Articles tagged with Observational Astronomy
Researchers analyzed deuterium abundance ratios in protoplanetary disks and found significant variations within a single disk, suggesting differences in chemical composition and physical state at formation sites. The study also reveals the presence of complex organic molecules, including nitriles, in planet-forming disks.
A nearly $2 million NSF grant will accelerate the hunt for low-frequency gravitational waves using high-precision timing observations of exotic stars called millisecond pulsars. WVU's Maura McLaughlin is principal investigator on the project, which aims to discover new types of gravitational waves and expand the IPTA's reach globally.
Researchers from Osaka University and NASA discovered that cold planets exist throughout the Milky Way, even in the Galactic bulge, a region previously thought to be inhospitable to planet formation. The study used gravitational microlensing to determine the distribution of planets across the galaxy.
A new study published in Nature Communications sheds light on the nature of Betelgeuse's mysterious dimming, which was observed from October 2019 to March 2020. The research team found that a temperature drop of 170 K could explain the dimming, suggesting the presence of a large dark star-spot on Betelgeuse's surface.
Researchers use Keck Observatory's MOSFIRE instrument to analyze the layer-cake structure of a nearby free-floating brown dwarf's atmosphere. The study reveals complex cloud formations, including hot sand grains and exotic elements, with depths reaching up to 446 miles.
Recent theoretical findings and astrophysical modeling suggest that scientists can accurately interpret gravitational wave signals from these events, hinting at the existence of so-called 'hierarchical' black holes. The detection of GW190521 in 2019 is thought to be the most promising candidate for such an event.
Astronomers have discovered a 0.6-second gamma-ray burst caused by the implosion of a massive star, revealing that some short GRBs might be imposters in disguise. The discovery suggests that most collapsing stars fail to produce a GRB jet, making this event an effective fizzle.
Researchers have made a groundbreaking discovery about the Sun's magnetic field, revealing that field lines become knotted before emerging at the visible surface. The findings provide conclusive evidence for one of two dominant theories explaining how solar activity occurs.
Scientists use infrared sensors to study the nighttime weather of Venus, discovering that north-south winds run in the opposite direction at night. This observation could help build more accurate models of the Venusian weather system and provide insights into Earth's weather patterns.
Researchers have developed a new radio receiver capable of capturing radio waves at frequencies several times wider than conventional ones. This allows for the detection of multiple types of molecules in space simultaneously, enabling significant progress in studying the evolution of the Universe and star formation.
Researchers at Shinshu University and the National Polar Research Institute found a Forbush decrease in cosmic ray counts during a CME event, but the CR density exceeded its original level before exiting the Magnetic Flux Rope. The high-speed solar wind caused this unusual enhancement of CR density through local compression of the MFR.
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.
The newly discovered exoplanet, TOI-1231 b, has a substantial atmosphere making it an attractive target for atmospheric studies. Its similarity in size and density to Neptune suggests it may have a large, gaseous atmosphere.
Researchers at Tohoku University have discovered a dying supermassive black hole in the Arp 187 galaxy through analyzing radio images and multi-wavelength data. The study indicates that AGN turn-off occurs within a 3000-year time scale, with the nucleus becoming over 1000 times fainter during the last 3,000 years.
Scientists have recorded the most energetic radiation and longest gamma-ray afterglow of a gamma-ray burst, revealing similar spectral characteristics between X-ray and very-high energy gamma-rays. This challenge to established theory highlights the need for further studies of very-high energy GRB afterglow emission.
The Hubble Space Telescope has captured the first-ever direct image of a giant exoplanet, PDS 70b, which is feeding off material surrounding its young star. The observations provide a unique look at radiation from extremely hot gas falling onto the planet, allowing scientists to estimate how fast it's gaining mass.
An international team of researchers searched for pieces of the small asteroid 2018 LA, tracked in space and observed to impact Botswana on June 2, 2018. The recovered meteorites showed it likely came from Vesta, a second-largest asteroid in our Solar System.
The University of Texas at Austin, in partnership with the Arecibo Observatory and other organizations, has successfully moved telescope data to a secure storage system. This move will ensure the continued discovery and innovation sparked by Arecibo's legacy, making its vast astronomy data accessible for over 50 years.
Researchers observed that X-ray emissions coincide with giant radio pulses from the Crab Pulsar, providing constraints on mechanisms underlying these phenomena. The study found that total emitted energy during GRPs is tens to hundreds of times higher than previously known.
Researchers discovered a 800-meter diameter comet nucleus with large grains of phyllosilicate, similar to talcum powder, and evidence of organic molecules. The team used the Subaru Telescope to observe thermal infrared radiation, indicating the surface temperature had reached over 330 degrees Celsius in the past.
Astronomers discovered over 800 dense gas and dust cores near the Galactic Center, which may be 'stellar eggs' hatching into baby stars despite harsh conditions. The findings suggest that star formation is more resilient than thought, with ALMA observations detecting small outflows indicative of star birth.
Scientists have imaged a rare bolide, an extremely bright meteoroid explosion, in Jupiter's upper atmosphere using the Ultraviolet Spectrograph on board the Juno spacecraft. The event was observed for just 17 milliseconds and had distinct spectral characteristics different from the planet's auroras.
The latest observations from Insight-HXMT have discovered the origin of fast radio bursts (FRBs), revealing they come from soft-gamma repeater (SGR) J1935+2154, a magnetar in our Milky Way. This discovery resolves the longstanding puzzle concerning the origin of FRBs.
Researchers have developed a method to reconstruct the early Universe's state, removing gravitational effects from large-scale structure. The ATERUI II supercomputer was used to create simulated universes, revealing that the method can correct primordial density fluctuations and improve inflation constraints.
A team led by Masato Shirasaki applied a reconstruction method to turn back the cosmic clock and remove gravitational effects from simulated universes. They found that their method can correct for gravitational effects and improve constraints on primordial density fluctuations.
An international team of astronomers has developed a new system to directly image exoplanets in the habitable zone of nearby stars, potentially harboring life. Using mid-infrared imaging and adaptive optics, they captured images of planets about three times the size of Earth within habitable zones around Alpha Centauri A and B.
Researchers observed complex magnetic field behavior in a 'radio-loud' magnetar, deviating from previous theories. The findings suggest that the radio pulses originate from loops of magnetic field lines connecting two closely spaced poles.
Researchers at Goethe University and the University of Oklahoma have successfully filmed a quantum wave in a helium dimer. The study uses an extremely powerful laser flash to twist the bond between two helium atoms, allowing them to observe and record the atom flying away as a wave.
The five-layer sunshield of the James Webb Space Telescope has completed a final series of large-scale deployment and tensioning tests, putting the observatory one step closer to its launch. The sunshield protects the telescope from heat and light, maintaining an extremely cold temperature for groundbreaking science in infrared light.
Researchers used combined signals from binary neutron star mergers to study ultra-dense matter and constrain the Hubble constant. The analysis, led by Tim Dietrich, provided new insights into neutron star equation of state and expansion rate of the Universe.
Astronomers observing a dark vortex on Neptune noticed it change direction by August 2020, doubling back to the north. A smaller dark spot, possibly a fragment of the giant vortex, was also spotted near its larger cousin in January this year.
Astronomers use a novel spectrograph to measure the redshift of GN-z11, a ancient galaxy located 13.4 billion light years away, marking it as the farthest detectable galaxy in the universe. The team's precise measurement improves the accuracy of the galaxy's distance by a factor of 100.
Researchers have successfully combined radar and optical observations to study interplanetary dust, gaining insights into meteor mass and composition. By correlating subtle signals in radar data with detailed optical information, scientists can now explore comets and aspects of solar system evolution.
The Five-hundred-meter Aperture Spherical radio Telescope (FAST) detected a weak correlation between fast radio bursts and soft gamma-ray repeater J1935+2154, suggesting a magnetar origin for FRBs. The study provides crucial clues to the generation of FRBs.
A team of researchers used the FAST telescope to detect over 15 fast radio bursts, revealing a galaxy 3 billion light years away as the source. The bursts' polarization signals showed diverse swings, indicating production in compact star magnetospheres and disfavoring shock models.
The study provides new insights into the asteroid's composition, suggesting it may be a dense, metallic object made of iron and nickel. The findings also indicate that oxidation is occurring on the surface, which could be a result of solar wind interaction.
Tropical Storm Nangka generated up to 30 mm of rain per hour around its center, while fragmented bands experienced rates between 5-15 mm/hour. The storm is forecast to strengthen in the Gulf of Tonkin before weakening as it moves towards Vietnam.
A team of astronomers studied sunspots to characterize star conditions, which is crucial for finding exoplanets. The research aimed to create a single emission profile similar to other stars, allowing astronomers to identify dimming caused by exoplanet shadows.
The NASA/ESA Hubble Space Telescope has captured a stunning image of the Great Barred Spiral Galaxy NGC 1365, showcasing hundreds of baby stars and dusty sites of future stellar nurseries. The PHANGS survey, conducted jointly with ALMA in Chile, aims to understand how galaxy environments influence star formation.
Heavy rainfall was found to be occurring around the compact eye of Major Hurricane Marie, with NASA's Integrated Multi-satellitE Retrievals for GPM (IMERG) estimating rainfall rates ranging from 3-20mm/hour. The satellite data provides valuable insights into the storm's intensity and helps improve hurricane forecasting.
NASA estimated Post-tropical Cyclone Beta's rainfall rates as it moved over Mississippi, Alabama, and Tennessee, with heavy rainfall across the region expected. The storm is generating rain at a rate of 10-15 mm per hour over Alabama, while lighter rainfall rates occurred over Mississippi and Tennessee.
Tropical Storm Wilfred formed in the Eastern Atlantic Ocean on September 18, marking the end of the 2020 hurricane season. The storm is generating heavy rainfall rates, with estimates suggesting up to 30 mm per hour around its center.
A new forecasting method, developed with public input, shows increased accuracy in predicting coronal mass ejections and their impact on Earth. The Solar Stormwatch project demonstrated the value of wide-field CME imaging cameras on future space weather monitoring missions.
Researchers found a 1.5 ° C increase in near-ground temperature over four decades at the Paranal Observatory, threatening telescope quality due to air turbulence. Climate change also affects image resolution, contrast capabilities, and potentially limits exoplanet studies.
The OSIRIS-REx mission reveals that asteroid Bennu sheds material periodically, with particles ejecting from the surface and orbiting or falling back onto it. The spacecraft's observations provide insight into the processes likely causing this activity, shedding new light on dynamic asteroids.
A team of researchers found evidence confirming theoretical predictions about gravitational interactions between multi-star systems, resulting in warped disks and misaligned rings. The discovery sheds light on the formation process of planets with extreme orbital angles.
Astronomers detect the most massive black hole collision ever observed, involving two mammoth black holes weighing 85 and 66 times the mass of the Sun. The larger black hole is considered 'impossible' due to its mass exceeding predicted limits.
The discovery of radio jets in the Phoenix Galaxy Cluster suggests that a supermassive black hole is actively heating intra-cluster gas, preventing star formation. This finding has significant implications for our understanding of galaxy evolution and coevolution.
The James Webb Space Telescope successfully completed a critical ground segment test, demonstrating the complete end-to-end flow from planning science observations to downlinking data. This milestone validates the observatory's ability to respond to commands and function in space.
For the first time, researchers have measured the global magnetic field of the solar corona. By applying magneto-seismology to observations from Coronal Multi-channel Polarimeter (CoMP), they mapped the magnetic field in the global corona using wave propagation speed and density data.
NASA's Solar and Terrestrial Relations Observatory (STEREO) has observed unusual dimming in Betelgeuse, a star experiencing an early minimum brightness cycle. The observations, made between late June and early August, show that the star is dimming unexpectedly again, adding to ongoing questions about its behavior.
Researchers tracked the evolution of stellar eggs in Taurus, discovering internal structures and bipolar gas streams that indicate a star's birth. The team used ALMA's compact array to observe starless cores and found evidence for 'first hydrostatic cores,' short-lived objects formed before a baby star's birth.
Astronomers have discovered an exoplanet, K2-25b, that is surprisingly dense for its size and age, defying current planet formation theories. The exoplanet, orbiting a young star in the Hyades cluster, has a mass of 25 Earth-masses and a size slightly smaller than Neptune.
The Apple Fire in Banning Canyon, California, has consumed 20,516 acres and is burning in an area with not had fire activity in recent years. NASA satellites provide critical information on the fire's spread, detecting actively burning fires and tracking smoke transport.
Scientists developed a new model using NASA's Solar Dynamics Observatory data, predicting seven of the Sun's biggest flares from the last solar cycle. The model identified key characteristics in active regions, including magnetic reconnection and unstable arches, to predict massive flares.
Astronomers have successfully detected a superflare on the nearby red dwarf AD Leonis, with one flare being 20 times larger than those emitted by our sun. The high-quality data from the Seimei Telescope has revealed intriguing phenomena, including an increase in high-energy electrons and unusual light patterns.
Astronomers using TESS and Spitzer data report the discovery of AU Mic b, a Neptune-like planet that orbits its young star in under 10 days. The system offers a unique laboratory for studying planetary atmospheres and interactions with stars.
Astronomers have detected a supermassive black hole's heartbeat, which has been ongoing for over ten years. The signal was spotted again in 2018 using X-ray satellite observations, providing valuable information about the black hole's event horizon.
Astronomers have observed a confirmed heartbeat in a supermassive black hole for over ten years, with the signal repeating every hour. The research provides new insights into the black hole's size and structure close to its event horizon.
A four-year study at Jodrell Bank Observatory reveals a repeating Fast Radio Burst (FRB) follows a cyclic pattern with radio bursts observed every 90 days, followed by a silent period of 67 days, repeating every 157 days. This discovery provides an important clue to identifying the origin of FRBs.