Astronomers have used a new technique to measure the ages of 22 Sun-like stars, revealing properties similar to our Sun. The study's lead author found 'solar twins' that can be studied to predict planetary system evolution.
Researchers used MESSENGER data to detect solar neutrons created in solar flares, providing a direct link to the flare process. The combined use of NASA mission data from MESSENGER and STEREO spacecraft offers new information about particle acceleration in solar flares.
Scientists have discovered the corona extends far beyond previous observations, with implications for NASA's Solar Probe Plus mission. Direct measurements of the heliosphere's inner boundary provide new insights into solar particle behavior and the origin of the solar wind.
Comet Siding Spring is producing about 2 billion water molecules per second, equivalent to filling an Olympic-size pool in 14 hours. The icy nucleus is estimated to be around 2,300 feet across, placing it at the lower end of a size range.
Chronic UV radiation stimulates endorphin production, causing physical dependence and addiction-like behavior in mice. This finding could explain why people have an instinctive desire for sunlight despite its health risks. Researchers suggest that a conscious effort to limit sun exposure is needed to mitigate skin cancer risk.
The sun experienced three X-class flares in two days, with the third flare peaking at 5:06 a.m. EDT on June 11, 2014. The solar activity was captured by NASA's Solar Dynamics Observatory and originated from an active region on the sun.
A new report by NREL found that Concentrated Solar Power (CSP) projects add a value of 5-6 cents per kilowatt hour in California, where renewables will reach 33% by 2020. CSP helps maintain firm capacity and reduces curtailment of variable generation technologies.
Researchers at New Jersey Institute of Technology have made a groundbreaking discovery about the structure and activity of the Sun. They found that buoyant magnetic-flux ropes on the solar surface can trigger powerful plasma eruptions in the atmosphere, leading to intense heating and rapid acceleration of plasma.
A record-breaking X-class flare was observed by four NASA spacecraft and one ground-based observatory on March 29, 2014. The coordinated efforts provided the most comprehensive data set ever collected, shedding light on the origins of solar eruptions and their effects on space weather near Earth.
Researchers at Drexel University have created a method for 3D printing living cancer tumors using cervical cancer cells and hydrogel substances. This breakthrough technology allows for more accurate modeling of tumor behavior and response to treatment, potentially leading to new paradigms for cancer research and individual therapies.
Researchers use NASA's SDO to map dynamic magnetic fields and brightpoints in the sun's atmosphere, revealing deep-seated activity and potential cells of flowing material. This breakthrough offers near real-time mapping of the sun's interior, affecting solar flares and other events.
A study published in Nature Geoscience found that changes in the Sun's energy output may have led to marked natural climate change in Europe over the past 1000 years. The research suggests that regional climate variability associated with solar activity should be taken into account when making future climate projections.
Scientists at MIT and NASA have identified a process in the Earth's magnetosphere that reinforces its shielding effect, keeping incoming solar energy at bay. A plume of low-energy plasma particles slows magnetic reconnection, blunting the sun's effects on Earth.
A giant sunspot has reappeared over the sun's horizon, marking its third trip around the sun in approximately 27 days. This region has produced two X-class solar flares and numerous mid-level flares during its previous trips.
On January 28, 2014, NASA's Interface Region Imaging Spectrograph (IRIS) witnessed a strong solar flare, emitting x-rays and light into space. The IRIS mission offers unprecedented resolution to study the sun's lower atmosphere, providing valuable insights into solar flares.
The PLATO mission aims to discover and characterize Earth-like planets in the Sun's neighborhood. With an array of telescopes, it will measure planetary sizes, masses, and ages to determine their habitability. By observing one million stars, PLATO is expected to find thousands of new exoplanets.
A University of Colorado study shows that teens who watched a video about the cosmetic effects of UV exposure were more likely to use sunscreen than those who watched a health-based video. This finding suggests that addressing appearance-related concerns can be an effective way to modify sun-protective behaviors in teenagers.
The asteroid belt's diverse composition suggests that giant planets' migrations reshaped the solar system, potentially delivering water to Earth and influencing its habitability. Small asteroids show particularly varied compositions, suggesting a complex history of collisions and re-deposition.
A NASA-funded sounding rocket will launch into the aurora borealis to gather data on its formation and behavior. The mission, GREECE, aims to understand the sun-Earth connection and how energy particles interact with Earth's magnetosphere.
Researchers have built a system that converts the sun's energy into hydrogen fuel and stores it for later use, allowing for nighttime power. The 'solar fuels' system uses natural photosynthesis as inspiration and has the potential to be a major piece of the puzzle for a solar energy future.
Scientists observe enormous sunspot AR1944, two Earths wide, moving toward the sun's center. The sunspot is part of active regions that can cause space weather events, such as solar flares and coronal mass ejections.
A new scientific study by the University of Edinburgh found that variations in heat from the sun do not strongly influence climate change. Volcanic eruptions were the primary cause of periodic changes in climate until 1800, and greenhouse gases have been the main driver since then.
Astronomers have made precise measurements of a failed star system near the Sun, suggesting it harbors a third planetary-mass object. The system, Luhman 16AB, consists of two brown dwarfs with masses between 30 and 50 Jupiter masses.
Comet ISON successfully passed close to the sun, shedding light on its composition and behavior. Despite initial hopes for a bright display, the comet's nucleus likely broke apart due to intense heat, producing limited dust tail observations.
IRIS has captured detailed images of the interface region between the sun's surface and corona, revealing more violent and turbulent phenomena than previously understood. The mission's observations also provide new insights into solar eruptive events and the dynamics of the low solar atmosphere.
A massive ejection of material from the sun in 2012 could have created a technological disaster if it hit Earth, short-circuiting satellites and power grids. The event highlights the need for society to prepare for severe space weather events.
The Total Solar Irradiance Calibration Transfer Experiment (TCTE) mission aims to provide accurate measurements of the sun's energy impact on Earth. The new instrument, deployed in November 2013, will overlap with the existing TIM instrument to ensure continuous data flow and improve accuracy.
Comet ISON's size reduced significantly as it approached the sun, with observations revealing a potential debris field and unclear nucleus remnants. The comet's unprecedented observation history will provide valuable data for scientists to study in the years to come.
Researchers carefully measure Comet ISON's brightness to infer its current state, as it approaches perihelion on November 28, 2013. The comet's behavior over several days suggests it may be disintegrating or intact.
Comet ISON, a time capsule from the solar system's formation, will be observed by NASA's solar observing fleet as it approaches the sun. The comet's journey will provide valuable insights into the solar wind and atmosphere.
Two large sunspots, AR1890 and AR1897, are active on the sun, with AR1890 producing significant flares and AR1897 nearing its appearance on Earth-side of the sun. The sun's 11-year activity cycle is increasing towards solar maximum conditions, leading to an uptick in flares.
FORTIS will observe the comet's molecules and atoms by separating incoming light into its component wavelengths, gathering information from several areas at once. The comet's rate of sublimation increases as it approaches the sun, allowing FORTIS to capture observations of this material coming off the comet.
The sun recently emitted a powerful X1.1 flare, disturbing the layer where GPS and communications signals travel. Increased flares are common during the sun's peak activity cycle, which is currently ramping up toward solar maximum conditions.
A new study by Professor Terry Sloan and Professor Sir Arnold Wolfendale found that changes in solar activity had a negligible impact on global temperatures. The researchers compared data on cosmic rays entering the atmosphere with global temperature records, concluding that less than 14% of the twentieth century's warming was attribut...
The sun emitted its fourth X-class flare since October 23, 2013, peaking at 5:54 p.m. on October 29, 2013. The X2.3 class flare may disrupt radio signals for hours due to its intense radiation.
The sun continues to produce mid-level and significant solar flares, including an X1.0 flare on Oct. 27 and an M5.1 flare on Oct. 28, potentially impacting Earth's atmosphere and electronic systems. The recent activity is part of the sun's normal 11-year activity cycle.
Researchers Drs. Michael Hahn and Daniel Wolf Savin found evidence that magnetic waves can heat the corona, depositing most of their energy at low heights for widespread heat distribution. This discovery helps answer a 70-year-old solar physics conundrum about the Sun's extreme corona temperature.
A new study finds that high carbon dioxide levels in the ancient atmosphere may have counteracted the effects of a weak young Sun, allowing life to thrive on Earth. The researchers used tiny air samples trapped in quartz rocks to reconstruct the atmosphere's composition, finding higher-than-expected CO2 levels.
The Sunrise mission revealed complex patterns in the chromosphere, including dark regions and bright points thought to be magnetic flux tubes. The ultraviolet radiation from the chromosphere is highly suitable for visualizing detailed structures and processes.
Astronomers have discovered an ancient solar twin that is 8.2 billion years old, providing insights into the Sun's life-giving properties and lithium content. The star, HIP 102152, has low levels of lithium, supporting the theory that stars destroy their lithium as they age.
Scientists have overturned previous notions of how the sun's writhing insides move from equator to pole and back again. The team found a double-layered circulation system with two cycles on top of each other, providing new opportunities for studying solar magnetism and cycles.
Researchers created ring-shaped complexes of protein and pigments that absorb more sunlight than natural ones. The designs use a combination of synthetic and natural pigments to capture a broader spectrum of light, allowing for efficient energy harvesting.
Scientists predict the sun's magnetic field will reverse in three to four months, affecting space weather and potentially cosmic rays. This change marks the midpoint of Solar Cycle 24, with half of 'solar max' behind and half yet to come.
The discovery of GJ 504b challenges traditional planet-formation theories, suggesting alternative formation methods may be needed. The exoplanet orbits its star at nearly 9 times the distance of Jupiter from the sun.
VERIS will focus on the very hot material present in active regions of the corona, magnetically complex spots that can cause solar flares and coronal mass ejections. The rocket's six-minute flight will yield rich information about the tiny details of these processes.
The IRIS mission provides state-of-the-art observations of the interface region, revealing fine structures and energy transport mechanisms. The data will help scientists understand how the sun's lower atmosphere powers solar events and impacts Earth's climate.
A gigantic coronal hole has been observed by NASA's SOHO near the sun's north pole, providing valuable insights into space weather. The coronal hole is a dark region of the sun's corona with lower temperatures and appears much darker than its surroundings.
Researchers from UCL's Mullard Space Science Laboratory used data from the Japanese Hinode spacecraft to measure the Sun's magnetic field. The study found that the field is approximately ten times weaker than previously estimated.
A powerful coronal mass ejection (CME) from the sun has been directed towards Earth and Mercury, posing a risk to electronic systems and communication signals. The CME's magnetic fields can cause geomagnetic storms, potentially leading to aurora displays.
Astronomers have discovered that the Sun's corona loops appear as a constant width due to an optical illusion, but in reality, they are tapered structures. This finding has significant implications for coronal heating models.
NASA's Solar Dynamics Observatory captured spectacular images of June 7, 2011 solar eruption and splashdown. The event provided an 'up close' view of what happens on distant stars during accretion. Astronomers can now learn about young star growth by analyzing ultraviolet light emission.
Scripps Research Institute scientists have identified key triggers of an important cancer-blocking mechanism in cells, known as oncogene-induced senescence. The study reveals a cascading interaction of three enzymes necessary to initiate this response.
Astronomers studied young star TW Hydrae to understand the birth of our Sun, finding it was clumpy and episodic in accretion. The study revealed that accretion drove magnetic activity on TW Hydrae.
IRIS aims to unravel the interface region by providing high-resolution images and spectrograph data, revealing structures like giant jets that affect the solar wind and Earth's climate. The mission will utilize advanced computing to interpret the light flowing out of this region.
IRIS will provide high-resolution images and spectra to unravel the interface region, allowing scientists to track solar material as it is accelerated and heated. The mission enables the observation of temperature ranges from 5,000 to 10 million kelvins.
Scientists have developed a mechanism to understand the cyclical nature of the Sun's magnetic activity, which is responsible for 'space weather' phenomena like solar flares and coronal mass ejections. This discovery provides a solution to mathematical equations governing fluids and electromagnetism for large astrophysical bodies.
Experimental NASA research models show that three coronal mass ejections (CMEs) have erupted from the sun, with speeds of up to 625 miles per second. The CMEs may pass by NASA's Messenger and STEREO-A satellites, posing a risk of particle radiation to interplanetary spacecraft.
Two new super-Earths and a Mars-sized planet have been found in the habitable zone of Kepler-62, a star similar to our Sun. These planets are thought to be solid and rocky or rocky with frozen water, making them potentially hospitable to life.
The NASA Wind spacecraft has detected 'SLAMS' waves in the region between the Earth's magnetosphere and the sun, showing that these structures may accelerate narrow jets of charged particles. The discovery provides new insights into how radiation and energy from the sun can cross the magnetosphere and impact near-Earth space.
Researchers from various disciplines are collaborating on a four-year project to encourage vacationers to use advanced sun protection behaviors. The program, launched at 40 resorts nationwide, aims to reduce skin cancer cases through education and awareness.