NGC 94

Last updated
NGC 94
NGC94 - SDSS DR14.jpg
SDSS image of NGC 94
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 00h 22m 13.516s [1]
Declination +22° 28 59.22 [1]
Redshift 0.019604 [2]
Helio radial velocity 5877 [2]
Distance 260  Mly (80  Mpc) [2]
Apparent magnitude  (B)15.6 [3]
Characteristics
Type S0 [4]
Size50,000  ly (15,000  pc) [4]
Apparent size  (V)0.45 × 0.4 [4]
Other designations
PGC 1423 [3]

NGC 94 (PGC 1423) 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. [4]

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<span class="mw-page-title-main">NGC 3554</span> Galaxy in the constellation Ursa Major

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<span class="mw-page-title-main">NGC 584</span> Galaxy in the constellation Cetus

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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 3501</span> Spiral galaxy in the constellation Leo

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<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 79</span> Elliptical galaxy in the constellation Andromeda

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<span class="mw-page-title-main">NGC 81</span> Lenticular galaxy in the constellation Andromeda

NGC 81 is a lenticular galaxy estimated to be about 270 million light-years away in the constellation of Andromeda.

<span class="mw-page-title-main">NGC 83</span> Elliptical galaxy in the constellation Andromeda

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

NGC 85 is an interacting spiral or lenticular galaxy estimated to be about 200 million light-years away in the constellation of Andromeda. It was discovered by Ralph Copeland in 1873 and its apparent magnitude is 15.7. The galaxy appears to be interacting with the companion spiral IC 1546.

<span class="mw-page-title-main">NGC 96</span> Lenticular galaxy in the constellation Andromeda

NGC 96 is a lenticular galaxy estimated to be about 290 million light-years away in the constellation of Andromeda. It was discovered by Guillaume Bigourdan in 1884 and its apparent magnitude is 17.

<span class="mw-page-title-main">NGC 97</span> Galaxy in the constellation Andromeda

NGC 97 is an elliptical galaxy estimated to be about 230 million light-years away in the constellation of Andromeda. It was discovered by John Herschel in 1828 and its apparent magnitude is 13.5.

<span class="mw-page-title-main">NGC 102</span> Galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 1222</span> Lenticular galaxy in the constellation Eridanus

NGC 1222 is an early-type lenticular galaxy located in the constellation of Eridanus. The galaxy was discovered on 5 December 1883 by the French astronomer Édouard Stephan. John Louis Emil Dreyer, the compiler of the New General Catalogue, described it as a "pretty faint, small, round nebula" and noted the presence of a "very faint star" superposed on the galaxy.

<span class="mw-page-title-main">NGC 5470</span> Spiral galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 920</span> Barred spiral galaxy in the constellation Andromeda

NGC 920 is a barred spiral galaxy in the Andromeda constellation. The celestial object was discovered on September 11, 1885 by the American astronomer Lewis A. Swift.

<span class="mw-page-title-main">NGC 939</span> Elliptical or lenticular galaxy in the constellation Eridanus

NGC 939 is a lenticular or elliptical galaxy in the constellation Eridanus. It is estimated to be 241 million light-years from the Milky Way and has a diameter of approximately 80,000 ly. NGC 939 was discovered on October 18, 1835 by astronomer John Herschel.

<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 5619</span> Spiral galaxy in the constellation Virgo

NGC 5619 is an intermediate spiral galaxy in the constellation Virgo. The galaxy was found on April 10, 1828 by the British astronomer John Herschel. It is located about 390 million light-years away from the Sun.

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 "NED results for object NGC 0094". National Aeronautics and Space Administration / Infrared Processing and Analysis Center . Retrieved 19 February 2017.
  3. 1 2 "NGC 94". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 19 February 2017.
  4. 1 2 3 4 Seligman, Courtney. "Celestial Atlas NGC Objects: NGC 77". Celestial Atlas. Retrieved 8 August 2015.