The Spaghetti Nebula, Sh2-240 // Rafael Schmall

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The Spaghetti Nebula, Sh2-240 // Rafael Schmall

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Electric Threads of the Lightning Spaghetti Nebula (Simeis 147)
© Shaoyu Zhang
© Saverio Ferretti
It's easy to get lost following the intricate, looping, twisting filaments in this detailed image of supernova remnant Simeis 147 or, as it’s better known as, the Spaghetti Nebula. Seen about 3,000 light years away, toward the boundary of the constellations Taurus and Auriga, it covers nearly 3 degrees or 6 full moons on the sky- about 150 light-years wide. This composite image includes data taken through narrow-band filters where the reddish emission is from ionized hydrogen atoms and doubly ionized oxygen atoms is in faint blue-green hues. The supernova remnant has an estimated age of about 40,000 years, meaning light from the massive stellar explosion first reached Earth 40,000 years ago. But the expanding remnant is not the only aftermath. The cosmic catastrophe also left behind a spinning neutron star, or pulsar. It’s all that remains of the original star's core.
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Image Credit & Copyright: Jason Dain
Simeis 147.
Credit: Jerry Lodriguss

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Simeis 147: Supernova Remnant
It's easy to get lost following intricate filaments in this detailed image of faint supernova remnant Simeis 147. Also cataloged as Sharpless 2-240 it goes by the popular nickname, the Spaghetti Nebula. Seen toward the boundary of the constellations Taurus and Auriga, it covers nearly 3 degrees or 6 full moons on the sky. That's about 150 light-years at the stellar debris cloud's estimated distance of 3,000 light-years. This composite includes image data taken through narrow-band filters, enhancing the reddish emission from ionized hydrogen atoms to trace the shocked, glowing gas. The supernova remnant has an estimated age of about 40,000 years, meaning light from the massive stellar explosion first reached Earth 40,000 years ago. But the expanding remnant is not the only aftermath. The cosmic catastrophe also left behind a spinning neutron star or pulsar, all that remains of the original star's core.
Credit: Daniel López / IAC
The Spaghetti Nebula (Sh2-240) and the star Elnath (β Tauri) // Artem Mironov
The Spaghetti Nebula, Simeis 147 // jmarinotero