NGC 7812

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NGC 7812
NGC 7812 legacy dr10.jpg
Observation data (J2000 epoch)
Constellation Sculptor
Right ascension 00h 02m 54.460s [1]
Declination −34° 14 08.40 [1]
Redshift 0.022799 [2]
Heliocentric radial velocity 6757 ± 19 km/s [2]
Distance 314.2 ± 22.0  Mly (96.33 ± 6.76  Mpc) [3]
Apparent magnitude  (B)13.99 [4]
Characteristics
Type SAB(rs)b: [3]
Other designations
MCG -06-01-016, PGC 195 [2]

NGC 7812 (also known PGC 195) as is an intermediate spiral galaxy in the constellation Sculptor. [5] The galaxy was discovered on 25 September 1865 by Sir John Hershel. At its widest, it measures approximately 100-thousand light years (30660 parsecs) across, and is 315 million light years away from Earth. [6]

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See also

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<span class="mw-page-title-main">NGC 4780</span> Spiral galaxy in the constellation Virgo

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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 467</span> Galaxy in the constellation Pisces

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<span class="mw-page-title-main">NGC 74</span> Galaxy in the constellation Andromeda

NGC 74 is a lenticular galaxy located in the Andromeda constellation. It was discovered on 7 October 1855 by Irish astronomer William Parsons.

<span class="mw-page-title-main">NGC 75</span> Galaxy in the constellation Pisces

NGC 75 is a lenticular galaxy estimated to be about 260 million light-years away in the constellation of Pisces. It was discovered by Lewis A. Swift from the USA in 1886 and its magnitude is 13.2.

<span class="mw-page-title-main">NGC 113</span> Galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 115</span> Galaxy in the constellation of Sculptor

NGC 115 is a barred spiral galaxy located in the southern constellation of Sculptor. It was discovered by the British astronomer John Herschel on September 25, 1834. The galaxy is approximately 85 million light-years from the Sun, and is about 50,000 light-years in diameter, nearly half the size of our home galaxy, the Milky Way.

<span class="mw-page-title-main">NGC 178</span> Magellanic spiral galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 479</span> Spiral galaxy in the constellation Pisces

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

NGC 1326 is a lenticular galaxy in the constellation Fornax, 63 million light-years away. It was discovered by English astronomer John Herschel on 29 November 1837. It is a member of the Fornax Cluster, an NGC 1316 subgroup and has a diameter of 70 000 light-years.

<span class="mw-page-title-main">NGC 4380</span> Galaxy in the constellation Virgo

NGC 4380 is an unbarred spiral galaxy located in the constellation of Virgo. Located about 52.2 million light-years away, is a member of the Virgo Cluster, a large galaxy cluster. It was discovered on March 10, 1826, by the astronomer John Herschel.

<span class="mw-page-title-main">NGC 880</span> Galaxy in the constellation Cetus

NGC 880 is a spiral galaxy located in the constellation Cetus about 590 million light-years from the Milky Way. It was discovered by the American astronomer Francis Leavenworth in 1886.

<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.

<span class="mw-page-title-main">NGC 532</span> Spiral galaxy in the constellation Pisces

NGC 532 is a spiral galaxy in the constellation Pisces. The galaxy is approximately 100 million light-years away from the Earth, and was discovered on September 21, 1786, by the German-British astronomer William Herschel.

<span class="mw-page-title-main">NGC 3902</span> Spiral galaxy in the constellation Leo

NGC 3902 is an intermediate spiral galaxy in the constellation Leo. It was discovered on April 6, 1785, by William Herschel and observed on February 19, 1827, by John Herschel. It is estimated to be 180 to 185 million light-years away, and its redshift-independent distance estimates to about 185 to 240 million light-years. It is around 75,000 light-years in diameter.

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 "NGC 7812". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2021-02-21.
  3. 1 2 "Results for object NGC 7812 (NGC 7812)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-21.
  4. "Search specification: NGC 7812". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-21.
  5. "NGC 7812 Facts". Universe Guide. Retrieved 2019-12-11.
  6. "New General Catalog Objects: NGC 7800 - 7840". cseligman.com. Retrieved 2019-12-10.