NGC 950

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NGC 950
NGC 950 DECam.jpg
DECam image of NGC 950
Observation data (J2000 epoch)
Constellation Cetus
Right ascension 02h 29m 11.777s [1]
Declination −11° 01′ 28.78″ [1]
Redshift 0.015775 [2]
Helio radial velocity 4692 km/s [2]
Distance 204.5  Mly (62.71  Mpc) [3]
Apparent magnitude  (B)14.48 [2]
Characteristics
Type SB(rs)b: [4]
Other designations
MCG -02-07-021, PGC 9461 [2]

NGC 950 is a barred spiral galaxy in the constellation Cetus. It is approximately 205 million light-years [3] away from the Solar System and has a diameter of about 85,000 light-years. The object was discovered in 1886 by American astronomer and mathematician Ormond Stone. [5]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 1683</span> Spiral galaxy in the constellation Orion

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<span class="mw-page-title-main">NGC 5201</span> Spiral galaxy in the constellation Ursa Major

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<span class="mw-page-title-main">NGC 1326</span> Galaxy in the constellation Fornax

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<span class="mw-page-title-main">NGC 990</span> Galaxy located in the constellation Aries

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<span class="mw-page-title-main">NGC 670</span> Galaxy in the constellation Triangulum

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<span class="mw-page-title-main">NGC 790</span> Galaxy in the constellation Cetus

NGC 790 is a lenticular galaxy in the constellation Cetus. It is estimated to be 233 million light-years from the Milky Way and has a diameter of approximately 90,000 light years. NGC 790 was discovered on September 10, 1785 by the German-British astronomer William Herschel.

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<span class="mw-page-title-main">NGC 996</span> Galaxy in the constellation Andromeda

NGC 996 is an elliptical galaxy of the Hubble type E0 in the constellation Andromeda. It is estimated to be 210 million light years from the Milky Way and has a diameter of approximately 75,000 ly. The supernova SN 1996bq occurred in this galaxy. NGC 996 was discovered on December 7, 1871 by astronomer Édouard Stephan.

<span class="mw-page-title-main">NGC 736</span> Galaxy in the constellation Triangulum

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<span class="mw-page-title-main">NGC 766</span> Galaxy in the constellation Pisces

NGC 766 is an elliptical galaxy located in the Pisces constellation about 362 million light years from the Milky Way. It was discovered by British astronomer John Herschel in 1828.

<span class="mw-page-title-main">NGC 861</span> Spiral galaxy in the constellation Triangulum

NGC 861 is a spiral galaxy in the constellation Triangulum. It is estimated to be 360 million light-years from the Milky Way and has a diameter of approximately 165,000 light-years. The object was discovered on September 18, 1865 by Heinrich d'Arrest.

References

  1. 1 2 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. 1 2 3 4 "NGC 950". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-05-30.
  3. 1 2 Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 790–813. arXiv: astro-ph/0610732 . Bibcode:2007ApJ...655..790C. doi:10.1086/510201. S2CID   11672751.
  4. ↑ "Results for object NGC 0950 (NGC 950)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020-05-30.
  5. ↑ "Revised NGC Data for NGC 950". spider.seds.org. Retrieved 2020-02-12.


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