A team of astronomers has observed an unusual 'baby' star, LRLL 54361, periodically emitting infrared light bursts, hinting at the presence of a companion star. The discovery provides a rare chance to study what appears to be a developing binary star system.
Researchers have discovered a way to identify and explain the luminosity generated during common envelope events involving binary stars. The events result in bright red outbursts, similar to recently discovered Luminous Red Novae. Natalia Ivanova's analysis provided new insights into these celestial phenomena.
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.
A recent study found that wide binary stars in planetary systems can lead to dramatic events over time. In one hypothetical system, at least one of four giant planets was ejected in almost half of the simulations. The researchers also discovered substantial evidence that this process occurs regularly in known extrasolar planetary systems.
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.
Astrophysicists found that wide binary stars have a significant impact on planetary systems, causing violent disruptions and scattering planets. The researchers conducted computer simulations and found that planets in these systems are often ejected to interstellar space.
The study reveals differences in the speed of evolution among globular clusters, with fast-aging clusters experiencing core collapse within a few hundred million years. In contrast, slow-aging clusters would take several times the current age of the universe to undergo core collapse.
Researchers used the MPG/ESO 2.2-metre telescope and Hubble Space Telescope to study 21 globular clusters, finding that a few were young with blue stragglers distributed throughout, while others were old with the stars clumped in the centre. This reveals big differences in the speed of evolution from cluster to cluster.
Research reveals successful solo rock/pop stars are twice as likely to die early as those in equally famous bands. Adverse childhood experiences are also significantly more common among those who died from drug and alcohol misuse.
A team of researchers at MIT analyzed light from a quasar, which is the most distant object known, to study the era of the first stars and galaxies. They found no evidence of heavy elements in the surrounding gaseous cloud, suggesting that the quasar dates back to an era nearing the universe's first stars.
Researchers found that planets in solar systems with similar stars may be warmer and more dynamic, potentially hosting microbial life. This could expand the habitable zone around those stars, making them more suitable for life.
Researchers find two super-luminous supernovae at high redshifts, consistent with pair-instability supernova mechanism. The explosions are thought to have occurred in massive stars that formed in the early universe.
Researchers from UC Irvine and NASA's Jet Propulsion Laboratory have discovered that galaxy halos are likely caused by orphan stars ejected from galaxies during violent mergers. The team used data from the Spitzer Space Telescope to study the patterns of diffuse light, finding that it is too strong to be explained by earlier theories.
Astronomers discovered a quasar hidden behind a dusty galaxy, where no starlight is visible due to intense dust blocking. The James Webb Space Telescope will help detect the underlying stars, which were not seen by Hubble.
Two O-type stars in the Cygnus OB2 #9 binary system emit intense X-rays as their stellar winds collide during closest approach. The interaction reveals details about the stars' masses, luminosity, and orbits, shedding light on star formation and galaxy evolution.
Astronomers found a cloud of hydrogen and helium plunging toward the galactic center, which represents the remains of a planet-forming disk. The discovery suggests that planets can still form near black holes due to stars in a ring orbiting the galaxy's central black hole.
Researchers at Tel Aviv University develop method to observe stars that formed when the universe was 180 million years old. By detecting radio waves from hydrogen atoms, they reveal patterns in the sky indicating early galaxies, providing insight into the universe's origins.
A team of astronomers has detected gravitational waves at optical wavelengths in light from a pair of eclipsing white dwarf stars. The effect, predicted by Einstein's theory of general relativity, causes the stars to inch closer together and orbit each other faster.
Astronomers have discovered the first multi-planet system orbiting a binary star, characterized by the University of Texas at Austin's McDonald Observatory. The system, Kepler-47, features an outer planet within the habitable zone, where liquid water could exist.
UT Southwestern Medical Center has been named the official healthcare team of the Dallas Stars, marking a significant expansion of their longstanding relationship with the club. The team will oversee the health needs of players, including injury evaluation and treatment, and promote healthy messages through initiatives such as "Hockey ...
Astronomers using Hubble data observe two massive star clusters in the Large Magellanic Cloud that may be in early stages of merger. The discovery sheds light on the origin of large star clusters and helps scientists understand galaxy formation.
Researchers from University of Bonn discover most massive stars form double systems, with over three-quarters orbiting a companion. The study reveals material transfer and merging between stars, challenging previous assumptions about single stars.
A study using the VLT found that 75% of O-type stars are in binary systems, with a higher proportion of interacting pairs than previously thought. This discovery has profound implications for galaxy evolution, as these heavyweights play a key role in shaping galaxies through violent phenomena such as stellar mergers and gamma-ray bursts.
Researchers found that two closely related sea star species diverged around 6,000-22,000 years ago, ruling out slow genetic changes over time. The boundary between cold and warm water in the Coral Sea may have isolated a small population of ancestral sea stars.
A previously unappreciated open star cluster, Ruprecht 147, has been found to be an important tool in understanding stellar astrophysics and the search for Earth-like planets. The cluster is close to Earth and contains stars similar in mass and age to the Sun, making it a valuable laboratory for studying bright stars.
Researchers have found that terrestrial planets like Earth could have formed earlier than expected in the universe's history. The study suggests that rocky worlds don't need to orbit metal-rich stars to form and that their sizes are not directly linked to the star's metallicities.
New research reveals small planets can form around stars with low heavy element content, challenging previous assumptions. This discovery suggests Earth-like planets may be widespread in the universe, contradicting earlier theories on planetary formation requirements.
Despite lacking a brain, brittle stars exhibit coordinated movement by designating a central arm and two rowing arms to propel it along. They can also change direction by choosing a new central arm and moving its accompanying limbs.
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.
For the first time, astronomers have detected arsenic and selenium in an ancient star, revealing insights into the origin of these elements. The discovery sheds light on how stars produce heavier elements, including those found on Earth.
The new Hubble image reveals millions of young stars in the 30 Doradus star-forming complex, with some stars weighing over 100 times the mass of our sun. The nebula is home to the fastest rotating and highest velocity stars ever observed.
Astronomers have identified two 11- to 12-billion-year-old white dwarf stars, the oldest and closest known to Earth. Located 100 light years away, these stars are believed to be among the first formed in the Universe soon after the Big Bang.
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.
Researchers used radio and infrared telescopes to study a giant cloud about 770 light-years from Earth, discovering a 'pristine' clump of gas that may be on the verge of forming dense cores. The observations reveal previously unseen substructures within the clump that could lead to the formation of ten new stars.
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.
Astronomers have discovered a young cluster of blue stars surrounding an intermediate-mass black hole in a cannibal galaxy. The star cluster is thought to be less than 200 million years old and may be the remnant of a dwarf galaxy that was swallowed by the larger galaxy.
Two new planets, Kepler-34 and Kepler-35, have been discovered orbiting binary suns in the Cygnus constellation. The discovery indicates that planets can revolve around double stars, challenging our understanding of solar systems.
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.
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.
Astronomers using NASA's Hubble Space Telescope found a large population of hot, bright blue stars in the center of the Andromeda galaxy. The stars, which are aging sun-like stars, have prematurely shed their outer layers to expose their extremely blue-hot cores.
Researchers have discovered two new planets, Kepler-34b and Kepler-35b, orbiting a binary star system using data from NASA's Kepler mission. The low-density gas giants are comparable in size to Jupiter but much less massive, with Kepler-34 being about 24% smaller and Kepler-35 being about 26% smaller.
A team led by LSU Professor Bradley Schaefer and graduate student Ashley Pagnotta discovered the origin of thermonuclear supernovae as a pair of white dwarf stars. The study resolves the decades-long 'progenitor problem' in astrophysics, with no remaining possible explanations for the explosions.
Two new transiting circumbinary planet systems have been discovered using data from NASA's Kepler Mission. The planets, Kepler-34 b and Kepler-35 b, orbit two stars in the constellation Cygnus, with climates that could experience dramatic temperature changes due to the variable distance between the planet and its stars.
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.
Scientists have discovered two new circumbinary planets, Kepler-34b and Kepler-35b, orbiting two stars in the constellation Cygnus. The discovery suggests that planets with two suns are common, potentially existing in millions in the Galaxy. This finding sheds light on the formation of these unique planetary systems.
The Cygnus X region is home to thousands of massive stars and many more stars around the size of our sun or smaller. Infrared data from NASA's Spitzer Space Telescope reveals a complex of star-forming clouds, with bubbles carved out by radiation and winds from massive stars.
A Caltech-led team of astronomers has discovered 18 new planets orbiting massive stars, with masses similar to Jupiter's. The findings provide valuable insights into planetary formation and support the theory that planets grow from seed particles accumulating gas and dust in a disk surrounding a newborn star.
Researchers have found the largest batch of young, supermassive stars yet observed in our galaxy, including dozens of massive blue stars. The intense light emitted by these newborn stars has carved out a glowing hollow shell around them, offering a unique opportunity to study energy transmission and star formation.
Researchers studying a binary star system in the Whirlpool Galaxy have detected a star dimming noticeably before its companion exploded in a supernova. The study provides evidence that certain patterns of brightening and dimming may signal an impending doom for stars, making it possible to predict when a star is near death.
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 found two distinct populations of neutron stars, suggesting different supernova channels. The findings shed light on stellar evolution and open new research areas.
Complex organic compounds found throughout Universe contain aromatic and aliphatic components, resembling coal and petroleum. Stars produce these compounds on short time scales, ejecting them into interstellar space.
A team of astronomers has discovered three new planets and a mystery object orbiting giant, dying stars. The research provides insights into the evolution of planetary systems around these stars and how metal content influences their behavior.
Astronomers detect a double sunset on the newly discovered Kepler-16b, a planet similar to Saturn in size and mass. The planet orbits two smaller, cooler stars and is estimated to be around -100°C due to its distance from its parent bodies.
Astronomers have discovered a planet that orbits around a pair of stars, providing direct evidence for the existence of circumbinary planets. The discovery was made using data from the NASA Kepler space telescope and confirms long-speculated theories about these systems.
A CSIRO study reveals galaxies have less molecular hydrogen gas than in the past, leading to fewer stars forming. The decline in gas availability is linked to Dark Energy's acceleration of the Universe's expansion.
Astrophysicists are using Type Ia supernovae, also known as 'zombie' stars, to build a map of the universe's history and understand dark energy. The stars' explosive deaths can be used to measure distances in the universe.
A team of astronomers using NASA's Fermi Gamma-ray Space Telescope observed a unique binary system that produced dual gamma-ray flares during its closest approach. The flares were many times stronger than expected and occurred despite the star following an eccentric orbit, making them only visible every 3.4 years.
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.