| NGC 688 | |
|---|---|
| Pan-STARRS image of NGC 688 | |
| Observation data (J2000 epoch) | |
| Constellation | Triangulum |
| Right ascension | 01h 50m 44.2s [1] |
| Declination | 35° 17′ 04″ [1] |
| Redshift | 0.013846 [1] |
| Heliocentric radial velocity | 4151 km/s [1] |
| Distance | 193 Mly (59.2 Mpc) [1] |
| Group or cluster | Abell 262 |
| Apparent magnitude (V) | 13.35 [1] |
| Characteristics | |
| Type | SBb [2] (R')SAB(rs)b [1] |
| Size | ~150,000 ly (45 kpc) (estimated) [1] |
| Apparent size (V) | 2.5 x 1.5 [1] |
| Other designations | |
| CGCG 522-20, IRAS 01478+3502, KUG 0147+350, MCG 6-5-15, Mrk 1009, PGC 6799, UGC 1302 [1] | |
NGC 688 is a barred spiral galaxy [3] [4] with starburst activity [5] [6] located 190 million light-years away [6] in the constellation Triangulum. It was discovered by astronomer Heinrich d'Arrest on September 16, 1865 [5] and is a member of the galaxy cluster Abell 262. [7] [8] [9]