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EI2GYB > ASTRO 20.09.21 10:03l 62 Lines 5118 Bytes #999 (0) @ WW
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Subj: Solving Supernova Mysteries
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Solving Supernova Mysteries
This week, astronomers have solved one supernova mystery and predicted a new one - to be solved in 2037.
Solving a 900-year-old Supernova Mystery
Almost a millenium ago, in 1181 AD, Chinese astronomers noted a "guest star" that appeared as bright as Saturn in their skies. This guest marked a supernova that gradually dimmed over the next six months before disappearing from naked-eye view. But even though they recorded an approximate location on the sky, no modern astronomer has been able to identify the supernova source.
Now, Albert Zijlstra (University of Manchester, UK) and colleagues announce the detection of the gaseous remnants of a supernova, a giant bubble expanding at about 1,100 km/s (2.5 million mph). Calculating based on the current rate of expansion, the team estimates the gases originated in a supernova explosion some 1,000 years ago, at a point near the recorded location of the ancient guest star.
The supernova was likely the merger of two white dwarfs in a type of explosion astronomers classify as Type Iax, a rare beast that makes up only 10% of the supernova menagerie. The merger left behind an extreme stellar remnant that the researchers have dubbed "Parker's Star."
This week, astronomers have solved one supernova mystery and predicted a new one - to be solved in 2037.
Solving a 900-year-old Supernova Mystery
Parker's Star and supernova remnant
Infrared images from the Widefield Infrared Survey Explorer (WISE) show the supernova remnant. At left, blue-green represents emission at 11 microns and longer 22-micron wavelengths. At right, green is 11 microns and red 22 microns, while yellow shows ultraviolet emission recorded by the Galex space telescope, and contours show X-ray emission. The UV and X-rays come largely from the core of the nebula, where Parker's Star burns bright and hot.
Andreas Ritter et al. / Astrophysical Journal Letters
Almost a millenium ago, in 1181 AD, Chinese astronomers noted a "guest star" that appeared as bright as Saturn in their skies. This guest marked a supernova that gradually dimmed over the next six months before disappearing from naked-eye view. But even though they recorded an approximate location on the sky, no modern astronomer has been able to identify the supernova source.
Now, Albert Zijlstra (University of Manchester, UK) and colleagues announce the detection of the gaseous remnants of a supernova, a giant bubble expanding at about 1,100 km/s (2.5 million mph). Calculating based on the current rate of expansion, the team estimates the gases originated in a supernova explosion some 1,000 years ago, at a point near the recorded location of the ancient guest star.
The supernova was likely the merger of two white dwarfs in a type of explosion astronomers classify as Type Iax, a rare beast that makes up only 10% of the supernova menagerie. The merger left behind an extreme stellar remnant that the researchers have dubbed "Parker's Star."
Read more about the Chinese guest star of 1181 in the University of Manchester press release and the study appearing in the September 10th Astrophysical Journal Letters.
Supernova Reprise
Ten billion years ago, a star exploded. Its photons journeyed through the universe, passing through a massive galaxy cluster some 6 billion years later. The gravity of those galaxies and their attendant retinues of hot gas acted like a cosmic lens, bending and magnifying the supernova's light, distorting it until it became multiple images.
Those images appeared in a Hubble Space Telescope photo in 2016 before fading away. By 2019, there was no visible remnant of the supernova, dubbed Requiem.
But we'll see Requiem again. By the way the cluster has bent the background light, astronomers predict that some photons took a fourth, longer path, and they'll take another 16 years to arrive. In 2037, astronomers will see if they're right.
Gravitationally lensed supernovae have been observed before (Supernova Refsdal and iPTF16geu are two notable examples), but the more of them the better. Because their light takes multiple paths to Earth, they are powerful probes of cosmology, giving astronomers an independent measure of the much-debated current expansion rate of the universe.
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