NGC 2800

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NGC 2800
NGC2800 - SDSS DR14.jpg
SDSS image of NGC 2800
Observation data (J2000 epoch)
Constellation Ursa Major
Right ascension 09h 18m 35.164s [1]
Declination +52° 30′ 52.49″ [1]
Redshift 0.025338 [2]
Helio radial velocity 7500 km/s [2]
Distance 374.4 ± 26.3  Mly (114.80 ± 8.05  Mpc) [3]
Apparent magnitude  (B)14.0 [2]
Characteristics
Type E [3]
Other designations
UGC 4920, MCG +09-15-117, PGC 26302 [2]

NGC 2800, also known as PGC 26302, is an elliptical galaxy in the constellation Ursa Major. It was discovered February 17, 1831 by William Herschel. [4]

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<span class="mw-page-title-main">NGC 850</span> Lenticular galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 860</span> Elliptical galaxy in the constellation Triangulum

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<span class="mw-page-title-main">NGC 890</span> Galaxy in the constellation Triangulum

NGC 890 is a lenticular galaxy in the constellation Triangulum. It is estimated to be 180 million light-years from the Milky Way and has a diameter of approximately 130,000 ly. NGC 890 was discovered on September 13, 1784 by Wilhelm Herschel.

<span class="mw-page-title-main">NGC 902</span> Spiral galaxy in the constellation Cetus

NGC 902 is a barred spiral galaxy in the constellation Cetus. It is estimated to be 314 million light-years from the Milky Way and has a diameter of approximately 50,000 ly. NGC 902 was discovered on November 28, 1885 by Francis Leavenworth.

<span class="mw-page-title-main">NGC 550</span> Spiral galaxy in the constellation Cetus

NGC 550 is a spiral galaxy in the constellation Cetus. It is estimated to be about 300 million light-years from the Milky Way and has a diameter of approximately 110,000 light years. The German-British astronomer William Herschel discovered it on 8 October 1785.

<span class="mw-page-title-main">NGC 906</span> Galaxy in the constellation Andromeda

NGC 906 is a barred spiral galaxy in the constellation Andromeda in the northern sky. It is estimated to be 215 million light years from the Milky Way and has a diameter of approximately 110,000 ly. NGC 906 was discovered on October 30, 1878 by astronomer Édouard Stephan.

<span class="mw-page-title-main">NGC 812</span> Spiral galaxy in the constellation Andromeda

NGC 812 is a spiral galaxy located in the Andromeda constellation, an estimated 175 million light-years from the Milky Way. NGC 812 was discovered on December 11, 1876 by astronomer Édouard Stephan.

<span class="mw-page-title-main">NGC 813</span> Lenticular galaxy in the constrellation Hydrus

NGC 813 is a lenticular galaxy in the constellation Hydrus. It is estimated to be 390 million light-years from the Milky Way and has a diameter of approximately 140,000 ly. NGC 813 was discovered on November 24, 1834 by the British astronomer John Herschel.

<span class="mw-page-title-main">NGC 992</span> Spiral galaxy in the constellation Aries

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<span class="mw-page-title-main">NGC 937</span> Barred spiral galaxy in the constellation Andromeda

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<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 736</span> Galaxy in the constellation Triangulum

NGC 736 is an elliptical galaxy in the constellation Triangulum. It is an estimated 200 million light years from the Milky Way and has a diameter of approximately 85,000 light years. NGC 736 was discovered on September 12, 1784 by the German-British astronomer William Herschel.

<span class="mw-page-title-main">NGC 768</span> Galaxy in the constellation Cetus

NGC 768 is a barred spiral galaxy located in the constellation Cetus about 314 million light years from the Milky Way. It was discovered by the American astronomer Lewis Swift in 1885.

<span class="mw-page-title-main">NGC 656</span> Lenticular galaxy in the constellation Pisces

NGC 656 is a barred lenticular galaxy located in the Pisces constellation about 175 million light-years from the Milky Way. It was discovered by the Prussian astronomer Heinrich d'Arrest in 1865.

<span class="mw-page-title-main">NGC 677</span> Galaxy in Constellation of Aries

NGC 677 is an elliptical galaxy located in the constellation Aries. It was discovered on September 25, 1886, by the astronomer Lewis A. Swift. It is located about 200 million light-years from Earth at the center of a rich galaxy cluster. It has a LINER nucleus.

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 2800". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-06-05.
  3. 1 2 "Results for object NGC 2800 (NGC 2800)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020-06-05.
  4. ↑ "New General Catalog Objects: NGC 2800 - 2849".


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