Astronomers detected X-ray eclipses from a fast pulsar, shedding light on compressed matter and testing relativity. The system's unique properties revealed the size and mass of the companion star with unprecedented accuracy.
Researchers credited with discovery, PSR J2007+2722, a neutron star rotating 41 times per second, has no orbiting companion and is likely recycled or young, sparking interest in basic physics of neutron stars. This is the first genuine astronomical discovery by a public volunteer distributed computing project.
Astronomers have discovered a brown dwarf companion to a young sun-like star, PZ Tel A. The discovery reveals the early stages of solar system formation and provides insights into planetary formation.
Singapore's A*STAR and Cytos Biotechnology collaborate on a virus-like particle (VLP) vaccine targeting influenza hemagglutinin protein. The partnership aims to develop an independent supply of vaccines for Singapore and ASEAN countries, extending Cytos' R&D pipeline.
The discovery of exoplanet Beta Pictoris b, located 60 light-years from Earth, confirms that giant planets can form in time-spans as short as a few million years. The planet has a massive nine-Jupiter-mass orbit, challenging previous theories on planetary formation.
Astronomers discovered a runaway star in the Large Magellanic Cloud's 30 Doradus Nebula, with a speed of over 400,000 km/h. The star is estimated to be around 10 times hotter than the Sun and has been ejected from its home cluster through dynamical interaction.
Corot-9b, a gas giant planet, has an interior similar to that of Jupiter and Saturn, allowing it to maintain liquid water. The planet's distance from its star and lack of tidal forces make this possibility plausible.
A newly discovered star in the Sculptor dwarf galaxy has a chemical makeup similar to the Milky Way's oldest stars, lending support to the 'bottom-up model' of galaxy formation. The star's unusually low metal abundance resembles those of old Milky Way stars, further validating the theory.
New neutron studies provide strong evidence that magnetic properties are behind high-temperature superconductivity in both copper-based and iron-based materials. The research suggests that spin excitations play a key role in the formation of macroscopic quantum states giving rise to superconductivity.
Astronomers have found a giant magnetic loop stretching from one star to the other in the Algol binary system. The discovery was made using an international collection of radio telescopes and helps explain previous observations at X-ray and radio wavelengths.
Researchers found two brown dwarf-sized masses around an ordinary star, which is extremely rare. The discovery suggests that planets may assemble around stars more quickly and efficiently than thought possible.
Astronomers have discovered a 'super-Earth' orbiting a red dwarf star 40 light-years from Earth. The planet, GJ1214b, is about 6.5 times as massive as the Earth and orbits its star once every 38 hours.
Researchers discover supernova that fits predictions for a star hundreds of times the sun's mass, revealing new insights into star formation and heavy metal creation. The study also suggests hyper-giant stars may exist beyond 150 suns, challenging our understanding of celestial physics.
The Fermi Gamma-ray Space Telescope has detected high-energy gamma-rays from the enigmatic binary system Cygnus X-3, a genuine microquasar. The system's unique properties and strong emission across various wavelengths offer new insights into how high-energy particles are accelerated and move through jets.
Scientists confirm ultra-thin coating of carbon on neutron star using Chandra's X-ray spectrum and theoretical models. The discovery resolves a ten-year mystery surrounding the object, explaining its lack of pulsations.
Astronomers have identified the youngest neutron star ever discovered, located 11,000 light years from Earth. The star was born in a violent supernova explosion 330 years ago and features a unique carbon atmosphere just 10 centimeters thick.
The study reveals two distinct dust disks around the star 51 Ophiuchi, with the inner disk spanning 4 Astronomical Units from the star and tapering off rapidly. The outer disk extends hundreds of times farther and appears more puffed up, holding smaller particles similar in size to those in smoke.
Mathematicians at the University of Leeds propose that black holes are directly responsible for producing gamma ray bursts, contradicting the orthodox model. The theory suggests that rotating black holes can devour nearby stars, creating long-lasting jets of plasma that produce the high-energy radiation.
Astronomers have discovered the first close-up of a white dwarf star orbiting a companion star, set to explode into a supernova in a few million years. The white dwarf is unusual, with twice its expected mass and a diameter half that of Earth.
Researchers believe that Galileo's notebooks from 1613 may reveal evidence of his discovery of a new planet, which is now known as Neptune. The planet was observed by Galileo as a faint star near Jupiter and moved relative to an actual nearby star.
UC Berkeley researchers have found that Betelgeuse, the bright reddish star in the constellation Orion, has steadily shrunk over the past 15 years. The star's diameter has decreased by more than 15% since 1993, a change that is striking to observe.
Astronomers have discovered a unique double-star system that represents a 'missing link' stage in the birth process of millisecond pulsars. The system, J1023, shows evidence for an accretion disk surrounding the neutron star before it disappeared and the pulsar emerged.
Scientists are synchronizing lenses of the Whole Earth Telescope network to monitor a white dwarf, shedding light on its composition and applying knowledge to Earth's weather. The star, WDJ1524-0030, is losing brightness as it cools, with astronomers studying its pulses to understand internal movements.
Researchers at Harvard-Smithsonian Center for Astrophysics have created an 'astro-comb' to help detect lighter planets around distant stars. The technique sharpens spectroscopy, enabling more accurate pinpointing of planet locations and opening possibilities for detecting more Earth-like planets.
Research by Charles Horowitz at Indiana University reveals that the crusts of neutron stars are 10 billion times stronger than steel or other earth's strongest metal alloys. The findings have significant implications for understanding surface irregularities, star quakes, and magnetar giant flares.
Astronomers have discovered a gamma-ray burst from a star that died 630 million years ago, marking the most distant cosmic explosion ever seen. The burst, dubbed GRB 090423, is approximately 13 billion light-years away.
Researchers at Brookhaven National Laboratory used Nimbus cloud computing infrastructure to dynamically provision virtual clusters on commercial cloud computers, enabling faster simulation results for the Quark Matter physics conference. The successful collaboration demonstrates the potential of virtualization and cloud computing for r...
The Einstein@Home project is analyzing Arecibo radio data to find binary systems consisting of neutron stars or black holes. The large computational capabilities of the project will enable detection of pulsars in binary systems with orbital periods as short as 11 minutes.
Scientists have directly observed a gigantic star blowing up, supporting the idea that massive stars end as black holes. The explosion revealed most of the star's mass collapsed into a dense core, creating an invisible black hole.
Astronomers detect frequent X-ray and gamma-ray flares from a soft-gamma-ray repeater, a rare type of neutron star. The object has erupted with over 100 flares in 20 minutes, releasing more energy than the sun does in 20 years.
A new study published in Science resolves the mystery of how massive stars can form without blowing away the gas and dust that feed their growth. The research found that instabilities develop in the collapsing gas cloud, creating channels where radiation blows out into space while gas continues to fall inward.
Fermi Gamma-ray Space Telescope has discovered 12 new gamma-ray-only pulsars and detected pulses from 18 others. The finds are challenging our previous understanding of how pulsars work, with gamma rays now believed to originate far above the neutron star.
Researchers have captured a rare binary star explosion inside a planetary nebula, offering new insights into stellar evolution. The study predicts that the combined mass of the two stars could lead to a larger supernova explosion.
Gemini Observatory's groundbreaking discovery reveals two planets orbiting a young, massive star called HR 8799. The system consists of three planets, including the 'first family' member, which are still glowing from heat released as they contracted, and are about seven and ten times the mass of Jupiter.
NASA's Hubble Space Telescope has directly observed a planet circling another star, Fomalhaut b. The exoplanet orbits Fomalhaut at a distance of 10.7 billion miles, 10 times that of Saturn from the sun.
A team of astrophysicists from the University of Montreal has discovered and measured the most massive star ever found, a binary system with a total mass of over 100 solar masses. The star, located in the NGC 3603 cluster, has a rotation period of 3.77 days and emits X-rays at unprecedented levels.
Researchers used thermal neutron attenuation to measure in-situ water content and uptake of nutrients by plants, providing a non-invasive method for studying root systems. The technique, called neutron computed tomography, has potential applications in agricultural practices and ecosystem sustainability.
Scientists at Washington University in St. Louis have detailed the interaction between a superfluid and a superconductor, which could change our understanding of neutron stars' motion. The research reveals exotic behavior at the boundary between type I and type II superconductors, with unexpected effects on magnetic fields.
Researchers used a rare double-star system to test Albert Einstein's theory of General Relativity, finding that the famed physicist's 93-year-old theory has passed yet another test. The study confirmed that the strong gravity of the neutron stars causes one to wobble or precess.
A team of European astronomers has discovered a triple system of super-Earths around the star HD 40307 using the HARPS instrument. The planets have masses between 4.2 and 9.4 times that of Earth, and orbit the star with periods ranging from 4.3 to 20.4 days.
A team of astronomers led by David Bennett discovered a planet with a mass about three times that of Earth, orbiting a star with a mass 6% of the sun's, potentially hosting conditions suitable for life. The discovery was made using the gravitational microlensing method and confirms predictions made in 1996.
Researchers used LIGO data to analyze the Crab Pulsar, detecting signals that reveal no more than 4% of energy loss is due to gravitational radiation. The findings suggest other mechanisms, such as electromagnetic radiation and high-velocity particles, are responsible for the pulsar's slowing spin.
Researchers at Thomas Jefferson National Accelerator Facility found that protons are about 20 times more likely to pair up with neutrons in the nucleus. This discovery could have significant implications for understanding the structure of nuclear systems, from light nuclei to neutron stars.
Astronomers have detected a giant ring around a rare and exotic star known as a magnetar, which was likely produced by a massive flare. The discovery provides valuable insights into the phenomenon associated with magnetars, a type of neutron star with incredibly strong magnetic fields.
Astronomers have caught a supernova explosion in the act, providing valuable insights into the process. The observation, made possible by NASA's Swift satellite, has helped scientists form a detailed picture of star explosions and shed light on long-standing puzzles.
A small red dwarf star called EV Lacertae unleashed an unprecedented stellar flare, detected by NASA's Swift satellite. The star's fast rotation and magnetic fields generated the powerful flare, releasing energy across the electromagnetic spectrum.
A rare and intense stellar flare was detected by NASA's Swift satellite from the normally quiet red dwarf star EV Lacertae. The flare, which lasted for 8 hours, would have sterilized life-bearing planets' surfaces if they were nearby.
Scientists have discovered a timing mechanism in neutron stars that allows them to predict when incredibly powerful X-ray bursts will occur, releasing energy equivalent to 100 hydrogen bombs exploding simultaneously.
Researchers found two star systems with yellow supergiant eclipsing binary characteristics, which may be the progenitors of rare supernovae. The discovery was made using the Large Binocular Telescope and suggests that these systems could explain the unusual nature of certain supernovae.
A team of astronomers from Queen's University Belfast have discovered the nature of five supernova precursor stars using Hubble images. The study reveals that stars with masses as low as seven times the mass of the Sun can explode as supernovae, challenging current understanding of massive star collapse.
Researchers developed a new optical method to detect individual neutrons with improved efficiency, promising better measurements and new physics tests. The Lyman alpha neutron detector (LAND) has the potential to detect both single and large numbers of neutrons.
Researchers have discovered a neutron star that undergoes a dramatic transformation from a pulsar to a magnetar, providing insight into the evolutionary connection between these two types of ultradense objects. The discovery was made using data from NASA's Rossi X-ray Timing Explorer and Chandra X-ray Observatory satellites.
Astronomers have found a clue to the evolutionary relationship between pulsars and magnetars by examining archival RXTE data of a young neutron star. The study reveals that a regular pulsar can produce powerful bursts similar to those from magnetars, challenging current understanding of their life cycles.
Astronomers have discovered a solar system nearly 5,000 light years away with scaled-down versions of Jupiter and Saturn. The planets are similar in size to our own, suggesting that planetary systems like ours may be more common than previously thought.
Researchers have discovered a multi-planet system with two large planets similar to Jupiter and Saturn, suggesting that planetary systems like our own may be common in the Milky Way galaxy. This is the first discovery of its kind, using a new gravitational microlensing technique.
Researchers using Chandra X-ray Observatory data have reported a possible detection of a binary star system that was later destroyed in a supernova explosion. The new method provides great promise for finding the detailed origin of these cosmic events.
Astronomers have determined that a hyperfast star, HE 0437-5439, originated from the Large Magellanic Cloud, contradicting its initial assumption of coming from the Milky Way. The star's elemental composition and velocity indicate it was ejected from the LMC by a massive black hole.
New research by Arecibo Observatory increases the mass limit for neutron star formation into black holes, suggesting they may be more rare. Neutron stars are found to remain stable between 1.9 and 2.7 sun masses, contradicting previous thought.
A team of astronomers discovered that a white dwarf, AE Aquarii, emits high-energy X-rays as it whirls around on its axis, similar to the Crab Nebula's pulsar. This behavior indicates that white dwarfs can accelerate charged particles to near-light speed, potentially contributing to cosmic rays.
A team of astronomers, led by Dr. Edo Berger, have observed a surprisingly active magnetic field on the ultracool low-mass star TVLM513-46546, challenging the theory that cooler stars are simple and quiet. The star's complex magnetic field environment may indicate unusual activity beneath its surface or possibly even an unseen companion.