Share to: share facebook share twitter share wa share telegram print page

NGC 690

NGC 690
NGC 690 imaged by the Sloan Digital Sky Survey
Observation data (J2000 epoch)
ConstellationCetus
Right ascension01h 47m 48.074s[1]
Declination−16° 43′ 19.88″[1]
Redshift0.01721±0.00003[2]
Heliocentric radial velocity5,160.03±9.89[2] km/s
Distance235.6 ± 16.5 Mly (72.25 ± 5.07 Mpc)[2]
Characteristics
TypeSAB(s)c:[2]
Other designations
AGC 410352, LEDA 6587[3]

NGC 690 is an intermediate spiral galaxy located in the constellation Cetus about 236 million light-years from the Milky Way. It was discovered by the American astronomer Francis Leavenworth in 1885.[4][5]

References

  1. ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
  2. ^ a b c d de Vaucouleurs, G.; et al. (1991). "Third reference catalogue of bright galaxies". 3.9. New York: Springer-Verlag. {{cite journal}}: Cite journal requires |journal= (help)
  3. ^ "NGC 690". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-01-10.
  4. ^ Ford, Dominic. "The galaxy NGC 690 - In-The-Sky.org". in-the-sky.org. Retrieved 2019-12-12.
  5. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-12-12.
  • Media related to NGC 690 at Wikimedia Commons


Kembali kehalaman sebelumnya