AB - SN 1006 is the milestone of understanding the acceleration mechanism of cosmic rays, and this year is the millennium year for the remnant. Find out about the supernova remnant. … These results were presented at a meeting of High Energy Astrophysics Division of the American Astronomical Society in Monterey, CA. Locate the supernova remnant's associated constellation on a star map. H.E.S.S. 2006a). Have students look at several Fast Fact tables, including this one. This is possibly the brightest supernova in human history. SN 1006 is originally thought to be a binary star, where one of the cosmic companions, a white dwarf, exploded when gas from its companion caused it to exceed the Chandrasekhar limit – the maximum possible mass of a white dwarf-type star. In fact, the ancient Egyptian astronomer Ali ibn Ridwan wrote in a comment on Ptolemy’s Tetrabiblos that “[the] spectacle was … Fast Facts: Supernova Remnant SN 1006. SN 1006 is located about 7,000 light years from Earth. Age: About 1,000 years: Location: Located in the constellation Lupus, in the Southern Hemisphere: Distance from Earth: About 7,200 light-years: Size: About 60 light-years across: This gaseous ribbon is a very thin section of a supernova remnant. also observed the Vela pulsar region in 2004 and 2005, and detected a strong gamma-ray signal at the 50% Crab level above 1 TeV (Aharonian et al. 2001, 2003;Haraetal.2001). The Crab Nebula was created by the remnants of SN 1504, a supernova first observed on July 4th, 1054. More Space Facts. The brightest supernova ever recorded was SN 1006 in 1006 AD, it was observed in China, Europe, Egypt, Iraq and Japan. In contrast, only a small linear filament in the northwest corner of the shell is visible in the optical data. Millenium study of SN 1006 with Suzaku. The rest of the SN 1006 supernova is located at an estimated distance of 7,200 light-years (2.2 kiloparsecs), resulting in a diameter of approximately 70 light-years. Teachers can use Fast Facts: Supernova Remnant SN 1006 as: • A source of information. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and exploded. • A mapping activity. The Crab Nebula was created by the remnants of SN 1504, a supernova first observed on July 4th, 1054. These facts might have information of efficient cosmic ray acceleration and background plasma. And finally, SN 1006. It was likely a white dwarf star that had been pulling matter off an orbiting companion star. The radio data show much of the extent that the X-ray image shows. Appearing between April 30 and May 1 of the year 1006, this spectacular light show was bright enough to cast shadows, and was visible during daytime for weeks. SN 1006 resides within our Milky Way Galaxy. A picture of the supernova remnant is included.
We now know that SN 1006 heralded not the appearance of a new star, but the cataclysmic death of an old one located about 7,000 light years from Earth. Researchers say the supernova of 1006 (SN 1006) occurred as a result of collision and merger of two white dwarfs of … … It is observed and described in China, Japan, the Middle East, Europe, and elsewhere. The new Chandra image of SN 1006 contains over 8 days worth of observing time by the telescope. The SN 1987 supernova, which was first observed on February 18th, 1987, was the first one that astronomers could study in detail.
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