
M1 · supernova remnant
Crab Nebula
The Crab Nebula is a supernova remnant and pulsar wind nebula in the constellation of Taurus.
Image: NASA, ESA, J. Hester and A. Loll (Arizona State University).
Identity & coordinates
Identification
- Primary designation
- M1
- All designations
- M1 · NGC 1952 · Crab Nebula
- Object type
- Supernova Remnant
- Constellation
- Taurus
- Best viewing
- Winter
Coordinates & physical
- Right ascension (J2000)
- 05h 34m 31s
- Declination (J2000)
- +22° 00' 52"
- Apparent magnitude (V)
- —
- Distance
- —
Visibility tonight
The science
The Crab Nebula is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The common name comes from a drawing that somewhat resembled a crab with arms produced by William Parsons, 3rd Earl of Rosse, in 1842 or 1843 using a 36-inch (91 cm) telescope. The nebula was discovered by English astronomer John Bevis in 1731. It corresponds with a bright supernova observed in AD 1054 by Mayan, Japanese, and Arab stargazers; this supernova was also recorded by Chinese astronomers as a guest star. The nebula was the first astronomical object identified that corresponds with a historically-observed supernova explosion.
Summary adapted from Wikipedia · CC-BY-SA-4.0
References
- SIMBAD Not resolved
- NED Fetched May 8, 2026 View in NED ↗
- Wikipedia Fetched May 8, 2026 Read full article ↗
1 merge conflict resolved
- coordinates: SIMBAD missing → NED used



