Crab Nebula, M 1

06.05

The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. It is not, as its name might suggest, in Cancer. The now-current name is due to William Parsons, 3rd Earl of Rosse who observed the object in 1840 using a 36-inch telescope and produced a drawing that looked somewhat like a crab. Corresponding to a bright supernova recorded by Chinese astronomers in 1054, the nebula was observed later by English astronomer John Bevis in 1731. The nebula was the first astronomical object identified with a historical supernova explosion.

  • Imaging telescopes or lenses: Takahashi FSQ 106 ED
  • Imaging cameras: Atik 460 EX Mono
  • Mounts: Takahashi EM 200 Temma 2
  • Guiding telescopes or lenses: Takahashi FS 60 CB
  • Guiding cameras: QHYCCD QHY5 II Mono
  • Software: Main Sequence Software Sequence Generator Pro,  PixInsight
  • Filters: Astronomik OIII 12nm,  Astronomik Ha 12nm,  Astronomik SII 12nm
  • Accessories: Atik EFW2 Filter Wheel
  • Resolution: 1282×1023
  • Dates: Jan. 28, 2014
  • Frames:
    Astronomik Ha 12nm: 12×300″
    Astronomik OIII 12nm: 12×300″
  • Integration: 2.0 hours
  • Avg. Moon age: 26.17 days
  • Avg. Moon phase: 12.25%
  • RA center: 83.628 degrees
  • DEC center: 22.010 degrees
  • Pixel scale: 1.767 arcsec/pixel
  • Orientation: 87.704 degrees
  • Field radius: 0.403 degrees

Author: Kingo

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