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. The SN 1987 supernova, which was first observed on February 18th, 1987, was the first one that astronomers could study in detail. Aya Bamba, Hiroya Yamaguchi, Katsuji Koyama, Junko S. Hiraga, Steve Holt, John Hughes, Hideaki Katagiri, Jun Kataoka, Shunji Kitamoto, Motohide Kokubun, Hironori Matumoto, Emi Miyata, Koji Mori, Hiroshi Nakajima, Masanobu Ozaki, Robert Petre, Akiko Sekiguchi, Tadayuki Takahashi, Takaaki Tanaka, Yukikatsu Terada Show 7 others Show less Hiroshi …
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. This image is a composite of visible (or optical), radio, and X-ray data of the full shell of the supernova remnant from SN 1006. 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. The emission is dif-fuseovertheX-ray(0.9–2.0keV)jet-likeimage,whichwasfirst detected by ROSAT (Markwardt & Ogelman¨ 1995), and … Have students look at several Fast Fact tables, including this one.
Constantine X, emperor of Byzantium (d. 1067) Deaths. 2006a). And finally, SN 1006. Locate the supernova remnant's associated constellation on a star map. Lithograph: Supernova Remnant SN 1006 (PDF) (700KB; Adobe Reader required) This Hubble Space Telescope image shows a portion of the visible-light remnants of a supernova explosion that was observed in 1006. The radio data show much of the extent that the X-ray image shows. It was likely a white dwarf star that had been pulling matter off an orbiting companion star. 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. 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 supernova of 1006, or SN 1006, may have been the brightest supernova on record. It is located around 7,200 … 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. May 1 – The brightest supernova ever recorded, SN 1006, occurs in the constellation of Lupus.

The new Chandra image of SN 1006 contains over 8 days worth of observing time by the telescope.

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. SN 1006 resides within our Milky Way Galaxy. It is observed and described in China, Japan, the Middle East, Europe, and elsewhere. … • A mapping activity.


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