Articles tagged with Astrophysics
The study suggests that Venus' atmosphere plays a crucial role in determining its rotation speed, with fast winds dragging along the surface and slowing it down. This has significant consequences for the sweltering Venusian climate, with average temperatures of up to 900 degrees Fahrenheit.
Astronomers identify GNz7q, a dusty compact object with properties of both galaxies and quasars, born 750 million years after Big Bang. The discovery provides new insights into the rapid growth of supermassive black holes in early universe.
A new experimental setup provides precise calibration references for soft X-ray transition energies in neon, carbon dioxide, and sulfur hexafluoride gases. This improves the accuracy of astrophysical plasma analysis, enabling scientists to access techniques currently not available.
Researchers have discovered a large sample of compact galaxies, including the rare 'Green Pea', 'Blueberry' and 'Purple Grape' types. These galaxies are found to have high star formation rates and low metallicity, providing new insights into galaxy formation and evolution.
Researchers have created the Thesan simulation, a cubic volume spanning 300 million light years across, to study cosmic reionization and galaxy formation. The simulation aligns with observations and sheds light on key processes, such as how far light can travel in the early universe.
Physicists from Cracow-based Institute of Nuclear Physics found that the proton's charm structure might affect our understanding of cosmic neutrinos. Recent LHCb detector measurements support a model with a higher charm quark contribution, which could mislead astronomers about high-energy neutrino origins.
Researchers suggest that asteroid Ryugu could be a relic of an ancient comet due to its high organic content and spinning top shape. The study proposes a simple physical model that fits the observed data, suggesting that comets can leave behind rocky debris in the inner solar system.
Three exoplanets mistakenly identified as planets are actually small stars, according to a new MIT study. The discovery was made using updated measurements of planet-hosting stars from the European Space Agency's Gaia mission.
Researchers propose a new mechanism for eccentric black hole mergers, suggesting that interactions between three black holes in a flat disk environment could lead to chaotic orbits. This finding challenges previous studies on the rarity of such events.
Researchers used simulations to compare Einstein's theory and modified gravity, finding that 'dark gravity' may be equally good at explaining data from binary neutron star collisions. This could lead to the discovery of new phenomena detectable by next-generation gravitational interferometers.
A team of international scientists has created a detailed radio image of over 4.4 million objects in the northern sky, including galaxies with massive black holes and new star-forming regions. The discovery is made possible by state-of-the-art data processing algorithms and high-performance computing resources.
Neutrinos, produced by astrophysical sources and artificial means, interact subtly with matter due to their chargelessness and masslessness. The study of neutrinos challenges our understanding of particle physics, particularly the phenomenon of neutrino oscillation, where particles transition between three flavours.
The study provides the first detailed view of an exoplanet's global atmosphere, revealing a water cycle that dwarfs Earth's jetstream. The planet's night side is home to iron clouds, titanium rain, and winds that whip around at speeds of up to 5 kilometers per second.
Researchers propose that cognitive activity operating on a planetary scale is necessary to tackle global issues. A mature technosphere involves integrating technological systems with Earth through feedback loops, making it self-maintaining and exhibiting emergent behavior.
Researchers have updated the lunar chronology model using radiometric ages of new Chang'E-5 samples and crater counting data from the landing area. The new model provides a more accurate timescale, essential for understanding lunar and planetary history.
Physicists at the University of Sussex have developed a remote monitoring system for quantum devices, allowing for real-time control and issue resolution. This system enables researchers to monitor environmental factors such as temperature, pressure, and laser beams in ultracold quantum laboratories.
Physicists have measured the oscillation frequency of Bs0 mesons with unprecedented accuracy, revealing that they oscillate between matter and antimatter three trillion times per second. This measurement agrees with quantum mechanics predictions and narrows search areas for particles undescribed by the Standard Model.
The CUNY Graduate Center is introducing a comprehensive and fully funded Astrophysics master’s program, alleviating financial barriers for low-income students from underrepresented communities. The program, supported by the Simons Foundation, will provide tuition-free education and research opportunities.
Researchers found that passing stars, misaligned binary stars, and passing gas clouds can warp protoplanetary discs, disrupting spiral structures. This warping heats up the disc, making it harder for planets to form via gravitational instability.
A team led by Basmah Riaz has detected deuterated methane in three proto-brown dwarfs, indicating a warmer gas composition than expected. This finding suggests that brown dwarfs may not be simply scaled-down versions of stars.
A team of astronomers has discovered a mysterious object releasing giant bursts of energy three times an hour, which could be a neutron star or white dwarf with an ultra-powerful magnetic field. The object is incredibly bright and smaller than the Sun, emitting highly-polarised radio waves.
Scientists at Osaka University demonstrated the ability to generate gigagauss magnetic fields via gyro motion of relativistic electrons, with polarity reverse occurring instantly. The study, published in Scientific Reports, reveals a new mechanism for magnetic field growth and amplification.
Astronomers have captured detailed images of sinuous stellar jets emanating from young stars, suggesting that their sidewinding appearances are caused by gravitational attraction from companion stars. The observations were made using the Gemini South telescope's adaptive optics system.
Researchers have discovered a giant gas planet, TOI-2180 b, with a diameter comparable to Jupiter's and a mass nearly three times that of Earth. The planet is also believed to contain 105 times the mass of elements heavier than helium and hydrogen.
Researchers have found the Milky Way to be significantly lighter than previously thought, with a total mass of 500-800 billion solar masses. This new estimate is based on high-precision data from Gaia EDR3 and advanced dynamical modeling methods.
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.
The ARC Centre of Excellence for All Sky Astrophysics in 3D has discovered that the youngest generation of stars will eventually stop contributing metals back to the universe. This change affects the composition of the galaxy over time, with around half of the carbon and all elements heavier than iron synthesized by stars like our Sun.
The FAST telescope detected accurate magnetic field strength in molecular cloud L1544, suggesting an early transition to supercriticality. The HINSA Zeeman effect revealed a coherent magnetic field structure throughout the interstellar medium.
A new study proposes that life could neutralize acidic environment, creating habitable pockets in Venus' clouds. The researchers identified a chemical pathway by which life could produce ammonia, explaining observed anomalies and anomalies.
Researchers have discovered that vast ice forms on Pluto's surface are formed by the sublimation of nitrogen ice, powering convection in the ice layer of Sputnik Planitia. This process is consistent with climate models and has implications for other planetary bodies.
An international team of astronomers has created a new map of the Milky Way's outer disc using data from the Gaia space mission. The findings reveal many previously unknown coherently rotating filamentary structures at the edge of the disc.
A team of astronomers has developed a new technique to detect active black holes in galaxies, measuring their impact on galaxy evolution. The method can be applied to millions of galaxies, searching for bright supermassive black holes at the centre of galaxies and studying their effect on star formation.
Researchers discovered a compact object in supernova AT2018cow, which was a product of a dying star. The team found X-ray pulses indicating an object measuring no more than 1,000 kilometers wide and with a mass smaller than 800 suns.
Physicists at Technical University of Munich discover potential existence of tetra-neutron, a bound state of four neutrons, which could significantly alter our understanding of nuclear forces. The experiment's results suggest a half-life of 450 seconds and stability comparable to the neutron.
Researchers at the DOE's Princeton Plasma Physics Laboratory discovered a process in plasma swirling around black holes that causes previously unexplained emissions of light and heat. The process, known as magnetic reconnection, also jettisons huge plumes of plasma billions of miles in length.
A team of researchers has discovered a new object orbiting a Sun-like star that was missed by previous searches. The object is estimated to be between 10 and 20 times the mass of Jupiter and is thought to be a large planet or a small brown dwarf.
Astronomers observed a young, sun-like star ejecting a massive burst of energy and charged particles, potentially bad news for satellites and power grids. The study suggests that similar events could have shaped planets like Earth and Mars over billions of years.
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.
A team of astrophysicists led by Boston University's Merav Opher has made a groundbreaking discovery about the heliosphere, the bubble surrounding our solar system. Their research suggests that neutral hydrogen particles play a crucial role in shaping the heliosphere's structure and stability.
Scientists from Niigata University, Academia Sinica Institute of Astronomy and Astrophysics, and the National Astronomical Observatory of Japan detected a newborn star and its surrounding cocoon of complex organic molecules in the extreme outer Galaxy. The discovery reveals the hidden chemical complexity of our Universe.
A new study reveals how Earth's volatile elements, such as hydrogen, nitrogen, and carbon, were formed through a combination of deep Earth processes, oceans' formation, and meteor impacts. The research suggests that these elements played a crucial role in creating the habitable environment necessary for life to emerge.
A team of astronomers discovered eight new stars and three more previously known stars belonging to the rare 'Main-sequence Radio Pulse emitters' (MRPs) using the GMRT. These discoveries suggest that MRPs may be more common than thought, but are difficult to detect due to their radio pulses being visible only at certain times.
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.
Researchers have successfully created an experimental model of a skyrmion particle in a beam of light, providing a real system to demonstrate the behavior of this elusive type of fundamental particle. The study reveals the intricate structure and topological properties of skyrmions, which can be distorted but not broken.
Astronomers have discovered two previously invisible galaxies 29 billion light-years away that were camouflaged by cosmic dust. The discovery suggests that up to one in five such distant galaxies may still be hiding behind the cosmic veil.
The WVU-led Dolly Sods GPU cluster enables researchers to accelerate computational research in fields like drug development, interstellar phenomena, and biometrics. The cluster will facilitate the analysis of massive datasets and enable real-time processing of signals from satellites in space.
Researchers used NASA's Hubble Space Telescope to focus on a post-starburst galaxy nearly 500 million light years away. They discovered two periods of intense starburst before the galaxy stopped forming stars, shedding new light on its history and evolution.
An international research team has measured neutron form factors with previously unattained precision, filling a blank space on the map. The new data provides a more comprehensive picture of the neutron's size and lifetime, and reveals oscillating patterns in its form factor.
Theoretical physicists modelled the region around M87's supermassive black hole, confirming that gravity plays a key role in accelerating particles out to thousands of light years. The findings provide further evidence for Einstein's theory of general relativity and its application to astrophysical phenomena.
A new study suggests that black holes grow in lockstep with the expanding universe, a phenomenon called cosmological coupling. This idea improves the explanation for large black hole masses observed in gravitational wave observatories.
A new study suggests that a gravitational 'kick' from colliding supermassive black holes could be responsible for the strange shape of stars at the center of the Andromeda Galaxy. The team used computer simulations to track the consequences of such a merger, finding that it could knock millions of stars into wonky orbits.
Researchers recreated superionic ice using advanced tools and found a new phase of matter. The ice has unique properties that make it less dense but darker, and its behavior affects planetary magnetic fields.
Researchers at MIT and UNH find that binary neutron star mergers produce two to 100 times more heavy metals than neutron star-black hole mergers. The study suggests that binary neutron stars are a likely cosmic source for gold, platinum, and other heavy metals.
Researchers have discovered evidence of a giant impact that occurred in a nearby star system, stripping part of the planet's atmosphere. The team observed carbon monoxide gas around the star, which they believe was released from a massive impact involving two proto-planets.
The Chang'E-5 mission has provided new insights into the Moon's surface features, including the Ocean of Storms, which may have been even more stormy than previously thought. The samples also reveal a distinct lunar basalt composition different from Earth-based basalt.
A team of researchers observed the evolution of warm gas coming from an active black hole for unprecedented detail, revealing structures reminiscent of volcanic eruptions. These gas bubbles, rings, and 'intergalactic smoke' filaments are formed when black holes consume surrounding matter and release energy, influencing galaxy evolution.
The special issue covers observations of exoplanet geology, composition, atmosphere, and potential habitability. SwRI researchers Dr. Natalie Hinkel and Dr. Cayman Unterborn collaborated with Dr. Oliver Shorttle to create a diverse overview of exoplanets, making it accessible to a wide community of scientists.
A new analysis suggests that a gap existed within the protoplanetary disk around 4.567 billion years ago, near the asteroid belt, affecting the composition of infant planets. The team found that meteorites from the outer region had stronger magnetic fields than those from the inner region.
Two independent research groups unveil new measurements to explain the birth of half the universe's elements. One group uses laboratory techniques to hunt for 'astromers,' while the other compares heavy elements in stars to better understand their origin.
A new study by WMU Professor Michael Famiano and colleagues finds that high magnetic fields in neutron stars can alter the composition of ashes and affect electron capture rates. This discovery has significant implications for our understanding of stellar environments and the formation of elements.