NGC 93

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NGC 93
N90s.jpg
NGC 93 (top right) and its spiral companion to the left, NGC 90
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 00h 22m 03.211s [1]
Declination +22° 24 29.15 [1]
Redshift 0.017946 [2]
Helio radial velocity 5380 ± 10 km/s [2]
Distance 259.7 ± 68.1 Mly
(79.633 ± 20.875 Mpc) [2]
Apparent magnitude  (V)14.34 [2]
Characteristics
Type S [2]
Apparent size  (V)1.4' x 0.7' [3]
Other designations
UGC 209, [2] MCG+04-02-012,PGC 1412 [2]

NGC 93 is an interacting spiral galaxy estimated to be about 260 million light-years away in the constellation of Andromeda. It was discovered by R. J. Mitchell in 1854. [3] The galaxy is currently interacting with NGC 90 and has some signs of interacting with it.

NGC 93 and NGC 90 form the interacting galaxy pair Arp 65.

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<span class="mw-page-title-main">NGC 5613</span> Galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 5545</span> Spiral galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 5755</span> Galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 5754</span> Galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 5752</span> Galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 42</span> Galaxy located in the constellation Pegasus

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<span class="mw-page-title-main">NGC 4634</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 80</span>

"Legacy Survey Sky Browser". www.legacysurvey.org. Retrieved 2023-05-19.

<span class="mw-page-title-main">NGC 50</span> Galaxy in the constellation Cetus

NGC 50 is an elliptical galaxy in the constellation Cetus with a diameter of 170,000 light-years. It was discovered in 1865 by Gaspare Ferrari. The galaxy is, in comparison to the Milky Way, about 1.5-2 times as large. It is also physically close to NGC 49.

<span class="mw-page-title-main">NGC 78</span> A pair of spiral galaxies in the constellation Pisces

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<span class="mw-page-title-main">NGC 85</span> Lenticular galaxy in the constellation Andromeda

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<span class="mw-page-title-main">NGC 90</span> Galaxy in the constellation Andromeda

NGC 90 is an interacting spiral galaxy estimated to be about 300 million light-years away in the constellation of Andromeda. It was discovered by R. J. Mitchell in 1854 and its apparent magnitude is 13.7. The galaxy is currently interacting with NGC 93 and exhibits two highly elongated and distorted spiral arms with bright blue star clusters indicative of star formation, likely caused by the interaction with its neighbor.

<span class="mw-page-title-main">NGC 94</span> Lenticular galaxy in the constellation Andromeda

NGC 94 is a lenticular galaxy in the constellation Andromeda. It was discovered by Guillaume Bigourdan in 1884. This object is extremely faint and small. A little above the galaxy is NGC 96. NGC 94 is about 260 million light-years away and 50,000 light-years across.

<span class="mw-page-title-main">NGC 6052</span> Interacting galaxies in the constellation Hercules

NGC 6052 is a pair of galaxies in the constellation of Hercules. It was discovered on 11 June 1784 by William Herschel. It was described as "faint, pretty large, irregularly round" by John Louis Emil Dreyer, the compiler of the New General Catalogue.

<span class="mw-page-title-main">NGC 5011</span> Galaxy in the constellation Centaurus

NGC 5011 is an elliptical galaxy in the constellation of Centaurus. It was discovered on 3 June 1834 by John Herschel. It was described as "pretty bright, considerably small, round, among 4 stars" by John Louis Emil Dreyer, the compiler of the New General Catalogue.

<span class="mw-page-title-main">NGC 810</span> Elliptical galaxy in the constellation Cetus

NGC 810 is an unbarred elliptical galaxy located in the constellation Cetus, approximately 360 million light-years from the Milky Way. It was discovered by the French astronomer Édouard Stephan in 1871.

<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.

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 5 6 7 "NED results for object NGC 0093". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. 2008. Retrieved 26 November 2016.
  3. 1 2 "NGC Objects: NGC 50 - 99".