Ðekel
The Living Force
thought this might be of interest here.
Nasa's site currently has a piece on "Tycho's star", another name for the supernova that appeared in Earth's skies in 1572 in the constellation of "Cassiopeia".
the article discusses gamma ray bursts.
excerpt;
full article here: http://www.nasa.gov/mission_pages/GLAST/news/tycho-star.html
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another article that catches the eye, this time about a "cloud" of material that is vectored towards the black hole in the center of the galaxy, is this one:
http://www.newscientist.com/article/dn21288-cloud-suicide-will-wake-black-hole-sleeping-giant.html
full text of the article below with portions highlighted which stood out to me;
it seems that everyday scientists are discovering more and more unusual events that seem to be taking place in our near future.
Nasa's site currently has a piece on "Tycho's star", another name for the supernova that appeared in Earth's skies in 1572 in the constellation of "Cassiopeia".
the article discusses gamma ray bursts.
excerpt;
Better understanding the origins of cosmic rays is one of Fermi's key goals. Its Large Area Telescope (LAT) scans the entire sky every three hours, gradually building up an ever-deeper view of the gamma-ray sky. Because gamma rays are the most energetic and penetrating form of light, they serve as signposts for the particle acceleration that gives rise to cosmic rays.
"This detection gives us another piece of evidence supporting the notion that supernova remnants can accelerate cosmic rays," said co-author Stefan Funk, an astrophysicist at the Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), jointly located at SLAC National Accelerator Laboratory and Stanford University, Calif.
In 1949, physicist Enrico Fermi -- the satellite's namesake -- suggested that the highest-energy cosmic rays were accelerated in the magnetic fields of interstellar gas clouds. In the decades that followed, astronomers showed that supernova remnants may be the galaxy's best candidate sites for this process.
{image caption}:
The gamma-ray emission from Tycho's supernova remnant can be explained by pion production. A proton traveling close to the speed of light strikes a slower-moving proton. Their interaction creates an unstable particle -- a pion -- with only 14 percent of the proton's mass. In 10 millionths of a billionth of a second, the pion decays into a pair of gamma rays.
When a star explodes, it is transformed into a supernova remnant, a rapidly expanding shell of hot gas bounded by the blast's shockwave. Scientists expect that magnetic fields on either side of the shock front can trap particles between them in what amounts to a subatomic pingpong game.
"A supernova remnant's magnetic fields are very weak relative to Earth's, but they extend across a vast region, ultimately spanning thousands of light-years. They have a major influence on the course of charged particles," said co-author Melitta Naumann-Godo at Paris Diderot University and the Atomic Energy Commission in Saclay, France, who led the study with Giordano.
full article here: http://www.nasa.gov/mission_pages/GLAST/news/tycho-star.html
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another article that catches the eye, this time about a "cloud" of material that is vectored towards the black hole in the center of the galaxy, is this one:
http://www.newscientist.com/article/dn21288-cloud-suicide-will-wake-black-hole-sleeping-giant.html
full text of the article below with portions highlighted which stood out to me;
The sleeping giant at the centre of the Milky Way is about to wake up. A suicidal gas cloud is heading towards the galaxy's supermassive black hole, which will probably swallow the cloud, generating enormous flares of radiation that could help explain why the black hole is normally so placid.
The doomed cloud was a surprise to astronomers. "We have been looking at the galactic centre for 20 years, but mainly to observe the motion of stars," says Reinhard Genzel of the Max Planck Institute for Extraterrestrial Physics in Garching, Germany.
Genzel's colleague Stefan Gillessen spotted the cloud in images from the Very Large Telescope array in Chile, taken in March this year. It is an unusually dense cloud, not much bigger than our solar system and carrying about three times the mass of Earth.
Shredded cloud
The team realised that the cloud also appears in earlier images, giving them a sequence that reveals its path. It is moving at almost 2500 kilometres per second towards our galaxy's black hole, Sagittarius A*.
At present Sagittarius A* is strangely quiet, unlike quasars, the hyperactive black holes that emit huge amounts of radiation, fuelled by inflowing gas. Our black hole gets much less gas, and for some reason this starvation state makes it much less efficient than a quasar, producing only a thousandth as much radiation per kilogram of fuel.
While a star would just sail past our black hole unscathed, the loose mass of gas heading towards it is more vulnerable. It is already being stretched out by the black hole's gravity, and when it gets closer in 2013 it will plough into the halo of hot gas around the hole.
Unlucky timing
That should send shockwaves through the cloud to heat it to several million degrees, and according to the group's simulations the gaseous collision will shred the cloud into filaments. This turmoil may mean that much of the cloud ends up swirling right down into the black hole.
"By dumping more material in there, the cloud could drive the system into a higher efficiency regime," says Ginzel. There may be one huge flare of radiation or several over the coming decades.
There's no danger of the active black hole harming Earth. And though sadly not visible to the naked eye, this radiation will give astronomers clues as to why our black hole is normally so different from quasars.
"There is evidence that the galactic centre was more luminous within the last few thousand years, and we are unlucky in living at a time when it appears to be unusually dormant," says astrophysicist Martin Rees at the University of Cambridge, who was not part of the study.
it seems that everyday scientists are discovering more and more unusual events that seem to be taking place in our near future.