Articles tagged with Observational Astrophysics
Researchers confirm coronal heating mechanism using observations from NASA's IRIS and Japan's Hinode solar observatory. Resonant absorption process converts magnetic waves into heat energy, explaining why the sun's corona is hotter than its surface.
A research team combined high-resolution observations from Hinode and IRIS with numerical simulations to detect resonant absorption in a solar prominence. This process heats the prominence through turbulent flow, providing a solution to the long-standing coronal heating problem.
The causes of stellar explosions known as Type Ia supernovae have been debated for decades. Recent studies suggest that either one or two white dwarfs can trigger these events, shedding light on the evolution of galaxies and dark energy. Understanding this phenomenon will inform our study of the universe's expansion.
A new stellar model developed by researchers at SISSA reveals that cosmological 'lost' lithium in metal-poor stars was not destroyed, but rather accreted from the surrounding environment. The model, which agrees with observations, provides a plausible explanation for the low abundance of lithium-7 in ancient stars.
Astronomers confirm exoplanet orbiting far from its central star using gravitational microlensing, opening new discovery space for long-period orbits. The Uranus-sized planet is about 370 million miles from its parent star, with a host star about 70% as massive as our Sun.
Researchers at the University of York have revealed a new understanding of nucleosynthesis in stars, providing insight into massive star evolution and the origins of the Solar System. By studying radioactive aluminium production, scientists can now better understand gamma radiation maps of the galaxy and simulate star behavior.
A recent study suggests that dense star clusters in the universe could be 'factories' of binary black holes. Researchers predict that advanced observatories will detect over 100 merging black holes per year from these clusters.
A team of researchers discovered a massive black hole with nearly 7 billion solar masses in an otherwise normal, distant galaxy called CID-947. The finding contradicts previous theories on the co-evolution of galaxies and their central black holes.
Astronomers detected high-energy x-rays from five previously clouded supermassive black holes, supporting the theory of millions more existing but hidden from view. The research uses NuSTAR to study nine candidate black holes, confirming five were obscured by dust and gas.
A collaborative project between Caltech and the Weizmann Institute of Science observed a unique radiation spike in ultraviolet range, supporting a giant companion model for white dwarf explosions. The findings highlight the importance of ultraviolet-range observations in understanding type Ia supernovae.
Researchers found strong outflows in ultra-luminous X-ray sources (ULXs), suggesting smaller black holes than expected. The team's observations shed light on ULXs and their impact on our understanding of supermassive black hole formation.
Scientists used Sandia's Z machine to verify the metallic phase of hydrogen, solving a long-standing discrepancy in Saturn's age. The experiment found that dense hydrogen can become atomic, releasing energy that could explain Saturn's temperature.
A team of astronomers using the European Southern Observatory's Very Large Telescope discovered the brightest galaxy yet found in the early universe. The galaxy, CR7, contains massive blue stars - the first generation of stars that forged the heavy elements necessary for life.
The Rosetta spacecraft's ultraviolet instrument has made a surprising discovery about Comet 67P/Churyumov-Gerasimenko, revealing that electrons near the comet's surface break up water and carbon dioxide molecules, not solar photons. This finding fundamentally transforms our knowledge of comets.
Recent NuSTAR observations of supernova SN 1987A confirm the predicted lopsided nature of stellar giant deaths, with most material moving away from the observer. This finding supports supercomputer simulations that assume asymmetrical core collapse and could help solve the mystery of dual black hole and neutron star formation.
Researchers at Yale University and the University of California-Santa Cruz have detected an exceptionally luminous galaxy more than 13 billion years in the past, EGS-zs8-1. The galaxy is one of the brightest and most massive objects in the early universe, with a mass equivalent to over 15% of our Milky Way.
Scientists at NJIT's Big Bear Solar Observatory have captured groundbreaking images of the Sun's interior structure, revealing complex dynamics of sunspots' dark cores. The high-resolution images show finely structured plasma flows and oscillating cool jets piercing the hot atmosphere.
A 3D map of galaxy superclusters has been created, providing insights into dark matter and its distribution in the universe. The map, published online in Monthly Notices of the Royal Astronomical Society, spans nearly two billion light years.
Astronomers have combined telescopes across the Earth to create the Event Horizon Telescope, which will take detailed images of the supermassive black hole at the center of the Milky Way galaxy. The South Pole Telescope has joined the EHT, bringing a two-to-three times increase in resolution to study black holes and test Einstein's the...
The LEECH exoplanets survey has obtained new images of HR 8799, a 30-million-year-old star with four known giant planets. The team found that the system likely consists of multiple double resonances, indicating gravitational interactions between the planets.
Astronomers have determined the pre-explosion mass of a white dwarf star that blew up thousands of years ago using archival data from the Japan-led Suzaku X-ray satellite. The study suggests that only a single white dwarf was involved in the explosion, contradicting a well-established alternative scenario.
Research from the University of Waterloo and Perimeter Institute demonstrates that quantum mechanics can distinguish between cause-effect relations and common causes, unlike classical physics. This breakthrough enables a new approach to causal inference, potentially solving long-standing problems in science.
Researchers from UGR have set limits to the properties of axions, which aspire to be identified as dark matter. The study uses numerical simulations of stellar evolution and suggests that axion emission can significantly affect the timing of helium burning in stars.
A team of researchers has discovered a very distant galaxy that contains a large amount of dust, changing astronomers' previous calculations of how quickly the dust was formed. The discovery suggests that galaxies were enriched with dust particles containing elements such as carbon and oxygen, which could form planets.
Researchers successfully demonstrate a new technique combining a solar telescope with a laser frequency comb to analyze distant stars with unprecedented accuracy, potentially leading to the discovery of Earth-like planets. The technique enhances spectral analysis and advances research in astrophysics.
An international team of astrophysicists has witnessed the formation of a quadruple star system, consisting of a young star and three gas clouds that will develop into stars in 40,000 years. The system is unstable and prone to interference due to its multiple members.
The $344 million Daniel K Inouye Solar Telescope will utilize cameras designed by a UK university consortium led by Queen's University Belfast to observe the Sun's surface in unprecedented detail. The telescope aims to address fundamental questions in contemporary solar physics.
A team of astronomers successfully restored the Half-wave Spectropolarimeter (HPOL) instrument, allowing it to conduct measurements with improved performance. The upgraded HPOL is now fully operational at the University of Toledo's Ritter Observatory and enables researchers to study variable or transient objects more effectively.
A team of researchers from Case Western Reserve University has discovered new features of the 'Whirlpool Galaxy', M51a, using a 20-hour exposure photograph. The image reveals faint plumes extending from the galaxy's northeast and south, providing valuable insights into its history and interaction with neighboring galaxies.
A recent study confirms that galactic contaminants are too intense to distinguish cosmological gravitational waves, casting doubt on the detection. The Planck-BICEP2 collaboration used multiple instruments to rule out contamination, but acknowledge the need for sharper eyes to detect the signal.
An international team of astronomers has observed a fast radio burst happening live for the first time, providing new insights into this mysterious phenomenon. The burst is believed to have originated up to 5.5 billion light years away, making it an extremely bright and potentially useful tool for understanding our universe.
Astronomers successfully observed a 'fast radio burst', a brief flash of radio waves, in real-time using the Parkes telescope. The event was detected up to 5.5 billion light years away and suggested the presence of a magnetic field nearby.
The University of Warwick's Next Generation Transit Survey (NGTS) aims to detect small planets from Neptune size down to twice the size of Earth. Researchers hope to study the atmospheres and composition of these super-Earths, which are thought to be common around other stars.
Astronomers have developed a comprehensive picture of Eta Carinae, including Hubble Space Telescope images showing ionized gas racing away from the star at high speeds. New 3-D models reveal features of the stars' interactions, including spine-like protrusions in the gas flow along the edges of a spiral cavity.
Researchers found that stars in large middle-aged clusters are of similar age, suggesting a complex formation process. The discovery challenges current understanding of stellar evolution and may require re-evaluation of models.
A team of astronomers successfully measured the passing of a super-Earth in front of a nearby Sun-like star using a ground-based telescope. The detection bodes well for characterizing dozens of super-Earths revealed by upcoming surveys.
Astronomers have successfully detected a super-Earth's transit using a ground-based telescope, marking the first time this has been done. The transit occurred in front of a bright Sun-like star and demonstrates that small planets can be characterized with existing facilities.
A team led by Andrea Ghez determined that G2 is most likely a pair of binary stars that had been orbiting the black hole in tandem and merged together into an extremely large star. The research suggests that many of the stars at the center of the galaxy are massive and mostly binaries.
Astronomers have discovered a pulsar that emits an incredible amount of energy, shining brighter than previously thought possible. This find challenges the previous assumption that ultra-luminous X-ray sources are likely black holes.
Researchers at the University of Bonn and Cardiff develop a new observational strategy for imaging extremely distant galaxies, using ALMA radio telescope data. This method improves upon previous efforts by accurately estimating molecular hydrogen presence in these galaxies, providing insights into galaxy formation and star creation.
Researchers found large patches of trace gases shining brightly near Titan's poles, with unexpected east-to-west variations. These findings are consistent with observations made by NASA's Cassini spacecraft, which found cloud caps and high concentrations of gases over the poles.
New observations from the Interface Region Imaging Spectrograph (IRIS) suggest that miniature solar flares called 'nanoflares' could be partly responsible for heating the Sun's million-degree corona. High-energy electrons generated by these nanoflares may deposit energy in the plasma, leading to coronal heating.
Researchers from around the world have successfully explained the formation and propagation of stellar jets emitted by young stars. The team used a patented experimental device and numerical simulations to demonstrate that interstellar magnetic fields play a key role in confining these jets, which can travel vast distances.
Researchers analyzed images from the Russian spacecraft RadioAstron and found small spots in the overall image, which they call substructure. This phenomenon can be used to infer the actual size of the underlying source, including the black hole's emission region.
A team of scientists used NASA's Hubble Space Telescope to create a detailed map of the atmosphere of WASP-43b, an extremely hot and gaseous planet. The findings reveal that the planet has extreme temperature fluctuations between day and night, with winds howling at supersonic speeds.
Scientists from China and the US report results from the first stage of the PandaX-I experiment, a dark matter search in an underground lab. The data from this experiment place strong constraints on previously reported dark matter-like signals.
The Interface Region Imaging Spectrograph (IRIS) mission has captured a unique perspective on an X-class solar flare, highlighting the transition region and corona. The observations provide insight into the dynamics of these powerful flares, which can have significant effects on Earth's magnetic field and radiation environment.
The Large Synoptic Survey Telescope (LSST) will image the entire visible sky twice per week, providing a vast amount of information on short-lived transient events, dark matter, and dark energy. The project is a partnership among NSF, DOE, and private contributors, with operational support from researchers worldwide.
Scientists observed six minutes worth of data from NASA's EUNIS mission, gathering strong evidence for nanoflares as the source of the sun's corona heat. The detection is consistent with only one current theory: constant bursts of impulsive heating provide the mysterious extra heat.
Astronomers have mapped the mass within a galaxy cluster, MCS J0416.1-2403, more precisely than ever before using unprecedented depth of data from Hubble's Frontier Fields programme. The team identified 51 new multiply imaged galaxies around the cluster, quadrupling the number found in previous surveys.
The Advanced Technology Large-Aperture Space Telescope (ATLAST) mission aims to study dark energy, the mysterious form of energy that accelerates the universe's expansion. ATLAST would also detect signatures of life in the atmospheres of Earth-like planets and resolve stars in distant galaxies.
Researchers simulate bubble universe collisions to predict observable signatures, ruling out certain models and providing a proof of principle for the multiverse hypothesis. By producing testable predictions, the multiverse model has crossed the line between appealing story and real science.
Scientists observe electrons jumping between molecular fragments up to a distance of about 20 Ångström, marking the transition from molecular to atomic regimes. The study provides insights into charge transfer mechanisms that play a role in numerous chemical processes, including photosynthesis and solar cells.
Researchers at the Telescope Array observatory detected a disproportionate number of high-energy cosmic rays emanating from a specific area in the northern sky. The discovery provides a promising lead in identifying the sources of these enigmatic particles, which are believed to originate from beyond our galaxy.
Scientists have discovered the corona extends far beyond previous observations, with implications for NASA's Solar Probe Plus mission. Direct measurements of the heliosphere's inner boundary provide new insights into solar particle behavior and the origin of the solar wind.
Researchers David Trilling and Michael Mommert found asteroid 2011 MD to be 65% empty, consisting of a cloud of rocks or dust with a solid rock at its nucleus. This challenges long-held assumptions about the nature of small asteroids.
Researchers investigated two successive three-ribbon solar flares using high-resolution data, revealing a 'fish-bone-like' morphology and surge-like flows. The study suggests magnetic reconnection along the coronal null line is involved in producing the flares and associated coronal mass ejections.
The Interface Region Imaging Spectrograph (IRIS) successfully observed a gigantic coronal mass ejection (CME) on May 9, 2014. The spacecraft caught the event in extraordinary detail, revealing its unprecedented size and structure.
The Palomar Transient Factory successfully observed a supernova exploding in real-time, providing unique spectral features that suggest its progenitor was a nitrogen-rich Wolf-Rayet star. This discovery will aid in understanding massive star evolution and identifying potential supernova precursors.
For the first time, scientists have direct confirmation that a Wolf-Rayet star died in a violent explosion known as a Type IIb supernova. The discovery was made using the iPTF pipeline, which caught the supernova within hours of its explosion and triggered ground- and space-based telescopes to observe the event.