SPACE
NOAA has issued a severe geomagnetic storm watch for Friday. It follows days of strong solar flares and coronal mass ejections. It could cause disruptions in power grids, radio, satellites and communications. It will also trigger spectacular Aurora Borealis light displays. Aurora Borealis seen in highlighting the Chicago area from the International Space Station.
File Photo by NASA/UPI | License Photo
May 10 (UPI) -- The NOAA's Space Weather Prediction Center warned of a severe geomagnetic storm Friday with wide-ranging impacts that could potentially disrupt communications, the electric power grid, navigation, radio and satellite operations.
The agency issued a Severe (G4) Geomagnetic Storm Watch for Friday evening, adding that "additional solar eruptions could cause geomagnetic storm conditions to persist through the weekend."
It's the most severe warning in 20 years.
May 10 (UPI) -- The NOAA's Space Weather Prediction Center warned of a severe geomagnetic storm Friday with wide-ranging impacts that could potentially disrupt communications, the electric power grid, navigation, radio and satellite operations.
The agency issued a Severe (G4) Geomagnetic Storm Watch for Friday evening, adding that "additional solar eruptions could cause geomagnetic storm conditions to persist through the weekend."
It's the most severe warning in 20 years.
NOAA said it's monitoring the sun after a series of strong solar flares and coronal mass ejections.
"CMEs are explosions of plasma and magnetic fields from the sun's corona," NOAA said in a statement. "They cause geomagnetic storms when they are directed at Earth. Geomagnetic storms can impact infrastructure in near-Earth orbit and on Earth's surface, potentially disrupting communications, the electric power grid, navigation, radio and satellite operations. SWPC has notified the operators of these systems so they can take protective action."
These storms can trigger "spectacular displays of aurora on Earth", according to NOAA. These aurora borealis "northern lights" could be seen as far south as Alabama and Northern California.
NOAA said a large sunspot cluster has produced several moderate to strong solar flares since Wednesday. NOAA and NASA space assets will be monitored for the onset of a geomagnetic storm.
According to SpaceWeather.com, "If geomagnetic storms were hurricanes, 'severe' would be category 4."
More solar eruptions could cause geomagnetic storm conditions to last through the weekend.
Scientists hope new data will shed light on how black holes consume matter
A NASA infrared composite image taken by the Spitzer Space Telescope shows a panoramic view of the Andromeda galaxy in 2006. New data from the galaxy is helping scientists understand the eating habits of supermassive black holes, they announced Thursday
A NASA infrared composite image taken by the Spitzer Space Telescope shows a panoramic view of the Andromeda galaxy in 2006. New data from the galaxy is helping scientists understand the eating habits of supermassive black holes, they announced Thursday
. Image courtesy of NASA/UPI | License Photo
May 9 (UPI) -- Researchers are hoping that new images and data from NASA can help explain the voracious appetites of black holes and give scientists new information about why some of the massive and largely unexplained regions of immense gravity shine brighter than others when consuming space dust, researchers reported Thursday.
Space scientists are using data gathered from the retired Spitzer Space Telescope to analyze dust and gas that have been flowing toward the center of the massive black hole at the heart of the Andromeda galaxy.
The steams of gas and dust entering the black hole can help scientists understand how black holes, which are billions of times the mass of our sun, can remain what are known as "quiet" eaters.
"As supermassive black holes gobble up gas and dust, the material gets heated up just before it falls in, creating incredible light shows -- sometimes brighter than an entire galaxy full of stars," a release from NASA said. "When the material is consumed in clumps of different sizes, the brightness of the black hole fluctuates."
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May 9 (UPI) -- Researchers are hoping that new images and data from NASA can help explain the voracious appetites of black holes and give scientists new information about why some of the massive and largely unexplained regions of immense gravity shine brighter than others when consuming space dust, researchers reported Thursday.
Space scientists are using data gathered from the retired Spitzer Space Telescope to analyze dust and gas that have been flowing toward the center of the massive black hole at the heart of the Andromeda galaxy.
The steams of gas and dust entering the black hole can help scientists understand how black holes, which are billions of times the mass of our sun, can remain what are known as "quiet" eaters.
"As supermassive black holes gobble up gas and dust, the material gets heated up just before it falls in, creating incredible light shows -- sometimes brighter than an entire galaxy full of stars," a release from NASA said. "When the material is consumed in clumps of different sizes, the brightness of the black hole fluctuates."
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The black holes at the center of the Milky Way and its galactic neighbor, Andromeda, are among the "quietest" eaters in the universe.
"What little light they emit does not vary significantly in brightness, suggesting they are consuming a small but steady flow of food, rather than large clumps. The streams approach the black hole little by little, and in a spiral, similar to the way the water swirls down a drain," NASA said.
Earlier this year, researchers simulated how dust and gas near Andromeda's black hole might behave over time.
Researchers found "that those streams [of gas and dust] have to stay within a particular size and flow rate; otherwise, the matter would fall into the black hole in irregular clumps, causing more light fluctuation," NASA reported.
The authors then compared their findings with data gathered from Spitzer and NASA's Hubble Space Telescope, and found spirals of dust previously identified by Spitzer that fit the necessary constraints. With that information, the researchers concluded that the spirals are feeding Andromeda's supermassive black hole.
"This is a great example of scientists re-examining archival data to reveal more about galaxy dynamics by comparing it to the latest computer simulations," said Almudena Prieto, an astrophysicist at the Institute of Astrophysics of the Canary Islands and the University Observatory Munich, and a co-author on the study published this year. "We have 20-year-old data telling us things we didn't recognize in it when we first collected it."
Europe's Gaia probe observes starquakes, stellar DNA
Soon, 1 out of every 15 points of light in the sky will be a satellite
The black holes at the center of the Milky Way and its galactic neighbor, Andromeda, are among the "quietest" eaters in the universe.
"What little light they emit does not vary significantly in brightness, suggesting they are consuming a small but steady flow of food, rather than large clumps. The streams approach the black hole little by little, and in a spiral, similar to the way the water swirls down a drain," NASA said.
Earlier this year, researchers simulated how dust and gas near Andromeda's black hole might behave over time.
Researchers found "that those streams [of gas and dust] have to stay within a particular size and flow rate; otherwise, the matter would fall into the black hole in irregular clumps, causing more light fluctuation," NASA reported.
The authors then compared their findings with data gathered from Spitzer and NASA's Hubble Space Telescope, and found spirals of dust previously identified by Spitzer that fit the necessary constraints. With that information, the researchers concluded that the spirals are feeding Andromeda's supermassive black hole.
"This is a great example of scientists re-examining archival data to reveal more about galaxy dynamics by comparing it to the latest computer simulations," said Almudena Prieto, an astrophysicist at the Institute of Astrophysics of the Canary Islands and the University Observatory Munich, and a co-author on the study published this year. "We have 20-year-old data telling us things we didn't recognize in it when we first collected it."
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