inverse P Cygni profile seen in some accreting T Tauri stars and interpreted as evidence of infalling cold gas from accretion, although we cannot formally rule out all other nonaccretion origins for AB Aur b’s MUSE detection.

    AB Aurigae hosts only the second protoplanetary system detected in Hα thus far and the first with a source showing a spectrum resembling an inverse P Cygni profile. Future modeling and new optical data will be needed to assess how much of AB Aur b’s emission source(s) originates from protoplanet accretion reprocessed by the disk, a localized scattered-light feature with a unique Hα profile, or another mechanism.

    Thayne Currie, Jun Hashimoto, Yuhiko Aoyama, Ruobing Dong, Misato Fukagawa, Takayuki Muto, Erica Dykes, Mona El Morsy, Motohide Tamura

    Comments: 23 pages, 16 figures, 3 tables; ApJ Letters in press
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM)
    Cite as: arXiv:2508.18351 [astro-ph.EP] (or arXiv:2508.18351v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2508.18351
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    From: Thayne Currie
    [v1] Mon, 25 Aug 2025 18:00:02 UTC (1,915 KB)
    https://arxiv.org/abs/2508.18351

    Astrobiology

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • The Mid-infrared Spectrum Of Beta Pictoris b. First VLTI/MATISSE Interferometric Observations Of An Exoplanet

    The Mid-infrared Spectrum Of Beta Pictoris b. First VLTI/MATISSE Interferometric Observations Of An Exoplanet

    Detection maps of β Pic b with MATISSE. The maps show the reduced χ2 values after fitting the stellar contamination for each tested planet astrometry (∆α, ∆δ) in the grid. The grids are centered on MATISSE’s pointing during the planet observations. The left map is the size of the pinhole (1.5λ/D at 3.5 µm) and has a resolution of 1 mas. The right map was generated at higher resolution (0.1 mas) on a smaller 20×20 mas grid. The most likely astrometry from the MATISSE observations is shown as a blue ellipse, found by fitting a 2D Gaussian curve on the lowest χ2r peak. The planet location and uncertainties predicted by whereistheplanet from the orbital fitting of GRAVITY observations (Lacour et al. 2021) are shown as a green ellipse. The multiplicity of χ2r peaks is due to the interferometric nature of our data. As coherent flux is periodic as a function of α. ⃗ ⃗u (see Eq. (7)), an infinity of astrometric solutions can reproduce the signal. This degeneracy gradually disappears when combining data from different baseline lengths and orientations. The χ2r of neighbour peaks can nonetheless still remain close. Using covariances between baselines and wavelengths could help increase the difference between peaks, and will be studied in a future work. — astro-ph.EP

    Few spectra of directly-imaged exoplanets have been obtained in the mid-infrared (> 3 μm). This region is particularly rich in molecular spectral signatures, whose measurements can help recover atmospheric parameters and provide a better understanding of giant planet formation and atmospheric dynamics.

    In the past years, exoplanet interferometry with the VLTI/GRAVITY instrument has provided medium-resolution spectra of a dozen substellar companions in the near infrared. The 100-meter interferometric baselines allow for the stellar and planetary signals to be efficiently disentangled at close angular separations (< 0.3”).

    We aim to extend this technique to the mid-infrared using MATISSE, the VLTI’s mid-infrared spectro-interferometer. We take advantage of the fringe tracking and off-axis pointing capabilities recently brought by the GRA4MAT upgrade. Using this new mode, we observed the giant planet β Pictoris b in L and M bands (2.75-5 μm) at a spectral resolution of 500.

    We developed a method to correct chromatic dispersion and non-common paths effects in the fringe phase and modelled the planet astrometry and stellar contamination. We obtained a high-signal-to-noise spectrum of β Pictoris b, showing the planet continuum in L (for the first time) and M bands, which contains broad absorption features of H2O and CO.

    In conjunction with a new GRAVITY spectrum, we modelled it with the ForMoSA nested sampling tool and the Exo-REM grid of atmospheric models, and found a solar carbon-to-oxygen ratio in the planet atmosphere.

    This study opens the way to the characterization of fainter and closer-in planets with MATISSE, which could complement the JWST at angular separations too close for it to obtain exoplanet spectra. Starting in 2025, the new adaptive optics system brought by the GRAVITY+ upgrade will further extend the detection limits of MATISSE.

    M. Houllé, F. Millour, P. Berio, J. Scigliuto, S. Lacour, B. Lopez, F. Allouche, J.-C. Augereau, D. Blain, M. Bonnefoy, M. Carbillet, G. Chauvin, J. Leftley, A. Matter, J. Milli, P. Mollière, E. Nasedkin, M. Nowak, P. Palma-Bifani, É. Pantin, P. Priolet, M. Ravet, J. Woillez, W. Balmer, P. Boley, V. Gámez Rosas, J. H. Girard, X. Haubois, S. Hinkley, M. Hogerheijde, W. Jaffe, J. Kammerer, L. Kreidberg, O. Lai, S. Lagarde, A. Labdon, J.-B. Le Bouquin, A. Meilland, A. Mérand, C. Paladini, R. Petrov, E. Rickman, Th. Rivinius, S. Robbe-Dubois, R. van Boekel, J. Varga, A. Vigan, J. J. Wang, G. Weigelt

    Comments: 21 pages, 17 figures. Accepted for publication in A&A
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM)
    Cite as: arXiv:2508.18366 [astro-ph.EP] (or arXiv:2508.18366v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2508.18366
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    From: Mathis Houllé
    [v1] Mon, 25 Aug 2025 18:00:11 UTC (4,268 KB)
    https://arxiv.org/abs/2508.18366

    Astrobiology

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  • Scientists Leaving Elon Musk’s X are Driving Growth on Bluesky: Study

    Scientists Leaving Elon Musk’s X are Driving Growth on Bluesky: Study

    Bluesky now has more than 38 million users. Matteo Della Torre/NurPhoto via Getty Images

    Bluesky is increasingly emerging as a rival to X, and nowhere is that more evident than in the platform’s burgeoning scientific research community. According to a new study, Bluesky boasts higher interactive engagement and content originality for scholarly posts than X.

    The research, conducted by the University of Sheffield in England and the Renmin University of China, claims to be the first large-scale analysis of scientific communication on Bluesky. The study—still awaiting peer review—found that scholarly activity on the platform has surged since November 2024, coinciding with a broader migration away from X toward alternative social media sites.

    Bluesky was created in 2019, initially incubated under Twitter and became independent in 2021. Officially launching in 2023 under CEO Jay Graber, the platform has since grown to more than 38 million users. While its interface looks strikingly similar to X, Bluesky differentiates itself with a decentralized, open-source network that gives users more control and personalization.

    The study analyzed more than 2.6 million Bluesky posts referencing scholarly content between January 2023 and July 2025. It found that posts, users and referenced articles have all been on an upward trajectory. In October 2024, for example, there were around 10,000 posts, 3,200 users and 6,500 referenced articles. By November, those figures had surged to 239,000, 35,000 and 54,000. They peaked in January of this year at 324,000 posts by 45,000 users referencing 71,000 unique articles.

    Activity has since stabilized, with a slight decline. “The stabilization of posts, users and referenced articles suggests that Bluesky has already established itself as a credible and lasting platform for science communication, rather than a short-lived trend,” Er-Te Zheng, one of the study’s authors and a Ph.D. student at the University of Sheffield, told Observer via email.

    Bluesky’s growth comes amid an exodus of X users dissatisfied with Musk’s leadership and changes such as loosened content moderation. A January poll by Nature found that more than half of 5,300 respondents—most of them scientists—said they had left X.

    Those who have turned to Bluesky are showing higher levels of engagement. More than 48 percent of scholarly posts received at least 10 likes, while 34 percent were reposted at least 10 times. By contrast, previous research on X found that only 3.9 percent to 7.5 percent of scientific research posts received more than 10 likes, and just 1.4 percent to 4.4 percent received 10 reposts or more.

    Bluesky also fosters more original content, as shown in the low number of posts that simply replicate a research paper’s title, the study found. Only 6.3 percent of the analyzed Bluesky posts contained nothing more than an article title. On X, title replication rates have been shown to range anywhere from 11. 8 percent to 92.4 percent, depending on various scientific disciplines.

    Bluesky still pales in size compared to X, which Elon Musk claimed had around 600 million monthly active users as of May 2024. But the platform’s high levels of engagement and originality suggest it’s carving out a distinct niche. “This suggests that Bluesky users participate more actively and with greater originality in interactions around scholarly articles,” Zheng said.

    Scientists Leaving Elon Musk’s X are Driving Growth on Bluesky: Study


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