NGC 1073
Coordinates: 
02h 43m 40.5s, +01° 22′ 34″
02h 43m 40.5s, +01° 22′ 34″J2000 epoch) | |
|---|---|
| Constellation | Cetus |
| Right ascension | 02h 43m 40.5s[1] |
| Declination | +01° 22′ 34″[1] |
| Redshift | 1208 ± 5 km/s[1] |
| Apparent magnitude (V) | 11.5[1] |
| Characteristics | |
| Type | SB(rs)c[1] |
| Apparent size (V) | 4.9′ × 4.5′[1] |
| Other designations | |
| UGC 2210,[1] PGC 10329[1] | |
NGC 1073 is a
NGC 1073 is similar to the Milky Way only in their shared possession of a galactic bar. NGC 1073, however, does not possess the well-defined symmetrical arm structure the Milky Way exhibits, and retains a central bar larger than our home galaxy's.[4] NGC 1073 can be viewed with a mid-sized telescope in rural, dark skies.
One supernova has been observed in NGC 1073: SN 1962L (type Ic, mag. 13.9) was discovered by Leonida Rosino on 23 November 1962,[5] and independently by Enrique Chavira and Guillermo Haro.[6]
References
- ^ a b c d e f g h NED (February 25, 2007), Results for search on NGC 1073
- S2CID 17086638
- ^ Staff (3 February 2012). "Hubble Telescope Spies Milky Way Galaxy's Twin". Space.com. Retrieved 3 February 2012.
- ^ National Radio Astronomy Observatory Milky Way
- ^ Thernoe, K. A. (3 December 1962). "Circular No. 1809". Central Bureau for Astronomical Telegrams. Smithsonian Astrophysical Observatory. Retrieved 1 December 2024.
- ^ "SN 1962L". Transient Name Server. IAU. Retrieved 1 December 2024.
External links
Wikimedia Commons has media related to NGC 1073.
- NGC 1073 on
- Video (01:18)
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