NGC 1169

NGC 1169
Image of NGC 1169 taken by Adam Block
Observation data (J2000 epoch)
Right ascension	03^h 03^m 34.756^s [1]
Declination	+46° 23′ 10.74″ [1]
Redshift	0.007962 ± 0.000017 [2]
Helio radial velocity	2387 ± 5 km/s [2]
Galactocentric velocity	2508 ± 5 km/s [2]
Distance (comoving)	35.1 ± 8.4 kpc (114 ± 27 kly)h−1 0.73 [2]
Apparent magnitude (V)	9.02 [2]
Apparent magnitude (B)	13.2 [1]
Absolute magnitude (V)	-23.6 [2]
Characteristics
Type	SAB(r)b [2]
Mass	4.5×10^11 [3] M☉
Mass/Light ratio	10 [3] M☉/L☉
Size	120,000 × 84,000 ly [2]
Apparent size (V)	4.2 × 2.8 arcmin [2]
Other designations
NGC 1169, UGC 2503, LEDA 11521

NGC 1169 (UGC 2503) is an intermediate barred spiral galaxy in the constellation of Perseus. NGC 1169 has a reddish center, indicating the region is dominated by older stars. In contrast, the outer ring contains larger blue-white stars, a sign of recent star formation.^[4][5] The entire galaxy is rotating at approximately 265 km/s ^[3]

NGC 1169 was discovered on December 11, 1786 by William Herschel.^[6] Measurements of its distance range from 20.9 Mpc - 49.7 Mpc with an average of 35.1 Mpc.^[2] and exhibits a slight ring structure.

References

1. "SIMBAD Astronomical Database". Results for NGC 1169. Retrieved 2015-11-30.
2. "NASA/IPAC Extragalactic Database". Results for NGC 1169. Retrieved 2015-11-30.
3. van Driel, W.; van Woerden, H. (1994). "Distribution and motions of HI in the Sa galaxies NGC 1169 and NGC 3898" (PDF). Astronomy and Astrophysics. 284: 395–407.
4. "Astronomy Photo of the Day: 1/03/15 — NGC 1169". futurism.com. Retrieved 2015-12-01.
5. Plait, Phil. "The Beauty of a Grain of Sand on the Cosmic Beach". slate.com. Retrieved 2015-12-01.
6. "New General Catalog Objects: NGC 1150 - 1199". cseligman.com. Retrieved 2015-12-01.

External links

• SIMBAD Astronomical Database
• NASA/IPAC Extragalactic Database
• Paper on NGC 1169 and NGC 3898