NGC 5378
| NGC 5378 | |
|---|---|
 NGC 5378 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Canes Venatici |
| Right ascension | 13h 56m 51.0361s[1] |
| Declination | +37° 47′ 50.188″[1] |
| Redshift | 0.009957±0.00000667[1] |
| Heliocentric radial velocity | 2,985±2 km/s[1] |
| Distance | 152.8 ± 10.7 Mly (46.85 ± 3.29 Mpc)[1] |
| Group or cluster | NGC 5378 group (LGG 364) |
| Apparent magnitude (V) | 13.4g[1] |
| Characteristics | |
| Type | (R')SB(r)a[1] |
| Size | ~154,400 ly (47.35 kpc) (estimated)[1] |
| Apparent size (V) | 1.71′ × 1.37′[1] |
| Other designations | |
| 2MASX J13565101+3747494, UGC 8869, MCG +06-31-027, PGC 49598, CGCG 191-020[1] | |
NGC 5378 is a barred spiral galaxy in the constellation of Canes Venatici. Its velocity with respect to the cosmic microwave background is 3,176±14 km/s, which corresponds to a Hubble distance of 152.8 ± 10.7 Mly (46.85 ± 3.29 Mpc).[1] It was discovered by British astronomer John Herschel on 11 March 1831.[2][3]
NGC 5378 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[4][5]
NGC 5378 group
[edit]NGC 5378 is a member the NGC 5378 group (also known as LGG 364), which contains three galaxies, including NGC 5380 and UGC 8778.[6][7]
Supernova
[edit]One supernova has been observed in NGC 5378:
See also
[edit]References
[edit]- 1 2 3 4 5 6 7 8 9 10 11 "Results for object NGC 5378". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 26 December 2025.
- ↑ Herschel, J. F. W (1864). "Catalogue of Nebulae and Clusters of Stars". Philosophical Transactions of the Royal Society of London. 154: 1–137. Bibcode:1864RSPT..154....1H. doi:10.1098/rstl.1864.0001.
- ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 5378". Celestial Atlas. Retrieved 26 December 2025.
- ↑ Toba, Y.; Oyabu, S.; Matsuhara, H.; Malkan, M. A.; Gandhi, P.; Nakagawa, T.; Isobe, N.; Shirahata, M.; Oi, N.; Ohyama, Y.; Takita, S.; Yamauchi, C.; Yano, K. (2014). "Luminosity and Redshift Dependence of the Covering Factor of Active Galactic Nuclei viewed with WISE and Sloan Digital Sky Survey". The Astrophysical Journal. 788 (1): 45. arXiv:1404.4937. Bibcode:2014ApJ...788...45T. doi:10.1088/0004-637X/788/1/45.
- ↑ "NGC 5378". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 December 2025.
- ↑ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
- ↑ "LGG 364". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 December 2025.
- ↑ Wild, P. (1991). "Supernova 1991ak in NGC 5378". International Astronomical Union Circular (5309): 1. Bibcode:1991IAUC.5309....1W.
- ↑ "SN 1991ak". Transient Name Server. IAU. Retrieved 26 December 2025.
External links
[edit]
Media related to NGC 5378 at Wikimedia Commons- NGC 5378 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
