M1 – Crab nebula

in Taurus

m1 crab nebula

The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The common name comes from William Parsons, 3rd Earl of Rosse, who observed the object in 1842 and produced a drawing that looked somewhat like a crab. The nebula was discovered by English astronomer John Bevis in 1731, and it corresponds with a bright supernova recorded by Chinese astronomers in 1054. The nebula was the first astronomical object identified that corresponds with a historical supernova explosion. The nebula was independently rediscovered in 1758 by Charles Messier as he was observing a bright comet. Messier catalogued it as the first entry in his catalog of comet-like objects – the Messier catalog. From Wikipedia.

Imaging Details

 

Telescope: 6 inch f/4 Newtonian with Paracorr Type 2 (effective focal length 690mm) and 2” Feather Touch Focuser
Camera: SBIG 8300C (3326 x 2504 pixels, 5.4 x 5.4µ)
FOV: ~1.13° x 1.02°
Mount: Mesu Mount 200
Guiding: Orion 60mm guidescope with helical focuser and ZWO ASI290MM Mini guide camera
Exposure Length: 120 sec x 99, 300 sec x 5, 600 sec x 18
Location: Naples, FL
Date: 2/7/2019, 11/27/2019
Software: SciTech, SkyGuide (Innovations Foresight), Sequence Generator Pro, Optic FocusLynx, Pixinsight, SkySafari Pro