Articles tagged with Stars
The discovery of KOI-314c reveals a planet weighing as much as Earth but 60% larger in diameter, indicating a thick, gaseous atmosphere. The planet's mass was measured using transit timing variations (TTV), a young method for studying low-mass planets.
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.
The AGORA project aims to resolve inconsistencies in supercomputer simulations of galaxy evolution by comparing results from different codes and processes. By applying the principle of reproducibility, researchers hope to identify key physics ingredients that produce realistic galaxies.
A young star formed in the Milky Way galaxy underwent an explosive growth, becoming 100 times brighter than its current state within the past 100-1,000 years. This sudden increase was caused by a chemical reaction that enabled the formation of complex molecules like methanol.
Two teams of scientists used NASA's Hubble Space Telescope to detect faint water signals in the atmospheres of five distant planets. The strengths of their water signatures varied, with some planets having stronger signals than expected.
Researchers from HZDR simulated a plasma jet at high resolution, following the electrons in the jet. The simulation used enormous computing power to analyze billions of particles, enabling comparison with astronomical observations.
SPIRou, a near-infrared spectropolarimeter and high-precision velocimeter, will detect habitable Earth twins orbiting nearby red dwarf stars and study the formation of Sun-like stars and their planets. The instrument's advanced technology will reveal the existence of liquid water on planetary surfaces.
Astronomers at UMass Amherst and UT at Austin identify the most distant galaxy, with a redshift parameter of z = 7.51, indicating it is 700 million years old. The discovery challenges theories on galaxy formation and suggests intense star-forming galaxies may be more common than thought.
Researchers at MIT have discovered an exoplanet named Kepler 78b that is approximately 1.2 times the size of Earth and has a mass about 1.7 times that of our planet. The planet's density is also similar to Earth's, suggesting it may be composed mainly of rock and iron.
Researchers provide physical explanation for Larson's Laws, showing that three correlations are due to the same underlying physics of supersonic turbulence. The study uses six simulations to support this interpretation and sheds light on molecular cloud structure formation.
Researchers at Caltech's intermediate Palomar Transient Factory have detected a rare type of supernova in a nearby galaxy, providing evidence for the theory that it originated from a Wolf-Rayet star. Additionally, they found the afterglow of a gamma-ray burst, precisely locating its position using optical telescopes alone.
A team of researchers from MIT has generated the first map of clouds on an exoplanet, Kepler 7b, which reveals a dense layer of clouds on one hemisphere. The study suggests that this cloud cover creates an atmosphere conducive to further cloud formation and regulates the planet's temperature.
The recently discovered ultra-compact dwarf galaxy M60-UCD1 has a density of stars about 15,000 times greater than in the Milky Way. The galaxy's central bright X-ray source suggests a massive black hole weighing 10 million times the sun's mass.
Astronomers have discovered a massive population of globular clusters within Abell 1689, the largest number ever found. The study reveals that this galaxy cluster could contain over 160,000 globulars, with 10,000 identified in Hubble observations.
Researchers propose a new spatio-temporal model to investigate molecular cloud fluctuations and their pulsational dynamics. The model takes into account nonlinear gravito-electrostatic coupling, helping elucidate basic features of cloud collapse, star formation, and galactic structures.
Astronomers used ESO's VISTA telescope to create the best 3D map yet of the Milky Way's central bulge, revealing an X-shaped structure. The galactic bulge is composed of 22 million red giant stars that can be used as standard candles to measure distances.
Researchers Struck and Elmegreen found that the gravitational pull of young galaxy clumps is responsible for the smooth universal brightness profile in older disk galaxies. This process takes a few hundred million years to a few billion years, scattering stars from their original orbits.
A UNSW-led team is mapping the location of giant gas clouds in our galaxy, which can be up to 100 light years across. The research aims to understand how these clouds form and play a key role in the cosmic cycle of birth and death of stars.
Astronomers have found strong evidence that a galaxy's central black hole is blowing massive amounts of gas out of the galaxy, limiting its growth and rate of star formation. The process, observed in a galaxy called 4C12.50, is thought to be key to understanding how galaxies develop and regulate the growth of their central black holes.
A team of astronomers used NASA's Chandra X-ray space telescope to solve a long-standing mystery about super massive black hole accretion rates. They found that most SMBHs swallow very little cosmic material and instead reject hot gases due to their high temperatures.
Astronomers using NASA's Chandra X-ray Observatory have found that less than 1 percent of the gas within 26,000 light-years of the Milky Way Galaxy's giant black hole reaches its event horizon. Instead, most gas is ejected before it can brighten and emit X-rays.
Researchers at UC Berkeley propose that 'zombie vortices' play a crucial role in the birth of new stars. The team's computer models show how variations in gas density lead to instability, resulting in whirlpool-like vortices that help the star form.
Astronomers use Hubble to study distant galaxies 11 billion years ago, confirming the Hubble Sequence holds true as far back as 8 billion years. The study finds that all galaxies fit into different classifications of the sequence, with blue star-forming galaxies and massive red galaxies dominating at these early times.
Researchers have found that mature-looking galaxies existed 11.5 billion years ago, pushing back the timeline of galaxy formation by 2.5 billion years. This discovery confirms the Hubble Sequence, a classification system used to describe galaxy morphology, even at early stages of the universe's history.
Astronomers at Durham University developed a new way to measure supermassive black holes' spin, which is linked to their role in driving galaxy growth. The technique uses the distance between a black hole and its feeding disc to estimate spin.
A new UMD-led study suggests that a burst of star formation in galaxies can blow out most of the remaining gas, resulting in a long period of starvation. This process is crucial in understanding the universe's surprising paucity of high-mass galaxies.
Astronomers have tracked the orbital motion of 33,000 stars in one of the Galaxy's oldest globular clusters, offering new insights into the formation of the Milky Way. The study reveals two distinct generations of stars within globular cluster 47 Tucanae, differing in age by 100 million years.
Astronomers use ALMA to image a snow line around TW Hydrae, a young star 175 light-years away, providing clues about the early Solar System. The discovery sheds light on the role of snow lines in planet formation and potentially seeds life with essential organic molecules.
Researchers find that debris disks can produce narrow rings on their own, without the presence of a planet. Gas and dust interactions lead to clumping and pattern formation, making it harder for astronomers to detect planets.
For the first time, Hubble has measured the visible color of an exoplanet, revealing HD 189733b to be a deep azure blue due to its hazy and turbulent atmosphere. The planet's atmosphere is scorching with temperatures over 1000 degrees Celsius and features glass rain.
The NASA Hubble Space Telescope has confirmed the presence of a true blue planet, HD 189733b, by detecting changes in light color as it passes behind its star. The observations indicate a deep blue color due to a hazy atmosphere with high clouds containing silicate particles.
A team of astronomers has spotted a distant galaxy consuming nearby gas, which fuels star formation and drives rotation. This discovery supports the theory that galaxies pull in material to grow and form stars.
Researchers used CSIRO's Australia Telescope Compact Array to study distant star-forming clumps and discovered massive amounts of molecular hydrogen gas, a key fuel for star formation. The telescope's upgraded bandwidth and sensitivity enabled the detection of carbon monoxide, allowing scientists to estimate galaxy star-formation rates.
Cities are likened to social reactors and networks, attracting people and accelerating social interaction. The new framework predicts statistical relationships observed in thousands of real cities worldwide, providing insights into urban growth and development.
A team of scientists at the University of California, Irvine, has discovered a rare mega-galaxy dubbed HXMM01, which is 10 times larger than the Milky Way. The galaxy was formed after a 11-billion-year collision between two young galaxies and is rapidly fading away due to its own cataclysmic birth.
Researchers detected a surprising clutch of hydrogen clouds, each as massive as a dwarf galaxy, in the space between M31 and M33. The clouds were found to be traveling through space at velocities similar to their parent galaxies, suggesting they are independent entities.
A new study highlights how women credit themselves in joint success, finding that they undervalue their contributions when working with men but not with other women. The research contributes to a body of work on stereotypes affecting women in the workplace and underscores how gender influences individual performance expectations.
Astronomers discovered a rare galaxy that turns gas into stars with near 100% efficiency, outperforming even the most efficient engines. This highly tuned galaxy forms stars at a rate hundreds of times faster than our Milky Way, with the majority of its starlight emitted by a small region.
A team of astronomers at the University of Toronto propose a mechanism for forming very large stars, where baby stars are fed gas from surrounding older stars, allowing them to grow in mass. They observed evidence of this phenomenon in the Westerhout 3 cloud, located 6,500 light years from Earth.
Astronomers using NSF-funded South Pole Telescope and ALMA observatory discover galaxies producing stars at high rates, challenging previous understanding of galaxy formation. The discovery provides valuable data to refine computer models of star and galaxy formation in the early universe.
Researchers have discovered vigorous starbursts in young galaxies, indicating the universe produced stars much earlier than thought. The findings reveal a rate of star formation 1,000 times greater than today's Milky Way and provide new insights into the history of the universe.
Astronomers using ALMA telescope discover starburst galaxies earlier than thought, representing massive galaxies in energetic youth. These galaxies are forming 1,000 stars per year, compared to just 1 for the Milky Way, making them 'monstrous bursts of star formation'.
Astronomers found dust-enshrouded, star-forming galaxies that were previously unknown in the universe. The newly discovered galaxies produce stars at a prodigious rate, creating thousands of new suns annually.
Astronomers use ALMA to observe distant galaxies that churned out tens of thousands of stars each year at dawn of the universe. The study finds that these galaxies are more abundant than thought and host intense bursts of star formation.
Astronomers use ALMA to detect 26 distant galaxies, revealing the most distant detection of water in the cosmos. The findings show that star birth bursts occurred much earlier than previously thought, with some galaxies as bright as 40 trillion Suns.
A team of astronomers has discovered two ancient, highly active galaxies in the early Universe, formed soon after the Big Bang. These galaxies are characterized by an unusually high rate of star formation and will help improve our understanding of star formation in the early Universe.
A team of astronomers has found galaxies producing stars at a prodigious rate when the universe was just a billion years old. The discovery, enabled by the Atacama Large Millimeter Array (ALMA), provides valuable data for refining theoretical models of star and galaxy formation in the early universe.
Theoretical models demonstrate that gas giant planets can survive periodic outbursts of mass transfer from the gas disk onto the young star. These models show that Jupiter and Saturn could have formed through this process, supporting the presence of 20% of sun-like stars with gas giants.
Naveen Reddy, an assistant professor at UC Riverside, has been awarded a Sloan Research Fellowship to study the physics of early universe and extragalactic astronomy. The fellowship will support his research on faint galaxies in the distant universe.
The James Webb Space Telescope will be displayed life-size at the South by Southwest festival in Austin, Texas, featuring exhibits and educational activities for all ages. The telescope model weighs 12,000 lbs. and is being assembled at NASA's Goddard Space Flight Center.
A Penn State research team has developed a new model to determine whether discovered planets can support liquid water and life. The updated model suggests that habitable zones are farther away from stars than previously thought, potentially reclassifying some previously believed habitable planets as non-habitable.
The G0.253+0.016 cloud defies conventional wisdom on star formation, with a dense gas content 25 times higher than the Orion Nebula but only producing small stars. The cloud's high velocities and presence of silicon monoxide suggest it may be two colliding clouds, preventing star formation due to its dynamic nature.
Astronomers have discovered hundreds of previously-unknown sites of massive star formation in the Milky Way, including the most distant such objects yet found. These regions serve as markers of the Galaxy's structure and help refine its understanding.
Astronomers have identified a new structure in the Milky Way, a long tendril of dust and gas dubbed a 'bone'. This feature is part of a web connecting spiral arms and is similar to fibulae found in human skeletons.
Astronomers discovered a mysterious planet circling the nearby star Fomalhaut with an unusual elliptical orbit. The team hypothesizes that another undetected planet may have gravitationally ejected Fomalhaut B, sending it on a collision course with a vast dust ring.
Scientists have discovered six likely comets around distant stars, which could be a sign that comets are as common in other stellar systems as planets. The discovery was made using the high-resolution spectrograph of the McDonald Observatory telescope and suggests that comets may play a crucial role in planetary formation.
Farhad Zadeh has discovered a new tool for detecting dusty clouds and stars using radio waves, allowing astronomers to image exotic features in the galaxy's center. The technique reveals dark features that indicate interactions between cold gas clouds and hot radiation fields.
Researchers using NASA's Kepler spacecraft have found that about 17% of stars have an Earth-sized planet in an orbit closer than Mercury. This means there are at least 17 billion possible Earth-like planets in the Milky Way, with 50% of stars having a planet of Earth-size or larger in a close orbit.
Astronomers from NASA's Goddard Space Flight Center and Penn State have released a vast image gallery featuring ultraviolet and optical images captured by the Swift satellite's Ultraviolet/Optical Telescope. The collection includes early images, stunning views of galaxies, and rare types of stars.
Astronomers using ALMA have observed the first direct evidence of vast gas streams flowing across a gap in a young star's disc, thought to be created by giant planets guzzling gas as they grow. The discovery provides insight into planet formation theories.