A spinning supermassive black hole destroyed a Sun-like star, causing the most luminous supernova ever recorded. The observation is attributed to a tidal disruption event rather than an extraordinary bright supernova.
Researchers observed L2 Puppis, a star similar to the Sun 5 billion years ago, to understand its evolution and potential impact on planets. A planet orbiting the giant star may offer clues about Earth's ultimate fate.
SourceKU Leuven·JournalAstronomy and Astrophysics·DateDec 8, 2016
Researchers used asteroseismology to determine the oblateness of a slowly rotating star, revealing a difference of only 3 kilometers between equatorial and polar radii. The star's small oblateness is surprising, as it rotates three times more slowly than the Sun.
SourceMax-Planck-Gesellschaft·JournalScience Advances·DateNov 16, 2016
The study found that sunflower sea star populations dropped dramatically after the disease outbreak, while other species such as leather stars and certain sea urchins increased in number. The virus outbreak is expected to have lasting effects on the ecosystem, potentially leading to more browsing on kelp.
SourceUniversity of California - Davis·JournalPLOS ONE·DateOct 26, 2016
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Scientists have observed a young stellar system fragmenting into multiple stars, supporting two theories on star formation: disk fragmentation and cloud instability. The discovery was made using ALMA and VLA observations of the L1448 IRS3B system in the Perseus constellation.
SourceNational Radio Astronomy Observatory·JournalNature·DateOct 26, 2016
A study found dramatic declines in sunflower sea star populations due to sea star wasting disease, affecting the Salish Sea ecosystem's balance. The disease has effectively disappeared these key predators from the area.
A rare triple-star system has been discovered by a University of Oklahoma-led research team using ALMA observations, providing insights into the formation of young binary and multiple star systems. The team found that the disk surrounding the tri-star system appeared susceptible to fragmentation, leading to the creation of newborn stars.
Researchers have observed a binary star system with two stars and three rotating planet-forming accretion discs, all misaligned with each other. The discovery challenges current understanding of planetary system formation and prompts further study to understand the physics behind this unusual system.
SourceUniversity of Copenhagen - Niels Bohr Institute·JournalThe Astrophysical Journal Letters·DateOct 11, 2016
Proxima Centauri, a small red dwarf star, has a regular cycle of starspots similar to our Sun. The study suggests that this cycle may impact the potential habitability of its planet, Proxima b.
SourceCenter for Astrophysics | Harvard & Smithsonian·JournalMonthly Notices of the Royal Astronomical Society·DateOct 11, 2016
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Astronomers have detected superhot blobs of gas being ejected near the dying star V Hydrae, with each blob twice as massive as Mars and traveling at half-million miles per hour. The plasma balls are thought to be launched by an unseen companion star in an elliptical orbit, shedding new light on planetary nebulae.
SourceNASA/Goddard Space Flight Center·JournalThe Astrophysical Journal·DateOct 6, 2016
Astronomers analyze Kepler observations of KIC 8462852 and find the star dimming slowly for almost three years before suddenly losing 2% of its brightness. The star's unusual behavior has sparked speculation about comets, alien megastructures, or planetary collisions, but the new findings will make it harder to explain.
SourceCarnegie Institution for Science·JournalThe Astrophysical Journal·DateOct 3, 2016
Researchers at the University of Surrey have discovered hundreds of undetectable black holes within a globular cluster, overturning old theories on their formation. The study uses advanced simulations to map the cluster and its behavior, revealing the effects of these massive objects on the surrounding stars.
SourceUniversity of Surrey·JournalMonthly Notices of the Royal Astronomical Society·DateSep 7, 2016
Astronomers have found a potentially habitable exoplanet, Proxima b, orbiting the red dwarf star Proxima Centauri, just 11 days from its parent star. The planet's mass is at least 1.3 times that of Earth and orbits within the star's habitable zone.
SourceCarnegie Institution for Science·JournalNature·DateAug 24, 2016
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Sony Alpha a7 IV (Body Only) delivers reliable low-light performance and rugged build for astrophotography, lab documentation, and field expeditions.
Scientists detect a potentially habitable exoplanet, Proxima b, orbiting Proxima Centauri every 11 days. The planet's surface temperature may allow for liquid water and life support, making it an exciting target for future observations.
Researchers have identified a young star over 30 times the mass of our Sun, which could help us understand how massive stars are formed. The discovery suggests that massive stars form in a similar way to smaller stars like our Sun.
SourceUniversity of Cambridge·JournalMonthly Notices of the Royal Astronomical Society·DateAug 21, 2016
Researchers at The Scripps Research Institute (TSRI) found that members of a cluster of microRNAs work together throughout the stages of immune cell generation. Different miRNAs dominate different stages as disease-targeting immune cells develop, guiding the development of therapies against autoimmune diseases.
SourceScripps Research Institute·JournalNature Communications·DateAug 2, 2016
Astronomers have peer into a nearby star's past, using low-frequency radio observations to fine-tune our understanding of stellar explosions. The team found the red supergiant lost matter at a slower rate and generated slower winds, improving knowledge of space composition.
SourceInternational Centre for Radio Astronomy Research·JournalMonthly Notices of the Royal Astronomical Society·DateAug 1, 2016
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Astronomers using NASA/ESA Hubble Space Telescope discover a new type of exotic binary star system where a rapidly spinning white dwarf powers electrons to almost the speed of light, causing radiation blasts that lash the companion red dwarf star, resulting in dramatic pulses every 1.97 minutes.
SourceESA/Hubble Information Centre·JournalNature·DateJul 27, 2016
Researchers at the University of Warwick have discovered a new type of exotic binary star that produces powerful beams of particles and radiation, affecting its nearby companion star. The star, AR Scorpii, has a white dwarf with intense magnetic fields that accelerate electrons in the atmosphere of the red dwarf to close to the speed o...
Astronomers confirm 104 exoplanets outside our solar system using NASA's Kepler spacecraft on its K2 mission. The discoveries include a planetary system with four promising rocky planets orbiting the M dwarf star K2-72.
SourceUniversity of Arizona·JournalThe Astrophysical Journal Supplement Series·DateJul 18, 2016
Astronomers have observed a water 'snowline' in a protoplanetary disk using the Atacama Large Millimeter/submillimeter Array (ALMA) telescope. The snowline marks the transition point where temperatures and pressures are low enough for water ice to form, and its distance from the star was found to be approximately 40 astronomical units.
SourceNational Radio Astronomy Observatory·JournalNature·DateJul 13, 2016
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Researchers directly detected a gas giant planet with a wide orbit in the young triple star system HD 131399, challenging existing knowledge about exoplanet detection. The unusual arrangement of the three stars and the planet's size, containing water and methane, may have formed through interactions between planets or binary stars.
SourceAmerican Association for the Advancement of Science (AAAS)·JournalScience·DateJul 7, 2016
The Crab Nebula is home to a spinning neutron star with a 'heartbeat' radiation signature, emitting clock-like pulses of energy. The neutron star is surrounded by expanding debris and glowing gas, revealing the intricate details of this cosmic object.
Researchers analyzed UV spectrum of BD+44 493, a second-generation star thought to have been enriched by one of the first stars. They found phosphorus, sulfur, and zinc, which reveal the star was likely massive and exploded as a supernova.
SourceUniversity of Notre Dame·JournalThe Astrophysical Journal Letters·DateJun 17, 2016
Astrophysicists at Northwestern University predict that LIGO's first detection of merging black holes could have been formed through dynamic interactions in the star-dense core of an old globular cluster. The theory, known as dynamical formation, is one of two recognized main channels for forming binary black holes detected by LIGO.
SourceNorthwestern University·JournalThe Astrophysical Journal Letters·DateJun 15, 2016
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Astronomers at Lund University propose that Planet 9, a mysterious object in our solar system, may be an exoplanet captured by the sun. The study suggests that the sun stole the planet from its original star during a close encounter.
SourceLund University·JournalMonthly Notices of the Royal Astronomical Society·DateMay 31, 2016
Researchers at Rice University have discovered a giant planet, CI Tau b, orbiting a young star in the constellation Taurus. The planet, at least eight times larger than Jupiter, orbits its 2 million-year-old star every nine days and is thought to have formed rapidly, with surrounding gas and dust still present.
A team of astronomers discovered a brown dwarf born as a full-fledged star, stripped to its current mass through stellar cannibalism. The brown dwarf was detected in a binary system with a tight orbit around a white dwarf, where the white dwarf's gravity removes about 90% of the companion's mass.
SourceUniversity of Southampton·JournalNature·DateMay 18, 2016
The 2013-2014 sea star wasting epidemic had a significant impact on the Oregon coast population, with up to 80% of sea stars dying during the outbreak. However, by spring 2015, the population was recovering in numbers, with study sites having up to 300 times as many new sea stars as in 2014.
Researchers discovered unique starspots on nearby star Zeta Andromedae, differing significantly from the Sun's spots. The findings offer a rare glimpse into the Sun's infancy and challenge current theories about star magnetic fields.
SourceUniversity of Exeter·JournalNature·DateMay 4, 2016
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Astrophysicists have observed a distant star in Andromeda with a different positioning of sunspots, indicating a magnetic field driven by unique internal dynamics. The star's rapid rotation creates a powerful magnetic field, resulting in asymmetrical distribution of sunspots on its surface.
SourceUniversity of Copenhagen - Niels Bohr Institute·JournalNature·DateMay 4, 2016
An international team of astronomers has discovered three Earth-sized planets orbiting a nearby ultracool dwarf star, TRAPPIST-1. The planets are located within the star's habitable zone and may have conditions suitable for life.
SourceUniversity of California - San Diego·JournalNature·DateMay 2, 2016
Three exoplanets, similar to Earth and Venus, orbit an ultracool dwarf star just 40 light years from Earth. The planets may have regions with temperatures suitable for liquid water and life.
SourceMassachusetts Institute of Technology·JournalNature·DateMay 2, 2016
A team of astronomers has discovered three planets with sizes similar to Earth's orbiting the ultracool dwarf star TRAPPIST-1, which may possess habitable regions. The planets' orbits are extremely close to their host star, receiving four times and twice less radiation than Earth.
A giant star exploded 30 million years ago in a galaxy near Earth, releasing energy equivalent to 100 million suns. The analysis revealed the star's mass, radius, and chemical composition before its spectacular demise.
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The Bubble Nebula, observed by Hubble, is a vast bubble being blown into space by a super-hot, massive star. The nebula is 7 light-years across and resides 7,100 light-years from Earth. A seething star forms this nebula, with gas escaping at over 4 million miles per hour.
Physicists have found a simple formula for the maximum mass of neutron stars, which depends on their rotation rate. The research, published in Monthly Notices of the Royal Astronomical Society, suggests that rotating neutron stars can support masses up to 20% higher than non-rotating ones.
SourceGoethe University Frankfurt·JournalMonthly Notices of the Royal Astronomical Society·DateApr 7, 2016
Astronomers have captured unprecedented details of the TW Hydrae disk, which may host a super-Earth or an infant version of our home planet. The images show concentric dusty bright rings and dark gaps, including a tantalizing gap at Earth's distance from the star.
SourceNational Radio Astronomy Observatory·JournalThe Astrophysical Journal Letters·DateMar 31, 2016
Astronomers used Hubble to study the Milky Way's nuclear star cluster, discovering a rich tapestry of over half a million stars. The cluster surrounds the galaxy's central supermassive black hole and offers insights into its formation.
Researchers suggest that twin black holes detected by LIGO might have formed inside a single, massive star. The star's death generated a gamma-ray burst, which was observed by the Fermi Space Telescope.
SourceCenter for Astrophysics | Harvard & Smithsonian·JournalThe Astrophysical Journal Letters·DateFeb 23, 2016
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Astronomers have discovered a crescent-shaped dust cloud in the outer reaches of a binary star's protoplanetary disk, providing fresh insights into planet formation. The cloud may be the key to forming planets in binary systems, with its lack of free-floating gases likely due to freezing out and forming ice on dust grains.
New Atacama Large Millimeter/submillimeter Array (ALMA) images provide detail on the binary star system HD 142527, revealing a broad ring of dust and ice. The system's formation is expected to yield insights into planetary systems around binary stars.
Researchers found a massive star pretending to be a supernova, emitting X-rays consistent with a neutron star core. The system's unique pairing suggests it may be one of the rarest types of binary systems, offering insights into star formation and evolution.
SourceUniversity of Washington·JournalMonthly Notices of the Royal Astronomical Society·DateFeb 12, 2016
Researchers discovered that stars undergo sharp stellar brightening caused by gravitational instabilities in massive gaseous disks, leading to a new understanding of star formation and evolution. The discovery may imply that our Sun experienced several such episodes, affecting the formation of giant planets.
SourceUniversity of Vienna·JournalScience Advances·DateFeb 5, 2016
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Astronomers studied the ionized gas outflow from NGC 6240, a starburst galaxy driven by intense star-forming activity. They found complex structures in the H-alpha nebula, including large 'broken bubbles' and evidence of past superwinds.
SourceNational Institutes of Natural Sciences·DateFeb 3, 2016
Researchers discovered young star populations in old globular clusters that formed from gas flowing in from outside the cluster itself. This challenge traditional understanding of star birth and highlights the complex nature of globular clusters.
SourceNorthwestern University·JournalNature·DateJan 27, 2016
A study published in Physical Review Letters shows that a galaxy cluster's formation history plays a role in its interaction with the surrounding dark matter halo. The researchers found that clusters formed from more dispersed galaxies were clumpier and interacted differently with their environment.
SourceCarnegie Mellon University·JournalPhysical Review Letters·DateJan 25, 2016
Astronomers have detected a massive galaxy cluster, IDCS J1426.5+3508, 10 billion light years from Earth, formed just 3.8 billion years after the Big Bang. The cluster is about 1,000 times more massive than the Milky Way and is undergoing significant upheaval.
SourceMassachusetts Institute of Technology·DateJan 7, 2016
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Researchers argue that globular clusters can host planets with conditions suitable for life, despite initial concerns. The environment of these dense star clusters may allow for stable planetary systems to form and survive for billions of years.
SourceCenter for Astrophysics | Harvard & Smithsonian·DateJan 6, 2016
Researchers have developed a new technique to accurately measure the surface gravity of distant stars, allowing for more precise analysis of exoplanet sizes and habitability. This breakthrough will play a crucial role in the study of planets beyond our Solar System.
SourceUniversity of British Columbia·JournalScience Advances·DateJan 1, 2016
Scientists discovered twisted magnetic fields in dusty disks orbiting young stars, affecting disk growth. The study used the VLA radio telescope to observe a 750-light-year-old protostar in Perseus, finding millimeter- to centimeter-sized particles in the disk.
SourceNational Radio Astronomy Observatory·JournalThe Astrophysical Journal Letters·DateDec 21, 2015
NASA's Hubble Space Telescope has photographed a newborn star with twin jets, reminiscent of a Star Wars lightsaber, in the Orion B molecular cloud complex. The protostar is feeding on surrounding material and shooting gas into space, creating shock fronts that heat up the surrounding gas.
Astronomers at the University of New South Wales have discovered three potentially habitable planets around a nearby red dwarf star called Wolf 1061. The middle planet, Wolf 1061c, is located within the Goldilocks zone and may be able to support liquid water and life.
SourceUniversity of New South Wales·JournalThe Astrophysical Journal Letters·DateDec 16, 2015
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Astronomers have discovered a planetary system with an enormous planet sandwiched between a Sun-like star and a dwarf star. The planet's massive eccentric orbit indicates gravitational influence from the dwarf star, leading to Kozai oscillations that cause it to 'dance' between the two stars.
SourceCarnegie Institution for Science·JournalThe Astrophysical Journal·DateDec 16, 2015
A University of Sydney graduate student has reconstructed images of the star CW Leo, which appears to be a changing 'inkblot pattern' due to dust and gas ejections. The star's appearance evolved over eight years, revealing it is not buried under its own dust as previously thought.
SourceUniversity of Sydney·JournalMonthly Notices of the Royal Astronomical Society·DateDec 3, 2015
A supercomputer simulation demonstrates that a collapsing massive star can generate enormous magnetic fields, focusing gas along the rotation axis to create jets producing oppositely directed blasts of highly energetic gamma rays. This breakthrough model sheds light on the process behind hypernovae and gamma-ray bursts.
SourceUniversity of California - Berkeley·JournalNature·DateNov 30, 2015
An international team of astrophysicists led by Johns Hopkins University scientist Sjoert van Velzen witnessed a star being destroyed by a supermassive black hole, ejecting a jet of plasma at nearly the speed of light. The team observed this event over several months using multi-wavelength telescopes and satellites.
SourceJohns Hopkins University·JournalScience·DateNov 26, 2015
Researchers found that tiny dips in a star's brightness can indicate a planet passing in front of it, but star KIC 8462852 had deep and irregular dips. The astronomers concluded that the destruction of a family of comets near the star is the most likely explanation for the mysterious dimming.
SourceIowa State University·JournalThe Astrophysical Journal Letters·DateNov 24, 2015
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University of Arizona researchers captured the first photo of a planet forming in a gap within LkCa15's disk, providing insights into protoplanetary formation. The study utilized advanced telescopes and imaging techniques to observe the young star and its surrounding disk.
The Indian star tortoise is being poached on a massive scale, with at least 55,000 individuals seized in a single year from one trade hub in India. The tortoises are sold to consumers for exotic pets or spiritual purposes, often for low prices, threatening their conservation and welfare.
SourcePensoft Publishers·JournalNature Conservation·DateNov 9, 2015