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.
The new data includes exceptionally accurate measurements of the 300,000 stars within the closest 326 light years to the Sun. Researchers predict how the star background will change in the next 1.6 million years and confirm that the Solar system is accelerating in its orbit around the Galaxy.
Scientists have detected new types of solar electron bursts accelerated by shock waves from coronal mass ejections. The Voyager spacecraft, over 14 billion miles from the sun, recorded these bursts, which were linked to cosmic rays and provided valuable insights into interstellar physics.
A Rutgers-led study suggests the most habitable region for life on Mars would be up to several miles below its surface due to subsurface melting of thick ice sheets. Liquid water may have been stable at great depths, allowing life to thrive through hydrothermal activity and rock-water reactions.
A study found that telemedicine adoption in emergency rooms significantly shortened average length of stay and wait time. This is achieved through efficient information exchange, flexible resource allocation, and improved specialist consultations.
The Borexino experiment has successfully measured neutrinos from the sun's second fusion process, the Carbon Nitrogen Oxygen cycle (CNO cycle), confirming theoretical predictions. The findings provide evidence on the metallicity of the sun and have implications for understanding the properties of stars.
A team of scientists has detected neutrinos from the sun directly revealing that the carbon-nitrogen-oxygen (CNO) fusion-cycle is at work in our sun. This detection confirms the CNO cycle as the dominant energy source powering stars heavier than the sun.
The Borexino Collaboration has directly detected CNO cycle neutrinos in the Sun for the first time, providing conclusive proof of this fusion process. The researchers estimated that CNO neutrinos account for about 1% of the energy produced by the Sun.
The NSF's National Solar Observatory has predicted the arrival of a large sunspot on November 18, coinciding with Thanksgiving. The prediction uses helioseismology to detect changes in sound waves from the Sun's interior and is valuable for understanding space weather effects.
A study of ancient star orbits reveals unexpected patterns, contradicting previous assumptions about the Galaxy's metal-poor stars. The research, conducted by a team of astronomers, found that some of these stars orbit in previously unpredicted paths, similar to the Sun's path within the disk.
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.
Scientists have successfully measured the iron lines in the solar spectrum using a laser frequency comb and HARPS instrument, verifying one of Einstein's predictions - the gravitational redshift effect. This confirms that General Relativity theory is correct and has significant implications for satellite navigation systems like GPS.
A new study has discovered that accumulated DNA damage in skin cells can be used to estimate the risk of deadly skin cancer. Researchers sequenced DNA from individual melanocytes and found a significant number of mutations associated with melanoma, even in people without visible moles.
The desert locust's two internal compasses rely on the sun's position and sky polarization patterns. The protocerebral bridge in the central complex encodes 360 degrees of space, enabling navigation based on combined cues from the sky.
Researchers use NASA's IRIS mission to spot nanojets in the solar corona, revealing a potential coronal heating candidate: nanoflares. The observations confirm that nanojets are a telltale signature of magnetic reconnection and nanoflares contributing to coronal heating.
A study of over 260,000 people found that genetics play a key role in sun-seeking behaviour, making it more challenging to address excessive sun exposure. The research identified five genes linked to behavioural traits associated with risk-taking and addiction.
Astronomers using NSF's NOIRLab facilities and citizen science project Backyard Worlds have discovered approximately 100 cool brown dwarfs near the Sun, with several of these worlds approaching Earth's temperature. These discoveries provide new insights into the formation and atmospheres of planets beyond our Solar System.
Scientists have discovered helium structures in the Sun's atmosphere using a NASA sounding rocket, revealing new insights into the origin and acceleration of the solar wind. The findings suggest that the abundance of helium is strongly connected to the magnetic field and speed of the solar wind in the corona.
Researchers have developed a new method to map the magnetic field of the solar corona using near-infrared observations. The technique, presented in a recent study, can provide detailed maps of the coronal magnetic field across the entire observable corona.
Researchers at Aalto University found that the quiet Sun is more active than previously thought, with radio brightenings and solar storms detected during the solar minimum period. These findings suggest that solar activity cycles may not always follow traditional 11-year patterns.
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.
Researchers have developed a highly efficient solar-flow battery that can store and redeliver renewable electricity from the sun. The device achieved a record efficiency of 20 percent conversion, outperforming previous records by 40%. This breakthrough could potentially yield a new way to harness, store and use the sun's energy for sol...
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.
Researchers discovered that Sun-like stars create lithium later in their lives, after swelling into red giants, contradicting previous theories. This finding will help improve understanding and modeling of Sun-like stars, including their contribution to the lithium content of our Galaxy and planets like Earth.
UTEP research reveals a new target for tuberculosis drug development by investigating the mechanisms of Mtb pathogenesis and discovering that Nα-acetylation of EsxA drastically affects the course of infection. The study provides a beautiful story in the prestigious Journal of Biological Chemistry.
Researchers have detected a system of super-Earths orbiting the nearby star Gliese 887, a red dwarf with conditions suitable for liquid water and potentially hosting life. The newly discovered planets are large enough to be rocky worlds and could retain their atmospheres due to the star's low activity.
Researchers from NYU Abu Dhabi used helioseismology to analyze the Sun's interior and found that the meridional flow is a single cell in each hemisphere. This process determines the characteristics of the sunspot cycle, supporting the flux-transport dynamo model.
Scientists studied sunspots and their movement, discovering a giant cell in each hemisphere with plasma moving towards the equator at 15 km/h. The meridional flow explains why sunspots emerge closer to the equator as solar cycles progress.
The study uses IBEX's long record to examine how the Sun's mood swings play out at the edge of the heliosphere. The results show the shifting outer heliosphere in great detail, hinting at processes behind one of its most puzzling features.
Citizen scientist Trygve Prestgard discovers 4,000th comet in SOHO data, part of the Kreutz family of sungrazers. The comet is extremely faint and close to the Sun when discovered, making it impossible to see without a telescope.
A team of scientists at Tata Institute of Fundamental Research has detected tiny flashes of radio light from all over the Sun, identified as evidence for small magnetic explosions. These discoveries could explain the long-standing coronal heating problem, with preliminary estimates suggesting that these tiny explosions collectively hav...
Researchers have found large clones of skin cells caused by UV exposure can be targeted to reduce skin cancers. This study suggests that stopping these clones may help win the battle against skin cancer.
The Solar Ring mission aims to study the Sun and its influence on the inner heliosphere using a novel six-spacecraft configuration. The mission will provide unprecedented capabilities, including determining the photospheric vector magnetic field with unambiguity and resolving solar wind structures at multiple scales.
Researchers found that stem cell treatment eliminates sun-damaged elastin network and replaces it with normal tissues and structures, even in deeper layers of skin. The treatment triggers cellular- and molecular-level pathways involved in skin repair and regeneration.
A study of 369 solar-like stars reveals that the Sun's solar brightness variations are among the weakest, with fluctuations typically about 5 times stronger in other stars. The research suggests that our star may have been unusually inactive over the past 9000 years.
Researchers analyzed 369 solar-like stars and found that the Sun is less magnetically active and variable than similar stars. The study suggests that most stars are five times more variable than the Sun over the last 140 years, with potential explanations including long-term variability or unrecognized differences.
University of Wisconsin-Madison physicists have provided an explanation for the discrepancy in solar wind temperature. By applying mirror machine theory, they found that the hot electrons stream from the sun to large distances, losing energy slowly and distributing it to trapped particles.
Researchers identified ammonium salts as a substantial source of nitrogen in comets like 67P/Churyumov-Gerasimenko. This discovery resolves the long-standing N/C ratio discrepancy between comets and the Sun.
A new study has refined our understanding of the amount of hydrogen, helium, and other elements present in violent outbursts from the Sun. The research found that helium and neon are enriched in coronal mass ejections, providing clues to the underlying physics in the Sun.
Researchers observed solar energetic particle events and found that pre-accelerated particles build up in front of coronal mass ejections, creating a new phase of the energization process critical for radiation hazards. The study highlights the complex interplay between flares, particle populations and CMEs.
A SwRI-led team used data from NASA's Parker Solar Probe to identify low-energy particles near the Sun, likely originating from solar wind interactions beyond Earth orbit. The particles are thought to be created by stream interaction regions and can pose a radiation threat to space travelers and technology.
The NSF's Daniel K. Inouye Solar Telescope has produced its first images, showcasing a pattern of turbulent plasma that covers the entire sun. This breakthrough will enable scientists to better understand space weather and its impacts on Earth.
Ants cultivate plants in full sun to obtain more floral food, but this condition also leads to increased plant damage and fewer plant numbers. In contrast, shade-cultivated plants produce less food for the ants but receive more nitrogen fertilizer input.
Scientists observe a new type of magnetic explosion, known as forced reconnection, triggered by a solar eruption. This discovery confirms a decade-old theory and may help predict space weather and understand the Sun's atmosphere.
The first identified interstellar comet, 2I -- Borisov, is being tracked by NASA's Hubble Space Telescope as it passes close to the Sun. The comet's nucleus is estimated to be smaller than half a kilometer in diameter and has a chemical composition similar to comets found within our solar system.
The Parker Solar Probe has returned significant data on the Sun's atmosphere, revealing insights into the solar wind and its effects on space weather. The probe's findings have shed light on magnetic disturbances in the solar wind and the processes that heat the Sun's outer atmosphere.
The Illinois-led project aims to provide a transformative leap in revealing the sun's corona, an aura of plasma surrounding stars. The distributed telescope will utilize novel technologies like precision formation flying and diffractive optics for breakthroughs in space imaging.
The Parker Solar Probe has discovered new evidence on how the solar wind is accelerated away from the Sun's surface, finding that bursty 'spikes' originate in holes near the equator and are generated by magnetic reconnection. The probe also measured a sideways speed of the solar wind, which contradicts previous predictions.
The Parker Solar Probe has mapped the source of the slow solar wind to coronal holes on the sun's surface, which are cooler and less dense than surrounding corona. The probe also detected switchbacks in the magnetic field that may accelerate particles toward Earth, posing potential damage to electrical grids and orbiting satellites.
New data from NASA's Parker Solar Probe reveals that energetic particles hurtling out of the sun are more varied and numerous than previously thought, according to results from the Integrated Science Investigation of the Sun instrument suite. This discovery could provide early warnings for solar storms and improve space weather forecasts.
The Parker Solar Probe mission has unveiled a surprisingly chaotic world within the sun's corona, characterized by rogue plasma waves, flipping magnetic fields, and distant solar winds. The findings have significant implications for space weather forecasting and our understanding of the sun's behavior.
The Parker Solar Probe has completed three passes through the Sun's atmosphere, revealing new information about the material and particles that speed away from the star. The data shows a complicated, active system with quick reversals in the magnetic field and sudden, faster-moving jets of material.
Teams from Cerro Tololo and Kitt Peak Observatories imaged Mercury's transit with different telescopes and cameras. The goal is to measure the parallax shift caused by Mercury's apparent position on the Sun to calculate the distance to the Sun.
A team led by Queen's University Belfast scientist Dr. David Jess discovered that the Sun's magnetic waves strengthen and grow due to the formation of an 'acoustic resonator', where temperature changes create boundaries that trap the waves, allowing them to intensify.
New research suggests that ancient microbes played a crucial role in forming massive iron ore deposits and keeping the early atmosphere warm. The findings provide strong evidence for the 'faint-young-sun' paradox theory, which proposes that life emerged on Earth despite a less intense sun.
Researchers at NJIT's Big Bear Solar Observatory have uncovered a likely mechanism for the Sun's upper atmosphere heating, revealing jets of magnetized plasma known as spicules. High-resolution images show spicules erupting from the Sun's surface at speeds of up to 100 km/s.
Magnetic reconnection near the solar surface generates solar spicules, which channel hot plasma into the corona. The study reveals that energy released from magnetic field realignment triggers enhanced spicular activity, causing local heating of the upper atmosphere.
Scientists at Helmholtz-Zentrum Dresden-Rossendorf have identified a new form of magnetic instability in the Sun's rotating plasma, which may contribute to its magnetic field generation. This discovery could be a significant step forward in understanding sunspots and their cycles.
Astronomers have observed the first confirmed interstellar comet, 2I/Borisov, using NASA's Hubble Space Telescope. The comet has a central concentration of dust around its nucleus and is traveling at an extraordinary speed of 110,000 miles per hour.
A recent study found that the SunSmart skin cancer prevention program contributed to a decline in melanoma among younger Australians. The use of sun protection behaviors increased rapidly after the program commenced, with maximal sun protection including shade also seeing significant improvements.