Two Iowa State University astronomers are using Spitzer Space Telescope data to study big cool-temperature stars and dusty disks. The telescope is also identifying regions within the Milky Way that are forming intermediate-mass stars.
A new study using Spitzer data reveals a large amount of dust around three mature double-star systems, possibly resulting from planetary collisions. The research suggests that tight double-star systems might not be suitable for life to thrive due to the increased likelihood of chaotic events.
Scientists have discovered a star with a mass of 265 solar masses in the Large Magellanic Cloud, exceeding previous records. This finding raises questions about the formation process of such massive stars and their role in shaping the universe.
Astronomers have detected a wave of massive star formation within the M17 SWex dark cloud, revealing 488 newly forming stars, including 200 blue-white class B stars. The discovery sheds light on how and when massive stars form, with theories suggesting an expanding shock wave or later formation may be necessary.
Researchers at Durham University use huge computer simulations to recreate the beginnings of the Milky Way, finding that many ancient stars originated from smaller galaxies torn apart by galaxy collisions. The simulations provide a blueprint for galaxy formation and reveal clues to the early history of the Milky Way.
A new study suggests that many well-known comets, including Halley and Hale-Bopp, may have formed in orbit around other stars. The Sun is believed to have captured small icy bodies from its sibling stars, creating a reservoir for observed comets.
Newberg's team will use LAMOST data to plot the position, speed, and composition of over 7 million stars, shedding light on dark matter distribution and galaxy formation
An international team of astronomers will conduct a closer look at the mega star birthing cloud, located 8,000 light years away in the Southern sky constellation Carina. The cloud is collapsing in on itself, offering an unusual view into behemoth star birth and providing insights into the formation of our solar system.
Researchers have discovered a massive cloud of cosmic gas and dust collapsing in on itself, which could help solve the mystery of massive star formation. The CSIRO radio telescope detected two types of molecules indicative of collapse, suggesting the gas is falling at an incredibly high rate.
Research from the University of Manchester and Western Sydney found that sports stars' behavior has little impact on young people's drinking habits. Young people tend to overestimate their friends' drinking, with actual drinking levels influenced more by sport-specific cultural habits.
A massive galaxy in the early Universe created stars like our sun at a rate equivalent to 250 suns per year, researchers say. The team observed four star-forming regions within the galaxy, each over 100 times brighter than similar regions in the Milky Way.
Researchers have solved a 20-year-old astrophysical puzzle using gas dynamical simulations. Filamentary structures formed during the collapse of infalling gas absorb massive stars' radiation, shielding surrounding nebulae from heating.
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.
Scientists have discovered a relic star from the early universe, which has a remarkably similar chemical composition to the Milky Way's oldest stars. The discovery supports the theory that our galaxy underwent a 'cannibal' phase by swallowing smaller galaxies and other galactic building blocks.
Astronomers have found that typical galaxies still hold sufficient quantities of gas and dust for star formation, but their efficiency has slowed down over cosmic time. This means that present-day galaxies form fewer stars due to a decrease in gas and dust supplies rather than a change in their ability to make stars.
A team of researchers has resolved a long-standing conflict in the theory of galaxy formation, using millions of hours of supercomputer simulations. The study reveals that cosmic explosions, such as supernovas, play a key role in preventing the formation of stars and dark matter at the centers of dwarf galaxies.
Researchers found blue stragglers with different properties, indicating both collision-induced and vampirism-based formation. These findings provide direct evidence of star cluster dynamics on stellar evolution.
Astronomers have discovered that blue stragglers, which appear youthful despite being older than expected, steal mass from companion stars through stellar smashups. In a star cluster, binary systems brush up against each other, sometimes leading to collision-course orbits and the formation of more massive stars.
Astronomers found two types of blue stragglers that defy aging: those rejuvenated by cosmic collisions and those formed by vampirism. The latter is thought to be caused by a smaller star siphoning hydrogen from its companion, while the former occurs in nearly head-on collisions where stars merge, mixing their nuclear fuel.
Researchers have discovered two new planetary systems with low-mass 'super-Earths' orbiting nearby sun-like stars. The planets are smaller than previously discovered worlds and may be habitable.
A faint star Alcor has been found to have a smaller red dwarf companion, orbiting it every 90 years. The discovery was made using the 'common parallactic motion' technique developed by Project 1640, which measures the movement of nearby stars relative to more distant ones.
A new study led by CU-Boulder suggests that the first large black holes in the universe formed and grew inside gigantic, starlike cocoons. These cocoons likely prevented surrounding gases from being blown away and smothered powerful x-ray radiation.
A new time-lapse movie shows the birth of massive stars in Orion's Great Nebula, revealing signs of rotating accretion disk and outflow streams. The data suggest magnetic fields may play a crucial role in star formation.
Researchers have found two Earth-sized bodies with oxygen-rich atmospheres, which are not planets but rather unusual white dwarf stars. The discovery was made using data from the Sloan Digital Sky Survey and suggests that these stars may have descended from massive progenitor stars.
Astronomers have discovered that Sun-like stars with planetary systems tend to have lower levels of lithium than those without planets. The study, which analyzed 500 stars, found that planet-bearing stars had less than 1% of the lithium present in other similar stars.
Scientists at Durham University discovered rapid star formation in 'stellar nurseries' of infant galaxies, creating new stars at a rate 100 times faster than expected. This finding provides insight into the birth of our own galaxy and how it formed its first stars.
Researchers at CU-Boulder are developing a precise laser ruler to measure tiny changes in infrared light caused by the gravitational wobble of small, cool stars as they interact with rocky planets. The technique will allow them to detect Earth-like planets around M stars, which are much more common than larger stars.
New research suggests that dirty stars with a high abundance of elements like iron and oxygen are more likely to host planets. The study's findings support the idea that the composition of a star reflects its disk, leading to an increased number of exoplanets around such stars.
The mosaic image reveals stellar evolution, bright young stars, and a supermassive black hole at the Galactic center. Giant X-ray flares from Sgr A* have occurred about 50 and 300 years earlier.
Researchers used high-resolution spectrograph to reveal unexpected tilt of up to 70 degrees from vertical in binary star DI Herculis. The discovery resolves longstanding mystery and sheds light on formation and evolution of binary stars, with implications for Einstein's theory of relativity.
Astronomers, including Queen's University physicist Larry Widrow, have discovered a nearby cosmic encounter between the Andromeda and Triangulum galaxies, which collided about two to three billion years ago. The collision caused millions of stars to be ripped from the Triangulum disk, forming a faint stream visible in the PAndAS data.
A team of international researchers has challenged the long-held idea that the ratio of massive stars to lighter ones in star-forming regions remains consistent. They found that this ratio, known as the initial mass function, varies significantly between different galaxies, with some forming more low-mass stars than expected.
A NASA/Goddard Space Flight Center simulation found that the universe's first black holes grew slowly due to a lack of gas, contrary to expectations. The findings have significant implications for understanding galaxy formation and the role of black holes in shaping the universe.
Researchers measured the motion of stars in a distant galaxy and found they are moving at incredible speeds, contradicting expectations of small galaxy size.
Researchers created a detailed computer simulation of early star formation, revealing the existence of twin stars. The simulations showed that these stars provide seeds for next-generation star formation, helping scientists understand how galaxies formed.
Astronomers at the University of Hawaii have discovered a binary star-disk system with two stars surrounded by dust disks capable of forming planetary systems. The system, 253-1536, is the first known example of two optically visible stars with enough mass to form an Earth-like planet.
The AUA Foundation has awarded the 2009 Astellas Rising Stars in Urology to William Roberts, MD and Edward Schaeffer, MD for their groundbreaking research projects on Benign Prostatic Hyperplasia and Phospholipase A2 signaling in prostate development. The award aims to support young urologists in pursuing careers in urologic research.
Astronomers from Queen's University Belfast have proposed a new physical interpretation of the 2008 supernova SN2008ha, suggesting it could be from a massive star. The team, led by Dr. Stefano Valenti, found a weak explosion with unusual properties that differ from those associated with white dwarf stars.
Researchers discovered that ultracool subdwarfs have unique and diverse orbits around the Milky Way, with some stars traveling at speeds of over a million miles per hour. One star may be an intergalactic visitor, originating from another galaxy.
Researchers at UBC found that warmer, more acidic waters enable Purple Ochre Sea Stars to grow twice as fast as normal over 10 weeks. This discovery complicates current assumptions about climate change's impact on marine species.
Tabetha Boyajian, a GSU astronomy graduate student, has been awarded the prestigious Hubble Fellowship to pursue postdoctoral research on stellar sizes and planetary systems. She will use the CHARA Array to measure the size of stars and determine their effective temperature, shedding light on the habitable zones of planets.
Astronomers have found evidence of planet destruction caused by a star's tides, with some planets falling into their parent stars. The research uses computer models and observations to show that the tidal forces can misshape the star's surface, leading to the planet's demise.
Researchers have proven that supernovae are caused by the explosion of two dying red supergiant stars, providing a breakthrough in understanding massive star death and the formation of chemical elements. This discovery sheds light on the origin of the universe's heaviest elements.
In a groundbreaking study, scientists have discovered that stars were forming at an incredible rate in the core region of an infant galaxy. With a diameter of just 4000 light-years, the star-forming core of J1148+5251 is incredibly productive and reaches its physical limit.
Researchers found evidence of cosmic dust forming around a dying star in a nearby galaxy, similar to those that formed soon after the Big Bang. This discovery provides insight into the early stages of the Universe and challenges the long-held theory that supernovae explosions are the primary source of dust.
A Cornell-led team has observed dust forming around a dying star in a nearby galaxy, providing insights into the early universe and the evolution of galaxies. The discovery sheds new light on how cosmic dust was created in the universe's early stages.
Researchers at Lawrence Livermore National Laboratory have found a way for massive stars to grow despite radiation pressure that should prevent it. Gravitational instabilities cause companion stars to form around massive stars, allowing them to feed on gas and dust.
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.
Researchers found that blue stragglers are the result of 'stellar cannibalism' where plasma is gradually pulled from one star to another to form a massive, unusually hot star. This process takes place in binary stars and helps resolve a long-standing mystery in stellar evolution.
A team of scientists discovered that blue stragglers, massive rogue stars found in globular clusters, are formed through a process known as stellar cannibalism. This theory is supported by observations of over 50 globular clusters and suggests that binary star systems play a key role in the formation of these stars.
The team found a cosmic puzzle that booms six times louder than predicted, ruling out origins from primordial stars and known radio sources. The source of this cosmic radio background remains a mystery, complicating efforts to detect the first stars in the universe.
Researchers identified two protostars located just a few light-years from the Milky Way's central black hole, defying expectations that gravitational tides would prevent star formation. The discovery suggests molecular gas at the galactic center is denser than previously thought, allowing it to form new stars.
A new study found that gas giants like Jupiter must form extremely fast, in less than 5 million years, or they won't form at all. This rapid growth spurt is necessary because the material from which they formed probably disappeared within a few million years.
The University of Virginia is conducting a new project, APOGEE, as part of the Sloan Digital Sky Survey III to study the chemical and dynamical fingerprints of Milky Way red giant stars. The team aims to understand the assembly of the Milky Way galaxy and its evolution.
Astronomers discovered strong evidence that brown dwarfs form like stars using the Submillimeter Array. Brown dwarfs are on the line between planets and stars with masses between 15 and 75 Jupiters.
A team of Australian astronomers discovered a puzzling lack of hydrogen gas in distant galaxies, which contradicts expectations based on the Universe's life cycle. The observed absence may be due to the destruction of hydrogen by quasars' intense radiation, leaving behind only ionised particles.
Researchers will use chromospheres to measure star ages by studying sunspots and solar cycles. The team aims to extend the activity-age relation for solar-type stars up to the Milky Way's age, about 10 billion years.
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.
A team of astronomers discovered a new planet closely orbiting the giant star HD 102272, nearly six times the mass of Jupiter. The planet's location near the star raises questions about how aging stars influence nearby planets.
Researchers analyzed data from the CoRoT space telescope mission, finding that three nearby stars have larger vibrations and finer surface texture than our Sun. The study provides valuable information about the physical properties of nearby stars and sheds new light on the Sun's interior.