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S147
Simeis 147
Exposure Data
  • Image Field of View: 5.63° x 3.75°
  • Camera Field of View: 7.67° x 3.75°
  • Lens: Nikkor 180 mm f/2.8 ED AI-S
  • Focal Length: 180 mm
  • Focal Ratio: f/2.8
  • Camera:
    • Modified Canon Digital Rebel XS (1000D)
    • Canon 20Da
  • ISO: 1600
  • Exposure: 4 Hours total
    • Ha: 8 x 900 seconds
    • 30 x 240 seconds
  • Filter:
    • Ha: Astronomik 6nm narrowband
    • RGB: Astronomik CLS filter
  • SQM: 21.81

Simeis 147, the Flying Spaghetti Monster Nebula, is a large, extremely faint, supernova remnant located on the border between the constellations of Taurus and Auriga 3 degrees east of Elnath (Beta Tauri).

Also cataloged as Sh2-240, the faint tendrils of the nebula cover more than 3 x 3 degrees of sky. At its estimated distance of 3,000 light-years, this covers 150 light-years in space.

The supernova explosion, which occurred 30,000 years ago, left behind the nebula, and at its core, a spinning neutron star known as pulsar PSR J0538+2817.

Simeis 147 was discovered by Grigori Abramovich Shajn and V.T. Hase in 1952 at the Crimean Astrophysical Observatory at Simeis in the former U.S.S.R. with a 25-inch Schmidt camera on photographic plates.

A small ionized HII nebula, SH2-242 (LBN 826), is at lower left in the image.

North is to the top in the above image.

Simeis 147
  • Catalogs: S147, Sh2-240
  • Common Name: Flying Spaghetti Monster
  • Object Type: Supernova Remnant
  • Size: 6° x 4°
  • Constellation: Taurus
  • Image Field Centered At:
    • RA: 05h 40m 42s
    • Dec: +27° 53' 42"




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