Researchers found that stars in large middle-aged clusters are of similar age, suggesting a complex formation process. The discovery challenges current understanding of stellar evolution and may require re-evaluation of models.
Researchers have made significant breakthroughs in understanding galaxy evolution by modeling the effects of stellar activity on star formation. By running complex supercomputer simulations, they found that feedback from stars plays a crucial role in regulating galaxy growth.
Planets close to low-mass stars may have formed with water and atmospheres burned away, reducing habitability. These 'Mirage Earths' could resemble Earth from afar but lack essential components for life.
A new virus, Sea Star Associated Densovirus (SSaDV), has been identified as the cause of a widespread disease affecting sea stars along the Pacific Coast. The study found that the virus was present in museum specimens dating back to 1942 and had likely existed at low levels for over 72 years.
A genomic analysis of a newly discovered virus prevalent in symptomatic sea stars has linked Sea Star Associated Densovirus to the devastating wasting disease, potentially triggering an unprecedented ecological upheaval. The research lays the groundwork for understanding how the virus kills sea stars and what triggers outbreaks.
Astronomers find compact, young galaxies shut down their prodigious star production due to a lack of cool dense gas, rather than supermassive black holes. The energy from the star formation itself creates a shortage of gas within the galaxy.
Researchers detected a diffuse cosmic glow originating from stripped stars flung out into space after galaxies collided and merged. The findings suggest previously undetected stars permeate dark spaces between galaxies, forming an interconnected sea of stars.
A team led by Andrea Ghez determined that G2 is most likely a pair of binary stars that had been orbiting the black hole in tandem and merged together into an extremely large star. The research suggests that many of the stars at the center of the galaxy are massive and mostly binaries.
The Hubble Space Telescope has observed the faint glow of stars ejected from ancient galaxies torn apart within the Pandora's Cluster. The scattered stars are estimated to contribute approximately 10% of the cluster's brightness and are rich in heavier elements.
Researchers at Johns Hopkins University found that massive black holes can block the formation of new stars in mature galaxies. The study suggests that these jets of radio-frequency feedback streaming from central black holes prevent hot gas from cooling and collapsing into baby stars.
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.
Astronomers have discovered a pulsating, dead star beaming with the energy of about 10 million suns. Pulsars are dense stellar remnants leftover from supernovas, and this one is the brightest ever recorded.
Researchers used simulations to study primordial supermassive stars that may have exploded as supernovae, leaving no black hole behind. This process could create a distinct observational signature detectable by upcoming telescopes and enrich their host galaxy with heavy elements.
A long-term laboratory experiment showed that young sea stars grow more slowly and eat less in acidic conditions, even after a prolonged acclimation period. The study suggests that young sea stars may not adapt to the effects of ocean acidification, potentially affecting entire ecosystems.
Researchers found a star with extremely low iron content, which could be evidence of the universe's first supernovae. The star's unusual chemical composition supports the theory that massive stars formed in the early universe and exploded as supernovae.
New modeling studies show most stars were formed from unstable protostar clusters that broke up, leaving behind single or binary stars. These clusters, however, rarely form stable multi-star systems, instead ejecting stars to achieve stability.
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.
Astronomers used computational simulations to show that rapid mixing in cloud formation creates uniform chemical composition among born stars, supporting the idea of 'chemical tagging' and potential discovery of Sun's siblings. The study also found that even clouds without many stars produce similar abundances.
A study published in Nature found that the chemical uniformity of stars in the same cluster is due to turbulent mixing in star-forming clouds. This mixing occurs before much of the gas has turned into stars, resulting in nearly identical chemical signatures among sibling stars.
Astronomers used a global network of radio telescopes to measure the distance to the Pleiades star cluster, resolving a long-standing controversy. The result is a precise measurement of 443 light-years, accurate to within one percent.
Astronomers have observed the earliest stages of massive galaxy construction, dubbed 'Sparky', which contains about twice as many stars as our Milky Way. The discovery was made possible through combined observations from NASA's Hubble and Spitzer space telescopes.
Researchers at Lund University found that toothpaste fluorine is formed in stars similar to our sun, supporting a theory about its origins. By analyzing light emitted by stars, they calculated the amount of fluorine present and compared it with predictions.
Dallas high school students Dominik Fritz and Jason Barton discovered five new variable stars as part of the SMU QuarkNet program, analyzing data from a telescope in New Mexico. The discoveries have been accepted into the VSX catalog and will be forever linked with their students' names.
A new study by Cornell University researchers found that the Guiding Stars System brands items with zero, one, two or three star rating leads to a decline in sales of less healthy foods. Sales of healthy food purchases rose by 1.39% while 'junk food' sales fell by 8.31%. This trend may be due to consumers making healthier choices.
A team of astronomers has created new maps of the interstellar medium in the Milky Way, revealing clues about the composition and distribution of mysterious complex molecules. The findings could provide insights into how stars form and the conditions that lead to their creation.
Researchers at the University of Warwick found that white dwarf stars crashing into neutron stars could be responsible for the loneliest supernovae. The team used observations from the Very Large Telescope and Hubble Space Telescope to rule out other explanations, such as binary systems or massive stars.
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.
A team of 20 scientists monitored the 'heartbeats' of young stars using data from two space telescopes. They found that emerging stars pulsate slowly at first, then faster as they near ignition, revealing insights into their internal structures and ages.
Astronomers have developed a method to distinguish between infant and adolescent stars based on their sound waves, with 'young' stars vibrating slower. This technique uses ultrasound technology similar to medical applications, offering new insights into star formation and evolution.
New observations from NASA's Hubble Space Telescope reveal small galaxies are responsible for forming a significant number of the universe's stars. This finding supports a decade-long investigation into the relationship between a galaxy's mass and its star-forming activity, providing new insights into the early universe's history.
Two low-cost, car battery-sized Canadian nanosatellites are part of the BRITE-Constellation project, monitoring brightness and color variations of brightest stars. The satellites will uncover clues about star origins, including our Sun and Earth.
A historic epidemic of sea star wasting syndrome has exploded along Oregon's coast, with 30-50% of ochre sea stars affected and potentially leading to local extinctions. The outbreak could disrupt the marine intertidal ecosystem, causing widespread damage.
Scientists detect the first Thorne-Żytkow object, a bizarre type of hybrid star formed from red supergiant and neutron stars. The discovery provides evidence for a new model of stellar interiors and offers insights into heavy element production in the universe.
Scientists identified the mix of elements thrown off by the star before its explosion, which helped paint a picture of how heavy elements in the universe are formed. The findings revealed a nitrogen-rich wind similar to those of Wolf-Rayet stars, providing a window into the workings of the cosmos.
A team of astronomers has identified a Wolf-Rayet star as the probable progenitor of a recently exploded supernova using flash spectroscopy. This technique allows for rapid identification of pre-explosion stars at greater distances than previously possible.
Researchers have developed a model to estimate the effect of Earth-like planet ingestion on star chemical composition. By analyzing twin stars with planets, they found significant changes in refractory element abundance, supporting the connection between exoplanets and stellar hosts.
Researchers have detected circularly polarized light from a recently formed black hole, confirming a theoretical model. The discovery was made using the VLT telescope and is considered an extraordinary event due to its high degree of polarization.
Astronomers have found the closest, second-brightest hypervelocity star, speeding at 1 million mph. The star probes the supermassive black hole at the galaxy's center and the halo of mysterious dark matter, providing insights into the galaxy's structure.
Modjaz will observe host environments of stellar explosions to investigate which kinds of stars have exploded and why. Her research aims to determine the make-up of stellar progenitors that yield stripped envelope supernovae and gamma-ray bursts.
New research from UT Arlington suggests that F-type stars may be a good place to look for habitable planets due to their wider habitability zone. The study found encouraging results, with some damage estimates similar to those on Earth, if an atmosphere is assumed.
Researchers at SISSA have discovered that neutron stars can be described with just three parameters: mass, angular momentum, and quadrupole moment, independent of the equation of state. This finding has major implications for understanding these complex objects.
A team of astronomers discovered mature galaxies at a record-breaking distance, containing 100 billion stars each. These galaxies formed rapidly over 1 billion years, with star formation rates hundreds of times higher than observed today.
The spiral galaxy ESO 137-001 is zooming through the Norma cluster at nearly 4.5 million miles per hour, stripping gas from its home and forming new stars in intergalactic space. Astronomers hope that studying this galaxy can help them understand how galaxies form stars and evolve over time.
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.
Researchers from the Niels Bohr Institute detected a stream of stars in Andromeda II, revealing a remnant of a merged dwarf galaxy. The findings provide insight into the rare event of low-mass galaxy mergers, which are expected during galaxy formation.
A team of astrophysicists has created the first-ever map of radioactive material in a supernova remnant using NuSTAR. The findings suggest that massive dying stars likely rip apart with distorted shock waves, ending their lives.
Researchers found that strongly interacting binary stars are necessary for powerful, bipolar jets of gas and dust to form in planetary nebulae. The jets are produced by accretion processes that provide fuel for the outflows.
The discovery of the oldest known star in the Universe allows scientists to study its chemistry, providing a clearer idea of the early universe. The ancient star is around 6,000 light years from Earth and formed shortly after the Big Bang.
Circumbinary planets are thought to have formed far from their binary star systems before migrating to their current location. Researchers used computer simulations to model the early stages of planet formation around Kepler-34(AB)b and found that the majority must have formed much further away.
Scientists discovered that massive galaxies in the early universe were formed by explosive star formation triggered by galaxy collisions. This theory contradicts the traditional view that galaxies grew larger over time through constant star formation and mergers.
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.
Researchers found that star radiation can push matter out of galaxies, accounting for the missing galactic mass in previous calculations. The FIRE simulations demonstrate that feedback from stars alters galaxy growth and history in a dramatic way.
An international team of astronomers has discovered a surprising new class of hypervelocity stars moving fast enough to escape the gravitational grasp of the Milky Way galaxy. The new stars are relatively small and have different ejection mechanisms than previously discovered hypervelocity stars.
Astronomers are studying the newly formed stars in M83 using citizen science project STAR DATE: M83. The project aims to estimate ages for approximately 3000 star clusters. Citizen scientists analyze the image to identify objects such as supernova remnants and foreground stars, shedding light on stellar birth and death.
The Hubble Space Telescope has revealed a glittering treasure trove of more than 800,000 stars and protostars embedded inside the Tarantula Nebula. The observations were obtained as part of the Hubble Tarantula Treasury Program, which will produce a large catalog of stellar properties.
The Gemini Planet Imager has successfully captured its first light images of exoplanets, allowing scientists to study their atmospheres and characteristics in unprecedented detail. The instrument's advanced technology enables it to detect planets that are millions of times fainter than their parent stars.
AAS meeting highlights four unusually bright galaxies, a galaxy cluster image, and sampling of galaxies thought to be responsible for most stars in the universe. These ultra-bright, young galaxies are forming stars approximately 50 times faster than our Milky Way galaxy.
Scientists discovered previously unseen binary companions to young protostars using upgraded VLA capabilities. The findings support the disk-fragmentation idea, which suggests double stars form when a gas and dust disk fragments, forming a new star in orbit with the first.
A study of massive stars confirms the Milky Way has four spiral arms, contradicting previous findings from NASA's Spitzer Space Telescope. The researchers used data from radio telescopes in Australia, USA and China to analyze the distribution of massive stars across the galaxy.