NGC 1954
Appearance
NGC 1954 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Lepus |
Right ascension | 05h 32m 48.3304s[1] |
Declination | −14° 03′ 45.99″[1] |
Redshift | 0.010437[1] |
Heliocentric radial velocity | 3129 ± 2 km/s[1] |
Distance | 152.6 ± 10.7 Mly (46.79 ± 3.28 Mpc)[1] |
Apparent magnitude (V) | 11.8[1] |
Characteristics | |
Type | SA(rs)bc pec?[1] |
Size | ~194,000 ly (59.49 kpc) (estimated)[1] |
Apparent size (V) | 4.2' x 2.0'[1] |
Other designations | |
IRAS 05305-1405, 2MASX J05324835-1403460, MCG -02-15-003, PGC 17422[1] |
NGC 1954 is a large spiral galaxy in the constellation of Lepus. Its velocity with respect to the cosmic microwave background is 3,172 ± 4 km/s, which corresponds to a Hubble distance of 46.8 ± 3.3 Mpc Mpc (∼153 million light-years).[1] It was discovered by German-British astronomer William Herschel on 14 December 1786.
Three supernovae have been observed in NGC 1954: SN 2010ko (type Ia, mag. 16.8),[2] SN 2011fi (type II, mag. 17.8),[3] and SN 2013ex (type Ia, mag. 15.6).[4]
See also
[edit]References
[edit]- ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 1954. Retrieved 24 July 2024.
- ^ Transient Name Server entry for SN 2010ko. Retrieved 24 July 2024.
- ^ Transient Name Server entry for SN 2011fi. Retrieved 24 July 2024.
- ^ Transient Name Server entry for SN 2013ex. Retrieved 24 July 2024.
External links
[edit]- Media related to NGC 1954 at Wikimedia Commons
- NGC 1954 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images