Astronomers have discovered that the Milky Way's stars are moving in unexpected ways, suggesting a recent encounter with a small galaxy or dark matter structure. The team found a north-south asymmetry in the distribution of stars, which may be caused by a vertical wave formed by the object's passage.
Recent studies with the Green Bank Telescope indicate that two neighbor galaxies may have had a close encounter. The discovery confirms a disputed finding from 2004 and shows six dense clumps of gas in the stream, strengthening the argument that they are part of a bridge between the two galaxies.
The Milky Way is destined for a head-on collision with the Andromeda galaxy in 4 billion years. Computer simulations show that stars will be thrown into different orbits around the new galactic center, and our solar system may be tossed farther from the core.
A recent study proposes that up to 100,000 nomad planets might exist in the Milky Way Galaxy for every star, with an estimated quadrillion number of total nomads. If confirmed, this could mean nomad planets play a significant role in the universe.
Research suggests hundreds of billions of free-floating, Earth-sized life-bearing planets exist between stars in the Milky Way. These 'missing mass' planets could mix cosmic primordial life on a galaxy-wide scale.
Astronomers discovered that hot Jupiter-type planets are likely to have no companions in their systems, supporting the theory of a close encounter with another body causing orbital elongation. This study used Kepler mission data and found compelling evidence for companion planets around warm Jupiters and hot Neptunes.
Astronomers at Queen's University Belfast have gathered direct evidence of a supermassive black hole shredding a star that wandered too close. The discovery provides insights into the harsh environment around black holes and the types of stars swirling around them.
Astronomers have discovered a group of over 675 hypervelocity stars on the outskirts of the Milky Way, which are believed to have been ejected from the galactic core. These stars, found in intergalactic space between the Milky Way and Andromeda galaxy, exhibit high metallicity indicating an inner galactic origin.
The closest large elliptical galaxy to the Milky Way, Centaurus A has a twisted disc of dust near its centre, formed from a cosmic collision with another galaxy. The galaxy's powerful heart features two massive jets streaming from a massive black hole, emitting strong radio emission and visible in far-infrared images.
New research reveals that supermassive black holes can double in mass by ripping apart double-star systems and swallowing one of the stars. This process is thought to be the dominant method for growing these massive objects.
A University of Utah astrophysicist has proposed that supermassive black holes in galaxy centers grow by consuming single stars from wandering binary pairs. The study found that this process is an efficient way to bring stars close to black holes, outperforming gas clouds as a growth mechanism.
The Baryon Oscillation Spectroscopic Survey (BOSS) has made precision measurements of the large-scale structure of the universe five to seven billion years ago. By using a technique called baryon acoustic oscillation, BOSS can determine the distances to faraway galaxies with unprecedented accuracy.
Researchers have identified hypervelocity planets and stars that are ejected from the Milky Way at millions of miles per hour due to their close interaction with a massive black hole. The study suggests that these high-speed objects can provide valuable insights into planetary formation and evolution near the central black hole.
Astronomers captured a unique image of over 10,000 stars in the Milky Way's centre, revealing large structures like gas and dust clouds. The image, created by combining infra-red light data from two telescopes, offers new insights into the galaxy's structure.
The discovery of the most distant galaxy cluster reveals that it is located 10.5 billion light-years away from our Milky Way galaxy and contains a dense concentration of 30 galaxies. This finding provides insights into the evolution of galaxy clusters and the formation of large urban centers in the universe's earliest moments.
A team of researchers from MIT has detected tellurium, a rare Earth element, for the first time in three ancient stars. The finding supports the theory that tellurium and other heavy elements likely originated from a rare type of supernova during nuclear fusion.
McMaster University's Christine Wilson presents findings on galaxy Arp 220's dazzling rate of star formation, which is 200 times faster than our own Milky Way. The star forming core of Arp 220 is only about 3,000 light years across.
These powerful telescopes enable forefront research in astrophysics, unlocking the secrets of star- and planet-formation processes. The new facilities will study gas and dust motion around young stars, testing theories of planet formation.
The study suggests a massive cloud of trillions of asteroids and comets surrounds Sgr A*, where they are vaporized by friction as they pass through the hot gas flowing onto the black hole. The flares observed by Chandra could be explained by the frequent collision of asteroids with the black hole.
Researchers at the Max Planck Institute for Astrophysics have created a high-precision map of the Milky Way's magnetic field using radio observations from over 30 researchers and 41,000 measurements. The map reveals both large-scale and small-scale features of the Galactic magnetic field, including turbulence in the gas.
The CalTech-led Catalina Real-Time Transient Survey has released a massive dataset of 200 million celestial objects, including stars, supernovae, and asteroids. This unprecedented data set will enable scientists to study the evolution of stars, massive black holes, and the structure of the Milky Way.
The new data set contains the brightness histories of two hundred million stars and other objects, incorporating over 20 billion independent measurements. This extensive dataset enables numerous studies by the astronomical community.
The Hubble Space Telescope has created the sharpest visible-light image ever made of the nucleus of an external galaxy, the Andromeda galaxy. The blue stars surrounding the massive black hole are just 200 million years old and formed in a burst of star formation near the black hole.
The discovery of three smallest confirmed planets ever detected outside our solar system may boost the likelihood of existence of habitable planets. The planets, all rocky with a solid surface, orbit a small star called KOI-961, which is similar to red dwarfs, the most common type in the Milky Way.
A team of astronomers using gravitational microlensing detected three exoplanets, including a super-Earth and planets comparable to Neptune and Jupiter. Combining this data with previous findings, the researchers conclude that planets are more common than stars in the Milky Way.
Most of the Milky Way's 100 billion stars have planets similar to Mercury, Venus, Earth and Mars. The research found an average of 1.6 planets in the habitable zone around each star.
Astronomers are observing a unique opportunity to study how a black hole gulps gas, dust, and stars as it grows bigger. The gas cloud is currently 550 Kelvin or 280 degrees Celsius and will be ripped apart by the tidal forces around the black hole.
Astronomers have discovered two gigantic black holes with masses about 10 billion times the mass of our sun, surpassing previous measurements by more than 50 per cent. The discovery suggests that these massive black holes may be the dormant remains of extremely luminous quasars from billions of years ago.
Galaxies continuously recycle immense volumes of hydrogen gas and heavy elements, allowing successive generations of stars to form. The process is driven by gas-rich star-forming spiral galaxies that can evolve into elliptical galaxies without star formation.
Researchers have discovered that ancient stars in the Milky Way's halo contain abnormally large amounts of heavy elements like gold and uranium. By analyzing the motions of these stars, they found evidence suggesting that exploding supernovae may have sent jets of enriched gas into space, creating the heavy-element rich stars.
Astronomers have uncovered an extraordinary population of young dwarf galaxies brimming with star formation, forcing a re-evaluation of their understanding of galaxy evolution. These galaxies are estimated to be 9 billion years old and produce stars at rates 100 times faster than the Milky Way.
A team of researchers measured the bar length of over 5,000 galaxies using amateur astronomers' data from the Galaxy Zoo project. The study reveals that redder galaxies have longer bars and are more likely to display spiral arms.
A new theory suggests that high-speed collisions between planets and asteroids near supermassive black holes create microscopic dust clouds. This process blocks harmful radiation, creating a more hospitable environment for life in the galaxy's central region.
Galaxy collisions may be a key process driving galaxy assembly, rapid star formation, and accretion of gas onto central black holes. New analysis combines Hubble images with supercomputer simulations to estimate merger rates, clearing up discrepant results from previous studies.
A new study suggests that short-hard interstellar radiation events could have a significant impact on life on Earth, depleting the ozone layer and allowing deadly ultraviolet radiation to penetrate. The rate of these events is estimated to be about once per 100 million years, with potential effects on extinctions in the fossil record.
Researchers at Princeton University and NYU have developed a method to detect the collision of stars with primordial black holes, which are believed to be a source of dark matter. The new technique uses existing solar observation methods to identify subtle vibrations in a star's surface caused by a passing black hole.
A supercomputer simulation by University of Pittsburgh researcher Christopher W. Purcell suggests that the Milky Way's spiral arms were triggered by a collision with the Sagittarius Dwarf galaxy. The impact stripped off 80-90% of the dark matter halo, producing instabilities that eventually formed the spiral arms and ring structures.
Researchers discover that a dwarf galaxy may have created the Milky Way's spiral arms through a collision with our galaxy. Astronomer Curtis Struck cautions that these collisions can have significant effects on galaxy growth and evolution.
Researchers at UC Irvine discovered that the Milky Way's spiral arms are a result of an intergalactic collision course with a dwarf galaxy named Sagittarius. The force of the impact sent stars streaming from both galaxies into long loops, which were then swelled and tugged outward by the Milky Way's rotation.
Astronomers propose a new way to search for supernova precursors by studying the spin of white dwarfs. This process could lead to a time delay of up to a billion years before the explosion, allowing for detection by upcoming surveys.
Researchers at University of California, Santa Cruz and Institute for Theoretical Physics in Zurich simulate formation of massive spiral galaxy like Milky Way, resolving key features with high-resolution simulation. The result supports prevailing cold dark matter theory, which predicts galaxies form within dark matter halos.
Astronomers have detected a planet orbiting a rapidly spinning pulsar, dubbed PSR J1719-1438. The discovery suggests that the planet is composed primarily of carbon and oxygen, likely forming a diamond-like material due to its high density.
A new study by Nicolas Lehner and Christopher Howk reveals that massive clouds of ionized gas in the Milky Way's halo are a reservoir of fuel for galactic star formation. The researchers measured the distances to these clouds using the Cosmic Origins Spectrograph on the Hubble Space Telescope, confirming models that predicted gas falli...
Astronomers have discovered a massive reservoir of water vapor 30 billion light-years away in a quasar, which is 100,000 times more massive than the sun. The water vapor is distributed around a black hole and provides insights into its environment.
Astronomers have found the largest and farthest reservoir of water ever detected in the universe, located in a distant quasar with a massive black hole. The discovery provides valuable information about the early universe's water vapor behavior and its influence on cosmic evolution.
Astronomers discovered a massive black hole in a distant galaxy that ripped apart a star, creating a powerful beam of energy that crossed 3.8 billion light years to Earth. The extreme brightness of this event was due to the small fraction of the sky illuminated by the jet of light towards the Milky Way.
Researchers have found that galaxies previously thought to be dead and devoid of star formation are actually still producing new stars. Using the Hubble Space Telescope, scientists observed individual young stars and clusters in four galaxies, revealing an average star-formation rate of one sun every 10,000 years.
The discovery of blue stragglers in the Milky Way's hub suggests that the galaxy stopped making stars billions of years ago. The findings provide new constraints for models of the star-formation history of the bulge.
The Milky Way belongs to a rare subset of galaxies with two satellites as bright and close by as the Large and Small Magellanic Clouds. Researchers analyzed over 20,000 galaxies similar to the Milky Way using the Sloan Digital Sky Survey data.
Researchers found that just four percent of galaxies are similar to the Milky Way, with two satellites as bright and close by as the Magellanic Clouds. The study used data from the Sloan Digital Sky Survey and computer simulations to understand how the Milky Way fits into the broader context of the universe.
The Hubble Space Telescope has observed the historic variable star V1, which helped confirm the size of the universe and its expansion. The observations, conducted in collaboration with amateur astronomers, provide new insights into the properties of Cepheid variables and their role in measuring distances to galaxies.
Astronomers have updated the census of sun-like stars with data from NASA's Kepler Mission, detecting changes in brightness in 500 stars. This provides a much better understanding of the stars' properties and their evolution, allowing for detailed measurements of star basics such as mass and age.
Astronomer Heidi Newberg is using a new $382,000 NSF grant to map the distribution of dark matter in our galaxy. She will utilize the massive computing power of the international MilkyWay@Home project to simulate how stars in stellar streams got to their current positions.
Researchers have discovered a thick stellar disc in the Andromeda galaxy, composed of older stars with distinct chemical and orbital properties. This finding sheds light on the formation and evolution of spiral galaxies like our own Milky Way.
Researchers develop method to locate satellite galaxies based on hydrogen gas distribution, predicting Galaxy X's mass and location. The technique has broad implications for dark matter detection and alternative gravity theories.
Elliptical galaxies are found to contain five to ten times as many red dwarfs as thought, with implications for galaxy formation and evolution. The discovery could lead to a reevaluation of dark matter in these galaxies.
Astronomers at Yale University have discovered that small red dwarfs are much more prolific than previously believed, increasing the total number of stars in the universe. The discovery found 20 times more red dwarfs in elliptical galaxies than in the Milky Way, with potential implications for galaxy formation and evolution.
Astronomers have discovered a planet from another galaxy orbiting a star that has entered our Milky Way, providing the first confirmed detection of an extragalactic exoplanet. The planet, HIP 13044 b, was detected using high-resolution spectrograph FEROS attached to the MPG/ESO telescope at ESO's La Silla Observatory.
Astronomers from Bonn and St. Andrews discover that the discrepancy between calculated and observed star numbers may be due to an overestimation of stellar crowding, a phenomenon where young stars are born in groups, leading to more massive stars being overlooked.
The telescope discovered two gamma-ray-emitting bubbles that span 50,000 light-years north and south of the galactic center