Articles tagged with Binary Stars
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Researchers have identified a second circumbinary planet, BEBOP-1c, in the TOI-1338/BEBOP-1 system using state-of-the-art instruments. The newly discovered planet has a mass 65 times larger than Earth and orbits both stars at once.
A study by UCLA astronomers reveals that none of the 16 young supermassive stars orbiting the Milky Way's black hole are found in pairs, contradicting previous assumptions about stellar formation. The researchers suggest that the extreme environment around the black hole may be driving nearby binary stars to merge or be disrupted.
Researchers discovered two massive touching stars that will eventually become black holes and collide, generating waves in space-time. The stars are currently feeding each other every three days before the smaller star collapses into a black hole in 700,000 years.
Astronomers have discovered the tightest ultracool dwarf binary system ever observed, consisting of two stars that orbit each other in less than one Earth day. The newly discovered LP 413-53AB system is estimated to be billions of years old, similar to our sun, and has an orbital period three times shorter than previous discoveries.
Embry-Riddle astronomers report a rare binary star system with an uncommon circular orbit, formed when a supernova fizzled out without the usual bang. The discovery sheds light on the origins of the universe and the formation of heavy elements.
Scientists discover first gamma-ray eclipses from spider star systems using Fermi data, calculating system tilt and pulsar mass. The discovery helps researchers measure pulsar masses, constraining physics within extreme environments.
The Butterfly Nebula's unique shape is caused by a second star orbiting the central star, creating wing-like lobes. New research reveals powerful winds are altering the material within these lobes, contradicting existing models of planetary nebulae formation and evolution.
Researchers at the University of Washington have discovered a unique binary star system where a small companion star is surrounded by a large disk of dusty material. The companion star caused a seven-year-long eclipse of the main star, Gaia17bpp, which is one of the longest recorded eclipses.
Researchers have discovered the tightest ultracool dwarf binary system, comprising two stars that orbit each other in less than a day. The newly discovered LP 413-53AB system is composed of ultracool dwarfs and has an orbital period at least three times shorter than previously detected systems.
Researchers used 69 confirmed binaries to test two origin stories of black holes, but found that the current catalog is not enough to reveal anything fundamental about their formation. The study suggests that the universe's spin and tilt can be 'spun' in different ways depending on the model used.
Researchers from the University of Sydney explain that the James Webb Space Telescope's 'spiderweb' image is not an alien megastructure but rather a series of concentric dust shells created by a binary system. The team discovered that the stars in the system interact through stellar winds, producing shock fronts and spiral-shaped plumes.
Astronomers have observed dust plumes from the binary star system WR140 being accelerated into interstellar space by intense starlight. The team used the James Webb Space Telescope to capture images of the dusty plumes, which form a cone-shaped shock front between the two stars.
Astronomers have discovered a stellar binary with an extremely short orbit of just 51 minutes, confirming a decades-old prediction. The system is believed to be a cataclysmic variable, in which a white dwarf is accreting material from its companion star.
Astronomers used the VLBA to trace a wobble in a nearby star's motion and discovered a Jupiter-like planet orbiting one of its stars. The planet has twice the mass of Jupiter and orbits every 284 days, with an inclined orbit of 148 degrees from the stars.
Researchers have discovered a new technique for detecting dim bodies, including planets, orbiting Cataclysmic Variables (CVs). The method analyzes changes in brightness caused by perturbations of a third body orbiting the inner two stars. Two out of four studied CV systems show signs of planetary mass objects in orbit around them.
A team of astronomers, known for debunking black hole discoveries, found a dormant stellar-mass black hole in the Large Magellanic Cloud. The newly discovered black hole is at least nine times the mass of the Sun and orbits a hot star weighing 25 times the Sun's mass.
A team of Chinese and Australian astronomers has discovered direct evidence for binary common envelope evolution, a key process in star evolution. The observation provides a way to accurately characterize this process through direct detection.
A Northwestern University-led team of astrophysicists observed a star-forming cloud and discovered a twisted magnetic field that suggests the formation of a binary star system. The researchers believe a previously hidden sibling star may be responsible for the twisted field, which shifted the dynamics of the cloud to form a new star.
Researchers found that planetary systems around binary stars form differently than those around single stars, potentially creating new targets for extraterrestrial life. The study also suggests that comets could play a key role in delivering organic molecules necessary for life.
Astronomers have used observations from the Hobby-Eberly Telescope to better understand how massive stars live and die. The study of supernova 2014C revealed a unique process where the hydrogen envelopes of two stars merged, forming a common-envelope configuration that shed light on the stellar explosion.
Researchers using ALMA and Hubble Space Telescope observe V Hydrae, a carbon-rich star, expelling matter in six slowly-expanding rings and two hourglass-shaped structures. The discovery confirms the traditional model of AGB star death is incomplete or incorrect.
Researchers observed a binary star system in formation, revealing two stars with disks of gas and dust surrounding them. The newly discovered disks may be the beginnings of new planet systems that will orbit the binary stars in the future. This study provides unprecedented detail on a binary system in formation.
A team of astronomers discovered neutron stars blowing hot, warm and cold winds while consuming matter from a nearby star. The discovery provides key information about the behaviors of these extreme cosmic objects, which contribute to the formation of new stars and galaxy evolution.
For the first time, scientists have measured a large difference between a black hole's rotation axis and the axis of its orbiting binary star system. This finding forces astronomers to add a new dimension to their models, offering new insights into black hole formation and physics.
A team of astronomers led by the University of Birmingham detected a rare circumbinary planet, Kepler-16b, using radial velocity method. The discovery provides clues on planetary accretion and demonstrates that ground-based telescopes can be used for modern exoplanet research.
A team of astronomers has discovered a rare pair of brown dwarfs that have the widest separation of any brown dwarf binary system found to date. The two brown dwarfs are about 12 billion miles apart, or three times the separation of Pluto from the Sun.
Researchers use ALMA and VLA to detect chaotic dust and gas streams caused by an intruder object interacting with the binary protostar. The study provides evidence of flyby events in nature, which can dramatically perturb circumstellar disks and impact planet formation.
Astronomers have discovered a binary system consisting of a rapidly spinning neutron star and the precursor to an extremely-low-mass white dwarf, dubbed a 'cosmic spider'. The system emits powerful gamma-rays and has been observed using the SOAR Telescope in Chile.
Researchers studied 15 unusual stars in the Milky Way galaxy, discovering that all have recently undergone a rare phase where one star engulfs another. The findings provide new insight into the sky's most dramatic phenomena and may help answer questions about how stars live and die.
Researchers have captured a 1,000-year-old supernova in 3D images, revealing unprecedented details about the elements ejected during a star's explosion. The study provides a three-dimensional map of these elements, shedding light on the conditions at the time of the explosion and the importance of asymmetries in supernovae.
Astronomers have detected a white dwarf star that spins at an incredible rate of once every 25 seconds, completing one rotation faster than Earth. The star is thought to be the size of the Earth but massive enough to pull material from its companion star, creating a magnetic propeller system.
A new technique developed by University of Hawaii astronomer Nader Haghighipour has successfully detected a transiting circumbinary planet in TESS data. The discovery validates the method, which reduces the time to detect such planets from over a year to just five days.
A team of scientists used uGMRT to study eclipses of millisecond pulsars, finding that absorption by magnetized materials from the companion star is the cause. The study provides insight into the evolutionary processes and ultimate fate of these exotic systems.
Astronomer Dr. Lauri Jetsu discovers multiple new companion star candidates for the eclipsing binary Algol AB, with orbital periods between 20 and 219 years. The companions are too faint to be detected by modern space telescopes, but their periodic signals can predict observed O-C changes.
Researchers analyzed ALMA data to create the first animation of a young twin star system's orbital motion over three years. The study found that the disks surrounding each star are significantly misaligned with respect to each other, supporting the idea that the system was formed via molecular cloud fragmentation.
Astronomers discovered a stellar collision that triggered a supernova explosion in a companion star. The collision was detected using the VLA and VLASS survey, revealing a centuries-long death dance between two massive stars.
Astronomers have discovered a rare teardrop-shaped star system that will eventually become a Type Ia supernova. The system, HD265435, is comprised of a hot subdwarf and a white dwarf star orbiting each other closely, with the white dwarf being as heavy as our Sun but slightly smaller than Earth's radius.
Astronomers using Gemini Observatory and WIYN 3.5-meter Telescope found 73 binary star systems among TESS exoplanet hosts, which could be hiding Earth-sized planets. The team discovered that small planets are harder to detect in binary systems due to glare from the companion star.
Researchers have discovered a unique 'blinking giant' binary star system, where a giant star is eclipsed by an unseen orbital companion every few decades. The system has been spotted near the centre of the Milky Way, more than 25,000 light years away.
Researchers identify five double star systems, Kepler-34, -35, -38, -64 and -413, as potential candidates for supporting life. The study shows that these systems have a permanent Habitable Zone, where liquid water could persist on the surface of any Earth-like planets.
Astronomers have studied the rare RV Tauri variable U Monocerotis, a binary system with two stars orbiting within a sprawling disk of dust. The 130-year dataset reveals predictable brightness changes and X-ray emissions.
Astronomers have created a massive atlas of widely separated binary stars within 3,000 light years of Earth, comprising 1.3 million pairs. This increase in sample size provides insights into the evolutionary phases of these binaries, including 17,000 white dwarfs.
Researchers have mapped the orbit of a rare Nitrogen-rich Wolf-Rayet star in the WR 133 binary system, marking the first-ever visually observed orbit of this type. The team determined the dynamical mass of both stars, with the WN star having 9.3 times more mass than our Sun.
Researchers discovered that the two stars in the HS Hydrae system were almost completely eclipsing each other 50 years ago but now barely overlap. The team predicts that the eclipses will cease around February 2021, marking the end of this rare stellar dance.
Researchers have discovered a binary system of brown dwarfs, orbiting each other at an unprecedented distance, with one object being similar in mass to Jupiter and the other about 8 times less massive. This rare find suggests that star formation processes can create binary systems like those found in our solar system on smaller scales.
Astronomers have measured the motion of a massive Jupiter-like planet in an unlikely orbit around a double star, sparking questions about its formation and evolution. The discovery offers evidence that such oddball orbits are possible and may hold clues to the mysterious Planet Nine in our solar system.
Astronomers have confirmed an exoplanet, HD 106906 b, with a highly eccentric orbit around its binary star, similar to the hypothetical Planet Nine. The planet's orbit is likely bound, and its presence suggests that distant planets can form within the first tens of millions of years of a star's life.
A team of researchers has analyzed data to infer the nature of compact object orbiting within LS 5039, the brightest gamma-ray binary system in the Galaxy. The team suggests that particle acceleration process is caused by interactions between dense stellar winds and ultra-strong magnetic fields of a rotating magnetar.
The team observed the nebula with two different spectrographs on large telescopes, finding that the central star is inflated and signatures of accretion are present. The data suggest a merging binary star system, offering a clear view of the central stellar remnant.
A new study reveals the binary nature of a trans-Neptunian object, with two objects orbiting each other only 350 kilometers apart. The discovery was made possible by the Research and Education Collaborative Occultation Network (RECON), a citizen science project.
Interactions with binary companions generate complex planetary nebula shapes by influencing the stellar wind of elderly stars. Leen Decin and colleagues observed AGB star winds using ALMA, finding none with spherical symmetry and instead distinct geometries similar to those in PNe.
Researchers found three large, misaligned dust rings around the young triple star system GW Ori, with sufficient dust for planet formation. A computer simulation suggests that a hidden planet may have carved out a dust gap and broken the disk at the location of the current inner and outer rings.
Scientists have made key discovery using pre-solar grains found in primitive meteorites, providing new insights into stellar explosions and element formation. The new method involves analyzing chemical and isotopic composition of grains to study nuclear reactions like proton capture on chlorine.
Researchers at the University of Sheffield have discovered a pulsating ancient star in a double star system, allowing them to study the internal structure of a white dwarf in detail for the first time. The discovery provides key insights into the structure, evolution, and death of white dwarf stars, including their composition.
Astronomers have discovered a one-sided pulsator in the Milky Way, with citizen scientists providing crucial clues. The star's unusual single-sided pulsation is caused by its location in a binary star system with a red dwarf companion.
Astronomers have discovered a rare opportunity to study the evolution of a planetary system, with the DS Tuc binary system providing insights into how planets form without being heavily impacted by external forces. The findings suggest that the planet DS Tuc Ab formed through relatively calm processes.
Swedish and Japanese researchers found a new explanation for the emission lines of SN 2006gy, a superluminous supernova. The discovery led to a revised understanding of how the supernova arose, with a double star system involving a white dwarf and massive hydrogen-rich star implicated.
Astronomers have discovered a new class of bizarre objects at the center of the Milky Way galaxy, which resemble gas and behave like stars. The objects are thought to be binary stars that merged due to the strong gravitational force of the supermassive black hole, with four additional objects found in the same orbit.
Researchers have discovered that tidal effects from a close binary companion can cause a star to spin fast enough to launch material into space, forming a gamma-ray burst. This phenomenon is necessary for creating the most luminous events in the universe, observable from Earth when their jet of material is pointed directly at us.
LSU astronomers predict that binary star V Sagittae will become the brightest in the Milky Way galaxy, outshining Sirius and Venus, around 2083. The star is currently faintly visible but will brighten rapidly due to its rapid orbital decay.