Articles tagged with Sun
A new study led by NCAR suggests that many coronal loops on the Sun are actually wrinkles in a bright plasma veil, rather than distinct strands of plasma. This finding has significant implications for understanding the Sun's atmosphere and density, temperature, and other physical characteristics.
A team of researchers detected a ring of planetary debris surrounding the white dwarf WD1054–226, suggesting a nearby planet may be present in its habitable zone. The study found that the debris is kept in a precise arrangement by a nearby planet's gravitational influence.
Astronomers at Harvard & Smithsonian Center for Astrophysics offer a new explanation for mysterious downflows in solar flares, which are not generated by magnetic reconnection. Instead, they form from the interaction of two fluids with different densities, resulting in 'dark finger-like voids'.
A new study by Rice University astrophysicist André Izidoro suggests that the sun had rings before planets formed, explaining many solar system features. The model simulates the solar system's formation hundreds of times and reproduces several features missed by previous models, including pressure bumps and rings.
Researchers found that local gravitational tides modulate the cyclical behavior of organisms, even in the absence of other rhythmic influences. The study questions the validity of free-run experiments and highlights the importance of considering gravitational oscillations in biological research.
Parker Solar Probe successfully flew through the Sun's corona, sampling particles and magnetic fields, revealing critical information about the Sun's evolution and impact on solar system. The probe made new discoveries, including identifying the origin of switchbacks in the solar wind, which form near the solar surface.
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.
The Solar Jet Hunter project, led by researchers at the University of Minnesota and supported by NASA, allows volunteers to identify solar jets in images captured over 11 years. By annotating images, citizen scientists contribute to a database that helps narrow down data on the Sun for further review.
Researchers from Washington University in St. Louis have discovered a new type of exoplanet known as 'eggshell planets,' which are likely to have little topography and no plate tectonics. These planets may resemble the lowlands on Venus, with vast expanses of lava but little high-standing terrain.
Scientists have discovered that hypervelocity dust impacts on a spacecraft can produce plasma explosions and create debris clouds, disturbing its operations. These events can also generate clouds of debris that expand away from the spacecraft.
Researchers have discovered a way to harness hot helium ash to drive rotation in fusion reactors, reducing instabilities and turbulence. By capturing the energy of hot fusion ash via alpha channeling, plasma rotation can be stabilized, leading to improved performance and reduced operating costs.
A team of researchers used paleomagnetism models and historical documents to create a map of the auroral zone over the last 3,000 years. They found that the auroral zone has moved significantly over time, with notable changes occurring in the 12th century and 18th century.
A research team from Göttingen University observed magnetic forces arranging gas particles in solar prominences, with charged particles moving at speeds of up to 42 km/s. This phenomenon is significant for understanding astrophysical processes, including star and planet formation.
Researchers from DTU Space and The Hebrew University of Jerusalem found that solar eruptions reduce cosmic ray flux, leading to reduced aerosol production and decreased cloud cover. This results in an increase in the Earth's energy budget by almost 2 W/m2 within 4-6 days.
Researchers at Skoltech have identified a favorable window of opportunity for manned Mars missions in the mid-2030s. The study suggests that launching during the decaying phase of solar activity can help shield astronauts from cosmic rays, allowing for longer flight durations.
A NASA model describes Kappa 1 Ceti, a 30-light-year-away star with similar mass and surface temperature to our young Sun. The study sheds light on what allowed our Sun to foster life on nearby planets, including Earth's atmosphere and the development of biological molecules.
The newly launched NEID spectrometer will measure the minute gravitational tug of planets on their host stars, enabling the detection of rocky planets and characterization of exoplanetary atmospheres. By utilizing this technology, scientists aim to push the boundaries for searching smaller exoplanets and probing beyond past challenges.
A new method has been developed to detect stealth coronal mass ejections (CMEs) that can wreak havoc on Earth. By analyzing slow changes in the lower corona using difference images, researchers have successfully predicted the trajectory and potential impact of four stealth CMEs.
Scientists at Stanford University have developed a technique using solar radio signals to measure the depth of ice sheets and glaciers, which could lead to large-scale insight into melting ice sheets and sea-level rise. The passive radar system uses naturally occurring radio waves from the sun to detect changes in ice thickness.
Researchers calculate sun's electric field distribution, revealing its impact on solar wind acceleration. The study provides new insights into the sun's interaction with charged particles and their effect on Earth's activities.
Scientists found that Mercury's large iron core is linked to the early sun's strong magnetic field, which pulled metal grains inward. This discovery sheds light on the formation of rocky planets' cores and their elemental distribution.
Researchers have determined that a massive star, rather than the young sun, was responsible for the split in oxygen isotopes found in the sun and other planets. The study, led by Lionel Vacher, used an unusual meteorite named Acfer 094 to gain insight into the solar system's past.
A new study from the University of Maryland disputes the prevailing hypothesis on Mercury's big core, instead attributing it to solar magnetism. The model shows that a planet's core density and proportion of iron are correlated with the strength of the sun's magnetic field during planetary formation.
During their marathon flights, great snipes change elevation depending on time of day, typically flying higher in daylight to escape heat and finding a behavior that's optimal for them. They reach astonishing altitudes, with one bird flying as high as 8,700 meters, nearly as high as Mount Everest.
Researchers used Gaia eDR3 catalog data to determine which stars pass through the Earth Transit Zone over a 10,000-year period. This allows nearby star-systems to potentially detect Earth, with 1,715 systems having had this opportunity since human civilization began.
For the first time, scientists have created a 3D map of the heliosphere boundary using data from NASA's Interstellar Boundary Explorer (IBEX) satellite. The boundary marks the edge of the solar system and protects Earth from interstellar radiation.
Researchers propose comprehensive explanation of sun cycles based on planetary attractive forces, reproducing known solar activity fluctuations. However, long-term forecasts become impossible due to chaotic process in activity over thousands of years.
Astronomers observed a massive protostar called Cep A HW2, revealing two distinct features: a wide-angle wind near the star and a highly-collimated jet at a greater distance. The discovery raises questions about the formation mechanisms of stars across different mass spectrums.
Researchers developed new software for improved space weather prediction, leveraging supercomputers and advanced computing techniques to analyze magnetized solar wind plasma. This effort aims to enhance the accuracy of predictions for coronal mass ejections and their impact on Earth's magnetosphere.
A NASA mission evaluates interactions between the sun and earth's magnetic fields, which can cause explosive energy transfers disrupting technology systems. A UTA professor recruits a first-year doctoral student to join the mission, where he will learn about meaningful magnetospheric events.
Researchers have discovered a persistent signature of plasma waves in the interstellar medium using Voyager 1's Plasma Wave System. The detection allows scientists to understand how the solar wind interacts with the interstellar environment.
Researchers at DOE's Princeton Plasma Physics Laboratory receive $2 million in funding to investigate magnetic reconnection and plasma blobs that can disrupt communications satellites. They aim to recreate conditions in the magnetosphere using a device resembling an enormous silvery barrel tipped on its side.
Three carbon-based materials have been predicted to exhibit omnidirectional auxetic behavior due to their negative Poisson's ratio. The findings suggest that these materials could be useful in photovoltaic devices or as light-powered catalysts.
Scientists at Princeton Plasma Physics Laboratory have developed a new computer model that accurately predicts the behavior of plasma in the sun's solar corona. This breakthrough could lead to better space weather predictions and improve the understanding of magnetic reconnection, which drives the fusion reactions that power the sun.
The Interstellar Probe mission aims to study how our Sun interacts with the local interstellar medium and learn more about the formation and evolution of the heliosphere. The probe will take 'images' of the heliosphere using energetic neutral atoms and observe extragalactic background light, shedding new light on the region.
A massive flare from Proxima Centauri, the star closest to our sun, has been detected, shattering previous records. The flare was observed for 40 hours using nine telescopes and produced a wide spectrum of radiation.
Astronomers have observed a record-breaking flare from Proxima Centauri, the Sun's nearest neighbor, using nine instruments. This extreme outburst offers valuable insights into stellar flares and their potential impact on exoplanet life.
A team of experts, including Phoebe Zarnetske and Jessica Gurevitch, investigate the ecological impacts of reflecting sunlight to cool the planet. Their research highlights the complexity of cascading relationships between ecosystem function and climate under different scenarios.
Researchers suggest most of Earth's carbon was delivered from the interstellar medium, avoiding vaporization entirely. This discovery sheds light on the origin of life on Earth and suggests a delicate balance between too little or too much carbon for habitability.
Researchers discover that filters used in solar storm detectors are losing their ability due to another stowaway from Earth, not just carbonization. This issue affects satellite data quality and reliability, sparking efforts to create more accurate space weather forecasts.
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.
Researchers have found a curious signal that could be the first known world around Vega. The alien planet would orbit close to Vega and rank as the second hottest world known to science.
A wayward comet-like object has been spotted near a family of captured ancient asteroids, called Trojans, orbiting the Sun alongside Jupiter. The object shows signs of comet activity, such as a tail, outgassing, and an enshrouding coma of dust and gas.
Sun and Tong's project aims to make AI workflows more shareable and replicable. The researchers will further develop the open-source GeoWeaver system into a stable operational platform for NASA's EOSDIS archive.
The CLASP2 sounding rocket experiment charted the magnetic field strength all the way up to the top of the chromosphere, a long-sought goal. This breakthrough brings scientists closer to understanding how magnetic fields heat the solar corona.
The stellar-mass black hole in the Cygnus X-1 binary system was found to have a mass 21 times that of the Sun and is rotating at a speed close to the speed of light. This discovery challenges astronomers' thoughts on how black holes formed.
A new study by Harvard researchers suggests that a comet originating from the Oort cloud was bumped off-course by Jupiter's gravitational field, increasing the rate of impacts on Earth. The theory provides a satisfactory explanation for the origin and composition of Chicxulub impactor, potentially shedding light on other similar craters.
Farfarout is the most distant known object in our Solar System, with an orbit taking it 175 au from the Sun at its farthest point. Its discovery provides insights into the history of the outer Solar System and the potential for future interactions with Neptune.
The team discovered a planetoid dubbed 'Farfarout,' located 132 astronomical units (au) from the Sun, making it the most distant object ever observed. It has a highly elongated orbit that takes approximately 1,000 years to complete, crossing Neptune's orbit every time.
Researchers link magnetic waves in chromosphere to areas of abundant ionised particles in hot outer atmosphere, explaining the Sun's unique chemical make-up. The discovery provides a foundation for understanding the solar wind and its impact on Earth.
Scientists have gained new insight into the solar structures that create the Sun's flow of high-speed solar wind. Using NASA data and cutting-edge image processing, researchers discovered plumelets, smaller strands of material within solar plumes, which shape the solar wind's characteristics.
A team of astronomers has created the most complete 3D map of cool brown dwarfs in the Sun's local neighborhood, cataloging over 500 objects including 38 new discoveries. The results provide evidence that the Sun's immediate neighborhood is unusually diverse relative to other parts of the Milky Way Galaxy.
A Northwestern University study discovered that stellar flares could play an important role in a planet's atmospheric evolution and habitability. Flares may drive a new chemical equilibrium in a planet's atmosphere, potentially making it easier to detect signs of life.
Researchers predicted the corona's appearance using NASA data, but the actual appearance was hazier and calmer than expected due to changes in the Sun's magnetic field. The team made adjustments for the Sun's increasing activity, which affects space weather.
Sunscreen reduces skin cancer risk by blocking solar radiation; use of sunscreen is crucial beyond just sun protection, also for premature aging prevention.
The Borexino detector successfully detected CNO neutrinos, revealing the final secret of our sun's fusion cycle. The detection confirms predictions that carbon and nitrogen catalyze hydrogen burning, releasing these 'ghost particles' that provide insight into the sun's interior.
The Parker Solar Probe has discovered that the densities of dust particles around the sun vary wildly over months, contradicting scientists' expectations. This finding suggests a more complex and fast-shifting dusty environment than previously thought, with implications for understanding planet formation.
Researchers find preferential heating of heavier ions like silicon in the transition region, which is thought to be a key mechanism for coronal heating. The study provides insights into how magnetic reconnection and ion cyclotron heating contribute to the sun's super-hot atmosphere.
Researchers at the University of Huddersfield and Montanuniversitaet Leoben in Austria have developed a new aluminium alloy that resists radiation damage, making it suitable for use in spacecraft. The alloy's T-phase has a complex crystal structure that prevents hardening precipitates from dissolving under high radiation doses.
The Borexino experiment has successfully detected low-energy neutrinos from the Sun's carbon-nitrogen-oxygen (CNO) cycle, a process that produces about 1% of the Sun's energy output. This detection provides valuable insights into the CNO cycle and its role in the energy production of stars, including our own Sun.