Scientists at UC Riverside developed a new method to help LIGO detect weaker gravitational-wave events by measuring heat-induced distortions in mirrors. The technique combines thermal imaging with existing wavefront measurements and computer models, enabling the observatory to improve its sensitivity and detect more distant events.
SourceUniversity of California - Riverside·JournalClassical and Quantum Gravity·TypeExperimental study·DateJul 21, 2026
A physicist at Mississippi State University has received a prestigious CAREER Award to study stellar explosions and their role in forming elements. The five-year project aims to improve computer models of supernovae and neutron stars, shedding light on the universe's elemental composition.
Astronomers have confirmed the connection between magnetars and superluminous supernovae, finding definitive evidence for a magnetar forming in the core collapse of a recent supernova. The discovery corroborates a theory proposed 16 years ago and establishes a new phenomenon in exploding stars.
SourceUniversity of California - Berkeley·JournalNature·DateMar 11, 2026
A team of international researchers led by a UC Santa Barbara graduate student has confirmed a long-standing theory of stellar death by applying the principles of general relativity to a superluminous supernova. The discovery suggests that a magnetar, a rapidly spinning neutron star with a massive magnetic field, powers the supernova, ...
SourceUniversity of California - Santa Barbara·JournalNature·DateMar 11, 2026
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Apple iPhone 17 Pro delivers top performance and advanced cameras for field documentation, data collection, and secure research communications.
Researchers analyzed gravitational-wave data from LIGO and Virgo detectors, revealing an oval orbit just before merger, which is unlikely according to theoretical models. The study corrects underestimated black hole mass and overestimated neutron star mass, suggesting a birthplace in an environment with many interacting stars.
SourceUniversity of Birmingham·JournalThe Astrophysical Journal Letters·TypeObservational study·DateMar 11, 2026
The Crab Pulsar's unique zebra stripes are shaped by the combination of gravity's lensing effects and plasma's defocusing power. Light rays are spread apart by plasma and pulled inward by gravity, creating interference patterns that produce bright bands and darkness between them.
A team of astronomers used multiple NSF NOIRLab facilities, including Gemini and Blanco telescopes, to study the longest gamma-ray burst ever witnessed. Analysis revealed that the event likely originated from a relativistic jet crashing into the surrounding material in a massive, extremely dusty galaxy.
SourceAssociation of Universities for Research in Astronomy (AURA)·JournalThe Astrophysical Journal Letters·DateDec 8, 2025
Researchers found that neutrino flavor transformations alter the composition and signals of what's left after a neutron star collision, impacting the creation of heavy metals and rare earth elements. The simulations also influenced the matter ejected from the merger and electromagnetic emissions detectable from Earth.
SourcePenn State·JournalPhysical Review Letters·TypeComputational simulation/modeling·DateSep 19, 2025
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Apple AirPods Pro (2nd Generation, USB-C) provide clear calls and strong noise reduction for interviews, conferences, and noisy field environments.
The XRISM mission reveals an unexpected difference between winds launching from a disc around a neutron star and those from material circling supermassive black holes. The surprisingly dense wind blowing from the stellar system challenges our understanding of how such winds form and drive change in their surroundings.
SourceEuropean Space Agency·JournalNature·TypeObservational study·DateSep 17, 2025
Astronomers discovered a greedy white dwarf star consuming its closest celestial companion at an unprecedented rate. The study found that the super-dense white dwarf is burning brightly due to the mass transfer between the two stars, potentially leading to a massive explosion visible from Earth.
SourceUniversity of Southampton·JournalMonthly Notices of the Royal Astronomical Society·TypeMeta-analysis·DateSep 9, 2025
A team of researchers has proposed that massive star collapse can create a 'neutrino collider,' leading to dramatic changes in supernova outcomes. This process could produce a neutron core or even a black hole remnant, depending on the presence of secret neutrino interactions.
SourceUniversity of California - San Diego·JournalPhysical Review Letters·TypeComputational simulation/modeling·DateJul 14, 2025
Researchers discovered that magnetar flares can produce the universe's heaviest elements, including gold and platinum. The discovery resolves a decades-long mystery concerning a bright flash of light and particles spotted by a space telescope in 2004.
SourceSimons Foundation·JournalThe Astrophysical Journal Letters·DateApr 29, 2025
A new study finds that a millisecond magnetar could have triggered the flashes of GRB 230307A, an extremely bright GRB detected in March 2023. The observation suggests that the magnetar model is consistent with the features of the prompt emission and the long-lasting X-ray plateau.
SourceScience China Press·JournalNational Science Review·TypeObservational study·DateApr 15, 2025
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Ryan Amberger, a Ph.D. candidate in physics at Texas A&M University, has been selected for a 2025 Los Alamos-Texas A&M Fellowship to conduct dissertation research on nuclear astrophysics. He aims to improve understanding of the s-process by studying neutron cross sections.
Physicists have measured a nuclear reaction that can occur in neutron star collisions, providing direct experimental data for a process previously only theorized. The study provides new insight into how the universe's heaviest elements are forged, with potential applications in nuclear reactor physics.
SourceUniversity of Surrey·JournalPhysical Review Letters·DateMar 18, 2025
The StarBurst Multimessenger Pioneer will detect short-duration bursts of gamma-rays from neutron star mergers, providing fundamental insight into these extreme explosions. With an effective area four times greater than the Fermi Gamma-ray Burst Monitor, it will increase the detection rate of EM counterparts to NS mergers.
The Einstein Probe mission aims to probe X-ray transient sources and explosive astrophysical phenomena, contributing significantly to astronomical research. The mission's sophisticated observational instruments will enhance the detection of sudden X-ray transients and monitor variability in known celestial sources.
SourceScience China Press·JournalScience China Physics Mechanics and Astronomy·TypeSystematic review·DateMar 6, 2025
A new machine learning algorithm can fully characterize systems of merging neutron stars in under a second, compared to traditional methods which take around an hour. This allows for rapid localization of the source and pointing of telescopes towards the merging neutron stars.
SourceMax Planck Institute for Intelligent Systems·JournalNature·TypeComputational simulation/modeling·DateMar 5, 2025
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Researchers found a remarkable X-ray flash in archived Chandra Observatory data, hinting at possible explanations: X-ray burst, magnetar flare, or new cosmic event. The discovery showcases the potential of AI for scientific breakthroughs in astronomical archives.
SourceRoyal Astronomical Society·JournalMonthly Notices of the Royal Astronomical Society·DateFeb 17, 2025
Researchers have discovered a strong connection between the long ringdown phase of post-merger gravitational waves and the properties of dense regions in neutron-star cores. Analyzing this phase can significantly reduce uncertainties in the equation of state at very high densities, shedding light on what neutron stars are made of.
SourceGoethe University Frankfurt·JournalNature Communications·TypeComputational simulation/modeling·DateFeb 6, 2025
Scientists studying neutron 'starquakes' hope to gain new insights into the properties of neutron stars, improving our understanding of the universe. This research has potential implications for fields like health, security, and energy.
SourceUniversity of Bath·JournalPhysical Review C·TypeData/statistical analysis·DateFeb 5, 2025
Researchers identified a new process leading to formation of low-field magnetars, solving the mystery that puzzled scientists since their discovery in 2010. The team used advanced simulations to model magneto-thermal evolution of neutron stars, finding that a specific dynamo process can generate weaker magnetic fields.
SourceNewcastle University·JournalNature Astronomy·DateFeb 4, 2025
Researchers used a new method to precisely locate a fast radio burst, finding it in the outskirts of an old elliptical galaxy. This discovery raises questions about how energetic events occur in regions without new star formation, and challenges existing theories about FRB origins.
SourceUniversity of California - Berkeley·JournalThe Astrophysical Journal Letters·DateJan 21, 2025
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Astronomers have observed the same supermassive black hole exhibiting unprecedented behavior, with X-ray flashes increasing in frequency over two years. The source of these flashes is believed to be a spinning white dwarf core orbiting around the black hole's edge.
SourceMassachusetts Institute of Technology·JournalNature·DateJan 13, 2025
A nearby supernova explosion could produce gamma rays that pinpoint the mass of a key dark matter candidate, the axion. The Fermi Gamma-ray Space Telescope would need to be in position to detect these gamma rays within 10 seconds of the supernova's core collapse.
SourceUniversity of California - Berkeley·JournalPhysical Review Letters·DateNov 21, 2024
Scientists have found that black holes inherit their magnetic fields from their parent stars, specifically the surrounding disk of swirling matter during collapse. This discovery resolves a longstanding mystery and opens doors for further studies of jets.
SourceSimons Foundation·JournalThe Astrophysical Journal Letters·TypeComputational simulation/modeling·DateNov 18, 2024
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A recent study reveals that fast radio bursts are more commonly associated with massive and metal-rich star-forming galaxies. This suggests that magnetars, the thought-to-be-triggers of FRBs, likely form in environments conducive to stellar mergers. The discovery was made using Caltech's Deep Synoptic Array-110 project.
SourceCalifornia Institute of Technology·JournalNature·DateNov 6, 2024
Researchers from DTU have discovered a neutron star that rotates at an astonishing 716 times per second, making it one of the fastest-spinning objects ever observed. The neutron star is part of an X-ray binary star system and is located in the Sagittarius constellation.
SourceTechnical University of Denmark·JournalThe Astrophysical Journal·DateOct 30, 2024
Astronomers have observed a black hole triple system for the first time, featuring a central black hole consuming a star and a distant companion that orbits every 70,000 years. The discovery raises questions about the origins of the black hole itself.
SourceMassachusetts Institute of Technology·JournalNature·DateOct 23, 2024
Researchers from the Universiteit van Amsterdam and other institutions show that axion clouds around neutron stars could provide a new way to observe these elusive particles. The formation and properties of these clouds are studied, offering new opportunities for axion research and potentially solving the dark matter puzzle.
SourceUniversiteit van Amsterdam·JournalPhysical Review X·TypeComputational simulation/modeling·DateOct 18, 2024
Astronomers have recorded hundreds of gamma-ray bursts (GRBs) in a massive global effort that rivals the 250-year-old Messier catalogue. The collection includes 64,813 photometric observations and showcases collaborative research across nations.
SourceRoyal Astronomical Society·JournalMonthly Notices of the Royal Astronomical Society·TypeObservational study·DateSep 12, 2024
Sky & Telescope Pocket Sky Atlas, 2nd Edition
Sky & Telescope Pocket Sky Atlas, 2nd Edition is a durable star atlas for planning sessions, identifying targets, and teaching celestial navigation.
Researchers unveil previously unseen properties of neutron stars through gravitational wave analysis, providing insight into internal composition and dynamic material properties. The study places observational constraints on viscosity within neutron stars.
SourceUniversity of Illinois at Urbana-Champaign, News Bureau·JournalNature Astronomy·TypeComputational simulation/modeling·DateSep 5, 2024
Researchers at Brookhaven National Laboratory's STAR Collaboration have discovered a new kind of antimatter nucleus, antihyperhydrogen-4, composed of four antimatter particles. The discovery was made using the Relativistic Heavy Ion Collider and analyzed details of collision debris.
SourceDOE/Brookhaven National Laboratory·JournalNature·DateAug 21, 2024
Scientists have captured the first-ever image of an S-shaped jet coming from a confirmed neutron star, providing strong evidence for precessing jets. The discovery was made using the MeerKAT telescope and reveals valuable insights into the extreme physics behind the launching of the jet.
Astronomers have uncovered 21 neutron stars in wide orbits around stars like our Sun, revealing the first dark neutron star population. The discovery was made possible by the European Space Agency's Gaia mission, which scanned the sky and measured wobbles of over a billion stars.
SourceCalifornia Institute of Technology·JournalThe Open Journal of Astrophysics·DateJul 16, 2024
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SAMSUNG T9 Portable SSD 2TB transfers large imagery and model outputs quickly between field laptops, lab workstations, and secure archives.
Researchers have proposed a new model explaining neutron star glitches, suggesting that the power-law behavior of glitch energies is due to the formation of twisted clusters of superfluid vortices. The study found that the exponent for the power-law behavior closely matched the observed data.
SourceInternational Institute for Sustainability with Knotted Chiral Meta Matter (SKCM2)·JournalScientific Reports·DateJun 26, 2024
Researchers have discovered a hidden treasure in the Milky Way, identifying Cygnus X-3 as an ultra-luminous X-ray source. The use of X-ray polarized vision has revealed the configuration of dense matter surrounding the black hole, sparking new insights into extreme matter consumption.
SourceUniversity of Turku·JournalNature Astronomy·DateJun 24, 2024
New simulations show that neutrinos created during neutron star collisions can be trapped at the interface of merging stars and interact with matter for 2-3 milliseconds. This brief out-of-equilibrium phase is crucial in understanding the physics of these extreme events.
SourcePenn State·JournalPhysical Review Letters·TypeComputational simulation/modeling·DateJun 18, 2024
Astronomers have detected a neutron star spinning at an unprecedentedly slow rate, defying the typical mind-bending speeds of these ultra-dense stars. The object emits radio signals every 54 minutes, offering new insights into its complex life cycle and potential implications for our understanding of stellar objects.
SourceUniversity of Manchester·JournalNature Astronomy·DateJun 5, 2024
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Fluke 87V Industrial Digital Multimeter is a trusted meter for precise measurements during instrument integration, repairs, and field diagnostics.
Sean McWilliams' team will study stellar-mass and massive binary inspirals, improving modeling accuracy for the Laser Interferometer Space Antenna (LISA). The project aims to enhance the instrument's science mission by making necessary dramatic improvements in modeling accuracy.
Astronomers from the University of Sydney and CSIRO have detected a slow-spinning neutron star with a period of nearly an hour, breaking all known rules. This discovery provides new insights into the complex life cycles of stellar objects and may prompt a reconsideration of our understanding of neutron stars or white dwarfs.
SourceUniversity of Sydney·JournalNature Astronomy·TypeObservational study·DateJun 4, 2024
Researchers at MIT have developed a new method to measure the spin of supermassive black holes by tracking the pattern of X-ray flashes produced during tidal disruption events. By analyzing the wobble of the accretion disk, they were able to determine that the nearby black hole was spinning at less than 25% the speed of light.
SourceMassachusetts Institute of Technology·JournalNature·DateMay 22, 2024
Apple Watch Series 11 (GPS, 46mm)
Apple Watch Series 11 (GPS, 46mm) tracks health metrics and safety alerts during long observing sessions, fieldwork, and remote expeditions.
Researchers have discovered three of the oldest stars in the universe, forming between 12 and 13 billion years ago. The team believes these 'Small Accreted Stellar System' (SASS) stars originated from small primitive galaxies absorbed by the Milky Way.
SourceMassachusetts Institute of Technology·JournalMonthly Notices of the Royal Astronomical Society·DateMay 14, 2024
An international team of researchers, including those from the University of Geneva, detected a giant magnetar eruption coming from a neutron star with an exceptionally strong magnetic field. The discovery was made using ESA's satellite INTEGRAL and confirms that magnetars are young neutron stars.
SourceUniversité de Genève·JournalNature·TypeNews article·DateApr 24, 2024
Researchers detected unusual radio pulses from a dormant star with powerful magnetic field, challenging previous explanations. The signals suggest superheated plasma above the magnetar's pole is acting like a polarizing filter.
SourceCSIRO Australia·JournalNature Astronomy·TypeObservational study·DateApr 8, 2024
Physicists calculated that neutron stars can heat up quickly due to energy transfer from dark matter particles, providing a potential way to detect dark matter. This process could reveal the nature of dark matter and its interactions with regular matter.
SourceUniversity of Melbourne·JournalJournal of Cosmology and Astroparticle Physics·TypeObservational study·DateApr 4, 2024
Astronomers have discovered a new black hole behavior where a smaller black hole repeatedly punches through the disk of a larger black hole, releasing plumes of gas. The findings challenge conventional views on black hole accretion disks and suggest they may be more varied in their contents.
SourceMassachusetts Institute of Technology·JournalScience Advances·DateMar 27, 2024
Kestrel 3000 Pocket Weather Meter
Kestrel 3000 Pocket Weather Meter measures wind, temperature, and humidity in real time for site assessments, aviation checks, and safety briefings.
For the first time, astronomers have measured the speed of fast-moving jets in space, crucial to star formation and the distribution of elements needed for life. The jets of matter, expelled by stars deemed 'cosmic cannibals', were found to travel at over one-third of the speed of light.
Researchers have discovered unique electromagnetic signals in the debris of a neutron star merger, which could provide new constraints on axion-like particles and their potential role in dark matter. The findings were made using data from NASA's Fermi-LAT gamma-ray telescope.
SourceWashington University in St. Louis·JournalPhysical Review Letters·DateMar 6, 2024
Researchers have detected tellurium in a kilonova afterglow, indicating that neutron star mergers can create rare heavy elements. This discovery sheds light on the formation of elements heavier than iron and provides new insights into the universe's chemical composition.
SourceClemson University·JournalNature·TypeData/statistical analysis·DateFeb 29, 2024
The James Webb Space Telescope has found direct evidence for emission from a probable young neutron star at the site of the recently observed supernova SN 1987A. Spectral analysis revealed strong signals due to ionized argon and five times ionized argon, indicating high-energy radiation from the compact object.
SourceNASA/Goddard Space Flight Center·JournalScience·DateFeb 22, 2024
Researchers at the University of Tokyo have developed a method to accurately measure and predict neutron-induced transmutation, which can make nuclear waste more stable. This technique could lead to improved nuclear waste treatment facilities and new theories about the creation of heavier elements in the universe.
SourceUniversity of Tokyo·JournalPhysics Letters B·TypeExperimental study·DateFeb 15, 2024
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Auburn University researchers are using a $400K NSF award to study the ionization and recombination of heavy elements in kilonovae, shedding light on their origins. The team's calculations will help determine which elements were produced in neutron star mergers.
SourceAuburn University College of Sciences and Mathematics·TypeComputational simulation/modeling·DateFeb 14, 2024
Researchers visualize second sound, a wave-like movement of heat, independent of physical particle motion in a superfluid. The findings expand understanding of heat flow in superconductors and neutron stars.
SourceMassachusetts Institute of Technology·JournalScience·DateFeb 8, 2024
Astronomers have found a direct link between massive star explosions and the formation of compact objects like black holes and neutron stars. The study used ESO's VLT and NTT to observe a supernova explosion in a nearby galaxy, revealing evidence for a compact remnant left behind.
A new study places the likelihood of massive neutron stars having deconfined quark matter at 80-90%. This is made possible through Bayesian statistical inference and massive supercomputer runs. The research has implications for our understanding of particle and nuclear physics, as well as astrophysics.
SourceUniversity of Helsinki·JournalNature Communications·TypeComputational simulation/modeling·DateDec 28, 2023
Researchers have identified a population of massive stars stripped of their hydrogen envelopes by their companions in binary systems. These hot helium stars are believed to be the origins of hydrogen-poor core-collapse supernovae and neutron star mergers, shedding new light on a long-theorized phenomenon.
SourceUniversity of Toronto·JournalScience·TypeObservational study·DateDec 14, 2023
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Sky-Watcher EQ6-R Pro Equatorial Mount provides precise tracking capacity for deep-sky imaging rigs during long astrophotography sessions.
Researchers found that ancient stars created elements with atomic masses greater than 260, challenging current knowledge. This discovery provides insight into the process of heavy element formation in stars and could help explain the diversity of elements on Earth.
SourceNorth Carolina State University·JournalScience·TypeData/statistical analysis·DateDec 7, 2023
Researchers found a correlation between light precision metals like silver and rare earth nuclei like europium, indicating a consistent process operating during heavy element formation. The pattern provides a clear signature of fission creating these elements.
SourceDOE/Los Alamos National Laboratory·JournalScience·TypeObservational study·DateDec 7, 2023
Scientists have successfully simulated neutron star glitches using ultracold supersolids, revealing a link between quantum mechanics and astrophysics. The study sheds light on the internal structure and dynamics of neutron stars, providing valuable insights into extreme conditions.
SourceUniversity of Innsbruck·JournalPhysical Review Letters·TypeComputational simulation/modeling·DateDec 5, 2023
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