NGC 688

NGC 688
Pan-STARRS image of NGC 688
Observation data (J2000 epoch)
ConstellationTriangulum
Right ascension01h 50m 44.2s
Declination35° 17′ 04″
Redshift0.013846
Heliocentric radial velocity4151 km/s
Distance193 Mly (59.2 Mpc)
Group or clusterAbell 262
Apparent magnitude (V)13.35
Characteristics
TypeSBb (R')SAB(rs)b
Size~150,000 ly (45 kpc) (estimated)
Apparent size (V)2.5 x 1.5
Other designations
CGCG 522-20, IRAS 01478+3502, KUG 0147+350, MCG 6-5-15, Mrk 1009, PGC 6799, UGC 1302

NGC 688 is a barred spiral galaxy with starburst activity located 190 million light-years away in the constellation Triangulum. It was discovered by astronomer Heinrich d'Arrest on September 16, 1865 and is a member of the galaxy cluster Abell 262.

See also

References

  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 688. Retrieved 2018-11-19.
  2. ↑ "SIMBAD Astronomical Database". Results for NGC 688. Retrieved 2018-11-19.
  3. ↑ "NGC 0688". Retrieved 2018-11-20.
  4. ↑ "HyperLeda -object description". leda.univ-lyon1.fr. Retrieved 2018-11-20.
  5. 1 2 "New General Catalog Objects: NGC 650 - 699". cseligman.com. Retrieved 2018-11-14.
  6. 1 2 "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-11-20.
  7. ↑ P., Fouque; E., Gourgoulhon; P., Chamaraux; G., Paturel (May 1992). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members". Astronomy and Astrophysics Supplement Series. 93: 211. Bibcode:1992A&AS...93..211F. ISSN 0365-0138.
  8. ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-11-20.
  9. ↑ "NGC 688". Retrieved 2018-11-20.