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Showing 1–50 of 10983 results
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  • A 10-Earth-mass planet is detected in the habitable zone of the solar-type star Kepler-725 using the transit timing variation technique. This study proposes a complementary pathway to probe low-mass exoplanets (including Earth-like planets) in the habitable zones of Sun-like stars.

    • L. Sun
    • S. Gu
    • G. Zhao
    Research
    Nature Astronomy
    Volume: 9, P: 1184-1194
  • The study introduces radio interferometric multiplexed spectroscopy (RIMS), a method designed to efficiently monitor the radio emissions of massive samples of stars. Applying it to LOFAR data, the authors identify stellar bursts, offering clues to possible star–planet magnetic interactions.

    • Cyril Tasse
    • Philippe Zarka
    • Xiang Zhang
    Research
    Nature Astronomy
    P: 1-10
  • The Parker Solar Probe mission has reached the inner heliosphere of the Sun and made measurements of energetic particle events in the near-Sun radiation environment.

    • D. J. McComas
    • E. R. Christian
    • A. P. Rouillard
    Research
    Nature
    Volume: 576, P: 223-227
  • Aadvanced computer simulations of three-dimensional turbulence reveal that the ab initio generation of large-scale magnetic fields is driven by shear-flow-induced jets; an analytical model is derived which reproduces the essential features of the flow- and field-generation mechanisms.

    • B. Tripathi
    • A. E. Fraser
    • R. Fan
    Research
    Nature
    Volume: 649, P: 848-852
  • Muscularis macrophages, housekeepers of enteric nervous system integrity and intestinal homeostasis, modulate α-synuclein pathology and neurodegeneration in models of Parkinson’s disease, and understanding the accompanying mechanisms could pave the way for early-stage biomarkers.

    • Sebastiaan De Schepper
    • Viktoras Konstantellos
    • Tim Bartels
    ResearchOpen Access
    Nature
    P: 1-11
  • Splitting water using sunlight is a promising route to green hydrogen, yet inefficient charge carrier utilization in photocatalysts limits their solar-to-hydrogen efficiency. Here the authors introduce excitonic quantum superlattices to prolong exciton lifetimes and optimize charge steering, achieving a solar-to-hydrogen efficiency of 3% under ambient conditions.

    • Yuyang Pan
    • Bingxing Zhang
    • Zetian Mi
    Research
    Nature Energy
    P: 1-10
  • SOHO has provided a high-quality, continuous record of the Sun and its atmosphere. Marking the thirtieth anniversary since SOHO’s launch, this Review highlights its legacy, shaping our understanding of the Sun, and the new space missions it has inspired.

    • Daniel Müller
    • Jack Ireland
    • Bernhard Fleck
    Reviews
    Nature Astronomy
    Volume: 10, P: 24-33
  • Rapidly growing satellite constellations pose a substantial threat to astronomical observations, with projections indicating that future space telescopes will have more than 96% of their exposures affected by satellite trails, necessitating urgent mitigation strategies.

    • Alejandro S. Borlaff
    • Pamela M. Marcum
    • Steve B. Howell
    ResearchOpen Access
    Nature
    Volume: 648, P: 51-57
  • The Huayuan biota exhibits extraordinary biodiversity, illuminating the impact of the Phanerozoic mass extinction around 513 million years ago and offering critical insights into the transformation of global ecosystems in the early Cambrian.

    • Han Zeng
    • Qi Liu
    • Maoyan Zhu
    Research
    Nature
    P: 1-9
  • Large-effect variants in autism remain elusive. Here, the authors use long-read sequencing to assemble phased genomes for 189 individuals, identifying pathogenic variants in TBL1XR1, MECP2, and SYNGAP1, plus nine candidate structural variants missed by short-read methods.

    • Yang Sui
    • Jiadong Lin
    • Evan E. Eichler
    ResearchOpen Access
    Nature Communications
    P: 1-16
  • High-resolution solar flare observations captured rapid brightening in the Sun’s lower atmosphere. Their speeds of thousands of kilometres per second provide a missing piece of evidence for magnetic reconnection in three dimensions.

    • Juraj Lörinčík
    • Jaroslav Dudík
    • Bart De Pontieu
    ResearchOpen Access
    Nature Astronomy
    Volume: 9, P: 45-54
  • Here, the authors develop AMPLiT a tool for screening antimicrobial peptides in metagenomic datasets, and apply it to human coprolite metagenomes, finding that Segatella copri, an ancient prevalent human gut bacterium declined in modern populations, harbors unexplored antimicrobial reservoir, offering an alternative approach against modern pathogenic infections.

    • Sizhe Chen
    • Yue Yuan
    • Qi Su
    ResearchOpen Access
    Nature Communications
    P: 1-12
  • Native state proteomics of PV interneurons revealed unique molecular features of high translational and metabolic activity, and enrichment of Alzheimer’s risk genes. Early amyloid pathology exerted unique effects on mitochondria, mTOR signaling and neurotransmission in PV neurons.

    • Prateek Kumar
    • Annie M. Goettemoeller
    • Srikant Rangaraju
    ResearchOpen Access
    Nature Communications
    Volume: 15, P: 1-26
  • JWST’s COSMOS-Web survey is used to create an ultra-high-detail dark matter map, revealing hidden filaments, clusters and distant structures. By tracing features out to z = 2, this map shows how dark and luminous matter build the cosmic web across cosmic time.

    • Diana Scognamiglio
    • Gavin Leroy
    • John R. Weaver
    Research
    Nature Astronomy
    P: 1-10
  • A long-duration campaign to image the Sun’s middle corona—a region about 1.5–3 solar radii from the centre—reveals three dynamical processes that shape and restructure the middle corona. The dynamics can influence the global coronal structure and beyond.

    • Daniel B. Seaton
    • J. Marcus Hughes
    • Gregory Slater
    Research
    Nature Astronomy
    Volume: 5, P: 1029-1035
  • Identifying jets originating from heavy quarks plays a fundamental role in hadronic collider experiments. In this work, the ATLAS Collaboration describes and tests a transformer-based neural network architecture for jet flavour tagging based on low-level input and physics-inspired constraints.

    • G. Aad
    • E. Aakvaag
    • L. Zwalinski
    ResearchOpen Access
    Nature Communications
    Volume: 17, P: 1-22
  • A full understanding of the heating and dynamics of the Sun's atmosphere remains elusive, but magnetohydrodynamic waves are believed to be crucial. Using observations from the ROSA imager, this study finds compressive waves in the solar chromosphere, which may provide the energy needed for coronal heating.

    • Richard J. Morton
    • Gary Verth
    • Robertus Erdélyi
    Research
    Nature Communications
    Volume: 3, P: 1-8
  • The formation of glycylglycine, a simple peptide molecule, is possible under non-aqueous interstellar conditions, according to laboratory experiments. Thus, complex organics with biological relevance may predate planetary accretion.

    • Alfred Thomas Hopkinson
    • Ann Mary Wilson
    • Sergio Ioppolo
    Research
    Nature Astronomy
    P: 1-9
  • The authors consider the changing sensitivity of the leaf-onset date to temperature (ST) for boreal deciduous broadleaf forests. ST increased between 1982–1996 and 1998–2012—potentially linked to enhanced chilling accumulation—but this increase is underestimated in phenology models.

    • Wenyu Li
    • Hui Lu
    • Peng Gong
    Research
    Nature Climate Change
    P: 1-7
  • The inclusion of magnetohydrodynamic instabilities in the transport of both angular momentum and material within the Sun can simultaneously explain the internal rotation regime of the Sun, its surficial lithium abundance and the helium abundance in the envelope, which were inconsistent with the predictions of previous standard solar models.

    • P. Eggenberger
    • G. Buldgen
    • M. Asplund
    Research
    Nature Astronomy
    Volume: 6, P: 788-795
  • Here, the authors show learning tasks with similar structures can initially cause interference and slow down learning, but both the brain and artificial networks gradually reorganize information over time, enabling them to perform better and adapt more efficiently.

    • Nicholas Menghi
    • W. Jeffrey Johnston
    • Christian F. Doeller
    ResearchOpen Access
    Nature Communications
    Volume: 16, P: 1-13
  • Two main acceleration mechanisms in the auroral acceleration region are electric potential and Alfvénic acceleration but associated energy dynamics are not completely resolved. Here, the authors show that Alfvén waves power the Earth’s auroral arc through a static potential drop in the auroral acceleration region.

    • S. Tian
    • Z. Yao
    • G. D. Reeves
    ResearchOpen Access
    Nature Communications
    Volume: 17, P: 1-10
  • Applications of optical laser-based techniques are limited by the long wavelengths of the lasers. Now, observations of phonons and thermal transport at nanometre length scales are reported with an all-hard X-ray transient-grating spectroscopy technique.

    • Haoyuan Li
    • Nan Wang
    • Diling Zhu
    Research
    Nature Physics
    P: 1-6
  • An analogue to a type II burst from the early M dwarf StKM 1-1262 exhibits identical frequency, time and polarization properties to fundamental plasma emission from a solar type II burst.

    • J. R. Callingham
    • C. Tasse
    • P. Zucca
    Research
    Nature
    Volume: 647, P: 603-607
  • The transport of aerosols from distant fires in deforested and savannah regions supplies phosphorus to undisturbed Amazon rainforests and influences their productivity, according to modelled phosphorus deposition estimates and satellite data.

    • Adrià Descals
    • Ivan A. Janssens
    • Josep Peñuelas
    Research
    Nature Geoscience
    P: 1-5
  • The authors present a deep learning approach to uncover complex genetic effects on circulating protein levels. They reveal new interactions and dominance patterns using UK Biobank proteomics data.

    • Arnor I. Sigurdsson
    • Justus F. Gräf
    • Simon Rasmussen
    ResearchOpen Access
    Nature Communications
    Volume: 17, P: 1-15
  • WD 0032–317B is a 75–88-Jupiter mass companion orbiting a hot white dwarf with a period of 2.3 h. It has a day-side temperature of about 8,000 K and a day–night difference of ~6,000 K. WD 0032–317B is amenable to detailed characterization and can be used as a proxy for strongly irradiated ultra-hot giant planets.

    • Na’ama Hallakoun
    • Dan Maoz
    • Alberto Rebassa-Mansergas
    Research
    Nature Astronomy
    Volume: 7, P: 1329-1340