Researchers have discovered a single nanowire can concentrate sunlight up to 15 times the normal intensity, raising the potential for highly efficient solar cells. The breakthrough could lead to a significant impact on solar cell development and energy extraction.
NASA's Voyager 1 spacecraft has traveled beyond the influence of the Sun and exited the heliosphere, a region dominated by the Sun's wind. Anomalous cosmic rays dropped to less than 1% of previous amounts while galactic cosmic rays spiked to levels not seen since launch.
Astronomers have discovered the closest star system to the Sun, located 6.5 light years from Earth, making it an ideal target for planet-hunting expeditions. The star system consists of a pair of brown dwarfs, which are too small in mass to ignite hydrogen fusion.
NASA's Solar Dynamics Observatory (SDO) observed two transits: an Earth transit from March 2-3 and a lunar transit from March 11. The eclipses showed distinct features due to Earth's atmosphere and the moon's curved shape.
On July 19, 2012, NASA's Solar Dynamics Observatory (SDO) detected a rare event: coronal rain. This phenomenon occurs when hot plasma in the sun's corona cools and condenses along strong magnetic fields. The SDO's footage shows the plasma as it slowly falls back to the solar surface, outlining the magnetic fields.
Scientists observed a flux rope forming ahead of time in a coronal mass ejection (CME), providing a case study on its formation. The high-temperature plasma glow helped highlight the flux rope, which was then severed from the sun's surface, releasing billions of tons of solar material.
A coronal mass ejection erupted from the sun on January 31, 2013, leaving the sun at speeds of around 575 miles per second, which is a fairly typical speed for CMEs. This event had historically mild effects but could cause geomagnetic storms if it connects with the outside of the Earth's magnetic envelope.
The Solar Coronal Imager (Hi-C) has provided a major piece of the solar corona puzzle by capturing images of magnetic reconnection. This complex process heats the corona to temperatures up to 7 million degrees F, powered by magnetic fields that constantly warp and collide in bursts of energy.
Researchers aim to explore the mysteries of Alfvèn waves, fueling the Sun's heat and magnetic influence on planets. The study uses advanced simulations and observational data from NASA's Hinode solar observatory and Swedish Solar Telescope.
The Interface Region Imaging Spectrograph (IRIS) will study the lower levels of the sun's atmosphere, including the chromosphere and transition region. The mission aims to unravel how matter, light, and energy move from the surface to the corona, with implications for solar flares and coronal mass ejections.
Tau Ceti, the closest single star to our Sun, has been found to have a planetary system with five planets. The estimated masses range from two to six times that of Earth, making it the lowest-mass planetary system yet detected.
The EUNIS mission will gather data on the sun's corona by observing extreme ultraviolet light over a six-minute flight, providing insights into temperature ranges of solar plasma. The instrument will observe wavelengths from 525 to 630 Angstroms, covering temperatures from near the surface to millions of degrees Fahrenheit.
The discovery of L1527 IRS marks the oldest known solar system in formation, with a rotating dust disk and a protostar expected to grow to match the Sun's mass. The system is thought to be around 300,000 years old, compared to the 4.6 billion-year age of our own Solar System.
Researchers found that planets in solar systems with similar stars may be warmer and more dynamic, potentially hosting microbial life. This could expand the habitable zone around those stars, making them more suitable for life.
The Hinode spacecraft observed two solar eclipses in 2012 and 2013, capturing distinct views of total and partial eclipses. The mission provided valuable insights into the Sun's surface magnetism, shedding light on sunspot activity.
A narrow corridor in the southern hemisphere experienced a total solar eclipse on Nov. 13, 2012, with observers in northern Australia witnessing dim structures around the sun's edge. The corona, made of electrified gas and plasma, was observed to be constantly moving in response to magnetic fields.
The Hinode mission will coordinate with ground-based observations during the November 13, 2012, total solar eclipse to produce a combined dataset. This study will focus on the sun's corona, including its temperature distribution and magnetic fields.
A mid-level solar flare, classified as M6, was observed by NASA's Solar Dynamics Observatory on November 13, 2012. The flare caused a moderate radio blackout affecting GPS and communications signals for several minutes to hours.
FOXSI will study nanoflares on the sun using a state-of-the-art x-ray telescope that focuses incoming x-rays. The mission aims to understand energy transfer and coronal heating by observing how these small flares impact the sun's atmosphere.
A significant solar flare occurred on Oct. 22, 2012, peaking at an X1.8-class intensity, impacting radio communications for about an hour. The National Oceanic and Atmospheric Association categorized the radio blackout as R3 on a scale from R1 to R5.
Astronomers detect the lightest exoplanet ever found around a Sun-like star, orbiting about six million kilometers away from the star. The newly discovered planet has a mass similar to Earth and orbits Alpha Centauri B every 3.2 days.
A new graphene-cobalt material has been developed that can catalyze the oxygen reduction reaction nearly as well as platinum, with improved durability. The material is substantially cheaper than platinum and has shown promise for use in hydrogen fuel cells.
Scientists optimize SDO's HMI instrument to improve resolution quickly after eclipses. By adjusting heater timing and temperature, they've reduced the recovery time from 60 minutes to around 45-50 minutes.
A team of space scientists has shed light on the mysterious physical mechanisms underlying coronal mass ejections (CMEs) that can impact Earth-based power grids and satellites. The study, published in Nature Physics, uses state-of-the-art computer simulations to connect motions in the sun's interior with CMEs.
A low-cost sun protection intervention, including mailed kits with resources and educational activities, led to higher frequency of sun-protective behaviors among children. The study found significant gains in sun-protective behavior and awareness across all measures.
Researchers analyze temperatures, shapes, and densities of coronal cavities to understand space weather disruption. By studying these structures, scientists aim to get advance warning on CME eruptions and improve technology protection near Earth.
A team of researchers from Arizona State University found that painting building roofs white can reduce average temperatures in urban areas but also disrupt regional hydroclimates. The study, focusing on Arizona's Sun Corridor, shows a 12% reduction in rainfall and an additional 4% decrease with white roofs.
A University of Colorado Cancer Center study found that parents' concern about skin cancer does not affect their children's outdoor play time or obesity rates. The research suggests that children can get plenty of physical activity and prevent skin cancer by using sun protection measures.
Astronomers using ALMA detected glycolaldehyde, a simple form of sugar, in the gas surrounding a young binary star. This discovery suggests that the building blocks of life existed in this system at the time of planet formation.
Scientists study electron strahl, a stream of high-energy electrons from the sun, using five years of data. They found that widths vary, with some being much wider than expected, indicating an unknown scattering mechanism.
New data from the Hinode mission reveals insights into the Sun's coronal magnetic field structure and an unusual asymmetry in its magnetic field. This finding could impact the behavior and prediction of the next solar cycle, which is critical for understanding our nearest star.
Scientists at NASA's Goddard Space Flight Center recorded a coronal mass ejection traveling at unprecedented speeds using data from the STEREO spacecraft. The event produced a strong magnetic field and intense solar radiation, offering insights into the causes of space weather events.
A study by Arizona State University reveals that megapolitan expansion could lead to local maximum summertime warming of nearly 4 degrees Celsius, surpassing the warming caused by increased greenhouse gases. The research found that incorporating 'cool roofs' into urban planning can alleviate summertime warming substantially.
A new technique has revealed a significant amount of dark matter near the Sun, contradicting previous studies that found less. The researchers used a simulation of the Milky Way to test their method and obtained a high measure of local dark matter density.
A new UV dosimeter monitor is set to be commercially available, helping prevent sunburn and over-exposure to ultra-violet radiation. The device, developed at the University of Strathclyde, provides a visual warning when risk levels increase, allowing users to enjoy the sun safely.
Researchers modelled comets and asteroid particles to explain their origins and compositions. The study found that these particles could have been processed in the hot inner disk of the Solar System before traveling out to icy comets, shedding light on the puzzle of how comets acquired different rim compositions.
A mid-level solar flare, classified as M7.7, was detected by NASA on July 19, 2012, causing brief radio communications blackouts at the poles. Increased numbers of flares are expected during the sun's peak activity cycle, which is approaching its maximum in 2013.
A new technique developed by NASA scientist Nicholeen Viall uses color-coded images to track the 12-hour history of cooling and heating on the sun. The technique reveals that coronal heating is likely caused by numerous nanobursts of energy, lending credence to those theories.
Researchers at Brown University have discovered a pyramid in El Zotz, Guatemala, that provides new information about the Maya civilization. The temple features ornate masks depicting different phases of the sun and stucco carvings revealing how the Maya conceived of the heavens.
Researchers have created an 'MRI' of the Sun's interior plasma motions, revealing that convective motions are approximately 100 times slower than previously projected. This challenges existing theories on heat transport and magnetic field generation, requiring a re-evaluation of sunspot formation and solar dynamics.
The HI-C mission will observe the solar corona at a resolution of up to 100 miles, surpassing existing instruments. The telescope's finely crafted mirrors, some of the best ever made, will capture structures in the sun's atmosphere with unprecedented detail.
Astronomers have observed a young star, V1647 Orionis, exhibiting intense X-ray activity in the McNeil's Nebula, driven by strong magnetic fields. The star's rapid rotation is also evident in its X-ray emission patterns.
A team of researchers, including a Rice astrophysicist, used Doppler measurements to observe loops of plasma flowing up from the sun's surface at high speeds. These findings may help predict solar flares and coronal mass ejections that threaten satellites and power grids.
The Solar Ultraviolet Magnetograph Investigation (SUMI) mission aims to study the intricate magnetic fields in the sun's chromosphere, a hard-to-observe area of the sun's low atmosphere. By observing ultraviolet light, SUMI will create a three-dimensional magnetic map of the region.
Hi-C will capture the highest-resolution images of the sun's corona, providing unprecedented views of dynamic activity in the solar atmosphere. The mission aims to understand coronal heating and structuring, placing significant new constraints on theories.
Mathematicians at the University of Sheffield have discovered space tornadoes in the Sun's atmosphere, which can channel energy from below the surface to heat the magnetised solar plasma. The process has the potential to develop technology for producing free, clean, and green energy on Earth.
Researchers at H. Lee Moffitt Cancer Center found a synergy between sun exposure and cutaneous HPV infection in developing non-melanoma skin cancers like basal cell carcinoma and squamous cell carcinoma. People with low melanin production, such as those with light skin, are more susceptible to these risks.
A previously unappreciated open star cluster, Ruprecht 147, has been found to be an important tool in understanding stellar astrophysics and the search for Earth-like planets. The cluster is close to Earth and contains stars similar in mass and age to the Sun, making it a valuable laboratory for studying bright stars.
A population-based study has found that high levels of ultraviolet radiation at birth, sun-sensitive skin type, and a history of skin cancer decreased the risk of pancreatic cancer. Participants born in areas with high UV radiation had a 24% lower risk compared to those born in low UV areas.
The UK Space Agency has invested £11.5M in the Solar Orbiter mission, which will discover how the Sun creates and controls the heliosphere by flying closer than ever before to the Sun. The mission will study the Sun's magnetic field and solar activity, including coronal mass ejections that can affect Earth.
Researchers at Sandia National Laboratories created a solar nanowire array that can absorb a wider range of the sun's wavelengths, leading to increased efficiency. The array, grown on a phalanx of nanowires, allows for higher indium percentages and lower absorption base energies.
Researchers used NASA's Solar Dynamics Observatory and New Solar Telescope to observe ultrafine loops in the sun's corona. These narrow loops are connected to higher lying, wider loops and may help explain how temperatures rise throughout the corona.
Fermi detects the highest-energy gamma rays ever associated with a solar flare, surpassing visible light by two billion times. The discovery showcases Fermi's capabilities as a solar observatory, providing insights into solar outbursts and charged particles acceleration.
Researchers will observe the Arc of Venus, a glowing rim around Venus, to learn about its atmosphere and super-rotation. The phenomenon reveals temperature and density structures in Venus' middle atmosphere, shedding light on the planet's mysterious evolution.
The RHESSI satellite will utilize the June 5-6, 2012 Venus transit to improve its measurements of the sun's diameter. By analyzing the sharpness of the Venus disk as it crosses the sun, scientists can calibrate their instrument and refine their observations of the sun's horizon.
The NASA Solar Dynamics Observatory (SDO) will observe the June 2012 Venus transit to calibrate its instruments and learn more about Venus' atmosphere. The transit provides a unique opportunity to test the SDO's orientation accuracy and understand the point spread function of the telescope.
University of Iowa professor Jack Scudder and colleagues have observed a milestone discovery in astrophysics: the first experimentally resolved site of collision in magnetic reconnection. This process links magnetic field lines from the sun to the Earth's core, allowing charged particles to cross previously forbidden boundaries.
Scientists discover that the sun does not have a bow shock due to insufficient speed to create one in the tenuous region. The new data from IBEX and Voyager spacecraft indicates a strong external magnetic field influencing the heliosphere's structure, leading to a new paradigm.
Young people are at risk of severe skin damage from autumn UV levels, which can lead to cancer-causing skin aging and wrinkles. Researchers used a unique non-invasive UV camera to measure the relationship between lifetime sun exposure and skin cancer risk.
A team of scientists has sequenced the whole genomes of 25 metastatic melanoma tumors, confirming the role of chronic sun exposure and revealing new genetic changes. The study identified a gene called PREX2, which is mutated in 44% of patients and appears to accelerate tumor development.