Researchers at Kyoto University have proposed a new theory on the formation of binary black holes within collapsing stars. Their study suggests that these black holes could form through dynamical fragmentation of the star's inner core, leading to two fragments becoming black holes and orbiting each other.
The neutron star collision has challenged existing theories of dark energy and gravity, ruling out a class of dark energy theories that modify gravity. The observation also supports the simplest theories, suggesting that the timing between gravitational waves and light is crucial in understanding these phenomena.
The Graphene Flagship has successfully tested graphene for two space-related applications: loop heat pipes and solar sails. The experiments, conducted in microgravity, showed excellent thermal properties and radiation pressure behavior, paving the way for a commercial product.
Researchers at the University of California, Irvine have developed a new satellite-based drought severity index that incorporates groundwater storage. This tool provides reliable information on drought conditions, enabling effective water management and impact assessment.
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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.
A new study by Brazilian researchers resolves the 'fundamental paradox of stellar dynamics', describing galaxy clusters' violent relaxation as displaying unique behavior with entropy oscillation. Entropy increases at the end of the process, but fluctuates in the initial stage, contrary to conventional understanding.
Researchers have observed weak gravity signals related to earthquakes and found they are sensitive to the magnitude of quakes. These signals may aid in early identification of major earthquakes.
Researchers have discovered a faster method for estimating large earthquake magnitudes by analyzing 'elasto-gravity' signals, which travel at the speed of light. These signals consistently arrive before seismic wave counterparts, allowing for near-real-time magnitude detection and more accurate estimates.
Researchers at Institute for Basic Science developed a method to create dynamic tubular structures by exploiting centripetal force of rotating fluids, enabling self-assembly of particles under non-equilibrium conditions. This breakthrough could lead to creation of various shapes of microcomposites useful in photonics applications.
A proposed NASA mission employs lobster-eye optics to locate the source of gravitational waves, a key feature in understanding cosmic ripples. The Transient Astrophysics Observatory on the International Space Station aims to characterize and alert other observatories to these events.
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Researchers at Ural Federal University found that a popular theory of gravity is flawed when applied to real-world astrophysical conditions. They propose new Horndeski models to stabilize black holes, addressing modern physics prerequisites and inconsistencies. The study aims to develop a new theory of gravity meeting all requirements.
Researchers from Germany's Technische Universität Braunschweig uncovered a crucial link between the formation of cometary 'dust pebbles' and planet accretion. The study, based on Rosetta mission data, reveals that these pebbles are concentrated by solar instability, leading to collapse and the birth of comets.
For the first time, astronomers have observed a celestial event through both conventional telescopes and gravitational waves. The collision of two super-dense neutron stars just 120 million light-years from Earth was captured by both gravity wave observatories and telescopes.
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For the first time, scientists have detected both gravitational waves and electromagnetic radiation from the merger of two neutron stars, creating a new black hole. The detection marks the beginning of a new era in multi-messenger space exploration.
RIT researchers played a significant role in the groundbreaking detection of colliding neutron stars by LIGO. This event marked the first time both gravitational waves and light were detected from the same cosmic collision.
For the first time, scientists have detected the collision of two neutron stars using both gravitational waves and light. The historic discovery ushers in a new era in astronomy with multi-messenger astronomy, confirming theoretical predictions and providing new mysteries to understand.
For the first time, three detectors tracked gravitational waves emitted by a merger of two black holes, allowing scientists to more closely locate their birthplace in space. The detection highlights the scientific potential of a three-detector network of gravitational-wave detectors.
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The LIGO and Virgo observatories have jointly detected a black hole collision, emitting ripples in space and time. The event, located 1.8 billion light-years away, resulted in a spinning black hole with about 53 times the mass of our sun.
Researchers found a lower density in Mars' crust, indicating possible porosity, which could impact the planet's formation and evolution. The new gravity map reveals variations in crust thickness beneath volcanoes.
Researchers from SLAC and Stanford used neural networks to analyze images of strong gravitational lensing, performing complex analyses in a fraction of a second. The technique has the potential to transform astrophysics by analyzing vast amounts of data quickly and automatically.
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Researchers have accurately measured the Sun's core rotation rate, discovering it takes just one week for the core to complete a full rotation. This groundbreaking finding has the potential to refine models of the Sun's birth, evolution, and structure, shedding new light on its internal dynamics.
Scientists have grown cucumbers in space to study the effects of water and gravity on plant roots. In their experiments, they found that water has a greater influence on controlling root growth than gravity, which will help inform future space farming strategies.
Scientists developed an algorithm for a robotic harness that provides personalized support to address motor defects in stroke and spinal cord injury patients. Wearing the harness allows participants to walk with abilities comparable to healthy individuals, offering a promising alternative to traditional rehabilitation programs.
A team of scientists from Instituto de Astrofísica de Canarias discovered a very distant galaxy, some 10 thousand million light years away, about a thousand times brighter than the Milky Way. The galaxy is notable for having a high rate of star formation, forming stars at a rate of 1000 solar masses per year.
Historians and physicists reveal the post-WWII transformation of Einstein's General Relativity into a bonafide physics theory. New insights highlight the extension of the foundation and complementation by pre-relativistic physics and philosophical considerations, ultimately leading to its renaissance.
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Astronomers use gravitational lens to magnify light from distant galaxy, revealing two dozen clumps of newborn stars. This contradicts earlier theories suggesting larger star-forming regions in the early universe.
Researchers observe intense gas motions at filament junctions, indicating strong acceleration gradients and massive core formation. The study reveals that interstellar filaments and hub systems are privileged locations for forming the most massive stars in the Galaxy.
Mathematicians used complex modeling to study a specific pulsar exhibiting 'glitching' and 'wobbling' behaviors. They found accepted theories conflict with each other, suggesting errors in current explanations.
Astronauts are exposed to DNA damage due to zero gravity and cosmic radiation; an automated diagnostic procedure is being adapted for use in space, promising constant conditions for each sample. The device could also be used to evaluate the effects of radiotherapy.
A KAIST research team identified a software glitch in smartphones' screen rotation-tracking algorithms as the cause of frequent document photo orientation errors. Their novel technique can correct phone orientation in document-capturing tasks at 93% accuracy and seamlessly work with existing methods.
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Scientists have successfully observed a white dwarf star using the bending of distant starlight by gravity, allowing them to determine its mass for the first time. This observation demonstrates a way to measure the masses of objects that cannot be easily measured by other means.
Researchers applied novel method to test 'Einstein's equivalence principle' using rubidium atoms in quantum superposition states, confirming its validity with high precision. The study has potential applications in navigation, time measurements, and searching for mineral deposits.
Physicists at the University of Maryland contribute to the detection of a third gravitational wave event, GW170104, using data from Advanced LIGO detectors. The merger occurred approximately 3 billion years ago and produced a single, more massive black hole.
The Abell 370 galaxy cluster is a rich mix of various galaxy shapes, including massive elliptical and spiral galaxies. Nearly a hundred distant galaxies have multiple images caused by the lensing effect, with some featuring mysterious-looking arcs of blue light.
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A team of astronomers used the Hubble Space Telescope to analyze four images of a gravitationally lensed Type Ia supernova, measuring the expansion of the Universe without theoretical assumptions. The discovery provides clues about the Universe's expansion rate and has implications for cosmology.
Astronomers have captured images of a Type Ia supernova appearing in four different locations on the sky due to gravitational lensing. This rare event has opened up new possibilities for measuring the rate of the Universe's expansion with unprecedented accuracy and understanding the distribution of matter.
Researchers modelled midge swarm cohesion and found that the faster individual midges fly, the stronger gravitational-like force they experience. This speed-dependent force increases with distance from the centre of the swarm.
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Astrophysicists at the University of Birmingham made progress in understanding how two black holes can merge, using Advanced LIGO data. The team found that all three observed events can be formed via isolated binary evolution via a common-envelope phase.
The UBC-developed system uses a combination of fibre membranes and beneficial bacteria to remove contaminants from non-potable water. This innovative approach aims to provide an efficient and low-maintenance solution for communities with limited access to clean drinking water.
Astronomers have discovered three young stars that were ejected from an unstable multi-star system, providing new clues to the breakup of such systems. The stars are moving at speeds of up to nearly 30 times faster than most other stars in the same region.
A new mathematical framework explains why plants have different shapes, attributing it to a 'sense of self' and its interaction with gravity and environment. The study uses simple ideas to quantify plant stem diversity.
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Researchers propose 'ballistic sorting' as mechanism underlying size-sorting of particles on asteroid Itokawa. The theory suggests that small pebbles rebound from boulders but sink into pebble-rich regions, leading to lateral separation of particles.
Researchers have discovered a repeating one-per-cent spike in the light of Iota Orionis, a binary star system with a mass 35 times that of the Sun. The unusual variation is caused by the gravitational interaction between the two stars, triggering quakes that allow astronomers to probe the star's inner workings.
Researchers found that mammalian cells can respond to changes in gravitational conditions extremely quickly, recovering full function within 42 seconds. This rapid adaptation challenges previous assumptions about cell behavior in space, providing good news for manned space flight.
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Astronomers found that the Galaxy's gravitational field can interfere with determining the coordinates of distant objects, causing a
Caltech's Stan Whitcomb, a key figure in LIGO's development, will share insights into the project's groundbreaking discovery. He'll discuss how the detection confirmed Einstein's general theory of relativity and opened up new avenues for astronomy. The talk also touches on the technical challenges faced by LIGO detectors.
A team led by Case Western Reserve University researchers found a tight correlation between observed acceleration and gravitational acceleration from visible mass in various galaxy types. This discovery suggests a universal law governing galactic systems, similar to Kepler's planetary law. The findings require rethinking dark matter an...
Scientists estimate that solitary supermassive black holes in galactic centers may be responsible for fewer observed stars being captured by black holes. The researchers found that gravitational effects from merging galaxies can explain the discrepancy, suggesting that tidal disruption events occur without our knowledge.
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The international team released a large dataset of exoplanet-detecting observations using the radial velocity method, identifying over 100 potential planets, including one orbiting the fourth-closest star to our Solar System. The data will enable astronomers around the globe to search for new planets and follow up on existing signals.
A new study suggests that determining the speed of gravity in the cosmos from gravitational waves could resolve the puzzle. If gravitational waves are found to travel at the speed of light, it would rule out alternative gravity theories and support Einstein's Cosmological Constant.
Astronomers have found strong evidence for an intermediate-mass black hole (IMBH) weighing 2,200 solar masses at the center of the globular star cluster 47 Tucanae. The IMBH is believed to be the missing link between stellar-mass and supermassive black holes, potentially providing insight into the formation of galaxies.
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Gabriela González, a professor at LSU and LIGO scientist, receives the 2017 Rossi Prize for her groundbreaking work on gravitational waves. Her discoveries have opened a new era in gravitational-wave astronomy.
Astronomers observe IRAS 14348-1447, a gas-rich spiral galaxy merger, showcasing intense gravitational interactions. The galaxy's extreme infrared emission is fueled by massive molecular gas reserves.
Astronomers have discovered a shadow sweeping across the face of a vast pancake-shaped gas-and-dust disk surrounding a young star, possibly caused by an unseen planet gravitationally pulling on material. The twisted inner disk is casting its shadow onto the outer region.
Researchers are sequencing the genome of an ancient apple tree that inspired Isaac Newton's discovery of gravity. The study aims to understand how technological advancements have affected the evolution of apples over the past 350 years.
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A liquid ocean beneath Pluto's surface is suggested as the best explanation for its unique features, including Sputnik Planitia. The study provides evidence for a subsurface ocean and challenges traditional theories about Pluto's composition.
Theoretical physicists suggest creating a ring of ultracold atoms to measure gravity at short distances, potentially clarifying the universe's accelerating expansion. This concept has practical applications in motion sensors and quantum computing.
Researchers from the University of Extremadura and Sapienza University of Rome have discovered a new type of convection in granular fluids. This lateral-wall thermal convection is produced by inert walls and exhibits distinct properties compared to traditional fluid dynamics.
Researchers modeled massive star formation using high-performance computers, discovering episodic luminosity bursts that outshine the collective effect of 100,000 Suns. These bursts are thought to be caused by the migration of dense clumps through accretion disks, offering new insights into the birth process of massive stars.
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Two studies based on GRAIL data provide clearer pictures of the Orientale impact basin, one of the largest and youngest craters on the Moon. The studies reveal that the transient crater has a smaller diameter than previously thought and estimate a minimum amount of material redistributed from the lunar crust during the impact.
A team of researchers found that the shape of a tube, in addition to its size, affects whether liquids will spill. When tubes are elliptical or triangular, gravity can't overcome surface tension, causing liquids to remain inside, unlike circular tubes.