M1 Crab Nebula

M1 - NGC 1952 Crab Nebula - 100% Crop
Object Type: 

Despite to the long focal lenght this object should deserve, here a wide image of M1 Crab Nebula (with a huge crop!): stack of 7,75 hrsin L 15x900" bin1 and RGB 16x300" bin2, calibrated and stacked and processed in Pixinsight and CS5.

Full-Res Image

Image Calibration 

Center (RA, Dec): (83.641, 22.034)
Center (RA, hms): 05h 34m 33.827s
Center (Dec, dms): +22° 02' 01.016"
Size: 41.1 x 32.9 arcmin
Radius: 0.438 deg
Pixel scale: 0.986 arcsec/pixel
Orientation: Up is 0.835 degrees E of N


M1 Crab Nebula

The Crab Nebula, Messier 1 (M1, NGC 1952), is the most famous and conspicuous known supernova remnant, the expanding cloud of gas created in the explosion of a star as supernova which was observed in the year 1054 AD. It shines as a nebula of magnitude 8.4 near the southern "horn" of Taurus, the Bull.
The supernova was noted on July 4, 1054 A.D. by Chinese astronomers as a new or "guest star," and was about four times brighter than Venus, or about mag -6. According to the records, it was visible in daylight for 23 days, and 653 days to the naked eye in the night sky. It was probably also recorded by Anasazi Indian artists (in present-day Arizona and New Mexico), as findings in Navaho Canyon and White Mesa (both Arizona) as well as in the Chaco Canyon National Park (New Mexico) indicate; there's a review of the research on the Chaco Canyon Anasazi art online. In addition, Ralph R. Robbins of the University of Texas has found Mimbres Indian art from New Mexico, possibly depicting the supernova.
The Supernova 1054 was also assigned the variable star designation CM Tauri. It is one of few historically observed supernovae in our Milky Way Galaxy. The nebulous remnant was discovered by John Bevis in 1731, who added it to his sky atlas, Uranographia Britannica. Charles Messier independently found it on August 28, 1758, when he was looking for comet Halley on its first predicted return, and first thought it was a comet. Of course, he soon recognized that it had no apparent proper motion, and cataloged it on September 12, 1758. It was the discovery of this object which caused Charles Messier to begin with the compilation of his catalog. It was also the discovery of this object, which closely resembled a comet (1758 De la Nux, C/1758 K1) in his small refracting telescope, which brought him to the idea to search for comets with telescopes (see his note). Messier acknowledged the prior, original discovery by Bevis when he learned of it in a letter of June 10, 1771. Although Messier's catalog was primarily compiled for preventing confusion of these objects with comets, M1 was again confused with comet Halley on the occasion of that comet's second predicted return in 1835. This nebula was christened the "Crab Nebula" on the ground of a drawing made by Lord Rosse about 1844.