The Event Horizon Telescope detected magnetic fields near the event horizon of the Milky Way's central black hole, Sgr A*, for the first time. The findings suggest that these magnetic fields are disordered in some regions and organized in others, possibly related to jet generation.
A new study suggests that vast quantities of radiation from superflaring Red Dwarf stars like Kepler-438 can strip away an atmosphere and make a planet uninhabitable. The energy released by each superflare is equivalent to 100 billion megatons of TNT, posing a significant threat to life on Earth-like planets.
Researchers have discovered thousands of stellar pulses in the galaxy Messier 87 (M87), providing a new method for calculating a galaxy's age. The pulsations are caused by bright, pulsating stars that were previously unknown to affect distant galaxies' light.
The Visible Nulling Coronagraph (VNC) technology has demonstrated improved sensitivity over a broader spectral range, making it a stronger contender for a future astrophysics mission. The instrument will enable spectroscopy to study exoplanet atmospheres and identify signs of life.
Astronomers have found nine ancient stars near the Milky Way's center, forming before the galaxy existed, with surprising purity and a possible hypernova origin.
The discovery of GJ 1132b, a rocky planet orbiting a red dwarf star, has sparked excitement among astronomers. With temperatures potentially conducive to hosting an atmosphere, this planet is close enough (39 light-years away) to be studied in detail with the Hubble Space Telescope and future observatories.
A new study suggests that disk gaps may be a cosmic illusion and not necessarily caused by hidden planets. The researchers used models to show that growth, migration, and destruction of small particles can create apparent gaps in the disk.
PhD student Elise Hampton uses AI to analyze thousands of galaxy spectra, identifying the most turbulent and messy galaxies. Her goal is to understand how galaxies form, live, and die, and how different processes compete in these galactic systems.
Astronomers have spotted a large, rocky object disintegrating in its death spiral around a distant white dwarf star, confirming a long-standing theory behind the source of white dwarf 'pollution' by metals. The system shows signs of surrounding debris disk and at least one compact, rocky object.
Astrosat observes cosmic objects in visible light, ultraviolet waveband, and X-ray wavebands from very low to high energy. The satellite addresses fundamental scientific problems like testing Einstein's general theory of relativity and studying superdense cold matter.
Researchers propose a new technique to detect stars at galactic center by looking for radio waves from supersonic stars. Stars with high speeds can create shock waves, producing radio emission that can be detected.
A new study proposes that if life can travel between stars through panspermia, it would spread in a characteristic pattern, creating clusters of life-forms. These clusters could resemble bubbles in a pot of boiling water, growing and overlapping with each other.
Astronomers have solved a mystery over blue hook stars, which form when a star's outer layers are destroyed by rapid rotation. The international team found that these stars consume hydrogen fuel more slowly due to their high spin rates.
A team of astronomers has discovered a massive star cluster in the NGC 5253 dwarf galaxy, containing over 7,000 massive O-type stars. The cluster, dubbed Cloud D, is incredibly efficient at forming stars and creating dust, with a gas cloud rate that is ten times greater than in our own Milky Way.
Researchers have imaged tube-like structures in the Earth's magnetosphere, which are 500 to 700 kilometers above the surface. The structures were detected by mapping variations in radio source positions and exploiting the MWA's rapid snapshot capabilities.
The Large Synoptic Survey Telescope (LSST) will survey the entire Southern Hemisphere's sky, collecting 30 terabytes of data nightly. The telescope aims to map 20 billion galaxies and observe supernovae, offering stringent tests on dark matter and dark energy.
Theoretical work suggests water vapor could have existed in pockets of space a billion years after the Big Bang, with temperatures around 80 degrees Fahrenheit allowing for its formation. The team found equilibrium levels similar to those seen in our local universe.
Researchers identified 200 previously unknown compact elliptical galaxies using public archives of data from the Sloan Digital Sky Survey and the GALEX satellite. Of these, 11 isolated compact galaxies were found moving faster than their cluster counterparts
New research using high-resolution observations reveals that magnetic fields in the Cat's Paw Nebula preserve their direction from large to small scales. This suggests that self-gravity and turbulence cannot significantly alter the field direction, allowing for a more detailed understanding of star formation.
A team of physicists has successfully cooled highly-charged ions to sub-Kelvin temperatures, forming a Coulomb crystal that opens up new fields in laser spectroscopy. This breakthrough enables precision tests of quantum electrodynamics, measurement of nuclear properties, and laboratory astrophysics.
Scientists have identified the fastest-moving unbound star in our galaxy, breaking the galactic speed record with a speed of 1,200 kilometers per second. The star, US708, was once part of a double-star solar system and is now expected to leave the Milky Way.
Researchers successfully demonstrate a new technique combining a solar telescope with a laser frequency comb to analyze distant stars with unprecedented accuracy, potentially leading to the discovery of Earth-like planets. The technique enhances spectral analysis and advances research in astrophysics.
Harvard-Smithsonian astronomers created a new 3-D map of the interior of Cas A using a CAT scan equivalent. They found six massive cavities, or bubbles, that likely formed from radioactive nickel generated during the supernova explosion.
Researchers designed an X-ray polarimeter, X-Calibur, to study high-energy processes near black holes. The instrument measures X-ray polarization properties to study extreme objects in the Universe.
The discovery of enormous radiation bubbles in the Milky Way's center may hold clues to understanding the galaxy's past and potentially revealing dark matter. Studies of these Fermi bubbles could offer insight into the history of our galaxy, including the activity of its black hole.
A new study by Professor Ulf-G Meißner finds that fundamental physics constants are fine-tuned to allow for the emergence of a life-enabling universe. The researcher used high-performance computers to simulate worlds with altered light quark masses and found that variations up to 2-3% do not prevent the formation of carbon and oxygen.
Astronomers discovered eight new planets in the habitable zone of their stars, doubling the number of small planets believed to exist. Two of these, Kepler-438b and Kepler-442b, are the most Earth-like known exoplanets, with a high probability of being rocky and having liquid water on their surface.
Astronomers have found evidence that the recipe for Earth applies to terrestrial exoplanets orbiting distant stars. The HARPS-North instrument measured the masses of small, Earth-sized worlds and found a tight relationship between mass and size, suggesting rocky compositions similar to those of Venus and Earth.
Researchers have developed a method to calculate the ages of individual stars by measuring their spin periods and masses. The technique, known as gyrochronology, uses mathematical relationships between mass, rotation rate, and age to determine stellar ages with precision.
Research suggests that super-Earths can maintain oceans for at least 10 billion years due to a planet-wide recycling process. This finding implies that older super-Earths are more suitable for searching for complex life.
Researchers from around the world have successfully explained the formation and propagation of stellar jets emitted by young stars. The team used a patented experimental device and numerical simulations to demonstrate that interstellar magnetic fields play a key role in confining these jets, which can travel vast distances.
New observations from the Interface Region Imaging Spectrograph (IRIS) suggest that miniature solar flares called 'nanoflares' could be partly responsible for heating the Sun's million-degree corona. High-energy electrons generated by these nanoflares may deposit energy in the plasma, leading to coronal heating.
Astronomers develop a new laser-based technology called the green astro-comb to detect tiny Doppler shifts, helping identify habitable zone planets. The device will enable precise measurements of exoplanet gravity, allowing for better detection of rocky worlds like Earth.
Researchers have found that stars that oscillate at the same frequency as gravitational waves can absorb energy from those waves and brighten temporarily. This effect could provide scientists with another method to indirectly detect gravitational waves.
Researchers confirm lithium-6 production in Big Bang energy range, contradicting observed lithium concentrations in stars. The study resolves the 'lithium problem,' a stubborn issue in astrophysics.
Researchers at Harvard-Smithsonian Center for Astrophysics propose that silicon-capped hydrocarbons like SiC3H, SiC4H and SiC5H may be responsible for the diffuse interstellar bands. The team analyzed laboratory spectra and theoretical calculations to support their hypothesis.
Researchers found water vapour abundance to be between ten and a thousand times less than predicted models, raising questions about the chemical processes involved in planet formation. The discovery has implications for searching for life on exoplanets capable of supporting it.
Researchers propose using industrial pollution as a sign of intelligent life, which could be detectable with the James Webb Space Telescope. The team found that CFCs could be used to identify advanced civilizations, but this method requires an ideal environment, such as an Earth-like planet circling a white dwarf star.
The Advanced Technology Large-Aperture Space Telescope (ATLAST) mission aims to study dark energy, the mysterious form of energy that accelerates the universe's expansion. ATLAST would also detect signatures of life in the atmospheres of Earth-like planets and resolve stars in distant galaxies.
Researchers detected striking similarities between a recent gamma-ray burst and the expected features from the first stars in the universe. The ultra-long burst is thought to be caused by an explosion from a blue supergiant star, providing evidence for this class of objects.
Astronomers have used a new technique to measure the ages of 22 Sun-like stars, revealing properties similar to our Sun. The study's lead author found 'solar twins' that can be studied to predict planetary system evolution.
Scientists detect a split-second burst of radio waves from the Arecibo telescope, marking the first time such an event has been recorded using an instrument other than the Parkes radio telescope. The finding suggests that these mysterious pulses are truly of cosmic origin and may be caused by exotic astrophysical objects.
Scientists at NIST and IU developed a tool that calculates fundamental properties of most atoms with historic accuracy, improving the prediction of atomic properties for fields like nuclear medicine and astrophysics. The technique enables precise determination of base energy levels, crucial for fundamental atomic research.
A team of astronomers led by Ivana Damjanov has found a treasure trove of compact, densely packed 'red nugget' galaxies in online archives. These galaxies are abundant in the middle-aged universe, providing new constraints on theoretical models of galaxy formation and evolution.
Astrophysicists at Penn State University have solved the Lunar Farside Highlands Problem, a long-standing mystery about the absence of maria on the far side of the moon. The researchers found that the difference in crustal thickness between the near and far sides is due to the moon's original formation process.
A team of astronomers has discovered a new type of planet, Kepler-10c, a mega-Earth with a diameter of approximately 18,000 miles. The planet's mass is 17 times that of Earth, indicating it is composed primarily of rocks and other solids.
Two planets in the Kepler-56 system will meet their fate when they are dragged into the star's expanding orbit. The inner planets will be destroyed due to tidal forces and intense heat from the growing star.
A new study reveals that red dwarf planets may be stripped of their atmospheres due to harsh space weather, making life potentially even rarer. The extreme environment also triggers spectacular aurorae, but would lead to constant darkness and hurricane-force winds.
Researchers found that planets between 1.7 and 3.9 times the size of Earth are dubbed 'gas dwarfs' with thick atmospheres of hydrogen and helium. The study also revealed that metallicity plays a crucial role in determining planetary composition, with stars hosting gas giants containing about 50% more metals than our Sun.
The Interface Region Imaging Spectrograph (IRIS) successfully observed a gigantic coronal mass ejection (CME) on May 9, 2014. The spacecraft caught the event in extraordinary detail, revealing its unprecedented size and structure.
The 2014 Kavli Prize winners made significant contributions to our understanding of cosmic inflation, nano-optics, and brain networks. Their discoveries have revolutionized fields like astrophysics, nanoscience, and neuroscience.
The Illustris simulation recreates the evolution of the universe with unprecedented resolution, including spiral galaxies, elliptical galaxies, and large-scale structures. It also accurately models chemistries of individual galaxies, offering a realistic view of cosmic evolution.
Researchers found a runaway star cluster named HVGC-1 in the M87 galaxy, moving at over two million miles per hour. The cluster was likely flung out of the galaxy by supermassive black holes at its core.
Researchers have made significant advancements in sensitivity and believe a dark matter particle interacts with ordinary matter rarely, according to conference discussions. The hunt for dark matter continues, with the LHC yet to find evidence of supersymmetry, but potential discovery could reveal dominant form of universe-seeding matter.
Researchers at Northwestern University are observing the closest approach between Sgr A*, a supermassive black hole, and gas cloud G2, which could reveal insights into black hole growth. The data from Chandra X-ray Observatory and Very Large Array may provide clues about the feeding habits of these massive objects.
Researchers from BICEP2 collaboration announce groundbreaking discovery of cosmic inflation, providing first direct image of gravitational waves. The data also confirm a deep connection between quantum mechanics and general relativity.
The study provides new insights into stellar nurseries, showing that high-mass stars form in groups rather than alone and that these seeds can be fragmented into individual star seeds early in the formation process.
The five Neimark Award winners explore biostatistics, molecular plant sciences, and particle astrophysics among other areas. Their research in second language acquisition also sheds light on human cognition.
The asteroid belt's diverse composition suggests that giant planets' migrations reshaped the solar system, potentially delivering water to Earth and influencing its habitability. Small asteroids show particularly varied compositions, suggesting a complex history of collisions and re-deposition.
A team of researchers has confirmed a long-standing puzzle about the birth of massive stars, showing that dense filamentary structures absorb ultraviolet radiation and shield surrounding gas. The findings provide new insights into how massive stars form and influence their host galaxies.