Explanation: Its popular nickname is the Spaghetti Nebula. Officially cataloged as Simeis 147 and Sharpless 2-240, it is easy to get lost following the looping and twisting filaments of this intricate supernova remnant. Seen toward the boundary of the constellations of the Bull (Taurus) and the Charioteer (Auriga), the impressive gas structure covers nearly 3 degrees on the sky, equivalent to 6 full moons. That's about 150 light-years at the stellar debris cloud's estimated distance of 3,000 light-years. The supernova remnant has an estimated age of about 40,000 years, meaning light from this powerful stellar explosion first reached the Earth when woolly mammoths roamed free. Besides the expanding remnant, this cosmic catastrophe left behind a pulsar, a fast-spinning neutron star that is the remnant of the original star's core. The featured image was captured last month from Forca Canapine, Italy.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: supernova remnant Publikacii so slovami: supernova remnant
Sm. takzhe: NGC 6960: tumannost' Ved'mina Metla Mezhdu Scilloi i Haribdoi: dvoinoe kosmicheskoe otkrytie Ostatok sverhnovoi Kassiopeya A Bol'shoi i malen'kii ostatki sverhnovyh Ostatok sverhnovoi tumannost' Rusalka Volokna ostatka sverhnovoi v Parusah Neobychnaya tumannost' Pa 30 Vse publikacii na tu zhe temu >>