Nebula
Supernova remnant
Hubble Space Telescope mosaic image assembled from 24 individual Wide Field and Planetary Camera 2 exposures taken in October 1999, January 2000, and December 2000
Observation data: J2000.0 epoch
Right ascension05 34 31.8 ICRS1
Declination+22° 01′ 03″ ICRS1
Distance6500±1600 ly (2000±5002 pc)
Apparent magnitude (V)8.43
Apparent dimensions (V)420″ × 290″4
ConstellationTaurus
Physical characteristics
Radius~5.5 ly (~1.75 pc)
Absolute magnitude (V)−3.1±0.5
Notable featuresOptical pulsar
DesignationsMessier 1, NGC 1952, Taurus A, Sh2-2441

Crab Nebula

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Footnotes

  1. “M 1”. SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 7 May 2025. 2 3

  2. Kaplan, David L.; et al. (2008). “A Precise Proper Motion for the Crab Pulsar, and the Difficulty of Testing Spin-Kick Alignment for Young Neutron Stars”. The Astrophysical Journal. 677 (2): 1201–1215. arXiv:0801.1142. Bibcode:2008ApJ…677.1201K. doi:10.1086/529026. S2CID 17840947.

  3. “Messier 1”. SEDS Messier Catalog. Retrieved 21 July 2024.

  4. Trimble, Virginia Louise (1973). “The Distance to the Crab Nebula and NP 0532”. Publications of the Astronomical Society of the Pacific. 85 (507): 579–585. Bibcode:1973PASP…85..579T. doi:10.1086/129507. JSTOR 40675440. S2CID 122277030.

  5. Hester, J. J. (2008). “The Crab Nebula: An Astrophysical Chimera”. Annual Review of Astronomy and Astrophysics. 46: 127–155. Bibcode:2008ARA&A..46..127H. doi:10.1146/annurev.astro.45.051806.110608.